Liquid xenon calorimeter for observation of cosmic line gamma-rays in the GeV region

Details Liquid xenon calorimeter for observation of cosmic line gamma-rays in the GeV region Liquid xenon calorimeter for observation of cosmic line gamma-rays in the GeV region

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nuphs..10..150d&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 10, Issue 2, p. 150-158.

Physics

Nuclear Physics

2

Scientific paper

A liquid xenon calorimeter designed on the basis of a new principle has been proposed to be used for observing cosmic line gamma-rays in the GeV region. This calorimeter has a geometric factor of 1 m2 sr or more, an energy resolution of the order of 0.1 % for GeV gamma-rays; and an angular resolution of about 1 degree. These characteristics satisfy most of the conditions theoretically required for observation of line gamma-rays produced by pair annihilation of heavy majorana fermions in the galactic halo.

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