Planck Scale Effects in Astrophysics and Cosmology
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The Sagnac Effect: Does It Contradict Relativity?
The Sagnac Effect: Does it Contradict Relativity? By Doug Marett 2012 A number of authors have suggested that the Sagnac effect contradicts the original postulates of Special Relativity, since the postulate of the constancy of the speed of light is violated in rotating systems. [1,2,3] Sagnac himself designed the experiment of 1913 to prove the existence of the aether [4]. Other authors have attempted to explain the effect within the theoretical framework of relativity, even going as far as calling the effect “relativistic”.[5] However, we seek in this paper to show how the Sagnac effect contravenes in principle the concept of the relativity of time and motion. To understand how this happens and its wider implications, it is necessary to look first at the concept of absolute vs. relative motion, what the Sagnac effect implies about these motions, and what follows logically about the broader notions of space and time. Early Ideas Regarding Rotation and Absolute Motion: The fundamental distinction between translational and rotational motion was first pointed out by Sir Isaac Newton, and emphasized later by the work of Ernest Mach and Heinrich Hertz. One of the first experiments on the subject was Newton’s bucket experiment of 1689. It was an experiment to demonstrate that true rotational motion cannot be defined as relative rotation of a body with respect to surrounding bodies – that true motion and rest should be defined relative to absolute space instead. In Newton’s experiment, a bucket is filled with water and hung by a rope. If the rope is twisted around and around until it is tight and then released, the bucket begins to spin rapidly, not only with respect to the observers watching it, but also with respect to the water in the bucket, which at first doesn’t move and remains flat on its surface. -
Vacuum GR in Chang--Soo Variables: Hilbert Space Structure In
Vacuum GR in Chang–Soo variables: Hilbert space structure in anisotropic minisuperspace Eyo Eyo Ita III January 20, 2009 Department of Applied Mathematics and Theoretical Physics Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road Cambridge CB3 0WA, United Kingdom [email protected] Abstract In this paper we address the major criticism of the pure Kodama state, namely its normalizability and its existence within a genuine Hilbert space of states, by recasting Ashtekar’s general relativity into set of new variables attributed to Chang–Soo/CDJ. While our results have been shown for anisotropic minisuperspace, we reserve a treat- ment of the full theory for a following paper which it is hoped should finally bring this issue to a close. We have performed a canonical treat- ment of these new variables from the level of the classical/quantum algebra of constraints, all the way to the construction of the Hilbert space of states, and have demonstrated their relevance to the principle arXiv:0901.3041v1 [gr-qc] 20 Jan 2009 of the semiclassical-quantum correspondence. It is hoped that these new variables and their physical interpretation should provide a new starting point for investigations in classical and quantum GR and in the construction of a consistent quantum theory. 1 1 Introduction The main focus of the present paper to establish a new Hilbert space struc- ture for quantum gravity by recasting general relativity in terms of a set of new variables. The traditional approach in loop variables utilizes the spin network states, which have been rigorously shown to meet the requirements of a Hilbert space [1]. -
Theoretical Analysis of Generalized Sagnac Effect in the Standard Synchronization
Theoretical Analysis of Generalized Sagnac Effect in the Standard Synchronization Yang-Ho Choi Department of Electrical and Electronic Engineering Kangwon National University Chunchon, Kangwon-do, 200-701, South Korea Abstract: The Sagnac effect has been shown in inertial frames as well as rotating frames. We solve the problem of the generalized Sagnac effect in the standard synchronization of clocks. The speed of a light beam that traverses an optical fiber loop is measured with respect to the proper time of the light detector, and is shown to be other than the constant c, though it appears to be c if measured by the time standard-synchronized. The fiber loop, which