"What Is Space?" by Frank Wilczek
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Toy Models for Black Hole Evaporation
UCSBTH-92-36 hep-th/9209113 Toy Models for Black Hole Evaporation∗ Steven B. Giddings† Department of Physics University of California Santa Barbara, CA 93106-9530 Abstract These notes first present a brief summary of the puzzle of information loss to black holes, of its proposed resolutions, and of the flaws in the proposed resolutions. There follows a review of recent attempts to attack this problem, and other issues in black hole physics, using two-dimensional dilaton gravity theories as toy models. These toy models contain collapsing black holes and have for the first time enabled an explicit semiclassical treatment of the backreaction of the Hawking radiation on the geometry of an evaporating black hole. However, a complete answer to the information conundrum seems to require physics beyond the semiclassical approximation. Preliminary attempts to make progress arXiv:hep-th/9209113v2 11 Nov 1992 in this direction, using connections to conformal field theory, are described. *To appear in the proceedings of the International Workshop of Theoretical Physics, 6th Session, String Quantum Gravity and Physics at the Planck Energy Scale, 21 – 28 June 1992, Erice, Italy. † Email addresses: [email protected], [email protected]. Since the discovery of black holes, physicists have been faced with the possibility that they engender a breakdown of predictability. At the classical level this breakdown arises at the singularity. Classically we do not know how to evolve past it. Inclusion of quantum effects may serve as a remedy, allowing predictable evolution, by smoothing out the singularities of general relativity. However, as suggested by Hawking [1,2], quantum effects also present another sharp challenge to predictability through the mechanism of Hawking evaporation. -
Quantum Vacuum Energy Density and Unifying Perspectives Between Gravity and Quantum Behaviour of Matter
Annales de la Fondation Louis de Broglie, Volume 42, numéro 2, 2017 251 Quantum vacuum energy density and unifying perspectives between gravity and quantum behaviour of matter Davide Fiscalettia, Amrit Sorlib aSpaceLife Institute, S. Lorenzo in Campo (PU), Italy corresponding author, email: [email protected] bSpaceLife Institute, S. Lorenzo in Campo (PU), Italy Foundations of Physics Institute, Idrija, Slovenia email: [email protected] ABSTRACT. A model of a three-dimensional quantum vacuum based on Planck energy density as a universal property of a granular space is suggested. This model introduces the possibility to interpret gravity and the quantum behaviour of matter as two different aspects of the same origin. The change of the quantum vacuum energy density can be considered as the fundamental medium which determines a bridge between gravity and the quantum behaviour, leading to new interest- ing perspectives about the problem of unifying gravity with quantum theory. PACS numbers: 04. ; 04.20-q ; 04.50.Kd ; 04.60.-m. Key words: general relativity, three-dimensional space, quantum vac- uum energy density, quantum mechanics, generalized Klein-Gordon equation for the quantum vacuum energy density, generalized Dirac equation for the quantum vacuum energy density. 1 Introduction The standard interpretation of phenomena in gravitational fields is in terms of a fundamentally curved space-time. However, this approach leads to well known problems if one aims to find a unifying picture which takes into account some basic aspects of the quantum theory. For this reason, several authors advocated different ways in order to treat gravitational interaction, in which the space-time manifold can be considered as an emergence of the deepest processes situated at the fundamental level of quantum gravity. -
Spacetime Geometry from Graviton Condensation: a New Perspective on Black Holes
