cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Fampridine Prolonged Release: A Review in Multiple Sclerosis Patients with Walking Disability
Creators: name: Kim, Esther S.
Publisher: name: Adis Journals
Year: 2018
Subjects: Medicine

description: Compliance with Ethical Standards
Funding: The preparation of this review was not supported by any external funding.
Conflicts of interest: Esther Kim is a salaried employee of Adis/Springer, is responsible for the article content and declares no relevant conflict of interest.
Additional information about this Adis Drug Review can be found here.
Abstract
Oral fampridine prolonged release (PR) [Fampyra®] is a lipid-soluble selective potassium channel blocker that is approved in the EU for the improvement of walking in adult multiple sclerosis (MS) patients with walking disability (expanded disability status scale score of 4–7). In clinical trials (MS-F203 and MS-F204) using an objective measure of walking improvement [the timed 25-foot walk (T25FW)], more than one-third of patients receiving fampridine PR achieved a consistent on-treatment improvement in walking speed (i.e. became TW responders) over 9–14 weeks of treatment. Fampridine PR recipients who fulfilled the definition of TW responder had mean improvements of ≈25% from baseline in T25FW walking speed. In a clinical trial (ENHANCE) that used a patient-rated measure of walking improvement [12-item MS walking scale (MSWS-12)], a significantly greater proportion of fampridine PR recipients than placebo recipients achieved a ≥8-point improvement on the MSWS-12 with 24 weeks of treatment. Where reported, adverse events were mostly mild or moderate in severity, and generally consistent with the underlying disease or mechanism of action of fampridine PR. Fampridine PR is a useful treatment option to consider in adult MS patients with walking disability. Access to the full article can be found here.
© Springer International Publishing AG, part of Springer Nature 2017
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Cart. 189 (11 H 74), 316 folios, f. 0268r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Archives départementales de la Côte-d'Or, Cart. 189 (11 H 74), 316 folios, f. 0268r, 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 V, Archives départementales de la Côte-d'Or, Cart. 189 (11 H 74), 316 folios, f. 0268r, 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
BFKL Pomeron in string models
Creators: name: Danilov, G. S.
name: Lipatov, L. N.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider scattering amplitudes in string models in the Regge limit of high energies and fixed momentum transfers with the use of the unitarity in direct channels. Intermediate states are taken in the multi-Regge kinematics corresponding to the production of resonances with fixed invariant masses and large relative rapidities. In QCD such kinematics leads to the BFKL equation for the Pomeron wave function in the leading logarithmic approximation. We derive a similar equation in the string theory and discuss its properties. The purpose of this investigation is to find a generalization of the BFKL approach to the region of small momentum transfers where non-perturbative corrections to the gluon Regge trajectory and reggeon couplings are essential. The BFKL equation in the string theory contains additional contributions coming from a linear part of the Regge trajectory and from the soft Pomeron singularity appearing already in the tree approximation. In higher dimensions in addition, a non-multi-Regge kinematics corresponding to production of particles with large masses is important. We solve the equation for the Pomeron wave function in the string theory for D=4 and discuss integrability properties of analogous equations for composite states of several reggeised gluons in the multi-colour limit.
description: 48 pages, 2 figures
Sharp one component regularity for Navier-Stokes
Creators: name: Han, Bin
name: Lei, Zhen
name: Li, Dong
name: Zhao, Na
Publisher: name: arXiv
Year: 2017
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: We consider the conditional regularity of mild solution $v$ to the incompressible Navier-Stokes equations in three dimensions. Let $e \in \mathbb{S}^2$ and $0 < T^\ast < \infty$. J. Chemin and P. Zhang \cite{CP} proved the regularity of $v$ on $(0,T^\ast]$ if there exists $p \in (4, 6)$ such that $$\int_0^{T^\ast}\|v\cdot e\|^p_{\dot{H}^{\frac{1}{2}+\frac{2}{p}}}dt < \infty.$$ J. Chemin, P. Zhang and Z. F. Zhang \cite{CPZ} extended the range of $p$ to $(4, \infty)$. In this article we settle the case $p \in [2, 4]$. Our proof also works for the case $p \in (4,\infty)$.
Higher-order topology in honeycomb lattice with Y-Kekulé distortions
Creators: name: Jiang, Yong-Cheng
name: Kariyado, Toshikaze
name: Hu, Xiao
Publisher: name: arXiv
Year: 2024
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We investigate higher-order topological states in honeycomb lattice with Y-Kekulé distortions that preserve $C_{6v}$ crystalline symmetry. The gapped states in expanded and shrunken distortions are adiabatically connected to isolated hexamers and Y-shaped tetramer states, respectively, where the former possesses nontrivial higher-order topology characterized by a $\mathbb{Z}_6$ invariant. Topological corner states exist in a flake structure with expanded distortion where the hexamers are broken at the corners. Our work reveals that honeycomb lattice with Y-Kekulé distortions serves as a promising platform to study higher-order topological states.
description: 5 pages, 3 figures
Mementos of GNR Charles F Dickinson
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: Many mementos of GNR Charles F Dickinson No 967217, the second son of 9 siblings.
