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      Design of Prototype Front-end Digital Module for Direct Dark Matter Detection based on LAr

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          Abstract

          Liquid argon (LAr) with a high light yield of approximately 40 photons per keV is an attractive target for the direct detection of weakly interacting massive particles (WIMPs), which are well motivated galactic dark matter candidates. We studies a front-end electronics design for a LAr dark matter detector with the scintillation read out by PMT, which has an input dynamic range from 5pC to 1nC, and high resolution that single photoelectron can be distinguished. In this paper, we present the design of front-end digital module (FDM) which is the important portion of electronics. The prototype FDM is equipped with 14-bit 1-GSPS analog-to-digital converters (ADC), and the performance of prototype FDM had been test in lab (e.g. ENOB is 10.40 bits @298 MHz). Moreover, this prototype FDM had been tested with LAr detector collaboratively and test results are also presented.

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          Effect of ionization density on the time dependence of luminescence from liquid argon and xenon

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            Average energy expended per ion pair in liquid argon

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              Liquid Xenon Detectors for Particle Physics and Astrophysics

              This article reviews the progress made over the last 20 years in the development and applications of liquid xenon detectors in particle physics, astrophysics and medical imaging experiments. We begin with a summary of the fundamental properties of liquid xenon as radiation detection medium, in light of the most current theoretical and experimental information. After a brief introduction of the different type of liquid xenon detectors, we continue with a review of past, current and future experiments using liquid xenon to search for rare processes and to image radiation in space and in medicine. We will introduce each application with a brief survey of the underlying scientific motivation and experimental requirements, before reviewing the basic characteristics and expected performance of each experiment. Within this decade it appears likely that large volume liquid xenon detectors operated in different modes will contribute to answering some of the most fundamental questions in particle physics, astrophysics and cosmology, fulfilling the most demanding detection challenges. From experiments like MEG, currently the largest liquid xenon scintillation detector in operation, dedicated to the rare mu -> e + gamma decay, to the future XMASS which also exploits only liquid xenon scintillation to address an ambitious program of rare event searches, to the class of time projection chambers like XENON and EXO which exploit both scintillation and ionization of liquid xenon for dark matter and neutrinoless double beta decay, respectively, we anticipate unrivaled performance and important contributions to physics in the next few years.
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                Author and article information

                Journal
                24 June 2018
                Article
                1806.09253
                6dfa6666-7741-4d61-aa20-1d0884ec1d4d

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                3 pages, 8 figures, 21st IEEE Real Time Conference
                physics.ins-det

                Technical & Applied physics
                Technical & Applied physics

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