cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Strongly coupled theories beyond the Standard Model
Creators: name: Dobado, Antonio
name: Espriu, Domènec
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: This article presents a number of technical tools and results that may be instrumental to discern the nature of the Higgs particle. In scenarios where an additional strongly interacting sector is present in the electroweak theory resulting in a composite Higgs and longitudinal components of the massive gauge bosons, unitarity, analyticity and related techniques will be crucial to understand the properties of such a sector. The situation today may be reminiscent of the pre-QCD days: a strongly interacting theory governs the short-distances, but we have only access to long-distance experiment involving Nambu-Goldstone or pseudo Nambu-Goldstone bosons. Like in those days we can only rely on symmetry and general properties of field theory. Luckily, unlike in the pre-QCD days, we have now a much clearer idea of what we may be after. After presenting a classification of the various types of effective theories, we establish the criteria as to under which conditions different representations are possible and their equivalence. We discuss in detail the implications of analyticity, causality and unitarity; describe various unitarization methods and establish the properties of dynamically generated resonances and form factors. The relation to effective Lagrangians with explicit resonances is explained in the context of beyond the Standard Model (BSM) physics and the Higgs effective field theory (HEFT). We discuss how various BSM models may be reduced to the HEFT as well as implications from holography and lattice studies in establishing BSM phenomenology. The methods presented are then applied to various processes relevant to disentangle the existence and nature of an extended electroweak symmetry breaking sector visible in $VV$ fusion: two-Higgs production, vector resonances, $γγ$ physics and top-antitop production.
Imaging the Sun's Far-Side Active Regions by Applying Multiple Measurement Schemes on Multi-Skip Acoustic Waves
Creators: name: Zhao, Junwei
name: Hing, Dominick
name: Chen, Ruizhu
name: Webber, Shea Hess
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Being able to image active regions on the Sun's far side is useful for modeling the global-scale magnetic field around the Sun, and for predicting the arrival of major active regions that rotate around the limb onto the near side. Helioseismic methods have already been developed to image the Sun's far-side active regions using near-side high-cadence Doppler-velocity observations; however, the existing methods primarily explore the 3-, 4-, and 5-skip helioseismic waves, leaving room for further improvement in the imaging quality by including waves with more multi-skip waves. Taking advantage of the facts that 6-skip waves have the same target-annuli geometry as 3- and 4-skip waves, and that 8-skip waves have the same target-annuli geometry as 4-skip waves, we further develop a time--distance helioseismic code to include a total of 14 sets of measurement schemes. We then apply the new code on the SDO/HMI-observed Dopplergrams, and find that the new code provides substantial improvements over the existing codes in mapping newly-emerged active regions and active regions near both far-side limbs. Comparing 3 months of far-side helioseismic images with the STEREO/EUVI-observed 304A images, we find that 97.3% of the helioseismically detected far-side active regions that are larger than a certain size correspond to an observed region with strong EUV brightening. The high reliability of the new imaging tool will potentially allow us to further calibrate the far-side helioseismic images into maps of magnetic flux.
description: accepted for publication in ApJ
title: Programme de la conférence du projet amorce IDENTITES_NATIONALES, ATRI 5
Creators: name: IREMAM (UMR 7310)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2017

description: Programme de la conférence organisée dans le cadre de l'ATRI 5, projet amorce IDENTITES_NATIONALES, Normes juridiques et religieuses du 14 décembre 2013
Can we describe charged nanoparticles with electrolyte theories? Insight from mesoscopic simulation techniques
Creators: name: Dahirel, Vincent
name: Bernard, Olivier
name: Jardat, Marie
Publisher: name: arXiv
Year: 2020
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Electrolyte theories enable to describe the structural and dynamical properties of simple electrolytes in solution, such as sodium chloride in water. Using these theories for aqueous solutions of charged nanoparticles is a straightforward route to extract their charge and size from experimental data. Nevertheless, for such strongly asymmetric electrolytes, the validity of the underlying approximations have never been properly challenged with exact simulation results. In the present work, well established mesoscopic numerical simulations are used to challenge the ability of advanced electrolyte theories to predict the electrical conductivity of suspensions of charged nanoparticles, in the salt-free case. The theories under investigation are based on the Debye-Fuoss-Onsager treatment of electrolyte transport. When the nanoparticles are small enough (about one nanometer large), the theoretical results agree remarkably well with the simulation ones, even in the high concentration regime (packing fraction of in nanoparticles larger than 3$\%$ ). Strikingly, for highly charged nanoparticles, the theory is able to capture the non-monotonic variation of the ratio of the electrical conductivity to its value at infinite dilution (ideal value) as a function of the concentration. However, the tested theories fail to describe the conductivity of suspensions containing larger nanoparticles ({\em e.g.} of diameter $4$~nm). Finally, only small charged nanoparticles can be considered as {\em ions}, as far as electrolyte theories are concerned.
MOESM3 of Reduced culture temperature attenuates oxidative stress and inflammatory response facilitating expansion and differentiation of adipose-derived stem cells
Creators: name: Tirza, Gal
name: Solodeev, Inna
name: Sela, Meirav
name: Greenberg, Ilanit
name: Metsada Pasmanik-Chor
name: Gur, Eyal
name: Shani, Nir
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Plant Biology

