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1 Muon Veto System and Expected Backgrounds at Dayabay Hongshan Kevin Zhang, BNL DayaBay Collaboration DNP08, Oakland 2 DayaBay Experiment The goal of the DayaBay neutrino…
Folie 1for GERDA and LArGe DPG Göttingen, 2012 Part 2: light instrumentation design options in GERDA Germanium Detector Array Germanium Detector Array Double beta decay:
A new cylindrical photon-veto detector for the KOTO experiment Osaka University Manabu Togawa for the KOTO collaboration - We installed a new photon-veto detector Inner Barrel…
MC for t H and SM backgroundsStefano Pozzorini Zurich University Large backgrounds in ttH searches Dominant ttH(bb) channel suffers from heavy tt+jets contamination ∼
Probabilistic Termination and Composability of Cryptographic Protocols Crypto ‘16 Ran Cohen TAU Sandro Coretti NYU Juan Garay Yahoo Research Vassilis Zikas RPI Motivation…
External Backgrounds (s) in partial-fill and the Rope AnalysisPouya Khaghani August 13, 2021 Pouya Khaghani (LU) External Backgrounds (γs) in partial-fill and the Rope
Heavy Radiation Backgrounds in the LSBB Tom Girard Ana Fernandes Miguel Felizardo Advanced Detectors Group Centro de Física Nuclear Universidade de Lisboa SIMPLE gas 25…
The NA62 rare kaon decay experiment Photon Veto System Vito Palladino for NA62 Coll. The NA62 experiment aims to measure the Branching Ratio of the ultrarare decay K+→π…
Chapter 2 Prospect Theory and Expected Utility Theory A.Von-Neumann-Morgenstern Expected Utility Theory Von-Neumann-Morgenstern Axioms :Certain, identifiable Outcomes C:…
Properties of Variations of Power-Expected-Posterior Priors Ioannis Ntzoufras [email protected] Joint work with: Dimitris Fouskakis Dep. of Mathematics, NTUA Konstantinos…
Variance and Standard Deviation Christopher Croke University of Pennsylvania Math 115 Christopher Croke Calculus 115 Expected value The expected value E X of a discrete random…
Discrete Random Variables Expectation 1805 Spring 2018 http:wwwmathsisfuncomdataquincunxhtml http:wwwyoutubecomwatchv=9xUBhhM4vbM http:wwwmathsisfuncomdataquincunxhtml http:wwwyoutubecomwatchv=9xUBhhM4vbM…
Bulk Product List Q1.2015.html[31/03/2015 14:47:12] Company Name Product Code Host Principal name Expected species cross-reactivity Clonality Contact details Absea Antibody…
Cleanliness backgrounds and surface contaminations in CuoreStefano Pirro INFN-MilanoStefano Pirro LRT-2004 Sudbury December 13, 2004Surface contaminations bolometersSum energy:…
1.00 1.00 -1.00 -1.00 XB Portfolio weight in stock A 0 XA Portfolio weight in stock B Isoexpected return line 10% 12% 16% 18% 20% B XB MVP -1.00 0 1.00 XA 30% 28% 21% 26%…
Neutrino detectors for Super-Beams, β-Beams and ν Factories Paolo Strolin NUFACT04 Low-Z Tracking Calorimeter Water Čerenkov Liquid Argon TPC Magnetised Iron Calorimeter…
QUANTIZATION OF NON-GEOMETRIC FLUX BACKGROUNDS Richard Szabo Heriot–Watt University Edinburgh Maxwell Institute for Mathematical Sciences Workshop on Nonassociativity in…
Introduction Cosmological perturbations Basics of FRW cosmology Scalar-vector-tensor decomposition Evolution of cosmological perturbations Power spectra, r, Ωgw Summary…
Dark Matter @ Charged lepton flavour violation experiments Niklaus Berger Institut für Kernphysik Johannes-Gutenberg Universität Mainz Dark Matter @ LHC Heidelberg April…
2 QUESTION PAPER CODE 65/1/B EXPECTED ANSWERS/VALUE POINTS SECTION - A 1. x = 2 , y = 9 (½ for correct x or y) x + y = 111 ½ m 2. order 3 , or degree 1 ½ m Degree…