Please use this identifier to cite or link to this item: https://libjncir.jncasr.ac.in/xmlui/handle/10572/1142
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dc.contributor.authorSantra, A K-
dc.contributor.authorSheelam, Radha Rani-
dc.contributor.authorRao, C N R-
dc.date.accessioned2012-11-30T11:46:08Z-
dc.date.available2012-11-30T11:46:08Z-
dc.date.issued1992-
dc.identifier0921-4534en_US
dc.identifier.citationPhysica C 192(3-4), 311-314 (1992)en_US
dc.identifier.urihttps://libjncir.jncasr.ac.in/xmlui/10572/1142-
dc.descriptionRestricted Accessen_US
dc.description.abstractThe relative intensity of the Cu 2p satellite in YBa2Cu3O7 compositions where Y is partially substituted by Pr or Ca or Cu by Zn, Ni or Fe decreases with increasing hole concentration, n(h), or decrease in T(c). La1.8Sr0.2CuO4 compositions where La is partially substituted by another rare earth or Cu by Zn or Ni also show a decrease in the Cu 2p satellite intensity with increasing n(h) or decrease in T(c).en_US
dc.description.urihttp://dx.doi.org/10.1016/0921-4534(92)90836-2en_US
dc.language.isoenen_US
dc.publisherElsevier Science BVen_US
dc.rights© 1992 Elsevier Science BVen_US
dc.subjectSpectroscopyen_US
dc.subjectTCen_US
dc.subjectphotoemission intensitiesen_US
dc.subjectcation derivativesen_US
dc.titleDependence of the Cu 2p photoemission intensities and the superconducting transition temperatures in cation-substituted derivatives of YBa2Cu3O7 and La1.8Sr0.2CuO4 on the hole concentration and related factorsen_US
dc.typeArticleen_US
Appears in Collections:Research Papers (Prof. C.N.R. Rao)

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