Quantum mechanical Gaussian wavepackets of single relativistic particles

arXiv:2309.09429 · quant-ph, gr-qc, hep-th · Submitted 2023-09-18 · Read on arXiv

Listen

Radio episode about this paper

Transcript

Introduction to the show: ident: Quantum Radio. Generated commentary on the latest quantum physics and condensed matter papers.

Kai: We're looking at the paper: "Quantum mechanical Gaussian wavepackets of single relativistic particles".

Mira: Here's the gist of the paper. The gist: The minimal initial width of a wavepacket for a good Gaussian approximation in position space is about the Compton wavelength of the particle divided by its Lorentz factor at the initial moment, which can be considered as a manifestation of relativistic length contraction Relativistic Wavepacket Evolution The study investigates how selected quasi-(1+1) dimensional wavepacket solutions to the Klein-Gordon equation for a relativistic charged particle in uniform motion or accelerated by a uniform electric field in Minkowski space.

Kai: The research explores how good the charge density of a Klein-Gordon wavepacket can be approximately described by a Gaussian state with the single-particle interpretation.

Mira: A key finding is that for free relativistic particles in uniform motion, the minimal initial width for the KG charge density of a Gaussian KG wavefunction evolving like a Gaussian wavepacket centered at its classical trajectory is about λC /γ0, where γ0 = 1/p1 − (v0/c)2 is the Lorentz factor of the particle initially at speed v0.

Kai: Gaussian Approximation Justification The paper addresses a question regarding the range of validity or the cutoff for an effective theory like Refs.

Paper summary: Kai: To recap, this paper "Quantum mechanical Gaussian wavepackets of single relativistic particles" investigates the evolution of Klein-Gordon solutions for charged particles in uniform motion or under an electric field. They are checking if the charge density looks like a Gaussian function over time.

Mira: The paper claims that for free relativistic particles moving at a constant speed, the minimal initial width required to get a good Gaussian approximation is about lambda C divided by gamma zero, where gamma zero is the Lorentz factor of the particle initially at speed v0.

Lev: From an engineering standpoint, what this means is that if we try to model this with an effective theory like six or seven, the initial width needs to be kept small enough for the Gaussian assumption in probability density to hold up <ref:2309.09429#pg2>.

Kai: They construct these KG wavepackets initially Gaussian for both free particles at constant speed and for particles accelerated in a uniform electric field.

Mira: When they calculate the charge densities of these moving KG wavepacket solutions, they find that if the initial width is well below the Compton wavelength, say c theta is zero point one in Figure one the charge density behaves very non-Gaussian.

Lev: That's a bit of a warning for us on hardware; if our initial state isn't narrow enough to meet this criterion, we can't trust that simple Gaussian description when we look at the resulting charge distribution.

Kai: They then calculate the projection G psi and estimate it by calculating G rho, which shows how close the KG charge densities are to a normalized Gaussian function of half-width sigma centered at x equals x bar of t.

Mira: They observe that for the same wavepacket solution, G psi drops faster than G rho as time increases because the phase of psi becomes highly nonlinear in x for t greater than zero.

Lev: That non-linearity in phase is exactly what we worry about when trying to keep things simple on real quantum hardware; it means the single-particle picture gets harder to maintain quickly.

Conclusion: Kai: So, looking at "Quantum mechanical Gaussian wavepackets of single relativistic particles", the authors are pointing out a specific initial width limit for these wavepackets to maintain that Gaussian shape in position space.

Mira: The title and the authors suggest this work is about finding simple, mathematically tractable descriptions—Gaussian states—for complex relativistic quantum dynamics.

Kai: What this really means is that if you're looking at single electrons moving in electromagnetic fields, the effective theory they are using has a cutoff related to lambda C divided by gamma bar t.

Lev: For us building real hardware, that tells us the ultraviolet cutoff for the electron-photon interaction in an effective theory quantized in Minkowski coordinates might be around that lambda C divided by gamma bar t.

Mira: They link this minimal initial width directly to relativistic length contraction, which is something they also see numerically in how the charge density spreads over time.

Kai: It suggests that as the particle moves or accelerates, its effective description needs to account for this changing scale dictated by its velocity and field strength.

