A MAPS Based Micro-Vertex Detector for the STAR Experiment

For the 2014 heavy ion run of RHIC a new micro-vertex detector called the Heavy Flavor Tracker (HFT) was installed in the STAR experiment. The HFT consists of three detector subsystems with various silicon technologies arranged in 4 approximately concentric cylinders close to the STAR interaction point designed to improve the STAR detector's vertex resolution and extend its measurement capabilities in the heavy flavor domain. The two innermost HFT layers are placed at radii of 2.8 cm and 8 cm from the beam line. These layers are constructed with 400 high resolution sensors based on CMOS Monolithic Active Pixel Sensor (MAPS) technology arranged in 10-sensor ladders mounted on 10 thin carbon fiber sectors to cover a total silicon area of 0.16 m 2 . Each sensor of this PiXeL (\u201cPXL\u201d) sub-detector combines a pixel array of 928 rows and 960 columns with a 20.7 \u3bcm pixel pitch together with front-end electronics and zero-suppression circuitry in one silicon die providing a sensitive area of 3c3.8 cm 2 . This sensor architecture features 185.6 \u3bcs readout time and 170 mW/cm 2 power dissipation. This low power dissipation allows the PXL detector to be air-cooled, and with the sensors thinned down to 50 \u3bcm results in a global material budget of only 0.4% radiation length per layer. A novel mechanical approach to detector insertion allows us to effectively install and integrate the PXL sub-detector within a 12 hour period during an on-going multi-month data taking period. The detector requirements, architecture and design, as well as the performance after installation, are presented in this paper

STAR Vertex Detector Upgrade Development

We report on the development and prototyping efforts undertaken with the goal of producing a micro-vertex detector for the STAR experiment at the RHIC accelerator at BNL. We present the basic detector requirements and show a sensor development path, conceptual mechanical design candidates and readout architecture. Prototyping and beam test results with current generation MimoSTAR-2 sensors and a readout system featuring FPGA based on-the-fly hit finding and data sparsification are also presented

The STAR MAPS-based PiXeL detector

The PiXeL detector (PXL) for the Heavy Flavor Tracker (HFT) of the STAR experiment at RHIC is the first application of the state-of-the-art thin Monolithic Active Pixel Sensors (MAPS) technology in a collider environment. Custom built pixel sensors, their readout electronics and the detector mechanical structure are described in detail. Selected detector design aspects and production steps are presented. The detector operations during the three years of data taking (2014-2016) and the overall performance exceeding the design specifications are discussed in the conclusive sections of this paper

Small-Scale Readout Systems Prototype for the STAR PIXEL Detector

A prototype readout system for the STAR PIXEL detector in the Heavy Flavor Tracker (HFT) vertex detector upgrade is presented. The PIXEL detector is a Monolithic Active Pixel Sensor (MAPS) based silicon pixel vertex detector fabricated in a commercial CMOS process that integrates the detector and front-end electronics layers in one silicon die. Two generations ofMAPS prototypes designed specifically for the PIXEL are discussed. We have constructed a prototype telescope system consisting of three small MAPS sensors arranged in three parallel and coaxial planes with a readout system based on the readout architecture for PIXEL. This proposed readout architecture is simple and scales to the size required to readout the final detector. The real-time hit finding algorithm necessary for data rate reduction in the 400 million pixel detector is described, and aspects of the PIXEL system integration into the existing STAR framework are addressed. The complete system has been recently tested and shown to be fully functional

Potential of Core-Collapse Supernova Neutrino Detection at JUNO

JUNO is an underground neutrino observatory under construction in Jiangmen, China. It uses 20kton liquid scintillator as target, which enables it to detect supernova burst neutrinos of a large statistics for the next galactic core-collapse supernova (CCSN) and also pre-supernova neutrinos from the nearby CCSN progenitors. All flavors of supernova burst neutrinos can be detected by JUNO via several interaction channels, including inverse beta decay, elastic scattering on electron and proton, interactions on C12 nuclei, etc. This retains the possibility for JUNO to reconstruct the energy spectra of supernova burst neutrinos of all flavors. The real time monitoring systems based on FPGA and DAQ are under development in JUNO, which allow prompt alert and trigger-less data acquisition of CCSN events. The alert performances of both monitoring systems have been thoroughly studied using simulations. Moreover, once a CCSN is tagged, the system can give fast characterizations, such as directionality and light curve

Detection of the Diffuse Supernova Neutrino Background with JUNO

As an underground multi-purpose neutrino detector with 20 kton liquid scintillator, Jiangmen Underground Neutrino Observatory (JUNO) is competitive with and complementary to the water-Cherenkov detectors on the search for the diffuse supernova neutrino background (DSNB). Typical supernova models predict 2-4 events per year within the optimal observation window in the JUNO detector. The dominant background is from the neutral-current (NC) interaction of atmospheric neutrinos with 12C nuclei, which surpasses the DSNB by more than one order of magnitude. We evaluated the systematic uncertainty of NC background from the spread of a variety of data-driven models and further developed a method to determine NC background within 15\% with {\it{in}} {\it{situ}} measurements after ten years of running. Besides, the NC-like backgrounds can be effectively suppressed by the intrinsic pulse-shape discrimination (PSD) capabilities of liquid scintillators. In this talk, I will present in detail the improvements on NC background uncertainty evaluation, PSD discriminator development, and finally, the potential of DSNB sensitivity in JUNO

