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Quark Matter

Critical Exponents of Quark Matter

Critical Exponents of Quark Matter

... I investigate the ferromagnetic phase transition inside strong quark matter (SQM) with one gluon exchange interaction between strong quarks. I use a variational method and the Landau-Fermi liquid theory and ...

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String Cloud and Domain Walls with Quark Matter in Lyra Geometry

String Cloud and Domain Walls with Quark Matter in Lyra Geometry

... attach quark matter to the string cloud and domain ...strange quark matter and normal matter in the non-static and stationary Gödel universes with cosmological ...for quark ...

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Inhomogeneous Spherical Symmetric Models with Quark and Strange Quark Matter and Varying Cosmological Term

Inhomogeneous Spherical Symmetric Models with Quark and Strange Quark Matter and Varying Cosmological Term

... constant). Also, in the framework of this model, the quark matter is composed of massless u, d quark, massive s quarks and electrons. In the simplified version of this model, on which our study is ...

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Behaviour of the Strange Quark Matter with Domain walls in 5D Kaluaza-Klein Theory of Gravitation

Behaviour of the Strange Quark Matter with Domain walls in 5D Kaluaza-Klein Theory of Gravitation

... Recently quark matter and the relations between quark matter and domain walls and also strings have been studied by several ...strange quark matter for Robertson Walker model in ...

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Vortex structure in superfluid color-flavor locked quark matter

Vortex structure in superfluid color-flavor locked quark matter

... Abstract. The core region of a neutron star may feature quark matter in the color-flavor- locked (CFL) phase. The CFL condensate breaks the baryon number symmetry, such that the phenomenon of superfluidity ...

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Dense quark matter with chiral and isospin imbalance: NJL-model consideration

Dense quark matter with chiral and isospin imbalance: NJL-model consideration

... dense quark matter is quantum chromodynamics (QCD) which is a gauge field theory associated with S U(3) group, where gauge bosons (gluons) play the role of interaction carriers and the spinor representation ...

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Strange Quark Matter Coupled to the String Cloud in Kaluza Klein Theory of Gravitation

Strange Quark Matter Coupled to the String Cloud in Kaluza Klein Theory of Gravitation

... strange quark matter coupled with string cloud in the frame work of Kaluza- Klein theory of ...strange quark matter for (n = 1) which was ignored by Yilmaz (2006) by assuming G H and  H 2 ...

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Looking for Strange Quark Matter in Cosmic Rays.

Looking for Strange Quark Matter in Cosmic Rays.

... Though formally two-component model presents a good approximation of the real spectrum form in knee area there are a number of unresolved problems which call for a more close look. Some experimental results, basically ...

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Conditions for the existence of stable strange quark matter

Conditions for the existence of stable strange quark matter

... strange quark matter first within a purely theo- retical approach, by using three different chiral models for quark matter and after within phenomeno- logical approach through the measurements ...

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On Bianchi Type III String Cloud Universe Containing Strange Quark Matter

On Bianchi Type III String Cloud Universe Containing Strange Quark Matter

... Considering Bianchi type III space-time we present the model Universe containing strange quark matter which is expanding, anisotropic, with a sign of dark energy that help in accelerated expan- sion of this ...

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Calculations for Density of Quark Core Consisting of Mono Flavored Closely Packed Quarks inside Neutron Star

Calculations for Density of Quark Core Consisting of Mono Flavored Closely Packed Quarks inside Neutron Star

... the quark matter possessing u and d quark flavors with different sizes it is impossible to calculate the density of the core or matter using any crystallography ...flavored quark ...

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Limits on quark nugget dark matter from cosmic ray detectors

Limits on quark nugget dark matter from cosmic ray detectors

... Fluorescence detection is complicated by the extended duration of the air shower. The production of visible and ultraviolet emission, to which fluorescence detectors are sensitive, will continue over time scales of a few ...

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Exploring phases of dense QCD with compact stars

Exploring phases of dense QCD with compact stars

... hadronic matter description is based on relativis- tic density functional of nuclear matter with density-dependent couplings, see ...The quark matter equation of state is based on the ...

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Strange matter in compact stars

Strange matter in compact stars

... strange matter could be absolutely stable, bases on the observation that the ap- pearance of strange quarks lowers the energy per ...flavor quark matter is evidently less stable than Fe (otherwise Fe ...

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Dense and hot matter in compact stars and heavy-ion collisions

Dense and hot matter in compact stars and heavy-ion collisions

... MIT-bag quark model [8] or in combined quark-hadron approaches based on the CMF model [9], a big latent energy is found in the phase transition to ...a quark core are not stable static solutions of ...

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The improved Ginzburg-Landau technique

The improved Ginzburg-Landau technique

... cold quark matter, the IGL method can be used to rapidly evaluate the free energy of the various crystalline color superconducting configurations considered in [13], eventually extending the analysis to ...

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Effective Field Theories for Hot and Dense Matter

Effective Field Theories for Hot and Dense Matter

... The second part provides a detailed introduction to the Polyakov-loop Nambu–Jona-Lasinio model [9] for ther- modynamics and mesonic correlations [10] in the phase diagram of quark matter. Important ...

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QCD at finite temperature and density on the lattice

QCD at finite temperature and density on the lattice

... of Quark Matter, the International Conference on Ultrarelativistic Heavy Ion Collisions, usually include reviews on recent lattice results; the pro- ceedings of The International Symposium on Lattice Field ...

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New Analytical Solutions for Quark Stars with Charged Anisotropic Matter

New Analytical Solutions for Quark Stars with Charged Anisotropic Matter

... be quark stars. The existence of quark stars in hydrostatic equilibrium was first by Itoh [7] in a seminal ...of quark matter has stimulated much interest since could represent the most ...

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Vol 3, No 2 (2012)

Vol 3, No 2 (2012)

... with quark matter attached to the string cloud and domain ...Typically quark matter is modeled with equation of state (EOS) which is based on the phenomenological bag model of quark ...

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