Department of Physics, National Tsing Hua University · Department of Physics, National Changhua University of Education

quant-ph, gr-qc, hep-th

Submitted: 2023-09-18

Updated: 2026-10-21

Comments: 17 pages, 8 figures. v2: Ref.[6] has been added. v3: Eq.(24) has been corrected, and Figs. 6 and 7 have been revised accordingly. The observation and conclusion remain unchanged

Journal ref: Chinese J. Phys. 87 (2024) 486-495; Corrigendum, Chinese J. Phys. 104 (2026) 775-776

DOI: 10.1016/j.cjph.2023.11.017 10.1016/j.cjph.2026.09.023

License: http://creativecommons.org/licenses/by/4.0/

Importance score: 77/100

The gist: The gist: The minimal initial width of a wavepacket for a good Gaussian approximation in position space is about the Compton wavelength of the particle divided by its Lorentz factor at the initial

Key concepts

Klein-Gordon Equation
This is a relativistic wave equation used to describe the behavior of charged particles. It incorporates both quantum mechanics and special relativity, making it suitable for studying particles moving at high speeds or in electromagnetic fields.
Gaussian Approximation
The researchers attempt to model the complex charge density of a relativistic wavepacket using a simple Gaussian function. This approximation is used to check how well the single-particle interpretation holds for these quantum states.
Compton Wavelength ($\lambda_C$)
This is a fundamental unit of length in relativistic physics, representing the characteristic scale associated with the particle's rest mass. The paper uses it as a benchmark to determine the minimum size required for a wavepacket to maintain its Gaussian shape.
Lorentz Factor ($\gamma_0$)
The Lorentz factor quantifies how much a particle's motion affects its relativistic properties, such as time dilation and length contraction. The minimal initial width is found to be inversely proportional to this factor, showing the effect of relativistic motion on the wavepacket's initial size.

Summary

The gist: The minimal initial width of a wavepacket for a good Gaussian approximation in position space is about the Compton wavelength of the particle divided by its Lorentz factor at the initial moment, which can be considered as a manifestation of relativistic length contraction

Relativistic Wavepacket Evolution

The study investigates how selected quasi-(1+1) dimensional wavepacket solutions to the Klein-Gordon equation for a relativistic charged particle in uniform motion or accelerated by a uniform electric field in Minkowski space. The research explores how good the charge density of a Klein-Gordon wavepacket can be approximately described by a Gaussian state with the single-particle interpretation. A key finding is that for free relativistic particles in uniform motion, the minimal initial width for the KG charge density of a Gaussian KG wavefunction evolving like a Gaussian wavepacket centered at its classical trajectory is about λC /γ0, where γ0 = 1/p1 − (v0/c)2 is the Lorentz factor of the particle initially at speed v0.

Gaussian Approximation Justification

The paper addresses a question regarding the range of validity or the cutoff for an effective theory like Refs. [6, 7] for single electrons moving in EM fields, specifically whether a Gaussian probability density of the wavefunctions can be justified to mimic a nearly Gaussian charge density of the KG wavefunction or Dirac spinor. The authors construct KG wavepackets initially Gaussian for free particles at constant speed and for accelerated particles in a uniform electric field. They find that if the initial width is well below the Compton wavelength of the particle, i.e., cϑ = 0.1 in Figure 1, the charge density behaves very non-Gaussian.

Similarity to Gaussian Functions

The authors calculate the projection GΨ and estimate it by calculating Gρ (Eq. (14)) to see how close the KG charge densities are to a normalized Gaussian function of half-width σ centered at x = ¯x(t). They observe that for the same wavepacket solution, GΨ drops faster than Gρ as t increases because the phase of Ψ becomes highly nonlinear in x for t > 0. The half-widths σ for Ψ and ρ tend to overlap as t → ∞.

Momentum Spectrum Analysis

The peak-splitting of the charge density with initial width well below its Compton wavelength indicates that the momentum spectrum of the corresponding wavepacket is so broad that many modes of high positive and negative momenta are included. When cϑ mc = ħ/λ¯C involved in the wavepacket, which are moving at speeds close to c and would constructively interfere around the lightcone in the t-x diagram.

Uniform Electric Field Dynamics

For a charged particle initially at rest, they find that ρ can be close to a Gaussian function with the value of σ0 as small as 3. For a charged particle initially at rest, the minimal initial width for a long-lasting Gaussian charge density goes down to O(1/γ0) of the Compton wavelength as shown in Figure 1. The spreading rate of ρ is lower for a particle moving faster when both speed and field strength are small, and this can be considered a manifestation of length contraction.

Conclusion on Cutoff

The minimal initial width of ρ we found in this paper actually implies that, to keep the single-particle interpretation and the Gaussianity, the charge density of a nearly Gaussian KG wavepacket at each moment t can at most be squeezed to a width about λC /γ¯(t). This suggests that the UV cutoff of the electron-photon interaction could be about λC /γ¯(t) in an effective theory quantized in Minkowski coordinates for single electrons interacting with EM fields [6, 7].

