Search for new particles decaying into b¯b and produced in association with w bosons decaying into eν or μν at the fermilab tevatron
Physical Review Letters 79:20 (1997) 3819-3824
Abstract:
We search for new particles that decay into b¯b and are produced with W bosons in p¯p collisions at √s = 1.8TeV. The search uses 109 ± 7pb-1 accumulated by the CDF experiment at Fermilab. We select events with an eν or μν, and two jets, one of them b tagged. The number of events and the two-jet mass distribution are consistent with expectations. Using W+Higgs production as a model for the acceptance, we set an upper limit on the production cross section times branching ratio for the new particle ranging from 14 to 19 pb (95% C.L.) as the particle mass varies from 70 to 120GeV/c2. © 1997 The American Physical Society.Search for the decay [Formula presented]
Physical Review D - Particles, Fields, Gravitation and Cosmology 56:9 (1997) R5297-R5300
Abstract:
We have searched for the decay of the [Formula presented] lepton into seven charged particles and zero or one [Formula presented]. The data used in the search were collected with the CLEO II detector at the Cornell Electron Storage Ring (CESR) and correspond to an integrated luminosity of 4.61 [Formula presented]. No evidence for a signal is found. Assuming all the charged particles are pions, we set an upper limit on the branching fraction [Formula presented] at the 90% confidence level. This limit represents a significant improvement over the previous limit. © 1997 The American Physical Society.Status of construction and first tests of the CLEO III RICH
2011 IEEE Nuclear Science Symposium Conference Record Institute of Electrical and Electronics Engineers (IEEE) 1 (1997) 348-352 vol.1
Study of flavor-tagged baryon production in B decay
Physical Review D American Physical Society (APS) 55:1 (1997) 13-18
Study of gluon versus quark fragmentation in [Formula presented] and [Formula presented] events at [Formula presented]=10 GeV
Physical Review D - Particles, Fields, Gravitation and Cosmology 56:1 (1997) 17-22