PPT-Correlation Between IceCube Neutrinos and X-ray Flaring Blazars

Matthew Fu 1 Timothy Govenor 1 Quentin King 1 Parisa Roustazadeh 12 Markus Boettcher 3 1 Bishop Watterson High School Columbus OH USA 2 Columbus State Community College Columbus OH USA. 林貴林. IOP, NCTU. (1). F.-F. Lee and GLL, Phys. Rev. D85, 023529 (2012). (2). F.-F. Lee, GLL, . Sming. Tsai, Phys. Rev. D87, 025003 (2013). (3). . . F. .-F. Lee, GLL, . Sming. Tsai, . Phys. . Rev. D89, . 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. distance indications from Fermi and . TeV. data: an empirical approach. E. . Prandini. , Padova University & INFN. G. . Bonnoli. , L. . Maraschi. , M. . Mariotti. and F. . Tavecchio. SciNeGHE. 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?. Aoife McCloskey. Supervisors: D. Shaun Bloomfield & Peter T. Gallagher. Using Sunspot . Group . Evolution . to . Forecast . Solar Flares. Most . current forecasting techniques use . point-in-time. Lee-Ann Martin, Program Manager, PRV. Amy Lunt, Asset Valuation. Disclaimer. 2. The . statements or opinions expressed in all ONRR presentations and panel discussions at the 2017 PASO-Tulsa Federal/Indian Royalty Compliance Workshop do not necessarily represent the views of ONRR or the Department of the . 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 ). Resent Discoveries and Results. Vladimir Papitashvili, Program Director. Antarctic Astrophysics & Geospace Sciences. NSF/Office of Polar Programs. Interagency Astronomy . and Astrophysics Advisory . Roma International Conference on . Astroparticle. Physics. September 2018. Juande Zornoza (IFIC, UV-CSIC). Disclaimer. ~. 3. 0 plenary talks . on these topics… big challenge to . summarize .  rather personal thoughts. by energy-momentum reconstruction of atomic K-capture events. Peter F Smith (UCLA). interdisciplinary collaboration (particle physics, nuclear physics, atomic physics):. Jeff . Martoff. , Francesco . University of Alabama. IceCube. . Bootcamp. 2016. Madison, WI. 6/12/16. IceCube Flashers - Bootcamp. 1. IceCube. 6/12/16. IceCube Flashers - Bootcamp. 2. Strings are numbered 1-86. DOMs are numbered 1-60, top to bottom (in ice).