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Strange quark mass dependence of strange quark star properties [PDF]
European Physical Journal C: Particles and Fields, 2021 The 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 $$M_{\mathrm {TOV}} >
Bo-Lin Li, Yan Yan, Jia-Lun Ping
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Properties of strange quark matter and strange quark stars [PDF]
European Physical Journal C: Particles and Fields, 2021 A Polyakov chiral $$\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.
Manisha Kumari, Arvind Kumar
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Magnetized strange quark matter and magnetized strange quark stars [PDF]
Physical Review C, 2007 Strange quark matter could be found in the core of neutron stars or forming strange quark stars. As is well known, these astrophysical objects are endowed with strong magnetic fields which affect the microscopic properties of matter and modify the ...
Felipe, R. Gonzalez +3 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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Repeating fast radio bursts from collapses of the crust of a strange star [PDF]
The Innovation, 2021 Summary: Strange stars (SSs) are compact objects made of deconfined quarks. It is hard to distinguish SSs from neutron stars as a thin crust composed of normal hadronic matter may exist and obscure the whole surface of the SS.
Jinjun Geng, Bing Li, Yongfeng Huang
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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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Electrically charged strange quark stars
Physical Review D, 2009 The possible existence of compact stars made of absolutely stable strange quark matter--referred to as strange stars--was pointed out by E. Witten almost a quarter of a century ago.
Fridolin Weber +2 more
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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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Probing CP symmetry and weak phases with entangled double-strange baryons [PDF]
Nature, 2022 P Adlarson, W Gradl, M Kuessner
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