Fact and Folklore in Quantum Gravity∗
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Experimental Tests of Quantum Gravity and Exotic Quantum Field Theory Effects
Advances in High Energy Physics Experimental Tests of Quantum Gravity and Exotic Quantum Field Theory Effects Guest Editors: Emil T. Akhmedov, Stephen Minter, Piero Nicolini, and Douglas Singleton Experimental Tests of Quantum Gravity and Exotic Quantum Field Theory Effects Advances in High Energy Physics Experimental Tests of Quantum Gravity and Exotic Quantum Field Theory Effects Guest Editors: Emil T. Akhmedov, Stephen Minter, Piero Nicolini, and Douglas Singleton Copyright © 2014 Hindawi Publishing Corporation. All rights reserved. This is a special issue published in “Advances in High Energy Physics.” All articles are open access articles distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Editorial Board Botio Betev, Switzerland Ian Jack, UK Neil Spooner, UK Duncan L. Carlsmith, USA Filipe R. Joaquim, Portugal Luca Stanco, Italy Kingman Cheung, Taiwan Piero Nicolini, Germany EliasC.Vagenas,Kuwait Shi-Hai Dong, Mexico Seog H. Oh, USA Nikos Varelas, USA Edmond C. Dukes, USA Sandip Pakvasa, USA Kadayam S. Viswanathan, Canada Amir H. Fatollahi, Iran Anastasios Petkou, Greece Yau W. Wah, USA Frank Filthaut, The Netherlands Alexey A. Petrov, USA Moran Wang, China Joseph Formaggio, USA Frederik Scholtz, South Africa Gongnan Xie, China Chao-Qiang Geng, Taiwan George Siopsis, USA Hong-Jian He, China Terry Sloan, UK Contents Experimental Tests of Quantum Gravity and Exotic Quantum Field Theory Effects,EmilT.Akhmedov, -
Quantum Gravity from the QFT Perspective
Quantum Gravity from the QFT perspective Ilya L. Shapiro Universidade Federal de Juiz de Fora, MG, Brazil Partial support: CNPq, FAPEMIG ICTP-SAIFR/IFT-UNESP – 1-5 April, 2019 Ilya Shapiro, Quantum Gravity from the QFT perspective April - 2019 Lecture 5. Advances topics in QG Induced gravity concept. • Effective QG: general idea. • Effective QG as effective QFT. • Where we are with QG?. • Bibliography S.L. Adler, Rev. Mod. Phys. 54 (1982) 729. S. Weinberg, Effective Field Theory, Past and Future. arXive:0908.1964[hep-th]; J.F. Donoghue, The effective field theory treatment of quantum gravity. arXive:1209.3511[gr-qc]; I.Sh., Polemic notes on IR perturbative quantum gravity. arXiv:0812.3521 [hep-th]. Ilya Shapiro, Quantum Gravity from the QFT perspective April - 2019 I. Induced gravity. The idea of induced gravity is simple, while its realization may be quite non-trivial, depending on the theory. In any case, the induced gravity concept is something absolutely necessary if we consider an interaction of gravity with matter and quantum theory concepts. I. Induced gravity from cut-off Original simplest version. Ya.B. Zeldovich, Sov. Phys. Dokl. 6 (1967) 883. A.D. Sakharov, Sov. Phys. Dokl. 12 (1968) 1040. Strong version of induced gravity is like that: Suppose that the metric has no pre-determined equations of motion. These equations result from the interaction to matter. Main advantage: Since gravity is not fundamental, but induced interaction, there is no need to quantize metric. Ilya Shapiro, Quantum Gravity from the QFT perspective April - 2019 And we already know that the semiclassical approach has no problems with renormalizability! Suppose we have a theory of quantum matter fields Φ = (ϕ, ψ, Aµ) interacting to the metric gµν . -
Emergent Gravity: from Condensed Matter Analogues to Phenomenology
Emergent gravity: From Condensed matter analogues to Phenomenology. Emergent properties of space-time. CERN. Stefano Liberati SISSA - INFN Trieste, Italy GR, a beautiful but weird theory… Some tantalising features of General Relativity Singularities Critical phenomena in gravitational collapse Horizon thermodynamics Spacetime thermodynamics: Einstein equations as equations of state. The “dark ingredients” of our universe? Faster than light and Time travel solutions AdS/CFT duality, holographic behaviour Gravity/fluid duality Gravity as an emergent phenomenon? Emergent gravity idea: quantizing the metric or the connections does not help because perhaps these are not fundamental objects but collective variables of more fundamental structures. GR ⇒ Hydrodynamics Metric as a collective variable All the sub-Planckian physics is low energy physics Spacetime as a condensate of some more fundamental objects Spacetime symmetries as emergent symmetries Singularities as phase transitions (big bang as geometrogenesis) Cosmological constant as deviation from the real ground state Many models are nowadays resorting to emergent gravity scenarios Causal sets Quantum graphity models Group field theories condensates scenarios AdS/CFT scenarios where the CFT is considered primary Gravity as an entropic force ideas Condensed matter analogues of gravity Gravity as an emergent phenomenon? Emergent gravity idea: quantizing the metric or the connections does not help because perhaps these are not fundamental objects but collective variables of more fundamental -
Impulse Gravity Generator Based on Charged Y Ba2cu3o7−Y
