Realism About the Wave Function
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Simulating Quantum Field Theory with a Quantum Computer
Simulating quantum field theory with a quantum computer John Preskill Lattice 2018 28 July 2018 This talk has two parts (1) Near-term prospects for quantum computing. (2) Opportunities in quantum simulation of quantum field theory. Exascale digital computers will advance our knowledge of QCD, but some challenges will remain, especially concerning real-time evolution and properties of nuclear matter and quark-gluon plasma at nonzero temperature and chemical potential. Digital computers may never be able to address these (and other) problems; quantum computers will solve them eventually, though I’m not sure when. The physics payoff may still be far away, but today’s research can hasten the arrival of a new era in which quantum simulation fuels progress in fundamental physics. Frontiers of Physics short distance long distance complexity Higgs boson Large scale structure “More is different” Neutrino masses Cosmic microwave Many-body entanglement background Supersymmetry Phases of quantum Dark matter matter Quantum gravity Dark energy Quantum computing String theory Gravitational waves Quantum spacetime particle collision molecular chemistry entangled electrons A quantum computer can simulate efficiently any physical process that occurs in Nature. (Maybe. We don’t actually know for sure.) superconductor black hole early universe Two fundamental ideas (1) Quantum complexity Why we think quantum computing is powerful. (2) Quantum error correction Why we think quantum computing is scalable. A complete description of a typical quantum state of just 300 qubits requires more bits than the number of atoms in the visible universe. Why we think quantum computing is powerful We know examples of problems that can be solved efficiently by a quantum computer, where we believe the problems are hard for classical computers. -
Synopsis of a Unified Theory for All Forces and Matter
Synopsis of a Unified Theory for All Forces and Matter Zeng-Bing Chen National Laboratory of Solid State Microstructures, School of Physics, Nanjing University, Nanjing 210093, China (Dated: December 20, 2018) Assuming the Kaluza-Klein gravity interacting with elementary matter fermions in a (9 + 1)- dimensional spacetime (M9+1), we propose an information-complete unified theory for all forces and matter. Due to entanglement-driven symmetry breaking, the SO(9, 1) symmetry of M9+1 is broken to SO(3, 1) × SO(6), where SO(3, 1) [SO(6)] is associated with gravity (gauge fields of matter fermions) in (3+1)-dimensional spacetime (M3+1). The informational completeness demands that matter fermions must appear in three families, each having 16 independent matter fermions. Meanwhile, the fermion family space is equipped with elementary SO(3) gauge fields in M9+1, giving rise to the Higgs mechanism in M3+1 through the gauge-Higgs unification. After quantum compactification of six extra dimensions, a trinity—the quantized gravity, the three-family fermions of total number 48, and their SO(6) and SO(3) gauge fields—naturally arises in an effective theory in M3+1. Possible routes of our theory to the Standard Model are briefly discussed. PACS numbers: 04.50.+h, 12.10.-g, 04.60.Pp The tendency of unifying originally distinct physical fields (together as matter), a fact called the information- subjects or phenomena has profoundly advanced modern completeness principle (ICP). The basic state-dynamics physics. Newton’s law of universal gravitation, Maxwell’s postulate [8] is that the Universe is self-created into a theory of electromagnetism, and Einstein’s relativity state |e,ω; A..., ψ...i of all physical contents (spacetime theory are among the most outstanding examples for and matter), from no spacetime and no matter, with the such a unification. -
Prediction in Quantum Cosmology
Prediction in Quantum Cosmology James B. Hartle Department of Physics University of California Santa Barbara, CA 93106, USA Lectures at the 1986 Carg`esesummer school publshed in Gravitation in As- trophysics ed. by J.B. Hartle and B. Carter, Plenum Press, New York (1987). In this version some references that were `to be published' in the original have been supplied, a few typos corrected, but the text is otherwise unchanged. The author's views on the quantum mechanics of cosmology have changed in important ways from those originally presented in Section 2. See, e.g. [107] J.B. Hartle, Spacetime Quantum Mechanics and the Quantum Mechan- ics of Spacetime in Gravitation and Quantizations, Proceedings of the 1992 Les Houches Summer School, ed. by B. Julia and J. Zinn-Justin, Les Houches Summer School Proceedings Vol. LVII, North Holland, Amsterdam (1995).) The general discussion and material in Sections 3 and 4 on the classical geom- etry limit and the approximation of quantum field theory in curved spacetime may still be of use. 1 Introduction As far as we know them, the fundamental laws of physics are quantum mechanical in nature. If these laws apply to the universe as a whole, then there must be a description of the universe in quantum mechancial terms. Even our present cosmological observations require such a description in principle, although in practice these observations are so limited and crude that the approximation of classical physics is entirely adequate. In the early universe, however, the classical approximation is unlikely to be valid. There, towards the big bang singularity, at curvatures characterized by the Planck length, 3 1 (¯hG=c ) 2 , quantum fluctuations become important and eventually dominant. -
