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000093366 1001_ $$aKaban, I.
000093366 1101_ $$aDESY$$bExperiments with synchrotron radiation
000093366 245__ $$aStructure of $GeSe_4-In$ and $GeSe_5-In$ glasses
000093366 260__ $$aBristol$$bIOP Publ.$$c2010
000093366 300__ $$a404205
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000093366 440_0 $$0PERI:(DE-600)1472968-4$$aJ. Phys. Condens. Matter$$v22$$x0953-8984$$y40
000093366 500__ $$3Converted on 2013-05-30 14:43
000093366 500__ $$3Converted on 2013-06-21 19:21
000093366 520__ $$a(Ge(0.2)Se(0.8))(100-x)In(x) and (Ge(0.17)Se(0.83))(100-x)In(x) (x = 0, 5, 10, 15 at.%) chalcogenide glasses have been studied with high-energy x-ray diffraction, neutron diffraction and extended x-ray absorption spectroscopy at Ge, Se and In K-edges. The experimental data were modelled simultaneously with the reverse Monte Carlo simulation method. GeSe(4/2) tetrahedra are shown to be the main structural units in the binary and ternary glasses investigated. Indium bonds to the excess Se atoms in the ternary Ge-Se-In glasses. While the majority of In atoms have three Se neighbours, some In atoms may be tetrahedrally coordinated by Se.
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000093366 650_7 $$07440-56-4$$2NLM Chemicals$$aGermanium
000093366 650_7 $$07440-74-6$$2NLM Chemicals$$aIndium
000093366 650_7 $$07782-49-2$$2NLM Chemicals$$aSelenium
000093366 650_2 $$2MeSH$$aComputer Simulation
000093366 650_2 $$2MeSH$$aGermanium: chemistry
000093366 650_2 $$2MeSH$$aGlass: chemistry
000093366 650_2 $$2MeSH$$aIndium: chemistry
000093366 650_2 $$2MeSH$$aModels, Chemical
000093366 650_2 $$2MeSH$$aMonte Carlo Method
000093366 650_2 $$2MeSH$$aSelenium: chemistry
000093366 650_2 $$2MeSH$$aX-Ray Absorption Spectroscopy
000093366 650_2 $$2MeSH$$aX-Ray Diffraction
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000093366 7001_ $$aJóvári, P.
000093366 7001_ $$aPetkova, T.
000093366 7001_ $$aPetkov, P.
000093366 7001_ $$aStoilova, A.
000093366 7001_ $$aHoyer, W.
000093366 7001_ $$aBeuneu, B.
000093366 773__ $$0PERI:(DE-600)1472968-4$$a10.1088/0953-8984/22/40/404205$$gVol. 22, p. 404205$$p404205$$q22<404205$$tJournal of physics / Condensed matter$$v22$$x0953-8984$$y2010
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000093366 9141_ $$a(c) Institute of Physics.$$y2010
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