The AGASA and SUGAR Anisotropies and TeV Gamma Rays from the Galactic Center: A Possible Signature of Extremely High Energy Neutrons

doi:10.1086/427972

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Roland M. Crocker et al. 2005 ApJ 622 892 doi:10.1086/427972

The AGASA and SUGAR Anisotropies and TeV Gamma Rays from the Galactic Center: A Possible Signature of Extremely High Energy Neutrons

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Roland M. Crocker^1,2, Marco Fatuzzo³, J. R. Jokipii⁴, Fulvio Melia⁵ and Raymond R. Volkas²

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rcrocker@cfa.harvard.edu r.crocker@physics.unimelb.edu.au r.volkas@physics.unimelb.edu.au fatuzzo@cerebro.cs.xu.edu jokipii@lpl.arizona.edu melia@physics.arizona.edu

¹ Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138
² Research Centre for High Energy Physics, School of Physics, University of Melbourne, Parkville 3010, Australia
³ Physics Department, Xavier University, Cincinnati, OH 45207
⁴ Department of Planetary Sciences, Lunar and Planetary Observatory, University of Arizona, 1629 East University Boulevard, Tucson, AZ 85721
⁵ Physics Department and Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721

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Abstract References Cited By

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The AGASA and SUGAR Anisotropies and TeV Gamma Rays from the Galactic Center: A Possible Signature of Extremely High Energy Neutrons

Injected spectrum for TeV γ-ray emission from the galactic center

Probing new physics with astrophysical neutrinos

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A Possible Link between the Galactic Center HESS Source and Sagittarius A*

Cosmic rays: the Second Knee and beyond

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Potential Neutrino Signals from Galactic γ-Ray Sources

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High Energy Emission from the Galactic Center

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Sgr A East as a high energy neutron and neutrino factory in the galactic centre

Enhanced Cosmic-Ray Flux and Ionization for Star Formation in Molecular Clouds Interacting with Supernova Remnants

Observation of Gamma Rays from the Galactic Center with the MAGIC Telescope

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Annihilation Emission from the Galactic Black Hole

Pulsar Wind Nebulae and the Nonthermal X-Ray Emission of Millisecond Pulsars

Capture of a Red Giant by the Black Hole Sagittarius A* as a Possible Origin for the TeV Gamma Rays from the Galactic Center

A Persistent High-Energy Flux from the Heart of the Milky Way: INTEGRAL's View of the Galactic Center

Detectable neutrino fluxes due to enhanced cosmic ray densities in the Galactic Centre region

Primary versus Secondary Leptons in the EGRET Supernova Remnants

A Variability and Localization Study of the Galactic Center Gamma-Ray Source 3EG J1746–2851

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