cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Scrophularia frutescens Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Scrophulariaceae
Scrophularia
Scrophularia frutescens

description: Scrophularia frutescens Linnaeus, Species Plantarum 2: 621. 1753.
"Habitat in Lusitania." RCN: 4487.
 Neotype (Ortega & Devesa in Ruizia 11: 138. 1993): UNEX 6183, central specimen (UNEX).
 Current name:  Scrophularia frutescens  L. (Scrophulariaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 832, DOI: 10.5281/zenodo.291971
Electronic and vibrational properties of V$_2$C-based MXenes: from experiments to first-principles modeling
Creators: name: Champagne, Aurélie
name: Shi, Lu
name: Ouisse, Thierry
name: Hackens, Benoît
name: Charlier, Jean-Christophe
Publisher: name: arXiv
Year: 2017
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: In the present work, the electronic and vibrational properties of both pristine V$_2$C and fully-terminated V$_2$CT$_2$ (where T = F, O, OH) 2D monolayers are investigated using density functional theory. Firstly, the atomic structures of V$_2$C-based MXene phases are optimized and their respective dynamical stabilities are discussed. Secondly, electronic band structures are computed indicating that V$_2$C is metallic as well as all the corresponding functionalized systems. Thirdly, the vibrational properties (phonon frequencies and spectra) of V$_2$C-based MXenes are computed thanks to density functional perturbation theory and reported for the first time. Both Raman (E$_g$, A$_{1g}$) and infrared active (E$_u$, A$_{2u}$) vibrational modes are predicted \textit{ab initio} with the aim to correlate the experimental Raman peaks with the calculated vibrational modes and to assign them with specific atomic motions. The effect of the terminal groups on the vibrational properties is emphasized as well as on the presence and position of the corresponding Raman peaks. Our results provide new insights for the identification and characterization of V$_2$C-based samples using Raman spectroscopy.
Non-LTE modeling of supernova-fallback disks
Creators: name: Werner, K.
name: Nagel, T.
name: Rauch, T.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a first detailed spectrum synthesis calculation of a supernova-fallback disk composed of iron. We assume a geometrically thin disk with a radial structure described by the classical alpha-disk model. The disk is represented by concentric rings radiating as plane-parallel slabs. The vertical structure and emission spectrum of each ring is computed in a fully self-consistent manner by solving the structure equations simultaneously with the radiation transfer equations under non-LTE conditions. We describe the properties of a specific disk model and discuss various effects on the emergent UV/optical spectrum. We find that strong iron-line blanketing causes broad absorption features over the whole spectral range. Limb darkening changes the spectral distribution up to a factor of four depending on the inclination angle. Consequently, such differences also occur between a blackbody spectrum and our model. The overall spectral shape is independent of the exact chemical composition as long as iron is the dominant species. A pure iron composition cannot be distinguished from silicon-burning ash. Non-LTE effects are small and restricted to few spectral features.
description: ApSS, accepted, Proceedings of Isolated Neutron Stars: from the Interior to the Surface, April 24-28, 2006, London, UK
MOESM1 of Efficacy and safety of artemether–lumefantrine, artesunate–amodiaquine, and dihydroartemisinin–piperaquine for the treatment of uncomplicated Plasmodium falciparum malaria in three provinces in Angola, 2017
Creators: name: Davlantes, Elizabeth
name: Dimbu, Pedro
name: Ferreira, Carolina
name: Joao, Maria Florinda
name: Dilunvuidi Pode
name: Félix, Jacinto
name: Sanhangala, Edgar
name: Andrade, Benjamin
name: Samaly Santos Souza
name: Talundzic, Eldin
name: Venkatachalam Udhayakumar
name: Owens, Chantelle
name: Mbounga, Eliane
name: Wiesner, Lubbe
name: Halsey, Eric
name: Martins, José
name: Fortes, Filomeno
name: Plucinski, Mateusz
Publisher: name: figshare
Year: 2018
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Additional file 1. Consort flow diagrams for follow-up outcomes in all six study arms, 2017.
Regge and Okamoto symmetries
Creators: name: Boalch, Philip
Publisher: name: arXiv
Year: 2006
Subjects: subject: Representation Theory (math.RT)
subject: Quantum Algebra (math.QA)
subject: FOS: Mathematics

