Deeply penetrating particles in the 10 to the 17th power eV cosmic ray flux were investigated. No such events were found in 8.2 x 10 to the 6th power sec of running time. Limits were set on the following: quark-matter in the primary cosmic ray flux; long-lived, weakly interacting particles produced in p-air collisions; the astrophysical neutrino flux. In particular, the neutrino flux limit at 10 to the 17th power eV implies that z, the red shift of maximum activity is 10 in the model of Hill and Schramm
The cosmic ray spectrum has been shown to extend well beyond 10^{20}eV. With nearly 20 events observ...
An array of two spark chambers and six trays of plastic scintillation counters was used to search fo...
Precision measurements of the acoustic peaks of the cosmic microwave background indicate that neutri...
Journal ArticleWe report on a search for deeply penetrating particles in the > 10^17 eV cosmic-ray f...
We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Trans...
Some solutions of the hierarchy problem of particle physics can lead to significantly increased neut...
Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre A...
The expected proton and neutrino fluxes from decays of massive metastable relic particles is calcula...
In order to facilitate the identification of possible new physics signatures in neutrino telescopes,...
Cosmic rays from outer space enter the atmosphere with energies of up to 10^{11} GeV. The initial pa...
We give a brief overview of the current experimental and theoretical status of cosmic rays above ~10...
We constrain high-energy neutrino fluxes with the observed cosmic ray and gamma ray fluxes, include ...
The central regions of cosmic-ray air showers near sea level have been studied with the Leeds cloud ...
The surface detector array of the Pierre Auger Observatory is sensitive to ultra-high energy neutrin...
We report constraints on the sources of ultrahigh-energy cosmic rays (UHECRs) above 10^{9} GeV, bas...
The cosmic ray spectrum has been shown to extend well beyond 10^{20}eV. With nearly 20 events observ...
An array of two spark chambers and six trays of plastic scintillation counters was used to search fo...
Precision measurements of the acoustic peaks of the cosmic microwave background indicate that neutri...
Journal ArticleWe report on a search for deeply penetrating particles in the > 10^17 eV cosmic-ray f...
We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Trans...
Some solutions of the hierarchy problem of particle physics can lead to significantly increased neut...
Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre A...
The expected proton and neutrino fluxes from decays of massive metastable relic particles is calcula...
In order to facilitate the identification of possible new physics signatures in neutrino telescopes,...
Cosmic rays from outer space enter the atmosphere with energies of up to 10^{11} GeV. The initial pa...
We give a brief overview of the current experimental and theoretical status of cosmic rays above ~10...
We constrain high-energy neutrino fluxes with the observed cosmic ray and gamma ray fluxes, include ...
The central regions of cosmic-ray air showers near sea level have been studied with the Leeds cloud ...
The surface detector array of the Pierre Auger Observatory is sensitive to ultra-high energy neutrin...
We report constraints on the sources of ultrahigh-energy cosmic rays (UHECRs) above 10^{9} GeV, bas...
The cosmic ray spectrum has been shown to extend well beyond 10^{20}eV. With nearly 20 events observ...
An array of two spark chambers and six trays of plastic scintillation counters was used to search fo...
Precision measurements of the acoustic peaks of the cosmic microwave background indicate that neutri...
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