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Journal of Mathematical Physics, Vol. 64, Issue 12 DOI: 10.1063/5.0144924

Considering a Superposition of Classical Reference Frames

Elliott Tammaro Department of Physics, Chestnut Hill College, 9601 Germantown Ave., Philadelphia, 19118, PA, USA    H. Angle Department of Biology, University of Delaware, 210 South College Ave., Newark, 19716, DE, USA    E. Mbadu Department of Computer Science, Drexel University, 3141 Chestnut St., Philadelphia, 19104, PA, USA
(20 December 2023)
Abstract

A ubiquitous feature of quantum mechanical theories is the existence of states of superposition. This is expected to be no different for a quantum gravity theory. Guided by this consideration and others we consider a framework in which classical reference frames may be in superposition relative to one another. Mirroring standard quantum mechanics we introduce a complex-valued wavefunctional, which takes as input the transformations between the coordinates, Ψ[x(x)]\Psi[x(x^{\prime})], with the interpretation that an interaction between the reference frames may select a particular transformation with probability distribution given by the Born rule — P[x(x)]=probability distribution functional|Ψ[x(x)]|2P[x(x^{\prime})]=\text{probability distribution functional}\equiv|\Psi[x(x^{\prime})]|^{2}. The cases of two and three reference frames in superposition are considered explicitly. It is shown that the set of transformations is closed. A rule for transforming wavefunctions from one system to another system in superposition is proposed and consistency with the Schrodinger equation is demonstrated.

preprint: AIP/123-QED

I Introduction

Quantum theories, by virtue of their linearity, include states of superposition. Superpositions are states that consist of a sum over (typically classically distinct) states, such as position, momentum, energy, et cetera. It is expected that a quantum gravity theory must also include superpositions. In the case of a quantum gravity theory that resembles classical general relativity so that the gravitational field remains a manifestation of spacetime curvature, states corresponding to superpositions of spacetime metrics must be considered. Interpreting the meaning of such states, which is an end goal, is an open question, which likely cannot be resolved without recourse to a particular quantum gravity theory Foo, Mann, and Zych (2021); Jensen (2011); Giacomini and Brukner (2022, 2020); Christodoulou and Rovelli (2019); Anastopoulos and Hu (2020); Rovelli (1991); Wu and Zhang (2006); Crowther (2018). This present work considers a superposition of otherwise classical reference frames. The hope of gaining insight into the notion of a superposition of spacetimes or spacetime metrics by first considering a superposition of reference frames on a background spacetime should be apparent.

The concept and treatment of a superposition of reference frames, both in connection to a quantum gravity theory, and for other purposes, is well-motivated and has been explored in numerous contexts Aharonov and Kaufherr (1984a); Aharonov and Susskind (1967); Bartlett, Rudolph, and Spekkens (2007); Palmer, Girelli, and Bartlett (2014a); Giacomini, Castro-Ruiz, and Brukner (2019); Belenchia et al. (2018); de la Hamette and Galley (2020); Vanrietvelde et al. (2020); Palmer, Girelli, and Bartlett (2014b); Streiter, Giacomini, and Brukner (2021); Greenberger (2001); Mikusch, Barbado, and Brukner (2021); Ballesteros, Giacomini, and Gubitosi (2021); Aharonov and Kaufherr (1984b); Angelo et al. (2011); Angelo and Ribeiro (2012); Pienaar (2016); Smith, Piani, and Mann (2016). In quantum mechanics, as is familiar from classical mechanics, a system under investigation is described from an inertial reference frame. The reference frame is itself an extended system, which permits study of the investigated system from its platform. The reference frame has often been treated as a large (perhaps lab-sized) system, and accordingly, is strictly classical. However, the size of systems that exhibit quantum behavior has been steadily growing with the improvement of experimental technique. It is prudent to inquire about the possibility for a system under investigation to serve as a frame of reference in its own right. A treatment of the problem of a quantum observer making observations of an observer has also been considered in several approaches, including notably Everett’s relative state interpretation and relational quantum mechanics Everett III (1957); Rovelli (1996, 2005). This reasoning motivates the incorporation of the observer as part of the quantum system and therefore describes the system from a single Hilbert space. A complementary approach, like the one pursued here, seeks a transformation rule between coexisting Hilbert spaces. As will be apparent, this more closely mirrors the state of affairs classically where frames of reference do not play a dynamical role in the theory. In classical theories there exist transformation rules between reference frames for coordinate-dependent quantities and in this approach there is a similar construct. It is also more desirable for the purpose of comparing results in this present work, and in future related work, to the diffeomorphism invariance of General Relativity. To this end, we work in position space.

In section II the case of two reference frames in superposition relative to one another is considered. A complex-valued wavefunctional defined on the set of coordinate transformations between the two reference frames, Ψ[x(x)]\Psi[x(x^{\prime})], is introduced. An example of a superposition of two rotations is considered. In section III a third reference frame is introduced. The closure of coordinate system transformations is extended to reference frames in superposition. The case of a superposition of two rotations is again used as an example. In section IV a rule for using the wavefunctional to transform wavefunctions is posited and consistency with the Schrodinger equation is demonstrated.

II Two Classical Reference Frames in Superposition

Let O and O’ be two frames of reference. Classically, each frame has a set of coordinates (measuring rods) for establishing positions and clocks for recording times. The coordinates will be denoted in the usual way xα=(x,y,z,t)x_{\alpha}=(x,y,z,t) and xβ=(x,y,z,t)x^{\prime}_{\beta}=(x^{\prime},y^{\prime},z^{\prime},t^{\prime}). Greek letter indices will run from 1 to 4, while Roman letter indices will run from 1 to 3. Unless otherwise stated, summation notation is in use. When there is no risk of confusion indices may not be written explicitly. There is a transformation between the OO and OO^{\prime} frames such that xα=xα(x)x_{\alpha}=x_{\alpha}(x^{\prime}). The transformation must, of course, be invertible so that xβ=xβ(x)x^{\prime}_{\beta}=x^{\prime}_{\beta}(x).

We wish to consider that these two reference frames are in superposition with respect to one another. What should this mean? A system is in a superposition of “classical states” (states with well-defined properties such as position, momentum, energy, et cetera) when a wavefunction is introduced, which assigns a complex number (amplitude) to a set of classical states. For example, a particle is in a superposition of two classical position states, 𝐱0\mathbf{x}_{0} and 𝐱1\mathbf{x}_{1}, when its wavefunction, ψ\psi, is such that

ψδ(𝐱𝐱0)+δ(𝐱𝐱1).\psi\propto\delta(\mathbf{x}-\mathbf{x}_{0})+\delta(\mathbf{x}-\mathbf{x}_{1}). (1)

To mirror this notion of superposition while extending it to include superposed reference frames, the transformation between the reference frames should not be fixed, but instead replaced with a complex-valued function(al) on the space of transformations. We introduce just such an amplitude ΨOO\Psi_{OO^{\prime}} and allow

ΨOO=ΨOO[xα(x)].\Psi_{OO^{\prime}}=\Psi_{OO^{\prime}}\left[x_{\alpha}(x^{\prime})\right]. (2)

Equation 2 is defined on the “forward" transformations x(x)x(x^{\prime}) (we ignore coordinate indices here for clarity). As will be demonstrated it will take quantities from frame OO^{\prime} to OO. We expect that there should be a wavefunctional defined on the “reverse" transformation x(x)x^{\prime}(x) taking quantities from OO to OO^{\prime}. That is, there must be a wavefunctional ΨOO[xα(x)]\Psi_{O^{\prime}O}\left[x^{\prime}_{\alpha}(x)\right], which is “inverse" to Ψ[xα(x)]\Psi[x_{\alpha}(x)]. The precise sense in which these two wavefunctional can be said to be inverse to one another will be made clear in the next section.

