Single Photon Michelson-Morley Experiment Via De Broglie-Bohm Picture: an Interpretation Based on the Hypothesis of Frame Dragging
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A Basic Michelson Laser Interferometer for the Undergraduate Teaching Laboratory Demonstrating Picometer Sensitivity Kenneth G
A basic Michelson laser interferometer for the undergraduate teaching laboratory demonstrating picometer sensitivity Kenneth G. Libbrechta) and Eric D. Blackb) 264-33 Caltech, Pasadena, California 91125 (Received 3 July 2014; accepted 4 November 2014) We describe a basic Michelson laser interferometer experiment for the undergraduate teaching laboratory that achieves picometer sensitivity in a hands-on, table-top instrument. In addition to providing an introduction to interferometer physics and optical hardware, the experiment also focuses on precision measurement techniques including servo control, signal modulation, phase-sensitive detection, and different types of signal averaging. Students examine these techniques in a series of steps that take them from micron-scale sensitivity using direct fringe counting to picometer sensitivity using a modulated signal and phase-sensitive signal averaging. After students assemble, align, and characterize the interferometer, they then use it to measure nanoscale motions of a simple harmonic oscillator system as a substantive example of how laser interferometry can be used as an effective tool in experimental science. VC 2015 American Association of Physics Teachers. [http://dx.doi.org/10.1119/1.4901972] 8–14 I. INTRODUCTION heterodyne readouts, and perhaps multiple lasers. Modern interferometry review articles tend to focus on complex optical Optical interferometry is a well-known experimental tech- configurations as well,15 as they offer improved sensitivity and nique for making precision displacement measurements, stability over simpler designs. While these advanced instru- with examples ranging from Michelson and Morley’s famous ment strategies are becoming the norm in research and indus- aether-drift experiment to the extraordinary sensitivity of try, for educational purposes we sought to develop a basic modern gravitational-wave detectors. -
Detector Description and Performance for the First Coincidence
ARTICLE IN PRESS Nuclear Instruments and Methods in Physics Research A 517 (2004) 154–179 Detector description and performance for the first coincidence observations between LIGO and GEO B. Abbotta, R. Abbottb, R. Adhikaric, A. Ageevao,1, B. Allend, R. Amine, S.B. Andersona, W.G. Andersonf, M. Arayaa, H. Armandulaa, F. Asiria,2, P. Aufmuthg, C. Aulberth, S. Babaki, R. Balasubramaniani, S. Ballmerc, B.C. Barisha, D. Barkeri, C. Barker-Pattonj, M. Barnesa, B. Barrk, M.A. Bartona, K. Bayerc, R. Beausoleill,3, K. Belczynskim, R. Bennettk,4, S.J. Berukoffh,5, J. Betzwieserc, B. Bhawala, I.A. Bilenkoao, G. Billingsleya, E. Blacka, K. Blackburna, B. Bland-Weaverj, B. Bochnerc,6, L. Boguea, R. Borka, S. Bosen, P.R. Bradyd, V.B. Braginskya,o, J.E. Brauo, D.A. Brownd, S. Brozekg,7, A. Bullingtonl, A. Buonannop,8, R. Burgessc, D. Busbya, W.E. Butlerq, R.L. Byerl, L. Cadonatic, G. Cagnolik, J.B. Campr, C.A. Cantleyk, L. Cardenasa, K. Carterb, M.M. Caseyk, J. Castiglionee, A. Chandlera, J. Chapskya,9, P. Charltona, S. Chatterjic, Y. Chenp, V. Chickarmanes, D. Chint, N. Christensenu, D. Churchesi, C. Colacinog,v, R. Coldwelle, M. Colesb,10, D. Cookj, T. Corbittc, D. Coynea, J.D.E. Creightond, T.D. Creightona, D.R.M. Crooksk, P. Csatordayc, B.J. Cusackw, C. Cutlerh, E. D’Ambrosioa, K. Danzmanng,v,x, R. Daviesi, E. Daws,11, D. DeBral, T. Delkere,12, R. DeSalvoa, S. Dhurandary,M.D!ıazf, H. Dinga, R.W.P. Dreverz, R.J. Dupuisk, C. Ebelingu, J. Edlunda, P. Ehrensa, E.J. -
THE MICHELSON INTERFEROMETER Intermediate ( First Part) to Advanced (Latter Parts)
