Local Quantum Theory with Fluids in Space-Time
Mordecai Waegell1,2
1Institute for Quantum Studies, Chapman University, Orange, CA 92866, USA 2Schmid College of Science and Technology, Chapman University, Orange, CA 92866, USA July 14, 2021
A local theory of relativistic quantum article we lay out the general framework for lo- physics in space-time, which makes all of cal realist collapse-free theory quantum mechan- the same empirical predictions as the con- ics, and work through the simplest examples, ventional delocalized theory in configura- with all dynamics occurring explicitly in space- tion space, is presented and interpreted. time. This realizes an unachieved goal of Ein- Each physical system is characterized by stein, Schr¨odinger,and Lorentz, who were never a local memory and a set of indexed satisfied with the configuration space treatment, piece-wise single-particle wavefunctions in precisely because it introduced fundamental non- space-time, each with with its own coeffi- locality [2]. The new model makes identical em- cient, and these wave-fields replace entan- pirical predictions to standard quantum theory, gled states in higher-dimensional spaces. and can serve as a full replacement. This model is Each wavefunction of a fundamental sys- consistent with the Lorentz covariant Heisenberg- tem describes the motion of a portion Schr¨odinger model proposed by Schwinger in of a conserved fluid in space-time, with 1948 [3], and restores the equivalence between the fluid decomposing into many classical the local Heisenberg and Schr¨odingerpictures. point particles, each following a world-line However, we now know from Bell’s theorem and recording a local memory. Local in- [4,5,6,7,8] that if we wish to maintain inde- teractions between two systems take the pendence of measurement settings, then this is form of local boundary conditions between unavoidably a theory of many local worlds [9]. the differently indexed pieces of those sys- It it important to emphasize here the breadth tems’ wave-fields, with new indexes encod- of Schwinger’s accomplishment. In deriving ing each orthogonal outcome of the inter- quantum electrodynamics in parallel to Fey- action. The general machinery is intro- namn, he obtained a new Lorentz covariant state duced, including the local mechanisms for vector, defined on a single space-like hypersur- entanglement and interference. The expe- face, with information at each point in that sur- rience of collapse, Born rule probability, face restricted to that point’s past light cone. and environmental decoherence are dis- He also obtained the localized Schr¨odinger-like cussed. A number of illustrative examples dynamics that shows how this state evolves lo- are given, including a Von Neumann mea- cally to the next parallel space-like hypersurface, surement, and a test of Bell’s theorem. and obtained a space-time invariant local inter- action unitary for QED. This treatment is at arXiv:2107.06575v2 [quant-ph] 22 Sep 2021 1 Introduction the heart of modern particle physics, but these state vectors are completely inconsistent with Despite insubstantial but influential claims from the configuration-space wavefunctions in preva- the early days of quantum theory, Bohm proved lent use throughout modern quantum founda- in 1952 [1] that it is possible to give a straightfor- tions and information theory. ward realist interpretation of quantum mechan- The present model is an attempt to interpret ics with particles in space-time. However, in that the empirical data from table-top quantum ex- theory the underlying dynamics occurs in higher- periments, rather than high energy particle colli- dimensional configuration space, resulting in ex- sions, given Schwinger’s theory, by deconstruct- plicitly nonlocal dynamics in space-time. In this ing his new state vector into more familiar single-
