Goal: To understand how stars generate their energy Objectives: To learn about the Proton â Proton Chain To learn about the Carbon â Nitrogen â Oxygen Cycle (Horsehead…

* Astro-Particle Physics 3 Acceleration mechanisms Manfred Jeitler * man-made accelerators: inside of an Alvarez-type accelerating structure * Cyclotron r.............orbit…

Troitsk ADS project Russia Institute for Nuclear Research RAS, Moscow Outline Linac and experimental complex Pulse neutron sources and its infrastructure Development and…

MEG Experiment Motivation & Event Signature MEG Experiment & Detector Paul Scherrer Institut The most powerful machine in the world. Proton energy: 590MeV Nominal…

Luminosity Monitor UKNF Meeting 7 June 2010 Paul Soler, David Forrest Danielle MacLennan * Purpose of Luminosity Monitors Luminosity monitor to determine particle rate close…

Title Author Date Collimator Materials for LHC Luminosity Upgrade: Proposal of Irradiation Studies at BNL Collimation Upgrade Specification Meeting 15/02/2013 N. Mariani…

Energy deposition studies at IR7 M. Santana, M. Magistris, A. Ferrari, V. Vlachoudis Introduction Motivation Large Hadron Collider : 27 km cryogenic installation LHC is a…

Alternatives to CsI(Tl) O. Tengblad/T. Nilsson Phoswich solutions GEANT-4 simulations Read-out electronics Multiplexing Swedish plans (Chalmers/KTH) Olof Tengblad Developments…

Feb/21/2013 HEP Detectors (AP240) * Particle Physics and Detectors Su Dong HEP Detectors (AP240) Feb/21/2013 HEP Detectors (AP240) * Fundamental Building Blocks Muon ~ âheavy…

The 28th ICRC (ICRC2003, Tsukuba, Japan) Oral session on Solar&Heliospheric Phenomena (SH3.4; Long-term variations) Solar modulation effect on the cosmic-ray proton spectra…