Abstract
Ultra high energy particles arrive at Earth constantly. They provide a beam at energies higher than any man-made accelerator, but at a very low rate. Two large experiments, the Pierre Auger Observatory and the Telescope Array experiment, have been taking data for several years now covering together the whole sky. I summarize the most recent measurements from both experiments, I compare their results and, for a change, I highlight their agreements.
| Original language | English (US) |
|---|---|
| State | Published - Dec 1 2011 |
| Event | 31st International Conference on Physics in Collision, PIC 2011 - Vancouver, BC, Canada Duration: Aug 28 2011 → Sep 1 2011 |
Other
| Other | 31st International Conference on Physics in Collision, PIC 2011 |
|---|---|
| Country | Canada |
| City | Vancouver, BC |
| Period | 8/28/11 → 9/1/11 |
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All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics
Cite this
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Ultra high energy cosmic rays. / Mostafa, Miguel.
2011. Paper presented at 31st International Conference on Physics in Collision, PIC 2011, Vancouver, BC, Canada.Research output: Contribution to conference › Paper
TY - CONF
T1 - Ultra high energy cosmic rays
AU - Mostafa, Miguel
PY - 2011/12/1
Y1 - 2011/12/1
N2 - Ultra high energy particles arrive at Earth constantly. They provide a beam at energies higher than any man-made accelerator, but at a very low rate. Two large experiments, the Pierre Auger Observatory and the Telescope Array experiment, have been taking data for several years now covering together the whole sky. I summarize the most recent measurements from both experiments, I compare their results and, for a change, I highlight their agreements.
AB - Ultra high energy particles arrive at Earth constantly. They provide a beam at energies higher than any man-made accelerator, but at a very low rate. Two large experiments, the Pierre Auger Observatory and the Telescope Array experiment, have been taking data for several years now covering together the whole sky. I summarize the most recent measurements from both experiments, I compare their results and, for a change, I highlight their agreements.
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M3 - Paper
AN - SCOPUS:84884649657
ER -