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Magnetized strange quark matter and magnetized strange quark stars [PDF]
Physical Review C, 2008 9 pages, 9 ...
Milva Orsaria +4 more
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Thermodynamics, strange quark matter, and strange stars [PDF]
Physical Review C, 2000 6 pages, 6 PS figures, REVTeX ...
Guang-Xiong Peng +4 more
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THE STRANGE QUARK-GLUON PLASMA [PDF]
Relativistic Aspects of Nuclear Physics, 2001 36 pages, including 16 figures; Presented in October 2000 at the 6th International Workshop on Relativistic Aspects of Nuclear Physics Tabatinga, Sao Paulo ...
Johann Rafelski +2 more
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Strange-quark-matter stars [PDF]
, 1989 We investigate the implications of rapid rotation corresponding to the frequency of the new pulsar reported in the supernovae remnant SN1987A. It places very stringent conditions on the equation of state if the star is assumed to be bound by gravity alone. We find that the central energy density of the star must be greater than 13 times that of nuclear
Norman K. Glendenning
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Strange quark matter and compact stars [PDF]
Progress in Particle and Nuclear Physics, 2005 Astrophysicists distinguish between three different types of compact stars. These are white dwarfs, neutron stars, and black holes. The former contain matter in one of the densest forms found in the Universe which, together with the unprecedented progress in observational astronomy, make such stars superb astrophysical laboratories for a broad range of
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Properties of strange quark matter and strange quark stars [PDF]
The European Physical Journal C, 2021 AbstractA Polyakov chiral$$\text {SU(3)}$$SU(3)quark mean-field (PCQMF) model is applied to study the properties of strange quark matter (SQM) and strange quark star (SQS) in$$\beta $$β-equilibrium. The effect of increasing the strength of vector interactions on the effective constituent quark mass, particle fractions, and the thermodynamical ...
Manisha Kumari, Arvind Kumar
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Strange quark mass dependence of strange quark star properties [PDF]
The European Physical Journal C, 2021 AbstractThe effects of strange quark mass on masses, radii, and tidal deformabilities of strange quark stars are studied via the quasiparticle model that includes the non-perturbative features of QCD in low density region. The constraints of $$M_{\mathrm {TOV}} > 2.0 M_{\odot }$$ M
Li, Bo-Lin, Yan, Yan, Ping, Jia-Lun
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The strange-quark distribution [PDF]
Zeitschrift für Physik C: Particles and Fields, 1996 We discuss the latest CCFR determination of the strange sea density of the proton. We comment on the differences with a previous, leading--order, result and point out the relevance of quark mass effects and current non--conservation effects. By taking them into account it is possible to solve the residual discrepancy with another determination of the ...
Marco Genovese +5 more
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Strangeness and quark–gluon plasma [PDF]
Journal of Physics G: Nuclear and Particle Physics, 2003 30 pages including numerouse figures, tables. Opening Lecture: Strangeness and Quark Gluon Plasma -- what has been learned so far and where do we go at SQM2003, North Carolina, March 2003, submitted to J.
Jean Letessier +2 more
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The Ω− and the strange quark mass [PDF]
Nuclear Physics B - Proceedings Supplements, 2005 Three pages, proceedings of the Lattice-04 symposium. (Corrected typographical errors)
Davies, C., Toussaint, Doug
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