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arXiv:1711.01132 · Physical Review A

Class of exactly solvable scattering potentials in two dimensions, entangled-state pair generation, and a grazing-angle resonance effect

Farhang Loran, Ali Mostafazadeh

Published Dec 26, 2017• 12 citations
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Abstract

We provide an exact solution of the scattering problem for the potentials of the form $v(x,y)={\ensuremath{\chi}}_{a}(x)[{v}_{0}(x)+{v}_{1}(x){e}^{i\ensuremath{\alpha}y}]$, where ${\ensuremath{\chi}}_{a}(x):=1$ for $x\ensuremath{\in}[0,a]$, ${\ensuremath{\chi}}_{a}(x):=0$ for $x\ensuremath{\notin}[0,a]$, ${v}_{j}(x)$ are real or complex-valued functions, ${\ensuremath{\chi}}_{a}(x){v}_{0}(x)$ is an exactly solvable scattering potential in one dimension, and $\ensuremath{\alpha}$ is a positive real parameter. If $\ensuremath{\alpha}$ exceeds the wave number $k$ of the incident wave, the scattered wave does not depend on the choice of ${v}_{1}(x)$. In particular, $v(x,y)$ is invisible if ${v}_{0}(x)=0$ and $k<\ensuremath{\alpha}$. For $k>\ensuremath{\alpha}$ and ${v}_{1}(x)\ensuremath{\ne}0$, the scattered wave consists of a finite number of coherent plane-wave pairs ${\ensuremath{\psi}}_{n}^{\ifmmode\pm\else\textpm\fi{}}$ with wave vector: ${\mathbf{k}}_{n}=(\ifmmode\pm\else\textpm\fi{}\sqrt{{k}^{2}\ensuremath{-}{[n\ensuremath{\alpha}]}^{2}},n\ensuremath{\alpha})$, where $n=0,1,2,...<k/\ensuremath{\alpha}$. This generalizes to the scattering of wave packets and suggests means for generating quantum states with a quantized component of momentum and pairs of states with an entangled momentum. We examine a realization of these potentials in terms of certain optical slabs. If $k=N\ensuremath{\alpha}$ for some positive integer $N$, ${\ensuremath{\psi}}_{N}^{\ifmmode\pm\else\textpm\fi{}}$ coalesce and their amplitude diverge. If $k$ exceeds $N\ensuremath{\alpha}$ slightly, ${\ensuremath{\psi}}_{N}^{\ifmmode\pm\else\textpm\fi{}}$ have a much larger amplitude than ${\ensuremath{\psi}}_{n}^{\ifmmode\pm\else\textpm\fi{}}$ with $n<N$. This marks a resonance effect that arises for the scattered waves whose wave vector makes a small angle with the faces of the slab.

