Radio Detection of High Energy Particles: Coherence Versus Multiple Scales
arXiv:astro-ph/0003408 · doi:10.1103/PhysRevD.65.016003
Abstract
Radio Cherenkov emission underlines detection of high energy particles via a signal growing like the particle-energy-squared. Cosmic ray-induced electromagnetic showers are a primary application. While many studies have treated the phenomenon approximately, none have attempted to incorporate all the physical scales involved in problems with time- or spatially- evolving charges. We find it is possible to decompose the calculated fields into the product of a form factor, characterizing a moving charge distribution, multiplying a general integral which depends on the charge evolution. In circumstances of interest for cosmic ray physics, the resulting expressions can be evaluated explicitely in terms of a few parameters obtainable from shower codes. The classic issues of Frauhofer and Fresnel zones play a crucial role in the coherence.
25 pages, 10 figures
References in corpus (3)
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- Extra dimensions and Strong Neutrino-Nucleon interactions above eV : Breaking the GZK Barrier
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