Matches in SemOpenAlex for { <https://semopenalex.org/work/W2081569889> ?p ?o ?g. }
- W2081569889 abstract "We have investigated the temperature dependence of the upper critical field ${H}_{mathrm{c}2}$($T$ ) in a LiFeAs single crystal by direct measurements of resistivity under static magnetic fields up to 36 T. We find in the case of a magnetic field $H$ along the $ab$ plane that ${H}_{mathrm{c}2}^{ab}$(0) $=$ 30 T is clearly lower than the orbital limiting field ${H}_{mathrm{c}2}^{mathrm{orb},ab}$(0) $=$ 39.6 T estimated by the |${mathit{dH}}_{mathrm{c}2}^{ab}$/$mathit{dT}$ |${}_{Tc}$, suggesting the presence of both Pauli- and orbital-limiting effects in the pair breaking process. The best fit of ${H}_{mathrm{c}2}^{ab}$($T$ ) to the Werthamer--Helfand--Hohenberg formula results in the Maki parameter ensuremath{alpha} $=$ 0.9 and negligible spin-orbit scattering constant (${ensuremath{lambda}}_{mathrm{so}}$ $=$ 0.0). On the other hand, for $H$ along the $c$ axis, ${H}_{mathrm{c}2}^{c}$($T$ ) increases linearly down to our lowest temperature of 0.8 K, which can be explained by the multiband effects. The anisotropy ratio ${H}_{mathrm{c}2}^{ab}$($T$ )/${H}_{mathrm{c}2}^{c}$($T$ ) is 3 near ${T}_{mathrm{c}}$ and systematically decreases upon lowering temperature to become 1.3 at zero temperature. A comparative overview of the behavior of ${H}_{mathrm{c}2}^{ab}$($T$ ) in various Fe-based superconductors shows that, similar to LiFeAs, the calculated ${H}_{mathrm{c}2}^{mathrm{orb},ab}$(0) is generally much larger than the measured ${H}_{mathrm{c}2}^{ab}$(0) and thus finite ensuremath{alpha} values ranging from ensuremath{sim}0.4 to 3 are necessary to describe the low temperature ${H}_{mathrm{c}2}^{ab}$($T$ ) behaviors. Moreover, LiFeAs is found to have the smallest |${mathit{dH}}_{mathrm{c}2}^{ab}$/$mathit{dT}$ |${}_{Tc}$ values, indicating that LiFeAs is one of the cleanest Fe-based superconductors with a finite Maki parameter. We also discuss the implications of multiband effects and spin-orbit scattering based on the finding that the estimated Pauli-limiting field is generally much larger than the BCS prediction in the Fe-based superconductors." @default.
- W2081569889 created "2016-06-24" @default.
- W2081569889 creator A5044566727 @default.
- W2081569889 creator A5051307137 @default.
- W2081569889 creator A5056137840 @default.
- W2081569889 creator A5060612800 @default.
- W2081569889 creator A5070920491 @default.
- W2081569889 creator A5075247114 @default.
- W2081569889 date "2011-09-06" @default.
- W2081569889 modified "2023-09-30" @default.
- W2081569889 title "Pauli-limiting effects in the upper critical fields of a clean LiFeAs single crystal" @default.
- W2081569889 cites W1480030948 @default.
- W2081569889 cites W1568459688 @default.
- W2081569889 cites W1573086958 @default.
- W2081569889 cites W1600789377 @default.
- W2081569889 cites W1632691808 @default.
- W2081569889 cites W1800261904 @default.
- W2081569889 cites W1801966322 @default.
- W2081569889 cites W1820636537 @default.
- W2081569889 cites W1967146507 @default.
- W2081569889 cites W1976175889 @default.
- W2081569889 cites W1982087566 @default.
- W2081569889 cites W1994245883 @default.
- W2081569889 cites W2003296753 @default.
- W2081569889 cites W2007082889 @default.
- W2081569889 cites W2007496958 @default.
