1995
DOI: 10.1103/physrevd.52.6717
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Bubble nucleation incphi4models at all temperatures

Abstract: One possible way in which phase transitions in the early universe may have occurred is via nucleation of bubbles of the new phase (true vacuum) in the old phase (false vacuum). The technique most widely used to compute the probability of bubble nucleation is based on instanton methods in the context of the semiclassical approximation. At zero temperature in 3+1 dimensions the nucleation rate is dominated by the O(4) symmetric instanton, a sphere of radius R, while a t temperatures T >> R-' the decay is dominat… Show more

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Cited by 23 publications
(29 citation statements)
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“…The aim of this paper is to investigate the nature of the phase transition for ϕ 4 theory with a ϕ 3 symmetry-breaking term and compare our results with those of Ferrera [8] who discussed a ϕ symmetry-breaking term.…”
Section: Algorithmmentioning
confidence: 99%
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“…The aim of this paper is to investigate the nature of the phase transition for ϕ 4 theory with a ϕ 3 symmetry-breaking term and compare our results with those of Ferrera [8] who discussed a ϕ symmetry-breaking term.…”
Section: Algorithmmentioning
confidence: 99%
“…Our aim is to obtain the bounce solutions at all temperatures, to compute the action and to determine the nature of the phase transition from quantum tunneling to thermal hopping. Our work therefore follows a parallel track to that of Ferrera [8], and it is of interest to compare the results for the two theories. We find that, for small values of f , the action shows a kink when plotted against temperature or its inverse β.…”
Section: Introductionmentioning
confidence: 99%
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“…Recently, much attention is paid to quantum-classical decay-rate transition in various branches of physics such as spin tunneling systems [1][2][3], field theoretical models [4][5][6], and cosmology [7][8][9]. An important issue in this field is to determine the type of the decayrate transition.…”
Section: Introductionmentioning
confidence: 99%