The effect of double counting, spin density, and Hund interaction in the different DFT+$U$ functionals
Creators: name: Ryee, Siheon
name: Han, Myung Joon
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A systematic comparative study has been performed to better understand DFT$+U$ (density functional theory + $U$) method. We examine the effect of choosing different double counting and exchange-correlation functionals. The calculated energy distribution and the Hund-$J$ dependence of potential profile for representative configurations clearly show the different behaviors of each DFT$+U$ formalism. In particular, adopting spin-dependent exchange-correlation functionals likely leads to undesirable magnetic solution. Our analyses are further highlighted by real material examples ranging from insulating oxides (MnO and NiO) to metallic magnetic systems (SrRuO$_3$ and BaFe$_2$As$_2$). The current work sheds new light on understanding DFT$+U$ and provides a guideline to use the related methods.
description: Accepted for publication in Scientific Reports
Rolapitant: A Review in Chemotherapy-Induced Nausea and Vomiting
Creators: name: Young-A Heo
name: Deeks, Emma
Publisher: name: Adis Journals
Year: 2018
Subjects: Medicine

description: Compliance with Ethical Standards
Funding: The preparation of this review was not supported by any external funding.
Conflicts of interest: Young-A Heo and Emma Deeks are salaried employees of Adis/Springer, are responsible for the article contentand declare no relevant conflicts of interest/a potential conflict of interest.
Additional information about this Adis Drug Review can be found here.
Abstract
Oral rolapitant (Varubi™; Varuby®), a long-acting neurokinin-1 (NK1) receptor antagonist (RA), is indicated in the USA and EU as part of an antiemetic regimen to prevent delayed chemotherapy-induced nausea and vomiting (CINV) in adults receiving highly or moderately emetogenic chemotherapy (HEC or MEC). In randomized, phase III trials, a single oral dose of rolapitant 180 mg was effective in preventing delayed CINV compared with placebo, when each was used in combination with a 5-HT3 RA plus dexamethasone, in adults receiving their first course of HEC or MEC. The benefits of rolapitant were maintained over multiple cycles of chemotherapy. The tolerability profile of rolapitant is similar to that of placebo and consistent with that of other NK1 RAs. However, rolapitant differs from other existing NK1 RAs in that it does not interact with CYP3A4, thereby negating the need for dexamethasone dose adjustments and potentially making rolapitant a more suitable option for patients receiving CYP3A4 substrates. Thus, oral rolapitant is an effective and well tolerated NK1 RA that expands the treatment options for preventing delayed CINV in adults receiving HEC or MEC. Access to the full article can be found here.
© Springer International Publishing AG, part of Springer Nature 2017
Fimbristylis autumnalis Roem. & Schult.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Cyperaceae
Fimbristylis
Fimbristylis autumnalis

description: Scirpus autumnalis Linnaeus, Mantissa Plantarum Altera: 180. 1771.
"Habitat in Virginia." RCN: 417.
 Lectotype (Blake in Rhodora 20: 24. 1918): Clayton 772 (BM-000553915; iso- LINN 71.24).
 Current name:  Fimbristylis autumnalis  (L.) Roem. & Schult. (Cyperaceae).
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 828, DOI: 10.5281/zenodo.291971
Spin foam propagator: A new perspective to include a cosmological constant
Creators: name: Han, Muxin
name: Huang, Zichang
name: Zipfel, Antonia
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In recent years, the calculation of the first non-vanishing order of the metric 2-point function or graviton propagator in a semiclassical limit has evolved as a standard test for the credibility of a proposed spin foam model. The existing results of spinfoam graviton propagator rely heavily on the so-called double scaling limit where spins $j$ are large and the Barbero-Immirzi parameter $γ$ is small such that the area $A\propto jγ$ is approximately constant. However, it seems that this double scaling limit is bound to break down in models including a cosmological constant. We explore this in detail for the recently proposed model by Haggard, Han, Kaminski and Riello and discuss alternative definitions of a graviton propagator, in which the double scaling limit can be avoided.
description: 15 pages, 1 figure
A Manchester Family's Contributions and Sacrifices
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: Two photographs attached- of Kathleen Walker in her ATS uniform. One of her brothers was in intelligence. W Walker was the eldest, and then her younger brother L Walker was a pilot. She lived in Manchester at this point. Therefore, all the family were involved and had a role to play in the Second World War.My father's logbook depicts him flying a spitfire on 28th November 1942. In the book, he details the flight over Tunis. He was attacked and shot down. Details are included of his injuries and how his 2nd was shot down and killed. The book records how many hours they flew, where they went and when. Logbook 2 outlines what he did after being shot down.The air force diary records what happened on 28th November 1942 when he got shot down. The diary is a lot more detailed and personal compared to his logbook. Attached is a printed copy of what is written in the diary as its difficult to read.The letter attached to his parents is interesting. It is dated 24th December 1942 as he is still in Africa in December, even though he was shot down in November. All letters were numbered (this is number 10) as they didn’t know when and in what order the letters would be received. It was his first Christmas ever away from home.
