cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 3: of The effect of introducing a financial incentive to promote application of fluoride varnish in dental practice in Scotland: a natural experiment
Creators: name: Gnich, Wendy
name: Sherriff, Andrea
name: Bonetti, Debbie
name: Conway, David
name: Macpherson, Lorna
Publisher: name: figshare
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Frequency of fluoride varnish application for children 6Â years and over by caries risk and Childsmile pilot practice status at time 1 and time 2. (DOCX 92 kb)
Constraints on radiative decay of the 17-keV neutrino from COBE Measurements
Creators: name: Nath, Biman B.
Publisher: name: arXiv
Year: 1992
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that, for a nontrivial radiative decay channel of the 17-keV neutrino, the photons would distort the microwave background radiation through ionization of the universe. The constraint on the branching ratio of such decays from COBE measurements is found to be more stringent than that from other considerations. The limit on the branching ratio in terms of the Compton $y$ parameter is $B_γ< 1.5 \times 10^{-7} ({τ_ν\over 10^{11} sec})^{0.45} ({y \over 10^{-3}})^{1.11} h^{-1}$ for an $Ω=1, Ω_b=0.1$ universe.
description: 7 pages. (figures will be sent on request) (To appear in Phys. Rev. D.)
Bose-Fermi Pair Correlations in Attractively Interacting Bose-Fermi Atomic Mixtures
Creators: name: Watanabe, Takayuki
name: Suzuki, Toru
name: Schuck, Peter
Publisher: name: arXiv
Year: 2007
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study static properties of attractively interacting Bose-Fermi mixtures of uniform atomic gases at zero temperature. Using Green's function formalism we calculate boson-fermion scattering amplitude and fermion self-energy in the medium to lowest order of the hole line expansion. We study ground state energy and pressure as functions of the scattering length for a few values of the boson-fermion mass ratio $m_b/m_f$ and the number ratio $N_b/N_f$. We find that the attractive contribution to energy is greatly enhanced for small values of the mass ratio. We study the role of the Bose-Fermi pair correlations in the mixture by calculating the pole of the boson-fermion scattering amplitude in the medium. The pole shows a standard quasiparticle dispersion for a Bose-Fermi pair, for $m_b/m_f\geq 1$. For small values of the mass ratio, on the other hand, a Bose-Fermi pair with a finite center-of-mass momentum experiences a strong attraction, implying large medium effects. In addition, we also study the fermion dispersion relation. We find two dispersion branches with the possibility of the avoided crossings. This strongly depends on the number rario $N_b/N_f$.
description: 14 pages, 27 figures
Modelling the UV spectrum of SDSS-III/BOSS galaxies: hints towards the detection of the UV upturn at high-z
Creators: name: Cras, Claire Le
name: Maraston, Claudia
name: Thomas, Daniel
name: York, Donald G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We exploit stellar population models of absorption line indices in the ultraviolet (from 2000 - 3200 Angstrom) to study the spectra of massive galaxies. Our central aim is to investigate the occurrence at high-redshift of the UV upturn, i.e. the increased UV emission due to old stars observed in massive galaxies and spiral bulges in the local Universe. We use a large (~275,000) sample of z~0.6 massive (log M*/Msun > 11.5) galaxies using both individual spectra and stacks and employ a suite of models including a UV contribution from old populations, spanning various effective temperatures, fuel consumptions and metallicities. We find that a subset of our indices, Mg I, Fe I, and BL3096, are able to differentiate between old and young UV ages. We find evidence for old stars contributing to the UV in massive galaxies, rather than star formation. The data favour models with low/medium upturn temperatures (10,000 - 25,000K) consistent with local galaxies, depending on the assumed metallicity, and with a larger fuel (f ~ 0.065 Msun). Models with one typical temperature are favoured over models with a temperature range, which would be typical of an extended horizontal branch. Old UV-bright populations are found in the whole galaxy sample (~92%), with a mass fraction peaking around 20-30%. Upturn galaxies are massive and have redder colours, in agreement with findings in the local Universe. We find that the upturn phenomenon appears at z~1 and its frequency increases towards lower redshift, as expected by stellar evolution of low mass stars. Our findings will help constrain stellar evolution in the exotic UV upturn phase.
