Search results for Dark Matter and Dark Energy from the solution of the strong CP problem

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Models of coupled dark matter to dark energy Alkistis Pourtsidou Department of Physics Astronomy, Bologna University, Italy Work in collaboration with Ed Copeland and Costas…

Michael Viderman∗ Haifa, 32000, Israel. {viderman}@cs.technion.ac.il November 26, 2012 Abstract An error-correcting code C ⊆ Fn is called (q, ε)-strong

WITH A CRYSTALLINE NORM ALESSIO FIGALLI, YI RU-YA ZHANG Abstract. Let K be a convex polyhedron and F its Wulff energy, and let C (K) denote the set of convex polyhedra close

Non-normalizable densities for strong anomalous diffusion Eli Barkai Bar-Ilan University Rebenshtok Denisov Hänggi Phys Rev Lett 2014 TAU 2015 Eli Barkai Bar-Ilan Univ Eli…

CP violation measurements in beauty and charm hadrons at LHCb Angelo Di Canto on behalf of LHCb observables CP-conserving observables CP-violating T eV Λ Lo w er b ou nd…

Looking for SUSY Dark Matter with ATLAS The Story of a Lonely Lepton Nadia Davidson Supervisor: Elisabetta Barberio The Standard Model In high agreement with experimental…

Have neutrinos to do with Dark Energy ? Why neutrinos may play a role Mass scales : Dark Energy density : ρ ~ ( 2×10 -3 eV )- 4. Neutrino mass : eV or below. Cosmological…

The Accelerating Universe,Inflation, & the Dark Energy Ta-Pei Cheng Univ of Missouri - St. Louis Material based on the book “Relativity, Gravitation & Cosmology:…

LUX: A Liquid Xenon Dark Matter Detector Masahiro Morii Harvard University August 24, 2010 * LUX Dark Matter Detector New Physics — Where? * From the labs — Unexplained…

No Slide Title The Backreaction Conjecture to explain Dark Energy Thomas Buchert, CRALyon MPIK May 26, 2014 ‹Nr.› The Standard Model G =  T ? a(t) δij…

Have neutrinos to do with Dark Energy ? Why neutrinos may play a role Mass scales : Dark Energy density : ρ ~ ( 2×10 -3 eV )- 4. Neutrino mass : eV or below. Cosmological…

Ethan Siegel1,2, Mark Hertzberg3, JNF2 1University of Wisconsin, 2University of Florida, 3MIT Cosmic Cartography 4 December 2007 M = 5× 1014 M • Weak Field General

THE DARK SIDE OF THE COSMOLOGICAL CONSTANTCAMILO POSADA AGUIRRE 10/04/11 Outline 2 Einstein’s Greatest Blunder 3 The FLRW Universe 4 A Dynamical Universe 5 Resurrection

Slide 1 Fermilab Dark Energy Program Josh Frieman Introduction and Motivation Dark Energy Survey Sloan Digital Sky Survey Results Future Projects Slide 2 Josh Frieman - Fermilab…

Heraeus School Flavour Physics and CP Violation 29./30. August 2005 Historical Intro: Discovery of the tau Basic Properties Branching Ratios Kinematics Mass Lifetime Hot…

Slide 1 Part III CP Violation and K Physics Chris Parkes Chris Parkes ‹#› Outline PHENOMENOLOGY AND EXPERIMENTS CP violation and Kaon physics T-violation: CPLEAR An angle…

τ→ Kπν decays and CP violation Kang Young Lee: KAIST D. Kimura, K. Nakagawa, T. Morozumi: Hiroshima Univ. Oct. 25 (Thu.) 1. Motivation There are a lot of data of τ+τ-…

CP measurements in Bs decays to charm Azizur Rahaman (for the CDF collaboration) University of Pittsburgh 4th International Workshop on the Unitarity Triangle Nagoya University,…

Microsoft PowerPoint - caltech.ppt [Read-Only]Recent Results on CP Violation from Belle Particle Physics Seminar Caltech Daniel Marlow Princeton University Talk Outline –

XEUS and Strong Gravity from Black Holes AC Fabian IoA Cambridge UK With help from Giovanni Miniutti, Jon Miller, Chris Reynolds, Rubens Reis and Randy Ross Accretion makes…