Probing early Universe supercooled phase transitions with gravitational wave data

被引:19
作者
Badger, Charles [1 ]
Fornal, Bartosz [2 ]
Martinovic, Katarina [1 ]
Romero, Alba [3 ]
Turbang, Kevin [4 ,5 ]
Guo, Huai-Ke [6 ]
Mariotti, Alberto [4 ,7 ,8 ]
Sakellariadou, Mairi [1 ,4 ,7 ,8 ]
Sevrin, Alexander [4 ,5 ,7 ,8 ]
Yang, Feng-Wei [6 ]
Zhao, Yue [6 ]
机构
[1] Univ London, Kings Coll London, Phys Dept, Theoret Particle Phys & Cosmol Grp, London WC2R 2LS, England
[2] Barry Univ, Dept Chem & Phys, Miami Shores, FL 33161 USA
[3] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, E-08193 Barcelona, Spain
[4] Vrije Univ Brussel, Theoret Natuurkunde, Pleinlaan 2, B-1050 Brussels, Belgium
[5] Univ Antwerp, Prinsstr 13, B-2000 Antwerp, Belgium
[6] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA
[7] Vrije Univ Brussel, ELEM, IIHE, Pleinlaan 2, B-1050 Brussels, Belgium
[8] Int Solvay Inst, Pleinlaan 2, B-1050 Brussels, Belgium
基金
美国国家科学基金会;
关键词
RADIATION; VACUUM;
D O I
10.1103/PhysRevD.107.023511
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the reach of the LIGO/Virgo/KAGRA detectors in the search for signatures of first-order phase transitions in the early Universe. Utilizing data from the first three observing runs, we derive constraints on the parameters of the underlying gravitational-wave background, focusing on transitions characterized by strong supercooling. As an application of our analysis, we determine bounds on the parameter space of two representative particle physics models. We also comment on the expected reach of third-generation detectors in probing supercooled phase transitions.
引用
收藏
页数:13
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