PPT-Gravitational Physics using

Atom Interferometry Mark Kasevich Stanford University Lightpulse a tom interferometers 2015 laboratory sensor atomic wavepackets separate by 12 cm before interfering 1e13 g resolution after 1 hr. Chapter 2 UNITS AND MEASUREMENTS 4 hours Unitof measurement System of units SI units undamental and derived units Length mass and time measurements Accuracy and precision of measuring instruments rrors in measurement Significant figures Dimensions collapses. In . collaboration. . with. . Wen-Biao. Han, & Remo . Ruffini. . ICRANet. & . Physics. . Department. , . University. . of. . Rome. She-Sheng. . Xue. MG13, Stockholm, July 5. To demonstrate the physical reality of gravitational waves, consider the example system of the previous section. We will concentrate our attention on three of the test masses, one chosen arbitrarily from the plane, along with its nearest neighbors in the +x and +y directions. Imagine that we have equipped the mass at the vertex of this “L” with a lamp that can be made to emit very brief pulses of light. Imagine also that the two masses at the ends of the “L” are fitted with mirrors aimed so that they will return the flashes of light back toward the vertex mass. The Child of General Relativity. A Necessary Change. Concepts after Einstein :-. Time is not absolute. There is no ether frame. Notion of . spacetime. Concepts before Einstein :-. There is a preferred reference frame ether. (& Gravitons ?). -. Vishal. . Kasliwal. Classical Electromagnetism. Vacuum. Maxwell Field Equations. Light!!. Electromagnetic waves. Quantum Electromagnetism. Hamiltonian of Quantized. Field. where. ULTRA-RELATIVISTIC COLLISIONS. Theodore Tomaras. University of Crete. Motivation. The relevance of classical gravity. A slightly simpler model – scalar radiation. The local and the non-local source. Presentation for . 11. th. . Amaldi. Conference on Gravitational Waves. By. ASHOK TIWARI . June 25, 2015. Tribhuvan. University, Kathmandu, Nepal. 1. Outline. . Statement of the Problem. Introduction. versus convective . blueshifts. , and wavelength variations across stellar disks. Dainis Dravins. – Lund . Observatory. , Sweden. www.astro.lu.se. /~. dainis. KVA. IAU Comm.30, IAU XXVIII GA Beijing, August 2012. Overview of Why and How. Dan Burbank and Tony Young. AST5022. Introduction. Background. Physics. Sources. Detectors and Detector Implications. Questions. Gravitational Waves . Speed-of-light wave propagation solution of Einstein’s Field Equations. Interferometry. Prof. Mark Kasevich. Dept. of Physics and Applied Physics. Stanford University, Stanford CA. Atom . interferometric. inertial sensors. Pulses of light are used to coherently manipulated the center-of-mass motion of atomic . European Gravitational Observatory. EGO. “Raison d'être”, origin, structure . & future perspectives. Federico Ferrini . – EGO Director. Welcome to. The Einstein Telescope. Design Study Presentation. -12 . cm. A world-shaking discovery. James Clerk Maxwell. Professor at King’s College. London: 1860 – 1865. Unified theory of electricity and . . magnetism. Predicted electromagnetic waves. Identified light as due to these waves. https://www.ligo.caltech.edu/system/video_items/files/4/EinsteinsMessengerLIGO.mp4?1436490806. 2017 Nobel Prize in Physics. : Rainer Weiss - Barry C. . Barish. -Kip S. . Thorne. "for . decisive contributions to the LIGO detector and the observation of gravitational waves". Learn how to excel in AP Physics with this comprehensive guide. Explore essential concepts, study strategies, and resources to ace your AP Physics exam.