cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Cart. 186 (11 H 71), f. 0062r
Creators: name: de la Côte d'Or, Archives départementales
name: CBMA/CG21/F.PETOT/2012
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la Côte-d'Or, C
art. 186 (11 H 71). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la
 Côte-d'Or, Cart. 186 (11 H 71), f. 0062r, 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
Belle J/psi+eta_c anomaly and a very light scalar boson
Creators: name: Cheung, Kingman
name: Keung, Wai-Yee
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The large rate of the $J/ψ+η_c$ production observed by the Belle collaboration has posed a serious challenge to our understanding of the quarkonium. We examine a scenario that there exists a light scalar boson around 5 GeV, with an enhanced coupling solely to the charm quark. Such a scenario would explain the Belle anomaly. It also predicts a significant increase in $J/ψ$ plus open charm pair production. An immediate test for the scalar boson is to look for a peak around 5 GeV in the recoil mass spectrum of $J/ψ$, because the scalar boson can also be produced in association with the $J/ψ$. Finally, we also point out that the process $e^+ e^- \to H γ$ is sizable for observation.
description: 10 pages, 5 figures
Conservative model reduction for finite-volume models
Creators: name: Carlberg, Kevin
name: Choi, Youngsoo
name: Sargsyan, Syuzanna
Publisher: name: arXiv
Year: 2017
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 35L65, 65L05, 65L06, 65L60, 65M08, 65M15, 65M22, 68U20, 76M12

description: This work proposes a method for model reduction of finite-volume models that guarantees the resulting reduced-order model is conservative, thereby preserving the structure intrinsic to finite-volume discretizations. The proposed reduced-order models associate with optimization problems characterized by a minimum-residual objective function and nonlinear equality constraints that explicitly enforce conservation over subdomains. Conservative Galerkin projection arises from formulating this optimization problem at the time-continuous level, while conservative least-squares Petrov--Galerkin (LSPG) projection associates with a time-discrete formulation. We equip these approaches with hyper-reduction techniques in the case of nonlinear flux and source terms, and also provide approaches for handling infeasibility. In addition, we perform analyses that include deriving conditions under which conservative Galerkin and conservative LSPG are equivalent, as well as deriving a posteriori error bounds. Numerical experiments performed on a parameterized quasi-1D Euler equation demonstrate the ability of the proposed method to ensure not only global conservation, but also significantly lower state-space errors than nonconservative reduced-order models such as standard Galerkin and LSPG projection.
description: Submitted of Journal of Computational Physics
Open-path, closed-path and reconstructed aerosol extinction at a rural site
Creators: name: Gordon, Timothy D.
name: Prenni, Anthony J.
name: Renfro, James R.
name: McClure, Ethan
name: Hicks, Bill
name: Onasch, Timothy B.
name: Freedman, Andrew
name: McMeeking, Gavin R.
name: Chen, Ping
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
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: Ecology
subject: Inorganic Chemistry

description: The Handix Scientific Open-Path Cavity Ringdown Spectrometer (OPCRDS) was deployed during summer 2016 in Great Smoky Mountains National Park (GRSM). Extinction coefficients from the relatively new OPCRDS and from a more well-established extinction instrument agreed to within 7%. Aerosol hygroscopic growth (f(RH)) was calculated from the ratio of ambient extinction measured by the OPCRDS to dry extinction measured by a closed-path extinction monitor (Aerodyne’s Cavity Attenuated Phase Shift Particulate Matter Extinction Monitor, CAPS PMex). Derived hygroscopicity (RH < 95%) from this campaign agreed with data from 1995 at the same site and time of year, which is noteworthy given the decreasing trend for organics and sulfate in the eastern U.S. However, maximum f(RH) values in 1995 were less than half as large as those recorded in 2016—possibly due to nephelometer truncation losses in 1995. Two hygroscopicity parameterizations were investigated using high time resolution OPCRDS+CAPS PMex data, and the Kext model was more accurate than the γ model. Data from the two ambient optical instruments, the OPCRDS and the open-path nephelometer, generally agreed; however, significant discrepancies between ambient scattering and extinction were observed, apparently driven by a combination of hygroscopic growth effects, which tend to increase nephelometer truncation losses and decrease sensitivity to the wavelength difference between the two instruments as a function of particle size. There was not a statistically significant difference in the mean reconstructed extinction values obtained from the original and the revised IMPROVE (Interagency Monitoring of Protected Visual Environments) equations. On average IMPROVE reconstructed extinction was ~25% lower than extinction measured by the OPCRDS, which suggests that the IMPROVE equations and 24-hr aerosol data are moderately successful in estimating current haze levels at GRSM. However, this conclusion is limited by the coarse temporal resolution and the low dynamic range of the IMPROVE reconstructed extinction.
Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
Creators: name: Yi, Ze-Long
name: Zhang, Tong-Jie
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the absolute ages of passively evolving galaxies observed at different redshifts, one can obtain the differential ages, the derivative of redshift $z$ with respect to the cosmic time $t$ (i.e. ${\rm d} z/{\rm d}t$). Thus, the Hubble parameter $H(z)$ can be measured through the relation $H(z)=-({\rm d} z/{\rm d}t)/(1+z)$. By comparing the measured Hubble parameter at different redshifts with the theoretical one containing free cosmological parameters, one can constrain current cosmological models. In this paper, we use this method to present the constraint on a spatially flat Friedman-Robert-Walker Universe with a matter component and a holographic dark energy component, in which the parameter $c$ plays a significant role in this dark energy model. Firstly we consider three fixed values of $c$=0.6, 1.0 and 1.4 in the fitting of data. If we set $c$ free, the best fitting values are $c=0.26$, $Ω_{\rm m0}=0.16$, $h=0.9998$. It is shown that the holographic dark energy behaves like a quintom-type at the $1σ$ level. This result is consistent with some other independent cosmological constrains, which imply that $c<1.0$ is favored. We also test the results derived from the differential ages using another independent method based on the lookback time to galaxy clusters and the age of the universe. It shows that our results are reliable.
description: 18 pages including 7 figures and 1 tables. Final version for publication in Modern Physics Letters A (MPLA)[minor revision to match the appear version]
Cistus crispus Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malvales
Cistaceae
Cistus
Cistus crispus

description: Cistus crispus, spec. nov.
 8. Cistus arborescens, foliis lanceolatis hirsutis repandis, alis nudis. Hort. cliff. 206. Roy. lugdb. 475. Sauv. Monsp. 147.
 Cistus mas, foliis chamaedryos. Bauh. pin. 464.
 Cistus mas 5. Clus. hist. 1. p. 69.
 Habitat in Lusitania . ♄
 Ramuli, pedunculi & calyces tenui lana adspersi.
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 524, DOI: 10.5281/zenodo.3931989
Post-Newtonian evolution of massive black hole triplets in galactic nuclei -- II. Survey of the parameter space
Creators: name: Bonetti, Matteo
name: Haardt, Francesco
name: Sesana, Alberto
name: Barausse, Enrico
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Massive black hole binaries (MBHBs) are expected to form at the centre of merging galaxies during the hierarchical assembly of the cosmic structure, and are expected to be the loudest sources of gravitational waves (GWs) in the low frequency domain. However, because of the dearth of energy exchanges with background stars and gas, many of these MBHBs may stall at separations too large for GW emission to drive them to coalescence in less than a Hubble time. Triple MBH systems are then bound to form after a further galaxy merger, triggering a complex and rich dynamics that can eventually lead to MBH coalescence. Here we report on the results of a large set of numerical simulations, where MBH triplets are set in spherical stellar potentials and MBH dynamics is followed through 2.5 post-Newtonian order in the equations of motion. From our full suite of simulated systems we find that a fraction $\simeq 20-30$% of the MBH binaries that would otherwise stall are led to coalesce within a Hubble time. The corresponding coalescence timescale peaks around 300 Myr, while the eccentricity close to the plunge, albeit small, is non-negligible ($\lesssim 0.1$). We construct and discuss marginalised probability distributions of the main parameters involved and, in a companion paper of the series, we will use the results presented here to forecast the contribution of MBH triplets to the GW signal in the nHz regime probed by Pulsar Timing Array experiments.
description: 19 pages, 14 figures, accepted for publication in MNRAS
Melatonin in Chronic Pain Syndromes
Creators: name: Danilov, Andrei
name: Kurganova, Julia
Publisher: name: Adis Journals
Year: 2018
Subjects: subject: Medicine
subject: 110301 Anaesthesiology
subject: FOS: Clinical medicine

description: Article full text
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Do Dogs See the Ponzo illusion?
