The supercooling window at weak and strong coupling

被引:20
|
作者
Levi, Noam [1 ]
Opferkuch, Toby [2 ,3 ]
Redigolo, Diego [4 ]
机构
[1] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, IL-69978 Tel Aviv, Israel
[2] Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA
[3] Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA
[4] Sez Firenze, INFN, Via G Sansone 1, I-50019 Sesto Fiorentino, Italy
关键词
Early Universe Particle Physics; Phase Transitions in the Early Universe; COSMOLOGICAL CONSEQUENCES; GRAVITATIONAL-RADIATION; SYMMETRY-BREAKING; GAUGE-INVARIANCE; PHASE-TRANSITION; INFLATION; VACUUM;
D O I
10.1007/JHEP02(2023)125
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Supercooled first order phase transitions are typical of theories where conformal symmetry is predominantly spontaneously broken. In these theories the fate of the flat scalar direction is highly sensitive to the size and the scaling dimension of the explicit breaking deformations. For a given deformation, the coupling must lie in a particular region to realize a supercooled first order phase transition. We identify the supercooling window in weakly coupled theories and derive a fully analytical understanding of its boundaries. Mapping these boundaries allows us to identify the deformations enlarging the supercooling window and to characterize their dynamics analytically. For completeness we also discuss strongly coupled conformal field theories with an holographic dual, where the complete characterization of the supercooling window is challenged by calculability issues.
引用
收藏
页数:44
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