Skip to main content

Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

Arrival Time Distributions of Spin-1/2 Particles

Abstract

The arrival time statistics of spin-1/2 particles governed by Pauli’s equation, and defined by their Bohmian trajectories, show unexpected and very well articulated features. Comparison with other proposed statistics of arrival times that arise from either the usual (convective) quantum flux or from semiclassical considerations suggest testing the notable deviations in an arrival time experiment, thereby probing the predictive power of Bohmian trajectories. The suggested experiment, including the preparation of the wave functions, could be done with present-day experimental technology.

Introduction

In non-relativistic quantum mechanics, the probability of finding a particle in a small spatial volume d3r around position r at a fixed time t is given by Born’s rule |Ψ(r, t)|2d3r, where Ψ(r, t) is the wave function of the particle. This formula is experimentally well established. However, a formula for the probability of finding the particle at a fixed point r between times t and t + dt is the matter of an ongoing debate1,2,3,4,5,6. Let us consider a typical time of arrival experiment, in which a particle is initially trapped in a region \({\rm{\Sigma }}\,\subset \,{{\mathbb{R}}}^{3}\), e.g., the interior of a potential well. The trap is released at, say, t = 0, allowing the particle to propagate freely in space. If the trapping potential is deep enough, the wave function of the particle at this instant, Ψ0(r) ≡ Ψ(r, t = 0), practically vanishes outside the region Σ. Particle detectors placed on the boundary ∂Σ measure the time of arrival of the particle, denoted by τ. If the experiment is repeated many times, the recorded arrival times are random, even if the initial wave function of the particle (Ψ0) is kept unchanged in each experiment. What is the probability distribution of arrival times \({{\rm{\Pi }}}^{{{\rm{\Psi }}}_{0}}(\tau )\) as a functional depending on Ψ0 and on ∂Σ?

Measurement in quantum mechanics has become in recent decades a tricky notion. Traditionally, measurement outcomes were solely associated with observables, represented by self-adjoint operators on the Hilbert space of the measured system. However, it has long been known that for time measurements, such as arrival times, no such observable exists [2, §8.5]. In fact, the notion of self-adjoint operators defining quantum observables does not apply to many other experiments as well. To remedy this situation, the notion of an observable was generalized to positive operator valued measures (POVMs), and there are various suggestions for arrival time POVMs (see7,8 for a discussion). In Dürr et al.9, all measurements describable by POVMs were called linear measurements. Another class of measurements have also been performed, the so-called weak measurements10, which are nonlinear in the sense of9. So far, however, no theoretical predictions for the arrival time distribution \({{\rm{\Pi }}}^{{{\rm{\Psi }}}_{0}}(\tau )\) have been backed up by experiments (see1,2,8,11,12,13 for various proposals). On the other hand, recent ‘attoclock’ experiments (claimed to be measuring the tunnel delay time of ionized electrons) have shown some of the theoretical ideas to be empirically inadequate14,15.

One problem with arrival time measurements is that detection events are based on interactions of the detectors with the detected particle, which may disturb its wave function in an uncontrollable way, leading to backscattering and in extreme cases to the quantum Zeno effect. While this is a valid concern, we note that the double-slit experiment (mentioned also below) is an example where the distribution of arrival positions of the particle on the detector screen (the ubiquitous interference picture) is analyzed without any reference to the presence of the detector. Note well that the particles strike the detector surface at random times, a fact blissfully ignored in the usual discussions of the double-slit experiment–and there are good reasons why that is justified. We expect that in the experiment proposed in this paper the same will be true, i.e., the detection event should not be drastically disturbed by the presence of the detector. Our expectation is based on our results, namely, on the very striking articulated features of the computed arrival time distributions, which should survive mild disturbances.

A further problem is that the notion of arrival time is most naturally connected with that of particle trajectories, an idea which is hard to concretize in the orthodox interpretation of quantum mechanics. Bohmian mechanics (or de Broglie-Bohm pilot wave theory) is a quantum theory (and not simply an alternative interpretation of quantum mechanics) where particles move on well defined smooth trajectories, hence it is naturally suited for computing arrival times of a particle. See Kocsis et al.10 for a weak measurement of average quantum trajectories in a double-slit experiment, which can indeed be seen as Bohmian trajectories. Bohmian mechanics has been proven to be empirically equivalent to standard quantum mechanics, wherever the latter is unambiguous (e.g., in position and momentum measurements)9,16. It has been shown that Bohmian mechanics provides in (far field) scattering situations ideal (i.e. devise independent) arrival time statistics for spin-0 particles6, via the quantum flux (or the probability current) J:

$${{\rm{\Pi }}}^{{\Psi }_{0}}(\tau )\,=\,{\int }_{\partial \Sigma }\,{\bf{J}}({\boldsymbol{r}},\tau )\,\cdot \,{\rm{ds}}\,\,(\,=\,:{{\rm{\Pi }}}_{{\rm{q}}{\rm{f}}}(\tau \mathrm{)).}$$
(1)

Only in scattering situations (i.e., when the detector surface ∂Σ is far away from the support of the initial wave function Ψ0), is the surface integral in (1) demonstrably positive6, otherwise it cannot be interpreted as a probability density (see7 for a discussion of POVMs versus flux statistics). Although often not recognized or emphasized in textbooks, it is the quantum flux J, integrated over time, that yields the double-slit interference pattern of arrival positions of particles on the screen—as there is no given time at which the particles arrive at the screen.

Here, we must mention as well another flux based (Bohmian) arrival time distribution derived by C. R. Leavens (Eq. (9) of17), which is valid only in one space dimension (as discussed in1, [Ch. 5]). Therefore, it is not applicable for particles with spin-1/2, except perhaps in some idealized situations. In this paper, we propose a Bohmian formula for the distribution of first arrival times of a spin-1/2 particle (Eq. (9) below), which may be referred to as an ideal or intrinsic distribution, since it is formulated without referring to any particular measurement device, just as equation (1). In fact, the spin-1/2 analogue of (1) becomes a special case of (9), whenever the so-called current positivity condition6 is met. Evaluating our formula numerically for a specific, carefully chosen experiment, we find that the resulting arrival time distributions show drastic and unexpected changes when control parameters are varied. Since the predicted distributions show such interesting and significant behavior, we suggest that the proposed experiment be performed to test the predictive power of Bohmian mechanics for spin-1/2 particles.

