Results 201 to 210 of about 1,078 (229)
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Classical and Quantum Gravity, 1991
The authors calculate the mass, radius, moment of inertia and surface gravitational red shift of quark stars described by three models: the noninteracting Fermi gas model of Itoh (1970), the asymptotic MIT bag model, and the perturbative QCD model of Chapline and Nauenberg (1977). They report the results of phase transition calculations, and comment on
T Overgard, E Ostgaard
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The authors calculate the mass, radius, moment of inertia and surface gravitational red shift of quark stars described by three models: the noninteracting Fermi gas model of Itoh (1970), the asymptotic MIT bag model, and the perturbative QCD model of Chapline and Nauenberg (1977). They report the results of phase transition calculations, and comment on
T Overgard, E Ostgaard
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2000
We study the relativistic quadrupole oscillations (ι= 2) of strange quark stars by calculating their quasi-normal modes, and we thus explore the possibility of using these oscillation frequencies and damping times to differentiate among relativistic polytropic stars, neutron stars, pure light-quark stars, and hybrid neutron stars with quark cores.
C. W. Yip, M. C. Chu, P. T. Leung
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We study the relativistic quadrupole oscillations (ι= 2) of strange quark stars by calculating their quasi-normal modes, and we thus explore the possibility of using these oscillation frequencies and damping times to differentiate among relativistic polytropic stars, neutron stars, pure light-quark stars, and hybrid neutron stars with quark cores.
C. W. Yip, M. C. Chu, P. T. Leung
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Chinese Journal of Astronomy and Astrophysics, 2006
Members of the family of pulsar-like stars are distinguished by their different manifestations observed, i.e., radio pulsars, accretion-driven X-ray pulsars, X-ray bursts, anomalous X-ray pulsars/soft gamma-ray repeaters, certral compact objects, and dim thermal neutron stars.
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Members of the family of pulsar-like stars are distinguished by their different manifestations observed, i.e., radio pulsars, accretion-driven X-ray pulsars, X-ray bursts, anomalous X-ray pulsars/soft gamma-ray repeaters, certral compact objects, and dim thermal neutron stars.
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Stable Up-Down Quark Matter Nuggets, Quark Star Crusts, and a New Family of White Dwarfs
Galaxies, 2021Cheng-Jun Xia, Jian-Feng Xu, G X Peng
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Regular quark star model with pressure anisotropy
Pramana - Journal of Physics, 2022Jefta M Sunzu, Sunzu Jefta M
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Examination of the multitude of signals from the phase transition of a neutron star to a quark star
Physical Review C, 2022Debojoti Kuzur +2 more
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