Forecasting F(Q) cosmology with $\Lambda$CDM background using standard sirens

Abstract

Forecast constraints for a Symmetric Teleparallel Gravity model with a $\Lambda$CDM background are made using forthcoming ground and space based gravitational waves observatories. A Bayesian analysis resorting to generated mock catalogs shows that LIGO is not expected to be able to distinguish this model from $\Lambda$CDM, while both LISA and the ET will, with the ET outperforming LISA. We also show that low redshift events are favored in order to improve the quality of the constrains.

10 pages, 8 figures, fixed typo on equation (42)

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• Testing $\Lambda$-Free f(Q) Cosmology
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• How different connections in flat FLRW geometry impact energy conditions in $f(Q)$ theory?
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• Equivalence of $f(Q)$ cosmology with quintom-like scenario: the phantom field as effective realization of the non-trivial connection
• Dynamical system analysis of scalar field cosmology in coincident $f(Q)$ gravity
• Forecasts on interacting dark energy with standard sirens
• Prospects of constraining $f(T)$ gravity with the third-generation gravitational-wave detectors
• Cosmological study of a symmetric teleparallel gravity model
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Bulk viscous fluid in symmetric teleparallel cosmology: theory versus experiment
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Gravitational Wave Signatures of Primordial Black Hole Reheating in Upcoming Interferometry Missions
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• Vulnerability of f(Q) gravity theory and a possible resolution
• About the (in)equivalence between holonomic versus non-holonomic theories of gravity