Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation

A. Li; X. R. Zhou; G. F. Burgio; H. J. Schulze

doi:10.1103/PhysRevC.81.025806

Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation

A. Li, X. R. Zhou, G. F. Burgio, H. J. Schulze

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

33 Scopus citations

Abstract

We study the properties of hot neutrino-trapped β-stable stellar matter using an equation of state of nuclear matter within the Brueckner-Hartree-Fock approach including three-body forces, combined with a standard chiral model for kaon condensation at finite temperature. The properties of (proto)neutron stars are then investigated within this framework.

Original language	English
Article number	025806
Journal	Physical Review C - Nuclear Physics
Volume	81
Issue number	2
DOIs	https://doi.org/10.1103/PhysRevC.81.025806
State	Published - 18 Feb 2010
Externally published	Yes

Access to Document

10.1103/PhysRevC.81.025806

Cite this

@article{4fce8c394ecd459fbf68b74192074ee7,

title = "Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation",

abstract = "We study the properties of hot neutrino-trapped β-stable stellar matter using an equation of state of nuclear matter within the Brueckner-Hartree-Fock approach including three-body forces, combined with a standard chiral model for kaon condensation at finite temperature. The properties of (proto)neutron stars are then investigated within this framework.",

author = "A. Li and Zhou, \{X. R.\} and Burgio, \{G. F.\} and Schulze, \{H. J.\}",

year = "2010",

month = feb,

day = "18",

doi = "10.1103/PhysRevC.81.025806",

language = "英语",

volume = "81",

journal = "Physical Review C - Nuclear Physics",

issn = "0556-2813",

publisher = "American Physical Society",

number = "2",

}

TY - JOUR

T1 - Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation

AU - Li, A.

AU - Zhou, X. R.

AU - Burgio, G. F.

AU - Schulze, H. J.

PY - 2010/2/18

Y1 - 2010/2/18

N2 - We study the properties of hot neutrino-trapped β-stable stellar matter using an equation of state of nuclear matter within the Brueckner-Hartree-Fock approach including three-body forces, combined with a standard chiral model for kaon condensation at finite temperature. The properties of (proto)neutron stars are then investigated within this framework.

AB - We study the properties of hot neutrino-trapped β-stable stellar matter using an equation of state of nuclear matter within the Brueckner-Hartree-Fock approach including three-body forces, combined with a standard chiral model for kaon condensation at finite temperature. The properties of (proto)neutron stars are then investigated within this framework.

UR - https://www.scopus.com/pages/publications/77649152667

U2 - 10.1103/PhysRevC.81.025806

DO - 10.1103/PhysRevC.81.025806

M3 - 文章

AN - SCOPUS:77649152667

SN - 0556-2813

VL - 81

JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

IS - 2

M1 - 025806

ER -

Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation

Abstract

Access to Document

Other files and links

Fingerprint

Cite this