TY - GEN
T1 - Is the present day, local cosmic ray spectral index representative of the average?
AU - Eichler, David
AU - Kumar, Rahul
AU - Pohl, Martin
N1 - Publisher Copyright:
© 2013 Sociedade Brasileira de Fisica. All Rights Reserved.
PY - 2013/1/1
Y1 - 2013/1/1
N2 - The hypothesis is considered that the present, local Galactic cosmic ray spectrum is, due to source intermittency, softer than average over time and over the Galaxy. Measurements of muogenic nuclides underground could provide an independent measurement of the time averaged spectrum. Source intermittency could also account for the surprising low anisotropy reported by the IceCube collaboration. Predictions for Galactic emission of ultrahigh-energy quanta, such as UHE gamma rays and neutrinos, might be higher or lower than previously estimated.
AB - The hypothesis is considered that the present, local Galactic cosmic ray spectrum is, due to source intermittency, softer than average over time and over the Galaxy. Measurements of muogenic nuclides underground could provide an independent measurement of the time averaged spectrum. Source intermittency could also account for the surprising low anisotropy reported by the IceCube collaboration. Predictions for Galactic emission of ultrahigh-energy quanta, such as UHE gamma rays and neutrinos, might be higher or lower than previously estimated.
KW - Cosmic rays
KW - Cosmogenic nuclei
UR - http://www.scopus.com/inward/record.url?scp=85052320096&partnerID=8YFLogxK
M3 - Conference contribution
AN - SCOPUS:85052320096
T3 - Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013
BT - Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013
PB - Sociedade Brasileira de Fisica
T2 - 33rd International Cosmic Rays Conference, ICRC 2013
Y2 - 2 July 2013 through 9 July 2013
ER -