One may legitimately ask, how can the idea of an ideal first arrival time distribution be entertained at all? Our standpoint on this is as follows: Given the relative simplicity of making the Bohmian prediction for the ideal arrival time distribution, and given the ambiguity of quantum mechanical proposals mentioned above, why not just do the experiment to check it? However the experimental results turn out, they provide in any case valuable experimental data that would enrich our understanding of quantum mechanics and of Bohmian mechanics as well. A word of clarification is, however, in order: we do not construe in our work any contradiction to quantum mechanics, since an unambiguous answer to the question of arrival times has not been given within this framework. The main advantage of Bohmian mechanics is the clear picture of reality, independent of observation, it provides and which in the problem of arrival times allows an unambiguous answer in contrast to the answers given in quantum mechanics, so far.

We proceed now to a description of the proposed experiment. A spin-1/2 particle of mass m is constrained to move within a semi-infinite cylindrical waveguide (Fig. 1). Initially, it is trapped between the end face of the waveguide and an impenetrable potential barrier placed at a distance d. At the start of the experiment, the particle is prepared in a ground state Ψ0 of this cylindrical box, then the barrier at d is suddenly switched off, allowing the particle to propagate freely within the waveguide. The arrival surface ∂Σ is the plane situated at distance L (>d) from the end face of the waveguide. We then compute numerically from the Bohmian equations of motion how long it takes for the particle to arrive at ∂Σ, and determine the empirical distribution \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{{{\rm{\Psi }}}_{0}}(\tau )\) from typical trajectories (trajectories whose initial points are randomly drawn from the Born |Ψ0|2 distribution) for different initial ground state wave functions.

Figure 1
figure1

Schematic drawing of the experimental setup. The barrier at d is switched off at t = 0 and arrival times are monitored at z = L.

The Bohmian equations for spin-1/2 particles are as follows: The wave function Ψ(r, t) is a two-component complex-valued spinor solution of the Pauli equation

$$i\hslash \frac{\partial }{\partial t}{\rm{\Psi }}({\boldsymbol{r}},t)\,=\,-\,\frac{{\hslash }^{2}}{2\,m}{(\sigma \cdot {\boldsymbol{\nabla }})}^{2}{\rm{\Psi }}({\boldsymbol{r}},t)+V({\boldsymbol{r}},t){\rm{\Psi }}({\boldsymbol{r}},t),$$
(2)

with given initial condition Ψ0(r). Here, V(r, t) is an external potential, and \({\boldsymbol{\sigma }}\,=\,{\sigma }_{{\rm{x}}}\,\hat{{\boldsymbol{x}}}+{\sigma }_{{\rm{y}}}\,\hat{{\boldsymbol{y}}}+{\sigma }_{{\rm{z}}}\,\hat{{\boldsymbol{z}}}\) is a 3-vector of Pauli spin matrices. The quantum continuity equation for the Pauli equation reads18,19

$$\frac{\partial |{\rm{\Psi }}{|}^{2}}{\partial t}\,=\,\frac{\hslash }{m}\,{\rm{\nabla }}\,\cdot \,({\rm{Im}}\,[{{\rm{\Psi }}}^{\dagger }{\rm{\nabla }}{\rm{\Psi }}]+\frac{1}{2}\,{\rm{\nabla }}\,\times \,({{\rm{\Psi }}}^{\dagger }{\boldsymbol{\sigma }}{\rm{\Psi }}))\,=\,{\rm{\nabla }}\,\cdot \,{{\rm{J}}}_{\mathrm{Pauli}}=\,:{\rm{\nabla }}\,\cdot \,({{\boldsymbol{v}}}_{\mathrm{Bohm}}^{{\rm{\Psi }}}|{\rm{\Psi }}{|}^{2}),$$
(3)

where \({{\rm{\Psi }}}^{\dagger }\) is the adjoint of Ψ, and \(|{\rm{\Psi }}{|}^{2}={{\rm{\Psi }}}^{\dagger }{\rm{\Psi }}\). The rightmost equality of (3) defines the Bohmian velocity field \({{\boldsymbol{v}}}_{\mathrm{Bohm}}^{{\rm{\Psi }}}={{\bf{J}}}_{\mathrm{Pauli}}/|{\rm{\Psi }}{|}^{2}\). The term \(\frac{\hslash }{m}{\rm{I}}{\rm{m}}[{{\rm{\Psi }}}^{\dagger }{\boldsymbol{\nabla }}{\rm{\Psi }}]\) is the so-called convective flux, while \(\frac{\hslash }{2m}\,{\boldsymbol{\nabla }}\times ({{\rm{\Psi }}}^{\dagger }{\boldsymbol{\sigma }}{\rm{\Psi }})\) is the spin flux. The alert reader will recognize that the spin flux is divergenceless, hence one may argue that neither the flux JPauli nor the Bohmian velocity are uniquely defined. However, observing that the Pauli equation and its flux emerge as non-relativistic limits of the Dirac equation and the Dirac flux, respectively, which are unique20,21,22, one is led directly to the current and Bohmian velocity given here.

