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arXiv:2306.12000 · Physical Review A

Space-time-symmetric extension of quantum mechanics: Interpretation and arrival-time predictions

Rodrigo Gomes de Araujo, Ricardo Ximenes, Eduardo O. Dias

Published Jan 24, 2024• 6 citations
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Abstract

An alternative quantization rule, in which time becomes a self-adjoint operator and position is a parameter, was proposed by Dias and Parisio [Phys. Rev. A 95, 032133 (2017)]. In this approach, the authors derived a space-time-symmetric (STS) extension of quantum mechanics (QM) where a new quantum state (intrinsic to the particle) $|\ensuremath{\phi}(x)\ensuremath{\rangle}$ is defined at each point in space. The quantum state $|\ensuremath{\phi}(x)\ensuremath{\rangle}$ obeys a space-conditional (SC) Schr\"odinger equation and its projection on $|t\ensuremath{\rangle}, \ensuremath{\langle}t|\ensuremath{\phi}(x)\ensuremath{\rangle}$, represents the probability amplitude of the particle's arrival time at $x$. In this work we provide an interpretation of the SC Schr\"odinger equation and the eigenstates of observables in the STS extension. Analogous to the usual QM, we propose that by knowing the initial state $|\ensuremath{\phi}({x}_{0})\ensuremath{\rangle}$, which predicts any measurement on the particle performed by a detector localized at ${x}_{0}$, the SC Schr\"odinger equation provides $|\ensuremath{\phi}(x)\ensuremath{\rangle}=\stackrel{\ifmmode \hat{}\else \^{}\fi{}}{\mathbb{U}}(x,{x}_{0})|\ensuremath{\phi}({x}_{0})\ensuremath{\rangle}$, enabling us to predict measurements when the detector is at $x\ensuremath{\lessgtr}{x}_{0}$. We also verify that for space-dependent potentials, momentum eigenstates in the STS extension $|{P}_{b}(x)\ensuremath{\rangle}$ depend on position just as energy eigenstates in the usual QM depend on time for time-dependent potentials. In this context, whereas a particle in the momentum eigenstate in the standard QM, $|\ensuremath{\psi}(t)\ensuremath{\rangle}={|P\ensuremath{\rangle}|}_{t}$, at time $t$, has momentum $P$ (and indefinite position), the same particle in the state $|\ensuremath{\phi}(x)\ensuremath{\rangle}=|{P}_{b}(x)\ensuremath{\rangle}$ arrives at position $x$ with momentum ${P}_{b}(x)$ (and indefinite arrival time). By investigating the fact that $|\ensuremath{\psi}(t)\ensuremath{\rangle}$ and $|\ensuremath{\phi}(x)\ensuremath{\rangle}$ describe experimental data of the same observables collected at $t$ and $x$, respectively, we conclude that they provide complementary information about the same particle. Finally, we solve the SC Schr\"odinger equation for an arbitrary space-dependent potential. We apply this solution to a potential barrier and compare it with a generalized Kijowski distribution, showing that they can predict distinct traversal times.

