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2007 (English)In: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 98, no 7, p. 071103-Article in journal (Refereed) Published
Abstract [en]
The Moon provides a huge effective detector volume for ultrahigh energy cosmic neutrinos, which generate coherent radio pulses in the lunar surface layer due to the Askaryan effect. We report systematic Monte Carlo simulations which show that radio instruments on board a Moon-orbiting satellite can detect Askaryan pulses from neutrinos with energies above 10^{19} eV, i.e. near and above the interesting GZK limit, at the very low fluxes predicted in different scenarios.
National Category
Physical Sciences
Identifiers
urn:nbn:se:uu:diva-26236 (URN)10.1103/PhysRevLett.98.071103 (DOI)000244250300016 ()
2007-02-152007-02-152017-12-07Bibliographically approved