SYNTHESIS, CHARACTERIZATION, AND BONDING OF INDIUM CLUSTERS - NA7IN11.8, A NOVEL NETWORK STRUCTURE CONTAINING CLOSO-IN16 AND NIDO-IN11 CLUSTERS

被引:88
作者
SEVOV, SC
CORBETT, JD
机构
[1] IOWA STATE UNIV SCI & TECHNOL,DEPT CHEM,AMES,IA 50011
[2] IOWA STATE UNIV SCI & TECHNOL,AMES LAB,DOE,AMES,IA 50011
关键词
D O I
10.1021/ic00036a032
中图分类号
O61 [无机化学];
学科分类号
070301 ; 081704 ;
摘要
Reactions of the elements in proportions near 37.3 at. % Na at approximately 500, 410, and then 250-degrees-C readily produce the well-crystallized title phase. The tetragonal structure at the indium-rich limit was solved by standard single-crystal X-ray means at room temperature (P4(2)/nmc, Z = 12; a = 16.093 (4) angstrom, c = 23.384 (8) angstrom; R(F)/R(W) = 3.4/3.6%). The network structure consists of interbonded clusters-the first example of closo-In16 icosioctahedra (4m2BAR symmetry) that are 8-exo-bonded, 10-bonded nido icosahedra (fractional occupancy of the eleventh cluster site generates approximately 36% 1,3-arachno units) and four-bonded indium atoms in pairs of triangles (In16:In11(10):In1 = 1:4:12). Extended Huckel calculations that include significant interactions between directional nonbonding pairs on atoms in neighboring In16 and In11 units indicate 2n + 4 skeletal electrons are necessary for each, with no nonbonding pairs on the latter, and a closed shell for 504 electrons per cell vs 507 for the refined stoichiometry. Observed properties are in good agreement; at the indium-rich limit, the phase is a poor metal (rho-295 approximately 540-mu-OMEGA.cm) with a Pauli-like paramagnetism chi(M) = (1.7 - 1.8) X 10(-4) emu/mol after correction for core and orbital diamagnetism. The intercluster interactions appear to be closely correlated with a small region of nonstoichiometry and changes in the c lattice parameter. Some general factors in a diverse indium cluster chemistry are noted.
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页码:1895 / 1901
页数:7
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