'Cosmic ray muons' presentation slideshows

Studies of nucleon structure in hadronic collisions

Outline. The importance of looking forward Measurements of forward jets Measurements of forward dijets Outlook. Studies of nucleon structure in hadronic collisions. L.C. Bland Brookhaven National Lab 14 June 2013. x 1. x 2. The Importance of Looking Forward - I.

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Low Energy n Astronomy in Super-Kamiokande

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Relativity 1

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Relativity 1

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Cosmic Rays

Cosmic Rays. What is a cosmic Ray?. A cosmic ray is a high-speed particle Could be an electron Could be an atomic nucleus like hydrogen or helium stripped of its electrons These particles travel throughout the Milky Way galaxy Some come from the sun Some from outside the solar system

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Muon Tomography Algorithms for Nuclear Threat Detection

Muon Tomography Algorithms for Nuclear Threat Detection. R. Hoch, D. Mitra, M. Hohlmann, K. Gnanvo. Tomography. Imaging by sections Image different sides of a volume Use reconstruction algorithms to combine 2D images into 3D Used in many applications Medical Biological Oceanography

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INDIA-BASED NEUTRINO OBSERVATORY (INO) Plans & Status

INDIA-BASED NEUTRINO OBSERVATORY (INO) Plans & Status. Naba K Mondal Tata Institute of Fundamental Research Mumbai, India. India-based Neutrino Observatory Proposal. A large mass detector with charge identification capability. Physics goal:. Reconfirm atmospheric neutrino oscillation

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Analyzing Power for Forward Jet Production in Polarized Proton Collisions at ? s = 500 GeV

Analyzing Power for Forward Jet Production in Polarized Proton Collisions at ? s = 500 GeV. Chris Perkins UC Berkeley/Space Sciences Laboratory Stony Brook University. For The A N DY Collaboration. DNP 2012. 10 / 26 /2012. Motivation to Measure Jet A N. ?s=200 GeV. from p ? + p ? p+ X.

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Hawaii Anti-Neutrino Observatory

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DHC 101

DHC 101. Introduction to scintillation detectors. How many PE/MIP should we expect?. Scintillation & Fluorescence. m (MIP). PMT. PEs. W S F. Energy loss by heavy particles.

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Cosmic ray physics in ALICE

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The MINOS Detectors

The MINOS Detectors. Outline The MINOS Experiment Detector Technology Far, Near and Calibration Detector Detector Performance Summary. Chris Smith California Institute of Technology EPS Conference 2003. Far. Near. The MINOS Experiment.

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Muon Lifetime

Muon Lifetime. Sara Lim & Elizabeth Ann Pollock University of Rochester PHY 243: Advanced Lab Professor Regina Demina, Sergey Korjenevski, Dave Starling. Cosmic Ray Muons. Mass : 105.6 MeV/c 2 = 206.7*m e Lifetime : 2.2 ?s (Muon rest frame) Flux of cosmic ray muons :

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Activity for the Gerda-specific part

Activity for the Gerda-specific part. Gerda geometry. top m -veto. water tank. neck. lead shielding. cryo vessel. Description of the Gerda setup including shielding (water tank, Cu tank, liquid Nitrogen), crystals array and kapton cables. Ge array. Small flux, small Ge volume:.

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SVD software meeting summary Jan. 14 th , 2004

SVD software meeting summary Jan. 14 th , 2004. Data quality (Ishino) Alignment and IP resolution (Kibayashi) Gsim-svd status (T.Hara) Trak status (Karim) via e-mail Tag Vertex (T.Higuchi) Trigger simulator (K.Hara) MC generation (Shibata). Data quality (Ishino). Run 48. Run 90.

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The MoNA Detector of NSCL She Has Secrets To Tell!

The MoNA Detector of NSCL She Has Secrets To Tell!. Presented By The Team. Gary Kunzi Jenison Public High School. J.T. Miller Thornapple Kellogg High School. Rich Lund St. Johns High School. Who is MoNA ?.

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DAQ hardware: NIM crate: HV power for the GEMs, LV & control signals for the FE cards

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Sector 10

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The Life and Times of Cosmic-ray Muons

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A Muon Veto for the Ultra Cold Neutron Asymmetry Experiment

Cosmic Ray Muon. Beta detector. Introduction. Figure 4:Experimental Area B - The UCNA Experiment. Cosmic Ray Muons. Goals. Muon Veto Paddle. Beta spectrometer. d. d. n. u. u. p. d. u. e -. W -. v. Ultra Cold Neutrons. electron. antineutrino. Active Veto Concept.

141 views • 1 slides