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Author Correction: Proton acceleration in thermonuclear nova explosions revealed by gamma rays

Nature Astronomy 2022年 760页

作者： V. A. Acciari J. Becerra González E. Colombo R. J. García López J. Herrera A. López-Oramas C. Maggio V. Moreno M. Nievas Rosillo J. Otero-Santos G. Vanzo M. Vazquez Acosta S. Ansoldi B. De Lotto A. Donini F. Longo D. Miceli M. Palatiello M. Persic L. A. Antonelli C. Bigongiari S. Covino V. D’Elia F. Dazzi A. Lamastra F. Leone S. Lombardi L. Maraschi L. Nava S. Paiano C. Righi F. G. Saturni A. Stamerra F. Tavecchio A. Tutone A. Biland S. Fukami M. Artero O. Blanch S. M. Colak M. Delfino J. Delgado E. Do Souto Espiñeira L. Fariña Alonso L. Jouvin D. Kerszberg M. Martínez A. Moralejo E. Moretti C. Nigro C. Priyadarshi J. Rico K. Asano D. Hadasch M. Hütten T. Inada Y. Iwamura Y. Kobayashi D. Mazin K. Noda Y. Ohtani T. Saito S. Sakurai J. Sitarek M. Strzys M. Takahashi R. Takeishi M. Teshima I. Vovk D. Baack H. Bökenkamp D. Elsaesser A. Fattorini L. Linhoff S. Mender W. Rhode K. Schmidt A. Babić Ž. Bošnjak S. Cikota A. Baquero J. A. Barrio J. L. Contreras M. V. Fonseca J. Hoang M. López-Moya A. Mas Aguilar T. Miener D. Morcuende P. Peñil U. Barres de Almeida B. Machado de Oliveira Fraga I. Batković M. Bernardos G. Busetto A. De Angelis M. Doro R. López-Coto M. Mallamaci M. Mariotti E. Prandini A. Spolon W. Bednarek P. Gliwny K. Ishio D. Sobczynska L. Bellizzi S. Menchiari J. M. Miranda R. Paoletti S. Truzzi S. Ventura C. Wunderlich E. Bernardini W. Bhattacharyya M. Garczarczyk K. Satalecka A. Arbet Engels A. Berti J. Besenrieder G. Ceribella Y. Chai G. D’Amico C. Fruck J. G. Green D. Green A. Hahn L. Heckmann R. Mirzoyan D. Paneque M. Pihet T. Schweizer D. Strom J. van Scherpenberg M. Will G. Bonnoli R. Carosi P. Da Vela P. G. Prada Moroni A. Rugliancich M. Cerruti E. Molina J. M. Paredes M. Ribó A. Chilingarian J. Cortina C. Delgado Mendez T. Hassan I. Jiménez Martínez A. Del Popolo D. Depaoli F. Di Pierro C. F. Vigorito L. Di Venere N. Giglietto F. Giordano S. Loporchio D. Dominis Prester M. Manganaro S. Mićanović L. Pavletić T. Terzić D. Dorner K. Mannheim B. Schleicher V. Fallah Ramazani J. Jormanainen E. Lindfors Instituto de Astrofísica de Canarias and Dpto. de Astrofísica Universidad de La Laguna La Laguna Tenerife Spain Departament de Física and CERES-IEEC Universitat Autònoma de Barcelona Bellaterra Spain Università di Udine and INFN Trieste Udine Italy International Center for Relativistic Astrophysics (ICRA) Rome Italy Dipartimento di Fisica Università di Trieste Trieste Italy Laboratoire d’Annecy de Physique des Particules (LAPP) CNRS-IN2P3 Annecy Cedex France INAF Trieste and Dept. of Physics and Astronomy University of Bologna Bologna Italy National Institute for Astrophysics (INAF) Rome Italy ETH Zürich Zürich Switzerland Institut de Física d’Altes Energies (IFAE) The Barcelona Institute of Science and Technology (BIST) Bellaterra Barcelona Spain Port d’Informació Científica (PIC) Bellaterra Barcelona Spain Japanese MAGIC Group: Institute for Cosmic Ray Research (ICRR) The University of Tokyo Kashiwa Chiba Japan Max-Planck-Institut für Physik München Germany Technische Universität Dortmund Dortmund Germany Croatian MAGIC Group: University of Zagreb Faculty of Electrical Engineering and Computing (FER) Zagreb Croatia IPARCOS Institute and EMFTEL Department Universidad Complutense de Madrid Madrid Spain Department of Astronomy University of California Berkeley Berkeley CA USA Centro Brasileiro de Pesquisas Físicas (CBPF) Rio de Janeiro RJ Brazil Università di Padova and INFN Padova Italy University of Lodz Faculty of Physics and Applied Informatics Department of Astrophysics Lodz Poland Università di Siena and INFN Pisa Siena Italy Deutsches Elektronen-Synchrotron (DESY) Zeuthen Germany Department for Physics and Technology University of Bergen Bergen Norway Instituto de Astrofísica de Andalucía-CSIC Glorieta de la Astronomía s/n Granada Spain Università di Pisa and INFN Pisa Pisa Italy University of Innsbruck Innsbruck Austria Universitat de Barcelona ICCUB IEEC-UB Barcelona Spain Armenian MAGIC Group: A. Alikhanyan National Science Labo