Creators: name: Byosiere, Sarah-Elizabeth
name: Feng, Lynna
name: Rutter, Nicholas
name: Dawson, Jessica
name: Chouinard, Philippe
name: Howell, Tiffani
name: Bennett, Pauleen
Publisher: name: La Trobe
Year: 2023
Subjects: Uncategorized

description: While domestic dogs (Canis familiaris) play a large role in human daily lives, little is known about how they perceive the visual world. Recent research suggests that dogs may perceive certain visual illusions differently than humans. To further evaluate geometric illusion susceptibility, eight dogs were assessed on their susceptibility to the Ponzo illusion. Four experiments were conducted: 1) a presentation of the Ponzo illusion with target circles in a ‘grid inducer context’, 2) a re-test of Experiment 1 after additional training, 3) a presentation of the Ponzo illusion with target rectangles in a ‘grid inducer context’ and 4) a presentation of the Ponzo illusion with target circles in a ‘converging lines context.’ A one-sample t-test of the dogs’ responses to the Ponzo stimuli in Experiment 1 demonstrated illusion susceptibility at the group level; however, no individual dog performed significantly above chance in binomial tests. In Experiments 2, 3, and 4, one-sample t-tests found no significant results at the group level, although one or more dogs did demonstrate a small but significant effect. Taken together, then, there was limited evidence for dogs’ susceptibility to the Ponzo illusion in a two-choice discrimination paradigm. As most animals tested previously have demonstrated human-like susceptibility to the Ponzo illusion, these findings have implications for theoretical explanations. The divergence of results between dogs and humans/other animals suggest that mechanisms underlying perception of the Ponzo illusion may differ across species and that care should be taken when using visual paradigms to test dogs’ cognitive skills.
Bottom Quark Mass Determination from low-n Sum Rules
Creators: name: Corcella, Gennaro
name: Hoang, Andre H.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the uncertainties in the MSbar bottom quark mass determination using relativistic sum rules to O(alpha_S^2). We include charm mass effects and secondary b bbar production and treat the experimental continuum region more conservatively than previous analyses. The PDG treatment of the region between the resonances Upsilon (4S) and Upsilon (5S) is reconsidered. Our final result reads: m_b(m_b)=(4.20 \pm 0.09) GeV.
description: 4 pages, Talk given at QCD 03, Montpellier, France, 2-9 July 2003
Cistus halimifolius Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malvales
Cistaceae
Cistus
Cistus halimifolius

description: Cistus halimifolius, spec. nov.
 9. Cistus arborescens, alis nudis, foliolis duobus calycinis linearibus. Hort. cliff. 205. Roy. lugdb. 475. Sauv. monsp. 147.
 Cistus femina, portulacae marinae folio latiore obtuso. Bauh. pin. 465.
 Cistus folio halimi 1. Clus. hist. 1. p. 71.
 β. Cistus femina, portulacae marinae folio angustiore mucronato. Bauh. pin. 465.
 Cistus halimi folio 2. Clus. hist. 1. p. 71.
 Habitat in Lusitaniae maritimis. ♄    * Exstipulatae, suffruticosae.
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on pages 524-525, DOI: 10.5281/zenodo.3931989
Orientational Dynamics of Fluctuating Dipolar Particles Assembled in a Mesoscopic Colloidal Ribbon
Creators: name: Massana-Cid, Helena
name: Martinez-Pedrero, Fernando
name: Cebers, Andrejs
name: Tierno, Pietro
Publisher: name: arXiv
Year: 2017
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We combine experiments and theory to investigate the dynamics and orientational fluctuations of ferromagnetic microellipsoids that form a ribbon-like structure due to attractive dipolar forces. When assembled in the ribbon, the ellipsoids displays orientational thermal uctuations with an amplitude that can be controlled via application of an in-plane magnetic field. We use video microscopy to investigate the orientational dynamics in real time/space. Theoretical arguments are used to derive an analytical expression that describes how the distribution of the different angular configurations depends on the strength of the applied field. The experimental data are in good agreement with the developed model for all the range of field parameters explored. Understanding the role of uctuations in chains composed of dipolar particles is important not only from a fundamental point of view, but it may also help understanding the stability of such structures against thermal noise, which is relevant in micro uidics and lab-on-a-chip applications.