can have an arbitrary shape, is described by an infinite number of straight lines such that it can be handled by the general framework of Mansouri and Sexl (MS). For a complete analysis of the Sagnac effect, the motion of the laboratory should be taken into account. The MS framework is introduced to deal with its motion relative to a preferred reference frame. Though the one-way speed of light is other than c, its two-way speed is shown to be c with respect to the proper time. The theoretical analysis of the generalized Sagnac effect corresponds to the experimental results, and shows the usefulness of the standard synchronization. The introduction of the standard synchrony can make mathematical manipulation easy and can allow us to deal with relative motions between inertial frames without information on their velocities relative to the preferred frame. Keywords: Generalized Sagnac effect, Standard synchronization, Speed of light, Test theory, General framework for transformation PACS numbers: 03.30.+p, 02.10.Yn, 42.25.Bs This paper will be published in Can. -
The Sagnac Effect and Pure Geometry Angelo Tartaglia and Matteo Luca Ruggiero
The Sagnac effect and pure geometry Angelo Tartaglia and Matteo Luca Ruggiero Citation: American Journal of Physics 83, 427 (2015); doi: 10.1119/1.4904319 View online: http://dx.doi.org/10.1119/1.4904319 View Table of Contents: http://scitation.aip.org/content/aapt/journal/ajp/83/5?ver=pdfcov Published by the American Association of Physics Teachers Articles you may be interested in Temperature insensitive refractive index sensor based on single-mode micro-fiber Sagnac loop interferometer Appl. Phys. Lett. 104, 181906 (2014); 10.1063/1.4876448 Transmission and temperature sensing characteristics of a selectively liquid-filled photonic-bandgap-fiber-based Sagnac interferometer Appl. Phys. Lett. 100, 141104 (2012); 10.1063/1.3699026 Sagnac-loop phase shifter with polarization-independent operation Rev. Sci. Instrum. 82, 013106 (2011); 10.1063/1.3514984 Sagnac interferometric switch utilizing Faraday rotation J. Appl. Phys. 105, 07E702 (2009); 10.1063/1.3058627 Magnetic and electrostatic Aharonov–Bohm effects in a pure mesoscopic ring Low Temp. Phys. 23, 312 (1997); 10.1063/1.593401 This article is copyrighted as indicated in the article. Reuse of AAPT content is subject to the terms at: http://scitation.aip.org/termsconditions. Downloaded to IP: 130.192.119.93 On: Tue, 21 Apr 2015 17:40:31 The Sagnac effect and pure geometry Angelo Tartagliaa) and Matteo Luca Ruggiero DISAT, Politecnico di Torino, Corso Duca degli Abruzzi 24, Torino, Italy and INFN, Sezione di Torino, Via Pietro Giuria 1, Torino, Italy (Received 24 July 2014; accepted 2 December 2014) The Sagnac effect is usually deemed to be a special-relativistic effect produced in an interferometer when the device is rotating. -
The Chern-Simons State and Topological Quantum Field Theory
Adv. Studies Theor. Phys., Vol. 1, 2007, no. 8, 395 - 404 The Chern-Simons State and Topological Quantum Field Theory Ichiro Oda Department of Physics, Faculty of Science University of the Ryukyus Nishihara, Okinawa 903-0213, Japan [email protected] Abstract We study a relation between the Chern-Simons state and topological quantum field theory. It is shown that the Chern-Simons state describes a topological state with unbroken diffeomorphism invariance in Yang- Mills theory and Einstein’s general relativity in four dimensions. We give a clear explanation of ”why” such a topological state exists. 1 Introduction It has been known for a long time that Yang-Mills theory in four dimensions has an exact zero energy state of the Schrodinger equation [1], which is, what we call, the Chern-Simons state, and is expressed by the exponential of the Chern-Simons form Ψ = exp(±cSCS), (1) with c being a suitable constant and SCS being explicitly given by SCS = 1 ∧ 1 ∧ ∧ Tr( 2 A dA + 3 A A A). On the other hand, in the community of loop quantum gravity, this state is called the Kodama state since Kodama has first pointed out that the exponential of the Chern-Simons form solves the quantum Ashtekar constraints [2] by starting from the solution for Bianchi IX model and generalizing it [3]. This state has been extensively investigated by Smolin [4] since it shows that, at least for de Sitter space-time, loop quantum gravity does have a good low energy limit, thereby reproducing familiar general relativity and quantum field theory at the low energy as desired. -
