Physics
Scientific paper
Jul 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...282..398o&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 282, July 15, 1984, p. 398-401. Research supported by the Conselho Nacional
Physics
5
Coherent Scattering, Cosmic Rays, Neutrinos, Particle Mass, Matter (Physics), Particle Flux Density, Scattering Cross Sections
Scientific paper
According to recent studies, the dominant mass in the universe may very well be massive cosmic neutrinos. For the detection of cosmic neutrinos, Opher (1974, 1982) has suggested a method which is based on coherent scattering. Only second-order in G coherent scattering would be possible, if the massive cosmic neutrino flux equals the massive cosmic antineutrino flux. G represents the weak coupling constant. A study is conducted regarding the optimum manner in which matter can be arranged in order to obtain a maximum value for the second-order in G momentum transfer. The inhomogeneous matter is characterized by independent scattering spheres of arbitrary diameter. The study is based on a utilization of Rayleigh-Gans scattering theory. It is found that a large increase in the scattering is obtained for optimized inhomogeneous matter.
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