Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles

G. I. González-Pedreros; J. A. Camargo-Martínez; F. Mesa

doi:10.1038/s41598-021-87028-x

Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles

G. I. González-Pedreros, J. A. Camargo-Martínez, F. Mesa

Research output: Contribution to journal › Article › peer-review

3 Scopus citations

Abstract

In this paper, we report Cooper Pairs Distribution function D_cp(ω, T_c) for bcc Niobium under pressure. This function reveals information about the superconductor state through the determination of the spectral regions for Cooper-pairs formation. D_cp(ω, T_c) is built from the well-established Eliashberg spectral function and phonon density of states, calculated by first-principles. D_cp(ω, T_c) for Nb suggests that the low-frequency vibration region (ω<6meV) is where Cooper-pairs are possible. From D_cp(ω, T_c) , it is possible to obtain the N_cp parameter, which is proportional to the total number of Cooper-Pairs formed at a temperature T_c. The N_cp parameter allows an approach to the understanding of the Nb T_c anomalies, measured around 5 and 50 GPa.

Original language	English (US)
Article number	7646
Journal	Scientific Reports
Volume	11
Issue number	1
DOIs	https://doi.org/10.1038/s41598-021-87028-x
State	Published - Dec 2021

All Science Journal Classification (ASJC) codes

General

Access to Document

10.1038/s41598-021-87028-x

Cite this

@article{a14e3f93f1ff4dd2b3d9c64816ead21f,

title = "Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles",

abstract = "In this paper, we report Cooper Pairs Distribution function Dcp(ω, Tc) for bcc Niobium under pressure. This function reveals information about the superconductor state through the determination of the spectral regions for Cooper-pairs formation. Dcp(ω, Tc) is built from the well-established Eliashberg spectral function and phonon density of states, calculated by first-principles. Dcp(ω, Tc) for Nb suggests that the low-frequency vibration region (ω<6meV) is where Cooper-pairs are possible. From Dcp(ω, Tc) , it is possible to obtain the Ncp parameter, which is proportional to the total number of Cooper-Pairs formed at a temperature Tc. The Ncp parameter allows an approach to the understanding of the Nb Tc anomalies, measured around 5 and 50 GPa.",

author = "Gonz{\'a}lez-Pedreros, {G. I.} and Camargo-Mart{\'i}nez, {J. A.} and F. Mesa",

note = "Publisher Copyright: {\textcopyright} 2021, The Author(s).",

year = "2021",

month = dec,

doi = "10.1038/s41598-021-87028-x",

language = "English (US)",

volume = "11",

journal = "Scientific Reports",

issn = "2045-2322",

publisher = "Nature Publishing Group",

number = "1",

}

TY - JOUR

T1 - Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles

AU - González-Pedreros, G. I.

AU - Camargo-Martínez, J. A.

AU - Mesa, F.

PY - 2021/12

Y1 - 2021/12

N2 - In this paper, we report Cooper Pairs Distribution function Dcp(ω, Tc) for bcc Niobium under pressure. This function reveals information about the superconductor state through the determination of the spectral regions for Cooper-pairs formation. Dcp(ω, Tc) is built from the well-established Eliashberg spectral function and phonon density of states, calculated by first-principles. Dcp(ω, Tc) for Nb suggests that the low-frequency vibration region (ω<6meV) is where Cooper-pairs are possible. From Dcp(ω, Tc) , it is possible to obtain the Ncp parameter, which is proportional to the total number of Cooper-Pairs formed at a temperature Tc. The Ncp parameter allows an approach to the understanding of the Nb Tc anomalies, measured around 5 and 50 GPa.

AB - In this paper, we report Cooper Pairs Distribution function Dcp(ω, Tc) for bcc Niobium under pressure. This function reveals information about the superconductor state through the determination of the spectral regions for Cooper-pairs formation. Dcp(ω, Tc) is built from the well-established Eliashberg spectral function and phonon density of states, calculated by first-principles. Dcp(ω, Tc) for Nb suggests that the low-frequency vibration region (ω<6meV) is where Cooper-pairs are possible. From Dcp(ω, Tc) , it is possible to obtain the Ncp parameter, which is proportional to the total number of Cooper-Pairs formed at a temperature Tc. The Ncp parameter allows an approach to the understanding of the Nb Tc anomalies, measured around 5 and 50 GPa.

UR - http://www.scopus.com/inward/record.url?scp=85103994701&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85103994701&partnerID=8YFLogxK

U2 - 10.1038/s41598-021-87028-x

DO - 10.1038/s41598-021-87028-x

M3 - Article

C2 - 33828157

AN - SCOPUS:85103994701

SN - 2045-2322

VL - 11

JO - Scientific Reports

JF - Scientific Reports

IS - 1

M1 - 7646

ER -

Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles

Abstract

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this