Evaluating a momentum operator

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Homework Statement
Show that the momentum operator ##\hat{\vec P}## yields



$$\hat{\vec P} = \int d^3 \vec x \frac{1}{c^2} \mathcal{N} \left( \dot A_{\mu} \nabla A^{\mu} \right) = \sum_{\vec k} \hbar \vec k N( \vec k)$$



Where ##\mathcal{N}## stands for normal-ordering and ##N( \vec k)## is the number operator

##N( \vec k) = \sum_{r=0}^3 \zeta_r a_r^{\dagger} (\vec k) a_r^{\dagger} (\vec k)## (for instance, EQ ##5.33## Mandl & Shaw)
Relevant Equations
Please see below
I think I get the approach. We first need to evaluate the term ##\dot A_{\mu} \nabla A^{\mu}## and then evaluate the 3D space integral; we may need to take the limit ##V \rightarrow \infty## (i.e ##\sum_{\vec k} (2 \pi)^3/V \rightarrow \int d^3 \vec k##) at some point.

The mode expansions of the vector potential ##A^{\mu}=A_{+}^{\mu} + A_{-}^{\mu}## are

$$A_{-}^{\mu}=\sum_{r=0}^3 \sum_{\vec k} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \epsilon_r^{\mu} a_r^{\dagger}(\vec k) e^{ik \cdot x} \right] \tag{1.1}$$

$$A_{+}^{\mu}=\sum_{r=0}^3 \sum_{\vec k} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \epsilon_r^{\mu} a_r(\vec k) e^{-i \vec k \cdot \vec x} \right] \tag{1.2}$$

The time-derivatives of ##(1.1)## and ##(1.2)## are

$$\dot A_{-}^{\mu} = ik^0 e^{ik^0 x^0}\sum_{r=0}^3 \sum_{\vec k} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \epsilon_r^{\mu} a_r^{\dagger}(\vec k) e^{-i \vec k \cdot \vec x} \right]$$

$$\dot A_{+}^{\mu} = -ik^0 e^{-ik^0 x^0}\sum_{r=0}^3 \sum_{\vec k} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \epsilon_r^{\mu} a_r(\vec k) e^{i \vec k \cdot \vec x} \right]$$

The spatial-derivatives of ##(1.1)## and ##(1.2)## are

$$ \nabla A_-^{\mu} = -i e^{ik^0 x^0}\sum_{r=0}^3 \sum_{\vec k} \left[ \vec k \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \epsilon_r^{\mu} a_r^{\dagger}(\vec k) e^{-i \vec k \cdot \vec x} \right]$$

$$ \nabla A_+^{\mu} = i e^{-ik^0 x^0}\sum_{r=0}^3 \sum_{\vec k} \left[ \vec k \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \epsilon_r^{\mu} a_r(\vec k) e^{i \vec k \cdot \vec x} \right]$$

We evaluate ##\dot A_{\mu} \nabla A^{\mu}##

$$\dot A_{\mu} \nabla A^{\mu}=(\dot A^{+}_{\mu}+ \dot A^{-}_{\mu})(\nabla A_+^{\mu} +\nabla A_-^{\mu})=\dot A^{+}_{\mu}\nabla A_+^{\mu} + \dot A^{-}_{\mu}\nabla A_-^{\mu} + \dot A^{+}_{\mu}\nabla A_-^{\mu}+\dot A^{+}_{\mu}\nabla A_+^{\mu}$$

Let's evaluate ##\dot A^{+}_{\mu}\nabla A_+^{\mu}## explicitly

$$\dot A^{+}_{\mu}\nabla A_+^{\mu}=-ik^0 e^{-ik^0 x^0}\sum_{r=0}^3 \sum_{\vec k} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \eta_{\mu \nu} \epsilon_r^{\nu} a_r(\vec k) e^{i \vec k \cdot \vec x} \right]i e^{-ik^0 x^0} \sum_{r=0}^3 \sum_{\vec k} \left[ \vec k \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \epsilon_r^{\mu} a_r(\vec k) e^{i \vec k \cdot \vec x} \right] \tag{*}$$

OK ##(*)## looks messy; let's focus on relevant terms

$$\dot A^{+}_{\mu}\nabla A_+^{\mu} \sim \eta_{\mu \nu} \epsilon_r^{\nu} a_r(\vec k) \vec k \epsilon_r^{\mu} a_r(\vec k)= \eta_{\mu \nu} \epsilon_r^{\nu} \vec k \epsilon_r^{\mu} a_r(\vec k) a_r(\vec k)\tag{**}$$

Once here, based on the orthonormality and completeness of the polarization vectors

55456765677.png


And the customary choice of polarization vectors

1212121212121213454.png


So the idea would be using ##(5.19)## but we do not have the ##\zeta_r## factor. Besides, the 3-vector ##\vec k## suggests we may have to use the orthogonal conditions ##(5.22b)##.

How could we evaluate ##(*), (**)## then?

Thank you :biggrin:
 
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It's a pretty longish calculation. You have to be a bit more careful though when looking at products and use different momenta for each of the factors and then interchange the momentum integrals with the spatial integral making use of
$$\int_{\mathbb{R}^3} \mathrm{d}^3 x \exp(\mathrm{i} (\vec{k}_1-\vec{k}_2) \cdot \vec{x})=(2 \pi)^3 \delta^{(3)}(\vec{k}_1-\vec{k}_2).$$
Then you can do one of the then trivial momentum integrations and are left with the other momentum integral leading to the right-hand side of the formula you want to prove. Just keep calculating!
 