Fusion reactions in multicomponent dense matter
Creators: name: Yakovlev, D. G.
name: Gasques, L. R.
name: Beard, M.
name: Wiescher, M.
name: Afanasjev, A. V.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We analyze thermonuclear and pycnonuclear fusion reactions in dense matter containing atomic nuclei of different types. We extend a phenomenological expression for the reaction rate, proposed recently by Gasques et al. (2005) for the one-component plasma of nuclei, to the multi-component plasma. The expression contains several fit parameters which we adjust to reproduce the best microscopic calculations available in the literature. Furthermore, we show that pycnonuclear burning is drastically affected by an (unknown) structure of the multi-component matter (a regular lattice, a uniform mix, etc.). We apply the results to study nuclear burning in a carbon_12-oxygen_16 mixture. In this context we present new calculations of the astrophysical S-factors for carbon-oxygen and oxygen-oxygen fusion reactions. We show that the presence of a CO lattice can strongly suppress carbon ignition in white dwarf cores and neutron star crusts at densities > 3e9 g cm^{-3} and temperatures T<1e8 K.
description: 16 pages, 5 figures, to appear in Phys. Rev. C
Transverse-Momentum Resummation for Slepton-Pair Production at the LHC
Creators: name: Bozzi, G.
name: Fuks, B.
name: Klasen, M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We perform a first precision calculation of the transverse-momentum (q_T) distribution of slepton pair and slepton-sneutrino associated production at the CERN Large Hadron Collider (LHC). We implement soft-gluon resummation at the next-to-leading logarithmic (NLL) level and consistently match the obtained result to the pure fixed-order perturbative result at leading order (LO) in the QCD coupling constant, i.e. O(alpha_s). We give numerical predictions for stau_1 stau_1^* and stau_1 sneutrino_tau^* + stau_1^* sneutrino_tau production, also implementing recent parameterizations of non-perturbative effects. The results show a relevant contribution of resummation both in the small and intermediate q_T-regions and little dependence on unphysical scales and non-perturbative contributions.
description: 4 pages, 2 figures
The inverse problem of the calculus of variations for discrete systems
Creators: name: Barbero-Liñán, María
name: Puiggalí, Marta Farré
name: Ferraro, Sebastián
name: de Diego, David Martín
Publisher: name: arXiv
Year: 2017
Subjects: subject: Differential Geometry (math.DG)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 37M15, 49N45, 53D12, 58E30, 65P10, 70F25

description: We develop a geometric version of the inverse problem of the calculus of variations for discrete mechanics and constrained discrete mechanics. The geometric approach consists of using suitable Lagrangian and isotropic submanifolds. We also provide a transition between the discrete and the continuous problems and propose variationality as an interesting geometric property to take into account in the design and computer simulation of numerical integrators.
description: 30 pages
Image denoising by statistical area thresholding
Creators: name: Coupier, David
name: Desolneux, Agnès
name: Ycart, Bernard
Publisher: name: arXiv
Year: 2006
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 68U10, 62H35

description: Area openings and closings are morphological filters which efficiently suppress impulse noise from an image, by removing small connected components of level sets. The problem of an objective choice of threshold for the area remains open. Here, a mathematical model for random images will be considered. Under this model, a Poisson approximation for the probability of appearance of any local pattern can be computed. In particular, the probability of observing a component with size larger than $k$ in pure impulse noise has an explicit form. This permits the definition of a statistical test on the significance of connected components, thus providing an explicit formula for the area threshold of the denoising filter, as a function of the impulse noise probability parameter. Finally, using threshold decomposition, a denoising algorithm for grey level images is proposed.
