cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Nature, Aesthetics, and Ecological Ethics: Michael Northcott, and Robert Doran in Dialogue
Creators: name: Whelan, Gerard
Publisher: name: Mimesis Edizioni
Year: 2019

description: This issue of “Filosofia” is dedicated to the theme “Images of Nature”. While issuing the call for papers, the editor explained the choice of the theme as follows: “the problem of ecological crisis that arises nowadays has forced philosophy to break out of the classic schemes of modernity, developing new categories and a renewed philosophy of nature”. The editor adds: “nature becomes a thought-laboratory, from which to think new ethical, political, aesthetic, and metaphysical perspectives”. In this article, I introduce the thought of two thinkers who exhibit the characteristics identified by the editor. The first is Michael Northcott, an important English-speaking ecological ethicist; the second is Robert Doran, a Jesuit theologian, whose critical realist thought can help to provide foundations for the orientations found in Northcott. Taken together, their reflections are worthy of consideration by those who consider their thought as a renewal of the philosophy of nature for nowadays.
description: "Filosofia", N. 64 (2019): Immagini della natura
J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817
Creators: name: Utsumi, Yousuke
name: Tanaka, Masaomi
name: Tominaga, Nozomu
name: Yoshida, Michitoshi
name: Barway, Sudhanshu
name: Nagayama, Takahiro
name: Zenko, Tetsuya
name: Aoki, Kentaro
name: Fujiyoshi, Takuya
name: Furusawa, Hisanori
name: Kawabata, Koji S.
name: Koshida, Shintaro
name: Lee, Chien-Hsiu
name: Morokuma, Tomoki
name: Motohara, Kentaro
name: Nakata, Fumiaki
name: Ohsawa, Ryou
name: Ohta, Kouji
name: Okita, Hirofumi
name: Tajitsu, Akito
name: Tanaka, Ichi
name: Terai, Tsuyoshi
name: Yasuda, Naoki
name: Abe, Fumio
name: Asakura, Yuichiro
name: Bond, Ian A.
name: Miyazaki, Shota
name: Sumi, Takahiro
name: Tristram, Paul J.
name: Honda, Satoshi
name: Itoh, Ryosuke
name: Itoh, Yoichi
name: Kawabata, Miho
name: Morihana, Kumiko
name: Nagashima, Hiroki
name: Nakaoka, Tatsuya
name: Ohshima, Tomohito
name: Takahashi, Jun
name: Takayama, Masaki
name: Aoki, Wako
name: Baar, Stefan
name: Doi, Mamoru
name: Finet, François
name: Kanda, Nobuyuki
name: Kawai, Nobuyuki
name: Kim, Ji Hoon
name: Kuroda, Daisuke
name: Liu, Wei
name: Matsubayashi, Kazuya
name: Murata, Katsuhiro L.
name: Nagai, Hiroshi
name: Saito, Tomoki
name: Saito, Yoshihiko
name: Sako, Shigeyuki
name: Sekiguchi, Yuichiro
name: Tamura, Yoichi
name: Tanaka, Masayuki
name: Uemura, Makoto
name: Yamaguchi, Masaki S.
name: collaboration, the J-GEM
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The first detected gravitational wave from a neutron star merger was GW170817. In this study, we present J-GEM follow-up observations of SSS17a, an electromagnetic counterpart of GW170817. SSS17a shows a 2.5-mag decline in the $z$-band from 1.7 days to 7.7 days after the merger. Such a rapid decline is not comparable with supernovae light curves at any epoch. The color of SSS17a also evolves rapidly and becomes redder for later epochs; the $z-H$ color changed by approximately 2.5 mag in the period of 0.7 days to 7.7 days. The rapid evolution of both the optical brightness and the color are consistent with the expected properties of a kilonova that is powered by the radioactive decay of newly synthesized $r$-process nuclei. Kilonova models with Lanthanide elements can reproduce the aforementioned observed properties well, which suggests that $r$-process nucleosynthesis beyond the second peak takes place in SSS17a. However, the absolute magnitude of SSS17a is brighter than the expected brightness of the kilonova models with the ejecta mass of 0.01 $\Msun$, which suggests a more intense mass ejection ($\sim 0.03 \Msun$) or possibly an additional energy source.
description: 7 pages, 5 figures. Published in PASJ (Publications of the Astronomical Society of Japan)
Moduli Space of Torsional Manifolds
Creators: name: Becker, Melanie
name: Tseng, Li-Sheng
name: Yau, Shing-Tung
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We characterize the geometric moduli of non-Kaehler manifolds with torsion. Heterotic supersymmetric flux compactifications require that the six-dimensional internal manifold be balanced, the gauge bundle be hermitian Yang-Mills, and also the anomaly cancellation be satisfied. We perform the linearized variation of these constraints to derive the defining equations for the local moduli. We explicitly determine the metric deformations of the smooth flux solution corresponding to a torus bundle over K3.
description: 23 pages, harvmac; v2: typos corrected, minor clarifications, reference added
Lingua vivente, materia di fuoco. Michelstaedter, la Cabala e Spinoza
Creators: name: Pardi, Aldo
Publisher: name: Mimesis Edizioni
Year: 2019

