##H=i\hbar\frac{d}{dt}## is weird

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Discussion Overview

The discussion revolves around the implications of the time-dependent Schrödinger equation and the behavior of probability density in quantum mechanics, particularly focusing on the expression ##H=i\hbar\frac{d}{dt}##. Participants explore the conditions under which probability density remains constant and the nature of wavefunctions, including their real and complex characteristics.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants argue that the probability density ##P(x,t)## does not change over time for energy eigenstates, while questioning the validity of this conclusion.
  • Others clarify that the correct expression for probability density is ##P(x,t)=\langle\Psi(t)|x\rangle\langle x|\Psi(t)\rangle##, challenging earlier assumptions.
  • There is a discussion about the implications of assuming a real wavefunction, with some participants noting that if the wavefunction is real, certain derivatives yield zero results.
  • Participants explore the nature of wavefunctions in the context of the Schrödinger equation, debating whether they can be real or must be complex.
  • Some contributions highlight that energy eigenfunctions can be chosen to be real, yet the full wavefunction must remain complex due to the structure of the Schrödinger equation.
  • Mathematical derivations are presented to illustrate how probability distributions remain time-independent for energy eigenstates, while also discussing the continuity equation related to probability density.

Areas of Agreement / Disagreement

Participants express differing views on the nature of wavefunctions and the conditions under which probability density changes. While some agree on the stationary nature of energy eigenstates, others question the implications of real versus complex wavefunctions, indicating that the discussion remains unresolved on certain points.

Contextual Notes

There are limitations regarding the assumptions made about wavefunctions and the definitions used in the context of the Schrödinger equation. The discussion also reflects varying interpretations of mathematical expressions and their physical implications.

Who May Find This Useful

This discussion may be of interest to students and professionals in quantum mechanics, particularly those exploring the foundations of wavefunctions, probability density, and the implications of the Schrödinger equation.

Foracle
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TL;DR
I tried calculating the time derivative of the probability density of a wavefunction but end up getting $$\frac{d}{dt}P(x,t)=0$$ for any wavefunction.
##\frac{d}{dt}P(x,t)=\frac{d}{dt}<\Psi|\Psi>##
##=<\frac{d}{dt}\Psi|\Psi>+<\Psi|\frac{d}{dt}\Psi>##

By using ##\frac{d}{dt}=\frac{-i}{\hbar}H## ,

##\frac{d}{dt}P(x,t)=<\frac{-i}{\hbar}H\Psi|\Psi>+<\Psi|\frac{-i}{\hbar}H\Psi>##
##=\frac{i}{\hbar}<\Psi|H\Psi> - \frac{i}{\hbar}<\Psi|H\Psi> = 0##
The above equation shows that the probability density is not changing in time for any state, though clearly this situation only applies to energy eigenstate. Can someone tell me where I went wrong?

Edit : Another problem that I have that resembles this is :
For a time independent operator Q, a quick (and probably naive) calculation shows that [H,Q] = 0. But take position operator for example ##\hat{x}##. It's clear that ##\frac{d}{dt}<\hat{x}>## which can be written as ##\frac{d}{dt}<\hat{x}> = \frac{i}{\hbar}<[H,\hat{x}]>## is not zero for most states.
 
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##P(x,t)\neq \langle\Psi|\Psi\rangle##. The correct equality is
$$P(x,t)=\langle\Psi(t)|x\rangle\langle x|\Psi(t)\rangle$$
 
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Demystifier said:
##P(x,t)\neq \langle\Psi|\Psi\rangle##. The correct equality is
$$P(x,t)=\langle\Psi(t)|x\rangle\langle x|\Psi(t)\rangle$$
Thanks for pointing out!
Following the previous calculation, I end up with ##\frac{d}{dt}P(x,t) = \frac{i}{\hbar}[<H\Psi|x><x|\Psi> - <\Psi|x><x|H\Psi>]##
If I assume ##<\Psi|x> = \Psi^{*}(x)>## , I get
$$\frac{d}{dt}P(x,t) = \frac{i}{\hbar}[H\Psi^{*}\Psi - \Psi^{*}H\Psi]$$
If the wavefunction is real, than this is 0 again. Did I do some mistake?
 