Impulse Gravity Generator Based on Charged YBa2Cu3O7 y Superconductor with Composite Crystal − Structure Evgeny Podkletnov1, Giovanni Modanese2 1 Moscow Chemical Scientific Research Centre 113452 Moscow - Russia E-mail: [email protected] 2 California Institute for Physics and Astrophysics 366 Cambridge Ave., Palo Alto, CA 94306 and University of Bolzano – Industrial Engineering Via Sernesi 1, 39100 Bolzano, Italy E-mail: [email protected] Abstract The detection of apparent anomalous forces in the vicinity of high-Tc supercon- ductors under non equilibrium conditions has stimulated an experimental research in which the operating parameters of the experiment have been pushed to values higher than those employed in previous attempts. The results confirm the existence of an unexpected physical interaction. An apparatus has been constructed and tested in which the superconductor is subjected to peak currents in excess of 104 A, surface potentials in excess of 1 MV , trapped magnetic field up to 1 T , and temperature down to 40 K. In order to produce the required currents a high voltage discharge technique has been employed. Discharges originating from a superconducting ceramic electrode are accompanied by the emission of radiation which propagates in a focused beam without noticeable attenuation through different materials and exerts a short repulsive force on small movable objects along the propagation axis. Within the measurement error (5 to 7 %) the impulse is proportional to the mass of the objects and independent on their composition. It therefore resembles a gravitational impulse. The observed phenomenon appears to be absolutely new and unprecedented in the literature. It cannot be understood in the framework of general relativity. -
Classical Chaos Described by a Density Matrix
Article Classical Chaos Described by a Density Matrix Andres Mauricio Kowalski , Angelo Plastino * and Gaspar Gonzalez IFLP, Universidad Nacional de La Plata, La Plata 1900, Argentina; kowalski@fisica.unlp.edu.ar (A.M.K.); [email protected] (G.G.) * Correspondence: plastino@fisica.unlp.edu.ar Abstract: In this paper, a reference to the semiclassical model, in which quantum degrees of freedom interact with classical ones, is considered. The classical limit of a maximum-entropy density matrix that describes the temporal evolution of such a system is analyzed. Here, it is analytically shown that, in the classical limit, it is possible to reproduce classical results. An example is classical chaos. This is done by means a pure-state density matrix, a rather unexpected result. It is shown that this is possible only if the quantum part of the system is in a special class of states. Keywords: classical limit; semiclassical system; semiclassical chaos; clasiccal chaos; maximum entropy density matrix 1. Introduction The quantum–classical transition is a frontier issue, a rather transcendental physics topic [1–5]. The use of semi-classical systems to describe problems in physics has a long history; see, e.g., [6–12]. A particularly important case to be highlighted is the one, in which the quantum features of one of the two components of a composite system are negligible in comparison with those of the other. Regarding the first component as a classical one simplifies the description and provides deep insight into the combined system Citation: Kowalski, A.M.; Plastino, dynamics [13]. This methodology is used for the interaction of matter with a field. -
Semiclassical Modeling of Multiparticle Quantum Mechanics
UNIVERSITY OF CALIFORNIA Los Angeles Semiclassical Modeling of Quantum-Mechanical Multiparticle Systems using Parallel Particle-In-Cell Methods A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Physics by Dean Edward Dauger 2001 © Copyright by Dean Edward Dauger 2001 To my parents, Alan and Marlene, who were always fully supportive of my work and my endeavors. And Charlie and Allegra, my cats. And to all those who have a vision, a dream of something new and inspiring, to express that Idea, limited only by its own conclusion if it has one. iii Contents I. Introduction A. Motivation ···················································································1 B. Existing Methods ···················································································6 C. Outline ···················································································8 D. Conventions ···················································································9 II. Theory A. The Approach ·················································································11 B. Feynman Path Integrals···············································································13 C. The Semiclassical Approximation·······························································18 D. Initial Position and Final Momentum·························································21 E. The Matrix ··················································································23 F. The Determinant -
An Alternative to Dark Matter and Dark Energy: Scale-Dependent Gravity in Superfluid Vacuum Theory