THE MICHELSON INTERFEROMETER Intermediate ( first part) to Advanced (latter parts) Goal: There is a progression of goals for this experiment but you do not have to do Reading: the last goal. The first goal is to align the interferometer and calibrate it. Calibration ADC should be done both mechanically and Michelson program writeup optically with a HeNe laser. The second Stepper motors goal is a study of the sodium doublet. One measures the average wavelength of the two Good optics text lines and the separation of the lines. The Fourier transforms and FFT final experimental goal is to find interference fringes for white light and measure it’s coherence length. Homework: 1. Indicate how the standard michelson interferometer optics is the same as the Introduction: optics shown in fig. 2. Figure 1 The optics of the Michelson Interferometer. Note the light directed away from the mirrors is offset from the light directed toward the mirrors for clarity Note: The observation of fringes associated with the sodium doublet is a rather difficult Figure 2 The optics of the Michelson experiment and the observation of white Interferometer is equivalent to the that of light fringes is even more difficult. two sources S1 ans S2, that are emitting Understanding how the concept of light that is in phase. Note: source S1 is coherence length relates to this experiment movable. is almost essential to complete these goals. 2. Explain changes the optics in fig.1 and 2 required to account for the finite size of the light source Page -1- 3. For the optics shown in fig.2, at what Experimental tasks distance should the detector (eye) be There are three experimental tasks, focused? but only the first two are required. -
On the Phenomena of Optodynamics
Crimson Publishers Mini Review Wings to the Research On the Phenomena of Optodynamics Bagrat Melkoumian* Prokhorov General Physics Institute, Russian Academy of Sciences, Russia Abstract Precise optical devices for full measurement of the accelerated motion are presented. The proposed devices are implemented on the basis of the linear semiconductor laser, without moving or tensioned parts and without ring resonators, and could be arranged on the belt fastened around the object to be measured. Presented method consists in the using of standing wave of the coherent radiation in the resonator as the sensitive element of the accelerated movement measurement. Keywords: Accelerometer, Control, Navigation, Linear laser resonator, Optodynamics Introduction Known phenomena of Optodynamics in moving resonators We consider the dynamic action of external forces on a rigid resonator with an invariable geometry, with resonator elements and a photodetector stationary relative to each other during the interaction time, which leads to an accelerated motion of the resonator with radiation. We also consider the radiation medium to be stationery and uniform in the intrinsic frame of *Corresponding author: Prokhorov constant. At the same time, the movement of the source and the receiver of radiation relative reference of the moving resonator, when the dielectric ε and the magnetic μ permeability are General Physics Institute, Russian to each other under the action of external forces, or the movement of the active medium [1,2] Academy of Sciences, ul. Vavilova 38, Moscow, 119991, Russia in the cavity, additionally lead to the Doppler, Fresnel-Fizeau effects, etc. [3,4]. Today, the term “Optodynamics” corresponds to the processes of motion of particles of a medium under the Submission: August 18, 2020 Published: September 15, 2020 Optodynamics in moving resonators” is used to refer to phenomena in the case of uneven influence of light, including laser cutting and drilling. -
Increasing the Sensitivity of the Michelson Interferometer Through Multiple Reflection Woonghee Youn
Rose-Hulman Institute of Technology Rose-Hulman Scholar Graduate Theses - Physics and Optical Engineering Graduate Theses Summer 8-2015 Increasing the Sensitivity of the Michelson Interferometer through Multiple Reflection Woonghee Youn Follow this and additional works at: http://scholar.rose-hulman.edu/optics_grad_theses Part of the Engineering Commons, and the Optics Commons Recommended Citation Youn, Woonghee, "Increasing the Sensitivity of the Michelson Interferometer through Multiple Reflection" (2015). Graduate Theses - Physics and Optical Engineering. Paper 7. This Thesis is brought to you for free and open access by the Graduate Theses at Rose-Hulman Scholar. It has been accepted for inclusion in Graduate Theses - Physics and Optical Engineering by an authorized administrator of Rose-Hulman Scholar. For more information, please contact bernier@rose- hulman.edu. Increasing the Sensitivity of the Michelson Interferometer through Multiple Reflection A Thesis Submitted to the Faculty of Rose-Hulman Institute of Technology by Woonghee Youn In Partial Fulfillment of the Requirements for the Degree of Master of Science in Optical