description: 30 pages, 27 figures, 6 tables
Additional file 5: of ETV4 transcription factor and MMP13 metalloprotease are interplaying actors of breast tumorigenesis
Creators: name: Dumortier, Mandy
name: Ladam, Franck
name: Damour, Isabelle
name: Vacher, Sophie
name: BiĂ¨Che, Ivan
name: Marchand, Nathalie
name: Launoit, Yvan De
name: Tulasne, David
name: Chotteau-LeliĂ¨Vre, Anne
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Figure S3. ChIP experiment for ETV4 and MMP13 in MMT and TAC cells. PCR detection of the MMP13 promoter region after ETV4 immunoprecipitation in MMT-ETV4 (left panel) and TAC-ETV4 (right panel). Primers allowing the amplification of the proximal MMP13 promoter region containing EBS are schematized in the lower panel of Fig. 2. Cyclin D2 was used as a positive control [8]. Immunoprecipitation with a nonrelevant antibody (IgG) was used as negative control. (PDF 60 kb)
Gravitational Microlensing by Dark Clusters in the Galactic Halo
Creators: name: Maoz, Eyal
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The dark matter in Galactic halos, or some fraction of it, may be in the form of dark clusters which consist of small mass objects. Carr & Lacey (1987) have derived the permissible properties of such systems, and proposed the existence of dark clusters with mass of order $10^6\solarmass$ to explain some of the observed dynamical properties of the stellar disk of the Galaxy. A population of bound systems with mass of $\sim 10^5-10^6\solarmass$ is also an attractive possibility since it is close to the baryon Jeans mass at recombination, which may be the preferred mass scale for the first bound objects to form in the universe. At the present, the existence of dark clusters which consist of brown dwarfs, Jupiters, or black hole remnants of an early generation of stars, is not indicated, nor can be excluded on observational grounds. We describe how dark clusters can be discovered in a sample of gravitational microlensing events in LMC stars. Alternatively, it could provide strict bounds on the fraction of halo mass which resides in such systems. If MACHOs are clustered, the implied degeneracy in their spatial and velocity distributions would result in a strong autocorrelation in the sky position of microlensing events on an angular scale $\lesssim 20$ arcsec, along with a correlation in the event duration. We argue that a small number of events could be enough to indicate the existence of clusters, and demonstrate that a sample of $\simeq 10$ events would be sufficient to reject the proposal of Carr & Lacey (1987) at the $95\%$ confidence level.
description: 9 pages (no figures), Latex (AAS macros v3.0)
Investigating the Impacts of Food Choices on Food Carbon, Energy and Water Footprints
Creators: name: Spence, Porche
Publisher: name: QUBES Educational Resources
Year: 2025

description: The purpose of this activity is to introduce STEM and non-STEM majors to the FEW nexus by encouraging them to think about the impact of their food choices on food carbon footprint and rating, foods miles (energy) and water use. During this four-week activity, they will select a recipe of their choice, gather information from their local grocery store to calculate/estimate the food carbon footprint and rating, food miles (estimated distance between country of origin and grocery store - energy), and water footprint (amount of water needed to grow or produce the food), use a class dataset to evaluate the impacts of the recipes on FEW, and self-reflect on their experiences and learning gains. Students will connect their food choices with ecosystems, quantitative reasoning, communication, apply ecology, and human dependence on the environment.
Superspace Dynamics and Perturbations Around "Emptiness"
Creators: name: Soo, Chopin
name: Chang, Lay Nam
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: Superspace parametrized by gauge potentials instead of metric three-geometries is discussed in the context of the Ashtekar variables. Among other things, an "internal clock" for the full theory can be identified. Gauge-fixing conditions which lead to the natural geometrical separation of physical from gauge modes are derived with the use of the metric in connection-superspace. A perturbation scheme about an unconventional background which is inaccessible to conventional variables is presented. The resultant expansion retains much of the simplicity of Ashtekar's formulation of General Relativity.
description: 16 pages.(Revised 9/93) Preprint VPI-IHEP-93-5, CGPG-93/9-2, gr-qc/9307018
Additional file 1 of Long-term ambient PM2.5 exposure associated with cardiovascular risk factors in Chinese less educated population
Creators: name: Lin, Jianfeng
name: Zheng, Hua
name: Xia, Peng
name: Cheng, Xinqi
name: Wu, Wei
name: Li, Yang
name: Ma, Chaochao
name: Zhu, Guangjin
name: Xu, Tao
name: Zheng, Yali
name: Qiu, Ling
name: Chen, Limeng
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Biotechnology
Environmental Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Science Policy

description: Additional file 1.
