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Detecting gravitational waves from cosmological phase transitions with LISA: an update

2020

MC was funded by the Royal Society under the Newton International Fellowship program. GD would like to thank CNPq (Brazil) for financial support. MH was supported by the Science and Technology Facilities Council (grant number ST/P000819/1), and the Academy of Finland (grant number 286769). SJH was supported by the Science and Technology Facilities Council (grant number ST/P000819/1). The work of JK was supported by Department of Energy (DOE) grant DE-SC0019195 and NSF grant PHY-1719642. TK and GS are funded by the Deutsche Forschungsgemeinschaft under Germany's Excellence Strategy - EXC 2121 \Quantum Universe" - 390833306. JMN is supported by Ramon y Cajal Fellowship contract RYC-2017-22986…

Phase transitionCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelDark matterstandard modelFOS: Physical sciencesContext (language use)gravitational radiation: direct detection01 natural sciencesdark matterbubble: nucleationGravitational wavesTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)effective field theory0103 physical sciencesEffective field theoryenergy: densitynumerical calculationsCosmological phase transitionsperturbation theoryPhysics:Matematikk og Naturvitenskap: 400::Fysikk: 430 [VDP]wave: acousticLISACOSMIC cancer database010308 nuclear & particles physicsGravitational wavenew physicsGravitational theorygravitational radiationAstronomy and Astrophysicscritical phenomenagravitational radiation detectorHigh Energy Physics - PhenomenologyGravitational sourcesgravitational radiation: emission[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Higgs modelPerturbation theory (quantum mechanics)gravitational radiation: power spectrum[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]dilatonAstrophysics - Cosmology and Nongalactic Astrophysics
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