cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Cart. 177 (11 H 289), 197 folios, f. 0248
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0248, 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. 177 (11 H 289), 197 folios, f. 0248, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Symphlebia creon Vincent & Laguerre 2013
Creators: name: Vincent, Benoît
name: Laguerre, Michel
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Arctiidae
Symphlebia
Symphlebia creon

description: Symphlebia creon (Druce, 1897) n. comb.
Amaxia creon Druce, 1897: 369.
Epimolis creon – Watson & Goodger 1986: 8.
Epimolis zatrephica Dyar, 1913: 286, n. syn.
ARGUMENTAIRE TAXONOMIQUE
Amaxia creon Druce, 1897 est décrit de Jalapa dans la province de Vera Cruz au Mexique, sur un mâle unique. Epimolis zatrephica Dyar, 1913 est décrit sur une unique femelle de Misantla de la même province de Vera Cruz. Dyar (1913) crée pour ce taxon le genre Epimolis. Or, après consultation d’importantes collections, dont les riches séries mexicaines conservées à l’USNM, nous n’avons jamais pu observer un spécimen femelle du taxon A. creon et aucun mâle du taxon E. zatrephica. Watson & Goodger (1986) remarquent leur similarité dans l’habitus et transfèrent le taxon creon du genre Amaxia vers le genre Epimolis. Ils n’ont pas jugé nécessaire de mettre les deux taxons en synonymie, peut-être afin d’éviter de rendre le genre Epimolis invalide. Ne pouvant comparer les genitalia des deux holotypes, nous aurions souhaité séquencer des spécimens mexicains des deux sexes. Bien que nous n’ayons pas eu la possibilité de séquencer des spécimens récents, nous décidons pourtant de rapprocher ces deux espèces, en nous basant uniquement sur leur habitus, en particulier un dimorphisme sexuel modéré, les ailes jaune vif avec une partie basale brun-rouge et une tache blanche plus trois taches apicales brun-rouge. De plus, l’analyse des genitalia mâles d’ A. creon permet d’associer ce spécimen au genre Symphlebia. Nous proposons donc cette synonymie, même si cette hypothèse devra être confirmée par l’examen de séquences moléculaires si des spécimens récents sont obtenus.
description: Published as part of Vincent, Benoît & Laguerre, Michel, 2013, Changements nomenclaturaux chez les Arctiinae nÉotropicales (Insecta, Lepidoptera, Erebidae); seconde partie, pp. 425-455 in Zoosystema 35 (3) on page 429, DOI: 10.5252/z2013n3a5, http://zenodo.org/record/5165260
On the scattering over the GKP vacuum
Creators: name: Fioravanti, Davide
name: Piscaglia, Simone
name: Rossi, Marco
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: By converting the Asymptotic Bethe Ansatz (ABA) of ${\cal N}=4$ SYM into non-linear integral equations, we find 2D scattering amplitudes of excitations on top of the GKP vacuum. We prove that this is a suitable and powerful set-up for the understanding and computation of the whole S-matrix. We show that all the amplitudes depend on the fundamental scalar-scalar one.
description: final version, 14 pages, to appear in Physics Letters B
The quasi-periodic quantum Ising transition in 1D
Creators: name: Crowley, P. J. D.
name: Chandran, A.
name: Laumann, C. R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Unlike random potentials, quasi-periodic modulation can induce localisation-delocalisation transitions in one dimension. In this article, we analyse the implications of this for symmetry breaking in the quasi-periodically modulated quantum Ising chain. Although weak modulation is irrelevant, strong modulation induces new ferromagnetic and paramagnetic phases which are fully localised and gapless. The quasi-periodic potential and localised excitations lead to quantum criticality that is intermediate to that of the clean and randomly disordered models with exponents of $ν=1^{+}$, and $z\approx 1.9$, $Δ_σ\approx 0.16$, $Δ_γ\approx 0.63$ (up to logarithmic corrections). Technically, the clean Ising transition is destabilized by logarithmic wandering of the local reduced couplings. We conjecture that the wandering coefficient $w$ controls the universality class of the quasi-periodic transition and show its stability to smooth perturbations that preserve the quasi-periodic structure of the model.
description: 11 pages, 6 figures
The Late Time Behavior of False Vacuum Decay: Possible Implications for Cosmology and Metastable Inflating States
Creators: name: Krauss, Lawrence M.
name: Dent, James
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We describe here how the late time behavior of the decaying states, which is predicted to deviate from an exponential form, while normally of insignificant consequence, may have important cosmological implications in the case of false vacuum decay. It may increase the likelihood of eternal inflation, and may help explain the likelihood of observing a small vacuum energy at late times, as well as arguing against decay into a large negative energy (anti-de Sitter space), vacuum state as has been motivated by some string theory considerations. Several interesting open questions are raised, including whether observing the cosmological configuration of a metastable universe can constrain its inferred lifetime.
