Closed Timelike Curves Make Quantum and Classical Computing Equivalent
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Limits on Efficient Computation in the Physical World
Limits on Efficient Computation in the Physical World by Scott Joel Aaronson Bachelor of Science (Cornell University) 2000 A dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in Computer Science in the GRADUATE DIVISION of the UNIVERSITY of CALIFORNIA, BERKELEY Committee in charge: Professor Umesh Vazirani, Chair Professor Luca Trevisan Professor K. Birgitta Whaley Fall 2004 The dissertation of Scott Joel Aaronson is approved: Chair Date Date Date University of California, Berkeley Fall 2004 Limits on Efficient Computation in the Physical World Copyright 2004 by Scott Joel Aaronson 1 Abstract Limits on Efficient Computation in the Physical World by Scott Joel Aaronson Doctor of Philosophy in Computer Science University of California, Berkeley Professor Umesh Vazirani, Chair More than a speculative technology, quantum computing seems to challenge our most basic intuitions about how the physical world should behave. In this thesis I show that, while some intuitions from classical computer science must be jettisoned in the light of modern physics, many others emerge nearly unscathed; and I use powerful tools from computational complexity theory to help determine which are which. In the first part of the thesis, I attack the common belief that quantum computing resembles classical exponential parallelism, by showing that quantum computers would face serious limitations on a wider range of problems than was previously known. In partic- ular, any quantum algorithm that solves the collision problem—that of deciding whether a sequence of n integers is one-to-one or two-to-one—must query the sequence Ω n1/5 times. -
Summer 2017 Astron 9 Week 5 Final Version
RELATIVITY OF SPACE AND TIME IN POPULAR SCIENCE RICHARD ANANTUA PREDESTINATION (MON JUL 31) REVIEW OF JUL 24, 26 & 28 • Flying atomic clocks, muon decay, light bending around stars and gravitational waves provide experimental confirmation of relativity • In 1919, Einstein’s prediction for the deflection of starlight was confirmed by • The 1971 Hafele-Keating experiment confirmed • The 1977 CERN muon experiment confirmed • In 2016 LIGO confirmed the existence of REVIEW OF JUL 24, 26 & 28 • Flying atomic clocks, muon decay, light bending around stars and gravitational waves provide experimental confirmation of relativity • In 1919, Einstein’s prediction for the deflection of starlight was confirmed by Sir Arthur Eddington • The 1971 Hafele-Keating experiment confirmed motional and gravitational time dilation • The 1977 CERN muon experiment confirmed motional time dilation • In 2016 LIGO confirmed the existence of gravitational waves TIME TRAVEL IN RELATIVITY • Methods of time travel theoretically possible in relativity are • (Apparently) faster than light travel – window into the past? • Closed timelike curved • (Apparent) paradoxes with time travel • Kill your grandfather – past time travel may alter seemingly necessary conditions for the future time traveler to have started the journey • Predestination - apparent cause of past event is in the future SPECIAL RELATIVISTIC VELOCITY ADDITION • In special relativity, no object or information can travel faster than light, a fact reflected in the relativistic law of composition of velocities v &v vAB v = $% %' A !" v$%v%' (& * ) vBC B C • vAB is the (1D) velocity of A with respect to B • vBC is the (1D) velocity of B with respect to C POP QUIZ - FASTER THAN LIGHT TRAVEL • A spaceship traveling at v>c is returning from a moving planet (L0 away right before the journey). -
Light Rays, Singularities, and All That
