<<

of travel through post-selected

The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story .

Citation Lloyd, Seth et al. “Quantum mechanics of through post- selected teleportation.” Physical Review D 84 (2011): n. pag. Web. 8 Nov. 2011. © 2011 American Physical Society

As Published http://dx.doi.org/10.1103/PhysRevD.84.025007

Publisher American Physical Society

Version Final published version

Citable link http://hdl.handle.net/1721.1/66971

Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. PHYSICAL REVIEW D 84, 025007 (2011) Quantum mechanics of time travel through post-selected teleportation

Seth Lloyd,1 Lorenzo Maccone,1,2 Raul Garcia-Patron,1 Vittorio Giovannetti,3 and Yutaka Shikano1,4 1xQIT, Massachusetts Institute of Technology, 77 Mass Avenue, Cambridge Massachusetts, USA 2Dippartimento Fisica ‘‘A. Volta’’, INFN Sez. Pavia, Univ. of Pavia, via Bassi 6, I-27100 Pavia, Italy 3NEST, Scuola Normale Superiore and Istituto Nanoscienze-CNR, p.zza dei Cavalieri 7, I-56126 Pisa, Italy 4Department , Tokyo Institute of Technology, 2-12-1 Oh-Okayama, Meguro, Tokyo, 152-8551, Japan (Received 13 November 2010; published 13 July 2011) This paper discusses the quantum mechanics of closed-timelike curves (CTCs) and of other potential methods for time travel. We analyze a specific proposal for such quantum time travel, the quantum description of CTCs based on post-selected teleportation (P-CTCs). We compare the theory of P-CTCs to previously proposed quantum theories of time travel: the theory is inequivalent to Deutsch’s theory of CTCs, but it is consistent with path-integral approaches (which are the best suited for analyzing quantum- field theory in curved -time). We derive the dynamical equations that a -respecting system interacting with a CTC will experience. We discuss the possibility of time travel in the absence of general-relativistic closed-timelike curves, and investigate the implications of P-CTCs for enhancing the power of computation.

DOI: 10.1103/PhysRevD.84.025007 PACS numbers: 03.67.a, 03.65.Ud, 04.60.m, 04.62.+v

Einstein’s theory of allows the exis- communication channel from the to the . tence of closed-timelike curves, paths through space-time Quantum time travel, then, should be described by a quan- that, if followed, allow a time traveler—whether human tum communication channel to the past. A well-known being or elementary particle—to interact with her former quantum communication channel is given by quantum self. The possibility of such closed-timelike curves teleportation, in which shared entanglement combined (CTCs) was pointed out by Kurt Go¨del [1], and a variety with quantum measurement and classical communication of containing closed-timelike curves have allows quantum states to be transported between the sender been proposed [2,3]. As in all versions of time travel, and the receiver. We show that if is closed-timelike curves embody apparent paradoxes, such combined with post-selection, then the result is a quantum as the , in which the time traveller channel to the past. The entanglement occurs between the inadvertently or on purpose performs an action that causes forward- and backward-going parts of the curve, and post- her future self not to exist. Einstein (a good friend of selection replaces the quantum measurement and obviates Go¨del) was himself seriously disturbed by the discovery the need for classical communication, allowing time travel of CTCs [4]. to take place. The resulting theory allows a possible de- Reconciling closed-timelike curves with quantum me- scription of the quantum mechanics of general-relativistic chanics is a difficult problem that has been addressed closed-timelike curves. repeatedly, for example, using path-integral techniques The two basic types of paradoxes that arise in time travel [5–10]. This paper explores a particular version of to the past are the grandfather paradox, in which the time closed-timelike curves based on combining quantum tele- traveller, accidentally or on purpose, kills her grandfather portation with post-selection. The resulting post-selected as young man before he as had any children. So, she does closed-timelike curves (P-CTCs) provide a self-consistent not exist; so, she cannot go to the past and kill her grand- picture of the quantum mechanics of time travel. P-CTCs father, etc. Phrased in physical terms, the grandfather para- offer a theory of closed-timelike curves that is inequivalent dox is essentially an issue of the self-consistency of to other Hilbert-space based theories, e.g., that of Deutsch dynamics in the presence of closed-timelike curves. The [11]. Because the theory of P-CTCs rely on post-selection, type of paradox is based on the unproved theorem they provide self-consistent resolutions to such paradoxes: paradox, in which the time traveller reads an elegant proof anything that happens in a P-CTC can also happen in of a theorem in a book. Going back in time, she shows the conventional quantum mechanics with some probability. proof to a mathematician, who decides to include the proof Similarly, the post-selected nature of P-CTCs allows the in his book. The book, of course, is the same book in which predictions and retrodictions of the theory to be tested she read the theorem in the first place. Phrased in terms of experimentally, even in the absence of an actual general- physical law, the unproved theorem paradox raises issues relativistic closed-timelike curve. of indeterminacy. Space- that possess closed-timelike To provide our unifying description of closed-timelike curves typically do not possess Cauchy surfaces: the be- curves in quantum mechanics, we start from the havior of particles and fields cannot be obtained simply by prescription that time travel effectively represents a specifying initial conditions and integrating the equations

