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Vacancy motion in rare-earth-deficient R_(1-x)Ni_2 Laves phases observed by perturbed angular correlation spectroscopy

dc.contributor.authorForker, M.
dc.contributor.authorPresa Muñoz De Toro, Patricia Marcela De La
dc.contributor.authorMüller, S:
dc.contributor.authorLindbaum, A.
dc.contributor.authorGratz, E.
dc.date.accessioned2023-06-20T12:40:19Z
dc.date.available2023-06-20T12:40:19Z
dc.date.issued2004-07
dc.description©2004 The American Physical Society. Two of the authors would like to express their gratitude for financial support, P.P. from “Deutscher Akademischer Austauschdienst” (DAAD) and A.L. from the Austrian Academy of Sciences (APART 10739) and the Austrian Science Fund FWF (P14932).
dc.description.abstractRare-earth-deficient R_(1-x)Ni_2 Laves phases, which reportedly crystallize in a C15 superstructure with ordered R vacancies, have been investigated by perturbed angular correlation (PAC) measurements of electric quadrupole interactions at the site of the probe nucleus ^111Cd. Although ^111Cd resides on the cubic R site, a strong axially symmetric quadrupole interaction (QI) with frequencies ν(q)approximate to265-275 MHz has been found in the paramagnetic phases of R_(1-x)Ni_2 with R=Pr,Nd,Sm,Gd. This interaction is not observed for the heavy R constituents R=Tb,Dy,Ho,Er. The fraction of probe nuclei subject to the QI in R_(1-x)Ni_2, R=Pr,Nd,Sm,Gd, decreases from 100% at low temperatures to zero at T>300 K and 500 K for R=Sm,Gd and R=Pr,Nd, respectively. At T=100 K the QI is static within the PAC time window, but at T=200 K fluctuations with correlation times τ_(C)<10^(-6) s, have been detected. These observations can be explained consistently by two assumptions: (i) the mother isotope ^111In of the PAC probe ^111Cd constitutes an attractive potential for vacancies and (ii) the R vacancies in R_(1-x)Ni_2 are highly mobile at temperatures T<300 K, which is incompatible with a static vacancy superstructure. The measurements indicate a decrease of the vacancy-probe binding energy from the light to the heavy R constituents of R_(1-x)Ni_2. For R=Pr,Nd,Sm,Gd the binding energy is in the range 0.15 - 0.40 eV. The activation energy E_(A) for vacancy jumps near the probe derived from the temperature dependence of the nuclear spin relaxation at 200 ≤ K ≤ T ≤ 300 K is small. The values observed in different samples cover a range of 0.1 eV ≤ 0.23 eV. The trial frequency w_(0) of these jumps appears to be correlated to the activation energy: ln w_(0)(MHz)approximate 58E_(A)(eV). At high temperatures T > 500 K nuclear spin relaxation related to vacancy hopping is observed in nearly all R_(1-x)N_i2. Auxiliary ^111Cd PAC measurements have been carried in Sc_0.95Ni_2, ScNi_2, ScNi_0.97, Gd_2Ni_(17), GdNi_5, GdNi_3, and GdNi.
dc.description.departmentDepto. de Física de Materiales
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipDeutscher Akademischer Austauschdienst (DAAD)
dc.description.sponsorshipAustrian Academy of Sciences
dc.description.sponsorshipAustrian Science Fund FWF
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/45593
dc.identifier.doi10.1103/PhysRevB.70.014302
dc.identifier.issn1098-0121
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevB.70.014302
dc.identifier.relatedurlhttps://journals.aps.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/52155
dc.issue.number1
dc.journal.titlePhysical review B
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.projectIDAPART 10739
dc.relation.projectIDP14932
dc.rights.accessRightsopen access
dc.subject.cdu538.9
dc.subject.keywordElectric hyperfine interactions
dc.subject.keywordQuadrupole interactions
dc.subject.keyword^111Cd
dc.subject.keywordTemperature
dc.subject.keywordRCo_2
dc.subject.ucmFísica de materiales
dc.subject.ucmFísica del estado sólido
dc.subject.unesco2211 Física del Estado Sólido
dc.titleVacancy motion in rare-earth-deficient R_(1-x)Ni_2 Laves phases observed by perturbed angular correlation spectroscopy
dc.typejournal article
dc.volume.number70
dspace.entity.typePublication
relation.isAuthorOfPublication84282349-b588-49a8-812f-1f807d37d425
relation.isAuthorOfPublication.latestForDiscovery84282349-b588-49a8-812f-1f807d37d425

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