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Handbook of Solvents - George Wypych - ChemTech - Ventech!

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8.2 Basic simplifications <strong>of</strong> quantum model 421<br />

∂<br />

∂t<br />

i� Ψ( xt , ) HΨ( xt , )<br />

= [8.2]<br />

In practice, it expresses how the stateΨ(x) <strong>of</strong> the system evolves in time (i.e., it gives ∂Ψ(x)/<br />

∂t when Ψ(x) is known).<br />

Note that in eq. [8.1] the time t was not included among the parameters defining H<br />

(and Ψ): with eq. [8.1] we are looking at stationary states, not depending on time. In spite <strong>of</strong><br />

this, eq. [8.1] may be applied to liquids, which are characterized by a continuous dynamic<br />

exchange <strong>of</strong> energy through collisions, and by a continuous displacement <strong>of</strong> the constituting<br />

molecules. This is not a problem for the use <strong>of</strong> the time independent formulation <strong>of</strong> the<br />

Schrödinger equation for liquids: eq. [8.1] actually includes kinetic energy and all related<br />

dynamic aspects. A direct use <strong>of</strong> eq. [8.1] for liquids means to treat liquids at equilibrium.<br />

We shall not make explicit use <strong>of</strong> the second equation, even when the nonequilibrium problem<br />

is considered; the use <strong>of</strong> the semiclassical approximation permits us to treat time dependent<br />

phenomena at the classical level, simpler to use.<br />

Let us come back to the expression <strong>of</strong> H(x). The number <strong>of</strong> parameters within (x) is exceedingly<br />

large if the system is a liquid. Fortunately, things may be simplified by using<br />

factorization techniques.<br />

When a system contains two subsystems (say A and B) that do not interact, the<br />

Hamiltonian can be partitioned so:<br />

( ) ( ) ( )<br />

H x = H x + H x<br />

[8.3]<br />

A A B B<br />

This rigorously leads to a factorization <strong>of</strong> Ψ:<br />

( x) ( x ) ( x )<br />

Ψ = Ψ + Ψ<br />

[8.4]<br />

A A B B<br />

and to a partition <strong>of</strong> the energy:<br />

E = E A + E B<br />

[8.5]<br />

Equation [8.1] is in consequence transformed, without simplifications, into two simpler<br />

equations:<br />

( ) Ψ ( ) Ψ ( )<br />

H x x = E x<br />

[8.6a]<br />

A A A A A A A<br />

( ) Ψ ( ) Ψ ( )<br />

H x x = E x<br />

[8.6b]<br />

B B B B B B B<br />

In practice, there are always interactions between A and B. The Hamiltonian may always<br />

be written as:<br />

( ) ( ) ( ) ( )<br />

H x = H x + H x + H x<br />

[8.7]<br />

A A B B AB<br />

The relative magnitude <strong>of</strong> the coupling term permits us to distinguish among three notable<br />

cases.<br />

1) If the coupling term is very small, it may be neglected, coming back to<br />

equations [8.6].

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