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Gravitational Wave Polarizations in $f(R)$ Gravity and Scalar-Tensor Theory

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arxiv 1709.03313 v2 pith:MG55HUEG submitted 2017-09-11 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords gravitationalpolarizationsgravitylongitudinalpolarizationwavesdetectscalar
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abstract

The detection of gravitational waves by the Laser Interferometer Gravitational-Wave Observatory opens a new era to use gravitational waves to test alternative theories of gravity. We investigate the polarizations of gravitational waves in $f(R)$ gravity and Horndeski theory, both containing scalar modes. These theories predict that in addition to the familiar $+$ and $\times$ polarizations, there are transverse breathing and longitudinal polarizations excited by the massive scalar mode and the new polarization is a single mixed state. It would be very difficult to detect the longitudinal polarization by interferometers, while pulsar timing array may be the better tool to detect the longitudinal polarization.

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Cited by 1 Pith paper

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

  1. Neutron star in Logarithmic model of Cartan $F(R)$ gravity

    gr-qc 2024-12 reject novelty 6.0 of 10

    In Cartan F(R) gravity with a logarithmic potential, a scalar field can raise the minimum neutron star mass to near one solar mass, but only for hand-tuned parameters that imply a huge vacuum energy.

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