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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4975
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dc.contributor.authorChatterjee, S-
dc.date.accessioned2010-01-13T12:20:43Z-
dc.date.available2010-01-13T12:20:43Z-
dc.date.issued1989-12-
dc.identifier.citationAstrophysics and Space Science, Vol. 162, No. 1, pp. 167 - 170en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4975-
dc.descriptionOpen Access-
dc.description.abstractIt is shown that, in the non-interacting limit, a one-dimensional metallic system has a transition to an insulating phase, in presence of external magnetic field H, if mu(B)H is greater than E(B), where mu(B) is the Bohr magneton and E(B) is the energy band width of the electronic states. Possible realization of this effect in the atmosphere of neutron stars is pointed out.en
dc.description.sponsorshipThe original publication is available at springerlink.comen
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://dx.doi.org/10.1007/BF00653354en
dc.relation.urihttp://adsabs.harvard.edu/abs/1989Ap%26SS.162..167C-
dc.rights© Kluwer Academic Publishersen
dc.subjectElectron Transitionsen
dc.subjectMetallicityen
dc.subjectNeutron Starsen
dc.subjectStellar Atmospheresen
dc.subjectStellar Magnetic Fieldsen
dc.subjectElectron Orbitalsen
dc.subjectElectron Statesen
dc.subjectEnergy Bandsen
dc.subjectThermal Conductivityen
dc.titleMagnetic field induced metal-insulator transition in a one-dimensional chain: application to neutron star atmospheresen
dc.typeArticleen
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