Einstein Metrics on Rational Homology Spheres
Creators: name: Boyer, Charles P.
name: Galicki, Krzysztof
Publisher: name: arXiv
Year: 2003
Subjects: subject: Differential Geometry (math.DG)
subject: High Energy Physics - Theory (hep-th)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 53C20,53C12,14E30

description: We prove the existence of Sasakian-Einstein metrics on infinitely many rational homology spheres in all odd dimensions greater than 3. In dimension 5 we obain somewhat sharper results. There are examples where the number of effective parameters in the Einstein metric grows exponentially with dimension.
description: 8 pages
Environmental Pollution and Radiological Hazards Assessment of Quarrying Activities in Southwestern Nigeria
Creators: name: Olabamiji, A.O
name: Makinde, S.C.O
name: Balogun, F.O
name: Olanlege, A.O
name: Akintelu, M.T
Publisher: name: Lagos State University
Year: 2024
Subjects: subject: Quarrying dust
subject: Hazard indices
subject: Health impact
subject: Pollution
subject: Environment

description: The introduction of pollutants to any environment poses a significant threat to human health and the overall wellbeing of ecosystems, thus undermining the Sustainable Development Goal (SDG). In 2019, the World Health Organization (WHO) reported that approximately 9 million annual deaths were attributed to air pollution resulting from human activities. The research investigated radiological pollution hazards caused by quarryingrelated dust emissions. The assessment includes estimations of internal hazard index (H ), external hazard index in (H ), radium equivalent activity (Ra ), absorbed gamma dose rate (D), Annual Effective Dose Equivalent ex eq (AEDE), and Excess Lifetime Cancer Risk (ELCR). Two-hundred-gram (200g) of each dried dust sample was placed into gas-tight, radon impermeable cylindrical polyethylene containers with a uniform base diameter of2cm and then sealed for 28 days to achieve secular equilibrium before using NaI(Tl) gamma-ray spectrometer for counting. The highest activity concentrations of 1691.9Bqkg-1, 55.0 Bqkg-1, and 124.8 Bqkg-1 were recorded for40K,226Ra and 232Th respectively. Radiological hazard indices were computed and compared with the International Commission on Radiological Protection (ICRP) and it was observed to be slightly higher than the standard limit. The results suggested that more attention is required in monitoring dust from quarrying-related activities in the study areas. It emphasizes the inclusion of proper ventilation in residential structures to mitigate the accumulation of radon. Quarrying dust'spotential impact on the environment, human health, and Sustainable Development Goal (SDG) has been addressed.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Cart. 188 (11 H 73), f. 0008r
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2012
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
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 général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0008r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0008r, 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
Prospective evaluation of relationships between radiotherapy dose to masticatory apparatus and trismus
Creators: name: Hague, Christina
name: Beasley, William
name: Garcez, Kate
name: Lip W. Lee
name: McPartlin, Andrew
name: McWilliam, Alan
name: Ryder, David
name: Sykes, Andrew J.
