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Phys. Rev. Lett. 103, 191301 (2009) [4 pages]

Improved Flux Limits for Neutrinos with Energies above 1022  eV from Observations with the Westerbork Synthesis Radio Telescope

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O. Scholten1, S. Buitink2,3, J. Bacelar4, R. Braun5, A. G. de Bruyn6,7, H. Falcke2, K. Singh1, B. Stappers8, R. G. Strom7,9, and R. al Yahyaoui1
1Kernfysisch Versneller Instituut, University of Groningen, 9747 AA, Groningen, The Netherlands
2Department of Astrophysics, IMAPP, Radboud University, 6500 GL Nijmegen, The Netherlands
3Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
4ASML Netherlands BV, P.O. Box 324, 5500 AH Veldhoven, The Netherlands
5CSIRO-ATNF, P.O. Box 76, Epping NSW 1710, Australia
6Kapteyn Institute, University of Groningen, 9747 AA, Groningen, The Netherlands
7ASTRON, 7990 AA Dwingeloo, The Netherlands
8Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom
9Astronomical Institute “A. Pannekoek,” University of Amsterdam, 1098 SJ Amsterdam, The Netherlands

Received 4 July 2009; revised 25 October 2009; published 6 November 2009

Particle cascades initiated by ultrahigh energy neutrinos in the lunar regolith will emit an electromagnetic pulse with a time duration of the order of nanoseconds through a process known as the Askaryan effect. It has been shown that in an observing window around 150 MHz there is a maximum chance for detecting this radiation with radio telescopes commonly used in astronomy. In 50 h of observation time with the Westerbork Synthesis Radio Telescope array we have set a new limit on the flux of neutrinos, summed over all flavors, with energies in excess of 4×1022  eV.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.103.191301
DOI:
10.1103/PhysRevLett.103.191301
PACS:
95.35.+d, 95.85.Bh, 98.70.Sa