The Bohmian trajectories are integral curves of the velocity field \({{\boldsymbol{v}}}_{\mathrm{Bohm}}^{{\rm{\Psi }}}\), hence the Bohmian guidance law reads

$$\frac{{\rm{d}}}{{\rm{d}}t}\,{\boldsymbol{R}}(t)\,=\,{{\boldsymbol{v}}}_{\mathrm{Bohm}}^{{\rm{\Psi }}}\,({\boldsymbol{R}}(t),t)\,=\,\frac{\hslash }{m}\,{\rm{Im}}\,[\frac{{{\rm{\Psi }}}^{\dagger }{\rm{\nabla }}{\rm{\Psi }}}{{{\rm{\Psi }}}^{\dagger }{\rm{\Psi }}}]\,({\boldsymbol{R}}(t),t)\,+\,\frac{\hslash }{2m}[\frac{{\rm{\nabla }}\,\times \,({{\rm{\Psi }}}^{\dagger }\sigma {\rm{\Psi }})}{{{\rm{\Psi }}}^{\dagger }{\rm{\Psi }}}]\,({\boldsymbol{R}}(t),t)\mathrm{.}$$
(4)

Here, R(t) is the position of the particle at time t. In Bohm’s theory, the spin-1/2 particle has no degrees of freedom other than those specifying its position in space, so spin is not an extra degree of freedom. Thus, all quantum mechanical phenomena attributed to spin (such as the deflection of particles in the Stern-Gerlach experiment) arise solely from the non-linear equation of motion23,24. The guidance law ((4) is time reversal invariant and its right-hand side transforms as a velocity under Galilean transformations (see16,21 for further discussion). We integrate Eq. (4) for a statistical ensemble of |Ψ0|2-distributed initial particle positions R(0) (see25 for a justification).

Methods

Our computations and results are for the following setup: Let the cylindrical waveguide be mounted on the xy−plane of a right-handed orthogonal coordinate system, the axis of the cylinder defining the z−axis (Fig. 1). Employing cylindrical coordinates r ≡ (ρ, ϕ, z), we model the potential field of the waveguide as \(V({\boldsymbol{r}},t)={V}_{\perp }(\rho )+{V}_{\parallel }(z,t)\), where \({V}_{\perp }(\rho )=\frac{1}{2}\,m\,{\omega }^{2}{\rho }^{2}\) is a transverse confining potential, and \({V}_{\parallel }(z,t)=v(z)+\theta (-t)v(d-z)\) is a time dependent axial potential comprised of an impenetrable hard-wall at z = 0, viz.,

$$v(z)\,=\,\{\begin{array}{cc}\infty & z\,\le \,0\\ 0 & z\, > \,0\end{array},$$
(5)

and another impenetrable potential barrier v(dz) that is switched off at t = 0. The wall at z = 0 is the end face of the waveguide and θ(x) is Heaviside’s step function. Fortunately, near perfect harmonic confinements can be realized in conventional (ultrahigh vacuum) Penning traps, which can trap single electrons26,27 and protons28 over a wide range of trapping frequencies. For electrons, typical waveguide parameters read: L ≈ 6−10 mm, ω ≈ 109−1011 rad/s26,29. In30 we give a detailed analysis of the proposed experiment for a quadrupole ion trap (Paul trap) waveguide.

The particle is prepared in a ground state of the cylindrical box at t = 0, which can be written as Ψ0(r) = ψ0(r)χ, where (setting ħ = m = d = 1),

$${{\boldsymbol{\psi }}}_{0}({\boldsymbol{r}})\,=\,\sqrt{\frac{2{\boldsymbol{\omega }}}{\,\pi }}\,{\boldsymbol{\theta }}(z){\boldsymbol{\theta }}\mathrm{(1}-z)\,\sin (\pi z)\,\exp \,(-\frac{{\boldsymbol{\omega }}}{2}{\rho }^{2})$$
(6)

is the spatial part of the wave function, and

$${\rm{\chi }}=(\begin{array}{c}\cos \,(\alpha /\mathrm{2)}\\ \sin \,(\alpha /\mathrm{2)}\,{e}^{i\beta }\end{array}),\,0\,\le \,\alpha \,\le \,\pi ,\,0\,\le \,\beta \, < \,2\pi ,$$
(7)

is a normalized Bloch spinor \({(\chi }^{\dagger }\chi =1)\). Fixing α and β, we obtain different ground state wave functions. For instance, α = 0 (π) gives the spin-up (spin-down) ground state wave function, usually denoted by Ψ), while \(\alpha \,=\,\frac{\pi }{2}\) yields the so-called up-down ground state wave function \({{\rm{\Psi }}}_{\updownarrow }\,=\,\frac{1}{\sqrt{2}}({{\rm{\Psi }}}_{\uparrow }+{{\rm{\Psi }}}_{\downarrow })\). We refer to α and β as spin orientation angles, because they specify the orientation of the “spin vector” \({\bf{s}}\,:\,=\,\frac{1}{2}({{\rm{\Psi }}}_{0}^{\dagger }{\boldsymbol{\sigma }}{{\rm{\Psi }}}_{0})/|{{\rm{\Psi }}}_{0}{|}^{2}\), given by

$${\bf{s}}\,=\,\frac{1}{2}(\sin \alpha \,\cos \beta \,\hat{{\boldsymbol{x}}}+\sin \alpha \,\sin \beta \,\hat{{\boldsymbol{y}}}+\cos \alpha \,\hat{{\boldsymbol{z}}}).$$