description: 4 pages, submitted to PRL, one reference changed, and changes to abstract and concluding sentences to stem possible confusions regarding observation and metastability
Generative Model Selection Using a Scalable and Size-Independent Complex Network Classifier
Creators: name: Motallebi, Sadegh
name: Aliakbary, Sadegh
name: Habibi, Jafar
Publisher: name: arXiv
Year: 2013
Subjects: subject: Social and Information Networks (cs.SI)
subject: Machine Learning (cs.LG)
subject: Physics and Society (physics.soc-ph)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: Real networks exhibit nontrivial topological features such as heavy-tailed degree distribution, high clustering, and small-worldness. Researchers have developed several generative models for synthesizing artificial networks that are structurally similar to real networks. An important research problem is to identify the generative model that best fits to a target network. In this paper, we investigate this problem and our goal is to select the model that is able to generate graphs similar to a given network instance. By the means of generating synthetic networks with seven outstanding generative models, we have utilized machine learning methods to develop a decision tree for model selection. Our proposed method, which is named "Generative Model Selection for Complex Networks" (GMSCN), outperforms existing methods with respect to accuracy, scalability and size-independence.
Absorption spectrum of Ca atoms attached to $^4$He nanodroplets
Creators: name: Hernando, Alberto
name: Barranco, Manuel
name: Krośnicki, Marek
name: Mayol, Ricardo
name: Pi, Martí
Publisher: name: arXiv
Year: 2007
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Within density functional theory, we have obtained the structure of $^4$He droplets doped with neutral calcium atoms. These results have been used, in conjunction with newly determined {\it ab-initio} $^1Σ$ and $^1Π$ Ca-He pair potentials, to address the $4s4p$ $^1$P$_1 \leftarrow 4s^2$ $^1$S$_0$ transition of the attached Ca atom, finding a fairly good agreement with absorption experimental data. We have studied the drop structure as a function of the position of the Ca atom with respect of the center of mass of the helium moiety. The interplay between the density oscillations arising from the helium intrinsic structure and the density oscillations produced by the impurity in its neighborhood plays a role in the determination of the equilibrium state, and hence in the solvation properties of alkaline earth atoms. In a case of study, the thermal motion of the impurity within the drop surface region has been analyzed in a semi-quantitative way. We have found that, although the atomic shift shows a sizeable dependence on the impurity location, the thermal effect is statistically small, contributing by about a 10% to the line broadening. The structure of vortices attached to the calcium atom has been also addressed, and its effect on the calcium absorption spectrum discussed. At variance with previous theoretical predictions, we conclude that spectroscopic experiments on Ca atoms attached to $^4$He drops will be likely unable to detect the presence of quantized vortices in helium nanodrops.
description: 33 pages with 11 figures
Andromeda's Dust
Creators: name: Draine, B. T.
name: Aniano, G.
name: Krause, Oliver
name: Groves, Brent
name: Sandstrom, Karin
name: Braun, Robert
name: Leroy, Adam
name: Klaas, Ulrich
name: Linz, Hendrik
name: Rix, Hans-Walter
name: Schinnerer, Eva
name: Schmiedeke, Anika
name: Walter, Fabian
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Spitzer Space Telescope and Herschel Space Observatory imaging of M31 is used, with a physical dust model, to construct maps of dust surface density, dust-to-gas ratio, starlight heating intensity, and PAH abundance, out to R=25kpc. The global dust mass is M_d=5.4x10^7Msol, the global dust/H mass ratio is M_d/M_H=0.0081, and the global PAH abundance is =0.039. The dust surface density has an inner ring at R=5.6kpc, a maximum at R=11.2kpc, and an outer ring at R=15.1kpc. The dust/gas ratio varies from M_d/M_H=0.026 at the center to ~0.0027 at R=25kpc. From the dust/gas ratio, we estimate the ISM metallicity to vary by a factor ~10, from Z/Zsol=3 at R=0 to ~0.3 at R=25kpc. The dust heating rate parameter peaks at the center, with approx 35, declining to approx 0.25 at R=20kpc. Within the central kpc, the starlight heating intensity inferred from the dust modeling is close to what is estimated from the stars in the bulge. The PAH abundance reaches a peak q_PAH=0.045 at R=11.2kpc. When allowance is made for the different spectrum of the bulge stars, q_PAH for the dust in the central kpc is similar to the overall value of q_PAH in the disk. The silicate-graphite-PAH dust model used here is generally able to reproduce the observed dust spectral energy distribution across M31, but overpredicts 500um emission at R=2-6kpc, suggesting that at R=2-6kpc, the dust opacity varies more steeply with frequency (with beta approx 2.3 between 200 and 600um) than in the model
description: Final version (corrected and revised), to appear in ApJ, 780, 172 (2014 Jan 10)
Size Complexity of Volume Meshes vs. Surface Meshes
Creators: name: Benoit  Hudson
name: Miller, Gary L.
name: Phillips, Todd
name: Sheehy, Donald
Publisher: name: Carnegie Mellon University
Year: 1996
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Typical volume meshes in three dimensions are designed to conform to an underlying two-dimensional surface mesh, with volume mesh element size growing larger away from the surface. The surface mesh may be uniformly spaced or highly graded, and may have fine resolution due to extrinsic mesh size concerns. When we desire that such a volume mesh have good aspect ratio, we require that some space-filling scaffold vertices be inserted off the surface. We analyze the number of scaffold vertices in a setting that encompasses many existing volume meshing algorithms. We show that under simple preconditions, the number of scaffold vertices will be linear in the number of surface vertices.
