Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles
Abstract In this paper, we report Cooper Pairs Distribution function $${D}_{cp}(\omega ,{T}_{c})$$ 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. $${D}_{cp...
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2021
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oai:doaj.org-article:74ddddcfda99469cb1d2af8c8518fee22021-12-02T14:21:16ZCooper Pairs Distribution function for bcc Niobium under pressure from first-principles10.1038/s41598-021-87028-x2045-2322https://doaj.org/article/74ddddcfda99469cb1d2af8c8518fee22021-04-01T00:00:00Zhttps://doi.org/10.1038/s41598-021-87028-xhttps://doaj.org/toc/2045-2322Abstract In this paper, we report Cooper Pairs Distribution function $${D}_{cp}(\omega ,{T}_{c})$$ D cp ( ω , T c ) for bcc Niobium under pressure. This function reveals information about the superconductor state through the determination of the spectral regions for Cooper-pairs formation. $${D}_{cp}(\omega ,{T}_{c})$$ D cp ( ω , T c ) is built from the well-established Eliashberg spectral function and phonon density of states, calculated by first-principles. $${D}_{cp}(\omega ,{T}_{c})$$ D cp ( ω , T c ) for Nb suggests that the low-frequency vibration region $$\left(\omega <6 \,{\text{meV}}\right)$$ ω < 6 meV is where Cooper-pairs are possible. From $${D}_{cp}(\omega ,{T}_{c})$$ D cp ( ω , T c ) , it is possible to obtain the $${N}_{cp}$$ N cp parameter, which is proportional to the total number of Cooper-Pairs formed at a temperature $${T}_{c}$$ T c . The $${N}_{cp}$$ N cp parameter allows an approach to the understanding of the Nb $${T}_{c}$$ T c anomalies, measured around 5 and 50 GPa.G. I. González-PedrerosJ. A. Camargo-MartínezF. MesaNature PortfolioarticleMedicineRScienceQENScientific Reports, Vol 11, Iss 1, Pp 1-6 (2021) |
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Medicine R Science Q G. I. González-Pedreros J. A. Camargo-Martínez F. Mesa Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles |
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Abstract In this paper, we report Cooper Pairs Distribution function $${D}_{cp}(\omega ,{T}_{c})$$ D cp ( ω , T c ) for bcc Niobium under pressure. This function reveals information about the superconductor state through the determination of the spectral regions for Cooper-pairs formation. $${D}_{cp}(\omega ,{T}_{c})$$ D cp ( ω , T c ) is built from the well-established Eliashberg spectral function and phonon density of states, calculated by first-principles. $${D}_{cp}(\omega ,{T}_{c})$$ D cp ( ω , T c ) for Nb suggests that the low-frequency vibration region $$\left(\omega <6 \,{\text{meV}}\right)$$ ω < 6 meV is where Cooper-pairs are possible. From $${D}_{cp}(\omega ,{T}_{c})$$ D cp ( ω , T c ) , it is possible to obtain the $${N}_{cp}$$ N cp parameter, which is proportional to the total number of Cooper-Pairs formed at a temperature $${T}_{c}$$ T c . The $${N}_{cp}$$ N cp parameter allows an approach to the understanding of the Nb $${T}_{c}$$ T c anomalies, measured around 5 and 50 GPa. |
format |
article |
author |
G. I. González-Pedreros J. A. Camargo-Martínez F. Mesa |
author_facet |
G. I. González-Pedreros J. A. Camargo-Martínez F. Mesa |
author_sort |
G. I. González-Pedreros |
title |
Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles |
title_short |
Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles |
title_full |
Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles |
title_fullStr |
Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles |
title_full_unstemmed |
Cooper Pairs Distribution function for bcc Niobium under pressure from first-principles |
title_sort |
cooper pairs distribution function for bcc niobium under pressure from first-principles |
publisher |
Nature Portfolio |
publishDate |
2021 |
url |
https://doaj.org/article/74ddddcfda99469cb1d2af8c8518fee2 |
work_keys_str_mv |
AT gigonzalezpedreros cooperpairsdistributionfunctionforbccniobiumunderpressurefromfirstprinciples AT jacamargomartinez cooperpairsdistributionfunctionforbccniobiumunderpressurefromfirstprinciples AT fmesa cooperpairsdistributionfunctionforbccniobiumunderpressurefromfirstprinciples |
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