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RESEARCH PRODUCT
Detecting gravitational waves from cosmological phase transitions with LISA: an update
Germano NardiniMikael ChalaMikael ChalaDavid J. WeirDavid J. WeirG. C. DorschG. C. DorschGeraldine ServantJonathan KozaczukJonathan KozaczukJonathan KozaczukPedro SchwallerChiara CapriniStephan J. HuberMark HindmarshMark HindmarshAnders TranbergKari RummukainenThomas KonstandinJose Miguel NoJose Miguel Nosubject
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 Astrophysicsdescription
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, and also acknowledges support from the Spanish MINECO's "Centro de Excelencia Severo Ochoa" Programme under grant SEV-2016-0597, from the European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreements 690575 (RISE InvisiblesPlus) and 674896 (ITN ELUSIVES) and from the Spanish Proyectos de I+D de Generacion de Conocimiento via grant PGC2018-096646-A-I00. KR is funded by the Academy of Finland grants 308791, 319066 and 320123. PS is supported by the Cluster of Excellence "Precision Physics, Fundamental Interactions, and Structure of Matter"(PRISMA+ EXC 2118/1) funded by the German Research Foundation(DFG). PS would like to thank Moritz Breitbach and Eric Madge for providing the data for figures (14), (15) and (16), and Eric Madge for checking the ptplot code. DJW (ORCID ID 0000-00016986-0517) was supported by an Science and Technology Facilities Council Ernest Rutherford Fellowship, grant no. ST/R003904/1, by the Research Funds of the University of Helsinki, and by the Academy of Finland, grant nos. 286769, 324882 and 328958. The original LISA Cosmology Working Group preprint number of this paper is \LISA CosWG-19-04".
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2020-01-01 |