name: Thomson, David
name: Herk, Marcel Van
name: West, Catharine
name: Slevin, Nick J.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 60506 Virology

description: Aims: This feasibility study aimed to identify relationships between radiation doses to the masticatory apparatus as a combined block or as individual subunits with changes in trismus following radiotherapy. Material and methods: Twenty patients from a single center were recruited prospectively as part of a randomized trial comparing proactive exercises in the management of trismus. Patients with stage III/IV oral cavity or oropharyngeal squamous cell cancers received intensity-modulated radiotherapy with concurrent systemic therapy. All patients had trismus prior to radiotherapy. Maximal inter-incisor distance (MID) was measured pre- and 6 months from the start of radiotherapy. Bilateral muscles of mastication: medial and lateral pterygoids (MP and LP), masseters (M), temporalis (T), temporomandibular joint (TMJ) were contoured on CT images. The block comprised all muscles excluding the TMJ below the orbital floor. Mean dose, equivalent uniform dose (EUD) and V35–V60 Gy were compared with change in MID. Results: In six patients, the MID deteriorated at 6 months from the start of radiotherapy compared with 14 whose MID improved. No significant association was observed between age, gender, smoking, alcohol status, exercise compliance, cisplatin, tumor site, stage, V35–V60 Gy or EUD with change in MID. A clinical outlier was excluded. Without the outlier (n = 19), a significant association was seen between mean dose and change in MID at 6 months for the ipsilateral block (p = .01), LP (p = .04) and M (p 40 Gy to the block. Conclusion: Higher mean radiation doses to the ipsilateral block, LP and M were significantly associated with deterioration in trismus. Limiting dose to these structures to ≤40 Gy for tumors not invading the masticatory muscles may improve treatment-related sequelae. The ipsilateral block, LP and M should be studied further as possible alternative avoidance structures in radiotherapy treatment planning.
Molecular Origin of Contact Line Friction in Dynamic Wetting
Creators: name: Johansson, Petter
name: Hess, Berk
Publisher: name: arXiv
Year: 2017
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: A hydrophilic liquid, such as water, forms hydrogen bonds with a hydrophilic substrate. The strength and locality of the hydrogen bonding interactions prohibit slip of the liquid over the substrate. The question then arises how the contact line can advance during wetting. Using large-scale molecular dynamics simulations we show that the contact line advances by single molecules moving ahead of the contact line through two distinct processes: either moving over or displacing other liquid molecules. In both processes friction occurs at the molecular scale. We measure the energy dissipation at the contact line and show that it is of the same magnitude as the dissipation in the bulk of a droplet. The friction increases significantly as the contact angle decreases, which suggests suggests thermal activation plays a role. We provide a simple model that is consistent with the observations.
Contact-Induced Semiconductor-to-Metal Transition in Single-Layer WS$_2$
Creators: name: Dendzik, Maciej
name: Bruix, Albert
name: Michiardi, Matteo
name: Ngankeu, Arlette S.
name: Bianchi, Marco
name: Miwa, Jill A.
name: Hammer, Bjørk
name: Hofmann, Philip
name: Sanders, Charlotte E.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Low-resistance ohmic contacts are a challenge for electronic devices based on two-dimensional materials. We show that an atomically precise junction between a two-dimensional semiconductor and a metallic contact can lead to a semiconductor-to-metal transition in the two-dimensional material--a finding which points the way to a possible method of achieving low-resistance junctions. Specifically, single-layer WS$_2$ undergoes a semiconductor-to-metal transition when epitaxially grown on Ag(111), while it remains a direct band gap semiconductor on Au(111). The metallicity of the single layer on Ag(111) is established by lineshape analysis of core level photoemission spectra. Angle-resolved photoemission spectroscopy locates the metallic states near the Q point of the WS$_2$ Brillouin zone. Density functional theory calculations show that the metallic states arise from hybridization between Ag bulk bands and the local conduction band minimum of WS$_2$ near the Q point.
description: Main text: 21 pages, 4 figures. Supplement: 7 pages, 4 figures, 1 table
Supersymmetric Higgs production at the Large Hadron Collider
Creators: name: Harlander, Robert
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We review the status of theoretical predictions for the production of neutral Higgs bosons at the LHC. Special emphasis is put on the role of bottom quarks in the gluon fusion process and in the associated production of Higgs bosons with bb-bar pairs.
description: LaTeX, 3 pages, 9 PostScript files included. Talk given at the HEP2003 Europhysics Conference in Aachen, Germany (EPS 2003), July 17-23, 2003
Cistus umbellatus Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malvales
Cistaceae
Cistus
Cistus umbellatus

description: Cistus umbellatus, spec. nov.
10. Cistus suffruticosus procumbens exstipulatus, foliis oppositis, floribus umbellatis.
 Cistus foliis linearibus non stipulatis, caule florali umbellato lignoso. Guett. stamp. 2. p.180. Dalib. paris. 158.