description: We will relate the surprising Regge symmetry of the Racah-Wigner 6j symbols to the surprising Okamoto symmetry of the Painleve VI differential equation. This then presents the opportunity to give a conceptual derivation of the Regge symmetry, as the representation theoretic analogue of the author's previous derivation of the Okamoto symmetry. [The resulting derivation is quite simple, so it would be surprising if it has not been previously observed. Any references would be appreciated!]
description: 14 pages
Composition and distribution of sedimentary organic matter in nearshore Berriasian strata ('German Wealden') of the eastern Lower Saxony Basin, NW Germany
Creators: name: Stoepke, Fritz-Lukas
name: Götz, Annette E.
name: Blumenberg, Martin
name: Gravendyck, Julia
name: Erbacher, Jochen
name: Pierau, Roberto
name: Schöner, Robert
name: Heimhofer, Ulrich
Publisher: name: Geological Society of London
Year: 2024
Subjects: classificationCode: 3705
subject: Geology
subject: FOS: Earth and related environmental sciences

description: Tables showing geochemical data, palynofacies data and palynofacies counts
Mid-infrared Electro-Optic Modulation in Few-layer Black Phosphorus
Creators: name: Peng, Ruoming
name: Khaliji, Kaveh
name: Youngblood, Nathan
name: Grassi, Roberto
name: Low, Tony
name: Li, Mo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Black phosphorus stands out from the family of two-dimensional materials as a semiconductor with a direct, layer-dependent bandgap in energy corresponding to the spectral range from the visible to the mid-infrared (mid-IR), as well as many other attractive optoelectronic attributes. It is, therefore, a very promising material for various optoelectronic applications, particularly in the important mid-IR range. While mid-IR technology has been advancing rapidly, both photodetection and electro-optic modulation in the mid-IR rely on narrow-band compound semiconductors, which are difficult and expensive to integrate with the ubiquitous silicon photonics. For mid-IR photodetection, black phosphorus has been proven to be a viable alternative. Here, we demonstrate electro-optic modulation of mid-IR absorption in few-layer black phosphorus under field applied by an electrostatic gate. Our experimental and theoretical results find that, within the doping range obtainable in our samples, the quantum confined Franz-Keldysh effect is the dominant mechanism of electro-optic modulation. Spectroscopic study on samples with varying thickness reveals strong layer-dependence in the inter-band transition between different sub-bands. Our results show black phosphorus is a very promising material to realizing efficient mid-IR modulators.
Statistical Algorithms for Identification of Astronomical X-Ray Sources
Creators: name: Ziaeepour, Houri
name: Rosen, Simon
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: Observations of present and future X-ray telescopes include a large number of serendipidious sources of unknown types. They are a rich source of knowledge about X-ray dominated astronomical objects, their distribution, and their evolution. The large number of these sources does not permit their individual spectroscopical follow-up and classification. Here we use Chandra Multi-Wavelength public data to investigate a number of statistical algorithms for classification of X-ray sources with optical imaging follow-up. We show that up to statistical uncertainties, each class of X-ray sources has specific photometric characteristics which can be used for its classification. We assess the relative and absolute performance of classification methods and measured features by comparing the behaviour of physical quantities for statistically classified objects with what is obtained from spectroscopy. We find that among methods we have studied, multi-dimensional probability distribution is the best for both classifying source type and redshift, but it needs a sufficiently large input (learning) data set. In absence of such data, a mixture of various methods can give a better final result. We also discuss the enhancement of information obtained from statistical identification, and the effect of classification method and the input set on the astronomical conclusions about distribution and properties of the X-ray selected sources.
description: 23 pages, 16 figures, 3 tables. Figures should be printed in color. v2 accepted for publication in Astron. Nachr
On a Minkowski-like inequality for asymptotically flat static manifolds
Creators: name: McCormick, Stephen
Publisher: name: arXiv
Year: 2017
Subjects: subject: Differential Geometry (math.DG)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 53C20 (Primary), 83C99, 53C44 (Secondary)

