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- W1123573619 abstract "In this paper, using both quantum magnetohydrodynamic (MHD) and magnetohydrostatic (MHS) models of a relativistically degenerate magnetic compact star, the fundamental role of Landau orbital ferromagnetism (LOFER) on the magneto-gravitational stability of such star is revealed. It is shown that the previously suggested magnetic equation of state for LOFER with some generalization of form $B=beta rho^{2s/3}$ only within the range $0leq sleq 1$ and $0leq beta< sqrt{2pi}$ leads to magneto-gravitational stability with distinct critical value $beta_{cr}=sqrt{2pi}$ governing the magnetohydrostatic stability of the compact star. Furthermore, the value of the parameters $s$ and $beta$ is shown to fundamentally control both the quantum and Chandrasekhar gravitational collapse mechanisms and the previously discovered mass-limit on white dwarfs. Current findings can help to understand the origin of magnetism and its inevitable role on the stability of the relativistically degenerate super-dense magnetized matter encountered in many white-dwarfs and neutron stars." @default.
- W1123573619 created "2016-06-24" @default.
- W1123573619 creator A5058577547 @default.
- W1123573619 date "2012-01-21" @default.
- W1123573619 modified "2023-09-27" @default.
- W1123573619 title "Landau Ferromagnetism and the Chandrasekhar Mass-Limit" @default.
- W1123573619 hasPublicationYear "2012" @default.
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