Rotating twin stars and signature of quark-hadron phase transition

被引：21

作者：

Bhattacharyya, A

Ghosh, SK

Hanauske, M

Raha, S

机构：

[1] Scottish Church Coll, Dept Phys, Kolkata 700006, India

[2] Bose Inst, Dept Phys, Kolkata 700009, W Bengal, India

[3] Goethe Univ Frankfurt, Inst Theoret Phys, D-60054 Frankfurt, Germany

来源：

PHYSICAL REVIEW C | 2005年 / 71卷 / 04期

关键词：

D O I：

10.1103/PhysRevC.71.048801

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

The quark-hadron phase transition in a rotating compact star has been studied. The NLZ (nonlinear consistent zero point energy) model has been used for the hadronic sector and the MIT bag model has been used for the quark sector. It has been found that rotating twin star (third family) solutions are obtained up to Omega approximate to 4000 s(-1). Stars that are rotating faster than this limit do not show twin star solution. A backbending in the moment of inertia is also observed in the supermassive rest mass sequences. The braking index is found to diverge for a star having a larger region of mixed phase.

引用

页数：4

共 18 条

[1] Electromagnetic probes of quark gluon plasma [J].