description: The Minkowski inequality is a classical inequality in differential geometry, giving a bound from below, on the total mean curvature of a convex surface in Euclidean space, in terms of its area. Recently there has been interest in proving versions of this inequality for manifolds other than R^n; for example, such an inequality holds for surfaces in spatial Schwarzschild and AdS-Schwarzschild manifolds. In this note, we adapt a recent analysis of Y. Wei to prove a Minkowski-like inequality for general static asymptotically flat manifolds.
description: 10 pages. Proc. Amer. Math. Soc. V4: Fixed typo in eq (1.1)
Sharp geometric condition for null-controllability of the heat equation on $\mathbb{R}^d$ and consistent estimates on the control cost
Creators: name: Egidi, Michela
name: Veselic, Ivan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: In this note we study the control problem for the heat equation on $\mathbb{R}^d$, $d\geq 1$, with control set $ω\subset\mathbb{R}^d$. We provide a necessary and sufficient condition (called $(γ, a)$-\emph{thickness}) on $ω$ such that the heat equation is null-controllable in any positive time. We give an estimate of the control cost with explicit dependency on the characteristic geometric parameters of the control set. Finally, we derive a control cost estimate for the heat equation on cubes with periodic, Dirichlet, or Neumann boundary conditions, where the control sets are again assumed to be thick. We show that the control cost estimate is consistent with the $\mathbb{R}^d$ case.
description: To appear in Archiv der Mathematik with DOI :10.1007/s00013-018-1185-x. A section added with discussion of approximation of the control problem on cubes by the control problem on whole Euclidean space
Twisted Flavors and Tri/bi-Maximal Neutrino Mixing
Creators: name: Haba, Naoyuki
name: Watanabe, Atsushi
name: Yoshioka, Koichi
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A new framework for handling flavor symmetry breaking in the neutrino sector is discussed where the source of symmetry breaking is traced to the global property of right-handed neutrinos in extra-dimensional space. Light neutrino phenomenology has rich and robust predictions such as the tri/bi-maximal form of generation mixing, controlled mass spectrum, and no need of flavor mixing couplings in the theory.
description: 11 pages
Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
Creators: name: Côté, Benoit
name: Silvia, Devin
name: O'Shea, Brian W.
name: Smith, Britton
name: Wise, John H.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use a cosmological hydrodynamic simulation calculated with Enzo and the semi-analytic galaxy formation model (SAM) GAMMA to address the chemical evolution of dwarf galaxies in the early universe. The long-term goal of the project is to better understand the origin of metal-poor stars and the formation of dwarf galaxies and the Milky Way halo by cross-validating these theoretical approaches. We combine GAMMA with the merger tree of the most massive galaxy found in the hydrodynamic simulation and compare the star formation rate, the metallicity distribution function (MDF), and the age-metallicity relationship predicted by the two approaches. We found that the SAM can reproduce the global trends of the hydrodynamic simulation. However, there are degeneracies between the model parameters and more constraints (e.g., star formation efficiency, gas flows) need to be extracted from the simulation to isolate the correct semi-analytic solution. Stochastic processes such as bursty star formation histories and star formation triggered by supernova explosions cannot be reproduced by the current version of GAMMA. Non-uniform mixing in the galaxy's interstellar medium, coming primarily from self-enrichment by local supernovae, causes a broadening in the MDF that can be emulated in the SAM by convolving its predicted MDF with a Gaussian function having a standard deviation of ~0.2 dex. We found that the most massive galaxy in the simulation retains nearby 100% of its baryonic mass within its virial radius, which is in agreement with what is needed in GAMMA to reproduce the global trends of the simulation.
description: 26 pages, 13 figures, 2 tables, submitted to ApJ (version 2)
Additional file 3: of Metabolic correlates of reserve and resilience in MCI due to Alzheimer's Disease (AD)
Creators: name: Bauckneht, Matteo
name: Chincarini, Andrea
name: Piva, Roberta
name: Arnaldi, Dario
name: Girtler, Nicola
name: Massa, Federico
name: Pardini, Matteo
name: Grazzini, Matteo
name: Hulya Efeturk
name: Pagani, Marco
name: Sambuceti, Gianmario
name: Nobili, Flavio
name: Morbelli, Silvia
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology
subject: Marine Biology

description: Supplementary Table. (DOCX 22 kb)
Effects of Misorientation on Single Crystal Plasticity by Finite Element Methods
Creators: name: Shimanek, John D.
name: Liu, Zi-Kui
name: Beese, Allison M.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The crystal plasticity finite element method (CPFEM) is a widely used technique for resolving macroscopic stress and strain onto the physically relevant length scales of grains and slip systems in ductile crystalline materials like structural metals. Here, the calibration of a CPFEM model for single crystal applications was found to depend critically on loading orientation, with an effect significant even at an angle of 0.1 degrees. Slight misorientation from high symmetry loading affected lattice rotation during tensile deformation, changing the number of active slip systems, and, as a result, the overall stress-strain behavior. The strongest misorientation effects occurred around the multi-slip orientations of [001], [111], [101], and [102], while the single slip orientation of [213] showed a negligible effect, as expected, and the double slip orientation of [112] showed less of an effect than [102] due to its relative lattice orientation stability. The magnitude of the misorientation effect increased dramatically with the strength of slip system interaction, which, in the chosen hardening framework, is represented by the latent hardening coefficient. In a case study on [001] Cu, offsets of 0.3-2.0 degrees gave stress values at an engineering strain of 0.25 that were lower by 15-18% relative to the direct loading values, highlighting the importance of exact orientations for single crystal plasticity parameterization and application.
The SSIP approach to solvation
Creators: name: Driver, Mark David
Publisher: name: Apollo - University of Cambridge Repository
Year: 2020
Subjects: Solvation
logP
VLE
chemistry
SSIP
SSIMPLE
simulation
prediction
computational
modelling
FGIP
Similarity