Light Rays, Singularities, and All That Edward Witten School of Natural Sciences, Institute for Advanced Study Einstein Drive, Princeton, NJ 08540 USA Abstract This article is an introduction to causal properties of General Relativity. Topics include the Raychaudhuri equation, singularity theorems of Penrose and Hawking, the black hole area theorem, topological censorship, and the Gao-Wald theorem. The article is based on lectures at the 2018 summer program Prospects in Theoretical Physics at the Institute for Advanced Study, and also at the 2020 New Zealand Mathematical Research Institute summer school in Nelson, New Zealand. Contents 1 Introduction 3 2 Causal Paths 4 3 Globally Hyperbolic Spacetimes 11 3.1 Definition . 11 3.2 Some Properties of Globally Hyperbolic Spacetimes . 15 3.3 More On Compactness . 18 3.4 Cauchy Horizons . 21 3.5 Causality Conditions . 23 3.6 Maximal Extensions . 24 4 Geodesics and Focal Points 25 4.1 The Riemannian Case . 25 4.2 Lorentz Signature Analog . 28 4.3 Raychaudhuri’s Equation . 31 4.4 Hawking’s Big Bang Singularity Theorem . 35 5 Null Geodesics and Penrose’s Theorem 37 5.1 Promptness . 37 5.2 Promptness And Focal Points . 40 5.3 More On The Boundary Of The Future . 46 1 5.4 The Null Raychaudhuri Equation . 47 5.5 Trapped Surfaces . 52 5.6 Penrose’s Theorem . 54 6 Black Holes 58 6.1 Cosmic Censorship . 58 6.2 The Black Hole Region . 60 6.3 The Horizon And Its Generators . 63 7 Some Additional Topics 66 7.1 Topological Censorship . 67 7.2 The Averaged Null Energy Condition . -
Computational Pseudorandomness, the Wormhole Growth Paradox, and Constraints on the Ads/CFT Duality
Computational Pseudorandomness, the Wormhole Growth Paradox, and Constraints on the AdS/CFT Duality Adam Bouland Department of Electrical Engineering and Computer Sciences, University of California, Berkeley, 617 Soda Hall, Berkeley, CA 94720, U.S.A. [email protected] Bill Fefferman Department of Computer Science, University of Chicago, 5730 S Ellis Ave, Chicago, IL 60637, U.S.A. [email protected] Umesh Vazirani Department of Electrical Engineering and Computer Sciences, University of California, Berkeley, 671 Soda Hall, Berkeley, CA 94720, U.S.A. [email protected] Abstract The AdS/CFT correspondence is central to efforts to reconcile gravity and quantum mechanics, a fundamental goal of physics. It posits a duality between a gravitational theory in Anti de Sitter (AdS) space and a quantum mechanical conformal field theory (CFT), embodied in a map known as the AdS/CFT dictionary mapping states to states and operators to operators. This dictionary map is not well understood and has only been computed on special, structured instances. In this work we introduce cryptographic ideas to the study of AdS/CFT, and provide evidence that either the dictionary must be exponentially hard to compute, or else the quantum Extended Church-Turing thesis must be false in quantum gravity. Our argument has its origins in a fundamental paradox in the AdS/CFT correspondence known as the wormhole growth paradox. The paradox is that the CFT is believed to be “scrambling” – i.e. the expectation value of local operators equilibrates in polynomial time – whereas the gravity theory is not, because the interiors of certain black holes known as “wormholes” do not equilibrate and instead their volume grows at a linear rate for at least an exponential amount of time. -
NP-Complete Problems and Physical Reality
NP-complete Problems and Physical Reality Scott Aaronson∗ Abstract Can NP-complete problems be solved efficiently in the physical universe? I survey proposals including soap bubbles, protein folding, quantum computing, quantum advice, quantum adia- batic algorithms, quantum-mechanical nonlinearities, hidden variables, relativistic time dilation, analog computing, Malament-Hogarth spacetimes, quantum gravity, closed timelike curves, and “anthropic computing.” The section on soap bubbles even includes some “experimental” re- sults. While I do not believe that any of the proposals will let us solve NP-complete problems efficiently, I argue that by studying them, we can learn something not only about computation but also about physics. 1 Introduction “Let a computer smear—with the right kind of quantum randomness—and you create, in effect, a ‘parallel’ machine with an astronomical number of processors . All you have to do is be sure that when you collapse the system, you choose the version that happened to find the needle in the mathematical haystack.” —From Quarantine [31], a 1992 science-fiction novel by Greg Egan If I had to debate the science writer John Horgan’s claim that basic science is coming to an end [48], my argument would lean heavily on one fact: it has been only a decade since we learned that quantum computers could factor integers in polynomial time. In my (unbiased) opinion, the showdown that quantum computing has forced—between our deepest intuitions about computers on the one hand, and our best-confirmed theory of the physical world on the other—constitutes one of the most exciting scientific dramas of our time. -
