Ehrenfest theorem for kinetic energy

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SUMMARY

The Ehrenfest theorem establishes a relationship between quantum mechanics and classical mechanics by showing that the time derivative of the expectation value of an observable operator is equivalent to the classical equations of motion under certain conditions. Specifically, for a Hamiltonian that is not explicitly time-dependent, the covariant time derivative of an observable operator is given by the commutator with the Hamiltonian, expressed as \(\frac{\mathrm{D} \hat{A}}{\mathrm{D} t}=\mathring{\hat{A}}=\frac{1}{\mathrm{i} \hbar} [\hat{A},\hat{H}]\). The discussion emphasizes that while the final results are independent of the chosen picture (Heisenberg or Schrödinger), the proof is more straightforward in the Heisenberg picture. Corrections to the equations were made to ensure accuracy in the derivations presented.

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  • Understanding of quantum mechanics principles, particularly the Ehrenfest theorem
  • Familiarity with Hamiltonian mechanics and operator algebra
  • Knowledge of the Heisenberg and Schrödinger pictures in quantum mechanics
  • Proficiency in using commutators and covariant derivatives in quantum theory
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  • Study the derivation of the Ehrenfest theorem in detail
  • Explore the differences between the Heisenberg and Schrödinger pictures in quantum mechanics
  • Learn about the implications of the covariant time derivative in quantum mechanics
  • Investigate the role of potential energy in the context of Ehrenfest's theorem
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Physicists, particularly those specializing in quantum mechanics, educators teaching advanced mechanics, and researchers exploring the foundations of quantum theory will benefit from this discussion.

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In classical mechanics, the time derivative of the kinetic energy of a particle is given by the particle velocity multiplied by the force. Specifically, in one dimension, this translates into:
(d/dt)(p^2/2m)= −p/m ∂V/∂x

I'm unsure how to prove this...
 
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It's of course independent of the picture. The covariant time derivative of operators, representing observables, is given by
\frac{\mathrm{D} \hat{A}}{\mathrm{D} t}=\mathring{\hat{A}}=\frac{1}{\mathrm{i} \hbar} [\hat{A},\hat{H}],
where I have assumed that there is no explicit time dependence.

For a Hamiltonian that is not explicitly time dependent you thus find
\mathring{\hat{H}}=\frac{1}{\mathrm{i} \hbar} [\hat{H},\hat{H}]=0.
If, further, you have the motion of a particle in an external (time-independent) potential, you have
\hat{H}=\frac{\hat{\vec{p}}^2}{2m} + V(\hat{\vec{x}}),
and from the Heisenberg algebra, you can easily deduce
\mathring{\hat{\vec{p}}}= \frac{1}{\mathrm{i} \hbar} <br /> \left [\hat{\vec{p}},V(\hat{\vec{x}}) \right]=-\vec{\nabla} V(\hat{\vec{x}}).
From this it follows
\frac{\mathrm{D}}{\mathrm{D} t} \frac{\hat{\vec{p}}^2}{2m} = \frac{1}{\mathrm{i} \hbar 2m} \left (\hat{\vec{p}} \cdot [\hat{\vec{p}},V(\hat{\vec{x}})]+[\vec{p},V(\hat{\vec{x}})] \cdot \hat{\vec{p}} \right ) = -\frac{1}{2m} \left (\hat{\vec{p}} \cdot \vec{\nabla} V(\hat{\vec{x}}) + \vec{\nabla} V(\hat{\vec{x}}) \cdot \hat{\vec{p}} \right).

Ehrenfests theorem tells you that for any state \hat{R} in any picture of time evolution you have
\frac{\mathrm{d}}{\mathrm{d} t} \langle A \rangle=\frac{\mathrm{d}}{\mathrm{d} t} \mathrm{Tr} (\hat{R} \hat{A})=\mathrm{Tr} (\hat{R} \mathring{\hat{A}}).
Note that the Averaging goes over \mathring{\hat{A}}, and the equations of motion for the averages are in general not identical with the classical equations of motion for the average values. That's the case only for the linear oscillator or for the motion in a constant force field, because only then \langle \vec{\nabla} V(\vec{x}) \rangle=\vec{\nabla} V(\langle \vec{x} \rangle).
 
Last edited:
some correction is needed in fourth line above.
 
andrien said:
some correction is needed in fourth line above.

Argh! Thanks, I've done the corrections. I hope, it's right now.
 
vanhees71 said:
It's of course independent of the picture.
The final result is of course independent, but the proof is simpler in the Heisenberg picture.

vanhees71 said:
The covariant time derivative of operators, representing observables, is given by
\frac{\mathrm{D} \hat{A}}{\mathrm{D} t}=\mathring{\hat{A}}=\frac{1}{\mathrm{i} \hbar} [\hat{A},\hat{H}],
where I have assumed that there is no explicit time dependence.
In the Heisenberg picture this is correct. But in the Schrödinger picture, \hat{A} wouldn't depend on time even implicitly, so the left-hand side would be zero.
 
No! Note that I defined the covariant derivative of an observable operator as the commutator with the Hamiltonian. In general, it's not the time derivative of the operator in the sense of a differential quotient of an operator valued function of time. That's the case only in the Heisenberg picture. As you say, in the Schrödinger picture the "mathematical time derivative" would indeed be 0 (except for explicitly time dependent operators, but this I don't consider here, because this would make the whole issue even more complicated).
 

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