description: Intermolecular interactions, including hydrogen bonding, are important for governing many processes, including solvation, protein ligand binding and crystallisation. Previously in the Hunter group, the Surface Site Interaction Point (SSIP) model of intermolecular interactions has been used to describe molecules as a set of discrete hydrogen bonding sites. In this thesis I describe the prediction of phase properties using this molecular description, after giving an introduction to the wider area of phase property prediction. Experimental equilibrium constants for formation of hydrogen bonded complexes was collated to allow for the reparameterisation of the relationship used to convert calculated electrostatic potentials into the hydrogen bond parameters used to describe the interaction properties of SSIPs, and a curated database of this information was created. An overhaul of the software infrastructure, to allow greater exploitation of automation in the workflow, was undertaken. Canonicalisation of data formats for information produced during the calculation has also been undertaken to provide a foundation for work in the following chapters. Calculation of partition coefficients for a series of molecular datasets have been used to benchmark the performance of the surface site interaction model for liquids at equilibrium (SSIMPLE) which uses the SSIP description for molecules to calculate free energies. Functional Group Interaction Profiles (FGIP) describe the energy change of two solute SSIPs interacting as a function of solute SSIP values. These profiles provide insight into the strength of interactions within different solvents. A selection of profiles for a range of solvents are included as examples. The profiles provide a useful guide for how to tune interactions when designing systems which rely on intermolecular interactions for association. Consideration of the solvation free energy of a single SSIP in a solvent as a function of SSIP value, has led to the development of a metric for solvent similarity. The comparison of solvation free energy curves for different solvents and solvent mixtures led to the construction of similarity dendrograms that can be used for solvent selection in experimental systems. Expansion of the approach to be used to examine the temperature dependence of the interactions, allowed the exploration of vapour liquid equilibria.
description: EPSRC doctoral training studentship (grant code EP/M506485/1)
Scrophularia lucida Linnaeus 1759
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Scrophulariaceae
Scrophularia
Scrophularia lucida

description: Scrophularia lucida Linnaeus, Systema Naturae, ed. 10, 2: 1114. 1759.
["Habitat in Oriente, Creta, Neapoli, in ipsis muris Hydrunti."] Sp. Pl., ed. 2, 2: 866 (1763). RCN: 4492.
Type not designated.
Original material: none traced.
 Current name:  Scrophularia lucida  L. (Scrophulariaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 832, DOI: 10.5281/zenodo.291971
Quantum stabilization of a hedgehog type of cosmic string
Creators: name: Quandt, M.
name: Graham, N.
name: Weigel, H.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Within a slightly simplified version of the electroweak standard model we investigate the stabilization of cosmic strings by fermion quantum fluctuations. Previous studies of quantum energies considered variants of the Nielsen-Olesen profile embedded in the electroweak gauge group and showed that configurations are favored for which the Higgs vacuum expectation value drops near the string core and the gauge field is suppressed. This work found that the strongest binding was obtained from strings that differ significantly from Nielsen-Olesen configurations, deforming essentially only the Higgs field in order to generate a strong attraction without inducing large gradients. Extending this analysis, we consider the leading quantum correction to the energy per unit length of a hedgehog type string, which, in contrast to the Nielsen-Olesen configuration, contains a pseudoscalar field. To employ the spectral method we develop the scattering and bound state problems for fermions in the background of a hedgehog string. Explicit occupation of bound state levels leads to strings that carry the quantum numbers of the bound fermions. We discuss the parameter space for which stable, hedgehog type cosmic strings emerge and reflect on phenomenological consequences of these findings.
description: 34 pages
Memorandum Regarding Options in Import-Export Credit Decision Making
Creators: name: United States. White House
Publisher: name: The University of Texas at Austin
Year: 1964
Subjects: Box 232 Folder 5
Box 232 Folder 05
Yugoslavia -- Politics and government -- 1945-1980
Yugoslavia -- Foreign relations -- 1945-1980 -- Soviet Union

