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相关论文: Quark matter nucleation in hot hadronic matter

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A qualitative analysis of the chiral phase transition in QCD with two massless quarks and non--zero baryon density is performed. It is assumed that at zero baryonic density, $\rho=0$, the temperature phase transition is of the second order.…

高能物理 - 唯象学 · 物理学 2016-11-23 M. N. Chernodub , B. L. Ioffe

We analyze the effect of color superconductivity in the transition from hot hadron matter to quark matter in the presence of a gas of trapped electron neutrinos. We adopt a two-phase picture in which the hadronic phase is described trough a…

核理论 · 物理学 2013-07-30 Taiza A. S. do Carmo , Germán Lugones

Quark matter may appear due to a hadronic-quark transition in the core of a hybrid star. Quarkyonic matter is an approach in which both quarks and nucleons appear as quasi-particles in a crossover transition, and provides an explicit…

高能天体物理现象 · 物理学 2020-07-22 Tianqi Zhao , James M. Lattimer

Different extensions of the Nambu-Jona-Lasinio model, known to satisfy expected QCD chiral symmetry aspects, are used to investigate a possible hadron-quark phase transition at zero temperature and to build the corresponding binodal…

高能天体物理现象 · 物理学 2019-01-16 Clebson A. Graeff , Marcelo D. Alloy , Kauan D. Marquez , Constança Providência , Débora P. Menezes

During the last years it has become possible to address the cold and dense regime of QCD directly for sufficiently heavy quarks, where combined strong coupling and hopping expansions are convergent and a 3d effective theory can be derived,…

高能物理 - 格点 · 物理学 2018-12-06 Owe Philipsen , Jonas Scheunert

We investigate the phase transition to a deconfined phase and the consequences in the formation of neutron stars. We use the recently proposed effective field theory motivated relativistic mean field theory for hadron and the MIT Bag model…

核理论 · 物理学 2008-11-26 B. K. Sharma , P. K. Panda , S. K. Patra

With combined hopping parameter and strong coupling expansions, we calculate a dimensionally reduced Polyakov-loop effective theory valid for heavy quarks at nonzero temperature and arbitrary chemical potential. We numerically compute the…

高能物理 - 格点 · 物理学 2015-06-11 Michael Fromm , Jens Langelage , Stefano Lottini , Mathias Neuman , Owe Philipsen

Our quasi-particle model for deconfined matter near T_c is reviewed. The extrapolation of lattice QCD data to a finite baryo-chemical potential is discussed. Determined by the chiral transition temperature T_c, the resulting equation of…

高能物理 - 唯象学 · 物理学 2017-08-23 B. Kampfer , A. Peshier , G. Soff

The properties of baryonic matter have been investigated at finite density and temperature using different models. The variation of baryon masses and fractional number densities with baryon density and temperature obtained from different…

核理论 · 物理学 2014-11-18 Abhijit Bhattacharyya , Sanjay K. Ghosh

The up-dated three-phase concept of nuclear matter evolution in course of cooling down - from the phase of quark-qluon plasma (QGP) through the intermediate phase allowing for massive constituent quarks (valons), pions and kaons (QPK) to…

高能物理 - 唯象学 · 物理学 2007-05-23 O. D. Chernavskaya , I. I. Royzen

The cooling of compact isolated objects for different values of the gravitational mass has been simulated for two alternative assumptions. One is that the interior of the star is purely hadronic and second that the star can have a rather…

天体物理学 · 物理学 2009-11-10 H. Grigorian

The three phase transitions - the GUT, the electro-weak and the quark-hadron, which the universe is assumed to have undergone produce very important physical effects if they are assumed to be of first order. It is also important that enough…

天体物理学 · 物理学 2015-06-24 B. Banerjee , R. V. Gavai

For the past 20 years it had been thought that the coexistence phase of the confined hadronic and quark matter phases, assumed to be a first order transition, was strictly excluded from neutron stars. This, however, was due to a seemingly…

天体物理学 · 物理学 2007-05-23 Fridolin Weber , Norman K. Glendenning , Shouyong Pei

Central nuclear collisions at energies far above 1 GeV/nucleon may provide for conditions, where the transition from highly excited hadronic matter into quark matter or quark-gluon plasma can be probed. Here I review our current…

核理论 · 物理学 2009-10-22 Berndt Mueller

Based on hot big bang theory, the cosmological matter is conjectured to undergo QCD phase transition(s) to hadrons, when the universe was about $1-10 \mu$s old. In the present work, we study the quark-hadron phase transition, by taking into…

宇宙学与河外天体物理 · 物理学 2012-04-26 A. Tawfik , T. Harko

We review the results of a phenomenological model for cold and dense nuclear matter exhibiting a chiral phase transition. The idea is to model the quark-hadron phase transition under neutron star conditions within a single model, but…

核理论 · 物理学 2022-11-30 Eduardo S. Fraga , Rodrigo da Mata , Savvas Pitsinigkos , Andreas Schmitt

The effect of strong quantizing magnetic field on the nucleation of quark matter droplets and on the chemical evolution of nascent quark phase at the core of a neutron star are investigated. The surface energy of quark phase diverges…

天体物理学 · 物理学 2009-10-31 Tanusri Ghosh , Somenath Chakrabarty

Hot hypernuclear matter is investigated in an explicit SU(3) quark model based on a mean field description of nonoverlapping baryon bags bound by the self-consistent exchange of scalar $\sigma, \zeta$ and vector $\omega, \phi$ mesons. The…

核理论 · 物理学 2009-10-31 I. Zakout , H. R. Jaqaman , S. Pal , H. Stöcker , W. Greiner

Quark-hadron phase transition in QCD in the presence of magnetic field is studied. It is shown that both the temperature of a phase transition and latent heat decrease compared to the case of zero magnetic field. The phase diagram in the…

高能物理 - 唯象学 · 物理学 2008-11-26 N. O. Agasian , S. M. Fedorov

We analyze the different possibilities for the hadron-quark phase transition occurring in beta-stable matter including hyperons in neutron stars. We use a Brueckner-Hartree-Fock approach including hyperons for the hadronic equation of state…

核理论 · 物理学 2008-11-26 Toshiki Maruyama , Satoshi Chiba , Hans-Josef Schulze , Toshitaka Tatsumi
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