Ultra High Energy Cosmic Rays: the present position and the need for mass composition measurements

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

11 pages with 5 figures. Based on invited talk at `Thinking, Observing and Mining the Universe', Sorrento Italy: 22 - 27 Septe

Scientific paper

The present situation with regard to experimental data on ultra high-energy cosmic rays is briefly reviewed. Whilst detailed knowledge of the shape of the energy spectrum is still lacking, it is clear that events above 10^20 eV do exist. Evidence for clustering of the directions of some of the highest energy events remains controversial. Clearly, more data are needed and these will come from the southern branch of the Pierre Auger Observatory in the next few years. What is evident is that our knowledge of the mass composition of cosmic rays is deficient at all energies above 10^18 eV. It must be improved if we are to discover the origin of the highest energy cosmic rays. The major part of the paper is concerned with this problem: it is argued that there is no compelling evidence to support the common assumption that cosmic rays of the highest energies are protons.

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

Ultra High Energy Cosmic Rays: the present position and the need for mass composition measurements 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 Ultra High Energy Cosmic Rays: the present position and the need for mass composition measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultra High Energy Cosmic Rays: the present position and the need for mass composition measurements will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-307341

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