EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN)

 CERN-EP-2024-098 LHCb-PAPER-2023-044 30 April 2024

1.25 Template for writing LHCb papers

LHCb collaboration†††Authors are listed at the end of this paper.

The four decays, $\Lbdecays$, are observed for the first time using proton-
proton collision data collected with the LHCb detector at a centre-of-mass
energy of $13\text{\,Te\kern-1.00006ptV}$, corresponding to an integrated
luminosity of $6\text{\,fb}^{-1}$. By considering the decay as reference
channel, the following branching fraction ratios are measured to be,

$\begin{split}\frac{{\mathcal{B}}\left(\LbtoScDmK\right)}{{\mathcal{B}}\left(\LbtoLcDzK\right)}&=\RBRresult{0.282}{0.016}{0.016}{0.005},\\\
\frac{{\mathcal{B}}(\LbtoScstDmK)}{{\mathcal{B}}(\LbtoScDmK)}&=\RBRresultNoBrErr{0.460}{0.052}{0.028},\\\
\frac{{\mathcal{B}}(\LbtoScDstK)}{{\mathcal{B}}(\LbtoScDmK)}&=\RBRresult{2.261}{0.202}{0.129}{0.046},\\\
\frac{{\mathcal{B}}(\LbtoScstDstK)}{{\mathcal{B}}(\LbtoScDmK)}&=\RBRresult{0.896}{0.137}{0.066}{0.018},\end{split}$

where the first uncertainties are statistical, the second are systematic, and
the third are due to uncertainties in the branching fractions of intermediate
particle decays. These initial observations mark the beginning of pentaquark
searches in these modes, with more data set to become available following the
LHCb upgrade.

Submitted to Phys. Rev. D (Lett.)

© 2024 CERN for the benefit of the LHCb collaboration. CC BY 4.0 licence.

##  1 Introduction

The existence of exotic pentaquark states, comprising four quarks and an anti-
quark, has been predicted since the establishment of the quark model
[GellMann:1964nj, *Zweig:352337]. The search for pentaquark candidates has
been performed by many experiments in the past 50 years [Pennington:2016dpj,
Amaryan:2022iij, Rossi:2020ezg] but only the LHCb experiment has given
conclusive results. In 2015, the LHCb experiment reported the observation of
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}p$ resonant structures [LHCb-
PAPER-2015-029, LHCb-PAPER-2016-009], consistent with pentaquark candidates
made up of minimal quark content $c\bar{c}uud$, produced in
${{\Lambda}^{0}_{\mathrm{b}}}\rightarrow{{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}p{{\mathrm{K}}^{-}}$
decays.111Inclusion of charge-conjugate processes is implied throughout. An
amplitude analysis showed that the data is best described with the inclusion
of two pentaquark states, the $P_{\psi}^{N}(4380)^{+}$ and
$P_{\psi}^{N}(4450)^{+}$. With additional data and an improved selection
strategy, it was found that the $P_{\psi}^{N}(4450)^{+}$ structure resolves
into two narrower substructures, the $P_{\psi}^{N}(4440)^{+}$ and
$P_{\psi}^{N}(4457)^{+}$. In addition, a new narrow pentaquark candidate, the
$P_{\psi}^{N}(4312)^{+}$ was discovered [LHCb-PAPER-2019-014].

The newly observed exotic candidates have masses less than
$10\text{\,Me\kern-1.00006ptV}$ below the $\Sigma_{c}\DorDstarb$
thresholds.222Natural units with $\hbar=c=1$ are used throughout. The
proximity of the pentaquark candidates to open-charm thresholds, as well as
their very narrow widths, favor the loosely bound (so-called molecular)
pentaquark model, in which the $\DorDstarb$ meson and the $\Sigma_{c}^{(*)}$
baryon are bound by a residual strong force similar to that binding a proton
and neutron to form a deuteron [Weinberg:Deuteron1965]. In addition, several
molecular pentaquark models predict that a ${P_{\psi}^{N+}}$ with $3/2^{-}$
spin-parity would decay substantially into $\Sigma_{c}^{(*)}{\kern
0.0pt\overline{\kern 0.0pt\mathrm{D}}}$ [Du:2021fmf, Burns:2021jlu,
He:2019rva, Pan:2023hrk]. This motivates the search for $\Lbdecays$
decays,333The symbols and refer to $\Sigma_{c}(2455)^{++}$ and
$\Sigma_{c}(2520)^{++}$. whose tree-level Feynman diagrams, shown in Fig. 1
(left), are color-suppressed but not forbidden [Liu:2015fea]. The
topologically similar $\LbtoLcDzK$ process is chosen as the reference mode,
which has contributions from both color-suppressed and color-favored tree-
level diagrams. As shown in Fig. 1 (right) for the color-favored process, the
spectator quarks ($ud$) of the ${{\Lambda}^{0}_{\mathrm{b}}}$ baryon directly
propagate into the charmed baryon ($udc$), which must preserve the isospin-0
quantum number of the parent ${{\Lambda}^{0}_{\mathrm{b}}}$ baryon, and thus
be a ${{\Lambda}^{+}_{\mathrm{c}}}$ state.

$u[d]$$u[d]$$\,\,\,\,\,\,\,b$$c\,\,\,\,\,\,\,$$u\,\,\,\,\,\,\,$$\bar{u}\,\,\,\,\,\,\,$$d[u]$$d[u]$$s\,\,\,\,\,\,\,$$\bar{c}\,\,\,\,\,\,\,$$(c1)!0.5!(c3)-(1.5cm,0)$$(e1)!0.5!(e3)-(1.8cm,0)$${\mathrm{W}^{-}}$${{\Lambda}^{0}_{\mathrm{b}}}$pt$\scstpp\,\,\,\,\,\,\,\,\,\,\,\,$$[{{\Lambda}^{+}_{\mathrm{c}}}/{{\Sigma}_{\mathrm{c}}^{+}}]$${{\mathrm{K}}^{-}}$pt$\DorDstarm$$[\DorDstarbz]$

$d$$d$$u$$u$$b$$c$$s$$\bar{u}$$u$$\bar{c}$$(c1)!0.5!(c3)-(1.8cm,0)$$(e1)!0.5!(e3)-(1.2cm,0)$${\mathrm{W}^{-}}$${{\Lambda}^{0}_{\mathrm{b}}}$${{\Lambda}^{+}_{\mathrm{c}}}$$\DorDstarbz$${{\mathrm{K}}^{-}}$

Figure 1: Feynman diagrams for (left) color-suppressed and (right) color-
favored tree processes of the ${\Lambda}^{0}_{\mathrm{b}}$ baryon decaying
into $\Sigma_{c}^{(*)}\DorDstarb{{\mathrm{K}}^{-}}$ or
${{\Lambda}^{+}_{\mathrm{c}}}\DorDstarbz{{\mathrm{K}}^{-}}$.

This Letter presents the search for four new $\Lbdecays$ decay modes using
proton-proton ($pp$) collision data collected by the LHCb experiment at a
centre-of-mass energy of $13\text{\,Te\kern-1.00006ptV}$ during the Run 2
data-taking period from 2015 to 2018, corresponding to an integrated
luminosity of $6\text{\,fb}^{-1}$. The relative branching fractions,
$\frac{{\mathcal{B}}\left(\LbtoScDmK\right)}{{\mathcal{B}}\left(\LbtoLcDzK\right)}$,
$\frac{{\mathcal{B}}(\LbtoScstDmK)}{{\mathcal{B}}(\LbtoScDmK)}$,
$\frac{{\mathcal{B}}(\LbtoScDstK)}{{\mathcal{B}}(\LbtoScDmK)}$, and
$\frac{{\mathcal{B}}(\LbtoScstDstK)}{{\mathcal{B}}(\LbtoScDmK)}$ are measured.
Given that the decay modes in the last three ratios have the same number of
final tracks and final states similar to those of the decay mode, their
relative branching fractions with respect to the decay are measured to
facilitate the cancelation of several systematic uncertainties due to the
effects from detector acceptance, triggers, and tracking.

##  2 Detector and simulation

The LHCb detector [LHCb-DP-2008-001, LHCb-DP-2014-002] is a single-arm forward
spectrometer covering the pseudorapidity range $2<\eta<5$, designed for the
study of particles containing $\mathrm{b}$ or $\mathrm{c}$ quarks. The
detector elements that are particularly relevant to this analysis are: a
silicon-strip vertex detector surrounding the $pp$ interaction region that
allows $\mathrm{c}$ and $\mathrm{b}$ hadrons to be identified from their
characteristically long flight distance; a tracking system that provides a
measurement of the momentum, $p$, of charged particles; and two ring-imaging
Cherenkov detectors that are able to discriminate between different species of
charged hadrons.

The online event selection is performed by a trigger [LHCb-DP-2012-004], which
consists of a hardware and a software stage. At the hardware stage, events are
required to have a muon with high transverse momentum, $p_{\mathrm{T}}$, or a
hadron, photon, or electron with high transverse energy in the calorimeters.
The triggered objects can be either hadrons from the
${\Lambda}^{0}_{\mathrm{b}}$ decays of interest (trigger on signal, TOS) or
any particle from the rest of the event (trigger independently of signal,
TIS). The software trigger applies a full event reconstruction, and
subsequently requires at least one charged particle from the event to have a
larger $p_{\mathrm{T}}$ and be inconsistent with originating from any
reconstructed primary $pp$ interaction vertex (PV). Furthermore, the
reconstructed events must have signal candidates forming a two-, three-, or
four-track secondary vertex significantly displaced from any PV. The secondary
vertices are filtered by a multivariate algorithm [LHCb-PROC-2015-018] to be
consistent with the decay of a beauty hadron.

Simulation is required to model the resolution effects of event reconstruction
and to calculate the efficiencies due to detector acceptance and selection
requirements. In the simulation, $pp$ collisions are generated using Pythia
[Sjostrand:2007gs, *Sjostrand:2006za] with a specific LHCb configuration
[LHCb-PROC-2010-056]. Decays of unstable particles are described by EvtGen
[Lange:2001uf], in which final-state radiation is generated using Photos
[davidson2015photos]. The interaction of the generated particles with the
detector, and its response, are implemented using the Geant4 toolkit
[Allison:2006ve, *Agostinelli:2002hh] as described in Ref. [LHCb-
PROC-2011-006]. The particle-identification (PID) response is not well
described in the LHCb simulation and is corrected to match that in data using
dedicated calibration samples. The corrections are based on a four-dimensional
kernel density estimation for distributions in the PID response,
$p_{\mathrm{T}}$ and $\eta$ of the track, and the multiplicity of the event
[Poluektov:2014rxa].

##  3 Candidate selection

The candidates are reconstructed through the decay chains
$\scstpp\rightarrow{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}$ with
${{\Lambda}^{+}_{\mathrm{c}}}\rightarrow p{{\mathrm{K}}^{-}}{{\uppi}^{+}}$ and
${{\mathrm{D}}^{-}}\rightarrow{{\mathrm{K}}^{+}}{{\uppi}^{-}}{{\uppi}^{-}}$ or
${{\mathrm{D}}^{*-}}\rightarrow{{\kern 0.0pt\overline{\kern
0.0pt\mathrm{D}}}{}^{0}}{{\uppi}^{-}}$ with ${{\kern 0.0pt\overline{\kern
0.0pt\mathrm{D}}}{}^{0}}\rightarrow{{\mathrm{K}}^{+}}{{\uppi}^{-}}$. The
reconstructed final-state particles are required to have PID information
consistent with their respective mass hypotheses and be inconsistent with
originating from any PV. At least one of them must have
$p>10\text{\,Ge\kern-1.00006ptV}$ and
$p_{\mathrm{T}}>1.7\text{\,Ge\kern-1.00006ptV}$. Each of the
${{\Lambda}^{+}_{\mathrm{c}}}$, ${{\kern 0.0pt\overline{\kern
0.0pt\mathrm{D}}}{}^{0}}$, and $\DorDstarm$ decay vertices must have a good
vertex-fit quality and be significantly displaced from its associated PV,
defined as the primary vertex that fits best to the flight direction of the
candidate. The reconstructed masses of the charmed hadron candidates must be
consistent with their known values [PDG2022], within
$15\text{\,Me\kern-1.00006ptV}$ for the ${{\Lambda}^{+}_{\mathrm{c}}}$ baryon
and $25\text{\,Me\kern-1.00006ptV}$ for the charmed mesons. Subsequently, the
${{\Lambda}^{0}_{\mathrm{b}}}$ candidate is reconstructed by combining
${{\Lambda}^{+}_{\mathrm{c}}}$, $\DorDstarm$, $K^{-}$ and ${{\uppi}^{+}}$
candidates to form a good vertex. The momentum vector of the
${\Lambda}^{0}_{\mathrm{b}}$ candidate is required to be consistent with the
flight direction. The sum of transverse momentum of the
${{\Lambda}^{0}_{\mathrm{b}}}$ decay products must be greater than
$5\text{\,Ge\kern-1.00006ptV}$ and the decay time of the
${{\Lambda}^{0}_{\mathrm{b}}}$ candidate is required to be greater than
$0.2\text{\,ps}$. Clone tracks are pairs of reconstructed tracks that share a
majority of their detector hits. They are rejected by requiring the opening
angle between any pair of final-state tracks from the
${{\Lambda}^{0}_{\mathrm{b}}}$ candidate to be greater than
$0.5\text{\,mrad}$. The reference channel $\LbtoLcDzK$ is reconstructed from
the same ${{\Lambda}^{+}_{\mathrm{c}}}$ and ${{\kern 0.0pt\overline{\kern
0.0pt\mathrm{D}}}{}^{0}}$ decay channels by applying the same selections.

Non-negligible peaking backgrounds in the signal and reference channels result
from ${{\Lambda}^{0}_{\mathrm{b}}}$ decays to the same final state but without
one or both intermediate charm hadrons. These are denoted by non-doubly-
charmed (NDC) backgrounds. Genuine ${\Lambda}^{+}_{\mathrm{c}}$ and ${\kern
0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{0}$ (${\mathrm{D}}^{-}$) hadrons
have nonzero lifetimes and decay at tertiary vertices in the forward direction
with respect to the ${\Lambda}^{0}_{\mathrm{b}}$ baryon decay vertex. To
suppress this background, the separation along the beam direction $z$ between
the charmed hadrons and the ${\Lambda}^{0}_{\mathrm{b}}$ decay vertex is
required to be greater than $-1\text{\,mm}$ and its significance must be
greater than $1$, $-2.5$, $-1.5$, and $-2.0$ for ${\mathrm{D}}^{-}$ in signal
decay, ${\Lambda}^{+}_{\mathrm{c}}$ in signal decay, ${\kern
0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{0}$ in reference decay, and
${\Lambda}^{+}_{\mathrm{c}}$ in reference decay, respectively. The negative
values of these requirements account for the limited resolution of the vertex
reconstruction.

Specific backgrounds from misreconstructed or misidentified particles are
vetoed by applying selections on the invariant masses. A misreconstructed
background can arise from the two final-state kaons being correctly identified
but assigned to the wrong ${\Lambda}^{+}_{\mathrm{c}}$ and
${\Lambda}^{0}_{\mathrm{b}}$ parent particles. Therefore, peaks in
${{\Lambda}^{+}_{\mathrm{c}}}\rightarrow(p{{\uppi}^{+}})_{{\Lambda}^{+}_{\mathrm{c}}}K^{-}_{{{\Lambda}^{0}_{\mathrm{b}}}}$
are vetoed, where the subscript in each final state particle denotes the
assumed parent during reconstruction.

For misidentified backgrounds, the vetoes are applied by assigning an
alternative mass hypothesis to the final state particles, and rejecting
candidates that have a recalculated invariant mass consistent with known
resonances. Misidentified background vetoes are applied for
${{\mathrm{D}}^{+}_{\mathrm{s}}}\rightarrow(\\{{{\mathrm{K}}^{+}}\Rightarrow
p\\}{{\mathrm{K}}^{-}}{{\uppi}^{+}})_{{\Lambda}^{+}_{\mathrm{c}}}$,
$\phi\rightarrow(\\{{{\mathrm{K}}^{+}}\Rightarrow
p\\}{{\mathrm{K}}^{-}})_{{\Lambda}^{+}_{\mathrm{c}}}$,
$\phi\rightarrow\\{{{\mathrm{K}}^{+}}\Rightarrow
p\\}_{{\Lambda}^{+}_{\mathrm{c}}}K^{-}_{{{\Lambda}^{0}_{\mathrm{b}}}}$,
${{\mathrm{D}}^{0}}\rightarrow({{\mathrm{K}}^{-}}\\{{{\uppi}^{+}}\Rightarrow
p\\})_{{\Lambda}^{+}_{\mathrm{c}}}$,
${{\Lambda}^{+}_{\mathrm{c}}}\rightarrow(p{{\uppi}^{+}})_{{\Lambda}^{+}_{\mathrm{c}}}\\{{{\mathrm{K}}^{-}}\Rightarrow{{\uppi}^{-}}\\}_{{{\kern
0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{0}}/{{\mathrm{D}}^{-}}}$ and
${{\mathrm{D}}^{*-}}\rightarrow{{\kern 0.0pt\overline{\kern
0.0pt\mathrm{D}}}{}^{0}}_{{\Lambda}^{0}_{\mathrm{b}}}\\{\pi^{-}\Rightarrow{{\mathrm{K}}^{-}}\\}_{{{\Lambda}^{0}_{\mathrm{b}}}/{{\Lambda}^{+}_{\mathrm{c}}}}$
decays444The particle species on the left and right of the arrow
($\Rightarrow$) correspond to the alternative and default mass hypotheses,
respectively., where the subscript denotes the parent assumed during
reconstruction. The last veto is only applied to decay chains with a ${{\kern
0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{0}}$ meson, while the others are
applied to all decay modes.

After applying all selections, a few percent of events contain multiple
candidates. These are mostly due to duplicated use of the same tracks. In such
events, the candidate with the smallest value of $\chi^{2}$ from a kinematic
fit with constrained decay vertices is retained.

##  4 Mass fit

The yields of the  () signal decays are determined from unbinned two-
dimensional maximum likelihood fits to the
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}}$ and
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$
($m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{*-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$)
invariant mass distributions, where the subscript denotes the particle
combination used to calculate the invariant masses. The
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}}$ dimension is used to
disentangle the contributions from , and nonresonant
${{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}$. To reduce the correlation between
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}}$ and
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$
($m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{*-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$)
and improve the resolution of their mass spectra, the invariant mass
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}}$ is reconstructed by a
kinematic fit which requires the ${\Lambda}^{0}_{\mathrm{b}}$ to originate
from its associated PV and constrains the ${\Lambda}^{0}_{\mathrm{b}}$,
${\Lambda}^{+}_{\mathrm{c}}$ and ${\mathrm{D}}^{-}$ (${\mathrm{D}}^{*-}$) to
their known masses[PDG2022]. The same PV constraint is also applied when
reconstructing
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$
($m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{*-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$)
but only the ${\Lambda}^{+}_{\mathrm{c}}$ and ${\mathrm{D}}^{-}$
(${\mathrm{D}}^{*-}$) masses are constrained.

Both two-dimensional fits contain six components each. The signal decays  and
include a resonant and a peaking ${\Lambda}^{0}_{\mathrm{b}}$ component. The
resonant distribution is modeled by an incoherent relativistic Breit–Wigner
distribution convolved with a Gaussian resolution function. The Breit–Wigner
masses and widths of the state are fixed to their known values[PDG2022], while
the detector resolution is obtained from simulation. The
${\Lambda}^{0}_{\mathrm{b}}$ mass peak is modeled by the sum of two Crystal
Ball [Skwarnicki:1986xj] functions, one with a low-mass tail and the other
with a high-mass tail. The two functions share a common mean. For each decay
mode, the shape parameters are determined from fits to simulation, except for
the mean and a width scale factor which are free parameters in the data fit to
account for imperfections in the simulation.