Spacetime Geometry from Graviton Condensation: A new Perspective on Black Holes Sophia Zielinski née Müller München 2015 Spacetime Geometry from Graviton Condensation: A new Perspective on Black Holes Sophia Zielinski née Müller Dissertation an der Fakultät für Physik der Ludwig–Maximilians–Universität München vorgelegt von Sophia Zielinski geb. Müller aus Stuttgart München, den 18. Dezember 2015 Erstgutachter: Prof. Dr. Stefan Hofmann Zweitgutachter: Prof. Dr. Georgi Dvali Tag der mündlichen Prüfung: 13. April 2016 Contents Zusammenfassung ix Abstract xi Introduction 1 Naturalness problems . .1 The hierarchy problem . .1 The strong CP problem . .2 The cosmological constant problem . .3 Problems of gravity ... .3 ... in the UV . .4 ... in the IR and in general . .5 Outline . .7 I The classical description of spacetime geometry 9 1 The problem of singularities 11 1.1 Singularities in GR vs. other gauge theories . 11 1.2 Defining spacetime singularities . 12 1.3 On the singularity theorems . 13 1.3.1 Energy conditions and the Raychaudhuri equation . 13 1.3.2 Causality conditions . 15 1.3.3 Initial and boundary conditions . 16 1.3.4 Outlining the proof of the Hawking-Penrose theorem . 16 1.3.5 Discussion on the Hawking-Penrose theorem . 17 1.4 Limitations of singularity forecasts . 17 2 Towards a quantum theoretical probing of classical black holes 19 2.1 Defining quantum mechanical singularities . 19 2.1.1 Checking for quantum mechanical singularities in an example spacetime . 21 2.2 Extending the singularity analysis to quantum field theory . 22 2.2.1 Schrödinger representation of quantum field theory . 23 2.2.2 Quantum field probes of black hole singularities . -
A Short History of Physics (Pdf)
A Short History of Physics Bernd A. Berg Florida State University PHY 1090 FSU August 28, 2012. References: Most of the following is copied from Wikepedia. Bernd Berg () History Physics FSU August 28, 2012. 1 / 25 Introduction Philosophy and Religion aim at Fundamental Truths. It is my believe that the secured part of this is in Physics. This happend by Trial and Error over more than 2,500 years and became systematic Theory and Observation only in the last 500 years. This talk collects important events of this time period and attaches them to the names of some people. I can only give an inadequate presentation of the complex process of scientific progress. The hope is that the flavor get over. Bernd Berg () History Physics FSU August 28, 2012. 2 / 25 Physics From Acient Greek: \Nature". Broadly, it is the general analysis of nature, conducted in order to understand how the universe behaves. The universe is commonly defined as the totality of everything that exists or is known to exist. In many ways, physics stems from acient greek philosophy and was known as \natural philosophy" until the late 18th century. Bernd Berg () History Physics FSU August 28, 2012. 3 / 25 Ancient Physics: Remarkable people and ideas. Pythagoras (ca. 570{490 BC): a2 + b2 = c2 for rectangular triangle: Leucippus (early 5th century BC) opposed the idea of direct devine intervention in the universe. He and his student Democritus were the first to develop a theory of atomism. Plato (424/424{348/347) is said that to have disliked Democritus so much, that he wished his books burned. -
Black Holes and Gravitational Waves in Models of Minicharged Dark Matter
Home Search Collections Journals About Contact us My IOPscience Black holes and gravitational waves in models of minicharged dark matter This content has been downloaded from IOPscience. Please scroll down to see the full text. JCAP05(2016)054 (http://iopscience.iop.org/1475-7516/2016/05/054) View the table of contents for this issue, or go to the journal homepage for more Download details: IP Address: 62.210.105.116 This content was downloaded on 28/06/2016 at 17:13 Please note that terms and conditions apply. ournal of Cosmology and Astroparticle Physics JAn IOP and SISSA journal Black holes and gravitational waves in models of minicharged dark matter JCAP05(2016)054 Vitor Cardoso,a;b Caio F.B. Macedo,a Paolo Pania;c and Valeria Ferraric aCENTRA, Departamento de F´ısica,Instituto Superior T´ecnico| IST, Universidade de Lisboa | UL, Avenida Rovisco Pais 1, 1049 Lisboa, Portugal bPerimeter Institute for Theoretical Physics, 31 Caroline Street North Waterloo, Ontario N2L 2Y5, Canada cDipartimento di Fisica, \Sapienza" Universit`adi Roma and Sezione INFN Roma1, Piazzale A. Moro 5, 00185, Roma, Italy E-mail: [email protected], [email protected], [email protected], [email protected] Received April 29, 2016 Revised May 16, 2016 Accepted May 17, 2016 Published May 23, 2016 Abstract. In viable models of minicharged dark matter, astrophysical black holes might be charged under a hidden U(1) symmetry and are formally described by the same Kerr- Newman solution of Einstein-Maxwell theory. These objects are unique probes of minicharged dark matter and dark photons. -