Missing flux in VLBI observations of SiO maser at 7mm in IRC+10011
Creators: name: Desmurs, J. -F.
name: Alcolea, J.
name: Bujarrabal, V.
name: Colomer, F.
name: Soria-Ruiz, R.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: VLBI observations of SiO masers recover at most 40-50% of the total flux obtained by single dish observations at any spectral channel. Some previous studies seems to indicate that, at least, part of the lost flux is divided up into many weak components rather than in a large resolved emission area. Taking benefit of the high sensitivity and resolution of the HSA, we investigate the problem of the missing flux in VLBI observations of SiO maser emission at 7mm in the AGB stars and obtain a high dynamic range map of IRC+10011. We conclude that the missing flux is mostly contained in many very weak maser components.
description: 2 pages, 1 figure, to appear in proceedings of IAU Symposium 336 "Astrophysical Masers: Unlocking the Mysteries of the Universe", Editors: A. Tarchi, M. J. Reid & P. Castangia
Pseudepimolis arcifera Vincent & Laguerre 2013
Creators: name: Vincent, Benoît
name: Laguerre, Michel
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Erebidae
Pseudepimolis
Pseudepimolis arcifera

description: Pseudepimolis arcifera (Dognin, 1912) n. comb.
Neonerita arcifera Dognin, 1912: 129.
Epimolis arcifera – Watson & Goodger 1986: 9.
description: Published as part of Vincent, Benoît & Laguerre, Michel, 2013, Changements nomenclaturaux chez les Arctiinae nÉotropicales (Insecta, Lepidoptera, Erebidae); seconde partie, pp. 425-455 in Zoosystema 35 (3) on page 431, DOI: 10.5252/z2013n3a5, http://zenodo.org/record/5165260
Climate change and human health in sub-Saharan Africa: evidence mapping and interpretative review.
Creators: name: PROTUS MUSOTSI
name: Ouma, Luke
name: Manyara, Anthony Muchai
name: Gichunge, Catherine
name: Aduo-Adjei, Kofi
name: Kamya, Carol Nakaye
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Medicine and Health Sciences

description: Climate change is a global threat. Research on climate change and health is increasing in sub-Saharan Africa but few synthesis of current evidence have been conducted. This study aims to conduct evidence mapping and interpretative review to 1) explore the current scope of empirical studies on climate change and human health with regards to the WHO global research priorities for protecting human health from climate change in SSA (Phase 1 – evidence mapping); 2) comprehensively collate potential climate change causal pathways of NCDs in SSA (Phase 2 – interpretative review). Related research questions will be: 1) How does current empirical evidence on climate change and human health in SSA map onto the WHO global research priorities?; and 2) Based on known NCD risk factors, how might climate change exacerbate their occurrence?
Stellar Halos in Illustris- Probing the Histories of Milky Way-Mass Galaxies
Creators: name: Elias, Lydia M.
name: Sales, Laura V.
name: Creasey, Peter
name: Cooper, Michael C.
name: Bullock, James S.
name: Rich, Michael R.
name: Hernquist, Lars
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The existence of stellar halos around galaxies is a natural prediction of the hierarchical nature of the LambdaCDM model. Recent observations of Milky Way-like galaxies have revealed a wide range in stellar halo mass, including cases with no statistically significant detection of a stellar halo, as in the case of M101, NGC3351 and NGC1042. We use the Illustris simulation to investigate the scatter in stellar halo content and, in particular, to study the formation of galaxies with the smallest fraction of this diffuse component. Stellar halos are far from spherical, which diminishes the surface brightness of the stellar halo for face-on disks. Once accounting for projection effects, we find that the stellar halo fraction f_SH correlates strongly with galaxy morphology and star formation rate, but not with environment, in agreement with observations. Galaxies with the lowest stellar halo fractions are disk-dominated, star-forming and assemble their dark matter halos on average earlier than galaxies with similar stellar masses. Accreted satellites are also lower in stellar mass and have earlier infall times than centrals with high f_SH. In situ rather than accreted stars dominate the stellar halos of galaxies with the lowest stellar halo fractions, with a transition radius from in situ to accretion-dominated r~45 kpc. Our results extrapolated to real galaxies such as M101 may indicate that these galaxies inhabit old halos which endured mergers only at higher redshifts and evolved relatively unperturbed in the last ~10 Gyrs.
