| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1778935 | New Astronomy | 2015 | 4 Pages |
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.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Ashok Razdan,