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Search for Gravitational Waves Associated with Fast Radio Bursts Detected by CHIME/FRB during the LIGO-Virgo Observing Run O3a

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Astrophysical Journal 2023年第2期955卷 155-155页

作者： Abbott, R. Abbott, T.D. Acernese, F. Ackley, K. Adams, C. Adhikari, N. Adhikari, R.X. Adya, V.B. Affeldt, C. Agarwal, D. Agathos, M. Agatsuma, K. Aggarwal, N. Aguiar, O.D. Aiello, L. Ain, A. Ajith, P. Akutsu, T. Albanesi, S. Allocca, A. Altin, P.A. Amato, A. Anand, C. Anand, S. Ananyeva, A. Anderson, S.B. Anderson, W.G. Ando, M. Andrade, T. Andres, N. Andrić, T. Angelova, S.V. Ansoldi, S. Antelis, J.M. Antier, S. Appert, S. Arai, Koya Arai, Y. Araki, S. Araya, A. Araya, M.C. Areeda, J.S. Arène, M. Aritomi, N. Arnaud, N. Aronson, S.M. Arun, K.G. Asada, H. Asali, Y. Ashton, G. Aso, Y. Assiduo, M. Aston, S.M. Astone, P. Aubin, F. Austin, C. Babak, S. Badaracco, F. Bader, M.K.M. Badger, C. Bae, S. Bae, Y. Baer, A.M. Bagnasco, S. Bai, Y. Baiotti, L. Baird, J. Bajpai, R. Ball, M. Ballardin, G. Ballmer, S.W. Balsamo, A. Baltus, G. Banagiri, S. Bankar, D. Barayoga, J.C. Barbieri, C. Barish, B.C. Barker, D. Barneo, P. Barone, F. Barr, B. Barsotti, L. Barsuglia, M. Barta, D. Bartlett, J. Barton, M.A. Bartos, I. Bassiri, R. Basti, A. Bawaj, M. Bayley, J.C. Baylor, A.C. Bazzan, M. Bécsy, B. Bedakihale, V.M. Bejger, M. Belahcene, I. Benedetto, V. Beniwal, D. Bennett, T.F. Bentley, J.D. BenYaala, M. Bergamin, F. Berger, B.K. Bernuzzi, S. Berry, C.P.L. Bersanetti, D. Bertolini, A. Betzwieser, J. Beveridge, D. Bhandare, R. Bhardwaj, U. Bhattacharjee, D. Bhaumik, S. Bilenko, I.A. Billingsley, G. Bini, S. Birney, R. Birnholtz, O. Biscans, S. Bischi, M. Biscoveanu, S. Bisht, A. Biswas, B. Bitossi, M. Bizouard, M.-A. Blackburn, J.K. Blair, C.D. Blair, D.G. Blair, R.M. Bobba, F. Bode, N. Boer, M. Bogaert, G. Boldrini, M. Bonavena, L.D. Bondu, F. Bonilla, E. Bonnand, R. Booker, P. Boom, B.A. Bork, R. Boschi, V. Bose, N. Bose, S. Bossilkov, V. Boudart, V. Bouffanais, Y. Boumerdassi, A. Bozzi, A. Bradaschia, C. Brady, P.R. Bramley, A. Branch, A. Branchesi, M. Brau, J.E. Breschi, M. Briant, T. Briggs, J.H. Brillet, A. Brinkmann, M. Brockill, P. Brooks, A.F. Brooks, J. Brown, D.D. Brunett, S. Bruno, G. Bruntz, R. Bryant, J. Buchanan, J. B LIGO Laboratory California Institute of Technology Pasadena 91125 CA United States Louisiana State University Baton Rouge 70803 LA United States Dipartimento di Farmacia Università di Salerno Fisciano Salerno I-84084 Italy INFN Sezione di Napoli Complesso Universitario di Monte S. Angelo Napoli I-80126 Italy OzGrav School of Physics & Astronomy Monash University Clayton 3800 VIC Australia LIGO Livingston Observatory Livingston 70754 LA United States University of Wisconsin-Milwaukee Milwaukee 53201 WI United States OzGrav Australian National University Canberra 0200 ACT Australia Max Planck Institute for Gravitational Physics (Albert Einstein Institute) Hannover D-30167 Germany Leibniz Universität Hannover Hannover D-30167 Germany Inter-University Centre for Astronomy and Astrophysics Pune 411007 India University of Cambridge Cambridge CB2 1TN United Kingdom Theoretisch-Physikalisches Institut Friedrich-Schiller-Universität Jena Jena D-07743 Germany University of Birmingham Birmingham B15 2TT United Kingdom Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA) Northwestern University Evanston 60208 IL United States Instituto Nacional de Pesquisas Espaciais São Paulo São José dos Campos 12227-010 Brazil Gravity Exploration Institute Cardiff University Cardiff CF24 3AA United Kingdom INFN Sezione di Pisa Pisa I-56127 Italy International Centre for Theoretical Sciences Tata Institute of Fundamental Research Bengaluru 560089 India Gravitational Wave Science Project National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan Advanced Technology Center National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan INFN Sezione di Torino Torino I-10125 Italy Università di Napoli “Federico II Complesso Universitario di Monte S. Angelo Napoli I-80126 Italy Université de Lyon Université Claude Bernard Lyon 1 CNRS Institut Lumière Matière Villeurbanne F-69622

