Searching for neutrino radio flashes from the Moon with LOFAR

Stijn Buitink, Arthur Corstanje, Emilio Enriquez, Heino Falcke, Wilfred Frieswijk, Jörg Hörandel, Maaijke Mevius, Anna Nelles, Satyendra Thoudam, Pim Schellart, Olaf Scholten, Sanderter Veen, Martin Van Den Akker

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

4 Scopus citations

Abstract

Ultra-high-energy neutrinos and cosmic rays produce short radio flashes through the Askaryan effect when they impact on the Moon. Earthbound radio telescopes can search the Lunar surface for these signals. A new generation of lowfrequency, digital radio arrays, spearheaded by LOFAR, will allow for searches with unprecedented sensitivity. In the first stage of the NuMoon project, low-frequency observations were carried out with the Westerbork Synthesis Radio Telescope, leading to the most stringent limit on the cosmic neutrino flux above 1023 eV. With LOFAR we will be able to reach a sensitivity of over an order of magnitude better and to decrease the threshold energy.

Original languageBritish English
Title of host publication5th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2012
Pages27-31
Number of pages5
DOIs
StatePublished - 2013
Event5th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2012 - Erlangen, Germany
Duration: 19 Jun 201222 Jun 2012

Publication series

NameAIP Conference Proceedings
Volume1535
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

Conference5th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2012
Country/TerritoryGermany
CityErlangen
Period19/06/1222/06/12

Keywords

  • cosmic rays
  • Moon
  • neutrinos
  • radio emission
  • radio telescopes

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