description: The topic of the paper is an inquiry about Carlo Michelstaedter’s reference to the Kabbalah, and the relationship existing between his attention for Jewish mystic and his reference to Spinoza’s philosophy. In a letter sent to his friend Chiavacci, Michelstaedter quotes in a sentence about mystic both Kabbalah and Spinoza. Analyzing this passage, where Nietzsche is quoted too, the paper discusses Michelstaedter’s reference to the Kabbalah, through Spinoza, about the problem of the philosophical statute of language and the nature of his orders, so central for his theoretical research concerning the conditions of reality and the dispositions of its moments.
description: "Filosofia", N. 64 (2019): Immagini della natura
title: ADCO, Cartulaire de Fontenay, premier fragment (XIIIe siècle), Cart. 201 (15 H 9), 175 folios, f. 016v
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2009
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP

description: Cartulaire de Fontenay, premier fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), 175 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Fontenay, premier fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), 175 folios, f. 016v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb119679755
description: Provenance: https://www.geonames.org/7874015
description: Provenance: http://www.idref.fr/027691802/id
description: Provenance: abbaye de Fontenay
description: Provenance: http://www.wikidata.org/entity/Q464918
Il complotto interiore. Affrontare le nuove forme di alienazione
Creators: name: Lomartire, Alessandro
Publisher: name: Mimesis Edizioni
Year: 2019

description: Il Pendolo di Foucault was published in 1988, and was immediately available in every bookshop. The plot tells the story of an apparent universal conspiracy which then turns out to be only a great misunderstanding. Thirty years later we realize that the phenomenon of good plot for a novel has become more and more widespread, invading fields unimaginable until recent times such as politics and the intellectual community. But what is a conspiracy theory? What kind of people believe in it? How to face this rising phenomenon and its implications? Recent studies on conspiracy theory and the work of Castoriadis suggest an answer to all these questions: revitalizing Democracy and educating people to autonomy.
description: "Filosofia", N. 64 (2019): Immagini della natura
Additional file 2: of Outdoor air pollution, green space, and cancer incidence in Saxony: a semi-individual cohort study
Creators: name: Datzmann, Thomas
name: Markevych, Iana
name: Trautmann, Freya
name: Heinrich, Joachim
name: Schmitt, Jochen
name: Tesch, Falko
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Computational Biology

description: Table S1. ICD-10 Codes; Analyzed cancer entities and corresponding ICD-10-GM codes are shown. (DOCX 12 kb)
Power Supply Options for a Naval Railgun
Creators: name: Hundertmark, Stephan
name: Liebfried, Oliver
Publisher: name: arXiv
Year: 2017
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Applied Physics (physics.app-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Large railguns require powerful power supply units. At the French-German Research Institute of Saint-Louis (ISL) most experimental railguns are driven by power supply units based on capacitors. Recent investigations at ISL explore the possibility to use coil based systems to increase the energy density of the power supply. In this study an electrical circuit simulation is used to investigate the difference for railgun operation in between a capacitor and a coil based power supply with respect to current amplitude behavior and projectile velocity. For this a scenario of a 25 MJ muzzle energy railgun is simulated with two different power supply options, replacing capacitors by coils and using a range of circuit resistances. The resistance determines to a large part the losses of the system and defines therefore the efficiency of the launch and the size of the power supply. The interpretation of the results of the performed simulations leads to the conclusion that the capacitor based system "naturally" pro- duces a favorable current pulse trace with respect to launching a mechanical delicate payload. Further simulations show that the disadvantage of the inductor based supply can be mitigated by increasing the power supply unit subdivision into smaller units.
description: Submitted to IEEE Transactions on Plasma Physics
title: 01_1969
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Histogram-based approach for docking parameters optimization
Creators: name: Kravchenko, Anna
name: Smail-Tabbone, Malika
name: de Vries, Sjoerd Jacob
name: de Beauchene, Isaure Chauvot
Publisher: name: Zenodo
Year: 2021
Subjects: docking
ssRNA-protein
histogram
fragment-based

