Question:
What is the general definition of one particle states |→p⟩ in an interacting QFT? By general I mean non-perturbative and non-asymptotic.
Context. 1)
For example, in Weigand's notes, page 42, we can read (edited by me):
As [H,→P]=0, these operators can be diagonalised simultaneously. Write the eigenstates as H|λ(→p)⟩=E(λ)|λ(→p)⟩→P|λ(→p)⟩=→p|λ(→p)⟩ One particle states are those with E(→p)=√→p2+m2.
For me, this is on the right track as a general definition, because we are defining |→p⟩ as the eigenstates of operators that commute, which is fine. But there are some issues with this definition:
Why is E a function of →p? why is E not an independent label on |→p⟩? Just as px,py,pz are independent, why is p0 not independent as well[1]?
Once we know that E=E(→p), how do we know that E2−→p2 is a constant? (we define mass as that constant, but only once we know that it is actually a constant). By covariance, I can see that p2 has to be a scalar, but I'm not sure what's the reason that this scalar has to be independent of p (for example, in principle we could have p2=m2+p4/m2).
How do we know that these |→p⟩ are non-degenerate? Why couldn't we have, for example, H|→p,n⟩=En(→p)|→p,n⟩, with En∼α/n2, as in the hydrogen atom?
These properties are essential to prove, for example, the Källén-Lehmann spectral representation, which is itself a non-perturbative, non-asymptotic result.
Context. 2)
In Srednicki's book, page 53, we can read (edited by me):
Let us now consider ⟨p|ϕ(x)|0⟩, where |p⟩ is a one-particle state with four-momentum p. Using ϕ(x)=eiPxϕ(0)e−iPx, we can see that ⟨p|ϕ(x)|0⟩=eipx
This only works if Pμ|p⟩=pμ|p⟩, which we could take as the definition of |p⟩. Yet again, I don't know why we would expect p2 to be a constant (that we could identify with mass). Or why are the eigenstates of Pμ non-degenerate.
The expression (2) is essential to scattering theory, but the result itself is supposedly non-asymptotic (right?). Also, it fixes the residue of the two-point function, which is one of the renormalisation conditions on the self-energy (Π′(m2)=0). This means that (2) is a very important result, so I'd like to have a formal definition of |p⟩.
[1] in standard non-relativistic QM, E is a function of →p because H is a function of →P. But in QFT, H is not a function of →P, it is a different operator.
Answer
I'll address your issues with definition (1):
E is a function of →p because |λ→p⟩∼|λ0⟩ where by ∼ I mean that they are related by a Lorentz boost. That is, to "construct" these states, you actually first sort out all the states |λ0⟩,λ0∈Λ (Λ now denotes the index set from which the λ0 are drawn) with →P|λ0⟩=0 and H|λ0⟩=E0(λ)|λ0⟩ and then you obtain the state λ→p by applying the Lorentz boost associated to →v=→p/E0(λ) to |λ0⟩. Since H and →P area components of the same four-vector, that means that E→p(λ) is a function of E0(λ) and →p - and E0(λ) is determined by λ, so E→p(λ) is really a function of →p and λ.
Conversely, every state of momentum →p can be boosted to a state with zero momentum. We examine this zero-momentum state for what λ0 it is and then name the state we started with λp, so this really constructs all states.
From the above it also directly follows that E→p(λ)2−→p2=E0(λ)2. I'm not sure what your issue with degeneracy is - degeneracy in P and H is not forbidden - nowhere is imposed that E→p(λ)≠E→p(λ′) should hold for λ≠λ′.
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