cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Energetics and beaming of gamma-ray burst triggers
Creators: name: Meszaros, P.
name: Rees, M. J.
name: Wijers, R. A. M. J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A wide range of mechanisms have been proposed to supply the energy for gamma-ray bursts (GRB) at cosmological distances. It is a common misconception that some of these, notably NS-NS mergers, cannot meet the energy requirements suggested by recent observations. We show here that GRB energies, even at the most distant redshifts detected, are compatible with current binary merger or collapse scenarios involving compact objects. This is especially so if, as expected, there is a moderate amount of beaming, since current observations constrain the energy per solid angle much more strongly and directly than the total energy. All plausible progenitors, ranging from NS-NS mergers to various hypernova-like scenarios, eventually lead to the formation of a black hole with a debris torus around it, so that the extractable energy is of the same order, 1E+54 ergs, in all cases. MHD conversion of gravitational into kinetic and radiation energy can significantly increase the probability of observing large photon fluxes, although significant collimation may achieve the same effect with neutrino annihilation in short bursts. The lifetime of the debris torus is dictated by a variety of physical processes, such as viscous accretion and various instabilities; these mechanisms dominate at different stages in the evolution of the torus and provide for a range of gamma-ray burst lifetimes.
description: submitted to New Astronomy, for the David N. Schramm memorial volume, 14 pages LaTeX, no figures, minor changes
Faint Blue Galaxies as a Probe of the X-ray Background at High Redshift
Creators: name: Treyer, M. A.
name: Lahav, O.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a formalism describing the physical content of cross-correlation functions between a diffuse background and a population of discrete sources. The formalism is used to interpret cross-correlation signals between the unresolved X-ray background and a galaxy population resolved to high redshift in another spectral band. Specifically, we apply it to the so-called faint blue galaxy population and constrain their X-ray emissivity and clustering properties. A model is presented which satisfies the recently measured constraints on all 3 correlation functions (galaxy/galaxy, background/background and galaxy/background). This model predicts that faint galaxies in the magnitude range B=18-23 (cvering redshifts $z \lsim 0.5$) make up $\sim 22 \%$ of the X-ray background in the 0.5-2 keV band. At the mean redshift of the galaxy sample, $\bar z=0.26$, the comoving volume emissivity is $ρ_X \sim 6-9 \times 10^{38}h$ ergs s$^{-1}$Mpc$^{-3}$ . When extrapolated to fainter magnitudes, the faint blue galaxy population can account for most of the residual background at soft energy. We show how the measurement of the angular and zero-lag cross-correlation functions between increasingly faint galaxies and the X-ray background can allow us to map the X-ray emissivity as a function of redshift.
description: uuencoded compressed postscript, without figures. The preprint is available with figures at http://www.ast.cam.ac.uk/preprint/PrePrint.html
Deep learning for the R-parity violating supersymmetry searches at the LHC
Creators: name: Guo, Jun
name: Li, Jinmian
name: Li, Tianjun
name: Xu, Fangzhou
name: Zhang, Wenxing
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Supersymmetry with hadronic R-parity violation in which the lightest neutralino decays into three quarks is still weakly constrained. This work aims to further improve the current search for this scenario by the boosted decision tree method with additional information from jet substructure. In particular, we find a deep neural network turns out to perform well in characterizing the neutralino jet substructure. We first construct a Convolutional Neutral Network (CNN) which is capable of tagging the neutralino jet in any signal process by using the idea of jet image. When applied to pure jet samples, such a CNN outperforms the N-subjettiness variable by a factor of a few in tagging efficiency. Moreover, we find the method, which combines the CNN output and jet invariant mass, can perform better and is applicable to a wider range of neutralino mass than the CNN alone. Finally, the ATLAS search for the signal of gluino pair production with subsequent decay $\tilde{g} \to q q \tildeχ^0_1 (\to q q q)$ is recasted as an application. In contrast to the pure sample, the heavy contamination among jets in this complex final state renders the discriminating powers of the CNN and N-subjettiness similar. By analyzing the jets substructure in events which pass the ATLAS cuts with our CNN method, the exclusion limit on gluino mass can be pushed up by $\sim200$ GeV for neutralino mass $\sim 100$ GeV.