Analysis of Nonlinear Dynamics in a Classical Transmon Circuit
Analysis of Nonlinear Dynamics in a Classical Transmon Circuit Sasu Tuohino B. Sc. Thesis Department of Physical Sciences Theoretical Physics University of Oulu 2017 Contents 1 Introduction2 2 Classical network theory4 2.1 From electromagnetic fields to circuit elements.........4 2.2 Generalized flux and charge....................6 2.3 Node variables as degrees of freedom...............7 3 Hamiltonians for electric circuits8 3.1 LC Circuit and DC voltage source................8 3.2 Cooper-Pair Box.......................... 10 3.2.1 Josephson junction.................... 10 3.2.2 Dynamics of the Cooper-pair box............. 11 3.3 Transmon qubit.......................... 12 3.3.1 Cavity resonator...................... 12 3.3.2 Shunt capacitance CB .................. 12 3.3.3 Transmon Lagrangian................... 13 3.3.4 Matrix notation in the Legendre transformation..... 14 3.3.5 Hamiltonian of transmon................. 15 4 Classical dynamics of transmon qubit 16 4.1 Equations of motion for transmon................ 16 4.1.1 Relations with voltages.................. 17 4.1.2 Shunt resistances..................... 17 4.1.3 Linearized Josephson inductance............. 18 4.1.4 Relation with currents................... 18 4.2 Control and read-out signals................... 18 4.2.1 Transmission line model.................. 18 4.2.2 Equations of motion for coupled transmission line.... 20 4.3 Quantum notation......................... 22 5 Numerical solutions for equations of motion 23 5.1 Design parameters of the transmon................ 23 5.2 Resonance shift at nonlinear regime............... 24 6 Conclusions 27 1 Abstract The focus of this thesis is on classical dynamics of a transmon qubit. First we introduce the basic concepts of the classical circuit analysis and use this knowledge to derive the Lagrangians and Hamiltonians of an LC circuit, a Cooper-pair box, and ultimately we derive Hamiltonian for a transmon qubit. -
Path Integrals in Quantum Mechanics
Path Integrals in Quantum Mechanics Emma Wikberg Project work, 4p Department of Physics Stockholm University 23rd March 2006 Abstract The method of Path Integrals (PI’s) was developed by Richard Feynman in the 1940’s. It offers an alternate way to look at quantum mechanics (QM), which is equivalent to the Schrödinger formulation. As will be seen in this project work, many "elementary" problems are much more difficult to solve using path integrals than ordinary quantum mechanics. The benefits of path integrals tend to appear more clearly while using quantum field theory (QFT) and perturbation theory. However, one big advantage of Feynman’s formulation is a more intuitive way to interpret the basic equations than in ordinary quantum mechanics. Here we give a basic introduction to the path integral formulation, start- ing from the well known quantum mechanics as formulated by Schrödinger. We show that the two formulations are equivalent and discuss the quantum mechanical interpretations of the theory, as well as the classical limit. We also perform some explicit calculations by solving the free particle and the harmonic oscillator problems using path integrals. The energy eigenvalues of the harmonic oscillator is found by exploiting the connection between path integrals, statistical mechanics and imaginary time. Contents 1 Introduction and Outline 2 1.1 Introduction . 2 1.2 Outline . 2 2 Path Integrals from ordinary Quantum Mechanics 4 2.1 The Schrödinger equation and time evolution . 4 2.2 The propagator . 6 3 Equivalence to the Schrödinger Equation 8 3.1 From the Schrödinger equation to PI’s . 8 3.2 From PI’s to the Schrödinger equation . -
Relativistic Quantum Mechanics 1
Relativistic Quantum Mechanics 1 The aim of this chapter is to introduce a relativistic formalism which can be used to describe particles and their interactions. The emphasis 1.1 SpecialRelativity 1 is given to those elements of the formalism which can be carried on 1.2 One-particle states 7 to Relativistic Quantum Fields (RQF), which underpins the theoretical 1.3 The Klein–Gordon equation 9 framework of high energy particle physics. We begin with a brief summary of special relativity, concentrating on 1.4 The Diracequation 14 4-vectors and spinors. One-particle states and their Lorentz transforma- 1.5 Gaugesymmetry 30 tions follow, leading to the Klein–Gordon and the Dirac equations for Chaptersummary 36 probability amplitudes; i.e. Relativistic Quantum Mechanics (RQM). Readers who want to get to RQM quickly, without studying its foun- dation in special relativity can skip the first sections and start reading from the section 1.3. Intrinsic problems of RQM are discussed and a region of applicability of RQM is defined. Free particle wave functions are constructed and particle interactions are described using their probability currents. A gauge symmetry is introduced to derive a particle interaction with a classical gauge field. 1.1 Special Relativity Einstein’s special relativity is a necessary and fundamental part of any Albert Einstein 1879 - 1955 formalism of particle physics. We begin with its brief summary. For a full account, refer to specialized books, for example (1) or (2). The- ory oriented students with good mathematical background might want to consult books on groups and their representations, for example (3), followed by introductory books on RQM/RQF, for example (4). -
