Origin of the peaks in the Nernst coefficient of bismuth in strong magnetic fields

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dc.creatorSharlai, Yu. V.
dc.creatorMikitik, G. P.
dc.date2008-12-23
dc.date.accessioned2026-07-07T13:00:33Z
dc.date.available2026-07-07T13:00:33Z
dc.descriptionWe explain the origin of most of the peaks in the Nernst coefficient that were recently observed at magnetic fields directed along the trigonal axis and the bisectrix direction in bismuth. Additional experiments are discussed that enable one to verify our explanation.
dc.descriptionSubmitted to Physical Review B. 4 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0812.4376
dc.identifierhttp://arxiv.org/abs/0812.4376
dc.identifierPhys. Rev. B 79, 081102(R) (2009)
dc.identifierdoi:10.1103/PhysRevB.79.081102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/225875
dc.subjectStrongly Correlated Electrons
dc.titleOrigin of the peaks in the Nernst coefficient of bismuth in strong magnetic fields
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