Prospects of detecting baryon and quark superfluidity from cooling neutron stars

Dany Page; Madappa Prakash; James M. Lattimer; Andrew W. Steiner

doi:10.1103/PhysRevLett.85.2048

Prospects of detecting baryon and quark superfluidity from cooling neutron stars

Dany Page
, Madappa Prakash
, James M. Lattimer
, Andrew W. Steiner

Physics and Astronomy

Universidad Nacional Autónoma de México
Stony Brook University

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

130 Scopus citations

Abstract

The superfluidity of baryon and quark in neutron stars cooling was studied. An invisible quark matter for cooling was produced by quark gaps in a hybrid star with a mixed hadron-quark phase. The quark gaps have to be larger than a few tenths of a MeV to produce significant results.

Original language	English
Pages (from-to)	2048-2051
Number of pages	4
Journal	Physical Review Letters
Volume	85
Issue number	10
DOIs	https://doi.org/10.1103/PhysRevLett.85.2048
State	Published - Sep 4 2000

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10.1103/PhysRevLett.85.2048

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title = "Prospects of detecting baryon and quark superfluidity from cooling neutron stars",

abstract = "The superfluidity of baryon and quark in neutron stars cooling was studied. An invisible quark matter for cooling was produced by quark gaps in a hybrid star with a mixed hadron-quark phase. The quark gaps have to be larger than a few tenths of a MeV to produce significant results.",

author = "Dany Page and Madappa Prakash and Lattimer, \{James M.\} and Steiner, \{Andrew W.\}",

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AU - Page, Dany

AU - Prakash, Madappa

AU - Lattimer, James M.

AU - Steiner, Andrew W.

PY - 2000/9/4

Y1 - 2000/9/4

N2 - The superfluidity of baryon and quark in neutron stars cooling was studied. An invisible quark matter for cooling was produced by quark gaps in a hybrid star with a mixed hadron-quark phase. The quark gaps have to be larger than a few tenths of a MeV to produce significant results.

AB - The superfluidity of baryon and quark in neutron stars cooling was studied. An invisible quark matter for cooling was produced by quark gaps in a hybrid star with a mixed hadron-quark phase. The quark gaps have to be larger than a few tenths of a MeV to produce significant results.

UR - https://www.scopus.com/pages/publications/0034274498

U2 - 10.1103/PhysRevLett.85.2048

DO - 10.1103/PhysRevLett.85.2048

M3 - Article

AN - SCOPUS:0034274498

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VL - 85

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EP - 2051

JO - Physical Review Letters

JF - Physical Review Letters

IS - 10

ER -

Prospects of detecting baryon and quark superfluidity from cooling neutron stars

Abstract

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