This wavefunctional is, by its nature, a relational quantity. We cannot speak of a reference frame in superposition in any absolute sense. We may only state that a reference frame is in superposition relative to another frame. We give a physical interpretation that again mirrors the case of standard quantum mechanics. Two reference frames are in superposition when the the transformation rule between them is completely described by a wavefunctional on the space of transformations ΨOO[xα(x)]\Psi_{OO^{\prime}}[x_{\alpha}(x^{\prime})]. If the reference frames were to interact so as to ascertain a specific transformation then the physical interaction would drive the wavefunctional toward a delta functional, which selects one particular transformation. That is to say that if two reference frames were in superposition then a mutual interaction, or coupling, would, in the phrasing of standard quantum mechanics, collapse the superposition. There is an issue with this if the wavefunctional is to be seen as a functional of xα(x)x_{\alpha}(x^{\prime}), because xα(x)x_{\alpha}(x^{\prime}) contains time as a coordinate and includes the time component of the transformation. If the interaction that led to collapse-like behavior occurred at a time t1t_{1} then the transformation function would supposedly be known for all time. If the coordinate systems are, however, again isolated then it is expected that they, by some dynamics, may again evolve to be superposition. This is inconsistent with the claim that the transformation was established at time t1t_{1} and remains valid for all times. We remedy this situation in this present work by considering superpositions of time-independent transformations. Then we have,

ΨOO[xα(xβ)]ΨOO[xi(xj)],\Psi_{OO^{\prime}}\left[x_{\alpha}(x^{\prime}_{\beta})\right]\xrightarrow[]{}\Psi_{OO^{\prime}}\left[x_{i}(x^{\prime}_{j})\right], (3)

where again Roman indices are restricted to 1,2,and 31,2,\text{and }3.

ΨOO[xi(xj)]interactionδ[xi(xj)xi0(xj)].\Psi_{OO^{\prime}}[x_{i}(x^{\prime}_{j})]\xrightarrow[]{interaction}\delta[x_{i}(x^{\prime}_{j})-x^{0}_{i}(x^{\prime}_{j})]. (4)

The probability density for the interaction to select xi(xj)x_{i}(x^{\prime}_{j}) is, in accord with the Born rule,

𝒫[xi(x)]=ΨOO[xi(xj)]ΨOO[xi(xj)].\mathcal{P}\left[x_{i}(x^{\prime})\right]=\Psi^{*}_{OO^{\prime}}\left[x_{i}(x^{\prime}_{j})\right]\Psi_{OO^{\prime}}\left[x_{i}(x^{\prime}_{j})\right]. (5)

The path integral of 𝒫[xi(x)]\mathcal{P}\left[x_{i}(x^{\prime})\right] over a subset SS of all possible transformations xi(x)x_{i}(x^{\prime}) would give the probability of the transformation, upon interaction, to be an element of SS, in accord with the Born rule Feynman, Hibbs, and Styer (2010). That is,

S𝒟x1(x)𝒟x2(x)𝒟x3(x)𝒫[xi(x)]=\displaystyle\int_{S}\mathcal{D}x_{1}(x^{\prime})\mathcal{D}x_{2}(x^{\prime})\mathcal{D}x_{3}(x^{\prime})\mathcal{P}[x_{i}(x^{\prime})]=
Probability O and O′′are related by a transformation in S.\displaystyle\text{Probability }O\text{ and }O^{\prime\prime}\text{are related by a transformation in }S.

For clarity it is worthwhile to consider an explicit example. For simplicity assume the transformations between reference frames OO and OO^{\prime} are restricted to rotations, so that

xi(xj)=Rijxj.x_{i}(x^{\prime}_{j})=R_{ij}x^{\prime j}. (6)

Upon substituting equation 6 into equation 2, ΨOO[Rijxj]=ΨOO(Rij)\Psi_{OO^{\prime}}\left[R_{ij}x^{\prime}_{j}\right]=\Psi_{OO^{\prime}}\left(R_{ij}\right). The wavefunctional is reduced to a function of the parameters of the rotation matrix RijR_{ij}. In analogy to the state defined in 1, consider a superposition of two possible rotations Rij(+θ,𝕟^)R_{ij}(+\theta,\mathbb{\hat{n}}) and Rij(θ,𝕟^)R_{ij}(-\theta,\mathbb{\hat{n}})

ΨOO[x(x)]=δ(RijRij(+θ,𝐧^))+δ(RijRij(θ,𝐧^)).\Psi_{OO^{\prime}}[x(x^{\prime})]=\delta\left(R_{ij}-R_{ij}(+\theta,\mathbf{\hat{n}})\right)+\delta\left(R_{ij}-R_{ij}(-\theta,\mathbf{\hat{n}})\right). (7)

Where delta functions of rotation matrices vanish unless the argument vanishes, thereby enforcing Rij=Rij(+θ,𝕟^)R_{ij}=R_{ij}(+\theta,\mathbb{\hat{n}}) or Rij=Rij(θ,𝕟^)R_{ij}=R_{ij}(-\theta,\mathbb{\hat{n}}). Note that normalization of the state is ignored here for elegance. Upon interaction between the reference frames the transformation between them will be xi=Rij(+θ,𝕟^)xjx_{i}=R_{ij}(+\theta,\mathbb{\hat{n}})x^{\prime}_{j} with 50% probability and will be Rij(θ,𝕟^)xjR_{ij}(-\theta,\mathbb{\hat{n}})x^{\prime}_{j} the remainder. This example will be further explored in the next section.

III Three Observers in Superposition

When a third reference frame, O′′O^{\prime\prime}, is introduced and the transformation from OO to OO^{\prime} as well as the transformation from OO^{\prime} to O′′O^{\prime\prime} is specified, then the transformation from OO to O′′O^{\prime\prime} is fixed by the action of composition. If x(x)x^{\prime}(x) takes coordinates from OO to OO^{\prime} and x′′(x)x^{\prime\prime}(x^{\prime}) takes coordinates from OO^{\prime} to O′′O^{\prime\prime}, then the composition x′′(x(x))x^{\prime\prime}(x^{\prime}(x)) takes coordinates from OO to O′′O^{\prime\prime}. It is expected that if OO and OO^{\prime} are in superposition, and the wavefunctional ΨOO[x(x)]\Psi_{OO^{\prime}}[x(x^{\prime})] is known, and that OO^{\prime} and O′′O^{\prime\prime} are also in superposition with a known wavefunctional ΨOO′′[x(x′′)]\Psi_{O^{\prime}O^{\prime\prime}}[x^{\prime}(x^{\prime\prime})], then OO and O′′O^{\prime\prime} are also in superposition and that the wavefunctional ΨOO′′[x(x′′)]\Psi_{OO^{\prime\prime}}[x(x^{\prime\prime})] may be calculated from ΨOO[x(x)]\Psi_{OO^{\prime}}[x(x^{\prime})] and ΨOO′′[x(x′′)]\Psi_{O^{\prime}O^{\prime\prime}}[x^{\prime}(x^{\prime\prime})]. That is to say, there must be a rule for composing transformations when the systems are in mutual superposition. We do not seek a derivation from first principles but instead, as will be demonstrated, there seems to be only one natural choice.

