Even when the central flow is boost invariant, large-rapidity deviations can slow the acoustic horizon's recession, giving finite redshift Hawking radiation that may affect momentum distributions.
Again, from allowed values ( η′ h, τ′ h), and corresponding ( t′ h, z′ h), we choose values for which |∆t′ obs| is lowest
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Doppler shifted Hawking radiation from acoustic black holes in ultra-relativistic heavy-ion collisions
Even when the central flow is boost invariant, large-rapidity deviations can slow the acoustic horizon's recession, giving finite redshift Hawking radiation that may affect momentum distributions.