1550-7998=2011=84(2)=025007(11) 025007-1 Ó 2011 American Physical Society SETH LLOYD et al. PHYSICAL REVIEW D 84, 025007 (2011) of over time. Both the grandfather paradox and the As described in previous work [18], the notion that unproved theorem paradox give rise to physical issues entanglement and projection can give rise to closed- which must be resolved in a quantum theory of CTCs. timelike curves has arisen independently in a variety of Although Einstein’s theory of general relativity implic- contexts. This combination lies at the heart of the itly allows travel to the past, it took several decades before Horowitz-Maldacena model for to escape Go¨del proposed an explicit space-time geometry contain- from black holes [19–22], and Gottesman and Preskill ing CTCs. The Go¨del universe consists of a cloud of note in passing that this mechanism might be used for swirling dust, of sufficient gravitational power to support time travel [21]. Pegg explored the use of a related - closed-timelike curves. Later, it was realized that closed- nism for ‘‘probabilistic time machines’’ [23]. Bennett and timelike curves are a generic feature of highly curved, Schumacher have explored similar notions in unpublished rotating spacetimes: the Kerr solution for a rotating black work [24]. Laforest, Baugh, and Laflamme analyzed their hole contains closed-timelike curves within the proposal, its consistency with the tensor product structure, horizon; and massive rapidly rotating cylinders typically and a proof-of-principle experiment that tests the symme- are associated with closed-timelike curves [2,9,12]. The try of information flow and of apparent breaking topic of closed-timelike curves in general relativity con- [25]. Coecke [26] studies the symmetry of information tinues to inspire debate: Hawking’s chronology protection flow using entanglement as mediation, and interpreting postulate, for example, suggests that the conditions needed entanglement as sending information back in time in to create closed-timelike curves cannot arise in any physi- such a way that the information sent back in time is altered cally realizable space-time [13]. For example, while Gott depending on the outcome of a (future) Bell measurement. showed that geometries can contain closed- Ralph suggests using teleportation for time traveling, timelike curves [3], Deser et al. showed that physical although in a different setting, namely, displacing the en- cosmic strings cannot create CTCs from scratch [14,15]. tangled resource in time [27]. Svetlichny describes experi- At the bottom, the behavior of is governed by the mental techniques for investigating quantum travel based laws of quantum mechanics. Considerable effort has gone on entanglement and projection [28]. Chiribella et al. con- into constructing quantum mechanical theories for closed- sider this mechanism while analyzing extensions to the timelike curves. The initial efforts to construct such theories quantum computational model [29]. Brukner et al. have involved path-integral formulations of quantum mechanics. analyzed probabilistic teleportation (where only the cases Hartle and Politzer pointed out that in the presence of in which the Bell measurement yields the desired result are closed-timelike curves, the ordinary correspondence be- retained) as a computational resource in [30]. Greenberger tween the path-integral formulation of quantum mechanics and Svozil [31] show how the grandfather paradox can be and the formulation in terms of unitary evolution of states in solved using quantum interference when feedback back- Hilbert space breaks down [6,8]. Morris et al. explored the ward in time is allowed using unitary couplings similar to quantum prescriptions needed to construct closed-timelike beam splitters: one can set up the quantum interference in curves in the presence of , bits of space-time this interferometer analogue such that self-contradictory geometry that, like the handle of a coffee cup, ‘‘break off’’ events cannot happen. In [32], it is shown that the existence from the main body of the Universe and rejoin it in the past of time-travel paradoxes would lead to violations in the [5]. Meanwhile, Deutsch formulated a theory of closed- probability rules in a simple finite-state model. timelike curves in the context of Hilbert space, by postulat- The outline of the paper follows. In Sec. I, we describe ing self-consistency conditions for the states that enter and P-CTCs and Deutsch’s mechanism in detail, emphasizing exit the closed-timelike curve [11]. the differences between the two approaches. Then, in General-relativistic closed-timelike curves provide one Sec. II, we relate P-CTCs to the path-integral formulation potential mechanism for time travel, but they need not of quantum mechanics. This formulation is particularly provide the only one. For example, even in the context of suited for the description of quantum-field theory in , faster-than-light communication is curved space-time [33], and has been used before to known to generate temporal paradoxes and causal loops provide quantum descriptions of closed-timelike curves (e.g., see [16] for a recent review). Nonetheless, quantum [6–8,10,34–37]. Our proposal is consistent with these mechanics supports a variety of counter-intuitive phe- path-integral approaches. In particular, the path-integral nomena which might allow time travel even in the absence description of fermions using Grassmann fields given by of a closed-timelike curve in the geometry of space-time. Politzer [6] yields a dynamical description which coincides One of the best-known versions of non-general-relativistic with ours for systems of quantum bits. Other descriptions, quantum versions of time travel comes from Wheeler, as such as Hartle’s [8], are more difficult to compare as they described by Feynman in his Nobel Prize lecture [17]. As do not provide an explicit prescription to calculate the we will see, post-selected closed-timelike curves make up details of the dynamics of the interaction with systems a precise physical theory, which instantiates Wheeler’s inside closed-timelike curves. In any case, their general whimsical idea. framework is consistent with our derivations. By contrast,

025007-2 QUANTUM MECHANICS OF TIME TRAVEL THROUGH ... PHYSICAL REVIEW D 84, 025007 (2011) Deutsch’s CTCs are not compatible with the Politzer path- features [38–41]. By contrast, although any quantum the- integral approach, and are analyzed by him on a different ory of time-travel quantum mechanics is likely to yield footing [6]. Indeed, suppose that the path integral is strange and counterintuitive results, P-CTCs appear to be performed over classical paths which agree both at the less pathological [18]. They are based on a different self- entrance to—and at the exit from—the CTC, so that x-in, consistent condition that states that self-contradictory p-in are the same as x-out, p-out. Similarly, in the events do not happen (Novikov principle [34]). Pegg points Grassmann case, suppose that spin-up along the z axis at out that this can arise because of destructive interference of the entrance emerges as spin-up along the z axis at the exit. self-contradictory [23]. Here we further compare Then, the quantum version of the CTC must exhibit the Deutsch’s and post-selected closed-timelike curves, and same perfect correlation between input and output. But, as give an in-depth analysis of the latter, showing how they the grandfather-paradox experiment [18] shows, Deutsch’s can be naturally obtained in the path-integral formulation CTCs need not exhibit such correlations: spin-up in is of quantum theory and deriving the equations of mapped to spin-down out (although the overall quantum that describe the interactions with CTCs. As noted, in state remains the same). By contrast, P-CTCs exhibit per- addition to general-relativistic CTCs, our proposed theory fect correlation between in and out versions of all varia- can also be seen as a theoretical elaboration of Wheeler’s bles. Note that a quantum-field theoretical justification of assertion to Feynman that ‘‘an electron is a positron mov- Deutsch’s solution is proposed in [38,39] and is based on ing backward in time’’ [17]. In particular, any quantum introducing additional Hilbert subspaces for particles and theory which allows the nonlinear process of post-selection fields along the : observables at different points supports time travel even in the absence of general- along the geodesic commute because they act on different relativistic closed-timelike curves. Hilbert . The mechanism of P-CTCs [18] can be summarized by The path-integral formulation also shows that using saying that they behave exactly as if the initial state of the P-CTCs it is impossible to assign a well defined state to system in the P-CTC were in a maximal entangled state the system in the CTC. This is a natural requirement (or, at (entangled with an external purification space) and the final least, a desirable property), given the cyclicity of time state were post-selected to be in the same entangled state. there. In contrast, Deutsch’s consistency condition (2)is When the probability amplitude for the transition between explicitly built to provide a prescription for a definite these two states is null, we postulate that the related CTC of the system in the CTC. does not happen (so that the Novikov principle [34]is In Sec. III, we go beyond the path-integral formulation enforced). As we will show in the following, this is equiva- and provide the dynamical evolution formulas in the con- lent to requiring that the time evolution of the system text of generic quantum mechanics (the Hilbert-space for- external to the CTC is given by mulation). Namely, we treat the CTC as a generic quantum N C C y; transformation, where the transformed system emerges at a ½ / A A (1) previous time ‘‘after’’ eventually interacting with some where CA ¼ TrE½UAE is the partial trace, over the Hilbert chronology-respecting systems that are external to the space E of the system in the CTC, of the unitary evolution CTC. In this framework, we obtain the explicit prescription UAE that couples it to the external system. To enforce the of how to calculate the nonlinear evolution of the state of Novikov principle, we also have to suppose that the evo- the system in the chronology-respecting part of the space- lution described in (1) will not take place if the right-hand time. This nonlinearity is exactly of the form that previous side is null [42]. A formulation equivalent to Eq. (1) investigations (e.g., Hartle’s [8]) have predicted. consists in requesting that a pure state jc i evolves to In Sec. IV, we consider time-travel situations that are 0 jc i/CAjc i (when this in not a null vector). This will independent from general-relativistic CTCs. We then con- be derived below also using the path-integral formulation clude in Sec. V with considerations on the computational of quantum theory, by showing that the transition ampli- power of the different models of CTCs. tude from an initial state jc i to an arbitrary final state jFi is proportional to hFjTrE½UAEjc i. I. P-CTCS AND DEUTSCH’S CTCS By contrast, Deutsch’s CTCs are based on imposing the consistency condition Any quantum theory of will have to propose a y prescription to deal with the unavoidable [8] nonlinearities CTC ¼ TrA½UðA CTCÞU ; (2) that plague CTCs. This requires some sort of modification of the dynamical equations of motions of quantum me- where CTC is the state of the system inside the closed- chanics that are always linear. Deutsch in his seminal paper timelike curve, A is the state of the system outside (i.e., of [11] proposed one such prescription, based on a self- the chronology-respecting part of space-time), U is the consistency condition referred to the state of the systems unitary transformation that is responsible for eventual in- inside the CTC. Deutsch’s theory has recently been cri- teractions among the two systems, and where the trace tiqued by several authors as exhibiting self-contradictory is performed over the chronology-respecting system.