A purely combinatorial background component is described by a threshold
function in $m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}}$ and an exponential
function in
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$
($m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{*-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$),
whose parameters are determined from data. Two background components with
resonant states but non-peaking in the ${\Lambda}^{0}_{\mathrm{b}}$ invariant
mass share the shape parameters with the signal modes and share the
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$
($m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{*-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$)
exponential slope with each other, but not with the pure combinatorial
background. A peaking ${\Lambda}^{0}_{\mathrm{b}}$ background component with
nonresonant ${\Lambda}^{+}_{\mathrm{c}}$ ${\uppi}^{+}$ shares the peaking
${\Lambda}^{0}_{\mathrm{b}}$ shape parameters with the signal modes and shares
the $m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}}$ threshold function
parameters with the pure combinatorial background.

The one-dimensional projections of both fits are shown in Fig. 2. The obtained
yields are $480\pm 25$ for , $279\pm 26$ for , $243\pm 17$ for and $116\pm 15$
for signal decays. These results are tested for stability by generating and
fitting 3000 pseudoexperiments with the default model described above, and no
significant bias was observed.

Figure 2: Two-dimensional invariant mass fits of the decay, projected onto
(top left) $m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}}$ and (top right)
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$.
A similar fit to decay is projected onto (bottom left)
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}}$ and (bottom right)
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{D}}^{*-}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}}$.
The two signal contributions with resonant and are drawn as a single component
(red dashed line). Similarly, the two resonant backgrounds without
${\Lambda}^{0}_{\mathrm{b}}$ peaks are drawn together (cyan fill).

The yield of the  reference mode is determined by a one-dimensional fit to
$m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\kern 0.0pt\overline{\kern
0.0pt\mathrm{D}}}{}^{0}}{{\mathrm{K}}^{-}}}$. Similar to the treatment of the
signal decay modes, $m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\kern
0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{0}}{{\mathrm{K}}^{-}}}$ is
reconstructed by constraining the ${\Lambda}^{0}_{\mathrm{b}}$ candidate to
originate from its associated PV and applying mass constraints to the
intermediate ${\Lambda}^{+}_{\mathrm{c}}$ and ${\kern 0.0pt\overline{\kern
0.0pt\mathrm{D}}}{}^{0}$ particles to improve the mass resolution. For both
signal and background components, the ${\Lambda}^{0}_{\mathrm{b}}$ candidate
spectrum is modeled in the same way as for the signal. The fitted yield of the
reference decay is $4032\pm 75$.

##  5 Ratio of branching fractions

The yields of the signal and reference modes are corrected for the Dalitz
distribution of the ${\Lambda}^{0}_{\mathrm{b}}$ decay by considering per-
event efficiencies,

$N_{\text{corr}}=\sum_{i}\frac{s\mathcal{W}_{i}}{\epsilon(s^{12}_{i},s^{13}_{i})}$
(1)

where $N_{\text{corr}}$ is the corrected yield, $s\mathcal{W}_{i}$ is the per-
event signal weight from the method [Pivk:2004ty] and the efficiency,
$\epsilon(s^{12}_{i},s^{13}_{i})$, is calculated event-by-event based on the
Dalitz variables $s^{12}$ and $s^{13}$. These Dalitz variables represent the
square of the invariant mass of $\scstpp D^{(*)-}$ system and
$\scstpp{{\mathrm{K}}^{-}}$ system in the three-body decay of the
${\Lambda}^{0}_{\mathrm{b}}$ baryon. The efficiency is obtained by applying
the candidate selection on simulated ${\Lambda}^{0}_{\mathrm{b}}$ decays with
flat distribution over the phase space.

Given the corrected yields $N_{\text{corr}}$, the ratios of branching
fractions are calculated via

$\displaystyle\frac{\mathcal{B}(\LbtoScDmK)}{\mathcal{B}(\LbtoLcDzK)}=$
$\displaystyle\frac{N_{\text{corr}}(\LbtoScDmK)}{N_{\text{corr}}(\LbtoLcDzK)}\cdot\frac{\mathcal{B}(\DzbtoKpi)}{\mathcal{B}(\DmtoKpipi)},$
(2) $\displaystyle\frac{\mathcal{B}(\LbtoScstDmK)}{\mathcal{B}(\LbtoScDmK)}=$
$\displaystyle\frac{N_{\text{corr}}(\LbtoScstDmK)}{N_{\text{corr}}(\LbtoScDmK)},$
(3) $\displaystyle\frac{\mathcal{B}(\LbtoScDstK)}{\mathcal{B}(\LbtoScDmK)}=$
$\displaystyle\frac{N_{\text{corr}}(\LbtoScDstK)}{N_{\text{corr}}(\LbtoScDmK)}\cdot\frac{\mathcal{B}(\DmtoKpipi)}{\mathcal{B}(\DstmtoDzbpi)\mathcal{B}(\DzbtoKpi)},$
(4) $\displaystyle\frac{\mathcal{B}(\LbtoScstDstK)}{\mathcal{B}(\LbtoScDmK)}=$
$\displaystyle\frac{N_{\text{corr}}(\LbtoScstDstK)}{N_{\text{corr}}(\LbtoScDmK)}\cdot\frac{\mathcal{B}(\DmtoKpipi)}{\mathcal{B}(\DstmtoDzbpi)\mathcal{B}(\DzbtoKpi)},$
(5)

where the branching fractions ($\mathcal{B}$) of charmed mesons assume the
values published in Ref. [PDG2022]. The
$\scstpp\rightarrow{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}$ decays are not
considered in the formulas above because they are the only strong processes
allowed by the mass threshold limit, and their branching fractions are assumed
to be unity.

##  6 Systematic uncertainties

The four signal decay channels have the same final state and similar decay
topologies, hence the systematic uncertainties from the modeling of track
reconstruction efficiency in the simulation are assumed to cancel out in the
efficiency ratios. This cancelation does not apply between  (reference) and
(signal) decays because the latter has two extra pions and an intermediate .
The modeling of the track reconstruction efficiency in simulation results in a
systematic uncertainty of $1.61\%$ for each extra pion in the decays due to
the imperfect simulation of hadronic interactions with the detector material
[LHCb-DP-2013-002].

Similarly, imperfections in hardware trigger efficiencies between signal modes
are assumed to cancel out in the efficiency ratios, but not in the ratio
between  and  decays. To correct for this, the TISTOS method [LHCb-
DP-2012-004] is used to derive data-driven corrections to the simulated
values. Such factors are binned in maximum $p_{\mathrm{T}}$ of the final state
particles, for both the  and  decays. By default, the correction table derived
from decays is used to correct the simulation, and likewise when correcting
the simulation. As a systematic, only a single correction table is used to
correct both decay modes, or the correction factors derived from and decays
are used to correct and simulation respectively. The largest change in the
efficiency ratio between and decays is $0.77\%$, which is assigned as the
systematic uncertainty due to the hardware trigger efficiency correction.

The simulation PID response correction has two sources of uncertainty, one
from the kernel density estimation and one from the finite size of the
calibration samples. The width of the kernel is increased by $50\%$ and the
variation in the efficiency ratios is assigned as the systematic uncertainty.
For the finite size of the PID calibration sample, a bootstrapping
method[LHCb-PUB-2016-021] finds a change of less than $0.02\%$ in the
efficiency ratios which is thus neglected.

Systematic uncertainties due to the mass fit model are estimated by using
alternative signal and background probability density functions (PDFs). There
are two alternative Breit–Wigner PDFs: either the Blatt–Weiskopf form factor
barrier radius [Blatt:1952ije], $d$, is doubled, or the mass and width are
floated while the $m_{\Sigmacstarpp}-m_{\Sigmacpp}$ mass difference is fixed.
The two alternative peaking ${\Lambda}^{0}_{\mathrm{b}}$ PDFs are: either the
fixed tail parameters are varied by $\pm 1\sigma$ of their simulation fit
uncertainties or a Hypatia function [Santos:2013gra] is used instead of the
two Crystal Ball functions. The alternative background parameterization in
$m_{{{\Lambda}^{0}_{\mathrm{b}}}}$ uses a second-order Chebychev polynomial
instead of the default exponential function. For the threshold function
background PDFs in $m_{{{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{+}}}$, an
additional quadratic term is multiplied to the default threshold function as
an alternative PDF. The six alternative PDFs are used one-at-a-time and two-
at-a-time as alternative models to fit data, where the latter accounts for the
correlation between alternative PDFs. The largest difference in fitted yields
between any two models, default or alternative, is taken as the systematic
uncertainty on the fitted yields. These uncertainties are subsequently
propagated to the ratio of branching fractions by accounting for the
correlation between different decay modes.

When calculating the default efficiencies, the kinematic distributions of the
simulated ${\Lambda}^{0}_{\mathrm{b}}$ particles are corrected in bins of
$\eta$ and $p_{\mathrm{T}}$ to better match those in data using  decays. The
systematic uncertainty of this correction is estimated by using an alternative
(narrower) binning scheme. A systematic uncertainty of $0.05\%$ is estimated
for the ratio of branching fractions
$\mathcal{B}(\LbtoScDmK)/\mathcal{B}(\LbtoLcDzK)$ and is negligible for the
ratios of branching fractions between signal modes.

The systematic uncertainty due to the limited size of the simulated signal and
reference modes is estimated by assuming that the efficiencies follow a
binomial distribution. The systematic uncertainty due to multiple candidate
removal is calculated by assuming all removed candidates would increase the
signal or reference mode yields by the number of candidates removed. The
ratios of branching fractions are recalculated with the increased yields, and
the differences are assigned as a systematic uncertainty.

Although the simulated decay
${{\Lambda}^{+}_{\mathrm{c}}}\rightarrow{\mathrm{p}}{{\mathrm{K}}^{+}}{{\uppi}^{-}}$
includes intermediate resonances, its simulated Dalitz distribution does not
perfectly match that of real data. The ${\Lambda}^{+}_{\mathrm{c}}$ Dalitz
distribution correction is estimated from decays by comparing the
${\Lambda}^{+}_{\mathrm{c}}$ Dalitz distribution in data to simulation. This
correction is then applied to the simulated signal decay modes, and the
differences in the ratios of branching fractions are taken as systematic
uncertainties.

The contamination by NDC decays of ${\Lambda}^{0}_{\mathrm{b}}$ candidates can
be estimated by fitting the $m_{{{\Lambda}^{0}_{\mathrm{b}}}}$ distribution in
the sideband regions of $m_{{\mathrm{p}}{{\mathrm{K}}^{+}}{{\uppi}^{-}}}$ and
$m_{{{\mathrm{K}}^{+}}{{\uppi}^{-}}}$
($m_{{{\mathrm{K}}^{+}}{{\uppi}^{-}}{{\uppi}^{-}}}$), then extrapolating the
yields of NDC ${\Lambda}^{0}_{\mathrm{b}}$ to the ${\Lambda}^{+}_{\mathrm{c}}$
and ${\mathrm{D}}^{-}$ (or ${\mathrm{D}}^{*-}$) signal window. This procedure
estimates an NDC contamination of $0.9\%$ for , $4.8\%$ for , $1.1\%$ for ,
$4.1\%$ for and $3.2\%$ for . However, the ${\Lambda}^{+}_{\mathrm{c}}$ and
${\mathrm{D}}^{-}$ (or ${\mathrm{D}}^{*-}$) mass constraints smear the
$m_{{{\Lambda}^{0}_{\mathrm{b}}}}$ mass peaks of NDC backgrounds reducing the
potential bias that NDC backgrounds would have on the yields of doubly-charmed
decay modes. As a conservative estimate, half of the NDC contamination rate is
taken as a systematic uncertainty on the fitted yields, which is then
propagated to the ratios of branching fractions. A summary of the systematic
uncertainties is shown in Table 1, and the total systematic uncertainty for
each ratio is calculated by considering the correlation between different
sources of systematic uncertainties.

Table 1: Summary of systematic uncertainties. The correlation between those
due to the limited statistics of simulated samples and other sources is
considered. Systematics uncertainties due to the modeling of track
reconstruction and trigger efficiencies are assumed to cancel out in the
ratios between signal modes.

Source | $\frac{{\mathcal{B}}\left(\LbtoScDmK\right)}{{\mathcal{B}}\left(\LbtoLcDzK\right)}$ | $\frac{{\mathcal{B}}(\LbtoScstDmK)}{{\mathcal{B}}(\LbtoScDmK)}$ | $\frac{{\mathcal{B}}(\LbtoScDstK)}{{\mathcal{B}}(\LbtoScDmK)}$ | $\frac{{\mathcal{B}}(\LbtoScstDstK)}{{\mathcal{B}}(\LbtoScDmK)}$
---|---|---|---|---
Track reconstruction | 3.22% | $-$ | $-$ | $-$
Trigger efficiency | 0.77% | $-$ | $-$ | $-$
PID correction algorithm | 0.20% | 0.05% | 0.06% | 0.28%
Fitting model | 1.36% | 3.67% | 2.00% | 1.29%
Kinematic reweight | 0.05% | $<0.01\%$ | $<0.01\%$ | $<0.01\%$
Statistics of simulated samples | 2.71% | 4.01% | 3.59% | 5.58%
NDC backgrounds | 1.66% | 2.44% | 0.71% | 2.10%
Modeling of ${\Lambda}^{+}_{\mathrm{c}}$ decay amplitude | 1.28% | 0.09% | 1.58% | 0.41%
Multiple candidates | 0.06% | 1.51% | 0.38% | 3.44%
Total | 5.64% | 6.21% | 5.70% | 7.35%

##  7 Significance of signal modes

To determine the statistical significance of the signal modes, two methods are
employed. For the modes, and , the statistical significances are estimated via
Wilks’ theorem [Wilks:1938dza], which relies on the log-likelihood difference,
$\Delta\mathcal{L}$, between the default fit and a fit without the signal
mode. Under the null (no signal) hypothesis, Wilks’ theorem specifies that the
value of $2\Delta\mathcal{L}$ follows a $\chi^{2}$ distribution, with a number
of degrees-of-freedom equal to the number of additional floating parameters in
the default fit. The $p$-values calculated reject the null hypothesis at
significances of $32\sigma$ for  and $21\sigma$ for . Because these are well
above the $5\sigma$ observation threshold, the effects of systematic
uncertainties are not considered.

For the modes, pseudoexperiments are used to determine the significances of
the and signal modes. The pseudoexperiments are generated from the mass fit
model which gives the lowest yield of  (). This lowest yield model can be the
default model or one of the alternative models, which incorporates systematic
uncertainties into the calculation of statistical significance. The lowest
yield model is used to generate 5000 pseudoexperiments with the yields of
signal mode set to zero. Each pseudoexperiment is then fitted twice, once with
the signal mode yield floating to determine the signal hypothesis log-
likelihood, $\mathcal{L}_{\Sigmacstarpp}$, and once without the aforementioned
signal component to determine the null hypothesis log-likelihood
$\mathcal{L}_{0}$. The
$-2\Delta\mathcal{L}=-2\times(\mathcal{L}_{0}-\mathcal{L}_{\Sigmacstarpp})$
distribution is then modeled as a $\chi^{2}$ distribution. Subsequently, the
upper tail of this distribution is extrapolated to the data
$-2\Delta\mathcal{L}$ value to estimate a $p$-value, which rejects the null
hypotheses at significances of $13\sigma$ for and $9\sigma$ for .

##  8 Conclusion

The decays , , , and  have been observed for the first time by employing the
LHCb data sample collected during the Run 2 data-taking period, corresponding
to an integrated luminosity of 6$\text{\,fb}^{-1}$. Their measured relative
branching fractions are

$\displaystyle\frac{{\mathcal{B}}\left(\LbtoScDmK\right)}{{\mathcal{B}}\left(\LbtoLcDzK\right)}$
$\displaystyle=\RBRresult{0.282}{0.016}{0.016}{0.005},$
$\displaystyle\frac{{\mathcal{B}}(\LbtoScstDmK)}{{\mathcal{B}}(\LbtoScDmK)}$
$\displaystyle=\RBRresultNoBrErr{0.460}{0.052}{0.028},$
$\displaystyle\frac{{\mathcal{B}}(\LbtoScDstK)}{{\mathcal{B}}(\LbtoScDmK)}$
$\displaystyle=\RBRresult{2.261}{0.202}{0.129}{0.046},$
$\displaystyle\frac{{\mathcal{B}}(\LbtoScstDstK)}{{\mathcal{B}}(\LbtoScDmK)}$
$\displaystyle=\RBRresult{0.896}{0.137}{0.066}{0.018},$

where the first uncertainties are statistical, the second are systematic, and
the third are due to uncertainties in the branching fractions of intermediate
particle decays. These results provide important inputs for theoretical
studies of pentaquark production, in particular in terms of the molecular
picture.

These four decay modes only have $\mathcal{O}(100)$ candidates each in the
LHCb Run 2 dataset, which is statistically insufficient to perform an
amplitude analysis. This limitation will be overcome with Run 3 data which is
expected to increase the statistics by a large factor thanks to the increase
in luminosity and trigger efficiency [LHCb-TDR-012, LHCb-DP-2022-002]. A
future amplitude analysis of these four decay modes will help constrain the
characteristics of the three observed pentaquark candidates, which, so far,
have only been observed in the discovery channel
${{\Lambda}^{0}_{\mathrm{b}}}\rightarrow{{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}p{{\mathrm{K}}^{-}}$.

## Appendices

##  Appendix A Standard References

Below is a list of common references, as well as a list of all LHCb
publications. As they are already in prepared bib files, they can be used as
simply as \cite{LHCb-DP-2008-001} to get the LHCb detector paper. The
references are defined in the files main.bib, LHCb-PAPER.bib, LHCb-CONF.bib,
LHCb-DP.bib LHCb-TDR.bib files, with obvious contents. Each of these have
their LHCb-ZZZ-20XX-0YY number as their cite code. If you believe there is a
problem with the formatting or content of one of the entries, then get in
contact with the Editorial Board rather than just editing it in your local
file, since you are likely to need the latest version just before submitting
the article.