description: Memorandum from Bundy to President concerning the authorizations of export-import bank credit guarantees
The star formation histories of galaxies in the Sloan Digital Sky Survey
Creators: name: Panter, Ben
name: Jimenez, Raul
name: Heavens, Alan F.
name: Charlot, Stephane
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a MOPED analysis of ~3 x 10^5 galaxy spectra from the Sloan Digital Sky Survey Data Release Three (SDSS DR3), with a number of improvements in data, modelling and analysis compared with our previous analysis of DR1. The improvements include: modelling the galaxies with theoretical models at a higher spectral resolution of 3Å; better calibrated data; an extended list of excluded emission lines, and a wider range of dust models. We present new estimates of the cosmic star formation rate, the evolution of stellar mass density and the stellar mass function from the fossil record. In contrast to our earlier work the results show no conclusive peak in the star formation rate out to a redshift around 2 but continue to show conclusive evidence for `downsizing' in the SDSS fossil record. The star formation history is now in good agreement with more traditional instantaneous measures. The galaxy stellar mass function is determined over five decades of mass, and an updated estimate of the current stellar mass density is presented. We also investigate the systematic effects of changes in the stellar population modelling, the spectral resolution, dust modelling, sky lines, spectral resolution and the change of data set. We find that the main changes in the results are due to the improvements in the calibration of the SDSS data, changes in the initial mass function and the theoretical models used.
description: replaced to match accepted version in MNRAS
Permutations without long decreasing subsequences and random matrices
Creators: name: Sniady, Piotr
Publisher: name: arXiv
Year: 2006
Subjects: subject: Combinatorics (math.CO)
subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 05E10, 15A52, 60J65

description: We study the shape of the Young diagram λassociated via the Robinson-Schensted-Knuth algorithm to a random permutation in S_n such that the length of the longest decreasing subsequence is not bigger than a fixed number d; in other words we study the restriction of the Plancherel measure to Young diagrams with at most d rows. We prove that in the limit n\to\infty the rows of λbehave like the eigenvalues of a certain random matrix (traceless Gaussian Unitary Ensemble) with d rows and columns. In particular, the length of the longest increasing subsequence of such a random permutation behaves asymptotically like the largest eigenvalue of the corresponding random matrix.
description: 11 pages
Memorandum Regarding Germanic Relations
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1964
Subjects: Box 232 Folder 6
Box 232 Folder 06
Yugoslavia -- Politics and government -- 1945-1980
Yugoslavia -- Foreign relations -- 1945-1980 -- Soviet Union

description: Memorandum of conversation between Job, Yugoslav Press Attache, and David Klein discussing German stance on diplomatic relations, economic relations, and attitude of the U.S. towards Yugoslavia.
Non-Ergodic Delocalization in the Rosenzweig-Porter Model
Creators: name: von Soosten, Per
name: Warzel, Simone
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Physics (math-ph)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We consider the Rosenzweig-Porter model $H = V + \sqrt{T}\, Φ$, where $V$ is a $N \times N$ diagonal matrix, $Φ$ is drawn from the $N \times N$ Gaussian Orthogonal Ensemble, and $N^{-1} \ll T \ll 1$. We prove that the eigenfunctions of $H$ are typically supported in a set of approximately $NT$ sites, thereby confirming the existence of a previously conjectured non-ergodic delocalized phase. Our proof is based on martingale estimates along the characteristic curves of the stochastic advection equation satisfied by the local resolvent of the Brownian motion representation of $H$.
Hidden-Sector Spectroscopy with Gravitational Waves from Binary Neutron Stars
Creators: name: Croon, Djuna
name: Nelson, Ann E.
name: Sun, Chen
name: Walker, Devin G. E.
name: Xianyu, Zhong-Zhi
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show that neutron star binaries can be ideal laboratories to probe hidden sectors with a long range force. In particular, it is possible for gravitational wave detectors such as LIGO and Virgo to resolve the correction of waveforms from ultralight dark gauge bosons coupled to neutron stars. We observe that the interaction of the hidden sector affects both the gravitational wave frequency and amplitude in a way that cannot be fitted by pure gravity.
description: 7 pages, ApJL accepted version
Study on Strong Decays of $D_{sJ}(2632)$
Creators: name: Ke, Hong-Wei
name: Yu, Yan-Ming
name: Ding, Yi-Bing
name: Guo, Xin-Heng
name: Jin, Hong-Ying
name: Li, Xue-Qian
name: Shen, Peng-Nian
name: Wang, Guo-Li
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The resonance $D_{sJ}(2632)$ observed by SELEX, has attracted great interests and meanwhile brought up serious dispute. Its spin-parity, so far has not finally determined and if it exists, its quark-structure might be exotic. Following the previous literature where $D_{sJ}(2632)$ is assumed to be a radial-excited state of $1^-$, we consider the possibilities that it might be a $q\bar q$ ground state of $2^+$ or the first radial-excited state of $0^+$ $D_{sJ}(2317)$ and re-calculate its strong decay widths in terms of the Bethe-Salpeter equation. Our results indicate that there still is a sharp discrepancy between the theoretical evaluation and data.
description: 11 pages, 6 figures
Thermal runaway of metal nano-tips during intense electron emission
Creators: name: Kyritsakis, A.
name: Veske, M.
name: Eimre, K.
name: Zadin, V.
name: Djurabekova, F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: When an electron emitting tip is subjected to very high electric fields, plasma forms even under ultra high vacuum conditions. This phenomenon, known as vacuum arc, causes catastrophic surface modifications and constitutes a major limiting factor not only for modern electron sources, but also for many large-scale applications such as particle accelerators, fusion reactors etc. Although vacuum arcs have been studied thoroughly, the physical mechanisms that lead from intense electron emission to plasma ignition are still unclear. In this article, we give insights to the atomic scale processes taking place in metal nanotips under intense field emission conditions. We use multi-scale atomistic simulations that concurrently include field-induced forces, electron emission with finite-size and space-charge effects, Nottingham and Joule heating. We find that when a sufficiently high electric field is applied to the tip, the emission-generated heat partially melts it and the field-induced force elongates and sharpens it. This initiates a positive feedback thermal runaway process, which eventually causes evaporation of large fractions of the tip. The reported mechanism can explain the origin of neutral atoms necessary to initiate plasma, a missing key process required to explain the ignition of a vacuum arc. Our simulations provide a quantitative description of in the conditions leading to runaway, which shall be valuable for both field emission applications and vacuum arc studies.
MOESM1 of Analysis of factors associated with waiting times for GP appointments in Finnish health centres: a QUALICOPC study
Creators: name: Tolvanen, Elina
name: Koskela, Tuomas
name: Mattila, Kari
name: Kosunen, Elise
Publisher: name: figshare
Year: 2018
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. The description of the participants. This file contains a table considering the background factors of the current sample of patients.
Telegram Regarding Foreign Office Impressions
Creators: name: United States. Embassy (Belgrade)
Publisher: name: The University of Texas at Austin
Year: 1967
Subjects: Box 232 Folder 9
Box 232 Folder 09
Yugoslavia -- Politics and government -- 1945-1980
Yugoslavia -- Foreign relations -- 1945-1980 -- Soviet Union

