Results 251 to 260 of about 2,490,142 (296)
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Strange Matter and Strange Stars With Tsallis Statistics
International Journal of Modern Physics D, 2007We investigate the properties of β-equilibrated electrically charged neutral strange matter and strange stars at finite temperature in the framework of Tsallis statistics [C. Tsallis, J. Stat. Phys.52 (1988) 479]. As the main result of our study we find out that a QHD description of nuclear matter combined with Tsallis statistics may open new ...
Moisés Razeira
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Strange Quark Matter Fragmentation in Astrophysical Events
The conjecture of Bodmer–Witten–Terazawa suggesting a form of quark matter(Strange Quark Matter)as the ground state of hadronic interactions has been studied in laboratory and astrophysical contexts by a large number of authors.If strange stars exist ...
Laura Paulucci, J E Horvath
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Combustion of nuclear matter into strange matter
Physical Review D, 1994We study the properties of the combustion of pure neutron matter into strange matter in the framework of relativistic hydrodynamical theory of combustion. Because of the uncertainties in the actual properties of neutron matter, we employ the free neutron, Bethe-Johnson, Lattimer-Ravenhall, and Walecka equations of state and for strange matter we adopt ...
, Lugones, , Benvenuto, , Vucetich
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Radial Oscillations of Strange Quark Stars Admixed With Dark Matter
We investigate the equilibrium structure and radial oscillations of strange quark stars admixed with fermionic dark matter. For strange quark matter, we employ a stiff equation of state from a color-superconductivity improved bag model.
Huan Chen, Zi-Yue Zheng, Yu Zhen
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Phase structure of strange matter
Physical Review D, 1993We present a detailed discussion of the phase structure of hadronic matter with finite strangeness content and discuss the thermodynamic conditions for the formation of metastable strange quark droplets ( strangelets'') in relativistic nuclear collisions.
, Lee, , Heinz
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Radioactivity in strange quark matter
Physical Review C, 1987We develop a mass formula for finite lumps of strange quark matter near flavor equilibrium. Our Fermi-gas model includes surface tension and Coulomb energy but not quantum-chromodynamic radiative corrections. Assuming strange matter is stable in bulk, we investigate the radioactive decays of finite strangelets (clumps of strange matter with baryon ...
, Berger, , Jaffe
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Properties of strange quark matter
Physical Review D, 1993Assuming that the novel nuclei of [ital A]=370 amu and [ital Z]=14 recently observed in high-energy cosmic rays are really strange quark matter (SQM), the relationship between parameters describing SQM is discussed and the mass formula for SQM is derived by requiring that it yields the observed value of [ital A]=370 amu and [ital Z]=14.
, Kasuya, , Saito, , Yasuè
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