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Title: Experimental search for a time-modulated muon flux from the direction of Cygnus X-3

Thesis/Dissertation ·
OSTI ID:6896501

Two underground experiments have recently reported detection of an anomalously large muon flux from the direction of the binary X-ray source cygnus X-3, with the 4.8-hour period characteristic of this source. A muon flux of the claimed magnitude, combined with constraints from surface observations, is inconsistent with the production of these muons by photons from Cygnus X-3 in normal air showers. This flux would require either unexpected photon interactions at very high energy (>5 TeV)( or a new type of neutral particle in the flux from Cygnus X-3. This thesis documents measurements with the HPW (Harvard-Purdue-Wisconsin) large underground water Cerenkov detector which do not confirm the claimed muon flux. The author places an upper limit on the flux of time-modulated muons from the direction of Cygnus X-3 of 5 x 10/sup -11/ muons-cm/sup -2/sec/sup -1/ at a vertical depth of 1450 MWE meters of water equivalent, with 90% confidence. This upper limit may be compared with the flux of 7 x 10/sup -11/ muons-cm/sup 2/sec/sup -1/ at a vertical depth of 1800 MWE which was claimed by another experiment. The HPW measurements are consistent with no anomalous muon flux from Cygnus X-3.

Research Organization:
Harvard Univ., Boston, MA (USA)
OSTI ID:
6896501
Resource Relation:
Other Information: Thesis (Ph. D.)
Country of Publication:
United States
Language:
English