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The Potential of Spaced-based High-Energy Neutrino Measurements via the Airshower Cherenkov Signal
Future space-based experiments, such as OWL and JEM-EUSO, view large
atmospheric and terrestrial neutrino targets. With energy thresholds slightly
above 10^19 eV for observing airshowers via air fluorescence, the potential for
observing the cosmogenic neutrino flux associated with the GZK effect is
limited. However, the forward Cherenkov signal associated with the airshower
can be observed at much lower energies. A simulation was developed to determine
the Cherenkov signal strength and spatial extent at low-Earth orbit for
upward-moving airshowers. A model of tau neutrino interactions in the Earth was
employed to determine the event rate of interactions that yielded a tau lepton
which would induce an upward-moving airshower observable by a space-based
instrument. The effect of neutrino attenuation by the Earth forces the viewing
of the Earth's limb to observe the nu_tau-induced Cherenkov airshower signal at
above the OWL Cherenkov energy threshold of ~10^16.5 eV for limb-viewed events.
Furthermore, the neutrino attenuation limits the effective terrestrial neutrino
target area to ~3x10^5 km^2 at 10^17 eV, for an orbit of 1000 km and an
instrumental full Field-of-View of 45 degrees. This translates into an
observable cosmogenic neutrino event rate of ~1/year based upon two different
models of the cosmogenic neutrino flux, assuming neutrino oscillations and a
10% duty cycle for observation.Comment: Contribution to the 32nd ICRC, Beijing, China, August 2011;
Paper#1331, 4 pages, 4 figure
Organic atmospheric particulate material
Carbonaceous compounds comprise a substantial fraction of atmospheric particulate matter (PM). Particulate organic material can be emitted directly into the atmosphere or formed in the atmosphere when the oxidation products of certain volatile organic compounds condense. Such products have lower volatilities than their parent molecules as a result of the fact that adding oxygen and/or nitrogen to organic molecules reduces volatility. Formation of secondary organic PM is often described in terms of a fractional mass yield, which relates how much PM is produced when a certain amount of a parent gaseous organic is oxidized. The theory of secondary organic PM formation is outlined, including the role of water, which is ubiquitous in the atmosphere. Available experimental studies on secondary organic PM formation and molecular products are summarized
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Light Quark Masses and Mixing Angles
I review the present state of our knowledge about the masses and weak mixing
elements of the u, d, s quarks. This is the written version of lectures given
in the 1993 Theoretical Advanced Study Institute (TASI).Comment: UMHEP-402, Latex file, 27 page
New insights concerning dimension-eight effects in weak decays
Most past work on weak nonleptonic decays has mixed dimensional
regularization in the weak operator product expansion with some form of a
cutoff regularization in the evaluation of the matrix elements. Even with the
usual technique of matching the two schemes, this combination misses physics at
short distance which can be described by dimension eight (and higher dimension)
operators. I describe some recent work with V. Cirigliano and E. Golowich which
clarifies these effects and provides a numerical estimate suggesting that they
are important.Comment: 3 pages, talk presented at the Division of Particles and Fields
Meeting, DPF 2000, Columbus, Ohio, Aug. 200
The Controversy Concerning Nomenclature Vis-A-Vis Homosexuality
Father Harvey\u27s article contemplates the changes that have and will accrue from the recent AP A decision regarding homosexuals
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