Fractionally Charged Particles and Supersymmetry Breaking in 4D Strings
Creators: name: Antoniadis, I.
name: Benakli, K.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Four-dimensional string theories predict in general the existence of light exotic particles with fractional electric charges. Such particles could escape present observations if they are confined by a gauge group of the "hidden" sector into integrally charged states. It is conceivable that the same gauge group is also responsible for dynamical supersymmetry breaking, via gaugino and scalar condensation. The communication of the breaking to the observable sector is now mediated by ordinary gauge interactions, implying that the confining scale can be in the TeV-region. We study the main phenomenological implications of this possibility. In particular, we analyze the pattern of supersymmetry breaking and the mass-spectrum of the sparticles. We also show that this scenario can be consistent with the unification of all coupling constants at the string scale.
description: Revised version incorporating the erratum hep-ph/9707204 (to appear in Physics Letters B)
title: ADCO, Ordre cistercien : comptes (1403-1423) (11 H 1161), f. 00120
Creators: name: de la Côte-d'Or, Archives départementales
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Ordre cistercien : comptes (1403-1423), Archives départementales de la Côte-d'Or, (11 H 1161). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien : comptes (1403-1423), Archives départementales de la Côte-d'Or, (11 H 1161), f. 00120, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
Generalized Sums over Histories for Quantum Gravity II. Simplicial Conifolds
Creators: name: Schleich, Kristin
name: Witt, Donald M.
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: This paper examines the issues involved with concretely implementing a sum over conifolds in the formulation of Euclidean sums over histories for gravity. The first step in precisely formulating any sum over topological spaces is that one must have an algorithmically implementable method of generating a list of all spaces in the set to be summed over. This requirement causes well known problems in the formulation of sums over manifolds in four or more dimensions; there is no algorithmic method of determining whether or not a topological space is an n-manifold in five or more dimensions and the issue of whether or not such an algorithm exists is open in four. However, as this paper shows, conifolds are algorithmically decidable in four dimensions. Thus the set of 4-conifolds provides a starting point for a concrete implementation of Euclidean sums over histories in four dimensions. Explicit algorithms for summing over various sets of 4-conifolds are presented in the context of Regge calculus. Postscript figures available via anonymous ftp at black-hole.physics.ubc.ca (137.82.43.40) in file gen2.ps.
description: 82pp., plain TeX, To appear in Nucl. Phys. B,FF-92-2
The rest-frame UV-to-optical spectroscopy of APM 08279+5255 - BAL classification and black hole mass estimates
Creators: name: Saturni, F. G.
name: Bischetti, M.
name: Piconcelli, E.
name: Bongiorno, A.
name: Cicone, C.
name: Feruglio, C.
name: Fiore, F.
name: Gallerani, S.
name: Giustini, M.
name: Piranomonte, S.
name: Vietri, G.