description: This poster was presented at the SCS 2021 Virtual Conference on 23rd-24th July 2021.
The unpolarized macronova associated with the gravitational wave event GW170817
Creators: name: Covino, S.
name: Wiersema, K.
name: Fan, Y. Z.
name: Toma, K.
name: Higgins, A. B.
name: Melandri, A.
name: D'Avanzo, P.
name: Mundell, C. G.
name: Palazzi, E.
name: Tanvir, N. R.
name: Bernardini, M. G.
name: Branchesi, M.
name: Brocato, E.
name: Campana, S.
name: Alighieri, S. di Serego
name: Gotz, D.
name: Fynbo, J. P. U.
name: Gao, W.
name: Gomboc, A.
name: Gompertz, B.
name: Greiner, J.
name: Hjorth, J.
name: Jin, Z. P.
name: Kaper, L.
name: Klose, S.
name: Kobayashi, S.
name: Kopac, D.
name: Kouveliotou, C.
name: Levan, A. J.
name: Mao, J.
name: Malesani, D.
name: Pian, E.
name: Rossi, A.
name: Salvaterra, R.
name: Starling, R. L. C.
name: Steele, I.
name: Tagliaferri, G.
name: Troja, E.
name: van der Horst, A. J.
name: Wijers, R. A. M. J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The merger of two dense stellar remnants including at least one neutron star (NS) is predicted to produce gravitational waves (GWs) and short duration gamma ray bursts (GRBs). In the process, neutron-rich material is ejected from the system and heavy elements are synthesized by r-process nucleosynthesis. The radioactive decay of these heavy elements produces additional transient radiation termed "kilonova" or "macronova". We report the detection of linear optical polarization P = (0.50 +/- 0.07)% at 1.46 days after detection of the GWs from GW170817, a double neutron star merger associated with an optical macronova counterpart and a short GRB. The optical emission from a macronova is expected to be characterized by a blue, rapidly decaying, component and a red, more slowly evolving, component due to material rich of heavy elements, the lanthanides. The polarization measurement was made when the macronova was still in its blue phase, during which there is an important contribution from a lanthanide-free outflow. The low degree of polarization is consistent with intrinsically unpolarized emission scattered by Galactic dust, suggesting a symmetric geometry of the emitting region and low inclination of the merger system. Stringent upper limits to the polarization degree from 2.45 - 9.48 days post-burst are consistent with the lanthanides-rich macronova interpretation.
description: 18 pages, 1 figure, 2 tables, Nature Astronomy, in press
Dalla “Jamesian idea” alla “Jewish idea”: il caso di Trust di Cynthia Ozick
Creators: name: Porro, Simona
Publisher: name: Mimesis Edizioni
Year: 2019

description: The present paper focuses on Trust, Cynthia Ozick’s first novel. In my reading, the text epitomizes a significant transition, in the novelist’s career, from the “Jamesian idea” to the “Jewish idea”. The “Jamesian idea” can be traced back to what Ozick calls her “youthful intoxication” with James’s work, i.e. an idolatrous worship of his prose, which led her to an unnatural isolation from life in pursuit of a literary achievement that would emulate the Master’s legendary prowess. Ozick saw her mistake when, having decided to educate herself on Jewish theology and philosophy, she became familiar with Leo Baeck’s work. His essay Romantic Religion started her on a path that she would go on to pursue throughout her long career: the exploration of Jewish theology in literary form. Written during the aforementioned self-study period, Trust is characterized by two dimensions: a conspicuous intertextual dialogue with James’s prose, and an equally noticeable emphasis on Jewish themes. In that respect, the novel shows Ozick’s evolution from an “American” writer to a “Jewish writer”.
description: "Filosofia", N. 64 (2019): Immagini della natura
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0498
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
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: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0498, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0498, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
title: Empirical model for assessing dynamic susceptibility of post-earthquake debris flows
Creators: name: Hu, Kaiheng
name: Wang, Zhang
name: Chen, Cheng
name: Li, Xiuzhen
Publisher: name: Mountain Scholar
Year: 2019
Subjects: debris flow
susceptibility
earthquake
rainfall
dynamic assessment