 Cistus Ledon foliis thymi. Bauh. pin. 467.
 Ledon X. Clus. hist. 1. p. 81.
 Habitat in Gallia , Hispania . ♄
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 525, DOI: 10.5281/zenodo.3931989
John Spenser's Story
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: John Spenser served in the Scottish regiment. Changed name to Jock and known as that for rest of life. Book called 'The Melancholy State'. Story of PoWs. In Italy and marched - mistake in the book.
After the war in Brighton. Went to Capetown in 1946, not 1945 as it says in book.Went to war with black hair and came back with white hair. Captured in El-Alamein, forced march to Libya and Prisoner of War in Italy. Then marched to Germany. Very hungry.Very much did not want to talk about the war.
Cohomology characterizations of non-abelian extensions of Hom-Lie algebras
Creators: name: Song, Lina
name: Tang, Rong
Publisher: name: arXiv
Year: 2017
Subjects: subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics

description: In this paper, first we show that under the assumption of the center of h being zero, diagonal non-abelian extensions of a regular Hom-Lie algebra g by a regular Hom-Lie algebra h are in one-to-one correspondence with Hom-Lie algebra morphisms from g to Out(h). Then for a general Hom-Lie algebra morphism from g to Out(h), we construct a cohomology class as the obstruction of existence of a non-abelian extension that induce the given Hom-Lie algebra morphism.
Origin of the Counter-Rotating Gas in NGC 1596
Creators: name: Chung, Aeree
name: Koribalski, Baerbel
name: Bureau, Martin
name: van Gorkom, J. H.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Australia Telescope Compact Array (ATCA) HI imaging of the edge-on galaxy NGC 1596, which was recently found to have counter-rotating ionized gas in its center (<15"). We find a large HI envelope associated with a nearby companion, the dwarf irregular galaxy NGC 1602. The HI covers a region \~11.9'x13.4' (62x70 kpc^2) and the total HI mass detected is 2.5+/-0.1x10^9 Msun (assuming an 18 Mpc distance). The HI is centered on NGC 1602 but appears to have two tidal tails, one of which crosses over NGC 1596. The HI located at the position of NGC 1596 has a velocity gradient in the same sense as the ionized gas, i.e. opposite to the stellar rotation. Both the existence of a large gas reservoir and the velocity gradient of the HI and the ionized gas strongly suggest that the ionized gas in NGC 1596 originated from NGC 1602. From the length of the HI tails we conclude that the interaction started at least 1 Gyr ago, but the unsettled, asymmetric distribution of the ionized gas suggests that the accretion occured more recently. NGC 1596 thus provides a good example where the presence of counter-rotating gas can be directly linked to an accretion event. After the accretion has stopped or the merging is complete, NGC 1596 may evolve to a system with more extended counter-rotating gas but no obvious signature of interaction. There is a substantial local HI peak in one of the two tails, where we also find a faint stellar counterpart. The M_HI/L_B ratio in this region is too high for a normal dwarf elliptical or a low surface brightness galaxy, so we conclude that a tidal dwarf is currently forming there.
