cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The relative impact of photoionizing radiation and stellar winds on different environments
Creators: name: Haid, Sebastian
name: Walch, Stefanie
name: Seifried, Daniel
name: Wünsch, Richard
name: Dinnbier, František
name: Naab, Thorsten
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Photoionizing radiation and stellar winds from massive stars deposit energy and momentum into the interstellar medium (ISM). They might disperse the local ISM, change its turbulent multi-phase structure, and even regulate star formation. Ionizing radiation dominates the massive stars' energy output, but the relative effect of winds might change with stellar mass and the properties of the ambient ISM. We present simulations of the interaction of stellar winds and ionizing radiation of 12, 23, and 60 M$_{\odot}$ stars within a cold neutral (CNM, $n_{0}$ = 100 cm$^{-3}$), warm neutral (WNM, $n_{0}$ = 1, 10 cm$^{-3}$) or warm ionized (WIM, $n_{0}$ = 0.1 cm$^{-3}$) medium. The FLASH simulations adopt the novel tree-based radiation transfer algorithm TreeRay. With the On-the-Spot approximation and a temperature-dependent recombination coefficient, it is coupled to a chemical network with radiative heating and cooling. In the homogeneous CNM, the total momentum injection ranges from 1.6$\times$10$^{4}$ to 4$\times$10$^{5}$ M$_{\odot}$ km s$^{-1}$ and is always dominated by the expansion of the ionized H$_{\text{II}}$ region. In the WIM, stellar winds dominate (2$\times$10$^{2}$ to 5$\times$10$^{3}$ M$_{\odot}$ km s$^{-1}$), while the input from radiation is small ($\sim$ 10$^{2}$ M$_{\odot}$ km s$^{-1}$). The WNM ($n_{0}$ = 1 cm$^{-3}$) is a transition regime. Energetically, stellar winds couple more efficiently to the ISM ($\sim$ 0.1 percent of wind luminosity) than radiation ($
Understanding the Galaxy
Creators: name: Eyer, Laurent
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A general overview of the understanding of our Galaxy is presented following the lines of its main structures: halo, disc, bulge/bar. This review is emphasising some "Time Domain Astronomy" contributions. On the one hand the distance and tangential motion of the stars are essential to this understanding and are obtained through multi-epoch surveys, on the other hand the chemistry of the stars, and their radial velocity are also key elements to map Galactic (sub-)structures and unravel their history and evolution. Contemporary surveys are revolutionising our view of the Milky Way and galaxies in general. Among these, the Gaia mission excels by its precision astrometry of 1.3 billion stars stretching through the Milky Way and beyond, providing the first 3D view of a major part of the Milky Way.
description: 6 pages, 1 figure, proceedings of the IAU Symposium 339 Southern Horizons in Time-Domain Astronomy, 13-17 November 2017, Stellenbosch, South Africa
Physics from Vacuum Alignment in A Technicolor Model
Creators: name: Georgi, Howard
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I describe a technicolor model (without walking) of all interactions up to energies of the order of 1000~TeV. The low energy extended technicolor model has the CTSM form. But at intermediate energy scales, additional interactions are required to give the KM mixing. I discuss the characteristic flavor changing neutral current interactions arising from this flavor physics below 1000~TeV.
description: 13pages (landscape mode) LATEX + PICTEX
Additional file 1: of Participation of father in perinatal care: a qualitative study from the perspective of mothers, fathers, caregivers, managers and policymakers in Iran
Creators: name: Vahideh Firouzan
name: Noroozi, Mahnaz
name: Mirghafourvand, Mojgan
name: Farajzadegan, Ziba
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Interview guide during the face-to-face interviews with women who were pregnant or had just delivered for the study conducted on participation of fathers in perinatal care from the perspective of mothers, fathers, caregivers, managers and policymakers in Tabriz Town, Iran, 2017 (See methods section for further description). (DOCX 16 kb)
The effect of mean pore size in collagen-glycosaminoglycan scaffolds on cell migration and differentiation for bone tissue engineering applications
Creators: name: Murphy, Ciara M.