Imagine that both ΨOO[x(x)]\Psi_{OO^{\prime}}[x(x^{\prime})] and ΨOO′′[x(x′′)]\Psi_{O^{\prime}O^{\prime\prime}}[x^{\prime}(x^{\prime\prime})] are proportional to delta functionals that enforce particular transformations between OO and OO^{\prime} and OO^{\prime} and O′′O^{\prime\prime}. That is,

ΨOO[x(x)]\displaystyle\Psi_{OO^{\prime}}[x(x^{\prime})] =\displaystyle= δ[x(x)x0(x)]\displaystyle\delta\left[x(x^{\prime})-x_{0}(x^{\prime})\right] (8)
ΨOO′′[x(x′′)]\displaystyle\Psi_{O^{\prime}O^{\prime\prime}}[x^{\prime}(x^{\prime\prime})] =\displaystyle= δ[x(x′′)x0(x′′)]\displaystyle\delta\left[x^{\prime}(x^{\prime\prime})-x^{\prime}_{0}(x^{\prime\prime})\right] (9)

The delta functionals enforce x(x)=x0(x)x(x^{\prime})=x_{0}(x^{\prime}) and x(x′′)=x0(x′′)x^{\prime}(x^{\prime\prime})=x^{\prime}_{0}(x^{\prime\prime}), where x0(x)x_{0}(x^{\prime}) and x0(x′′)x^{\prime}_{0}(x^{\prime\prime}), are particular transformation functions. Note that the indices for the coordinates have been suppressed. These wavefunctionals do not represent a superposition. The transformations are fixed, and thus the transformation from OO to O′′O^{\prime\prime} is also fixed. Namely, the transformation from OO to O′′O^{\prime\prime} is formed from composition: x(x′′)=x(x(x′′))=x0(x0(x′′))x(x^{\prime\prime})=x(x^{\prime}(x^{\prime\prime}))=x_{0}(x^{\prime}_{0}(x^{\prime\prime})). As a result it must be that

ΨOO′′[x(x′′)]=δ[x(x′′)x0(x0(x′′))]\Psi_{OO^{\prime\prime}}[x(x^{\prime\prime})]=\delta\left[x(x^{\prime\prime})-x_{0}(x^{\prime}_{0}(x^{\prime\prime}))\right] (10)

Equation 10 enforces the known transformation from OO to O′′O^{\prime\prime}. There is seemingly only one way that equation 10 can be expressed in terms of equations 8 and 9. Multiply equations 8 and 9. The product is

δ[x(x)x0(x)]δ[x(x′′)x0(x′′)].\delta\left[x(x^{\prime})-x_{0}(x^{\prime})\right]\delta\left[x^{\prime}(x^{\prime\prime})-x^{\prime}_{0}(x^{\prime\prime})\right]. (11)

This defines a functional of both x(x)x(x^{\prime}) and x(x′′)x^{\prime}(x^{\prime\prime}). It should not be worrisome to see the coordinates xx^{\prime} treated as both independent and dependent quantities in the same expression since equation 11 being a functional expression depends only on the distinct functions x(x)x(x^{\prime}) and x(x′′)x^{\prime}(x^{\prime\prime}), while making the physical operation clearer.

We need to construct a functional of a single function x(x′′)x(x^{\prime\prime}). To do so, functionally integrate equation 11 over x(x)x(x^{\prime}) and x(x′′)x^{\prime}(x^{\prime\prime}) with the restriction that x(x(x′′))=x(x′′)x(x^{\prime}(x^{\prime\prime}))=x(x^{\prime\prime}). That is, compute

𝒮x(x′′)Dx(x)Dx(x′′)ΨOO[x(x)]ΨOO′′[x(x′′)],\iint_{\mathcal{S}_{x(x^{\prime\prime})}}Dx(x^{\prime})Dx^{\prime}(x^{\prime\prime})\Psi_{OO^{\prime}}[x(x^{\prime})]\Psi_{O^{\prime}O^{\prime\prime}}[x^{\prime}(x^{\prime\prime})], (12)

where 𝒮x(x′′)\mathcal{S}_{x(x^{\prime\prime})} is the set of paired functions (x(x),x(x′′))\left(x(x^{\prime}),x^{\prime}(x^{\prime\prime})\right), such that the composition of x(x)x(x^{\prime}) and x(x′′)x^{\prime}(x^{\prime\prime}) yields x(x′′)x(x^{\prime\prime}), that is so that x(x(x′′))=x(x′′)x(x^{\prime}(x^{\prime\prime}))=x(x^{\prime\prime}). i.e.

𝒮x(x′′)={(x(x),x(x′′))|x(x(x′′))=x(x′′)}.\mathcal{S}_{x(x^{\prime\prime})}=\{\left(x(x^{\prime}),x^{\prime}(x^{\prime\prime})\right)|x(x^{\prime}(x^{\prime\prime}))=x(x^{\prime\prime})\}. (13)

The restricted path integral in equation 12 yields a functional of a single function x(x′′)x(x^{\prime\prime}), as a valid transformation composition rule must do.

Expression 12 for wavefunctionals 8 and 9 is

Sx(x′′)Dx(x)Dx(x′′)δ[x(x)x0(x)]δ[x(x′′)x0(x′′)].\iint_{S_{x(x^{\prime\prime})}}Dx(x^{\prime})Dx^{\prime}(x^{\prime\prime})\delta\left[x(x^{\prime})-x_{0}(x^{\prime})\right]\delta\left[x^{\prime}(x^{\prime\prime})-x^{\prime}_{0}(x^{\prime\prime})\right]. (14)

Evaluating functional integrals is generally very difficult. Here we will argue for the result of the integral, and in appendix A a more detailed discussion and conjecture is provided. We claim that equation 14 evaluates to

δ[x(x′′)x0(x0(x′′))],\delta[x(x^{\prime\prime})-x_{0}(x^{\prime}_{0}(x^{\prime\prime}))], (15)

which it must if it is to reproduce our expectation. Equation 14 consists of an integral over Sx(x′′)S_{x(x^{\prime\prime})}. The integral sums over a range of functions x(x)x(x^{\prime}) and x(x′′)x^{\prime}(x^{\prime\prime}). Without restricting the integral to Sx(x′′)S_{x(x^{\prime\prime})}, there would be no consistent function x(x′′)x(x^{\prime\prime}) formed by the composition x(x(x′′))x(x^{\prime}(x^{\prime\prime}))). Thus, this restriction ensures that the function x(x′′)x(x^{\prime\prime}) is well-defined and that 14 may be regarded as a functional of x(x′′)x(x^{\prime\prime}). The integrand in equation 14 consists of a product of delta functionals. The first delta functional, and therefore the whole expression, will vanish if x(x)x0(x)x(x^{\prime})\neq x_{0}(x^{\prime}). The second functional, and therefore the expression, will vanish if x(x′′)x0(x0(x′′))x^{\prime}(x^{\prime\prime})\neq x_{0}(x^{\prime}_{0}(x^{\prime\prime})). We conclude that expression 14 will vanish unless x(x′′)=x0(x0(x′′))x(x^{\prime\prime})=x_{0}(x^{\prime}_{0}(x^{\prime\prime})). Now consider

