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Spectroscopic evidence of superconductivity pairing at 83 K in single-layer FeSe/SrTiO3 films
Single-layer FeSe films grown on the SrTiO 3 substrate (FeSe/STO) have attracted much attention because of their possible record-high superconducting critical temperature (T c ) and distinct electronic structures. However, it has been under debate on how high its T c can really reach due to the inco...
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Published in: | Nature communications 2021-05, Vol.12 (1), p.2840-2840, Article 2840 |
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Main Authors: | , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Single-layer FeSe films grown on the SrTiO
3
substrate (FeSe/STO) have attracted much attention because of their possible record-high superconducting critical temperature (T
c
) and distinct electronic structures. However, it has been under debate on how high its T
c
can really reach due to the inconsistency of the results from different measurements. Here we report spectroscopic evidence of superconductivity pairing at 83 K in single-layer FeSe/STO films. By preparing high-quality single-layer FeSe/STO films, we observe strong superconductivity-induced Bogoliubov back-bending bands that extend to rather high binding energy ~ 100 meV by high-resolution angle-resolved photoemission measurements. They provide a new definitive benchmark of superconductivity pairing that is directly observed up to 83 K. Moreover, we find that the pairing state can be further divided into two temperature regions. These results indicate that either T
c
as high as 83 K is achievable, or there is a pseudogap formation from superconductivity fluctuation in single-layer FeSe/STO films.
How high the superconducting transition temperature can reach in single layer FeSe/SrTiO
3
films has been under debate. Here, the authors use Bogoliubov back-bending bands as a benchmark and demonstrate that superconductivity pairing can be realized up to 83 K in this system. |
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ISSN: | 2041-1723 2041-1723 |
DOI: | 10.1038/s41467-021-23106-y |