Publisher: name: Royal College of Surgeons in Ireland
Year: 2019
Subjects: Uncategorized

description: Tissue engineering was born from the belief that primary cells could be isolated from a patient, expanded in vitro and seeded onto a substrate that could be grafted back into the patient (Yang et a/, 2001) providing a biological alternative to transplantations and prosthesis. There are three main components in tissue engineering, scaffolds, cells and signalling mechanisms that make up the tissue engineering triad. This thesis focuses on the interplay between cell behaviour and scaffold structural properties. Recent studies from our laboratory have developed novel freeze-drying techniques to vary the structure of collagen-glycosaminoglycan (GAG) scaffolds producing scaffolds with mean pores ranging from 85 pm - 325 pm (Haugh et a/, 2010). The general aim of this thesis was to investigate, using this range of scaffolds, the effect of mean pore size on cell behaviour in the scaffolds and see how this behaviour varies with different cell types. A non-linear effect was seen on initial cell attachment but ultimately scaffolds with the largest pores size of 325 pm facilitated optimal osteoblast attachment, proliferation and migration. A comparison of stem cell (MSC) behaviour to semi-differentiated osteoblasts in the scaffolds demonstrated a similar non-linear effect on cell attachment but poorer MSC migration was observed highlighting the difference in cell type behaviour. Further analysis shed some light on this effect whereby MSCs were physically bigger cells and less motile. Longer term studies were carried out to determine the effect of mean pore size on osteoblast differentiation, matrix mineralisation and cell-mediated contraction. The largest scaffold mean pore size of 325 pm facilitated improved cell distribution, an earlier onset of osteogenic differentiation and a higher level of mineralisation. The final study of this thesis investigated the potential of human amniotic fluid derived stem cells as a readily accessible source of pluripotent stem cells (AFSCs). These cells demonstrated osteogenic differentiation and an ability to attach to the collagen-GAG scaffold. In conclusion, mean pore size was shown to have an effect on cell behaviour in collagen-GAG scaffolds. Ultimately the larger pores of 325 pm facilitate optimal cell attachment, migration, osteogenic differentiation, matrix mineralisation and cellmediated contraction. In addition, the osteogenic potential of a readily accessible source of pluripotent stem cells has demonstrated their future potential in bone tissue engineering.
Analysis of interacting and isolated quasars
Creators: name: Donoso, L.
name: Alonso, M. V.
name: Lambas, D. Garcia
name: Coldwell, G.
name: Schmidt, E. O.
name: Oio, G. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The main goal of this study was to determine the effects on equivalent widths (EWs) of some spectral lines produced in the quasars by the presence of surrounding galaxies. To carry this out, a sample of 4663 quasars (QSOs) in the redshift range of 0.20 to 0.40 from the Sloan Digital Sky Survey--Data Release 7 was analyzed. Three QSO sub-samples were defined, taking into account the projected separations and radial velocity differences with neighboring galaxies. In this way, we utilized two sub-samples of QSOs with strong and weak galaxy interactions, with projected separations smaller than 70 kpc, and between 70 and 140 kpc, respectively, and with radial velocity differences less than $5000~$\kms. These sub-samples were compared with isolated QSOs defined as having greater projected separations and radial velocity differences to the galaxies. From a statistical study of the EWs of relevant spectral lines in the QSOs, we show an increment of the EWs of about 20\% in the [OIII]4959,5007 lines and 7\% in H$_α$ for QSOs with stronger galaxy interactions relative to the isolated QSOs. These results indicate that some line EWs of QSOs could be marginally influenced by the environment and that they are not affected by the emission of the host galaxy, which was estimated to be around 10\% of the total emission. Furthermore, in order to gain a better understanding of the origin of the H$_α$ emission line, we performed broad and narrow line decomposition in 100 QSOs in the restricted Sint sub-sample and also 100 randomly selected QSOs in the Iso sub-sample. When these QSOs were compared, the narrow component remained constant whereas the broad component was incremented. Our results, which reveal slight differences in EWs of some emission lines, suggest that galaxy interactions with QSOs may affect the QSO activity.
description: Accepted for publication in the Astronomy & Astrophysics. 9 pages, 9 figures
X-Ray and Optical Properties of Groups of Galaxies
Creators: name: Dell'Antonio, I. P.
name: Geller, M. J.
name: Fabricant, D. G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the relationship between the group x-ray luminosity in the 0.3-3.5 keV band and the measured velocity dispersion, and galaxy surface number density. We find definite correlations. Richer groups follow the same relation as rich clusters (cf. Quintana & Melnick 1982) with $L_x \propto σ^{4.0\pm 0.6}$, but the relation flattens for lower luminosity systems which have velocity dispersions below 300 km/s). We suggest that the $L_x-σ$ relation arises from a combination of extended cluster emission and emission associated with individual galaxies. The x-ray emission for the richer groups is dominated by emission from the intra-group medium, as for the richer clusters; emission from the poorer clusters is dominated by less extended emission associated with the individual group galaxies. This is a corrected version of the paper which appeared in the Astronomical Journal (February 1994). We include a new version of the affected figure.