DOI
10.1103/physreva.96.063837

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We provide an exact solution of the scattering problem for the potentials of the form v(x,y)=\ensuremathχa(x)[v0(x)+v1(x)ei\ensuremathαy]v(x,y)={\ensuremath{\chi}}_{a}(x)[{v}_{0}(x)+{v}_{1}(x){e}^{i\ensuremath{\alpha}y}]v(x,y)=\ensuremathχa​(x)[v0​(x)+v1​(x)ei\ensuremathαy], where \ensuremathχa(x):=1{\ensuremath{\chi}}_{a}(x):=1\ensuremathχa​(x):=1 for x\ensuremath∈[0,a]x\ensuremath{\in}[0,a]x\ensuremath∈[0,a], \ensuremathχa(x):=0{\ensuremath{\chi}}_{a}(x):=0\ensuremathχa​(x):=0 for x\ensuremath∉[0,a]x\ensuremath{\notin}[0,a]x\ensuremath∈/[0,a], vj(x){v}_{j}(x)vj​(x) are real or complex-valued functions, \ensuremathχa(x)v0(x){\ensuremath{\chi}}_{a}(x){v}_{0}(x)\ensuremathχa​(x)v0​(x) is an exactly solvable scattering potential in one dimension, and \ensuremathα\ensuremath{\alpha}\ensuremathα is a positive real parameter. If \ensuremathα\ensuremath{\alpha}\ensuremathα exceeds the wave number kkk of the incident wave, the scattered wave does not depend on the choice of v1(x){v}_{1}(x)v1​(x). In particular, v(x,y)v(x,y)v(x,y) is invisible if v0(x)=0{v}_{0}(x)=0v0​(x)=0 and k<\ensuremathαk<\ensuremath{\alpha}k<\ensuremathα. For k>\ensuremathαk>\ensuremath{\alpha}k>\ensuremathα and v1(x)\ensuremath≠0{v}_{1}(x)\ensuremath{\ne}0v1​(x)\ensuremath=0, the scattered wave consists of a finite number of coherent plane-wave pairs \ensuremathψn\ifmmode±\else\textpm\fi{\ensuremath{\psi}}_{n}^{\ifmmode\pm\else\textpm\fi{}}\ensuremathψn\ifmmode±\else\textpm\fi​ with wave vector: kn=(\ifmmode±\else\textpm\fik2\ensuremath−[n\ensuremathα]2,n\ensuremathα){\mathbf{k}}_{n}=(\ifmmode\pm\else\textpm\fi{}\sqrt{{k}^{2}\ensuremath{-}{[n\ensuremath{\alpha}]}^{2}},n\ensuremath{\alpha})kn​=(\ifmmode±\else\textpm\fik2\ensuremath−[n\ensuremathα]2​,n\ensuremathα), where n=0,1,2,...<k/\ensuremathαn=0,1,2,...<k/\ensuremath{\alpha}n=0,1,2,...<k/\ensuremathα. This generalizes to the scattering of wave packets and suggests means for generating quantum states with a quantized component of momentum and pairs of states with an entangled momentum. We examine a realization of these potentials in terms of certain optical slabs. If k=N\ensuremathαk=N\ensuremath{\alpha}k=N\ensuremathα for some positive integer NNN, \ensuremathψN\ifmmode±\else\textpm\fi{\ensuremath{\psi}}_{N}^{\ifmmode\pm\else\textpm\fi{}}\ensuremathψN\ifmmode±\else\textpm\fi​ coalesce and their amplitude diverge. If kkk exceeds N\ensuremathαN\ensuremath{\alpha}N\ensuremathα slightly, \ensuremathψN\ifmmode±\else\textpm\fi{\ensuremath{\psi}}_{N}^{\ifmmode\pm\else\textpm\fi{}}\ensuremathψN\ifmmode±\else\textpm\fi​ have a much larger amplitude than \ensuremathψn\ifmmode±\else\textpm\fi{\ensuremath{\psi}}_{n}^{\ifmmode\pm\else\textpm\fi{}}\ensuremathψn\ifmmode±\else\textpm\fi​ with n<Nn<Nn<N. This marks a resonance effect that arises for the scattered waves whose wave vector makes a small angle with the faces of the slab.
A qubit (a spin-1/2 particle) prepared in the up state is scattered by local spin-flipping potentials produced by the two target qubits (two fixed spins), both prepared in the down state, to generate an entangled state in the latter when the former is found in the down state after scattering. The scattering process is analyzed in three dimensions, both to lowest order and in full order in perturbation, with an appropriate renormalization for the latter. The entanglement is evaluated in terms of the concurrence as a function of the incident and scattering angles, the size of the incident wave packet, and the detector resolution to clarify the key elements for obtaining an entanglement with high quality. The characteristics of the results are also discussed in the context of (in)distinguishability of alternative paths for a quantum particle.
In J.~Phys.~A {\bf 31}, 3493 (1998), Berry provides an analytic solution of the problem of determining the diffracted beam intensities for atoms incident upon a grating given by the potential, v(x,y):=iV0(eiK y−1)v(x,y):=iV_0(e^{i\mathfrak{K}\,y}-1)v(x,y):=iV0​(eiKy−1) for 0≤x≤ℓ0\leq x\leq\ell0≤x≤ℓ and v(x,y):=0v(x,y):=0v(x,y):=0 otherwise, where V0,KV_0, \mathfrak{K}V0​,K, and ℓ\ellℓ are positive real parameters. This result, which relies on the paraxial approximation, readily applies to the diffraction of transverse electric (TE) waves by the nonmagnetic optical grating given by the relative permittivity, ε^(x,y):=1−v(x,y)/k2\hat\varepsilon(x,y):=1-v(x,y)/k^2ε^(x,y):=1−v(x,y)/k2, where kkk is the incident wavenumber. We show that Berry's grating belongs to a larger class of possibly magnetic diffraction gratings whose scattering problem for both TE and transverse magnetic (TM) waves are exactly solvable. Our analysis makes use of a recently developed dynamical formulation of stationary scattering that is based on the idea of mapping the scattering problem to the quantum dynamics generated by an effective non-Hermitian Hamiltonian operator. {We use this formulation to derive explicit analytic expressions for the diffracted beam amplitudes that are valid beyond paraxial approximation.} As a concrete example, we offer the exact solution of the scattering problem for TE and TM waves incident upon a generalization of Berry's grating.