025007-3 SETH LLOYD et al. PHYSICAL REVIEW D 84, 025007 (2011) The existence of a state that satisfies (2) is ensured by the |ψ> a) 2 b) fact that any completely-positive map of the form L½¼ y TrA½UðA ÞU always has at least one fixed point Alice V 1 t (or, equivalently, one eigenvector with eigenvalue one). |ψ> M Bob If more than one state CTC satisfies the consistency con- 3 dition (2), Deutsch separately postulates a ‘‘maximum |ψ> 13 |ψ> rule,’’ requesting that the maximum entropy one 2 must be chosen. Note that Deutsch’s formulation assumes that the state exiting the CTC in the past is factorized with the chronology-preserving variables (the properties per- FIG. 1. Description of closed-timelike curves through telepor- taining to systems that are external to all CTCs) at that tation. a) Conventional teleportation: Alice and Bob start from a time: the time traveler’s ‘‘memories’’ of events in the maximallyS entangled state shared among them represented by future are no longer valid. ‘‘ ’’. Alice performs a Bell measurement M on her half of the The primary conceptual difference between Deutsch’s shared state and on the unknown state jc i she wants to transmit. CTCs and P-CTCs lies in the self-consistency condition This measurement tells her which entangled state the two imposed. Consider a measurement that can be made either systems are in. She then communicates (dotted line) the mea- on the state of the system as it enters the CTC, or on the surement result to Bob who performs a unitary V on his half of c state as it emerges from the CTC. Deutsch demands that the entangled state, obtaining the initial unknown state j i. The these two measurements yield the same statistics for the numbers refer to the systems as indicated by the subscripts in Eq. (3). b) Post-selected teleportation: the system in state jc i CTC state alone: that is, the density matrix of the system as S and halfT of the Bell state ‘‘ ’’ are projected onto the same Bell it enters the CTC is the same as the density matrix of the state ‘‘ .’’ This means that the other half of the Bell state is system as it exits the CTC. By contrast, we demand that projected into the initial state of the system jc i even before this these two measurements yield the same statistics for the state is available. CTC state together with its correlations with any chronology-preserving variables. It is this demand that closed-timelike curves respect both statistics for the time- purification system 3 are post-selected to be in the same Bell ðÞ traveling state together with its correlations with other state j i13 as the initial one, then only the first of variables that distinguishes P-CTCs from Deutsch’s Eq. (3) survives. Apart from an inconsequential minus sign, CTCs. The fact that P-CTCs respect correlations effec- this implies that the system 2 emerging from the CTC is in tively enforces the Novikov principle [34], and, as will the state jc i2, which is exactly the same state of the system be seen below, makes P-CTCs consistent with path-integral that has entered (rather, will enter) the CTC. approaches to CTCs. It seems that, based on what is currently known on these The connection between P-CTCs and teleportation [43] two approaches, we cannot conclusively choose P-CTCs is illustrated (see Fig. 1) with the following simple example over Deutsch’s, or vice versa. Both arise from reasonable that employs qubits (extensions to higher dimensional physical assumptions and both are consistent with differ- ent approaches to reconciling quantum mechanics with systems are straightforward). Supposepffiffiffi that the initial Bell state is jðÞi¼ðj01ij10iÞ= 2 (but any maximally en- closed-timelike curves in general relativity. A final deci- tangled Bell state will equivalently work), and suppose that sion on which of the two is ‘‘actually the case’’ may have the initial state of the system entering the CTC is jc i. Then to be postponed to when a full quantum theory of gravity the joint state of the three systems (system 1 entering the is derived (which would allow one to calculate from first CTC, system 2 emerging from the CTC, and system 3, its principles what happens in a CTC) or when a CTC is ðÞ purification) is given by jc i1j i23. These three systems discovered that can be tested experimentally. However, are denoted by the three vertical lines of Fig. 1(b).Itis because of the huge recent interest on CTCs in physics immediate to see that this state can be also written as and in computer (e.g., see [40,41,45–49]), it is important to point out that there are reasonable alterna- ðÞ ðþÞ ðÞ tives to the leading theory in the field. We also point out ðj i13jc i2 j i13zjc i2 þj i13xjc i2 that our post-selection based description of CTCs seems to ðþÞ þ ij i13yjc i2Þ=2; (3) be less pathological than Deutsch’s: for example, P-CTCs pffiffiffi have less computational power and do not require to ðÞ 01 10 = 2 ðÞ 00 wherepjffiffiffi i¼ðj ij iÞ and j i¼ðj i separately postulate a maximum entropy rule [18]. j11iÞ= 2 are the four states in a Bell basis for qubit systems Therefore, they are in some sense preferable, at least and s are the three Pauli matrices. Equation (3) is equiva- from an Occam’s razor perspective. Independent of such lent to Eq. (5) of Ref. [43], where the extension to higher questions of aesthetic preference, as we will now show, dimensional systems is presented (the extension to infinite- P-CTCs are consistent with previous path-integral formu- dimensional systems is presented in [44]). It is immediate to lations of closed-timelike curves, whereas Deutsch’s see that, if the system 1 entering the CTC together with the CTCs are not.

