Let me be sort of specific. We consider a Weyl particles on S1, with the following Hamiltonian H=v∫2π0ψ†(x)(−i∂x)ψ(x)dx Such particles have the property that ρ(x)=ψ†(x)ψ(x) is ill defined, in the sense that the expectation value of ρ(x) diverges. For this reson we change the definition of normal ordering to ρ(x)=:ψ†(x)ψ(x):=ψ†(x)ψ(x)−ˉρ(x) Where the over bar is the expectation value. With this symbolism, we have that [ρ(x),ρ(x′)]=i2πδ′(x−x′) Istead of usual [ρ(x),ρ(x′)]=0. We also know that for chiral bosons one has [φ(x),φ(x′)]=−iπ sign(x-x') So by differentiating the bosonic commutator twice with respect to x and then with respect to x′, we get precisely the commutator of densities, provided that ρ(x)=12π∂xφ(x) So far so good. Than one sees that [ρ(x),ψ(x′)]=−ψ(x)δ(x−x′) In order to satisfy this commutation relation we have to make a clever guess. That is, if one asumes ψ(x)=eiφ(x), it is easy to show that indeed the algebra is satisfied. I'm pretty much satisfied with everithing by this point, it seems that we've found a canonical transformation and bla-bla-bla. What normally is then claimed in the literature that H=v∫2π0ψ†(x)(−i∂x)ψ(x)dx=v4π∫2π0(∂xφ(x))2dx And this is a place where I get stuck. So ψ†(x)(−i∂x)ψ(x)=e−iφ(x)(−i∂x)eiφ(x)=e−iφ(x)(∂xφ(x))eiφ(x)=e−i[φ(x),⋅]∂xφ(x)=? I.e. what is the commutator [∂xφ(x),φ(x)]? Does it even make sense? In this expression may also write (∂xφ(x))eiφ(x)=2πρ(x)ψ(x)=2πρ(x)ψ(x′)|x′=x=2πψ(x′)ρ(x)|x′=x−2πψ(x)δ(x−x′)|x′=x=2πψ(x)ρ(x)+?=eiφ(x)∂xφ(x)+? What am I doing wrong?
Answer
I am basically following the first chapter of Bosonization by Michael Stone.
Starting from the bosonization formula: ψ(x)=:eiϕ(x): And the Hamiltonian H=i∫dxψ†R(x)∂xψR(x)
In the bosonization of the composite terms, we need to point split and take care of the normal ordering according to:
:eiaϕ(x1)::eibϕ(x2):=:eiaϕ(x1)+ibϕ(x2):eablog(x1−x2)
Thus we have: ψ†R(x)∂xψR(x)=lim The singular term is taken care of by the normal ordering of the right hand side: Thus we get: H = i \int dx (\psi^{\dagger}_R(x) \partial_x \psi_R(x) = i \int dx :( \partial_x \phi(x))^2 :
Update: Proof of the normal ordering identity:
:e^{ia\phi(x_1)}::e^{ib\phi(x_2)}: = e^{ia\phi_{-}(x_1)+ia \phi_{+}(x_1)} e^{ib\phi_{-}(x_2)+ib \phi_{+}(x_2)}
where \phi_{+} contains only creation operators and \phi_{-} annihilation operators. In order to normal order the expression we need to commute between the second and third terms.
Using the Campbell–Baker–Hausdorff (CBH)
e^{A} e^{B} = e^{A+B} e^{[A, B]/2}
(for [A, B] = const.)
The relevant modes from the mode expansion
\phi_{-}(x)= \sum_{n>0} \sqrt{\frac{2}{n}} a_n e^{-\frac{nx}{L}} \phi_{+}(x)= \sum_{n>0} \sqrt{\frac{2}{n}} a_n^{\dagger}e^{\frac{nx}{L}}
L is the quantization box length which will be taken eventually to infinity
Using [a_n, a_m^{\dagger}] = \delta_{mn} We get: [\phi_{-}(x_1), \phi_{+}(x_2)] = 2\sum_{n>0}\frac{1}{n}e^{-\frac{ n(x_1-x_2)} {L} } = 2 \log(1-e^{-\frac{ (x_1-x_2)} {L} })\rightarrow_{L\to \infty} 2\log(x_1-x_2) + \mathrm{const.}
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