Quantum Lower Bound for Recursive Fourier Sampling
Quantum Lower Bound for Recursive Fourier Sampling Scott Aaronson Institute for Advanced Study, Princeton [email protected] Abstract One of the earliest quantum algorithms was discovered by Bernstein and Vazirani, for a problem called Recursive Fourier Sampling. This paper shows that the Bernstein-Vazirani algorithm is not far from optimal. The moral is that the need to “uncompute” garbage can impose a fundamental limit on efficient quantum computation. The proof introduces a new parameter of Boolean functions called the “nonparity coefficient,” which might be of independent interest. Like a classical algorithm, a quantum algorithm can solve problems recursively by calling itself as a sub- routine. When this is done, though, the algorithm typically needs to call itself twice for each subproblem to be solved. The second call’s purpose is to uncompute ‘garbage’ left over by the first call, and thereby enable interference between different branches of the computation. Of course, a factor of 2 increase in running time hardly seems like a big deal, when set against the speedups promised by quantum computing. The problem is that these factors of 2 multiply, with each level of recursion producing an additional factor. Thus, one might wonder whether the uncomputing step is really necessary, or whether a cleverly designed algorithm might avoid it. This paper gives the first nontrivial example in which recursive uncomputation is provably necessary. The example concerns a long-neglected problem called Recursive Fourier Sampling (henceforth RFS), which was introduced by Bernstein and Vazirani [5] in 1993 to prove the first oracle separation between BPP and BQP. Many surveys on quantum computing pass directly from the Deutsch-Jozsa algorithm [8] to the dramatic results of Simon [14] and Shor [13], without even mentioning RFS. -
Quantum Fluctuations and Thermodynamic Processes in The
Quantum fluctuations and thermodynamic processes in the presence of closed timelike curves by Tsunefumi Tanaka A thesis submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Physics Montana State University © Copyright by Tsunefumi Tanaka (1997) Abstract: A closed timelike curve (CTC) is a closed loop in spacetime whose tangent vector is everywhere timelike. A spacetime which contains CTC’s will allow time travel. One of these spacetimes is Grant space. It can be constructed from Minkowski space by imposing periodic boundary conditions in spatial directions and making the boundaries move toward each other. If Hawking’s chronology protection conjecture is correct, there must be a physical mechanism preventing the formation of CTC’s. Currently the most promising candidate for the chronology protection mechanism is the back reaction of the metric to quantum vacuum fluctuations. In this thesis the quantum fluctuations for a massive scalar field, a self-interacting field, and for a field at nonzero temperature are calculated in Grant space. The stress-energy tensor is found to remain finite everywhere in Grant space for the massive scalar field with sufficiently large field mass. Otherwise it diverges on chronology horizons like the stress-energy tensor for a massless scalar field. If CTC’s exist they will have profound effects on physical processes. Causality can be protected even in the presence of CTC’s if the self-consistency condition is imposed on all processes. Simple classical thermodynamic processes of a box filled with ideal gas in the presence of CTC’s are studied. If a system of boxes is closed, its state does not change as it travels through a region of spacetime with CTC’s. -
Cosmic String Lensing and Closed Timelike Curves