description: 17 pages, 6 figures, version accepted by PRD
Actif Santé - Jean-Pierre Bibard
Creators: name: Leibowitch, Jacques (1942-2020)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: 1 fichier (2 pages). Autre destinataire : Xavier Rey-Coquais
title: ADCO, Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Cart. 178 (11 H 80), 82 folios, f. 0058
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 178 (11 H 80), 82 folios, f. 0058, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 178 (11 H 80), 82 folios, f. 0058, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
MPEC 2024-G120 : 2023 TS3
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Applications of Minkowski Functionals to the Statistical Analysis of Dark Matter Models
Creators: name: Platzoeder, Michael
name: Buchert, Thomas
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A new method for the statistical analysis of 3D point processes, based on the family of Minkowski functionals, is explained and applied to modelled galaxy distributions generated by a toy-model and cosmological simulations of the large-scale structure in the Universe. These measures are sensitive to both, geometrical and topological properties of spatial patterns and appear to be very effective in discriminating different point processes. Moreover by the means of conditional subsampling, different building blocks of large-scale structures like sheets, filaments and clusters can be detected and extracted from a given distribution.
description: 13 pages, Latex, 2 gzipped tar-files, to appear in: Proc. ``1st SFB workshop on Astro-particle physics'', Ringberg, Tegernsee, 1995
Falco subbuteo Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Falconiformes
Falconidae
Falco
Falco subbuteo

description: Falco subbuteo [spec. nov.]
F. cera pedibusque flavis, dorso fusco, nucha alba, abdomine pallido maculis oblongis fuscis. Fn. svec. 64.
Falconaria ars ad aucupium & venatum instruendi Falcones transiit in Scientiam; inter auctores plurimos eminet d' Esparon Falconaria. Francf. 1617. quarr.
Subbuteo. Alb. av. 1. p. 6. t. 6. Raj. av. 15.
Habitat in Europa, Alaudis infestus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 89-90, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 2: of A novel photic entrainment mechanism for the circadian clock in an insect: involvement of c-fos and cryptochromes
Creators: name: Kutaragi, Yuki
name: Tokuoka, Atsushi
name: Tomiyama, Yasuaki
name: Nose, Motoki
name: Watanabe, Takayuki
name: Bando, Tetsuya
name: Moriyama, Yoshiyuki
name: Tomioka, Kenji
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Figure S1. Effect of RNAi of cry genes on locomotor activity during the first 3 h after light-on in the cricket Gryllus bimaculatus. The activity was measured on the first day after 6 h phase advance of light-on. Error bars indicate SEM. Numbers in parenthesis indicate the number of animals used. Gb’cry2RNAi and Gb’cry1RNAi/Gb’cry2RNAi significantly reduced the light-induced locomotor activity compared to DsRed2RNAi treatment (*P
Reducibility for a fast driven linear Klein-Gordon equation
Creators: name: Franzoi, Luca
name: Maspero, Alberto
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35L10 - 37K55

description: We prove a reducibility result for a linear Klein-Gordon equation with a quasi-periodic driving on a compact interval with Dirichlet boundary conditions. No assumptions are made on the size of the driving, however we require it to be fast oscillating. In particular, provided that the external frequency is sufficiently large and chosen from a Cantor set of large measure, the original equation is conjugated to a time independent, diagonal one. We achieve this result in two steps. First, we perform a preliminary transformation, adapted to fast oscillating systems, which puts the original equation in a perturbative setting. Then we show that this new equation can be put to constant coefficients by applying a KAM reducibility scheme, whose convergence requires a new type of Melnikov conditions.
Molecular Gas in the z=2.8 Submillimeter Galaxy SMM 02399-0136
Creators: name: Frayer, D. T.
name: Ivison, R. J.
name: Scoville, N. Z.
name: Yun, M.
name: Evans, A. S.
name: Smail, Ian
name: Blain, A. W.
name: Kneib, J. -P.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the detection of CO(3-2) emission from the submillimeter-selected hyperluminous galaxy SMM 02399-0136. This galaxy is the brightest source detected in the recent SCUBA surveys of the submillimeter sky. The optical counterpart of the submillimeter source has been identified as a narrow-line AGN/starburst galaxy at z=2.8. The CO emission is unresolved, theta < 5 arcsec, and is coincident in redshift and position with the optical counterpart. The molecular gas mass derived from the CO observations is 8x10^{10} h_{75}^{-2} M_{sun}, after correcting for a lensing amplification factor of 2.5. The large CO luminosity suggests that a significant fraction of the infrared luminosity of SMM 02399-0136 arises from star formation. The high inferred star-formation rate of 10^{3} M_{sun}/yr and the large gaseous reservoir may suggest that we are seeing the formation phase of a massive galaxy. Future CO observations of other galaxies detected in deep submillimeter surveys will test the generality of these conclusions for the bulk of the faint submillimeter population.