1 particle spatial wavefunctions. This turns out theory. The empirical experience of collapse and to be the natural theoretical framework for re- many of its consequences are explained later, but fining the local Schr¨odingerpicture of the Par- for now, the right intuition is that each funda- allel Lives interpretation of quantum mechanics mental quantum system comprises a conserved [10, 11], and should also be consistent with the nonclassical fluid in space-time - and it helps to local Heisenberg picture frameworks that have keep in mind that the fluid is composed of parti- been developed elsewhere [12, 13, 14, 15, 16, 17, cles on world-lines. 18, 19, 20, 21, 22]. This is a local ballistic model of the uni- In the present model, all (quantum) systems verse, meaning all interactions are local scatter- are comprised by pseudo-classical fluids in a sin- ing events between ballistic classical particles, gle objective locally-Minkowski space-time and and there are no nonlocal or long-range interac- the classical particles in these fluids follow world- tions or objects of any kind (i.e., all long-range lines through space-time. There are many worlds effects are mediated by force-carrying particles on only in the sense that there are many world- world-lines which undergo local collisions). In the lines for the many particles in space-time, and most general local ballistic model, classical par- each particle experiences a unique perspective ticles can carry an internal memory tape with an from its location in space-time. According to arbitrary amount of information, and when two relativity theory, all empirical experiences nec- particles interact locally, nature performs a com- essarily follow from these unique local perspec- putation using those two memory tapes, and then tives, and are fully restricted to an observer’s updates both of them. In the coarse-grained fluid past light cone. There are no global ‘worlds’ in picture, the set of scattering rules for such local this theory - there is only the one global space- collisions should ultimately come from the Stan- time, containing many particles on world-lines. dard Model Lagrangian, and these take the form To be very explicit, even though their resolu- of boundary conditions between different packets tions to the measurement problem are similar, of fluid, while the memories become local prop- the local space-time model presented here is fun- erties of the continuum fluid packets. damentally different from the many-worlds the- A single quantum system may comprise a ory of Everett [23, 24], which is delocalized in superposition of many different indexed single- configuration space. particle wavefunctions, each evolving indepen- There are some similarities between the dently of the others in space-time, in the ab- present model and the work of Madelung [25], sence of an interaction with another system. We and also various works on many-interacting- can think of the indexes that delineate the differ- worlds [26, 27, 28, 29, 30, 31] for single quantum ent wavefunctions of a given system as belonging particles. to its internal memory tape. For each system, We will not be working with the individual it is the local scattering interactions with other trajectories of the classical particles in the fluids fluid particles (of the same system) that produces here, since we do not yet know how to choose a the collective Schr¨odinger/Diracwave evolution unique solution. The decomposition of the single- in the fluid. particle quantum probability current into fluid We call the collective description of all in- streamlines is always possible, and serves as the dexed packets of a quantum systems in space- simplest example of a viable set of trajectories. time a wave-field. As we will show later, the Here we consider the continuum fluid equa- wave-field for a single fundamental system is ex- tions obtained by coarse-graining over the bal- pressed as a piece-wise multi-valued wavefunc- listic trajectories of the individual particles com- tion in space-time, where each indexed value prising the fluid - and we take these to be the evolves independently according to the single- single-particle Schr¨odinger/Diracequations. The particle Schr¨odinger/Dirac equation. The pieces behavior for multiple quantum particles is com- are separated in space-time by interaction-based pletely different than in the standard treatment, boundary conditions, which are also where the which is the main focus of this article. The fluid number of indexes changes. The wave-field of a is conserved, which corresponds to conservation system is a separable mathematical description of probability current in collapse-free quantum for that system alone - even if it is entangled
