'Muons' diaporamas de présentation

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Magnetic field and flavor effects on the neutrino fluxes from cosmic accelerators

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Search for Pair Production of Scalar Leptoquarks with the CMS Experimen t

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General Physics (PHY 2140)

General Physics (PHY 2140). Lecture 25. Modern Physics Relativity Time dilation, length contraction. http://www.physics.wayne.edu/~apetrov/PHY2140/. Chapter 26. If you want to know your progress so far, please send me an email request at apetrov@physics.wayne.edu. Lightning Review.

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Commissioning with cosmic rays of the Muon Spectrometer of the ATLAS Experiment at LHC

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Current and future upgrades in STAR

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Progress report on Calorimeter design comparison simulations

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A Business Inspired by Muon Colliders (Can it contribute to electron-ion colliders?)

m. Muons, Inc. A Business Inspired by Muon Colliders (Can it contribute to electron-ion colliders?) Rolland P. Johnson Muons , Inc. ( http://www.muonsinc.com/ )

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Mentorship

Mentorship . James C ostlow , Ryan Wilken , and Arnav Joshi Capstone B7. Project overview. with this mentorship we will be collecting data from the Cosmic Ray Muon Detector(CRMD) The data we will be collecting is the number of M uons that come through the atmosphere

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Main priorities for the next years

Main priorities for the next years. Where do we stand. Muon system in good shape (in my opinion) Sub-systems hardware quite robust (see later for main problems) All sub-systems have >97% active channels High data taking efficiency and rather smooth operations

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Cherenkov Detectors

Cherenkov Detectors. When light passes through matter its velocity decreases. Index of refraction n . The index depends on the medium. Wavelength dependence A 0 , l 0 medium dependent The index can be viewed as a result of scattering. Scattering amplitude A(0). Index of Refraction.

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The Status of MICE

1/13. The Status of MICE. V. Blackmore, University of Oxford, on the behalf of the MICE Collaboration. 2/13. About MICE. Ionisation cooling The Muon Ionisation Cooling Experiment (MICE) Key systems. 3/13. Ionisation Cooling.

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W .Iwanski

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Level-1 Topology Processor for Phase 0/1 - Hardware Studies and Plans -

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Time structure and useful muon rates for MICE at RAL Alain Blondel, Rob Edgecock

Time structure and useful muon rates for MICE at RAL Alain Blondel, Rob Edgecock. UPDATED version with ISIS cycle length = 2 ms 2. ORIGINAL VERSION with ISIS cycle assumed to be 100 microseconds long. Time structure and useful muon rates for MICE at RAL Alain Blondel, Rob Edgecock.

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Saturation effects in MCPs

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W/Z to Muons (Preshutdown)

W/Z to Muons (Preshutdown). Muon Trigger Rates Single Muons: For L=5e30 the L1 Rate: mu1cmsc_fz ~ 70 hz. Forward was about the same. Trigger was prescaled by >20 X. Dimuon Trigger was unprescaled Acceptance & Efficiency Muon ID requires A-layer.

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Muon Traffic Relative to the Suns Position Around Earth

Muon Traffic Relative to the Suns Position Around Earth Aaron McNamara, Vic England, Dustin Clark and Adam Wiessner University of Wisconsin River Falls Physics Department. MATERIALS AND METHODS. RESULTS. BACKGROUND. Materials Outside Scintillators GPS Circuit Board QNet2

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Muons, Inc. 2008 Phase I Proposals

Muons, Inc. 2008 Phase I Proposals.

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