Table 2: Standard references. Description |  Ref. cite code
---|---
Lee, Weinberg, Zumino |  [Lee:1967iu] Lee:1967iu
Cabibbo, Kobayashi, Maskawa |  [Cabibbo:1963yz, *Kobayashi:1973fv] Cabibbo:1963yz,*Kobayashi:1973fv
Gell-Mann, Zweig |  [GellMann:1964nj, *Zweig:352337] GellMann:1964nj,*Zweig:352337
Baryon asymmetry & SM $C\\!P$ |  [Gavela:1994dt] Gavela:1994dt
Baryon asymmetry & SM $C\\!P$ |  [Gavela:1993ts] Gavela:1993ts
EW Baryogenesis & $C\\!P$ |  [Huet:1994jb] Huet:1994jb
Dalitz Plot555Dalitz invented the method, Fabri added relativistic corrections. |  [Dalitz:1953cp, *Fabri:1954zz] Dalitz:1953cp,*Fabri:1954zz
PDG 2020 |  [PDG2020] PDG2020
PDG 2019 |  [PDG2019] PDG2019
PDG 2018 |  [PDG2018] PDG2018
PDG 2016 |  [PDG2016] PDG2016
PDG 2014 |  [PDG2014] PDG2014
HFlav 2018 |  [HFLAV18] HFLAV18
HFlav 2016 |  [HFLAV16] HFLAV16
HFlav (pre-2016) |  [Amhis:2014hma] Amhis:2014hma
CKMfitter group |  [CKMfitter2005] CKMfitter2005
CKMfitter group |  [CKMfitter2015] CKMfitter2015
UTfit (Standard Model/CKM) |  [UTfit-UT] UTfit-UT
UTfit (New Physics) |  [UTfit-NP] UTfit-NP
Pythia |  [Sjostrand:2007gs, *Sjostrand:2006za] Sjostrand:2007gs,*Sjostrand:2006za
LHCb Pythia tuning |  [LHCb-PROC-2010-056] LHCb-PROC-2010-056
EvtGen |  [Lange:2001uf] Lange:2001uf
Photos |  [davidson2015photos] davidson2015photos
Geant4 |  [Allison:2006ve, *Agostinelli:2002hh] Allison:2006ve, *Agostinelli:2002hh
LHCb simulation |  [LHCb-PROC-2011-006] LHCb-PROC-2011-006
RapidSim |  [Cowan:2016tnm] Cowan:2016tnm
Dirac |  [Tsaregorodtsev:2010zz, *BelleDIRAC] Tsaregorodtsev:2010zz,*BelleDIRAC
HLT2 topological trigger |  [BBDT] BBDT
Topological trigger reoptimization — Run 2 |  [LHCb-PROC-2015-018] LHCb-PROC-2015-018
Turbo and real-time alignment — Run 2 |  [LHCb-PROC-2015-011] LHCb-PROC-2015-011
TisTos method |  [LHCb-PUB-2014-039] LHCb-PUB-2014-039
Allen |  [Aaij:2019zbu] Aaij:2019zbu
PIDCalib (for Run 1) |  [LHCb-PUB-2016-021] LHCb-PUB-2016-021
Ghost probability |  [DeCian:2255039] DeCian:2255039
Primary vertex reconstruction |  [Kucharczyk:1756296] Kucharczyk:1756296
DecayTreeFitter |  [Hulsbergen:2005pu] Hulsbergen:2005pu
SMOG |  [FerroLuzzi:2005em] FerroLuzzi:2005em
Run-2 tagging |  [Fazzini:2018dyq] Fazzini:2018dyq
OS $\mathrm{K}$, $\upmu$, $\mathrm{e}$ and VS tagging |  [LHCb-PAPER-2011-027] LHCb-PAPER-2011-027
OS charm tagging |  [LHCb-PAPER-2015-027] LHCb-PAPER-2015-027
SS kaon tagging |  [LHCb-PAPER-2015-056] LHCb-PAPER-2015-056
SS proton and pion tagging |  [LHCb-PAPER-2016-039] LHCb-PAPER-2016-039
Reommendations for multiple candidates |  [Koppenburg:2017zsh] Koppenburg:2017zsh
See also Table LABEL:tab:LHCb-DPs for LHCb performance references.
sPlot |  [Pivk:2004ty] Pivk:2004ty
sFit |  [Xie:2009rka] Xie:2009rka
Punzi’s optimization |  [Punzi:2003bu] Punzi:2003bu
BDT |  [Breiman] Breiman
BDT training |  [AdaBoost] AdaBoost
TMVA666Do not cite this instead of the actual reference for the MVA being used. |  [Hocker:2007ht, *TMVA4] Hocker:2007ht,*TMVA4
RooUnfold |  [Adye:2011gm] Adye:2011gm
scikit-learn |  [Scikit-learn-paper] Scikit-learn-paper
Laura++ |  [Back:2017zqt] Back:2017zqt
hep_ml |  [Rogozhnikov:2016bdp] Rogozhnikov:2016bdp
root_numpy |  [root-numpy] root-numpy
GammaCombo777Always cite this along with Ref. [LHCb-PAPER-2016-032] as \cite{GammaCombo,*LHCb-PAPER-2016-032} (unless LHCb-PAPER-2016-032 is cited elsewhere). |  [GammaCombo] GammaCombo
TensorFlow |  [tensorflow2015-whitepaper] tensorflow2015-whitepaper
Crystal Ball function888A valid alternative for most papers where the normalisation is not critical is to use the expression“Gaussian function with a low-mass power-law tail” or “Gaussian function with power-law tails”. In that case, no citation is needed |  [Skwarnicki:1986xj] Skwarnicki:1986xj
Hypatia function |  [Santos:2013gra] Santos:2013gra
Modified Novosibirsk function |  [Ikeda:1999aq] Ikeda:1999aq
Bukin function |  [Bukin:2007] Bukin:2007
Wilks’ theorem |  [Wilks:1938dza] Wilks:1938dza
CLs method |  [CLs] CLs
BLUE method |  [Nisius:2020jmf] Nisius:2020jmf
Bootstrapping |  [efron:1979] efron:1979
Blatt–Weisskopf barrier |  [Blatt:1952ije] Blatt:1952ije
$f_{s}/f_{d}$ at 7–8 TeV |  [fsfd] fsfd
LHC beam energy uncertainty |  [PhysRevAccelBeams.20.081003] PhysRevAccelBeams.20.081003
Table 3: LHCb detector performance papers. LHCb-DP number | Title
---|---
LHCb-DP-2021-005 [LHCb-DP-2021-005] | TBD
LHCb-DP-2021-004 [LHCb-DP-2021-004] | TBD
LHCb-DP-2021-003 [LHCb-DP-2021-003] | TBD
LHCb-DP-2021-002 [LHCb-DP-2021-002] | Centrality determination in heavy-ion collisions with the LHCb detector
LHCb-DP-2021-001 [LHCb-DP-2021-001] | TBD
LHCb-DP-2020-003 [LHCb-DP-2020-003] | TBD
LHCb-DP-2020-002 [LHCb-DP-2020-002] | TBD
LHCb-DP-2020-001 [LHCb-DP-2020-001] | TBD
LHCb-DP-2019-006 [LHCb-DP-2019-006] | TBD
LHCb-DP-2019-005 [LHCb-DP-2019-005] | TBD
LHCb-DP-2019-004 [LHCb-DP-2019-004] | Diphoton discrimination
LHCb-DP-2019-003 [LHCb-DP-2019-003] | Electron reconstruction efficiency
LHCb-DP-2019-002 [LHCb-DP-2019-002] | Real-Time analysis
LHCb-DP-2019-001 [LHCb-DP-2019-001] | Run 2 trigger performance
LHCb-DP-2018-004 [LHCb-DP-2018-004] | ReDecay
LHCb-DP-2018-003 [LHCb-DP-2018-003] | Radiation damage in TT
LHCb-DP-2018-002 [LHCb-DP-2018-002] | VeLo material map using SMOG
LHCb-DP-2018-001 [LHCb-DP-2018-001] | PIDCalib for Run 2 (use Ref. [LHCb-PUB-2016-021] for Run 1)
LHCb-DP-2017-001 [LHCb-DP-2017-001] | Performance of the Outer Tracker — Run 2
LHCb-DP-2016-003 [LHCb-DP-2016-003] | HeRSCheL
LHCb-DP-2016-001 [LHCb-DP-2016-001] | TESLA project — Run 2
LHCb-DP-2014-002 [LHCb-DP-2014-002] | LHCb detector performance
LHCb-DP-2014-001 [LHCb-DP-2014-001] | Performance of the LHCb Vertex Locator
LHCb-DP-2013-003 [LHCb-DP-2013-003] | Performance of the LHCb Outer Tracker — Run 1
LHCb-DP-2013-002 [LHCb-DP-2013-002] | Measurement of the track reconstruction efficiency at LHCb
LHCb-DP-2013-001 [LHCb-DP-2013-001] | Performance of the muon identification at LHCb
LHCb-DP-2012-005 [LHCb-DP-2012-005] | Radiation damage in the LHCb Vertex Locator
LHCb-DP-2012-004 [LHCb-DP-2012-004] | The LHCb trigger and its performance in 2011
LHCb-DP-2012-003 [LHCb-DP-2012-003] | Performance of the LHCb RICH detector at the LHC
LHCb-DP-2012-002 [LHCb-DP-2012-002] | Performance of the LHCb muon system
LHCb-DP-2012-001 [LHCb-DP-2012-001] | Radiation hardness of the LHCb Outer Tracker
LHCb-DP-2011-002 [LHCb-DP-2011-002] | Simulation of machine induced background …
LHCb-DP-2011-001 [LHCb-DP-2011-001] | Performance of the LHCb muon system with cosmic rays
LHCb-DP-2010-001 [LHCb-DP-2010-001] | First spatial alignment of the LHCb VELO …
LHCb-DP-2008-001 [LHCb-DP-2008-001] |  LHCb detector
Table 4: LHCb TDRs. LHCb-TDR number | Title
---|---
LHCb-TDR-023 [LHCb-TDR-023] | Framework TDR for LHCb Upgrade II
LHCb-TDR-022 [LHCb-TDR-022] | PLUME
LHCb-TDR-021 [LHCb-TDR-021] | Allen
LHCb-TDR-020 [LHCb-TDR-020] | SMOG Upgrade
LHCb-TDR-018 [LHCb-TDR-018] | Upgrade computing model
LHCb-PII-Physics [LHCb-PII-Physics] | Phase-II upgrade physics case
LHCb-PII-EoI [LHCb-PII-EoI] | Expression of interest for Phase-II upgrade
LHCb-TDR-017 [LHCb-TDR-017] | Upgrade software and computing
LHCb-TDR-016 [LHCb-TDR-016] | Trigger and online upgrade
LHCb-TDR-015 [LHCb-TDR-015] | Tracker upgrade
LHCb-TDR-014 [LHCb-TDR-014] | PID upgrade
LHCb-TDR-013 [LHCb-TDR-013] | VELO upgrade
LHCb-TDR-012 [LHCb-TDR-012] | Framework TDR for the upgrade
LHCb-TDR-011 [LHCb-TDR-011] | Computing
LHCb-TDR-010 [LHCb-TDR-010] | Trigger
LHCb-TDR-009 [LHCb-TDR-009] | Reoptimized detector
LHCb-TDR-008 [LHCb-TDR-008] | Inner Tracker
LHCb-TDR-007 [LHCb-TDR-007] | Online, DAQ, ECS
LHCb-TDR-006 [LHCb-TDR-006] | Outer Tracker
LHCb-TDR-005 [LHCb-TDR-005] | VELO
LHCb-TDR-004 [LHCb-TDR-004] | Muon system
LHCb-TDR-003 [LHCb-TDR-003] | RICH
LHCb-TDR-002 [LHCb-TDR-002] | Calorimeters
LHCb-TDR-001 [LHCb-TDR-001] | Magnet
Table 5: LHCb-PAPERs (which have their identifier as their cite code). DNE: Does not exist.  LHCb-PAPER-2022-020 [LHCb-PAPER-2022-020] |  LHCb-PAPER-2022-019 [LHCb-PAPER-2022-019] |  LHCb-PAPER-2022-018 [LHCb-PAPER-2022-018] |  LHCb-PAPER-2022-017 [LHCb-PAPER-2022-017] |  LHCb-PAPER-2022-016 [LHCb-PAPER-2022-016]
---|---|---|---|---
LHCb-PAPER-2022-015 [LHCb-PAPER-2022-015] |  LHCb-PAPER-2022-014 [LHCb-PAPER-2022-014] |  LHCb-PAPER-2022-013 [LHCb-PAPER-2022-013] |  LHCb-PAPER-2022-012 [LHCb-PAPER-2022-012] |  LHCb-PAPER-2022-011 [LHCb-PAPER-2022-011]
LHCb-PAPER-2022-010 [LHCb-PAPER-2022-010] |  LHCb-PAPER-2022-009 [LHCb-PAPER-2022-009] |  LHCb-PAPER-2022-008 [LHCb-PAPER-2022-008] |  LHCb-PAPER-2022-007 [LHCb-PAPER-2022-007] |  LHCb-PAPER-2022-006 [LHCb-PAPER-2022-006]
LHCb-PAPER-2022-005 [LHCb-PAPER-2022-005] |  LHCb-PAPER-2022-004 [LHCb-PAPER-2022-004] |  LHCb-PAPER-2022-003 [LHCb-PAPER-2022-003] |  LHCb-PAPER-2022-002 [LHCb-PAPER-2022-002] |  LHCb-PAPER-2022-001 [LHCb-PAPER-2022-001]
LHCb-PAPER-2021-053 [LHCb-PAPER-2021-053] |  LHCb-PAPER-2021-052 [LHCb-PAPER-2021-052] |  LHCb-PAPER-2021-051 [LHCb-PAPER-2021-051] |  |
LHCb-PAPER-2021-050 [LHCb-PAPER-2021-050] |  LHCb-PAPER-2021-049 [LHCb-PAPER-2021-049] |  LHCb-PAPER-2021-048 [LHCb-PAPER-2021-048] |  LHCb-PAPER-2021-047 [LHCb-PAPER-2021-047] |  LHCb-PAPER-2021-046 [LHCb-PAPER-2021-046]
LHCb-PAPER-2021-045 [LHCb-PAPER-2021-045] |  LHCb-PAPER-2021-044 [LHCb-PAPER-2021-044] |  LHCb-PAPER-2021-043 [LHCb-PAPER-2021-043] |  LHCb-PAPER-2021-042 [LHCb-PAPER-2021-042] |  LHCb-PAPER-2021-041 [LHCb-PAPER-2021-041]
LHCb-PAPER-2021-040 [LHCb-PAPER-2021-040] |  LHCb-PAPER-2021-039 [LHCb-PAPER-2021-039] |  LHCb-PAPER-2021-038 [LHCb-PAPER-2021-038] |  LHCb-PAPER-2021-037 [LHCb-PAPER-2021-037] |  LHCb-PAPER-2021-036 [LHCb-PAPER-2021-036]
LHCb-PAPER-2021-035 [LHCb-PAPER-2021-035] |  LHCb-PAPER-2021-034 [LHCb-PAPER-2021-034] |  LHCb-PAPER-2021-033 [LHCb-PAPER-2021-033] |  LHCb-PAPER-2021-032 [LHCb-PAPER-2021-032] |  LHCb-PAPER-2021-031 [LHCb-PAPER-2021-031]
LHCb-PAPER-2021-030 [LHCb-PAPER-2021-030] |  LHCb-PAPER-2021-029 [LHCb-PAPER-2021-029] |  LHCb-PAPER-2021-028 [LHCb-PAPER-2021-028] |  LHCb-PAPER-2021-027 [LHCb-PAPER-2021-027] |  LHCb-PAPER-2021-026 [LHCb-PAPER-2021-026]
LHCb-PAPER-2021-025 [LHCb-PAPER-2021-025] |  LHCb-PAPER-2021-024 [LHCb-PAPER-2021-024] |  LHCb-PAPER-2021-023 [LHCb-PAPER-2021-023] |  LHCb-PAPER-2021-022 [LHCb-PAPER-2021-022] |  LHCb-PAPER-2021-021 [LHCb-PAPER-2021-021]
LHCb-PAPER-2021-020 [LHCb-PAPER-2021-020] |  LHCb-PAPER-2021-019 [LHCb-PAPER-2021-019] |  LHCb-PAPER-2021-018 [LHCb-PAPER-2021-018] |  LHCb-PAPER-2021-017 [LHCb-PAPER-2021-017] |  LHCb-PAPER-2021-016 [LHCb-PAPER-2021-016]
LHCb-PAPER-2021-015 [LHCb-PAPER-2021-015] |  LHCb-PAPER-2021-014 [LHCb-PAPER-2021-014] |  LHCb-PAPER-2021-013 [LHCb-PAPER-2021-013] |  LHCb-PAPER-2021-012 [LHCb-PAPER-2021-012] |  LHCb-PAPER-2021-011 [LHCb-PAPER-2021-011]
LHCb-PAPER-2021-010 [LHCb-PAPER-2021-010] |  LHCb-PAPER-2021-009 [LHCb-PAPER-2021-009] |  LHCb-PAPER-2021-008 [LHCb-PAPER-2021-008] |  LHCb-PAPER-2021-007 [LHCb-PAPER-2021-007] |  LHCb-PAPER-2021-006 [LHCb-PAPER-2021-006]
LHCb-PAPER-2021-005 [LHCb-PAPER-2021-005] |  LHCb-PAPER-2021-004 [LHCb-PAPER-2021-004] |  LHCb-PAPER-2021-003 [LHCb-PAPER-2021-003] |  LHCb-PAPER-2021-002 [LHCb-PAPER-2021-002] |  LHCb-PAPER-2021-001 [LHCb-PAPER-2021-001]
LHCb-PAPER-2020-048 [LHCb-PAPER-2020-048] |  LHCb-PAPER-2020-047 [LHCb-PAPER-2020-047] |  LHCb-PAPER-2020-046 [LHCb-PAPER-2020-046] |  |
LHCb-PAPER-2020-045 [LHCb-PAPER-2020-045] |  LHCb-PAPER-2020-044 [LHCb-PAPER-2020-044] |  LHCb-PAPER-2020-043 [LHCb-PAPER-2020-043] |  LHCb-PAPER-2020-042 [LHCb-PAPER-2020-042] |  LHCb-PAPER-2020-041 [LHCb-PAPER-2020-041]
LHCb-PAPER-2020-040 [LHCb-PAPER-2020-040] |  LHCb-PAPER-2020-039 [LHCb-PAPER-2020-039] |  LHCb-PAPER-2020-038 [LHCb-PAPER-2020-038] |  LHCb-PAPER-2020-037 [LHCb-PAPER-2020-037] |  LHCb-PAPER-2020-036 [LHCb-PAPER-2020-036]
LHCb-PAPER-2020-035 [LHCb-PAPER-2020-035] |  LHCb-PAPER-2020-034 [LHCb-PAPER-2020-034] |  LHCb-PAPER-2020-033 [LHCb-PAPER-2020-033] |  LHCb-PAPER-2020-032 [LHCb-PAPER-2020-032] |  LHCb-PAPER-2020-031 [LHCb-PAPER-2020-031]
LHCb-PAPER-2020-030 [LHCb-PAPER-2020-030] |  LHCb-PAPER-2020-029 [LHCb-PAPER-2020-029] |  LHCb-PAPER-2020-028 [LHCb-PAPER-2020-028] |  LHCb-PAPER-2020-027 [LHCb-PAPER-2020-027] |  LHCb-PAPER-2020-026 [LHCb-PAPER-2020-026]
LHCb-PAPER-2020-025 [LHCb-PAPER-2020-025] |  LHCb-PAPER-2020-024 [LHCb-PAPER-2020-024] |  LHCb-PAPER-2020-023 [LHCb-PAPER-2020-023] |  LHCb-PAPER-2020-022 [LHCb-PAPER-2020-022] |  LHCb-PAPER-2020-021 [LHCb-PAPER-2020-021]
LHCb-PAPER-2020-020 [LHCb-PAPER-2020-020] |  LHCb-PAPER-2020-019 [LHCb-PAPER-2020-019] |  LHCb-PAPER-2020-018 [LHCb-PAPER-2020-018] |  LHCb-PAPER-2020-017 [LHCb-PAPER-2020-017] |  LHCb-PAPER-2020-016 [LHCb-PAPER-2020-016]
LHCb-PAPER-2020-015 [LHCb-PAPER-2020-015] |  LHCb-PAPER-2020-014 [LHCb-PAPER-2020-014] |  LHCb-PAPER-2020-013 [LHCb-PAPER-2020-013] |  LHCb-PAPER-2020-012 [LHCb-PAPER-2020-012] |  LHCb-PAPER-2020-011 [LHCb-PAPER-2020-011]
LHCb-PAPER-2020-010 [LHCb-PAPER-2020-010] |  LHCb-PAPER-2020-009 [LHCb-PAPER-2020-009] |  LHCb-PAPER-2020-008 [LHCb-PAPER-2020-008] |  LHCb-PAPER-2020-007 [LHCb-PAPER-2020-007] |  LHCb-PAPER-2020-006 [LHCb-PAPER-2020-006]
LHCb-PAPER-2020-005 [LHCb-PAPER-2020-005] |  LHCb-PAPER-2020-004 [LHCb-PAPER-2020-004] |  LHCb-PAPER-2020-003 [LHCb-PAPER-2020-003] |  LHCb-PAPER-2020-002 [LHCb-PAPER-2020-002] |  LHCb-PAPER-2020-001 [LHCb-PAPER-2020-001]
LHCb-PAPER-2019-046 [LHCb-PAPER-2019-046] |  |  |  |
LHCb-PAPER-2019-045 [LHCb-PAPER-2019-045] |  LHCb-PAPER-2019-044 [LHCb-PAPER-2019-044] |  LHCb-PAPER-2019-043 [LHCb-PAPER-2019-043] |  LHCb-PAPER-2019-042 [LHCb-PAPER-2019-042] |  LHCb-PAPER-2019-041 [LHCb-PAPER-2019-041]
LHCb-PAPER-2019-040 [LHCb-PAPER-2019-040] |  LHCb-PAPER-2019-039 [LHCb-PAPER-2019-039] |  LHCb-PAPER-2019-038 [LHCb-PAPER-2019-038] |  LHCb-PAPER-2019-037 [LHCb-PAPER-2019-037] |  LHCb-PAPER-2019-036 [LHCb-PAPER-2019-036]
LHCb-PAPER-2019-035 [LHCb-PAPER-2019-035] |  LHCb-PAPER-2019-034 [LHCb-PAPER-2019-034] |  LHCb-PAPER-2019-033 [LHCb-PAPER-2019-033] |  LHCb-PAPER-2019-032 [LHCb-PAPER-2019-032] |  LHCb-PAPER-2019-031 [LHCb-PAPER-2019-031]
LHCb-PAPER-2019-030 [LHCb-PAPER-2019-030] |  LHCb-PAPER-2019-029 [LHCb-PAPER-2019-029] |  LHCb-PAPER-2019-028 [LHCb-PAPER-2019-028] |  LHCb-PAPER-2019-027 [LHCb-PAPER-2019-027] |  LHCb-PAPER-2019-026 [LHCb-PAPER-2019-026]
LHCb-PAPER-2019-025 [LHCb-PAPER-2019-025] |  LHCb-PAPER-2019-024 [LHCb-PAPER-2019-024] |  LHCb-PAPER-2019-023 [LHCb-PAPER-2019-023] |  LHCb-PAPER-2019-022 [LHCb-PAPER-2019-022] |  LHCb-PAPER-2019-021 [LHCb-PAPER-2019-021]
LHCb-PAPER-2019-020 [LHCb-PAPER-2019-020] |  LHCb-PAPER-2019-019 [LHCb-PAPER-2019-019] |  LHCb-PAPER-2019-018 [LHCb-PAPER-2019-018] |  LHCb-PAPER-2019-017 [LHCb-PAPER-2019-017] |  LHCb-PAPER-2019-016 [LHCb-PAPER-2019-016]
