Preprint PUBDB-2021-03536

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Effect of density fluctuations on gravitational wave production in first-order phase transitions

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2021

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Report No.: DESY-21-131; arXiv:2108.11947

Abstract: We study the effect of density perturbations on the process of first-order phase transitions and gravitational wave production in the early Universe. We are mainly interested in how the distribution of nucleated bubbles is affected by fluctuations in the local temperature. We find that large-scale density fluctuations ($H_* < k_* < \beta$) result in a larger effective bubble size at the time of collision, enhancing the produced amplitude of gravitational waves. The amplitude of the density fluctuations necessary for this enhancement is ${\cal P}_\zeta (k_*) \gtrsim (\beta / H_*)^{-2}$, and therefore the gravitational wave signal from first-order phase transitions with relatively large $\beta / H_*$ can be significantly enhanced by this mechanism even for fluctuations with moderate amplitudes.

Keyword(s): density: fluctuation ; effect: density ; density: perturbation ; bubble: size ; gravitational radiation: emission ; bubble: nucleation ; critical phenomena ; temperature: fluctuation ; cosmological phase transitions ; gravitational waves / sources

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Note: 22 pages, 14 figures

Contributing Institute(s):
  1. Theorie-Gruppe (T)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF4-611) (POF4-611)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2021
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http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Journal Article  ;  ;  ;
Effect of density fluctuations on gravitational wave production in first-order phase transitions
Journal of cosmology and astroparticle physics 2021(12), 019 () [10.1088/1475-7516/2021/12/019]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2021-08-25, last modified 2023-05-10