Engineering August 2015 © 2015 Woonghee Youn 2 ABSTRACT Youn, Woonghee M.S.O.E Rose-Hulman Institute of Technology August 2015 Increase a sensitivity of the Michelson interferometer through the multiple reflection Dr. Charles Joenathan Michelson interferometry has been one of the most famous and popular optical interference system for analyzing optical components and measuring optical metrology properties. Typical Michelson interferometer can measure object displacement with wavefront shapes to one half of the laser wavelength. As testing components and devices size reduce to micro and nano dimension, Michelson interferometer sensitivity is not suitable. The purpose of this study is to design and develop the Michelson interferometer using the concept of multiple reflections. -
The Holometer: a Measurement of Planck-Scale Quantum Geometry
The Holometer: A Measurement of Planck-Scale Quantum Geometry Stephan Meyer November 3, 2014 1 The problem with geometry Classical geometry is made of definite points and is based on “locality.” Relativity is consistent with this point of view but makes geometry “dynamic” - reacts to masses. Quantum physics holds that nothing happens at a definite time or place. All measurements are quantum and all known measurements follow quantum physics. Anything that is “real” must be measurable. How can space-time be the answer? Stephan Meyer SPS - November 3, 2014 2 Whats the problem? Start with - Black Holes What is the idea for black holes? - for a massive object there is a surface where the escape velocity is the speed of light. Since nothing can travel faster than the speed of light, things inside this radius are lost. We can use Phys131 to figure this out Stephan Meyer SPS - November 3, 2014 3 If r1 is ∞, then To get the escape velocity, we should set the initial kinetic energy equal to the potential energy and set the velocity equal to the speed of light. Solving for the radius, we get Stephan Meyer SPS - November 3, 2014 4 having an object closer than r to a mass m, means it is lost to the world. This is the definition of the Schwarzshild radius of a black hole. So for stuff we can do physics with we need: Stephan Meyer SPS - November 3, 2014 5 A second thing: Heisenberg uncertainty principle: an object cannot have its position and momentum uncertainty be arbitrarily small This can be manipulated, using the definition of p and E to be What we mean is that to squeeze something to a size λ, we need to put in at least energy E. -
High-Stability Single-Frequency Green Laser with a Wedge Nd:YVO4 As a Polarizing Beam Splitter
Optics Communications 283 (2010) 309–312 Contents lists available at ScienceDirect Optics Communications journal homepage: www.elsevier.com/locate/optcom High-stability single-frequency green laser with a wedge Nd:YVO4 as a polarizing beam splitter Yaohui Zheng, Fengqin Li, Yajun Wang, Kuanshou Zhang *, Kunchi Peng State Key Laboratory of Quantum Optics and Quantum Optics Devices, Institute of Opto-Electronics, Shanxi University, Taiyuan 030006, China article info abstract Article history: The effect of the large power depletion of the fundamental wave in the phase-matched polarization on Received 17 May 2009 the stability of the second-harmonic wave output from an intracavity frequency-doubled ring laser is dis- Received in revised form 11 July 2009 cussed. It has been demonstrated that the instability resulting from the unbalanced power depletion of Accepted 5 October 2009 the fundamental waves can be eliminated by using a wedge laser rod. The function dependence of the wedge angle and the laser power is concluded. An intracavity frequency-doubled ring laser with a wedge Nd:YVO4 laser crystal and a LBO doubler is designed and built. Comparing with similar lasers but without using the wedge laser crystal, the frequency-conversion efficiency, the power stability and the polariza- tion purity of the second-harmonic wave output from the laser with a wedge laser rod are significantly improved. The single-frequency green laser of 6.5 W at 532 nm, with the polarization degree more than 500:1 and the power stability better than ±0.3% for 3 h, was experimentally achieved. Ó 2009 Elsevier B.V. All rights reserved. -
Canterbury Ring Laser and Tests for Nonreciprocal Phenomena*