description: 13 pages, 12 figures
title: ADCO, Cartulaire de Cîteaux pour la grange et seigneurie d'Ouges (XVe siècle), Cart. 173 (11 H 939), 226 folios, f. 0036
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Cîteaux pour la grange et seigneurie d'Ouges (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 173 (11 H 939), 226 folios, f. 0036, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour la grange et seigneurie d'Ouges (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 173 (11 H 939), 226 folios, f. 0036, 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
Pseudepimolis marpessa Vincent & Laguerre 2013
Creators: name: Vincent, Benoît
name: Laguerre, Michel
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Erebidae
Pseudepimolis
Pseudepimolis marpessa

description: Pseudepimolis marpessa (Druce, 1906) n. comb.
Idalus marpessa Druce, 1906: 407.
Epimolis marpesa – Watson & Goodger 1986: 9.
description: Published as part of Vincent, Benoît & Laguerre, Michel, 2013, Changements nomenclaturaux chez les Arctiinae nÉotropicales (Insecta, Lepidoptera, Erebidae); seconde partie, pp. 425-455 in Zoosystema 35 (3) on page 430, DOI: 10.5252/z2013n3a5, http://zenodo.org/record/5165260
Time reversal symmetry breakdown in normal and superconducting states in frustrated three-band systems
Creators: name: Bojesen, Troels
name: Babaev, Egor
name: Sudbø, Asle
Publisher: name: arXiv
Year: 2013
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We discuss the phase diagram and phase transitions in $U(1)\times \groupZ{2}$ three-band superconductors with broken time reversal symmetry. We find that beyond mean field approximation and for sufficiently strong frustration of interband interactions there appears an unusual metallic state precursory to a superconducting phase transition. In that state, the system is not superconducting. Nonetheless, it features a spontaneously broken $\groupZ{2}$ time reversal symmetry. By contrast, for weak frustration of interband coupling the energy of a domain wall between different $\groupZ{2}$ states is low and thus fluctuations restore broken time reversal symmetry in the superconducting state at low temperatures.
description: 4 pages, 4 figures (In addition, 2 pages of supplementary material with 2 figures). V2, published version
Size Competitive Meshing without Large Angles
Creators: name: Miller, Gary L.
name: Phillips, Todd
name: Sheehy, Donald
Publisher: name: Carnegie Mellon University
Year: 1995
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: We present a new meshing algorithm for the plane, Overlay Stitch Meshing (OSM), accepting as input an arbitrary Planar Straight Line Graph and producing a triangulation with all angles smaller than 170°. The output triangulation has competitive size with any optimal size mesh having equally bounded largest angle. The competitive ratio is O(log(L/s)) where L and s are respectively the largest and smallest features in the input. OSM runs in O(n log(L/s) + m) time/work where n is the input size and m is the output size. The algorithm first uses Sparse Voronoi Refinement to compute a quality overlay mesh of the input points alone. This triangulation is then combined with the input edges to give the final mesh.
Hybrid Higgs Inflation: The Use of Disformal Transformation
Creators: name: Sato, Seiga
name: Maeda, Kei-ichi
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We propose a hybrid type of the conventional Higgs inflation and new Higgs inflation models. We perform a disformal transformation into the Einstein frame and analyze the background dynamics and the cosmological perturbations in the truncated model, in which we ignore the higher-derivative terms of the Higgs field. From the observed power spectrum of the density perturbations, we obtain the constraint on the non-minimal coupling constant $ξ$ and the mass parameter $M$ in the derivative coupling. Although the primordial tilt $n_s$ in the hybrid model barely changes, the tensor-to-scalar ratio $r$ moves from the value in new Higgs inflationary model to that in the conventional Higgs inflationary model as $|ξ|$ increases. We confirm our results by numerical analysis by ADM formalism of the full theory in the Jordan frame.
description: 16 pages, 6 figures, 1 table
Pseudepimolis incisa Vincent & Laguerre 2013
Creators: name: Vincent, Benoît
name: Laguerre, Michel
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Erebidae
Pseudepimolis
Pseudepimolis incisa

description: Pseudepimolis incisa(Rothschild, 1909)
n. comb.
Prumala incisa Rothschild, 1909: 25.
Eupseudosoma parapessa Dognin, 1911: 9, synonymie dans Watson & Goodger 1986: 8.
Aphyle intorta Schaus, 1910: 402, synonymie dans Watson & Goodger 1986: 9.
