Robert

Johnson's work is in the areas of experimental particle physics and, recently, high-energy astrophysics. Before coming to UCSC he spent five years working at the CERN laboratory in Geneva, Switzerland on the ALEPH experiment at the Large Electron-Positron collider (LEP). After coming to UCSC he continued working on that experiment in collaboration with Prof. Alan Litke. The ALEPH experiment collected data from 1989 to 1995 at the energy of the Z resonance and since then has been collecting data above the threshold for production of W pairs. Members of the SCIPP group made important contributions to the installation, debugging, and operation of the Aleph silicon-strip vertex detector. They are now concentrating on exploiting that state-of-the-art device for physics analysis, both for studies of the production and decays of B hadrons at the Z resonance and for searches for new phenomena, such as the Higgs boson and supersymmetry, in the newer high-energy operation.

A more recent project concerns the design and construction of an experiment (BaBar) at the new B-Factory accelerator of the Stanford Linear Accelerator Center (SLAC). The B-Factory, which began running in 1999, will make detailed studies of CP violation in decays of B hadrons. Johnson was responsible for the design, prototyping, and testing of part of the fast, radiation-hard readout electronics of a silicon-strip vertex detector that is at the heart of this new detector. He worked in a collaboration of physicists and engineers from UCSC, LBNL, and INFN institutes in Pavia and Pisa to design a 128-channel CMOS VLSI chip to perform the amplification, discrimination, buffering, and data acquisition functions necessary for readout of the 150,000 channel detector. The SCIPP group is also responsible for the data transmission electronics of the BaBar vertex detector and for much of the software development needed for analysis of the data. This experiment is still operational and has published many measurements, including parameters of CP violation in the B system.

Johnson's principal current interest is a NASA/D.O.E. project, named GLAST, to build an orbiting gamma-ray telescope based on the silicon-strip technology in which SCIPP specializes. This second-generation device promises to deliver a two-order-of-magnitude improvement in sensitivity to astrophysical sources of high-energy gamma rays, compared with the current highly successful EGRET experiment on the Compton Gamma Ray Observatory. The project calls for about 900,000 silicon-strip channels operating on a power budget of less than two hundred watts. Johnson has concentrated on development of the low-power, low-noise readout electronics needed for this application. A CMOS VLSI chip set similar in concept to what was developed for the B-Factory was designed in the SCIPP lab, together with the necessary supporting electronics. Prototypes were extensively tested in a full-scale tracker module assembled in the SCIPP lab and operated in December 1999 and January 2000 in the SLAC test beam and in 2001 on a high-altitude balloon flight.

GLAST will provide vast amounts of data on gamma ray sources in our galaxy, such as pulsars, as well as on extra-galactic sources such as active galactic nuclei and the even more mysterious gamma-ray bursts. The GLAST mission will include a Large-Area Telescope (LAT) and a smaller Gamma-Ray Burst Monitor. The silicon-strip based instrument design was selected by NASA for the LAT instrument in March of 2000. Johnson is the manager for the design and fabrication of the silicon-strip tracker subsystem of the LAT, which also includes a CsI crystal calorimeter and a plastic-scintillator veto shield. The Critical Design Review for the Tracker subsystem was held in March of 2003, after which the collaboration (USA, Italy, Japan) engaged in manufacturing and assembly of the flight hardware. In addition to the management responsibilities, Johnson’s UCSC group was responsible for delivering the Tracker readout electronics, including 648 multi-chip modules, each with 1536 amplifier channels, and the flexible-circuit readout cables. The first tracker tower module was completed in January of 2005, and in October of 2005 the last of the 18 Tracker tower modules (including 2 spares) was completed and tested. Here you can find a view of the 16 flight Tracker modules mounted in the LAT, along with 16 calorimeter modules (not visible). The remainder of the instrument was completed in the winter of 2006, and in September of 2006 the LAT successfully completed its environmental testing at the Naval Research Laboratory and was ready to be integrated with the spacecraft (photo of the completed, tested instrument). The instrument is currently at General Dynamics in Arizona where it was integrated with the spacecraft (photo of the LAT and GBM NaI detectors on the spacecraft). The integrated observatory recently completed thermal-vacuum testing at the Naval Research Laboratory, and it is scheduled to launch into orbit in May of 2008.

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Links

· SCIPP Home Page

· Physics Home Page

· Astronomy and Astrophysics

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Selected Recent Publications

· M. Ziegler, B.M. Baughman, R.P. Johnson, W.B. Atwood, A Search for Radio Quiet Gamma-Ray Pulsars in EGRET Data Using a Time Differencing Technique, to be published in Ap.J.

· W. Atwood et al., Design and Initial Tests of the Tracker-Converter of the Gamma-ray Large Area Space Telescope, Astroparticle Physics 28, 422-434, 2007.

· W.B. Atwood, M. Ziegler, R.P. Johnson, B.M. Baughman, A Time Differencing Technique for Detecting Radio-Quiet Gamma-Ray Pulsars, Ap.J. 652, L49-L52, 2006.

· L. Baldini et al., Fabrication of the GLAST Silicon Tracker Readout Electronics, IEEE Trans. Nucl. Sci. 53, 3013-3020, 2006.

· L. Baldini et al., The Silicon Tracker Readout Electronics of the Gamma-Ray Large Area Space Telescope, IEEE Trans. Nucl. Sci. 53, 466, 2006.

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Last Revised: February 28, 2008