Modelling the dynamics of superfluid neutron stars

被引:0
作者
N. Andersson
机构
[1] University of Southampton,School of Mathematics
来源
Astrophysics and Space Science | 2007年 / 308卷
关键词
Neutron stars; Superfluids; Dissipation;
D O I
暂无
中图分类号
学科分类号
摘要
In this brief summary I describe our recent work on superfluid neutron star dynamics. I review results on shear viscosity, hyperon bulk viscosity, vortex mediated mutual friction and the modelling of multifluid systems in general. For each problem I provide a set of questions that need to be addressed by future work.
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页码:395 / 402
页数:7
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共 44 条
[1]  
Alpar M.A.(1988)undefined Astrophys. J. 327 723-725
[2]  
Sauls J.A.(1984)undefined Astrophys. J. 282 533-541
[3]  
Alpar M.A.(2006)undefined Class. Quantum Grav. 23 5505-110
[4]  
Langer S.A.(2004)undefined Mon. Not. Roy. Astron. Soc. 354 101-229
[5]  
Sauls J.A.(2005)undefined Nucl. Phys. A 763 212-170
[6]  
Andersson N.(2006)undefined Mon. Not. Roy. Astron. Soc. 368 162-241
[7]  
Comer G.L.(2006)undefined Class. Quantum Grav. 23 5367-348
[8]  
Andersson N.(1987)undefined Astrophys. J. 314 234-809
[9]  
Comer G.L.(2006)undefined Mon. Not. Roy. Astron. Soc. Lett. 371 L74-1232
[10]  
Prix R.(2005)undefined Nucl. Phys. A 761 333-637