New possible detection schemes for relic Galactic neutrinos

Details New possible detection schemes for relic Galactic neutrinos New possible detection schemes for relic Galactic neutrinos

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cqgra..13a.207s&link_type=abstract

Classical and Quantum Gravity, Volume 13, Issue 11A, pp. A207-A217 (1996).

Computer Science

Scientific paper

We discuss the feasibility of the detection of relic neutrinos that may be present in the Galactic halo. We analyse their effect on macroscopic targets, comparing the detection proposals made so far and presenting new experimental schemes. In all cases the acceleration of the test masses is bounded by the value of the refractive index of neutrinos N as follows: 0264-9381/13/11A/030/img5, where 0264-9381/13/11A/030/img6 for all materials and x = 0.5 in the best case. 1315, 9880, 0480

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