3D simulations in an expanding background show cosmic expansion drives nonlinear growth that amplifies gravitational-wave spectra from slow phase transitions by factors of 10 to 100.
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Nonlinear growth and amplification of phase-transition gravitational waves induced by cosmic expansion
3D simulations in an expanding background show cosmic expansion drives nonlinear growth that amplifies gravitational-wave spectra from slow phase transitions by factors of 10 to 100.
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Phase Transitions and Gravitational Wave Production at the End of Thermal Inflation
Lattice simulations of the first-order phase transition terminating thermal inflation confirm bubble nucleation and yield gravitational-wave spectra potentially detectable by BBO and DECIGO.