025007-4 QUANTUM MECHANICS OF TIME TRAVEL THROUGH ... PHYSICAL REVIEW D 84, 025007 (2011) II. P-CTCS AND PATH INTEGRALS have previously appeared in the literature (e.g., see [10] and, in the classical context, in the seminal paper [52]). Path integrals [50,51] allow one to calculate the transi- To show that Eq. (6) is the same formula that one obtains tion amplitude for going from an initial state jIi to a final using post-selected teleportation, we have to calculate state jFi as an integral over paths of the action, i.e., i hFjhj expð HÞ1jIiji, where ji is a maximally   Z ℏ i þ1 entangled state in position and where the Hamiltonian acts hFj exp H jIi¼ dxdyIðxÞFðyÞ ℏ only on the system and on the first of the two Hilbert spaces 1   Z y i of ji. As a maximally entangledR state in position, we use DxðtÞ exp S ; the EPR [53] state ji/ dxjxxi. Since this state is non- x ℏ Z normalizable, a rigorous treatment requires a regulariza- where S ¼ dtLðx; x_ Þ; (4) tion and will be given in the Appendix. Here we employ the 0 non-normalizable EPR state ji just to provide the idea and where L is the Lagrangian, H the Hamiltonian, S is the behind the proof. We use Eq. (5) for the system and for the action, IðxÞ and FðxÞ are the positionR representations of jIi first Hilbert space of j i to obtain   and jFi, respectively (i.e., jIi¼ dxIðxÞjxi),R and the paths i Dx t hFjhj exp H 1jIiji in the integration over paths—indicated by ð Þ—all ℏ start in x and end in y. Of course, in this form it is suited Z þ1 only to describing the dynamics of a particle in space (or a / dxdx0dydy0dzdz0IðxÞFðyÞðx0 zÞ collection of particles). It will be extended to other systems 1 Z y;y0 i in the next section. ðy0 z0Þhzj1jz0i DxðtÞ exp½ S In order to add a CTC, we first divide the space-time into x;x0 ℏ two parts, Z 1   ¼ dxdx0dydy0IðxÞFðyÞðx0 y0Þ i 1 0 0   hFj hF j exp H jIijI i Z 0 C ℏ C y;y i DxðtÞ exp S ; (7) Z þ1 x;x0 ℏ 0 0 ¼ dxdxCdydyCIðxÞI ðxCÞF ðyÞF ðyCÞ 1   where we have used the position representation Z y;y i C Dx t exp S ; Z ð Þ (5) dx0dz x0 z x0 z x;xC ℏ h j/ ð Þh jh j and Z where the first part will represent the chronology- ji/ dy0dz0ðy0 z0Þjy0ijz0i; respecting system outside the CTC, and the second part (indicated with the subscript C) will represent the system with hzjz0i¼ðz z0Þ. Note that this result is independent in the CTC, once appropriate conditions are enforced. The ‘‘conventional’’ strategy to deal with CTCs using path of the particular form of the EPR state j i as long as it integrals is to send the system C to a prior time unchanged is maximally entangled in position (and hence in (i.e., with the same values of x, x_ ), while the other system momentum). (the chronology-respecting one) evolves normally. This is All of the above discussion holds for initial and final enforced by imposing periodic boundary conditions on the pure states. However, the extension to mixed states in the CTC boundaries. Namely, the probability amplitude for the path-integral formulation is straightforward: one only chronology-respecting system is needs to employ appropriate purification spaces [54,55].   The formulas then reduce to the previous ones. i Z þ1 Here we briefly comment on the two-state vector for- hFjexp H jIi/ dxdxCdydyCIðxÞF ðyÞðxC yCÞ ℏ 1 malism of quantum mechanics [56,57]. It is based on Z   y;yC i post-selection of the final state and on renormalizing the DxðtÞexp S ; (6) x;x ℏ resulting transition amplitudes: it is a time-symmetrical C formulation of quantum mechanics in which not only the where the -function ensures that the initial and final initial state, but also the final state is specified. As such, it boundary conditions in the CTC system are the same. shares many properties with our post-selection based 0 0 Note that we have removed I ðxCÞ and F ðyCÞ, but we are treatment of CTCs. In particular, in both theories it is coherently adding all possible initial and final conditions impossible to assign a definite quantum state at each time: (through the xC and yC integrals). This implies that it is not in the two-state formalism, the unitary evolution forward possible to assign a definite state to the system inside a CTC: in time from the initial state might give a different mid- one could consistently assign to the system any possible time state with respect to the unitary evolution backward state that is compatible with the (periodic) boundary con- in time from the final state. Analogously, in a P-CTC, it is ditions. Note also that the boundary conditions of Eq. (6) impossible to assign a definite state to the CTC system at