PHYSICAL REVIEW D 72, 043532 (2005) Cosmic string lensing and closed timelike curves Benjamin Shlaer* and S.-H. Henry Tye† Laboratory for Elementary Particle Physics, Cornell University, Ithaca, New York 14853, USA (Received 3 March 2005; revised manuscript received 21 July 2005; published 31 August 2005) In an analysis of the gravitational lensing by two relativistic cosmic strings, we argue that the formation of closed timelike curves proposed by Gott is unstable in the presence of particles (e.g. the cosmic microwave background radiation). Because of the attractorlike behavior of the closed timelike curve, we argue that this instability is very generic. A single graviton or photon in the vicinity, no matter how soft, is sufficient to bend the strings and prevent the formation of closed timelike curves. We also show that the gravitational lensing due to a moving cosmic string is enhanced by its motion, not suppressed. DOI: 10.1103/PhysRevD.72.043532 PACS numbers: 98.80.Cq, 04.20.Gz, 04.60.Kz, 11.27.+d I. INTRODUCTION strings in the sense opposite to their motion becomes a CTC. This is sometimes called the Gott spacetime or Gott Although cosmic strings as the seed of structure forma- time machine. tion [1] has been ruled out by observations, their presence Although there is no proof that a time machine cannot at a lower level is still possible. Indeed, cosmic strings are exist in our world [13], their puzzling causal nature leads generically present in brane inflation in superstring theory, many physicists to believe that CTCs cannot be formed. and their properties are close to, but within all observatio- This skepticism has been encoded in Hawking’s chronol- nal bounds [2–7]. -
Closed Timelike Curves Via Postselection: Theory and Experimental Test of Consistency
Closed Timelike Curves via Postselection: Theory and Experimental Test of Consistency The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Lloyd, Seth, et al. "Closed Timelike Curves via Postselection: Theory and Experimental Test of Consistency." American Physical Society, 2011, 106:4, © 2011 The American Physical Society. As Published http://dx.doi.org/10.1103/PhysRevLett.106.040403 Publisher American Physical Society Version Final published version Citable link http://hdl.handle.net/1721.1/63096 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. week ending PRL 106, 040403 (2011) PHYSICAL REVIEW LETTERS 28 JANUARY 2011 Closed Timelike Curves via Postselection: Theory and Experimental Test of Consistency Seth Lloyd,1 Lorenzo Maccone,1 Raul Garcia-Patron,1 Vittorio Giovannetti,2 Yutaka Shikano,1,3 Stefano Pirandola,1 Lee A. Rozema,4 Ardavan Darabi,4 Yasaman Soudagar,4 Lynden K. Shalm,4 and Aephraim M. Steinberg4 1xQIT, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, Massachusetts 02139-4307, USA 2NEST-CNR-INFM & Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126, Pisa, Italy 3Department of Physics, Tokyo Institute of Technology, 2-12-1 Oh-Okayama, Meguro, Tokyo, 152-8551, Japan 4CQIQC, IOS, Department of Physics, University of Toronto, Canada M5S 1A7 (Received 12 May 2010; revised manuscript received 22 November 2010; published 27 January 2011) Closed timelike curves (CTCs) are trajectories in spacetime that effectively travel backwards in time: a test particle following a CTC can interact with its former self in the past. -
Causality Violation and Singularities
TIT/HEP-302/COSMO-59 October, 1995 Causality violation and singularities Kengo Maeda 1 and Akihiro Ishibashi 2 Department of Physics, Tokyo Institute of Technology, Oh-Okayama Meguro-ku, Tokyo 152, Japan ABSTRACT We show that singularities necessarily occur when a boundary of causality violating set exists in a space-time under the physically suitable assumptions except the global causality condition in the Hawking-Penrose singularity theo- rems. Instead of the global causality condition, we impose some restrictions on the causality violating sets to show the occurrence of singularities. 1 Introduction Space-time singularities have been discussed for a long time in general relativity. In 1970, Hawking and Penrose[1] showed that singularities, which mean causal arXiv:gr-qc/9606075v1 27 Jun 1996 geodesic incompleteness, could occur in a space-time under seemingly reasonable conditions in classical gravity. Their singularity theorem has an important impli- cation that our universe has an initial singularity if we do not consider quantum effects. However, this theorem is physically unsatisfactory in the sense that the causality requirement everywhere in a space-time seems too restrictive. We can only experience local events and there is no guarantee that the causality holds in the entire universe. As is well known, Kerr type black holes have causality violating sets if the space-time is maximally extended. Therefore, it will be im- portant to investigate occurrence of singularities in a space-time in which the global causality condition is violated. There are some works on a causality violation concerned with the occurrence of singularity. Tipler[2,3] showed that any attempt to evolve closed timelike curves from an initial regular Cauchy data would cause singularities to form in a 1e-mail:[email protected] 2e-mail:[email protected] 1 space-time. -