We search for gravitational-wave (GW) transients associated with fast radio bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst Project, during the first part of the third observing run of Advanced LIGO and Advanced Virgo (2019 April 1 15:00 UTC-2019 October 1 15:00 UTC). Triggers from 22 FRBs were analyzed with a search that targets both binary neutron star (BNS) and neutron star-black hole (NSBH) mergers. A targeted search for generic GW transients was conducted on 40 FRBs. We find no significant evidence for a GW association in either search. Given the large uncertainties in the distances of our FRB sample, we are unable to exclude the possibility of a GW association. Assessing the volumetric event rates of both FRB and binary mergers, an association is limited to 15% of the FRB population for BNS mergers or 1% for NSBH mergers. We report 90% confidence lower bounds on the distance to each FRB for a range of GW progenitor models and set upper limits on the energy emitted through GWs for a range of emission scenarios. We find values of order 10⁵¹-10⁵⁷ erg for models with central GW frequencies in the range 70-3560 Hz. At the sensitivity of this search, we find these limits to be above the predicted GW emissions for the models considered. We also find no significant coincident detection of GWs with the repeater, FRB 20200120E, which is the closest known extragalactic FRB. © 2023. The Author(s). Published by the American Astronomical Society.

关键词： Gravitational wave astronomy Radio transient sources

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Hybrid Monte Carlo and continuum modeling of electrolytes with concentration-induced dielectric variations

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Physical Review E 2016年第5期94卷 053312-053312页

作者： Xiaofei Guan Manman Ma Zecheng Gan Zhenli Xu Bo Li School of Mathematical Sciences Tongji University 1239 Siping Road Shanghai 200092 China School of Mathematical Sciences and Institute of Natural Sciences Shanghai Jiao Tong University Shanghai 200240 China Department of Mathematics University of Michigan Ann Arbor Michigan 48109 USA School of Mathematical Sciences Institute of Natural Sciences and MoE Key Lab of Scientific and Engineering Computing Shanghai Jiao Tong University Shanghai 200240 China Department of Mathematics and Graduate Program in Quantitative Biology University of California San Diego California 92093-0112 USA

