Theory of antiferromagnetic pairing in cuprate superconductors (Review article)
A review of the antiferromagnetic exchange and spin-fluctuation pairing theory in the cuprate
 superconductors is given. We briefly discuss a phenomenological approach and a theory in the
 limit of weak Coulomb correlations. A microscopic theory in the strong correlation limit&#x...
Gespeichert in:
| Veröffentlicht in: | Физика низких температур |
|---|---|
| Datum: | 2006 |
| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
2006
|
| Schlagworte: | |
| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/120190 |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | Theory of antiferromagnetic pairing in cuprate
 superconductors
 (Review article) / N.M. Plakida // Физика низких температур. — 2006. — Т. 32, № 4-5. — С. 483–498. — Бібліогр.: 106 назв. — англ. |
Institution
Digital Library of Periodicals of National Academy of Sciences of Ukraine| Zusammenfassung: | A review of the antiferromagnetic exchange and spin-fluctuation pairing theory in the cuprate
superconductors is given. We briefly discuss a phenomenological approach and a theory in the
limit of weak Coulomb correlations. A microscopic theory in the strong correlation limit
is presented in more detail. In particular, results of our recently developed theory for the effective
p–d Hubbard model and the reduced t–J model are given. We have proved that retardation effects
for the antiferromagnetic exchange interaction are unimportant that results in pairing of all charge
carriers in the conduction band and high Tc proportional to the Fermi energy. The spin-fluctuation
interaction caused by kinematic interaction gives an additional contribution to the d-wave pairing.
Dependence of Tc on the hole concentration and the lattice constant (or pressure) and an oxygen
isotope shift are discussed.
|
|---|---|
| ISSN: | 0132-6414 |