Heisenberg equation of motion for the Dirac field?

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SUMMARY

The discussion centers on deriving the Heisenberg equation of motion for the Dirac field and its equivalence to the Dirac equation. Participants emphasize the importance of using anti-commutation relations and proper Hamiltonian formulation. The Hamiltonian for the Dirac field is expressed as H = ∫ψ†(-iγ·∇ + m)ψ d³x, and the commutation relations are critical for the derivation. Key insights include the necessity of correctly applying anti-commutation rules and the realization that missteps in these calculations can lead to incorrect conclusions.

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pellman
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I would expect that the Heisenberg equation of motion for the Dirac field would yield the Dirac equation. Indeed, these lecture notes claim it as a fact in eq 7.7 but without proof. My trouble is that I know the anti-commutation rules for the Dirac field but I don't know how to calculate the commutator with Hamiltonian, even if the Hamiltonian is expressed in terms of the field itself.

Can someone here provide some hints or tips?

Here is an old thread I started years ago on the same question.
https://www.physicsforums.com/showthread.php?t=235116
 
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The trick is to decompose the commutator in terms of anti-commutators. Since the Hamiltonian for the Dirac field is quadratic in the fermion fields, you use identities such as

<br /> [A,BC] = \{A,B\}C - B\{C,A\}<br />

Since you know these anti-commutators, the rest of the calculation is straight-forward.
 
Using the lagrangian (in natural units)

\mathcal{L}=\bar{\psi}(i\gamma^\mu \partial_\mu -m)\psi

where \psi(x) is the 4-spinor field and \bar{\psi}={\psi}^\dagger \gamma^0 we get the Hamiltonian

H=\int{\bar{\psi}(x&#039;)(-i\vec{\gamma}\cdot\nabla + m)\psi(x&#039;)d^3x&#039;}

where \vec{\gamma} are three space gamma matrices. The commutation rule is

\{\psi_j(\vec{x},t),\psi^{\dagger}_k (\vec{x}&#039;,t)\}=\delta_{jk}\delta^3(\vec{x}-\vec{x}&#039;)

Using [H,\psi_j]=2H\psi_j-\{H,\psi_j\} we get for the Heisenberg equation of motion

-i\partial_t \psi_j=[H,\psi_j]=2H\psi_j-\{H,\psi_j\}

\{H,\psi_j\}=-i{\gamma^0}_{jk}\vec{\gamma}_{kl}\cdot\nabla\psi_l + m{\gamma^0}_{jk}\psi_k

Multiplying by \gamma^0 and rearranging, we get

2\gamma^0 H\psi+(i\gamma^\mu \partial_\mu -m)\psi=0

So for the Heisenberg equation of motion to be equivalent to the Dirac equation would require that \gamma^0 H\psi =0. But I don't know how to show that is the case. Or maybe I went wrong somewhere?
 
Your evaluation of {H,ψ} is not correct. If you write it out, and keep track of the ordering of the ψ's, you will find that you don't get the anticommutator of ψ and ψ, but rather the commutator (and this doesn't simplify). You need to follow the previous suggestion to get this to work.
 
pellman said:
Using the lagrangian (in natural units)

\mathcal{L}=\bar{\psi}(i\gamma^\mu \partial_\mu -m)\psi

where \psi(x) is the 4-spinor field and \bar{\psi}={\psi}^\dagger \gamma^0 we get the Hamiltonian

H=\int{\bar{\psi}(x&#039;)(-i\vec{\gamma}\cdot\nabla + m)\psi(x&#039;)d^3x&#039;}

where \vec{\gamma} are three space gamma matrices. The commutation rule is

\{\psi_j(\vec{x},t),\psi^{\dagger}_k (\vec{x}&#039;,t)\}=\delta_{jk}\delta^3(\vec{x}-\vec{x}&#039;)

Using [H,\psi_j]=2H\psi_j-\{H,\psi_j\} we get for the Heisenberg equation of motion

-i\partial_t \psi_j=[H,\psi_j]=2H\psi_j-\{H,\psi_j\}

\{H,\psi_j\}=-i{\gamma^0}_{jk}\vec{\gamma}_{kl}\cdot\nabla\psi_l + m{\gamma^0}_{jk}\psi_k

Multiplying by \gamma^0 and rearranging, we get

2\gamma^0 H\psi+(i\gamma^\mu \partial_\mu -m)\psi=0

So for the Heisenberg equation of motion to be equivalent to the Dirac equation would require that \gamma^0 H\psi =0. But I don't know how to show that is the case. Or maybe I went wrong somewhere?