description: Debris-flow susceptibility is controlled not only by static effective factors such as topography and lithology, but also by dynamic effective factors such as earthquake, rainfall and human activity. In this paper, a simple model of calculating the dynamic susceptibility is developed based on the assumption of linear relationship between the static and dynamic susceptibilities. The influence of earthquake and rainfall events is represent by two coefficients. The earthquake coefficient is considered as an exponential function of intensity, and a negative power function of elapsed time. The rainfall coefficient is proportional to the occurrence days of heavy rainfall. This model is applied to assess the debris-flow susceptibility of Hengduan mountainous area from 2000 to 2015. Four static effective factors including relative relief, slope, lithology and fault density are used to calculate the static susceptibility by ARCGIS grid toolbox. There are six earthquake events since 1995 whose intensity zones of >= VI are intersected with the Hengduan area. The earthquake coefficient is calculated with the intensity zoning data of each of the six events and then is accumulated to get the final earthquake coefficient in each year. TRMM satellite rainfall data from 2000 to 2015 are collected to extract the occurrence days of heavy rainfall which is used to calculate the rainfall coefficient. The dynamic susceptibilities from 2000 to 2015 are obtained by multiplying the static susceptibility with the earthquake and rainfall coefficients in respective year. The 2015 susceptibility map shows a qualitative agreement with the distribution map of disasters in 2015.
Kilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817
Creators: name: Tanaka, Masaomi
name: Utsumi, Yousuke
name: Mazzali, Paolo A.
name: Tominaga, Nozomu
name: Yoshida, Michitoshi
name: Sekiguchi, Yuichiro
name: Morokuma, Tomoki
name: Motohara, Kentaro
name: Ohta, Kouji
name: Kawabata, Koji S.
name: Abe, Fumio
name: Aoki, Kentaro
name: Asakura, Yuichiro
name: Baar, Stefan
name: Barway, Sudhanshu
name: Bond, Ian A.
name: Doi, Mamoru
name: Fujiyoshi, Takuya
name: Furusawa, Hisanori
name: Honda, Satoshi
name: Itoh, Yoichi
name: Kawabata, Miho
name: Kawai, Nobuyuki
name: Kim, Ji Hoon
name: Lee, Chien-Hsiu
name: Miyazaki, Shota
name: Morihana, Kumiko
name: Nagashima, Hiroki
name: Nagayama, Takahiro
name: Nakaoka, Tatsuya
name: Nakata, Fumiaki
name: Ohsawa, Ryou
name: Ohshima, Tomohito
name: Okita, Hirofumi
name: Saito, Tomoki
name: Sumi, Takahiro
name: Tajitsu, Akito
name: Takahashi, Jun
name: Takayama, Masaki
name: Tamura, Yoichi
name: Tanaka, Ichi
name: Terai, Tsuyoshi
name: Tristram, Paul J.
name: Yasuda, Naoki
name: Zenko, Tetsuya
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Recent detection of gravitational waves from a neutron star (NS) merger event GW170817 and identification of an electromagnetic counterpart provide a unique opportunity to study the physical processes in NS mergers. To derive properties of ejected material from the NS merger, we perform radiative transfer simulations of kilonova, optical and near-infrared emissions powered by radioactive decays of r-process nuclei synthesized in the merger. We find that the observed near-infrared emission lasting for > 10 days is explained by 0.03 Msun of ejecta containing lanthanide elements. However, the blue optical component observed at the initial phases requires an ejecta component with a relatively high electron fraction (Ye). We show that both optical and near-infrared emissions are simultaneously reproduced by the ejecta with a medium Ye of ~ 0.25. We suggest that a dominant component powering the emission is post-merger ejecta, which exhibits that mass ejection after the first dynamical ejection is quite efficient. Our results indicate that NS mergers synthesize a wide range of r-process elements and strengthen the hypothesis that NS mergers are the origin of r-process elements in the Universe.
description: 7 pages, 4 figures. Published in PASJ (Publications of the Astronomical Society of Japan)
Additional file 3: of A PSTOL-like gene, TaPSTOL, controls a number of agronomically important traits in wheat
Creators: name: Milner, Matthew
name: Howells, Rhian
name: Craze, Melanie
name: Bowden, Sarah
name: Graham, Neil
name: Wallington, Emma
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Figure S2. T-DNA structure for the three TaPSTOL constructs used in this study. (DOCX 30 kb) (DOCX 80 kb)
Extracting molecular Hamiltonian structure from time-dependent fluorescence intensity data
Creators: name: Brif, Constantin
name: Rabitz, Herschel
Publisher: name: arXiv
Year: 2000
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We propose a formalism for extracting molecular Hamiltonian structure from inversion of time-dependent fluorescence intensity data. The proposed method requires a minimum of \emph{a priori} knowledge about the system and allows for extracting a complete set of information about the Hamiltonian for a pair of molecular electronic surfaces.
description: 7pages, no figures, LaTeX2e
title: Affiche de la conférence de Iván Armenteros Martínez
Creators: name: LA3M (UMR 7298)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2017