description: 6 pages including 2 figures Accepted: ApJ Letters, 11 Aug. 1998
Additional file 3: of Diagnostic role of circulating extracellular matrix-related proteins in non-small cell lung cancer
Creators: name: Andriani, Francesca
name: Landoni, Elena
name: Mensah, Mavis
name: Facchinetti, Federica
name: Miceli, Rosalba
name: Tagliabue, Elda
name: Giussani, Marta
name: Callari, Maurizio
name: Cecco, Loris De
name: Colombo, Mario
name: Roz, Luca
name: Pastorino, Ugo
name: Sozzi, Gabriella
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Table S2. Sensitivity and specificity data for SPARC cutoffs. (DOCX 18 kb)
Seeking the Ultraviolet Ionizing Background at z~3 with the Keck Telescope
Creators: name: Bunker, Andrew J.
name: Marleau, Francine R.
name: Graham, James R.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe the initial results of a deep long-slit emission line search for redshifted (2.7
description: 22 pages, 2 postscipt figures. Latex requires aaspp4.sty and epsf.sty (included). Accepted for publication in the Astronomical Journal (Nov 1998)
Céramique
Cratère apulien à fond rouge
Cratère apulien à Fond rouge
Creators: name: SAM
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016

description: Provenance: Ruvo, museo Jatta
description: date: Pouilles
description: date: 400
The Great Circle Camera: A New Drift Scanning Instrument
Creators: name: Zaritsky, Dennis
name: Shectman, Stephen A.
name: Bredthauer, Gregory
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss the design, construction, and use of a new class of scanning camera that eliminates a critical limitation of standard CCD drift-scan observations. A standard scan, which involves no correction for the differential drift rates and curved stellar paths across the field-of-view, suffers from severe image degradation even when one observes at moderate declinations. Not only does this effect limit the area of the sky over which drift scanning is viable, but as detector sizes increase, CCD mosaics become standard, and dome/telescope seeing improves, the area of sky for which scanning is acceptable (image degradation $\ltsim$ seeing) will be further reduced unless some action is taken. By modifying the scan path (the path on the sky traced by signal accumulated along a single CCD column) to lie along a great circle on the sky rather than along a path of constant declination, image degradation is minimized. In this paper, we discuss the design and implementation of a stage that rotates and translates the CCD during a drift-scan exposure so that the scan path is along a great circle on the sky. Data obtained during the commissioning run of the Great Circle Camera at the Las Campanas 1-m telescope are presented.
description: Second attempt at a readable archival file. 7 pages (gzip'ed and uuencoded postscript). A version of the preprint with Figures 2 and 3 can be obtained from D. Zaritsky. Accepted for publication in PASP
Inverse Compton Emission of TeV Gamma Rays from PSR B1259-63
Creators: name: Kirk, J. G.
name: Ball, Lewis
name: Skjaeraasen, Olaf
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We derive light curves for the hard gamma-ray emission, at energies up to several TeV, expected from the unique pulsar/Be-star binary system PSR B1259-63. This is the only known system in our galaxy in which a radio pulsar is orbiting a main sequence star. We show that inverse Compton emission from the electrons and positrons in the shocked pulsar wind, scattering target photons from the Be star, produces a flux of hard gamma-rays that should be above the sensitivity threshold of present day atmospheric Cerenkov detectors. Furthermore, we predict that the flux of hard gamma-rays produced via this mechanism has a characteristic variation with orbital phase that should be observable, and which is not expected from any other mechanism.
description: To be published in Astroparticle Physics. 24 pages, 8 figures
Optical control of magnetism in NiFe/VO2 heterostructures
Creators: name: Wei, Guodong
name: Lin, Xiaoyang
name: Si, Zhizhong
name: Wang, Dong
name: Wang, Xinhe
name: Liu, Kai
name: Jiang, Kaili
name: Wang, Zhaohao
name: Lei, Na
name: Chen, Yanxue
name: Mangin, Stephane
name: Zhao, Weisheng
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Optical methods for magnetism manipulation have been considered as a promising strategy for ultralow-power and ultrahigh-speed spin switches, which becomes a hot spot in the field of spintronics. However, a widely applicable and efficient method to combine optical operation with magnetic modulation is still highly desired. Here, the strongly correlated electron material VO2 is introduced to realize phase-transition based optical control of the magnetism in NiFe. The NiFe/VO2 bilayer heterostructure features appreciable modulations in electrical conductivity (55%), coercivity (60%), and magnetic anisotropy (33.5%). Further analyses indicate that interfacial strain coupling plays a crucial role in this modulation. Utilizing this optically controlled magnetism modulation feature, programmable Boolean logic gates (AND, OR, NAND, NOR, XOR, NXOR and NOT) for high-speed and low-power data processing are demonstrated based on this engineered heterostructure. As a demonstration of phase-transition spintronics, this work may pave the way for next-generation electronics in the post-Moore era.