025007-5 SETH LLOYD et al. PHYSICAL REVIEW D 84, 025007 (2011) any time, given the cyclicity of time there. This is evident, nonlinearity: according to our approach, a chronology- for example, from Eq. (6): in the CTC system no state is respecting system in a state that interacts with a assigned, only periodic boundary conditions. Another CTC using a unitary U will undergo the nonlinear trans- aspect that the two-state formalism and P-CTCs share is formation the nonlinear renormalization of the states and probabil- y y ities. In both cases, this arises because of the post- N ½¼CACA=Tr½CACA; (10) selection. In addition to the two-state formalism, our approach can also be related to weak values [56,58], since where we suppose that this evolution is impossible when- Tr C Cy 0 we might be performing measurements between when the ever A½ A A¼ . More specifically, all evolutions system emerges from the CTC and when it reenters it. that would lead to a vanishing denominator in Eq. (10) Considerations analogous to the ones presented above are forbidden: they cannot happen (e.g., see also [23]). An apply. It would be a mistake, however, to think that the equivalent condition is to request that the evolution is y theory of post-selected closed-timelike curves in some possible if and only if CACA is a strictly positive operator. sense requires or even singles out the weak-value theory. The comparison with (8) is instructive: there the non- Although the two are compatible with each other, the unitarity comes from the inaccessibility of the environ- theory of P-CTCs is essentially a ‘‘free-standing’’ theory ment. Analogously, in (10) the nonunitarity comes from that does not give preference to one interpretation of the fact that, after the CTC is closed, for the chronology- quantum mechanics over another. respecting system it will be forever inaccessible. The nonlinearity of (10) is more difficult to interpret, but is III. GENERAL SYSTEMS connected with the periodic boundary conditions in the CTC. Note that this general evolution equation (10)is The formula (6) was derived in the path-integral formu- consistent with previous derivations based on path inte- lation of quantum mechanics, but it can be easily extended grals. For example, it is equivalent to Eq. (4.6) of Ref. [8] to generic quantum evolution. by Hartle. However, in contrast to here, the actual form of We start by recalling the usual Kraus decomposition of a the evolution operators C is not provided there. As a further generic quantum evolution (that can describe the evolution example, consider Ref. [6], where Politzer derives a path- of both isolated and open systems). It is given by integral approach of CTCs for qubits, using Grassmann X y y fields. His Eq. (5) is compatible with Eq. (9). He also L ½¼TrE½Uð jeihejÞU ¼ BiBi ; (8) i derives a nonunitary evolution that is consistent with Eq. (10) in the case in which the initial state is pure. In where jei is the initial state of the environment (or, equiv- particular, this implies that, also in the general qubit case, alently, of a putative abstract purification space), U is the our post-selected teleportation approach gives the same unitary operator governing the interaction between system result one would obtain from a specific path-integral for- initially in the state and environment, and Bi hijUjei is mulation. In addition, it has been pointed out many times the Kraus operator (fjiig being an arbitrary basis for the before (e.g., see [35,59]) that when quantum fields inside a Hilbert space of the environment). In contrast, the evolu- CTC interact with external fields, linearity and unitarity is tion of our post-selected teleportation scheme is given by lost. It is also worth to notice that there have been various proposals to restore unitarity by modifying the structure of A ! TrEE0 ½ðUAE 1E0 ÞðA jiEE0 hjÞ quantum mechanics itself or by postulating an inaccessible y ðU 1E0 Þð1A jiEE0 hjÞ purification space that is added to uphold unitarity [60,61]. X AE 0 y 0 y The evolution (10) coming from our approach is to be ¼ hlEjUAEjlEiAhlEjUAEjlEi¼CAACA; (9) 0 compared with Deutsch’s evolution, lE;lE y D ½¼TrE½Uð CTCÞU ; (11) where CAP TrE½UAE, fjlEig is a set of basis states, and jiEE0 / jliEjliE0 (or any other maximally entangled l where state, which would give the same result). In Eq. (9), the A y subscript refers to the Hilbert space of the external CTC ¼ TrA½Uð CTCÞU (12) system, and E and E0 refer to the Hilbert spaces of the forward- and backward-propagating parts of the CTC. satisfies the consistency condition and where the trace in Note that CA is equal to one of the Kraus operators Bi of (11) refers to the degrees of freedom inside the CTC. The the system, as can be immediately seen by choosing a basis direct comparison of Eqs. (10) and (12) highlights the fjiig of the EE0 Hilbert space that contains the state ji as differences in the general prescription for the dynamics one of its elements. The evolution in (9) does not preserve of CTCs of these two approaches. the state’s normalization because of the post-selection en- Even though the results presented in this section are di- tailed by the projection onto the final state jiEE0 . Then, rectly applicable only to general finite-dimensional systems, we need to renormalize the final state, introducing a the extension to systems living in infinite-dimensional

025007-6 QUANTUM MECHANICS OF TIME TRAVEL THROUGH ... PHYSICAL REVIEW D 84, 025007 (2011) separable Hilbert spaces seems conceptually straightfor- quantum computation with Deutsch’s closed-timelike ward, although mathematically involved. curves allows the solution of any problem in PSPACE, In his path-integral formulation of CTCs, Hartle notes the set of problems that can be solved using polynomial that CTCs might necessitate abandoning not only unitarity space resources [47]. Similarly, Aaronson has shown that and linearity, but even the familiar Hilbert-space formula- quantum computation combined with post-selection allows tion of quantum mechanics [8]. Indeed, the fact that the state the solution of any problem in the computational class of a system at a given time can be written, as the tensor probabilistic polynomial time (PP) (where a probabilistic 1 product states of subsystems relies crucially on the fact that polynomial Turing machine accepts with probability 2 if operators corresponding to spacelike separated regions of and only if the answer is ‘‘yes’’). Quantum computation space-time commute with each other. When CTCs are in- with post-selection explicitly allows P-CTCs, and P-CTCs troduced, the notion of ‘‘spacelike’’ separation becomes in turn allow the performance of any desired post-selected muddied. The formulation of closed-timelike curves in quantum computation. Accordingly, quantum computation terms of P-CTCs shows, however, that the Hilbert-space with P-CTCs can solve any problem in PP, including NP- structure of quantum mechanics can be retained. complete problems. Since the class PP is thought to be strictly contained in PSPACE, quantum computation with IV. TIME TRAVEL IN THE ABSENCE OF P-CTCs is apparently strictly less powerful than quantum GENERAL-RELATIVISTIC CTCS computation with Deutsch’s CTCs. In the case of quantum computing with Deutschian Although the theory of P-CTCs was developed to ad- CTCs, Bennett et al. [40] have questioned whether the dress the question of quantum mechanics in general- notion of programming a quantum computer even makes relativistic closed-timelike curves, it also allows us to sense. Reference [40] notes that in Deutsch’s closed- address the possibility of time travel in other contexts. timelike curves, the nonlinearity introduces ambiguities Essentially, any quantum theory that allows the nonlinear in the definition of state preparation: as is well known in process of projection onto some particular state, such as the nonlinear quantum theories, the result of sending either the entangled states of P-CTCs, allows time travel even when state jc i through a closed-timelike curve or the state ji no space-time closed-timelike curve exists. Indeed, is no longer equivalent to sending the mixed state the mechanism for such time travel closely follows ð1=2Þðjc ihc jþjihjÞ through the curve. The problem Wheeler’s famous telephone call above. Non-general- with computation arises because, as is clear from our relativistic P-CTCs can be implemented by the creation grandfather-paradox circuit [18], Deutsch’s closed- of and projection onto entangled particle-antiparticle pairs. Such a mechanism is just what is used in our experimental timelike curves typically break the correlation between tests of P-CTCs [18]: although projection is a nonlinear chronology-preserving variables and the components of a process that cannot be implemented deterministically in mixed state that enters the curve: the component that enters 0 1 ordinary quantum mechanics, it can easily be implemented the CTC as j i can exit the curve as j i, even if the overall in a probabilistic fashion. Consequently, the effect of mixed state exiting the curve is the same as the one that P-CTCs can be tested simply by performing quantum tele- enters. Consequently, Bennett et al. argue, the programmer portation experiments, and by post-selecting only the re- who is using a Deutschian closed-timelike curve as part of sults that correspond to the desired entangled-state output. her quantum computer typically finds the output of the If it turns out that the linearity of quantum mechanics is curve is completely decorrelated from the problem she only approximate, and that projection onto particular states would like to solve: the curve emits random states. does in fact occur—for example, at the singularities of In contrast, because P-CTCs are formulated explicitly to black holes [19–22]—then it might be possible to imple- retain correlations with chronology-preserving curves, ment time travel even in the absence of a general- quantum computation using P-CTCs do not suffer from relativistic closed-timelike curve. The formalism of state-preparation ambiguity. That is not to say that P-CTCs P-CTCs shows that such quantum time travel can be are computationally innocuous: their nonlinear nature typi- thought of as a kind of quantum tunneling backwards in cally renormalizes the probability of states in an input time, which can take place even in the absence of a superposition, yielding to strange and counterintuitive ef- classical path from future to past. fects. For example, any CTC can be used to compress any computation to depth one, as shown in Fig. 2. Indeed, it is exactly the ability of nonlinear quantum mechanics to V. COMPUTATIONAL POWER OF CTCS renormalize probabilities from their conventional values It has been long known that nonlinear quantum mechan- that gives rise to the amplification of small components of ics potentially allows the rapid solution of hard problems quantum superpositions that allows the solution of hard such as NP-complete problems [62]. The nonlinearities in problems. Not the least of the counterintuitive effects of the quantum mechanics of closed-timelike curves is no P-CTCs is that they could still solve hard computational exception [47–49]. Aaronson and Watrous have shown problems with ease. The ‘‘excessive’’ computational power

