Energy budget of cosmological first-order phase transition in FLRW background
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摘要:
We study the hydrodynamics of bubble expansion in cosmological first-order phase transition in the Friedmann-Lema(i)tre-Robertson-Walker (FLRW) background with probe limit.Different from previous studies for fast first-order phase transition in flat background,we find that,for slow first-order phase transition in FLRW background with a given peculiar velocity of the bubble wall,the efficiency factor of energy transfer into bulk motion of thermal fluid is significantly reduced,thus decreasing the previously-thought dominated contribution from sound wave to the stochastic gravitational-wave background.