description: 17 pages +1 postscript figure, plain tex w/included macros
$D^6R^4$ curvature corrections, modular graph functions and Poincaré series
Creators: name: Ahlén, Olof
name: Kleinschmidt, Axel
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Number Theory (math.NT)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: In this note we study the U-duality invariant coefficient functions of higher curvature corrections to the four-graviton scattering amplitude in type IIB string theory compactified on a torus. The main focus is on the $D^6R^4$ term that is known to satisfy an inhomogeneous Laplace equation. We exhibit a novel method for solving this equation in terms of a Poincaré series ansatz and recover known results in $D=10$ dimensions and find new results in $D<10$ dimensions. We also apply the method to modular graph functions as they arise from closed superstring one-loop amplitudes.
description: 27 pages
Integrals of Motion in the Two Killing Vector Reduction of General Relativity
Creators: name: Manojlović, Nenad
name: Spence, Bill
Publisher: name: arXiv
Year: 1993
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We apply the inverse scattering method to the midi-superspace models that are characterized by a two-parameter Abelian group of motions with two spacelike Killing vectors. We present a formulation that simplifies the construction of the soliton solutions of Belinski\v i and Zakharov. Furthermore, it enables us to obtain the zero curvature formulation for these models. Using this, and imposing periodic boundary conditions corresponding to the Gowdy models when the spatial topology is a three torus $T ^3$, we show that the equation of motion for the monodromy matrix is an evolution equation of the Heisenberg type. Consequently, the eigenvalues of the monodromy matrix are the generating functionals for the integrals of motion. Furthermore, we utilise a suitable formulation of the transition matrix to obtain explicit expressions for the integrals of motion. This involves recursion relations which arise in solving an equation of Riccati type. In the case when the two Killing vectors are hypersurface orthogonal the integrals of motion have a particularly simple form.
description: 20 pages, plain TeX, SU-GP-93/7-8, UM-P-93/77
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1202
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: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1202, 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. 1202, 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
A large sample of shear selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A wide field mass maps
Creators: name: Miyazaki, Satoshi
name: Oguri, Masamune
name: Hamana, Takashi
name: Shirasaki, Masato
name: Koike, Michitaro
name: Komiyama, Yutaka
name: Umetsu, Keiichi
name: Utsumi, Yousuke
name: Okabe, Nobuhiro
name: More, Surhud
name: Medezinski, Elinor
name: Lin, Yen-Ting
name: Miyatake, Hironao
name: Murayama, Hitoshi
name: Ota, Naomi
name: Mitsuishi, Ikuyuki
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the result of searching for clusters of galaxies based on weak gravitational lensing analysis of the $\sim 160$~deg$^2$ area surveyed by Hyper Suprime-Cam (HSC) as a Subaru Strategic Program. HSC is a new prime focus optical imager with a 1.5 diameter field of view on the 8.2-meter Subaru telescope. The superb median seeing on the HSC $i$-band images of $0.56$ arcsec allows the reconstruction of high angular resolution mass maps via weak lensing, which is crucial for the weak lensing cluster search. We identify 65 mass map peaks with signal-to-noise (SN) ratio larger than 4.7, and carefully examine their properties by cross-matching the clusters with optical and X-ray cluster catalogs. We find that all the 39 peaks with SN$>5.1$ have counterparts in the optical cluster catalogs, and only 2 out of the 65 peaks are probably false positives. The upper limits of X-ray luminosities from ROSAT All Sky Survey (RASS) imply the existence of an X-ray under-luminous cluster population. We show that the X-rays from the shear selected clusters can be statistically detected by stacking the RASS images. The inferred average X-ray luminosity is about half that of the X-ray selected clusters of the same mass. The radial profile of the dark matter distribution derived from the stacking analysis is well modeled by the Navarro-Frenk-White profile with a small concentration parameter value of $c_{500}\sim 2.5$, which suggests that the selection bias on the orientation or the internal structure for our shear selected cluster sample is not strong.
description: 25 pages, 17 figures Appeared in Publication of Astronomical Society of Japan, Hyper Suprime-Cam Special Issue
Sémélé
Creators: name: de La Motte, Antoine
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: Académie royale de musique
Première génération d'opéras français
Paris
Livret d'Opéra
Tragédie en musique

description: Tragédie représentée par l'Académie royale de musique en 1709. Les paroles sont d'Antoine de La Motte et la musique de Marin Marais. Le livret est consultable de manière publique par un portail qui donne accès simultanément au fac-similé, à une version du corpus qui respecte la graphie d’origine et une version du corpus normalisé exploitable à travers toutes les fonctionnalités de la plateforme TXM : http://fanum-txm.univ-fcomte.fr/txm/?command=edition&path=/LIVRETSOPERA&editions=facs,originale,normalis%C3%A9e&textid=49_SEMELE
description: Bibliographic citation: Cote (ELLIADD) : 49_SEMELE
description: URL TXM : http://fanum-txm.univ-fcomte.fr/txm/?command=edition&path=/LIVRETSOPERA&editions=facs,originale,normalis%C3%A9e&textid=49_SEMELE
Supersymmtric Baryogenesis
Creators: name: Cohen, A.
