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dc.contributor.author |
Nagasawa, M. |
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dc.date.accessioned |
2019-02-08T20:56:15Z |
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dc.date.available |
2019-02-08T20:56:15Z |
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dc.date.issued |
2010 |
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dc.identifier.citation |
Cosmological Symmetry Breaking and Generation of Electromagnetic Field / M. Nagasawa // Symmetry, Integrability and Geometry: Methods and Applications. — 2010. — Т. 6. — Бібліогр.: 21 назв. — англ. |
uk_UA |
dc.identifier.issn |
1815-0659 |
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dc.identifier.other |
2010 Mathematics Subject Classification: 83F05 |
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dc.identifier.other |
doi:10.3842/SIGMA.2010.053 |
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dc.identifier.uri |
http://dspace.nbuv.gov.ua/handle/123456789/146325 |
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dc.description.abstract |
Cosmological phase transitions accompanied by some kind of symmetry breaking would cause the creation of topological defects and the resulting production of primordial magnetic field. Moreover, such a procedure inevitably affects the cosmic background radiation and it may be observed today. Motivated by the existence of stabilized embedded defects in the standard model of elementary interactions, we discuss their application to the cosmological electromagnetic field generation. |
uk_UA |
dc.description.sponsorship |
This paper is a contribution to the Proceedings of the Eighth International Conference “Symmetry in Nonlinear Mathematical Physics” (June 21–27, 2009, Kyiv, Ukraine). The full collection is available at http://www.emis.de/journals/SIGMA/symmetry2009.html.
The numerical calculations were carried out on SX8 at YITP in Kyoto University. |
uk_UA |
dc.language.iso |
en |
uk_UA |
dc.publisher |
Інститут математики НАН України |
uk_UA |
dc.relation.ispartof |
Symmetry, Integrability and Geometry: Methods and Applications |
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dc.title |
Cosmological Symmetry Breaking and Generation of Electromagnetic Field |
uk_UA |
dc.type |
Article |
uk_UA |
dc.status |
published earlier |
uk_UA |
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