GLUON CONDENSATES, QUARK MATTER EQUATION OF STATE AND QUARK STARS

被引：4

作者：

MISHRA, A ^{[1
]}

MISHRA, H ^{[1
]}

PANDA, PK ^{[1
]}

MISRA, SP ^{[1
]}

机构：

[1] INST PHYS,BHUBANESWAR 751005,INDIA

来源：

ZEITSCHRIFT FUR PHYSIK C-PARTICLES AND FIELDS | 1994年 / 63卷 / 04期

关键词：

D O I：

10.1007/BF01557635

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We consider here quark matter equation of state including strange quarks and taking into account a nontrivial vacuum structure for QCD with gluon condensates. The parameters of condendsate function are determined from minimisation of the thermodynamic potential. The scale parameter of the gluon condensates is fixed from the SVZ parameter in the context of QCD sum rules at zero temperature and zero baryon density. The equation of state for strange matter at zero temperature as derived is used to study quark star structure using Tolman Oppenheimer Volkoff equations. Stable solutions for quark stars are obtained with a large Chandrasekhar limit as 3.2 M. and radii around 17 kms.

引用

页码：681 / 688

页数：8

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