Aust. J. Phys., 1993, 46, 87-101 Canterbury Ring Laser and Tests for Nonreciprocal Phenomena* G. E. Stedman, H. R. Bilger,A Li Ziyuan, M. P. Poulton, C. H. Rowe, 1. Vetharaniam and P. V. Wells Department of Physics, University of Canterbury, Christchurch 1, New Zealand. A School of Electrical and Computer Engineering, Oklahoma State University, Stillwater, OK 74078-0321, U.S.A. Abstract An historic and simple experiment has been revitalised through the availability of supercavity mirrors and also through a heightened interest in interferometry as a test of physical theory. We describe our helium-neon ring laser, and present results demonstrating a fractional frequency resolution of 2·1x10-18 (1·0 mHz in 474 THz). The rotation of the earth unlocks the counterrotating beams. A new field of spectroscopy becomes possible, with possible applications to geophysical measurements such as seismic events and earth tides, improved measurements of Fresnel drag, detection of ultraweak nonlinear optical propert~es of matter, and also searches for preferred frame effects in gravitation and for pseudoscalar particles. 1. Introduction A few years after the advent of the laser, Macek and Davis (1963) demonstrated the first ring laser, and also its unique potential as a rotation detector via the Sagnac effect. The optical lengths of the closed paths for the counterpropagating beams are made unequal by rotation of the whole device. In an active device the frequencies adapt to this, the corotating beam becoming more red and the counterrotating beam more blue (Heer 1964). Both beams take essentially the same path within the cavity, so that when the beams transmitted at any mirror interfere, the resulting beat frequency 8f reflects only the difference in optical path length, and not any common-mode effects such as frequency jitter. -
1 Laboratory 8: Michelson Interferometer 1.1 Theory: References:Optics,E.Hecht,Sec 9.4
1051-232-20033 Imaging Systems Laboratory II Week of 5/3/2004, Writeup Due 5/18/2004 (T) 1 Laboratory 8: Michelson Interferometer 1.1 Theory: References:Optics,E.Hecht,sec 9.4 1.1.1 Division-of-Wavefront Interferometry In the last lab, you saw that coherent (single-wavelength) light from point sources two different locations in an optical beam could be combined after having traveled along two different paths. The recombined light exhibited sinusoidal fringes whose spatial frequency depended on the difference in angle of the light beams when recombined. The regular variation in relative phase of the light beams resulted in constructive interference (when the relative phase difference is 2πn,wheren is an integer) and destructive interference where the relative phase difference is 2πn + π. The centers of the “bright” fringes occur where the optical paths differ by an integer multiple of λ0. “Division-of-Wavefront” Interferometry via Young’s Two-Slit Experiment. The period of the intensity fringes at the observation plane is D Lλ . ' d 1.1.2 Division-of-Amplitude Interferometry This laboratory will introduce a second class of interferometer where the amplitude of the light is separated into two (or more) parts at the same point in space via partial reflection by a beamsplitter. The beamsplitter is the light-dividing element in several types of interferometers. This lab will demostrate the action of the Michelson interferometer for both coherent light from a laser and for white light (with some luck!). Coherence of a Light Source If two points within the same beam of light exhibit a consistent and measurable phase difference, then the light at the two points is said to be coherent, and thus 1 the light at these two locations may be combined to create interference. -
Single-Frequency Fiber Ring Laser with 1W Output Power at 1.5 Mm
Single-frequency fiber ring laser with 1 W output power at 1.5 µm Alexander Polynkin, Pavel Polynkin, Masud Mansuripur, N. Peyghambarian Optical Sciences Center, University of Arizona, 1630 E. University Blvd., Tucson, AZ 85721 [email protected] Abstract: We report a single-frequency fiber laser with 1 W output power at 1.5 µm which is to our knowledge, five times the highest power from a single-frequency fiber laser reported to-date. The short unidirectional ring cavity approach is used to eliminate the spatial gain hole-burning associated with the standing-wave laser designs. A heavily-doped phosphate fiber inside the ring resonator serves as the active medium of the laser. Up to 700 mW of output power, the longitudinal mode hops have been completely