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. Author manuscript; available in PMC: 2015 Oct 7.
Published in final edited form as: Phys Chem Chem Phys. 2013 Apr 19;15(25):10094–10111. doi: 10.1039/c3cp50439e

Fig. 4.

Fig. 4

Computed IR spectra in the 900-400 cm−1 energy range: the theoretical spectrum Ip-IIn-IIIp from Figure 2 and the simulations also including a 10% contribution from IVn/gtt (Ip-IIn-IIIp+IVn/gtt), Vn (Ip-IIn-IIIp+Vn/gct) and VIp (Ip-IIn-IIIp+VIp/ttc). IR spectra line-shapes have been convoluted with Lorentzian functions with a HWHM of 1 cm−1.