Low-dimensional Lead-free Halide Perovskites for Resistive Switching Memory Devices
Creators: name: Kim, So-Yeon
name: Bisquert, Juan
name: Park, Nam-Gyu
Publisher: name: Zenodo
Year: 2024

description: Abstract presented at the '#OPTMS - Organic and Perovskite-Based Transistor Memristors and Synapses' symposium during the Materials for Sustainable Development Conference, MATSUS Spring 2024 Conference (MATSUS24).

Accepted for an oral presentation on Wed Mar 06 2024 by Kim, So-Yeon.
Proximal Splitting Meets Variance Reduction
Creators: name: Pedregosa, Fabian
name: Fatras, Kilian
name: Casotto, Mattia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optimization and Control (math.OC)
subject: FOS: Mathematics
subject: 65K10

description: Despite the rise to fame of incremental variance-reduced methods in recent years, their use in nonsmooth optimization is still limited to few simple cases. This is due to the fact that existing methods require to evaluate the proximity operator for the nonsmooth terms, which can be a costly operation for complex penalties. In this work we introduce two variance-reduced incremental methods based on SAGA and SVRG that can efficiently take into account complex penalties which can be expressed as a sum of proximal terms. This includes penalties such as total variation, group lasso with overlap and trend filtering, to name a few. Furthermore, we also develop sparse variants of the proposed algorithms which can take advantage of sparsity in the input data. Like other incremental methods, it only requires to evaluate the gradient of a single sample per iteration, and so is ideally suited for large scale applications. We provide a convergence rate analysis for the proposed methods and show that they converge with a fixed step-size, achieving in some cases the same asymptotic rate as their full gradient variants. Empirical benchmarks on 3 different datasets illustrate the practical advantages of the proposed methods.
The plane-wave spectrum from the worldsheet
Creators: name: Eberhardt, Lorenz
name: Ferreira, Kevin
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study string theory on $\mathrm{AdS}_3$ backgrounds with mixed flux using the hybrid formalism of Berkovits, Vafa and Witten. We solve the worldsheet description of the theory completely in the plane-wave limit. This constitutes a direct derivation of the plane-wave spectrum from the worldsheet with mixed flux.
description: 32 pages; v2: version accepted by JHEP
Search for energetic cosmic axions utilizing terrestrial/celestial magnetic fields
Creators: name: Zioutas, K.
name: Thompson, D. J.
name: Paschos, E. A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Orbiting $γ$-detectors combined with the magnetic field of the Earth or the Sun can work parasitically as cosmic axion telescopes. The relatively short field lengths allow the axion-to-photon conversion to be coherent for $m_{axion} \sim 10^{-4}$ eV, if the axion kinetic energy is above $\sim 500$ keV (Earth's field), or, $\sim 50$ MeV (Sun's field), allowing thus to search for axions from $e^+e^-$ annihilations, from supernova explosions, etc. With a detector angular resolution of $\sim 1^o$, a more efficient sky survey for energetic cosmic axions passing {\it through the Sun} can be performed. Axions or other axion-like particles might be created by the interaction of the cosmic radiation with the Sun, similarly to the axion searches in accelerator beam dump experiments; the enormous cosmic energy combined with the built-in coherent Primakoff effect might provide a sensitive detection scheme, being out of reach with accelerators. The axion signal will be an excess in $γ$-rays coming either from a specific celestial place behind the Sun, e.g. the Galactic Center, or, from any other direction in the sky being associated with a violent astrophysical event, e.g. a supernova. Earth bound detectors are also of potential interest. The axion scenario also applies to other stars or binary systems in the Universe, in particular to those with superstrong magnetic fields.
description: 9 pages, LaTeX, small changes in text and bibliography
Multilingual Hate Speech and Offensive Language Detection of Low Resource Languages
Creators: name: Gutha, Abhinav Reddy
name: Nidamanuri Sai Adarsh
name: Alekar, Ananya
name: Reddy, Dinesh
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 460208
subject: Natural language processing
classificationCode: 461103
subject: Deep learning
classificationCode: 461104
subject: Neural networks

description: The last decade has seen a steep rise in the use and dependence of society on social media. The need for detection and prevention of hate and offensive speech is more than ever. The everchanging form of natural language makes the detection of hate speech challenging, involving code-mixed text. The task becomes even more daunting in a country like India, where different languages and dialects are spoken across the country. This paper details the Code Fellas team’s approaches in the context of HASOC 2023 - Task 4: Annihilate Hate, an initiative aimed at extending hate speech detection to Bengali, Bodo, and Assamese languages. Here we describe our approaches which broadly involve Long Short Term Memory (LSTM) coupled with Convolutional Neural Networks (CNN) and pre-trained Bidirectional Encoder Representations from Transformers (BERT) based models like IndicBERT and MuRIL. Notably, our results showcase the effectiveness of these approaches, with IndicBERT achieving a remarkable F1 score of 69.726% for Assamese, MuRIL achieving 71.955% for Bengali, and a BiLSTM model enhanced with an additional Dense Layer attaining an impressive 83.513% for Bodo.