025007-7 SETH LLOYD et al. PHYSICAL REVIEW D 84, 025007 (2011) ACKNOWLEDGMENTS We tank C. Bennett and D. Deutsch for discussions and t suggestions. This work was supported by the W. M. Keck Foundation, Jeffrey Epstein, NSF, ONR, DARPA, and NEC. Y.S. acknowledges support from the Global Center FIG. 2. Closed-timelike loops can collapse the time depth of of Excellence Program ‘‘Nanoscience and Quantum any circuit to one, allowing to compute any problem not merely Physics’’ at the Tokyo Institute of Technology. efficiently, but instantaneously. of P-CTCs is effectively an argument for why the types of APPENDIX: REGULARIZATION OF MAXIMALLY nonlinearities that give rise to P-CTCs, if they exist, should ENTANGLED STATES IN POSITION only be found under highly exceptional circumstances such In this section, we prove the result presented in Eq. (7) as general-relativistic closed-timelike curves or black-hole using two different normalizable states, jai and ji (the singularities. first allows simple calculations, whereas the second is more physically motivated). To avoid technicalities, VI. CONCLUSIONS Eq. (7) was presentedR above using the un-normalizable ji/ dxjxxi This paper reviewed quantum mechanical theories for EPR state . time travel, focusing on the theory of P-CTCs [18]. Our purpose in presenting this work is to make precise the 1. First regularization similarities and differences between varying quantum Consider the normalized state theories of time travel. We summarize our findings here. sffiffiffiffi Z We have extensively argued that P-CTCs are inequiva- 2 2 2 2 2 j i dxdyea x eðxyÞ =a jxijyi: lent to Deutsch’s CTCs. In Sec. II, we showed that a (A1) P-CTCs are compatible with the path-integral formulation of quantum mechanics. This formulation is at the basis of In the limit a 0, this state tends to the EPR state, as most of the previous analysis of quantum descriptions of sffiffiffiffi Z Z closed timelike curves, since it is particularly suited to 2 2 2 02 2 j i¼ dxea x dy0ey =a jxijx y0i calculations of quantum mechanics in curved space-time. a P-CTCs are reminiscent of, and consistent with, the two- pffiffiffi Z Z state vector and weak-value formulation of quantum me- ’ 2a dx dy0ðy0Þjxijx y0i chanics. It is important to note, however, that P-CTCs do pffiffiffi Z not in any sense require such a formulation. Then, in ¼ 2a dxjxijxi; Sec. III, we extended our analysis to general systems where the path-integral formulation may not always be y0 x y y where we have usedffiffiffiffi and the fact that ð Þ¼ possible and derived a simple prescription for the calcu- y2=a2 p lima 0e =ða Þ. Replacing ji with jai in Eq. (7), lation of the CTC dynamics, namely, Eq. (10). In this way, ! and taking a 0, we reobtain the same result, apart from we have performed a complete characterization of P-CTC the inconsequential proportionality factor 2a2 that, as we in the most commonly employed frameworks for quantum will now show, can be removed by calculating the condi- mechanics, with the exception of algebraic methods tional probability amplitude. (e.g., see [63]). The path integral is a transition amplitude between an In Sec. IV, we have argued that, as Wheeler’s picture of initial state jii and a final state jfi. As such, it can always positrons as electrons moving backwards in time suggests, be written as [50], P-CTCs might also allow time travel in space-times with-   out general-relativistic closed-timelike curves. If nature i hfj exp H jii¼hfjUjii; somehow provides the nonlinear dynamics afforded by ℏ (A2) final-state projection, then it is possible for particles (and, in principle, people) to tunnel from the future to the past. where H is the Hamiltonian and U the unitary evolution of Finally, in Sec. V, we have seen that P-CTCs are com- the system. To derive (7), we consider three systems: the putationally very powerful, though less powerful than the system A external to the CTC, which starts in the system Aaronson-Watrous theory of Deutsch’s CTCs. jIiA and ends in the system jFiA; the system E in the CTC Our hope in elaborating the theory of P-CTCs is that this and an ancillary system E0, which are initially in a joint theory may prove useful in formulating a quantum theory state jaiEE0 and are (post-selected) in the same final state of gravity, by providing new insight on one of the most jaiEE0 .IfUAE is the unitary describing the interaction perplexing consequences of general relativity, i.e., the between the systems external and internal to the CTC, the possibility of time travel. path integral for these three systems is then

