Chiral plasma instability and primordial Gravitational wave
arXiv:1801.00650 · doi:10.1140/epjc/s10052-019-6619-5
Abstract
It is known that cosmic magnetic field, if present, can generate anisotropic stress in the plasma and hence, can act as a source of gravitational waves. These cosmic magnetic fields can be generated at very high temperature, much above electroweak scale, due to the gravitational anomaly in presence of the chiral asymmetry. The chiral asymmetry leads to instability in the plasma which ultimately leads to the generation of magnetic fields. In this article, we discuss the generation of gravitational waves, during the period of instability, in the chiral plasma sourced by the magnetic field created due to the gravitational anomaly. We have shown that such gravitational wave will have a unique spectrum. Moreover, depending on the temperature of the universe at the time of its generation, such gravitational waves can have a wide range of frequencies. We also estimate the amplitude and frequency of the gravitational waves and delineate the possibility of its detection by future experiments like eLISA.
8 pages, 2 figures
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Cited by in corpus (12)
- Chiral effects in astrophysics and cosmology
- Circular Polarization of Gravitational Waves from Early-Universe Helical Turbulence
- Relic gravitational waves from the chiral magnetic effect
- Gravitational wave generation in a viable scenario of inflationary magnetogenesis
- Big Bang Nucleosynthesis Limits and Relic Gravitational Waves Detection Prospects
- Simulating relic gravitational waves from inflationary magnetogenesis
- Gravitational waves in neutrino plasma and NANOGrav signal
- Chiral gravitational effect in time-dependent backgrounds
- Magnetic fields in a hot dense neutrino plasma and the Gravitational Waves
- Chiral gravitational waves from thermalized neutrinos in the early Universe
- Simulations of helical inflationary magnetogenesis and gravitational waves
- Generating Seed magnetic field à la Chiral Biermann battery