|Measurement of the atmospheric vµ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope|Adrián-Martínez, S.; van Haren, H.; ANTARES collaboration (2013). Measurement of the atmospheric vµ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope. Eur. Phys. J. C 73: 2606 1-12. hdl.handle.net/10.1140/epjc/s10052-013-2606-4
In: The European Physical Journal C. Springer: Berlin. ISSN 1434-6044, more
|Authors|| || Top |
- Adrián-Martínez, S.
- van Haren, H., more
- ANTARES collaboration
Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric ?µ+?¯µ energy spectrum in the energy range 0.1–200 TeV is presented, using data collected by the ANTARES underwater neutrino telescope from 2008 to 2011. Overall, the measured flux is ~25 % higher than predicted by the conventional neutrino flux, and compatible with the measurements reported in ice. The flux is compatible with a single power-law dependence with spectral index ? meas=3.58±0.12. With the present statistics the contribution of prompt neutrinos cannot be established.