025007-8 QUANTUM MECHANICS OF TIME TRAVEL THROUGH ... PHYSICAL REVIEW D 84, 025007 (2011) p F ps AhFjEE0 hajUAE 1E0 jIiAjaiEE0 that the post-selection happened, we can use ðj ij Þ¼ Z pðjFi; jaiÞ=pðpsÞ, where pðpsÞ is the probability that the 2 2 2 2 2 2 2 2 ¼ dx dx0dy ea ðx þx0 ÞðxyÞ =a ðx0yÞ =a post-selection succeeds independently of the final state. It can be simply calculated as F x U I x0 Ah jEh j AEj iAj iE (A3) Z p ps dF F U 1 I 2; sffiffiffiffi ð Þ¼ jAh jEE0 h aj AE E0 j iAj aiEE0 j (A5) Z 2 2 2 2 2 2 ¼ a dxdx0ea ðx þx0 Þðxx0Þ =a hFj hxjU jIi jx0i : A E AE A E where the integral runs over a basis of possible final states F (A4) j i. (Note that one could also enforce a similar condition on the initial state.) The square modulus of this quantity gives the joint proba- Hence, we see that the quantity in Eq. (A3) [and also the bility pðjFi; jaiÞ that final state of system A is jFi and quantities in Eqs. (6) and (7)] are only proportional to the 0 that the final state of systems E and E is jai. However, conditional probability amplitude we are interestedpffiffiffiffiffiffiffiffiffiffiffiffi in, our proposal is based on post-selecting the cases in which where the proportionality constant is given by 1= pðpsÞ. the latter event happens. To calculate the conditional From (A3), we see that the conditional probability ampli- probability pðjFijpsÞ that the final state of A is jFi given tude is given by

R 0 a2ðx2þx02Þðxx0Þ2=a2 0 AhFjEE0 hajUAE 1E0 jIiAjaiEE0 dx dx e hFjEhxjUAEjIiAjx iE pffiffiffiffiffiffiffiffiffiffiffiffi ¼ R R A : (A6) 0 a2ðx2þx02Þðxx0Þ2=a2 0 2 1=2 pðpsÞ ð dFj dx dx e AhFjEhxjUAEjIiAjx iEj Þ

We can now take the limit a ! 0, using again the property 2. Second regularization 2 2 pffiffiffiffi y lim ey =a = a ð Þ¼ a!0 ð Þ. The quantity in (A6) then As a more physically-motivated alternative to the state becomes in Eq. (A1), consider the two-mode squeezed state of two R optical modes dx hFj hxjU jIi jxi R A E AE A E 2 1=2 (A7) X1 ð dFjAhFjEhxjUAEjIiAjxiEj Þ 2 n jið1 Þ jnijni: (A11) n¼0

hFjCAjIiA We can write this state in the ‘‘position representation’’ ¼ A ; (A8) y 1=2 jxi ðTr½CAjIiAhIjCA Þ using an eigenbasis of the quadrature operator as X1 Z 2 n where CA TrE½UAE. Note that the proportionality factor ji¼ð1 Þ dxdyjxihxjnijyihyjni 2 2a that appears in the numerator when taking the limit n¼0 a 0  sffiffiffiffi ! is canceled by the same constant in the denominator. Z X1 2 n 2 1 Recalling that the path integral can be written in the form ¼ð1 Þ dxdy n n 0 2 n! (A2), it is simple to see that the numerator of Eq. (A7) ¼  written in the position representation will coincide with the pffiffiffi pffiffiffi H 2x H 2y ex2y2 x y ; last term of Eq. (7) (but was here obtained from a careful nð Þ nð Þ j ij i (A12) regularization): where we have used the relation Z   dx F x U I x 2 1=4 1 pffiffiffi Ah jEh j AEj iAj iE x2 hxjni¼ pffiffiffiffiffiffiffiffiffiffi Hnð 2xÞe ; (A13)   2nn! Z 1 Z y0;x i 0 0 ¼ dxdydy IðyÞF ðy Þ DxðtÞ exp S ; (A9) H 1 y;x ℏ with n the Hermite polynomial. We use the -function normalizationR of the quadrature basis to see that ji tends whereR we used theR position representation jIi¼ to the state dxjxijxi in the limit ! 1: dxIðxÞjxi and jFi¼ dxFðxÞjxi, and where the path xA xE X1 integral is used to relate the initial j i i, j i i and final ðx yÞ¼hyjxi¼ hyjnihnjxi xE xE A E j f i, j f i position states of the systems and as n¼0 sffiffiffiffi Z xA;xE 1 f f X 2 1 pffiffiffi pffiffiffi xA xE U xA xE Dx t eði=ℏÞS: x2y2 h f jh f j AEj i ij i i¼ ð Þ (A10) ¼ Hnð 2xÞHnð 2yÞe ; (A14) xA;xE 2nn! i i n¼0

025007-9 SETH LLOYD et al. PHYSICAL REVIEW D 84, 025007 (2011) whence it is clear that the term in square parentheses in Since the parameter is connected to the average of Eq. (A12) tends to ðx yÞ for ! 1. Again, replacing Rthe state (A11), it is clear that the maximally entangled state ji with ji in Eq. (7), and taking 1, we reobtain the dxjxijxi obtained from ji with ! 1 requires infinite same result apart from an inconsequential multiplication energy, and is unphysical. However, it is possible to approach factor ð1 2Þ2. it arbitrarily closely devoting sufficient energy to the task.

