Gravitational Higgs mechanism in inspiraling scalarized NS-WD binary
Jing Wang

TL;DR
This paper explores how scalar-tensor theories predict a gravitational Higgs mechanism in NS-WD binaries, leading to scalar radiation, mass effects, and Yukawa-like corrections to gravity, with implications for gravitational wave observations.
Contribution
It introduces a novel analysis of the gravitational Higgs mechanism in scalarized NS-WD binaries, highlighting scalar radiation and mass effects in the gravitational scalar field.
Findings
Scalar radiation emitted due to binding energy differences.
Estimated scalar masses around 10^{-21} eV/c^2.
Yukawa-like correction to Newtonian potential.
Abstract
We investigate the gravitational Higgs mechanism in the inspiraling scalarized neutron star - white dwarf (NS-WD) binaries, whose dynamics are described by the scalar-tensor theory. Because of the difference in binding energy of NS and WD, the orbital decay of scalarized NS-WD system actually sources an emission of dipolar gravitational scalar radiation, in addition to the tensor gravitational waves, which breaks the Lorentz invariance constructed in the framework of general relativity. The resulted gravitational scalar radiation field obtains a scalar-energy-density-dependent effective mass, arising from a gravitational scalar potential that consists of a monotonically decreasing self-interactions of gravitational scalar field and an increasing exponential coupling between the scalar field and the NS/WD matter. Owing to a thin-ring-orbit effect, the gravitational interactions encoded…
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