Published July 1987 | Version v1
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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.

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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.