activity
20002018
most citedSearch for Kaluza-Klein Graviton Emission in Collisions at TeV using the Missing Energy Signature

29 citations · 102 across the 7 of their papers we have counts for

collaborators

7 papers

hep-ex2018★ 23 cited

A submission to the 2020 update of the European Strategy for Particle Physics on behalf of the COMET, MEG, Mu2e and Mu3e collaborations

A. Baldini, D. Glenzinski, F Kapusta +8

Charged-lepton flavour-violating (cLFV) processes offer deep probes for new physics with discovery sensitivity to a broad array of new physics models - SUSY, Higgs Doublets, Extra…

physics.ins-det2018★ 17 cited

Expression of Interest for Evolution of the Mu2e Experiment

F. Abusalma, D. Ambrose, A. Artikov +124

We propose an evolution of the Mu2e experiment, called Mu2e-II, that would leverage advances in detector technology and utilize the increased proton intensity provided by the Fermi…

hep-ex2004

Comparison of Three-jet Events in Proton-Antiproton Collisions at sqrt{s}=1.8 TeV to Predictions from a Next-to-leading Order QCD Calculation

Sally Seidel

The properties of three-jet events with total transverse energy greater than 320 GeV and individual jet energy greater than 20 GeV have been analyzed and compared to absolute predi…

hep-ex2003★ 29 cited

Search for Kaluza-Klein Graviton Emission in Collisions at TeV using the Missing Energy Signature

D. Acosta

We report on a search for direct Kaluza-Klein graviton production in a data sample of 84 of \ppb collisions at = 1.8 TeV, recorded by the Collider Detector a…

hep-ex2003★ 21 cited

Observation of Radiative Decay

The Belle Collaboration, O. Tajima

We report the observation of the decay with a statistical significance of in $78.1 \ifb$ of data collected by the Belle experiment at the KEKB colli…

astro-ph2003★ 12 cited

Keck Spectroscopy of 4 QSO Host Galaxies

J. S. Miller, A. I. Sheinis

We present optical spectroscopy of the host galaxies of 4 QSO's: PG1444+407, PKS 2349-147, 3C 323.1, and 4C 31.63 having a redshift range (0.1 < z < 0.3). The spectra were obtained…