arXiv (All)
open access
How particle physics stops ultra-relativistic bubbles and shapes their gravitational waves
cosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-physics-phenomenology
The gravitational-wave spectrum produced by ultra-relativistic bubbles in a first-order cosmological phase transition can be approximated in terms of their energy density as a function of bubble size. Bubble collisions and post-collision classical evolution negligibly change it. The dominant energy
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