name: Nelson, A.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Requiring that the baryon number of the universe be generated by anomalous electroweak interactions places strong constraints on the minimal supersymmetric standard model. In particular, the electric dipole moment of the neutron must be greater than $10^{-27}$e-cm. Improvement of the current experimental bound on the neutron's electric dipole moment by one order of magnitude would constrain the lightest chargino to be lighter than 88 GeV, and the the lightest neutralino to be lighter than 44 GeV. In extensions of this model with gauge singlet superfields all of these bounds are eliminated.
description: 14 pages 3 fig.,BUHEP-92-20
A System for Estimating Drug Delivery from a Dry Powder Inhaler by Analysis of Acoustic Recordings of Time-Stamped Inhaler Events
Creators: name: Jansen N. Seheult
Publisher: name: Royal College of Surgeons in Ireland
Year: 2019
Subjects: Uncategorized

description: Inhaled medications are the mainstay of therapy in the treatment of chronic respiratory diseases like asthma and COPD because they allow delivery of the active ingredient directly to the site of action. Poor adherence to inhaled controller medications has been estimated to account for up to 60% of asthma-related hospitalizations and increased rates of 30- and 60- day hospital readmissions in patients with COPD. Numerous electronic monitoring devices have been developed over the last four decades to monitor temporal non-adherence; however, many of these devices do not monitor all or most aspects of inhaler technique. Currently used methods for monitoring inhaler technique, including subjective checklists, are suboptimal. There is a need to study the frequency of temporal and technique non-adherence in the Irish population and to investigate the impact of dosing and technique errors on drug delivery. Moreover, a comprehensive system of tracking the date and time of inhaler use, as well as the presence or absence of technique errors, on a daily basis is essential to not only an epidemiological understanding of inhaler use but to tailoring of inhaler training and clinical care plans to individual patients. This thesis describes the use of the INCATM device, a novel acoustic monitor, which provides longitudinal data on the date and time of inhaler use, as well as data on inhaler technique. Studies showed that inhalation flow rate, exhalation into the inhaler mouthpiece prior to inhalation, breath-hold duration and missed doses had a significant effect on delivered dose. Data on both temporal and technique adherence were combined in an algorithm, which provided a single measure of overall adherence, called “actual adherence”. The dose counter rate correlated poorly with INCATM derived adherence rates, highlighting the need to incorporate technologies, like the INCATM device, into clinical trials and patient care.
Multiplicative Noise: Applications in Cosmology and Field Theory
Creators: name: Habib, Salman
Publisher: name: arXiv
Year: 1993
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Physical situations involving multiplicative noise arise generically in cosmology and field theory. In this paper, the focus is first on exact nonlinear Langevin equations, appropriate in a cosmologica setting, for a system with one degree of freedom. The Langevin equations are derived using an appropriate time-dependent generalization of a model due to Zwanzig. These models are then extended to field theories and the generation of multiplicative noise in such a context is discussed. Important issues in both the cosmological and field theoretic cases are the fluctuation-dissipation relations and the relaxation time scale. Of some importance in cosmology is the fact that multiplicative noise can substantially reduce the relaxation time. In the field theoretic context such a noise can lead to a significant enhancement in the nucleation rate of topological defects.
description: 21 pages, LaTex, LA-UR-93-2105
On the importance of the nonequilibrium ionization of Si IV and O IV and the line-of-sight in solar surges
Creators: name: Nóbrega-Siverio, D.
name: Moreno-Insertis, F.
name: Martínez-Sykora, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Surges are ubiquitous cool ejections in the solar atmosphere that often appear associated with transient phenomena like UV bursts or coronal jets. Recent observations from the Interface Region Imaging Spectrograph (IRIS) show that surges, although traditionally related to chromospheric lines, can exhibit enhanced emission in Si IV with brighter spectral profiles than for the average transition region (TR). In this paper, we explain why surges are natural sites to show enhanced emissivity in TR lines. We performed 2.5D radiative-MHD numerical experiments using the Bifrost code including the nonequilibrium ionization of silicon and oxygen. A surge is obtained as a by-product of magnetic flux emergence; the TR enveloping the emerged domain is strongly affected by nonequilibrium effects: assuming statistical equilibrium would produce an absence of Si IV and O IV ions in most of the region. Studying the properties of the surge plasma emitting in the Si IV 1402.77 Å and O IV 1401.16 Å lines, we find that a) the timescales for the optically-thin losses and heat conduction are very short, leading to departures from statistical equilibrium, and b) the surge emits in Si IV more and has an emissivity ratio of Si IV to O IV larger than a standard TR. Using synthetic spectra, we conclude the importance of line-of-sight effects: given the involved geometry of the surge, the line-of-sight can cut the emitting layer at small angles and/or cross it multiple times, causing prominent, spatially intermittent brightenings both in Si IV and O IV.