Completed by Dufour & Prunier(1942)
Sagnac(1913) completed by Dufour & Prunier(1942) Robert Bennett [email protected] Abstract The 1913 Sagnac test proved to be a critical experiment that refuted Special Relativity (as Sagnac intended) and supported a model of aether that could be entrained like material fluids. But it also generated more questions, such as: What is the Speed of Light(SoL) in the lab frame? What if the optical components of the interferometer were moving relative to each other..some in the lab frame, some in the rotor frame…testing the emission model of light transmission? What if the half beams were directed above the plane of the rotor? All these questions were answered in an extension of the Sagnac test done 29 years after the SagnacX by D&P. An analytic review of On a Fringe Movement Registered on a Platform in Uniform Motion (1942). Dufour and F. Prunier J. de Physique. Radium 3 , 9 (1942) P 153-162 On a Fringe Movement Registered on a Platform in Uniform Motion (1942). A Review .. we used an optical circuit entirely fixed to the rotating platform, as did Sagnac. Under these same conditions we found that the movement of fringes observed are similar within 6%, whether the light source and photographic receiver be dragged in the rotation of the platform, as in the experiments of Sagnac, or they remain fixed in the laboratory. Sagnac and D&P both found SoL = c +- v in the rotor frame. D&P found SoL = c +- v also, in the lab frame (optical bench at rest, empty platform spinning below it) This alone disproves Special Relativity, as SoL <> c The second series of experiments described here was aimed to explore the fringe displacement due to rotation, in entirely new conditions where the optical circuit of the two superimposed interfering beams is composed of two parts in series, one of which remains fixed in relation to the laboratory while the other is attached to the rotating platform. -
Sagnac Effect: the Ballistic Interpretation
Sagnac Effect: The Ballistic Interpretation A. A. Faraj [email protected] Abstract: The primary objective, in the present investigation, is to calculate time-of-flight differences between the co-rotating beam and the counter-rotating beam, over the optical square loop of the Sagnac interferometer, in accordance with the assumption of velocity of light dependent upon the velocity of the light source; and then to compare the obtained results to the computed time-of-flight differences between the same two beams, based on the assumption of velocity of light independent of the velocity of the light source. And subsequently, on the basis of the numerical results of those calculations, it's concluded that, because of the presence of ballistic beaming, the Sagnac interferometer, and rotating interferometers, generally, are incapable of providing any conclusive experimental evidence for or against either one of the two diametrically opposed assumptions, under investigation. In the 1913 Sagnac experiment, for instance, the numerical values of the time-of-flight differences, as predicted by these two propositions, differ from each other by no more than an infinitesimal fraction equal to about 10-30 of a second. Keywords: Sagnac effect; fringe shift; constant speed of light; angular velocity; ballistic speed of light; headlight effect; rotating interferometer; ballistic beaming. Introduction: Undoubtedly, one of the most common oversights in the calculations of Sagnac effect and related phenomena, on the basis of the proposition of ballistic velocity of light, in the published literature, is the incorrect assumption that light traveling at the velocity of c and light traveling at the velocity resultant of c & v must always have together and share in harmony the same exact light path. -
Special Relativity: a Centenary Perspective