description: Affiche de la conférence de Iván Armenteros Martínez, post-doctorant LabexMed 2013 accueilli à TELEMME, le 3 novembre 2014
description: Relation: http://labexmed.hypotheses.org/954
Bichromatic Microwave Photoresistance of Two-Dimensional Electron System
Creators: name: Zudov, M. A.
name: Du, R. R.
name: Pfeiffer, L. N.
name: West, K. W.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We explore experimentally bichromatic (frequencies $ω_1$ and $ω_2$) photoresistance of a two-dimensional electron system in the regimes of microwave-induced resistance oscillations and zero-resistance states. We find bichromatic resistance to be well described by a superposition of $ω_1$ and $ω_2$ components, provided that both monochromatic resistances are positive. This relation holds even when the oscillation amplitudes are small and one could expect additive contributions from monochromatic photoresistances. In contrast, whenever a zero-resistance state is formed by one of the frequencies, such superposition relation breaks down and the bichromatic resistance is strongly suppressed.
description: To appear in Phys. Rev. Lett
Microbial Spoilage of Meat and Meat Products
Creators: name: Phool Kanwar, Durga Bai Sodha, Pooja Gurjar, Saroj Katara
Publisher: name: The Science world a Monthly e magazine
Year: 2024

description: Spoilage?

The process which deteriorates the food to the extent that the food is rendered inedible or inappropriate for consumption.

•        Spoilage of meat and meat products occurs due to;

Ø  Autolysis (souring)-

By enzymes present in meat especially lysozymes-

Ø  Oxidation or hydrolysis of fat.

Ø  Microbial action.
Automatic classification of 10 blood cell subtypes using transfer learning via pre-trained convolutional neural networks
Creators: name: Asghar, Rabia
name: Kumar, Sanjay
name: Hynds, Paul
Publisher: name: University of Limerick
Year: 2024
Subjects: classificationCode: 40
subject: Engineering

description: Human blood is primarily composed of plasma, red blood cells, white blood cells, and platelets. It plays a vital role in transporting oxygen and nutrients to all organs, and stores essential health-related data about the human body. Blood cells are utilized to defend the body against infections and disease. Hence, analysis of blood permits physicians to assess an individual’s physiological condition. Blood cells are sub-classified into eight groups: Neutrophils, eosinophils, basophils, lymphocytes, monocytes, immature granulocytes (promyelocytes, myelocytes, and metamyelocytes), erythroblasts, and platelets (thrombocytes) on the basis of their nucleus, shape and cytoplasm. Traditionally, pathologists and hematologists have identified and examined these via microscopy prior to manual classification, with this manual approach being slow and prone to human error. Therefore, it is essential to automate this process. In the current study, transfer learning with a series of pre-trained Convolutional Neural Network (CNN) models—VGG16, VGG19, ResNet-50, ResNet-101, ResNet-152, InceptionV3, MobileNetV2 and DenseNet-201 was applied to the normal peripheral blood cells dataset (PBC). The overall accuracy achieved with individual CNNs ranged from 91.4 % to 94.7 %. Based on these pre-trained architectures, a CNN-based architecture has been developed to automatically classify all ten blood cell types. The proposed transfer learning CNN model was tested on blood cell images from the PBC, Kaggle and LISC datasets. Achieved accuracy was 99.91 %, 99.68 % and 98.79 %, respectively, across these three datasets. The presented CNN architecture outperforms all previous results reported in the scientific/medical literature with a high capacity for framework generalization in future applications of blood cell classification.
MOESM1 of Skin autofluorescence predicts major adverse cardiovascular events in patients with type 1 diabetes: a 7-year follow-up study
Creators: name: C. Blanc-Bisson
name: F. Velayoudom-Cephise
name: A. Cougnard-Gregoire
name: C. Helmer
name: K. Rajaobelina
name: C. Delcourt
name: L. Alexandre
name: L. Blanco
name: K. Mohammedi
name: M. Monlun
name: V. Rigalleau
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy
subject: 60506 Virology

description: Additional file 1. Scatterplot for SAF over age.
Hydrodynamic Simulations of the Sunyaev-Zel'dovich effect(s)
Creators: name: Springel, Volker
name: White, Martin
name: Hernquist, Lars
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have performed a sequence of high resolution hydrodynamic simulations of structure formation in a LCDM model to study the thermal and kinetic Sunyaev-Zel'dovich (SZ) effects. Including only adiabatic gas physics, we demonstrate that our simulations for the thermal effect are converged down to sub-arcminute scales. In this model, the angular power spectrum of CMB anisotropies induced by the thermal effect peaks at l~10^4, and reaches an amplitude just below current observational upper limits. Fluctuations due to the kinetic effect are a factor of ~30 lower in power and peak at slightly smaller angular scales. We identify individual SZ sources and compute their counts as a function of source strength and angular size. We present a preliminary investigation of the consequences of an early epoch of energy injection which tends to suppress power on small angular scales, while giving rise to additional power on largescales from the reheated IGM at high redshift.
description: 7 pages, published in ApJ, flawed factor of h=0.67 in y/b-results corrected, see http://www.mpa-garching.mpg.de/~volker/erratum.ps.gz for detailed erratum
Subdiffusive discrete time random walks via Monte Carlo and subordination
Creators: name: Nichols, J. A.
name: Henry, B. I.
name: Angstmann, C. N.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 65C05

