Evolution of proto-neutron stars with quarks

J. A. Pons; A. W. Steiner; M. Prakash; J. M. Lattimer

doi:10.1103/PhysRevLett.86.5223

Evolution of proto-neutron stars with quarks

J. A. Pons
, A. W. Steiner
, M. Prakash
, J. M. Lattimer

Physics and Astronomy

Stony Brook University

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

139 Scopus citations

Abstract

The general relativistic transport and hydrostatic equations were solved to obtain the benchmark calculation with quarks. The observations in current and planned detectors were used to study metastability in proto-neutron (PNS) stars and the subsequent collapse of the star to a black hole. The results showed that stars with quarks depicted metastability intermediate time scales between those containing hyperons and kaon condensates.

Original language	English
Pages (from-to)	5223-5226
Number of pages	4
Journal	Physical Review Letters
Volume	86
Issue number	23
DOIs	https://doi.org/10.1103/PhysRevLett.86.5223
State	Published - Jun 4 2001

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10.1103/PhysRevLett.86.5223

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title = "Evolution of proto-neutron stars with quarks",

abstract = "The general relativistic transport and hydrostatic equations were solved to obtain the benchmark calculation with quarks. The observations in current and planned detectors were used to study metastability in proto-neutron (PNS) stars and the subsequent collapse of the star to a black hole. The results showed that stars with quarks depicted metastability intermediate time scales between those containing hyperons and kaon condensates.",

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AU - Pons, J. A.

AU - Steiner, A. W.

AU - Prakash, M.

AU - Lattimer, J. M.

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Y1 - 2001/6/4

N2 - The general relativistic transport and hydrostatic equations were solved to obtain the benchmark calculation with quarks. The observations in current and planned detectors were used to study metastability in proto-neutron (PNS) stars and the subsequent collapse of the star to a black hole. The results showed that stars with quarks depicted metastability intermediate time scales between those containing hyperons and kaon condensates.

AB - The general relativistic transport and hydrostatic equations were solved to obtain the benchmark calculation with quarks. The observations in current and planned detectors were used to study metastability in proto-neutron (PNS) stars and the subsequent collapse of the star to a black hole. The results showed that stars with quarks depicted metastability intermediate time scales between those containing hyperons and kaon condensates.

UR - https://www.scopus.com/pages/publications/0035805896

U2 - 10.1103/PhysRevLett.86.5223

DO - 10.1103/PhysRevLett.86.5223

M3 - Article

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VL - 86

SP - 5223

EP - 5226

JO - Physical Review Letters

JF - Physical Review Letters

IS - 23

ER -

Evolution of proto-neutron stars with quarks

Abstract

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