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DC Field | Value | Language |
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dc.contributor.author | Santra, A K | - |
dc.contributor.author | Sarma, D D | - |
dc.contributor.author | Rao, C N R | - |
dc.date.accessioned | 2012-11-16T10:19:59Z | - |
dc.date.available | 2012-11-16T10:19:59Z | - |
dc.date.issued | 1991 | - |
dc.identifier | 0163-1829 | en_US |
dc.identifier.citation | Physical Review B 43(7), 5612-5615 (1991) | en_US |
dc.identifier.uri | https://libjncir.jncasr.ac.in/xmlui/10572/991 | - |
dc.description | Restricted Access | en_US |
dc.description.abstract | Cu 2p core-level photoemission studies of La2-xSrxCuO4, BiPbSr2Y1-xCa1-xCu2O8, and other cuprates show that the relative intensity of the satellite varies with the composition in a direction opposite to that of the hole concentration, nh. The IS/IM-nh relations in the different cuprate series can be understood in terms of the Δ/tpd ratio, where Δ is the charge-transfer excitation energy and tpd is the hybridization strength between the Cu 3d and O 2p orbitals. Interestingly, the IS/IM ratio increases with the Δ/tpd ratio in the cuprates. At a given value of nh, e.g., around the value corresponding to maximum Tc, IS/IM increases in the same direction as Tc among the different series of cuprates, suggesting thereby that Tc itself may be determined by Δ/tpd. | en_US |
dc.description.uri | http://dx.doi.org/10.1103/PhysRevB.43.5612 | en_US |
dc.language.iso | en | en_US |
dc.publisher | American Physical Society | en_US |
dc.rights | © 1991 The American Physical Society | en_US |
dc.subject | Hole Concentration | en_US |
dc.subject | TC | en_US |
dc.subject | electronic structure | en_US |
dc.subject | superconductivity of cuprates | en_US |
dc.subject | Cu 2p core-level photoemission | en_US |
dc.title | Relation between the electronic structure and the superconductivity of cuprates as revealed by Cu 2p photoemission and theoretical investigations | en_US |
dc.type | Article | en_US |
Appears in Collections: | Research Papers (Prof. C.N.R. Rao) |
Files in This Item:
File | Description | Size | Format | |
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sl.no32.1991.Phys. Rev. B 43, 5612–5615 ().pdf Restricted Access | 183.94 kB | Adobe PDF | View/Open Request a copy |
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