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Propagation of Gravitational Waves in Chern-Simons Axion Einstein Gravity

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arxiv 1909.01324 v2 pith:YF5GDKUP submitted 2019-09-03 gr-qc hep-th

Propagation of Gravitational Waves in Chern-Simons Axion Einstein Gravity

classification gr-qc hep-th
keywords propagationaxioneinsteingravitationalgravityshallwaveschern-simons
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In this paper we shall investigate the propagation of gravitational waves in a flat Friedman-Robertson-Walker background, in the context of a string motivated corrected Einstein gravity. Particularly, we shall consider a misalignment axion Einstein gravity in the presence of a string originating Chern-Simons coupling of the axion field to the Chern-Pontryagin density in four dimensions. We shall focus our study on the propagation of the gravitational waves, and we shall investigate whether there exists any difference in the propagation of the polarization states of the gravitational waves. As we demonstrate, the dispersion relations are different in the Right-handed mode and the Left-handed mode. Finally, we compare the propagation of the axion Chern-Simons Einstein theory with that of standard $F(R)$ gravity.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

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    Axion-like fields coupled to the Nieh-Yan term generate a chiral GW background during radiation domination, with parameter space explored for detectability in PTA and space-based observatories.

  2. Spinfoams, $\gamma$-duality and parity violation in primordial gravitational waves

    gr-qc 2024-03 unverdicted novelty 6.0

    γ-duality in the EPRL spinfoam model determines the relation between parity-even and parity-odd terms in an effective gravity theory, allowing the Barbero-Immirzi parameter to be measured from inflationary tensor observables.

  3. Gravitational Wave Birefringence from Fuzzy Dark Matter

    gr-qc 2024-06 unverdicted novelty 5.0

    Fuzzy dark matter induces frequency-dependent amplitude birefringence in gravitational waves with periodic time modulation set by the scalar mass, but no velocity birefringence.