The instant the barrier is switched off, the wave function spreads dispersively, filling the volume of the waveguide. The particle moves according to (4) on the Bohmian trajectory \({\boldsymbol{R}}(t)=R(t)\,[\,\cos \,{\rm{\Phi }}\,(t)\,\hat{{\boldsymbol{x}}}\,+\,\sin \,{\rm{\Phi }}\,(t)\,\hat{{\boldsymbol{y}}}\,]+Z(t)\hat{{\boldsymbol{z}}}\). In this choice of coordinates the first arrival time of a trajectory starting at R(0) and arriving at z = L is

$$\tau ({\boldsymbol{R}}(0))\,=\,{\rm{i}}{\rm{n}}{\rm{f}}\{t\,|\,Z(t,{\boldsymbol{R}}(0))\,=\,L,\,{\boldsymbol{R}}(0)\in {\rm{s}}{\rm{u}}{\rm{p}}{\rm{p}}({{\rm{\Psi }}}_{0})\},$$
(8)

where Z(t, R(0)) ≡ Z(t) is the z−coordinate of the particle at time t, and supp(Ψ0) denotes the support of the initial wave function (the interior of the cylindrical box). Since the initial position R(0) is |Ψ0|2-distributed25, the distribution of τ(R(0)) is given by

$${{\rm{\Pi }}}_{\mathrm{Bohm}}^{{{\boldsymbol{\Psi }}}_{0}}(\tau )\,=\,{\int }_{\mathrm{supp}({{\boldsymbol{\Psi }}}_{0})}\,{d}^{3}{\boldsymbol{R}}(0)\delta ({\boldsymbol{\tau }}({\boldsymbol{R}}(0))\,-\,{\boldsymbol{\tau }})\,|{{\boldsymbol{\Psi }}}_{0}{|}^{2}({\boldsymbol{R}}(0))\,.$$
(9)

In general, there is no closed-form expression for (8), hence the integral in (9) cannot be evaluated analytically. However, if the Bohmian trajectories cross ∂Σ at most once, or in other words if the quantum flux JPauli is outward directed at every point of ∂Σ, at all times (also referred to as the current positivity condition), then \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{{{\rm{\Psi }}}_{0}}\,(\tau )\) reduces to the integrated quantum flux Πqf(τ), Eq. (1) with the Pauli current JPauli replacing J5,6.

Note well that by the very meaning of the quantum flux, (1) is a natural guess for the arrival time distribution from the point of view of standard quantum mechanics as well5. However, (1) makes sense only if the left-hand side is positive, which need not be the case. Of course, if the current positivity condition holds, the left-hand side of (1) ≥0, and Πqf becomes a special case of (9). Generally, this condition does not hold, in which case one computes \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{{{\rm{\Psi }}}_{0}}(\tau )\) numerically from a large number of Bohmian trajectories.

Results and Discussion

(i) For the spin-up (α = 0) and spin-down (α = π) wave functions the arrival time distribution \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{{{\rm{\Psi }}}_{0}}\,(\tau )\) coincides with the quantum flux expression (1), since in these cases the current positivity condition is satisfied. Moreover, in these cases JPauli(r,τ) can be replaced by the convective flux \(\frac{\hslash }{m}{\rm{I}}{\rm{m}}[{{\rm{\Psi }}}^{\dagger }{\boldsymbol{\nabla }}{\rm{\Psi }}]\) in (1). The resulting distribution has a heavy tail \(\sim {\tau }^{-4}\) as τ → ∞. (ii) For other initial wave functions \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{{{\rm{\Psi }}}_{0}}\,(\tau )\) differs from (1) and falls off faster than τ−4. For any initial ground state wave function, the arrival time distribution displays an infinite sequence of self-similar lobes below \(\tau \,=\,\frac{mdL}{2\pi \hslash }\) (see Fig. 2 below), which diminish in size as τ → 0. These lobes mirror typical wave function evolution when suddenly released to spread freely into the volume of the waveguide (see also31). (iii) If the initial wave function is an equal superposition of the spin-up and spin-down wave functions (\(\alpha \,=\,\frac{\pi }{2}\)), the arrival time distribution pinches off at a maximum arrival time τmax, i.e., no particle arrivals occur for τ > τmax. Moreover an even more striking manifestation of the lobes can be seen: characteristic “no-arrival windows” appear between the smaller lobes, inside which the arrival time distribution is zero. (iv) Time of flight measurements refer in general to semiclassical expressions based on the momentum distribution. Our distributions deviate significantly from this alleged semiclassical formula.

Figure 2
figure2

Arrival time histograms for spin-up \(({{\rm{\Pi }}}_{\mathrm{Bohm}}^{\mathrm{0|0}}(\tau ))\) and up-down \(({{\rm{\Pi }}}_{\mathrm{Bohm}}^{\frac{\pi }{2}\mathrm{|0}}(\tau ))\) wave functions, L = 100 and ω = 103 graphed along with the semiclassical arrival time distribution Πsc(τ) (dashed line) and the quantum (convective) flux distribution Πqf(τ) (solid line). We see agreement between \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{\mathrm{0|0}}(\tau )\) and Πqf(τ). For the up-down case, no arrivals are recorded for τ > 42.9 (= τmax). Note the disagreement of all distributions with Πsc(τ). Each histogram in this figure has been generated with 105 Bohmian trajectories. The time scale on the horizontal axis is ≈21.7 μs, assuming d = 50 μm. Inset: Magnified view of the self-similar smaller lobes of the up-down histogram, separated by distinct no-arrival windows.

A few details concerning the computation of our results are in order. First note that the Pauli equation (2) with initial condition Ψ0(r) can be solved in closed form, facilitating very fast numerical computation of Bohmian trajectories. The time dependent wave function takes the form Ψ(r, t) = ψ(r, t)χ, where the spin part is given by (7), while

$${\boldsymbol{\psi }}({\boldsymbol{r}},t)\,=\,\sqrt{\frac{2\omega }{\pi }}\,\exp (-\frac{\omega }{2}{\rho }^{2}\,-\,i\omega t)W(z,t),$$
(10)

where

$$W(z,t)\,=\,\theta (z)[{\mathscr{D}}(z\,-\,1,t)\,+\,{\mathscr{D}}(1\,-\,z,t)\,-\,{\mathscr{D}}(1\,+\,z,t)\,-\,{\mathscr{D}}(-\,1\,-\,z,t)\,],$$
(11)

which we call the ‘time evolution integral’. In (11):

