Tracing protons through the Galactic magnetic field: a clue for charge composition of ultra-high energy cosmic rays

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

6 pages, 3 figures, LaTeX

Scientific paper

10.1016/S0927-6505(02)00109-3

We reconstruct the trajectories of ultra-high energy cosmic rays (UHECR) - observed by the AGASA experiment - in the Galactic magnetic field assuming that all particles have the same charge. We then study correlations between the reconstructed events and BL Lacs. The correlations have significance below 10^{-3} in the case of particles with charge +1. In the case of charge -1 the correlations are absent. We interpret this as evidence that protons are present in the flux of UHECR. Observed correlation provides an independent evidence that BL Lacs emit UHECR.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Tracing protons through the Galactic magnetic field: a clue for charge composition of ultra-high energy cosmic rays does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Tracing protons through the Galactic magnetic field: a clue for charge composition of ultra-high energy cosmic rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tracing protons through the Galactic magnetic field: a clue for charge composition of ultra-high energy cosmic rays will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-720891

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.