Arxiv:0710.4474V1 [Gr-Qc] 24 Oct 2007 I.“Apdie Pctmsadspruia Travel Superluminal and Spacetimes Drive” “Warp III
Exotic solutions in General Relativity: Traversable wormholes and “warp drive” spacetimes Francisco S. N. Lobo∗ Centro de Astronomia e Astrof´ısica da Universidade de Lisboa, Campo Grande, Ed. C8 1749-016 Lisboa, Portugal and Institute of Gravitation & Cosmology, University of Portsmouth, Portsmouth PO1 2EG, UK (Dated: February 2, 2008) The General Theory of Relativity has been an extremely successful theory, with a well established experimental footing, at least for weak gravitational fields. Its predictions range from the existence of black holes, gravitational radiation to the cosmological models, predicting a primordial beginning, namely the big-bang. All these solutions have been obtained by first considering a plausible distri- bution of matter, i.e., a plausible stress-energy tensor, and through the Einstein field equation, the spacetime metric of the geometry is determined. However, one may solve the Einstein field equa- tion in the reverse direction, namely, one first considers an interesting and exotic spacetime metric, then finds the matter source responsible for the respective geometry. In this manner, it was found that some of these solutions possess a peculiar property, namely “exotic matter,” involving a stress- energy tensor that violates the null energy condition. These geometries also allow closed timelike curves, with the respective causality violations. Another interesting feature of these spacetimes is that they allow “effective” superluminal travel, although, locally, the speed of light is not surpassed. These solutions are primarily useful as “gedanken-experiments” and as a theoretician’s probe of the foundations of general relativity, and include traversable wormholes and superluminal “warp drive” spacetimes. Thus, one may be tempted to denote these geometries as “exotic” solutions of the Einstein field equation, as they violate the energy conditions and generate closed timelike curves. -
The Power of Unentanglement
The Power of Unentanglement Scott Aaronson∗ Salman Beigi Andrew Drucker Bill Fefferman MIT MIT MIT University of Chicago Peter Shor MIT Abstract The class QMA (k), introduced by Kobayashi et al., consists of all languages that can be verified using k unentangled quantum proofs. Many of the simplest questions about this class have remained embarrassingly open: for example, can we give any evidence that k quantum proofs are more powerful than one? Does QMA (k) = QMA (2) for k 2? Can QMA (k) protocols be amplified to exponentially small error? ≥ In this paper, we make progress on all of the above questions. We give a protocol by which a verifier can be convinced that a 3Sat formula of size m is • satisfiable, with constant soundness, given O (√m) unentangled quantum witnesses with O (log m) qubits each. Our protocol relies on the existence of very short PCPs. We show that assuming a weak version of thee Additivity Conjecture from quantum infor- • mation theory, any QMA (2) protocol can be amplified to exponentially small error, and QMA (k)= QMA (2) for all k 2. ≥ We prove the nonexistence of “perfect disentanglers” for simulating multiple Merlins with • one. 1 Introduction Quantum entanglement is often described as a complicated, hard-to-understand resource. But ironically, many questions in quantum computing are easiest to answer assuming unlimited entan- glement, and become much more difficult if entanglement is not allowed! One way to understand this is that Hilbert space—the space of all quantum states—has extremely useful linear-algebraic properties, and when we restrict to the set of separable states we lose many of those properties.