Fermi Golden Rule: Conservation of Energy

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SUMMARY

The Fermi Golden Rule describes the transition rate between quantum states, expressed as W_{fi} = \frac{2 \pi}{\hbar} \sum_{f} |V_{fi}|^2 \delta(\varepsilon_f - \varepsilon_i). In this context, the delta function indicates that energy conservation requires ( \varepsilon_f - \varepsilon_i) = 0. However, the introduction of an external potential V at time t=0 allows for energy non-conservation, leading to finite probabilities for transitions away from the delta function peak. This results in a transition rate that increases linearly with time for conserving transitions.

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mahblah
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A way to write Fermi golden rule is
W_{fi} = \sum{\frac{d P_{fi}}{dt}} = \frac{2 \pi}{\hbar} \sum_{f} |V_{fi}|^2 \delta(\varepsilon_f - \varepsilon_i)

where "i" is the initial unperturbed state and "f" is the final state of an ensemble of final states (i sum over them).

But because of \delta( \varepsilon_f - \varepsilon_i) I'm asking ( \varepsilon_f - \varepsilon_i) =0, so the inital and final state are the same??

they say that because of conservation energy must be ( \varepsilon_f - \varepsilon_i) =0, but the external potential V (i turn it on at time t=0) does not change the energy of the system (so it should be \varepsilon_f \neq \varepsilon_i)?

thanks all and sorry for my english,
MahBlah.
 
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Take a look at Messiah, Ch XVII, Sect I.4 where he has a good explanation of this. Energy does not have to be conserved, since you turned V on at t=0. However the energy disconserving transitions (away from the peak of the delta function) have a finite probability. Whereas the conserving ones (near the peak) have a probability that grows linearly with time, hence the transition rate w = dW/dt is finite.
 

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