dc.creatorRodríguez, Carlos Osvaldo
dc.creatorWeht, Rubén Oscar
dc.creatorPickett, W. E.
dc.date2000-07
dc.date2020-05-12T16:06:18Z
dc.date.accessioned2023-07-14T20:02:08Z
dc.date.available2023-07-14T20:02:08Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/95717
dc.identifierhttps://ri.conicet.gov.ar/11336/71729
dc.identifierhttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.84.3903
dc.identifierissn:0031-9007
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7437652
dc.descriptionElectron-hole mixing-induced fine structure in alkaline earth hexaborides leads to lower energy (temperature) scales, and thus a stronger tendency toward an excitonic instability than in their doped counterparts (viz. Ca₁₋ₓ LaₓB₆, x≈0.005\), which are high-Curie-temperature, small-moment ferromagnets. Comparison of Fermi surfaces and spectral distributions with de Haas–van Alphen, optical, transport, and tunneling data indicates that SrB₆ remains a fermionic semimetal down to (at least) 5 K, rather than forming an excitonic condensate. For the doped system the Curie temperature is higher than the degeneracy temperature.
dc.descriptionInstituto de Física de Líquidos y Sistemas Biológicos
dc.formatapplication/pdf
dc.format3903-3907
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectFísica
dc.subjectFirst principles
dc.titleElectronic Fine Structure in the Electron-Hole Plasma in SrB6
dc.typeArticulo
dc.typePreprint


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