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We investigate the quantum hadrodynamic equation of state for neutron stars (with and without including hyperons) in the presence of strong magnetic fields.
We deduce approximate equations of state from experimental measurements in proton-proton and proton-antiproton collisions.
We employ the lattice QCD data on Taylor expansion coefficients to extend our previous parametrization of the equation of state to finite baryon density.
We conclude our investigation on the QCD equation of state (EoS) with 2+1 staggered flavors and one-link stout improvement. We extend our previous study [JHEP 0601:089 (2006)] by choosing even finer l...
Using a global equation of state, empirically derived by Luding, we ac-curately model the density profile of a two-dimensional hard sphere system with diameter D and mass m under gravity with a given ...
We study the cosmological evolutions of the equation of state for dark energy wDE in the expo- nential and logarithmic as well as their combination f(T) theories. We show that the crossing of the pha...
We consider FLRW cosmological models with standard Friedmann equations, but leaving free the equation of state. We assume that the dark energy content of the universe is encoded in an equation of stat...
Following the basic prescriptions of the Tsallisnonextensive relativistic thermodynamics, we investigate the relevance of nonextensive statistical effects on the relativistic nuclear and subnuclear ...
We study the hadron-quark phase transition in the interior of neutron stars, and examine the influence of the nuclear equation of state on the phase transition and neutron star properties. The relativ...
We have conducted new equation of state measurements on liquid Fe2SiO4 in a collaborative, multi-technique study. The liquid density (r), the bulk modulus (K), and its pressure derivative (K′) were ...
We have conducted new equation of state measurements on liquid Fe2SiO4 in a collaborative, multi-technique study. The liquid density (r), the bulk modulus (K), and its pressure derivative (K′) were ...
2001Vol.36No.1pp.65-70DOI: The Influence of the Renormalization Condition to the Equation of State of the Nuclear Matter CHEN Wei, AI Bao-Quan, ZHENG Xiao-Ping and LIU Liang-Gan...
2007Vol.47No.6pp.1148-1152DOI: Reconstructing Equation of State for Dark Energy in Double Complex Symmetric Gravitational Theory SHAO Ying, GUI Yuan-Xing, and WANG Wei D...
2007Vol.47No.2pp.379-384DOI: Friedmann Cosmology with a Generalized Equation of State and Bulk Viscosity MENG Xin-He, REN Jie, and HU Ming-Guang Department of Physics, N...
2006Vol.45No.5pp.901-905DOI: Equation of State of Protoneutron Star with Trapped Neutrinos ZHANG Hua and JIA Huan-Yu Institute of Modern Physics, Southwest Jiaotong Univ...

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