Epimolis incisa – Watson & Goodger 1986: 9.
description: Published as part of Vincent, Benoît & Laguerre, Michel, 2013, Changements nomenclaturaux chez les Arctiinae nÉotropicales (Insecta, Lepidoptera, Erebidae); seconde partie, pp. 425-455 in Zoosystema 35 (3) on page 430, DOI: 10.5252/z2013n3a5, http://zenodo.org/record/5165260
Flavor Violating Higgs signals in the Texturized Two-Higgs Doublet Model (2HDM-Tx)
Creators: name: Arroyo-Ureña, M. A.
name: Diaz-Cruz, J. Lorenzo
name: Diaz, Enrique
name: Orduz-Ducuara, Javier A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Flavor violating Higgs signals, such as the top FCNC decay $t\to ch^0$ and the LFV Higgs decay $h^0\to τμ$, have been studied at the LHC. These signals can arise within the general Two-Higgs doublet model (THDM), where each Higgs doublet couples to all fermions types through Yukawa matrices $Y^f_1$ and $Y^f_2$. The Yukawa matrices can be assumed to have the same form or they could have different structures. In this paper we study the case when both $Y^f_1$ and $Y^f_2$ have completely different forms, but in such a way that they complement to produce a specific hermitian mass matrix. We find that for specific four-zero textures, the Flavor Violating Higgs couplings depend only on the free parameters $\tan β$, $γ_f$ and the fermion masses. We use the current bounds on the low energy processes, to derive constraints on the Heavy Higgs boson mass, $\tan β$ and $γ_f$. Then, we use these constraints to evaluate the LFV Higgs decays, which reach Branching ratios that could be tested at the LHC.
description: Version to be published in Chinese Physics C
Size and access inference for data-parallel programs
Creators: name: Siddhartha  Chatterjee
name: Blelloch, Guy E.
name: Fisher, Allan L.
Publisher: name: Carnegie Mellon University
Year: 2009
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Abstract: "Data-parallel programming languages have many desirable features, such as single-thread semantics and the ability to express fine-grained parallelism. However, it is challenging to implement such languages efficiently on conventional MIMD multiprocessors, because these machines incur a high overhead for small grain sizes. This paper presents compile-time analysis techniques for data-parallel program graphs that reduce these overheads in two ways: by stepping up the grain size, and by relaxing the synchronous nature of the computation without altering the program semantics.The algorithms partition the program graph into clusters of nodes such that all nodes in a cluster have the same loop structure, and futher refine these clusters into epochs based on generation and consumption patterns of data vectors. This converts the fine-grain parallelism in the original program to medium-grain loop parallelism, which is better suited to MIMD machines. A compiler has been implemented based on these ideas. We present performance results for data-parallel kernels analyzed by the compiler and converted to single-program multiple-data (SPMD) code running on an Encore Multimax."
C-projective symmetries of submanifolds in quaternionic geometry
Creators: name: Borówka, Aleksandra
name: Winther, Henrik
Publisher: name: arXiv
Year: 2018
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 58D19, 53B15, 53A20, 53C28

description: The generalized Feix--Kaledin construction shows that c-projective $2n$-manifolds with curvature of type $(1,1)$ are precisely the submanifolds of quaternionic $4n$-manifolds which are fixed points set of a special type of quaternionic $S^1$ action $v$. In this paper, we consider this construction in the presence of infinitesimal symmetries of the two geometries. First, we prove that the submaximally symmetric c-projective model with type $(1,1)$ curvature is a submanifold of a submaximally symmetric quaternionic model, and show how this fits into the construction. We give conditions for when the c-projective symmetries extend from the fixed points set of $v$ to quaternionic symmetries, and we study the quaternionic symmetries of the Calabi-- and Eguchi-Hanson hyperkähler structures, showing that in some cases all quaternionic symmetries are obtained in this way.
Auditing: Active Learning with Outcome-Dependent Query Costs
Creators: name: Sabato, Sivan
name: Sarwate, Anand D.
name: Srebro, Nathan
Publisher: name: arXiv
Year: 2013
Subjects: subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: We propose a learning setting in which unlabeled data is free, and the cost of a label depends on its value, which is not known in advance. We study binary classification in an extreme case, where the algorithm only pays for negative labels. Our motivation are applications such as fraud detection, in which investigating an honest transaction should be avoided if possible. We term the setting auditing, and consider the auditing complexity of an algorithm: the number of negative labels the algorithm requires in order to learn a hypothesis with low relative error. We design auditing algorithms for simple hypothesis classes (thresholds and rectangles), and show that with these algorithms, the auditing complexity can be significantly lower than the active label complexity. We also discuss a general competitive approach for auditing and possible modifications to the framework.
description: Corrections in section 5
Risk of bias- Use of CRISPR technology in gene editing for tolerance to biotic factors in plants: A systematic review
Creators: name: Marcelly Santana Mascarenhas, Fernanda dos Santos Nascimento, Anelita de Jesus Rocha, Mileide dos Santos Ferreira, Wanderley Diaciso, Lucymeire Moraes Lino, Tiago Antônio de Oliveira Mendes, Claudia Fortes Ferreira, Janay Almeida dos Santos Serejo, Edson Perito Amorim
Publisher: name: Zenodo
Year: 2024

description: This article is a systematic review of studies carried out over the last eight years on the use of CRISPR technology in gene editing for resistance to biotic factors in plants
Discovery of two neighboring satellites in the Carina constellation with MagLiteS
Creators: name: Torrealba, G.
