Explanation of Eq of Peskin's Intro to QFT Book

beta3
Messages
41
Reaction score
0
Hi

Can someone please explain to me Eq 2.30 in Schroeder's and Peskin's book? (page 21)

how does he simplify the long equation of the commutator to this delta distribution?
\imath\delta^(^3^)\ (x - x')



Thanks
 
Physics news on Phys.org
beta3 said:
how does he simplify the long equation of the commutator to this delta distribution?
\imath\delta^(^3^)\ (x - x')

He starts with:

[a_{\textbf p},a_{\textbf p'}^{\sp\dagger}]=(2\pi)^3\delta^{(3)}(\textbf p-\textbf p')

This means that:

[a_{-\textbf p}^{\sp\dagger},a_{\textbf p'}]-[a_{\textbf p},a_{-\textbf p'}^{\sp\dagger}]=-2(2\pi)^3\delta^{(3)}(\textbf p+\textbf p')

Substituting this in and integrating over the delta function (i.e. replacing p with -p'), you get:

i\int \frac{d^3p'}{(2\pi)^3}e^{i\textbf p'(\textbf x'-\textbf x)}

which is just i times the inverse Fourier transform of e^{i\textbf p'\textbf x'}:

[\phi(\textbf x),\pi(\textbf x')]=i\delta^{(3)}(\textbf x-\textbf x')
 
Last edited:
thanks, but there's one thing i still don't understand

after substituting it in and then if you integrate, what happens to the term
\sqrt{\frac{\omega_p_'}{\omega_p}}
 
beta3 said:
thanks, but there's one thing i still don't understand

after substituting it in and then if you integrate, what happens to the term
\sqrt{\frac{\omega_p_'}{\omega_p}}

since p = p' (where by p I mean the magnituide of the three-vector), the two omegas are equal.

Pat
 
nrqed said:
since p = p' (where by p I mean the magnituide of the three-vector), the two omegas are equal.

Pat

ah, yeah, now everything makes sense

Thank you two both soo much :wink:
 
Hello everyone, I’m considering a point charge q that oscillates harmonically about the origin along the z-axis, e.g. $$z_{q}(t)= A\sin(wt)$$ In a strongly simplified / quasi-instantaneous approximation I ignore retardation and take the electric field at the position ##r=(x,y,z)## simply to be the “Coulomb field at the charge’s instantaneous position”: $$E(r,t)=\frac{q}{4\pi\varepsilon_{0}}\frac{r-r_{q}(t)}{||r-r_{q}(t)||^{3}}$$ with $$r_{q}(t)=(0,0,z_{q}(t))$$ (I’m aware this isn’t...
Hi, I had an exam and I completely messed up a problem. Especially one part which was necessary for the rest of the problem. Basically, I have a wormhole metric: $$(ds)^2 = -(dt)^2 + (dr)^2 + (r^2 + b^2)( (d\theta)^2 + sin^2 \theta (d\phi)^2 )$$ Where ##b=1## with an orbit only in the equatorial plane. We also know from the question that the orbit must satisfy this relationship: $$\varepsilon = \frac{1}{2} (\frac{dr}{d\tau})^2 + V_{eff}(r)$$ Ultimately, I was tasked to find the initial...
Back
Top