<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-06-08T01:00:59Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/52155" metadataPrefix="mods">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/52155</identifier><datestamp>2024-08-29T17:49:37Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</setSpec></header><metadata><mods:mods xmlns:mods="http://www.loc.gov/mods/v3" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-1.xsd">
   <mods:name>
      <mods:namePart>Forker, M.</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Presa Muñoz De Toro, Patricia Marcela De La</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Müller, S:</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Lindbaum, A.</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Gratz, E.</mods:namePart>
   </mods:name>
   <mods:extension>
      <mods:dateAvailable encoding="iso8601">2023-06-20T12:40:19Z</mods:dateAvailable>
   </mods:extension>
   <mods:extension>
      <mods:dateAccessioned encoding="iso8601">2023-06-20T12:40:19Z</mods:dateAccessioned>
   </mods:extension>
   <mods:originInfo>
      <mods:dateIssued encoding="iso8601">2004-07</mods:dateIssued>
   </mods:originInfo>
   <mods:identifier type="issn">1098-0121</mods:identifier>
   <mods:identifier type="doi">10.1103/PhysRevB.70.014302</mods:identifier>
   <mods:identifier type="uri">https://hdl.handle.net/20.500.14352/52155</mods:identifier>
   <mods:identifier type="officialurl">http://dx.doi.org/10.1103/PhysRevB.70.014302</mods:identifier>
   <mods:identifier type="relatedurl">https://journals.aps.org</mods:identifier>
   <mods:abstract>Rare-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)&lt;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&lt;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.</mods:abstract>
   <mods:language>
      <mods:languageTerm>eng</mods:languageTerm>
   </mods:language>
   <mods:accessCondition type="useAndReproduction">open access</mods:accessCondition>
   <mods:titleInfo>
      <mods:title>Vacancy motion in rare-earth-deficient R_(1-x)Ni_2 Laves phases observed by perturbed angular correlation spectroscopy</mods:title>
   </mods:titleInfo>
   <mods:genre>journal article</mods:genre>
</mods:mods></metadata></record></GetRecord></OAI-PMH>