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Vorticity, Kinetic Energy, and Suppressed Gravitational-Wave Production in Strong First-Order Phase Transitions
Daniel Cutting1,2, Mark Hindmarsh1,2, David J Weir2,3
1Department of Physics and Astronomy, University of Sussex, Falmer, Brighton BN1 9QH, United Kingdom.
Simulations reveal that strong early universe phase transitions generate less gravitational waves than predicted. This is due to kinetic energy loss, particularly in deflagrations, impacting cosmic models.
Area of Science:
- Cosmology
- Early Universe Physics
- Phase Transitions
Background:
- First-order thermal phase transitions are crucial for early universe evolution.
- Previous models often simplified these transitions, potentially overestimating observable signals.
Purpose of the Study:
- To perform the first 3D simulations of strong first-order thermal phase transitions.
- To investigate the fluid velocity, kinetic energy transfer, and gravitational wave generation during these events.
Main Methods:
- Three-dimensional hydrodynamic simulations were conducted.
- The simulations focused on varying transition strengths for both deflagrations and detonations.
Main Results:
- For deflagrations, fluid velocity increased with transition strength; detonations showed constant, low velocity.
- Kinetic energy transfer efficiency decreased with increasing transition strength.
- Gravitational wave energy density for deflagrations was suppressed, with models overestimating signals by up to 10^3.
Conclusions:
- Current models significantly overestimate gravitational wave signals from strong deflagration transitions.
- The kinetic energy deficit, caused by reheated droplets, is a key factor in this discrepancy.
- Detonations are less affected by these strong transition effects.
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