scholarly journals False vacuum decay in a brane world cosmological model

2006 ◽  
Vol 38 (5) ◽  
pp. 953-962 ◽  
Author(s):  
Michal Demetrian
1991 ◽  
Vol T36 ◽  
pp. 269-275 ◽  
Author(s):  
V A Berezin ◽  
V A Kuzmin ◽  
I I Tkachev

2018 ◽  
Vol 2018 (10) ◽  
Author(s):  
Adalto R. Gomes ◽  
F. C. Simas ◽  
K. Z. Nobrega ◽  
P. P. Avelino
Keyword(s):  

2020 ◽  
Vol 102 (12) ◽  
Author(s):  
Victor Guada ◽  
Miha Nemevšek
Keyword(s):  

2020 ◽  
Vol 2020 (8) ◽  
Author(s):  
Takumi Hayashi ◽  
Kohei Kamada ◽  
Naritaka Oshita ◽  
Jun’ichi Yokoyama

Abstract False vacuum decay is a key feature in quantum field theories and exhibits a distinct signature in the early Universe cosmology. It has recently been suggested that the false vacuum decay is catalyzed by a black hole (BH), which might cause the catastrophe of the Standard Model Higgs vacuum if primordial BHs are formed in the early Universe. We investigate vacuum phase transition of a scalar field around a radiating BH with taking into account the effect of Hawking radiation. We find that the vacuum decay rate slightly decreases in the presence of the thermal effect since the scalar potential is stabilized near the horizon. However, the stabilization effect becomes weak at the points sufficiently far from the horizon. Consequently, we find that the decay rate is not significantly changed unless the effective coupling constant of the scalar field to the radiation is extremely large. This implies that the change of the potential from the Hawking radiation does not help prevent the Standard Model Higgs vacuum decay catalyzed by a BH.


2019 ◽  
Vol 2019 (12) ◽  
Author(s):  
Wen-Yuan Ai ◽  
Björn Garbrecht ◽  
Carlos Tamarit

1999 ◽  
Vol 120 (3) ◽  
pp. 1194-1212 ◽  
Author(s):  
V. A. Rubakov ◽  
S. M. Sibiryakov

2016 ◽  
Vol 31 (24) ◽  
pp. 1650131 ◽  
Author(s):  
Yuhei Goto ◽  
Kazumi Okuyama

In this paper, we study the false vacuum decay of a single scalar field [Formula: see text] coupled to gravity described by the Coleman–de Luccia (CdL) instanton. We show that it is possible to numerically calculate the bounce factor, which is related to the CdL tunneling rate, without using the thin-wall approximation. In this paper, we consider [Formula: see text]- and [Formula: see text]-type potentials as examples, which have cosmological and phenomenological applications. Especially, in the [Formula: see text]-type potential, we show that the range of values in which axion decay constant can take is restricted by the form of the periodic potential if the CdL tunneling occurs.


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