Real-time Monitoring for the Next Core-Collapse Supernova in JUNO

Core-collapse supernova (CCSN) is one of the most energetic astrophysical events in the Universe. The early and prompt detection of neutrinos before (pre-SN) and during the SN burst is a unique opportunity to realize the multi-messenger observation of the CCSN events. In this work, we describe the monitoring concept and present the sensitivity of the system to the pre-SN and SN neutrinos at the Jiangmen Underground Neutrino Observatory (JUNO), which is a 20 kton liquid scintillator detector under construction in South China. The real-time monitoring system is designed with both the prompt monitors on the electronic board and online monitors at the data acquisition stage, in order to ensure both the alert speed and alert coverage of progenitor stars. By assuming a false alert rate of 1 per year, this monitoring system can be sensitive to the pre-SN neutrinos up to the distance of about 1.6 (0.9) kpc and SN neutrinos up to about 370 (360) kpc for a progenitor mass of 30$M_{\odot}$ for the case of normal (inverted) mass ordering. The pointing ability of the CCSN is evaluated by using the accumulated event anisotropy of the inverse beta decay interactions from pre-SN or SN neutrinos, which, along with the early alert, can play important roles for the followup multi-messenger observations of the next Galactic or nearby extragalactic CCSN.Comment: 24 pages, 9 figure

Development of pixel detectors with integrated microcircuits for the vertex detector in the Star experiment at the RHIC collider

Ce travail contribue au programme de recherche et de développement des détecteurs monolithiques à pixels actifs (MAPS) pour la construction du prochain détecteur de vertex dans l'expérience STAR du collisionneur RHIC. Le détecteur à 135 million pixel, prévue pour 2011, augmentera le programme de physique grâce à sa résolution de pointage prévu du 30 m. La collaboration STAR développe ce détecteur dans la nouvelle technologie des MAPS qui fournit un capteur et l'e lectronique de lecture intégrée dans les processus standard de CMOS. Le travail présenté dans cette thèse, décrit la progression du développement des MAPS d'une simple architecture jusqu à des conceptions plus complexes qui intègrent le traitement des signaux sur le circuit. Une étude un amplificateur d'entrée intégré au niveau d'un pixel avec une consommation de puissance faible et à faible bruit, est présenté avec les résultats expérimentaux associés.L'intégration des capteurs MAPS au détecteur du vertex a été étudié dans ce travail avec un télescope de détecteurs composé de trois prototypes MAPS et un prototype du système de lecture. La réduction du débit des données d'un système portant sur plusieurs millions de pixels a été étudiée avec un algorithme trouvant dynamiquement les pixels touchés par le faisceau. L'opération du RHIC à une luminosité ultime exige des architectures plus avancées que la simple conception mise en application dans de premier prototype consacré à STAR. Dans ce travail les solutions présentées indiquent le chemin de développement pour les capteurs finaux avec une amplification du signal intégré dans les pixels et une numérisation des données sur le détecteur.This work is part of the Monolithic Active Pixel Sensor (MAPS) R&D program that is directed towards construction of a new, 135 million pixel vertex detector for the STAR experiment at the RHIC collider. The new detector is planned to be installed in 2011 to extend the current physics capabilities of the system by providing a pointing resolution of 30 m. The STAR collaboration is actively pursuing detector development in MAPS technology that offers thin monolithic detectors fabricated in standard CMOS processes. The work presented addresses the development of MAPS from basic architectures to simple integrated on-chip signal processing. A common element for most of the presented readout schemes is a compact low-noise, low power consumption, compact in-pixel amplifier. A review of possible solutions for this element together with experimental results is presented. MAPS operating in current mode have been investigated in this thesis as an alternative to the classical voltage mode. Integration of MAPS sensors in a complete detector system has been investigated with a prototype readout system coupled to a detector telescope composed from three MAPS prototypes. The optimization of the readout of a multi-million pixel detector has been addressed with a study of an "on-the-fly" cluster finding algorithm reducing the data rates. The operation of RHIC with increased luminosity will require more advanced pixel architectures than the simple design implemented in the first prototypes. The solutions presented indicate a development path for the final sensor with in-pixel signal amplification and on-chip data digitization

Small-Scale Readout System Prototype for the STAR PIXEL Detector

Development and prototyping efforts directed towards construction of a new vertex detector for the STAR experiment at the RHIC accelerator at BNL are presented. This new detector will extend the physics range of STAR by allowing for precision measurements of yields and spectra of particles containing heavy quarks. The innermost central part of the new detector is a high resolution pixel-type detector (PIXEL). PIXEL requirements are discussed as well as a conceptual mechanical design, a sensor development path, and a detector readout architecture. Selected progress with sensor prototypes dedicated to the PIXEL detector is summarized and the approach chosen for the readout system architecture validated in tests of hardware prototypes is discussed

Small-Scale Readout Systems Prototype for the STAR PIXEL Detector

A prototype readout system for the STAR PIXEL detector in the Heavy Flavor Tracker (HFT) vertex detector upgrade is presented. The PIXEL detector is a Monolithic Active Pixel Sensor (MAPS) based silicon pixel vertex detector fabricated in a commercial CMOS process that integrates the detector and front-end electronics layers in one silicon die. Two generations of MAPS prototypes designed specifically for the PIXEL are discussed. We have constructed a prototype telescope system consisting of three small MAPS sensors arranged in three parallel and coaxial planes with a readout system based on the readout architecture for PIXEL. This proposed readout architecture is simple and scales to the size required to readout the final detector. The real-time hit finding algorithm necessary for data rate reduction in the 400 million pixel detector is described, and aspects of the PIXEL system integration into the existing STAR framework are addressed. The complete system has been recently tested and shown to be fully functional