Appendix on Classical Action

The classical action for a charged particle moving in EM fields in the Minkowskitime gauge reads Scl = Z dt (−mc2r1 − 1/c2dzi/dt dzi/dt + qcA0(t, z(t)) + qdzi/dt Ai(t, z(t))). For a free particle in uniform motion at speed v0, one has Aµ = 0 and Scl = Z dt (−mc2r1 − v20c2). The phase of wavefunction (10) evaluated along the particle’s classical trajectory, namely, ϕ(t, x¯(t)), behaves similarly to the particle’s classical action Scl in (A.2) for sufficiently large t. For a charged particle moving in a uniform electric field considered in Section 3, Scl ∼ −mc2αt2/2 = −cFt 2/2. The phase ϕ(t, x(t)) of wavefunction (23) with (22) and (14) also behaves like Scl in (A.4) for sufficiently large t.

References

[1] W. Greiner, Relativistic Quantum Mechanics: Wave Equations, 3rd Ed., Springer, Berlin, 2000

[6] S.-Y. Lin and B. L. Hu, Relativistic single-electron wavepacket in quantum electromagnetic fields: Quantum coherence, correlations, and the Unruh effect [arXiv:2401.15404]

[7] S.-Y. Lin, Quantum coherence of relativistic wavepackets in electromagnetic vacuum, J. Phys.: Conf. Ser., 2482 012018 (2023)

[15] B. Rosenstein and M. Usher, Explicit illustration of causality violation: Noncausal relativistic wave-packet evolution, Phys. Rev. D 36, 2381 (1987)

[16] A. Torre, A Lattanzi, and D. Levi, Time-Dependent Free-Particle Salpeter Equation: Numerical and Asymptotic Analysis in the Light of the Fundamental Solution Ann. Physik 529, 1600231 (2017)

[17] X. Guti´errez de la Cal and A. Matzkin, Beyond the Light-Cone Propagation of Relativistic Wavefunctions: Numerical Results, Dynamics 3, 60 (2023)

[18] G. Dattoli, E. Sabia, K. G´orska, A. Horzela, and K. A. Penson, Relativistic wave equations: an operational approach, J. Phys.: A: Math., Theor., 48, 125203 (2015)

[19] K. Kowalski and J. Rembieli´nski, Salpeter equation and probability current in the relativistic Hamiltonian quantum mechanics, Phys. Rev. A 84, 012108 (2011)

[20] F. Rohrlich, Classical Charged Particles (Addison-Wesley, Redwood, 1965)

[21] I. S. Gradshteyn and I. M. Ryzhik, Table of Integrals, Series, and Products, 7th Ed., edited by A Jeffrey and D Zwillinger (Elsevier, Amsterdam, 2007), xxxviii

[5] C. Itzykson and J.-B. Zuber, Quantum Field Theory (McGraw-Hill, New York, 1980)

[8] W. G. Unruh, Notes on black hole evaporation, Phys. Rev.

Improvements for AI systems

  1. Improved modeling of quantum charge density in effective theories allows AI systems to approximate wavefunctions using Gaussian states when initial width is above O(lambda C)/gamma0, providing a justified description for single-particle interpretation in charged particle dynamics.

  2. Enhanced ability to predict the evolution of relativistic charged particle wavepackets under uniform motion or acceleration by utilizing the minimal initial width derived as about lambda C divided by its Lorentz factor at the initial moment.

  3. Development of a predictive framework where non-Gaussian features in KG charge density, such as double-peak structures, are identified when initial width is below lambda C, enabling AI to flag instances where single-particle interpretation fails and particle-antiparticle production is indicated.

  4. Capability to determine the range of validity for linearized effective theories describing single electrons in quantum electromagnetic fields by exploring parameter space based on the minimal initial width requirement for a good Gaussian approximation.

Abstract

We study the evolutions of selected quasi-(1+1) dimensional wavepacket solutions to the Klein-Gordon equation for a relativistic charged particle in uniform motion or accelerated by a uniform electric field in Minkowski space. We explore how good the charge density of a Klein-Gordon wavepacket can be approximately described by a Gaussian state with the single-particle interpretation. We find that the minimal initial width of a wavepacket for a good Gaussian approximation in position space is about the Compton wavelength of the particle divided by its Lorentz factor at the initial moment. This can be considered as a manifestation of relativistic length contraction, which is also observed numerically in the spreading of the wavepacket's charge density.

Sources

Related papers