Project VeSElkA: Abundance analysis of chemical species in HD41076 and HD148330
Creators: name: Khalack, V.
name: Gallant, G.
name: Thibeault, C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences
subject: J.2

description: A new semi-automatic approach is employed to carry out the abundance analysis of high-resolution spectra of HD41076 and HD148330 obtained recently with the spectropolarimetre ESPaDOnS at the CFHT. This approach allows to prepare in a semi-automatic mode the input data for the modified ZEEMAN2 code and to analyse several hundreds of line profiles in sequence during a single run. It also provides more information on abundance distribution for each chemical element at the deeper atmospheric layers. Our analysis of the Balmer profiles observed in the spectra of HD41076 and HD148330 has resulted in the estimates of their effective temperature, gravity, metallicity and radial velocity. The respective models of stellar atmosphere have been calculated with the code PHOENIX and used to carry out abundance analysis employing the modified ZEEMAN2 code. The analysis shows a deficit of the C, N, F, Mg, Ca, Ti, V, Cu, Y, Mo, Sm and Gd, and overabundance of Cr, Mn, Fe, Co, Ni, Sr, Zr, Ba, Ce, Nd and Dy in the stellar atmosphere of HD41076. In the atmosphere of HD148330, the C, N and Mo appear to be underabundant, while the Ne, Na, Al, Si, P, Ca, Ti, V, Cr, Mn, Fe, Co, Ni, Zn, Sr, Y, Zr, Ba, Ce, Pr, Nd, Sm, Eu, Gd and Dy are overabundant. We also have found signatures of vertical abundance stratification of Fe, Ti, Cr and Mn in HD41076, and of Fe, Ti, V, Cr, Mn, Y, Zr, Ce, Nd, Sm and Gd in HD148330.
description: 15 pages, 7 figures, 8 tables, accepted for publication in MNRAS
On the Search For Transits of the Planets Orbiting Gl 876
Creators: name: Shankland, P. D.
name: Rivera, E. J.
name: Laughlin, G.
name: Blank, D. L.
name: Price, A.
name: Gary, B.
name: Bissinger, R.
name: Ringwald, F.
name: White, G.
name: Henry, G. W.
name: McGee, P.
name: Wolf, A. S.
name: Carter, B.
name: Lee, S.
name: Biggs, J.
name: Monard, B.
name: Ashley, M. C. B.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results of a globally coordinated photometric campaign to search for transits by the P ~ 30 d and P ~ 60 d outer planets of the 3-planet system orbiting the nearby M-dwarf Gl 876. These two planets experience strong mutual perturbations, which necessitate use of a dynamical (four-body) model to compute transit ephemerides for the system. Our photometric data have been collected from published archival sources, as well as from our photometric campaigns that were targeted to specific transit predictions. Our analysis indicates that transits by planet "c" (P ~ 30 d) do not currently occur, in concordance with the best-fit i = 50 degree co-planar configuration obtained by dynamical fits to the most recent radial velocity data for the system. Transits by planet "b" (P ~ 60 d) are not entirely ruled out by our observations, but our data indicate that it is very unlikely that they occur. Our experience with the Gl 876 system suggests that a distributed ground-based network of small telescopes can be used to search for transits of very low mass M-stars by terrestrial-sized planets.
description: currently 17pp w/Figs, 10 figures; to appear in Astrophysical Journal article December 2006 v653n1
title:  Il convegno triennale dell’Associazione Italiana Paleografi e Diplomatisti ‘Lo scritto che non ti aspetti: Forme erratiche di libri, scritture, documenti (Roma, 12-14 settembre 2024)
Creators: name: De Luca, Elena
Publisher: name: Roma Tre University
publisherIdentifier: https://ror.org/05vf0dg29
publisherIdentifierScheme: ROR
Year: 2025

description: Cronaca del convegno dell’Associazione Italiana Paleografi e Diplomatisti (Roma, 12-14 settembre 2024), su ‘Lo scritto che non ti aspetti: Forme erratiche di libri, scritture, documenti’.

Report of the conference of the Italian Association of Paleographers and Diplomatists (Rome, 12-14 September 2024), on ‘The writing you don’t expect: Erratic forms of books, writings, documents’.
description: Cronaca del convegno dell’Associazione Italiana Paleografi e Diplomatisti (Roma, 12-14 settembre 2024), su ‘Lo scritto che non ti aspetti: Forme erratiche di libri, scritture, documenti’.

Report of the conference of the Italian Association of Paleographers and Diplomatists (Rome, 12-14 September 2024), on ‘The writing you don’t expect: Erratic forms of books, writings, documents’.
Energetics of the Kelvin-Helmholtz instability induced by transverse waves in twisted coronal loops
Creators: name: Howson, Thomas
name: De Moortel, Ineke
name: Antolin, Patrick
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Aims: We quantify the effects of twisted magnetic fields on the development of the magnetic Kelvin-Helmholtz instability (KHI) in transversely oscillating coronal loops. Methods: We modelled a fundamental standing kink mode in a straight, density-enhanced magnetic flux tube using the magnetohydrodynamics code, Lare3d. In order to evaluate the impact of an azimuthal component of the magnetic field, various degrees of twist were included within the flux tube's magnetic field. Results: The process of resonant absorption is only weakly affected by the presence of a twisted magnetic field. However, the subsequent evolution of the KHI is sensitive to the strength of the azimuthal component of the field. Increased twist values inhibit the deformation of the loop's density profile, which is associated with the growth of the instability. Despite this, much smaller scales in the magnetic field are generated when there is a non-zero azimuthal component present. Hence, the instability is more energetic in cases with (even weakly) twisted fields. Field aligned flows at the loop apex are established in a twisted regime once the instability has formed. Conclusions: The KHI may have implications for wave heating in the solar atmosphere due to the creation of small length scales and the generation of a turbulent regime. Whilst magnetic twist does suppress the development of the vortices associated with the instability, the formation of the KHI in a twisted regime will be accompanied by greater Ohmic dissipation due to the larger currents that are produced, even if only weak twist is present. The presence of magnetic twist will likely make the instability more difficult to detect in the corona, but will enhance its contribution to heating the solar atmosphere.