Nonlocal Single Particle Steering Generated Through Single Particle Entanglement L
www.nature.com/scientificreports OPEN Nonlocal single particle steering generated through single particle entanglement L. M. Arévalo Aguilar In 1927, at the Solvay conference, Einstein posed a thought experiment with the primary intention of showing the incompleteness of quantum mechanics; to prove it, he employed the instantaneous nonlocal efects caused by the collapse of the wavefunction of a single particle—the spooky action at a distance–, when a measurement is done. This historical event preceded the well-know Einstein– Podolsk–Rosen criticism over the incompleteness of quantum mechanics. Here, by using the Stern– Gerlach experiment, we demonstrate how the instantaneous nonlocal feature of the collapse of the wavefunction together with the single-particle entanglement can be used to produce the nonlocal efect of steering, i.e. the single-particle steering. In the steering process Bob gets a quantum state depending on which observable Alice decides to measure. To accomplish this, we fully exploit the spreading (over large distances) of the entangled wavefunction of the single-particle. In particular, we demonstrate that the nonlocality of the single-particle entangled state allows the particle to “know” about the kind of detector Alice is using to steer Bob’s state. Therefore, notwithstanding strong counterarguments, we prove that the single-particle entanglement gives rise to truly nonlocal efects at two faraway places. This opens the possibility of using the single-particle entanglement for implementing truly nonlocal task. Einstein eforts to cope with the challenge of the conceptual understanding of quantum mechanics has been a source of inspiration for its development; in particular, the fact that the quantum description of physical reality is not compatible with causal locality was critically analized by him. -
Antimatter in New Cartesian Generalization of Modern Physics
ACTA SCIENTIFIC APPLIED PHYSICS Volume 1 Issue 1 December 2019 Short Communications Antimatter in New Cartesian Generalization of Modern Physics Boris S Dzhechko* City of Sterlitamak, Bashkortostan, Russia *Corresponding Author: Boris S Dzhechko, City of Sterlitamak, Bashkortostan, Russia. Received: November 29, 2019; Published: December 10, 2019 Keywords: Descartes; Cartesian Physics; New Cartesian Phys- Thus, space, which is matter, moving relative to itself, acts as ics; Mater; Space; Fine Structure Constant; Relativity Theory; a medium forming vortices, of which the tangible objective world Quantum Mechanics; Space-Matter; Antimatter consists. In the concept of moving space-matter, the concept of ir- rational points as nested intervals of the same moving space obey- New Cartesian generalization of modern physics, based on the ing the Heisenberg inequality is introduced. With respect to these identity of space and matter Descartes, replaces the concept of points, we can talk about both the speed of their movement v, ether concept of moving space-matter. It reveals an obvious con- nection between relativity and quantum mechanics. The geometric which is equal to the speed of light c. Electrons are the reference and the speed of filling Cartesian voids formed during movement, interpretation of the thin structure constant allows a deeper un- points by which we can judge the motion of space-matter inside the derstanding of its nature and provides the basis for its theoretical atom. The movement of space-matter inside the atom suggests that calculation. It points to the reason why there is no symmetry be- there is a Cartesian void in it, which forces the electrons to perpetu- tween matter and antimatter in the world. -
Asymptotically Flat Boundary Conditions for the U(1)3 Model for Euclidean Quantum Gravity