LHCb-PAPER-2019-015 [LHCb-PAPER-2019-015] |  LHCb-PAPER-2019-014 [LHCb-PAPER-2019-014] |  LHCb-PAPER-2019-013 [LHCb-PAPER-2019-013] |  LHCb-PAPER-2019-012 [LHCb-PAPER-2019-012] |  LHCb-PAPER-2019-011 [LHCb-PAPER-2019-011]
LHCb-PAPER-2019-010 [LHCb-PAPER-2019-010] |  LHCb-PAPER-2019-009 [LHCb-PAPER-2019-009] |  LHCb-PAPER-2019-008 [LHCb-PAPER-2019-008] |  LHCb-PAPER-2019-007 [LHCb-PAPER-2019-007] |  LHCb-PAPER-2019-006 [LHCb-PAPER-2019-006]
LHCb-PAPER-2019-005 [LHCb-PAPER-2019-005] |  LHCb-PAPER-2019-004 [LHCb-PAPER-2019-004] |  LHCb-PAPER-2019-003 [LHCb-PAPER-2019-003] |  LHCb-PAPER-2019-002 [LHCb-PAPER-2019-002] |  LHCb-PAPER-2019-001 [LHCb-PAPER-2019-001]
LHCb-PAPER-2018-051 [LHCb-PAPER-2018-051] |  |  |  |
LHCb-PAPER-2018-050 [LHCb-PAPER-2018-050] |  LHCb-PAPER-2018-049 [LHCb-PAPER-2018-049] |  LHCb-PAPER-2018-048 [LHCb-PAPER-2018-048] |  LHCb-PAPER-2018-047 [LHCb-PAPER-2018-047] |  LHCb-PAPER-2018-046 [LHCb-PAPER-2018-046]
LHCb-PAPER-2018-045 [LHCb-PAPER-2018-045] |  LHCb-PAPER-2018-044 [LHCb-PAPER-2018-044] |  LHCb-PAPER-2018-043 [LHCb-PAPER-2018-043] |  LHCb-PAPER-2018-042 [LHCb-PAPER-2018-042] |  LHCb-PAPER-2018-041 [LHCb-PAPER-2018-041]
LHCb-PAPER-2018-040 [LHCb-PAPER-2018-040] |  LHCb-PAPER-2018-039 [LHCb-PAPER-2018-039] |  LHCb-PAPER-2018-038 [LHCb-PAPER-2018-038] |  LHCb-PAPER-2018-037 [LHCb-PAPER-2018-037] |  LHCb-PAPER-2018-036 [LHCb-PAPER-2018-036]
LHCb-PAPER-2018-035 [LHCb-PAPER-2018-035] |  LHCb-PAPER-2018-034 [LHCb-PAPER-2018-034] |  LHCb-PAPER-2018-033 [LHCb-PAPER-2018-033] |  LHCb-PAPER-2018-032 [LHCb-PAPER-2018-032] |  LHCb-PAPER-2018-031 [LHCb-PAPER-2018-031]
LHCb-PAPER-2018-030 [LHCb-PAPER-2018-030] |  LHCb-PAPER-2018-029 [LHCb-PAPER-2018-029] |  LHCb-PAPER-2018-028 [LHCb-PAPER-2018-028] |  LHCb-PAPER-2018-027 [LHCb-PAPER-2018-027] |  LHCb-PAPER-2018-026 [LHCb-PAPER-2018-026]
LHCb-PAPER-2018-025 [LHCb-PAPER-2018-025] |  LHCb-PAPER-2018-024 [LHCb-PAPER-2018-024] |  LHCb-PAPER-2018-023 [LHCb-PAPER-2018-023] |  LHCb-PAPER-2018-022 [LHCb-PAPER-2018-022] |  LHCb-PAPER-2018-021 [LHCb-PAPER-2018-021]
LHCb-PAPER-2018-020 [LHCb-PAPER-2018-020] |  LHCb-PAPER-2018-019 [LHCb-PAPER-2018-019] |  LHCb-PAPER-2018-018 [LHCb-PAPER-2018-018] |  LHCb-PAPER-2018-017 [LHCb-PAPER-2018-017] |  LHCb-PAPER-2018-016 [LHCb-PAPER-2018-016]
LHCb-PAPER-2018-015 [LHCb-PAPER-2018-015] |  LHCb-PAPER-2018-014 [LHCb-PAPER-2018-014] |  LHCb-PAPER-2018-013 [LHCb-PAPER-2018-013] |  LHCb-PAPER-2018-012 [LHCb-PAPER-2018-012] |  LHCb-PAPER-2018-011 [LHCb-PAPER-2018-011]
LHCb-PAPER-2018-010 [LHCb-PAPER-2018-010] |  LHCb-PAPER-2018-009 [LHCb-PAPER-2018-009] |  LHCb-PAPER-2018-008 [LHCb-PAPER-2018-008] |  LHCb-PAPER-2018-007 [LHCb-PAPER-2018-007] |  LHCb-PAPER-2018-006 [LHCb-PAPER-2018-006]
LHCb-PAPER-2018-005 [LHCb-PAPER-2018-005] |  LHCb-PAPER-2018-004 [LHCb-PAPER-2018-004] |  LHCb-PAPER-2018-003 [LHCb-PAPER-2018-003] |  LHCb-PAPER-2018-002 [LHCb-PAPER-2018-002] |  LHCb-PAPER-2018-001 [LHCb-PAPER-2018-001]
LHCb-PAPER-2017-050 [LHCb-PAPER-2017-050] |  LHCb-PAPER-2017-049 [LHCb-PAPER-2017-049] |  LHCb-PAPER-2017-048 [LHCb-PAPER-2017-048] |  LHCb-PAPER-2017-047 [LHCb-PAPER-2017-047] |  LHCb-PAPER-2017-046 [LHCb-PAPER-2017-046]
LHCb-PAPER-2017-045 [LHCb-PAPER-2017-045] |  LHCb-PAPER-2017-044 [LHCb-PAPER-2017-044] |  LHCb-PAPER-2017-043 [LHCb-PAPER-2017-043] |  LHCb-PAPER-2017-042 [LHCb-PAPER-2017-042] |  LHCb-PAPER-2017-041 [LHCb-PAPER-2017-041]
LHCb-PAPER-2017-040 [LHCb-PAPER-2017-040] |  LHCb-PAPER-2017-039 [LHCb-PAPER-2017-039] |  LHCb-PAPER-2017-038 [LHCb-PAPER-2017-038] |  LHCb-PAPER-2017-037 [LHCb-PAPER-2017-037] |  LHCb-PAPER-2017-036 [LHCb-PAPER-2017-036]
LHCb-PAPER-2017-035 [LHCb-PAPER-2017-035] |  LHCb-PAPER-2017-034 [LHCb-PAPER-2017-034] |  LHCb-PAPER-2017-033 [LHCb-PAPER-2017-033] |  LHCb-PAPER-2017-032 [LHCb-PAPER-2017-032] |  LHCb-PAPER-2017-031 [LHCb-PAPER-2017-031]
LHCb-PAPER-2017-030 [LHCb-PAPER-2017-030] |  LHCb-PAPER-2017-029 [LHCb-PAPER-2017-029] |  LHCb-PAPER-2017-028 [LHCb-PAPER-2017-028] |  LHCb-PAPER-2017-027 [LHCb-PAPER-2017-027] |  LHCb-PAPER-2017-026 [LHCb-PAPER-2017-026]
LHCb-PAPER-2017-025 [LHCb-PAPER-2017-025] |  LHCb-PAPER-2017-024 [LHCb-PAPER-2017-024] |  LHCb-PAPER-2017-023 [LHCb-PAPER-2017-023] |  LHCb-PAPER-2017-022 [LHCb-PAPER-2017-022] |  LHCb-PAPER-2017-021 [LHCb-PAPER-2017-021]
LHCb-PAPER-2017-020 [LHCb-PAPER-2017-020] |  LHCb-PAPER-2017-019 [LHCb-PAPER-2017-019] |  LHCb-PAPER-2017-018 [LHCb-PAPER-2017-018] |  LHCb-PAPER-2017-017 [LHCb-PAPER-2017-017] |  LHCb-PAPER-2017-016 [LHCb-PAPER-2017-016]
LHCb-PAPER-2017-015 [LHCb-PAPER-2017-015] |  LHCb-PAPER-2017-014 [LHCb-PAPER-2017-014] |  LHCb-PAPER-2017-013 [LHCb-PAPER-2017-013] |  LHCb-PAPER-2017-012 [LHCb-PAPER-2017-012] |  LHCb-PAPER-2017-011 [LHCb-PAPER-2017-011]
LHCb-PAPER-2017-010 [LHCb-PAPER-2017-010] |  LHCb-PAPER-2017-009 [LHCb-PAPER-2017-009] |  LHCb-PAPER-2017-008 [LHCb-PAPER-2017-008] |  LHCb-PAPER-2017-007 [LHCb-PAPER-2017-007] |  LHCb-PAPER-2017-006 [LHCb-PAPER-2017-006]
LHCb-PAPER-2017-005 [LHCb-PAPER-2017-005] |  LHCb-PAPER-2017-004 [LHCb-PAPER-2017-004] |  LHCb-PAPER-2017-003 [LHCb-PAPER-2017-003] |  LHCb-PAPER-2017-002 [LHCb-PAPER-2017-002] |  LHCb-PAPER-2017-001 [LHCb-PAPER-2017-001]
LHCb-PAPER-2016-065 [LHCb-PAPER-2016-065] |  LHCb-PAPER-2016-064 [LHCb-PAPER-2016-064] |  LHCb-PAPER-2016-063 [LHCb-PAPER-2016-063] |  LHCb-PAPER-2016-062 [LHCb-PAPER-2016-062] |  LHCb-PAPER-2016-061 [LHCb-PAPER-2016-061]
LHCb-PAPER-2016-060 [LHCb-PAPER-2016-060] |  LHCb-PAPER-2016-059 [LHCb-PAPER-2016-059] |  LHCb-PAPER-2016-058 [LHCb-PAPER-2016-058] |  LHCb-PAPER-2016-057 [LHCb-PAPER-2016-057] |  LHCb-PAPER-2016-056 [LHCb-PAPER-2016-056]
LHCb-PAPER-2016-055 [LHCb-PAPER-2016-055] |  LHCb-PAPER-2016-054 [LHCb-PAPER-2016-054] |  LHCb-PAPER-2016-053 [LHCb-PAPER-2016-053] |  LHCb-PAPER-2016-052 [LHCb-PAPER-2016-052] |  LHCb-PAPER-2016-051 [LHCb-PAPER-2016-051]
LHCb-PAPER-2016-050 [LHCb-PAPER-2016-050] |  LHCb-PAPER-2016-049 [LHCb-PAPER-2016-049] |  LHCb-PAPER-2016-048 [LHCb-PAPER-2016-048] |  LHCb-PAPER-2016-047 [LHCb-PAPER-2016-047] |  LHCb-PAPER-2016-046 [LHCb-PAPER-2016-046]
LHCb-PAPER-2016-045 [LHCb-PAPER-2016-045] |  LHCb-PAPER-2016-044 [LHCb-PAPER-2016-044] |  LHCb-PAPER-2016-043 [LHCb-PAPER-2016-043] |  LHCb-PAPER-2016-042 [LHCb-PAPER-2016-042] |  LHCb-PAPER-2016-041 [LHCb-PAPER-2016-041]
LHCb-PAPER-2016-040 [LHCb-PAPER-2016-040] |  LHCb-PAPER-2016-039 [LHCb-PAPER-2016-039] |  LHCb-PAPER-2016-038 [LHCb-PAPER-2016-038] |  LHCb-PAPER-2016-037 [LHCb-PAPER-2016-037] |  LHCb-PAPER-2016-036 [LHCb-PAPER-2016-036]
LHCb-PAPER-2016-035 [LHCb-PAPER-2016-035] |  LHCb-PAPER-2016-034 [LHCb-PAPER-2016-034] |  LHCb-PAPER-2016-033 [LHCb-PAPER-2016-033] |  LHCb-PAPER-2016-032 [LHCb-PAPER-2016-032] |  LHCb-PAPER-2016-031 [LHCb-PAPER-2016-031]
LHCb-PAPER-2016-030 [LHCb-PAPER-2016-030] |  LHCb-PAPER-2016-029 [LHCb-PAPER-2016-029] |  LHCb-PAPER-2016-028 [LHCb-PAPER-2016-028] |  LHCb-PAPER-2016-027 [LHCb-PAPER-2016-027] |  LHCb-PAPER-2016-026 [LHCb-PAPER-2016-026]
LHCb-PAPER-2016-025 [LHCb-PAPER-2016-025] |  LHCb-PAPER-2016-024 [LHCb-PAPER-2016-024] |  LHCb-PAPER-2016-023 [LHCb-PAPER-2016-023] |  LHCb-PAPER-2016-022 [LHCb-PAPER-2016-022] |  LHCb-PAPER-2016-021 [LHCb-PAPER-2016-021]
LHCb-PAPER-2016-020 [LHCb-PAPER-2016-020] |  LHCb-PAPER-2016-019 [LHCb-PAPER-2016-019] |  LHCb-PAPER-2016-018 [LHCb-PAPER-2016-018] |  LHCb-PAPER-2016-017 [LHCb-PAPER-2016-017] |  LHCb-PAPER-2016-016 [LHCb-PAPER-2016-016]
LHCb-PAPER-2016-015 [LHCb-PAPER-2016-015] |  LHCb-PAPER-2016-014 [LHCb-PAPER-2016-014] |  LHCb-PAPER-2016-013 [LHCb-PAPER-2016-013] |  LHCb-PAPER-2016-012 [LHCb-PAPER-2016-012] |  LHCb-PAPER-2016-011 [LHCb-PAPER-2016-011]
LHCb-PAPER-2016-010 [LHCb-PAPER-2016-010] |  LHCb-PAPER-2016-009 [LHCb-PAPER-2016-009] |  LHCb-PAPER-2016-008 [LHCb-PAPER-2016-008] |  LHCb-PAPER-2016-007 [LHCb-PAPER-2016-007] |  LHCb-PAPER-2016-006 [LHCb-PAPER-2016-006]
LHCb-PAPER-2016-005 [LHCb-PAPER-2016-005] |  LHCb-PAPER-2016-004 [LHCb-PAPER-2016-004] |  LHCb-PAPER-2016-003 [LHCb-PAPER-2016-003] |  LHCb-PAPER-2016-002 [LHCb-PAPER-2016-002] |  LHCb-PAPER-2016-001 [LHCb-PAPER-2016-001]
LHCb-PAPER-2015-060 [LHCb-PAPER-2015-060] |  LHCb-PAPER-2015-059 [LHCb-PAPER-2015-059] |  LHCb-PAPER-2015-058 [LHCb-PAPER-2015-058] |  LHCb-PAPER-2015-057 [LHCb-PAPER-2015-057] |  LHCb-PAPER-2015-056 [LHCb-PAPER-2015-056]
LHCb-PAPER-2015-055 [LHCb-PAPER-2015-055] |  LHCb-PAPER-2015-054 [LHCb-PAPER-2015-054] |  LHCb-PAPER-2015-053 [LHCb-PAPER-2015-053] |  LHCb-PAPER-2015-052 [LHCb-PAPER-2015-052] |  LHCb-PAPER-2015-051 [LHCb-PAPER-2015-051]
LHCb-PAPER-2015-050 [LHCb-PAPER-2015-050] |  LHCb-PAPER-2015-049 [LHCb-PAPER-2015-049] |  LHCb-PAPER-2015-048 [LHCb-PAPER-2015-048] |  LHCb-PAPER-2015-047 [LHCb-PAPER-2015-047] |  LHCb-PAPER-2015-046 [LHCb-PAPER-2015-046]
LHCb-PAPER-2015-045 [LHCb-PAPER-2015-045] |  LHCb-PAPER-2015-044 [LHCb-PAPER-2015-044] |  LHCb-PAPER-2015-043 [LHCb-PAPER-2015-043] |  LHCb-PAPER-2015-042 [LHCb-PAPER-2015-042] |  LHCb-PAPER-2015-041 [LHCb-PAPER-2015-041]
LHCb-PAPER-2015-040 [LHCb-PAPER-2015-040] |  LHCb-PAPER-2015-039 [LHCb-PAPER-2015-039] |  LHCb-PAPER-2015-038 [LHCb-PAPER-2015-038] |  LHCb-PAPER-2015-037 [LHCb-PAPER-2015-037] |  LHCb-PAPER-2015-036 [LHCb-PAPER-2015-036]
LHCb-PAPER-2015-035 [LHCb-PAPER-2015-035] |  LHCb-PAPER-2015-034 [LHCb-PAPER-2015-034] |  LHCb-PAPER-2015-033 [LHCb-PAPER-2015-033] |  LHCb-PAPER-2015-032 [LHCb-PAPER-2015-032] |  LHCb-PAPER-2015-031 [LHCb-PAPER-2015-031]
LHCb-PAPER-2015-030 [LHCb-PAPER-2015-030] |  LHCb-PAPER-2015-029 [LHCb-PAPER-2015-029] |  LHCb-PAPER-2015-028 [LHCb-PAPER-2015-028] |  LHCb-PAPER-2015-027 [LHCb-PAPER-2015-027] |  LHCb-PAPER-2015-026 [LHCb-PAPER-2015-026]
LHCb-PAPER-2015-025 [LHCb-PAPER-2015-025] |  LHCb-PAPER-2015-024 [LHCb-PAPER-2015-024] |  LHCb-PAPER-2015-023 [LHCb-PAPER-2015-023] |  LHCb-PAPER-2015-022 [LHCb-PAPER-2015-022] |  LHCb-PAPER-2015-021 [LHCb-PAPER-2015-021]
LHCb-PAPER-2015-020 [LHCb-PAPER-2015-020] |  LHCb-PAPER-2015-019 [LHCb-PAPER-2015-019] |  LHCb-PAPER-2015-018 [LHCb-PAPER-2015-018] |  LHCb-PAPER-2015-017 [LHCb-PAPER-2015-017] |  LHCb-PAPER-2015-016 [LHCb-PAPER-2015-016]
LHCb-PAPER-2015-015 [LHCb-PAPER-2015-015] |  LHCb-PAPER-2015-014 [LHCb-PAPER-2015-014] |  LHCb-PAPER-2015-013 [LHCb-PAPER-2015-013] |  LHCb-PAPER-2015-012 [LHCb-PAPER-2015-012] |  LHCb-PAPER-2015-011 [LHCb-PAPER-2015-011]
LHCb-PAPER-2015-010 [LHCb-PAPER-2015-010] |  LHCb-PAPER-2015-009 [LHCb-PAPER-2015-009] |  LHCb-PAPER-2015-008 [LHCb-PAPER-2015-008] |  LHCb-PAPER-2015-007 [LHCb-PAPER-2015-007] |  LHCb-PAPER-2015-006 [LHCb-PAPER-2015-006]
LHCb-PAPER-2015-005 [LHCb-PAPER-2015-005] |  LHCb-PAPER-2015-004 [LHCb-PAPER-2015-004] |  LHCb-PAPER-2015-003 [LHCb-PAPER-2015-003] |  LHCb-PAPER-2015-002 [LHCb-PAPER-2015-002] |  LHCb-PAPER-2015-001 [LHCb-PAPER-2015-001]
LHCb-PAPER-2014-070 [LHCb-PAPER-2014-070] |  LHCb-PAPER-2014-069 [LHCb-PAPER-2014-069] |  LHCb-PAPER-2014-068 [LHCb-PAPER-2014-068] |  LHCb-PAPER-2014-067 [LHCb-PAPER-2014-067] |  LHCb-PAPER-2014-066 [LHCb-PAPER-2014-066]
LHCb-PAPER-2014-065 [LHCb-PAPER-2014-065] |  LHCb-PAPER-2014-064 [LHCb-PAPER-2014-064] |  LHCb-PAPER-2014-063 [LHCb-PAPER-2014-063] |  LHCb-PAPER-2014-062 [LHCb-PAPER-2014-062] |  LHCb-PAPER-2014-061 [LHCb-PAPER-2014-061]
LHCb-PAPER-2014-060 [LHCb-PAPER-2014-060] |  LHCb-PAPER-2014-059 [LHCb-PAPER-2014-059] |  LHCb-PAPER-2014-058 [LHCb-PAPER-2014-058] |  LHCb-PAPER-2014-057 [LHCb-PAPER-2014-057] |  LHCb-PAPER-2014-056 [LHCb-PAPER-2014-056]
LHCb-PAPER-2014-055 [LHCb-PAPER-2014-055] |  LHCb-PAPER-2014-054 [LHCb-PAPER-2014-054] |  LHCb-PAPER-2014-053 [LHCb-PAPER-2014-053] |  LHCb-PAPER-2014-052 [LHCb-PAPER-2014-052] |  LHCb-PAPER-2014-051 [LHCb-PAPER-2014-051]
LHCb-PAPER-2014-050 [LHCb-PAPER-2014-050] |  LHCb-PAPER-2014-049 [LHCb-PAPER-2014-049] |  LHCb-PAPER-2014-048 [LHCb-PAPER-2014-048] |  LHCb-PAPER-2014-047 [LHCb-PAPER-2014-047] |  LHCb-PAPER-2014-046 [LHCb-PAPER-2014-046]
LHCb-PAPER-2014-045 [LHCb-PAPER-2014-045] |  LHCb-PAPER-2014-044 [LHCb-PAPER-2014-044] |  LHCb-PAPER-2014-043 [LHCb-PAPER-2014-043] |  LHCb-PAPER-2014-042 [LHCb-PAPER-2014-042] |  LHCb-PAPER-2014-041 [LHCb-PAPER-2014-041]
LHCb-PAPER-2014-040 [LHCb-PAPER-2014-040] |  LHCb-PAPER-2014-039 [LHCb-PAPER-2014-039] |  LHCb-PAPER-2014-038 [LHCb-PAPER-2014-038] |  LHCb-PAPER-2014-037 [LHCb-PAPER-2014-037] |  LHCb-PAPER-2014-036 [LHCb-PAPER-2014-036]
LHCb-PAPER-2014-035 [LHCb-PAPER-2014-035] |  LHCb-PAPER-2014-034 [LHCb-PAPER-2014-034] |  LHCb-PAPER-2014-033 [LHCb-PAPER-2014-033] |  LHCb-PAPER-2014-032 [LHCb-PAPER-2014-032] |  LHCb-PAPER-2014-031 [LHCb-PAPER-2014-031]
LHCb-PAPER-2014-030 [LHCb-PAPER-2014-030] |  LHCb-PAPER-2014-029 [LHCb-PAPER-2014-029] |  LHCb-PAPER-2014-028 [LHCb-PAPER-2014-028] |  LHCb-PAPER-2014-027 [LHCb-PAPER-2014-027] |  LHCb-PAPER-2014-026 [LHCb-PAPER-2014-026]
LHCb-PAPER-2014-025 [LHCb-PAPER-2014-025] |  LHCb-PAPER-2014-024 [LHCb-PAPER-2014-024] |  LHCb-PAPER-2014-023 [LHCb-PAPER-2014-023] |  LHCb-PAPER-2014-022 [LHCb-PAPER-2014-022] |  LHCb-PAPER-2014-021 [LHCb-PAPER-2014-021]
LHCb-PAPER-2014-020 [LHCb-PAPER-2014-020] |  LHCb-PAPER-2014-019 [LHCb-PAPER-2014-019] |  LHCb-PAPER-2014-018 [LHCb-PAPER-2014-018] |  LHCb-PAPER-2014-017 [LHCb-PAPER-2014-017] |  LHCb-PAPER-2014-016 [LHCb-PAPER-2014-016]
LHCb-PAPER-2014-015 [LHCb-PAPER-2014-015] |  LHCb-PAPER-2014-014 [LHCb-PAPER-2014-014] |  LHCb-PAPER-2014-013 [LHCb-PAPER-2014-013] |  LHCb-PAPER-2014-012 [LHCb-PAPER-2014-012] |  LHCb-PAPER-2014-011 [LHCb-PAPER-2014-011]
LHCb-PAPER-2014-010 [LHCb-PAPER-2014-010] |  LHCb-PAPER-2014-009 [LHCb-PAPER-2014-009] |  LHCb-PAPER-2014-008 [LHCb-PAPER-2014-008] |  LHCb-PAPER-2014-007 [LHCb-PAPER-2014-007] |  LHCb-PAPER-2014-006 [LHCb-PAPER-2014-006]
LHCb-PAPER-2014-005 [LHCb-PAPER-2014-005] |  LHCb-PAPER-2014-004 [LHCb-PAPER-2014-004] |  LHCb-PAPER-2014-003 [LHCb-PAPER-2014-003] |  LHCb-PAPER-2014-002 [LHCb-PAPER-2014-002] |  LHCb-PAPER-2014-001 [LHCb-PAPER-2014-001]
LHCb-PAPER-2013-070 [LHCb-PAPER-2013-070] |  LHCb-PAPER-2013-069 [LHCb-PAPER-2013-069] |  LHCb-PAPER-2013-068 [LHCb-PAPER-2013-068] |  LHCb-PAPER-2013-067 [LHCb-PAPER-2013-067] |  LHCb-PAPER-2013-066 [LHCb-PAPER-2013-066]
LHCb-PAPER-2013-065 [LHCb-PAPER-2013-065] |  LHCb-PAPER-2013-064 [LHCb-PAPER-2013-064] |  LHCb-PAPER-2013-063 [LHCb-PAPER-2013-063] |  LHCb-PAPER-2013-062 [LHCb-PAPER-2013-062] |  LHCb-PAPER-2013-061 [LHCb-PAPER-2013-061]
LHCb-PAPER-2013-060 [LHCb-PAPER-2013-060] |  LHCb-PAPER-2013-059 [LHCb-PAPER-2013-059] |  LHCb-PAPER-2013-058 [LHCb-PAPER-2013-058] |  LHCb-PAPER-2013-057 [LHCb-PAPER-2013-057] |  LHCb-PAPER-2013-056 [LHCb-PAPER-2013-056]