Falco buteo Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Falconiformes
Falconidae
Falco
Falco buteo

description: Falco buteo [spec. nov.]
F. cera pedibusque luteis, corpore fusco, abdomine pallido maculis fuscis.
Buteo vulgaris. Gesn. av. 46. Will. ornith. 38. t. 6. Raj. av. 16.
Buteo. Alb. av. 1. p. 1. t. 1.
Habitat in Europa, Cuniculis & Bufonibus infestus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 90, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
INSTITUTIONALISING PARTICIPATORY, CLIENT-DRIVEN RESEARCH AND TECHNOLOGY DEVELOPMENT IN AGRICULTURE
Creators: name: Ashby, Jacqueline
name: Sperling, Louise
name: Ashby, Jacqueline
name: Sperling, Louise
Publisher: name: Unknown
Year: 1994
Subjects: Research and Development/Tech Change/Emerging Technologies

description: This paper identifies key characteristics of participatory research and development (R&D): it is client-driven, requires decentralised technology development, devolves to farmers the major responsibility for adaptive testing, and requires institutions and individuals to become accountable for the relevance and quality of technology on offer. The paper then reviews ways by which institutions can respond to these characteristics. For creating clientdriven agenda options commonly include: representation by clients on their governing boards, joint research planning and the establishment of researchextension liaison units. However, more effective than this "representation" strategy might be to place a significant proportion of the available research resources directly under client control: client groups would then contract as they deem appropriate. Decentralising technology development requires scientists to shift away from a "pipeline" model which defines a limited number of products towards the development of menus of options, and prototypes, which are then adapted to "niche" conditions by others. Such localised testing, requiring a community-based adaptive research capacity, can be achieved through working with groups of fanners (rather than individuals) and with producer organisations. The devolution of trial testing is discussed in reference to experimental methods, statistical validity and cost. Institutionalising accountability sharing is probably the most challenging issue. While scientists' rewards might be tied to the success or failure of technologies, clients' contracts with research or third party evaluations probably serve as more binding options. Three issues are signalled for future attention. First, clarification is needed of the respective roles of fanners and scientists in prototype screening: e.g. what features should scientists be screening for and at what stage?; how. early in the process can farmers be involved and to what degree can they control decisions on trial design and measurement? Second, decentralised technology development requires corresponding reorientation in service provision (e.g. credit, extension and seed multiplication). Third, steps need to be taken to safeguard equity, both between the more and less vocal groups of fanners,and between the requirements of present and future generations (the latter referring particularly to environmental concerns). Finally, participatory R&D alone is insufficient to deliver innovations relevant to diverse client groups: explicit procedures are required to define which clients are to participate, whose agenda are to drive the process, and what organisational innovations are needed to move agricultural R&D in these directions.
Anomalous Antiferromagnetism in Metallic RuO$_2$ Determined by Resonant X-ray Scattering
Creators: name: Zhu, Z. H.
name: Strempfer, J.
name: Rao, R. R.
name: Pelliciari, J.
name: Choi, Y.
name: Kawaguchi, T.
name: You, H.
name: Mitchell, J. F.
name: Shao-Horn, Y.
name: Comin, R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We studied the magnetic ordering of thin films and bulk crystals of rutile RuO$_2$ using resonant X-ray scattering across the Ru L$_2$ absorption edge. Combining polarization analysis and azimuthal-angle dependence of the magnetic Bragg signal, we have established the presence of G-type antiferromagnetism in RuO$_2$ with T$_N$ $>$ 300 K. In addition to revealing a spin-ordered ground state in the simplest ruthenium oxide compound, the persistence of magnetic order even in nanometer-thick films lays the ground for potential applications of RuO$_2$ in antiferromagnetic spintronics.