[1] K. Go¨del, Rev. Mod. Phys. 21, 447 (1949). [26] B. Coecke, arXiv:quant-ph/0402014v2. [2] W. B. Bonnor, J. Phys. A 13, 2121 (1980). [27] T. C. Ralph, arXiv:quant-ph/0510038v1. [3] J. R. Gott, Phys. Rev. Lett. 66, 1126 (1991). [28] G. Svetlichny, arXiv:0902.4898. [4] A. Einstein, in Albert Einstein, Philosopher-Scientist: The [29] G. Chiribella, G. M. D’Ariano, P. Perinotti, and B. Valiron, Library of Living Philosophers Volume VII, edited by P. A. arXiv:0912.0195. Schilpp (Open Court, Chicago, 1998), 3rd ed.. [30] Cˇ . Brukner, J.-W. Pan, C. Simon, G. Weihs, and A. [5] M. S. Morris, K. S. Thorne, and U. Yurtsever, Phys. Rev. Zeilinger, Phys. Rev. A 67, 034304 (2003). Lett. 61, 1446 (1988). [31] D. M. Greenberger and K. Svozil, in Quo Vadis Quantum [6] H. D. Politzer, Phys. Rev. D 49, 3981 (1994). Mechanics?, edited by A. Elitzur, S. Dolev, and N. [7] D. G. Boulware, Phys. Rev. D 46, 4421 (1992). Kolenda (Springer, Berlin, 2005); in Between Chance [8] J. B. Hartle, Phys. Rev. D 49, 6543 (1994). and Choice, edited by H. Atmanspacher and R. Bishop [9] W. J. van Stockum, Proc. R. Soc. Edinburgh A 57, 135 (Imprint Academic, Thorverton England, 2002), (1937). pp. 293–308. [10] H. D. Politzer, Phys. Rev. D 46, 4470 (1992). [32] H. K. Lee, arXiv:1101.1927v1. [11] D. Deutsch, Phys. Rev. D 44, 3197 (1991). [33] N. D. Birrell and P.C. W. Davies, Quantum Fields in [12] C. Lanczos, Z. Phys. 21, 73 (1924). Curved Space (Cambridge University Press, Cambridge, [13] S. W. Hawking, Phys. Rev. D 46, 603 (1992). 1982). [14] S. Deser, R. Jackiw, and G.’t Hooft, Phys. Rev. Lett. 68, [34] J. Friedman, M. S. Morris, I. D. Novikov, F. Echeverria, G. 267 (1992). Klinkhammer, K. S. Thorne, and U. Yurtsever, Phys. Rev. [15] S. M. Carroll, E. Farhi, A. H. Guth, and K. D. Olum, Phys. D 42, 1915 (1990). Rev. D 50, 6190 (1994). [35] J. L. Friedman, N. J. Papastamatiou, and J. Z. Simon, Phys. [16] S. Liberati, S. Sonego, and M. Visser, Ann. Phys. (N.Y.) Rev. D 46, 4456 (1992). 298, 167 (2002). [36] J. L. Friedman and M. S. Morris, Phys. Rev. Lett. 66, 401 [17] R. Feynman, in Nobel Lectures, Physics 1963–1970 (1991). (Elsevier Publishing Company, Amsterdam, 1972). [37] P. F. Gonza´lez-Dı´az, Phys. Rev. D 58, 124011 (1998). [18] S. Lloyd, L. Maccone, R. Garcia-Patron, V. Giovannetti, [38] T. C. Ralph, Phys. Rev. A 76, 012336 (2007). Y. Shikano, S. Pirandola, L. A. Rozema, A. Darabi, Y. [39] T. C. Ralph, G. J. Milburn, and T. Downes, Phys. Rev. A Soudagar, L. K. Shalm, and A. M. Steinberg, Phys. Rev. 79, 022121 (2009). Lett. 106, 040403 (2011). [40] C. H. Bennett, D. Leung, G. Smith, and J. A. Smolin, Phys. [19] G. T. Horowitz and J. Maldacena, J. High Energy Phys. 02 Rev. Lett. 103, 170502 (2009). (2004) 8. [41] T. C. Ralph and C. R. Myers, Phys. Rev. A 82, 062330 [20] U. Yurtsever and G. Hockney, Classical (2010). 22, 295 (2005). [42] More precisely, the evolution may take place even when [21] D. Gottesman and J. Preskill, J. High Energy Phys. 03 the right-hand side tends to zero, if the proportionality (2004) 26. constant tends to zero in such a way that the total limit is a [22] S. Lloyd, Phys. Rev. Lett. 96, 061302 (2006). valid state; see the Appendix. [23] D. T. Pegg, in Time’s Arrows, Quantum Measurement and [43] C. H. Bennett, G. Brassard, C. Cre´peau, R. Jozsa, A. Peres, Superluminal Behaviour, edited by D. Mugnai et al. and W. K. Wootters, Phys. Rev. Lett. 70, 1895 (Consiglio Nazionale delle Richerche, Roma, 2001), p. 113. (1993). [24] C. H. Bennett and B. Schumacher, lecture at QUPON [44] S. L. Braunstein and H. J. Kimble, Phys. Rev. Lett. 80, 869 conference Vienna, Austria May 2005 http://www (1998). .research.ibm.com/people/b/bennetc/QUPONBshort.pdf; [45] D. Bacon, Phys. Rev. A 70, 032309 (2004). lecture at Tata Institute for Fundamental Research, [46] T. A. Brun, J. Harrington, and M. M. Wilde, Phys. Rev. Mumbai, India, February 2002 archived Aug 2003 at Lett. 102, 210402 (2009). http://web.archive.org/web/20030809140213/http://qpip- [47] S. Aaronson and J. Watrous, Proc. R. Soc. A 465, 631 server.tcs.tifr.res.in/~qpip/HTML/Courses/Bennett/TIFR5 (2009); arXiv:0808.2669. .pdf. [48] S. Aaronson, Proc. R. Soc. A 461, 3473 (2005); arXiv: [25] M. Laforest, J. Baugh, and R. Laflamme, Phys. Rev. A 73, quant-ph/0412187. 032323 (2006). [49] T. A. Brun, Found. Phys. Lett. 16, 245 (2003).

025007-10 QUANTUM MECHANICS OF TIME TRAVEL THROUGH ... PHYSICAL REVIEW D 84, 025007 (2011) [50] R. P. Feynman and A. R. Hibbs, Quantum Mechanics and I. L. Egusquiza (Springer, Berlin, 2001), p. 399; arXiv: Path Integrals (McGraw-Hill, New York, 1965). quant-ph/0105101. [51] R. P. Feynman, Rev. Mod. Phys. 20, 367 (1948). [57] Y. Aharonov, P.G. Bergmann, and J. L. Lebowitz, Phys. [52] F. Echeverria, G. Klinkhammer, and K. S. Thorne, Phys. Rev. 134, B1410 (1964). Rev. D 44, 1077 (1991). [58] Y. Aharonov, D. Z. Albert, and L. Vaidman, Phys. Rev. [53] A. Einstein, B. Podolsky, and N. Rosen, Phys. Rev. 47, 777 Lett. 60, 1351 (1988). (1935). [59] M. J. Cassidy, Phys. Rev. D 52, 5676 (1995). [54] Y. Shikano and A. Hosoya, J. Phys. A 43, 025304 [60] A. Anderson, Phys. Rev. D 51, 5707 (1995). (2010). [61] C. J. Fewster and C. G. Wells, Phys. Rev. D 52, 5773 [55] G. Chiribella, G. M. D’Ariano, and P. Perinotti, Phys. Rev. (1995). A 80, 022339 (2009). [62] D. S. Abrams and S. Lloyd, Phys. Rev. Lett. 81, 3992 [56] Y. Aharonov and L. Vaidman, in Time in Quantum (1998). Mechanics, edited by J. G. Muga, R. Sala Mayato, and [63] U. Yurtsever, Classical Quantum Gravity 11, 999 (1994).

025007-11