Dx(x′′)(Sx(x′′)Dx(x)Dx(x′′)δ[x(x)x0(x)]δ[x(x′′)x0(x′′)]).\int Dx(x^{\prime\prime})\left(\iint_{S_{x(x^{\prime\prime})}}Dx(x^{\prime})Dx^{\prime}(x^{\prime\prime})\delta\left[x(x^{\prime})-x_{0}(x^{\prime})\right]\delta\left[x^{\prime}(x^{\prime\prime})-x^{\prime}_{0}(x^{\prime\prime})\right]\right). (16)

The double integrals inside the parenthesis are restricted to set Sx(x′′)S_{x(x^{\prime\prime})}, while the exterior integral integrates over the restriction. Together, the whole function space is integrated over, and the result is unity. Sx(x′′)Dx(x)Dx(x′′)δ[x(x)x0(x)]δ[x(x′′)x0(x′′)]\iint_{S_{x(x^{\prime\prime})}}Dx(x^{\prime})Dx^{\prime}(x^{\prime\prime})\delta\left[x(x^{\prime})-x_{0}(x^{\prime})\right]\delta\left[x^{\prime}(x^{\prime\prime})-x^{\prime}_{0}(x^{\prime\prime})\right] vanishes if x(x′′)x0(x0(x′′))x(x^{\prime\prime})\neq x_{0}(x^{\prime}_{0}(x^{\prime\prime})) and gives unity when integrated with respect to x(x′′)x(x^{\prime\prime}). These are the two defining properties of a delta functional in x(x′′)x(x^{\prime\prime}), which is the claim.

For delta functional wavefunctionals equation 12 evaluates to equation 15, which is the expected form of the wavefunctional since it enforces the same transformation as equation 10. We generalize from this result and posit that the composition rule for wavefunctionals is as follows—

ΨOO′′[x(x′′)]=Sx(x′′)Dx(x)Dx(x′′)ΨOO[x(x)]ΨOO′′[x(x′′)].\Psi_{OO^{\prime\prime}}[x(x^{\prime\prime})]=\iint_{S_{x(x^{\prime\prime})}}Dx(x^{\prime})Dx^{\prime}(x^{\prime\prime})\Psi_{OO^{\prime}}[x(x^{\prime})]\Psi_{O^{\prime}O^{\prime\prime}}[x^{\prime}(x^{\prime\prime})]. (17)

To see how equation 17 works in the case of a superposition it is worthwhile to return to the case of two rotations in superposition begun in Section II. Take ΨOO\Psi_{OO^{\prime}} to be

ΨOO(Rij)=AOOδ(RijRij(+θ,𝕟^))+BOOδ(RijRij(θ,𝕟^)).\Psi_{OO^{\prime}}(R_{ij})=A_{OO^{\prime}}\delta\left(R_{ij}-R_{ij}(+\theta,\mathbb{\hat{n}})\right)+B_{OO^{\prime}}\delta\left(R_{ij}-R_{ij}(-\theta,\mathbb{\hat{n}})\right). (18)

Where AOOA_{OO^{\prime}} and BOOB_{OO^{\prime}} are (possibly complex) coefficients. Similarly, take ΨOO′′\Psi_{O^{\prime}O^{\prime\prime}} to be

ΨOO′′(Rij)=AOO′′δ(RijRij(+γ,𝕟^))+BOO′′δ(RijRij(γ,𝕟^)).\Psi_{O^{\prime}O^{\prime\prime}}(R^{\prime}_{ij})=A_{O^{\prime}O^{\prime\prime}}\delta\left(R^{\prime}_{ij}-R_{ij}(+\gamma,\mathbb{\hat{n^{\prime}}})\right)+B_{O^{\prime}O^{\prime\prime}}\delta\left(R^{\prime}_{ij}-R_{ij}(-\gamma,\mathbb{\hat{n^{\prime}}})\right). (19)

The two terms in equation 18 indicate that there are two possible transformations in superposition, x=R(+θ,𝕟^)xx=R(+\theta,\mathbb{\hat{n}})x^{\prime} or x=R(θ,𝕟^)xx=R(-\theta,\mathbb{\hat{n}})x^{\prime}. Likewise from equation 19 there are also two transformations, x=R(+γ,𝕟^)x′′x^{\prime}=R(+\gamma,\mathbb{\hat{n^{\prime}}})x^{\prime\prime} or x=R(γ,𝕟^)x′′x^{\prime}=R(-\gamma,\mathbb{\hat{n^{\prime}}})x^{\prime\prime}. As a result, there are four transformations between xx and x′′x^{\prime\prime} that are in superposition. They are, x=R(+θ,𝕟^)R(+γ,𝕟^)x′′x=R(+\theta,\mathbb{\hat{n}})R(+\gamma,\mathbb{\hat{n^{\prime}}})x^{\prime\prime}, x=R(+θ,𝕟^)R(γ,𝕟^)x′′x=R(+\theta,\mathbb{\hat{n}})R(-\gamma,\mathbb{\hat{n^{\prime}}})x^{\prime\prime}, x=R(θ,𝕟^)R(+γ,𝕟^)x′′x=R(-\theta,\mathbb{\hat{n}})R(+\gamma,\mathbb{\hat{n^{\prime}}})x^{\prime\prime}, or x=R(θ,𝕟^)R(γ,𝕟^)x′′x=R(-\theta,\mathbb{\hat{n}})R(-\gamma,\mathbb{\hat{n^{\prime}}})x^{\prime\prime}. That is, ΨOO′′\Psi_{OO^{\prime\prime}} should have four delta function terms enforcing the transformations. Explicitly,

ΨOO′′(Rij′′)=Cδ(Rij′′Rim(+θ,𝕟^)Rmj(+γ,𝕟^))\displaystyle\Psi_{OO^{\prime\prime}}(R^{\prime\prime}_{ij})=C\delta\left(R^{\prime\prime}_{ij}-R_{im}(+\theta,\mathbb{\hat{n}})R_{mj}(+\gamma,\mathbb{\hat{n^{\prime}}})\right)
+Dδ(Rij′′Rim(+θ,𝕟^)Rmj(γ,𝕟^))\displaystyle+D\delta\left(R^{\prime\prime}_{ij}-R_{im}(+\theta,\mathbb{\hat{n}})R_{mj}(-\gamma,\mathbb{\hat{n^{\prime}}})\right)
+Eδ(Rij′′Rim(θ,𝕟^)Rmj(+γ,𝕟^))\displaystyle+E\delta\left(R^{\prime\prime}_{ij}-R_{im}(-\theta,\mathbb{\hat{n}})R_{mj}(+\gamma,\mathbb{\hat{n^{\prime}}})\right)
+Fδ(Rij′′Rim(θ,𝕟^)Rmj(γ,𝕟^)).\displaystyle+F\delta\left(R^{\prime\prime}_{ij}-R_{im}(-\theta,\mathbb{\hat{n}})R_{mj}(-\gamma,\mathbb{\hat{n^{\prime}}})\right). (20)