LHCb-PAPER-2013-055 [LHCb-PAPER-2013-055] |  LHCb-PAPER-2013-054 [LHCb-PAPER-2013-054] |  LHCb-PAPER-2013-053 [LHCb-PAPER-2013-053] |  LHCb-PAPER-2013-052 [LHCb-PAPER-2013-052] |  LHCb-PAPER-2013-051 [LHCb-PAPER-2013-051]
LHCb-PAPER-2013-050 [LHCb-PAPER-2013-050] |  LHCb-PAPER-2013-049 [LHCb-PAPER-2013-049] |  LHCb-PAPER-2013-048 [LHCb-PAPER-2013-048] |  LHCb-PAPER-2013-047 [LHCb-PAPER-2013-047] |  LHCb-PAPER-2013-046 [LHCb-PAPER-2013-046]
LHCb-PAPER-2013-045 [LHCb-PAPER-2013-045] |  LHCb-PAPER-2013-044 [LHCb-PAPER-2013-044] |  LHCb-PAPER-2013-043 [LHCb-PAPER-2013-043] |  LHCb-PAPER-2013-042 [LHCb-PAPER-2013-042] |  LHCb-PAPER-2013-041 [LHCb-PAPER-2013-041]
LHCb-PAPER-2013-040 [LHCb-PAPER-2013-040] |  LHCb-PAPER-2013-039 [LHCb-PAPER-2013-039] |  LHCb-PAPER-2013-038 [LHCb-PAPER-2013-038] |  LHCb-PAPER-2013-037 [LHCb-PAPER-2013-037] |  LHCb-PAPER-2013-036 [LHCb-PAPER-2013-036]
LHCb-PAPER-2013-035 [LHCb-PAPER-2013-035] |  LHCb-PAPER-2013-034 [LHCb-PAPER-2013-034] |  LHCb-PAPER-2013-033 [LHCb-PAPER-2013-033] |  LHCb-PAPER-2013-032 [LHCb-PAPER-2013-032] |  LHCb-PAPER-2013-031 [LHCb-PAPER-2013-031]
LHCb-PAPER-2013-030 [LHCb-PAPER-2013-030] |  LHCb-PAPER-2013-029 [LHCb-PAPER-2013-029] |  LHCb-PAPER-2013-028 [LHCb-PAPER-2013-028] |  LHCb-PAPER-2013-027 [LHCb-PAPER-2013-027] |  LHCb-PAPER-2013-026 [LHCb-PAPER-2013-026]
LHCb-PAPER-2013-025 [LHCb-PAPER-2013-025] |  LHCb-PAPER-2013-024 [LHCb-PAPER-2013-024] |  LHCb-PAPER-2013-023 [LHCb-PAPER-2013-023] |  LHCb-PAPER-2013-022 [LHCb-PAPER-2013-022] |  LHCb-PAPER-2013-021 [LHCb-PAPER-2013-021]
LHCb-PAPER-2013-020 [LHCb-PAPER-2013-020] |  LHCb-PAPER-2013-019 [LHCb-PAPER-2013-019] |  LHCb-PAPER-2013-018 [LHCb-PAPER-2013-018] |  LHCb-PAPER-2013-017 [LHCb-PAPER-2013-017] |  LHCb-PAPER-2013-016 [LHCb-PAPER-2013-016]
LHCb-PAPER-2013-015 [LHCb-PAPER-2013-015] |  LHCb-PAPER-2013-014 [LHCb-PAPER-2013-014] |  LHCb-PAPER-2013-013 [LHCb-PAPER-2013-013] |  LHCb-PAPER-2013-012 [LHCb-PAPER-2013-012] |  LHCb-PAPER-2013-011 [LHCb-PAPER-2013-011]
LHCb-PAPER-2013-010 [LHCb-PAPER-2013-010] |  LHCb-PAPER-2013-009 [LHCb-PAPER-2013-009] |  LHCb-PAPER-2013-008 [LHCb-PAPER-2013-008] |  LHCb-PAPER-2013-007 [LHCb-PAPER-2013-007] |  LHCb-PAPER-2013-006 [LHCb-PAPER-2013-006]
LHCb-PAPER-2013-005 [LHCb-PAPER-2013-005] |  LHCb-PAPER-2013-004 [LHCb-PAPER-2013-004] |  LHCb-PAPER-2013-003 [LHCb-PAPER-2013-003] |  LHCb-PAPER-2013-002 [LHCb-PAPER-2013-002] |  LHCb-PAPER-2013-001 [LHCb-PAPER-2013-001]
LHCb-PAPER-2012-057 [LHCb-PAPER-2012-057] |  LHCb-PAPER-2012-056 [LHCb-PAPER-2012-056] |  |  |
LHCb-PAPER-2012-055 [LHCb-PAPER-2012-055] |  LHCb-PAPER-2012-054 [LHCb-PAPER-2012-054] |  LHCb-PAPER-2012-053 [LHCb-PAPER-2012-053] |  LHCb-PAPER-2012-052 [LHCb-PAPER-2012-052] |  LHCb-PAPER-2012-051 [LHCb-PAPER-2012-051]
LHCb-PAPER-2012-050 [LHCb-PAPER-2012-050] |  LHCb-PAPER-2012-049 [LHCb-PAPER-2012-049] |  LHCb-PAPER-2012-048 [LHCb-PAPER-2012-048] |  LHCb-PAPER-2012-047 [LHCb-PAPER-2012-047] |  LHCb-PAPER-2012-046 [LHCb-PAPER-2012-046]
LHCb-PAPER-2012-045 [LHCb-PAPER-2012-045] |  LHCb-PAPER-2012-044 [LHCb-PAPER-2012-044] |  LHCb-PAPER-2012-043 [LHCb-PAPER-2012-043] |  LHCb-PAPER-2012-042 [LHCb-PAPER-2012-042] |  LHCb-PAPER-2012-041 [LHCb-PAPER-2012-041]
LHCb-PAPER-2012-040 [LHCb-PAPER-2012-040] |  LHCb-PAPER-2012-039 [LHCb-PAPER-2012-039] |  LHCb-PAPER-2012-038 [LHCb-PAPER-2012-038] |  LHCb-PAPER-2012-037 [LHCb-PAPER-2012-037] |  LHCb-PAPER-2012-036 [LHCb-PAPER-2012-036]
LHCb-PAPER-2012-035 [LHCb-PAPER-2012-035] |  LHCb-PAPER-2012-034 [LHCb-PAPER-2012-034] |  LHCb-PAPER-2012-033 [LHCb-PAPER-2012-033] |  LHCb-PAPER-2012-032 [LHCb-PAPER-2012-032] |  LHCb-PAPER-2012-031 [LHCb-PAPER-2012-031]
LHCb-PAPER-2012-030 [LHCb-PAPER-2012-030] |  LHCb-PAPER-2012-029 [LHCb-PAPER-2012-029] |  LHCb-PAPER-2012-028 [LHCb-PAPER-2012-028] |  LHCb-PAPER-2012-027 [LHCb-PAPER-2012-027] |  LHCb-PAPER-2012-026 [LHCb-PAPER-2012-026]
LHCb-PAPER-2012-025 [LHCb-PAPER-2012-025] |  LHCb-PAPER-2012-024 [LHCb-PAPER-2012-024] |  LHCb-PAPER-2012-023 [LHCb-PAPER-2012-023] |  LHCb-PAPER-2012-022 [LHCb-PAPER-2012-022] |  LHCb-PAPER-2012-021 [LHCb-PAPER-2012-021]
LHCb-PAPER-2012-020 [LHCb-PAPER-2012-020] |  LHCb-PAPER-2012-019 [LHCb-PAPER-2012-019] |  LHCb-PAPER-2012-018 [LHCb-PAPER-2012-018] |  LHCb-PAPER-2012-017 [LHCb-PAPER-2012-017] |  LHCb-PAPER-2012-016 [LHCb-PAPER-2012-016]
LHCb-PAPER-2012-015 [LHCb-PAPER-2012-015] |  LHCb-PAPER-2012-014 [LHCb-PAPER-2012-014] |  LHCb-PAPER-2012-013 [LHCb-PAPER-2012-013] |  LHCb-PAPER-2012-012 [LHCb-PAPER-2012-012] |  LHCb-PAPER-2012-011 [LHCb-PAPER-2012-011]
LHCb-PAPER-2012-010 [LHCb-PAPER-2012-010] |  LHCb-PAPER-2012-009 [LHCb-PAPER-2012-009] |  LHCb-PAPER-2012-008 [LHCb-PAPER-2012-008] |  LHCb-PAPER-2012-007 [LHCb-PAPER-2012-007] |  LHCb-PAPER-2012-006 [LHCb-PAPER-2012-006]
LHCb-PAPER-2012-005 [LHCb-PAPER-2012-005] |  LHCb-PAPER-2012-004 [LHCb-PAPER-2012-004] |  LHCb-PAPER-2012-003 [LHCb-PAPER-2012-003] |  LHCb-PAPER-2012-002 [LHCb-PAPER-2012-002] |  LHCb-PAPER-2012-001 [LHCb-PAPER-2012-001]
LHCb-PAPER-2011-045 [LHCb-PAPER-2011-045] |  LHCb-PAPER-2011-044 [LHCb-PAPER-2011-044] |  LHCb-PAPER-2011-043 [LHCb-PAPER-2011-043] |  LHCb-PAPER-2011-042 [LHCb-PAPER-2011-042] |  LHCb-PAPER-2011-041 [LHCb-PAPER-2011-041]
LHCb-PAPER-2011-040 [LHCb-PAPER-2011-040] | LHCb-PAPER-2011-039999LHCb-PAPER-2011-039 does not exist. |  LHCb-PAPER-2011-038 [LHCb-PAPER-2011-038] |  LHCb-PAPER-2011-037 [LHCb-PAPER-2011-037] |  LHCb-PAPER-2011-036 [LHCb-PAPER-2011-036]
LHCb-PAPER-2011-035 [LHCb-PAPER-2011-035] |  LHCb-PAPER-2011-034 [LHCb-PAPER-2011-034] |  LHCb-PAPER-2011-033 [LHCb-PAPER-2011-033] |  LHCb-PAPER-2011-032 [LHCb-PAPER-2011-032] |  LHCb-PAPER-2011-031 [LHCb-PAPER-2011-031]
LHCb-PAPER-2011-030 [LHCb-PAPER-2011-030] |  LHCb-PAPER-2011-029 [LHCb-PAPER-2011-029] |  LHCb-PAPER-2011-028 [LHCb-PAPER-2011-028] |  LHCb-PAPER-2011-027 [LHCb-PAPER-2011-027] |  LHCb-PAPER-2011-026 [LHCb-PAPER-2011-026]
LHCb-PAPER-2011-025 [LHCb-PAPER-2011-025] |  LHCb-PAPER-2011-024 [LHCb-PAPER-2011-024] |  LHCb-PAPER-2011-023 [LHCb-PAPER-2011-023] |  LHCb-PAPER-2011-022 [LHCb-PAPER-2011-022] |  LHCb-PAPER-2011-021 [LHCb-PAPER-2011-021]
LHCb-PAPER-2011-020 [LHCb-PAPER-2011-020] |  LHCb-PAPER-2011-019 [LHCb-PAPER-2011-019] |  LHCb-PAPER-2011-018 [LHCb-PAPER-2011-018] |  LHCb-PAPER-2011-017 [LHCb-PAPER-2011-017] |  LHCb-PAPER-2011-016 [LHCb-PAPER-2011-016]
LHCb-PAPER-2011-015 [LHCb-PAPER-2011-015] |  LHCb-PAPER-2011-014 [LHCb-PAPER-2011-014] |  LHCb-PAPER-2011-013 [LHCb-PAPER-2011-013] |  LHCb-PAPER-2011-012 [LHCb-PAPER-2011-012] |  LHCb-PAPER-2011-011 [LHCb-PAPER-2011-011]
LHCb-PAPER-2011-010 [LHCb-PAPER-2011-010] |  LHCb-PAPER-2011-009 [LHCb-PAPER-2011-009] |  LHCb-PAPER-2011-008 [LHCb-PAPER-2011-008] |  LHCb-PAPER-2011-007 [LHCb-PAPER-2011-007] |  LHCb-PAPER-2011-006 [LHCb-PAPER-2011-006]
LHCb-PAPER-2011-005 [LHCb-PAPER-2011-005] |  LHCb-PAPER-2011-004 [LHCb-PAPER-2011-004] |  LHCb-PAPER-2011-003 [LHCb-PAPER-2011-003] |  LHCb-PAPER-2011-002 [LHCb-PAPER-2011-002] |  LHCb-PAPER-2011-001 [LHCb-PAPER-2011-001]
LHCb-PAPER-2010-002 [LHCb-PAPER-2010-002] |  LHCb-PAPER-2010-001 [LHCb-PAPER-2010-001] |  |  |
Table 6: LHCb-CONFs (which have their identifier as their cite code). Most CONF notes have been superseded by a paper and are thus retired. This is indicated in the bibtex entry. Do not cite retired CONF notes. DNE: Does not exist.  LHCb-CONF-2021-005 [LHCb-CONF-2021-005] |  LHCb-CONF-2021-004 [LHCb-CONF-2021-004] |  LHCb-CONF-2021-003 [LHCb-CONF-2021-003] |  LHCb-CONF-2021-002 [LHCb-CONF-2021-002] |  LHCb-CONF-2021-001 [LHCb-CONF-2021-001]
---|---|---|---|---
LHCb-CONF-2020-003 [LHCb-CONF-2020-003] |  LHCb-CONF-2020-002 [LHCb-CONF-2020-002] |  LHCb-CONF-2020-001 [LHCb-CONF-2020-001] |  |
LHCb-CONF-2019-005 [LHCb-CONF-2019-005] |  LHCb-CONF-2019-004 [LHCb-CONF-2019-004] |  LHCb-CONF-2019-003 [LHCb-CONF-2019-003] |  LHCb-CONF-2019-002 [LHCb-CONF-2019-002] |  LHCb-CONF-2019-001 [LHCb-CONF-2019-001]
LHCb-CONF-2018-006 [LHCb-CONF-2018-006] |  |  |  |
LHCb-CONF-2018-005 [LHCb-CONF-2018-005] |  LHCb-CONF-2018-004 [LHCb-CONF-2018-004] |  LHCb-CONF-2018-003 [LHCb-CONF-2018-003] |  LHCb-CONF-2018-002 [LHCb-CONF-2018-002]101010If you cite the gamma combination, always also cite the latest gamma paper as \cite{LHCb-PAPER-2013-020,*LHCb-CONF-2018-002} (unless you cite LHCb-PAPER-2013-020 separately too). |  LHCb-CONF-2018-001 [LHCb-CONF-2018-001]
LHCb-CONF-2017-005 [LHCb-CONF-2017-005] |  LHCb-CONF-2017-004 [LHCb-CONF-2017-004] |  LHCb-CONF-2017-003 [LHCb-CONF-2017-003] |  LHCb-CONF-2017-002 [LHCb-CONF-2017-002] |  LHCb-CONF-2017-001 [LHCb-CONF-2017-001]
LHCb-CONF-2016-018 [LHCb-CONF-2016-018] |  LHCb-CONF-2016-016 [LHCb-CONF-2016-016] |  |  |
LHCb-CONF-2016-015 [LHCb-CONF-2016-015] |  LHCb-CONF-2016-014 [LHCb-CONF-2016-014] |  LHCb-CONF-2016-013 [LHCb-CONF-2016-013] |  LHCb-CONF-2016-012 [LHCb-CONF-2016-012] |  LHCb-CONF-2016-011 [LHCb-CONF-2016-011]
LHCb-CONF-2016-010 [LHCb-CONF-2016-010] |  LHCb-CONF-2016-009 [LHCb-CONF-2016-009] |  LHCb-CONF-2016-008 [LHCb-CONF-2016-008] |  LHCb-CONF-2016-007 [LHCb-CONF-2016-007] |  LHCb-CONF-2016-006 [LHCb-CONF-2016-006]
LHCb-CONF-2016-005 [LHCb-CONF-2016-005] |  LHCb-CONF-2016-004 [LHCb-CONF-2016-004] |  LHCb-CONF-2016-003 [LHCb-CONF-2016-003] |  LHCb-CONF-2016-002 [LHCb-CONF-2016-002] |  LHCb-CONF-2016-001 [LHCb-CONF-2016-001]
LHCb-CONF-2015-005 [LHCb-CONF-2015-005] |  LHCb-CONF-2015-004 [LHCb-CONF-2015-004] |  LHCb-CONF-2015-003 [LHCb-CONF-2015-003] |  LHCb-CONF-2015-002 [LHCb-CONF-2015-002] |  LHCb-CONF-2015-001 [LHCb-CONF-2015-001]
LHCb-CONF-2014-004 [LHCb-CONF-2014-004] |  LHCb-CONF-2014-003 [LHCb-CONF-2014-003] |  LHCb-CONF-2014-002 [LHCb-CONF-2014-002] |  LHCb-CONF-2014-001 [LHCb-CONF-2014-001] |
LHCb-CONF-2013-013 [LHCb-CONF-2013-013] |  LHCb-CONF-2013-012 [LHCb-CONF-2013-012] |  LHCb-CONF-2013-011 [LHCb-CONF-2013-011] |  |
LHCb-CONF-2013-010 [LHCb-CONF-2013-010] |  LHCb-CONF-2013-009 [LHCb-CONF-2013-009] |  LHCb-CONF-2013-008 [LHCb-CONF-2013-008] |  LHCb-CONF-2013-007 [LHCb-CONF-2013-007] |  LHCb-CONF-2013-006 [LHCb-CONF-2013-006]
LHCb-CONF-2013-005 [LHCb-CONF-2013-005] |  LHCb-CONF-2013-004 [LHCb-CONF-2013-004] |  LHCb-CONF-2013-003 [LHCb-CONF-2013-003] |  LHCb-CONF-2013-002 [LHCb-CONF-2013-002] |  LHCb-CONF-2013-001 [LHCb-CONF-2013-001]
LHCb-CONF-2012-034 [LHCb-CONF-2012-034] |  LHCb-CONF-2012-033 [LHCb-CONF-2012-033] |  LHCb-CONF-2012-032 [LHCb-CONF-2012-032] |  LHCb-CONF-2012-031 [LHCb-CONF-2012-031] |
LHCb-CONF-2012-030 [LHCb-CONF-2012-030] |  LHCb-CONF-2012-029 [LHCb-CONF-2012-029] |  LHCb-CONF-2012-028 [LHCb-CONF-2012-028] |  LHCb-CONF-2012-027 [LHCb-CONF-2012-027] |  LHCb-CONF-2012-026 [LHCb-CONF-2012-026]
LHCb-CONF-2012-025 [LHCb-CONF-2012-025] |  LHCb-CONF-2012-024 [LHCb-CONF-2012-024] |  LHCb-CONF-2012-023 [LHCb-CONF-2012-023] |  LHCb-CONF-2012-022 [LHCb-CONF-2012-022] |  LHCb-CONF-2012-021 [LHCb-CONF-2012-021]
LHCb-CONF-2012-020 [LHCb-CONF-2012-020] |  LHCb-CONF-2012-019 [LHCb-CONF-2012-019] |  LHCb-CONF-2012-018 [LHCb-CONF-2012-018] |  LHCb-CONF-2012-017 [LHCb-CONF-2012-017] |  LHCb-CONF-2012-016 [LHCb-CONF-2012-016]
LHCb-CONF-2012-015 [LHCb-CONF-2012-015] |  LHCb-CONF-2012-014 [LHCb-CONF-2012-014] |  LHCb-CONF-2012-013 [LHCb-CONF-2012-013] |  LHCb-CONF-2012-012 [LHCb-CONF-2012-012] |  LHCb-CONF-2012-011 [LHCb-CONF-2012-011]
LHCb-CONF-2012-010 [LHCb-CONF-2012-010] |  LHCb-CONF-2012-009 [LHCb-CONF-2012-009] |  LHCb-CONF-2012-008 [LHCb-CONF-2012-008] |  LHCb-CONF-2012-007 [LHCb-CONF-2012-007] |  LHCb-CONF-2012-006 [LHCb-CONF-2012-006]
LHCb-CONF-2012-005 [LHCb-CONF-2012-005] |  LHCb-CONF-2012-004 [LHCb-CONF-2012-004] |  LHCb-CONF-2012-003 [LHCb-CONF-2012-003] |  LHCb-CONF-2012-002 [LHCb-CONF-2012-002] |  LHCb-CONF-2012-001 [LHCb-CONF-2012-001]
LHCb-CONF-2011-062 [LHCb-CONF-2011-062] |  LHCb-CONF-2011-061 [LHCb-CONF-2011-061] |  |  |
LHCb-CONF-2011-060 [LHCb-CONF-2011-060] |  LHCb-CONF-2011-059 [LHCb-CONF-2011-059] |  LHCb-CONF-2011-058 [LHCb-CONF-2011-058] |  LHCb-CONF-2011-057 [LHCb-CONF-2011-057] |  LHCb-CONF-2011-056 [LHCb-CONF-2011-056]
LHCb-CONF-2011-055 [LHCb-CONF-2011-055] |  LHCb-CONF-2011-054 [LHCb-CONF-2011-054] |  LHCb-CONF-2011-053 [LHCb-CONF-2011-053] |  LHCb-CONF-2011-052 [LHCb-CONF-2011-052] |  LHCb-CONF-2011-051 [LHCb-CONF-2011-051]
LHCb-CONF-2011-050 [LHCb-CONF-2011-050] |  LHCb-CONF-2011-049 [LHCb-CONF-2011-049] |  LHCb-CONF-2011-048 [LHCb-CONF-2011-048] |  LHCb-CONF-2011-047 [LHCb-CONF-2011-047] |  LHCb-CONF-2011-046 [LHCb-CONF-2011-046]
LHCb-CONF-2011-045 [LHCb-CONF-2011-045] |  LHCb-CONF-2011-044 [LHCb-CONF-2011-044] |  LHCb-CONF-2011-043 [LHCb-CONF-2011-043] |  LHCb-CONF-2011-042 [LHCb-CONF-2011-042] |  LHCb-CONF-2011-041 [LHCb-CONF-2011-041]
LHCb-CONF-2011-040 [LHCb-CONF-2011-040] |  LHCb-CONF-2011-039 [LHCb-CONF-2011-039] |  LHCb-CONF-2011-038 [LHCb-CONF-2011-038] |  LHCb-CONF-2011-037 [LHCb-CONF-2011-037] |  LHCb-CONF-2011-036 [LHCb-CONF-2011-036]
LHCb-CONF-2011-035 [LHCb-CONF-2011-035] |  LHCb-CONF-2011-034 [LHCb-CONF-2011-034] |  LHCb-CONF-2011-033 [LHCb-CONF-2011-033] |  LHCb-CONF-2011-032 DNE |  LHCb-CONF-2011-031 [LHCb-CONF-2011-031]
LHCb-CONF-2011-030 [LHCb-CONF-2011-030] |  LHCb-CONF-2011-029 [LHCb-CONF-2011-029] |  LHCb-CONF-2011-028 [LHCb-CONF-2011-028] |  LHCb-CONF-2011-027 [LHCb-CONF-2011-027] |  LHCb-CONF-2011-026 [LHCb-CONF-2011-026]
LHCb-CONF-2011-025 [LHCb-CONF-2011-025] |  LHCb-CONF-2011-024 [LHCb-CONF-2011-024] |  LHCb-CONF-2011-023 [LHCb-CONF-2011-023] |  LHCb-CONF-2011-022 [LHCb-CONF-2011-022] |  LHCb-CONF-2011-021 [LHCb-CONF-2011-021]
LHCb-CONF-2011-020 [LHCb-CONF-2011-020] |  LHCb-CONF-2011-019 [LHCb-CONF-2011-019] |  LHCb-CONF-2011-018 [LHCb-CONF-2011-018] |  LHCb-CONF-2011-017 [LHCb-CONF-2011-017] |  LHCb-CONF-2011-016 [LHCb-CONF-2011-016]
LHCb-CONF-2011-015 [LHCb-CONF-2011-015] |  LHCb-CONF-2011-014 [LHCb-CONF-2011-014] |  LHCb-CONF-2011-013 [LHCb-CONF-2011-013] |  LHCb-CONF-2011-012 [LHCb-CONF-2011-012] |  LHCb-CONF-2011-011 [LHCb-CONF-2011-011]
LHCb-CONF-2011-010 [LHCb-CONF-2011-010] |  LHCb-CONF-2011-009 [LHCb-CONF-2011-009] |  LHCb-CONF-2011-008 [LHCb-CONF-2011-008] |  LHCb-CONF-2011-007 [LHCb-CONF-2011-007] |  LHCb-CONF-2011-006 [LHCb-CONF-2011-006]
LHCb-CONF-2011-005 [LHCb-CONF-2011-005] |  LHCb-CONF-2011-004 [LHCb-CONF-2011-004] |  LHCb-CONF-2011-003 [LHCb-CONF-2011-003] |  LHCb-CONF-2011-002 [LHCb-CONF-2011-002] |  LHCb-CONF-2011-001 [LHCb-CONF-2011-001]
LHCb-CONF-2010-014 [LHCb-CONF-2010-014] |  LHCb-CONF-2010-013 [LHCb-CONF-2010-013] |  LHCb-CONF-2010-012 [LHCb-CONF-2010-012] |  LHCb-CONF-2010-011 [LHCb-CONF-2010-011] |
LHCb-CONF-2010-010 [LHCb-CONF-2010-010] |  LHCb-CONF-2010-009 [LHCb-CONF-2010-009] |  LHCb-CONF-2010-008 [LHCb-CONF-2010-008] |  |
Earlier documents in LHCb-CONF series are actually proceedings.