universe Article An Alternative to Dark Matter and Dark Energy: Scale-Dependent Gravity in Superfluid Vacuum Theory Konstantin G. Zloshchastiev Institute of Systems Science, Durban University of Technology, P.O. Box 1334, Durban 4000, South Africa; [email protected] Received: 29 August 2020; Accepted: 10 October 2020; Published: 15 October 2020 Abstract: We derive an effective gravitational potential, induced by the quantum wavefunction of a physical vacuum of a self-gravitating configuration, while the vacuum itself is viewed as the superfluid described by the logarithmic quantum wave equation. We determine that gravity has a multiple-scale pattern, to such an extent that one can distinguish sub-Newtonian, Newtonian, galactic, extragalactic and cosmological terms. The last of these dominates at the largest length scale of the model, where superfluid vacuum induces an asymptotically Friedmann–Lemaître–Robertson–Walker-type spacetime, which provides an explanation for the accelerating expansion of the Universe. The model describes different types of expansion mechanisms, which could explain the discrepancy between measurements of the Hubble constant using different methods. On a galactic scale, our model explains the non-Keplerian behaviour of galactic rotation curves, and also why their profiles can vary depending on the galaxy. It also makes a number of predictions about the behaviour of gravity at larger galactic and extragalactic scales. We demonstrate how the behaviour of rotation curves varies with distance from a gravitating center, growing from an inner galactic scale towards a metagalactic scale: A squared orbital velocity’s profile crosses over from Keplerian to flat, and then to non-flat. The asymptotic non-flat regime is thus expected to be seen in the outer regions of large spiral galaxies. -
Condensed Matter Physics and the Nature of Spacetime
Condensed Matter Physics and the Nature of Spacetime This essay considers the prospects of modeling spacetime as a phenomenon that emerges in the low-energy limit of a quantum liquid. It evaluates three examples of spacetime analogues in condensed matter systems that have appeared in the recent physics literature, and suggests how they might lend credence to an epistemological structural realist interpretation of spacetime that emphasizes topology over symmetry in the accompanying notion of structure. Keywords: spacetime, condensed matter, effective field theory, emergence, structural realism Word count: 15, 939 1. Introduction 2. Effective Field Theories in Condensed Matter Systems 3. Spacetime Analogues in Superfluid Helium and Quantum Hall Liquids 4. Low-Energy Emergence and Emergent Spacetime 5. Universality, Dynamical Structure, and Structural Realism 1. Introduction In the philosophy of spacetime literature not much attention has been given to concepts of spacetime arising from condensed matter physics. This essay attempts to address this. I look at analogies between spacetime and a quantum liquid that have arisen from effective field theoretical approaches to highly correlated many-body quantum systems. Such approaches have suggested to some authors that spacetime can be modeled as a phenomenon that emerges in the low-energy limit of a quantum liquid with its contents (matter and force fields) described by effective field theories (EFTs) of the low-energy excitations of this liquid. While directly relevant to ongoing debates over the ontological status of spacetime, this programme also has other consequences that should interest philosophers of physics. It suggests, for instance, a particular approach towards quantum gravity, as well as an anti-reductionist attitude towards the nature of symmetries in quantum field theory. -
Teleparallel Gravity and Dimensional Reductions of Noncommutative Gauge Theory
CORE Metadata, HWM–01–15citation and similar papers at core.ac.uk Provided by CERN Document Server EMPG–01–05 hep–th/0105094 May 2001 Teleparallel Gravity and Dimensional Reductions of Noncommutative Gauge Theory Edwin Langmann Department of Theoretical Physics, Royal Institute of Technology S-100 44 Stockholm, Sweden [email protected] Richard J. Szabo Department of Mathematics, Heriot-Watt University Riccarton, Edinburgh EH14 4AS, Scotland [email protected] Abstract We study dimensional reductions of noncommutative electrodynamics on flat space which lead to gauge theories of gravitation. For a general class of such reduc- tions, we show that the noncommutative gauge fields naturally yield a Weitzenb¨ock geometry on spacetime and that the induced diffeomorphism invariant field theory can be made equivalent to a teleparallel formulation of gravity which macroscopi- cally describes general relativity. The Planck length is determined in this setting by the Yang-Mills coupling constant and the noncommutativity scale. The effective field theory can also contain higher-curvature and non-local terms which are charac- teristic of string theory. Some applications to D-brane dynamics and generalizations to include the coupling of ordinary Yang-Mills theory to gravity are also described. 1 Introduction Yang-Mills theory on a flat noncommutative space arises as special decoupling limits of string theory [1, 2] and M-theory [2, 3]. In string theory it represents the low-energy effective field theory induced on D-branes in the presence of a constant background su- pergravity B-field. The inherent non-locality of the interactions in this field theory lead to many exotic effects that do not arise in ordinary quantum field theory, and which can be attributed to “stringy” properties of the model. -
Canonical Quantum Gravity and the Problem of Time