description: 9 pages, 7 figures, accepted for publication in MNRAS. A full resolution version is available at http://www.astro.columbia.edu/~archung/research/CRdisk/Paper/chung_n1596.pdf (highly recommended due to the resolution of the figures)
Practice-Based Research Networks: Integrating Clinical Data for Improved Pharmacoepidemiology
Creators: name: Sousa-Veloso, Tiago
Publisher: name: Adis Journals
Year: 2018
Subjects: subject: 110301 Anaesthesiology
subject: FOS: Clinical medicine
subject: Medicine

description: Article full text
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Optical properties of periodic, quasi-periodic, and disordered one-dimensional photonic structures
Creators: name: Bellingeri, Michele
name: Chiasera, Alessandro
name: Kriegel, Ilka
name: Scotognella, Francesco
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Photonic crystals are characterized by a spatial modulation of the dielectric constant on the length scale of the wavelength of light giving rise to energy ranges where light cannot propagate through the crystal - the photonic band gap. While mostly photonic crystals are referred to as periodic arrangements, in this review we aim to highlight as well how aperiodicity and disorder affects light modulation. In this review article, we introduce the concepts of periodicity, quasi-periodicity, and disorder in photonic crystals, focussing on the one-dimensional case. We discuss in detail the physical peculiarities, the fabrication techniques, and the applications of periodic, quasi-periodic, and disorder photonic structures, highlighting how the degree of crystallinity matters in the manipulation of light. We report different types of disorder in 1D photonic structures and we discuss their properties in terms of light transmission. We discuss the relationship between the average total transmission, in a range of wavelengths around the photonic band gap of the corresponding photonic crystal, and the homogeneity of the photonic structures, quantified by the Shannon index. Then we discuss the light transmission in structures in which the high refractive index layers are aggregated in clusters following a power law distribution. Finally, in the case of structures in which the high refractive index layers are aggregated in clusters with a truncated uniform distribution, we discuss: i) how different refractive index contrast tailors the total light transmission; ii) how the total light transmission is affected by the introduction of defects made with a third material.
description: 42 pages, 24 figures
Neutrinos in a spherical box
Creators: name: Giomataris
name: Vergados, J. D.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the present paper we study some neutrino properties as they may appear in the low energy neutrinos emitted in triton decay with maximum neutrino energy of 18.6 keV. The technical challenges to this end can be achieved by building a very large TPC capable of detecting low energy recoils, down to a a few tenths of a keV, within the required low background constraints. More specifically We propose the development of a spherical gaseous TPC of about 10-m in radius and a 200 Mcurie triton source in the center of curvature. One can list a number of exciting studies, concerning fundamental physics issues, that could be made using a large volume TPC and low energy antineutrinos: 1) The oscillation length involving the small angle of the neutrino mixing matrix, directly measured in this disappearance experiment, is fully contained inside the detector. Measuring the counting rate of neutrino-electron elastic scattering as a function of the distance of the source will give a precise and unambiguous measurement of the oscillation parameters free of systematic errors. In fact first estimates show that even with a year's data taking a sensitivity of a few percent for the measurement of the above angle will be achieved. 2) The low energy detection threshold offers a unique sensitivity for the neutrino magnetic moment which is about two orders of magnitude beyond the current experimental limit. 3) Scattering at such low neutrino energies has never been studied and any departure from the expected behavior may be an indication of new physics beyond the standard model. In this work we mainly focus on the various theoretical issues involved including a precise determination of the Weinberg angle at very low momentum transfer.
description: 16 Pages, LaTex, 7 figures, talk given at NANP 2003, Dubna, Russia, June 23, 2003
Cistus fumana Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malvales
Cistaceae
Cistus
Cistus fumana

description: Cistus fumana, spec. nov.
11. Cistus suffruticosus procumbens exstipulatus, foliis alternis linearibus, pedunculis unifloris.
 Cistus caule procumbente, foliis alternis. Fl. suec. 435. Guett. stamp. 157.
 Cistus fruticosus procumbens, foliis aciformibus nudis. Sauv. monsp.45.
 Helianthemum foliis linearibus saepius alternis non stipulatis, pedunculis unifloris, caule lignoso. Guett. stamp. 2. p.18.
 ChamaeCistus, ericae folio, luteus elatior. Bauh. pin. 466.
 Helianthemum tenuifolium glabrum erectum, luteo flore. Bauh. hist. 2. p.18.
 β. Cistus fruticosus procumbens, foliis aciformibus nudis, floribus auriculatis. Sauv. monsp.46.
 ChamaeCistus, ericae folio, luteus humilior. Bauh. pin. 466.
 Helianthemum tenuifolium glabrum, luteo flore, per humum sparsum. Bauh. hist. 2. p.18.
 Habitat in Gallia , Gotlandia , Helvetia . ♄
 Corolla calyce vix major est.
