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Electrons as Quasi-Bosons in Strong Magnetic Fields and the Stability of Magnetars

2002/09/23 by Soma Mandal, Mandal, Soma, Somenath Chakrabarty +1
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics (astro-ph) #Atomic and Subatomic Physics Research #FOS: Physical sciences #High-pressure geophysics and materials #Pulsars and Gravitational Waves Research #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0209462

5 pages, REVTEX, one figure (.eps), some references have been added

openalex publication_date 2002/09/23 · arxiv created 2002/09/24 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Following the recent ideas of Dryzek, Kato, Muñoz and Singleton \citeR1 (henceforth we call this paper as R1), that the composite system consisting of an electron along with its screened electric field and within the sphere of influence, the trapped magnetic field of white dwarf can behave like a boson, we have argued that such an exotic transition (bosonization) of electronic component in strongly magnetized neutron star matter in β-equilibrium can make the existence of magnetars physically viable.

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