##  Appendix B Standard symbols

As explained in Sect. LABEL:sec:typography this appendix contains standard
typesetting of symbols, particle names, units etc. in LHCb documents.

In the file lhcb-symbols-def.tex, which is included, a large number of symbols
is defined. While they can lead to quicker typing, the main reason is to
ensure a uniform notation within a document and between different LHCb
documents. If a symbol like \CP to typeset $C\\!P$ violation is available for
a unit, particle name, process or whatever, it should be used. If you do not
agree with the notation you should ask to get the definition in lhcb-symbols-
def.tex changed rather than just ignoring it.

All the main particles have been given symbols. The $\mathrm{B}$ mesons are
thus named ${{\mathrm{B}}^{+}}$, ${\mathrm{B}}^{0}$,
${\mathrm{B}}^{0}_{\mathrm{s}}$, and ${\mathrm{B}}_{\mathrm{c}}^{+}$. There is
no need to go into math mode to use particle names, thus saving the typing of
many $ signs. By default particle names are typeset in italic type to agree
with the PDG preference. To get roman particle names you can just change
\setboolean{uprightparticles}{false} to true at the top of this template.

There is a large number of units typeset that ensures the correct use of
fonts, capitals and spacing. As an example we have
${m_{{{\mathrm{B}}^{0}_{\mathrm{s}}}}}=5366.3\pm
0.6\text{\,Me\kern-1.00006ptV\\!/}c^{2}$. Note that $\,\upmu\text{m}$ is
typeset with an upright $\upmu$, even if the particle names have slanted Greek
letters.

