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dc.contributor.author | Bunkov Y. | |
dc.contributor.author | Golov A. | |
dc.contributor.author | L'Vov V. | |
dc.contributor.author | Pomyalov A. | |
dc.contributor.author | Procaccia I. | |
dc.date.accessioned | 2018-09-18T20:21:07Z | |
dc.date.available | 2018-09-18T20:21:07Z | |
dc.date.issued | 2014 | |
dc.identifier.issn | 1098-0121 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/138991 | |
dc.description.abstract | A nuclear capture reaction of a single neutron by ultracold superfluid He3 results in a rapid overheating followed by the expansion and subsequent cooling of the hot subregion, in a certain analogy with the big bang of the early universe. It was shown in a Grenoble experiment that a significant part of the energy released during the nuclear reaction was not converted into heat even after several seconds. It was thought that the missing energy was stored in a tangle of quantized vortex lines. This explanation, however, contradicts the expected lifetime of a bulk vortex tangle, 10-5-10-4 s, which is much shorter than the observed time delay of seconds. In this paper we propose a scenario that resolves the contradiction: the vortex tangle, created by the hot spot, emits isolated vortex loops that take with them a significant part of the tangle's energy. These loops quickly reach the container walls. The dilute ensemble of vortex loops attached to the walls can survive for a long time, while the remaining bulk vortex tangle decays quickly. © 2014 American Physical Society. | |
dc.relation.ispartofseries | Physical Review B - Condensed Matter and Materials Physics | |
dc.title | Evolution of a neutron-initiated micro big bang in superfluid He 3 -B | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 2 | |
dc.relation.ispartofseries-volume | 90 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS10980121-2014-90-2-SID84904369058 |