2 with other systems. The set of all wave-fields on Quantum tunneling through a finite barrier a given space-like hypersurface corresponds to co- highlights the nonclassicality of the fluid. As a variant state introduced by Schwinger. pulse is incident upon a barrier, the interference In the non-relativistic limit, we can use Bohm’s with the reflected wave may cause temporary ze- eikonal form of a single-particle wavefunction ros to form in front of the barrier, and the fluid to iS form a series of compressed and rarefied regions, ψi = Rie i to elucidate the fluid picture, where 2 which quickly vanish as the reflected pulse moves Ri is the fluid density, Si is Hamilton’s principal away. Part of the packet also penetrates inside function, and ∇~ Si/m is the local average veloc- the barrier, and the probability current there is ity field of the particles in the fluid. Then Ri nonzero, so the fluid particles’ world-lines are lit- and Si evolve according to the coupled continu- ity equation and Hamilton-Jacobi equation, as in erally passing through the barrier and continuing single-particle Bohmian mechanics. The coeffi- on the other side - and clearly with a nonzero iφa tunneling time. cients ai = |ai|e i give the total quantity and global phase of the packet of fluid with index i. As we will see, the complexity of the picture These are also the relative phases and propor- grows with the dimension of the usual Hilbert tions of the total fluid in the total wave-field, space, which only obscures some of the relevant which are relevant for interference. As we will features, and this is why we focus most of our see, it is still essential that each ballistic particle attention on examples with 2-level systems. This in the fluid carries its own copy of all of the lo- article begins with analysis of states of one, two, cal state in its memory, in order to properly de- and three spins in space-time, including Von Neu- fine the local transfer matrices for interactions. mann measurement and Born’s rule. We then The relativistic treatment is conceptually identi- give a full demonstration of the local treatment cal, with the fluid particles moving along world- of an experimental test of Bell’s theorem, treat- lines. ing Alice and Bob as spins. Spatial entangle- ment and the Stern-Gerlach are also discussed. In general, the fluid particles in different wave- Next, we present a possible experimental imple- functions of different systems can interact via lo- mentation of spin-spin entanglement that would cal scattering, and when this results in entangle- closely approximate the proper treatment given ment, this actually means that the scattering has here. We conclude with some discussion of the increased the number of wavefunctions of each historical context of this model as well as its po- system, with correlations encoded in their local tential future applications. memories, and the particles in the fluid divided up to occupy these new wavefunctions. These points of division form the spatial boundaries 2 Spins that separate the different pieces of the wave- field. In this model, the wave-field of an isolated Finally, to get some physical intuition for Pauli spinor comprises a superposition of two this model, it helps to think of each indexed indexed single-particle wavefunctions in space- 2 wave packet as an isolated drop of fluid float- time, which is to say a fluid density Ri (x, t) and ing through space. This is a very nonclassical a principal function Si(x, t) with velocity field fluid, which behaves more like a gas than a liquid, ∇~ Si(x, t)/m. If two spins are entangled, then allowing significant compression and rarefaction each spin comprises up to eight wavefunctions as it moves. This facilitates longitudinal waves on space-time, with four different interaction in- passing through the drop, which produces famil- dexes. For three entangled spins, each comprises iar wave behavior. Unlike a classical gas, these up to 32 wavefunctions space-time, with 16 in- waves can create zeros in the fluid density - for teraction different indexes. We can work in any example the nodes of a stationary state - so the basis without loss of generality, so we use the bi- local ballistic scattering rules for the particles in nary basis for all Pauli spinors, meaning i = 0, 1, the fluid must also be quite nonclassical. Despite corresponding to spin states |0i and |1i. this, fluid particles never cross these zeros, and For a single spin (system 1, denoted by super- 1 1 the entire motion can always be decomposed into script), the two wavefunctions aψ0(x) and bψ1(x) their world-lines. correspond to the spin states |0i1 and |1i1, re-