description: 18 pages, 11 figures (accepted in the Astrophysical Journal, ApJ)
Nuclear dynamics and particle production near threshold energies in heavy-ion collisions
Creators: name: Feng, Zhao-Qing
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Recent progress of the quantum molecular dynamics model for describing the dynamics of heavy-ion collisions is viewed, in particular the nuclear fragmentation, isospin physics, particle production and in-medium effect, hadron-induced nuclear reactions, hypernucleus etc. The neck fragmentation in Fermi-energy heavy-ion collisions is investigated for extracting the symmetry energy at subsaturation densities. The isospin effects, in-medium properties and the behavior of high-density symmetry energy in medium and high energy heavy-ion collisions are thoroughly discussed. The hypernuclide dynamics formed in heavy-ion collisions and in hadron induced reactions is analyzed and addressed in the future experiments at the High-Intensity heavy-ion Accelerator Facility (HIAF).
description: 31 pages, 27 figures (review article)
Testing Inflation with the Cosmic Microwave Background
Creators: name: Dodelson, Scott
name: Knox, Lloyd
name: Kolb, Edward W.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Cosmic microwave background (CMB) anisotropy may result from both scalar and tensor perturbations. For a sufficiently narrow range of angular scales, CMB perturbations can be characterized by four parameters. Results from the Cosmic Background Explorer fix one combination of the parameters, reducing the parameters to three. If CMB perturbations are from inflation, there is an additional relation, reducing the parameters to two. An appropriate combination of a medium-angle and a small-angle CMB observation can test the inflation hypothesis because inflation cannot explain a high signal in one experiment and a low signal in the other.
description: (differs from original inclusion of color version of figure 3 and corrected version of figure 2), 11 pages plus 4 figures (attached as a uuencoded postscript file), LaTeX, FNAL--PUB--94/053--A
Using late-time optical and near-infrared spectra to constrain Type Ia supernova explosion properties
Creators: name: Maguire, K.
name: Sim, S. A.
name: Shingles, L.
name: Spyromilio, J.
name: Jerkstrand, A.
name: Sullivan, M.
name: Chen, T. -W.
name: Cartier, R.
name: Dimitriadis, G.
name: Frohmaier, C.
name: Galbany, L.
name: Gutiérrez, C. P.
name: Hosseinzadeh, G.
name: Howell, D. A.
name: Inserra, C.
name: Rudy, R.
name: Sollerman, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The late-time spectra of Type Ia supernovae (SNe Ia) are powerful probes of the underlying physics of their explosions. We investigate the late-time optical and near-infrared spectra of seven SNe Ia obtained at the VLT with XShooter at $>$200 d after explosion. At these epochs, the inner Fe-rich ejecta can be studied. We use a line-fitting analysis to determine the relative line fluxes, velocity shifts, and line widths of prominent features contributing to the spectra ([Fe II], [Ni II], and [Co III]). By focussing on [Fe II] and [Ni II] emission lines in the ~7000-7500 Å region of the spectrum, we find that the ratio of stable [Ni II] to mainly radioactively-produced [Fe II] for most SNe Ia in the sample is consistent with Chandrasekhar-mass delayed-detonation explosion models, as well as sub-Chandrasekhar mass explosions that have metallicity values above solar. The mean measured Ni/Fe abundance of our sample is consistent with the solar value. The more highly ionised [Co III] emission lines are found to be more centrally located in the ejecta and have broader lines than the [Fe II] and [Ni II] features. Our analysis also strengthens previous results that SNe Ia with higher Si II velocities at maximum light preferentially display blueshifted [Fe II] 7155 Å lines at late times. Our combined results lead us to speculate that the majority of normal SN Ia explosions produce ejecta distributions that deviate significantly from spherical symmetry.