I tried looking in "Peskin & Schroeder" and they skirt the issue. In the case of boson fields, they prove that [H, \phi] = i \frac{d}{dt} \phi, but then they don't prove that for fermion fields.

On the one hand, it's got to be true, since they claim that \psi(\vec{x}, t) = e^{-iHt/\hbar} \psi(x,0) e^{+i Ht/\hbar}, but I'm with you, I don't see how it reproduces the Dirac equation.
 
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Avodyne said:
Your evaluation of {H,ψ} is not correct. If you write it out, and keep track of the ordering of the ψ's, you will find that you don't get the anticommutator of ψ and ψ, but rather the commutator (and this doesn't simplify). You need to follow the previous suggestion to get this to work.

I don't think so. You can see my steps in this image. http://s23.postimg.org/c8bzm0yej/dirac_commutator.jpg
 
Okay, we're trying to compute the commutator:

[H, \psi(x)]

H has the form \int d^3y\ \psi^\dagger(y)_\alpha \ O_{\alpha\beta}\ \psi(y)_\beta

where O involves gamma matrices, and the gradient and the mass, and so forth. Let's just look at [H, \psi(x)_\tau], one component. For simplicity, I'm going to leave off the integral sign, because it's easy enough to restore them later. So we have

\psi^\dagger(y)_\alpha \ O_{\alpha\beta}\ \psi(y)_\beta\ \psi(x)_\tau<br /> - \psi(x)_\tau\ \psi^\dagger(y)_\alpha \ O_{\alpha\beta}\ \psi(y)_\beta

We can write \psi(x)_\tau\ \psi^\dagger(y)_\alpha = \delta_{\tau \alpha} \delta^3(x-y) - \psi^\dagger(y)_\alpha\ \psi(x)_\tau. So substituting this into the above expression gives:

\psi^\dagger(y)_\alpha \ O_{\alpha\beta}\ \psi(y)_\beta\ \psi(x)_\tau<br /> - \delta_{\tau \alpha} \delta^3(x-y)\ O_{\alpha\beta}\ \psi(y)_\beta<br /> + \psi^\dagger(y)_\alpha\ \psi(x)_\tau\ O_{\alpha\beta}\ \psi(y)_\beta

Now, we can rewrite \psi(x)_\tau\ O_{\alpha\beta} = O_{\alpha\beta}\ \psi(x)_\tau.

The reason why is because O_{\alpha \beta} is not a matrix, but a single cell of a matrix. It's a scalar whose only operator part is \nabla, but since \nabla is a derivative with respect to y, not x, so it doesn't affect \psi(x). So they commute. So rearranging the three terms gives:

- \delta_{\tau \alpha} \delta^3(x-y)\ O_{\alpha\beta}\ \psi(y)_\beta<br /> + \psi^\dagger(y)_\alpha \ O_{\alpha\beta}\ \psi(y)_\beta\ \psi(x)_\tau<br /> + \psi^\dagger(y)_\alpha\ O_{\alpha\beta}\ \psi(x)_\tau\ \psi(y)_\beta

The last two terms can be combined using an anti-commutator, giving:

- \delta_{\tau \alpha} \delta^3(x-y)\ O_{\alpha\beta}\ \psi(y)_\beta<br /> + \psi^\dagger(y)_\alpha \ O_{\alpha\beta}\ \{ \psi(y)_\beta, \psi(x)_\tau \}

Since the anti-commutator is zero, we just get

- \delta_{\tau \alpha} \delta^3(x-y)\ O_{\alpha\beta}\ \psi(y)_\beta

After restoring the integral, and summing over the matrix indices, we have:

- O_{\tau \beta}\ \psi(x)_\beta = - (O\ \psi(x))_\tau

I think the operator O is just -i \alpha \cdot \nabla + \beta m. So I think it works out. Since there are two field operators in H, I think you get the same answer regardless of whether you use commutators or anti-commutators.
 
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pellman said:
I don't think so. You can see my steps in this image. http://s23.postimg.org/c8bzm0yej/dirac_commutator.jpg

I think I see the problem in your derivation: You write:

m \psi_k^\dagger(x&#039;,t) \gamma^0_{kl} \psi_l(x&#039;,t) \psi_j(x, t)
= + m \psi_k^\dagger(x&#039;,t) \psi_j(x, t) \gamma^0_{kl} \psi_l(x&#039;,t)

I think the right-hand side should be a minus sign, since the field operators anti-commute. Similarly for other terms.
 
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stevendaryl said:
I think the right-hand side should be a minus sign, since the field operators anti-commute. Similarly for other terms.

Right. Thanks! I will look over your other post closely and get back asap.
 
  • #10
That the field operators anti-commute was the key! It all fell right into place. Big thanks!
 

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