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 |
|