$${\mathscr{D}}(x,t):\,=\frac{{e}^{-i\frac{{\pi }^{2}}{2}t}}{8i}\{{e}^{i\pi x}\,{\rm{erfc}}\,[\frac{{i}^{\mathrm{3/2}}}{\sqrt{2}}(\frac{x}{\sqrt{t}}\,-\,\pi \sqrt{t})]\,-\,{e}^{-i\pi x}\,{\rm{erfc}}\,[\frac{{i}^{\mathrm{3/2}}}{\sqrt{2}}(\frac{x}{\sqrt{t}}\,+\,\pi \sqrt{t})]\},$$
(12)

where erfc(x) is the complementary error function. A detailed derivation of this result will be given elsewhere32. Substituting our solution for the time dependent wave function in the guidance law (4), we obtain coupled non-linear equations of motion for the spin-1/2 particle:

$$\dot{R}(t)\,=\,\sin \,\alpha \,\sin ({\rm{\Phi }}(t)\,-\,\beta )\,{\rm{Re}}\,[\frac{W^{\prime} }{W}]\,(Z(t),t),$$
(13a)
$$\dot{{\boldsymbol{\Phi }}}(t)\,=\,\frac{\sin \alpha }{{\boldsymbol{R}}(t)}\,\cos ({\boldsymbol{\Phi }}(t)\,-\,\beta )\,\mathrm{Re}\,[\frac{W^{\prime} }{W}]\,(Z(t),t)\,+\,{\boldsymbol{\omega }}\,\cos \,{\boldsymbol{\alpha }},$$
(13b)
$$\dot{Z}(t)\,=\,\text{Im}\,[\frac{W^{\prime} }{W}]\,(Z(t),t)\,+\,{\boldsymbol{\omega }}\,\sin \,\alpha \,\sin ({\boldsymbol{\Phi }}(t)\,-\,\beta )R(t),$$
(13c)

where R, Φ and Z are the cylindrical coordinates of R and W′ = ∂W/∂z. The parameters in the initial wave function are, in view of (7), α and β, so we denote \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{{{\rm{\Psi }}}_{0}}\,(\tau )\,\equiv \,{{\rm{\Pi }}}_{\mathrm{Bohm}}^{\alpha |\beta }\,(\tau )\). In fact, it is enough to consider β = 0 only since

$${{\rm{\Pi }}}_{\mathrm{Bohm}}^{\alpha |\beta }\,(\tau )\,=\,{{\rm{\Pi }}}_{\mathrm{Bohm}}^{\alpha \mathrm{|0}}\,(\tau ),$$
(14a)
$${{\rm{\Pi }}}_{\mathrm{Bohm}}^{\alpha |\beta }(\tau )\,=\,{{\rm{\Pi }}}_{\mathrm{Bohm}}^{\pi -\alpha |\beta }(\tau \mathrm{).}$$
(14b)

These properties follow partly from the symmetries of Eq. (13) and partly from the initial uniform distribution of Φ(0) due to the choice of the initial state Eq. (6) (see32 for further details). We sample N ≈ 105 initial positions from the |Ψ0|2 distribution, solve Eq. (13) numerically for each point in this ensemble, continuing until the trajectory hits z = L, then record the arrival time and plot the histogram for \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{\alpha \mathrm{|0}}(\tau )\).

For the spin-up and spin-down wave functions, Eq. (13c) reduces to \(\dot{Z}\,=\,{\rm{Im}}[W^{\prime} /W](Z(t),t)\) and numerically it turns out that Im[W′/W](L, t) > 0. Hence the spin-up and spin-down trajectories cross ∂Σ at most once, and the first arrival time distribution (or simply the arrival time distribution) in these cases equals (cf. Eq. (1))

$${{\rm{\Pi }}}_{{\rm{qf}}}(\tau )\,=\,2\,{\rm{Im}}[{W}^{\ast }(L,\tau )W^{\prime} (L,\tau )].$$
(15)

As noted, (15) is non-negative for all values of τ, and features prominently a large main lobe for \(\tau > \frac{L}{2\pi }\). The main lobe falls off as \({(\frac{L}{\pi })}^{3}\frac{4}{{\tau }^{4}},\,{\rm{a}}{\rm{s}}\,\,\tau \to {\rm{\infty }}.\) An infinite train of smaller lobes permeates the interval \(0 < \tau < \frac{L}{2\pi }\), which are well approximated by the formula \(\frac{4\pi }{L}\sin {c}^{2}(\frac{L}{\tau })\), whenever \(\tau \ll L\). Apart from that we find that Πqf(τ) is a function only of the arrival distance L. It is also independent of the trapping frequency ω, which is rather surprising. In fact, the spin-up (down) arrival time distributions are independent of the exact shape of the transverse confining potential V(ρ) of the waveguide as well32. Figure 2 depicts our results for L = 100 (≈5 mm for a d = 50 m trap) and ω = 103 (≈46.3 × 106 rad/s). Note: We have expressed L, ω and τ in units of d, \(\frac{\hslash }{m{d}^{2}}\) and \(\frac{m{d}^{2}}{\hslash }\), respectively. For a d = 50 μm trap, known electron mass m ≈ 9.11 × 10−31kg and reduced Planck’s constant ħ ≈ 1.05 × 10−34Js, the frequency and time units are ≈46.3 × 103 rad/s and ≈21.7 μs, respectively.

For wave functions corresponding to \(0 < \alpha \le \frac{\pi }{2}\) (cf. (14b)), the first arrival time distribution is not given by the integrated flux (1). This is because the Bohmian trajectories in these cases cross ∂Σ more than once, hence the aforementioned current positivity condition is not met. As α approaches \(\frac{\pi }{2}\), the tail of \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{\alpha \mathrm{|0}}(\tau )\) thins gradually, pinching off completely at a characteristic maximum arrival time τmax for \(\alpha =\frac{\pi }{2}\) (i.e. all Bohmian trajectories with wave function \({{\rm{\Psi }}}_{\updownarrow }\) strike the detector surface z = L before t = τmax). In Fig. 2 τmax ≈ 42.9, which corresponds to ≈1 ms. This behavior results in a sharp drop in the mean first arrival time τ in the vicinity of \(\alpha =\frac{\pi }{2}\), as shown in Fig. 3 below.

