Constraints on Extragalactic Point Source Flux from Diffuse Neutrino Limits
arXiv:0908.4266 · doi:10.1103/PhysRevD.81.023001
Abstract
We constrain the maximum flux from extragalactic neutrino point sources by using diffuse neutrino flux limits. We show that the maximum flux from extragalactic point sources is E^2(dN/dE) < 1.4 x 10^-9 (L_nu/2x10^43 erg/s)^1/3 GeV cm-^2 s^-1 from individual point sources with average neutrino luminosity per decade, L_nu. It depends only slightly on factors such as the inhomogeneous matter density distribution in the local universe, the luminosity distribution, and the assumed spectral index. The derived constraints are at least one order of magnitude below the current experimental limits from direct searches. Significant constraints are also derived on the number density of neutrino sources and on the total neutrino power density.
7 pages, 3 figures, and 2 tables
References in corpus (6)
- Correlation of the highest energy cosmic rays with nearby extragalactic objects
- The emptiness of voids: yet another over-abundance problem for the LCDM model
- Multi-year search for a diffuse flux of muon neutrinos with AMANDA-II
- Search for Point Sources of High Energy Neutrinos with Final Data from AMANDA-II
- Ultra-high energy Neutrinos from Centaurus A and the Auger hot spot
- Perspectives of High Energy Neutrino Astronomy
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