Magnetism of Neutron Stars and Planets

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dc.creatorSidharth, B. G.
dc.date1999-04-27
dc.date.accessioned2026-07-07T05:56:56Z
dc.date.available2026-07-07T05:56:56Z
dc.descriptionIt is shown in this paper that recent results that below the Fermi temperature, Fermions obey anomalous semionic statistics, could explain such apparently diverse phenomena as the magnetism of Pulsars and White Dwarfs on the one hand and earth like planets, on the other.
dc.description4 pages, TeX
dc.identifierhttps://arxiv.org/abs/physics/9904059
dc.identifierhttp://arxiv.org/abs/physics/9904059
dc.identifierChaotic Universe,Nova Science,New York,2001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/87800
dc.subjectGeneral Physics
dc.titleMagnetism of Neutron Stars and Planets
dc.typetext

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