position in the net baryon distribution.

![The space-time rapidity dependence of the difference between the flow and the space-time rapidities at the initial time (thin solid line) and those after ideal (thick solid line), baryon diffusive (dashed line), and energy dissipative (dotted line) hydrodynamic evolutions at $\tau = 20$ fm/$c$.[]{data-label="fig:2"}](flow.pdf){width="3.3in"}

Charged particle and net baryon rapidity distributions
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The charged hadron rapidity distributions are shown in Fig. \[fig:3\]. The effect of energy dissipation in the Eckart frame is visible while that of baryon diffusion is negligible when the off-equilibrium correction at freeze-out (\[eq:CF\]) is not taken into account. The difference comes from the difference in the Landau and the Eckart flow and the lack of the $\delta f$ corrections. When the correction is incorporated, the effect of energy dissipation becomes small and similar to that of baryon diffusion as found in Fig. \[fig:3\] (b).

![The rapidity distributions of charged particles (a) without and (b) with $\delta f$ correction at freeze-out for the ideal hydrodynamic system (solid line) compared to those for the systems with baryon diffusion in the Landau frame (dashed line) and with energy dissipation in the Eckart frame (dotted line).[]{data-label="fig:3"}](dnchdy.pdf "fig:"){width="3.3in"} ![The rapidity distributions of charged particles (a) 