universe Article Asymptotically Flat Boundary Conditions for the U(1)3 Model for Euclidean Quantum Gravity Sepideh Bakhoda 1,2,* , Hossein Shojaie 1 and Thomas Thiemann 2,* 1 Department of Physics, Shahid Beheshti University, Tehran 1983969411, Iran; [email protected] 2 Institute for Quantum Gravity, FAU Erlangen—Nürnberg, Staudtstraße 7, 91058 Erlangen, Germany * Correspondence: [email protected] (S.B.); [email protected] (T.T.) 3 Abstract: A generally covariant U(1) gauge theory describing the GN ! 0 limit of Euclidean general relativity is an interesting test laboratory for general relativity, specially because the algebra of the Hamiltonian and diffeomorphism constraints of this limit is isomorphic to the algebra of the corresponding constraints in general relativity. In the present work, we the study boundary conditions and asymptotic symmetries of the U(1)3 model and show that while asymptotic spacetime translations admit well-defined generators, boosts and rotations do not. Comparing with Euclidean general relativity, one finds that the non-Abelian part of the SU(2) Gauss constraint, which is absent in the U(1)3 model, plays a crucial role in obtaining boost and rotation generators. Keywords: asymptotically flat boundary conditions; classical and quantum gravity; U(1)3 model; asymptotic charges Citation: Bakhoda, S.; Shojaie, H.; 1. Introduction Thiemann, T. Asymptotically Flat In the framework of the Ashtekar variables in terms of which General Relativity (GR) Boundary Conditions for the U(1)3 is formulated as a SU(2) gauge theory [1–3], attempts to find an operator corresponding to Model for Euclidean Quantum the Hamiltonian constraint of the Lorentzian vacuum canonical GR led to the result [4] that Gravity. -
Spooky Action at a Distance Is Not Spooky-It Is Knowledge: Combining Entanglement and Negative Observation to Show How the EPR E
How Knowledge Can Lead to the Demise of Schrodinger’s Cat Through a Negative Measurement/Null Measurement (A Quantum Mechanical Measurement in Which There is No Physical Interaction Between a Physical Measuring Apparatus and the System Measured) Douglas M. Snyder 2020 APS March Meeting, Denver, Colorado http://meetings.aps.org/Meeting/MAR20/Session/C71.261 DOI: 10.13140/RG.2.2.27582.43843 forpsyarxiv_cat 5/26/2020 Copyright 2020 Douglas Michael Snyder 1 Abstract The Schrodinger cat experiment (SCE) is presented. An alteration follows where the LACK of radioactive decay leads to the demise of the cat instead of the ACT of radioactive decay. The lack of radioactive decay is a negative (null) measurement (where there is NO physical interaction between the radioactive material and the Geiger counter). The negative (null) measurement is non-trivial because all knowledge about the radioactive material (rm) is derived from its associated wave function which itself has no physical existence. The wave function is how we make probabilistic predictions regarding systems in quantum mechanics. So when the wave function changes in a negative (null) measurement, that is exactly what happens in a positive measurement where there is a physical interaction between entity measured and a physical measuring apparatus. (continued on next slide) 5/26/2020 2 Copyright 2020 Douglas Michael Snyder Abstract Before the box in the original SCE is opened, the wave function for the radioactive material is: ψrad_mat = 1/√2 [ψrad_mat_does_not_decay + ψrad_mat+_does_decay] -
General Relativity 05/12/2008 Lecture 15 1
General Relativity 05/12/2008 UCSD Physics 10 UCSD Physics 10 So Far, We Have… • Decided that constant velocity is the “natural” state of things General Relativity • Devised a natural philosophy in which Einstein Upsets the Applecart acceleration is the result of forces • Unified terrestrial and celestial mechanics & brought order to the Universe Spring 2008 2 UCSD Physics 10 UCSD Physics 10 Frames of Reference Science is Fraught with Assumptions This is all fine, but accelerating • The Earth is at the center of the universe... with respect to what?? • The Earth is at the center of the solar system... • The world is flat... • The geometry of the Universe is flat... • The surface of the Earth is the “natural” reference frame... • Time and space are independent concepts These assumptions can have a dramatic impact on our views of Nature Why the Earth, of course! Spring 2008 3 Spring 2008 4 Lecture 15 1 General Relativity 05/12/2008 UCSD Physics 10 UCSD Physics 10 Recall the Rotating Drum Example Imagine Being in a Car • Windows are painted black • Move the car to outer space • An accelerating frame of reference feels a lot like • Now imagine placing a few objects on the dashboard of gravity this blacked-out car, still in outer space. – In fact, it feels exactly like gravity • If the car accelerates forward, what happens to these • The essence of General Relativity is the objects on the dashboard? (Why?) recognition that “gravitational force” is an artifact • If you didn’t know the car was accelerating, what of doing physics in a particular reference frame! would you infer about a “force” acting on the objects? • How would that force depend on the masses of the objects? Spring 2008 5 Spring 2008 6 UCSD Physics 10 UCSD Physics 10 Gravity vs. -
