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Updated: Jul 3, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Gravitational radiation from primordial helical magnetohydrodynamic turbulence
Tina Kahniashvili1, Grigol Gogoberidze, Bharat Ratra
1CCPP, New York University, 4 Washington Plaza, New York, NY 10003, USA.
Abstract:
We consider gravitational waves (GWs) generated by primordial inverse-cascade helical magneto-hydrodynamical (MHD) turbulence produced by bubble collisions at the electroweak phase transitions (EWPT). Compared to the unmagnetized EWPT case, the spectrum of MHD-turbulence-generated GWs peaks at lower frequency with larger amplitude and can be detected by the proposed Laser Interferometer Space Antenna.
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