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Landau quantization and mass-radius relation of magnetized White Dwarfs in general relativity

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arxiv 1507.05439 v2 pith:H3UD7ELE submitted 2015-07-20 astro-ph.SR gr-qcnucl-th

Landau quantization and mass-radius relation of magnetized White Dwarfs in general relativity

classification astro-ph.SR gr-qcnucl-th
keywords magneticwhitedwarfsfieldlandaumagnetizedmass-radiusquantization
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Recently, several white dwarfs have been proposed with masses significantly above the Chandrasekhar limit, known as Super-Chandrasekhar White Dwarfs, to account for the overluminous Type Ia supernovae. In the present work, Equation of State of a completely degenerate relativistic electron gas in magnetic field based on Landau quantization of charged particles in a magnetic field is developed. The mass-radius relations for magnetized White Dwarfs are obtained by solving the Tolman-Oppenheimer-Volkoff equations. The effects of the magnetic energy density and pressure contributed by a density-dependent magnetic field are treated properly to find the stability configurations of realistic magnetic White Dwarf stars.

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  1. Strange quark star I: the maximum gravitational mass and deformation of magnetized spinning model

    astro-ph.HE 2026-01 conditional novelty 6.0

    A density-dependent bag EOS with Landau quantization produces strange quark stars up to 2.8 solar masses and deformation 1.55 at 1200 Hz and 5×10^17 G.