Imprint of ultralight vector fields on gravitational wave propagation - INSPIRE

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Imprint of ultralight vector fields on gravitational wave propagation

Alfredo D. Miravet
(
- Madrid U.
)
,
Antonio L. Maroto
(
- Madrid U.
)

Dec 14, 2020

10 pages

Published in:

Phys.Rev.D 103 (2021) 12, 123546

Published: Jun 15, 2021

e-Print:

2012.07505 [astro-ph.CO]

DOI:

10.1103/PhysRevD.103.123546 (publication)

View in:

reference search4 citations

Citations per year

Abstract: (APS)

We study the effects of ultralight vector field (ULVF) dark matter on gravitational wave propagation. We find that the coherent oscillations of the vector field induce an anisotropic suppression of the gravitational wave amplitude as compared to the standard cosmology prediction. The effect is enhanced for smaller vector field masses and peaks for modes around

k = H_{0} / \sqrt{a (H = m)}

. The suppression is negligible for astrophysically generated gravitational waves but could be sizable for primordial gravity waves. We discuss the possibility of detecting such an effect on the tensor power spectrum with future cosmic microwave background B-mode polarization detectors. We find that for the sensitivity of the upcoming LiteBIRD mission, the correction to the tensor power spectrum at decoupling time could be distinguishable from that of

Λ CDM

for ULVF masses

m ≲ 10^{- 26} eV

and sufficiently large abundances.

Note:

10 pages, 10 figures, matches version to appear in PRD

field theory: vector
gravitational radiation: propagation
cosmic background radiation: B-mode
anisotropy: suppression
oscillation: coherence
dark matter: density
cosmological model: parameter space
power spectrum
sensitivity
gravitation

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Figures(10)

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