Quantum Mechanics in 1-D Potentials
MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Electrical Engineering and Computer Science 6.007 { Electromagnetic Energy: From Motors to Lasers Spring 2011 Tutorial 10: Quantum Mechanics in 1-D Potentials Quantum mechanical model of the universe, allows us describe atomic scale behavior with great accuracy|but in a way much divorced from our perception of everyday reality. Are photons, electrons, atoms best described as particles or waves? Simultaneous wave-particle description might be the most accurate interpretation, which leads us to develop a mathe- matical abstraction. 1 Rules for 1-D Quantum Mechanics Our mathematical abstraction of choice is the wave function, sometimes denoted as , and it allows us to predict the statistical outcomes of experiments (i.e., the outcomes of our measurements) according to a few rules 1. At any given time, the state of a physical system is represented by a wave function (x), which|for our purposes|is a complex, scalar function dependent on position. The quantity ρ (x) = ∗ (x) (x) is a probability density function. Furthermore, is complete, and tells us everything there is to know about the particle. 2. Every measurable attribute of a physical system is represented by an operator that acts on the wave function. In 6.007, we're largely interested in position (x^) and momentum (p^) which have operator representations in the x-dimension @ x^ ! x p^ ! ~ : (1) i @x Outcomes of measurements are described by the expectation values of the operator Z Z @ hx^i = dx ∗x hp^i = dx ∗ ~ : (2) i @x In general, any dynamical variable Q can be expressed as a function of x and p, and we can find the expectation value of Z h @ hQ (x; p)i = dx ∗Q x; : (3) i @x 3. -
Spin Foam Vertex Amplitudes on Quantum Computer—Preliminary Results
universe Article Spin Foam Vertex Amplitudes on Quantum Computer—Preliminary Results Jakub Mielczarek 1,2 1 CPT, Aix-Marseille Université, Université de Toulon, CNRS, F-13288 Marseille, France; [email protected] 2 Institute of Physics, Jagiellonian University, Łojasiewicza 11, 30-348 Cracow, Poland Received: 16 April 2019; Accepted: 24 July 2019; Published: 26 July 2019 Abstract: Vertex amplitudes are elementary contributions to the transition amplitudes in the spin foam models of quantum gravity. The purpose of this article is to make the first step towards computing vertex amplitudes with the use of quantum algorithms. In our studies we are focused on a vertex amplitude of 3+1 D gravity, associated with a pentagram spin network. Furthermore, all spin labels of the spin network are assumed to be equal j = 1/2, which is crucial for the introduction of the intertwiner qubits. A procedure of determining modulus squares of vertex amplitudes on universal quantum computers is proposed. Utility of the approach is tested with the use of: IBM’s ibmqx4 5-qubit quantum computer, simulator of quantum computer provided by the same company and QX quantum computer simulator. Finally, values of the vertex probability are determined employing both the QX and the IBM simulators with 20-qubit quantum register and compared with analytical predictions. Keywords: Spin networks; vertex amplitudes; quantum computing 1. Introduction The basic objective of theories of quantum gravity is to calculate transition amplitudes between configurations of the gravitational field. The most straightforward approach to the problem is provided by the Feynman’s path integral Z i (SG+Sf) hY f jYii = D[g]D[f]e } , (1) where SG and Sf are the gravitational and matter actions respectively. -
Symmetry-Breaking and Zero-One Laws
version 1.2 Symmetry-breaking and zero-one laws Fay Dowker Perimeter Institute, 31 Caroline Street North, Waterloo ON, N2L 2Y5 Canada and Blackett Laboratory, Imperial College, Prince Consort Road, London SW7 2AZ, UK address for email: [email protected] and Rafael D. Sorkin Perimeter Institute, 31 Caroline Street North, Waterloo ON, N2L 2Y5 Canada and Raman Research Institute, C.V. Raman Avenue, Sadashivanagar, Bangalore { 560 080 India and Department of Physics, Syracuse University, Syracuse, NY 13244-1130, U.S.A. address for email: [email protected] Abstract We offer further evidence that discreteness of the sort inherent in a causal set cannot, in and of itself, serve to break Poincar´einvariance. In par- ticular we prove that a Poisson sprinkling of Minkowski spacetime can- not endow spacetime with a distinguished spatial or temporal orienta- tion, or with a distinguished lattice of spacetime points, or with a distin- guished lattice of timelike directions (corresponding respectively to break- ings of reflection-invariance, translation-invariance, and Lorentz invari- ance). Along the way we provide a proof from first principles of the zero- one law on which our new arguments are based. Keywords and phrases: discreteness, symmetry breaking, zero-one law, Poisson process, causal set, quantum gravity Introduction Will a discrete structure prove to be the kinematical basis of quantum gravity and if so should we expect it to preserve the known symmetries of Minkowski spacetime, at 1 least quasi-locally? One strand of thought has tended to answer these questions with \yes" followed by \no", and has held out effects like modified dispersion relations for electromagnetic waves as promising candidates for a phenomenology of spatiotemporal discreteness. -
