Nuclear astrophysics studies at the LENA facility: The γ-ray detection system

Details Nuclear astrophysics studies at the LENA facility: The γ-ray detection system Nuclear astrophysics studies at the LENA facility: The γ-ray detection system

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006nimpa.566..452l&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 566, Issue 2, p. 452-464.

Physics

3

Scientific paper

The detection system of The Laboratory for Experimental Nuclear Astrophysics is described, including methods for measuring weak capture-γ-ray resonances. Improved γγ-coincidence techniques are detailed, as well as the reduction of cosmic muon-induced background in the energy region of E=0.6 9.0MeV by the use of compact cosmic muon anti-coincidence shields. These techniques reduced background count rates in the regions of E=0.6 3.0 and 3.0 9.0 MeV with respect to unshielded singles count rates by factors of 3600 and 21, respectively.

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