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0.5 % Stars and other visible stuff Ay 127 ��� The Contents of the Universe Supernovae alone ⇒ Accelerating expansion ⇒ Λ > 0 CMB alone ⇒ Flat universe ⇒…
Cacac Dealing with “SUSY limit Inflation” for the Experimental PDG Review Oliver Buchmueller & Paul De Jong ‹#› Experimental SUSY, PDG Workshop 2013 O. Buchmüller…
Open Inflation for string landscape 2009/7/17 MG12@Paris 1 Evolutionary effects in one-bubble open inflation for string landscape Daisuke YAMAUCHI Yukawa Institute for…
PowerPoint Presentation Jonathan Ganc Physics Dept., Univ. of Texas July 6, 2011 PASCOS 2011, Univ. of Cambridge based on arXiv: 1104.0244 Overview of presentation July 6,…
Koichi Funakubo — Baryon Asymmetry of the Universe — 1/30 content¶ ³ §1. Evidence of the BAU §2. Requirements for the baryogenesis §3.
ŒÊŒÊflÊáÊËâòÊË ÃÕÊ ‚¢¬ÊŒ∑§ —ŒË¬∑§ Œ‚Ê߸ fl·¸— 5 •¢∑§ — 1 •π¢«U ∑˝§◊Ê¢∑§ — 49 Ÿflê’⁄U 2009…
Cargese - 6th July 2010 Cargese - 06/07/10 Patri% Pe'r Institut d’Astrophysique de Paris GR!CO Bouncing alternatives to inflation Cargese - 6th July 2010 2 Problems with…
Particle Physics at Colliders and in the early universe WS 201919 TUM PD Dr B Majorovits 1 Introduction to Cosmology I Short Introduction to Cosmology 1 Historical notes:…
The CLIC accelerating structure development program Walter Wuensch CARE05 23 November 2005 The CLIC design gradient of 150 MV/m was first achieved in a CLIC built structure…
a review of ILL research in fundamental and nuclear physics H I G H L I G H T S O F I L L R E S E A R C H Neutrons and the Universe u ud u dd –νe W e PROTON NEUTRON ILL…
Interest rate (r ) Inflation rate (π) Fed Reaction Rule If the Fed sees the inflation rate rising… …it moves to raise interest rates r0 r1 π1 π0 Income Aggregate Demand…
9th ECB Workshop on Forecasting Techniques: Forecast Uncertainty and Macroeconomic Indicators Components of Inflation Inflation Forecasting and the Phillips Relation…
What is our universe made of ? quintessence ! fire , air, water, soil ! Dark Energy dominates the Universe Energy - density in the Universe = Matter + Dark Energy 25 % +…
Alexey Boyarsky Spring semester 2015 Why do you need that? Things I consider known Beginning of the XXth century: attempts to explain atomic and nuclear physics, taking into
ar X iv :1 30 9. 43 68 v2 [ gr -q c] 19 M ar 20 14 Accelerating expansion or inhomogeneity? A comparison of the ΛCDM and Lemaˆıtre – Tolman models Andrzej Krasin´ski…
Al Parker January 18, 2009 Accelerating Gibbs sampling of Gaussians using matrix decompositions Colin Fox, Physics, University of Otago New Zealand Institute of Mathematics,…
Our place in the Universe The Universe is very very big Earth radius 6378 km Sun Earth radius of sun x 109 orbit of earth around sun x 214 orbit of Pluto x 39 Pluto Nearby…
Chapter Thirteen: Aggregate Supply, Aggregate Demand, and Inflation: Putting it All Together Aggregate Demand and Inflation Output (Y ) Inflation rate (π ) Aggregate Demand…
The Extreme UniverseThe Extreme Universe Rene A. Ong Brown University Colloquium University of California, Los Angeles 1 March 2004 (The Limits of Particle Physics and Astronomy)(The…
Working Paper Series Department of Economics University of Verona Inflation and Growth in the Long Run: A New Keynesian Theory and Further Semiparametric Evidence Andrea…