Energy of weak gravitational waves in spacetimes with a positive cosmological constant

P. T. Chruściel, Sk Jahanur Hoque, and Tomasz Smołka
Phys. Rev. D 103, 064008 – Published 5 March 2021

Abstract

We derive a formula for the total canonical energy, and its flux, of weak gravitational waves on a de Sitter background.

  • Received 9 March 2020
  • Accepted 6 January 2021

DOI:https://doi.org/10.1103/PhysRevD.103.064008

© 2021 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

P. T. Chruściel1,*, Sk Jahanur Hoque2,†, and Tomasz Smołka3,‡

  • 1Faculty of Physics, University of Vienna, Boltzmanngasse 5, A1090 Wien, Austria
  • 2Institute of Theoretical Physics, Faculty of Mathematics and Physics, Charles University, V Holešovičkách 2, 180 00 Prague 8, Czech Republic
  • 3Department of Mathematical Methods in Physics, Faculty of Physics, University of Warsaw, Pasteura 5, PL 02-093 Warszawa, Poland

  • *piotr.chrusciel@univie.ac.at
  • jahanur.hoque@utf.mff.cuni.cz
  • tomasz.smolka@fuw.edu.pl

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Issue

Vol. 103, Iss. 6 — 15 March 2021

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