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Helmuth Spieler (LBNL)23/02/2007, 14:00Invited TalkThe past two decades have provided a wealth of experience in highly integrated front-end electronics for high energy physics. The SLHC and ILC, however, pose formidable challenges, not so much to technology, but to optimum utiliza- tion of existing technology. The increased radiation load at the SLHC drives detectors to higher segmentation, which exacerbates the problems of reducing...Go to contribution page
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Ichiro Adachi (KEK)23/02/2007, 14:55Contributed TalkProximity focusing RICH based on silica aerogel Cherenkov radiator has been developed for new particle identification device in the Belle detector upgrade. To further improve detector performance, new concept for Cherenkov ring imaging has been introduced, where multiple aerogel layers with different indices are accumulated to increase detected photoelectrons without making a signle...Go to contribution page
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Jerry Va'vra (SLAC)23/02/2007, 15:55Contributed TalkBenefiting form from the recent introduction of new fast vacuum-based pho- ton detectors with a transit time distribution of σ_TTS ∼ 30-150ps, we are developing novel RICH detector capable of correcting the chromatic error by timing, attempted the first time ever on such a scale; we are also developing a novel TOF detector concept. We have built and successfully tested a novel...Go to contribution page
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Sergey A. Kononov (Budker Inst. Novosibirsk)23/02/2007, 16:20Contributed TalkThe work on aerogel Cherenkov counters was started in Novosibirsk in 1986. Our group produces silica aerogels with refractive indices of 1.006–1.13. Largest block dimensions achieved for n=1.03 are 200 × 200 × 50 mm^3. Optical transparency of Novosibirsk aerogel is one of the best in the world. The particle identification system for the KEDR detector based on the ASHIPH coun- ters...Go to contribution page
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Ryu Sawada (Uni Tokyo)23/02/2007, 16:45Contributed TalkMEG experiment is a rare muon decay search experiment. A muon rare decay μ + → e + γ violates lepton flavor conservation. The standard model predicts too small branching ratio to observe, however many new theories predict observable branching ratio. MEG experiment has sensitivity to the background ratio better than 10 −13 which is two orders of magnitude better than current...Go to contribution page
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Fabio Sauli (CERN)23/02/2007, 17:10Invited Talk
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