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Constraints on Ultra-high-energy Neutrino Flux from Radio Observations of the Moon : Volume 8, Issue 1 (22/08/2012)

By Buitink, S.

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Book Id: WPLBN0004002836
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File Size: Pages 5
Reproduction Date: 2015

Title: Constraints on Ultra-high-energy Neutrino Flux from Radio Observations of the Moon : Volume 8, Issue 1 (22/08/2012)  
Author: Buitink, S.
Volume: Vol. 8, Issue 1
Language: English
Subject: Science, Astrophysics, Space
Collections: Periodicals: Journal and Magazine Collection, Copernicus GmbH
Historic
Publication Date:
2012
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications

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Falcke, H., Singh, K., James, C., Scholten, O., Stappers, B., Buitink, S.,...Mevius, M. (2012). Constraints on Ultra-high-energy Neutrino Flux from Radio Observations of the Moon : Volume 8, Issue 1 (22/08/2012). Retrieved from http://www.ebooklibrary.org/


Description
Description: Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA. The NuMoon project aims to study ultra-high-energy neutrinos and cosmic rays by using radio telescopes to search for short pulses from the Moon. These pulses are created when a neutrino or cosmic ray impinges on the Moon and interacts below the lunar surface. Part of the energy is converted into a hadronic shower, which emits radio emission in a process known as the Askaryan effect. In the first phase of the NuMoon project, 46 hrs of data were collected with the Westerbork Synthesis Radio Telescope in a low frequency band: 40–80 MHz. This resulted in an upper limit on the neutrino flux above 1022 eV which is an order of magnitude lower than previous limits. Additionally, an upper limit has been set on the ultra-high-energy cosmic-ray flux. The second phase of NuMoon will consist of observations with LOFAR.

Summary
Constraints on ultra-high-energy neutrino flux from radio observations of the Moon

Excerpt
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