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Title: SOLAR SYSTEM OBJECTS AS COSMIC RAYS DETECTORS

Abstract

In a recent Letter, Jupiter is presented as an efficient detector for Ultra-High Energy Cosmic Rays (UHECRs), through measurement by an Earth-orbiting satellite of gamma rays from UHECRs showers produced in Jupiter's atmosphere. We show that this result is incorrect, due to erroneous assumptions on the angular distribution of shower particles. We evaluated other solar system objects as potential targets for UHECRs detection, and found that the proposed technique is either not viable or not competitive with traditional ground-based UHECRs detectors.

Authors:
 [1];  [2]
  1. Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 (United States)
  2. Department of Physics, University of Chicago, Chicago, IL 60637 (United States)
Publication Date:
OSTI Identifier:
22365361
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal Letters; Journal Volume: 791; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ANGULAR DISTRIBUTION; COSMIC RADIATION; DETECTION; GAMMA RADIATION; JUPITER PLANET; POTENTIALS; SATELLITES; SOLAR SYSTEM

Citation Formats

Privitera, P., and Motloch, P., E-mail: priviter@kicp.uchicago.edu. SOLAR SYSTEM OBJECTS AS COSMIC RAYS DETECTORS. United States: N. p., 2014. Web. doi:10.1088/2041-8205/791/1/L15.
Privitera, P., & Motloch, P., E-mail: priviter@kicp.uchicago.edu. SOLAR SYSTEM OBJECTS AS COSMIC RAYS DETECTORS. United States. doi:10.1088/2041-8205/791/1/L15.
Privitera, P., and Motloch, P., E-mail: priviter@kicp.uchicago.edu. Sun . "SOLAR SYSTEM OBJECTS AS COSMIC RAYS DETECTORS". United States. doi:10.1088/2041-8205/791/1/L15.
@article{osti_22365361,
title = {SOLAR SYSTEM OBJECTS AS COSMIC RAYS DETECTORS},
author = {Privitera, P. and Motloch, P., E-mail: priviter@kicp.uchicago.edu},
abstractNote = {In a recent Letter, Jupiter is presented as an efficient detector for Ultra-High Energy Cosmic Rays (UHECRs), through measurement by an Earth-orbiting satellite of gamma rays from UHECRs showers produced in Jupiter's atmosphere. We show that this result is incorrect, due to erroneous assumptions on the angular distribution of shower particles. We evaluated other solar system objects as potential targets for UHECRs detection, and found that the proposed technique is either not viable or not competitive with traditional ground-based UHECRs detectors.},
doi = {10.1088/2041-8205/791/1/L15},
journal = {Astrophysical Journal Letters},
number = 1,
volume = 791,
place = {United States},
year = {Sun Aug 10 00:00:00 EDT 2014},
month = {Sun Aug 10 00:00:00 EDT 2014}
}