Chiral gravitational waves in Palatini-Chern-Simons gravity

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dc.contributor.authorSulantay, Felipe
dc.contributor.authorLagos, Macarena
dc.contributor.authorBanados, Maximo
dc.date.accessioned2025-01-20T20:11:21Z
dc.date.available2025-01-20T20:11:21Z
dc.date.issued2023
dc.description.abstractWe study the parity-breaking higher-curvature gravity theory of Chern-Simons (CS), using the Palatini formulation in which the metric and connection are taken to be independent fields. We first show that Palatini-CS gravity leads to first-order derivative equations of motion and thus avoid the typical instabilities of CS gravity in the metric formalism. As an initial application, we analyze the cosmological propagation of gravitational waves (GWs) in Palatini-CS gravity. We show that, due to parity breaking, the polarizations of GWs suffer two effects during propagation: amplitude birefringence (which changes the polarization ellipticity) and velocity birefringence (which rotates the polarization plane). While amplitude birefringence is known to be present in CS gravity in the metric formalism, velocity birefringence is not present in metric CS gravity for high frequency waves, but now appears in Palatini-CS due to the fact that left-handed and right-handed GW polarizations have a different dispersion relation. In the approximation of small deviations from general relativity (GR), we do find however that velocity birefringence appears at least quadratically in the CS coupling parameter alpha, while amplitude birefringence appears linearly in alpha. This means that amplitude birefringence will be the most relevant effect in Palatini-CS and hence this model will behave similarly to metric CS. We confirm this by applying current constraints on amplitude and velocity birefringence to Palatini-CS, and showing that those from amplitude birefringence give the tightest bounds.
dc.fuente.origenWOS
dc.identifier.doi10.1103/PhysRevD.107.104025
dc.identifier.eissn2470-0029
dc.identifier.issn2470-0010
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.107.104025
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/92139
dc.identifier.wosidWOS:000995116400008
dc.issue.numero10
dc.language.isoen
dc.revistaPhysical review d
dc.rightsacceso restringido
dc.titleChiral gravitational waves in Palatini-Chern-Simons gravity
dc.typeartículo
dc.volumen107
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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