description: Telegram documenting conversation with Acting Foreign Minister Dimitrij Vosnak concerning hardening of American position and dialogue on Middle East.
Telegram Regarding Televised Interview
Creators: name: United States. Embassy (Belgrade)
Publisher: name: The University of Texas at Austin
Year: 1966
Subjects: Box 232 Folder 9
Box 232 Folder 09
Yugoslavia -- Politics and government -- 1945-1980
Yugoslavia -- Foreign relations -- 1945-1980 -- Soviet Union

description: Telegram concerning Secretary for Foreign Affairs Nikezic's televised interview and text of commentary.
The Advanced Compton Telescope Mission
Creators: name: Boggs, Steven E.
name: Kurfess, James
name: Ryan, James
name: Aprile, Elena
name: Gehrels, Neil
name: Kippen, Marc
name: Leising, Mark
name: Oberlack, Uwe
name: Wunderer, Cornelia
name: Zych, Allen
name: Bloser, Peter
name: Harris, Michael
name: Hoover, Andrew
name: Klimenk, Alexei
name: Kocevski, Dan
name: McConnell, Mark
name: Milne, Peter
name: Novikova, Elena I.
name: Phlips, Bernard
name: Polsen, Mark
name: Sturner, Steven
name: Tournear, Derek
name: Weidenspointner, Georg
name: Wulf, Eric
name: Zoglauer, Andreas
name: Baring, Matthew
name: Beacom, John
name: Bildsten, Lars
name: Dermer, Charles
name: Hartmann, Dieter
name: Hernanz, Margarita
name: Smith, David
name: Starrfield, Sumner
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The Advanced Compton Telescope (ACT), the next major step in gamma-ray astronomy, will probe the fires where chemical elements are formed by enabling high-resolution spectroscopy of nuclear emission from supernova explosions. During the past two years, our collaboration has been undertaking a NASA mission concept study for ACT. This study was designed to (1) transform the key scientific objectives into specific instrument requirements, (2) to identify the most promising technologies to meet those requirements, and (3) to design a viable mission concept for this instrument. We present the results of this study, including scientific goals and expected performance, mission design, and technology recommendations.
description: NASA Vision Mission Concept Study Report, final version. (A condensed version of this report has been submitted to AIAA.)
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Cart. 193 (11 H 78), f. 0010r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0010r, 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 IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0010r, 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
Neutrino Mass and New Physics
Creators: name: Mohapatra, R. N.
name: Smirnov, A. Y.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We review the present state of and future outlook for our understanding of neutrino masses and mixings. We discuss what we think are the most important perspectives on the plausible and natural scenarios for neutrinos and what may have the most promise to throw light on the flavor problem of quarks and leptons. We focus on the seesaw mechanism which fits into the big picture of particle physics such as supersymmetry and grand unification providing a unified approach to flavor problem of quarks and leptons. We argue that in combination with family symmetries, this may be at the heart of a unified understanding of flavor puzzle. We also discuss other new physics ideas such as neutrinos in models with extra dimensions and possible theoretical implications of sterile neutrinos. We outline some tests for the various schemes.
description: 90 pages and 9 figures; With permission from the Annual Review of Nuclear and Particle Science. Final version of this material is scheduled to appear in the Annual Review of Nuclear and Particle Science Vol. 56, to be published in November 2006 by Annual Reviews (http://www.annualreviews.org); some references and parts of text updated
In-Silico Analysis of Benzo-Selenadiazole Hybrids: Reactivity and Anticancer Potential Assessed Through DFT, Molecular Dynamics, Molecular Docking, and ADMET
Creators: name: Enneiymy, Mohamed
name: Mohammad-Salim, Haydar A.
name: Oubella, Ali
name: de Julián-Ortiz, Jesus Vicente
name: Fofack, Hans Merlin Tsahnang
name: Alotaibi, Saad A.
name: Mbake, Maraf Mbah
name: Itto, My Youssef Ait
Publisher: name: Taylor & Francis
Year: 2025
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Hematology