description: 17 pages, 12 figure, accepted for publication in MNRAS
Additional file 2: of Pilot testing of the Becoming Breastfeeding Friendly toolbox in Ghana
Creators: name: Richmond Aryeetey
name: Hromi-Fiedler, Amber
name: Adu-Afarwuah, Seth
name: Esi Amoaful
name: Gifty Ampah
name: Gatiba, Marian
name: Akosua Kwakye
name: Otoo, Gloria
name: Gyikua Plange-Rhule
name: Sagoe-Moses, Isabella
name: Selenje, Lilian
name: PĂŠrez-Escamilla, Rafael
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Appendix S2. Infographic. This document is an infographic which was developed and shared with key stakeholders in breastfeeding in Ghana who were invited to participate in the fifth committee meeting of the Becoming Breastfeeding Friendly Committee. (PDF 860 kb)
Additional file 2: of Personalised relaxation practice to improve sleep and functioning in patients with chronic fatigue syndrome and depression: study protocol for a randomised controlled trial
Creators: name: Macnamara, Claire
name: Cvejic, Erin
name: Parker, Gordon
name: Lloyd, Andrew
name: Lee, Gina
name: Beilharz, Jessica
name: Vollmer-Conna, Ute
Publisher: name: figshare
Year: 2018
Subjects: subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Participant informed consent form. (DOCX 1310 kb)
Additional file 3 of Identification of the miRNA signature and key genes in colorectal cancer lymph node metastasis
Creators: name: Wang, Xi
name: Gao, Guangyu
name: Chen, Zhengrong
name: Chen, Zhihao
name: Han, Mingxiao
name: Xie, Xiaolu
name: Jin, Qiyuan
name: Du, Hong
name: Cao, Zhifei
name: Zhang, Haifang
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Table S2. Identification of DEGs associated with lymph node metastasis of CRC
Time-Loop Formalism for Irreversible Quantum Problems: Steady State Transport in Junctions with Asymmetric Dynamics
Creators: name: Kakashvili, Paata
name: Bolech, C. J.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: High Energy Physics - Theory (hep-th)
subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Non-unitary quantum mechanics has been used in the past to study irreversibility, dissipation and decay in a variety of physical systems. In this letter, we propose a general scheme to deal with systems governed by non-Hermitian Hamiltonians. We argue that the Schwinger-Keldysh formalism gives a natural description for those problems. To elucidate the method, we study a simple model inspired by mesoscopic physics --an asymmetric junction. The system is governed by a non-Hermitian Hamiltonian which captures essential aspects of irreversibility.
description: 4 pages, 4 figures
Beliaev Damping in Spin-$\frac{1}{2}$ Interacting Bosons with Spin-Orbit Coupling
Creators: name: Wu, Rukuan
name: Liang, Zhaoxin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: Beliaev damping provides one of the most important mechanisms for dissipation of quasiparticles through beyond-mean-field effects at zero temperature. Here we present the first analytical result of Beliaev damping in low-energy excitations of spin-$\frac{1}{2}$ interacting bosons with equal Rashba and Dresslhaus spin-orbit couplings. We identify novel features of Beliaev decay rate due to spin-orbit coupling, in particular, it shows explicit dependence on the spin-density interaction and diverges at the interaction-modified phase boundary between the zero-momentum and plane-wave phases. This represents a manifestation of the effect of spin-orbit coupling in the beyond-mean-field regime, which by breaking Galilean invariance couples excitations in the density- and spin-channels. By describing the Beliaev damping in terms of the observable dynamic structure factors, our results allow direct experimental access within current facilities.
description: 6 pages, 2 figures
Estimates with an Effective Chiral Lagrangian for Heavy Mesons
Creators: name: Casalbuoni, R.
name: Deandrea, A.
name: Di Bartolomeo, N.
name: Gatto, R.
name: Feruglio, F.
name: Nardulli, G.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: On the basis of an effective lagrangian incorporating approximate chiral symmetry and heavy-quark spin and flavor symmetries, and by use of information on leptonic decays, we estimate the effective $D^\star Dπ$ coupling.
description: UGVA-DPT 1992/07-779, BARI-TH/92-117 Revised version, September 1992, LaTeX (style article), 7 pages
Cation Discrimination in Organic Electrochemical Transistors by Dual Frequency Sensing
Creators: name: Pecqueur, Sebastien
name: Guerin, David
name: Vuillaume, Dominique
name: Alibart, Fabien
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: In this work, we propose a strategy to sense quantitatively and specifically cations, out of a single organic electrochemical transistor (OECT) device exposed to an electrolyte. From the systematic study of six different chloride salts over 12 different concentrations, we demonstrate that the impedance of the OECT device is governed by either the channel dedoping at low frequency and the electrolyte gate capacitive coupling at high frequency. Specific cationic signatures, which originates from the different impact of the cations behavior on the poly(3,4-ethylenedioxythiophene):poly(styrenesulfonate) (PEDOT:PSS) polymer and their conductivity in water, allow their discrimination at the same molar concentrations. Dynamic analysis of the device impedance at different frequencies could allow the identification of specific ionic flows which could be of a great use in bioelectronics to further interpret complex mechanisms in biological media such as in the brain.
