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Related papers: On the Ground State of QCD inside a Compact Stella…

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We discuss the color-superconductivity and its effect on the cooling behavior of strange quark stars. The neutrino emissivity and specific heat of quark matter are calculated within the BCS theory. In the superconducting phase, the…

High Energy Physics - Phenomenology · Physics 2009-11-07 K. Yamaguchi , M. Iwasaki , O. Miyamura

We study the scenario that a new born strange quark star cools to the Quantum ChromoDynamics (QCD) phase transition temperature and converts to a neutron star, and we calculate the evolution of temperature and luminosity of the compact…

Astrophysics · Physics 2007-05-23 K. -W. Wong , M. -C. Chu

It is shown that extremely strong electric fields may be generated at the surface of strange quark matter in the color-flavor locked phase because of the surface effects. Some properties of strange stars made of this matter are briefly…

Astrophysics · Physics 2009-11-10 V. V. Usov

Recent indications for high neutron star masses (M \sim 2 M_sun) and large radii (R > 12 km) could rule out soft equations of state and have provoked a debate whether the occurence of quark matter in compact stars can be excluded as well.…

Nuclear Theory · Physics 2017-08-23 D. B. Blaschke , T. Klahn , F. Sandin

In this contributed paper the gapless phases of QCD are discussed.

High Energy Physics - Phenomenology · Physics 2009-11-10 R. Casalbuoni

I review in this work the properties of nuclear and quark matter equation of state under the influence of a strong magnetic field. We analyse the results when they are applied to compact stars description. Finally, we describe the emission…

Astrophysics · Physics 2007-05-23 G. F. Marranghello

As a model for nonideal behavior in the equation of state of QCD at high density, we consider cold quark matter in perturbation theory. To second order in the strong coupling constant, $\alpha_s$, the results depend sensitively on the…

High Energy Physics - Phenomenology · Physics 2009-12-31 Eduardo S. Fraga , Robert D. Pisarski , Jurgen Schaffner-Bielich

This paper is a brief journey into the amazing realm of crystalline color superconductors. Starting from a qualitative description of superfluids, superconductors and supersolids, we show how inhomogeneous phases may arise when the system…

High Energy Physics - Phenomenology · Physics 2015-06-18 Massimo Mannarelli

We review recent work on the phase structure of QCD at very high baryon density. We introduce the phenomenon of color superconductivity and discuss the use of weak coupling methods. We study the phase structure as a function of the number…

Nuclear Theory · Physics 2009-11-07 Thomas Schaefer

The status of lattice calculations in the light hadron sector is reviewed. Special emphasis is given to recent lattice determinations of the mass of the strange quark. The impact of non-perturbative renormalization and control over lattice…

High Energy Physics - Phenomenology · Physics 2008-11-26 Hartmut Wittig

Neutron stars provide a natural laboratory to test some unique implications of Quantum Chromodynamics (QCD)- the underlying theory of strong interactions- at extreme conditions of very high baryon density. It has been suggested that the…

High Energy Astrophysical Phenomena · Physics 2009-06-08 Ritam Mallick , Sanjay K. Ghosh , Sibaji Raha

In this talk I discuss the inhomogeneous (LOFF) color superconductive phases of Quantum Chromodynamics (QCD). In particular, I show the effect of a core of LOFF phase on the cooling of a compact star.

High Energy Physics - Phenomenology · Physics 2008-11-26 M. Ruggieri

I discuss three topics in physics of massive (two solar-mass and larger) neutron stars containing deconfined quark matter: (i) the equation of state of deconfined dense quark matter and its color superconducting phases, (ii) the thermal…

High Energy Astrophysical Phenomena · Physics 2013-05-24 Armen Sedrakian

A broad sample of computed realistic equations of state of superdense matter with quark phase transition is used to construct a series of models neutron stars with a strange quark core. The integral characteristics of the stellar…

Astrophysics · Physics 2009-11-10 G. B. Alaverdyan , A. R. Harutyunyan , Yu. L. Vartanyan

Strange quark matter in beta equilibrium at high densities is studied in a quark confinement model. Two equations of state are dynamically generated for the {\it same} set of model parameters used to describe the nucleon: one corresponds to…

Astrophysics · Physics 2008-11-26 M. Malheiro , M. Fiolhais , A. R. Taurines

We study effects of two-flavor color superconductivity on the structure of strange dwarfs, which are stellar objects with similar masses and radii with ordinary white dwarfs but stabilized by the strange quark matter core. We find that…

Astrophysics · Physics 2009-06-23 Masayuki Matsuzaki , Etsuchika Kobayashi

We study the effects of small chemical potentials associated with the three light quark flavors in QCD. We use a low-energy effective field theory that solely relies on the symmetries of the QCD partition function. We find three different…

High Energy Physics - Phenomenology · Physics 2009-11-07 J. B. Kogut , D. Toublan

According to quantum chromodynamics, matter at ultra-high density and low temperature is a quark liquid, with a condensate of Cooper pairs of quarks near the Fermi surface ("color superconductivity"). This paper reviews the physics of color…

Nuclear Theory · Physics 2009-11-18 Mark G. Alford

Since the incident nuclei in heavy-ion collisions do not carry strangeness, the global net strangeness of the detected hadrons has to vanish. We investigate the impact of strangeness neutrality on the phase structure and thermodynamics of…

High Energy Physics - Phenomenology · Physics 2020-04-03 Wei-jie Fu , Jan M. Pawlowski , Fabian Rennecke

The possible existence of compact stars made of absolutely stable strange quark matter--referred to as strange stars--was pointed out by E. Witten almost a quarter of a century ago. One of the most amazing features of such objects concerns…

Solar and Stellar Astrophysics · Physics 2009-10-29 Rodrigo P. Negreiros , Fridolin Weber , Manuel Malheiro , Vladimir Usov