The CLEO III silicon tracker

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment Elsevier 386:1 (1997) 37-45

Authors:

I Shipsey, J Alexander, K Arndt, A Bean, C Bebek, R Boyd, G Brandenburg, J Cherwinka, C Darling, J Duboscq, J Fast, A Foland, P Hopman, KK Gan, Y Gao, H Kagan, R Kass, P Kim, D Miller, W Miller, N Menon, B Nemati, J Oliver, C Rush, P Skubic, MB Spencer, C Ward, M Yurko, M Zoeller

Building Models Of Gauge Mediated Supersymmetry Breaking Without A Messenger Sector

(1997)

Authors:

Nima Arkani-Hamed, John March-Russell, Hitoshi Murayama

Dynamics of evaporative cooling for Bose-Einstein condensation

Physical Review A - Atomic, Molecular, and Optical Physics 56:1 (1997) 560-569

Authors:

H Wu, E Arimondo, CJ Foot

Abstract:

We have simulated the evaporative cooling of a dilute gas of Bose particles including quantum statistics using a Monte Carlo method. This approach can model situations which are far away from quasiequilibrium such as occur during forced evaporative cooling. We have also simulated the dynamical formation of Bose-Einstein condensate for homogeneous and inhomogeneous Bose gases under the random-phase approximation. It was found that the rate of accumulation of Bose particles into low-energy states through collisions is increased by forced evaporation; and a macroscopic population at ground state can be reached at a time scale characterized by classical collision time for an inhomogeneous gas in a harmonic potential. We present the results of simulations for the evaporative cooling and formation of a Bose-Einstein condensate in one-, two-, and three-dimensional position cuts and energy cuts. © 1997 The American Physical Society.

Nonequilibrium evolution of a trapped Bose gas

Conference on Quantum Electronics and Laser Science (QELS) - Technical Digest Series 12 (1997) 28-29

Authors:

H Wu, E Arimondo, CJ Foot

Abstract:

An investigation focusing on the nonequilibrium evolution of a trapped Bose gas revealed that the formation of a Bose gas can be classified into three stages, namely: kinetic evolution; the formation of short range order; and the off-diagonal long-range order. Using a homogeneous gas consisting of sodium atoms. The evolution of non-Gaussian velocity distribution was observed. This indicates the accumulation of Bose particles at low energy states, but not necessarily the signature of the appearance of a macroscopic Bose-Einstein condensate. The condensate fraction will be very small when the ensemble of sodium atoms magnetically trapped in a harmonic potential is considered.

Search for neutrinoless [Formula presented] decays: [Formula presented] and [Formula presented]

Physical Review D - Particles, Fields, Gravitation and Cosmology 55:7 (1997) R3919-R3923

Authors:

KW Edwards, A Bellerive, R Janicek, DB MacFarlane, KW McLean, PM Patel, AJ Sadoff, R Ammar, P Baringer, A Bean, D Besson, D Coppage, C Darling, R Davis, N Hancock, S Kotov, I Kravchenko, N Kwak, S Anderson, Y Kubota, M Lattery, JJ O’Neill, S Patton, R Poling, T Riehle, V Savinov, A Smith, MS Alam, SB Athar, Z Ling, AH Mahmood, H Severini, S Timm, F Wappler, A Anastassov, S Blinov, JE Duboscq, D Fujino, R Fulton, KK Gan, T Hart, K Honscheid, H Kagan, R Kass, J Lee, MB Spencer, M Sung, A Undrus, R Wanke, A Wolf, MM Zoeller, B Nemati, SJ Richichi, WR Ross, P Skubic, M Wood, M Bishai, J Fast, E Gerndt, JW Hinson, N Menon, DH Miller, EI Shibata, IPJ Shipsey, M Yurko, L Gibbons, SD Johnson, Y Kwon, S Roberts, EH Thorndike, CP Jessop, K Lingel, H Marsiske, ML Perl, SF Schaffner, D Ugolini, R Wang, X Zhou, TE Coan, V Fadeyev, I Korolkov, Y Maravin, I Narsky, V Shelkov, J Staeck, R Stroynowski, I Volobouev, J Ye, M Artuso, A Efimov, F Frasconi, M Gao, M Goldberg, D He, S Kopp, GC Moneti, R Mountain, Y Mukhin, S Schuh, T Skwarnicki

Abstract:

A search for the lepton-family-number-violating decays [Formula presented] and [Formula presented] has been performed using CLEO II data. No evidence of a signal has been found and the corresponding upper limits are [Formula presented] and [Formula presented] at 90% C.L. © 1997 The American Physical Society.