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dc.contributor.authorNakano, T.en
dc.contributor.authorFujiwara, N.en
dc.contributor.authorKamihara, Y.en
dc.contributor.authorHirano, M.en
dc.contributor.authorHosono, H.en
dc.contributor.authorOkada, H.en
dc.contributor.authorTakahashi, H.en
dc.contributor.alternative藤原, 直樹ja
dc.date.accessioned2011-01-06T03:10:55Z-
dc.date.available2011-01-06T03:10:55Z-
dc.date.issued2010-11-
dc.identifier.issn1098-0121-
dc.identifier.urihttp://hdl.handle.net/2433/134551-
dc.description.abstractThe relationship between antiferromagnetic (AF) fluctuation and superconductivity was investigated in the La1111 series, LaFeAsO_{1−x}F_{x} (x=0, 0.05, 0.08, 0.10, and 0.14) by examining nuclear relaxation rates (1/T1) at both ambient pressure and 3.0 GPa. The results show that the critical doping level at which low-frequency AF fluctuation vanishes is around the optimally doped regime (x∼0.10). Although the AF fluctuation is enhanced by applying pressure in the underdoped regime (0.05≤x<0.10), the increase in critical transition temperature (Tc) is small, whereas Tc remarkably increases in the overdoped regime (x=0.14), implying that the AF fluctuation is less important to the high-Tc mechanism than the density of states at the electron pocket. The x dependence of Tc at 3.0 GPa is similar to that of R1111 (R=Ce, Pr, Nd, etc.) with Tc≥40 K at ambient pressure. The relationship between Tc and the pnictogen height or lattice constant indicates that pressure application is equivalent to full rare-earth substitution. This equivalence suggests that high Tc above 40 K is realized when the AF fluctuation is absent.en
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherThe American Physical Societyen
dc.rights© 2010 The American Physical Societyen
dc.titleMagnetic fluctuations and superconductivity in LaFeAsO_{1−x}F_{x} under pressure as seen via ^{75}As NMRen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.ncidAA11187113-
dc.identifier.jtitlePhysical Review Ben
dc.identifier.volume82-
dc.identifier.issue17-
dc.relation.doi10.1103/PhysRevB.82.172502-
dc.textversionpublisher-
dc.identifier.artnum172502-
dcterms.accessRightsopen access-
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