(Goldstone
Lunar
Ultra-high energy neutrino
Experiment)
Other Web pages:
INSPIRE
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[1-1]
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Observation of the Askaryan effect: Coherent microwave Cherenkov emission from charge asymmetry in high energy particle cascades,
David Saltzberg et al.,
Phys. Rev. Lett. 86 (2001) 2802-2805,
arXiv:hep-ex/0011001.
[Saltzberg:2000bk]
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[1-2]
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Radio-frequency measurements of coherent transition and Cherenkov radiation: Implications for high-energy neutrino detection,
Peter Gorham et al.,
Phys. Rev. E62 (2000) 8590-8605,
arXiv:hep-ex/0004007.
[Gorham:2000ed]
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[2-1]
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Radio limits on an isotropic flux of > 100 EeV cosmic neutrinos,
P. W. Gorham, K. M. Liewer, C. J. Naudet, D. P. Saltzberg, D. R. Williams,
AIP Conf.Proc. 579 (2001) 177-188,
arXiv:astro-ph/0102435.
1st International Workshop on Radio Detection of High-Energy Particles (RADHEP 2000), Los Angeles, California, 16-18 Nov 2000.
[Gorham:2001aj]
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[2-2]
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Initial Results from a Search for Lunar Radio Emission from Interactions of > = 10^{19} eV Neutrinos and Cosmic Rays,
P. W. Gorham, K. M. Liewer, C. J. Naudet,
JETP Lett. 86 (2007) 287-291,
arXiv:astro-ph/9906504.
26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[Filonenko:2007zz]
Last Update: Thu 15 Oct 2026, 12:29:45 CET