description: Additional file 3: Table S3. Gene array results of the main pro-inflammatory genes appearing in the function analysis of the differentially expressed genes between 37 °C and 35 °C ASCs.
Additional file 2: of Survey indicated that core outcome set development is increasingly including patients, being conducted internationally and using Delphi surveys
Creators: name: Biggane, Alice
name: Brading, Lucy
name: Ravaud, Philippe
name: Young, Bridget
name: Williamson, Paula
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Hematology
subject: Computational Biology

description: Method Combinations. (DOCX 14 kb)
Optimal Monte Carlo Updating
Creators: name: Pollet, L.
name: Rombouts, S. M. A.
name: Van Houcke, K.
name: Heyde, K.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Based on Peskun's theorem it is shown that optimal transition matrices in Markov chain Monte Carlo should have zero diagonal elements except for the diagonal element corresponding to the largest weight. We will compare the statistical efficiency of this sampler to existing algorithms, such as heat-bath updating and the Metropolis algorithm. We provide numerical results for the Potts model as an application in classical physics. As an application in quantum physics we consider the spin 3/2 XY model and the Bose-Hubbard model which have been simulated by the directed loop algorithm in the stochastic series expansion framework.
description: 6 pages, 5 figures, replaced with published version
Additional file 1: of Detection and genetic characterization of feline bocavirus in Northeast China
Creators: name: Yi, Shushuai
name: Niu, Jiangting
name: Wang, Hualei
name: Dong, Guoying
name: Zhao, Yanli
name: Dong, Hao
name: Guo, Yanbing
name: Wang, Kai
name: Hu, Guixue
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: List of representative bocavirus strains obtained from the GenBank database for genetic analysis and phylogenetic tree construction. (DOC 64 kb)
Statistical properties of undulator radiation in the IOTA storage ring
Creators: name: Lobach, Ihar
name: Lebedev, Valeri
name: Nagaitsev, Sergei
name: Romanov, Aleksandr
name: Stancari, Giulio
name: Valishev, Alexander
name: Halavanau, Aliaksei
name: Huang, Zhirong
name: Kim, Kwang-Je
Publisher: name: arXiv
Year: 2019
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: We study turn-by-turn fluctuations in the number of spontaneously emitted photons from an undulator, installed in the Integrable Optics Test Accelerator (IOTA) electron storage ring at Fermilab. A theoretical model is presented, showing the relative contributions due to the discrete nature of light emission and to the incoherent sum of fields from different electrons in the bunch. The model is compared with a previous experiment at Brookhaven and with new experiments we carried out at IOTA. Our experiments focused on the case of a large number of longitudinal and transverse radiation modes, a regime where photon shot noise is significant and the total magnitude of the fluctuations is very small. The experimental and data analysis techniques, required to reach the desired sensitivity, are detailed. We discuss how the model and the experiment provide insights into this emission regime, enable diagnostics of small beam sizes, and improve our understanding of beam lifetime in IOTA.
Cosmological models described by a mixture of van der Waals fluid and dark energy
Creators: name: Kremer, G. M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The Universe is modeled as a binary mixture whose constituents are described by a van der Waals fluid and by a dark energy density. The dark energy density is considered either as the quintessence or as the Chaplygin gas. The irreversible processes concerning the energy transfer between the van der Waals fluid and the gravitational field are taken into account. This model can simulate: (a) an inflationary period where the acceleration grows exponentially and the van der Waals fluid behaves like an inflaton; (b) an inflationary period where the acceleration is positive but it decreases and tends to zero whereas the energy density of the van der Waals fluid decays; (c) a decelerated period which corresponds to a matter dominated period with a non-negative pressure; and (d) a present accelerated period where the dark energy density outweighs the energy density of the van der Waals fluid.
description: 5 pages, 5 figures. To be published in Physical Review D
Camallanus
Creators: name: Arai, Hisao P.
name: Smith, John W.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Secernentea
Camallanida
Camallanidae
Camallanus

description: Camallanus sp.
Site: alimentary tract
Hosts: Acipenser fulvescens (4); Esox lucius (2); Perca flavescens (1, 3) Distribution: Hudson Bay Drainage, Labrador, Manitoba, Ontario Records: 1. Tedla 1969 (ON); 2. Threlfall & Hanek 1970b (LB); 3. Tedla & Fernando 1972 (ON); 4. Choudhury &
Dick 1998 (HBD, MB)
description: Published as part of Arai, Hisao P. & Smith, John W., 2016, Guide to the Parasites of Fishes of Canada Part V: Nematoda, pp. 1-274 in Zootaxa 4185 (1) on page 64, DOI: 10.11646/zootaxa.4185.1.1, http://zenodo.org/record/165530
D4.5 Machine Learning Algorithms over Federated Operation Modes – Final version
Creators: name: Díaz, Roberto
name: Fernández, Marcos
name: Medina, Jaime
Publisher: name: Zenodo
Year: 2021
Subjects: Privacy Preserving Federated Machine Learning
Federated Machine Learning Algorithms
MUSKETEER Platform

