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000093368 1001_ $$aKaban, I.
000093368 1101_ $$aDESY$$bExperiments with synchrotron radiation
000093368 245__ $$aOn the atomic structure of $Zr_{60}Cu_{20}Fe_{20}$ metallic glass
000093368 260__ $$aBristol$$bIOP Publ.$$c2010
000093368 300__ $$a404208
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000093368 440_0 $$0PERI:(DE-600)1472968-4$$aJ. Phys. Condens. Matter$$v22$$x0953-8984$$y40
000093368 500__ $$3Converted on 2013-05-30 14:43
000093368 500__ $$3Converted on 2013-06-21 19:21
000093368 520__ $$aThe structure of Zr(60)Cu(20)Fe(20) metallic glass has been studied with high-energy x-ray diffraction, neutron diffraction and extended x-ray absorption spectroscopy and modelled with the reverse Monte Carlo simulation technique. It is found that Cu and Fe atoms prefer Zr as a nearest neighbour. The mean interatomic distance between Cu/Fe and Zr atoms in the glass is remarkably shorter than the sum of the respective atomic radii. The coordination numbers for Cu/Fe-Cu/Fe pairs are very close to each other, suggesting a regular distribution of Cu and Fe atoms in the Zr(60)Cu(20)Fe(20) metallic glass.
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000093368 650_7 $$00$$2NLM Chemicals$$aIron Compounds
000093368 650_7 $$07440-50-8$$2NLM Chemicals$$aCopper
000093368 650_7 $$07440-67-7$$2NLM Chemicals$$aZirconium
000093368 650_2 $$2MeSH$$aComputer Simulation
000093368 650_2 $$2MeSH$$aCopper: chemistry
000093368 650_2 $$2MeSH$$aGlass: chemistry
000093368 650_2 $$2MeSH$$aIron Compounds: chemistry
000093368 650_2 $$2MeSH$$aModels, Molecular
000093368 650_2 $$2MeSH$$aMonte Carlo Method
000093368 650_2 $$2MeSH$$aNeutron Diffraction
000093368 650_2 $$2MeSH$$aX-Ray Absorption Spectroscopy
000093368 650_2 $$2MeSH$$aX-Ray Diffraction
000093368 650_2 $$2MeSH$$aZirconium: chemistry
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000093368 7001_ $$aJóvári, P.
000093368 7001_ $$aBureau, B.
000093368 7001_ $$aStoica, M.
000093368 7001_ $$aMattern, N.
000093368 7001_ $$aEckert, J.
000093368 7001_ $$aHoyer, W.
000093368 7001_ $$aBeuneu, B.
000093368 773__ $$0PERI:(DE-600)1472968-4$$a10.1088/0953-8984/22/40/404208$$gVol. 22, p. 404208$$p404208$$q22<404208$$tJournal of physics / Condensed matter$$v22$$x0953-8984$$y2010
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