The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
Creators: name: Scolnic, D. M.
name: Jones, D. O.
name: Rest, A.
name: Pan, Y. C.
name: Chornock, R.
name: Foley, R. J.
name: Huber, M. E.
name: Kessler, R.
name: Narayan, G.
name: Riess, A. G.
name: Rodney, S.
name: Berger, E.
name: Brout, D. J.
name: Challis, P. J.
name: Drout, M.
name: Finkbeiner, D.
name: Lunnan, R.
name: Kirshner, R. P.
name: Sanders, N. E.
name: Schlafly, E.
name: Smartt, S.
name: Stubbs, C. W.
name: Tonry, J.
name: Wood-Vasey, W. M.
name: Foley, M.
name: Hand, J.
name: Johnson, E.
name: Burgett, W. S.
name: Chambers, K. C.
name: Draper, P. W.
name: Hodapp, K. W.
name: Kaiser, N.
name: Kudritzki, R. P.
name: Magnier, E. A.
name: Metcalfe, N.
name: Bresolin, F.
name: Gall, E.
name: Kotak, R.
name: McCrum, M.
name: Smith, K. W.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present optical light curves, redshifts, and classifications for 365 spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium Deep Survey. We detail improvements to the PS1 SN photometry, astrometry and calibration that reduce the systematic uncertainties in the PS1 SN Ia distances. We combine the subset of 279 PS1 SN Ia ($0.03 < z < 0.68$) with useful distance estimates of SN Ia from SDSS, SNLS, various low-z and HST samples to form the largest combined sample of SN Ia consisting of a total of 1048 SN Ia ranging from $0.01 < z < 2.3$, which we call the `Pantheon Sample'. When combining Planck 2015 CMB measurements with the Pantheon SN sample, we find $Ω_m=0.307\pm0.012$ and $w = -1.026\pm0.041$ for the wCDM model. When the SN and CMB constraints are combined with constraints from BAO and local H0 measurements, the analysis yields the most precise measurement of dark energy to date: $w0 = -1.007\pm 0.089$ and $wa = -0.222 \pm0.407$ for the w0waCDM model. Tension with a cosmological constant previously seen in an analysis of PS1 and low-z SNe has diminished after an increase of $2\times$ in the statistics of the PS1 sample, improved calibration and photometry, and stricter light-curve quality cuts. We find the systematic uncertainties in our measurements of dark energy are almost as large as the statistical uncertainties, primarily due to limitations of modeling the low-redshift sample. This must be addressed for future progress in using SN Ia to measure dark energy.
description: Accepted by ApJ. Data can be found here: http://dx.DOI.org/10.17909/T95Q4X
On Kasner solution in Bianchi I $f(T)$ cosmology
Creators: name: Skugoreva, Maria A.
name: Toporensky, Alexey V.
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Recently cosmological dynamics of anisotropic Universe in $f(T)$ gravity became an area of intense investigations. Some earlier papers devoted to this issue contain contradictory claims about the nature and propertied of vacuum solutions in this theory. The goal of the present paper is to clarify this situation. We compare properties of $f(T)$ and $f(R)$ vacuum solutions and outline differences between them. The Kasner solution appears to be an exact solution for the $T=0$ branch, and an asymptotic solution for $T \ne 0$ branch. It is shown that Kasner solution is the past attractor if $T<0$, being past and future attractor for $T>0$ branch.
description: 11 pages, 7 figures, v3: some new results added, v4: some clarifications added
Index formula for MacPherson cycles of affine algebraic varieties
Creators: name: Schuermann, Joerg
name: Tibar, Mihai
Publisher: name: arXiv
Year: 2006
Subjects: subject: Algebraic Geometry (math.AG)
subject: Complex Variables (math.CV)
subject: FOS: Mathematics
subject: 14C25; 14C17; 14R25; 32S60; 14D06; 32S20

description: We give explicit MacPherson cycles for the Chern-MacPherson class of a closed affine algebraic variety $X$ and for any constructible function $α$ with respect to a complex algebraic Whitney stratification of $X$. We define generalized degrees of the global polar varieties and of the MacPherson cycles and we prove a global index formula for the Euler characteristic of $α$. Whenever $α$ is the Euler obstruction of $X$, this index formula specializes to the Seade-Tibar-Verjovsky global counterpart of the Le-Teissier formula for the local Euler obstruction.