description: A class of discrete time random walks has recently been introduced to provide a stochastic process based numerical scheme for solving fractional order partial differential equations, including the fractional subdiffusion equation. Here we develop a Monte Carlo method for simulating discrete time random walks with Sibuya power law waiting times, providing another approximate solution of the fractional subdiffusion equation. The computation time scales as a power law in the number of time steps with a fractional exponent simply related to the order of the fractional derivative. We also provide an explicit form of a subordinator for discrete time random walks with Sibuya power law waiting times. This subordinator transforms from an operational time, in the expected number of random walk steps, to the physical time, in the number of time steps.
Structural Phase Transitions
Creators: name: Cowley, R. A
name: Shapiro, S. M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Gen Shirane began studying ferroelectrics while he was still based in Japan in the early 1950s. It was therefore natural that when he arrived at Brookhaven and began specialising in neutron scattering that he would devote much of his energy and expertise studying structural phase transitions. We review the ground breaking experiments that showed the behaviour of antiferroelectrics and ferroelectrics were reasonably described in terms of the soft mode concept of structural phase transitions. This work lead directly to Gen being awarded the Buckley prize and, jointly with John Axe, awarded the Warren prize. We then describe his work on incommensurate phase transitions and in particular how the giant Kohn anomalies are responsible for the structural instabilities in one-dimensional metals. Finally Gen carefully investigated the central peak and the two-length scale phenomena that occur at most if not all transitions. Due to Gens elegant experimental work we know a great deal about both of these effects but in neither case is theory able to explain all of his results
description: Submitted to Journal of Japanese Physical Society for special issue in memory of Gen Shirane
A Generalized Framework for Kullback-Leibler Markov Aggregation
Creators: name: Amjad, Rana Ali
name: Blöchl, Clemens
name: Geiger, Bernhard C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Systems and Control (eess.SY)
subject: Information Theory (cs.IT)
subject: Optimization and Control (math.OC)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: This paper proposes an information-theoretic cost function for aggregating a Markov chain via a (possibly stochastic) mapping. The cost function is motivated by two objectives: 1) The process obtained by observing the Markov chain through the mapping should be close to a Markov chain, and 2) the aggregated Markov chain should retain as much of the temporal dependence structure of the original Markov chain as possible. We discuss properties of this parameterized cost function and show that it contains the cost functions previously proposed by Deng et al., Xu et al., and Geiger et al. as special cases. We moreover discuss these special cases providing a better understanding and highlighting potential shortcomings: For example, the cost function proposed by Geiger et al. is tightly connected to approximate probabilistic bisimulation, but leads to trivial solutions if optimized without regularization. We furthermore propose a simple heuristic to optimize our cost function for deterministic aggregations and illustrate its performance on a set of synthetic examples.
description: 12 pages, 3 figures; submitted to a journal
The Rapid Reddening and Featureless Optical Spectra of the optical counterpart of GW170817, AT 2017gfo, During the First Four Days
Creators: name: McCully, Curtis
name: Hiramatsu, Daichi
name: Howell, D. Andrew
name: Hosseinzadeh, Griffin
name: Arcavi, Iair
name: Kasen, Daniel
name: Barnes, Jennifer
name: Shara, Michael M.
name: Williams, Ted B.
name: Väisänen, Petri
name: Potter, Stephen B.
name: Romero-Colmenero, Encarni
name: Crawford, Steven M.
name: Buckley, David A. H.
name: Cooke, Jeffery
name: Andreoni, Igor
name: Pritchard, Tyler A.
name: Mao, Jirong
name: Gromadzki, Mariusz
name: Burke, Jamison
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the spectroscopic evolution of AT 2017gfo, the optical counterpart of the first binary neutron star (BNS) merger detected by LIGO and Virgo, GW170817. While models have long predicted that a BNS merger could produce a kilonova (KN), we have not been able to definitively test these models until now. From one day to four days after the merger, we took five spectra of AT 2017gfo before it faded away, which was possible because it was at a distance of only 39.5 Mpc in the galaxy NGC 4993. The spectra evolve from blue ($\sim6400$K) to red ($\sim3500$K) over the three days we observed. The spectra are relatively featureless --- some weak features exist in our latest spectrum, but they are likely due to the host galaxy. However, a simple blackbody is not sufficient to explain our data: another source of luminosity or opacity is necessary. Predictions from simulations of KNe qualitatively match the observed spectroscopic evolution after two days past the merger, but underpredict the blue flux in our earliest spectrum. From our best-fit models, we infer that AT 2017gfo had an ejecta mass of $0.03M_\odot$, high ejecta velocities of $0.3c$, and a low mass fraction $\sim10^{-4}$ of high-opacity lanthanides and actinides. One possible explanation for the early excess of blue flux is that the outer ejecta is lanthanide-poor, while the inner ejecta has a higher abundance of high-opacity material. With the discovery and follow-up of this unique transient, combining gravitational-wave and electromagnetic astronomy, we have arrived in the multi-messenger era.
description: 10 pages, 4 figures, ApJL in press
How Trade Unions Explain the Development of Two-PartySystems in the Caribbean but not the Pacific
Creators: name: Bishop, Matthew
name: Corbett, Jack
name: Veenendaal, Wouter
Publisher: name: Canberra, ACT: Dept. of Pacific Affairs, Research School of Pacific and Asian Studies, The Australian National University
Year: 2019

