Superconductivity by Kinetic Energy Saving?
| dc.creator | van der Marel, D. | |
| dc.creator | Molegraaf, H. J. A. | |
| dc.creator | Presura, C. | |
| dc.creator | Santoso, I. | |
| dc.date | 2003-02-10 | |
| dc.date.accessioned | 2026-07-07T06:24:17Z | |
| dc.date.available | 2026-07-07T06:24:17Z | |
| dc.description | A brief introduction is given in the generic microscopic framework of superconductivity. The consequences for the temperature dependence of the kinetic energy, and the correlation energy are discussed for two cases: The BCS scenario and the non-Fermi liquid scenario. A quantitative comparison is made between the BCS-prediction for d-wave pairing in a band with nearest neighbor and next-nearest neighbor hoppping and the experimental specific heat and the optical intraband spectral weight along the plane. We show that the BCS-prediction produces the wrong sign for the kink at Tc of the intraband spectral weight, even though the model calculation agrees well with the specific heat. | |
| dc.description | 11 pages, ReVTeX, 7 figures in encapsulated postscript | |
| dc.identifier | https://arxiv.org/abs/cond-mat/0302169 | |
| dc.identifier | http://arxiv.org/abs/cond-mat/0302169 | |
| dc.identifier | in "Concepts in electron correlation", Edited by A. Hewson and V. Zlatic, Kluwer (2003), p 7-16 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/96495 | |
| dc.subject | Superconductivity | |
| dc.subject | Strongly Correlated Electrons | |
| dc.title | Superconductivity by Kinetic Energy Saving? | |
| dc.type | text |