Vacuum decay in the Lorentzian path integral

被引:8
|
作者
Hayashi, Takumi [1 ,2 ]
Kamada, Kohei [2 ]
Oshita, Naritaka [3 ]
Yokoyama, Jun'ichi [1 ,2 ,4 ,5 ]
机构
[1] Univ Tokyo, Grad Sch Sci, Dept Phys, Bunkyo Ku, Hongo 7-3-1, Tokyo 1130033, Japan
[2] Univ Tokyo, Grad Sch Sci, Res Ctr Early Universe RESCEU, Bunkyo Ku, Hongo 7-3-1, Tokyo 1130033, Japan
[3] RIKEN iTHEMS, Wako, Saitama 3510198, Japan
[4] Univ Tokyo, Kavli Inst Phys & Math Universe Kavli IPMU, UTIAS, WPI, Kashiwa, Chiba 2778568, Japan
[5] Univ Tokyo, Trans Scale Quantum Sci Inst, Bunkyo Ku, Hongo 7-3-1, Tokyo 1130033, Japan
关键词
cosmological phase transitions; physics of the early universe; FALSE VACUUM; STANDARD MODEL; BLACK-HOLES; QUANTUM-GRAVITY; OPEN UNIVERSE; HIGGS MASS; CREATION; BOUNDS; FATE; METASTABILITY;
D O I
10.1088/1475-7516/2022/05/041
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We apply the Lorentzian path integral to the decay of a false vacuum and estimate the false-vacuum decay rate. To make the Lorentzian path integral convergent, the deformation of an integration contour is performed by following the Picard-Lefschetz theory. We show that the nucleation rate of a critical bubble, for which the corresponding bounce action is extremized, has the same exponent as the Euclidean approach. We also extend our computation to the nucleation of a bubble larger or smaller than the critical one to which the Euclidean formalism is not applicable.
引用
收藏
页数:26
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