Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model

The two-orbital Hubbard model is used to obtain formulas for the fermion excitation spectrum in the energy bands hybridized by Anderson's interaction. A transition to the Hubbard operators, which diagonalizes the one-site part of the Hamiltonian, allows us to use the Green's temperature fu...

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Veröffentlicht in:Физика низких температур
Datum:1998
1. Verfasser: Kosov, A.A.
Format: Artikel
Sprache:Englisch
Veröffentlicht: Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України 1998
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Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/174987
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model / A.A. Kosov // Физика низких температур. — 1998. — Т. 24, № 3. — С. 204-214. — Бібліогр.: 22 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Kosov, A.A.
author_facet Kosov, A.A.
citation_txt Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model / A.A. Kosov // Физика низких температур. — 1998. — Т. 24, № 3. — С. 204-214. — Бібліогр.: 22 назв. — англ.
collection DSpace DC
container_title Физика низких температур
description The two-orbital Hubbard model is used to obtain formulas for the fermion excitation spectrum in the energy bands hybridized by Anderson's interaction. A transition to the Hubbard operators, which diagonalizes the one-site part of the Hamiltonian, allows us to use the Green's temperature function technique to take into account the interstitial jump term while studying the superconducting properties of the model. An analysis of the lower part of the energy spectrum leads to a formula for the superconducting transition temperature Tc associated with the pairing of quasiparticles in one of the correlated bands. The dependence of Tc on electron concentration and energy parameters determining the intraatomic correlation is studied. Proposing a simple relation between the value of pressure (P) and width of the correlated band, the dependence of Tc on the pressure was defined. Good agreement between the theoretical calculation of the dependence of Tc on the pressure and the experimental results for Y1-xPrxBa₂Cu₃O₇-δ is found. Comparison of the theoretical and experimental results for the dependence of Tc and its derivative d(lnTc)/dP on Sr and Bi-content (x) in La₂-xSrxCuO₄ has been made. It is concluded that the model under consideration can be used for the description of the shift in Tc under pressure for a number of superconductors.
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language English
last_indexed 2025-12-07T15:17:02Z
publishDate 1998
publisher Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
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spelling Kosov, A.A.
2021-01-29T11:28:04Z
2021-01-29T11:28:04Z
1998
Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model / A.A. Kosov // Физика низких температур. — 1998. — Т. 24, № 3. — С. 204-214. — Бібліогр.: 22 назв. — англ.
0132-6414
PACS: 74.20.-z
https://nasplib.isofts.kiev.ua/handle/123456789/174987
The two-orbital Hubbard model is used to obtain formulas for the fermion excitation spectrum in the energy bands hybridized by Anderson's interaction. A transition to the Hubbard operators, which diagonalizes the one-site part of the Hamiltonian, allows us to use the Green's temperature function technique to take into account the interstitial jump term while studying the superconducting properties of the model. An analysis of the lower part of the energy spectrum leads to a formula for the superconducting transition temperature Tc associated with the pairing of quasiparticles in one of the correlated bands. The dependence of Tc on electron concentration and energy parameters determining the intraatomic correlation is studied. Proposing a simple relation between the value of pressure (P) and width of the correlated band, the dependence of Tc on the pressure was defined. Good agreement between the theoretical calculation of the dependence of Tc on the pressure and the experimental results for Y1-xPrxBa₂Cu₃O₇-δ is found. Comparison of the theoretical and experimental results for the dependence of Tc and its derivative d(lnTc)/dP on Sr and Bi-content (x) in La₂-xSrxCuO₄ has been made. It is concluded that the model under consideration can be used for the description of the shift in Tc under pressure for a number of superconductors.
en
Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
Физика низких температур
Свеpхпpоводимость, в том числе высокотемпеpатуpная
Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model
Article
published earlier
spellingShingle Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model
Kosov, A.A.
Свеpхпpоводимость, в том числе высокотемпеpатуpная
title Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model
title_full Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model
title_fullStr Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model
title_full_unstemmed Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model
title_short Analysis of the shift in the superconducting transition under pressure in the Anderson-Hubbard two-orbital model
title_sort analysis of the shift in the superconducting transition under pressure in the anderson-hubbard two-orbital model
topic Свеpхпpоводимость, в том числе высокотемпеpатуpная
topic_facet Свеpхпpоводимость, в том числе высокотемпеpатуpная
url https://nasplib.isofts.kiev.ua/handle/123456789/174987
work_keys_str_mv AT kosovaa analysisoftheshiftinthesuperconductingtransitionunderpressureintheandersonhubbardtwoorbitalmodel