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Ultra-Transparent Antarctic Ice as a Supernova Detector
F. Halzen, J. E. Jacobsen, E. Zas
We have simulated the response of a high energy neutrino telescope in deep Antarctic ice to the stream of low energy neutrinos produced by a supernova. The passage of a large flux…
The Search for Neutrino Sources Beyond the Sun
S. Barwick, F. Halzen, P. B. Price
The hope is that in the near future neutrino astronomy, born with the identification of thermonuclear fusion in the sun and the particle processes controlling the fate of a nearby…
Colorless States in Perturbative QCD: Charmonium and Rapidity Gaps
J. F. Amundson, O. J. P. E'boli, E. M. Gregores +1
We point out that an unorthodox way to describe the production of rapidity gaps in deep inelastic scattering, recently proposed by Buchmüller and Hebecker, suggests a description o…
The Direct and Indirect Detection of Weakly Interacting Dark Matter Particles
F. Halzen
An ever-increasing body of evidence suggests that weakly interacting massive particles (WIMPs) constitute the bulk of the matter in the Universe. We illustrate how experimental dat…
Gamma Ray Astronomy with Underground Detectors
F. Halzen, T. Stanev
Underground detectors measure the directions of up-coming muons of neutrino origin. They can also observe down-going muons made by gamma rays in the Earth's atmosphere. Although ga…
The Direct and Indirect Detection of Weakly Interacting Dark Matter Particles
F. Halzen
An ever-increasing body of evidence suggests that weakly interacting massive particles (WIMPs) constitute the bulk of the matter in the Universe. Experimental data, dimensional ana…