The distribution of ions near a charged surface is an important quantity in many biological and material processes, and has been therefore investigated intensively. However, few theoretical and simulation approaches have included the influence of concentration-induced variations in the local dielectric permittivity of an underlying electrolyte solution. Such local variations have long been observed and known to affect the properties of ionic solution in the bulk and around the charged surface. We propose a hybrid computational model that combines Monte Carlo simulations with continuum electrostatic modeling to investigate such properties. A key component in our hybrid model is a semianalytical formula for the ion-ion interaction energy in a dielectrically inhomogeneous environment. This formula is obtained by solving for the Green's function Poisson's equation with ionic-concentration-dependent dielectric permittivity using a harmonic interpolation method and spherical harmonic series. We also construct a self-consistent continuum model of electrostatics to describe the effect of ionic-concentration-dependent dielectric permittivity and the resulting self-energy contribution. With extensive numerical simulations, we verify the convergence of our hybrid simulation scheme, show the qualitatively different structures of ionic distribution due to the concentration-induced dielectric variations, and compare our simulation results with the self-consistent continuum model. In particular, we study the differences between weakly and strongly charged surfaces and multivalencies of counterions. Our hybrid simulations conform particularly the depletion of ionic concentrations near a charged surface and also capture the charge inversion. We discuss several issues and possible further improvement of our approach for simulations of large charged systems.

关键词： Charge Dielectric properties Colloids Green's function methods Monte Carlo methods

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Floating-Point Adaptive Filter Architectures for the Cancelling of Harmonics Power Line Interference

Floating-Point Adaptive Filter Architectures for the Cancell...

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IEEE International Conference on Electronics, Circuits, and Systems

作者： Vagner Guidotti Eduardo Costa Sergio Almeida Mateus Fonseca Graduate Program on Electronic Engineering and Computing - Catholic University of Pelotas (UCPel) Engineering Center - Federal University of Pelotas (UFPel)

ISBN: (纸本)9781509002474

This work presents floating-point dedicated architectures of LMS (Least Mean Square) and NLMS (Normalized Least Mean Square) adaptive filtering algorithms for the harmonics power line interference cancelling. Among the various algorithms of adaptation, the (LMS is surely the most popular, mainly due to its low computational cost, robustness and tracking ability. On the other hand, the normalized version of the LMS algorithm, named NLMS presents as main characteristics the increase of speed of adaptation and small sensitivity to the power reference signal. This work explores these tradeoffs by developing floating-point dedicated architectures for both algorithms, and applying them to the harmonics cancelling structure. The developed architectures were described in hardware description language, and synthesized to 45 nm Nangate Open Cell using Cadence RTL Compiler. The main results show that the interference canceller with NLMS filters presents faster convergence at the cost of an increased area and power consumption as compared with the structure with LMS filters.

关键词： LMS NLMS Harmonics cancelling Power consumption

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Galactic transient sources with the Cherenkov Telescope Array Observatory

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Monthly Notices of the Royal Astronomical Society 2025年第1期540卷 205–238页

