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2012

Gravitational Radiation from First-Order Phase Transitions

Child, Hillary L., Giblin Jr, John T.

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It is believed that first-order phase transitions at or around the GUT scale will produce high-frequency gravitational radiation.

This radiation is a consequence of the collisions and coalescence of multiple bubbles during the transition.
We employ high-resolution lattice simulations to numerically evolve a system of bubbles using only scalar fields, track the anisotropic stress during the process and evolve the metric perturbations associated with gravitational radiation.
Although the radiation produced during the bubble collisions has previously been estimated, we find that the coalescence phase enhances this radiation even in the absence of a coupled fluid or turbulence.

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