3 spectively, and it is the sum of these two proba- equation. Local interactions take the form of spa- bility densities that is normalized in space (|a|2 + tial boundary conditions that connect the differ- 2 R ∞ 1 2 |b| = 1, −∞ |ψi (x)| dx = 1). The point is, if ent spatial wavefunctions. 1 1 1 ψ0(x) = ψ1(x) = ψ (x), then the spin-position After the local interaction, each of them carry a 1 1 1 12 1 2 Hilbert space product state (a|0i + b|1i )ψ (x1) copy of the information U |0i |0i in their local in standard quantum theory is replaced in the memories. This process of collecting local inter- new theory by the pair of fluid packets in 3-space action unitaries and initial states along a single 1 1 {aψ0(x), bψ1(x)}. Note that if the spin and po- world-line is the essence of the local Heisenberg sition were entangled the description would be treatment. It is important to emphasize that more complicated. We discuss the Stern-Gerlach each of these copies is separate and independent later, but the general case goes beyond the scope from the others, and each copy encodes local in- of this article. formation at a single point in space (a single fluid We can change the basis used for the repre- particle). Whenever two systems locally interact, sentation, which results in new coefficients, and before the new interaction unitary is applied, the a new division into two different fluids. These memories of the two systems first synchronize, so still evolve independently, and this still produces that they now share all unitary operations and the correct evolution of the state. From this it initial states from both of their past local interac- should be clear that the division into two fluids is tions. Then the new interaction unitary is added arbitrary, and thus each fluid particle must carry to both of them, resulting in an equal number of both coefficients a and b in its memory. indexed spatial wavefunctions for each system, with matching coefficients. 2.1 Two Spins Taking the simple case that the spin and spa- tial wavefunctions are not entangled, we have If two spins (initially in state |0i) have inter- 1 1 1 1 ψ(x) 2 = ψ(x) 2 = ψ(x) 2 = ψ(x) 2 = acted via a unitary U 12, then to find the spa- 0,|0i 0,|1i 1,|0i 1,|1i ψ(x)1 and ψ(x)2 = ψ(x)2 = ψ(x)2 = tial wavefunctions of each system, we construct 0,|0i1 1,|0i1 0,|1i1 2 2 the 2-spin Hilbert space state U 12|0i1|0i2 = ψ(x)1,|1i1 = ψ(x) , the Hilbert space state of two P1 1 2 entangled spins with separable position states of i,j=0 aij|ii |ji , and then treat the states of all other systems as indexes that delineate separate standard quantum theory, wavefunctions of the present system. For exam- 1 1 2 X 1 2 ple, the four local states of system 1 are, ψ(x1) ⊗ ψ(x2) ⊗ aij|ii |ji , (5) i,j=0 1 1 1 1 a00|0i 2 , a01|0i 2 , a10|1i 2 , a11|1i 2 , |0i |1i |0i |1i is replaced in the local theory by the above set of (1) eight fluid packets in 3-space, and the many lo- and the four corresponding wavefunctions are cal copies of the Hilbert-space state they carry 1 1 a00ψ(x)0,|0i2 , a01ψ(x)0,|1i2 , in memory. It should be clear that a change 1 1 (2) of (product) basis still results in new coefficients a10ψ(x)1,|0i2 , a11ψ(x)1,|1i2 , and a new set of indexed spatial wavefunctions, and it is the sum of these four probability densi- but the underlying memory state is unchanged. 2 2 ties that is normalized in space (|a00| + |a01| + Note that the local memories of each spin 2 2 |a10| + |a11| = 1). Likewise for system 2 the carry all of the same information as the entan- local states are, gled Hilbert space state of conventional quan- tum theory, and at the fine-grained scale, every a |0i2 , a |1i2 , a |0i2 , a |1i2 , 00 |0i1 01 |0i1 10 |1i1 11 |1i1 fluid particle of each system carries this informa- (3) tion as well. The main point here is that these and the four corresponding wavefunctions are eight fluid packets in space-time contain all of 2 2 the information needed to produce the correct a00ψ(x)0,|0i1 , a01ψ(x)1,|0i1 , 2 2 (4) empirical probabilities and entanglement corre- a10ψ(x) 1 , a11ψ(x) 1 . 0,|1i 1,|1i lations for these systems. As we will show, be- In the absence of an interaction, each of these cause all interactions are local, we can completely spatial wavefunctions evolves independently ac- discard the delocalized wavefunction in a higher- cording to the single-particle Schr¨odinger/Dirac dimensional space, and instead obtain all of the
