PPT-Can Standard Model Neutrinos

Be Majorana States and Other Puzzlers Inspired by Adrian Melissinos KT McDonald Princeton U March 7 2017 Seminar at University of Rochester httpphysicsprincetonedu mcdonaldexamplesmajorana170307pptx. From . Dark Matter . Annihilation. Jason Kumar. University of. H. a. w. a. i. i. collaborators. Jin In. Carsten. . Rott. Pearl Sandick. Jennifer Gaskins. David Yaylali. 1502. 02091, 15xx.xxxxx. dark matter and monoenergetic neutrinos. 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. 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. :. 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 ). And. High-Energy . Lorentz Violation. Damiano. . Anselmi. Cortona. 27/05/2010. The papers about the Lorentz violating Standard Model are. [1] D.A., . Standard Model Without Elementary Scalars And High Energy Lorentz Violation, . 1. John Beacom, The Ohio State University. 2. Plan of the Talk. Introduction to Supernova . N. eutrinos. Focus on . B. urst . D. etection. . What will we know after the next burst?. What . new capabilities do we need?. R.Svoboda. Sterile Neutrinos as DM?. As WIMP searches getting well below the weak interaction scale for large range of masses and collider limits now limit smaller masses. What if no . WIMPs. are found to well below weak scale?. and Earth Structures. By . Miriam Aczel. What are neutrinos?. They are almost . massless. —hardly feel the force of gravity. They have no electric charge—don’t feel the electromagnetic force. Have no . Neutrinos. Ghost . Particles . of the . Universe. Georg G. Raffelt. Max-Planck-Institut f. ür Physik, München, Germany. Neutron. Proton. Gravitation (Gravitons?) . Weak . Interaction (W and Z Bosons). :. 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 ). Dr Susan Cartwright. Department of Physics and Astronomy. Discovering neutrinos. Routes to scientific discovery:. Accident!. You find something unexpected in your data. For example, gamma-ray bursts (discovered by satellites designed to look for clandestine nuclear tests). 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.. 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.