description: 5 pages, 4 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Collision Avoidance ÑÐ¸ÑÑÐµÐ¼Ñ Ð½Ð° Ð±Ð°Ð·Ðµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° Velocity Obstacles
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
title: Development of a Collision Avoidance system based on the Velocity Obstacles algorithm
Creators: name: ÐÐµÑÑÐ¾Ð»Ð°, ÐÑÐµÐ²Ð¾Ð»Ð¾Ð´
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2025
Subjects: Ð¿ÑÐµÐ´Ð¾ÑÐ²ÑÐ°ÑÐµÐ½Ð¸Ðµ ÑÑÐ¾Ð»ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ð¹
Ð¿Ð¾Ð¸ÑÐº ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð¿ÑÑÐ¸ Ð² Ð³ÑÐ°ÑÐµ
ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
collision avoidance
shortest pathfinding in a graph
strategic planning
tactical management

description: ÐÑÐµÐ´Ð¾ÑÐ²ÑÐ°ÑÐµÐ½Ð¸Ðµ ÑÑÐ¾Ð»ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ð¹ â ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð°Ñ Ð·Ð°Ð´Ð°ÑÐ° Ð² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð°Ð³ÐµÐ½ÑÐ¾Ð² Ð´Ð»Ñ ÑÐ¾Ð±Ð¾ÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ¸, Ð¸Ð³ÑÐ¾Ð²ÑÑ ÑÐ¸Ð¼ÑÐ»ÑÑÐ¸Ð¹ Ð¸ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼, ÑÐ°ÐºÐ¸Ñ ÐºÐ°Ðº Ð¾ÑÐµÐ½ÐºÐ° Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ð¹ ÑÐµÑÐµÐ· Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð¶Ð°ÑÐ½Ð¾Ð¹ ÑÐ²Ð°ÐºÑÐ°ÑÐ¸Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð³Ð¸Ð±ÑÐ¸Ð´Ð½Ð°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ, Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÑÑÑÐ°Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ A* (ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÑÐ¾Ð²ÐµÐ½Ñ â Ð¿Ð¾Ð¸ÑÐº ÐºÑÐ°ÑÑÐ°Ð¹ÑÐµÐ³Ð¾ Ð¿ÑÑÐ¸ Ð² Ð³ÑÐ°ÑÐµ) Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ RVO (ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÑÐ¾Ð²ÐµÐ½Ñ â Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¸Ð·Ð±ÐµÐ³Ð°Ð½Ð¸Ðµ ÑÑÐ¾Ð»ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ð¹). ÐÐ»Ñ Ð²Ð°Ð»Ð¸Ð´Ð°ÑÐ¸Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¾ ÑÐµÑÑÐ¾Ð²Ð¾Ðµ Ð¾ÐºÑÑÐ¶ÐµÐ½Ð¸Ðµ, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐµÐµ Ð¾ÑÐµÐ½Ð¸ÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² ÐºÐ°Ðº Ð² Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð¼ ÑÐµÐ¶Ð¸Ð¼Ðµ, ÑÐ°Ðº Ð¸ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¸Ñ ÑÐ¾Ð²Ð¼ÐµÑÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ¶Ð´Ð°ÑÑ, ÑÑÐ¾ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¸Ñ A* Ð¸ RVO Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÐµÑ Ð±Ð°Ð»Ð°Ð½Ñ Ð¼ÐµÐ¶Ð´Ñ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½ÑÐ¼ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸ Ð»Ð¾ÐºÐ°Ð»ÑÐ½ÑÐ¼ Ð¼Ð°Ð½ÐµÐ²ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼, ÑÑÐ¾ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ Ð´Ð»Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¼Ð½Ð¾Ð³Ð¾Ð°Ð³ÐµÐ½ÑÐ½ÑÐ¼Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð°Ð¼Ð¸ Ð² ÑÐ»Ð¾Ð¶Ð½ÑÑ ÑÑÐµÐ´Ð°Ñ.
description: Collision avoidance is a fundamental challenge in developing agent behavior models for robotics, game simulations, and analytical systems, such as assessing building safety through fire evacuation modeling. This work proposes a hybrid model integrating the A* algorithm (strategic level â shortest pathfinding in a graph) and the RVO algorithm (tactical level â dynamic collision avoidance). A test environment was developed to validate the model, enabling evaluation of the algorithmsâ effectiveness both in standalone mode and in collaborative operation. The results demonstrate that the combination of A* and RVO achieves a balance between global planning and local maneuvering, which is critical for managing multi-agent systems in complex environments.
Observations of the X-ray Nova GRO~J0422+32: II: Optical Spectra Approaching Quiescence
Creators: name: Garcia, Michael R.
name: Callanan, Paul J.
name: McClintock, Jeffrey E.
name: Zhao, Ping
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results obtained from a series of 5~Å resolution spectra of the X-ray Nova GRO~J0422+32 obtained in 1993~October, when the system was approximately 2 magnitudes above quiescence, with ${\rm R \sim 19}$. The data were obtained in an effort to measure the orbital radial velocity curve of the secondary, but detection of the narrow photospheric absorption lines needed to do this proved elusive. Instead we found wide absorption bands reminiscent of M~star photospheric features. The parameters determined by fitting accretion disk line profiles (Smak profiles) to the H$α$ line are similar to those found in several strong black-hole candidates. Measurements of the velocity of the H$α$ line are consistent with an orbital period of 5.1~hours and a velocity semi-amplitude of the primary of $34 \pm 6$~\kms. These measurements, when combined with measurements of the velocity semi-amplitude of the secondary made by others, indicate that the mass ratio $q \sim 0.09$. If the secondary follows the empirical mass-radius relation found for CVs, the low $q$ implies a primary mass of $M_x \sim 5.6$\mo, and a rather low (face-on) inclination. The H$α$ EW is found to be modulated on the orbital period with a phasing that implies a partial eclipse of the disk by the secondary, but simultaneous R~band photometry shows no evidence for such an eclipse.
