Journal Article PUBDB-2021-01109

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Model-independent energy budget for LISA

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2021
IOP London

Journal of cosmology and astroparticle physics 01, 072 () [10.1088/1475-7516/2021/01/072]
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Report No.: CERN-TH-2020-170; DESY-20-173; arXiv:2010.09744

Abstract: We provide an easy method to obtain the kinetic energy fraction in gravitational waves, generated during a cosmological first-order phase transition, as a function of only the wall velocity and quantities that can be determined from the particle physics model at the nucleation temperature. This generalizes recent work that achieved this goal for detonations. Here we present the corresponding results for deflagrations and hybrids. Unlike for detonations, the sound speed in the symmetric phase also enters the analysis. We perform a detailed comparison between our model-independent approach and other approaches in the literature. We provide a Python code snippet to determine the kinetic energy fraction $K$ as a function of the wall velocity, the two speeds of sound and the strength parameter of the phase transition. We also assess how realistic sizable deviations in speed of sound are close to the phase transition temperature in a specific model.

Keyword(s): velocity: acoustic ; energy: kinetic ; critical phenomena: temperature ; gravitational radiation ; nucleation ; temperature ; hybrid ; benchmark ; hydrodynamics ; LISA ; numerical methods ; numerical calculations ; bubble: nucleation

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Contributing Institute(s):
  1. Theorie-Gruppe (T)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF4-611) (POF4-611)
  2. DFG project 390833306 - EXC 2121: Quantum Universe (390833306) (390833306)
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  1. No specific instrument

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Model-independent energy budget for LISA
1-30 () [10.3204/PUBDB-2020-04189]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2021-02-25, last modified 2025-07-24


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