Sudden Approximation and Adiabatic theorem

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The discussion centers on the conditions for the validity of the sudden approximation in quantum mechanics, specifically regarding the time-dependent Hamiltonian and its rapid changes. It raises concerns about the apparent conflict between the sudden approximation condition and the energy-time uncertainty principle, questioning whether the sudden approximation can ever be applied. Additionally, the conversation explores the adiabatic theorem, emphasizing the equivalence of projecting a wave function after evolving it versus evolving it to a certain state first and then projecting. The importance of the Hamiltonian's slow variation is highlighted, as it ensures that the instantaneous eigenstate evolves according to the Schrödinger equation. Overall, the dialogue clarifies the nuances of these quantum concepts and their interrelations.
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I am reading quantum mechanics (Messiah) now. And I get confused about the condition for the validity of the sudden approximation in CH. XVII. The author use perturbation theory to derive the result
<br /> T&lt;&lt;\hbar/\delta \overline{H}<br />
,when the Hamiltonian change over time T. The condition tells me that I have to vary the Hamiltonian fast enough such that the wave function is not able to response the sudden change. But uncertainty relation between energy and time tells me that
<br /> \delta t \delta H\geq \hbar<br />
Does the two condition violate each other? If it is so, does it means that in principle we can never use the sudden approximation?

My second question is about the adiabatic theorem.
The author mentions that
<br /> \lim_{T\rightarrow \infty} U_T(s)P_j(0)=P_j(s)\lim_{T\rightarrow\infty}U_T(s)<br />
in which the Hamiltonian is changing during time period T, s labels the portion the system has evolved. If s=1, means the system finishs the whole changing process. And P_j(s) is the projection operator of the eigenstate j at s.
The asymptotic property is hard for me to understand the physical meaning of it.
Does it means that when the evolving time, T, is large enough, projecting the wave function and then evolve it to s is equivalent to evolving the wave function to s first and then project to the eigen state j at s are actually the same?
 
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For the first question, you have to be careful about the energy time uncertainty principle. There are many different versions and they all have different (but precise meanings).

In your case, I suppose you are talking about the uncertainty relation described by Griffith Ch3 pg. 113, where it explicitly says Δt is the time needed for an observable to change by ~1 standard deviation, and that observable must have NO explicit time dependence, which is not your case here.

As for the second question, apply the equation to a state |n(t0)>, the instantaneous eigenstate for the time dependent Hamiltonian with continuously varying eigenvalue. This gives precisely the statement of adiabatic theorem,

U(t, t0)|n(t0)> = P_n U(t, t0)|n(t0)> so that U(t, t0)|n(t0)> is just |n(t)> (neglecting some additional phase factor, this comes from the fact that any eigenvector of the projection must either be 0 or in the space P_n projects to)

You might argue, isn't it kinda obvious |n(t0)> will evolve into |n(t)>? but keep in mind that n(t) DOES NOT solve the Schrodinger's eq in general, it is merely an eigenvector of H, the adiabatic theorem says that if H varies slowly enough, n(t) is actually a solution of the schrodinger eq. (neglecting time dependent phase factors)
 
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Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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