name: Belokurov, V.
name: Koposov, S. E.
name: Bechtol, K.
name: Drlica-Wagner, A.
name: Olsen, K. A. G.
name: Vivas, A. K.
name: Yanny, B.
name: Jethwa, P.
name: Walker, A. R.
name: Li, T. S.
name: Allam, S.
name: Conn, B. C.
name: Gallart, C.
name: Gruendl, R. A.
name: James, D. J.
name: Johnson, M. D.
name: Kuehn, K.
name: Kuropatkin, N.
name: Martin, N. F.
name: Martinez-Delgado, D.
name: Nidever, D. L.
name: Noël, N. E. D.
name: Simon, J. D.
name: Stringfellow, G. S.
name: Tucker, D. L.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the discovery of two ultra-faint satellites in the vicinity of the Large Magellanic Cloud (LMC) in data from the Magellanic Satellites Survey (MagLiteS). Situated 18$^{\circ}$ ($\sim 20$ kpc) from the LMC and separated from each other by only $18^\prime$, Carina~II and III form an intriguing pair. By simultaneously modeling the spatial and the color-magnitude stellar distributions, we find that both Carina~II and Carina~III are likely dwarf galaxies, although this is less clear for Carina~III. There are in fact several obvious differences between the two satellites. While both are well described by an old and metal poor population, Carina~II is located at $\sim 36$ kpc from the Sun, with $M_V\sim-4.5$ and $r_h\sim 90$ pc, and it is further confirmed by the discovery of 3 RR Lyrae at the right distance. In contrast, Carina~III is much more elongated, measured to be fainter ($M_V\sim-2.4$), significantly more compact ($r_h\sim30$ pc), and closer to the Sun, at $\sim 28$ kpc, placing it only 8 kpc away from Car~II. Together with several other systems detected by the Dark Energy Camera, Carina~II and III form a strongly anisotropic cloud of satellites in the vicinity of the Magellanic Clouds.
description: 14 pages, 7 figures. Accepted for publication in MNRAS
Siri : a constrained-object language for reactive program implementation
Creators: name: Horn, Bruce L.
Publisher: name: Carnegie Mellon University
Year: 2004
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Abstract: "Siri is a small language intended to simplify the design and implementation of programs with graphical user interfaces such as those available for the Apple Macintosh. The interfaces for such programs are usually based on three concepts: accurate and appealing visual metaphors, interaction by direct manipulation, and immediate reflection of changes in the data. Programs based on these concepts are called reactive, after Alan Kay's Reactive Engine [Kay69]. A well-designed reactive program maintains an internal model that is kept consistent with an end user model. The end user's model is created and modified by direct manipulation, using an input device such as a mouse to alter a visual representation.This puts the user in control, rather than the computer. Implementing reactive programs is difficult, due to computational mechanisms that are rarely supported in existing programming languages. Siri addresses these needs in a simple and uniform way. The declarative nature of Siri bypasses many issues of control flow; dependency networks and constraint satisfaction will transparently sequence updates. Siri's single abstraction mechanism, the constraint pattern, supports multiple object views simultaneously; seperate hierarchies for visual layout, encapsulation, and class/subclass; and multiple concurrent objects.In addition, Siri will provide a straightforward framework for creation and composition of Siri programs using direct manipulation."
The three-loop beta-function of SU(N) lattice gauge theories with overlap fermions
Creators: name: Constantinou, Martha
name: Panagopoulos, Haralambos
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We briefly report our calculation of the 2-loop coefficient of the coupling constant renormalization function Z_g in lattice perturbation theory. The quantity under study is defined through g_0 = Z_g g, where g_0 (g) is the bare (renormalized) coupling constant. The 2-loop expression for Z_g can be directly related to the 3-loop bare beta-function beta_L(g_0). Our calculation is performed using overlap fermions and Wilson gluons, and the background field technique has been chosen for convenience. Our results depend explicitly on the number of fermion flavors (N_f) and colors (N). Since the dependence of Z_g on the overlap parameter rho cannot be extracted analytically, we tabulate our results for different values of rho in the allowed range (0
description: 7 pages, 1 table, 4 figures. Presented at the XXV International Symposium on Lattice Field Theory, Regensburg, Germany
Simultaneous Source Location
Creators: name: Andreev, Konstantin
name: Garrod, Charles
name: Maggs, Bruce M
name: Meyerson, Adam
Publisher: name: Carnegie Mellon University
Year: 2004
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: We consider the problem of Simultaneous Source Location – selecting locations for sources in a capacitated graph such that a given set of demands can be satisfied. We give an exact algorithm for trees and show how this can be combined with a result of Räcke to give a solution that exceeds edge capacities by at most O(log2n log logn), where n is the number of nodes. On graphs of bounded treewidth, we show the problem is still NP-Hard, but we are able to give a PTAS with at most O(1+ε) violation of the capacities, or a (k+1)-approximation with exact capacities, where k is the treewidth and ε can be made arbitrarily small.
