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Polarization modes of gravitational waves in generalized Proca theory

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arxiv 2305.12516 v2 pith:V3OOT5Y6 submitted 2023-05-21 gr-qc hep-th

classification gr-qchep-th
keywords modesmodetensorvectorspeedallowsamplitudegravitational
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abstract

In this paper, we study polarization modes of gravitational waves in generalized Proca theory in the homogeneous and isotropic Minkowski background. The results show that the polarizations of gravitational waves depend on the parameter space of this gravity theory and can be divided into quite rich cases by parameters. In some parameter space, it only allows two tensor modes, i.e., the $+$ and $\times$ modes. In some parameter space, besides tensor modes, it also allows one scalar mode, or two vector (vector-$x$ and vector-$y$) modes, or both one scalar mode and two vector modes. The scalar mode is a mixture mode of a breathing mode and a longitudinal mode, or just a pure breathing mode. Interestingly, it is found that the amplitude of the vector modes is related to the speed of the tensor modes. This allows us to give the upper bound of the amplitude of the vector modes by detecting the speed of the tensor modes. Specifically, if the speed of tensor modes is strictly equal to the speed of light, then the amplitude of vector modes is zero.

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Cited by 2 Pith papers

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

  1. Proca theory of four-dimensional regularized Gauss-Bonnet gravity and black holes with primary hair

    gr-qc 2025-04 conditional novelty 7.0 of 10

    A Weyl-geometry vector field yields a four-dimensional generalized-Proca Gauss-Bonnet theory whose black holes carry two independent primary-hair constants, one of which becomes an effective cosmological constant afte...

  2. Gravitational Memory in Generalized Proca Gravity

    gr-qc 2025-08 conditional novelty 6.0 of 10

    The displacement memory formula for Generalized Proca gravity is derived for a massive Lorentz-invariant branch and a massless Lorentz-violating branch, with the dispersive branch requiring a frequency-integrated treatment.

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