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Search for anisotropies in the underground cosmic-ray muon flux

Thesis/Dissertation ·
OSTI ID:6578548
Over the last decade, several very and ultra high energy gamma ray detectors (E > 0.5 TeV) have reported observations of air showers exhibiting hadronic characteristics from the direction of two binary systems, Cygnus X-3 and Hercules X-1. In addition, two underground detectors, NUSEX and Soudan, observed muon signals correlated with the 4.8 hour x-ray period of Cygnus X-3. Either effect, if substantiated, would imply the existence of either a previously undetected light, neutral hadron or an enhanced photon-nucleon interaction above center-of-mass energies of 100 GeV. From January 1985, until May 1987, the author has searched for enhancements in the underground muon flux with a liquid scintillation detector in the Homestake Gold Mine, Lead, South Dakota. A survey of the Northern sky yielded no evidence for a time independent point source. The upper limit on this flux was 1.0 {times} 10{sup {minus}11} cm{sup {minus}2} s{sup {minus}1}. No phase correlated or short term effect from the region about Cygnus X-3 was observed. The Homestake upper limit for the NUSEX active phase interval was 1.1 {times} 10{sup {minus}12} cm{sup {minus}2} s{sup {minus}1}. No signal was detected at the time of the Soudan muon burst coincident with the October, 1985 radio flare. He also observed no enhancement from the direction of Hercules X-1 (F < 5.4 {times} 10{sup {minus}12} cm{sup {minus}2} s{sup {minus}1}). Two other potential sources were examined. Thus an upper limit can be set on the number of Galactic sources of underground muon progenitors at (12/{epsilon}), where {epsilon} is the typical long term duty cycle of these sources.
Research Organization:
Pennsylvania Univ., Philadelphia, PA (USA)
OSTI ID:
6578548
Country of Publication:
United States
Language:
English