'Secondary particles' presentation slideshows

Air Pollution Control Engineering

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Quarknet 2007

Quarknet 2007. Daniela Bortoletto. Goals. Welcome to Purdue This year program is focused on cosmic ray physics and cosmic ray detection The aim is how to use the Quarknet cosmic ray detector to introduce modern physics in the class room. Program. Program. Photo of a -particles

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Neutrinos in Minnesota

Peter Litchfield University of Minnesota Colloquium 12 th October 2005. 735 km. Neutrinos in Minnesota. A Short History of the Neutrino. 1930 Pauli proposes the neutrino to explain ? decay.

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Results from simulations of the production of secondary particles at the pipe walls

Results from simulations of the production of secondary particles at the pipe walls. M.Baznat 1 , K.K.Gudima 1 , E.I.Litvinenko 2 , Yu.Murin 2 1 Institute of Applied Physics, Academy of Science of Moldova, Moldova 2 JINR Dubna, Russia. Outline. Motivation of this study for CBM

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WASAVIES: Wa rning S ystem for Avi ation E xposure to S olar Energetic Particles

461 views • 31 slides

Nuclear Physics Institute

Detection of relativistic neutrons by BaF2 scintillators Simulation on MCNPX. Nuclear Physics Institute. Doctor V. Wagner Mitja Majerle Antonin Krasa Ondrej Svoboda. Ludovic BATTISTA. SETUP. 25 cm. 5.9 cm. view pz=3. view : py=0. Aluminium Separation. Description of the beam.

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Track etch based LET spectrometry in beams of neutrons with energies from 0.2 to 200 MeV

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Solar Variability and its Effect on Earth and its Inhabitants

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Other GEANT4 capabilities

Other GEANT4 capabilities. }. Alex Howard. Event biasing Parameterisation (fast simulation) Scoring Persistency Parallelisation and integration in a distributed computing environment . }. Susanna Guatelli. Ackowledgements.

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A CLUSTER OF ULTRAHIGH ENERGY COSMIC RAYS

A CLUSTER OF ULTRAHIGH ENERGY COSMIC RAYS. Glennys R. Farrar Center for Cosmology and Particle Physics New York University. Research supported by NSF, NASA and NYU. Results . A pointlike cluster of 5 ultrahigh energy cosmic rays has been found, with energies 10 19-20 eV

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Cosmic Ray Telescope for the Effects of Radiation (CRaTER) Instrument Requirements

Cosmic Ray Telescope for the Effects of Radiation (CRaTER) Instrument Requirements. Justin Kasper CRaTER Instrument Scientist MIT & Boston University. CRaTER Organization Chart. Theory of Operation. Pairs of thin and thick Silicon detectors. A-150 Human tissue equivalent plastic (TEP).

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Beam Composition for Biology

Beam Composition for Biology. The beam delivered to radiobiology samples at NSRL can have many components in addition to the nominal beam particles. These beam components may be important to account for when understanding the biological endpoints obtained in NSRL experiments.

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Primordial BHs

Primordial BHs. Main reviews and articles. astro-ph/0504034 Primordial Black Holes - Recent Developments astro-ph/0304478 Gamma Rays from Primordial Black Holes in Supersymmetric Scenarios gr-qc/0304042 Do black holes radiate?

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GEANT 4 simulation of energy deposited in KASCADE-Grande detectors

GEANT 4 simulation of energy deposited in KASCADE-Grande detectors. , , , ,. Department of Physics, University of Bucharest, Bucharest, Romania National Institute of Physics and Nuclear Engineering, Bucharest, Romania. Carpathian Summer School of Physics 2012. Contents:. Motivation

261 views • 15 slides

Measurement and simulation of radionuclide product yields in iron from 400 AMeV carbon ions

Measurement and simulation of radionuclide product yields in iron from 400 AMeV carbon ions. T.Ogawa, M.Morev, Takeshi Iimoto, Toshiso Kosako The university of Tokyo. SATIF-10, 2-4 June 2010, CERN. In-Target ?-emitting fragments. 400 MeV C ion. Abstract. Experiment

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Plots for (pre-)Approval

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Data Management for the VO auger

Pierre Auger Observatory. Cosmic Ray Showers. Virtual Organization auger. Data consistency checks. Distribution of files. Newly registered files in LFC. Pierre Auger Observatory is studying ultra-high energy cosmic rays, the most

124 views • 1 slides