Thesis advisor: Professor David Koltick
Group leader: Nobel Laureate Martin Perl
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ATLAS is a general purpose detector for the study of pp collisions at 14 TeV center-of-mass energy using the LHC collider at CERN. The collider is the highest energy and luminosity collider in the world. One of the major physics goal of the collider is to discover the Higgs, the particle responsible for generating mass of all particles. We are part of the pixel detector group. The pixel detector is the tracking device closest to the interaction region and is designed to improve the charged particle tracking and identification of b quarks in hadronic jets, critical for the Higgs search.
The extreme high energy of the LHC allows us to look for physics beyond the Standard Model. Lepton signatures have been used in the past for several major discoveries. The OSU groups therefore concentrate on using leptons as a tool in the searches for new physics, including the use of W and Z reconstructed in the leptonic decay modes. We can't list the ongoing searches publicly. However, we can provide links to two published analyses that we participated, study of WZ and ZZ productions.
The ATLAS pixel detector consists of three barrel layers and three forward and backward disks. The primary contribution of the OSU group is in the R&D, design, fabrication, and maintenance of the on-detector radiation-hard and high-speed optical communication. We built the fiber optic transceiver boards (opto-board) for the optical links. Each board contains both optical and electrical components, VCSELs, PINs, DORICs, and VDCs. The differential hit signal (LVDS) from the pixel electronics is converted by the VCSEL Driver Chip (VDC) on a board into a single-ended signal appropriate to drive a Vertical Cavity Surface Emitting Laser (VCSEL) and transmitted to the readout system using a fibre. The 40-MHz beam-crossing clock, encoded with the command signal to control the pixel electronics, is transmitted to a PIN diode via a fibre. The signal from the PIN diode is decoded using a Digital Opto-Receiver Integrated Circuit, DORIC. We use VCSEL and PIN diodes that are fabricated in the highly compact array and each array couples to a fibre ribbon inside an optical package (opto-pack). An opto-board contains one 8-channel PIN array opto-pack and one or two 8-channel VCSEL array opto-packs couple to two 4-channel DORICs and two or four 4-channel VDCs. OSU responsibilities include the design and testing of the radiation-hard VDC and DORIC, and the design, fabrication, and testing of opto-boards. The research is performed in collaboration with Siegen and Academic Sinica (Taiwan). The opto-board assembly document is available at here.
ATLAS plans to add a new pixel layer to the pixel detector in 2013. We propose to continue the use of the VCSEL and PIN arrays for this new generation of opto-links. In addition, we are developing an updated version of the chips in the 130 nm CMOS process with redundancy to bypass a broken PIN or VCSEL channel. For the so-called high luminosity LHC (HL-LHC) upgrade in 2020, we propose the continue use of the optical arrays for three reasons, compact, efficient, and robust, which we much appreciate after 10 years of experience in using the devices. The upgrade will take advantage of the work done by the GBT and VL projects at CERN. In collaboration with Siegen and NIKHEF, we are conducting R&D to enable such deployment.
OSU has perhaps the best equipped optical electronics lab for high energy physics research in US. The lab includes two automatic wire bonders (K&S 1470 and 8060), two manual wire bonders, wire-bond pull tester, dice probe station, high speed scope (6 GHz/20 GS/s), optical spectrum analyzer (OSA), optical comparator, precision vision measuring machine, fiber polisher and fusion splicer, high power UV light, precision scale (0.1 mg), high resolution IR camera, one humidity chamber, and two environmental chambers and ovens. The equipment are funded in part by a Major Research Instrumentation (MRI) grant of NSF. They are housed in the clean room and the adjacent staging room of the new physics building.
More technical information is available at Amir Rahimi, Jason Moore, and Shane Smith web sites.
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