Dynamical dark energy models in the light of gravitational-wave transient catalogues - INSPIRE

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Dynamical dark energy models in the light of gravitational-wave transient catalogues

Mar 2, 2021

24 pages

Published in:

JCAP 03 (2022) 03, 060

Published: Mar 29, 2022

e-Print:

2103.02097 [gr-qc]

DOI:

10.1088/1475-7516/2022/03/060

View in:

ADS Abstract Service

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Abstract: (IOP)

The study of current gravitational waves (GW) catalogues provide an interesting model independent way to understand further the nature of dark energy. In this work, we present an update of the constrains related to dynamical dark energy parametrisations using recent Gravitational-Wave Transient catalogues (GWTC-1 and GWTC-2) along with Type Ia supernova (SNeIa) and Cosmic Chronometers (CC) catalogues. According to our Bayesian results using the full SNeIa+CC+GW database, the ΛCDM model shows a strong preference against two dark energy parameterisation known as Barboza-Alcaniz (BA) and the Low Correlation (LC) models. Also, we obtain a very strong preference against the Chevallier-Polarski-Linder (CPL) model. Furthermore, we generated a mock GW catalogue and estimate that we require approximately 1000 standard sirens to have a constrain of H

_{0}

within 1% relative error, quantity that is out of reach of current standard sirens candidates in GWTC-1 and GWTC-2 catalogues.

Note:

24 pages, 6 figures and 6 tables. Version accepted in JCAP

dark energy theory
gravitational waves / theory
modified gravity

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Figures(10)

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