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CHEM01200604005 A. K. Pathak - Homi Bhabha National Institute

CHEM01200604005 A. K. Pathak - Homi Bhabha National Institute

CHEM01200604005 A. K. Pathak - Homi Bhabha National Institute

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3350-3500 cm -1 (scaling factor ~0.93) and 3500-3650 cm -1 (scaling factor ~0.90). The<br />

actual scaling factor is obtained by comparing the harmonic frequency with the<br />

experimentally observed spectrum. As large number of minimum energy structures are<br />

found, weighted average IR spectra are calculated which can be best comparable to the<br />

experimental spectra. The weight factor is calculated based on Boltzmann population at<br />

100K. The weight factor is also calculated at a temperature range from 75K to 200K as<br />

the cluster experiment (NVE ensemble) is carried out in this low temperature range. The<br />

calculated IR spectra ~100K for all this three systems are close to the experimental<br />

spectra. So, based on this scaling factor, weighted average scaled IR spectra are<br />

calculated at 100K for Cl •− 2 .nH 2 O (n=3-5) and are shown in Fig. 3.4(II) along with the<br />

experimental spectrum. An excellent agreement with experimental results is observed.<br />

Table 3.1. Population (P i ) of the conformers of clusters of each size have been calculated based on free<br />

energy change at 100 K (T) following Boltzmann distribution. Structures are shown in Fig. 3.2.<br />

Structure III-A III-B III-C III-D III-E III-F IV-A IV-B IV-C IV-D<br />

Population<br />

0.54 0.04 0.08 0.09 0.22 0.03 0.53 0.17 0.11 0.03<br />

(P i )<br />

Structure IV-E IV-F IV-G IV-H IV-I IV-J IV-K V-A V-B V-C<br />

Population<br />

0.01 0.03 0.05 0.02 0.02 0.02 0.01 0.15 0.11 0.24<br />

(P i )<br />

Structure V-D V-E V-F V-G V-H V-I V-J V-K V-L<br />

Population<br />

0.04 0.05 0.03 0.20 0.04 0.04 0.03 0.02 0.05<br />

(P i )<br />

65

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