Polarization modes of gravitational waves in general Einstein-vector theory
Xiao-Bin Lai, Yu-Qi Dong, Yu-Qiang Liu, and Yu-Xiao Liu

TL;DR
This paper investigates the polarization modes of gravitational waves in Einstein-vector theories with a background vector field, revealing a variety of possible modes and constraining them using recent gravitational wave and pulsar timing observations.
Contribution
It characterizes the polarization modes in Einstein-vector theories, showing their dependence on parameters and comparing them with observational constraints, which is a novel analysis.
Findings
At least two and up to five polarization modes are possible.
The background vector field causes anisotropy and diverse polarization contents.
The $P_b$ mode always propagates at light speed and is consistent with observations.
Abstract
We study the polarization modes of gravitational waves in general Einstein-vector theory with an arbitrary constant background vector field under a Minkowski background. We compare these polarization modes with those of other vector-tensor theories and constrain the parameter spaces based on the gravitational-wave event GW170817 with its electromagnetic counterpart GRB170817A and observations of pulsar timing arrays. The presence of the background vector field leads to the anisotropy of space and a rich variety of gravitational wave contents. Our results reveal that the polarization modes of gravitational waves depend on the parameter spaces. There are at least two and at most five independent polarization modes in one parameter space. In different parameter spaces, some mixture modes are allowed, including tensor-vector, tensor-scalar, tensor-vector-scalar, vector-scalar, and…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Pulsars and Gravitational Waves Research · Cosmology and Gravitation Theories
