Superfluid ³He in the zero temperature limit (Review Article)

dc.contributor.author	Pickett, G.R.
dc.date.accessioned	2021-01-31T16:59:56Z
dc.date.available	2021-01-31T16:59:56Z
dc.date.issued	1997
dc.identifier.citation	Superfluid ³He in the zero temperature limit (Review Article) / G.R. Pickett // Физика низких температур. — 1997. — Т. 23, № 5-6. — С. 499-508. — Бібліогр.: 12 назв. — англ.	uk_UA
dc.identifier.issn	0132-6414
dc.identifier.other	PACS: 67.50.FI
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/175282
dc.description.abstract	In this paper we discuss some (and only a small fraction) of the interesting properties of superfluid ³He at the low-temperature limit. We concentrate on the unique behavior and applications of the very dilute excitation gas at the lowest temperatures. This gas has been used for among other things, the probing of the A–B phase interface, the detection of low-energy particle events and in the simulation of the creation of cosmic strings.	uk_UA
dc.description.sponsorship	We would like to acknowledge all the members of the Lancaster group who have contributed to our work over the years, including especially: Ian Bradley, Yuri Bunkov, Derek Cousins, Mike Enrico, Shaun Fisher, Mike Follows, Tony Guenault, Will Hayes, Chris Kennedy, Simon Phillipson, Neil Shaw, Terry Sloan, Pierre Thibault, and Кiyoshi Torizuka, and also the Grenoble group of Christopher Bauerle, Yuri Bunkov, Shaun Fisher, and Henri Godfrin who made the cosmic strings experiment described above.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України	uk_UA
dc.relation.ispartof	Физика низких температур
dc.title	Superfluid ³He in the zero temperature limit (Review Article)	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA