Results 241 to 250 of about 2,838,718 (281)
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Strange Matter and Neutron Stars
, 2013Strange matter may be the true ground state of hadronic matter. Phenomenological model of strange matter is presented and possibilities of formation of strange matter in neutron stars are considered. Possible scenario of conversion of a neutron star into
P. Haensel
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Nuclear Physics A, 1992
Abstract I consider the strangeness degree of freedom in hot nuclear matter and its significance for the observation and identification of a quark-gluon plasma. Particular attention is given to the interpretation of new and intriguing results on strange antibaryon production.
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Abstract I consider the strangeness degree of freedom in hot nuclear matter and its significance for the observation and identification of a quark-gluon plasma. Particular attention is given to the interpretation of new and intriguing results on strange antibaryon production.
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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 ...
Robert L. Jaffe, Micheal S. Berger
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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.
Takesi Saito +2 more
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Symmetry energy of strange quark matter and tidal deformability of strange quark stars
Nuclear Science and Techniques, 2022Jian-Feng Xu +4 more
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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 ...
César A. Z. Vasconcellos +2 more
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Strange quark matter and quark stars with the Dyson-Schwinger quark model
, 2016.We calculate the equation of state of strange quark matter and the interior structure of strange quark stars in a Dyson-Schwinger quark model within rainbow or Ball-Chiu vertex approximation.
H. Chen, J. -. Wei, H. Schulze
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Strange Quark Matter as Dark Matter
Nonlinear Phenomena in Complex Systems, 2019New forms of matter such as super-hypernuclei (strange quark matter) and superhypernuclear stars (strange quark stars) as candidates for dark matter are discussed in some detail, based on the so-called "Bodmer–Terazawa–Witten hypothesis" assuming that they are stable absolutely or quasi-stable (decaying only weakly).
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Properties of strange quark matter objects with two types of surface treatments
, 2016We study strange quark matter (SQM) objects ranging from strangelets to strange stars based on our recently proposed unified description. The important interface effects are investigated by adopting a constant surface tension as well as the multiple ...
C. Xia, G. Peng, E. Zhao, Shan-Gui Zhou
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Nuclear Physics A, 1988
Abstract This talk surveys the role of strangeness in the physics of dense matter, including the nature of the absolute ground state of matter, strange neutron stars, strangeness in the early universe, and strangeness as a probe of ultrarelativistic heavy-ion collisions.
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Abstract This talk surveys the role of strangeness in the physics of dense matter, including the nature of the absolute ground state of matter, strange neutron stars, strangeness in the early universe, and strangeness as a probe of ultrarelativistic heavy-ion collisions.
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