Gravitational Waves Detections for Cosmological Measurements and Tests of General Relativity

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Cosmology".

Deadline for manuscript submissions: closed (31 December 2021) | Viewed by 1560

Special Issue Editor


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Guest Editor
1. French National Centre for Scientific Research (CNRS), 75016 Paris, France
2. Astroparticule et Cosmologie, University Paris Diderot, 75013 Paris, France
Interests: gravitational-wave physics; gravitational-wave data analysis; gravitational-wave cosmology and astrophysics; multi-messenger astronomy; tests of General Relativity with gravitational waves

Special Issue Information

Dear Colleagues,

GWs provide a new channel for studying and testing the cosmological expansion of the Universe. GW sources are cosmological standard sirens because it is possible to infer the luminosity distance of the source from their detection without any cosmological distance ladder.

Provided with a cosmological redshift, either from a direct electromagnetic counterpart or a galaxy survey, GW detections can be used to measure cosmological parameters, such as the Hubble constant. Nevertheless, it has been shown that GWs can also be used to probe general relativity on cosmological scales by studying their propagation.

This Special Issue will review and present progress and forecasts in the novel field of GW cosmology with current and future GW detectors. We welcome review papers on the status of the field, as well as research papers presenting novel methodologies for testing cosmology with GWs.

Dr. Simone Mastrogiovanni
Guest Editor

Manuscript Submission Information

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Keywords

  • Gravitational waves cosmology
  • Multi-messenger astronomy
  • Gravitational-waves data analysis
  • Cosmological tests of gravity
  • Cosmology beyond the standard cosmological model
  • Ground-based detectors
  • Space-based detectors

Published Papers (1 paper)

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Research

9 pages, 336 KiB  
Communication
The Stochastic Gravitational Wave Background from Magnetars
by Sourav Roy Chowdhury and Maxim Khlopov
Universe 2021, 7(10), 381; https://0-doi-org.brum.beds.ac.uk/10.3390/universe7100381 - 14 Oct 2021
Cited by 7 | Viewed by 1133
Abstract
Magnetars have already been a potential candidate as gravitational wave sources that could be detected by current and future terrestrial as well as ground-based gravitational wave detectors. In this article, we focus on the gravitational wave emission from the distorted rotating neutron stars. [...] Read more.
Magnetars have already been a potential candidate as gravitational wave sources that could be detected by current and future terrestrial as well as ground-based gravitational wave detectors. In this article, we focus on the gravitational wave emission from the distorted rotating neutron stars. The deformation is assumed to be symmetric around an axis that is perpendicular to the rotation axis. The form is applied in the context of a neutron star whose magnetic field has been deformed on its own. By introducing the effects from all magnetars in the Universe, based on various proposed magnetic field configurations, such as poloidal and toroidal, the stochastic gravitational wave background can be generated. We choose to figure out exactly how the observations of the stochastic gravitational wave background should be used to understand much more about physics correlated with the magnetar behavior, based on the restriction on the ellipticity of the magnetar. Full article
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