High Energy Neutrino Emission from Astrophysical Jets in the Galaxy
Joint Authors
Source
Advances in High Energy Physics
Issue
Vol. 2015, Issue 2015 (31 Dec. 2015), pp.1-7, 7 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2015-05-14
Country of Publication
Egypt
No. of Pages
7
Main Subjects
Abstract EN
We address simulated neutrino emission originated from astrophysical jets of compact objects within the Galaxy.
These neutrinos are of high energies (Eν of the order up to a few TeV) and for their observation specialized instruments are in operation, both on Earth and in orbit.
Furthermore, some next generation telescopes and detector facilities are in the process of design and construction.
The jet flow simulations are performed using the modern PLUTO hydrocode in its relativistic magnetohydrodynamic version.
One of the main ingredients of the present work is the presence of a toroidal magnetic field that confines the jet flow and furthermore greatly affects the distribution of the high energy neutrinos.
American Psychological Association (APA)
Smponias, T.& Kosmas, O. T.. 2015. High Energy Neutrino Emission from Astrophysical Jets in the Galaxy. Advances in High Energy Physics،Vol. 2015, no. 2015, pp.1-7.
https://search.emarefa.net/detail/BIM-1052617
Modern Language Association (MLA)
Smponias, T.& Kosmas, O. T.. High Energy Neutrino Emission from Astrophysical Jets in the Galaxy. Advances in High Energy Physics No. 2015 (2015), pp.1-7.
https://search.emarefa.net/detail/BIM-1052617
American Medical Association (AMA)
Smponias, T.& Kosmas, O. T.. High Energy Neutrino Emission from Astrophysical Jets in the Galaxy. Advances in High Energy Physics. 2015. Vol. 2015, no. 2015, pp.1-7.
https://search.emarefa.net/detail/BIM-1052617
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-1052617