Now apply equation 17. The product of ΨOO\Psi_{OO^{\prime}} and ΨOO′′\Psi_{O^{\prime}O^{\prime\prime}} is

ΨOOΨOO′′=\displaystyle\Psi_{OO^{\prime}}\Psi_{O^{\prime}O^{\prime\prime}}= (21)
AOOAOO′′δ(RijRij(+θ,𝕟^))δ(RijRij(+γ,𝕟^))+AOOBOO′′δ(RijRij(+θ,𝕟^))δ(RijRij(γ,𝕟^))\displaystyle A_{OO^{\prime}}A_{O^{\prime}O^{\prime\prime}}\delta\left(R_{ij}-R_{ij}(+\theta,\mathbb{\hat{n}})\right)\delta\left(R^{\prime}_{ij}-R_{ij}(+\gamma,\mathbb{\hat{n^{\prime}}})\right)+A_{OO^{\prime}}B_{O^{\prime}O^{\prime\prime}}\delta\left(R_{ij}-R_{ij}(+\theta,\mathbb{\hat{n}})\right)\delta\left(R^{\prime}_{ij}-R_{ij}(-\gamma,\mathbb{\hat{n^{\prime}}})\right)
+\displaystyle+ BOOAOO′′δ(RijRij(θ,𝕟^))δ(RijRij(+γ,𝕟^))+BOOBOO′′δ(RijRij(θ,𝕟^))δ(RijRij(γ,𝕟^)).\displaystyle B_{OO^{\prime}}A_{O^{\prime}O^{\prime\prime}}\delta\left(R_{ij}-R_{ij}(-\theta,\mathbb{\hat{n}})\right)\delta\left(R^{\prime}_{ij}-R_{ij}(+\gamma,\mathbb{\hat{n^{\prime}}})\right)+B_{OO^{\prime}}B_{O^{\prime}O^{\prime\prime}}\delta\left(R_{ij}-R_{ij}(-\theta,\mathbb{\hat{n}})\right)\delta\left(R^{\prime}_{ij}-R_{ij}(-\gamma,\mathbb{\hat{n^{\prime}}})\right).

Following equation 17 we integrate equation ΨOOΨOO′′\Psi_{OO^{\prime}}\Psi_{O^{\prime}O^{\prime\prime}} over all functions x(x)x(x^{\prime}) and x(x′′)x^{\prime}(x^{\prime\prime}), such that their composition x(x(x′′))x(x^{\prime}(x^{\prime\prime})) is x(x′′)x(x^{\prime\prime}). The transformations are restricted to be rotations only and thus the path integrals become integrals with respect to RijR_{ij} and RijR^{\prime}_{ij}. The restriction that x(x(x′′))x(x^{\prime}(x^{\prime\prime})) must equal x(x′′)x(x^{\prime\prime}) becomes Rij′′=RimRmjR^{\prime\prime}_{ij}=R_{im}R^{\prime}_{mj}, where Rij′′R^{\prime\prime}_{ij} will represent the transformation from OO to O′′O^{\prime\prime} so that xi=Rim′′xm′′x_{i}=R^{\prime\prime}_{im}x^{\prime\prime}_{m} if there was no superposition. The four terms of equation 21 are similar so it is sufficient to consider just one. The integral of the first term in equation 21 becomes

AOOAOO′′S𝑑Rij𝑑Rqr\displaystyle A_{OO^{\prime}}A_{O^{\prime}O^{\prime\prime}}\iint_{S}dR_{ij}dR^{\prime}_{qr} δ(RijRij(+θ,𝕟^))δ(RijRij(+γ,𝕟^))=AOOAOO′′δ(Rij′′Rim(+θ,𝕟^)Rmj(+γ,𝕟^)).\displaystyle\delta\left(R_{ij}-R_{ij}(+\theta,\mathbb{\hat{n}})\right)\delta\left(R^{\prime}_{ij}-R_{ij}(+\gamma,\mathbb{\hat{n^{\prime}}})\right)=A_{OO^{\prime}}A_{O^{\prime}O^{\prime\prime}}\delta\left(R^{\prime\prime}_{ij}-R_{im}(+\theta,\mathbb{\hat{n}})R_{mj}(+\gamma,\mathbb{\hat{n^{\prime}}})\right).

The three remaining terms are similar. The result is

ΨOO′′(Rij′′)=AOOAOO′′δ(Rij′′Rim(+θ,𝕟^)Rmj(+γ,𝕟^))+AOOBOO′′δ(Rij′′Rim(+θ,𝕟^)Rmj(γ,𝕟^))+BOOAOO′′δ(Rij′′Rim(θ,𝕟^)Rmj(+γ,𝕟^))+BOOBOO′′δ(Rij′′Rim(θ,𝕟^)Rmj(γ,𝕟^)).\Psi_{OO^{\prime\prime}}(R^{\prime\prime}_{ij})=\\ A_{OO^{\prime}}A_{O^{\prime}O^{\prime\prime}}\delta\left(R^{\prime\prime}_{ij}-R_{im}(+\theta,\mathbb{\hat{n}})R_{mj}(+\gamma,\mathbb{\hat{n^{\prime}}})\right)\\ +A_{OO^{\prime}}B_{O^{\prime}O^{\prime\prime}}\delta\left(R^{\prime\prime}_{ij}-R_{im}(+\theta,\mathbb{\hat{n}})R_{mj}(-\gamma,\mathbb{\hat{n^{\prime}}})\right)\\ +B_{OO^{\prime}}A_{O^{\prime}O^{\prime\prime}}\delta\left(R^{\prime\prime}_{ij}-R_{im}(-\theta,\mathbb{\hat{n}})R_{mj}(+\gamma,\mathbb{\hat{n^{\prime}}})\right)\\ +B_{OO^{\prime}}B_{O^{\prime}O^{\prime\prime}}\delta\left(R^{\prime\prime}_{ij}-R_{im}(-\theta,\mathbb{\hat{n}})R_{mj}(-\gamma,\mathbb{\hat{n^{\prime}}})\right). (22)

Comparing equation 22 with equation 20 it is easy to see that the coefficients C,D,E,and FC,D,E,\text{and }F are the products AOOAOO′′A_{OO^{\prime}}A_{O^{\prime}O^{\prime\prime}}, AOOBOO′′A_{OO^{\prime}}B_{O^{\prime}O^{\prime\prime}}, BOOAOO′′B_{OO^{\prime}}A_{O^{\prime}O^{\prime\prime}}, and BOOBOO′′B_{OO^{\prime}}B_{O^{\prime}O^{\prime\prime}}, respectively.

