How does TDPT handle time dependent perturbations?

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Discussion Overview

The discussion revolves around the nature and implications of time-dependent perturbation theory (TDPT) in quantum mechanics, specifically addressing the transition probabilities between eigenstates of a Hamiltonian when the Hamiltonian is time-dependent. Participants explore the mathematical framework and conceptual challenges associated with the application of TDPT, particularly regarding the eigenstates of the Hamiltonian at different times.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions the validity of calculating transition probabilities to an eigenstate |phi_f> when the Hamiltonian H(t) is not equal to H_0, suggesting that |phi_f> cannot be an eigenstate of H(t) and thus the probability should be zero.
  • Another participant argues that the focus should be on the transition probability between the initial state |phi_i> and the final state |phi_f>, both of which are eigenstates of H_0, during a short time interval under the perturbation.
  • A later reply emphasizes that while the wave function evolves according to the time-dependent Schrödinger equation, the measurement at time t will collapse the wave function into an eigenstate of H(t), which may not be |phi_f>, leading to confusion about the probability calculations.
  • One participant suggests that for times before and after the perturbation, H_0 can be considered a good approximation for the eigenstates, but acknowledges that the time evolution may skew these approximations.

Areas of Agreement / Disagreement

Participants express differing views on the implications of the Hamiltonian changing over time and its effect on the eigenstates. There is no consensus on whether the transition probabilities can be accurately calculated under these conditions, indicating an unresolved debate.

Contextual Notes

Participants highlight limitations in understanding the role of eigenstates in time-dependent scenarios and the assumptions made regarding the perturbation's duration and effects on the system's evolution.

quasar987
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Hi,

I have a problem with the very nature of time dependent perturbation theory (TDPT). In TDPT, we consider a system of Hamiltonian H(t) = H_0 (for t<0), H(t)=H_0 + kW(t) (for t>0) [where k<<1], where H_0 is, for simplicity, discrete, non-degenerate and time-independent, and given that at t=0, the state of the system is |phi_i> (an eigenstate of H_0), we are interested in calculating P_if(t), the probability of finding the system in another eigenstate of H_0, |phi_f>, at time t.

But this does not make sense because at t, the hamiltonian is no longer H_0, so it will, in general, not have |phi_f> as an eigenstates. But we know that the result of a measurement will project the wave-function into one of the eigenfunction. So as soon as |phi_f> is not an eigenstate of H(t), the probability of finding the system in |phi_f> will be 0.
 
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"So as soon as |phi_f> is not an eigenstate of H(t), the probability of finding the system in |phi_f> will be 0"

I'm not sure if i fully understand your question, but why does it worry you that |phi_f> will not in general be an eigenstate of H(t)? If i remember my last quarter of undergrad quantum correctly we are only worried about the probability of transition between |phi_i> and |phi_f> (both of which are eigenstates of H_0) under a time dependent pertubation that takes place for some delta t. As far as the results of measurements "forcing" the wave-function's projections onto one of the eigenstates, simply think about the TDP as having already measured the system before (hence our eigenstate |phi_i>) as well as after, (hence |phi_f>) and the TDP simply spits out the probability of this transition within the abovementioned delta t.
 
Gza said:
"So as soon as |phi_f> is not an eigenstate of H(t), the probability of finding the system in |phi_f> will be 0"

I'm not sure if i fully understand your question, but why does it worry you that |phi_f> will not in general be an eigenstate of H(t)? If i remember my last quarter of undergrad quantum correctly we are only worried about the probability of transition between |phi_i> and |phi_f> (both of which are eigenstates of H_0) under a time dependent pertubation that takes place for some delta t. As far as the results of measurements "forcing" the wave-function's projections onto one of the eigenstates, simply think about the TDP as having already measured the system before (hence our eigenstate |phi_i>) as well as after, (hence |phi_f>) and the TDP simply spits out the probability of this transition within the abovementioned delta t.

Like you said, we have measured the system before the perturbation to be |phi_i>. Then the TDP is turned on and the wave function evolves according to the time dependent SE

[tex]i\hbar\partial_t \Psi(t)=H(t)\Psi(t)[/tex]

with initial condition Psi(0)=phi_i. Now say we measure the energy at a time t. The wave function Psi(t) will collapse into an eigenstate of H(t). It is most likely that phi_f will not be such an eigenstate for H(t), so let's suppose for simplicity that it isn't.

Sure, mathematically, nothing stops us from expanding Psi(t) in a Fourier series in |phi_n> and we can even calculate the coefficient |<Psi(t)|phi_k>|², but it does not represent the probability of finding the system in state |phi_k>. According to the expansion postulate, this probability is 0, because phi_k is not an eigenstate of H(t).

But the books say that the probability is |<Psi(t)|phi_k>|², so this is where I'm confused, and I'm asking "where in the above am I mistaken"?
 
Last edited:
quasar987 said:
But this does not make sense because at t, the hamiltonian is no longer H_0, so it will, in general, not have |phi_f> as an eigenstates. But we know that the result of a measurement will project the wave-function into one of the eigenfunction. So as soon as |phi_f> is not an eigenstate of H(t), the probability of finding the system in |phi_f> will be 0.

You should actually consider the following:
for t<0, we have H0, and for t>t1, we also have H0 as hamiltonian.
We only consider the interaction "switched on" between t=0 and t=t1.
We prepare the state at t<0 and we measure it after t=t1.

The idea is that H0 is "good enough" as eigenstate generator, but not as time evolution generator. So we consider that, for short enough times, we can take the eigenstates of H0 as good approximations to the eigenstates of the full hamiltonian, but that the neglected parts do play a cumulative role in skewing this as time evolution.
 

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