name: Vignali, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the analysis of the rest-frame optical-to-UV spectrum of APM 08279+5255, a well-known lensed broad absorption line (BAL) quasar at $z = 3.911$. The spectroscopic data are taken with the optical DOLoRes and near-IR NICS instruments at TNG, and include the previously unexplored range between C III] $λ$1910 and [O III] $λλ$4959,5007. We investigate the possible presence of multiple BALs by computing "balnicity" and absorption indexes (i.e. BI, BI$_0$ and AI) for the transitions Si IV $λ$1400, C IV $λ$1549, Al III $λ$1860 and Mg II $λ$2800. No clear evidence for the presence of absorption features is found in addition to the already known, prominent BAL associated to C IV, which supports a high-ionization BAL classification for APM 08279+5255. We also study the properties of the [O III], H$β$ and Mg II emission lines. We find that [O III] is intrinsically weak ($F_{\rm [OIII]}/F_{\rm Hβ} \lesssim 0.04$), as it is typically found in luminous quasars with a strongly blueshifted C IV emission line ($\sim$2500 km s$^{-1}$ for APM 08279+5255). We compute the single-epoch black hole mass based on Mg II and H$β$ broad emission lines, finding $M_{\rm BH} = (2 ÷3) \times 10^{10}μ^{-1}$ M$_\odot$, with the magnification factor $μ$ that can vary between 4 and 100 according to CO and rest-frame UV-to-mid-IR imaging respectively. Using a Mg II equivalent width (EW)-to-Eddington ratio relation, the EW$_{\rm MgII} \sim 27$ Å measured for APM 08279+5255 translates into an Eddington ratio of $\sim$0.4, which is more consistent with $μ=4$. This magnification factor also provides a value of $M_{\rm BH}$ that is consistent with recent reverberation-mapping measurements derived from C IV and Si IV.
description: 10 pages, 4 figures, 4 tables, accepted for publication in A&A
ЎЗБЕКИСТОН РЕСПУБЛИКАСИ ХАЛҚАРО ШАРТНОМАЛАРИНИНГ МИЛЛИЙ ВА ХАЛҚАРО-ҲУҚУҚИЙ АСОСЛАРИ
Creators: name: Бозоров, З.З.
Publisher: name: Zenodo
Year: 2024

description: Мазкур мақолада халқаро шартномаларга оид муносабатларни тартибга солувчи қонунчилик базаси гуруҳларга ажратилган ҳолда таҳлил қилинган. Шунингдек, халқаро шартномаларни тузиш тартиби ва босқичларининг ўзига хос жиҳатлари ёритиб берилган.
The absence of a thin disc in M81
Creators: name: Young, A. J.
name: McHardy, I.
name: Emmanoulopoulos, D.
name: Connolly, S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the results of simultaneous Suzaku and NuSTAR observations of the nearest Low-Luminosity Active Galactic Nucleus (LLAGN), M81*. The spectrum is well described by a cut-off power law plus narrow emission lines from Fe K$α$, Fe XXV and Fe XXVI. There is no evidence of Compton reflection from an optically thick disc, and we obtain the strongest constraint on the reflection fraction in M81* to date, with a best-fit value of $R = 0.0$ with an upper limit of $R < 0.1$. The Fe K$α$ line may be produced in optically thin, $N_H = 1 \times 10^{23}$ cm$^{-2}$, gas located in the equatorial plane that could be the broad line region. The ionized iron lines may originate in the hot, inner accretion flow. The X-ray continuum shows significant variability on $\sim 40$ ks timescales suggesting that the primary X-ray source is $\sim 100$s of gravitational radii in size. If this X-ray source illuminates any putative optically thick disc, the weakness of reflection implies that such a disc lies outside a few $\times 10^3$ gravitational radii. An optically thin accretion flow inside a truncated optically thick disc appears to be a common feature of LLAGN that are accreting at only a tiny fraction of the Eddington limit.
description: 7 pages, 7 figures, to appear in MNARS
The evaluation of fundamental ability in acquiring minimally invasive surgical skill sets
Creators: name: Nugent, Emmeline
Publisher: name: Royal College of Surgeons in Ireland
Year: 2019
Subjects: Uncategorized

description: Background: Minimally invasive surgery (MIS) is an evolving area of surgery which is becoming more main-stream. However, when compared to the traditional open surgical approach MIS techniques have been demonstrated to be associated with a longer learning curve for the trainee surgeon. Aim: The overall objective of this thesis was to investigate and evaluate those factors that could influence the length of the learning curve and the capacity of a trainee to become a proficient minimally invasive surgeon. Materials & Methods: We evaluated three different areas; psychometric aptitude (visual spatial, depth perception & psychomotor), personality traits and non-technical skills (musical ability, playing sport & video games) and how these factors impacted on the surgical novice, junior and senior trainees ability to perform in both basic minimally invasive skills (laparoscopy, endoscopy & endovascular) and more advanced skills (laparoscopic colectomy) in a simulated setting. Results: The results demonstrated that there is a relationship between psychometric aptitude and MIS performance. This association was greatest in frequency and most consistent amongst the surgical novices with its effect decreasing with increasing surgical experience. However, the results also demonstrated that in trainees with significant surgical experience psychometric aptitude was associated with performance in an advanced MIS task (laparoscopic colectomy). Certain personality traits were also found to be associated with MIS performance (distractibility, confidence & energy). Finally, musical ability in particular was found to have the greatest association with MIS performance in contrast to the other nontechnical skills measured. Conclusion: We have shown that certain attributes influence the learning curve and the fundamental ability of the trainee surgeon in MIS techniques. These findings have relevance in the design of training curricula and when ensuring the optimum learning pathway for the individual trainee.