description: Accepted for ApJ, plain latex, 5 figures available as self-extracting uuendoced, compressed, tarfiles (from uufiles)
title: ADCO, Cartulaire de Cîteaux pour les possessions de Saulon-la-Chapelle et Saulon-la-Rue, Fénay, Noiron et la rivière Cent-fonds (XVe siècle), Cart. 179 (11 H 1075), 70 folios, f. 0146
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Petot, Frédéric
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de Cîteaux pour les possessions de Saulon-la-Chapelle et Saulon-la-Rue, Fénay, Noiron et la rivière Cent-fonds (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 179 (11 H 1075), 70 folios, f. 0146, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Saulon-la-Chapelle et Saulon-la-Rue, Fénay, Noiron et la rivière Cent-fonds (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 179 (11 H 1075), 70 folios, f. 0146, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
MOESM1 of Functional Heterogeneity within the CD44 High Human Breast Cancer Stem Cell-Like Compartment Reveals a Gene Signature Predictive of Distant Metastasis
Creators: name: Leth-Larsen, Rikke
name: Terp, Mikkel
name: Christensen, Anne
name: Elias, Daniel
name: KĂźhlwein, Thorsten
name: Jensen, Ole
name: Petersen, Ole
name: Ditzel, Henrik
Publisher: name: figshare
Year: 2012
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Supplementary material, approximately 1.91 MB.
Tertiary lymphoid organ neogenesis in grey matter pathology in multiple sclerosis
Creators: name: Browne, Eleanor
Publisher: name: Imperial College London
Year: 2015

description: Chronic meningeal inflammation is suggested to contribute to the progression of secondary progressive multiple sclerosis (SPMS) in part by driving cortical grey matter pathology. The presence of tertiary lymphoid organ-like (TLO) structures in a large proportion of SPMS cases is associated with faster clinical progression and more severe cortical pathology, suggesting that TLO neogenesis and chronic meningeal inflammation contribute to progression. Gene expression of the cytokine lymphotoxin-alpha (LTα), implicated in TLO formation and cytotoxicity, and the lymphoid chemokines CXCL13 and CCL21, was determined in post-mortem SPMS meninges by qPCR. LTα was increased in SPMS, while substantially increased CXCL13 expression was associated with the presence of TLOs in SPMS. As LTα induces CXCL13 during inflammation, we investigated the hypothesis that LTα drives TLO formation and exacerbates cortical pathology in SPMS, using an animal model of cortical demyelination driven by meningeal inflammation. Subclinical experimental autoimmune encephalomyelitis was induced in female dark agouti rats by immunisation with 5-10μg of recombinant mouse myelin oligodendrocyte glycoprotein (rmMOG) in incomplete Freund’s adjuvant. Injection of LTα and the cytokine interferon-γ into the subarachnoid space 21 days post-immunisation induced substantial meningeal infiltration with B cell-rich areas, T cells, macrophages and channel formation reminiscent of early TLOs, accompanied by microglial activation, extensive demyelination, and remyelination within 21 days. To study chronic meningeal cytokine expression we injected a VSV-G pseudotyped lentiviral vector (LV) expressing green fluorescent protein (GFP) or human LTα(LVLTα) into the subarachnoid space. Meningeal GFP expression was induced up to 90 days post-injection. Human LTα expression was detected in rat brain and CSF, with widespread microglial activation and meningeal infiltrates of macrophages, B and T cells resembling TLOs, in naïve and rmMOG-immunised rats at 90 days post-LVLTα, while extensive demyelination was present only in rmMOG-immunised rats. This suggests that chronic meningeal LTα expression is sufficient for widespread microglial activation, but demyelination requires an anti-myelin response in this model. These findings support the hypothesis that chronic meningeal inflammation drives cortical pathology, and LTα / TLO neogenesis may represent a novel therapeutic target for SPMS.
UV-C LED-induced cyclobutane pyrimidine dimer formation, lesion repair and mutagenesis in the biofilm-forming diatom, Navicula incerta
Creators: name: Whitworth, Paul
name: Aldred, Nick
name: Finlay, John A.
name: Reynolds, Kevin J.
name: Plummer, Joseph
name: Clare, Anthony S.