Special Relativity: A Centenary Perspective Clifford M. Will McDonnell Center for the Space Sciences and Department of Physics Washington University, St. Louis MO 63130 USA Contents 1 Introduction 1 2 Fundamentals of special relativity 2 2.1 Einstein’s postulates and insights . ....... 2 2.2 Timeoutofjoint ................................. 3 2.3 SpacetimeandLorentzinvariance . ..... 5 2.4 Special relativistic dynamics . ...... 7 3 Classic tests of special relativity 7 3.1 The Michelson-Morley experiment . ..... 7 3.2 Invariance of c ................................... 9 3.3 Timedilation ................................... 9 3.4 Lorentz invariance and quantum mechanics . ....... 10 3.5 Consistency tests of special relativity . ......... 10 4 Special relativity and curved spacetime 12 4.1 Einstein’s equivalence principle . ....... 13 4.2 Metrictheoriesofgravity. .... 14 4.3 Effective violations of local Lorentz invariance . ........... 14 5 Is gravity Lorentz invariant? 17 arXiv:gr-qc/0504085v1 19 Apr 2005 6 Tests of local Lorentz invariance at the centenary 18 6.1 Frameworks for Lorentz symmetry violations . ........ 18 6.2 Modern searches for Lorentz symmetry violation . ......... 20 7 Concluding remarks 21 References........................................ 21 1 Introduction A hundred years ago, Einstein laid the foundation for a revolution in our conception of time and space, matter and energy. In his remarkable 1905 paper “On the Electrodynamics of Moving Bodies” [1], and the follow-up note “Does the Inertia of a Body Depend upon its Energy-Content?” [2], he established what we now call special relativity as one of the two pillars on which virtually all of physics of the 20th century would be built (the other pillar being quantum mechanics). The first new theory to be built on this framework was general relativity [3], and the successful measurement of the predicted deflection of light in 1919 made both Einstein the person and relativity the theory internationally famous. -
Relativistic Effects on Satellite Navigation
Ž. Hećimivić Relativistički utjecaji na satelitsku navigaciju ISSN 1330-3651 (Print), ISSN 1848-6339 (Online) UDC/UDK 531.395/.396:530.12]:629.056.8 RELATIVISTIC EFFECTS ON SATELLITE NAVIGATION Željko Hećimović Subject review The base of knowledge of relativistic effects on satellite navigation is presented through comparison of the main characteristics of the Newtonian and the relativistic space time and by a short introduction of metric of a gravity field. Post-Newtonian theory of relativity is presented as a background in numerical treating of satellite navigation relativistic effects. Time as a crucial parameter in relativistic satellite navigation is introduced through coordinate and proper time as well as terrestrial time and clocks synchronization problem. Described are relativistic effects: on time dilation, on time differences because of the gravity field, on frequency, on path range effects, caused by the Earth rotation, due to the orbit eccentricity and because of the acceleration of the satellite in the theory of relativity. Overviews of treatment of relativistic effects on the GPS, GLONASS, Galileo and BeiDou satellite systems are given. Keywords: satellite navigation, GNSS, post-Newton theory of relativity, relativistic effects, GPS, GLONASS, Galileo, BeiDou Relativistički utjecaji na satelitsku navigaciju Pregledni rad Osnovna znanja o relativističkim utjecajima na satelitsku navigaciju objašnjena su usporedbom glavnih karakteristika Newtonovog i relativističkog prostora vremena te kratkim uvodom u metriku gravitacijskog polja. Post-Newtonova teorija relativnosti objašnjena je kao osnova pri numeričkoj obradi relativističkih utjecaja u području satelitske navigacije. Vrijeme, kao vrlo važan parametar u relativističkoj satelitskoj navigaciji, objašnjeno je kroz koordinatno i vlastito vrijeme te kroz terestičko vrijeme i problem sinkronizacije satova. -
Experiments on the Speed of Light
Journal of Applied Mathematics and Physics, 2019, 7, 1240-1249 http://www.scirp.org/journal/jamp ISSN Online: 2327-4379 ISSN Print: 2327-4352 Experiments on the Speed of Light José R. Croca1,2, Rui Moreira1, Mário Gatta1,3, Paulo Castro1 1Center for Philosophy of Sciences of the University of Lisbon (CFCUL), Lisbon, Portugal 2Department of Physics, Faculty of Sciences, University of Lisbon, Lisbon, Portugal 3CINAV and Escola Naval (Portuguese Naval Academy), Lisbon, Portugal How to cite this paper: Croca, J.R., Mo- Abstract reira, R., Gatta, M. and Castro, P. (2019) Experiments on the Speed of Light. Journal Many experiments concerning the determination of the speed of light have of Applied Mathematics and Physics, 7, been proposed and done. Here two important experiments, Michel- 1240-1249. son-Morley and Sagnac, will be discussed. A linear moving variation of Mi- https://doi.org/10.4236/jamp.2019.75084 chelson-Morley and Sagnac devices will then be proposed for probing expe- Received: February 21, 2019 rimentally the invariance of the speed of light. Accepted: May 28, 2019 Published: May 31, 2019 Keywords Copyright © 2019 by author(s) and Speed of Light, Michelson-Morley Experiment, Sagnac Experiment, One-Arm Scientific Research Publishing Inc. Linear Moving Michelson-Morley and One-Beam Sagnac Interferometer This work is licensed under the Creative Variants Commons Attribution International License (CC BY 4.0). http://creativecommons.org/licenses/by/4.0/ Open Access 1. Introduction Starting with Galileo, many experiments to study the speed of light have been proposed and done. One of the most famous, designed to study the existence of a hypothetical luminiferous aether, was undoubtedly the Michelson and Morley experiment [1]. -
Non-Hermitian Ring Laser Gyroscopes with Enhanced Sagnac Sensitivity
Non-Hermitian Ring Laser Gyroscopes with Enhanced Sagnac Sensitivity Mohammad P. Hokmabadi1, Alexander Schumer1,2, Demetrios N. Christodoulides1, Mercedeh Khajavikhan1* 1CREOL, College of Optics & Photonics, University of Central Florida, Orlando, Florida 32816, USA 2Institute for Theoretical Physics, Vienna University of Technology (TU Wien), 1040, Vienna, Austria, EU *Corresponding author: [email protected] Gyroscopes play a crucial role in many and diverse applications associated with navigation, positioning, and inertial sensing [1]. In general, most optical gyroscopes rely on the Sagnac effect- a relativistically induced phase shift that scales linearly with the rotational velocity [2,3]. In ring laser gyroscopes (RLGs), this shift manifests itself as a resonance splitting in the emission spectrum that can be detected as a beat frequency [4]. The need for ever-more precise RLGs has fueled research activities towards devising new approaches aimed to boost the sensitivity beyond what is dictated by geometrical constraints. In this respect, attempts have been made in the past to use either dispersive or nonlinear effects [5-8]. Here, we experimentally demonstrate an altogether new route based on non-Hermitian singularities or exceptional points in order to enhance the Sagnac scale factor [9-13]. Our results not only can pave the way towards a new generation of ultrasensitive and compact ring laser gyroscopes, but they may also provide practical approaches for developing other classes of integrated sensors. Sensing involves the detection of the signature that a perturbing agent leaves on a system. In optics and many other fields, resonant sensors are intentionally made to be as lossless as possible so as to exhibit high quality factors [14-17]. -
Quantum Enhancement of the Zero-Area Sagnac Interferometer Topology for Gravitational Wave Detection
View metadata, citation and similar papers at core.ac.uk brought to you by CORE week endingprovided by MPG.PuRe PRL 104, 251102 (2010) PHYSICAL REVIEW LETTERS 25 JUNE 2010 Quantum Enhancement of the Zero-Area Sagnac Interferometer Topology for Gravitational Wave Detection Tobias Eberle,1,2 Sebastian Steinlechner,1 Jo¨ran Bauchrowitz,1 Vitus Ha¨ndchen,1 Henning Vahlbruch,1 Moritz Mehmet,1,2 Helge Mu¨ller-Ebhardt,1 and Roman Schnabel1,* 1Max-Planck-Institut fu¨r Gravitationsphysik (Albert-Einstein-Institut) and Institut fu¨r Gravitationsphysik der Leibniz Universita¨t Hannover, Callinstraße 38, 30167 Hannover, Germany 2Centre for Quantum Engineering and Space-Time Research–QUEST, Leibniz Universita¨t Hannover, Welfengarten 1, 30167 Hannover, Germany (Received 26 February 2010; published 22 June 2010) Only a few years ago, it was realized that the zero-area Sagnac interferometer topology is able to perform quantum nondemolition measurements of position changes of a mechanical oscillator. Here, we experimentally show that such an interferometer can also be efficiently enhanced by squeezed light. We achieved a nonclassical sensitivity improvement of up to 8.2 dB, limited by optical loss inside our inter- ferometer. Measurements performed directly on our squeezed-light laser output revealed squeezing of 12.7 dB. We show that the sensitivity of a squeezed-light enhanced Sagnac interferometer can surpass the standard quantum limit for a broad spectrum of signal frequencies without the need for filter cavities as required for Michelson interferometers. The Sagnac topology is therefore a powerful option for future gravitational-wave detectors, such as the Einstein Telescope, whose design is currently being studied.