description: The main objective of this deliverable is to provide the final version of the MUSKETEER Machine Learning Library (MMLL) under Privacy Operation Modes (POMs) 1, 2 and 3.
 The final version of the library integrates a wrapper for using the cloud communications developed by IBM, enabling the communication between nodes at different machines. This provides an additional feature to the first release in which the communication among the nodes was restricted to processes running on the same machine or under the same private network.
 As far as the implementation of the algorithms is concerned, two additional variants are included within this release: The Federated Budget Support Vector Machine (FBSVM), available for the three POMs, and the Distributed Support Vector Machine (DSVM), available only for POM 1 due to impossibility of meeting the more restrictive requirements of the other two POMs. Regarding the K-means algorithm, an additional naïve sharding initialization has been included here in order to ensure the privacy requirements required at the workers which, for the previous version, could not be met under some particular circumstances. The implementation of the Neural Networks has been extended to include a model averaging approach as well as the gradient averaging already included in the first release. This translates into a more flexible configuration of the networks, enabling the user to solve both regression as well as classification problems. Furthermore, thanks to the inclusion of the model averaging, the performance of the models has been significantly improved and the communication overload has been reduced, resulting in faster training times.
 Some pre-processing capabilities have been included in this version of the library as a result of the work covered in D4.3. Normalization strategies, image as well as natural language processing or dimensionality reduction techniques are available. Finally, a complete set of demos and the corresponding instructions as well as a full documentation of the library is available at the public repository.
TeV signatures of compact UHECR accelerators
Creators: name: Neronov, A.
name: Tinyakov, P.
name: Tkachev, I.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study numerically particle acceleration by the electric field induced near the horizon of a rotating supermassive (M \sim 10^9-10^{10} M_{\odot}) black hole embedded in the magnetic field B. We find that acceleration of protons to energy E > 10^{20} eV is possible only at extreme values of M and B. We also find that the acceleration is very inefficient and is accompanied by a broad band MeV-TeV radiation whose total power exceeds at least by a factor of 1000 the total power emitted in ultra-high energy cosmic rays (UHECR). This implies that if O(10) nearby quasar remnants were sources of proton events with energy E > 10^{20} eV, then each quasar remnant would overshine e.g. the Crab nebula by more than two orders of magnitude in the TeV energy band. Recent TeV observations exclude this possibility. A model in which O(100) sources are situated at 100-1000 Mpc is not ruled out and can be experimentally tested by present TeV gamma-ray telescopes. Such a model can explain the observed UHECR flux at moderate energies E \sim (4-5) 10^{19} eV.
description: Replaced with published version
MOESM2 of Reduced culture temperature attenuates oxidative stress and inflammatory response facilitating expansion and differentiation of adipose-derived stem cells
Creators: name: Tirza, Gal
name: Solodeev, Inna
name: Sela, Meirav
name: Greenberg, Ilanit
name: Metsada Pasmanik-Chor
name: Gur, Eyal
name: Shani, Nir
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 2: Table S2. Function analysis of the differentially expressed genes between 37 °C and 35 °C ASCs.
Chandra Analysis and Mass Estimation of the Lensing Cluster of Galaxies CL0024+17
Creators: name: Ota, Naomi
name: Pointecouteau, Etienne
name: Hattori, Makoto
name: Mitsuda, Kazuhisa
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a detailed analysis of Chandra X-ray observations of the lensing cluster of galaxies CL0024+17 at z=0.395. We found that the radial temperature profile is consistent with being isothermal out to ~600 kpc and that the average X-ray temperature is 4.47 (+0.83, -0.54) keV. The X-ray surface brightness profile is represented by the sum of extended emission centered at the central bright elliptical galaxy with a small core of 50 kpc and more extended emission which can be well described by a spherical beta-model with a core radius of about 210 kpc. Assuming the X-ray emitting gas to be in hydrostatic equilibrium, we estimated the X-ray mass within the arc radius and found it is significantly smaller than the strong lensing mass by a factor of about 2--3. We detected a strong redshifted iron K line in the X-ray spectrum from the cluster for the first time and find the metal abundance to be 0.76 (+0.37, -0.31) solar.
description: 14 pages, 10 figures. Accepted for publication in ApJ, scheduled for January 2004. Version with high-quality figures at http://www-astro.phys.metro-u.ac.jp/users/ota/publications/index.html
Lachnomyrmex Wheeler 1910
Creators: name: DE ALBUQUERQUE, EMÍLIA ZOPPAS
name: PRADO, LÍVIA PIRES DO
name: ANDRADE-SILVA, JOUDELLYS
name: DE SIQUEIRA, EMELY LAIARA SILVA
name: DA SILVA SAMPAIO, KELLY LIANE
name: ALVES, DIEGO
name: BRANDÃO, CARLOS ROBERTO FERREIRA
name: ANDRADE, PALOMA L.
name: FEITOSA, RODRIGO MACHADO
name: DE AZEVEDO KOCH, ELMO BORGES
name: DELABIE, JACQUES HUBERT CHARLES
name: FERNANDES, ITANNA
name: BACCARO, FABRÍCIO BEGGIATO
name: SOUZA, JORGE LUIZ PEREIRA
name: ALMEIDA, RONY PETERSON SANTOS
name: SILVA, ROGÉRIO R.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Lachnomyrmex