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Hi vanhees71, I see it better now thanks to your comments.

OK let me rewrite ##(*)##, distinguishing momentum and polarization vectors. I also noticed I missed a ##1/c## factor (which pops up due to ##\partial_{0}=\partial/(c\partial t)##)

$$\dot A^{+}_{\mu}\nabla A_+^{\mu}=\sum_{r,s=0}^3 \sum_{\vec k, \vec k'} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \Big(\frac{\hbar c^2}{2V \omega_{\vec k'}} \Big)^{1/2} k^0/c \ \eta_{\mu \nu} \epsilon_r^{\nu}(\vec k) a_r(\vec k) e^{-i k \cdot x} \vec k' \epsilon_s^{\mu}(\vec k') a_s(\vec k') e^{-i k' \cdot x} \right]$$

$$=\sum_{r,s=0}^3 \sum_{\vec k, \vec k'} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \Big(\frac{\hbar c^2}{2V \omega_{\vec k'}} \Big)^{1/2} k^0/c \ \vec k'\epsilon_{r \mu}(\vec k)\epsilon_s^{\mu}(\vec k') a_r(\vec k) a_s(\vec k') e^{-i (k+k') \cdot x} \right]$$

Using the orthonormality condition ##(5.18)## and ##k^0 = \omega_{\vec k} / c##

$$=-\sum_{r,s=0}^3 \sum_{\vec k, \vec k'} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \Big(\frac{\hbar c^2}{2V \omega_{\vec k'}} \Big)^{1/2} k^0/c \ \vec k'\zeta_r \delta_{r,s}\delta_{\vec k, \vec k'} a_r(\vec k) a_s(\vec k') e^{-i (k+k') \cdot x} \right]$$ $$=-\sum_{r}^3 \sum_{\vec k} \left[ \Big(\frac{\hbar }{2V} \Big) \vec k \zeta_r a_r(\vec k) a_r(\vec k) e^{-2i k \cdot x} \right]$$

Mmm this (at least) smells good! We've got the ##\hbar \vec k## term and ##\zeta_r##. However there are two main issues: I do not get the number operator and ##e^{-2i k \cdot x}## is not the expected factor (we would expect something like ##e^{i (k-k') \cdot x}##, so that the Dirac-delta function could be obtained after integrating over momentum space).

I considered the possibility that this term may not contribute to the final answer but I do think it does, as none of the other 3 terms is ##\sim a_r(\vec k) a_r(\vec k)##...

Or maybe I just need to think more about it 😅
 
vanhees71 said:
You forgot the ##\vec{x}##-integral

Oh I see! Let's try again

$$\frac{1}{c^2} \int d^3 \vec x \sum_{r,s=0}^3 \sum_{\vec k, \vec k'} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \Big(\frac{\hbar c^2}{2V \omega_{\vec k'}} \Big)^{1/2} k^0 \ \vec k'\epsilon_{r \mu}(\vec k)\epsilon_{s}^{\mu}(\vec k') a_r(\vec k) a_s(\vec k') e^{-i (k+k') \cdot x} \right]=$$

$$= \frac{1}{c^2} \sum_{r,s=0}^3 \sum_{\vec k, \vec k'} \left[ \Big(\frac{\hbar c^2}{2V \omega_{\vec k}} \Big)^{1/2} \Big(\frac{\hbar c^2}{2V \omega_{\vec k'}} \Big)^{1/2} k^0 \ \vec k'\epsilon_{r \mu}(\vec k)\epsilon_{s}^{\mu}(\vec k') a_r(\vec k) a_s(\vec k') (2 \pi)^3 \delta^{(3)}(\vec k + \vec k') e^{-i (k^0+k'^0) x}\right] \tag{@}$$

Where I've performed the 3D integral. Taking the limit ##V \rightarrow \infty## (i.e ##\sum_{\vec k} (2 \pi)^3/V \rightarrow \int d^3 \vec k##) and the orthonormality condition ##(5.18)## we get

$$@ = \frac{1}{c^2} \sum_{r,s=0}^3 \sum_{\vec k} \int d^3 \vec k' \left[ \Big(\frac{\hbar c^2}{2 \omega_{\vec k}} \Big)^{1/2} \Big(\frac{\hbar c^2}{2 \omega_{\vec k'}} \Big)^{1/2} k^0 \ \vec k'\epsilon_{r \mu}(\vec k)\epsilon_{s}^{\mu}(\vec k') a_r(\vec k) a_s(\vec k') \delta^{(3)}(\vec k + \vec k') e^{-i (k^0+k'^0) x}\right]=$$

$$= \sum_{r,s=0}^3 \sum_{\vec k} \left[ \Big(\frac{\hbar }{2} \Big) \vec k \ \epsilon_{r \mu}(\vec k)\epsilon_{s}^{\mu}(\vec k) a_r(\vec k) a_s(\vec k) e^{-i (k^0+k'^0) x}\right]=$$

$$= -\frac{\hbar }{2} \sum_{r=0}^3 \sum_{\vec k} \left[ \vec k \
\zeta_r a_r(\vec k) a_r(\vec k) e^{-i (k^0+k'^0) x}\right]$$

Mmm it does not look right, as I am not getting the number operator, I get the extra factor ##e^{-i (k^0+k'^0) x}## and the -ive sign.

I have the same issue with the term

$$\dot A^{-}_{\mu}\nabla A_-^{\mu} \sim -a_r^{\dagger} (\vec k) a_r^{\dagger} (\vec k)$$

Thinking...