PPT-Macroscopic Interferometry

Achuta Kadambi MIT Media Lab Joint work with Jamie Schiel and Ramesh Raskar Computer VisionGraphics Computer VisionGraphics RealLife Electric field only shown 700 nanometer wavelength. measurements: . One physicist’s crooked . path from quantum optics to quantum information. Introduction . Squeezed states and optical . interferometry. Ramsey . interferometry. and cat states. Quantum information perspective. Berlin/. Zeuthen. ;. . May 2010. Dainis Dravins & . Hannes. Jensen. Lund Observatory, Sweden. www.astro.lu.se. /~dainis. HUNDRED TIMES SHARPER THAN . HUBBLE !. Intensity Interferometry with. . deformed. . commutators. . with. . macroscopic. . harmonic. . oscillators. Francesco . Marin. HUMOR. H. eisenberg . . U. ncertainty . M. easured with . O. pto. -mechanical . R. esonators. limits on . dark . energy. Jun. 17. 2011. Geena Kim. P. Hamilton, D. Schlippe, and H. Mueller. University of California, Berkeley. Paul Hamilton. Müller group. University of California at Berkeley. . Clare Burrage. University of Nottingham. Clare.Burrage@nottingham.ac.uk. Outline:. Chameleon dark energy. A . review of atom interferometry. Dark energy in the laboratory. Solutions to the Cosmological Constant Problem. Macroscopic Review - #1. When mold begins growing on an object, describe what is happening.. The fungus releases strong juices (enzymes) that break down the plant and animal matter. A typical fungus is made up of tiny tubes called “. of Ferromagnetic Nematics. Author: Tilen Potisk. Advisor: Doc. Dr. Daniel Svenšek. OUTLINE. Motivation. Theory of Macroscopic Dynamics. Experiments. Numerical results. Conclusion. MOTIVATION. Hypothesized in 1970 (Brochard and de Gennes).. Jonathan Singh . (. jonathan.singh@ed.ac.uk. ). A Curtis, I Main, A . Cartwright-Taylor, I . B . Butler, M Chapman, F . Fusseis. Outline. What is the Velocity?. CWI for Monitoring Velocity Change. Experimental Rock Physics Applications. Material for this talk: A.M.S. Richards, T.W.B.Muxlow, N.J.Jackson (JBCA Manchester); . R.A.Laing (ESO Garching); I. Marti-Vidal (OSO, Onsala); R. Perley (NRAO Socorro) and Wikipedia. Summary. Radio astronomy – key aspects. Dainis Dravins, . Hannes. Jensen . Lund Observatory, Sweden. Stephan LeBohec, Paul D.. . Nuñez. . The University of Utah, Salt Lake City. STELLAR INTENSITY INTERFEROMETRY. . Astrophysical targets for sub-. Very Long Baseline Interferometry. Very Long Baseline Interferometry. time.  . θ.  . t. Very Long Baseline Interferometry. Moving Sources.  .  .  .  .  .  . 0 .  .  .  .  .  .  . What is the signal made of?. during the last decade. Olivier CHESNEAU. delivered and distorted by John . Monnier. 2. 3. Albert A. Michelson (1852-1931). 1974: I2T. 4. . MIDI . First direct recombination (2T) in the mid-IR (8-13. microscopic states?. Hydrogen Atom. A particle in a 3D Box. Binary Model System. A System with Three Magnetic Dipoles. A Binary Alloy with two . c. hemical components . G. ussian. Approximation. Achuta . Kadambi. , Jamie . Schiel. and Ramesh . Raskar. , IEEE CVPR16 . An interferometric 3D camera for multipath imaging for meter scale scenes. Swept Frequency Electronic Interferometry. Take-home message:.