General solution for the time-dependent Schrödinger equation

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Discussion Overview

The discussion revolves around uncertainties related to the time-dependent Schrödinger equation in quantum mechanics, specifically focusing on the interpretation of coefficients in the general solution and the derivation of the exponential form of the solution. Participants seek clarification on concepts presented in a video lecture.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • One participant questions the meaning of the coefficients αi mentioned in the video, wondering if they represent probability densities, probability amplitudes, or absolute probabilities.
  • Another participant suggests that the square modulus of α is typically referred to as the probability amplitude and questions whether the lecturer assumed knowledge of the wavefunction at t=0 to derive the coefficients.
  • A different participant proposes that α can be called an expansion coefficient and provides a formula for calculating it, indicating that it relates to the initial state of the system.
  • Further elaboration is provided on how the coefficients a_n(t) represent the projection of the state vector onto the eigenstates, and how this relates to the Schrödinger equation in matrix form.
  • One participant expresses gratitude for the clarification received regarding the coefficients and their derivation.

Areas of Agreement / Disagreement

Participants generally express uncertainty regarding the terminology and interpretation of the coefficients α. There is no consensus on the exact nature of these coefficients, and multiple interpretations are presented without resolution.

Contextual Notes

The discussion reflects varying levels of understanding of quantum mechanics concepts, particularly in relation to the time-dependent Schrödinger equation and the mathematical formalism involved. Some assumptions about prior knowledge are evident, but not all participants share the same background.

Who May Find This Useful

This discussion may be useful for students and enthusiasts of quantum mechanics who are grappling with the concepts of the time-dependent Schrödinger equation and the interpretation of coefficients in quantum state representations.

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

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