Canonical transformation from canonical to kinetic momentum

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SUMMARY

This discussion centers on the feasibility of replacing canonical momentum with kinetic momentum through a canonical transformation in classical mechanics, specifically within the context of a charged particle in an electromagnetic field. The classical Hamiltonian is defined as H = (1/2m)(p - eA(q,t))^2 + eΦ, where p is the canonical momentum and P = p - eA represents the kinetic momentum. The analysis reveals that while the transformation can eliminate the potential A in one spatial dimension, it fails to account for the Lorentz force, which is inherently linked to three-dimensional motion. The discussion concludes that the transformation is valid in one dimension but highlights the necessity of considering spatial dimensions for accurate representation of forces.

PREREQUISITES
  • Understanding of classical Hamiltonian mechanics
  • Familiarity with canonical transformations
  • Knowledge of electromagnetic theory, particularly the Lorentz force
  • Basic concepts of quantum mechanics, especially regarding path integrals
NEXT STEPS
  • Study the implications of canonical transformations in multi-dimensional systems
  • Explore the derivation and applications of the Lorentz force in three-dimensional motion
  • Investigate the Aharonov-Bohm effect and its relation to electromagnetic potentials
  • Learn about the role of gauge transformations in quantum mechanics and their physical interpretations
USEFUL FOR

This discussion is beneficial for physicists, particularly those specializing in classical mechanics, electromagnetism, and quantum mechanics, as well as students seeking to deepen their understanding of canonical transformations and their implications in various physical contexts.

DrDu
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My classical mechanics is very rusty. Recently, I wondered if it is possible to replace the canonical momentum with the kinetic momentum using a canonical transformation (so this isn't homework). I tried to work this out, but somehow, the Lorenz force got lost. Maybe some of you has an idea what goes wrong:
Consider the classical hamiltonian for a particle of mass ##m## and charge ##e## in an electromagnetic field.
Its position is ##q(t)## and it's canonical momentum ##p(t)##.
$$
H=\frac{1}{2m}(p-eA(q,t))^2+e\Phi.
$$
The kinetic momentum is ##P=p-eA##.
Can we introduce it as new canonical momentum?
We need to find a generating function ##G(q,P,t)## so that
$$
p=\frac{\partial{G}}{\partial q},
$$
$$
Q=\frac{\partial{G}}{\partial P},
$$
and
$$
H'(Q,P)=H+\frac{\partial{G}}{\partial t}
$$

Integrating the first equation, we obtain
$$
G(q,P,t)=\int_0^q (P+eA)\; dq=Pq+e\int_0^q A(q,t)\;dq + f(P,t).
$$
We consider a transformation with ##f(P,t)=0##.
From the second equation, the canonical variable to ##P## is
$$
Q = q,
$$
so I will use ##q## furtheron instead of ##Q##.
With
$$
\frac{\partial A}{\partial t} =-E -\nabla \Phi.
$$
we obtain from the third equation
$$
H'= \frac{1}{2m}P^2- e\int_0^q E(q,t)dq.
$$
So the transformed hamiltonian is completely free of potentials. The integration paths seems to be arbitrary.

We get the equations of motion
$$
\dot{q}= \frac{\partial H}{\partial P}= \frac{P}{m}
$$
and
$$
\dot{P} = -\frac{\partial H}{\partial q} = eE(q)
$$
somehow, the Lorenz force got lost!
 
Last edited:
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You made a typo and a big conceptual error. The typo is that the last term in the new Hamiltonian should be ##\partial G/\partial t##, not ##\partial G/\partial P##. The big conceptual error is that you work with only 1 spatial dimension, while Lorentz force due to magnetic field does not exist in 1 spatial dimension.

Or to say the same thing in a positive way, what you have really shown is that in 1 spatial dimension the potential ##A## can be eliminated by a canonical transformation, which is a correct result.

Indeed, if you start with your initial Hamiltonian and never perform the canonical transformation, you get
$$\dot{q}=\frac{\partial H}{\partial p}=\frac{p-eA}{m}$$
$$\dot{p}=-\frac{\partial H}{\partial q}=\frac{p-eA}{m}e\frac{\partial A}{\partial q} -e\frac{\partial \Phi}{\partial q}$$
Inserting the first equation into the second, and using
$$\frac{\partial \Phi}{\partial q}=-E-\frac{\partial A}{\partial t}$$
you obtain
$$\dot{p}=eE +e\left( \frac{\partial A}{\partial t} + \frac{\partial A}{\partial q} \dot{q} \right) = eE +e\frac{dA}{dt}$$
Hence, taking the time derivative of the first equation you get
$$m\ddot{q}=\dot{p}-e\frac{dA}{dt} = eE$$
showing that there is no magnetic Lorentz force in 1 spatial dimension.
 
Last edited:
Thank you for your feedback! I corrected the typo. Of course p and q etc. are 3d vectors. But you are right insofar as I naively assumed the derivative of the line integral to be the integrand at the upper end. This is not correct in more than 1 dimension.
 
In 3 spatial dimensions you have an integral of the form ##\int {\bf A}\cdot d{\bf q}##, which depends on the path of integration. If you choose a path along which electric and magnetic fields are zero, perhaps in this way you can even obtain something that resembles the Aharonov-Bohm effect.
 
Of course I also had the AB effect in mind. The derivation should be correct for a 1d particle on a ring where ##q=\phi## which describes correctly the acceleration by a changing magnetic flux in the center of the ring. In QM, one would have to clarify how to cope with the multivaluedness of the integral.
Also ##\phi## is not representable as a Hermitian operator due to the same reason.
 
Last edited:
In QM, one could formally implement this transformation with the unitary ## U(q,t)=\exp(ie\int Adq)##. Again, this is hard to interpret if the integral over ##q## is multi-valued.
 
DrDu said:
In QM, one could formally implement this transformation with the unitary ## U(q,t)=\exp(ie\int Adq)##. Again, this is hard to interpret if the integral over ##q## is multi-valued.
Perhaps it helps to integrate over closed loops only, then the canonical variable is not ##q##, but an integral over the loop. Something similar is done in loop quantum gravity.
 
You were right pointing out path dependence. Integration of ##p=\nabla_q G## is only possible if ##p## is rotation free. ##p## is essentially ##A##, so we can at best transform away the rotation free part of ##A##. This corresponds to a change to Coulomb gauge.
 

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