Spin-orbit torques in NbSe$_2$/Permalloy bilayers
Creators: name: Guimaraes, Marcos H. D.
name: Stiehl, Gregory M.
name: MacNeill, David
name: Reynolds, Neal D.
name: Ralph, Daniel C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We present measurements of current-induced spin-orbit torques generated by NbSe$_2$, a fully-metallic transition-metal dichalcogenide material, made using the spin-torque ferromagnetic resonance (ST-FMR) technique with NbSe$_{2}$/Permalloy bilayers. In addition to the out-of-plane Oersted torque expected from current flow in the metallic NbSe$_{2}$ layer, we also observe an in-plane antidamping torque with torque conductivity $σ_{S} \approx 10^{3} (\hbar / 2e)$($Ω$m)$^{-1}$ and indications of a weak field-like contribution to the out-of-plane torque oriented opposite to the Oersted torque. Furthermore, in some samples we also measure an in-plane field-like torque with the form $\hat{m} \times \hat{z}$, where $\hat{m}$ is the Permalloy magnetization direction and $\hat{z}$ is perpendicular to the sample plane. The size of this component varies strongly between samples and is not correlated with the NbSe$_{2}$ thickness. A torque of this form is not allowed by the bulk symmetries of NbSe$_{2}$, but is consistent with symmetry breaking by a uniaxial strain that might result during device fabrication.
description: 14 pages, 3 figures
Robust Extraction of Tomographic Information via Randomized Benchmarking
Creators: name: Kimmel, Shelby
name: da Silva, Marcus P.
name: Ryan, Colm A.
name: Johnson, Blake R.
name: Ohki, Thomas
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We describe how randomized benchmarking can be used to reconstruct the unital part of any trace-preserving quantum map, which in turn is sufficient for the full characterization of any unitary evolution, or more generally, any unital trace-preserving evolution. This approach inherits randomized benchmarking's robustness to preparation, measurement, and gate imperfections, therefore avoiding systematic errors caused by these imperfections. We also extend these techniques to efficiently estimate the average fidelity of a quantum map to unitary maps outside of the Clifford group. The unitaries we consider correspond to large circuits commonly used as building blocks to achieve scalable, universal, and fault-tolerant quantum computation. Hence, we can efficiently verify all such subcomponents of a circuit-based universal quantum computer. In addition, we rigorously bound the time and sampling complexities of randomized benchmarking procedures, proving that the required non-linear estimation problem can be solved efficiently.
description: v1: 13 pages, 2 figures v2: Update to published version, including correction to proof in Appendix C
Simultaneous source location
Creators: name: Andreev, Konstantin
Publisher: name: Carnegie Mellon University
Year: 2005
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Abstract: "We consider the problem of Simultaneous Source Location -- selecting locations for sources in a capacitated graph such that a given set of demands can be satisfied. We give an exact algorithm for trees and show how this can be combined with a result of Ra╠êcke to give a solution that exceeds edge capacities by at most O(log n log log n), where n is the number of nodes. On graphs of bounded treewidth, we show the problem is still NP-Hard, but we are able to give a PTAS with at most O(1 + [epsilon]) violation of the capacities, or a (k + 1)-approximation with exact capacities, where k is the treewidth and [epsilon] can be made arbitrarily small."
Particles Systems for Mean Reflected BSDEs
Creators: name: Briand, Philippe
name: Hibon, Hélène
Publisher: name: arXiv
Year: 2017
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics

description: In this paper, we deal with Reflected Backward Stochastic Differential Equations for which the constraint is not on the paths of the solution but on its law as introduced by Briand, Elie and Hu in [3]. We extend the recent work [2] of Briand, Chaudru de Raynal, Guillin and Labart on the chaos propagation for mean reflected SDEs to the backward framework. When the driver does not depend on z, we are able to treat general reflexions for the particles system. We consider linear reflexion when the driver depends also on z. In both cases, we get the rate of convergence of the particles system towards the square integrable deterministic flat solution to the mean reflected BSDE.
Symphlebia venusta
Creators: name: Vincent, Benoît
name: Laguerre, Michel
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Arctiidae
Symphlebia
Symphlebia venusta

description: Symphlebia venusta (Dognin, 1921)
Prumala venusta Dognin, 1921: 2.
Symphlebia venusta – Watson & Goodger 1986: 8.
Prumala foliosa Seitz, 1921: 345, n. syn.
Symphlebia foliosa – Watson & Goodger 1986: 8.
