2020
DOI: 10.1103/physrevd.101.076009
|View full text |Cite
|
Sign up to set email alerts
|

Effects of the transverse coherence length in relativistic collisions

Abstract: Effects of the quantum interference in collisions of particles have a twofold nature: they arise because of the auto-correlation of a complex scattering amplitude and due to spatial coherence of the incoming wave packets. Both these effects are neglected in a conventional scattering theory dealing with the delocalized plane waves, although they sometimes must be taken into account in particle and atomic physics. Here, we study the role of a transverse coherence length of the packets, putting special emphasis o… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
2
1

Citation Types

0
34
0

Year Published

2020
2020
2022
2022

Publication Types

Select...
5

Relationship

1
4

Authors

Journals

citations
Cited by 21 publications
(34 citation statements)
references
References 56 publications
(107 reference statements)
0
34
0
Order By: Relevance
“…Thus, the particle packet acquires a quantized orbital angular momentum when leaving the solenoid field. Equations (6) and 7represent a quantum counterpart of the classical Busch theorem. Due to similarities of the fringe fields of the solenoid and those of a tip of a magnetic needle, the effect is somewhat analogous to that arising from the interaction with an effective magnetic monopole [16]-the particle's wave function gets an Aharonov-Bohm phase,…”
Section: Quantum Particle In a Solenoidmentioning
confidence: 99%
See 2 more Smart Citations
“…Thus, the particle packet acquires a quantized orbital angular momentum when leaving the solenoid field. Equations (6) and 7represent a quantum counterpart of the classical Busch theorem. Due to similarities of the fringe fields of the solenoid and those of a tip of a magnetic needle, the effect is somewhat analogous to that arising from the interaction with an effective magnetic monopole [16]-the particle's wave function gets an Aharonov-Bohm phase,…”
Section: Quantum Particle In a Solenoidmentioning
confidence: 99%
“…The generation of vortex beams as twisted photons [1], vortex neutrons [2], or vortex electrons has inspired versatile theoretical studies and interesting experiments or proposals to unveil the basic properties of such beams and of effects of quantum interference and coherence in particle collisions, inaccessible with ordinary beams [3][4][5][6][7][8][9]. Quantized vortex electrons-i.e., electron beams carrying a quantized orbital angular momentum (OAM)-generated in electron microscopes [10][11][12] can be applied as probes for the study of chiral [13] or magnetic structures [14] and enable magnetic mapping with atomic resolution [15].…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…If the initial photons are in Bessel twisted states, we represent each photon, neglecting its polarization degrees of freedom, as a superposition of plane waves [ 28,36–38 ] : |ϰ,m=eiωt+ikzzd2k(2π)2aϰm(boldk)eikr\begin{equation} |\varkappa ,m\rangle = e^{-i \omega t + i k_z z} \int {\text{d}^2 k_\perp \over (2\pi )^2}a_{\varkappa m}({\bf k}_\perp ) e^{i{\bf k}_\perp {\bf r}_\perp } \end{equation}where aϰm(boldk)=false(ifalse)meimφk2πϰδ(|k|ϰ)\begin{equation} a_{\varkappa m}({\bf k}_\perp )= (-i)^m e^{im\varphi _k}\sqrt {2\pi \over \varkappa }\; \delta (|{\bf k}_\perp |-\varkappa ) \end{equation}is the corresponding Fourier amplitude. The S ‐matrix element of the two twisted photon excitation is S=d2k1(2π)2d2k2(2π)2aϰ1m1(boldk1)aϰ2,m2(boldk2)SPW\begin{eq...…”
Section: Absorbing Two Twisted Photonsmentioning
confidence: 99%
“…Since they lead to the same final state, the two PW configurations interfere. Squaring (8) and following the standard regularization, [ 28,36–38 ] we obtain the generalized cross section in the form dσδfalse(normalΣEfalse)·δfalse(normalΣkzfalse)|J|2d3K=δfalse(Ei+ω1+ω2Effalse)|J|2d2boldK\begin{eqnarray} && d\sigma \propto \delta (\Sigma E)\cdot \delta (\Sigma k_z)\, |{\cal J}|^2 \, d^3K = \delta (E_i + \omega _1 +\omega _2 - E_f)\, |{\cal J}|^2 \, d^2{\bf K}_\perp \nonumber\\ \end{eqnarray}The energy conservation law expressed in Equation (5) still holds. However, unlike the plane‐wave collision where the final momentum was completely fixed by the initial kinematics, we have here a distribution over boldK${\bf K}_\perp$ inside the annular region defined by Equation (11).…”
Section: Absorbing Two Twisted Photonsmentioning
confidence: 99%