PPT-Supernova Neutrinos

Physics Opportunities with Supernova Neutrinos Georg Raffelt MaxPlanckInstitut für Physik München Sanduleak 69 202 Sanduleak 69 202 Large Magellanic Cloud Distance 50 kpc 160000 light years. 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. 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 ). Original source: Arnett. , W.D.; et al. (1989). "Supernova 1987A". . Annual Review of Astronomy and Astrophysics. . 27. : 629–700. .. From Wikipedia article, downloaded 9/8/14, . http. ://. en.wikipedia.org/wiki/SN_1987A. Cecilia Lunardini. Arizona State University . And RIKEN BNL Research Center. INT workshop “Long-Baseline Neutrino Physics and Astrophysics”. Motivations . Current status. The future:. Detection potential. 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. 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?. N. eutron . Stars Foreseen. . Supernova . End Products?. When a . supernova. goes off, we can speculate that:. The star might blow itself to smithereens, . scattering all its material into space and leaving . NOVA Counselor and . SUPERNOVA Mentor Training. Introduction. This course is intended to provide potential Nova Counselors and Supernova Mentors with the basic information they need to assist Scouts in completing the requirements to earn the Nova and Supernova awards.. 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). Highlights of the past 25 years. Outstanding mysteries and surprises. What we can expect to learn, sooner and later. TOPICS. Supernova Energy Sources. Core collapse: . :. 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 ). Instrument Chemistries for each step in the decontamination process. Pre-cleaning. Manual cleaning. Automated cleaning. © 2010 Case Medical, Inc.. Case Solutions. CSR Ink and adhesive remover. SchmutzOff stainless steel, acid based re-conditioner and . ?. 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.