Figure 3
figure3

Mean first arrival time 〈τ〉 vs. spin orientation angle α for L = 10 and β = 0. The symmetry of the curves about \(\alpha =\frac{\pi }{2}\) is a consequence of property (14b).

Unlike the spin-up (down) case, the up-down arrival time statistics are influenced by the trapping frequency ω. Keeping L fixed, we find that the maximum arrival time τmax, mean first arrival time 〈τ〉, and the standard deviation σ corresponding to \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{\frac{\pi }{2}\mathrm{|0}}(\tau )\) decrease with increasing ω, each approaching a constant for \(\omega \gg 1\). Conversely, when these quantities are graphed as functions of L with ω fixed, we see a clear linear growth in each (see Fig. 4).

Figure 4
figure4

(a) Graphs of mean first arrival time \(\langle \tau \rangle \), standard deviation σ and maximum arrival time τmax for the up-down wave function vs. L, keeping ω fixed. The mean arrival time of Πqf(τ) is also shown here. (b) Graphs of mean, standard deviation and maximum arrival time vs. ω, keeping L fixed.

Remarkably, these effects persist even for large L, provided ω is also made suitably large (a welcome feature for Penning traps). Increasing L causes the arrival time distributions to shift to larger values of τ, thus the smaller lobes can be easily seen, especially in experiments incapable of resolving very small arrival times.

Since the smaller (self-similar) lobes become progressively smaller, resolving the nth lobe (denoting the main lobe by n = 1) is limited by the least time count (δt) of the measuring apparatus. Roughly, δt < width of nthlobe should suffice to resolve the first n lobes. This translates into32

$$\delta t\, < \,(\frac{md}{\pi \hslash })\frac{L}{{n}^{2}}.$$
(16)

For d = 50 μm and L = 5 mm (Fig. 2), a modest δt ≈ 10 μs will successfully resolve 8 lobes (main + 7 smaller lobes), while δt ≈ 0.1 μs will resolve as many as 83 lobes (main + 82 smaller lobes). However, we must also understand that only a few data points (about \((\frac{2}{{\pi }^{2}})\frac{N}{{n}^{4}}\) in N experiments) contribute to the nth lobe, especially when \(n\gg 1\). This number, being independent of any tunable parameters like L, ω, etc., sets an intrinsic limit on the experimenter’s ability to resolve the distant lobes.

Finally, we come to the semiclassical arrival time distribution (dashed line in Fig. 2),

$${{\rm{\Pi }}}_{{\rm{s}}{\rm{c}}}(\tau )\,=\,{\int }_{{\rm{\partial }}{\rm{\Sigma }}}\,\frac{{\boldsymbol{r}}\cdot {\rm{d}}{\bf{s}}}{{\tau }^{4}}{|{\mathop{\psi }\limits^{ \sim }}_{0}(\frac{{\boldsymbol{r}}}{\tau })|}^{2},$$
(17)

routinely used in the interpretation of time-of-flight experiments. Here, \({\mathop{\psi }\limits^{ \sim }}_{0}\) denotes the Fourier transform of the initial wave function ψ0. Although (17) is based on the tacit assumption that the particle moves classically between preparation and measurement stages (see § 5.3.1 of5), it can also be motivated from the scattering formalism6, [pg 971], provided the detector surface (∂Σ) is placed far away from the support of the initial wave function ψ0 (far field regime), where the external potentials are negligible. In typical cold atom experiments these conditions are met, hence the semiclassical formula (17) is empirically adequate. Therefore, soliciting deviations from (17), theorists have recommended “moving the detectors closer to the region of coherent wave packet production, or closer to the interaction region”2,33, pg 419] (i.e. L ≈ d). However, such a relocation may disturb the wave function of the particle in an undesirable way.

For a meaningful comparison with our results, Eq. (17) (which is only applicable for free propagation) must be generalized to account for the presence of the waveguide. This is done with the help of Newtonian trajectories for our setup and the quantum mechanical distribution of the initial momenta of the particle. A careful calculation32 yields

$${\Pi }_{{\rm{sc}}}(\tau )\,=\,\frac{8\pi L}{{\tau }^{2}}\frac{{{\rm{c}}{\rm{o}}{\rm{s}}}^{2}(L/2\tau )}{{((L/\tau {)}^{2}-{\pi }^{2})}^{2}},$$
(18)

which falls off as \((\frac{8}{{\pi }^{3}})\frac{L}{{\tau }^{2}}\) (compare this with Eq. (15) and its τ−4 fall-off). In Fig. 2, we see that the semiclassical formula (18) for L = 100 remains distinctly different from the Bohmian arrival time distributions, notwithstanding the largeness of L. This is because the (spin dependent) Bohmian trajectories for our setup do not approach Newtonian trajectories even at large L, unlike the Bohmian trajectories of a free particle, which become approximately Newtonian at large distances6.

Bohmian mechanics has been fruitfully applied in various physical disciplines with reference to technical advances34,35,36,37, and to a better understanding of quantum phenomena, even in quantum gravity38,39. We have proposed here a simple experiment that can possibly be performed with a detection mechanism as discussed in13,40,41,42, and we have provided the Bohmian arrival times as a benchmark: Our results demonstrate that the distribution of first arrival times of a spin-1/2 particle bears clear signatures of Bohm’s guidance law. The deviations of \({{\rm{\Pi }}}_{\mathrm{Bohm}}^{{{\rm{\Psi }}}_{0}}(\tau )\) from the quantum flux distribution (1), so strikingly in evidence, are particularly noteworthy.

Data Availability

The datasets generated and analyzed during the current study are available from the corresponding author on reasonable request.

References

  1. 1.

    Muga, J. G., Mayato, R. S. & Egusquiza, Í. L. (eds.) Time in Quantum Mechanics, vol. 1 of Lect. Notes Phys. 734, second edn. (Springer, Berlin Heidelberg, 2008).

