2023ApJ...954..106A


Query : 2023ApJ...954..106A

2023ApJ...954..106A - Astrophys. J., 954, 106 (2023/September-1)

Feasibility of Correlated Extensive Air Shower Detection with a Distributed Cosmic-Ray Network.

ALBIN E.K. and WHITESON D.

Abstract (from CDS):

We explore the sensitivity offered by a global network of cosmic-ray detectors to a novel, unobserved phenomenon: widely separated simultaneous extended air showers. Existing localized observatories work independently to observe individual showers, offering insight into the source and nature of ultrahigh-energy cosmic rays. However no current observatory is large enough to provide sensitivity to anticipated processes such as the Gerasimova-Zatsepin effect or potential new physics that generate simultaneous air showers separated by hundreds to thousands of kilometers. A global network of consumer electronics (the Cosmic Rays Found In Smartphones (CRAYFIS) experiment), may provide a novel opportunity for observation of such phenomena. Two user scenarios are explored. In the first, with maximal user adoption, we find that statistically significant discoveries of spatially separated but coincident showers are possible within a couple years. In the second, more practical adoption model with 106 active devices, we find a worldwide CRAYFIS to be sensitive to novel “burst” phenomena where many simultaneous extensive air showers (EAS) occur at once.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Ultra-high-energy cosmic radiation - Cosmic ray showers - Particle astrophysics - Cosmic rays - High energy astrophysics

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Fermi Bubbles bub 17 45 -29.0           ~ 525 0

Query : 2023ApJ...954..106A

Basic data :
NAME Fermi Bubbles -- Bubble
Other object types:
otypes_help
bub (), gam ()
ICRS coord. (ep=J2000) :
17 45 22.9 -29 01 17 (Gamma-ray) [ ] E ~
FK4 coord. (ep=B1950 eq=1950) :
17 42 12.2 -29 00 07 [ ]
Gal coord. (ep=J2000) :
359.9000 -00.0000 [ ]
Angular size (arcmin):
6000 2580 120 (~) E 2010ApJ...724.1044S
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Identifiers (2) :
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NAME Fermi Bubbles NAME Fermi Bubble

References (525 between 1850 and 2026) (Total 525)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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