PPT-Gravitational Physics with Atom

Author : lois-ondreau | Published Date : 2017-12-17

Interferometry Prof Mark Kasevich Dept of Physics and Applied Physics Stanford University Stanford CA Atom interferometric inertial sensors Pulses of light are

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Gravitational Physics with Atom: Transcript


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 centerofmass motion of atomic . 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. Also Known As. Static Electricity. Chemistry Refresher. Atom. the basic unit that makes up all . matter. Made up of protons, neutrons, and electrons. Chemistry Refresher. Proton. Part of an atom that has a positive charge. Dipartimento. . di. . Fisica. . U. niversità. . di. Roma . La . Sapienza. & . INFN . Sezione. . di. Roma. Napoli 2 . Aprile. 2014. Experimental Gravitation. Theoretical motivations . supporting the new deal of experiments in Gravitation. 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. Yair . Margalit. The Atom Chip . Group. Ben-Gurion University. www.bgu.ac.il/atomchip. Y. . Margalit, Z. Zhou, S. . Machluf. , D. . Rohrlich. , Y. . Japha. ,. and R. . Folman. , Science . 349. , 1205 (2015).. "for decisive contributions to the LIGO detector and the observation of gravitational waves". Peter Berg. Department of Science. University of Alberta. www.peterberg.net . Source: https://www.mpg.de/11646260/neutron-star-merger-gravitational-waves. Objectives of the presentation. To get an appreciation of the role of . physics . in . our day to day living. Acquaint ourselves to a novel and . widely used . research tool: Mass Spectrometer. To . introduce the basic physics of mass . Objectives of the presentation. To get an appreciation of the role of . physics . in . our day to day living. Acquaint ourselves to a novel and . widely used . research tool: Mass Spectrometer. To . introduce the basic physics of mass . European Gravitational Observatory. EGO. “Raison d'être”, origin, structure . & future perspectives. Federico Ferrini . – EGO Director. Welcome to. The Einstein Telescope. Design Study Presentation. Atom . Interferometry. Mark Kasevich. Stanford University. Light-pulse . a. tom interferometers. 2015 laboratory sensor, atomic wavepackets separate by 12 cm before interfering, . 1e-13 . g resolution after 1 hr.. P3 Challenge – A rotating fan completes 1200 revolutions every minute. Consider the tip of a blade, at a radius of 0.15 m. a) Through what distance does the tip move in one revolution? What are b) the tip’s speed and c) the magnitude of its centripetal acceleration? . Tim Kovachy. Department of Physics and Astronomy and Center for Fundamental Physics, Northwestern University. NPS Colloquium. February 1, 2019 . Conceptual overview of atom interferometry. Motivation for gravitational wave detection in the “mid-band” frequency range of ~ 0.1 Hz to 10 Hz. Mark Kasevich. Stanford Physics (Prof. Physics and Applied Physics). AOSense. , Inc. (Consulting Chief Scientist). Young’s double slit with atoms. Young’s 2 slit with Helium atoms. Slits. Interference fringes. Tim Kovachy. Department of Physics and Astronomy and Center for Fundamental Physics (CFP), Northwestern University. CPAD 2021. Brief overview of atom interferometry. Enabling technology advances for large-area/long-baseline atom interferometry demonstrated with 10-meter baselines.

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