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NASA NTRS · 19850039053

Supermassive monopole stars

Abstract

In 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.

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BibTeXRIS

Fry, J. N., Fuller, G. M.. 1984-11-15. Supermassive monopole stars. https://ntrs.nasa.gov/citations/19850039053

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