1999
DOI: 10.1007/bf02557343
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Wigner function for free relativistic particles

Abstract: A generalization of the Wigner function for the case of a free particle with the "relativistic" Hamiltonian p 2 + m 2 is given.

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Cited by 11 publications
(16 citation statements)
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“…We now summarize the basic facts about the Wigner function introduced in ref. 2. The point of departure in [2] was the following form of the nonrelativistic Wigner function W (x, p, t) = 1 (2π) 3 1 6 d 3 p 1 d 3 p 2φ * (p 1 , t)φ(p 2 , t)δ(p − 1 2 (p 1 + p 2 ))e i(p 2 −p 1 )·x , (2.1) whereφ(p, t) is the Fourier transform of the wave function φ(x, t), that is φ(p, t) = 1 (2π) 3 2 d 3 x e −i p·x φ(x, t).…”
Section: Definition Of the Wigner Functionmentioning
confidence: 99%
See 1 more Smart Citation
“…We now summarize the basic facts about the Wigner function introduced in ref. 2. The point of departure in [2] was the following form of the nonrelativistic Wigner function W (x, p, t) = 1 (2π) 3 1 6 d 3 p 1 d 3 p 2φ * (p 1 , t)φ(p 2 , t)δ(p − 1 2 (p 1 + p 2 ))e i(p 2 −p 1 )·x , (2.1) whereφ(p, t) is the Fourier transform of the wave function φ(x, t), that is φ(p, t) = 1 (2π) 3 2 d 3 x e −i p·x φ(x, t).…”
Section: Definition Of the Wigner Functionmentioning
confidence: 99%
“…Now we have the parametric form of the Wigner function introduced in ref. [2] that can be easily obtained from (2.20) by switching to coordinates p 1,2 = mc sinh γ 1,2 on the mass-shell hyperboloid:…”
Section: )mentioning
confidence: 99%
“…is not manifestly Lorentz invariant. Here: ψ(p, t) = ψ(p) e −itε(p) , ε(p) = p 2 + m 2 , d 3 p (2π) 3 |ψ(p, t)| 2 = d 3 p (2π) 3 1 2ε(p) |Ψ(p, t)| 2 = d 3 x d 3 p (2π) 3 n(r, p, t) = 1 = inv. (2) Along with a "non-relativistic" wave function ψ(p), we have also introduced a "relativistic" one, Ψ(p) = 2ε(p) ψ(p).…”
mentioning
confidence: 99%
“…The results that were found, reinforce our belief that one can successfully apply this formalism to other relativistic particles in searching for their relativistic Wigner functions. [ 10,27–33 ] On the other hand the problems with interpretation of the vector truex are to be expected since for relativistic particles the operator truex̂ does not represent the position observable. [ 16,24,26,34–39 ] So the natural question arises if one can construct the Weyl – Wigner – Moyal formalism for photon employing the position operator introduced by Margaret Hawton.…”
Section: Discussionmentioning
confidence: 99%