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ANALYTIC APERTURE CALCULATION AND SCALING LAWS FOR RADIO DETECTION OF LUNAR-TARGET ULTRA-HIGH-ENERGY NEUTRINOS

Journal Article · · Astrophysical Journal
; ;  [1]
  1. Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52245 (United States)
We derive analytic expressions and approximate them in closed form, for the effective detection aperture for Cerenkov radio emission from ultra-high-energy neutrinos striking the Moon. The resulting apertures are in good agreement with recent Monte Carlo simulations and support the conclusion of James and Protheroe that neutrino flux upper limits derived from the GLUE search were too low by an order of magnitude. We also use our analytic expressions to derive scaling laws for the aperture as a function of observational and lunar parameters. We find that at low frequencies downward-directed neutrinos always dominate, but at higher frequencies, the contribution from upward-directed neutrinos becomes increasingly important, especially at lower neutrino energies. Detecting neutrinos from Earth near the Greisen-Zatsepin-Kuz'min regime will likely require radio telescope arrays with extremely large collecting area (A{sub e} approx 10{sup 6} m{sup 2}) and hundreds of hours exposure time. Higher-energy neutrinos are most easily detected using lower frequencies. Lunar surface roughness is a decisive factor for obtaining detections at higher frequencies (nuapprox> 300 MHz) and higher energies (E approx> 10{sup 21} eV).
OSTI ID:
21378087
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 706; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English