Constraining cosmological extra dimensions with gravitational wave standard sirens: From theory to current and future multimessenger observations

Corman, M., Ghosh, A., Escamilla-Rivera, C., Hendry, M. A. , Marsat, S. and Tamanini, N. (2022) Constraining cosmological extra dimensions with gravitational wave standard sirens: From theory to current and future multimessenger observations. Physical Review D, 105(6), 064061. (doi: 10.1103/PhysRevD.105.064061)

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Abstract

The propagation of gravitational waves (GWs) at cosmological distances offers a new way to test the gravitational interaction at the largest scales. Many modified theories of gravity, usually introduced to explain the observed acceleration of the Universe, can be probed in an alternative and complementary manner with respect to standard electromagnetic (EM) observations. In this paper we consider a homogeneous and isotropic cosmology with extra spatial dimensions at large scales, which represents a simple phenomenological prototype for extradimensional modified gravity cosmological models. By assuming that gravity propagates through the higher-dimensional spacetime, while photons are constrained to the usual four dimensions of general relativity, we derive from first principles the relation between the luminosity distance measured by GW detectors and the one inferred by EM observations. We then use this relation to constrain the number of cosmological extra dimensions with the binary neutron star event GW170817 and the binary black hole merger GW190521. We further provide forecasts for the Laser Interferometer Space Antenna (LISA) by simulating multimessenger observations of massive black hole binary (MBHB) mergers. This paper extends and updates previous analyses which crucially neglected an additional redshift dependency in the GW-EM luminosity distance relation which affects results obtained from multimessenger GW events at high redshift, in particular constraints expected from LISA MBHBs.

Item Type:Articles
Keywords:Alternative gravity theories, cosmological parameters, cosmology, gravitational waves.
Status:Published
Refereed:Yes
Glasgow Author(s) Enlighten ID:Hendry, Professor Martin
Authors: Corman, M., Ghosh, A., Escamilla-Rivera, C., Hendry, M. A., Marsat, S., and Tamanini, N.
Subjects:Q Science > QB Astronomy
Q Science > QC Physics
College/School:College of Science and Engineering > School of Physics and Astronomy
Research Centre:College of Science and Engineering > School of Physics and Astronomy > Institute for Gravitational Research
Journal Name:Physical Review D
Publisher:American Physical Society
ISSN:1550-7998
ISSN (Online):1550-2368
Published Online:29 March 2022
Copyright Holders:Copyright © 2022 American Physical Society
First Published:First published in Physical Review D 105(6):064061
Publisher Policy:Reproduced in accordance with the copyright policy of the publisher

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Project CodeAward NoProject NamePrincipal InvestigatorFunder's NameFunder RefLead Dept
169451Investigations in Gravitational RadiationSheila RowanScience and Technology Facilities Council (STFC)ST/L000946/1P&S - Physics & Astronomy