description: 17 pages, shorter version, same results
Application of a Zero-latency Whitening Filter to Compact Binary Coalescence Gravitational-wave Searches
Creators: name: Tsukada, Leo
name: Cannon, Kipp
name: Hanna, Chad
name: Keppel, Drew
name: Meacher, Duncan
name: Messick, Cody
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Joint electromagnetic and gravitational-wave (GW) observation is a major goal of both the GW astronomy and electromagnetic astronomy communities for the coming decade. One way to accomplish this goal is to direct follow-up of GW candidates. Prompt electromagnetic emission may fade quickly, therefore it is desirable to have GW detection happen as quickly as possible. A leading source of latency in GW detection is the whitening of the data. We examine the performance of a zero-latency whitening filter in a detection pipeline for compact binary coalescence (CBC) GW signals. We find that the filter reproduces signal-to-noise ratio (SNR) sufficiently consistent with the results of the original high-latency and phase-preserving filter for both noise and artificial GW signals (called "injections"). Additionally, we demonstrate that these two whitening filters show excellent agreement in $χ^2$ value, a discriminator for GW signals.
description: 8 pages, 12 figures
The fundamental symmetries in the neutral kaon system -- a pedagogical choice --
Creators: name: Fidecaro, Maria
name: Gerber, Hans-Juerg
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: During the recent years experiments with neutral kaons have yielded remarkably sensitive results which are pertinent to such fundamental phenomena as CPT invariance (protecting causality), time-reversal invariance violation, coherence of wave functions, and entanglement of kaons in pair states. We describe the phenomenological developments and the theoretical conclusions drawn from the experimental material. An outlook to future experimentation is indicated. An overview of formal similarities in fields outside neutral kaons is included.
description: 63 pages, 15 figures. Corrections have been applied to Eq. (133) and to the Table in Section 4.1
Interfacial exchange interactions and magnetism of Ni2MnAl/Fe bilayers
Creators: name: Yanes, Rocio
name: Simon, Eszter
name: Keller, Sebastian
name: Nagyfalusi, Balazs
name: Khmelevsky, Sergii
name: Szunyogh, Laszlo
name: Nowak, Ulrich
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Based on a multi-scale calculations, combining ab-initio methods with spin dynamics simulations, we perform a detailed study of the magnetic behavior of Ni2MnAl/Fe bilayers. Our simulations show that such a bilayer exhibits a small exchange bias effect when the Ni2MnAl Heusler alloy is in a disordered B2 phase. Additionally, we present an effective way to control the magnetic structure of the Ni2MnAl antiferromagnet, in the pseudo-ordered B2-I as well as the disordered B2 phases, via a spin-flop coupling to the Fe layer.
description: 7 pages, 6 figures
On Secure mmWave RSMA Systems
Creators: name: Lei, Hongjiang
name: Zhou, Sha
name: Chen, Xinhu
name: Ansari, Imran Shafique
name: Li, Yun
name: Pan, Gaofeng
name: Alouini, Mohamed-Slim
Publisher: name: arXiv
Year: 2024
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: This work considers a multiple-input-single-output mmWave RSMA system wherein a base station serves two users in the presence of a passive eavesdropper. Different eavesdropping scenarios are considered corresponding to the overlapped resolvable paths between the main and the wiretap channels under the considered transmission schemes. The analytical expressions for the secrecy outage probability are derived respectively through the Gaussian Chebyshev quadrature method. Monte Carlo simulation results are presented to validate the correctness of the derived analytical expressions and demonstrate the effects of system parameters on the SOP of the considered mmWave RSMA systems.
description: 12 pages,8 figures, accepted by IEEE Internet of Things Journal
Finite temperature Green's function approach for excited state and thermodynamic properties of cool to warm dense matter
Creators: name: Kas, J. J.
name: Rehr, J. J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We present a finite-temperature extension of the retarded cumulant Green's function for calculations of exited-state and thermodynamic properties of electronic systems. The method incorporates a cumulant to leading order in the screened Coulomb interaction $W$ and improves excited state properties compared to the $GW$ approximation of many-body perturbation theory. Results for the homogeneous electron gas are presented for a wide range of densities and temperatures, from cool to warm dense matter regime, which reveal several hitherto unexpected properties. For example, correlation effects remain strong at high $T$ while the exchange-correlation energy becomes small. In addition, the spectral function broadens and damping increases with temperature, blurring the usual quasi-particle picture. Similarly Compton scattering exhibits substantial many-body corrections that persist at normal densities and intermediate $T$. Results for exchange-correlation energies and potentials are in good agreement with existing theories and finite-temperature DFT functionals.