A set of useful symbols are defined for working groups. More of these symbols
can be included later. As an example in the Rare Decay group we have several
different analyses looking for a measurement of
$\mathcal{C}_{7}^{{}^{\prime}\mathrm{(eff)}}$ and
$\mathcal{O}_{7.}^{{}^{\prime}}$

##  Appendix C List of all symbols

###  C.1 Experiments

\lhcb | LHCb | \atlas | ATLAS | \cms | CMS
---|---|---|---|---|---
\alice | ALICE | \babar | BaBar | \belle | Belle
\belletwo | Belle II | \besiii | BESIII | \cleo | CLEO
\cdf | CDF | \dzero | D0 | \aleph | ALEPH
\delphi | DELPHI | \opal | OPAL | \lthree | L3
\sld | SLD | \cern | CERN | \lhc | LHC
\lep | LEP | \tevatron | Tevatron | \bfactories | $\mathrm{B}$ Factories
\bfactory | $\mathrm{B}$ Factory | \upgradeone | Upgrade I | \upgradetwo | Upgrade II

####  C.1.1 LHCb sub-detectors and sub-systems

\velo | VELO | \rich | RICH | \richone | RICH1
---|---|---|---|---|---
\richtwo | RICH2 | \ttracker | TT | \intr | IT
\st | ST | \ot | OT | \herschel | HeRSCheL
\spd | SPD | \presh | PS | \ecal | ECAL
\hcal | HCAL | \MagUp | MagUp | \MagDown | MagDown
\ode | ODE | \daq | DAQ | \tfc | TFC
\ecs | ECS | \lone | L0 | \hlt | HLT
\hltone | HLT1 | \hlttwo | HLT2 |  |

###  C.2 Particles

####  C.2.1 Leptons

\electron | $\mathrm{e}$ | \en | $\mathrm{e}^{-}$ | \ep | $\mathrm{e}^{+}$
---|---|---|---|---|---
\epm | $\mathrm{e}^{\pm}$ | \emp | $\mathrm{e}^{\mp}$ | \epem | $\mathrm{e}^{+}\mathrm{e}^{-}$
\muon | $\upmu$ | \mup | $\upmu^{+}$ | \mun | $\upmu^{-}$
\mupm | $\upmu^{\pm}$ | \mump | $\upmu^{\mp}$ | \mumu | $\upmu^{+}\upmu^{-}$
\tauon | $\uptau$ | \taup | $\uptau^{+}$ | \taum | $\uptau^{-}$
\taupm | $\uptau^{\pm}$ | \taump | $\uptau^{\mp}$ | \tautau | $\uptau^{+}\uptau^{-}$
\lepton | $\ell$ | \ellm | $\ell^{-}$ | \ellp | $\ell^{+}$
\ellpm | $\ell^{\pm}$ | \ellmp | $\ell^{\mp}$ | \ellell | $\ell^{+}\ell^{-}$
\neu | $\upnu$ | \neub | $\overline{\upnu}$ | \neue | ${\upnu}_{e}$
\neueb | ${\overline{\upnu}}_{e}$ | \neum | ${\upnu}_{\mu}$ | \neumb | ${\overline{\upnu}}_{\mu}$
\neut | ${\upnu}_{\tau}$ | \neutb | ${\overline{\upnu}}_{\tau}$ | \neul | ${\upnu}_{\ell}$
\neulb | ${\overline{\upnu}}_{\ell}$ |  |  |  |

####  C.2.2 Gauge bosons and scalars

\g | $\upgamma$ | \H | $\mathrm{H}^{0}$ | \Hp | $\mathrm{H}^{+}$
---|---|---|---|---|---
\Hm | $\mathrm{H}^{-}$ | \Hpm | $\mathrm{H}^{\pm}$ | \W | $\mathrm{W}$
\Wp | $\mathrm{W}^{+}$ | \Wm | $\mathrm{W}^{-}$ | \Wpm | $\mathrm{W}^{\pm}$
\Z | $\mathrm{Z}$ |  |  |  |

####  C.2.3 Quarks

\quark | $\mathrm{q}$ | \quarkbar | $\overline{\mathrm{q}}$ | \qqbar | ${\mathrm{q}}{\overline{\mathrm{q}}}$
---|---|---|---|---|---
\uquark | $\mathrm{u}$ | \uquarkbar | $\overline{\mathrm{u}}$ | \uubar | ${\mathrm{u}}{\overline{\mathrm{u}}}$
\dquark | $\mathrm{d}$ | \dquarkbar | $\overline{\mathrm{d}}$ | \ddbar | ${\mathrm{d}}{\overline{\mathrm{d}}}$
\squark | $\mathrm{s}$ | \squarkbar | $\overline{\mathrm{s}}$ | \ssbar | ${\mathrm{s}}{\overline{\mathrm{s}}}$
\cquark | $\mathrm{c}$ | \cquarkbar | $\overline{\mathrm{c}}$ | \ccbar | ${\mathrm{c}}{\overline{\mathrm{c}}}$
\bquark | $\mathrm{b}$ | \bquarkbar | $\overline{\mathrm{b}}$ | \bbbar | ${\mathrm{b}}{\overline{\mathrm{b}}}$
\tquark | $\mathrm{t}$ | \tquarkbar | $\overline{\mathrm{t}}$ | \ttbar | ${\mathrm{t}}{\overline{\mathrm{t}}}$

####  C.2.4 Light mesons

\hadron | $\mathrm{h}$ | \pion | $\uppi$ | \piz | ${\uppi}^{0}$
---|---|---|---|---|---
\pip | ${\uppi}^{+}$ | \pim | ${\uppi}^{-}$ | \pipm | ${\uppi}^{\pm}$
\pimp | ${\uppi}^{\mp}$ | \rhomeson | $\uprho$ | \rhoz | ${\uprho}^{0}$
\rhop | ${\uprho}^{+}$ | \rhom | ${\uprho}^{-}$ | \rhopm | ${\uprho}^{\pm}$
\rhomp | ${\uprho}^{\mp}$ | \kaon | $\mathrm{K}$ | \Kbar | $\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}$
\Kb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}$ | \KorKbar |  ( ) [-.7ex] $\kern 0.0pt\mathrm{K}$ | \Kz | ${\mathrm{K}}^{0}$
\Kzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{0}$ | \Kp | ${\mathrm{K}}^{+}$ | \Km | ${\mathrm{K}}^{-}$
\Kpm | ${\mathrm{K}}^{\pm}$ | \Kmp | ${\mathrm{K}}^{\mp}$ | \KS | ${\mathrm{K}}^{0}_{\mathrm{S}}$
\Vzero | $V^{0}$ | \KL | ${\mathrm{K}}^{0}_{\mathrm{L}}$ | \Kstarz | ${\mathrm{K}}^{*0}$
\Kstarzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*0}$ | \Kstar | ${\mathrm{K}}^{*}$ | \Kstarb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*}$
\Kstarp | ${\mathrm{K}}^{*+}$ | \Kstarm | ${\mathrm{K}}^{*-}$ | \Kstarpm | ${\mathrm{K}}^{*\pm}$
\Kstarmp | ${\mathrm{K}}^{*\mp}$ | \KorKbarz | $\kern 0.0pt\shortstack{{(\rule[2.15277pt]{12.50002pt}{0.51212pt})} \\\ [-.7ex] $\kern 0.0pt\mathrm{K}$}{}^{0}$ | \etaz | $\upeta$
\etapr | $\upeta^{\prime}$ | \phiz | $\upphi$ | \omegaz | $\upomega$

####  C.2.5 Charmed mesons

\Dbar | $\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}$ | \D | $\mathrm{D}$ | \Db | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}$
---|---|---|---|---|---
\DorDbar |  ( ) [-.7ex] $\kern 0.0pt\mathrm{D}$ | \Dz | ${\mathrm{D}}^{0}$ | \Dzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{0}$
\Dp | ${\mathrm{D}}^{+}$ | \Dm | ${\mathrm{D}}^{-}$ | \Dpm | ${\mathrm{D}}^{\pm}$
\Dmp | ${\mathrm{D}}^{\mp}$ | \DpDm | ${{\mathrm{D}}^{+}}{\kern-1.60004pt{{\mathrm{D}}^{-}}}$ | \Dstar | ${\mathrm{D}}^{*}$
\Dstarb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{*}$ | \Dstarz | ${\mathrm{D}}^{*0}$ | \Dstarzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{*0}$
\theDstarz | ${\mathrm{D}}^{*}(2007)^{0}$ | \theDstarzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}^{*}(2007)^{0}$ | \Dstarp | ${\mathrm{D}}^{*+}$
\Dstarm | ${\mathrm{D}}^{*-}$ | \Dstarpm | ${\mathrm{D}}^{*\pm}$ | \Dstarmp | ${\mathrm{D}}^{*\mp}$
\theDstarp | ${\mathrm{D}}^{*}(2010)^{+}$ | \theDstarm | ${\mathrm{D}}^{*}(2010)^{-}$ | \theDstarpm | ${\mathrm{D}}^{*}(2010)^{\pm}$
\theDstarmp | ${\mathrm{D}}^{*}(2010)^{\mp}$ | \Ds | ${\mathrm{D}}^{+}_{\mathrm{s}}$ | \Dsp | ${\mathrm{D}}^{+}_{\mathrm{s}}$
\Dsm | ${\mathrm{D}}^{-}_{\mathrm{s}}$ | \Dspm | ${\mathrm{D}}^{\pm}_{\mathrm{s}}$ | \Dsmp | ${\mathrm{D}}^{\mp}_{\mathrm{s}}$
\Dss | ${\mathrm{D}}^{*+}_{\mathrm{s}}$ | \Dssp | ${\mathrm{D}}^{*+}_{\mathrm{s}}$ | \Dssm | ${\mathrm{D}}^{*-}_{\mathrm{s}}$
\Dsspm | ${\mathrm{D}}^{*\pm}_{\mathrm{s}}$ | \Dssmp | ${\mathrm{D}}^{*\mp}_{\mathrm{s}}$ | \DporDsp | ${\mathrm{D}}_{({\mathrm{s}})}^{+}$
\DmorDsm | ${\mathrm{D}}{}_{({\mathrm{s}})}^{-}$ | \DpmorDspm | ${\mathrm{D}}{}_{({\mathrm{s}})}^{\pm}$ |  |

####  C.2.6 Beauty mesons

\B | $\mathrm{B}$ | \Bbar | $\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}$ | \Bb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}$
---|---|---|---|---|---
\BorBbar |  ( ) [-.7ex] $\kern 0.0pt\mathrm{B}$ | \Bz | ${\mathrm{B}}^{0}$ | \Bzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}$
\Bd | ${\mathrm{B}}^{0}$ | \Bdb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}$ | \BdorBdbar |  ( ) [-.7ex] $\kern 0.0pt{{\mathrm{B}}^{0}}$
\Bu | ${\mathrm{B}}^{+}$ | \Bub | ${\mathrm{B}}^{-}$ | \Bp | ${{\mathrm{B}}^{+}}$
\Bm | ${{\mathrm{B}}^{-}}$ | \Bpm | ${\mathrm{B}}^{\pm}$ | \Bmp | ${\mathrm{B}}^{\mp}$
\Bs | ${\mathrm{B}}^{0}_{\mathrm{s}}$ | \Bsb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}_{\mathrm{s}}$ | \BsorBsbar |  ( ) [-.7ex] $\kern 0.0pt{{\mathrm{B}}^{0}_{\mathrm{s}}}$
\Bc | ${\mathrm{B}}_{\mathrm{c}}^{+}$ | \Bcp | ${\mathrm{B}}_{\mathrm{c}}^{+}$ | \Bcm | ${\mathrm{B}}_{\mathrm{c}}^{-}$
\Bcpm | ${\mathrm{B}}_{\mathrm{c}}^{\pm}$ | \Bds | ${\mathrm{B}}_{({\mathrm{s}})}^{0}$ | \Bdsb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}_{({\mathrm{s}})}^{0}$
\BdorBs | ${\mathrm{B}}_{({\mathrm{s}})}^{0}$ | \BdorBsbar | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}_{({\mathrm{s}})}^{0}$ |  |

####  C.2.7 Onia

\jpsi | ${\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}$ | \psitwos | $\uppsi{(2S)}$ | \psiprpr | $\uppsi(3770)$
---|---|---|---|---|---
\etac | $\upeta_{\mathrm{c}}$ | \psires | $\uppsi$ | \chic | $\upchi_{\mathrm{c}}$
\chiczero | $\upchi_{{\mathrm{c}}0}$ | \chicone | $\upchi_{{\mathrm{c}}1}$ | \chictwo | $\upchi_{{\mathrm{c}}2}$
\chicJ | $\upchi_{{\mathrm{c}}J}$ | \Upsilonres | $\Upsilon$ | \OneS | $\Upsilon{(1S)}$
\TwoS | $\Upsilon{(2S)}$ | \ThreeS | $\Upsilon{(3S)}$ | \FourS | $\Upsilon{(4S)}$
\FiveS | $\Upsilon{(5S)}$ | \chib | $\upchi_{b}$ | \chibzero | $\upchi_{{\mathrm{b}}0}$
\chibone | $\upchi_{{\mathrm{b}}1}$ | \chibtwo | $\upchi_{{\mathrm{b}}2}$ | \chibJ | $\upchi_{{\mathrm{b}}J}$
\theX | $\upchi_{c1}(3872)$ |  |  |  |

####  C.2.8 Light Baryons

\proton | $\mathrm{p}$ | \antiproton | $\overline{\mathrm{p}}$ | \neutron | $\mathrm{n}$
---|---|---|---|---|---
\antineutron | $\overline{\mathrm{n}}$ | \Deltares | $\Delta$ | \Deltaresbar | $\overline{\Delta}$
\Lz | $\Lambda$ | \Lbar | $\kern 0.0pt\overline{\kern 0.0pt\Lambda}$ | \LorLbar |  ( ) [-.7ex] $\kern 0.0pt\Lambda$
\Lambdares | $\Lambda$ | \Lambdaresbar | ${\kern 0.0pt\overline{\kern 0.0pt\Lambda}}$ | \Sigmares | $\Sigma$
\Sigmaz | ${\Sigma}{}^{0}$ | \Sigmap | ${\Sigma}{}^{+}$ | \Sigmam | ${\Sigma}{}^{-}$
\Sigmaresbar | $\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}$ | \Sigmabarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}{}^{0}$ | \Sigmabarp | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}{}^{+}$
\Sigmabarm | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}{}^{-}$ | \Xires | $\Xi$ | \Xiz | ${\Xi}^{0}$
\Xim | ${\Xi}^{-}$ | \Xiresbar | $\kern 0.0pt\overline{\kern 0.0pt{\Xi}}$ | \Xibarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}^{0}$
\Xibarp | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}^{+}$ | \Omegares | $\Omega$ | \Omegaresbar | $\kern 0.0pt\overline{\kern 0.0pt\Omega}$
\Omegam | ${\Omega}^{-}$ | \Omegabarp | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}^{+}$ |  |

####  C.2.9 Charmed Baryons

\Lc | ${\Lambda}^{+}_{\mathrm{c}}$ | \Lcbar | ${\kern 0.0pt\overline{\kern 0.0pt\Lambda}}{}^{-}_{\mathrm{c}}$ | \Xic | ${\Xi}_{\mathrm{c}}$
---|---|---|---|---|---
\Xicz | ${\Xi}^{0}_{\mathrm{c}}$ | \Xicp | ${\Xi}^{+}_{\mathrm{c}}$ | \Xicbar | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{c}}$
\Xicbarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{c}}^{0}$ | \Xicbarm | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{c}}^{-}$ | \Omegac | ${\Omega}^{0}_{\mathrm{c}}$
\Omegacbar | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}{}_{\mathrm{c}}^{0}$ | \Xicc | ${\Xi}_{{\mathrm{c}}{\mathrm{c}}}$ | \Xiccbar | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{{\mathrm{c}}{\mathrm{c}}}$
\Xiccp | ${\Xi}^{+}_{{\mathrm{c}}{\mathrm{c}}}$ | \Xiccpp | ${\Xi}^{++}_{{\mathrm{c}}{\mathrm{c}}}$ | \Xiccbarm | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{{\mathrm{c}}{\mathrm{c}}}^{-}$
\Xiccbarmm | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{{\mathrm{c}}{\mathrm{c}}}^{--}$ | \Omegacc | ${\Omega}^{+}_{{\mathrm{c}}{\mathrm{c}}}$ | \Omegaccbar | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}{}_{{\mathrm{c}}{\mathrm{c}}}^{-}$
\Omegaccc | ${\Omega}^{++}_{{\mathrm{c}}{\mathrm{c}}{\mathrm{c}}}$ | \Omegacccbar | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}{}_{{\mathrm{c}}{\mathrm{c}}{\mathrm{c}}}^{--}$ |  |

####  C.2.10 Beauty Baryons

\Lb | ${\Lambda}^{0}_{\mathrm{b}}$ | \Lbbar | ${\kern 0.0pt\overline{\kern 0.0pt\Lambda}}{}^{0}_{\mathrm{b}}$ | \Sigmab | ${\Sigma}_{\mathrm{b}}$
---|---|---|---|---|---
\Sigmabp | ${\Sigma}_{\mathrm{b}}^{+}$ | \Sigmabz | ${\Sigma}_{\mathrm{b}}^{0}$ | \Sigmabm | ${\Sigma}_{\mathrm{b}}^{-}$
\Sigmabpm | ${\Sigma}_{\mathrm{b}}^{\pm}$ | \Sigmabbar | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}$ | \Sigmabbarp | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}^{+}$
\Sigmabbarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}^{0}$ | \Sigmabbarm | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}^{-}$ | \Sigmabbarpm | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}^{-}$
\Xib | ${\Xi}_{\mathrm{b}}$ | \Xibz | ${\Xi}^{0}_{\mathrm{b}}$ | \Xibm | ${\Xi}^{-}_{\mathrm{b}}$
\Xibbar | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{b}}$ | \Xibbarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{b}}^{0}$ | \Xibbarp | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{b}}^{+}$
\Omegab | ${\Omega}^{-}_{\mathrm{b}}$ | \Omegabbar | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}{}_{\mathrm{b}}^{+}$ |  |

###  C.3 Physics symbols

####  C.3.1 Decays

\BF | $\mathcal{B}$ | \BR | $\mathcal{B}$ | \BRvis | ${\mathcal{B}}_{\mathrm{{vis}}}$
---|---|---|---|---|---
\ra | $\rightarrow$ | \to | $\rightarrow$ |  |

####  C.3.2 Lifetimes

\tauBs | $\tau_{{{\mathrm{B}}^{0}_{\mathrm{s}}}}$ | \tauBd | $\tau_{{{\mathrm{B}}^{0}}}$ | \tauBz | $\tau_{{{\mathrm{B}}^{0}}}$
---|---|---|---|---|---
\tauBu | $\tau_{{{{\mathrm{B}}^{+}}}}$ | \tauDp | $\tau_{{{\mathrm{D}}^{+}}}$ | \tauDz | $\tau_{{{\mathrm{D}}^{0}}}$
\tauL | $\tau_{\mathrm{L}}$ | \tauH | $\tau_{\mathrm{H}}$ |  |

####  C.3.3 Masses

\mBd | $m_{{{\mathrm{B}}^{0}}}$ | \mBp | $m_{{{{\mathrm{B}}^{+}}}}$ | \mBs | $m_{{{\mathrm{B}}^{0}_{\mathrm{s}}}}$
---|---|---|---|---|---
\mBc | $m_{{{\mathrm{B}}_{\mathrm{c}}^{+}}}$ | \mLb | $m_{{{\Lambda}^{0}_{\mathrm{b}}}}$ |  |

####  C.3.4 EW theory, groups

\grpsuthree | $\mathrm{SU}(3)$ | \grpsutw | $\mathrm{SU}(2)$ | \grpuone | $\mathrm{U}(1)$
---|---|---|---|---|---
\ssqtw | $\sin^{2}\\!\theta_{\mathrm{W}}$ | \csqtw | $\cos^{2}\\!\theta_{\mathrm{W}}$ | \stw | $\sin\theta_{\mathrm{W}}$
\ctw | $\cos\theta_{\mathrm{W}}$ | \ssqtwef | ${\sin}^{2}\theta_{\mathrm{W}}^{\mathrm{eff}}$ | \csqtwef | ${\cos}^{2}\theta_{\mathrm{W}}^{\mathrm{eff}}$
\stwef | $\sin\theta_{\mathrm{W}}^{\mathrm{eff}}$ | \ctwef | $\cos\theta_{\mathrm{W}}^{\mathrm{eff}}$ | \gv | $g_{\mbox{\tiny V}}$
\ga | $g_{\mbox{\tiny A}}$ | \order | $\mathcal{O}$ | \ordalph | $\mathcal{O}(\alpha)$
\ordalsq | $\mathcal{O}(\alpha^{2})$ | \ordalcb | $\mathcal{O}(\alpha^{3})$ |  |

####  C.3.5 QCD parameters

\as | $\alpha_{s}$ | \MSb | $\overline{\mathrm{MS}}$ | \lqcd | $\Lambda_{\mathrm{QCD}}$
---|---|---|---|---|---
\qsq | $q^{2}$ |  |  |  |