作者： Abe, K Abe, S Abhir, J Abhishek, A Acero, F Acharyya, A Adam, R Aguasca-Cabot, A Agudo, I Aguirre-Santaella, A Alfaro, J Alfaro, R Alvarez-Crespo, N Alves Batista, R Amans, J-P Amato, E Ambrosi, G Ambrosino, F Angüner, E O Antonelli, L A Aramo, C Arcaro, C Arnesen, T T H Asano, K Ascasibar, Y Aschersleben, J Ashkar, H Augusto Stuani, L Baack, D Backes, M Balazs, C Balbo, M Baquero Larriva, A Barbosa Martins, V Barres de Almeida, U Barrio, J A Barrios-Jiménez, L Batković, I Batzofin, R Baxter, J Becerra González, J Becker Tjus, J Belmont, R Benbow, W Bernete, J Bernlöhr, K Berti, A Bertucci, B Beshley, V Bhattacharjee, P Bhattacharyya, S Bigongiari, C Bissaldi, E Blanch, O Blazek, J Bocchino, F Boisson, C Bolmont, J Bonnoli, G Bonollo, A Bordas, P Bosnjak, Z Bottacini, E Böttcher, M Bradascio, F Bronzini, E Brown, A M Brunelli, G Bulgarelli, A Burelli, I Burger-Scheidlin, C Burmistrov, L Burton, M Buscemi, M Cailleux, J Campoy-Ordaz, A Cantlay, B K Capasso, G Caproni, A Capuzzo-Dolcetta, R Caraveo, P Caroff, S Carosi, A Carosi, R Carquin, E Carrasco, M-S Cascone, E Cassol, F Castaldini, L Castrejon, N Castro-Tirado, A J Cerasole, D Ceribella, G Cerruti, M Chadwick, P M Chaty, S Chen, A W Chernyakova, M Chiavassa, A Chudoba, J Chytka, L Cicciari, G M Cifuentes, A Coimbra Araujo, C H Colapietro, M Conforti, V Contreras, J L Cortina, J Costa, A Costantini, H Cotter, G Cristofari, P Cuevas, O Curtis-Ginsberg, Z D’Aì, A D’Amico, G D’Ammando, F Dai, S Dazzi, F de Bony de Lavergne, M De Caprio, V De Cesare, G De Frondat Laadim, F de Gouveia Dal Pino, E M De Lotto, B De Lucia, M de Martino, D de Menezes, R de Naurois, M de Ona Wilhelmi, E de Souza, V del Peral, L del Valle, M V Delgado, C Dell’aiera, M Della Valle, M della Volpe, D Depaoli, D Devin, J Di Girolamo, T Di Piano, A Di Pierro, F Di Tria, R Di Venere, L Diebold, S Dignam, C Dima, R Dinesh, A Djuvsland, J Dominik, R M Dominis Prester, D Donini, A Dorner, D Dörner, J Doro, M Dubos, C Ducci, L Dwarkadas, V V Ebr, J Eckner, C Egberts, K Einecke, S Elsässer, D Emery Department of Physics Tokai University 4-1-1 Kita-Kaname Hiratsuka Kanagawa 259-1292 Japan Institute for Cosmic Ray Research University of Tokyo 5-1-5 Kashiwa-no-ha Kashiwa Chiba 277-8582 Japan ETH Zürich Institute for Particle Physics and Astrophysics Otto-Stern-Weg 5 CH-8093 Zürich Switzerland INFN and Università degli Studi di Siena Dipartimento di Scienze Fisiche della Terra e dell’Ambiente (DSFTA) Sezione di Fisica Via Roma 56 I-53100 Siena Italy Université Paris-Saclay Université Paris Cité CEA CNRS AIM F-91191 Gif-sur-Yvette Cedex France FSLAC IRL 2009 CNRS/IAC E-38205 La Laguna Tenerife Spain University of Alabama Tuscaloosa Department of Physics and Astronomy Gallalee Hall Box 870324 Tuscaloosa AL 35487-0324 USA Université Côte d’Azur Observatoire de la Côte d’Azur CNRS Laboratoire Lagrange UF 06304 Nice France Laboratoire Leprince-Ringuet CNRS/IN2P3 École Polytechnique Institut Polytechnique de Paris F-91120 Palaiseau France Departament de Física Quàntica i Astrofísica Institut de Ciències del Cosmos Universitat de Barcelona IEEC-UB Martí i Franquès 1 E-08028 Barcelona Spain Instituto de Astrofísica de Andalucía-CSIC Glorieta de la Astronomía s/n E-18008 Granada Spain Institute for Computational Cosmology and Department of Physics Durham University South Road Durham DH1 3LE UK Pontificia Universidad Católica de Chile Av. Libertador Bernardo O’Higgins 340 8331150 Santiago Chile Universidad Nacional Autónoma de México Delegación Coyoacán 04510 Ciudad de México Mexico IPARCOS-UCM Instituto de Física de Partículas y del Cosmos and EMFTEL Department Universidad Complutense de Madrid E-28040 Madrid Spain Instituto de Física Teórica UAM/CSIC and Departamento de Física Teórica Universidad Autónoma de Madrid c/ Nicolás Cabrera 13-15 Campus de Cantoblanco UAM E-28049 Madrid Spain LUTH GEPI and LERMA Observatoire de Paris Université PSL Université Paris Cité CNRS 5 place Jules Janssen F-92190 Meudon France INAF – Osservatorio

