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Background rejection Physics ─ J/Ψ Z Vertex Trigger DAQ Compliance GTT Architecture HERA HERA after upgrade: Ep = 920 GeV Ee = 27 GeV LDesigned=1.5*10 31 cm-2s-1 Three…

Volume-Phase Transitions in Surface-Tethered Networks and Implications for Swelling Instabilities Ryan Toomey Department of Chemical & Biomedical Engineering University…

1. “ Ever New Locomotive Paradigm ” EV Master Plan to go…, Part 1. Project Background Fiber Road Inc. R&D Management Team ㊙ 2. Business Concept Σ Product Concept…

Technical Background 11 Directly Applied Noise Force FN Isolated Payload (M) Payload Motion Xp Spring (k) Damper (b) Earth Ground Motion Xe ω2 ω 02 2 + ω Qω0 Input +…

Background estimation for 4leptons * May 14, 2014 Jongseok Lee (Sungkyunkwan University) M(l+l+) and M(l-l-) * nlep+>=2, nlep->=2, µµµµ M(l+l+) M(l-l-) M(l+l+)…

Commun Math Phys 133 563-6151990 Communications ΪΠ Mathematical Physics ©Springer-Verlagl990 Torsion Constraints in Supergeometry John Lott* IHES F-91440 Bures-sur-Yvette…

Visit to CERCA Background on TCTPs R. Bruce 1 BPM buttons Courtesy O. Aberle, A. Bertarelli, F. Carra, A. Dallocchio, L. Gentini et al. Background TCTP: tertiary collimators…

Outline: Motivation GERDA Phase-I data and analysis: modeling of the background components decomposition of the background spectrum Conclusion Max-Planck-Institut für

Mathematical Background: Foundations of Infinitesimal Calculus second edition by K. D. Stroyan x y y=f(x) dx dy δx ε dx dy Figure 0.1: A Microscopic View of the Tangent…

1. 20 Απριλίου 2010Η Ανάπτυξη της Κορώνης Project PlanΠρόταση για το Μανιατάκειον Ίδρυμα Πρόγραμμα “Μελλοντικοί…

Hunting for Cosmological Neutrino Background (CvB) Gianpiero Mangano INFN, Sezione di Napoli, Italy NO-VE 2008 G. Mangano NO-VE 2008 CvB standard features Neutrinos decoupled…

Neslihan Becerici-Schmidt, Allen Caldwell and Bela Majorovits for the GERDA Collaboration Max-Planck-Institut fur Physik, Munchen Outline: • Motivation. Motivation GERDA

rio1.pptUros Seljak, UC Berkeley Rio de Janeiro, August 2014 Outline • Primordial nongaussianity • Introduction and basic physics • CMB temperature power spectrum

Extragalactic Background Fluctuation from the Numerical Galaxies Hideki Yahagi DTAP, NAOJ Masahiro Nagashima Univ. of Durham Yuzuru Yoshii IoA, Univ. of Tokyo Cosmic Background…

Chapter 4 Nuclear Radiation Background image source: Natural Radioactivity Unstable isotopes Elements with atomic numbers over 84 Repulsion within the nucleus Often written…

Including Elasticity and Attenuation Albert Tarantola Institut de Physique du Globe, 4 place Jussieu, 75005 Paris, France. Pure and Applied Geophysics, Vol. 128, Nos. 1/2,

Slide 1 Ca Isotopes Cheryl Zurbrick 1/29/2010 Slide 2 Background Slide 3 DePaolo Reviews in Mineral Geology (2004) 40 Ca produced by β-decay of 40 K Most Ca from primordial…

Presentation Background 1TrevorFest, October 2013 Trevorfest, October 2013 TrevorFest, April 2013 Results from HESS 3/23 The H.E.S.S. Observatory H.E.S.S. I • 4 telescope

Background modelling for γ-ray spectroscopy with INTEGRAL/SPI Thomas Siegert1, 2?, Roland Diehl1, 2, Christoph Weinberger1, Moritz M. M. Pleintinger1, Jochen Greiner1,