  2. 2.

    Muga, J. G. & Leavens, C. R. Arrival time in quantum mechanics. Phys. Rep. 338, 353–438, https://doi.org/10.1016/S0370-1573 (2000).

    ADS  MathSciNet  CAS  Article  Google Scholar 

  3. 3.

    Allcock, G. R. The time of arrival in quantum mechanics I. formal considerations. Ann. Phys. 53, 253–285, https://doi.org/10.1016/0003-4916 (1969).

    ADS  Article  Google Scholar 

  4. 4.

    Aharonov, Y. & Bohm, D. Time in the quantum theory and the uncertainty relation for time and energy. Phys. Rev. 122, 1649–1658, https://doi.org/10.1103/PhysRev.122.1649 (1961).

    ADS  MathSciNet  Article  MATH  Google Scholar 

  5. 5.

    Blanchard, P. & Fröhlich, J. (eds.) The Message of Quantum Science: Attempts Towards a Synthesis. Lect. Notes Phys. 899 (Springer, Berlin Heidelberg, 2015).

  6. 6.

    Daumer, M., Dürr, D., Goldstein, S. & ZanghÌ, N. On the quantum probability flux through surfaces. J. Stat. Phys. 88, 967–977, https://doi.org/10.1023/B:JOSS.0000015181.86864.fb (1997).

    ADS  MathSciNet  Article  MATH  Google Scholar 

  7. 7.

    Vona, N., Hinrichs, G. & Dürr, D. What does one measure when one measures the arrival time of a quantum particle? Phys. Rev. Lett. 111, 220404, https://doi.org/10.1103/PhysRevLett.111.220404 (2013).

    ADS  CAS  Article  PubMed  Google Scholar 

  8. 8.

    Tumulka, R. Distribution of the time at which an ideal detector clicks. ArXiv e-prints (2016).

  9. 9.

    Dürr, D., Goldstein, S. & ZanghÌ, N. Quantum equilibrium and the role of operators as observables in quantum theory. J. Stat. Phys. 116, 959–1055, https://doi.org/10.1023/B:JOSS.0000 (2004).

    ADS  MathSciNet  Article  MATH  Google Scholar 

  10. 10.

    Kocsis, S. et al. Observing the average trajectories of single photons in a two-slit interferometer. Science 332, 1170–1173, https://doi.org/10.1126/science.1202218 (2011).

    ADS  CAS  Article  PubMed  MATH  Google Scholar 

  11. 11.

    Yearsley, J. M. A review of the decoherent histories approach to the arrival time problem in quantum theory. J. Phys. Conf. Ser 306, 012056, https://doi.org/10.1088/1742-6596/306/1/012056 (2011).

    Article  Google Scholar 

  12. 12.

    Allcock, G. R. The time of arrival in quantum mechanics II. the individual measurement. Ann. Phys. 53, 286–310, https://doi.org/10.1016/0003-4916 (1969).

    ADS  Article  Google Scholar 

  13. 13.

    Allcock, G. R. The time of arrival in quantum mechanics III. the measurement ensemble. Ann. Phys. 53, 311–348, https://doi.org/10.1016/0003-4916 (1969).

    ADS  Article  Google Scholar 

  14. 14.

    Landsman, A. S. et al. Ultrafast resolution of tunneling delay time. Optica 1, 343–349, https://doi.org/10.1364/OPTICA.1.000343 (2014).

    CAS  Article  Google Scholar 

  15. 15.

    Zimmermann, T. et al. Tunneling time and weak measurement in strong field ionization. Phys. Rev. Lett. 116, 233603, https://doi.org/10.1103/PhysRevLett.116.233603 (2016).

    ADS  CAS  Article  PubMed  Google Scholar 

  16. 16.

    Bohm, D. & Hiley, B. J. The Undivided Universe: An Ontological Interpretation of Quantum Theory (Routledge, London and New York, 1993).

  17. 17.

    Leavens, C. R. Time of arrival in quantum and Bohmian mechanics. Phys. Rev. A 58, 840–847, https://doi.org/10.1103/PhysRevA.58.840 (1998).

    ADS  MathSciNet  CAS  Article  Google Scholar 

  18. 18.

    Shikakhwa, M. S., Turgut, S. & Pak, N. K. Derivation of the magnetization current from the non-relativistic pauli equation. Am. J. Phys. 79, 1177–1179, https://doi.org/10.1119/1.3630931 (2011).

    ADS  Article  Google Scholar 

  19. 19.

    Hodge, W. B., Migirditch, S. V. & Kerr, W. C. Electron spin and probability current density in quantum mechanics. Am. J. Phys. 82, 681–690, https://doi.org/10.1119/1.4868094 (2014).

    ADS  CAS  Article  Google Scholar 

  20. 20.

    Holland, P. R. Uniqueness of conserved currents in quantum mechanics. Ann. Phys. (Leipzig) 12, 446–462, https://doi.org/10.1002/andp.200310022 (2003).

    ADS  MathSciNet  Article  MATH  Google Scholar 

  21. 21.

    Holland, P. R. Uniqueness of paths in quantum mechanics. Phy. Rev. A 60, 4326–4330, https://doi.org/10.1103/PhysRevA.60.4326 (1999).

    ADS  CAS  Article  Google Scholar 

  22. 22.

    Holland, P. R. & Philippidis, C. Implications of lorentz covariance for the guidance equation in two-slit quantum interference. Phy. Rev. A 67, 062105, https://doi.org/10.1103/PhysRevA.67.062105 (2003).

    ADS  CAS  Article  Google Scholar 

  23. 23.

    Dewdney, C., Holland, P. R. & Kyprianidis, C. What happens in a spin measurement? Phys. Lett. A 119, 259–267, https://doi.org/10.1016/0375-9601 (1986).

    ADS  CAS  Article  Google Scholar 

  24. 24.

