Supersonic Deflagrations in Cosmological Phase Transitions

Details Supersonic Deflagrations in Cosmological Phase Transitions Supersonic Deflagrations in Cosmological Phase Transitions

1995-01-05

arxiv.org/abs/hep-ph/9501216v1

Phys.Rev. D51 (1995) 5431-5437

Physics

High Energy Physics

High Energy Physics - Phenomenology

8 pages, RevTeX, 6 figures. Complete paper appended as uuencoded postscript and at http://www.physics.helsinki.fi/tft/tft_prep

Scientific paper

10.1103/PhysRevD.51.5431

The classification of the hydrodynamical growth mechanisms for the spherical bubbles of the low-temperature phase in cosmological phase transitions is completed by showing that the bubbles can grow as supersonic deflagrations. Such deflagrations consist of a Jouguet deflagration, followed by a rarefaction wave. Depending on the amount of supercooling, the maximal velocity of supersonic deflagrations varies between the sound and the light velocities. The solutions faster than supersonic deflagrations are weak detonations.

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