####  C.3.6 CKM, $C\\!P$ violation

\eps | $\varepsilon$ | \epsK | $\varepsilon_{K}$ | \epsB | $\varepsilon_{B}$
---|---|---|---|---|---
\epsp | $\varepsilon^{\prime}_{K}$ | \CP | $C\\!P$ | \CPT | $C\\!PT$
\T | $T$ | \rhobar | $\overline{\rho}$ | \etabar | $\overline{\eta}$
\Vud | $V_{{\mathrm{u}}{\mathrm{d}}}^{\phantom{\ast}}$ | \Vcd | $V_{{\mathrm{c}}{\mathrm{d}}}^{\phantom{\ast}}$ | \Vtd | $V_{{\mathrm{t}}{\mathrm{d}}}^{\phantom{\ast}}$
\Vus | $V_{{\mathrm{u}}{\mathrm{s}}}^{\phantom{\ast}}$ | \Vcs | $V_{{\mathrm{c}}{\mathrm{s}}}^{\phantom{\ast}}$ | \Vts | $V_{{\mathrm{t}}{\mathrm{s}}}^{\phantom{\ast}}$
\Vub | $V_{{\mathrm{u}}{\mathrm{b}}}^{\phantom{\ast}}$ | \Vcb | $V_{{\mathrm{c}}{\mathrm{b}}}^{\phantom{\ast}}$ | \Vtb | $V_{{\mathrm{t}}{\mathrm{b}}}^{\phantom{\ast}}$
\Vuds | $V_{{\mathrm{u}}{\mathrm{d}}}^{\ast}$ | \Vcds | $V_{{\mathrm{c}}{\mathrm{d}}}^{\ast}$ | \Vtds | $V_{{\mathrm{t}}{\mathrm{d}}}^{\ast}$
\Vuss | $V_{{\mathrm{u}}{\mathrm{s}}}^{\ast}$ | \Vcss | $V_{{\mathrm{c}}{\mathrm{s}}}^{\ast}$ | \Vtss | $V_{{\mathrm{t}}{\mathrm{s}}}^{\ast}$
\Vubs | $V_{{\mathrm{u}}{\mathrm{b}}}^{\ast}$ | \Vcbs | $V_{{\mathrm{c}}{\mathrm{b}}}^{\ast}$ | \Vtbs | $V_{{\mathrm{t}}{\mathrm{b}}}^{\ast}$

####  C.3.7 Oscillations

\dm | $\Delta m$ | \dms | $\Delta m_{{\mathrm{s}}}$ | \dmd | $\Delta m_{{\mathrm{d}}}$
---|---|---|---|---|---
\DG | $\Delta\Gamma$ | \DGs | $\Delta\Gamma_{{\mathrm{s}}}$ | \DGd | $\Delta\Gamma_{{\mathrm{d}}}$
\Gs | $\Gamma_{{\mathrm{s}}}$ | \Gd | $\Gamma_{{\mathrm{d}}}$ | \MBq | $M_{{\mathrm{B}}_{\mathrm{q}}}$
\DGq | $\Delta\Gamma_{{\mathrm{q}}}$ | \Gq | $\Gamma_{{\mathrm{q}}}$ | \dmq | $\Delta m_{{\mathrm{q}}}$
\GL | $\Gamma_{\mathrm{L}}$ | \GH | $\Gamma_{\mathrm{H}}$ | \DGsGs | $\Delta\Gamma_{{\mathrm{s}}}/\Gamma_{{\mathrm{s}}}$
\Delm | $\Delta m$ | \ACP | ${\mathcal{A}}^{{C\\!P}}$ | \Adir | ${\mathcal{A}}^{\mathrm{dir}}$
\Amix | ${\mathcal{A}}^{\mathrm{mix}}$ | \ADelta | ${\mathcal{A}}^{\Delta}$ | \phid | $\phi_{{\mathrm{d}}}$
\sinphid | $\sin\\!{\phi_{{\mathrm{d}}}}$ | \phis | $\phi_{{\mathrm{s}}}$ | \betas | $\beta_{{\mathrm{s}}}$
\sbetas | $\sigma(\beta_{{\mathrm{s}}})$ | \stbetas | $\sigma(2\beta_{{\mathrm{s}}})$ | \stphis | $\sigma(\phi_{{\mathrm{s}}})$
\sinphis | $\sin\\!{\phi_{{\mathrm{s}}}}$ |  |  |  |

####  C.3.8 Tagging

\edet | $\varepsilon_{\mathrm{det}}$ | \erec | $\varepsilon_{\mathrm{rec/det}}$ | \esel | $\varepsilon_{\mathrm{sel/rec}}$
---|---|---|---|---|---
\etrg | $\varepsilon_{\mathrm{trg/sel}}$ | \etot | $\varepsilon_{\mathrm{tot}}$ | \mistag | $\omega$
\wcomb | $\omega^{\mathrm{comb}}$ | \etag | $\varepsilon_{\mathrm{tag}}$ | \etagcomb | $\varepsilon_{\mathrm{tag}}^{\mathrm{comb}}$
\effeff | $\varepsilon_{\mathrm{eff}}$ | \effeffcomb | $\varepsilon_{\mathrm{eff}}^{\mathrm{comb}}$ | \efftag | ${\varepsilon_{\mathrm{tag}}}(1-2\omega)^{2}$
\effD | ${\varepsilon_{\mathrm{tag}}}D^{2}$ | \etagprompt | $\varepsilon_{\mathrm{tag}}^{\mathrm{Pr}}$ | \etagLL | $\varepsilon_{\mathrm{tag}}^{\mathrm{LL}}$

####  C.3.9 Key decay channels

\BdToKstmm | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{K}}^{*0}}{\upmu^{+}}{\upmu^{-}}$ | \BdbToKstmm | ${{\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}}\\!\rightarrow{{\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*0}}{\upmu^{+}}{\upmu^{-}}$ | \BsToJPsiPhi | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}\phi$
---|---|---|---|---|---
\BdToJPsiKst | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}{{\mathrm{K}}^{*0}}$ | \BdbToJPsiKst | ${{\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}}\\!\rightarrow{{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}{{\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*0}}$ | \BsPhiGam | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow\phi{\upgamma}$
\BdKstGam | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{K}}^{*0}}{\upgamma}$ | \BTohh | ${\mathrm{B}}\\!\rightarrow\mathrm{h}^{+}\mathrm{h}^{\prime-}$ | \BdTopipi | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\uppi}^{+}}{{\uppi}^{-}}$
\BdToKpi | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{K}}^{+}}{{\uppi}^{-}}$ | \BsToKK | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{{\mathrm{K}}^{+}}{{\mathrm{K}}^{-}}$ | \BsTopiK | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{{\uppi}^{+}}{{\mathrm{K}}^{-}}$
\Cpipi | $C_{{{\uppi}^{+}}{{\uppi}^{-}}}$ | \Spipi | $S_{{{\uppi}^{+}}{{\uppi}^{-}}}$ | \CKK | $C_{{{\mathrm{K}}^{+}}{{\mathrm{K}}^{-}}}$
\SKK | $S_{{{\mathrm{K}}^{+}}{{\mathrm{K}}^{-}}}$ | \ADGKK | $A^{{\Delta\Gamma}}_{{{\mathrm{K}}^{+}}{{\mathrm{K}}^{-}}}$ |  |

####  C.3.10 Rare decays

\BdKstee | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{K}}^{*0}}{\mathrm{e}^{+}\mathrm{e}^{-}}$ | \BdbKstee | ${{\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}}\\!\rightarrow{{\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*0}}{\mathrm{e}^{+}\mathrm{e}^{-}}$ | \bsll | ${\mathrm{b}}\\!\rightarrow{\mathrm{s}}\ell^{+}\ell^{-}$
---|---|---|---|---|---
\AFB | $A_{\mathrm{FB}}$ | \FL | $F_{\mathrm{L}}$ | \AT#1 \AT2 | $A_{\mathrm{T}}^{2}$
\btosgam | ${\mathrm{b}}\\!\rightarrow{\mathrm{s}}{\upgamma}$ | \btodgam | ${\mathrm{b}}\\!\rightarrow{\mathrm{d}}{\upgamma}$ | \Bsmm | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{\upmu^{+}}{\upmu^{-}}$
\Bdmm | ${{\mathrm{B}}^{0}}\\!\rightarrow{\upmu^{+}}{\upmu^{-}}$ | \Bsee | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{\mathrm{e}^{+}\mathrm{e}^{-}}$ | \Bdee | ${{\mathrm{B}}^{0}}\\!\rightarrow{\mathrm{e}^{+}\mathrm{e}^{-}}$
\ctl | $\cos{\theta_{\ell}}$ | \ctk | $\cos{\theta_{K}}$ |  |

####  C.3.11 Wilson coefficients and operators

\C#1 \C9 | $\mathcal{C}_{9}$ | \Cp#1 \Cp7 | $\mathcal{C}_{7}^{{}^{\prime}}$ | \Ceff#1 \Ceff9 | $\mathcal{C}_{9}^{\mathrm{(eff)}}$
---|---|---|---|---|---
\Cpeff#1 \Cpeff7 | $\mathcal{C}_{7}^{{}^{\prime}\mathrm{(eff)}}$ | \Ope#1 \Ope2 | $\mathcal{O}_{2}$ | \Opep#1 \Opep7 | $\mathcal{O}_{7}^{{}^{\prime}}$

####  C.3.12 Charm

\xprime | $x^{\prime}$ | \yprime | $y^{\prime}$ | \ycp | $y_{{C\\!P}}$
---|---|---|---|---|---
\agamma | $A_{\Gamma}$ | \dkpicf | ${{\mathrm{D}}^{0}}\\!\rightarrow{{\mathrm{K}}^{-}}{{\uppi}^{+}}$ |  |

####  C.3.13 QM

\bra[1] \bra{a} | $\langle a|$ | \ket[1] \ket{b} | $|b\rangle$ | \braket[2] \braket{a}{b} | $\langle a|b\rangle$
---|---|---|---|---|---

###  C.4 Units (these macros add a small space in front)

\unit[1] \unit{kg} |  kg
---|---

####  C.4.1 Energy and momentum

\tev |  TeV | \gev |  GeV | \mev |  MeV
---|---|---|---|---|---
\kev |  keV | \ev |  eV | \gevgev | $\text{\,Ge\kern-1.00006ptV}^{2}$
\mevc | $\text{\,Me\kern-1.00006ptV\\!/}c$ | \gevc | $\text{\,Ge\kern-1.00006ptV\\!/}c$ | \mevcc | $\text{\,Me\kern-1.00006ptV\\!/}c^{2}$
\gevcc | $\text{\,Ge\kern-1.00006ptV\\!/}c^{2}$ | \gevgevcc | $\text{\,Ge\kern-1.00006ptV}^{2}\\!/c^{2}$ | \gevgevcccc | $\text{\,Ge\kern-1.00006ptV}^{2}\\!/c^{4}$

####  C.4.2 Distance and area (these macros add a small space)

\km |  km | \m |  m | \ma | $\text{\,m}^{2}$
---|---|---|---|---|---
\cm |  cm | \cma | $\text{\,cm}^{2}$ | \mm |  mm
\mma | $\text{\,mm}^{2}$ | \mum | $\,\upmu\text{m}$ | \muma | $\,\upmu\text{m}^{2}$
\nm |  nm | \fm |  fm | \barn |  b
\mbarn |  mb | \mub | $\,\upmu\text{b}$ | \nb |  nb
\invnb | $\text{\,nb}^{-1}$ | \pb |  pb | \invpb | $\text{\,pb}^{-1}$
\fb |  fb | \invfb | $\text{\,fb}^{-1}$ | \ab |  ab
\invab | $\text{\,ab}^{-1}$ |  |  |  |

####  C.4.3 Time

\sec |  s | \ms |  ms | \mus | $\,\upmu\text{s}$
---|---|---|---|---|---
\ns |  ns | \ps |  ps | \fs |  fs
\mhz |  MHz | \khz |  kHz | \hz |  Hz
\invps | $\text{\,ps}^{-1}$ | \invns | $\text{\,ns}^{-1}$ | \yr |  yr
\hr |  hr |  |  |  |

####  C.4.4 Temperature

\degc |  ∘C | \degk |  K
---|---|---|---

####  C.4.5 Material lengths, radiation

\Xrad | $X_{0}$ | \NIL | $\lambda_{\rm int}$ | \mip | MIP
---|---|---|---|---|---
\neutroneq | $n_{\text{eq}}$ | \neqcmcm | $n_{\text{eq}}/\text{cm}^{2}$ | \kRad |  kRad
\MRad |  MRad | \ci |  Ci | \mci |  mCi

####  C.4.6 Uncertainties

\sx | $\sigma_{x}$ | \sy | $\sigma_{y}$ | \sz | $\sigma_{z}$
---|---|---|---|---|---
\stat |  (stat) | \syst |  (syst) | \lumi |  (lumi)

####  C.4.7 Maths

\order | $\mathcal{O}$ | \chisq | $\chi^{2}$ | \chisqndf | $\chi^{2}/\mathrm{ndf}$
---|---|---|---|---|---
\chisqip | $\chi^{2}_{\text{IP}}$ | \chisqvs | $\chi^{2}_{\text{VS}}$ | \chisqvtx | $\chi^{2}_{\text{vtx}}$
\chisqvtxndf | $\chi^{2}_{\text{vtx}}/\mathrm{ndf}$ | \chisqfd | $\chi^{2}_{\text{FD}}$ | \gsim |  $>$$\sim$
\lsim |  $<$$\sim$ | \mean[1] \mean{x} | $\left\langle x\right\rangle$ | \abs[1] \abs{x} | $\left\|x\right\|$
\Real | $\mathcal{R}e$ | \Imag | $\mathcal{I}m$ | \PDF | PDF
\sPlot | sPlot | \sFit | sFit | \deriv | $\mathrm{d}$

###  C.5 Kinematics

####  C.5.1 Energy, Momenta

\Ebeam | $E_{\mbox{\tiny BEAM}}$ | \sqs | $\sqrt{s}$ | \sqsnn | $\sqrt{s_{\scriptscriptstyle\text{NN}}}$
---|---|---|---|---|---
\pt | $p_{\mathrm{T}}$ | \ptsq | $p_{\mathrm{T}}^{2}$ | \ptot | $p$
\et | $E_{\mathrm{T}}$ | \mt | $M_{\mathrm{T}}$ | \dpp | $\Delta p/p$
\msq | $m^{2}$ | \dedx | $\mathrm{d}E/\mathrm{d}x$ |  |

####  C.5.2 PID

\dllkpi | $\mathrm{DLL}_{{\mathrm{K}}{\uppi}}$ | \dllppi | $\mathrm{DLL}_{{\mathrm{p}}{\uppi}}$ | \dllepi | $\mathrm{DLL}_{{\mathrm{e}}{\uppi}}$
---|---|---|---|---|---
\dllmupi | $\mathrm{DLL}_{{\upmu}\pi}$ |  |  |  |

####  C.5.3 Geometry

\degrees | ∘ | \murad | $\,\upmu\text{rad}$ | \mrad |  mrad
---|---|---|---|---|---
\rad |  rad |  |  |  |

####  C.5.4 Accelerator

\betastar | $\beta^{*}$ | \lum | $\mathcal{L}$ | \intlum[1] \intlum{2 $\text{\,fb}^{-1}$ } | $\int\mathcal{L}=2\,\text{\,fb}^{-1}$
---|---|---|---|---|---

###  C.6 Software

####  C.6.1 Programs

\bcvegpy | Bcvegpy | \boole | Boole | \brunel | Brunel
---|---|---|---|---|---
\davinci | DaVinci | \dirac | Dirac | \evtgen | EvtGen
\fewz | Fewz | \fluka | Fluka | \ganga | Ganga
\gaudi | Gaudi | \gauss | Gauss | \geant | Geant4
\hepmc | HepMC | \herwig | Herwig | \moore | Moore
\neurobayes | NeuroBayes | \photos | Photos | \powheg | Powheg
\pythia | Pythia | \resbos | ResBos | \roofit | RooFit
\root | Root | \spice | Spice | \tensorflow | TensorFlow
\urania | Urania |  |  |  |

####  C.6.2 Languages

\cpp | C++ | \ruby | Ruby | \fortran | Fortran
---|---|---|---|---|---
\svn | svn | \git | git | \latex | LaTeX

####  C.6.3 Data processing

\kbit |  kbit | \kbps |  kbit/s | \kbytes |  kB
---|---|---|---|---|---
\kbyps |  kB/s | \mbit |  Mbit | \mbps |  Mbit/s
\mbytes |  MB | \mbyps |  MB/s | \gbit |  Gbit
\gbps |  Gbit/s | \gbytes |  GB | \gbyps |  GB/s
\tbit |  Tbit | \tbps |  Tbit/s | \tbytes |  TB
\tbyps |  TB/s | \dst | DST |  |

###  C.7 Detector related

####  C.7.1 Detector technologies

\nonn | $\mathrm{{\mathit{n^{+}}}\mbox{-}on\mbox{-}{\mathit{n}}}$ | \ponn | $\mathrm{{\mathit{p^{+}}}\mbox{-}on\mbox{-}{\mathit{n}}}$ | \nonp | $\mathrm{{\mathit{n^{+}}}\mbox{-}on\mbox{-}{\mathit{p}}}$
---|---|---|---|---|---
\cvd | CVD | \mwpc | MWPC | \gem | GEM

####  C.7.2 Detector components, electronics

\tell1 | TELL1 | \ukl1 | UKL1 | \beetle | Beetle
---|---|---|---|---|---
\otis | OTIS | \croc | CROC | \carioca | CARIOCA
\dialog | DIALOG | \sync | SYNC | \cardiac | CARDIAC
\gol | GOL | \vcsel | VCSEL | \ttc | TTC
\ttcrx | TTCrx | \hpd | HPD | \pmt | PMT
\specs | SPECS | \elmb | ELMB | \fpga | FPGA
\plc | PLC | \rasnik | RASNIK | \elmb | ELMB
\can | CAN | \lvds | LVDS | \ntc | NTC
\adc | ADC | \led | LED | \ccd | CCD
\hv | HV | \lv | LV | \pvss | PVSS
\cmos | CMOS | \fifo | FIFO | \ccpc | CCPC

####  C.7.3 Chemical symbols

\cfourften | $\mathrm{C_{4}F_{10}}$ | \cffour | $\mathrm{CF_{4}}$ | \cotwo | $\mathrm{CO_{2}}$
---|---|---|---|---|---
\csixffouteen | $\mathrm{C_{6}F_{14}}$ | \mgftwo | $\mathrm{MgF_{2}}$ | \siotwo | $\mathrm{SiO_{2}}$

###  C.8 Special Text

\eg | e.g. | \ie | i.e. | \etal | et al.
---|---|---|---|---|---
\etc | etc. | \cf | cf. | \ffp | ff.
\vs | vs. |  |  |  |

####  C.8.1 Helpful to align numbers in tables

\phz |
---|---

The author list for journal publications is generated from the Membership
Database shortly after ’approval to go to paper’ has been given. It will be
sent to you by email shortly after a paper number has been assigned. The
author list should be included in the draft used for first and second
circulation, to allow new members of the collaboration to verify that they
have been included correctly. Occasionally a misspelled name is corrected, or
associated institutions become full members. Therefore an updated author list
will be sent to you after the final EB review of the paper. In case line
numbering doesn’t work well after including the authorlist, try moving the
`\bigskip` after the last author to a separate line.

The authorship for Conference Reports should be “The LHCb collaboration”, with
a footnote giving the name(s) of the contact author(s), but without the full
list of collaboration names.

The authorship for Figure Reports should be “The LHCb collaboration”, with no
contact author and without the full list of collaboration names.