    Dewdney, C., Holland, P. R., Kyprianidis, C. & Vigier, J. P. Spin and non-locality in quantum mechanics. Nature 336, 536–544, https://doi.org/10.1038/336536a0 (1988).

    ADS  CAS  Article  Google Scholar 

  25. 25.

    Dürr, D., Goldstein, S. & ZanghÌ, N. Quantum equilibrium and the origin of absolute uncertainty. J. Stat. Phys. 67, 843–907, https://doi.org/10.1007/BF01049004 (1992).

    ADS  MathSciNet  Article  MATH  Google Scholar 

  26. 26.

    Wineland, D., Ekstrom, P. & Dehmelt, H. Monoelectron oscillator. Phys. Rev. Lett. 31, 1279–1282, https://doi.org/10.1103/PhysRevLett.31.1279 (1973).

    ADS  CAS  Article  Google Scholar 

  27. 27.

    Joseph, T. & Gabrielse, G. One electron in an orthogonalized cylindrical Penning trap. Appl. Phys. Lett. 55, 2144–2146, https://doi.org/10.1063/1.102084 (1989).

    ADS  Article  Google Scholar 

  28. 28.

    Ulmer, S. et al. Observation of spin flips with a single trapped proton. Phys. Rev. Lett. 106, 253001, https://doi.org/10.1103/PhysRevLett.106.253001 (2011).

    ADS  CAS  Article  PubMed  Google Scholar 

  29. 29.

    Dehmelt, H. G. Nobel lecture: Experiments with an isolated subatomic particle at rest. Rev. Mod. Phys. 62, 525–530, https://doi.org/10.1103/RevModPhys.62.525 (1990).

    ADS  CAS  Article  Google Scholar 

  30. 30.

    Das, S., Nöth, M. & Dürr, D. Exotic Bohmian arrival times of spin-1/2 particles (in preparation).

  31. 31.

    Moshinsky, M. Diffraction in time. Phys. Rev. 88, 625–631, https://doi.org/10.1103/PhysRev.88.625 (1952).

    ADS  MathSciNet  Article  MATH  Google Scholar 

  32. 32.

    Das, S. Arrival Time Distributions of Spin-1/2 Particles. Master’s thesis, LMU Munich & TU Munich http://www.mathematik.uni-muenchen.de/bohmmech/theses/Das_Siddhant_MA.pdf and Das, S. & Dürr, D. Arrival time distributions and spin in quantum mechanics–A Bohmian perspective (in preparation) (2017).

  33. 33.

    Delgado, V. Quantum probability distribution of arrival times and probability current density. Phys. Rev. A 59, 1010–1020, https://doi.org/10.1103/PhysRevA.59.1010 (1999).

    ADS  CAS  Article  Google Scholar 

  34. 34.

    Marian, D., Zanghì, N. & Oriols, X. Weak values from displacement currents in multiterminal electron devices. Phys. Rev. Lett. 116, 110404, https://doi.org/10.1103/PhysRevLett.116.110404 (2016).

    ADS  CAS  Article  PubMed  Google Scholar 

  35. 35.

    Wyatt, R. E. Quantum dynamics with Trajectories: Introduction to Quantum Hydrodynamics (Springer, New York, 2005).

  36. 36.

    Oriols, X. & Mompart, J. (eds.) Applied Bohmian Mechanics: From Nanoscale Systems to Cosmology (Pan Stanford Publishing Pvt. Ltd., Singapore, 2012).

  37. 37.

    Sanz, A. S. & Miret-Artés, S. (eds.) A Trajectory Description of Quantum Processes, vol. 2 of Lect. Notes Phys. 831, second edn. (Springer, Berlin Heidelberg, 2014).

  38. 38.

    Pinto-Neto, N. & Fabris, J. C. Quantum cosmology from the de Broglie–Bohm perspective. Classical and Quantum Gravity 30, 143001 (2013).

    ADS  MathSciNet  Article  Google Scholar 

  39. 39.

    Struyve, W. Loop quantum cosmology & singularities. Sci. Rep. 7, https://doi.org/10.1038/s41598-017-06616-y (2017).

  40. 40.

    Groot-Berning, K. et al. Trapping and sympathetic cooling of single thorium ions for spectroscopy. ArXiv e-prints (2018).

  41. 41.

    Damborenea, J. A., Egusquiza, Í. L., Hegerfeldt, G. C. & Muga, J. G. Measurement-based approach to quantum arrival times. Physical Review. A 66, https://doi.org/10.1103/PhysRevA.66.052104 (2002).

  42. 42.

    Uehara, Y. et al. High resolution time-of-flight electron spectrometer. Jpn. J. Appl. Phys 29, 2858–2863, https://doi.org/10.1143/JJAP.29.2858 (1990).

    ADS  CAS  Article  Google Scholar 

Download references

Acknowledgements

The authors would like to thank J. M. Wilkes for critically reviewing the manuscript. He and Markus Nöth verified our analytical calculations meticulously, which led to the correction of a mistake in the early stages of the work. The assistance of Grzesio Gradziuk and Leopold Kellers with the numerical simulations was essential, and greatly appreciated. Thanks are also due to Serj Aristarkhov, Lukas Nickel, Ward Struyve, Nikolai Leopold, Roderich Tumulka and Nicola Vona for inspiration and enriching discussions on the subject of this letter.

Author information

Affiliations

Authors

Contributions

S.D. conceived the experiment and conducted the numerical computations. The paper was written equally by S.D. and D.D.

Corresponding authors

Correspondence to Siddhant Das or Detlef Dürr.

Ethics declarations

Competing Interests

The authors declare no competing interests.

Additional information

Publisher’s note: Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Rights and permissions

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

Reprints and Permissions

About this article

Verify currency and authenticity via CrossMark

Cite this article

Das, S., Dürr, D. Arrival Time Distributions of Spin-1/2 Particles. Sci Rep 9, 2242 (2019). https://doi.org/10.1038/s41598-018-38261-4

Download citation

Further reading

Comments

By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.

Search

Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing