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ASIC needs for “observational cosmology” Gary S Varner University of Hawai’i HEPIC 2013 LBNL May 30th 2013 2 What’s in out • Very broad topic minimize overlap with…
1. QUANTUM CRYPTOGRAPHY Jennifer Nalley 2008 2. Cryptography κρυπτόσ(kryptós) “ hidden” + γράφω(grápho) “ write” = Hidden Writing 3. Classic Cryptography…
Slide 1 QUANTUM MECHANICS AND QUANTUM INFORMATION SCIENCE WHAT IS Ψ? Slide 2 IS Ψ ONTIC OR EPISTEMIC? WHAT IS A QUANTUM MEASUREMENT? Slide 3 QUANTUM PARADOXES THE DOUBLE-SLIT:…
Slide 1Ch. 23 - Cosmology Part 2 The Beginning & the End Slide 2 Skip Forward to 1964 Penzias & Wilson discover isotropic emission at λ=7.35 cm. If a blackbody,…
by Tomislav Prokopec A. The Friedmann-Lamatre-Robertson-Walker (FLRW) cosmology 1. The metric tensor We now consider the most general homogeneous space times, the Friedmann-Lematre-Robertson-
Slide 1 An Overview of Modern Cosmology Strings, Gravity and Locality: Slide 2 Physics at the Dawn of the 20 th Century: The Clockwork Universe Newton’s Third Law of Motion…
[ G eV ] tX [ sec ] 3He / D FIRAS 3 FIG. 1: The matter field at z = 99 for various PBH fractions. The PDM density field is represented by the colormap with white points indicating
1 COSMOLOGY Lecturer: Professor Komissarov SS Room: 1019 in Maths Satellite email: SSKomissarov@leedsacuk 2016 Contents Contents 2 1 Introduction 5 2 Euclidean plane 6 21…
Wayne Hu STScI, May 2008 The Cosmology of f (R) Models for Cosmic Acceleration Why Study f (R)? • Cosmic acceleration, like the cosmological constant, can either be viewed…
The Holographic Principal and its Interplay with Cosmology T. Nicholas Kypreos Final Presentation: General Relativity 09 December, 2008 T.N. Kypreos What is the temperature…
Slide 1 QUANTUM COMPUTATION AND QUANTUM INFORMATION GROVER'S ALGORITHM Igor Ilijašević1 / 26 Slide 2 Igor Ilijašević2 / 26 Slide 3 Igor Ilijašević3 / 26 COMPLEX…
PHY 102: Quantum Physics Topic 4 Introduction to Quantum Theory Wave functions Significance of wave function Normalisation The time-independent Schrodinger Equation. Solutions…
Fundamentals of Cosmology 3 The Formation of Structure in the Universe • Jeans’ Instability in the Expanding Universe • Non-relativistic case • Peculiar and Rotational…
Galaxies Cosmology HEAC II 5 points ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory Active galaxies Active galactic…
1 of 33 Twin Universes Cosmology Jean-Pierre Petit Marseille Observatory France Astrophysics and Space Science 226 273-307 1995 Abstract Starting from the field equation…
Eligio Lisi INFN Bari Italy 3ν masses mixings and CPV phases: status and prospects Tensions in flavor measurements: A path…
Scalar perturbations in f(R)-cosmology in the late universeJan Novak Jan Novak Department of theoretical physics at Charles University, Prague, Czech republic 11.August 2014
1. External Quantum Efficiency (EQE)Measurement Prasad Gandhi Advisor: Dr. Brendan O’Connor 9/23/2011 2. Solar cell technologies Silicon GaAs CuInGaSe CdTe α -Si + organic…
17. Quantum Gravity and Spacetime Quantum Electrodynamics (1940's) • RQFT of electromagnetic force. • Matter fields: leptons, quarks. • Force field: γ (photon).…