Neutron flux generated by cosmic-ray muons at 5200 hg/sq CM s.r. underground - Depth-neutron intensity curve

Details Neutron flux generated by cosmic-ray muons at 5200 hg/sq CM s.r. underground - Depth-neutron intensity curve Neutron flux generated by cosmic-ray muons at 5200 hg/sq CM s.r. underground - Depth-neutron intensity curve

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ncimc..12..467a&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 12 C, July-Aug. 1989, p. 467-477.

Physics

25

Cosmic Rays, Muons, Neutron Flux Density, Neutron Counters, Scintillation Counters, Temporal Distribution

Scientific paper

Neutrons induced by cosmic-ray muons are an important source of background for the new, huge underground detectors. Their characteristics (multiplicity and time distribution) are investigated by using the data recorded from December 1985 to February 1988 using the 90-ton liquid scintillator detector of the Mont Blanc Laboratory. The experimental results on the mean number of neutrons produced by a muon per g/sq cm, being 385 GeV, are found to be in good agreement with an expected distribution given by the theoretical power law (mean Nn = mean Emu exp 0.75.

Affiliated with

Also associated with

No associations

Rating

Neutron flux generated by cosmic-ray muons at 5200 hg/sq CM s.r. underground - Depth-neutron intensity curve does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Neutron flux generated by cosmic-ray muons at 5200 hg/sq CM s.r. underground - Depth-neutron intensity curve, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutron flux generated by cosmic-ray muons at 5200 hg/sq CM s.r. underground - Depth-neutron intensity curve will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1520370