4 correct empirical predictions from this set of flu- wavefunctions of system 2 into eight, such that ids in space-time. the entanglement correlations between systems 2 By way of notation in the present formalism, and 3 become physically manifest. Note that if we will use superscripts to indicate which system two interacting systems already share some uni- a spatial wavefunction belongs to, rather than taries or initial states in memory, they will nec- subcripts on the coordinates in the one configu- essarily match, and so the two memories can be ration space wavefunction. As shown above, all simply be merged, as in this case (before the in- internal degrees of freedom (like spin) now cor- teraction, system 2 had U 12|0i1|0i2). respond to additional indexed spatial wavefunc- Now the new interaction unitary is added to tions of a given system, and entanglement with both memories, resulting in other systems also results in additional spatial 1 wavefunctions for both systems. 23 13 12 1 2 3 X 1 3 2 W V U |0i |0i |0i = djkl|ki |li |ji , j,k,l=0 2.2 Three Or More Spins (9) and eight new wavefunctions for systems 2 and Now, suppose that system 1 interacts locally with 3. The eight wavefunctions of system 1 are not system 3, while system 2 is not involved, and involved in this interaction, and are unchanged. does not change in any way. The interaction uni- Hopefully the general picture for larger numbers tary is V 13 and the initial state of system 3 is of spins is clear at this point. |0i3, and system 3 carries no other relevant mem- A final issue is single-spin unitaries that act ory. First, the two systems synchronize memory, on any system in isolation. Those are added to so system 3 acquires a copy of the U 12|0i1|0i2, memory, and participate in synchronization as which splits system 3 into four indexed wavefunc- normal, and thus they seem like a simple case tion, whose coefficients match those of systems 1. to discuss. However, in actuality, all interactions Then V 13|0i3 is added to both memories, result- are of the pairwise type described above, and a ing in state, single-spin unitary is truly an approximation of 1 a case where entanglement is extremely weak (as 13 12 1 2 3 X 1 3 2 V U |0i |0i |0i = aijbikl|ki |li |ji with the momentum exchange between a photon i,j,k,l=0 and a beam splitter), which is a bit more compli- cated. 1 X 1 3 2 = cjkl|ki |li |ji . (6) j,k,l=0 2.3 Local Entanglement From this, we see that there are eight local spin What remains is to show how two systems in- states for each system, teract locally and become entangled in this way. We will begin with the simplest possible exam- n 1 o n 3 o cjkl|ki|li3|ji2 , cjkl|li|ki1|ji2 , (7) ple, which is also quite illustrative. We ex- pect the general theory to contain only one type where in either case the other two systems are of coupling potential, and this is of the form treated as indexes, and thus eight spatial wave- δ(x1 − x2)V , where V is a general space-time- functions for each system as well, independent potential. This says that when two systems meet at an event in space-time, the po- n 1 o n 3 o cjklψ(x)k,|li3|ji2 , cjklψ(x)l,|ki1|ji2 . (8) tential V produces the local scattering between them, via the unitary U = e−iV/~, and the new Now, systems 2 and 3 have not interacted, but states are written into the memories of the fluid there are now entanglement correlations between particles as this happens, causing them to sepa- them, which will effect what happens if they in- rate into more distinct fluids than before. This teract in the future. Let us consider that case general potential should be uniform throughout next. space-time, and encompass all possible scattering Systems 2 and 3 now interact via unitary events between all types of quantum systems. In W 23. First, their memories are synchronized to other words, all Standard Model particle interac- V 13U 12|0i1|0i2|0i3, which splits the four indexed tions should be encoded in V .