- W2081569889 cites W2011721578 @default.
- W2081569889 cites W2012188556 @default.
- W2081569889 cites W2013212876 @default.
- W2081569889 cites W2016421201 @default.
- W2081569889 cites W2020801097 @default.
- W2081569889 cites W2022761082 @default.
- W2081569889 cites W2022934982 @default.
- W2081569889 cites W2024333784 @default.
- W2081569889 cites W2025678989 @default.
- W2081569889 cites W2036356326 @default.
- W2081569889 cites W2044196606 @default.
- W2081569889 cites W2047475712 @default.
- W2081569889 cites W2047509300 @default.
- W2081569889 cites W2051694055 @default.
- W2081569889 cites W2053241105 @default.
- W2081569889 cites W2056078006 @default.
- W2081569889 cites W2056547846 @default.
- W2081569889 cites W2064990651 @default.
- W2081569889 cites W2071545965 @default.
- W2081569889 cites W2072287487 @default.
- W2081569889 cites W2073056092 @default.
- W2081569889 cites W2073427212 @default.
- W2081569889 cites W2075995380 @default.
- W2081569889 cites W2076376389 @default.
- W2081569889 cites W2079223380 @default.
- W2081569889 cites W2086877182 @default.
- W2081569889 cites W2090870829 @default.
- W2081569889 cites W2091904804 @default.
- W2081569889 cites W2095428523 @default.
- W2081569889 cites W2101288517 @default.
- W2081569889 cites W2130556287 @default.
- W2081569889 cites W2133853524 @default.
- W2081569889 cites W2146728849 @default.
- W2081569889 cites W2160746793 @default.
- W2081569889 cites W3098083725 @default.
- W2081569889 cites W3098979843 @default.
- W2081569889 cites W3099751844 @default.
- W2081569889 cites W3099828435 @default.
- W2081569889 cites W3101417844 @default.
- W2081569889 cites W3102429861 @default.
- W2081569889 cites W3102733187 @default.
- W2081569889 cites W3103213627 @default.
- W2081569889 doi "https://doi.org/10.1103/physrevb.84.104502" @default.
- W2081569889 hasPublicationYear "2011" @default.
- W2081569889 type Work @default.
- W2081569889 sameAs 2081569889 @default.
- W2081569889 citedByCount "92" @default.
- W2081569889 countsByYear W20815698892012 @default.
- W2081569889 countsByYear W20815698892013 @default.
- W2081569889 countsByYear W20815698892014 @default.
- W2081569889 countsByYear W20815698892015 @default.
- W2081569889 countsByYear W20815698892016 @default.
- W2081569889 countsByYear W20815698892017 @default.
- W2081569889 countsByYear W20815698892018 @default.
- W2081569889 countsByYear W20815698892019 @default.
- W2081569889 countsByYear W20815698892020 @default.
- W2081569889 countsByYear W20815698892021 @default.
- W2081569889 countsByYear W20815698892022 @default.
- W2081569889 countsByYear W20815698892023 @default.
- W2081569889 crossrefType "journal-article" @default.
- W2081569889 hasAuthorship W2081569889A5044566727 @default.
- W2081569889 hasAuthorship W2081569889A5051307137 @default.
- W2081569889 hasAuthorship W2081569889A5056137840 @default.
- W2081569889 hasAuthorship W2081569889A5060612800 @default.
- W2081569889 hasAuthorship W2081569889A5070920491 @default.
- W2081569889 hasAuthorship W2081569889A5075247114 @default.
- W2081569889 hasBestOaLocation W20815698891 @default.
- W2081569889 hasConcept C121332964 @default.
- W2081569889 hasConcept C127413603 @default.
- W2081569889 hasConcept C185592680 @default.
- W2081569889 hasConcept C188198153 @default.
- W2081569889 hasConcept C191486275 @default.
- W2081569889 hasConcept C26873012 @default.
- W2081569889 hasConcept C48496998 @default.