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Related papers: Strange quark matter with effective quark masses

200 papers

The production of strange particles in a hot medium as produced in collisions of heavy ions is considered one of the most important signals for the phase transition to a quark-gluon plasma. In the first part of this lecture, the theoretical…

Nuclear Theory · Physics 2009-11-10 J. Schaffner-Bielich

In this conference proceeding, we review important theoretical developments related to the production of strangeness in astrophysics. This includes its effects in supernova explosions, neutron stars, and compact-star mergers. We also…

High Energy Astrophysical Phenomena · Physics 2022-02-16 Veronica Dexheimer , Krishna Aryal

The quark matter may have great implications in astrophysical studies, which could appear in the early Universe, in compact stars, and/or as cosmic rays. After a general review of astrophysical quark matter, the density-dominated quark…

Astrophysics · Physics 2014-10-13 R. X. Xu

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 properties of strange mesons in vacuum and in the hot nuclear medium within unitarized coupled-channel effective theories. We determine transition probabilities, cross sections and scattering lengths for strange mesons. These…

We study the effect of SU(3) flavor breaking on high density quark matter. We discuss, in particular, the effect a non-zero electron chemical potential and a finite strange quark mass. We argue that these perturbations trigger pion or kaon…

High Energy Physics - Phenomenology · Physics 2008-11-26 P. F. Bedaque , T. Schaefer

We present results on the equation of state in QCD with two light quark flavors and a heavier strange quark. Calculations with improved staggered fermions have been performed on lattices with temporal extent Nt =4 and 6 on a line of…

Two twisted doublets, one containing the up and down quarks and the other containing the strange quark with an SU(2)-flavor partner, are used for studies in the meson sector. The relevant chiral perturbation theory is presented, and…

High Energy Physics - Lattice · Physics 2011-02-01 Abdou M. Abdel-Rehim , Randy Lewis , R. M. Woloshyn , Jackson M. S. Wu

We discuss quark antiquark energies and the screening mass in hot QCD using the non-perturbative lattice approach. For this purpose we analyze properties of quark antiquark energies and entropies at infinitely large separation of the quark…

High Energy Physics - Lattice · Physics 2007-05-23 O. Kaczmarek , F. Zantow

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…

High Energy Physics - Phenomenology · Physics 2009-09-29 A. Peshier , B. Kampfer , G. Soff

We present results on the sum of the masses of light and strange quark using improved staggered quarks. Our calculation uses 2+1 flavours of dynamical quarks. The effects of the dynamical quarks are clearly visible.

High Energy Physics - Lattice · Physics 2009-11-07 J. Hein , C. Davies , G. P. Lepage , Q. Mason , H. Trottier

At high density, matter is expected to undergo a phase transition to deconfined quark matter. Although the density at which it happens and the strength of the transition are still largely unknown, we can model it to be in agreement with…

Nuclear Theory · Physics 2023-11-21 Alexander Clevinger , Veronica Dexheimer , Jeffrey Peterson

It is argued that it is valid to use QCD sum rules to determine the scalar and pseudoscalar two-point functions at zero momentum, which in turn determine the ratio of the strange to non-strange quark condensates $R_{su} = \frac{<\bar{s}…

High Energy Physics - Phenomenology · Physics 2009-01-06 C. A. Dominguez , N. F. Nasrallah , K. Schilcher

The pervasive presence in space of a flux of high-speed, electrically uncharged dark matter particles is examined here for potential consequences. Dark matter interactions with ordinary matter are considered, and a model of the dark matter…

General Physics · Physics 2009-08-25 C. L. Herzenberg

The interface effects of quark matter play important roles in the properties of compact stars and small nuggets such as strangelets and $ud$QM nuggets. By introducing a density derivative term to the Lagrangian density and adopting…

High Energy Physics - Phenomenology · Physics 2022-08-30 Cheng-Jun Xia , Jian-Feng Xu , Guang-Xiong Peng , Ren-Xin Xu

Strangelets (hypothetical stable lumps of strange quarkmatter) of astrophysical origin may be ultimately detected in specific cosmic ray experiments. The initial mass distribution resulting from the possible astrophysical production sites…

Nuclear Theory · Physics 2010-03-26 Laura Paulucci , Jorge E. Horvath

If strange quark matter is the true ground state of matter, it must have lower energy than nuclear matter. Simultaneously, two-flavour quark matter must have higher energy than nuclear matter, for otherwise the latter would convert to the…

High Energy Physics - Phenomenology · Physics 2009-11-10 Vikram Soni , Dipankar Bhattacharya

I review the properties of mesons with one heavy quark. I start by examining the predicted masses and widths in the context of the quark model and heavy quark effective theory. Some recent experimental results are described and I conclude…

High Energy Physics - Phenomenology · Physics 2009-02-24 Stephen Godfrey

Motivated by the need for a solid state strange quark matter to better explain some observational phenomena, we discussed possibility of color singlet cluster formation in cold strange quark matter by a rough calculation following the…

Solar and Stellar Astrophysics · Physics 2009-12-11 Xuesen Na

Recent achievements of bare strange stars are briefly reviewed. A nascent protostrange star should be bare because of strong mass ejection and high temperature after the supernova detonation flame, and a crust can also hardly form except…

Astrophysics · Physics 2016-01-27 R. X. Xu