Abstract
The structure of Cu 12at.%In and Cu 23at.%In alloy melts were studied by using a high-temperature X-ray diffractometer. The radial distribution functions (RDF) were obtained, which reflect the structure information of melts in real space. Gaussian decomposition of the RDFs shows the changing behavior of Cu Cu type clusters in the melts. The interatomic distance and the atom number of the clusters decrease with increasing temperature. The structure evolution and the so-called “thermal contraction” of clusters in the melts are discussed.
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