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相关论文: Quark Stars in Chiral Colour Dielectric Model

200 篇论文

We investigate the properties of quark matter at finite density and temperature using the nonlinear chiral extension of Colour Dielectric Model (CCM). Assuming that the square of the meson fields devlop non- zero vacuum expectation value,…

核理论 · 物理学 2008-11-26 Sanjay K. Ghosh , S. C. Phatak

The properties of rotating quark star is studied using the equation of state obtained from Chiral Colour Dielectric model. The results are compared with the MIT bag model results. The frequencies in the corotating innermost circular orbits…

天体物理学 · 物理学 2008-11-26 Abhijit Bhattacharyya , Sanjay K. Ghosh

In the contact interaction model, the quark propagator has only one solution, chiral symmetry breaking solution, at vanish temperature and density. Inspire by Y. Jiang and Z.-F. Cui, we introduce 2+1 flavors quark condensates feedback on…

高能物理 - 唯象学 · 物理学 2021-10-15 Shu-Sheng Xu

Equations of state for strange quark matter in beta equilibrium at high densities are used to investigate the structure (mass and radius) of compact objects. The chromodielectric model is used as a general framework for the quark…

高能物理 - 唯象学 · 物理学 2009-11-07 M. Malheiro , E. O. Azevedo , L. G. Nuss , M. Fiolhais , A. R. Taurines

A quark-cluster state, rather than the color-super-conductivity state, may appear in matter with low-temperature but high density, since the phase transition of chiral symmetry broken and that of color-confinement could not occur…

天体物理学 · 物理学 2007-05-23 Weiwei Zhu , Renxin Xu

We review our quasiparticle model for the thermodynamics of strongly interacting matter at high temperature, and its extrapolation to non-zero chemical potential. Some implications of the resulting soft equation of state of quark matter at…

高能物理 - 唯象学 · 物理学 2009-09-29 A. Peshier , B. Kampfer , G. Soff

As is pointed out in a recent work (Phys. Rev. Lett. 120, 222001), quark matter may not be strange. Inspired by this argument, we use a new self-consistent mean field approximation method to study the equation of state of cold dense matter…

核理论 · 物理学 2019-08-26 Tong Zhao , Wei Zheng , Fei Wang , Cheng-Ming Li , Yan Yan , Yong-Feng Huang , Hong-Shi Zong

We study the equation of state (EOS) of quark matter at zero temperature, using the Color Dielectric Model (CDM) to describe confinement. Sensible results are obtained in the version of the CDM for which confinement is imposed {\it…

高能物理 - 唯象学 · 物理学 2019-08-17 Alessandro Drago , Manuel Fiolhais , Ubaldo Tambini

We investigate the properties of hybrid stars consisting of quark matter in the core and hadron matter in outer region. The hadronic and quark matter equations of state are calculated by using nonlinear Walecka model and chiral colour…

核理论 · 物理学 2015-06-26 Sanjay K. Ghosh , S. C. Phatak , Pradip K. Sahu

Following our recenty proposed self-consistent mean-field approximation approach, we have done some researches on the chiral phase transition of strong interaction matter within the framework of Nambu-Jona-Lasinio (NJL) model. The chiral…

高能物理 - 唯象学 · 物理学 2020-09-22 Qianyi Wang , Tong Zhao , Hongshi Zong

In this paper, the equation of state (EOS) of deconfined quark stars is studied in the framework of the two-flavor NJL model, and the self-consistent mean field approximation is employed by introducing a parameter $\alpha$ combining the…

核理论 · 物理学 2021-05-11 Li-Qun Su , Yan Yan , Cheng-Ming Li , Yong-Feng Huang , Hongshi Zong

The equation of state for quark matter is derived for a nonlocal, chiral quark model within the mean field approximation. Special emphasis is on the occurrence of a diquark condensate which signals a phase transition to color…

天体物理学 · 物理学 2009-11-07 H. Grigorian , D. Blaschke , D. N. Aguilera

Recent finite-temperature QCD lattice data are analyzed within a quasiparticle model, and extrapolated to nonzero chemical potential. Determined by the chiral transition temperature, the resulting equation of state of charge neutral,…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Peshier , B. Kampfer , G. Soff

We investigate the extension to finite temperatures and neutrino chemical potentials of a recently developed nonlocal chiral quark model approach to the equation of state of neutron star matter. We consider two light quark flavors and…

核理论 · 物理学 2024-03-05 J. P. Carlomagno , G. A. Contrera , A. G. Grunfeld , D. Blaschke

The properties of strange quark stars are studied within the quasi-particle model. Taking into account the chemical equilibrium and charge neutrality, the EOS of $ (2+1) $-flavor quark matter is obtained. We illustrate the parameter spaces…

高能物理 - 唯象学 · 物理学 2020-11-10 Wen-Hua Cai , Qing-Wu Wang

We investigate the properties of dense quark matter and strange quark stars within a nonperturbative, Poincar\'e-covariant framework. Employing a symmetry-preserving vector$\,\otimes\,$vector contact interaction model, we extend the quark…

核理论 · 物理学 2026-04-23 Hao-Ran Zhang , Bo-Lin Li , Zhu-Fang Cui

We investigate the properties of non-rotating, electrically charged strange quark stars in four-dimensional Einstein-Maxwell theory. For quark matter we adopt the well-motivated quantum chromodynamics (QCD) equation-of-state, while for the…

广义相对论与量子宇宙学 · 物理学 2022-05-04 Grigoris Panotopoulos , Takol Tangphati , Ayan Banerjee

In this paper we apply the equation of state (EOS) of QCD at finite chemical potential and zero temperature proposed in H. S. Zong and W. M. Sun [Int. J. Mod. Phys. {\bf A23}, 3591 (2008)] to the study of properties of quark star. This EOS…

高能物理 - 唯象学 · 物理学 2015-03-17 Hua Li , Xin-Lian Luo , Yu Jiang , Hong-Shi Zong

The equation of state for quark matter is derived for a nonlocal, chiral quark model within the mean field approximation.We investigate the effects of a variation of the formfactors of the interaction on the phase diagram of quark matter.…

核理论 · 物理学 2009-11-10 D. Blaschke , S. Fredriksson , H. Grigorian , A. M. "Oztas

We study the thermodynamics of two flavor color superconducting (2SC) quark matter within a nonlocal chiral quark model, using both instantaneous and covariant nonlocal interactions. For applications to compact stars, we impose conditions…

高能物理 - 唯象学 · 物理学 2008-11-26 A. G. Grunfeld , J. Berdermann , D. B. Blaschke , T. Klahn , D. Gomez Dumm , N. N. Scoccola
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