Cooling of neutron stars. Hadronic model

被引：99

作者：

Blaschke, D

Grigorian, H

Voskresensky, DN

机构：

[1] Univ Rostock, Fachbereich Phys, D-18051 Rostock, Germany

[2] Joint Inst Nucl Res, Bogoliubov Lab Theoret Phys, Dubna 141980, Russia

[3] Univ Bielefeld, Fak Phys, D-33615 Bielefeld, Germany

[4] Yerevan State Univ, Dept Phys, Yerevan 375025, Armenia

[5] Gesell Schwerionenforsch mbH, D-64291 Darmstadt, Germany

[6] Moscow Inst Phys & Engn, Moscow 115409, Russia

来源：

ASTRONOMY & ASTROPHYSICS | 2004年 / 424卷 / 03期

关键词：

dense matter; equation of state; neutrinos; stars : evolution; stars : neutron; stars : pulsars : general;

D O I：

10.1051/0004-6361:20040404

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study the cooling of isolated neutron stars. The main cooling regulators are introduced: equation of state (EoS), thermal transport, heat capacity, neutrino and photon emissivity, superfluid nucleon gaps. The neutrino emissivity includes the main processes. A strong impact of medium effects on the cooling rates is demonstrated. Taking into account medium effects on reaction rates and on nucleon superfluid gaps modern experimental data can be well explained.

引用

页码：979 / 992

页数：14

共 61 条

[1] Equation of state of nucleon matter and neutron star structure [J].

Akmal, A ;

Pandharipande, VR ;

Ravenhall, DG .

PHYSICAL REVIEW C, 1998, 58 (03) :1804-1828

[2]

[Anonymous], BLACK HOLES WHITE DW

[3]

[Anonymous], 1960, SOV PHYS JETP-USSR

[4]

BAHCALL JN, 1965, PHYS REV, V140, P1445

[5] Thermal conductivity of neutrons in neutron star cores [J].

Baiko, DA ;

Haensel, P ;

Yakovlev, DG .

ASTRONOMY & ASTROPHYSICS, 2001, 374 (01) :151-163

[6] Diquark condensates and compact star cooling [J].

Blaschke, D ;

Klähn, T ;

Voskresensky, DN .

ASTROPHYSICAL JOURNAL, 2000, 533 (01) :406-412

[7] Cooling of hybrid neutron stars and hypothetical self-bound objects with superconducting quark cores [J].

Blaschke, D ;

Grigorian, H ;

Voskresensky, DN .

ASTRONOMY & ASTROPHYSICS, 2001, 368 (02) :561-568

[8] NUCLEAR IN-MEDIUM EFFECTS AND NEUTRINO EMISSIVITY OF NEUTRON-STARS [J].

BLASCHKE, D ;

ROPKE, G ;

SCHULZ, H ;

SEDRAKIAN, AD ;

VOSKRESENSKY, DN .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1995, 273 (03) :596-602

[9] STRANGENESS CONDENSATION AND COOLING OF NEUTRON STARS [J].

BROWN, GE ;

KUBODERA, K ;

PAGE, D ;

PIZZOCHERO, P .

PHYSICAL REVIEW D, 1988, 37 (08) :2042-2046

[10]

Ericson TEO, 1988, PIONS NUCL

← 1 2 3 4 5 6 7 →