description: Lachnomyrmex Wheeler, 1910
 Lachnomyrmex amazonicus Feitosa & Brandão, 2008. Melgaço [ANTWEB; DZUP; MZSP; Feitosa & Brandão, 2008]; Parauapebas [ANTWEB; INPA; MZSP; Feitosa & Brandão, 2008; Ulysséa et al., 2015].
 Lachnomyrmex pilosus Weber, 1950. Marituba [Feitosa & Brandão, 2008]; Melgaço [DZUP; INPA; MZSP; Feitosa & Brandão, 2008]; Portel [Harada, 2016].
description: Published as part of DE ALBUQUERQUE, EMÍLIA ZOPPAS, PRADO, LÍVIA PIRES DO, ANDRADE-SILVA, JOUDELLYS, DE SIQUEIRA, EMELY LAIARA SILVA, DA SILVA SAMPAIO, KELLY LIANE, ALVES, DIEGO, BRANDÃO, CARLOS ROBERTO FERREIRA, ANDRADE, PALOMA L., FEITOSA, RODRIGO MACHADO, DE AZEVEDO KOCH, ELMO BORGES, DELABIE, JACQUES HUBERT CHARLES, FERNANDES, ITANNA, BACCARO, FABRÍCIO BEGGIATO, SOUZA, JORGE LUIZ PEREIRA, ALMEIDA, RONY PETERSON SANTOS & SILVA, ROGÉRIO R., 2021, Ants of the State of Pará, Brazil: a historical and comprehensive dataset of a key biodiversity hotspot in the Amazon Basin, pp. 1-83 in Zootaxa 5001 (1) on page 45, DOI: 10.11646/zootaxa.5001.1.1, http://zenodo.org/record/5122523
Yu-Shiba-Rusinov states of single magnetic molecule in an $s-wave$ superconductor
Creators: name: Pradhan, Saurabh
name: Fransson, Jonas
Publisher: name: arXiv
Year: 2020
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We use the numerical renormalization group theory to investigate the Yu-Shiba-Rusinov (YSR) bound state properties of single magnetic molecules placed in an s-wave superconducting substrate. The molecule consist of a large core spin and a single orbital, coupled via an exchange interaction. The critical Coulomb interaction for the singlet/doublet transition decreases in the presence of this exchange interaction for both ferro and anti-ferromagnetic couplings. The number of YSR states also increase to two pairs, however, in the singlet phase, one of the pairs have zero spectral weight. We explore the evolution of the in-gap states using the Anderson model. Away from the particle-hole symmetry point, the results suggest a doublet-singlet-doublet transition as the on-site energy is lowered while keeping the Coulomb interaction fixed. To understand these results, we write down an effective model for the molecule in the limit of large superconducting order parameter. Qualitatively, it explains the various phase transitions and spectral nature of the in-gap states. Finally, we analyze the effects of magnetic anisotropic fields of the core spin on in-gap states. Due to internal degrees of freedom of the spin excited states, a multitude of new states emerges within the gap. Depending on the sign and strength of the uniaxial anisotropic field, the results indicate up to three pairs of YSR states.
White-dwarf asteroseismology: an update
Creators: name: Córsico, Alejandro H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The vast majority of stars that populate the Universe will end their evolution as white-dwarf stars. Applications of white dwarfs include cosmochronology, evolution of planetary systems, and also as laboratories to study non-standard physics and crystallization. In addition to the knowledge of their surface properties from spectroscopy combined with model atmospheres, the global pulsations that they exhibit during several phases of their evolution allow spying on the deep interior of these stars. Indeed, by means of asteroseismology, an approach based on the comparison between the observed pulsation periods of variable white dwarfs and the periods predicted by representative theoretical models, we can infer details of the internal chemical stratification, the total mass, and even the stellar rotation profile and strength of magnetic fields. In this article, we review the current state of the area, emphasizing the latest findings provided by space-mission data.
description: 14 pages, 4 figures, 2 tables; contributed to the Proceedings of IAU Symposium No. 357, "White Dwarfs as Probes of Fundamental Physics and Tracers of Planetary, Stellar, and Galactic Evolution," held in Hilo, Hawaii, 21-25 October 2019
Perspectives in Fundamental Physics in Space
Creators: name: Bertolami, Orfeu
name: de Matos, Clovis Jacinto
name: Grenouilleau, Jean Christophe
name: Minster, Olivier
name: Volonte, Sergio
Publisher: name: arXiv
Year: 2004
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We discuss the fundamental principles underlying the current physical theories and the prospects of further improving their knowledge through experiments in space.
description: Gravitational waves, gravitomagnetism, Equivalence Principle, Antimatter, Pioneer Anomaly, Lorentz invariance. To appear in IAA - Acta Astronautica Journal (2006)
Bound States of Light Bullets in Passively-Mode-Locked Semiconductor Lasers
Creators: name: Dohmen, Fabian
name: Javaloyes, Julien
name: Gurevich, Svetlana V.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: In this paper, we analyze the dynamics and formation mechanisms of bound states (BSs) of light bullets in the output of a laser coupled to a distant saturable absorber. First we approximate the full three-dimensional set of Haus master equations by a reduced equation governing the dynamics of the transverse profile. This effective theory allows us to perform a detailed multiparameter bifurcation study and to identify the different mechanisms of instability of BSs. In addition, our analysis reveals a non-intuitive dependence of the stability region as a function of the linewidth enhancement factors and the field diffusion. Our results are confirmed by direct numerical simulations of the full system.
description: 8 pages 11 figures, submitted to Chaos special issue on nonequilibrium dynamics and patterns
Paratrachymyrmex Solomon 2019
Creators: name: DE ALBUQUERQUE, EMÍLIA ZOPPAS
name: PRADO, LÍVIA PIRES DO
name: ANDRADE-SILVA, JOUDELLYS
name: DE SIQUEIRA, EMELY LAIARA SILVA
name: DA SILVA SAMPAIO, KELLY LIANE
name: ALVES, DIEGO
name: BRANDÃO, CARLOS ROBERTO FERREIRA
name: ANDRADE, PALOMA L.
name: FEITOSA, RODRIGO MACHADO
name: DE AZEVEDO KOCH, ELMO BORGES
name: DELABIE, JACQUES HUBERT CHARLES
name: FERNANDES, ITANNA
name: BACCARO, FABRÍCIO BEGGIATO
name: SOUZA, JORGE LUIZ PEREIRA
name: ALMEIDA, RONY PETERSON SANTOS
name: SILVA, ROGÉRIO R.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Paratrachymyrmex

