<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:creator>Khasanov R</dc:creator>
  <dc:creator>Bendele M</dc:creator>
  <dc:creator>Amato A</dc:creator>
  <dc:creator>Conder K</dc:creator>
  <dc:creator>Keller H</dc:creator>
  <dc:creator>Klauss HH</dc:creator>
  <dc:creator>Luetkens H</dc:creator>
  <dc:creator>Pomjakushina E</dc:creator>
  <dc:date>2010</dc:date>
  <dc:description xmlns:ns0="xml" ns0:lang="en">The superfluid density, rho{s}, of the iron chalcogenide superconductor, FeSe1-x, was studied as a function of pressure by means of muon-spin rotation. The analysis of rho{s}(T) within the two-gap scheme reveals that the effect on both, the transition temperature T{c} and rho{s}(0), is entirely determined by the band(s) where the large superconducting gap develops, while the band(s) with the small gap become practically unaffected.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>https://sonar.ch/global/documents/278432</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevLett.104.087004</dc:relation>
  <dc:relation>info:eu-repo/semantics/altIdentifier/pmid/20366961</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:source>Physical review letters. - 2010</dc:source>
  <dc:title xmlns:ns1="xml" ns1:lang="en">Evolution of two-gap behavior of the superconductor FeSe1-x.</dc:title>
  <dc:type>http://purl.org/coar/resource_type/c_6501</dc:type>
</oai_dc:dc>