'Good energy resolution' diaporamas de présentation

Tackling the search for Lepton Flavor Violation with GHz waveform digitizing using the DRS chip

Tackling the search for Lepton Flavor Violation with GHz waveform digitizing using the DRS chip. Stefan Ritt Paul Scherrer Institute, Switzerland. Agenda. MEG Experiment searching for m ?e g down to 10 -13. DRS1. DRS2. DRS3. Motivation. Why should we search for m ? e g ?.

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Jim Matthews Louisiana State University

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The next 10 years in Particle Astrophysics

The next 10 years in Particle Astrophysics. Workshop summary Some personal observations Tribute to Alan. Solar flare shock acceleration . Coronal mass ejection 09 Mar 2000. SOHO/ LASCO CME of 06-Nov 1997. Lessons from the heliosphere. ACE energetic particle fluences:

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JSPS Core2CORE/SPHERE Meeting

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NEXT International Collaboration

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Neutrino interaction systematics for future experiments : The path forward NuInt14, 19/5/2014

Neutrino interaction systematics for future experiments : The path forward NuInt14, 19/5/2014 D.Autiero, IPNL Lyon. We are entering in a new era for long-baseline experiments which will be addressing the determination of the MH and CP violation

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???????? ??????????? ( ???? ) with the GLC calorimeter group (KEK, Kobe, Konan, Niigata, Shinshu, Tsukuba) 9-Mar-2004, ????????? 2 ???? in Tsukuba (Special thanks to Dr. Matsunaga). ??????????????? ??????????????. Introduction Hardware study with test beams Photon sensors

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Many-body Nuclear Structure, Few-Nucleon Systems and Hadron Structure: next 5 years

Many-body Nuclear Structure, Few-Nucleon Systems and Hadron Structure: next 5 years. TUNL Faculty: M.W. Ahmed, H. Karwowski and H.R. Weller; and C.R. Howell, W. Tornow and A. Young. Research Objectives (5-year program): 1. Many-body nuclear structure

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BESIII detector --- design considerations and its realization

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Collaboration

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I norganic Scintillators for Rare Event Searches

I norganic Scintillators for Rare Event Searches. Rare Event Searches with Scintillators. Standard Scintillation Detectors vs. Bolometers. Standard scintillation detector Crystal at RT, scintillation light detected by PMT Particle identification by pulseshape possible.

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A pixilated CZT drift detector

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Neutron detector for SPIRAL2

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classical novae, type I x-ray bursts, and ATLAS

classical novae, type I x-ray bursts, and ATLAS . Alan Chen Department of Physics and Astronomy McMaster University. model : binary star system accretion on neutron star thermonuclear runaway observations : light curves r esearch areas : Breakout from the Hot-CNO cycles

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Section on Supernova remnants and cosmic rays of the White Paper on the Status and Future of Ground-based Gamma-ray Astr

Section on Supernova remnants and cosmic rays of the White Paper on the Status and Future of Ground-based Gamma-ray Astronomy . 2008arXiv0810.0673 Pohl, et al. CGRO (Compton Gamma Ray Observatory): April 5, 1991 . VHE:100GeV--10TeV UHE:>10TeV Detection rate:10E-11/cm2/s (1/yr/m2).

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The MAGIC telescope and the GLAST satellite

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Physics of 9400 km Baseline Experiments

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Production of the Hard X-ray Mirror of the ASTRO-H satellite

Production of the Hard X-ray Mirror of the ASTRO-H satellite. Hironori Matsumoto (Nagoya University) & HXT team. 1. The ASTRO-H satellite. 3 . Mirror Production.

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Probe for New Physics

ACTIVITIES @ VALENCIA. q. e +. The 3rd generation as Experimental and technological approach. Probe for New Physics. q. e -. q 2. b. c. l. n l. V cb. Very High Resolution small animal PET

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