English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
  Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations

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

Item is

Basic

show hide
Genre: Journal Article

Files

show Files
hide Files
:
2109.08748.pdf (Preprint), 3MB
Name:
2109.08748.pdf
Description:
File downloaded from arXiv at 2021-09-23 10:24
Visibility:
Public
MIME-Type / Checksum:
application/pdf / [MD5]
Technical Metadata:
Copyright Date:
-
Copyright Info:
-
:
PhysRevD.105.064061.pdf (Publisher version), 805KB
 
File Permalink:
-
Name:
PhysRevD.105.064061.pdf
Description:
-
Visibility:
Restricted (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), MPGR; )
MIME-Type / Checksum:
application/pdf
Technical Metadata:
Copyright Date:
-
Copyright Info:
-
License:
-

Locators

show

Creators

show
hide
 Creators:
Corman, Maxence, Author
Ghosh, Abhirup1, Author              
Escamilla-Rivera, Celia, Author
Hendry, Martin A., Author
Marsat, Sylvain1, Author              
Tamanini, Nicola1, Author              
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

Content

show
hide
Free keywords: General Relativity and Quantum Cosmology, gr-qc,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO
 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 extra-dimensional 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 multi-messenger 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 multi-messenger GW events at high redshift, in particular constraints expected from LISA MBHBs.

Details

show
hide
Language(s):
 Dates: 2021-09-172022
 Publication Status: Published in print
 Pages: 20 pages, 3 figures
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 2109.08748
DOI: 10.1103/PhysRevD.105.064061
 Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show
hide
Title: Physical Review D
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: -
Pages: - Volume / Issue: 105 (6) Sequence Number: 064061 Start / End Page: - Identifier: -