Stochastic tunneling in de Sitter spacetime

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Miyachi, Taiga, Soda, Jiro, Tokuda, Junsei
Format: Preprint
Published: 2023
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866917743673999360
author Miyachi, Taiga
Soda, Jiro
Tokuda, Junsei
author_facet Miyachi, Taiga
Soda, Jiro
Tokuda, Junsei
contents Tunneling processes in de Sitter spacetime are studied by using the stochastic approach. We exploit the Martin-Siggia-Rose-Janssen-de Dominicis (MSRJD) functional integral to obtain the tunneling rate. The applicability conditions of this method are clarified using the Schwinger-Keldysh formalism. In the case of a shallow potential barrier, we reproduce the Hawking-Moss (HM) tunneling rate. Remarkably, in contrast to HM picture, the configuration derived from the MSRJD functional integral satisfies physically natural boundary conditions. We also discuss the case of a steep potential barrier and find an interesting Coleman-de Luccia (CDL) bubble-like configuration. Our results demonstrate how the bubble nucleation process could be described in the stochastic approach. Our method turns out to be useful for investigating various tunneling processes during inflation.
format Preprint
id arxiv_https___arxiv_org_abs_2309_07440
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Stochastic tunneling in de Sitter spacetime
Miyachi, Taiga
Soda, Jiro
Tokuda, Junsei
High Energy Physics - Theory
General Relativity and Quantum Cosmology
Tunneling processes in de Sitter spacetime are studied by using the stochastic approach. We exploit the Martin-Siggia-Rose-Janssen-de Dominicis (MSRJD) functional integral to obtain the tunneling rate. The applicability conditions of this method are clarified using the Schwinger-Keldysh formalism. In the case of a shallow potential barrier, we reproduce the Hawking-Moss (HM) tunneling rate. Remarkably, in contrast to HM picture, the configuration derived from the MSRJD functional integral satisfies physically natural boundary conditions. We also discuss the case of a steep potential barrier and find an interesting Coleman-de Luccia (CDL) bubble-like configuration. Our results demonstrate how the bubble nucleation process could be described in the stochastic approach. Our method turns out to be useful for investigating various tunneling processes during inflation.
title Stochastic tunneling in de Sitter spacetime
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2309.07440