A wide variety of Galactic sources show transient emission at soft and hard X-ray energies: low- and high-mass X-ray binaries containing compact objects, isolated neutron stars exhibiting extreme variability as magnetars as well as pulsar-wind nebulae. Although most of them can show emission up to MeV and/or GeV energies, many have not yet been detected in the TeV domain by Imaging Atmospheric Cherenkov Telescopes. In this paper, we explore the feasibility of detecting new Galactic transients with the Cherenkov Telescope Array Observatory (CTAO) and the prospects for studying them with Target of Opportunity observations. We show that CTAO will likely detect new sources in the TeV regime, such as the massive microquasars in the Cygnus region, low-mass X-ray binaries with low-viewing angle, flaring emission from the Crab pulsar-wind nebula or other novae explosions, among others. Since some of these sources could also exhibit emission at larger time-scales, we additionally test their detectability at longer exposures. We finally discuss the multiwavelength synergies with other instruments and large astronomical facilities.

关键词： binaries: general stars: magnetars novae cataclysmic variables pulsars: general gamma-rays: general

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Rapid improvement of students' soft-skills based on an agile-process approach

Rapid improvement of students' soft-skills based on an agile...

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Frontiers in Education (FIE) Conference

作者： Eduardo Valentin José Reginaldo Hughes Carvalho Raimundo Barreto Post-graduate Program in Informatics (PPGI) Federal University of Amazonas (UFAM) Coroado Manaus Brazil Post-graduate Program in Informatics (PPGI) Institute of Computing (ICOMP) Universidade Federal do Amazonas Manaus AM BR

ISBN: (纸本)9781479984558

Manaus, the capital city of the state of Amazonas and the sixth Brazilian largest gross domestic product, demands highly qualified hardware and software developers for consumer electronics and telecommunication sectors of its free trading zone. However, what can be viewed as an opportunity for the youth alumni of local institutions of higher education contrasts with the low level of qualification provided by such institutions. As a consequence, most positions either remain opened or are occupied by professionals from other Brazilian regions. Moreover, the issue relies more on soft skills than on hard skills, as the local institutions are aligned with International standard academic curriculum and cover modern technologies. Soft skill is the enter barrier to the job market. English proficiency, communication skill, writing (in both Portuguese and English) skill, among others, are top listed failure reasons in the hiring processes. As one project manager highlighted: “it is much cheaper and quicker for the company to fill in some specific technological gaps, than to leverage a poor English proficiency”. This paper presents a proposal of an involving activity aiming to address several soft skills at the same time, with minimal disturbance in the student daily routine. The concept is based on the impact of immersing the student in a systematic project development experience. Clear communicated project goal, where the students have specific roles, with assigned accountable peers, everything under the umbrella of an Agile-like software development process (derived from SCRUM) are in the core of the activity. This paper details the incremental implementation methodology of the program among four research areas, and 23 projects or project activities, involving 34 students. The results of the two years running program will also be described, including the increase of progress visibility by advisors, the improvement of students communication and writing skills and the qualifi

关键词： Software Writing Cities and towns Companies Scrum (Software development) Context Education

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Ubiquitous computing: Applications and research opportunities

Ubiquitous computing: Applications and research opportunitie...

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IEEE International Conference on Computational Intelligence and computing Research

作者： Jorge Luis Victoria Barbosa Apply Computing Graduate Program (Pipca) University of Vale do Rio dos Sinos (Unisinos) São Leopoldo Brazil

About 25 years ago, Mark Weiser introduced the concept of Ubiquitous computing. Ten years later, Mahadev Satyanarayanan revisited and reinforced the concept by publishing studies focused on components and architectures to achieve the Pervasive computing (synonym of ubiquitous computing). Since then, this computational paradigm has received increasing attention from researchers. Significantly, recent years have witnessed the proliferation of various technologies that enable the implementation of ubiquitous systems such as Location Systems and Location-based Services (LBSs). Furthermore, the application of ubiquitous computing in different knowledge areas has increasingly been studied, covering areas such as health (u-health), accessibility (u-accessibility), learning (u-learning), commerce (u-commerce) and games (u-games). This broad interest shows the relevance of this emergent technology and allows us to predict that the adoption of ubiquitous computing will generate a similar impact that the adoption of Internet has generated in various application areas (for example, e-commerce and e-learning). This article summarizes the evolution of ubiquitous computing and discusses emerging uses in some application areas. Additionally, the text discusses issues currently addressed by researchers that are considered challenges and consequently research opportunities. For example, studies related to Contexts Histories (also called Trails) and their use to support Profile Management and Context Prediction have been considered strategic. Finally, the article concludes by outlining trends in ubiquitous computing research.