description: Full text and supporting information
A van der Waals DFT study of chain length dependence of alkanethiol adsorption on Au(111): Physisorption vs.chemisorption
Creators: name: Mete, Ersen
name: Yortanlı, Merve
name: Danışman, Mehmet Fatih
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The energetics and structures of physisorbed and chemisorbed alkanethiols on Au(111) have been systematically investigated up to 10 carbon atoms using van der Waals (vdW) corrected density functional theory (DFT) calculations. The role of chain length, tilting angle and coverage on the adsorption characteristics have been examined to elucidate the energetics and plausible transformation mechanisms between lying down and standing up phases. Coverage and size dependent chain-chain electronic interactions counteract with the alkyl chain-gold surface interactions and the surface relaxation of the metal in the formation of standing up monolayer structures. For the striped phases of long chain alkanethiols, however, our calculations on decanethiol indicates alkyl chain-gold surface interactions to be strong enough to force the molecule to be perfectly parallel to the surface by lifting a gold atom up, in agreement with the proposed models for this film in the literature.
description: 11 pages, 10 figures, 4 tables
Psychiatric and physical comorbidity in adults with autism spectrum disorder
Creators: name: O'Rourke, Linda
Publisher: name: Royal College of Surgeons in Ireland
Year: 2019
Subjects: Uncategorized

description: Autism spectrum disorder (ASD) is a highly impairing neurodevelopmental condition, manifesting in childhood and continuing into adult life. Comorbid psychiatric and physical illness lends considerable increased mortality to the condition. An increased awareness of comorbid conditions in adults with normal IQ ASD could improve diagnostic formulation, facilitate targeted treatments and improve psychosocial outcomes. This study examines the prevalence of comorbid psychiatric and physical illness in 413 adults with normal IQ ASD, attending a tertiary referral neurodevelopmental clinic in South London, to determine if rates of comorbid illness would be greater than rates reported in the general population. This study noted autism spectrum disorder in 70% of participants, with a male-to-female ratio of 2.8:1. Milder forms of ASD were recorded for 88%. Participants with autism spectrum disorder were more likely to be single, unemployed and living in the company of others. Seventy-six percent suffered from a comorbid Axis I illness and 2% suffered from a comorbid Axis II condition. Anxiety spectrum disorders were the most common comorbid psychiatric illness, followed by attention deficit hyperactivity disorder, mood disorders and deliberate self-harm. Psychosis, substance-use disorder, eating disorder and tic disorder were rarely diagnosed. Participants with Asperger’s syndrome were statistically more likely to be diagnosed with a comorbid psychiatric illness, most commonly obsessive compulsive disorder. Eighty-four percent of participants had a history of physical illness, most frequently asthma followed by head injury. Sleep difficulties and eating disturbance were notably high at 42% and 25% respectively. Adults with normal IQ autism spectrum disorder suffer higher rates of physical and psychiatric morbidity, display a poorer ability to engage with treatment and have a lower chance of recovery compared to the general population. Increased awareness and a high degree of diagnostic skill to identify those with the disorder should be promoted among physicians and psychiatrists.
title: UMass ADVANCE Faculty Survey: Comparing STEM and Non-STEM Faculty Experiences
Creators: name: Mickey, Ethel L.
Publisher: name: University of Massachusetts Amherst
Year: 2020

description: The UMass ADVANCE program is working to ensure greater equity among faculty through the power of collaboration. In this research brief, we describe some of the key findings from our initial survey, conducted in 2018-19. We will conduct the same survey in 2022-23 to measure the impact of our interventions. In this research brief, we focus on patterns between STEM faculty and non-STEM faculty by gender in the areas of inclusion, shared decision-making, and research collaboration.
Texture-Induced Microwave Background Anisotropies
Creators: name: Borrill, Julian
name: Copeland, Edmund J
name: Liddle, Andrew R
name: Stebbins, Albert
name: Veeraraghavan, Shoba
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use numerical simulations to calculate the cosmic microwave background anisotropy induced by the evolution of a global texture field, with special emphasis on individual textures. Both spherically symmetric and general configurations are analysed, and in the latter case we consider field configurations which exhibit unwinding events and also ones which do not. We compare the results given by evolving the field numerically under both the expanded core (XCORE) and non-linear sigma model (NLSM) approximations with the analytic predictions of the NLSM exact solution for a spherically symmetric self-similar (SSSS) unwinding. We find that the random unwinding configuration spots' typical peak height is 60--75\% and angular size typically only 10\% of those of the SSSS unwinding, and that random configurations without an unwinding event nonetheless may generate indistinguishable hot and cold spots. The influence of these results on analytic estimates of texture induced microwave anisotropies is examined, and comparison made with other numerical work.
