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Published May 2021 | Version v1
Journal article

Gravitational wave emission from the CMB and other thermal fields

  • 1. Institute for Quantum Computing, University of Waterloo, Waterloo, Ontario, N2L 3G1 (Canada)
  • 2. Department of Applied Mathematics, University of Waterloo, Waterloo, Ontario, N2L 3G1 (Canada)
  • 3. Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5 (Canada)
  • 4. Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario, N2L 3G1 (Canada)

Description

We calculate the gravitational wave power density emitted by quantum thermal sources. As particular cases, we calculate the emission of gravitational waves from the cosmic microwave background and from stellar sources. We study how treating gravity classically affects the prediction of the thermal emission. We find that the predicted emitted gravitational wave radiation does not exhibit an ultraviolet divergence, even if gravity is treated classically, as long as the fields describing the thermal source are quantum mechanical.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.physletb.2021.136208

Additional details

Identifiers

DOI
10.1016/j.physletb.2021.136208;
PII
S0370269321001489;

Publishing Information

Journal Title
Physics Letters. Section B
Journal Volume
816
Journal Page Range
vp.
ISSN
0370-2693
CODEN
PYLBAJ

Optional Information

Copyright
Copyright (c) 2021 The Author(s). Published by Elsevier B.V.