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Crab pulsar spectrum: A non-extensive approach
Institution:1. School of Physics and Electronic Information, Huaibei Normal University, Huaibei 235000, Anhui Province, PR China;2. College of Science/Department of Physics & NAOC-GZU-Sponsored Center for Astronomy Research, GuiZhou University, Guiyang 550025, PR China;3. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, PR China;1. INAF – Catania Astrophysical Observatory, via S. Sofia, 78, I-95123 Catania, Italy;2. York Creek Observatory, Georgetown, Tasmania, Australia;3. Eastern University, St. Davids, PA, USA
Abstract:Non extensive statistical physics has been applied to various problems in physics including astrophysics. In this paper we explore the possibility of using non-extensive approach to explain the recently observed pulsed γ-ray from Crab pulsar above 100 GeV observed by VERITAS γ-ray telescope.
Keywords:Crab pulsar  Non-extensive statistical physics  Inverse Compton scattering
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