Equation 17 ensures that the composition of any number of wavefunctionals is also a wavefunctional, so that there is closure. Now also consider transforming from the OO frame to the OO^{\prime} frame followed by a transformation from the OO^{\prime} frame to the OO frame. The total transformation must be the identity transformation, so that x(x′′)=1x(x^{\prime\prime})=1, and the wavefunctionals must satisfy an identity. Using equation 17 we have

1=S1Dx(x)Dx(x′′)ΨOO[x(x)]ΨOO[(x(x′′))],1=\iint_{S_{1}}Dx(x^{\prime})Dx^{\prime}(x^{\prime\prime})\Psi_{OO^{\prime}}[x(x^{\prime})]\Psi_{O^{\prime}O}[(x^{\prime}(x^{\prime\prime}))], (23)

where S1S_{1}, not to be confused with the unit circle, is the set of transformation functions that compose to give the identity. That is to say, the integral is restricted to a set of functions x(x)x(x^{\prime}) and x(x′′)x^{\prime}(x^{\prime\prime}) such that x(x(x′′))=1x(x^{\prime}(x^{\prime\prime}))=1. Equation 23 makes precise the notion of an inverse wavefunctional. The similarity between equations 17 and 23 and matrix multiplication and matrix inverses should be apparent.

IV Consistency with the Schrödinger equation

The Schrödinger equation is invariant under rigid Euclidean motions (rotations and translations). Let us prove that the Schrödinger equation is invariant under any transformation to a superposition of rotated or translated frames. That is, the present formalism is consistent with Schrödinger equation. Assume that relative to a frame OO there is a system that is studied, which has a wavefunction ψ(x,t)\psi(x,t). Now consider a second frame OO^{\prime} in superposition relative OO. There is a wavefunctional Ψ[x(x)]\Psi[x(x^{\prime})] which governs the transformation between the two superposed frames. How are we to transform the known wavefunction ψ(x,t)\psi(x,t) in the OO frame to the wavefunction that would be associated to it in the OO^{\prime} frame? We hypothesize the following transformation rule:

ψ(x,t)=S𝒟x(x)Ψ[x(x)]ψ(x(x),t).\psi^{\prime}(x^{\prime},t)=\int_{S}\mathcal{D}x(x^{\prime})\Psi[x(x^{\prime})]\psi(x(x^{\prime}),t). (24)

where SS is the set of functions x(x)x(x^{\prime}). The transformation in equation 24 is natural. There are only a few distinct rules that can transform a function ψ(x,t)\psi(x,t) to a function of variables xx^{\prime}, and it ensures that if the system described by ψ(x,t)\psi(x,t) happened to be in position eigenstate relative to OO then OO^{\prime}, assumed to be in a superposition relative to OO, would associate a wavefunction ψ(x,t)\psi^{\prime}(x,t) to the system that corresponds to a superposition. This is ensured because eq. 24 obviously superposes ψ(x(x),t)\psi(x(x^{\prime}),t) for each function x(x)x(x^{\prime}) for which Ψ[x(x)]\Psi[x(x^{\prime})] does not vanish. We can extend equation 24 to wavefunctions of multi-particle systems as follows. Let ψ(x1,x2,,xn,t)\psi(x_{1},x_{2},...,x_{n},t) be the wavefunction of a multi-particle system in the OO frame. A generic transformation from the frame OO^{\prime} to OO will consist of map X:OOX:O\rightarrow O^{\prime} that takes as input the coordinates in OO^{\prime} and outputs the coordinates in OO. Let x1x^{\prime}_{1} map to x1x_{1} under XX, and let x2x^{\prime}_{2} map to x2x_{2}, and so on. Then the multi-particle extension of equation 24 takes the form —

ψ\displaystyle\psi (x1,x2,,xn,t)={}^{\prime}(x^{\prime}_{1},x^{\prime}_{2},...,x^{\prime}_{n},t)= (25)
S\displaystyle\int_{S} 𝒟X(x)Ψ[X(x)]ψ(X(x1),X(x2),,X(xn),t).\displaystyle\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]\psi(X(x^{\prime}_{1}),X(x^{\prime}_{2}),...,X(x^{\prime}_{n}),t).

Note that the wavefunctional, Ψ\Psi, and the path integral measure, 𝒟X\mathcal{D}X depend only on the form of the function XX and not on the value of the XX for any particular input xx^{\prime}, despite writing Ψ[X(x)]\Psi[X(x^{\prime})] and 𝒟X(x)\mathcal{D}X(x^{\prime}) in equation 25.

Using equations 24 and 25, we can now transform derivatives as well, such as ψ(x,t)xi\frac{\partial\psi^{\prime}(x^{\prime},t)}{\partial x^{{}^{\prime}i}}. Take the derivative of eq. 24 with respect to xix^{{}^{\prime}i}

ψ(x,t)xi=S𝒟x(x)Ψ[x(x)]ψ(x,t)xjxjxi.\frac{\partial\psi^{\prime}(x^{\prime},t)}{\partial x^{{}^{\prime}i}}=\int_{S}\mathcal{D}x(x^{\prime})\Psi[x(x^{\prime})]\frac{\partial\psi(x,t)}{\partial x^{j}}\frac{\partial x^{j}}{\partial x^{{}^{\prime}i}}. (26)

To extend equation 26 to multiple particles we adopt the following notation, xIix_{I}^{i} is the ithi^{th} spatial component of the IthI^{th} particle. Consequently,

ψxIi=S𝒟X(x)Ψ[X(x)]ψXIjXjxi,\frac{\partial\psi^{\prime}}{\partial x_{I}^{{}^{\prime}i}}=\int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]\frac{\partial\psi}{\partial X_{I}^{j}}\frac{\partial X^{j}}{\partial x^{{}^{\prime}i}}, (27)

where ψXIj\frac{\partial\psi}{\partial X_{I}^{j}} means differentiate ψ\psi with respect to the jthj^{th} spatial component of the IthI^{th} particle, while Xjxi\frac{\partial X^{j}}{\partial x^{{}^{\prime}i}} does not require an II index because X(x)X(x^{\prime}) is the same function for every particle. The Schrodinger equation is invariant under Euclidean transformations and so we restrict our superposition of coordinate systems to a superposition of Euclidean transformations. As a result, ψXIjXjxi\frac{\partial\psi}{\partial X_{I}^{j}}\frac{\partial X^{j}}{\partial x^{{}^{\prime}i}} would be a rotation, and we can readily compute the transformation of the Laplacian from equation 25.

