PPT-Studying Cosmic acceleration and neutrino masses with DES.

httpwwwdarkenergysurveyorg Outline DES what is it and update probes used Dark energy from DES Neutrino masses from DES Filipe Batoni Abdalla Future Dark Energy Surveys. Naba. K . Mondal. Tata Institute of Fundamental Research. Mumbai 400005, India. Brief History. Atmospheric neutrino experiments study neutrinos produced by cosmic ray interactions in the atmosphere.. Now. Josh Frieman. Fermilab. and . the University . of Chicago. Progress on Old and New Themes in Cosmology. Avignon, . April 18, 2014. Last Supper. (in earlier version of program). Cosmologists discuss BICEP2 results at PONT banquet. J. Brunner. 17/04/2013. APC. Outline. Oscillation Probabilities. Neutrino Cross Sections. The Proton Accelerator . The Neutrino Beam. Detector Performance. Event Rates / Result. Oscillation Probabilities. 25/09/2014. Day 1 review. Neutrino Cryogenics Requirements Meeting. 25/09/2014. Good / open presentations. Neutrino Cryogenics Requirements Meeting. 25/09/2014. Points to be discussed further:. Maximum temperature gradients allowed in the sensitive volume. COSMOLOGY. EVIDENCE FOR NEW PHYSICS?. STEEN . HANNESTAD, Aarhus . University. NuHorizons. 2011. n. e. n. m. n. t. Fermion Mass Spectrum. 10. 100. 1. 10. 100. 1. 10. 100. 1. 10. 100. 1. Alan Bross. N u F a c t 0 9. From . SuperBeams. to Neutrino Factories. Pre-Ramble. Neutrino Factory means different things to different people. Not so much for . SuperBeams. I will be talking about a muon-based Neutrino Factory as opposed to a . . . Neutrinos Are Very Elusive!. We now understand that neutrinos are produced in nuclear reactions, but they were actually . predicted several decades before they were finally discovered. . O. n what basis was that prediction made?. Art McDonald, Professor Emeritus. Queen’s University, Kingston, . Ontario, Canada. T. he middle of the sun is so hot that the centers of the atoms (nuclei). f. use together, giving off lots of energy and neutrinos. The neutrinos penetrate easily through the dense material in the Sun and reach the earth.. in collapsing phase. ～. towards comprehensive neutrino studies . Waseda. . univ.. . Yamada lab.. D1 Chinami Kato. Collaboration with . S. Yamada(. Waseda. ), H. . Nagakura. . (Caltech), W. . Iwakami. masses en g et kg. Niveau 1. CE2. plan de travail . n°4. Objectif . : . effectuer des conversions. Niveau 2. Complète en utilisant le tableau. Quelle . masse . est possible ? Entoure-la. Un . stylo. –. . COBAND. . Experiment –. Continuous. . Spectra. l. . Measurement. . in Far-Infrared Region using STJ. Shin-Hong Kim. 　. （. University of Tsukuba, . TCHoU. ）. for COBAND collaboration. Neutrino Oscillations in Susan Cartwright Neutrino Oscillations Principles Experimental techniques Neutrino oscillations: Principles The Standard Model contains three neutrinos These can be labelled by flavour as Acceleration is a measure of . the change in velocity per unit of time. When the velocity of an object is changing, it is . accelerating. Negative acceleration: . slowing down. Positive acceleration: . Maurizio . Spurio, . maurizio.spurio@unibo.it. . Università. di Bologna e INFN. 1. M. Spurio - Galactic template neutrino searches. Propagation induces accidents. M. Spurio - Galactic template neutrino searches.