Quantum evolution

Results: 71



#Item
11THE QUANTUM STRUCTURE OF GALAXIES IN KEV FERMIONIC WARM DARK MATTER H. J. de Vega LPTHE, CNRS/Universite´ P & M Curie (Paris VI). Chalonge Meudon Workshop 2014: From Large to Small Scale Structures in

THE QUANTUM STRUCTURE OF GALAXIES IN KEV FERMIONIC WARM DARK MATTER H. J. de Vega LPTHE, CNRS/Universite´ P & M Curie (Paris VI). Chalonge Meudon Workshop 2014: From Large to Small Scale Structures in

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Source URL: chalonge.obspm.fr

Language: English - Date: 2014-06-10 03:20:44
12Scientific Inquiry, vol. 8, No.1, June, 2007, pp. 29 – 34 IIGSS Academic Publisher BASIC FREQUENCY OF A-TEMPORAL PHYSICAL SPACE AS A DRIVING FORCE OF EVOLUTION

Scientific Inquiry, vol. 8, No.1, June, 2007, pp. 29 – 34 IIGSS Academic Publisher BASIC FREQUENCY OF A-TEMPORAL PHYSICAL SPACE AS A DRIVING FORCE OF EVOLUTION

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Source URL: fqxi.org

Language: English - Date: 2014-05-14 09:24:18
13The Time-Dependent Schr¨ odinger Equation Physics 3300, Weber State University, Spring Semester, 2012 In this project you will create a simulation to predict the time evolution of a quantum particle in one dimension. Yo

The Time-Dependent Schr¨ odinger Equation Physics 3300, Weber State University, Spring Semester, 2012 In this project you will create a simulation to predict the time evolution of a quantum particle in one dimension. Yo

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Source URL: physics.weber.edu

Language: English - Date: 2012-03-05 11:53:38
14Bounds on non-adiabatic evolution in single-field inflation Peter Adshead1, 2 and Wayne Hu3, 4 arXiv:1402.1677v1 [astro-ph.CO] 7 Feb

Bounds on non-adiabatic evolution in single-field inflation Peter Adshead1, 2 and Wayne Hu3, 4 arXiv:1402.1677v1 [astro-ph.CO] 7 Feb

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Source URL: background.uchicago.edu

Language: English - Date: 2015-01-06 12:05:25
15PHYSICAL REVIEW B 69, 035210 共2004兲 Evolution of voids in Al¿ -implanted ZnO probed by a slow positron beam Z. Q. Chen, M. Maekawa, S. Yamamoto, and A. Kawasuso Advanced Science Research Center, Japan Atomic Energy

PHYSICAL REVIEW B 69, 035210 共2004兲 Evolution of voids in Al¿ -implanted ZnO probed by a slow positron beam Z. Q. Chen, M. Maekawa, S. Yamamoto, and A. Kawasuso Advanced Science Research Center, Japan Atomic Energy

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Source URL: www.geocities.jp

Language: English - Date: 2004-02-02 06:41:33
16COPYRIGHT NOTICE: Dan Maoz: Astrophysics in a Nutshell is published by Princeton University Press and copyrighted, © 2007, by Princeton University Press. All rights reserved. No part of this book may be reproduced in an

COPYRIGHT NOTICE: Dan Maoz: Astrophysics in a Nutshell is published by Princeton University Press and copyrighted, © 2007, by Princeton University Press. All rights reserved. No part of this book may be reproduced in an

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Source URL: press.princeton.edu

Language: English - Date: 2007-02-26 14:24:26
17The maximum speed of dynamical evolution Norman Margolus 1 Boston University Center for Computational Science and MIT Artificial Intelligence Laboratory Lev B. Levitin

The maximum speed of dynamical evolution Norman Margolus 1 Boston University Center for Computational Science and MIT Artificial Intelligence Laboratory Lev B. Levitin

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Source URL: people.csail.mit.edu

Language: English - Date: 2005-01-16 13:05:58
18PHYSICAL REVIEW B 75, 245206 共2007兲 Thermal evolution of defects in as-grown and electron-irradiated ZnO studied by positron annihilation Z. Q. Chen* and S. J. Wang Hubei Nuclear Solid Physics Key Laboratory, Depart

PHYSICAL REVIEW B 75, 245206 共2007兲 Thermal evolution of defects in as-grown and electron-irradiated ZnO studied by positron annihilation Z. Q. Chen* and S. J. Wang Hubei Nuclear Solid Physics Key Laboratory, Depart

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Source URL: www.geocities.jp

Language: English - Date: 2007-11-11 12:26:46
19Curvelets Wave Evolution On the Evolution of Curvelets by the Wave Equation Hart F. Smith

Curvelets Wave Evolution On the Evolution of Curvelets by the Wave Equation Hart F. Smith

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Source URL: www.math.washington.edu

Language: English - Date: 2009-07-01 17:18:19
20Astronomy How does cosmic structure form? We study planets, stellar evolution, stellar seismology, compact stellar remnants, gravity waves, neutron star emission, supernovae, gamma-ray bursters, galaxy dynamics and evolu

Astronomy How does cosmic structure form? We study planets, stellar evolution, stellar seismology, compact stellar remnants, gravity waves, neutron star emission, supernovae, gamma-ray bursters, galaxy dynamics and evolu

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Source URL: physics.unc.edu

Language: English - Date: 2014-11-12 17:54:38