ψxIjxIi=S𝒟X(x)Ψ[X(x)]ψXInXImXnxjXmxi.\frac{\partial\psi^{\prime}}{\partial x_{I}^{{}^{\prime}j}\partial x_{I}^{{}^{\prime}i}}=\int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]\frac{\partial\psi}{\partial X_{I}^{n}X_{I}^{m}}\frac{\partial X^{n}}{\partial x^{{}^{\prime}j}}\frac{\partial X^{m}}{\partial x^{{}^{\prime}i}}. (28)

Letting i=ji=j, summing over the repeated indices, and noting that XnxjXmxi=δnm\frac{\partial X^{n}}{\partial x^{{}^{\prime}j}}\frac{\partial X^{m}}{\partial x^{{}^{\prime}i}}=\delta^{nm} yields the desired transformation —

ψxIixIi=I2ψ=S𝒟X(x)Ψ[X(x)]I2ψ.\frac{\partial\psi^{\prime}}{\partial x_{I}^{{}^{\prime}i}\partial x_{I}^{{}^{\prime}i}}=\nabla_{I}^{2}\psi^{\prime}=\int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]\nabla_{I}^{2}\psi. (29)

It is easy to see that

ψt=S𝒟X(x)Ψ[X(x)]ψt.\frac{\partial\psi^{\prime}}{\partial t}=\int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]\frac{\partial\psi}{\partial t}. (30)

The Schrodinger equation for NN particles in the OO reference frame is as follows—

I=1N22mII2ψ+V(x1,x2,,x3N)ψ=iψt,-\sum_{I=1}^{N}\frac{\hbar^{2}}{2m_{I}}\nabla_{I}^{2}\psi+V(x_{1},x_{2},...,x_{3N})\psi=i\hbar\frac{\partial\psi}{\partial t}, (31)

where each of the particles may have a different mass mIm_{I} and VV could depend upon any of the 3N3N configuration space coordinates. We may now transform the Schrodinger equation 31 to a system in superposition relative to the OO^{\prime} reference frame, which is assumed to be in superposition relative to the OO frame, with a wavefunctional Ψ[X(x)]\Psi[X(x^{\prime})]. Multiply equation 31 by Ψ[X(x)]\Psi[X(x^{\prime})], let xi=X(xi)x_{i}=X(x_{i}^{\prime}), and sum over all functions X(x)X(x^{\prime}). The result is

\displaystyle- I=1N22mIS𝒟X(x)Ψ[X(x)]I2ψ+\displaystyle\sum_{I=1}^{N}\frac{\hbar^{2}}{2m_{I}}\int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]\nabla_{I}^{2}\psi+ (32)
S\displaystyle\int_{S} 𝒟X(x)Ψ[X(s)]V(X(x1),X(x2),,X(x3N))ψ\displaystyle\mathcal{D}X(x^{\prime})\Psi[X(s^{\prime})]V(X(x_{1}^{\prime}),X(x_{2}^{\prime}),...,X(x_{3N}^{\prime}))\psi
=\displaystyle= iS𝒟X(x)ψt\displaystyle i\hbar\int_{S}\mathcal{D}X(x^{\prime})\frac{\partial\psi}{\partial t}

Using equations 28 and 30 we have

I=1N22mII2ψ+S𝒟X(x)Ψ[X(x)]V(X(x1),X(x2),,X(x3N))ψ=iψt,\displaystyle-\sum_{I=1}^{N}\frac{\hbar^{2}}{2m_{I}}\nabla_{I}^{2}\psi^{\prime}+\int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]V(X(x^{\prime}_{1}),X(x^{\prime}_{2}),...,X(x^{\prime}_{3N}))\psi=i\hbar\frac{\partial\psi^{\prime}}{\partial t}, (33)

where it should be apparent that I2\nabla_{I}^{2} acting on ψ\psi^{\prime} is i2xixi\sum_{i}\frac{\partial^{2}}{\partial x^{\prime}_{i}\partial x^{\prime}_{i}}. The potential energy must be invariant with respect to any Euclidean transformations (generally by being a function of the Euclidean distance of the differences of the coordinates). Therefore,

V(X(x1),X(x2),,X(x3N))=V(x1,x2,,x3N),V(X(x_{1}^{\prime}),X(x_{2}^{\prime}),...,X(x_{3N}^{\prime}))=V(x_{1}^{\prime},x_{2}^{\prime},...,x_{3N}^{\prime}), (34)

and

S𝒟X(x)Ψ[X(x)]V(X(x1),X(x2),,X(x3N))ψ=S𝒟X(x)Ψ[X(x)]V(x1,x2,,x3N)ψ.\int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]V(X(x_{1}^{\prime}),X(x_{2}^{\prime}),...,X(x_{3N}^{\prime}))\psi=\\ \int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]V(x_{1}^{\prime},x_{2}^{\prime},...,x_{3N}^{\prime})\psi. (35)

In equation 35, V(x1,x2,,x3N)V(x_{1}^{\prime},x_{2}^{\prime},...,x_{3N}^{\prime}) is a constant relative to the path integral over XX, and so comes out to yield

S𝒟X(x)Ψ[X(x)]V(X(x1),X(x2),,X(x3N))ψ=\displaystyle\int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]V(X(x_{1}^{\prime}),X(x_{2}^{\prime}),...,X(x_{3N}^{\prime}))\psi=
V(x1,x2,,x3N)S𝒟X(x)Ψ[X(x)]ψ\displaystyle V(x_{1}^{\prime},x_{2}^{\prime},...,x_{3N}^{\prime})\int_{S}\mathcal{D}X(x^{\prime})\Psi[X(x^{\prime})]\psi
=V(x1,x2,,x3N)ψ,\displaystyle=V(x_{1}^{\prime},x_{2}^{\prime},...,x_{3N}^{\prime})\psi^{\prime}, (36)

where we have used equation 25 in the last equality. Substituting equation 36 into equation 33 replaces the potential energy term with V(x1,x2,,x3N)ψV(x_{1}^{\prime},x_{2}^{\prime},...,x_{3N}^{\prime})\psi^{\prime}, and so demonstrates that under a superposition of transformations

I=1N22mII2ψ+V(x1,x2,,x3N)ψ=iψttransformation to superposed coordinatesI=1N22mII2ψ+V(x1,x2,,x3N)ψ=iψt,-\sum_{I=1}^{N}\frac{\hbar^{2}}{2m_{I}}\nabla_{I}^{2}\psi+V(x_{1},x_{2},...,x_{3N})\psi=i\hbar\frac{\partial\psi}{\partial t}\xrightarrow{\text{transformation to superposed coordinates}}\\ -\sum_{I=1}^{N}\frac{\hbar^{2}}{2m_{I}}\nabla_{I}^{2}\psi^{\prime}+V(x_{1}^{\prime},x_{2}^{\prime},...,x_{3N}^{\prime})\psi^{\prime}=i\hbar\frac{\partial\psi^{\prime}}{\partial t}, (37)

which was to be shown.

V Discussion and Future Work

This framework demonstrates the feasibility for coordinate systems to be considered in superposition relative to one another via a (complex-valued) wavefunctional Ψ[x(x)]\Psi[x(x^{\prime})], which takes as input transformation functions. It is posited that interaction between the frames will introduce collapse-like behavior and select a particular transformation amongst the superposed transformations with a probability given by the Born rule. A rule for composing wavefunctionals is provided. It is shown that with this composition rule, equation 17, they are closed. The wavefunctional, as introduced here, permits the transformation of wavefunctions “relative" to one frame to be expressed relative to another. This transformation of wavefunctions is consistent with the standard Schrodinger equation.

It is expected that frames may evolve to form superpositions so that after interaction between the frames, which may act to select a particular transformation x(x)x(x^{\prime}) by destroying superposition, is removed, they again will evolve into superposition. That is to say that this framework suggests, but does not single out, a kind of frame dynamics. Because of this possibility only the superposition of time-independent transformations is considered in this present work. The extension of this framework to time-dependent transformations, such as the Galilean transformations or Lorentz transformations and the form of the frame dynamics is a matter of future work.