Permutational symmetries for coincidence rates in multi-mode multi-photonic interferometry
Creators: name: Khalid, Abdullah
name: Spivak, Dylan
name: Sanders, Barry C.
name: de Guise, Hubert
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We obtain coincidence rates for passive optical interferometry by exploiting the permutational symmetries of partially distinguishable input photons, and our approach elucidates qualitative features of multi-photon coincidence landscapes. We treat the interferometer input as a product state of any number of photons in each input mode with photons distinguished by their arrival time. Detectors at the output of the interferometer count photons from each output mode over a long integration time. We generalize and prove the claim of Tillmann et al. [Phys. Rev. X 5 041015 (2015)] that coincidence rates can be elegantly expressed in terms of immanants. Immanants are functions of matrices that exhibit permutational symmetries and the immanants appearing in our coincidence-rate expressions share permutational symmetries with the input state. Our results are obtained by employing representation theory of the symmetric group to analyze systems of arbitrary number of photons in arbitrarily sized interferometers.
Bulbostylis capillaris C. B. Clarke
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Cyperaceae
Bulbostylis
Bulbostylis capillaris

description: Scirpus capillaris Linnaeus, Species Plantarum 1: 49. 1753.
"Habitat in Virginia, Aethiopia, Zeylona." RCN: 418.
 Lectotype (Fernald in Rhodora 40: 395, pl. 510. 1938): Herb. Linn. No. 71.25 (LINN).
 Current name:  Bulbostylis capillaris  (L.) C.B. Clarke (Cyperaceae).
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 pages 828-829, DOI: 10.5281/zenodo.291971
Nucleosynthesis in neutrino heated matter: The vp-process and the r-process
Creators: name: Martínez-Pinedo, G.
name: Kelic, A.
name: Langanke, K.
name: Schmidt, K. -H.
name: Mocelj, D.
name: Fröhlich, C.
name: Thielemann, F. -K.
name: Panov, I.
name: Rauscher, T.
name: Liebendörfer, M.
name: Zinner, N. T.
name: Pfeiffer, B.
name: Buras, R.
name: Janka, H. -Th.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This manuscript reviews recent progress in our understanding of the nucleosynthesis of medium and heavy elements in supernovae. Recent hydrodynamical models of core-collapse supernovae show that a large amount of proton rich matter is ejected under strong neutrino fluxes. This matter constitutes the site of the vp-process where antineutrino absorption reactions catalyze the nucleosynthesis of nuclei with A > 64. Supernovae are also associated with the r-process responsible for the synthesis of the heaviest elements in nature. Fission during the r-process can play a major role in determining the final abundance patter and in explaining the almost universal features seen in metal-poor r-process-rich stars.
description: 10 pages, 3 figures, invited talk at NIC-IX, International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, CERN, Geneva, Switzerland, 25-30 June, 2006
Spheres, Charges, Instantons, and Bootstrap: A Five-Dimensional Odyssey
Creators: name: Chang, Chi-Ming
name: Fluder, Martin
name: Lin, Ying-Hsuan
name: Wang, Yifan
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We combine supersymmetric localization and the conformal bootstrap to study five-dimensional superconformal field theories. To begin, we classify the admissible counter-terms and derive a general relation between the five-sphere partition function and the conformal and flavor central charges. Along the way, we discover a new superconformal anomaly in five dimensions. We then propose a precise triple factorization formula for the five-sphere partition function, that incorporates instantons and is consistent with flavor symmetry enhancement. We numerically evaluate the central charges for the rank-one Seiberg and Morrison-Seiberg theories, and find strong evidence for their saturation of bootstrap bounds, thereby determining the spectra of long multiplets in these theories. Lastly, our results provide new evidence for the $F$-theorem and possibly a $C$-theorem in five-dimensional superconformal theories.
description: 90 pages, 12 figures, 11 tables; v2: references added; v3: minor corrections
Axion Electrodynamics from Infeld-van der Waerden formalisms
Creators: name: Kuerten, André Martorano
name: Fernandes-Silva, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this article we will explore the spacetime phase structure inside the Infeld-van der Waerden formalisms, showing that Maxwell's theory in this scenario leads to an axion-like phase electrodynamics, which suggests that this phase may originate the axion field.
description: 15 pages
Is the fossil rat-kangaroo Palaeopotorous priscus the most basally branching stem macropodiform?
Creators: name: Boer, Wendy Den
name: Kear, Benjamin P.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy

description: Citation for this article: den Boer, W., and B. P. Kear. 2018. Is the fossil rat-kangaroo Palaeopotorous priscus the most basally branching stem macropodiform? Journal of Vertebrate Paleontology. DOI: 10.1080/02724634.2017.1428196.
