Chirality oscillation of primordial gravitational waves during inflation
arXiv:1608.06508 · doi:10.1007/JHEP03(2017)024
Abstract
We show that if the gravitational Chern-Simons term couples to a massive scalar field (), the primordial gravitational waves (GWs) will show itself the chirality oscillation, i.e., the amplitudes of the left- and right-handed GWs modes will convert into each other and oscillate in their propagations. This oscillation will eventually develop a permanent difference of the amplitudes of both modes, which leads to nearly opposite oscillating shapes in the power spectra of the left- and right-handed primordial GWs. We discuss its implication to the CMB B-mode polarization.
14 pages, 11 figures; published version in JHEP; one figure added; references and comments added
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Cited by in corpus (14)
- Parity breaking signatures from a Chern-Simons coupling during inflation: the case of non-Gaussian gravitational waves
- Polarized primordial gravitational waves in the ghost-free parity-violating gravity
- Parity violating gravitational waves at the end of inflation
- Generating enhanced parity-violating gravitational waves during inflation with violation of the null energy condition
- Generating enhanced primordial GWs during inflation with intermittent violation of NEC and diminishment of GW propagating speed
- Parity-violation in bouncing cosmology
- Generation of gravitational waves in dynamical Chern-Simons gravity
- Chiral Gravitational Waves in Palatini Chern-Simons
- Chiral primordial gravitational waves in extended theories of Scalar-Tensor gravity
- Parity violation in primordial tensor non-Gaussianities from matter bounce cosmology
- Cosmic topology. Part IIIa. Microwave background parity violation without parity-violating microphysics
- Parity-violating primordial gravitational waves from null energy condition violation
- Chiral Gravitational Wave Background from Audible Axion via Nieh-Yan Term
- Gravitational Waves from Primordial Black Holes formed by Null Energy Condition Violation during Inflation