Published September 1, 2018
| Version v1
Journal article
Tunneling in stochastic inflation
Creators
- 1. Department of Physics, University of Tehran, P.O. Box 14395-547 (Iran, Islamic Republic of)
- 2. Laboratoire Astroparticule et Cosmologie, Université Denis Diderot Paris 7, 10 rue Alice Domon et Léonie Duquet, 75013 Paris (France)
- 3. Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth, PO1 3FX (United Kingdom)
- 4. School of Astronomy, Institute for Research in Fundamental Sciences (IPM), Tehran, P.O. Box 19395-5531 (Iran, Islamic Republic of)
Description
The relative probability to decay towards different vacua during inflation is studied. The calculation is performed in single-field slow-roll potentials using the stochastic inflation formalism. Various situations are investigated, including falling from a local maximum of the potential and escaping from a local minimum. In the latter case, our result is consistent with that of Hawking and Moss, but is applicable to any potential. The decay rates are also computed, and the case of a generic potential with multiple minima and maxima is discussed.
Availability note (English)
Available from http://dx.doi.org/10.1088/1475-7516/2018/09/032Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Cosmology and Astroparticle Physics
- Journal Volume
- 2018
- Journal Issue
- 09
- Journal Page Range
- p. 032
- ISSN
- 1475-7516
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 51057447
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMOLOGICAL INFLATION; PROBABILITY; STOCHASTIC PROCESSES; TUNNEL EFFECT; VACUUM STATES