2005/06/07 by G. S. Japaridze, George Japaridze, Japaridze, George +2 · 1 citation
Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Neutrino Physics Research #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0506136
9 pages, 3 figures
arxiv created 2005/06/07 · openalex publication_date 2005/06/07 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The event reconstruction in high energy neutrino telescopes is based on the expression of the time delay distribution of the detected photons propagating to some distance from their emission point through a uniform and scattering medium. Considering a realistic detector with a finite time resolution, we derive an expression for the probability density function of the time delay of detected photons. The asymptotic properties of this function as well as its corresponding cumulative probability distribution are calculated and discussed.