5 Because this model does not support long- and the fully normalized piece-wise wave-field range interactions it is relatively complicated to |Ψ(x, t)is of each system includes contributions recover Coulomb-potential based interactions be- from all six, and all twelve for both systems. The tween charges, which are mediated by massless situation is shown in Fig.1. force carriers. To demonstrate the general mech- anism, we consider a gedanken experiment with 2.4 The Interaction Boundary just two quantum systems in space-time, where the only coupling potential is a spin-spin interac- The next important detail we need to examine tion - thus U = e−iV/~ is some 4 × 4 2-spin ma- is the actual location x12 between the systems, trix. With this potential, the spatial wavefunc- which is not a fixed boundary at all, but rather a tions never change or become entangled with the dynamic one that moves in time depending on the spins. Thus, if the two systems are incident upon shapes of the two incident systems’ wavefunctions one another, the fluid packets pass through the (in 3D this is a dynamic boundary surface). The interaction undeflected and undeformed, but the boundary is defined by a special rule that applies spin states interact locally as this occurs, caus- to all entanglement couplings in this model - the ing the fluid to acquire new indexes that separate fluid flux of the two systems across the boundary it into more distinct packets than before - each must be equal and opposite. For any two normal- moving independently but identically. These lo- ized wavefunctions ψ(x) and φ(x), there is always cal interactions are the origin of empirical entan- a boundary point where, glement correlations, so it is still appropriate to Z x12 Z ∞ 1 2 2 2 say that two systems became entangled during |ψ (x)| dx = |ψ (x)| dx, (10) −∞ x this interaction, even if there is no unfactorizable 12 state in configuration space. and
Z x12 Z ∞ We now consider such an entangling inter- |ψ2(x)|2dx = |ψ1(x)|2dx. (11) action for two spins that begin in a separable −∞ x12 state, each with two wavefunctions in space- The initial value of the boundary can be found in 1 1 2 time, a1ψ0(x, t) and b1ψ1(x, t), and a2ψ0(x, t) this way (ideally when the two packets are well- 2 and b2ψ1(x, t), respectively. They can only inter- separated), and then it moves according to, act locally, and thus the only reason they have 1 2 not interacted is that they have no overlapping j (x12, t) + j (x12, t) x˙ 12(t) = 1 2 2 2 , (12) support. In fact, there must be a boundary point |ψ (x12, t)| + |ψ (x12, t)| x12 that separates their supports. For this sim- ple one-dimensional example, we will begin with where js is the current density of each fluid. spin 1 located fully to the left of x12 and propa- This equal-and-opposite flux condition guaran- gating towards spin 2, which is fully to the right tees that the an equal amount of fluid from each of x12. In this example, once their supports begin system is always crossing the boundary in a given to overlap, the spins will directly interact via a 4- time. dimensional unitary U (strictly speaking, it need This condition is required to guarantee that 1 2 the a00 in a00ψ is the same as in a00ψ 1 2 , the not be unitary so long as it is norm-preserving), 00102 0 0 1 2 which maps the two pre-interaction wavefunc- a01 in a01ψ0,|1i2 is the same as the a01 in a01ψ|0i1 , tions of each system into its four post-interaction etc. As they cross the interaction boundary, the wavefunctions. Note that for spin 1 the two pre- fluid particles of both systems acquire all of the interaction wavefunctions are only supported at 2-spin entanglement information. Importantly, x ≤ x12, while the four post-interaction wave- these are independent copies of the coefficients, functions are only supported at x ≥ x12 (since in different memory records, and local interven- the wave-packets continue to propagate with the tions on one copy have no nonlocal effect on other same momentum). From here, it is clear that U copies. simply defines the boundary conditions that con- In 3D, there is no longer a unique boundary nect these six wavefunctions at x12 (four post- surface for two normalized functions, so an ini- interactions wavefunctions on one side, and two tial boundary must be assumed. The motion of pre-interaction wavefunctions on the other side), this boundary is then defined locally such that as
