摘要
在室温和液氮温度下研究了(n-C_(16)H_(33)NH_3)_2MX_4(简称C_(16)MX)及其相应化合物n-C_(16)H_(33)NH_3X(简称C_(16)X)于4000~50cm^(-1)范围的红外光谱。结果表明,它们都形成N-H…X型氢键,氢键强度是C_(16)X大于C_(16)MX。后者氢键的强度是按Cl>Br>I的顺序递减。C_(16)MX的光谱性质可按金属离子性质分为Cu^(2+)(Cu^(2+)、Cd^(2+)、Mn^(2+))和Zn^(2+)(Zn^(2+)、Co^(2+))两组,阴离子配位多面体的形状对其光谱性质有明显影响。还比较了室温与低温下的远红外光谱,证明了M—X键是离子键。
The infrared spectra of the perovskite compounds of general formula (n-C_(16)H_(33)NH_3)_2MX_4 (abbr. as C_(16)MX; M=Cu^(2+), Cd^(2+), Mn^(2+), Zn^(2+) or Co^(2+); X=Cl, Br or I) and their corresponding compounds n-C_(16)H_(33)NH_3X (abbr. as C_(16)X) have been studied in the 4000~50cm^(-1) range at room and liquid nitrogen temperature. The results showthat the hydrogen bonds are stronger in C_(16)X than in C_(16)MX and the strength of hydrogen bonds decrease in Cl>Br>I order for C_(16)MX. The characteristic of the spectra of C_(16)MX can be grouped under two heads—Cu^(2+) group (Cu^(2+), Cd^(2+), Mn^(2+)) and Zn^(2+) group (Zn^(2+), Co^(2+)) by means of the two different polyhedrons of anions. The comparison between the far infrared spectra at the two temperatures suggests that the M—X bonds are ionic.
出处
《光谱学与光谱分析》
SCIE
EI
CAS
CSCD
北大核心
1991年第5期8-12,共5页
Spectroscopy and Spectral Analysis