2008
DOI: 10.1039/b813076k
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Crystal structure of the new FeSe1−x superconductor

Abstract: The newly discovered superconductor FeSe(1-x) (x approximately 0.08, T(c)(onset) approximately 13.5 K at ambient pressure rising to 27 K at 1.48 GPa) exhibits a structural phase transition from tetragonal to orthorhombic below 70 K at ambient pressure-the crystal structure in the superconducting state shows remarkable similarities to that of the REFeAsO(1-x)F(x) (RE = rare earth) superconductors.

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Cited by 337 publications
(367 citation statements)
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“…Superconductivity in these materials has been discovered in 2008 by Hosono and his collaborators [24]. Later, superconductivity has been found also in Fe-chalcogenides -Fe-based compounds with elements from the 16th group: S, Se, Te [59,60,61,62].…”
Section: Superconductivity In Fe-pnictidesmentioning
confidence: 99%
“…Superconductivity in these materials has been discovered in 2008 by Hosono and his collaborators [24]. Later, superconductivity has been found also in Fe-chalcogenides -Fe-based compounds with elements from the 16th group: S, Se, Te [59,60,61,62].…”
Section: Superconductivity In Fe-pnictidesmentioning
confidence: 99%
“…For the Fe 1+x (Te-Se) system [9,[30][31][32][33], crystallographically there are two iron sites, one of which is partially occupied, while the (Te, Se) site is fully occupied. Hence the composition should be indicated as Fe 1+x (Te,Se).…”
Section: Fe 1+x (Te-se) Systemmentioning
confidence: 99%
“…Consequently, the issue of nematicity is more crucially posed for those systems where the structural transition precedes the magnetic one (T S T N ), leaving a finite temperature interval where C 4 symmetry is broken but the material remains paramagnetic [9][10][11][12]. The most notable example being FeSe where only a structural transition [13,14] is detected (the difference between the T s and T N being the largest) and the system remains paramagnetic till its SC phase [15,16], indicating that nematic degrees of freedom are not necessarily magnetic ones but probably orbital one. The microscopic origin of the nematic order is debatable with a few competitive probable scenarios [17].…”
Section: Introductionmentioning
confidence: 99%