When is it appropriate to use a time dependent Schrodinger's wave equation?

[roshan2004]

In what conditions do we use time dependent and time independent Schrödinger's wave equations?

 

[Eynstone]

The time independent Schrödinger's wave equation is used only for a stationary state.

 

[Gerenuk]

The time-dependent version is always the right choice.

However if your potential does not depend on time, but position only V(x) (unlike V(x,t)), then you can use the trial solution \psi(x,t)=\phi(x)e^{-i E t/\hbar} and derive an equation for the special part \phi of the wavefunction. You effectively get the time-independent version of the Schrödinger equation. From this time-indepedent special case you can first find \phi and E and finally put it back into the full wavefunction \psi(x,t). Please try that above exercise with the trial solution.

 

[SpectraCat]

The time-dependent version is always the right choice.

However if your potential does not depend on time, but position only V(x) (unlike V(x,t)), then you can use the trial solution \psi(x,t)=\phi(x)e^{-i E t/\hbar} and derive an equation for the special part \phi of the wavefunction. You effectively get the time-independent version of the Schrödinger equation. From this time-indepedent special case you can first find \phi and E and finally put it back into the full wavefunction \psi(x,t). Please try that above exercise with the trial solution.

I don't agree. It makes sense to use the time-dependent Schrödinger equation (TDSE) when solving a problem for a time-dependent potential. However quite often what one is most interested in is the energy spectrum and/or eigenstates of a time-independent potential. In such a case, it is preferable to solve the time-independent Schrödinger equation (TISE), either analytically (this is only rarely possible for meaningful real-world problems), or numerically (i.e. using the variational method and diagonalizing a large matrix).

Once the eigenstates are known, one then gets the time-dependent wavefunctions for free, since the time-dependent part of the wavefunction for the jth eigenstate is just:
f_j(t)=e^{-i\frac{E_j}{\hbar}t}
where E_j is just the jth eigenvalue. In fact, any time dependent wavefunction can be written as a linear combination of these solutions, since they form a complete basis.

I guess it is largely a matter of taste, but I find the latter approach simpler to understand and use.

 

[Gerenuk]

It's not a matter of taste. What you want to use merely depends on whether your potential is V(x,t) or V(x)[/tex]. What time-independent eigenstates do you want to find if you haven&#039;t even given a time-independent potential to deal with?<br /> <br /> Maybe you are referring to some perturbation theory approximations?

 

[SpectraCat]

It's not a matter of taste. What you want to use merely depends on whether your potential is V(x,t) or V(x)[/tex]. What time-independent eigenstates do you want to find if you haven&#039;t even given a time-independent potential to deal with?<br /> <br /> Maybe you are referring to some perturbation theory approximations?

<br /> <br /> Read my first sentence again .. you said it is *always* best to use the TDSE. I said it is best to use the TISE when solving a time independent potential. <br /> <br /> To answer your question, yes, I would also tend to use the TISE first in cases where it is appropriate to treat the time-variant part of the potential as a (weak) perturbation.<br /> <br /> In cases where there is truly a strongly-coupled time-dependent potential to deal with, I would probably not use either form of the Schrödinger equation, but instead I would formulate solutions in the interaction picture, where quantum propagators are used to describe the time-evolution of some initial state, which I would represent as a linear combination of eigenstates. Of course that choice is largely due to my own education and training, and the sorts of problems I run into in my research. Honestly, outside of fairly straightforward derivations and pedagogic illustrations, I have found little use for the TDSE.<br /> <br /> I understand that others will have a different take .. I was just providing a counter-example to your statement that, &quot;The time-dependent version is always the right choice.&quot;

 

[Gerenuk]

I understand that others will have a different take .. I was just providing a counter-example to your statement that, "The time-dependent version is always the right choice."

I wanted to emphasize that there is only one equation that describes the physics. Everything else is a special case. This is to prevent misconceptions about "dualities" and "special cases".
I had the impression the author of the initial question was thinking there are two different equations and you have to make a lucky guess which one to use. I prefer to teach that there are no dualities, i.e. conflicting definitions in physics. Absolutely everything in physics can be transformed consistently into each other.

You are right. I didn't mean to say that you should actually chose the most general equation to handle all problems.

 

[eaglelake]

In what conditions do we use time dependent and time independent Schrödinger's wave equations?

If you are interested in a) the possible results of an energy measurement and b) the probability distribution of those results, then you must solve the energy eigenvalue equation where the energy operator is the Hamiltonian \hat H = - {{\hbar ^2 } \over {2m}}{{\partial ^2 } \over {\partial x^2 }} + V(x) in one dimension for a time independent potential. This energy eigenvalue equation is what we call the time independent Schrödinger equation.

The solution gives us the energy eigenvalues E_n, which are the only possible results of an energy measurement. The state function, \psi (x), determined by the state preparation procedure, must then be written in the energy representation where the basis functions \left| {E_n } \right\rangle are the eigenfunctions of the Hamiltonian. Now \left| {\left\langle {{E_n }}<br /> \mathrel{\left | {\vphantom {{E_n } \psi }}<br /> \right. \kern-\nulldelimiterspace}<br /> {\psi } \right\rangle } \right|^2 gives us the probability of getting the energy value E_n when we know the system is in state \psi (x). Note that time is not a relevant parameter here.

However, all state functions will vary in time according to the time dependent Schrödinger equation i\hbar {{\partial \psi (x,t)} \over {\partial t}} = \hat H\psi (x,t). The probabilities might change with time, depending on the situation.