P-wave superfluidity in neutron stars and 3He

J. A. Sauls; D. L. Stein

doi:10.1016/0378-4363(81)90334-X

P-wave superfluidity in neutron stars and ³He

J. A. Sauls, D. L. Stein

Research output: Contribution to journal › Article › peer-review

Abstract

We discuss some of the similarities and differences between p-wave pairing in ³He and the ³P₂ neutron superfluid that is believed to exist in the interiors of neutron stars. The structure of vortices in the ³P₂ neutron superfluid is particularly interesting and is relevant to the astrophysics of pulsars.

Original language	English (US)
Pages (from-to)	55-56
Number of pages	2
Journal	Physica B+C
Volume	107
Issue number	1-3
DOIs	https://doi.org/10.1016/0378-4363(81)90334-X
State	Published - 1981

ASJC Scopus subject areas

General Engineering

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10.1016/0378-4363(81)90334-X

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title = "P-wave superfluidity in neutron stars and 3He",

abstract = "We discuss some of the similarities and differences between p-wave pairing in 3He and the 3P2 neutron superfluid that is believed to exist in the interiors of neutron stars. The structure of vortices in the 3P2 neutron superfluid is particularly interesting and is relevant to the astrophysics of pulsars.",

author = "Sauls, {J. A.} and Stein, {D. L.}",

note = "Funding Information: Part of this work was done in collaboration with Paul Muzikar and J.W. Serene. Research was supported in part by NSF DMR 802063 .",

year = "1981",

doi = "10.1016/0378-4363(81)90334-X",

language = "English (US)",

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pages = "55--56",

journal = "Physica B+C",

issn = "0378-4363",

publisher = "North-Holland Publ Co",

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T1 - P-wave superfluidity in neutron stars and 3He

AU - Sauls, J. A.

AU - Stein, D. L.

N1 - Funding Information: Part of this work was done in collaboration with Paul Muzikar and J.W. Serene. Research was supported in part by NSF DMR 802063 .

PY - 1981

Y1 - 1981

N2 - We discuss some of the similarities and differences between p-wave pairing in 3He and the 3P2 neutron superfluid that is believed to exist in the interiors of neutron stars. The structure of vortices in the 3P2 neutron superfluid is particularly interesting and is relevant to the astrophysics of pulsars.

AB - We discuss some of the similarities and differences between p-wave pairing in 3He and the 3P2 neutron superfluid that is believed to exist in the interiors of neutron stars. The structure of vortices in the 3P2 neutron superfluid is particularly interesting and is relevant to the astrophysics of pulsars.

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U2 - 10.1016/0378-4363(81)90334-X

DO - 10.1016/0378-4363(81)90334-X

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VL - 107

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EP - 56

JO - Physica B+C

JF - Physica B+C

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ER -

P-wave superfluidity in neutron stars and ³He

Abstract

ASJC Scopus subject areas

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