hunt for beyond standard model (BSM) physics is the presence of non-baryonic form of matter, or the so called dark matter (DM) in large amount in the present universe. Apart from the longstanding astrophysical evidences [@Zwicky:1933gu; @Rubin:1970zza; @Clowe:2006eq], the recent cosmology experiment Planck suggests that almost $26\%$ of the present Universe’s energy density is in the form of DM while only around $5\%$ is the usual baryonic matter leading the rest of the energy budget to mysterious dark energy [@Aghanim:2018eyx]. In terms of density parameter $\Omega_{\rm DM}$ and $h = \text{Hubble Parameter}/(100 \;\text{km} ~\text{s}^{-1} 
\text{Mpc}^{-1})$, the present DM abundance is conventionally reported as [@Aghanim:2018eyx]: $\Omega_{\text{DM}} h^2 = 0.120\pm 0.001$ at 68% CL. Since none of the SM particles can satisfy the requirements for being a DM candidate, several BSM proposals have been put forward out of which the weakly interacting massive particle (WIMP) paradigm is perhaps the most popular or the most widely studied one. The coincidence that a stable or cosmologically long lived particle having electroweak scale mass and interactions fulfilling the criteria for observed DM abundance is often referred to as the *WIMP Miracle*. However, if such particles having electroweak scale mass and interactions really exist in the 