Appendix A Integral of Delta Functions over Measure Zero Sets

Consider the integral

L𝑑xδ(xx0)={0x0L1x0L\int_{L}dx\delta(x-x_{0})=\left\{\begin{array}[]{ll}0&x_{0}\notin L\\ 1&x_{0}\in L\\ \end{array}\right. (38)

Consequently,

1LL𝑑xδ(xx0)={0x0L1Lx0L\frac{1}{L}\int_{L}dx\delta(x-x_{0})=\left\{\begin{array}[]{ll}0&x_{0}\notin L\\ \frac{1}{L}&x_{0}\in L\\ \end{array}\right. (39)

If the limit as LL approaches zero is taken, while LL is centered at XX, then

limL0L𝑑xδ(xx0)=δ(Xx0)\lim_{L\xrightarrow{}0}\int_{L}dx\delta\left(x-x_{0}\right)=\delta(X-x_{0}) (40)

LL is an interval in the limit whose length approaches zero. After the limit, it is a measure zero set, namely that of a single point.

Consider the integral in two dimensions.

Ad2xδ(xx0)δ(yy0)={0(x0,y0)A1(x0,y0)A\int_{A}d^{2}x\delta(x-x_{0})\delta(y-y_{0})=\left\{\begin{array}[]{ll}0&(x_{0},y_{0})\notin A\\ 1&(x_{0},y_{0})\in A\\ \end{array}\right. (41)

Or for infinitesimal area AA centered at (X,Y)(X,Y),

limA01AAd2xδ(xx0)δ(yy0)=δ(Xx0)δ(Yy0)\lim_{A\xrightarrow[]{}0}\frac{1}{A}\int_{A}d^{2}x\delta(x-x_{0})\delta(y-y_{0})=\delta(X-x_{0})\delta(Y-y_{0}) (42)

The area, however, may be made infinitesimal in many ways. For example, the area may be decreased by choosing points that form a curve. More precisely, let F(x,y)=0F(x,y)=0 be a curve, and let SS be a set of points that form the curve defined by FF and collection of points that lie infinitesimally around it so that SS has area AA. We conjecture,

limA01ASd2xδ(xx0)δ(yy0)=kδ(F(x0,y0)).\lim_{A\xrightarrow[]{}0}\frac{1}{A}\int_{S}d^{2}x\delta(x-x_{0})\delta(y-y_{0})=k\delta(F(x_{0},y_{0})). (43)

Where the limit that AA approaches zero is taken such that the remaining elements of SS are those points that satisfy F(x,y)=0F(x,y)=0. We have inserted a possible normalization constant kk, whose exact value would be computed in a proof. More generally, let SS be a measure zero set, defined by a membership function FF, which returns 0 for elements in the set. That is,

S={(x1,x2,,xN)|F(x1,x2,,xN)=0}.S=\{(x_{1},x_{2},...,x_{N})|F(x_{1},x_{2},...,x_{N})=0\}. (44)

We conjecture the following,

limV01VSdNxδ(x1x10)δ(x2x20)δ(xNxN0)=kδ(F(x10,x20,,xN0).\lim_{V\xrightarrow[]{}0}\frac{1}{V}\int_{S}d^{N}x\delta(x_{1}-x^{0}_{1})\delta(x_{2}-x^{0}_{2})\cdots\delta(x_{N}-x^{0}_{N})\\ =k\delta(F(x^{0}_{1},x^{0}_{2},\ldots,x^{0}_{N}). (45)

Where the area AA is generalized to a volume VV, and the coordinates are renamed in an obvious way Hörmander (2015). From equation 45 it follows in NN even dimensions that,

limV0\displaystyle\lim_{V\xrightarrow[]{}0} 1VSdN2xdN2y[δ(x1x10)δ(xN2xN20)]\displaystyle\frac{1}{V}\int_{S}d^{\frac{N}{2}}xd^{\frac{N}{2}}y\left[\delta(x_{1}-x^{0}_{1})\cdots\delta(x_{\frac{N}{2}}-x^{0}_{\frac{N}{2}})\right] (46)
×[δ(y1y10)δ(yN2yN20)]\displaystyle\times\left[\delta(y_{1}-y^{0}_{1})\cdots\delta(y_{\frac{N}{2}}-y_{{}^{0}\frac{N}{2}})\right]
=\displaystyle= kδ(F(x10,x20,xN20;y10,y20,yN20)).\displaystyle k\delta(F(x^{0}_{1},x^{0}_{2},\ldots x^{0}_{\frac{N}{2}};y^{0}_{1},y^{0}_{2},\ldots y^{0}_{\frac{N}{2}})).

In the limit that the number of dimensions approaches infinity, we have the

S\displaystyle\int_{S} Dg(x)Dh(x)δ[g(x)g0(x)]δ[h(x)h0(x)]\displaystyle Dg(x)Dh(x)\delta[g(x)-g_{0}(x)]\delta[h(x)-h_{0}(x)] (47)
=\displaystyle= kδ[F[g0(x),h0(x)]],\displaystyle k\delta\left[F[g_{0}(x),h_{0}(x)\right]],

where we are integrating over set SS, a set of paired functions (g(x),h(x))\left(g(x),h(x)\right), defined by a membership function F(g(x),h(x))F\left(g(x),h(x)\right). F(g(x),h(x))F\left(g(x),h(x)\right) returns 0 for paired functions (g(x),h(x))\left(g(x),h(x)\right) in SS. We do not prove that a set of functions defined by a membership function form a zero measure set, which would be difficult. However, in RnR^{n} subsets chosen by a membership function are, baring contrivance, zero volume measure sets and we operate under the assumption that this remains valid in the large NN limit. In equation 14, the membership function is as follows. A pair of functions, (x(x),x(x′′))(x(x^{\prime}),x^{\prime}(x^{\prime\prime})), are in set Sx(x′′)S_{x(x^{\prime\prime})} if x(x(x′′))=x(x′′)x(x^{\prime}(x^{\prime\prime}))=x(x^{\prime\prime}). Therefore, F[x0(x),x0(x′′)]=x(x′′)x0(x0(x′′))F[x_{0}(x^{\prime}),x^{\prime}_{0}(x^{\prime\prime})]=x(x^{\prime\prime})-x_{0}(x^{\prime}_{0}(x^{\prime\prime})) and we have that

Sx(x′′)Dx(x)Dx(x′′)δ[x(x)x0(x)]δ[x(x′′)x0(x′′)]=kδ[x(x′′)x0(x0(x′′)]].\int_{S_{x(x^{\prime\prime})}}Dx(x^{\prime})Dx^{\prime}(x^{\prime\prime})\delta[x(x^{\prime})-x_{0}(x^{\prime})]\delta[x^{\prime}(x^{\prime\prime})-x^{\prime}_{0}(x^{\prime\prime})]=\\ k\delta\left[x(x^{\prime\prime})-x_{0}(x^{\prime}_{0}(x^{\prime\prime})\right]]. (48)

This is the result that is argued for in the text.

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