Fourier Transformations & Understanding Uncertainty
Fourier Transformations & Understanding Uncertainty Uncertainty Relation: Fourier Analysis of Wave Packets Group 1: Brian Allgeier, Chris Browder, Brian Kim (7 December 2015) Introduction: In Quantum Mechanics, wave functions offer statistical information about possible results, not the exact outcome of an experiment. Two wave functions of interest are the position wave function and the momentum wave function; these wave functions represent the components of a state vector in the position basis and the momentum basis, respectively. These two can be related through the Fourier Transform and the Inverse Fourier Transform. This demonstration application will allow the users to define their own momentum wave function and use the inverse Fourier transformation to find the position wave function. If the Fourier transform were to be used on the resulting wave function, the result would then be the original momentum wave function. Both wave functions visually show the wave packets in momentum and position space. The momentum wave packet is a Gaussian while the corresponding position wave packet is a Gaussian envelope which contains an internal oscillatory wave. The two wave packets are related by the uncertainty principle, which states that the more defined (i.e. more localized) the wave function is in one basis, the less defined the corresponding wave function will be in the other basis. The application will also create an interactive 3-dimensional model that relates the two wave functions through the inverse Fourier transformation, or more specifically, by visually decomposing a Gaussian wave packet (in momentum space) into a specified number of components waves (in position space). Using this application will give the user a stronger knowledge of the relationship between the Fourier transform, inverse Fourier transform, and the relationship between wave packets in momentum space and position space as determined by the Uncertainty Principle. -
Informal Introduction to QM: Free Particle
Chapter 2 Informal Introduction to QM: Free Particle Remember that in case of light, the probability of nding a photon at a location is given by the square of the square of electric eld at that point. And if there are no sources present in the region, the components of the electric eld are governed by the wave equation (1D case only) ∂2u 1 ∂2u − =0 (2.1) ∂x2 c2 ∂t2 Note the features of the solutions of this dierential equation: 1. The simplest solutions are harmonic, that is u ∼ exp [i (kx − ωt)] where ω = c |k|. This function represents the probability amplitude of photons with energy ω and momentum k. 2. Superposition principle holds, that is if u1 = exp [i (k1x − ω1t)] and u2 = exp [i (k2x − ω2t)] are two solutions of equation 2.1 then c1u1 + c2u2 is also a solution of the equation 2.1. 3. A general solution of the equation 2.1 is given by ˆ ∞ u = A(k) exp [i (kx − ωt)] dk. −∞ Now, by analogy, the rules for matter particles may be found. The functions representing matter waves will be called wave functions. £ First, the wave function ψ(x, t)=A exp [i(px − Et)/] 8 represents a particle with momentum p and energy E = p2/2m. Then, the probability density function P (x, t) for nding the particle at x at time t is given by P (x, t)=|ψ(x, t)|2 = |A|2 . Note that the probability distribution function is independent of both x and t. £ Assume that superposition of the waves hold. -
Quantum Gravity: a Primer for Philosophers∗
Quantum Gravity: A Primer for Philosophers∗ Dean Rickles ‘Quantum Gravity’ does not denote any existing theory: the field of quantum gravity is very much a ‘work in progress’. As you will see in this chapter, there are multiple lines of attack each with the same core goal: to find a theory that unifies, in some sense, general relativity (Einstein’s classical field theory of gravitation) and quantum field theory (the theoretical framework through which we understand the behaviour of particles in non-gravitational fields). Quantum field theory and general relativity seem to be like oil and water, they don’t like to mix—it is fair to say that combining them to produce a theory of quantum gravity constitutes the greatest unresolved puzzle in physics. Our goal in this chapter is to give the reader an impression of what the problem of quantum gravity is; why it is an important problem; the ways that have been suggested to resolve it; and what philosophical issues these approaches, and the problem itself, generate. This review is extremely selective, as it has to be to remain a manageable size: generally, rather than going into great detail in some area, we highlight the key features and the options, in the hope that readers may take up the problem for themselves—however, some of the basic formalism will be introduced so that the reader is able to enter the physics and (what little there is of) the philosophy of physics literature prepared.1 I have also supplied references for those cases where I have omitted some important facts.