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Molecular Biology
subject: Pharmacology
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Plant Biology

description: The use of ultraviolet-C (UV-C) irradiation in marine biofouling control is a relatively new and potentially disruptive technology. This study examined effects of UV-C exposure on the biofilm-forming diatom, Navicula incerta. UV-C-induced mutations were identified via Illumina HiSeq. A de novo genome was assembled from control sequences and reads from UV-C-exposed treatments were mapped to this genome, with a quantitative estimate of mutagenesis then derived from the frequency of single nucleotide polymorphisms. UV-C exposure increased cyclobutane pyrimidine dimer (CPD) abundance with a direct correlation between lesion formation and fluency. Cellular repair mechanisms gradually reduced CPDs over time, with the highest UV-C fluence treatments having the fastest repair rates. Mutation abundances were, however, negatively correlated with CPD abundance suggesting that UV-C exposure may influence lesion repair. The threshold fluence for CPD formation exceeding CPD repair was >1.27 J cm−2. Fluences >2.54 J cm−2 were predicted to inhibit repair mechanisms. While UV-C holds considerable promise for marine antifouling, diatoms are just one, albeit an important, component of marine biofouling communities. Determining fluence thresholds for other representative taxa, highlighting the most resistant, would allow UV-C treatments to be specifically tuned to target biofouling organisms, whilst limiting environmental effects and the power requirement.
Chiral magnetohydrodynamic turbulence in core-collapse supernovae
Creators: name: Masada, Youhei
name: Kotake, Kei
name: Takiwaki, Tomoya
name: Yamamoto, Naoki
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Macroscopic evolution of relativistic charged matter with chirality imbalance is described by the chiral magnetohydrodynamics (chiral MHD). One such astrophysical system is high-density lepton matter in core-collapse supernovae where the chirality imbalance of leptons is generated by the parity-violating weak processes. After developing the chiral MHD equations for this system, we perform numerical simulations for the real-time evolutions of magnetic and flow fields, and study the properties of the chiral MHD turbulence. In particular, we observe the inverse cascade of the magnetic energy and the fluid kinetic energy. Our results suggest that the chiral effects that have been neglected so far can reverse the turbulent cascade direction from direct to inverse cascade, which would impact the magnetohydrodynamics evolution in the supernova core toward explosion.
description: 19 pages, 17 figures, Accepted for publication in PRD. Movies of the simulations are available at http://www.kusastro.kyoto-u.ac.jp/~masada/movie.mp4
Engineering and characterisation of quantum non-Gaussian states
Creators: name: Hughes, Catherine
Publisher: name: Imperial College London
Year: 2015

description: This thesis presents an investigation into the generation and characterisation of non-Gaussian states in continuous variable quantum optics. Beginning by placing the study of continuous variables within the context of quantum information processing more generally, we then motivate the need for non-Gaussianity within quantum computing protocols. The focus then narrows to the consideration of two particular sets of non-Gaussian states: orthogonal superposition states and the cubic resource state. The superposition of two orthogonal states has been shown to enhance certain continuous variable quantum information processing protocols that rely on entanglement, and within this section two distinct methods for generating such states are considered. While one of these methods provides a specific example, the other introduces a general orthogonaliser that relies solely on knowledge of the expectation value for the chosen orthogonalising operator in order to produce the superposition. The second case for non-Gaussian state generation employs current results demonstrating the production of a weak approximation of the cubic resource state in order to illustrate the use of such single-mode states to generate multimode states with similar features. These states are implemented as ancillas for a deterministic non-Gaussian gate operation on a system of choice. We show that generating multimode states through this distribution scheme allows an enhancement of the output state to better approximate the nonlinear features. Finally, we consider methods of characterising non-Gaussian states. In particular, we introduce a witness for pure states existing outside of the Gaussian convex hull. Such states exclude Gaussian pure states as well as non-Gaussian states generated from mixtures of squeezed and coherent states, and therefore consist of non-Gaussian states generated from non-Gaussian operations. We present a detection-independent bound for such states based on the generalised quasiprobability distribution.
Single-photon characteristics of superposed weak coherent states
Creators: name: Lee, Seung-Woo
name: Kim, Jaewan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study a superposed weak coherent state that can fundamentally mimic an ideal single photon not only with respect to the number of photons but also in terms of an indeterminate phase. It is close to the single-photon state with high fidelity and exhibits fundamental features of single photons such as antibunching and Hong-Ou-Mandel interference. The emergence and vanishing of single-photon characteristics can be directly observed by changing two parameters, i.e., the mean photon number and number of phases. Our result shows that the uncertainty between the photon number and phase indeed constitutes the characteristics of single photons. Finally, we apply the superposed weak coherent state to quantum key distribution and demonstrate that it outperforms the typical approach using phase-randomized weak coherent states.
description: 8 pages, 5 figures, title and abstract changed, published version
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Cart. 190 (11 H 75), 316 folios, f. 0285r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: LaMOP

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0285r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0285r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v