description: 15 pages, standard LaTeX with 5 postscript figures available on request, SUSSEX-AST 94/3-1
title: ADCO, Boursier de Cîteaux : comptes (1489-1493) (11 H 1166), f. 00518
Creators: name: de la Côte-d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Boursier de Cîteaux : comptes (1489-1493), Archives départementales de la Côte-d'Or, (11 H 1166). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Boursier de Cîteaux : comptes (1489-1493), Archives départementales de la Côte-d'Or, (11 H 1166), f. 00518, 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
Additional file 1 of Validity and reliability of the simplified Chinese patient-reported outcomes version of the common terminology criteria for adverse events
Creators: name: Yang, Shan-Shan
name: Chen, Lei
name: Liu, Ying
name: Lu, Hai-Jun
name: Huang, Bo-Jie
name: Lin, Ai-Hua
name: Sun, Ying
name: Ma, Jun
name: Xie, Fang-Yun
name: Mao, Yan-Ping
Publisher: name: figshare
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1 Table S1. Item clusters of the PRO-CTCAE. Table S2. Criteria-related validity: Pearson’s correlation coefficients between PRO-CTCAE items and QLQ-C30 functional domains (N = 1555). Table S3. Criteria-related validity: Pearson correlation coefficients between similar symptom items on the PRO-CTCAE and QLQ-C30 (N = 1555). Table S4. Correlation matrix of factors (N = 1555). Table S5. Cronbach’s alpha of each dimension of the simple Chinese PRO-CTCAE (N = 1555). Table S6. Responsiveness of the Chinese PRO-CTCAE (N = 618)
Elliptic symbol calculus: from elliptic polylogarithms to iterated integrals of Eisenstein series
Creators: name: Broedel, Johannes
name: Duhr, Claude
name: Dulat, Falko
name: Penante, Brenda
name: Tancredi, Lorenzo
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We present a generalization of the symbol calculus from ordinary multiple polylogarithms to their elliptic counterparts. Our formalism is based on a special case of a coaction on large classes of periods that is applied in particular to elliptic polylogarithms and iterated integrals of modular forms. We illustrate how to use our formalism to derive relations among elliptic polylogarithms, in complete analogy with the non-elliptic case. We then analyze the symbol alphabet of elliptic polylogarithms evaluated at rational points, and we observe that it is given by Eisenstein series for a certain congruence subgroup. We apply our formalism to hypergeometric functions that can be expressed in terms of elliptic polylogarithms and show that they can equally be written in terms of iterated integrals of Eisenstein series. Finally, we present the symbol of the equal-mass sunrise integral in two space-time dimensions. The symbol alphabet involves Eisenstein series of level six and weight three, and we can easily integrate the symbol in terms of iterated integrals of Eisenstein series.
description: 65 pages
Initial Density Reconstruction from Lyman Alpha Tomography
Creators: name: Horowitz; Benjamin
Publisher: name: Zenodo
Year: 2019

description: Recent Lyman-α forest tomography measurements of the intergalactic medium (IGM) have revealed a wealth of cosmic structures at high redshift (z ∼ 2.5), including detection of large voids and protoclusters. In this talk, I will present the Tomographic Absorption Reconstruction and Density Inference Scheme (TARDIS), a new chrono-cosmographic analysis tool for understanding the formation and evolution of these observed structures. We use maximum likelihood techniques with a fast non-linear gravitational model to reconstruct the initial density field of the observed regions. This allows us to not only accurately reconstruct the cosmic web at z~2.5 from the observed Lyman-alpha forest, but also to track the trajectories of coeval z = 2.5 galaxies to their z = 0 cosmic web environments and shed new insight in galaxy formation and evolution.
Tailoring magnetic and magnetocaloric properties of martensitic transitions in ferromagnetic Heusler alloys
Creators: name: Aksoy, Seda
name: Krenke, Thorsten
name: Acet, Mehmet
name: Wassermann, Eberhard F.
name: Moya, Xavier
name: Manosa, Lluis
name: Planes, Antoni
Publisher: name: arXiv
Year: 2007
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Ni$_{50}$Mn$_{34}$In$_{16}$ undergoes a martensitic transformation around 250 K and exhibits a field induced reverse martensitic transformation and substantial magnetocaloric effects. We substitute small amounts Ga for In, which are isoelectronic, to carry these technically important properties to close to room temperature by shifting the martensitic transformation temperature.
description: 3 pages, 5 figures. Accepted for publication in Applied Physics Letters
Additional file 2: of Hepatitis B virus infection among pregnant women in Ethiopia: a systematic review and Meta-analysis of prevalence studies
Creators: name: Kindie Kebede
name: Dejene Abateneh
name: Alemayehu Belay
Publisher: name: figshare
Year: 2018
Subjects: subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: JBI Critical Appraisal Checklist for Studies Reporting Prevalence Data. (DOCX 12 kb)