description: Paratrachymyrmex Solomon et al., 2019
 Paratrachymyrmex bugnioni (Forel, 1912). Marabá [DZUP]; Paragominas [Solar et al., 2016b]; Portel [Harada, 2016]; Santarém [Vasconcelos et al., 2006].
description: Published as part of DE ALBUQUERQUE, EMÍLIA ZOPPAS, PRADO, LÍVIA PIRES DO, ANDRADE-SILVA, JOUDELLYS, DE SIQUEIRA, EMELY LAIARA SILVA, DA SILVA SAMPAIO, KELLY LIANE, ALVES, DIEGO, BRANDÃO, CARLOS ROBERTO FERREIRA, ANDRADE, PALOMA L., FEITOSA, RODRIGO MACHADO, DE AZEVEDO KOCH, ELMO BORGES, DELABIE, JACQUES HUBERT CHARLES, FERNANDES, ITANNA, BACCARO, FABRÍCIO BEGGIATO, SOUZA, JORGE LUIZ PEREIRA, ALMEIDA, RONY PETERSON SANTOS & SILVA, ROGÉRIO R., 2021, Ants of the State of Pará, Brazil: a historical and comprehensive dataset of a key biodiversity hotspot in the Amazon Basin, pp. 1-83 in Zootaxa 5001 (1) on page 48, DOI: 10.11646/zootaxa.5001.1.1, http://zenodo.org/record/5122523
Accurately modeling the Internet topology
Creators: name: Zhou, Shi
name: Mondragon, Raul J.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences
subject: C.2.1 and C.2.5

description: Based on measurements of the Internet topology data, we found out that there are two mechanisms which are necessary for the correct modeling of the Internet topology at the Autonomous Systems (AS) level: the Interactive Growth of new nodes and new internal links, and a nonlinear preferential attachment, where the preference probability is described by a positive-feedback mechanism. Based on the above mechanisms, we introduce the Positive-Feedback Preference (PFP) model which accurately reproduces many topological properties of the AS-level Internet, including: degree distribution, rich-club connectivity, the maximum degree, shortest path length, short cycles, disassortative mixing and betweenness centrality. The PFP model is a phenomenological model which provides a novel insight into the evolutionary dynamics of real complex networks.
description: 20 pages and 17 figures
Oncophora Diesing 1851
Creators: name: Arai, Hisao P.
name: Smith, John W.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Secernentea
Camallanida
Camallanidae
Oncophora

description: Oncophora Diesing, 1851
Generic diagnosis (after Baudin-Laurencin 1971, Petter 1979, and Pinto et al. 1988). Camallanidae. Body elongated, tapering at each end. Buccal capsule with two valves, marked internally by numerous interrupted ridges in both sexes. Mouth opening slit-like. Pair of tridents associated with buccal capsule. Oesophagus comprises an anterior muscular portion, and a posterior glandular portion of about equal length. Cuticle thin, finely striated in both sexes.
One species, O. melanocephala, is known from one fish species in Canada.
description: Published as part of Arai, Hisao P. & Smith, John W., 2016, Guide to the Parasites of Fishes of Canada Part V: Nematoda, pp. 1-274 in Zootaxa 4185 (1) on page 64, DOI: 10.11646/zootaxa.4185.1.1, http://zenodo.org/record/165530
Mycetomoellerius Solomon 2019
Creators: name: DE ALBUQUERQUE, EMÍLIA ZOPPAS
name: PRADO, LÍVIA PIRES DO
name: ANDRADE-SILVA, JOUDELLYS
name: DE SIQUEIRA, EMELY LAIARA SILVA
name: DA SILVA SAMPAIO, KELLY LIANE
name: ALVES, DIEGO
name: BRANDÃO, CARLOS ROBERTO FERREIRA
name: ANDRADE, PALOMA L.
name: FEITOSA, RODRIGO MACHADO
name: DE AZEVEDO KOCH, ELMO BORGES
name: DELABIE, JACQUES HUBERT CHARLES
name: FERNANDES, ITANNA
name: BACCARO, FABRÍCIO BEGGIATO
name: SOUZA, JORGE LUIZ PEREIRA
name: ALMEIDA, RONY PETERSON SANTOS
name: SILVA, ROGÉRIO R.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Hexapoda
Hymenoptera
Formicidae
Mycetomoellerius