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Scratchpad memory management using data-prefetching

Scratchpad memory management using data-prefetching

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Conferencia Latinoamericana En Informatica (CLEI)

作者： Ivan Saraiva Silva Hildebrando Segundo Department of Computing Federal University Piauí Teresina Brazil Computer Science Graduate Program Federal University of Piauí Teresina Brazil

Nowadays, multicore processors including dozens of cores are a reality and the challenge of designing microprocessors with hundreds of cores does not appear far from being achieved. However, some questions remain open, despite the proposals found in the literature. Memory latency, data locality and programmability are some of the more critical ones. As the number of cores in multi-core processor architectures increases, so does the need of more efficient memory hierarchy and resource management scheme. The design of efficient memory hierarchy and memory management policy becomes a very important research subject in multi core architecture field. The usage of resource allocation strategies becomes increasingly necessary. This paper presents the design and implementation of a multi-core node with support to memory configuration and hardware-based scratchpad memory management. The node consists of 9 cores (8 slave cores and a master core) and a configurable local memory. The proposed architecture was implemented with VHDL and prototyped with FPGA development boards. Experimental results show that the proposed hardware-based scratchpad memory management unit can achieve 99,0 of hits in data address prediction and 97,1% of hit when searching data-frames in the local memory.

关键词： Multicore processing Resource management Memory management Hardware program processors Microprocessors

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A charge-redistribution based controller for keeping charge balance in neural stimulation

A charge-redistribution based controller for keeping charge ...

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Midwest Symposium on Circuits and Systems (MWSCAS)

作者： Lucas Teixeira Cesar Rodrigues Cesar Prior Graduate Program in Informatics Federal University of Santa Maria Dept. of Electronics and Computing - CT Federal University of Santa Maria

In this article, we present a circuit solution for sensing and controlling functional electrical stimulation (FES) currents. The objective is to keep both charge balance and residual electrode voltage under a safe limit throughout stimulation. In the proposed circuit, the stimulation current is set through an ultra-low-power charge-redistribution digital-to-analog converter (CR-DAC). Each stimulation pulse is copied by high-ratio current mirror into switched capacitors which integrate the residual direct current (DC) resulting from FES imbalances. As residual electrode voltage may buildup even for perfectly balanced current pulses, alternated cathodic-first and anodic-first stimulation is adopted to complement the charge-balancing mechanism. Simulation results suggest that the circuit is able to keep both residual charge and electrode voltage under safe limits, smaller than 0.05% and 64 mV respectively.

关键词： Electrodes Capacitors Sensors Voltage control Mirrors Voltage measurement Impedance

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SATD hardware architecture based on 8×8 Hadamard Transform for HEVC encoder

SATD hardware architecture based on 8×8 Hadamard Transform ...

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IEEE International Conference on Electronics, Circuits and Systems (ICECS)

作者： Eianca Silveira Cláudio Diniz Mateus Beck Fonseca Eduardo Costa Graduate Program on Electronic Engineering and Computing Catholic University of Pelotas (UCPel) Pelotas Brazil Engineering Center Federal University of Pelotas (UFPel) Pelotas Brazil Graduate Program on Health and Behavior Catholic University of Pelotas (UCPel) Pelotas Brazil

The most recent video compression standard is the High Efficient Video Coding (HEVC). It was created with the goal of reaching better videos compression compared to the existing ones. One of the most time-consuming modules of HEVC encoder is the Sum of Absolute Transform Differences (SATD), which is used in intra prediction mode decision and in Fractional pixel Motion Estimation (FME) modules. This paper proposes a dedicated architecture for SATD, based on 2-D 8×8 Hadamard Transform, which is divided into 1-D horizontal and 1-D vertical transforms. The architecture was synthesized to ASIC 45 nm technology and to FPGA. The results show that the whole SATD architecture consumes a total cell area of 12231 μm2, dissipates 3765.6 μW of total power and consumes 50.85 pJ of energy per SATD operation.

关键词： Transforms Computer architecture Registers Hardware Clocks Microprocessors Multiplexing

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