Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..202..101c&link_type=abstract
IN: Physics and astrophysics from a lunar base; Proceedings of the 1st NASA Workshop, Stanford, CA, May 19, 20, 1989 (A91-56551
Astronomy and Astrophysics
Astrophysics
Neutrinos, Nuclear Astrophysics, Radiation Detectors, Supernovae, Gravitational Wave Antennas, Gravity Waves, Inelastic Scattering, Scattering Cross Sections, Moon, Utilization, Lunar Base, Physics, Astrophysics, Science Aspects, Supernovas, Neutrinos, Bursts, Neutrons, Scattering, Particles, Design, Equipment, Calcium Carbonate, Calculations, Techniques, Gravity Waves, Technical Aspects, Spectra, Diagrams
Scientific paper
The feasibility of astrophysical neutrino detectors is studied, which is based on the detection of neutrons produced in neutrino-nucleus inelastic scattering events. Collective nuclear effects greatly enhancing the relevant interaction cross sections over those of single particle interactions are discussed. These effects can help to reduce the mass required for neutrino detectors. An example of a simple detector based on CaCO3 neutrino targets and BF3 neutron counters is presented. Neutron background limitations are discussed and the possibility of forming a coincidence between neutrino detectors and future gravity wave detectors is also considered.
Cline David
Fenyves E.
Foshe Tyler
Fuller Gary
Meyer Bertrand
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