PPT-Cosmic Structure as the Quantum Interference of a Coherent

Author : olivia-moreira | Published Date : 2017-12-21

HsiYu Schive 薛熙于 Tzihong Chiueh 闕志鴻 Tom Broadhurst PASCOS Nov 24 2013 Outline Introduction Cold dark matter CDM vs wave dark matter ѱ DM

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Cosmic Structure as the Quantum Interference of a Coherent: Transcript


HsiYu Schive 薛熙于 Tzihong Chiueh 闕志鴻 Tom Broadhurst PASCOS Nov 24 2013 Outline Introduction Cold dark matter CDM vs wave dark matter ѱ DM . particles and. distributions. of . particles . Robin . Hogan and Chris Westbrook. Deptartment. of Meteorology, University . of . Reading. 25 March 2014. Overview. Motivation. We need to be able to model the backscattered signal from clouds in order to interpret radar and lidar observations (particularly from space) in terms of cloud properties. One-dimensional ballistic/coherent transport. Landauer theory. The role of contacts. Quantum of electrical and thermal conductance. One-dimensional Wiedemann-Franz law. 1. “Ideal” Electrical Resistance in 1-D. reionization. : The last frontier in observational cosmology . . Chris Carilli (. NRAO. ). Summer . Student Lecture July 2010. Brief introduction to cosmic . reionization. Current observational constraints on . Quantum Computation. Sandy . Irani. Department of Computer Science. University of California, Irvine. “Simulating Physics with Computers”. Richard Feynman . – . Keynote Talk, 1. st. Conference on . Nuclear landscape. General . principles. Nuclear structure I (preliminaries). Witek. . Nazarewicz (UTK/. ORNL. ). National Nuclear Physics Summer School . 2014. William & Mary, VA. nuclear structure & reactions. A Copernican View. C. S. Unnikrishnan. Gravitation Lab, . Tata Institute of Fundamental Research, . Homi Bhabha Road, Mumbai 400005, India. . E-mail address: . unni@tifr.res.in. Website: . www.tifr.res.in/~filab. McsQPT. ). Joint work with: . S. . Rahimi-Keshari. , A. T. . Rezakhani. , T. C. Ralph. Masoud. Ghalaii. Nov. 2013. 1. Basic concepts—Phase space, Wigner . function, . HD, … . Harmonic oscillator. . Gödel-Cohen Incompleteness. and the Universe. Luis Gonzalez-Mestres. Cosmology Laboratory, John . Naisbitt. University. Belgrade and Paris. Abstract –. . What is the origin of Quantum Mechanics (QM)? Is it an ultimate principle of Physics or a property of standard particles generated at a more fundamental level?. ’. t understood it.. ”. --Niels Bohr. . The Quantum Information Revolution. . Paul Kwiat. DARPA. Kwiat’s. Quantum. Clan (2012). Graduate Students:. . Rebecca Holmes. . Aditya. Sharma. “Interacting Atomic Interferometry for Rotation Sensing Approaching the Heisenberg Limit,” . S. . Ragole. and J.M. Taylor, Phys. Rev. Lett., 117, 203002 . (. 2016). A ring-shaped arrangement of atoms, coaxed into a swirling quantum superposition by lasers, could probe gravity's strength down to very small scales. (Credit: E. Edwards/JQI). 2nd Millennium BCE. BC. . . Mesopotamian cosmology . has a flat,circular Earth enclosed in a cosmic Ocean. 12. th. century BCE. C. . Rigveda. has some cosmological hymns, most notably the Nasadiya Sukta. Physics . 2212. Light. Light has Wave properties. Light can Diffract. Light can Interfere. Constructively. Destructively. Wave Fronts. Lines that are perpendicular to the motion of the wave, indicate the location of the crests in the waves that are traveling together.. The Last Epoch Cosmic Structure Formation Today we have a matter-dominated universe ruled by the force of gravity. Slight variations in density produces formation regions for stars and galaxies. 1 st Minati. Barman. Head, Department of Physics. J N . College,Boko. Contents:. Conditions of observable interference. Fresnel’s biprism Experiment. Conditions of observable interference:. To obtain well-defined interference fringes following conditions must be satisfied-.

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