The LPM showers traversing the atmosphere

Details The LPM showers traversing the atmosphere The LPM showers traversing the atmosphere

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..39..432w&link_type=abstract

Journal of Physics: Conference Series, Volume 39, Issue 1, pp. 432-434 (2006).

Physics

1

Scientific paper

We simulate the LPM showers due to Extremely-High-Energy(EHE) neutrinos traversing atmosphere horizontally without colliding with the Earth. We calculate the LPM showers with energies of 1017eV to 1022eV, using the hybrid method as exactly as possible. Reffecting the complicated change in the air density along the trajectories of the shower developments, the variety of the LPM showers is shown to depend on their starting points and their heights. The EHE LPM showers in atmosphere are exclusively produced by EHE neutrinos. Therefore, the studies on the LPM showers are very important for EHE neutrino astrophysics. As an example, the air fluorescence photon profiles of the LPM showers are also given for the future satellite-based experiment.

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