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Big-Bang Model Without Singularities

Murphy, George L.·1973·Physical Review D

Abstract

A uniform cosmological model filled with fluid which possesses pressure and second viscosity is developed. The Einstein equations can be integrated exactly. One solution is the steady-state cosmology, but this is unstable. Other solutions start from the steady-state one in the infinite past but expand more and more slowly as viscosity dies out. At any finite proper time in the past the curvature is finite. Some comments on possible origins of this viscosity are given.

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Metadata

Authors
Murphy, G. L.
Venue
Physical Review D
Published
1973-12-15
Volume
8
Issue
12
Pages
4231-4233
ISSN
0556-2821 (ISSN-L)
OpenAlex
W2160215509
Cited by
542
References
0
FWCI
1.63
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Big-Bang Model Without Singularities. https://app.cochat.ai/papers/10.1103/physrevd.8.4231
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Murphy, G. L. (1973). Big-Bang Model Without Singularities. Physical Review D. https://doi.org/10.1103/physrevd.8.4231

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