Classical Behaviour After a Phase Transition: II. The Formation of Classical Defects

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dc.creatorRivers, R. J.
dc.creatorLombardo, F. C.
dc.creatorMazzitelli, F. D.
dc.date2002-02-05
dc.date.accessioned2026-07-07T03:46:27Z
dc.date.available2026-07-07T03:46:27Z
dc.descriptionClassical defects (monopoles, vortices, etc.) are a characteristic consequence of many phase transitions of quantum fields. Most likely these include transitions in the early universe and such defects would be expected to be present in the universe today. We continue our analysis of the onset of classical behaviour after a second-order phase transition in quantum field theory and show how defects appear after such transitions
dc.description10 pages, no figures, to be published in the Proceedings of the Peyresq VI, Cosmological inflation and primordial fluctuations. Energy desert and submillimeter gravity, Peyresq, June 2001
dc.identifierhttps://arxiv.org/abs/hep-ph/0202041
dc.identifierhttp://arxiv.org/abs/hep-ph/0202041
dc.identifierInt.J.Theor.Phys. 41 (2002) 2145-2160
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/41296
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectCondensed Matter
dc.subjectQuantum Physics
dc.titleClassical Behaviour After a Phase Transition: II. The Formation of Classical Defects
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