DOI
10.1103/physreva.109.012221

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An alternative quantization rule, in which time becomes a self-adjoint operator and position is a parameter, was proposed by Dias and Parisio [Phys. Rev. A 95, 032133 (2017)]. In this approach, the authors derived a space-time-symmetric (STS) extension of quantum mechanics (QM) where a new quantum state (intrinsic to the particle) ∣\ensuremathϕ(x)\ensuremath⟩|\ensuremath{\phi}(x)\ensuremath{\rangle}∣\ensuremathϕ(x)\ensuremath⟩ is defined at each point in space. The quantum state ∣\ensuremathϕ(x)\ensuremath⟩|\ensuremath{\phi}(x)\ensuremath{\rangle}∣\ensuremathϕ(x)\ensuremath⟩ obeys a space-conditional (SC) Schr"odinger equation and its projection on ∣t\ensuremath⟩,\ensuremath⟨t∣\ensuremathϕ(x)\ensuremath⟩|t\ensuremath{\rangle}, \ensuremath{\langle}t|\ensuremath{\phi}(x)\ensuremath{\rangle}∣t\ensuremath⟩,\ensuremath⟨t∣\ensuremathϕ(x)\ensuremath⟩, represents the probability amplitude of the particle's arrival time at xxx. In this work we provide an interpretation of the SC Schr"odinger equation and the eigenstates of observables in the STS extension. Analogous to the usual QM, we propose that by knowing the initial state ∣\ensuremathϕ(x0)\ensuremath⟩|\ensuremath{\phi}({x}_{0})\ensuremath{\rangle}∣\ensuremathϕ(x0​)\ensuremath⟩, which predicts any measurement on the particle performed by a detector localized at x0{x}_{0}x0​, the SC Schr"odinger equation provides ∣\ensuremathϕ(x)\ensuremath⟩=U\ifmmode^\elseˆ\fi(x,x0)∣\ensuremathϕ(x0)\ensuremath⟩|\ensuremath{\phi}(x)\ensuremath{\rangle}=\stackrel{\ifmmode \hat{}\else \^{}\fi{}}{\mathbb{U}}(x,{x}_{0})|\ensuremath{\phi}({x}_{0})\ensuremath{\rangle}∣\ensuremathϕ(x)\ensuremath⟩=U\ifmmode^\elseˆ\fi​(x,x0​)∣\ensuremathϕ(x0​)\ensuremath⟩, enabling us to predict measurements when the detector is at x\ensuremath≶x0x\ensuremath{\lessgtr}{x}_{0}x\ensuremath≶x0​. We also verify that for space-dependent potentials, momentum eigenstates in the STS extension ∣Pb(x)\ensuremath⟩|{P}_{b}(x)\ensuremath{\rangle}∣Pb​(x)\ensuremath⟩ depend on position just as energy eigenstates in the usual QM depend on time for time-dependent potentials. In this context, whereas a particle in the momentum eigenstate in the standard QM, ∣\ensuremathψ(t)\ensuremath⟩=∣P\ensuremath⟩∣t|\ensuremath{\psi}(t)\ensuremath{\rangle}={|P\ensuremath{\rangle}|}_{t}∣\ensuremathψ(t)\ensuremath⟩=∣P\ensuremath⟩∣t​, at time ttt, has momentum PPP (and indefinite position), the same particle in the state ∣\ensuremathϕ(x)\ensuremath⟩=∣Pb(x)\ensuremath⟩|\ensuremath{\phi}(x)\ensuremath{\rangle}=|{P}_{b}(x)\ensuremath{\rangle}∣\ensuremathϕ(x)\ensuremath⟩=∣Pb​(x)\ensuremath⟩ arrives at position xxx with momentum Pb(x){P}_{b}(x)Pb​(x) (and indefinite arrival time). By investigating the fact that ∣\ensuremathψ(t)\ensuremath⟩|\ensuremath{\psi}(t)\ensuremath{\rangle}∣\ensuremathψ(t)\ensuremath⟩ and ∣\ensuremathϕ(x)\ensuremath⟩|\ensuremath{\phi}(x)\ensuremath{\rangle}∣\ensuremathϕ(x)\ensuremath⟩ describe experimental data of the same observables collected at ttt and xxx, respectively, we conclude that they provide complementary information about the same particle. Finally, we solve the SC Schr"odinger equation for an arbitrary space-dependent potential. We apply this solution to a potential barrier and compare it with a generalized Kijowski distribution, showing that they can predict distinct traversal times.
