PPT-PHY582 ― Particle Physics II (Experiment)
Author : vamput | Published Date : 2020-08-28
Lecture 8 Dark Matter detectors Ar á n Garc í aBellido Introduction Dark matter WIMP detection Standard Halo model Signatures Backgrounds Classes of DM detectors
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PHY582 ― Particle Physics II (Experiment): Transcript
Lecture 8 Dark Matter detectors Ar á n Garc í aBellido Introduction Dark matter WIMP detection Standard Halo model Signatures Backgrounds Classes of DM detectors Crystal Scintillator Detectors DAMALIBRA ANAIS COSINE. Physics and Astrophysics Laboratory. Tutors:. Dr.A.Mahendrasingam (Singam) . a.mahendrasingam@keele.ac.uk. Dr.D.McLaughlin . d.e.mclaughlin@keele.ac.uk. Physics/Astrophysics Laboratory. . Lecture Course. ASPERA. 1. Roger Blandford. KIPAC. Stanford. One Hundred Years . of Cosmic Ray Physics . 21 xi 2011. ASPERA. 2. Roger Blandford. KIPAC. Stanford. …mi . ritrovai. per . una. . selva. . oscura. … . Tim Wiser. Splash P2506. 3 Nov 2012. Plan . Standard Model of Particle Physics. Particles, interactions, and the Higgs field. Drawing Feynman diagrams. These simple pictures are actually . calculational. . Gia. . Dvali. . . . CERN Theory Division . & Max Planck Institute for Physics . Spring 2011. (Chapter 1: getting started). . the elementary particles. the forces. the model . how can we understand it?. Elementary particle: . an entity not able to be further decomposed. . with a unique set of properties. Wrap Up. The Volume of the Red Ball. An engineer, mathematician, and physicist are each asked to determine the volume of a red metal ball.. The mathematician measures the diameter, divides it by two to obtain the radius, and then performs a double . . . Cumrun. . Vafa. . May 9, 2012. Phenomenology 2012 Symposium. University of Pittsburgh . Big Liquid Argon Neutrino Detector. Subgroup. Particle Physics Design Group Studies: The BLAND Subgroup. BLAND. The BLAND Group. Patrick Owen . Resolution and Efficiency. Laurie Hudson. General design and Charge readout . and Scholar. s. Symposium to . h. onour. our great friend and colleague on his retirement . from Princeton. AJS Smith. June 17, 2016. Early days: Kirk in Tucson, class of ‘66 . Grad School at Caltech 1966-71. Our vision is to solve the mysteries of matter, energy, space and time for the benefit of all. . We . strive to:. - lead the world in neutrino science with particle accelerators. - lead the nation in the development of particle colliders and their use for scientific discovery. Community Meeting. Input to European Strategy . Discussion Session. Process. Today wide discussion. . Hope at least to narrow down options to put forward. . Produce start of draft writeup. . Further meeting scheduled for . General & HEP. RECFA visit to DK. May 2013. Ulrik. I. . Uggerhøj. , Department of Physics and Astronomy, Aarhus University. Peter Hansen, Discovery center, Niels Bohr Institute University of Copenhagen. Norwegian Physics Teachers @ CERN. Slides from . Steinar. . Stapnes. . (CERN/. UiO. ) . + some from Mar . Capeans. (CERN). Presented . by Ole . Røhne. (. UiO. ). Goals and contents. Goals:. Motivation: detectors are . Kashif Mohammad. Senior Systems Manager. Strategy. When you arrive. Interactive Machines. Home and Data Area. Environment Modules. Batch System. Grid Computing. When you arrive. University Single Sign On(SSO).
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