English

Momentum correlation in pair production by spacetime dependent fields from scattered wave functions

High Energy Physics - Phenomenology 2025-10-07 v2 High Energy Physics - Theory

Abstract

We consider Sauter-Schwinger pair production by electric fields that depend on both time and space, E(t,z)E(t,z) and E(t,x,y)E(t,x,y). For space-independent fields, E(t)E(t), momentum conservation, δ(p+p)\delta({\bf p}+{\bf p}'), fixes the positron momentum, p{\bf p}', in terms of the electron momentum, p{\bf p}. For E(t,z)E(t,z), on the other hand, pzp_z and pzp'_z are independent. However, previous exact-numerical studies have considered only the probability as a function of a single momentum variable, P(pz)P(p_z), P(pz)P(p'_z) or P(pzpz)P(p'_z-p_z), but not the correlation P(pz,pz)P(p_z,p'_z). In this paper, we show how to obtain P(pz,pz)P(p_z,p'_z) by solving the Dirac equation numerically. To do so, we split the wave function into a background and a scattered wave, ψ(t,x)=ψback.(t,x)+ψscat.(t,x)\psi(t,{\bf x})=\psi_{\rm back.}(t,{\bf x})+\psi_{\rm scat.}(t,{\bf x}), where ψback.exp(±ipx+gauge term)\psi_{\rm back.}\propto\exp(\pm ipx+\text{gauge term}). ψscat.\psi_{\rm scat.} vanishes outside a past light cone and is obtained by solving (iγμDμm)ψscat.=(iγμDμm)ψback.(i\gamma^\mu D_\mu-m)\psi_{\rm scat.}=-(i\gamma^\mu D_\mu-m)\psi_{\rm back.} backwards in time starting with ψscat.(t+,x)=0\psi_{\rm scat.}(t\to+\infty,{\bf x})=0.

Keywords

Cite

@article{arxiv.2509.17770,
  title  = {Momentum correlation in pair production by spacetime dependent fields from scattered wave functions},
  author = {Greger Torgrimsson},
  journal= {arXiv preprint arXiv:2509.17770},
  year   = {2025}
}

Comments

11 pages, 6 figures. v2: added link to code for solving the Dirac equation on a GPU