Additional file 3: of Molecular diversity and function of jasmintides from Jasminum sambac
Creators: name: Kumari, Geeta
name: Wong, Ka
name: Serra, Aida
name: Shin, Joon
name: Yoon, Ho
name: Siu Sze
name: Tam, James
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences

description: Figure S2. Summary of sequential and medium NOE connectivity. Slowly exchanging amide protons (filled box) and backbone vicinal coupling constants (open circle: 3JHNα 8 Hz) are indicated. (DOCX 4739 kb)
Is a Massive Tau Neutrino Just What Cold Dark Matter Needs?
Creators: name: Dodelson, Scott
name: Gyuk, Geza
name: Turner, Michael S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The cold dark matter (CDM) scenario for structure formation in the Universe is very attractive and has many successes; however, when its spectrum of density perturbations is normalized to the COBE anisotropy measurement the level of inhomogeneity predicted on small scales is too large. This can be remedied by a tau neutrino of mass $1\MeV - 10\MeV$ and lifetime $0.1\sec - 100\sec$ whose decay products include electron neutrinos because it allows the total energy density in relativistic particles to be doubled without interfering with nucleosynthesis. The anisotropies predicted on the degree scale for ``$τ$CDM'' are larger than standard CDM. Experiments at $e^\pm$ colliders may be able to probe such a mass range.
description: 9 pages LaTeX plus 4 figures (available upon request) FERMILAB--Pub--94/026-A
The cosmic evolution of the spatially-resolved star formation rate and stellar mass of the CALIFA survey
Creators: name: Fernández, R. López
name: Delgado, R. M. González
name: Pérez, E.
name: García-Benito, R.
name: Fernandes, R. Cid
name: Schoenell, W.
name: Sánchez, S. F.
name: Gallazzi, A.
name: Sánchez-Blázquez, P.
name: Asari, N. Vale
name: Walcher, C. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the cosmic evolution of the absolute and specific star formation rate (SFR, sSFR) of galaxies as derived from a spatially-resolved study of the stellar populations in a set of 366 nearby galaxies from the CALIFA survey. The analysis combines GALEX and SDSS images with the 4000 break, H_beta, and [MgFe] indices measured from the datacubes, to constrain parametric models for the SFH, which are then used to study the cosmic evolution of the star formation rate density (SFRD), the sSFR, the main sequence of star formation (MSSF), and the stellar mass density (SMD). A delayed-tau model, provides the best results, in good agreement with those obtained from cosmological surveys. Our main results from this model are: a) The time since the onset of the star formation is larger in the inner regions than in the outer ones, while tau is similar or smaller in the inner than in the outer regions. b) The sSFR declines rapidly as the Universe evolves, and faster for early than for late type galaxies, and for the inner than for the outer regions of galaxies. c) SFRD and SMD agree well with results from cosmological surveys. At z< 0.5, most star formation takes place in the outer regions of late spiral galaxies, while at z>2 the inner regions of the progenitors of the current E and S0 are the major contributors to SFRD. d) The inner regions of galaxies are the major contributor to SMD at z> 0.5, growing their mass faster than the outer regions, with a lookback time at 50% SMD of 9 and 6 Gyr for the inner and outer regions. e) The MSSF follows a power-law at high redshift, with the slope evolving with time, but always being sub-linear. f) In agreement with galaxy surveys at different redshifts, the average SFH of CALIFA galaxies indicates that galaxies grow their mass mainly in a mode that is well represented by a delayed-tau model, with the peak at z~2 and an e-folding time of 3.9 Gyr.
