Published July 1987
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Chaotic universe dynamics using a Fokker-Planck equation
Description
A Fokker-Planck equation that accounts for fluctuations in field and its conjugate momentum is solved numerically for the case of a λ phi4 potential. Although the amount of inflation agrees closely with that expected classically, in certain cases (large initial fields or large dispersions),the ''slow rolling'' approximation appears invalid. In such cases inflation would stop prematurely before possibly restarting. 18 refs., 2 figs
Availability note (English)
Available from NTIS, PC A02/MF A01; 1 as DE87013481.Files
19015454.pdf
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Additional details
Publishing Information
- Imprint Pagination
- 15 p.
- Report number
- FNAL/Pub--87/116-A
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19015454
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- COSMOLOGICAL MODELS; DIFFUSION; FOKKER-PLANCK EQUATION; LINEAR MOMENTUM; NUMERICAL SOLUTION; THEORETICAL DATA
- Descriptors DEC
- DATA; DIFFERENTIAL EQUATIONS; EQUATIONS; INFORMATION; MATHEMATICAL MODELS; NUMERICAL DATA; PARTIAL DIFFERENTIAL EQUATIONS
Optional Information
- Notes
- Portions of this document are illegible in microfiche products.