Detecting Dark Energy Fluctuations with Gravitational Waves
arXiv:2007.13722 · doi:10.1103/PhysRevD.103.083506
Abstract
Luminosity distance estimates from electromagnetic and gravitational wave sources are generally different in models of dynamical dark energy and gravity beyond the standard cosmological scenario. We show that this leaves a unique imprint on the angular power-spectrum of fluctuations of the luminosity distance of gravitational-wave observations which tracks inhomogeneities in the dark energy field. Exploiting the synergy in supernovae and gravitational wave distance measurements, we build a joint estimator that directly probes dark energy fluctuations, providing a conclusive evidence for their existence in case of detection. Moreover, such measurement would also allow to probe the running of the Planck mass. We discuss experimental requirements to detect these signals.
9 pages, 2 figures. Matching published version
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- Constraining extended cosmologies with GWLSS cross-correlations
- No slip gravity in light of LISA standard sirens
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- Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure
- Electromagnetic Waves in Cosmological Space-Time II. Luminosity Distance
- Unifying gravitational waves and dark energy