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.
Note that, the fluid is moving with respect to the observer’s new location with vobs = tanh( Y ′ 0 − Y0)
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
hep-ph 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.