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Rotation and libration in a fluctuating cell

It was demonstrated in Chapter 6 that impact theory is able to describe qualitatively the main features of the drastic transformations of gas-phase spectra into liquid ones for the case of a linear molecule. The corresponding NMR projection of spectral collapse is also reproduced qualitatively. Does this reflect any pronounced physical mechanism of molecular dynamics In particular, can molecular rotation in dense media be thought of as free during short time intervals, interrupted by much shorter collisions  [Pg.224]

It seems that an affirmative answer is hardly possible on the contemporary level of our general understanding of condensed matter physics. On the other hand, it is necessary to find a reason for numerous successful expansions of impact theory outside its applicability limits. [Pg.224]

One possibility for this was demonstrated in Chapter 3. If impact theory is still valid in a moderately dense fluid where non-model stochastic perturbation theory has been already found applicable, then evidently the continuation of the theory to liquid densities is justified. This simplest opportunity of unified description of nitrogen isotropic Q-branch from rarefied gas to liquid is validated due to the small enough frequency scale of rotation-vibration interaction. The frequency scales corresponding to IR and anisotropic Raman spectra are much larger. So the common applicability region for perturbation and impact theories hardly exists. The analysis of numerous experimental data proves that in simple (non-associated) systems there are three different scenarios of linear rotator spectral transformation. The IR spectrum in rarefied gas is a P-R doublet with either resolved or unresolved rotational structure. In the process of condensation the following may happen. [Pg.224]

These times are supposed to be small enough to prevent significant reorientation of the molecule during free rotation [Pg.226]

Notice the similarity of criteria (7.3) and (1.58) the latter gives the non-adiabaticity of angular momentum changes due to collisions, the [Pg.226]


Rotation and libration in a fluctuating cell As a result, we have the following formula for the T operator... [Pg.244]


See other pages where Rotation and libration in a fluctuating cell is mentioned: [Pg.224]    [Pg.225]    [Pg.226]    [Pg.228]    [Pg.230]    [Pg.232]    [Pg.234]    [Pg.236]    [Pg.238]    [Pg.240]    [Pg.242]    [Pg.246]    [Pg.248]    [Pg.250]    [Pg.252]    [Pg.254]    [Pg.256]    [Pg.224]    [Pg.225]    [Pg.226]    [Pg.228]    [Pg.230]    [Pg.232]    [Pg.234]    [Pg.236]    [Pg.238]    [Pg.240]    [Pg.242]    [Pg.246]    [Pg.248]    [Pg.250]    [Pg.252]    [Pg.254]    [Pg.256]   


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