Neutrino emission from dense matter containing meson condensates

V. Thorsson; M. Prakash; T. Tatsumi; C. J. Pethick

doi:10.1103/PhysRevD.52.3739

Neutrino emission from dense matter containing meson condensates

V. Thorsson
, M. Prakash
, T. Tatsumi
, C. J. Pethick

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

16 Scopus citations

Abstract

We consider the rate at which energy is emitted by neutrinos from the dense interior of neutron stars containing a Bose condensate of pions or kaons. The rates obtained are larger, by a factor of 2, than those found earlier, and are consistent with those found for the direct Urca processes.

Original language	English
Pages (from-to)	3739-3741
Number of pages	3
Journal	Physical Review D
Volume	52
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevD.52.3739
State	Published - 1995
Externally published	Yes

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10.1103/PhysRevD.52.3739

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title = "Neutrino emission from dense matter containing meson condensates",

abstract = "We consider the rate at which energy is emitted by neutrinos from the dense interior of neutron stars containing a Bose condensate of pions or kaons. The rates obtained are larger, by a factor of 2, than those found earlier, and are consistent with those found for the direct Urca processes.",

author = "V. Thorsson and M. Prakash and T. Tatsumi and Pethick, \{C. J.\}",

note = "Publisher Copyright: {\textcopyright} 1995 The American Physical Society",

year = "1995",

doi = "10.1103/PhysRevD.52.3739",

language = "English",

volume = "52",

pages = "3739--3741",

journal = "Physical Review D",

issn = "0556-2821",

publisher = "American Institute of Physics",

number = "6",

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TY - JOUR

T1 - Neutrino emission from dense matter containing meson condensates

AU - Thorsson, V.

AU - Prakash, M.

AU - Tatsumi, T.

AU - Pethick, C. J.

PY - 1995

Y1 - 1995

N2 - We consider the rate at which energy is emitted by neutrinos from the dense interior of neutron stars containing a Bose condensate of pions or kaons. The rates obtained are larger, by a factor of 2, than those found earlier, and are consistent with those found for the direct Urca processes.

AB - We consider the rate at which energy is emitted by neutrinos from the dense interior of neutron stars containing a Bose condensate of pions or kaons. The rates obtained are larger, by a factor of 2, than those found earlier, and are consistent with those found for the direct Urca processes.

UR - https://www.scopus.com/pages/publications/0000661761

U2 - 10.1103/PhysRevD.52.3739

DO - 10.1103/PhysRevD.52.3739

M3 - Article

AN - SCOPUS:0000661761

SN - 0556-2821

VL - 52

SP - 3739

EP - 3741

JO - Physical Review D

JF - Physical Review D

IS - 6

ER -

Neutrino emission from dense matter containing meson condensates

Abstract

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