Orateur
Prof.
Olaf Scholten
(KVI, Univ. of Groningen)
Description
When an ultra-high energy (E>10^20 eV) neutrino hits the moon an electromagnetic pulse is generated. The instantaneous power of the pulse is so strong that they can be detected on Earth. In this presentation the observations will be described using the Westerbork Synthesis Radio Telescope on the basis of which more constraining limit have been set for the flux of neutrinos with energies exceeding 10^23 eV.
Auteur principal
Prof.
Olaf Scholten
(KVI, Univ. of Groningen)
Co-auteurs
A. G. de Bruyn
(Kapneyn Institute & ASTRON, Netherlands)
Heino Falcke
(IMAPP, Nijmegen, The Netherlands)
Jose Bacelar
(ASML, The Netherlands)
Kalpana Singh
(KVI, Groningen, The Netherlands)
R. al Yahyaoui
(KVI, The Netherlands)
R.G. Strom
(ASTRON & UvA, The Netherlands)
Robert Braun
(CSIRO-ATNF, Australia)
Stijn Buitink
(LBL, Berkeley, USA)