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 525, DOI: 10.5281/zenodo.3931989
Beyond the LSD method for the partial sums of multiplicative functions
Creators: name: Granville, Andrew
name: Koukoulopoulos, Dimitris
Publisher: name: arXiv
Year: 2017
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: The Landau-Selberg-Delange (LSD) method gives an asymptotic formula for the partial sums of a multiplicative function $f$ whose prime values are $α$ on average. In the literature, the average is usually taken to be $α$ with a very strong error term, leading to an asymptotic formula for the partial sums with a very strong error term. In practice, the average at the prime values may only be known with a fairly weak error term, and so we explore here how good an estimate this will imply for the partial sums of $f$, developing new techniques to do so.
description: Addressed referee's comments; added some references; corrected and simplified the proof of Theorem 9. 26 pages
Accretion Disks around Young Stars: Lifetimes, Disk Locking and Variability
Creators: name: Jayawardhana, Ray
name: Coffey, Jaime
name: Scholz, Alexander
name: Brandeker, Alexis
name: van Kerkwijk, Marten H.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the findings of a comprehensive study of disk accretion and related phenomena in four of the nearest young stellar associations spanning 6-30 million years in age, an epoch that may coincide with the late stages of planet formation. We have obtained ~650 multi-epoch high-resolution optical spectra of 100 low-mass stars that are likely members of the eta Chamaeleontis (~6 Myr), TW Hydrae (~8 Myr), beta Pictoris (~12 Myr) and Tucanae-Horologium (~30 Myr) groups. Our data were collected over 12 nights between 2004 December - 2005 July on the Magellan Clay 6.5m telescope. Based on H$α$ line profiles, along with a variety of other emission lines, we find clear evidence of on-going accretion in three out of 11 eta Cha stars and two out of 32 TW Hydrae members. None of the 57 beta Pic or Tuc-Hor members shows measurable signs of accretion. Together, these results imply significant evolution of the disk accretion process within the first several Myr of a low-mass star's life. While a few disks can continue to accrete for up to ~10 Myr, our findings suggest that disks accreting for beyond that timescale are rather rare. This result provides an indirect constraint on the timescale for gas dissipation in inner disks and, in turn, on gas giant planet formation. All accretors in our sample are slow rotators, whereas non-accretors cover a large range in rotational velocities. This may hint at rotational braking by disks at ages up to ~8 Myr. Our multi-epoch spectra confirm that emission-line variability is common even in somewhat older T Tauri stars, among which accretors tend to show particularly strong variations. Thus, our results indicate that accretion and wind activity undergo significant and sustained variations throughout the lifetime of accretion disks.
description: to appear in The Astrophysical Journal
title: 03_0473
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/
Distributed Quantum Sensing Using Continuous-Variable Multipartite Entanglement
Creators: name: Zhuang, Quntao
name: Zhang, Zheshen
name: Shapiro, Jeffrey H.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Distributed quantum sensing uses quantum correlations between multiple sensors to enhance the measurement of unknown parameters beyond the limits of unentangled systems. We describe a sensing scheme that uses continuous-variable multipartite entanglement to enhance distributed sensing of field-quadrature displacement. By dividing a squeezed-vacuum state between multiple homodyne-sensor nodes using a lossless beam-splitter array, we obtain a root-mean-square (rms) estimation error that scales inversely with the number of nodes (Heisenberg scaling), whereas the rms error of a distributed sensor that does not exploit entanglement is inversely proportional to the square root of number of nodes (standard quantum limit scaling). Our sensor's scaling advantage is destroyed by loss, but it nevertheless retains an rms-error advantage in settings in which there is moderate loss. Our distributed sensing scheme can be used to calibrate continuous-variable quantum key distribution networks, to perform multiple-sensor cold-atom temperature measurements, and to do distributed interferometric phase sensing.
description: 7 pages, 3 figures
Encountering a Neglected Area of a Healthcare System: A Decade of Improvement in Cancer Pain Clinical Practice in Iran
Creators: name: Gharehdaghi, Farid A.
name: Gorginzadeh, Mansoureh
name: Saeid Safari
Publisher: name: Adis Journals
Year: 2018
Subjects: subject: 110301 Anaesthesiology
subject: FOS: Clinical medicine
subject: Medicine

description: Article full text
 The full text of this article can be found here. https://link.springer.com/article/10.1007/s40122-016-0055-0
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 Other enhanced features include, but are not limited to:
 • Slide decks • Videos and animations • Audio abstracts • Audio slides