description: This In Brief explains how trade unions and their impact on party organisation are key to explaining how the Caribbean has two-party systems, but the Pacific does not. The absence of party system institutionalisation in the independent Pacific has puzzled scholars and frustrated reformers for decades. The Caribbean experience highlights that investing in trade unions, or civil society organisations more generally, may well be the best way to facilitate party system institutionalisation in the Pacific. However, it also offers a cautionary tale for would-be reformers who assume that stronger parties will curb the hyper-personalisation of politics.
title: V2_DU_LettreZ
Creators: name: Basnage de Beauval, Henri
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Ceci est la V2 du Dictionnaire universel, revu et corrigé en 1701 par Basnage de Beauval. Cette version a été obtenue avec GROBID dictionaries, après adaptation du système et renentraînement en juillet 2020.
Galaxy Spin Statistics and Spin-Density Correlation
Creators: name: Lee, Jounghun
name: Pen, Ue-Li
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a theoretical study of galaxy spin correlation statistics, with detailed technical derivations. We also find an expression for the spin-density cross-correlation, and apply that to the Tully galaxy catalog. The observational results appear qualitatively consistent with the theoretical predictions, yet the error bars are still large. However, we expect that currently ongoing large surveys such as the Sloan Digital Sky survey (SDSS) will enable us to make a precision measurement of these correlation statistics in the near future. These intrinsic galaxy alignments are expected to dominate over the weak lensing signal in SDSS, and we present the detailed algorithms for the density reconstruction for this case. These observables are tracers of the galaxy-gravity interaction, which may provide us deeper insights into the galaxy formation and large scale matter distribution as well.
description: Accepted version, ApJ in press, remaining mistakes and typos correctedd, LaTex file, 41 pages, 3 eps figures
Microtorus: a High Finesse Microcavity with Whispering-Gallery Modes
Creators: name: Ilchenko, Vladimir S.
name: Gorodetsky, Michael L.
name: Yao, X. Steve
name: Maleki, Lute
Publisher: name: arXiv
Year: 2000
Subjects: subject: Optics (physics.optics)
subject: Chemical Physics (physics.chem-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We have demonstrated a 165 micron oblate spheroidal microcavity with free spectral range 383.7 GHz (3.06nm), resonance bandwidth 25 MHz (Q ~ 10^7) at 1550nm, and finesse F > 10^4. The highly oblate spheroidal dielectric microcavity combines very high Q-factor, typical of microspheres, with vastly reduced number of excited whispering-gallery (WG) modes (by two orders of magnitude). The very large free spectral range in the novel microcavity - few hundred instead of few GigaHertz in typical microspheres - is desirable for applications in spectral analysis, narrow-linewidth optical and RF oscillators, and cavity QED.
description: 11 pages, 3 figures
Pethia padamya Data
Creators: name: Shangningam, Bungdon
name: Vishwanath, Waikhom
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Actinopterygii
Cypriniformes
Cyprinidae
Pethia
Pethia padamya

