Silicon Data Acquisition and Front-End Electronics

A highly integrated Front-End readout and Data Acquisition scheme for Silicon trackers is presented. In this context, a 16-channel readout chip for Silicon strips detector has been designed in 180nm CMOS technology, having in view a highly multiplexed and sparsified readout global strategy. First results are presented

Front-End and Readout Electronics for Silicon Trackers at the ILC

A highly integrated readout scheme for Silicon trackers making use of Deep Sub-Micron CMOS electronics is presented. In this context,a 16-channel readout chip for Silicon strips detector has been designed in 180nm CMOS technology, each channel comprising a low noise amplifier, a pulse shaper, a sample and hold and a comparator. First results are presented

Development of a sampling ASIC for fast detector signals

International audienceIn the context of the Large Area Picosecond Photodetector (LAPPD) pro ject the motivation to measure time-of-flight at the picosecond reso- lution has pushed towards a faster signal rise-time (below 100 ps) and a higher bandwidth output (higher than 1 GHz) detector, thus, leading to a new signal development and integrity studies of Micro-Channel Plates (MCP) photo-detectors. Similarly, the signal path, is being simulated and characterized, from the anodes to the input of the readout electronics, to minimise losses. Furthermore, to acquire the detector fast pulses a new 10 Gs/s high input bandwidth, 130 nm CMOS sampling chip is being de- veloped

Front-end Electronics for Silicon Trackers readout in Deep Sub-Micron CMOS Technology: The case of Silicon strips at the ILC

For the years to come, Silicon strips detectors will be read using the smallest available integrated technologies for room, transparency, and power considerations. CMOS, Bipolar- CMOS and Silicon-Germanium are presently offered in deepsubmicron (250 down to 90nm) at affordable cost through worldwide integrated circuits multiproject centers. As an example, a 180nm CMOS readout prototype chip has been designed and tested, and gave satisfactory results in terms of noise and power. Beam tests are under work, and prospectives in 130nm will be presented

A CMOS 130nm Evaluation digitzer chip for silicon strips readout

A CMOS 130nm evaluation chip intended to read Silicon strip detectors at the ILC has been designed and successfully tested. Optimized for a detector capacitance of 10 pF, it includes four channels of charge integration, pulse shaping, a 16-deep analogue sampler triggered on input analogue sums, and parallel analogue to digital conversion. Tests results of the full chain are reported, demonstrating the behaviour and performance of the full sampling process and analogue to digital conversion. Each channel dissipates less than one milli-Watt static power

Design of the Front-End Readout Electronics for ATLAS Tile Calorimeter at the sLHC

Abstract-We present a detailed upgrade design of the analog front-end electronics for the ATLAS Tile Calorimeter (TileCal) at the sLHC. Here we use the latest commercial off-the-shelf (COTS) components. We believe that with the latest technology based COTS devices, significant improvements in radiation tolerance are possible. The front-end analog electronics provides 17-bit dynamic range for readout of the PMT signals. Each PMT signal is processed with a 7-pole passive LC shaper, followed by a pair of bi-gain amplifiers and two 40 Msps sampling ADCs. The readout system is capable of measuring energy deposition from 220 MeV to 1.3 TeV in a single calorimeter cell and providing input to a fully digital Level-1 trigger. Other on-board features include a slow current integrator used for detector calibration with a cesium source to normalize the PMT gains and charge injectors for calibrating linearity and dynamic range of the readout electronics. A total of 10, 000 upgraded readout channels are needed to replace the current system at the LHC

Search for microwave emission from ultrahigh energy cosmic rays

We present a search for microwave emission from air showers induced by ultrahigh energy cosmic rays with the microwave detection of air showers experiment. No events were found, ruling out a wide range of power flux and coherence of the putative emission, including those suggested by recent laboratory measurements.Comment: 5 pages, 3 figure

Long-Lived Neutralino NLSPs

We investigate the collider signatures of heavy, long-lived, neutral particles that decay to charged particles plus missing energy. Specifically, we focus on the case of a neutralino NLSP decaying to Z and gravitino within the context of General Gauge Mediation. We show that a combination of searches using the inner detector and the muon spectrometer yields a wide range of potential early LHC discoveries for NLSP lifetimes ranging from 10^(-1)-10^5 mm. We further show that events from Z(l+l-) can be used for detailed kinematic reconstruction, leading to accurate determinations of the neutralino mass and lifetime. In particular, we examine the prospects for detailed event study at ATLAS using the ECAL (making use of its timing and pointing capabilities) together with the TRT, or using the muon spectrometer alone. Finally, we also demonstrate that there is a region in parameter space where the Tevatron could potentially discover new physics in the delayed Z(l+l-)+MET channel. While our discussion centers on gauge mediation, many of the results apply to any scenario with a long-lived neutral particle decaying to charged particles.Comment: 31 pages, 12 figure

Weak Lensing from Space I: Instrumentation and Survey Strategy

A wide field space-based imaging telescope is necessary to fully exploit the technique of observing dark matter via weak gravitational lensing. This first paper in a three part series outlines the survey strategies and relevant instrumental parameters for such a mission. As a concrete example of hardware design, we consider the proposed Supernova/Acceleration Probe (SNAP). Using SNAP engineering models, we quantify the major contributions to this telescope's Point Spread Function (PSF). These PSF contributions are relevant to any similar wide field space telescope. We further show that the PSF of SNAP or a similar telescope will be smaller than current ground-based PSFs, and more isotropic and stable over time than the PSF of the Hubble Space Telescope. We outline survey strategies for two different regimes - a ``wide'' 300 square degree survey and a ``deep'' 15 square degree survey that will accomplish various weak lensing goals including statistical studies and dark matter mapping.Comment: 25 pages, 8 figures, 1 table, replaced with Published Versio