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

被引:478
|
作者
Caprini, Chiara [1 ]
Chala, Mikael [2 ,3 ,4 ]
Dorsch, Glauber C. [5 ,6 ,21 ]
Hindmarsh, Mark [7 ,8 ,9 ]
Huber, Stephan J. [9 ]
Konstandin, Thomas [10 ]
Kozaczuk, Jonathan [11 ,12 ,13 ]
Nardini, Germano [14 ]
No, Jose Miguel [15 ,16 ]
Rummukainen, Kari [7 ,8 ]
Schwaller, Pedro [17 ,18 ]
Servant, Geraldine [10 ,19 ]
Tranberg, Anders [14 ]
Weir, David J. [7 ,8 ,20 ]
机构
[1] Univ Paris Diderot, CNRS UMR 7164, Lab Astroparticule & Cosmol, F-75013 Paris, France
[2] Univ Durham, Inst Particle Phys Phenomenol, Phys Dept, Durham DH1 3LE, England
[3] Univ Granada, CAFPE, E-18071 Granada, Spain
[4] Univ Granada, Dept Fis Teor & Cosmos, E-18071 Granada, Spain
[5] Univ Fed Espirito Santo, Ctr Astrophys & Cosmol, BR-29075910 Vitoria, ES, Brazil
[6] Univ Fed Espirito Santo, PPGCosmo, BR-29075910 Vitoria, ES, Brazil
[7] Univ Helsinki, Dept Phys, PL 64, FI-00014 Helsinki, Finland
[8] Univ Helsinki, Helsinki Inst Phys, PL 64, FI-00014 Helsinki, Finland
[9] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England
[10] DESY, Notkestr 85, D-22607 Hamburg, Germany
[11] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
[12] Univ Illinois, Dept Phys, Urbana, IL 61801 USA
[13] Univ Massachusetts, Amherst Ctr Fundamental Interact, Dept Phys, Amherst, MA 01003 USA
[14] Univ Stavanger, Fac Sci & Technol, N-4036 Stavanger, Norway
[15] Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain
[16] UAM, CSIC, Inst Fis Teor, Madrid 28049, Spain
[17] Johannes Gutenberg Univ Mainz, PRISMA Cluster Excellence, D-55099 Mainz, Germany
[18] Johannes Gutenberg Univ Mainz, Mainz Inst Theoret Phys, D-55099 Mainz, Germany
[19] Univ Hamburg, Inst Theoret Phys 2, D-22761 Hamburg, Germany
[20] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England
[21] Univ Fed Minas Gerais, Dept Fis, BR-31270901 Belo Horizonte, MG, Brazil
基金
英国科学技术设施理事会; 欧盟地平线“2020”; 芬兰科学院;
关键词
cosmological phase transitions; gravitational waves / sources; gravitational waves / theory; TEMPERATURE DIMENSIONAL REDUCTION; ELECTROWEAK BARYOGENESIS; BUBBLE NUCLEATION; HIGGS-BOSON; GROWTH; RADIATION; MSSM; INSTABILITY; STABILITY; SEARCH;
D O I
10.1088/1475-7516/2020/03/024
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the potential for observing gravitational waves from cosmological phase transitions with LISA in light of recent theoretical and experimental developments. Our analysis is based on current state-of-the-art simulations of sound waves in the cosmic fluid after the phase transition completes. We discuss the various sources of gravitational radiation, the underlying parameters describing the phase transition and a variety of viable particle physics models in this context, clarifying common misconceptions that appear in the literature and identifying open questions requiring future study. We also present a web-based tool, PTPlot, that allows users to obtain up-to-date detection prospects for a given set of phase transition parameters at LISA.
引用
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页数:60
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