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High Energy Gamma Rays and Neutrinos from Star-forming Activities in the Galactic and Extragalactic Sources

Published online by Cambridge University Press:  09 February 2017

Soebur Razzaque
Soebur Razzaque*
Affiliation:
Department of Physics, University of Johannesburg, PO Box 524, Auckland Park 2006, South Africa email: srazzaque@uj.ac.za
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Abstract

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The origin of the IceCube astrophysical neutrinos is an outstanding question. Star-forming activities which can accelerate particles to very high energies have been suggested as possible origin of these neutrinos. I will present a scenario where a subset of the neutrino events originate from the Galactic center region and Fermi Bubbles, resulting from star-forming activities. Multi-messenger signal in high energy gamma rays and neutrinos can probe this scenario. I will also present an analysis of the statistical association of the star-forming sources in our Galaxy and outside, with astrophysical neutrinos, as well as expected neutrino signal from these sources by fitting gamma-ray data.

Keywords

neutrinosgamma rays: theoryGalaxy: center
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S322: The Multi-Messenger Astrophysics of the Galactic Centre , July 2016 , pp. 218 - 219
Copyright
Copyright © International Astronomical Union 2017 

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