Advertisement
Perspective
Astronomy

New angle on cosmic rays

Science22 Sep 2017Vol 357, Issue 6357pp. 1240-1241DOI: 10.1126/science.aao5651

Abstract

Cosmic rays are nuclei that have been accelerated to relativistic velocities by astrophysical sources, arriving at Earth after traversing the space between us and the source. As electrically charged particles, they are deflected by magnetic fields, which scramble their directions in space (1). Finding deviations from the highly isotropic angular distribution of high-energy cosmic rays in the sky has long been a prime goal of cosmic-ray researchers. Marginal detections have been reported in the past that failed to hold up. On page 1266 of this issue, The Pierre Auger Collaboration (2) report a strong detection of a pronounced anisotropy in the arrival directions of cosmic rays with energies (E) of ≥8 EeV (8 × 1018 electron volts), indicating that they are of extragalactic origin.
Get full access to this article

View all available purchase options and get full access to this article.

Already a Subscriber?

References

1
T. K. Gaisser, R. Engel, E. Resconi, Cosmic Rays and Particle Physics (Cambridge University Press, ed. 2, 2016).
2
The Pierre Auger Collaboration, Science 357, 1266 (2017).
3
A. H. Compton, I. A. Getting, Phys. Rev. 47, 817 (1935).
4
M. Amenomori et al., Science 314, 439 (2006).
5
G. Guillian et al.(Super-Kamiokande Collaboration), Phys. Rev. D 75, 062003 (2007).
6
A. Abassi et al.(IceCube Collaboration), Astrophys. J. 740, 16 (2011).
7
M. Ahlers, P. Mertsch, Prog. Nucl. Part. Phys. 94, 184 (2017).
8
M. Kachelreiß, P. D. Serpico, Phys. Lett. B 640, 225 (2006).
9
M. Bilicki et al., Astrophys. J. 741, 31 (2011).
10
C. A. P. Bengaly Jr. et al., Month. Not. R. Astron. Soc. 464, 768 (2017).

Information & Authors

Information

Published In

Science
Volume 357 | Issue 6357
22 September 2017

Submission history

Published in print: 22 September 2017

Permissions

Request permissions for this article.

Authors

Affiliations

John S. Gallagher III
Department of Astronomy, University of Wisconsin-Madison, Madison, USA.
Francis Halzen
Department of Physics, University of Wisconsin-Madison, Madison, USA.

Notes

Metrics & Citations

Metrics

Article Usage
Altmetrics

Citations

Export citation

Select the format you want to export the citation of this publication.

View Options

Get Access

Log in to view the full text

AAAS ID LOGIN

AAAS login provides access to Science for AAAS Members, and access to other journals in the Science family to users who have purchased individual subscriptions.

Log in via OpenAthens.
Log in via Shibboleth.
More options

Purchase digital access to this article

Download and print this article for your personal scholarly, research, and educational use.

Purchase this issue in print

Buy a single issue of Science for just $15 USD.

View options

PDF format

Download this article as a PDF file

Download PDF

Media

Figures

Multimedia

Tables

Share

Share

Share article link

Share on social media