Ultrahigh energy neutrino interactions and weak-scale string theories
arXiv:astro-ph/0005309 · doi:10.1103/PhysRevD.62.103006
Abstract
It has been suggested that ultrahigh energy neutrinos can acquire cross-sections approaching hadronic size if the string scale is as low as 1-10 TeV. In this case, the vertical air showers observed with energies above the Greisen-Zatsepin-Kuzmin cutoff at E approximately 6x10^{19} eV could be initiated by neutrinos which are the only known primaries able to travel long distances unimpeded. We have calculated the neutrino-nucleon cross-section due to the exchange of Kaluza-Klein excitations of the graviton in a field theoretical framework. We have found that the neutrino-nucleon cross section and the transferred energy per interaction are too small to explain vertical showers even in the most optimistic scenario.
7 pages, 3 figures; discussion of the sensitivity of Auger/Owl shortened, matches version to be published
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