Preprint/Report PUBDB-2015-06258

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Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions

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2015

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Report No.: DESY 15-246; arXiv:1512.06239

Abstract: We investigate the potential for the eLISA space-based interferometer to detect the stochastic gravitational wave background produced by strong first-order cosmological phase transitions. We discuss the resulting contributions from bubble collisions, magnetohydrodynamic turbulence, and sound waves to the stochastic background, and estimate the total corresponding signal predicted in gravitational waves. The projected sensitivity of eLISA to cosmological phase transitions is computed in a model-independent way for various detector designs and configurations. By applying these results to several specific models, we demonstrate that eLISA is able to probe many well-motivated scenarios beyond the Standard Model of particle physics predicting strong first-order cosmological phase transitions in the early Universe.


Contributing Institute(s):
  1. Theorie-Gruppe (T)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF3-611) (POF3-611)
  2. EWPTBSM - The Electroweak Phase Transition Beyond the Standard Model (629425) (629425)
  3. PRACE - Partnership for Advanced Computing in Europe (211528) (211528)
  4. EWBGANDLHC - Electroweak Baryogenesis in the Era of the LHC (625809) (625809)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2015
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Science with the space-based interferometer eLISA. II: gravitational waves from cosmological phase transitions
Journal of cosmology and astroparticle physics 2016(04), 001 - 001 () [10.1088/1475-7516/2016/04/001]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2015-12-23, last modified 2021-11-10


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