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dc.creatorCanfield, PC
dc.creatorBudko, SL
dc.creatorCho, BK
dc.creatorLacerda, A.
dc.creatorFarrell, D.
dc.creatorJohnstonHalperin, E.
dc.creatorKalatsky, VA
dc.creatorPokrovsky, Valery L.
dc.date.accessioned2011-10-10T21:08:49Z
dc.date.available2011-10-10T21:08:49Z
dc.date.issued1997
dc.identifier.citationPC Canfield, SL Budko, BK Cho, A. Lacerda, D. Farrell, E. JohnstonHalperin, VA Kalatsky and Valery L. Pokrovsky. Phys.Rev.B 55 970-976 1997."Copyright (1997) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevB.55.970
dc.identifier.urihttps://hdl.handle.net/1969.1/127300
dc.descriptionJournals published by the American Physical Society can be found at http://journals.aps.org/en
dc.description.abstractDetailed measurements of M(2 K, H, theta) of HoNi2B2C, where theta is the angle that the applied field H makes with the [110] axis while remaining perpendicular to the crystallographic c axis, reveal three metamagnetic transitions with angular dependences H-c1 = (4.1 +/- 0.1 kG)/cos(theta), H-c2 = 8.4 +/- 0.2 kG/cos(phi), and H-c3 = (6.6 +/- 0.2 kG)/sin(phi), where phi = theta-45 is the angle from the [100] axis. The high-field saturated moment, M(sat) approximate to 10 mu(B)cos theta is consistent with the local moments being confined to the [110] direction. The locally saturated moments for fields between H-ci (i = 1, 2, 3) also manifest angular dependences that are consistent with combinations of local moments along [110] axes. Analysis of these data lead us to infer that the net distribution of moments is (up arrow down arrow up arrow down arrow up arrow down arrow) for H up arrow up arrow-->) for H-c2 up arrow up arrow-->) for H-c2 H-c3.en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectMAGNETIC-STRUCTUREen
dc.subjectSUPERCONDUCTIVITYen
dc.subjectTMNI2B2Cen
dc.subjectERNI2B2Cen
dc.subjectDYNI2B2Cen
dc.subjectSTATEen
dc.subjectHEATen
dc.subjectPhysicsen
dc.titleAngular dependence of metamagnetic transitions in HoNi2B2Cen
dc.typeArticleen
local.departmentPhysics and Astronomyen


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