We generalize a space-time-symmetric (STS) extension of non-relativistic quantum mechanics (QM) to describe a particle moving in three spatial dimensions. In addition to the conventional time-conditional (Schrödinger) wave function ψ(x,y,z∣t)ψ(x, y, z | t)ψ(x,y,z∣t), we introduce space-conditional wave functions such as ϕ(t,y,z∣x)ϕ(t, y, z | x)ϕ(t,y,z∣x), where xxx plays the role of the evolution parameter. The function ϕ(t,y,z∣x)ϕ(t, y, z | x)ϕ(t,y,z∣x) represents the probability amplitude for the particle to arrive on the plane x=constantx = \text{constant}x=constant at time ttt and transverse position (y,z)(y, z)(y,z). Within this framework, the coordinate xμ∈{t,x,y,z}x^μ\in \{t, x, y, z\}xμ∈{t,x,y,z} can be conveniently chosen as the evolution parameter, depending on the experimental context under consideration. This leads to a unified formalism governed by a generalized Schrödinger-type equation, P^μ∣ϕμ(xμ)⟩=−iℏ ημνddxν∣ϕμ(xμ)⟩\hat{P}^μ |ϕ^μ(x^μ)\rangle = -i\hbar \, η^{μν} \frac{d}{dx^ν} |ϕ^μ(x^μ)\rangleP^μ∣ϕμ(xμ)⟩=−iℏημνdxνd​∣ϕμ(xμ)⟩. It reproduces standard QM when xμ=tx^μ= txμ=t, with ∣ϕ0(x0)⟩=∣ψ(t)⟩|ϕ^0(x^0)\rangle = |ψ(t)\rangle∣ϕ0(x0)⟩=∣ψ(t)⟩, and recovers the STS extension when xμ=xi∈{x,y,z}x^μ= x^i \in \{x, y, z\}xμ=xi∈{x,y,z}. For a free particle, we show that ϕ(t,y,z∣x)=⟨t,y,z∣ϕ(x)⟩ϕ(t, y, z | x) = \langle t, y, z | ϕ(x) \rangleϕ(t,y,z∣x)=⟨t,y,z∣ϕ(x)⟩ naturally reproduces the same dependence on the momentum wave function as the axiomatic Kijowski distribution. Possible experimental tests of these predictions are discussed. Finally, we demonstrate that the different states ∣ϕμ(xμ)⟩|ϕ^μ(x^μ)\rangle∣ϕμ(xμ)⟩ can emerge by conditioning (i.e., projecting) a timeless and spaceless physical state onto the eigenstate ∣xμ⟩|x^μ\rangle∣xμ⟩, leading to constraint equations of the form P^μ∣Φμ⟩=0\hat{\mathbb{P}}^μ|Φ^μ\rangle = 0P^μ∣Φμ⟩=0. This formulation generalizes the spirit of the Wheeler-DeWitt-type equation: instead of privileging time as the sole evolution parameter, it treats all coordinates on equal footing.
Time continues to be an intriguing physical property in the modern era. On the one hand, we have the classical and relativistic notion of time, where space and time have the same hierarchy, essential in describing events in spacetime. On the other hand, in quantum mechanics, time appears as a classical parameter, meaning that it does not have an uncertain relation with its canonical conjugate. In this work we use a recent spacetime-symmetric proposal [Phys. Rev. A 95, 032133 (2017)] that tries to solve the unbalance in nonrelativistic quantum mechanics by extending the usual Hilbert space: the time parameter ttt and the position operator $\stackrel{\ifmmode \hat{}\else \^{}\fi{}}{X}$ in one subspace, and the position parameter xxx and time operator T\mathbb{T}T in the other subspace. Time as an operator is better suited for describing tunneling processes. We then solve the 1/21/21/2-fractional integrodifferential equation for a particle subjected to strong and weak potential limits and obtain an analytical expression for the tunneling time through a rectangular barrier. Using a Gaussian energy distribution, we demonstrate that for wave packets well resolved in time, the expectation value of the operator T\mathbb{T}T is the energy average of the classical time ${T}_{\text{class}}=\ensuremath{\partial}S/\ensuremath{\partial}E$, where SSS is the classical action, which can be real or imaginary. The imaginary classical time does not contribute to the traveling time. Furthermore, we apply our results to a Gaussian energy distribution and compare them to previous works. This work is a correction of a previous paper [Phys. Rev. A 107, 052220 (2023)].
A type of mechanics will be presented that possesses some distinctive properties. On the one hand, its physical description & rules of operation are readily comprehensible & intuitively clear. On the other, it fully satisfies all observable predictions of non-relativistic quantum mechanics. Within it, particles exist at points in space, follow continuous, piecewise differentiable paths, and their linear momentum is equal to their mass times their velocity along their path. Yet the probabilities for position and momentum, conditioned on the state of the particle's environment, follow the rules of quantum theory. Indeed, all observable consequences of quantum theory are satisfied; particles can be entangled, have intrinsic spin, this spin is not local to the particle, particle identity can effect probabilities, and so forth. All the rules of quantum mechanics are obeyed, and all arise in a straightforward fashion. After this is established, connections will be drawn out between this type of mechanics and other types of quantum worlds; those that obey Bohmian mechanics, stochastic mechanics, the many worlds interpretation, and physical collapse. In the final section, a relativistic version of the mechanics will be presented.
