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Prospects for radio detection of ultrahigh energy cosmic neutrinos from a satellite orbiting the moon
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Nuclear and Particle Physics, High Energy Physics. (Teoretisk högenergifysik)
2006 (English)In: Physica scripta. T, ISSN 0281-1847, Vol. T127, 78-79 p.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 surface layer through the Askaryan effect. Simulations show that radio instruments, on board a satellite in orbit around the Moon, can detect neutrinos with an energy above 1019 eV, i.e. near and beyond the interesting Greisen-Zatsepin-Kuzmin (GZK) limit. We summarize here our results from (Stl et al 2006 Preprint astro-ph/0604199) on the experimental efficiency for different satellite parameters.

Place, publisher, year, edition, pages
2006. Vol. T127, 78-79 p.
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Physical Sciences
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URN: urn:nbn:se:uu:diva-23178DOI: 10.1088/0031-8949/2006/T127/027ISI: 000246789900028OAI: oai:DiVA.org:uu-23178DiVA: diva2:50952
Available from: 2007-01-25 Created: 2007-01-25 Last updated: 2017-12-07Bibliographically approved

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Stål, Oscar

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