pith. sign in

arxiv: 1801.10161 · v1 · pith:FPHZ6V2Znew · submitted 2018-01-30 · ✦ hep-ph · astro-ph.HE· gr-qc

Searching for Dark Photon Dark Matter with Gravitational Wave Detectors

classification ✦ hep-ph astro-ph.HEgr-qc
keywords darkbosondetectorsgaugegravitationalmatterwavebackground
0
0 comments X
read the original abstract

If dark matter stems from the background of a very light gauge boson, this gauge boson could exert forces on test masses in gravitational wave detectors, resulting in displacements with a characteristic frequency set by the gauge boson mass. We outline a novel search strategy to hunt for such dark matter, and show that both ground-based and future space-based gravitational wave detectors have the capability to make a 5$\sigma$ discovery in unexplored parameter regimes.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 4 Pith papers

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

  1. Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter

    hep-ph 2025-07 unverdicted novelty 6.0

    Future high-frequency-sensitive GW detectors can distinguish binary neutron star from low-mass black hole mergers in late phases, enabling separation of merger rates and constraints on heavy non-annihilating dark matt...

  2. Black Hole Solutions in Dark Photon Models with Higher Order Corrections

    gr-qc 2025-05 conditional novelty 6.0

    Analytic perturbative black hole solutions in dark photon models with minimal and higher-order magnetic dipole corrections to the Schwarzschild geometry.

  3. Constraints on Ultralight Scalar and Dark Photon Dark Matter from PPTA-DR3 and EPTA-DR2

    astro-ph.CO 2026-05 unverdicted novelty 4.0

    Bayesian analysis of PPTA-DR3 and EPTA-DR2 finds no statistically significant ULDM signals and sets 95% CL upper limits on scalar and dark photon dark matter, improving prior bounds in most mass ranges.

  4. Gravitational waves of extreme-mass-ratio inspirals in a rotating black hole with Dehnen dark matter halo

    gr-qc 2026-04 unverdicted novelty 4.0

    EMRI waveforms in a rotating black hole with Dehnen DM halo show amplitude and phase shifts from Kerr, with mismatch rising as DM mass parameter and black hole spin increase.