PPT-Correlation Between IceCube Neutrinos and X-ray Flaring Blazars
Author : jainy | Published Date : 2024-06-08
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
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Correlation Between IceCube Neutrinos and X-ray Flaring Blazars: Transcript
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, . 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. :. 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 ). Askaryan. Radio Array . A . new instrument for the detection of highest energy neutrinos.. Hagar Landsman, UW Madison. High energy neutrinos….Why ?. n + . p. +. . P+. g. . . p + . :. 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 ). Rick Behal and . Travis Baer - August . 2017. Class Synopsis . Statewide Rule 10 (SWR 10). Rule. Exception. Application. Online Completions. Frac. Port Completions. . Applicable Statewide Rule. Applicable Statewide Rules:. 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. gov 50 W Town St Ste 700 PO Nox 1049 Oolumbus OH 43216-1049 614 644-3020 614 644-2737 faxUnderstanding the Basics of Gas Flaringas flaring is an integral part of the exploration production and pro Yicong Sui. Washington University in St. Louis. In collaboration with Bhupal Dev. Outline. Motivation:. PeV. bump in . IceCube. data. Astrophysical explanation:. Multi messenger method (Gamma Ray Constraint). 1. John Beacom, The Ohio State University. High Energy . Neutrino . Astronomy. Topic: Impossible. Requires. : sources that reach high energies. . sources that are luminous. . sources of different types. Swift. -BAT blazars with . NICER. Sergio Mundo, Richard . Mushotzky. University of Maryland, College Park. MARLAM 9, JHU, Baltimore, MD. Blazar characteristics. Radio-loud AGN with jet aligned close to line of sight. ?. 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. 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.
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