In quantum theory we refer to the probability of finding a particle between positions xxx and x+dxx+dxx+dx at the instant ttt, although we have no capacity of predicting exactly when the detection occurs. In this work, we first present an extended nonrelativistic quantum formalism where space and time play equivalent roles. It leads to the probability of finding a particle between xxx and x+dxx+dxx+dx during [t,t+dtt,\phantom{\rule{0.16em}{0ex}}t+dtt,t+dt]. Then, we find a Schr\"odinger-like equation for a ``mirror'' wave function $\ensuremath{\phi}(t,x)$ associated with the probability of measuring the system between ttt and t+dtt+dtt+dt, given that detection occurs at xxx. In this framework, it is shown that energy measurements of a stationary state display a nonzero dispersion, and that energy-time uncertainty arises from first principles. We show that a central result on arrival time, obtained through approaches that resort to ad hoc assumptions, is a natural, built-in part of the formalism presented here.
It is well known that nonrelativistic quantum mechanics presents a clear asymmetry between space and time. Much of this asymmetry is attributed to the lack of Lorentz invariance of the theory. Nonetheless, a recent work [Phys. Rev. A \textbf{95}, 032133 (2017)] showed that even though this is partially true, there is a broader physical scenario in which space and time can be handled in nonrelativistic quantum theory in a more symmetric way. In this space-time-symmetric formalism, an additional Hilbert space is defined so that time is raised to the status of operator and position becomes a parameter. As a consequence, the Hilbert space now requires a space-conditional quantum state governed by a new quantum dynamics. In this manuscript, we reveal some physical and mathematical properties of the space-time-symmetric formalism such as: symmetries between the Hamilton-Jacobi and the space-conditional equation; the general solution for a time-independent potential; and a new Lagrangian for a spinless particle in one dimensional. Finally, we present the space-conditional equation for a particle under the effect of an electromagnetic field, and the gauge invariance of this equation is proved.
Time-symmetric relativity theory (TSR) based on Zisman-Stueckelberg-Feynman (ZSF) interpretation includes reference frames going backward in time, maximally expanding their symmetry group to general Lorentz group O(1,3) with 4-inversion (Article 1). Similar time-symmetric (TS) extensions of relativistic quantum mechanics (TS RQM) (Article 2) and QFT (TS QFT) (this article) avoid problems of former RQM and QFT. Former QFT introduced unfounded hypotheses about physical quantum fields in entire space for each type of particle, and these hypotheses led to insoluble problems. TS QFT is limited to known external interaction fields, and describes particles using theory of many-particle systems. In second quantization method, single-particle wave functions and operators, which increase or decrease number of particles in system, form operator amplitudes of transition probabilities. These amplitudes are complex, act in their state spaces for given energy sign, and lead to positive state norm. As in quantum mechanics, they, together with conjugate amplitude, form canonical pair. Canonical formalism in relativity theory is consistent at using Hamilton-Jacobi (HJ) formalism, where 3-momentum and Hamiltonian enter into HJ equation in the same degree. Differential form of relativistic HJ equation is Klein-Gordon (KG) equation, expressing the relationship between energy and momentum, and is general equation for physical components of all operator amplitudes. For bosons, KG equation suffices; for fermions, linearization of HJ equation is required, leading to special first-order equations, such as Dirac equation. Operators of observables are normally ordered, and there are no zero-point fluctuations in ground states. Probability current is determined by 4-momentum and has the same sign; interaction currents are also proportional to probability current and change sign with 4-momentum, which corrects the currents in fermion theory. Introducing interactions into HJ equation leads to new contact terms. Time-symmetric orderings of operator amplitudes lead to causal propagators and usual diagram technique. Taking into account external gravitational field of quanta at Planck length, gravitational radius of the system, and dilation of their proper times in this field lead to gravitational self-regularization of loop diagrams. This makes perturbation theory series in Standard Model (SM) and quantum gravity finite and convergent. Contributions of chiral anomalies are finite and cancel out in SM.