Foracle said:
Thanks for pointing out!
Following the previous calculation, I end up with ##\frac{d}{dt}P(x,t) = \frac{i}{\hbar}[<H\Psi|x><x|\Psi> - <\Psi|x><x|H\Psi>]##
If I assume ##<\Psi|x> = \Psi^{*}(x)>## , I get
$$\frac{d}{dt}P(x,t) = \frac{i}{\hbar}[H\Psi^{*}\Psi - \Psi^{*}H\Psi]$$
If the wavefunction is real, than this is 0 again. Did I do some mistake?
How can a wavefunction be real if it satisfies the Schrödinger equation?
 
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PeroK said:
How can a wavefunction be real if it satisfies the Schrödinger equation?
Thanks for replying!
Can you please give me a quick explanation on why this is the case?
What about energy eigenfunction that can be chosen to be real?
 
Foracle said:
Thanks for replying!
Can you please give me a quick explanation on why this is the case?
What about energy eigenfunction that can be chosen to be real?
That's only the spatial function. There's a time-dependent function that is complex.
 
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PeroK said:
That's only the spatial function. There's a time-dependent function that is complex.
Ah I see..

Schrödinger equation : $$i\hbar\frac{d}{dt}\Psi = H\Psi$$
Since everything in this equation but i is real, nothing can counter the imaginary part hence ##\Psi## must be complex. Is this why wavefunction satisfying Schrödinger's equation must be complex?
 
Foracle said:
Ah I see..

Schrödinger equation : $$i\hbar\frac{d}{dt}\Psi = H\Psi$$
Since everything in this equation but i is real, nothing can counter the imaginary part hence ##\Psi## must be complex. Is this why wavefunction satisfying Schrödinger's equation must be complex?
Yes, the full wavefunction cannot be real.
 
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Foracle said:
If the wavefunction is real, than this is 0 again.
The full wave function cannot be real, as @PeroK said. But if the wave function is an energy eigenstate, then ##P(x,t)=P(x)## does not depend on time. There is nothing inconsistent with it, that's indeed why such states are called stationary.
 
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  • #10
Demystifier said:
if the wave function is an energy eigenstate, then ##P(x,t)=P(x)## does not depend on time.
Mathematically, this is because for an eigenstate, ##H \Psi^* = E \Psi^*## and ##H \Psi = E \Psi##, so the RHS of the equation in post #3 does vanish for this special case.
 
  • #11
PeterDonis said:
Mathematically, this is because for an eigenstate, ##H \Psi^* = \Psi^*## and ##H \Psi = \Psi##, so the RHS of the equation in post #3 does vanish for this special case.
An ##E## is missing on your right hand sides, but yes.
 
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  • #12
Demystifier said:
An ##E## is missing on your right hand sides, but yes.
Ah, yes. Fixed now. Thanks!
 
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  • #13
Foracle said:
Thanks for replying!
Can you please give me a quick explanation on why this is the case?
What about energy eigenfunction that can be chosen to be real?
The usual energy eigenfunction is calculated as a solution of the time-indpendent Schrödinger equation, but here you have to use the time-dependent equation. If ##u_E(x)## is the solution of the time-independent Schrödinger equation i.e., simply an eigenfunction of ##\hat{H}##) then ##\psi_E(t,x)=u_E(x) \exp(-\mathrm{i} E t/\hbar)## is a solution of the time-dependent equation. Nevertheless, and this is important to understand the probability distribution for position in this case
$$P(t,x)=|\psi(t,x)|^2=|u_E(x)|^2$$
is indeed time-independent. That shows that the energy-eigenfunctions lead to the stationary states of the system. The time-dependent phase factor doesn't change the state, because the state is defined by the wave function up to a phase factor, because the physics is in ##P=|\psi|^2## only.

