
We 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 possibilities for nuclear matter models.
nuclear matter, Galactic and stellar structure, strange matter stars, Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), neutron stars
nuclear matter, Galactic and stellar structure, strange matter stars, Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), neutron stars
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