Thermal production of superheavy magnetic monopoles in the new inflationary-Universe scenario

Collins, William ORCID: https://orcid.org/0000-0002-4463-9848 and Turner, Michael S. (1984) Thermal production of superheavy magnetic monopoles in the new inflationary-Universe scenario. Physical Review D, 29 (10). pp. 2158-2161. ISSN 0556-2821

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Abstract

In the new inflationary-Universe scenario monopoles are created in rare, very energetic particle collisions, and their predicted abundance, which is exp(-2m0TRH), is tiny, where m0=monopole mass, TRH=reheat temperature. During the reheating process the effective monopole mass oscillates about m0 as the vacuum expectation value of the scalar field oscillates about the symmetry-breaking minimum of the scalar potential. We find that owing to this effect monopole production is greatly increased, with 2m0TRH being replaced by 2f*m0TRH, where 0<f*<1 depends upon the form of the scalar potential and the details of reheating.

Item Type: Article
Uncontrolled Keywords: physics and astronomy (miscellaneous) ,/dk/atira/pure/subjectarea/asjc/3100/3101
Faculty \ School: Faculty of Science > School of Environmental Sciences
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Depositing User: LivePure Connector
Date Deposited: 07 Jul 2026 13:16
Last Modified: 08 Jul 2026 14:34
URI: https://ueaeprints.uea.ac.uk/id/eprint/103760
DOI: 10.1103/PhysRevD.29.2158

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