description: Fighting cancer is challenging, but targeting apoptosis pathways offers hope. Caspases 3 and 7 cleave substrates, leading to key features like phosphatidylserine exposure, nuclear condensation, and DNA fragmentation, driving cancer cell death. This understanding aids in developing targeted therapies to selectively eliminate cancer cells. This study explores the synthesis, characterization, and in-silico analysis of carvone-isoxazoline-selenadiazole hybrids (11a–e) as potential anticancer agents. Advanced NMR techniques, including COSY, HSQC, and HMBC, confirmed the structural integrity of the benzo[1–3]selenadiazole core. Among the derivatives, 11c stood out with a low HOMO-LUMO energy gap of 3.2 eV, indicating high reactivity. MEPS analysis revealed biologically active sites at −0.85 and 1.2 eV, while biological evaluations demonstrated 11c’s ability to induce apoptosis via caspase-3 activation with an IC50 of 2.1 μM, similar to doxorubicin. Strong docking interactions with apoptosis-related proteins further support this. Mature caspases 3 and 7 cleave a broad set of substrates, ultimately leading to apoptotic features such as phosphatidylserine exposure, nuclear condensation, and DNA fragmentation. ADMET analysis revealed favorable pharmacokinetics, with a logP of 2.5, and low toxicity risks, with an LD50 value of >1000 mg/kg. Structure-activity relationships highlighted selenium’s pivotal role in enhancing activity. With potent anticancer properties and a promising drug profile, 11c is a compelling candidate for further cancer therapy development.
Pulsed Accretion in the T Tauri Binary TWA 3A
Creators: name: Tofflemire, Benjamin M.
name: Mathieu, Robert D.
name: Herczeg, Gregory J.
name: Akeson, Rachel L.
name: Ciardi, David R.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: TWA 3A is the most recent addition to a small group of young binary systems that both actively accrete from a circumbinary disk and have spectroscopic orbital solutions. As such, it provides a unique opportunity to test binary accretion theory in a well-constrained setting. To examine TWA 3A's time-variable accretion behavior, we have conducted a two-year, optical photometric monitoring campaign, obtaining dense orbital phase coverage (~20 observations per orbit) for ~15 orbital periods. From U-band measurements we derive the time-dependent binary mass accretion rate, finding bursts of accretion near each periastron passage. On average, these enhanced accretion events evolve over orbital phases 0.85 to 1.05, reaching their peak at periastron. The specific accretion rate increases above the quiescent value by a factor of ~4 on average but the peak can be as high as an order of magnitude in a given orbit. The phase dependence and amplitude of TWA 3A accretion is in good agreement with numerical simulations of binary accretion with similar orbital parameters. In these simulations, periastron accretion bursts are fueled by periodic streams of material from the circumbinary disk that are driven by the binary orbit. We find that TWA 3A's average accretion behavior is remarkably similar to DQ Tau, another T Tauri binary with similar orbital parameters, but with significantly less variability from orbit to orbit. This is only the second clear case of orbital-phase-dependent accretion in a T Tauri binary.
description: 6 pages, 4 figures
Telegram Regarding Meeting with Tito
Creators: name: United States. Embassy (Belgrade)
Publisher: name: The University of Texas at Austin
Year: 1968
Subjects: Box 232 Folder 12
Yugoslavia -- Politics and government -- 1945-1980
Yugoslavia -- Foreign relations -- 1945-1980 -- Soviet Union

