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   Light and atoms  -  Part 1

   Quantum mechanics of time developement


   Stationary states - eigenstates of H  vs superpositions of states

   An eigenstate of H - eigenvalue of Energy - stationary probability distribution - NO CHANGE

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   We discuss first a very simple problem  - two identical potential wells for one electron

   The state in one well is known   -  what happens when 2 wells are present
   First  generally about superposition of 2 eigenstates - the original simple sum will be
   modified by the additional phase

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  In the above: TASK consider phi1 to be an 1s-state and phi2 an 2p0-state - opposite parity. Their superposition will be
                        a density concentration on the positive z-half. As the phase changes with time, it can become also simply (-1).
                        What would happen?  Make a sketch of the situation - for simplicity you can draw a similar 1-dimensional problem.


   The 2-well animation spread out in time

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   Well known result illustrated by animation                                                        (copied from last year)



This animation shows
time developement of
PROBABILITY DENSITY

We know that eigenstates of the whole                       H = H0 + V1  + V2           form a sort of split doublet (if the wells are moderately separated)
More details are below
Physics:   the "electron" is placed in a state at                   t=0                  confined to    ONE WELL ONLY         (1 well eigenstate)

The probability   is seen to be    OSCILLATING    between the two wells    
                                                                               This is seen from the EIGENSTATES of the whole problem
Note that we discuss two "sets" of state, the phi - eigenstates of simplified system, and the psi eigenstates of the whole
system


   The probability flows back and forth in this simple case.
   There are many realization of this 2-state time developement, usually described by the following matrix

                      | a   b  |
                      | b*  c  |


         Here we model it by two wells (  b is then a probability amplitude of transfer from one well to the other )

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    We assume here that the approximation of states being linear combinations is sufficiently precise
        ( we should remember that the actual solutions must be somewhat different; if the wells
          are "further from each other", this approximation is better. However, this is a detail not important
         for the understanding of the mechanism )

    Note that there are two set of states as indicated - this will be discussed several times below

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     In 2-state ( 2 well ) case  we get the 2 eigenstates (which are stationary - but delocalized - probability to be "both places" )
     One possible description is in terms of the two eigenstates

    Now considering the "asymetric case" - where the other well has a "quasi-continuum" of eigenstates
    There will also be "splitting", there will be N+1 eigenstates
    The "amplitude" of the "left" state in each of the eigenstates will be roughly such that
                                                     its square follows
                                                     the Lorentz profile   -  this will be also discussed later see next lecture here
    In this asymmetric case, the probability simply "flows away"  - if N is large enough
                                                                                                        - exponential decay in the  continuum limit                             

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    Solving TDSE  - Time Dependent Schrödinger Equation - by expansion in eigenstates                                ODE ordinary diff. equation
    This can be done exactly ( as exactly as the expansion is)  - by solving the below shown system of couple ODE
    or
    it is used as a basis for so called Time dependent perturbation theory

    Below - Solving TDSE using expansion with time-dependent expansion coefficients 

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       continuation - Solving TDSE using expansion with time-dependent expansion coefficients 
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          Solving TDSE using expansion with time-dependent expansion coefficients
          Time dependent perturbation theory
          in simple terms it is an assumption that the initial state basicaly continues to be close to 100%
                                                                  while the amplitudes of the "final states" remain very very small forever

          Here, eventually, it will be used for finding not the probabilities, but rate of change of the probability
          In some other applications, the actual probability is estimated (atomic and molecular collision theory etc)

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    NEXT:     Fermi Golden rule
                   The natural line width
                   Density of states for photons



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