description: Mycetomoellerius Solomon et al., 2019
 Mycetomoellerius farinosus (Emery, 1894). Municipality unavailable [ANTWEB; Emery, 1894b; Weber, 1958]; Belém [Kempf, 1972c]; Marituba [CPDC]; Moju [CPDC]; Novo Repartimento [CPDC]; Portel [Harada, 2016]; Santarém [Vasconcelos et al., 2006].
description: Published as part of DE ALBUQUERQUE, EMÍLIA ZOPPAS, PRADO, LÍVIA PIRES DO, ANDRADE-SILVA, JOUDELLYS, DE SIQUEIRA, EMELY LAIARA SILVA, DA SILVA SAMPAIO, KELLY LIANE, ALVES, DIEGO, BRANDÃO, CARLOS ROBERTO FERREIRA, ANDRADE, PALOMA L., FEITOSA, RODRIGO MACHADO, DE AZEVEDO KOCH, ELMO BORGES, DELABIE, JACQUES HUBERT CHARLES, FERNANDES, ITANNA, BACCARO, FABRÍCIO BEGGIATO, SOUZA, JORGE LUIZ PEREIRA, ALMEIDA, RONY PETERSON SANTOS & SILVA, ROGÉRIO R., 2021, Ants of the State of Pará, Brazil: a historical and comprehensive dataset of a key biodiversity hotspot in the Amazon Basin, pp. 1-83 in Zootaxa 5001 (1) on page 46, DOI: 10.11646/zootaxa.5001.1.1, http://zenodo.org/record/5122523
AI-POWERED RISK MANAGEMENT SYSTEM
Creators: name: Manwani, Prakash
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 460299
subject: Artificial intelligence not elsewhere classified
classificationCode: 460403
subject: Data security and protection
classificationCode: 460406
subject: Software and application security
classificationCode: 460501
subject: Data engineering and data science
classificationCode: 461103
subject: Deep learning
classificationCode: 461102
subject: Context learning

description: The increasing complexity of financial markets and the exponential growth of transactional data have necessitated the adoption of AI-powered risk management systems. These systems leverage machine learning, predictive analytics, and real-time data processing to enhance risk detection, assessment, and mitigation. Unlike traditional methods that rely on historical data and manual evaluation, AI-driven models enable proactive risk identification, optimize asset allocation, and improve decision-making in financial institutions.This article explores the core principles of AI in risk management, highlighting its role in credit risk assessment, fraud detection, regulatory compliance, and investment management. It also examines ethical concerns, data security, and regulatory constraints. Future developments, including quantum computing and blockchain integration, are also discussed. As AI adoption grows, a balanced approach integrating automation with human oversight is essential to ensure transparency, fairness, and resilience in financial risk management.
XMP gas-rich dwarfs in Nearby Voids: candidate selection
Creators: name: Pustilnik, S. A.
name: Egorova, E. S.
name: Perepelitsyna, Y. A.
name: Kniazev, A. Y.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We introduce a project aimed at systematically searching for eXtremely Metal-Poor (XMP) very gas-rich blue dwarfs in voids in the nearby Universe. Several such galaxies were first identified in the course of an unbiased study of the galaxy population in the nearby Lynx-Cancer void. These very rare and unusual galaxies appear to be the best proxies for the so-called Very Young Galaxies (VYGs) defined recently in the model simulations by Tweed et al. (2018). We discuss the main properties of ten prototype objects residing in nearby voids and formulate criteria to search for similar dwarfs in other voids. The recently published sample of 1354 Nearby Void Galaxies (NVG) is used to identify a subsample of 60 void dwarf XMP candidates. We provide a list of these XMP candidates with their main parameters and finding charts. These candidates are the subjects of subsequent spectral, photometric and HI studies in the accompanying papers. Looking ahead, with reference to the submitted accompanying papers, we find that this study results in the discovery of many new XMP dwarfs with 12+log(O/H) ~ 7.0-7.3 dex.
description: 14 pages, 5 figures, 2 tables. Accepted for publication in MNRAS
Classical and Quantum Strings in plane waves, shock waves and spacetime singularities: synthesis and new results
Creators: name: Sanchez, Norma G.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Key issues of classical and quantum strings in gravitational plane waves, shock waves and spacetime singularities are synthetically understood. This includes the string mass and mode number excitations, energy-momentum tensor, scattering amplitudes, vaccum polarization and wave-string polarization effect. The role of the real pole singularities characteristic of the tree level string spectrum (real mass resonances) and that of spacetime singularities is clearly exhibited. This throws light on the issue of singularities in string theory which can be thus classified and fully physically characterized in two different sets: strong singularities (poles of order equal or larger than 2, and black holes), where the string motion is collective and non oscillating in time, outgoing and scattering states do not appear, the string does not cross the singularities, and weak singularities (poles of order smaller than 2, Dirac delta, and conic/orbifold singularities) where the whole string motion is oscillatory in time, outgoing and scattering states exist, and the string crosses the singularities. Commom features of strings in singular plane backgrounds and in inflationary backgrounds are explicitly exhibited. The string dynamics and the scattering/excitation through the singularities (whatever their kind: strong or weak) is fully physically consistent and meaningful.
description: Synthesis and new material. 18 pages, no figures
Pheidole chrysops Wilson 2003
Creators: name: DE ALBUQUERQUE, EMÍLIA ZOPPAS
name: PRADO, LÍVIA PIRES DO
name: ANDRADE-SILVA, JOUDELLYS
name: DE SIQUEIRA, EMELY LAIARA SILVA
name: DA SILVA SAMPAIO, KELLY LIANE
name: ALVES, DIEGO
name: BRANDÃO, CARLOS ROBERTO FERREIRA
name: ANDRADE, PALOMA L.
name: FEITOSA, RODRIGO MACHADO
name: DE AZEVEDO KOCH, ELMO BORGES
name: DELABIE, JACQUES HUBERT CHARLES
name: FERNANDES, ITANNA
name: BACCARO, FABRÍCIO BEGGIATO
name: SOUZA, JORGE LUIZ PEREIRA
name: ALMEIDA, RONY PETERSON SANTOS
name: SILVA, ROGÉRIO R.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Pheidole
Pheidole chrysops

