A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neutrino telescope is presented. A (0.83 x 2 pi) sr sky was monitored for a total of 334 days of equivalent live time. The searched signal corresponds to an excess of events, produced by astrophysical sources, over the expected atmospheric neutrino background. The observed number of events is found compatible with the background expectation. Assuming an E-2 flux spectrum, a 90% c.l. upper limit on the diffuse nu(mu) flux of E-2 Phi(90%) = 5.3 x 10(-8) GeV cm(-2) s(-1) sr(-1) in the energy range 20 TeV-2.5 PeV is obtained. Other signal models with different energy spectra are also tested and some rejected. </p
The surface detector array of the Pierre Auger Observatory can detect neutrinos with energy E-nu bet...
14 pages, 6 figuresA search for a diffuse flux of astrophysical muon neutrinos, using data collected...
Solar Atmospheric Neutrinos (SA nu s) are produced by the interaction of cosmic rays with the solar ...
A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neu...
none143A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTA...
Results are presented of a search for cosmic sources of high-energy neutrinos with the ANTARES neutr...
Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic ra...
A search for cosmic neutrino sources using six years of data collected by the ANTARES neutrino teles...
A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neu...
The surface detector array of the Pierre Auger Observatory can detect neutrinos with energy E-nu bet...
14 pages, 6 figuresA search for a diffuse flux of astrophysical muon neutrinos, using data collected...
Solar Atmospheric Neutrinos (SA nu s) are produced by the interaction of cosmic rays with the solar ...
A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neu...
none143A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTA...
Results are presented of a search for cosmic sources of high-energy neutrinos with the ANTARES neutr...
Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic ra...
A search for cosmic neutrino sources using six years of data collected by the ANTARES neutrino teles...
A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neu...
The surface detector array of the Pierre Auger Observatory can detect neutrinos with energy E-nu bet...
14 pages, 6 figuresA search for a diffuse flux of astrophysical muon neutrinos, using data collected...
Solar Atmospheric Neutrinos (SA nu s) are produced by the interaction of cosmic rays with the solar ...