General solution for the time-dependent Schrödinger equation

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Dyatlov
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Hello! I have two uncertainties (hehe) about two concepts from a QM time-dependent Schrödinger equation video.
The video is
I cannot move on further if I don't fully grasp everything he explains in the video. My two issues are:
1) The general solution for the time-dependent Schrödinger equation starts at 55:20.He uses αi for a set of coefficients of states. What exactly are these? the probability densities? probability amplitudes? the absolute probabilities? He mentions any state vector can be written as a superposition of eigenvectors of the energy, so α should be a probability amplitude, so you can calculate it's squared modulus.
2) At 1:03:04 he comes up with the exponential solution e^-iEjt. Where exactly from does he gets α(0) from?
Appreciating any kind of answer which would help me shed some light on these two things. Cheers!
 
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1) Usually one calls the square modulus of ##\alpha## as the probability amplitude.
2) Didn't he say that he assumes he knows the wavefunction at t=0, and hence the corresponding expansion coefficients?
 
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blue_leaf77 said:
1) Usually one calls the square modulus of ##\alpha## as the probability amplitude.
2) Didn't he say that he assumes he knows the wavefunction at t=0, and hence the corresponding expansion coefficients?
Thanks for the reply.
1) Fair enough but my question was what does α stand for (he calls it coefficient of states).
 
If your problem is simply being confused as what to call ##\alpha##, you can also adopt what he said in the video. I personally would call it expansion coefficient, the way to obtain it is through the equation ##\alpha_i(t) = \langle i | e^{-iHt/\hbar} | \psi(0) \rangle ##. I guess you know about it already.
 
Dyatlov said:
Hello! I have two uncertainties (hehe) about two concepts from a QM time-dependent Schrödinger equation video.
The video is
I cannot move on further if I don't fully grasp everything he explains in the video. My two issues are:
1) The general solution for the time-dependent Schrödinger equation starts at 55:20.He uses αi for a set of coefficients of states. What exactly are these? the probability densities? probability amplitudes? the absolute probabilities? He mentions any state vector can be written as a superposition of eigenvectors of the energy, so α should be a probability amplitude, so you can calculate it's squared modulus.
2) At 1:03:04 he comes up with the exponential solution e^-iEjt. Where exactly from does he gets α(0) from?
Appreciating any kind of answer which would help me shed some light on these two things. Cheers!


When we write [tex]|\Psi(t) \rangle = \sum_{n} a_{n}(t) |n\rangle , \ \ \ \ a_{n}(t) = \langle n|\Psi(t)\rangle[/tex] we are simply representing the abstract state vector [itex]|\Psi\rangle[/itex] by a set of numbers [itex]a_{n}[/itex] which have all the information content in the state Psi. You should know that from vector algebra. Recall the similarity with the vector relations [tex]\vec{V}=\sum_{i} v_{i} \hat{e}_{i}, \ \ \ \ v_{i} = \hat{e}_{j} \cdot \vec{V} .[/tex] So, you say that [itex]a_{n}(t)[/itex] are the components of the “vector” [itex]|\Psi\rangle[/itex] in the [itex]|n\rangle[/itex] “direction”, projection of [itex]|\Psi\rangle[/itex] on [itex]|n\rangle[/itex], how much of the state [itex]|n\rangle[/itex] one can find in the state [itex]|\Psi\rangle[/itex], transition (or probability) amplitude from [itex]|\Psi\rangle[/itex] to [itex]|n\rangle[/itex], or (even better) matrix representation of the state vector [itex]|\Psi\rangle[/itex]. Notice that in [itex]a_{n}[/itex]-representation, the Schrödinger equation becomes [tex]i \frac{d}{d t} \langle m | \Psi \rangle = \sum_{n} \langle m |H| n \rangle \ a_{n}(t) ,[/tex] or [tex]i \frac{d a_{m}}{d t} = \sum_{n} H_{m n} \ a_{n}(t) .[/tex] This was the starting equation of the so-called Matrix Mechanics of Heisenberg. It is just an equivalent, matrix form of the differential equation of Schrödinger. Now, suppose that [itex]|n\rangle[/itex] form eigen-states of the Hamiltonian, [itex]H|n\rangle = E_{n}|n\rangle[/itex], then [tex]H_{m n} = \langle m | H | n \rangle = E_{n} \delta_{n m} ,[/tex] and the above matrix equation becomes (no sum on m) [tex]i \frac{d a_{m}(t)}{d t} = E_{m} a_{m}(t) .[/tex] Integrating this from [itex]t=0[/itex] to [itex]t[/itex], we find [tex]\int_{t=0}^{t} \frac{d a_{m}(t)}{a_{m}(t)} = - i E_{m} \int_{0}^{t} dt ,[/tex][tex]\ln |\frac{a_{m}(t)}{a_{m}(0)}| = - i E_{m} t ,[/tex] which we normally write as [tex]a_{m}(t) = a_{m}(0) e^{ - i E_{m} t}.[/tex]
 
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Thanks a lot, that helped.