ARGUMENTAIRE TAXONOMIQUE
Prumala foliosa Seitz, 1921 est décrit du Rio Songo, département de la Paz, en Bolivie. Prumala venusta Dognin, 1921 est décrit de la même localité type et présente la même coloration fondamentale verte. Les deux espèces ont été placées dans le genre Symphlebia par Watson & Goodger (1986). Les spécimens types, respectivement conservés au BMNH et à l’USNM, sont parfaitement identiques et il s’agit incontestablement de la même espèce. La description originale de Dognin (1921) est publiée le 8 juillet 1921. Pour le célèbre ouvrage de Seitz (1919 -1925) Die Gross-Schmetterlinge der Erde, Griffin (1936) propose à la page de description de l’espèce Symphlebia foliosa, la date de publication du 3 décembre 1921. Nous proposons donc cette synonymie.
description: Published as part of Vincent, Benoît & Laguerre, Michel, 2013, Changements nomenclaturaux chez les Arctiinae nÉotropicales (Insecta, Lepidoptera, Erebidae); seconde partie, pp. 425-455 in Zoosystema 35 (3) on page 430, DOI: 10.5252/z2013n3a5, http://zenodo.org/record/5165260
Quantum criticality in the pseudogap Bose-Fermi Anderson and Kondo models: Interplay between fermion- and boson-induced Kondo destruction
Creators: name: Pixley, J. H.
name: Kirchner, Stefan
name: Ingersent, Kevin
name: Si, Qimiao
Publisher: name: arXiv
Year: 2013
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We address the phenomenon of critical Kondo destruction in pseudogap Bose-Fermi Anderson and Kondo quantum impurity models. These models describe a localized level coupled both to a fermionic bath having a density of states that vanishes like |ε|^r at the Fermi energy (ε=0) and, via one component of the impurity spin, to a bosonic bath having a sub-Ohmic spectral density proportional to |ω|^s. Each bath is capable by itself of suppressing the Kondo effect at a continuous quantum phase transition. We study the interplay between these two mechanisms for Kondo destruction using continuous-time quantum Monte Carlo for the pseudogap Bose-Fermi Anderson model with 0
description: 16 pages, 16 figures. Replaced with published version, added discussion of particle hole asymmetry
ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
Creators: name: Amvrosiadis, A.
name: Eales, S. A.
name: Negrello, M.
name: Marchetti, L.
name: Smith, M. W. L.
name: Bourne, N.
name: Clements, D. L.
name: De Zotti, G.
name: Dunne, L.
name: Dye, S.
name: Furlanetto, C.
name: Ivison, R. J.
name: Maddox, S.
name: Valiante, E.
name: Baes, M.
name: Baker, A. J.
name: Cooray, A.
name: Crawford, S. M.
name: Frayer, D.
name: Harris, A.
name: Michałowski, M. J.
name: Nayyeri, H.
name: Oliver, S.
name: Riechers, D. A.
name: Serjeant, S.
name: Vaccari, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: With the advent of wide-area submillimeter surveys, a large number of high-redshift gravitationally lensed dusty star-forming galaxies (DSFGs) has been revealed. Due to the simplicity of the selection criteria for candidate lensed sources in such surveys, identified as those with $S_{500μm} > 100$ mJy, uncertainties associated with the modelling of the selection function are expunged. The combination of these attributes makes submillimeter surveys ideal for the study of strong lens statistics. We carried out a pilot study of the lensing statistics of submillimetre-selected sources by making observations with the Atacama Large Millimetre Array (ALMA) of a sample of strongly-lensed sources selected from surveys carried out with the Herschel Space Observatory. We attempted to reproduce the distribution of image separations for the lensed sources using a halo mass function taken from a numerical simulation which contains both dark matter and baryons. We used three different density distributions, one based on analytical fits to the halos formed in the EAGLE simulation and two density distributions (Singular Isothermal Sphere (SIS) and SISSA) that have been used before in lensing studies. We found that we could reproduce the observed distribution with all three density distributions, as long as we imposed an upper mass transition of $\sim$$10^{13} M_{\odot}$ for the SIS and SISSA models, above which we assumed that the density distribution could be represented by an NFW profile. We show that we would need a sample of $\sim$500 lensed sources to distinguish between the density distributions, which is practical given the predicted number of lensed sources in the Herschel surveys.
description: 14 pages, 7 figures, accepted for publication in MNRAS
Resonance widths in open microwave cavities studied by harmonic inversion
Creators: name: Kuhl, U.
name: Hoehmann, R.
name: Main, J.
name: Stoeckmann, H. -J.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: From the measurement of a reflection spectrum of an open microwave cavity the poles of the scattering matrix in the complex plane have been determined. The resonances have been extracted by means of the harmonic inversion method. By this it became possible to resolve the resonances in a regime where the line widths exceed the mean level spacing up to a factor of 10, a value inaccessible in experiments up to now. The obtained experimental distributions of line widths were found to be in perfect agreement with predictions from random matrix theory when wall absorption and fluctuations caused by couplings to additional channels are considered.
description: 4 pages, 6 figures