description: Pheidole chrysops Wilson, 2003. Mojuí dos Campos [MZCZ]; Oriximiná [CPDC]; Santarém [Wilson, 2003].
 Pheidole coffeicola Borgmeier, 1934. Municipality unavailable [Kempf, 1972c]; Belém [MPEG; Kempf, 1970]; Melgaço [MPEG]; Moju [CPDC].
description: Published as part of DE ALBUQUERQUE, EMÍLIA ZOPPAS, PRADO, LÍVIA PIRES DO, ANDRADE-SILVA, JOUDELLYS, DE SIQUEIRA, EMELY LAIARA SILVA, DA SILVA SAMPAIO, KELLY LIANE, ALVES, DIEGO, BRANDÃO, CARLOS ROBERTO FERREIRA, ANDRADE, PALOMA L., FEITOSA, RODRIGO MACHADO, DE AZEVEDO KOCH, ELMO BORGES, DELABIE, JACQUES HUBERT CHARLES, FERNANDES, ITANNA, BACCARO, FABRÍCIO BEGGIATO, SOUZA, JORGE LUIZ PEREIRA, ALMEIDA, RONY PETERSON SANTOS & SILVA, ROGÉRIO R., 2021, Ants of the State of Pará, Brazil: a historical and comprehensive dataset of a key biodiversity hotspot in the Amazon Basin, pp. 1-83 in Zootaxa 5001 (1) on page 49, DOI: 10.11646/zootaxa.5001.1.1, http://zenodo.org/record/5122523
MOESM1 of Reduced culture temperature attenuates oxidative stress and inflammatory response facilitating expansion and differentiation of adipose-derived stem cells
Creators: name: Tirza, Gal
name: Solodeev, Inna
name: Sela, Meirav
name: Greenberg, Ilanit
name: Metsada Pasmanik-Chor
name: Gur, Eyal
name: Shani, Nir
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology

description: Additional file 1: Table S1. Primer list.
AGN jets versus accretion as reionization sources
Creators: name: Torres-Albà, N.
name: Bosch-Ramon, V.
name: Iwasawa, K.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Cosmic reionization put an end to the dark ages that came after the recombination era. Observations seem to favor the scenario where massive stars generating photons in low-mass galaxies were responsible for the bulk of reionization. Even though a possible contribution from accretion disks of active galactic nuclei (AGN) has been widely considered, they are currently thought to have had a minor role in reionization. Our aim is to study the possibility that AGN contributed to reionization not only through their accretion disks, but also through ionizing photons coming from the AGN jets interacting with the IGM. We adopt an empirically derived AGN luminosity function at $z\simeq6$, use X-ray observations to correct it for the presence of obscured sources, and estimate the density of jetted AGN. We then use analytical calculations to derive the fraction of jet energy that goes into ionizing photons. Finally, we compute the contribution of AGN jets to the H II volume filling factor at redshifts $z\simeq15-5$. We show that the contribution of the AGN jet lobes to the reionization of the Universe at $z\sim6$ might have been as high as $\gtrsim 10$\% of that of star-forming galaxies, under the most favorable conditions of jetted and obscuration fraction. The contribution of AGN to the reionization, while most likely not dominant, could have been higher than previously assumed, thanks to the radiation originated in the jet lobes.
description: 7 pages, 3 figures, accepted for publication in A&A
Pheidole astur Wilson 2003
Creators: name: DE ALBUQUERQUE, EMÍLIA ZOPPAS
name: PRADO, LÍVIA PIRES DO
name: ANDRADE-SILVA, JOUDELLYS
name: DE SIQUEIRA, EMELY LAIARA SILVA
name: DA SILVA SAMPAIO, KELLY LIANE
name: ALVES, DIEGO
name: BRANDÃO, CARLOS ROBERTO FERREIRA
name: ANDRADE, PALOMA L.
name: FEITOSA, RODRIGO MACHADO
name: DE AZEVEDO KOCH, ELMO BORGES
name: DELABIE, JACQUES HUBERT CHARLES
name: FERNANDES, ITANNA
name: BACCARO, FABRÍCIO BEGGIATO
name: SOUZA, JORGE LUIZ PEREIRA
name: ALMEIDA, RONY PETERSON SANTOS
name: SILVA, ROGÉRIO R.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Pheidole
Pheidole astur

