PPT-Gamma Ray Constraints on New Physics Interpretations of IceCube Data

Author : kimberly | Published Date : 2022-06-28

Yicong Sui Washington University in St Louis In collaboration with Bhupal Dev Outline Motivation PeV bump in IceCube data Astrophysical explanation Multi messenger

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Gamma Ray Constraints on New Physics Interpretations of IceCube Data: Transcript


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. ASTROPHYSICAL SCENARIOS. Félix Mirabel. *. Neutron stars & Black . holes. in . stellar. . binary. . systems. . that. . radiate. in gamma-rays.. (Will not . refer. to . other. types gamma-ray . 84 . Hiroshi Nagai. (National Astronomical Observatory of Japan). In collaboration with. Monica . Orienti. , Motoki Kino, Kenta Suzuki, Keiichi Asada, Akihiro . Doi. , Gabriele . Giovannini. , Marcello . Andrew Levan. University of Warwick. Parameter space. Kouveliotou. et al. 1993. Parameter space. Kulkarni. & . Kasliwal. 2010. Parameter space. LGRBs. SGRBs. SGRs. ?. TDEs?. Galactic sources (SGR, LMXB, HMXB, . Polarimeter. for Solar flares . (. GRIPS. ). Recently funded NASA LCAS balloon mission. 3D position-sensitive germanium spectrometer. High spectral resolution (~2 keV FWHM at 662 keV). Compton-scatter track reconstruction. Manel. Martinez. 4. 3. rd. . Winter Meeting. March 2015-Benasque. Outline. 1) Introduction. 2) Basics on VHE Gamma Astronomy physics. 3) VHE gamma observatories. 4) CTA. 5. ) Conclusions. 1) INTRODUCTION. Resent Discoveries and Results. Vladimir Papitashvili, Program Director. Antarctic Astrophysics & Geospace Sciences. NSF/Office of Polar Programs. Interagency Astronomy . and Astrophysics Advisory . (. GammaSIG. ). (. PhysPAG. ). 231. st. AAS. Meeting (2018). Sylvain Guiriec . –. . sguiriec@gwu.edu. Gamma-ray Science Interest Group. (. GammaSIG. ). 2018/01/08. Agenda. PhysPAG. /. GammaSIG. “The e-ASTROGAM mission (exploring the extreme Universe with gamma rays in the MeV-GeV range)”. Liz Hays . (. NASA Goddard Space Flight Center). The Origin of Cosmic Rays. Credit S. . Swordy. Victor Hess and his . “Flight . Ops . Team”, . 1912. From protons. Pion decay. Accelerated protons (p) interact with matter. . Matthew Erenpreiss. Ohio Department of Natural Resources. Division of Geological Survey. Utica . Shale Play Book Study Workshop. Canonsburg, PA. July 14, 2015. Outline. Background. Spectral Gamma-Ray Scanner. Vikram . Dwarkadas. . (U Chicago). Matthieu. Renaud, . Alexandre. . Marcowith. . (LUPM, U Montpellier). Vincent . Tatischeff. . (. Univ. Paris-. Sud. ). August 11 2017. TevPA 2017 : VVD. 1. We acknowledge support from the FACCTS program at . from. the . high. . energy. . universe. Denis . WOUTERS. Service de Physique des Particules. Supervisor. : Pierre BRUN. D. Wouters and P. Brun, PRD, 2012, . Irregularity. in . g. -ray. source . 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). Flashes. Gamma Ray . Astronomy. . Beginning. started . as a small budget research program in 1959. monitor. ing. compliance with the 1963 Partial Test Ban Treaty by the Soviet Union, and other nuclear-capable states. T. elescope. Liz Hays. NASA GSFC. Lecture Plan. The Fermi Observatory. Science Motivation. Instruments. Detecting gamma rays with the Large . A. rea Telescope. Instrument Subsystems. Angular resolution.

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