description: Telegram recounting meeting with Ambassador Elbrick and Tito and discussions of impressions of Soviet intentions, Yugoslavia, and Jarring mission.
Memorandum Regarding Execution of PL-480 Agreement with Yugoslavia
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1966
Subjects: Box 232 Folder 14
Yugoslavia -- Politics and government -- 1945-1980
Yugoslavia -- Foreign relations -- 1945-1980 -- Soviet Union

description: Memorandum for the President concerning sale of edible oils to Yugoslavia as part of PL-480 agreement and relevant discussion points.
Telegram Regarding Fulbright Agreement
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1964
Subjects: Box 232 Folder 3
Box 232 Folder 03
Yugoslavia -- Politics and government -- 1945-1980
Yugoslavia -- Foreign relations -- 1945-1980 -- Soviet Union

description: Telegram concerning deferring signature until Senator Fulbright's arrival in Belgrade.
Scrophularia marilandica Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Scrophulariaceae
Scrophularia
Scrophularia marilandica

description: Scrophularia marilandica Linnaeus, Species Plantarum 2: 619. 1753.
"Habitat in Virginia." RCN: 4480.
 Lectotype (Reveal & al. in Huntia 7: 235. 1987): Clayton 220 (BM-000042216).
 Current name:  Scrophularia marilandica  L. (Scrophulariaceae).
 Note: Reveal & al. (in Huntia 7: 235. 1987) provide a review.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 832, DOI: 10.5281/zenodo.291971
A probabilistic view on the deterministic mutation-selection equation: dynamics, equilibria, and ancestry via individual lines of descent
Creators: name: Baake, Ellen
name: Cordero, Fernando
name: Hummel, Sebastian
Publisher: name: arXiv
Year: 2017
Subjects: subject: Probability (math.PR)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Mathematics
subject: FOS: Biological sciences
subject: 92D15, 60J28, 60J75, 05C80

description: We reconsider the deterministic haploid mutation-selection equation with two types. This is an ordinary differential equation that describes the type distribution (forward in time) in a population of infinite size. This paper establishes ancestral (random) structures inherent in this deterministic model. In a first step, we obtain a representation of the deterministic equation's solution (and, in particular, of its equilibrium) in terms of an ancestral process called the killed ancestral selection graph. This representation allows one to understand the bifurcations related to the error threshold phenomenon from a genealogical point of view. Next, we characterise the ancestral type distribution by means of the pruned lookdown ancestral selection graph and study its properties at equilibrium. We also provide an alternative characterisation in terms of a piecewise-deterministic Markov process. Throughout, emphasis is on the underlying dualities as well as on explicit results.
description: J. Math. Biol., in press
LIDAR - WP1.4
Creators: name: Arnaubec, Aurelien
name: Olu-Le Roy, Karine
name: Ferrera, Maxime
name: Escartin, Javier
Publisher: name: DeepSea'Nnovation
Year: 2023

description: Un outil novateur pour la métrologie topographique et l’imagerie à une échelle intermédiaire entre la bathymétrie acoustique et la reconstruction photogrammétrique
Active X-ray Optics for Generation-X, the Next High Resolution X-ray Observatory
Creators: name: Elvis, Martin
name: Brissenden, R. J.
name: Fabbiano, G.
name: Schwartz, D. A.
name: Reid, P.
name: Podgorski, W.
name: Eisenhower, M.
name: Juda, M.
name: Phillips, J.
name: Cohen, L.
name: Wolk, S.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: X-rays provide one of the few bands through which we can study the epoch of reionization, when the first galaxies, black holes and stars were born. To reach the sensitivity required to image these first discrete objects in the universe needs a major advance in X-ray optics. Generation-X (Gen-X) is currently the only X-ray astronomy mission concept that addresses this goal. Gen-X aims to improve substantially on the Chandra angular resolution and to do so with substantially larger effective area. These two goals can only be met if a mirror technology can be developed that yields high angular resolution at much lower mass/unit area than the Chandra optics, matching that of Constellation-X (Con-X). We describe an approach to this goal based on active X-ray optics that correct the mid-frequency departures from an ideal Wolter optic on-orbit. We concentrate on the problems of sensing figure errors, calculating the corrections required, and applying those corrections. The time needed to make this in-flight calibration is reasonable. A laboratory version of these optics has already been developed by others and is successfully operating at synchrotron light sources. With only a moderate investment in these optics the goals of Gen-X resolution can be realized.
description: Enhanced version of SPIE presentation. 11 pages, 5 figures
Spectromètre de masse in situ - WP2.1
Creators: name: Boulart, Cédric
name: Noel, Laura
name: Macé, Eric
Publisher: name: DeepSea'Nnovation
Year: 2023

description: Un spectromètre de masse miniaturisé pour la mesure in-situ et en temps réel des concentrations de gaz à haute résolution spatiale et temporelle