For an arbitrary solution of the time-dependent Schrödinger equation you get
$$\partial_t P(t,x)=\partial_t [\psi^*(t,x) \psi(t,x)]=(\partial_t \psi)^* \psi + \psi^* \partial_t \psi.$$
Now from the time-dependent Schrödinger equation you have
$$\partial_t \psi=-\mathrm{i}/\hbar \hat{H} \psi = -\frac{\mathrm{i}}{\hbar} \left [-\frac{\hbar^2 \partial_x^2}{2m} + V(x) \right] \psi$$
and taking the conjugate complex of this
$$\partial_t \psi^* = +\frac{\mathrm{i}}{\hbar} \left [-\frac{\hbar^2 \partial_x^2}{2m} + V(x) \right] \psi^*=+\frac{\mathrm{i}}{\hbar} \hat{H} \psi^*.$$
So you finally get
$$\partial_t P(t,x)=\frac{\mathrm{i}}{\hbar} [\psi \hat{H} \psi^*-\psi^* \hat{H} \psi]=-\frac{\mathrm{i} \hbar}{2m} [\psi \partial_x^2 \psi^*-\psi^* \partial_x^2 \psi].$$
From this you also get the very important continuity equation
$$\partial_t P(t,x)+\partial_x j(t,x)=0,$$
where the "probability current" is defined by
$$j=\frac{\mathrm{i} \hbar}{2m} [\psi \partial_x \psi^*-\psi^* \partial_x \psi].$$
Integrating over ##x## along the real axis you get (for a proper wave function which sufficiently quickly goes to 0 for ##x \rightarrow \pm \infty##)
$$\mathrm{d}_t \int_{R} \mathrm{d} x P(t,x)=0.$$
This means that, if ##P(t,x)## is properly normalized at ##t=0## it stays normalized forever, as it should be.
 
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  • #14
vanhees71 said:
The usual energy eigenfunction is calculated as a solution of the time-indpendent Schrödinger equation, but here you have to use the time-dependent equation. If ##u_E(x)## is the solution of the time-independent Schrödinger equation i.e., simply an eigenfunction of ##\hat{H}##) then ##\psi_E(t,x)=u_E(x) \exp(-\mathrm{i} E t/\hbar)## is a solution of the time-dependent equation. Nevertheless, and this is important to understand the probability distribution for position in this case
$$P(t,x)=|\psi(t,x)|^2=|u_E(x)|^2$$
is indeed time-independent. That shows that the energy-eigenfunctions lead to the stationary states of the system. The time-dependent phase factor doesn't change the state, because the state is defined by the wave function up to a phase factor, because the physics is in ##P=|\psi|^2## only.

For an arbitrary solution of the time-dependent Schrödinger equation you get
$$\partial_t P(t,x)=\partial_t [\psi^*(t,x) \psi(t,x)]=(\partial_t \psi)^* \psi + \psi^* \partial_t \psi.$$
Now from the time-dependent Schrödinger equation you have
$$\partial_t \psi=-\mathrm{i}/\hbar \hat{H} \psi = -\frac{\mathrm{i}}{\hbar} \left [-\frac{\hbar^2 \partial_x^2}{2m} + V(x) \right] \psi$$
and taking the conjugate complex of this
$$\partial_t \psi^* = +\frac{\mathrm{i}}{\hbar} \left [-\frac{\hbar^2 \partial_x^2}{2m} + V(x) \right] \psi^*=+\frac{\mathrm{i}}{\hbar} \hat{H} \psi^*.$$
So you finally get
$$\partial_t P(t,x)=\frac{\mathrm{i}}{\hbar} [\psi \hat{H} \psi^*-\psi^* \hat{H} \psi]=-\frac{\mathrm{i} \hbar}{2m} [\psi \partial_x^2 \psi^*-\psi^* \partial_x^2 \psi].$$
From this you also get the very important continuity equation
$$\partial_t P(t,x)+\partial_x j(t,x)=0,$$
where the "probability current" is defined by
$$j=\frac{\mathrm{i} \hbar}{2m} [\psi \partial_x \psi^*-\psi^* \partial_x \psi].$$
Integrating over ##x## along the real axis you get (for a proper wave function which sufficiently quickly goes to 0 for ##x \rightarrow \pm \infty##)
$$\mathrm{d}_t \int_{R} \mathrm{d} x P(t,x)=0.$$
This means that, if ##P(t,x)## is properly normalized at ##t=0## it stays normalized forever, as it should be.
Thank you for taking your time to write this answer!
 

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