Introducing Quantum and Statistical Physics in the Footsteps of Einstein: a Proposal †
universe Article Introducing Quantum and Statistical Physics in the Footsteps of Einstein: A Proposal † Marco Di Mauro 1,*,‡ , Salvatore Esposito 2,‡ and Adele Naddeo 2,‡ 1 Dipartimento di Matematica, Universitá di Salerno, Via Giovanni Paolo II, 84084 Fisciano, Italy 2 INFN Sezione di Napoli, Via Cinthia, 80126 Naples, Italy; [email protected] (S.E.); [email protected] (A.N.) * Correspondence: [email protected] † This paper is an extended version from the proceeding paper: Di Mauro, M.; Esposito, S.; Naddeo, A. Introducing Quantum and Statistical Physics in the Footsteps of Einstein: A Proposal. In Proceedings of the 1st Electronic Conference on Universe, online, 22–28 February 2021. ‡ These authors contributed equally to this work. Abstract: Introducing some fundamental concepts of quantum physics to high school students, and to their teachers, is a timely challenge. In this paper we describe ongoing research, in which a teaching–learning sequence for teaching quantum physics, whose inspiration comes from some of the fundamental papers about the quantum theory of radiation by Albert Einstein, is being developed. The reason for this choice goes back essentially to the fact that the roots of many subtle physical concepts, namely quanta, wave–particle duality and probability, were introduced for the first time in one of these papers, hence their study may represent a useful intermediate step towards tackling the final incarnation of these concepts in the full theory of quantum mechanics. An extended discussion of some elementary tools of statistical physics, mainly Boltzmann’s formula for entropy and statistical distributions, which are necessary but may be unfamiliar to the students, is included. -
Rethinking 'Classical Physics'
This is a repository copy of Rethinking 'Classical Physics'. White Rose Research Online URL for this paper: http://eprints.whiterose.ac.uk/95198/ Version: Accepted Version Book Section: Gooday, G and Mitchell, D (2013) Rethinking 'Classical Physics'. In: Buchwald, JZ and Fox, R, (eds.) Oxford Handbook of the History of Physics. Oxford University Press , Oxford, UK; New York, NY, USA , pp. 721-764. ISBN 9780199696253 © Oxford University Press 2013. This is an author produced version of a chapter published in The Oxford Handbook of the History of Physics. Reproduced by permission of Oxford University Press. Reuse Unless indicated otherwise, fulltext items are protected by copyright with all rights reserved. The copyright exception in section 29 of the Copyright, Designs and Patents Act 1988 allows the making of a single copy solely for the purpose of non-commercial research or private study within the limits of fair dealing. The publisher or other rights-holder may allow further reproduction and re-use of this version - refer to the White Rose Research Online record for this item. Where records identify the publisher as the copyright holder, users can verify any specific terms of use on the publisher’s website. Takedown If you consider content in White Rose Research Online to be in breach of UK law, please notify us by emailing [email protected] including the URL of the record and the reason for the withdrawal request. [email protected] https://eprints.whiterose.ac.uk/ 1 Rethinking ‘Classical Physics’ Graeme Gooday (Leeds) & Daniel Mitchell (Hong Kong) Chapter for Robert Fox & Jed Buchwald, editors Oxford Handbook of the History of Physics (Oxford University Press, in preparation) What is ‘classical physics’? Physicists have typically treated it as a useful and unproblematic category to characterize their discipline from Newton until the advent of ‘modern physics’ in the early twentieth century.