High Energy Neutrino Emission from Astrophysical Jets in the Galaxy
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 nex...
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| Format: | Article |
| Language: | English |
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Wiley
2015-01-01
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| Series: | Advances in High Energy Physics |
| Online Access: | http://dx.doi.org/10.1155/2015/921757 |
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| author | T. Smponias O. T. Kosmas |
| author_facet | T. Smponias O. T. Kosmas |
| author_sort | T. Smponias |
| collection | DOAJ |
| description | 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. |
| format | Article |
| id | doaj-art-b89fa5e31e8d4027a3b5bea45a56ddd0 |
| institution | Kabale University |
| issn | 1687-7357 1687-7365 |
| language | English |
| publishDate | 2015-01-01 |
| publisher | Wiley |
| record_format | Article |
| series | Advances in High Energy Physics |
| spelling | doaj-art-b89fa5e31e8d4027a3b5bea45a56ddd02025-02-03T06:42:04ZengWileyAdvances in High Energy Physics1687-73571687-73652015-01-01201510.1155/2015/921757921757High Energy Neutrino Emission from Astrophysical Jets in the GalaxyT. Smponias0O. T. Kosmas1Division of Theoretical Physics, University of Ioannina, GR-45110 Ioannina, GreeceChair of Applied Dynamics, University of Erlangen-Nuremberg, Haberstrasse 1, D-91058 Erlangen, GermanyWe 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.http://dx.doi.org/10.1155/2015/921757 |
| spellingShingle | T. Smponias O. T. Kosmas High Energy Neutrino Emission from Astrophysical Jets in the Galaxy Advances in High Energy Physics |
| title | High Energy Neutrino Emission from Astrophysical Jets in the Galaxy |
| title_full | High Energy Neutrino Emission from Astrophysical Jets in the Galaxy |
| title_fullStr | High Energy Neutrino Emission from Astrophysical Jets in the Galaxy |
| title_full_unstemmed | High Energy Neutrino Emission from Astrophysical Jets in the Galaxy |
| title_short | High Energy Neutrino Emission from Astrophysical Jets in the Galaxy |
| title_sort | high energy neutrino emission from astrophysical jets in the galaxy |
| url | http://dx.doi.org/10.1155/2015/921757 |
| work_keys_str_mv | AT tsmponias highenergyneutrinoemissionfromastrophysicaljetsinthegalaxy AT otkosmas highenergyneutrinoemissionfromastrophysicaljetsinthegalaxy |