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Supermassive monopole starsIn this paper, the evolution of a superheavy monopole-dominated universe is reexamined; in particular, the evolution of rotation-stabilized monopole-burning 'stars', balancing effects of radiation and annihilation are examined. In contrast to earlier results, it is found that this can lead to complete burning of all poles present in such an object within finite time. If monopoles can be brought within acceptable limits by dynamical processes, an inflationary epoch of the early universe need not be associated with grand unification.
Document ID
19850039053
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Fry, J. N.
(Chicago Univ. Chicago, IL, United States)
Fuller, G. M.
(Chicago, University Chicago, IL, United States)
Date Acquired
August 12, 2013
Publication Date
November 15, 1984
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 286
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
85A21204
Funding Number(s)
CONTRACT_GRANT: NSG-7212
CONTRACT_GRANT: DE-AC02-80ER-10773-A003
CONTRACT_GRANT: NSF AST-81-16750
Distribution Limits
Public
Copyright
Other

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