This thesis concerns quantum states that are superpositions of discrete or of continuum energy levels. It develops mathematical methods to characterize the physical properties of these states and finds important consequences. Regarding rational extensions of the harmonic oscillator, no other authors had constructed the coherent states associated with the ladder operators of Marquette and Quesne. It was our aim to proceed with this construction, then to calculate physical properties of these coherent states, looking for classical or quantum behaviour. The method of partial wave analysis was known to be not applicable to the Coulomb potential for the scattering of plane waves. It was my aim to repeat the calculation for wavepacket scattering, to investigate whether the method became applicable. Other authors have constructed relativistic probability amplitudes and compared them to the scalar Klein-Gordon amplitude. In this context, it was my aim to question the conclusion of a minimum width for a massive particle. In the same context, I investigated the possibility of a four-vector probability current with the Newton-Wigner position probability density as the zero component. In Chapter 12, my aim was to construct a measure of localization for the photon, knowing from the work of other authors that a point-localized photon state is not possible.In Chapters 3, 4 and 5, our measures of classicality for the Barut-Girardello coherent states included plotting energy expectations as functions of the magnitude of the coherent state para- meter, z, position probability densities for the coherent states and the even and odd cat states, the Wigner functions for particular choices of z, the two-photon number probability distribu- tion and the linear entropy for a coherent state on a beamsplitter, position spreads to look for squeezing and the Mandel Q parameter. In Chapter 6, it was necessary to approximate an integral containing a particular Wigner rotation matrix. An approximation of general Wigner rotation matrices, at low angle, was derived and its precision evaluated numerically in Chapter 7. The exact values for the Coulomb phase shifts were used to construct the incoming wavefunction. Time reversal and a rotation were used to construct the outgoing wavefunction. The sums over l were evaluated numerically. In Chapter 10, four arguments were used against the minimum width. Comparison of the scalar amplitude and the relativistic probability amplitude for a Newton-Wigner localized state showed the root of the problem. A Lorentz transformation was applied to the scalar function to see if the “minimum” width became even smaller. A simple construction produced scalar functions with arbitrarily small widths. A relevant argument from Almeida and Jabs was included here. In Chapter 11, the algebra involving the four components of a four-vector current (at the origin) and the boost generators was derived. All of these commutators must be satisfied by a four-vector, providing a test for the claimed four-vector probability currents of other authors. In Chapter 12, field expectations were taken in a coherent state with a mean photon number of unity, built from identical single-photon states.In Chapters 3, 4 and 5, we found a mix of classical and quantum behaviour for the coherent states. In none of the systems studied did we see the high degree of classicality of the unmodified harmonic oscillator. The investigation of cat states was relevant to the fundamental problem of measurement in quantum mechanics. In Chapter 6, the use of wavepackets introduced a convergence factor into the sum over l, which diverges in the plane wave treatment. The elimination of a divergence is the most significant result of this thesis. Scattering probabilities remained finite at all angles, in disagreement with the diverging Rutherford formula, but only on small angular regions around forward scattering. Future work will investigate the measurability of the phenomena predicted here. In Chapter 10, all four arguments pointed to no minimum width for a massive particle. In Chapter 11, it was found that there can be no four-vector current density with the Newton-Wigner position probability density as the zero component, for any spin. Other authors were found to be in error when they claimed to have produced such a four-vector current density. This result strengthens the position of the Dirac current as the appropriate current for an electron. In Chapter 12, the coherent state field expectations were found to provide a meaningful measure of localization. In summary, wavepackets give a realism to the description of a scattering experiment that is absent with the use of plane waves. Phenomena not captured by the plane wave scattering amplitude, such as time delays, are calculable in the wavepacket context. Relativistic probability amplitudes provide a complete description of free particles, consistent with quantum mechanics and with special relativity. They predict agreement with the Heisenberg uncertainty principle and relativistic effects such as Lorentz contraction. The absence of relativistic probability amplitudes from standard textbooks on relativistic quantum mechanics is a serious omission.