description: Pheidole astur Wilson, 2003 *. Marabá [DZUP]; Melgaço [MPEG].
 Pheidole biconstricta Mayr, 1870. Municipality unavailable [Kempf, 1972c]; Almeirim [DZUP]; Belém [Kempf, 1970]; Bragança [ANTWEB]; Conceição do Araguaia [MPEG]; Melgaço [MPEG; Andrade-Silva & Almeida, 2020; Mendoza-Penagos et al., 2020]; Oriximiná [CPDC].
description: Published as part of DE ALBUQUERQUE, EMÍLIA ZOPPAS, PRADO, LÍVIA PIRES DO, ANDRADE-SILVA, JOUDELLYS, DE SIQUEIRA, EMELY LAIARA SILVA, DA SILVA SAMPAIO, KELLY LIANE, ALVES, DIEGO, BRANDÃO, CARLOS ROBERTO FERREIRA, ANDRADE, PALOMA L., FEITOSA, RODRIGO MACHADO, DE AZEVEDO KOCH, ELMO BORGES, DELABIE, JACQUES HUBERT CHARLES, FERNANDES, ITANNA, BACCARO, FABRÍCIO BEGGIATO, SOUZA, JORGE LUIZ PEREIRA, ALMEIDA, RONY PETERSON SANTOS & SILVA, ROGÉRIO R., 2021, Ants of the State of Pará, Brazil: a historical and comprehensive dataset of a key biodiversity hotspot in the Amazon Basin, pp. 1-83 in Zootaxa 5001 (1) on page 49, DOI: 10.11646/zootaxa.5001.1.1, http://zenodo.org/record/5122523
Log-parabolic spectra and particle acceleration in blazars - II: The BeppoSAX wide band X-ray spectra of Mkn 501
Creators: name: Massaro, E.
name: Perri, M.
name: Giommi, P.
name: Nesci, R.
name: Verrecchia, F.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a spectral and temporal study of the complete set of BeppoSAX NFI (11) and WFC (71) observations of the BL Lac object Mkn 501. The WFC 2-28 keV data, reported here for the first time, were collected over a period of about five years, from September 1996 to October 2001. These observations, although not evenly distributed, show that Mkn 501, after going through a very active phase from spring 1997 to early 1999, remained in a low brightness state until late 2001. The data from the LECS, MECS and PDS instruments, covering the wide energy interval 0.1-150 keV, have been used to study in detail the spectral variability of the source. We show that the X-ray energy distribution of Mkn 501 is well described by a log-parabolic law in all luminosity states. This model allowed us to obtain good estimates of the SED synchrotron peak energy and of its associated power. The strong spectral variability observed, consisting of strictly correlated changes between the synchrotron peak energy and bolometric flux, suggests that the main physical changes are not only due to variations of the maximum Lorentz factor of the emitting particles but that other quantities must be varying as well. During the 1997 flare the high energy part of the spectrum of Mkn 501 shows evidence of an excess above the best fit log-parabolic law suggesting the existence of a second emission component that may be responsible for most of the observed variability.
description: Accepted for publication in Astronomy & Astrophysics (11 pages, 7 figures)
D4.7 Machine Learning Algorithms over Semi Honest Operation Modes – Final Version
Creators: name: Navia-Vázquez, Ángel
name: Sueiro, Jesús Cid
name: López, Manuel Vázquez
name: González-Serrano, Francisco
Publisher: name: Zenodo
Year: 2021
Subjects: Privacy Preserving Federated Machine Learning
Machine Learning Algorithms over Semi Honest Operation Modes
MUSKETEER Platform

description: This deliverable (D4.7 Machine Learning Algorithms over Semi Honest Operation Modes – Final Version) comprises the MUSKETEER Machine Learning Library (MMLL) needed to execute the distributed learning under POMs 4, 5 and 6, as well as some demonstration scripts to check the correct execution of the code. The list of available algorithms contains the models committed in this deliverable (Linear models (Linear Regression, Logistic Classifier, Ridge Regression), Kernel methods (Kernel Regression, Support Vector Machines) and Clustering (Kmeans)). The design and usage of the new models incorporated in this version of the library is analogous to the already available ones in the previous version, so the integration and use of the new methods do not present any special difficulty with respect to what is already integrated in the platform. MMLL has been successfully integrated in the MUSKETEER Client connector developed in WP7 and it is fully operative over the “pycloudmessenger” communication service implemented in WP3.
Thermal IR satellite sensor data application for earthquake research in China
Creators: name: Tronin, A. A.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: NOAA/AVHRR thermal images indicated the presence of positive thermal anomalies that are associated with the large linear structures and fault systems of the Earth's crust. The relation between thermal anomalies and seismic activity was established for Middle Asia on the basis of a 7-year series of thermal images. Thermal anomaly has been located near Beijing, on the border between the mountains and plain. The size of this anomaly is about 700 km long and 50 km wide. The anomaly appeared about 6-24 days before and continued about a week after an earthquake. The anomaly was sensitive to crust earthquakes with a magnitude more than 4.7 and for a distance of up to 500 km. The amplitude of this anomaly was about 3 C.
MOND and the "Dearth of Dark Matter in Ordinary Elliptical Galaxies"
Creators: name: Milgrom, Mordehai
name: Sanders, Robert H.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recent findings of Romanowsky et al., of an ``unexpectedly'' small mass discrepancy within 5 effective radii in several elliptical galaxies, are not surprising in the context of MOND. As we show here, they are, in fact, in full concordance with its predictions. One is dealing with high-surface-density galaxies with mean accelerations rather larger than the acceleration constant of MOND. These findings continue, and are now the extreme examples of, the trend predicted by MOND: the mass discrepancy sets in at larger and larger scaled radii in galaxies with larger and larger mean surface densities; or, equivalently, mean accelerations.
description: 9 pages, 2 figures, Version accepted for publication in ApJL. A discussion of other ellipticals added
An Alternative String Theory in Twistor Space for N=4 Super-Yang-Mills
Creators: name: Berkovits, Nathan
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this letter, an alternative string theory in twistor space is proposed for describing perturbative N=4 super-Yang-Mills theory. Like the recent proposal of Witten, this string theory uses twistor worldsheet variables and has manifest spacetime superconformal invariance. However, in this proposal, tree-level super-Yang-Mills amplitudes come from open string tree amplitudes as opposed to coming from D-instanton contributions.
description: 5 pages harvmac tex