Testing the Ginzburg-Landau approximation for three-flavor crystalline color superconductivity
Creators: name: Mannarelli, Massimo
name: Rajagopal, Krishna
name: Sharma, Rishi
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is an open challenge to analyze the crystalline color superconducting phases that may arise in cold dense, but not asymptotically dense, three-flavor quark matter. At present the only approximation within which it seems possible to compare the free energies of the myriad possible crystal structures is the Ginzburg-Landau approximation. Here, we test this approximation on a particularly simple "crystal" structure in which there are only two condensates $ \sim Δ\exp(i {\bf q_2}\cdot {\bf r})$ and $ \sim Δ\exp(i {\bf q_3}\cdot {\bf r})$ whose position-space dependence is that of two plane waves with wave vectors ${\bf q_2}$ and ${\bf q_3}$ at arbitrary angles. For this case, we are able to solve the mean-field gap equation without making a Ginzburg-Landau approximation. We find that the Ginzburg-Landau approximation works in the $Δ\to 0$ limit as expected, find that it correctly predicts that $Δ$ decreases with increasing angle between ${\bf q_2}$ and ${\bf q_3}$ meaning that the phase with ${\bf q_2}\parallel {\bf q_3}$ has the lowest free energy, and find that the Ginzburg-Landau approximation is conservative in the sense that it underestimates $Δ$ at all values of the angle between ${\bf q_2}$ and ${\bf q_3}$.
description: 16 pages, 6 figures. Small changes only. Version to appear in Phys. Rev. D
Effect of turbulent diffusion on iron abundance profiles
Creators: name: Rebusco, P.
name: Churazov, E.
name: Boehringer, H.
name: Forman, W.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compare the observed peaked iron abundance profiles for a small sample of groups and clusters with the predictions of a simple model involving the metal ejection from the brightest galaxy and the subsequent diffusion of metals by stochastic gas motions. Extending the analysis of Rebusco et al. (2005) we found that for 5 out of 8 objects in the sample an effective diffusion coefficient of the order of $10^{29}$ cm$^{2}$ s$^{-1}$ is needed. For AWM4, Centaurus and AWM7 the results are different suggesting substantial intermittence in the process of metal spreading across the cluster. There is no obvious dependence of the diffusion coefficient on the mass of the system. We also estimated the characteristic velocities and the spatial scales of the gas motions needed to balance the cooling losses by the dissipation of the same gas motions. A comparison of the derived spatial scales and the sizes of observed radio bubbles inflated in the ICM by a central active galactic nucleus (AGN) suggests that the AGN/ICM interaction makes an important (if not a dominant) contribution to the gas motions in the cluster cores.
description: 12 pages, 4 figures, accepted for publication on MNRAS
Classical limit theorems and high entropy MIXMAX random number generator
Creators: name: Poghosyan, Hayk
name: Savvidy, Konstantin
name: Savvidy, George
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mathematical Physics (math-ph)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We investigate the interrelation between the distribution of stochastic fluctuations of independent random variables in probability theory and the distribution of time averages in deterministic Anosov C-systems. On the one hand, in probability theory, our interest dwells on three basic topics: the laws of large numbers, the central limit theorem and the law of the iterated logarithm for sequences of real-valued random variables. On the other hand we have chaotic, uniformly hyperbolic Anosov C-systems defined on tori which have mixing of all orders and nonzero Kolmogorov entropy. These extraordinary ergodic properties of deterministic Anosov C-systems ensure that the above classical limit theorems for sums of independent random variables in probability theory are fulfilled by the time averages for the sequences generated by the C-systems. The MIXMAX generator of pseudorandom numbers represents the C-system for which the classical limit theorems are fulfilled.
description: 15 pages, 4 figures
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1153
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
name: Petot, Frédéric
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: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1153, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1153, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Eleocharis capitatus R. Br.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Cyperaceae
Eleocharis
Eleocharis capitatus

description: Scirpus capitatus Linnaeus, Species Plantarum 1: 48. 1753.
"Habitat in Virginia." RCN: 408.
 Lectotype (Blake in Rhodora 20: 23. 1918): Clayton 380 (BM-000051193).
 Current name:  Eleocharis capitatus  (L.) R. Br. (Cyperaceae).
 Note: Blake (1918) treated the Clayton material as the type but this choice provoked extensive discussion by Fernald (in Rhodora 23: 106. 1921), Mackenzie (l.c. 30: 237. 1928), Farwell (l.c. 32: 181. 1930), Blake (l.c. 32: 182. 1930) again, Svenson (l.c. 34: 195. 1932; 41: 50. 1939) and Furtado (in Gard. Bull. Straits Settlem. 9: 243. 1937). However, Blake’s original choice has priority.
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 829, DOI: 10.5281/zenodo.291971