| Full text | |
| Author(s): |
Becker‚ J.K.
;
Biermann‚ P.L.
;
Rhode‚ W.
Total Authors: 3
|
| Document type: | Journal article |
| Source: | Astroparticle Physics; v. 23, n. 4, p. 355-368, 2005. |
| Abstract | |
Water and ice Cherenkov telescopes of the present and future aim for the detection of a neutrino signal from extraterrestrial sources at energies E-V > PeV [Woschnagg and AMANDA Collaboration, Astro-ph/0409423, talk at Neutrino 2004; Montaruli, in: Peter W. Gorham, Particle Astrophysics Instrumentation, Proceedings of the SPIE, vol. 4858, 2003, p. 92; IceCube Collaboration, Astropart. Phys. 20 (2004) 507]. Some of the most promising extragalactic sources are active galactic nuclei (AGN). In this paper, the neutrino flux from two kinds of AGN sources will be estimated assuming p gamma interactions in the jets of the AGN. The first analyzed sample contains FR-II radio galaxies while the second AGN type examined are blazars. The result is highly dependent on the proton's index of the energy spectrum. To normalize the spectrum, the connection between neutrino and disk luminosity will be used by applying the jet-disk symbiosis model from Falcke and Biermann [Astron. Astrophys. 293 (1995) 665]. The maximum proton energy and thus, also the maximum neutrino energy of the source is connected to its disk luminosity, which was shown by Lovelace [Nature 262 (1976) 649] and was confirmed by Falcke et al. [Astron. Astrophys. 298 (1995) 375]. (c) 2005 Elsevier B.V. All rights reserved. (AU) | |
| FAPESP's process: | 00/06695-0 - Galaxy Evolution and Activity |
| Grantee: | Ronaldo Eustaquio de Souza |
| Support Opportunities: | Research Projects - Thematic Grants |