Gravitational wave birefringence in spatially curved teleparallel cosmology

Research output: Contribution to journalArticleResearchpeer review

Authors

  • Manuel Hohmann
  • Christian Pfeifer

External Research Organisations

  • University of Tartu
  • Center of Applied Space Technology and Microgravity (ZARM)
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Details

Original languageEnglish
Article number137437
JournalPhysics Letters B
Volume834
Early online date8 Sept 2022
Publication statusPublished - 10 Nov 2022
Externally publishedYes

Abstract

We study tensor perturbations around the most general cosmologically symmetric backgrounds in a class of teleparallel gravity theories known as New General Relativity. These theories comprise a one-parameter class, which is fully consistent with observations at the post-Newtonian level, and which contains the teleparallel equivalent of General Relativity as a special case. We find that for a particular class of cosmological background geometries these theories exhibit gravitational wave birefringence and dispersion, i.e., the dispersion relation for gravitational waves depends on their polarization and wave number. The strength of this effect is directly related to the spatial curvature of the cosmological background and the parameter describing the deviation of the theory from General Relativity. We discuss the possibility of observing this effect in gravitational wave experiments.

Keywords

    Gravitational waves, Teleparallel gravity, Tensor perturbations, Birefringence

ASJC Scopus subject areas

Cite this

Gravitational wave birefringence in spatially curved teleparallel cosmology. / Hohmann, Manuel; Pfeifer, Christian.
In: Physics Letters B, Vol. 834, 137437, 10.11.2022.

Research output: Contribution to journalArticleResearchpeer review

Hohmann M, Pfeifer C. Gravitational wave birefringence in spatially curved teleparallel cosmology. Physics Letters B. 2022 Nov 10;834:137437. Epub 2022 Sept 8. doi: 10.1016/j.physletb.2022.137437
Hohmann, Manuel ; Pfeifer, Christian. / Gravitational wave birefringence in spatially curved teleparallel cosmology. In: Physics Letters B. 2022 ; Vol. 834.
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