6 Figure 1: Three frames showing the local interaction ferent interaction boundaries for different wave- process as two particles in one dimension pass through functions of a given pair of systems. each other, with only their spins interacting. The spa- 2 Finally, the hard boundary presented here may tial density |ψ(x)i| of each fluid pulse is shown, each indexed by past interactions, for the particular case that be a proof of concept, rather than a physically 2 2 2 2 2 2 correct rule. A possible generalization is that |a1| = |b1| = |a2| = |b2| = 1/2 and |c| = |d| = |e|2 = |f|2 = 1/4. The piece-wise wave-field |Ψ(x, t)is when two fluids meet, only some fraction of them of each system formally includes all six wavefunctions as interacts, and the remainders simply continue in separated at the dynamic boundary x12(t) (stationary their pre-interaction states. This would effec- in this example) which all occupy the same space-time. tively smear the boundary between the pre- and Also consider this example in a boosted Lorentz frame, post-interaction wavefunctions, but it would also where the boundary is moving such that the fluid fluxes mean that two fluids can never fully switch into of the two systems are equal and opposite. their post-interaction states. In any event, for the purpose of this article, we will use the hard boundary. x 2.5 Boundary Conditions
x To obtain the boundary condition at x12, we consider the action of a general norm-preserving transformation matrix on a general product state of two spins. The matrix can be expanded as
x 12 X 1 2 1 2 U = uijkl|ii |ji hk| hl| (13) i,j,k,l∈[0,1] x
x 12 1 2 1 2 1 2 1 2 U a1a2|0i |0i +a1b2|0i |1i +b1a2|1i |0i +b1b2|1i |1i x 1 2 = u0000a1a2+u0001a1b2+u0010b1a2+u0011b1b2 |0i |0i x 1 2 + u0100a1a2+u0101a1b2+u0110b1a2+u0111b1b2 |0i |1i x 1 2 + u1000a1a2+u1001a1b2+u1010b1a2+u1011b1b2 |1i |0i 1 2 + u1100a1a2+u1101a1b2+u1110b1a2+u1111b1b2 |1i |1i x = c|0i1|0i2 + d|0i1|1i2 + e|1i1|0i2 + f|1i1|1i2 This allows us to define the two 4×2 transfer ma- x trices T1 and T2 that map the two pre-interaction wavefunctions of each system onto its four post- x interaction wavefunctions,
x U 12 2 2 T1 = U a2|0i + b2|1i
= X (u a + u b )|ii1|ji2hk|1 two systems move together, an equal amount of ijk0 2 ijk1 2 i,j,k∈[0,1] fluid from each crosses per unit time. At the fine- grained scale, the boundary corresponds to the u0000a2 + u0001b2 u0010a2 + u0011b2 locations where fluid particles of the two systems are locally scattering and synchronizing memory. u0100a2 + u0101b2 u0110a2 + u0111b2 A boundary like this exists between every pair = , of systems. It goes beyond the scope of this arti- u a + u b u a + u b 1000 2 1001 2 1010 2 1011 2 cle, but once the spatial degrees of freedom of a system are entangled, there can generally be dif- u1100a2 + u1101b2 u1110a2 + u1111b2
7 and and U 12 1 1 T2 = U a1|0i + b1|1i ˜2 ψ0,|0i1 x12(t), t " # 2 X 1 2 2 ˜2 ˜ ψ0 x12(t), t U † ψ0,|1i1 x12(t), t = (uij0la1 + uij1lb1)|ii |ji hl| = T , ψ˜2 x (t), t 2 ψ˜2 x (t), t i,j,l∈[0,1] 1 12 1,|0i1 12 ψ˜2 x (t), t 1,|1i1 12 u0000a1 + u0010b1 u0001a1 + u0011b1 (18) where the ψ˜ are general un-normalized individual u0100a1 + u0110b1 u0101a1 + u0111b1 wavefunctions for each index. = . These reduce back to simple mappings between u a + u b u a + u b 1000 1 1010 1 1001 1 1011 1 the spin coefficients, since all of the normalized packets are identical, so the transfer matrices re- u1100a1 + u1110b1 u1101a1 + u1111b1 ally only produce the coefficients c, d, e, and f, and show how as and bs define them. The piece-wise multivalued wave-fields of each † −1 Because U = U , we also have system are,