Imperial/TP/91-92/25 Canonical Quantum Gravity and the Problem of Time 1 2 C.J. Isham Blackett Laboratory Imperial College South Kensington London SW7 2BZ United Kingdom August 1992 Abstract The aim of this paper is to provide a general introduction to the problem of time in quantum gravity. This problem originates in the fundamental conflict between arXiv:gr-qc/9210011v1 21 Oct 1992 the way the concept of ‘time’ is used in quantum theory, and the role it plays in a diffeomorphism-invariant theory like general relativity. Schemes for resolving this problem can be sub-divided into three main categories: (I) approaches in which time is identified before quantising; (II) approaches in which time is identified after quantising; and (III) approaches in which time plays no fundamental role at all. Ten different specific schemes are discussed in this paper which also contain an introduction to the relevant parts of the canonical decomposition of general relativity. 1Lectures presented at the NATO Advanced Study Institute “Recent Problems in Mathematical Physics”, Salamanca, June 15–27, 1992. 2Research supported in part by SERC grant GR/G60918. Contents 1 INTRODUCTION 4 1.1 Preamble ................................... 4 1.2 PreliminaryRemarks ............................. 4 1.3 Current Research Programmes in Quantum Gravity . ..... 6 1.4 OutlineofthePaper ............................. 8 1.5 Conventions.................................. 9 2 QUANTUMGRAVITYANDTHEPROBLEMOFTIME 9 2.1 Time in Conventional Quantum Theory . .. 10 2.2 Time in a Diff( )-invariantTheory . 12 M 2.3 ApproachestotheProblemofTime. 16 2.4 Technical Problems With Time . 19 3 CANONICALGENERALRELATIVITY 20 3.1 IntroductoryRemarks ............................ 21 3.2 Quantum Field Theory in a Curved Background . -
A Connection Between Gravity and the Higgs Field
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server A connection between gravity and the Higgs field M. Consoli Istituto Nazionale di Fisica Nucleare, Sezione di Catania Corso Italia 57, 95129 Catania, Italy Abstract Several arguments suggest that an effective curved space-time structure (of the type as in General Relativity) can actually find its dynamical origin in an underlying condensed medium of spinless quanta. For this reason, we exploit the recent idea of density fluctuations in a ‘Higgs condensate’ with the conclusion that such long-wavelength effects might represent the natural dynamical agent of gravity. 1 Introduction Following the original induced-gravity models [1], one may attempt to describe gravity as an effective force induced by the vacuum structure, in analogy with the attractive interaction among electrons that can only exist in the presence of an ion lattice. If such an underlying ‘dynamical’ mechanism is found, one will also gain a better understanding of those pecu- liar ‘geometrical’ properties that are the object of classical General Relativity. In fact, by demanding the space-time structure to an undefined energy-momentum tensor, no clear dis- tinction between the two aspects is possible and this may be the reason for long-standing problems (e.g. the space-time curvature associated with the vacuum energy). A nice example to understand what aspects may be kinematical and what other as- pects may be dynamical has been given by Visser [2]. Namely, a curved space-time pseudo- Riemannian geometry arises when studying the density fluctuations in a moving irrotational fluid, i.e. -
Emergent Gravity As the Eraser of Anomalous Gauge Boson Masses, and QFT-GR Concord
General Relativity and Gravitation (2021) 53:22 https://doi.org/10.1007/s10714-021-02797-0 RESEARCH ARTICLE Emergent gravity as the eraser of anomalous gauge boson masses, and QFT-GR concord Durmu¸sDemir1 Received: 29 November 2020 / Accepted: 9 February 2021 / Published online: 22 February 2021 © The Author(s), under exclusive licence to Springer Science+Business Media, LLC part of Springer Nature 2021 Abstract In the same base setup as Sakharov’s induced gravity, we investigate emergence of gravity in effective quantum field theories (QFT), with particular emphasis on the gauge sector in which gauge bosons acquire anomalous masses in proportion to the 2 ultraviolet cutoff Λ℘. Drawing on the fact that Λ℘ corrections explicitly break the 2 gauge and Poincare symmetries, we find that it is possible to map Λ℘ to spacetime curvature as a covariance relation and we find also that this map erases the anoma- lous gauge boson masses. The resulting framework describes gravity by the general relativity (GR) and matter by the QFT itself with log Λ℘ corrections (dimensional regularization). This QFT-GR concord predicts existence of new physics beyond the Standard Model such that the new physics can be a weakly-interacting or even a non- interacting sector comprising the dark matter, dark energy and possibly more. The concord has consequential implications for collider, astrophysical and cosmological phenomena. Keywords Emergent gravity · Anomalous gauge boson masses · Extended general covariance Contents 1 Introduction ............................................. 2 2 UV cutoff and the UV sensitivity problems ............................. 3 3 How not to take effective QFTs into curved spacetime ....................... 5 2 4 Λ℘ versus log Λ℘ : Symmetry structures .............................