description: Pethia padamya:
Data from Kullander & Britz (2008).
description: Published as part of Shangningam, Bungdon & Vishwanath, Waikhom, 2018, Pethia poiensis, a new species of cyprinid fish from the Chindwin Basin of Manipur, India, pp. 585-593 in Zootaxa 4379 (4) on page 592, DOI: 10.11646/zootaxa.4379.4.10, http://zenodo.org/record/1175130
Ordering Nanoparticles with Polymer Brushes
Creators: name: Cheng, Shengfeng
name: Stevens, Mark J.
name: Grest, Gary S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Ordering nanoparticles into a desired super-structure is often crucial for their technological applications. We use molecular dynamics simulations to study the assembly of nanoparticles in a polymer brush randomly grafted to a planar surface as the solvent evaporates. Initially, the nanoparticles are dispersed in a solvent that wets the polymer brush. After the solvent evaporates, the nanoparticles are either inside the brush or adsorbed at the surface of the brush, depending on the strength of the nanoparticle-polymer interaction. For strong nanoparticle-polymer interactions, a 2-dimensional ordered array is only formed when the brush density is finely tuned to accommodate a single layer of nanoparticles. When the brush density is higher or lower than this optimal value, the distribution of nanoparticles shows large fluctuations in space and the packing order diminishes. For weak nanoparticle-polymer interactions, the nanoparticles order into a hexagonal array on top of the polymer brush as long as the grafting density is high enough to yield a dense brush. An interesting healing effect is observed for a low-grafting-density polymer brush that can become more uniform in the presence of weakly adsorbed nanoparticles.
description: 9 pages, 6 figures
Group Reduction of Heterotic Supergravity
Creators: name: Lu, H.
name: Pope, C. N.
name: Sezgin, E.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The reduction of ten-dimensional heterotic supergravity with Yang-Mills symmetry group K is performed on an arbitrary n-dimensional group manifold G. The reduction involves a nonvanishing 3-form flux, and the Lie algebra of G must have traceless structure constants to ensure the consistency of the reduction at the level of the action. A large class of gauged supergravities in d=10-n with (non)compact gaugings is obtained. The resulting models describe half-maximal gauged supergravities coupled to $ (n + {\rm dim} K)$ vector multiplets. We uncover their hidden $SO(n,n+{\rm dim} K)$ duality symmetry, and the $SO(n,n+{\rm dim} K) / SO(n)\times SO(n+{\rm dim} K)$ coset structure that governs the couplings of the scalar fields. We find that the local gauge symmetry of the d-dimensional theory is $K\times G \ltimes R^n$. Differences from the existing gauged supergravities are highlighted. The consistent truncation to pure half-maximal gauged supergravity in any dimension is shown, and the obstacle to performing a chiral truncation of the theory in d=6 dimensions is found. Among the results obtained are the complete diagonalisation of the fermionic kinetic terms, and other reduction formulae that are applicable to group reductions of supergravities in arbitrary dimensions.
description: 29 pages
China's Guide to Investment Cooperation in Papua NewGuinea
Creators: name: Smith, Graeme
Publisher: name: Canberra, ACT: Dept. of Pacific Affairs, Research School of Pacific and Asian Studies, The Australian National University
Year: 2019

description: This In Brief examines a key Chinese government document written in the lead up to the November 2018 APEC meeting in Port Moresby and published in January 2019. The 2018 Guide for Foreign Investment and Cooperation (Papua New Guinea) (hereafter ‘the guide’) is jointly issued by CAITEC (a Ministry of Commerce think tank), the Chinese embassy in PNG, and the Department of Outward Investment and Economic Cooperation (State Council 2018). The document represents a step forward from previous investor guides to PNG in its level of detail and sophistication of analysis. This In Brief provides an analysis of the guide, including the foreword by Liu Linlin, Economic Counselor to PNG for the People’s Republic of China (PRC).
Slow light in moving media
Creators: name: Leonhardt, U.
name: Piwnicki, P.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Optics (physics.optics)
subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: We review the theory of light propagation in moving media with extremely low group velocity. We intend to clarify the most elementary features of monochromatic slow light in a moving medium and, whenever possible, to give an instructive simplified picture.
Dynamics of the Electro-Optic response of Blue Bronze
Creators: name: Ladino, L.
name: Brill, J. W.
name: Freamat, M.
name: Uddin, M.
name: Dominko, D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We have studied the charge density wave (CDW) repolarization dynamics in blue bronze by applying square-wave voltages of different frequencies to the sample and measuring the changes in infrared transmittance, proportional to CDW strain. The frequency dependence of the electro-transmittance was fit to a modified harmonic oscillator response and the evolution of the parameters as functions of voltage, position, and temperature are discussed. Resonant frequencies decrease with distance from the current contacts, indicating that the resulting delays are intrinsic to the CDW with the strain effectively flowing from the contact. For a fixed position, the average relaxation time has a voltage dependence given by tau_0~V^-p, with 1
description: 36 pages, including 12 figures, submitted to Phys. Rev. B
Additional file 1 of Postnatal screening and care for non-medical risk factors by preventive child healthcare in deprived and non-deprived neighbourhoods
Creators: name: M. Van Minde
name: S. Hulst
name: H. Raat
name: E. Steegers
name: M. De Kroon
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Pharmacology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Table S1. Respondents’ opinion on which healthcare professional should care for families with non-medical risks (n = 85). List of healthcare professionals considered, to care for families with non-medical risk factors and PCHC professional opinion on who should be responsible to care for these families. Table S2. Respondents’ opinion on with which healthcare professional collaboration should be intensified (n = 85). List of healthcare professionals considered, with whom PCHC professionals could collaborate with and their opinion with which healthcare professional collaboration should be intensified. (DOCX 14 kb)