eliminated by using the adjustable coupled-cavity approach. At higher power levels, the laser still oscillates at a single longitudinal mode, but with infrequent mode hops that occur at a rate of few hops per minute. Compared to the Watt-level single-frequency amplified sources, our approach is simpler and offers better noise performance. © 2005 Optical Society of America OCIS codes: (060.2320) Fiber optics amplifiers and oscillators; (140.3510) Lasers, fiber; (140.3560) Lasers, ring; (140.3570) Lasers, single-mode References and links 1. C. Alegria, Y. Jeong, C. Codemard, J. K. Sahu, J. A. Alvarez-Chavez, L. Fu, M. Ibsen, and J. Nilsson, ”83- W Single-Frequancy Narrow-Linewidth MOPA Using Large-Core Erbium-Ytterbium Co-Doped Fiber,” IEEE Photon. Technol. Lett. 16, 1825–1827 (2004). 2. S. Alam, K. -
Integrated Optical Ti:Linbo3 Ring Resonator for Rotation Rate Sensing C
WE1 Integrated Optical Ti:LiNbO3 Ring Resonator for Rotation Rate Sensing C. Vannahme, H. Suche, S. Reza, R. Ricken, V. Quiring, and W. Sohler Angewandte Physik, Universität Paderborn, Warburger Str. 100, 33098 Paderborn, Germany email: [email protected] Abstract: Design, fabrication, packaging, and cha- Light can be coupled to the ring via a directional racterization of a high finesse Ti:LiNbO3 integrated coupler connecting a straight waveguide and the re- optical ring resonator are reported. First results of sonator. rotation rate sensing are presented. The directional coupler determines to a large degree the properties of the resonator and – as a consequen- Introduction ce – the properties of the rotation rate sensor. It is Optical rotation rate sensors utilizing the Sagnac ef- formed by the straight and the curved waveguides fect are attractive devices, which - in contrast to their approaching each other. As the Ti:LN waveguides mechanical counterparts - have no moving parts [1]. are anisotropic with polarization dependent mode Active ring laser gyroscopes and passive fiberoptic field dimensions also the properties of the directio- gyroscopes of high resolution are already used suc- nonal coupler will be polarization dependent. Never- cessfully for navigation of aircrafts and ships. How- theless, we will consider in the following the TE-po- ever, for consumer needs with low and medium reso- larization only as the corresponding waveguide los- lution like in car navigation and robotics, less com- ses are smaller than those of the TM-mode. There- plex and cheaper sensors systems are needed suited fore, for a given polarization (and wavelength) there for volume production. -
Modeling, Estimation and Control of Ring Laser Gyroscopes for the Accurate Estimation of the Earth Rotation
Sede Amministrativa: Università degli Studi di Padova Dipartimento di: INGEGNERIA DELL’INFORMAZIONE Scuola di dottorato di ricerca in: SCIENZE E TECNOLOGIE DELL’INFORMAZIONE Ciclo: 27° TITOLO TESI: Modeling, estimation and control of ring Laser Gyroscopes for the accurate estimation of the Earth rotation Direttore della Scuola : Ch.mo Prof. Matteo Bertocco Coordinatore : Ch.mo Prof. Carlo Ferrari Supervisore : Ch.mo Prof. Alessandro Beghi Dottorando: Davide Cuccato MODELING, ESTIMATION AND CONTROL OF RING LASER GYROSCOPES FOR THE ACCURATE ESTIMATION OF THE EARTH ROTATION davide cuccato Information Engineering Department (DEI) Faculty of Engineering University of Padua, Universitá degli studi di Padova February, 18, 2015 – version 2 Davide Cuccato: Modeling, estimation and control of ring Laser Gyro- scopes for the accurate estimation of the Earth rotation, © February, 18, 2015 supervisors: Alessandro Beghi Antonello Ortolan location: Padova, (Italy) time frame: February, 18, 2015 ...Ho presentato il dorso ai flagellatori, la guancia a coloro che mi strappavano la barba; non ho sottratto la faccia agli insulti e agli sputi.... —Libro di Isaia 50, 6.— Dedicated to the loving memory of Giovanni Toso. 1986 – 2014 ABSTRACT He Ne ring lasers gyroscopes are, at present, the most precise de- − vices for absolute angular velocity measurements. Limitations to their performances come from the non-linear dynamics of the laser. Ac- cordingly to the Lamb semi-classical theory of gas lasers, a model can be applied to a He–Ne ring laser gyroscope to estimate and remove the laser dynamics contribution from the rotation measurements. We find a set of critical parameters affecting the long term stabil- ity of the system.