How probable is inflation?
Jun, 198721 pages
Published in:
- Nucl.Phys.B 298 (1988) 789-809
- Published: 1988
Report number:
- Print-87-0739 (PENN STATE)
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Abstract: (Elsevier)
The Henneaux-Gibbons-Hawking-Stewart canonical measure on the set of classical universes is applied to a Friedmann-Robertson-Walker model containing a massive scalar field. Although a uniform probability distribution in this measure would solve the flatness problem, it gives an ambiguous probability for inflation, since both the set of inflationary solutions and the set of noninflationary solutions have infinite measure.- MODEL: INFLATION
- FIELD THEORY: SCALAR
- FIELD EQUATIONS: SOLUTION
- FIELD THEORY: HAMILTONIAN FORMALISM
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