PPT-Can Standard Model Neutrinos

Author : debby-jeon | Published Date : 2017-08-08

Be Majorana States and Other Puzzlers Inspired by Adrian Melissinos KT McDonald Princeton U March 7 2017 Seminar at University of Rochester httpphysicsprincetonedu

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Can Standard Model Neutrinos: Transcript

Be Majorana States and Other Puzzlers Inspired by Adrian Melissinos KT McDonald Princeton U March 7 2017 Seminar at University of Rochester httpphysicsprincetonedu mcdonaldexamplesmajorana170307pptx. Post-Merger Disks. Sherwood Richers. Dan Kasen, Evan O’Connor, . Rodrigo Fernandez, Christian . Ott. Daniel . Perley. Daniel . Perley. NINJA-2 Catalog. Daniel . Perley. NINJA-2 Catalog. Roland Haas. Susan Cartwright. University of Sheffield. Neutrinos and the Universe. Discovering neutrinos. Detecting neutrinos. Neutrinos and the Sun. Neutrinos and Supernovae. Neutrinos and Dark Matter. Neutrinos and the Universe. Angela Zhang. 7/11/14. Theory of Relativity. Faster than light?. Lab Spots of CERN. Antonio . Ereditato. The words “errors”, “mistakes” and “flop” were bandied about regarding what in actual fact is standard scientific procedure in experimental work.. Susan Cartwright. University of Sheffield. Introduction: . Massive neutrinos in the Standard Model. Dirac and . Majorana. masses. The mixing matrix and neutrino oscillations . Massive neutrinos in the . Neutrino . L. imits. Georg G. Raffelt, Max-Planck-Institut f. ür Physik, München. Sun. Globular Cluster. Supernova 1987A. Cosmology. Questions about Neutrinos. Standard properties of active neutrinos. AY 17. 10/19/2011. Outline. What is Multi-messenger astronomy?. Photons. Cosmic Rays. Neutrinos. Gravity-Waves. Sample-Return. Outline. What is Multi-messenger astronomy?. Photons. Cosmic Rays. Neutrinos. C.W. James, . ECAP, University of Erlangen,. on behalf of the ANTARES collaboration.. Cosmic . rays and neutrinos. What produces this spectrum?. Standard model: acceleration at relativistic astrophysical shocks. R.Svoboda. November 23, SLAC. 1. DUNE. 2. 3. Steel Cryostat. 12 m. 14.4 m. 3.6m. DUNE Far Detector Conceptual Design. Detector Parameters (One 10-kton Module) . 58 m x 12 m x 14.4 m (~50 times larger than ICARUS. Physics Opportunities with. Supernova Neutrinos. Georg Raffelt, Max-Planck-Institut für Physik, München. Sanduleak -69 202. Sanduleak . -. 69 202. Large Magellanic Cloud . Distance 50 kpc . (160.000 light years). Exclude Light Majorana Neutrinos?. http://. physics.princeton.edu. /~. mcdonald/examples/majorana.pdf. KT . McDonald. Princeton U.. . (October 21, 2016). Sun . Yat. -Sen University. Guangzhou. Beta Decay. Director. . of. ECT* . Trento. . since. . January. . first. 2016. Studies at Univ. Bonn . 1974-79 Dipl. + . Ph. . D. in Jülich/Bonn. 1979-83 . Stony. Brook. 1984-96 Univ. Illinois 1990 . Full. :. past present future. Heidi Schellman @ Frank Merritt Fest 2015. 1. What we knew in 1971. 2. Neutrinos exist (Cowan, . Reines. 1956). There are two kinds (Lederman, Schwartz, Steinberger - 1962 ). Cao Hoang Nam. Phenikaa. . University. Based on . arXiv. : 2007.xxx. ICISE - . Quy. Nhon, July 2020. Plan of the talk. GR+SM . and . m. otivations for beyond. Flipped . U(1) extended Standard Model and Majorana dark matter. ?. History in the Making?. 1862: Maxwell found that there should be electromagnetic waves travelling at approximately the (known) speed of light. 1905: Einstein used universal speed of light as foundation of geometric description of physics.

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