description: 23 pages, 16 figures, 6 tables, accepted for publication in Astronomy & Astrophysics. *Abridged abstract*
Additional file 2: of The effect of introducing a financial incentive to promote application of fluoride varnish in dental practice in Scotland: a natural experiment
Creators: name: Gnich, Wendy
name: Sherriff, Andrea
name: Bonetti, Debbie
name: Conway, David
name: Macpherson, Lorna
Publisher: name: figshare
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Item composition of theoretical domain scales. (DOC 61 kb)
Physics in the multiverse: an introductory review
Creators: name: Barrau, Aurelien
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: This brief note, written for non-specialists, aims at drawing an introductive overview of the multiverse issue.
description: 6 pages, html version available here : http://cerncourier.com/cws/article/cern/31860
Landscape Of Death And CommemorationBurial Space, Place and Evolution from Phoenician to Late Roman Malta
Creators: name: Cardona, David
Publisher: name: University of Leicester
Year: 2024

description: Malta’s thousands of rock-cut, underground burials are the result of a thousand years of funerary practices that evolved through the Phoenician, Punic, Roman and Byzantine periods. These have long attracted the interest of scholars but seldom has the data from these tombs been studied in a holistic manner, meaning that these temporal expressions of death, belief and commemoration have remained largely isolated from each other. This aim of my thesis is to investigate the sizeable corpus of funerary data available from Malta’s main ancient city of Melite in an attempt to recognise clusters and cemeteries over the various time phases being studied, in order to identify regional and chronological developments in form, design, content, décor and location. This includes relationships with the immediate environments of the tombs and hypogea, such as access and visibility. I also study related features, such as quarries, roads and cart-ruts. Critically, these analyses aim at getting to know the people involved in creating and being buried in these sites. Can we use the burials to learn more of contemporary communities and how they viewed these burial grounds? Were these sacred places within carefully selected landscape features or were utilitarian motives prevalent? My material is studied through several steps, starting with the detailed cataloguing and analysis of tombs and catacombs (many of which are only partially published or reported, if at all) with the aim of integrating all the typologies previously identified. This forms the basis onto which differences and similarities within and between the tombs – such as depositions, associated burial goods and decoration – as well as other features in tombs and in the landscape will be assessed. These relationships will be investigated both spatially and temporally, identifying links (or a lack of) between burial grounds through the different periods under review.
Thermal fluctuations in the conical state of monoaxial helimagnets
Creators: name: Laliena, Victor
name: Kato, Yusuke
name: Albalate, German
name: Campo, Javier
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The effect of thermal fluctuations on the phase structure of monoaxial helimagnets with external magnetic field parallel to the chiral axis is analyzed by means of a saddle point expansion of the free energy. The phase transition that separates the conical and forced ferromagnetic phases is changed to first order by the thermal fluctuations. In a purely monoaxial system the pitch of the conical state remains independent of temperature and magnetic field, as in mean field theory, even when fluctuations are taken into account. However, in presence of weak Dzyaloshinskii-Moriya interactions in the plane perpendicular to the chiral axis, thermal fluctuations induce a dependence of the pitch on temperature and magnetic field. This may serve to determine the nature of magnetic interactions in such systems.
description: 9 pages, 4 figures
Hidden Variables and the Two Theorems of John Bell
Creators: name: Mermin, N. David
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: Although skeptical of the prohibitive power of no-hidden-variables theorems, John Bell was himself responsible for the two most important ones. I describe some recent versions of the lesser known of the two (familar to experts as the "Kochen-Specker theorem") which have transparently simple proofs. One of the new versions can be converted without additional analysis into a powerful form of the very much better known "Bell's Theorem", thereby clarifying the conceptual link between these two results of Bell.
description: 27 pages, no figures. An initial page explains why I am posting this 25-year-old article
Proficiency-based simulation training in open and endovascular surgery.
Creators: name: Hseino, Hazem
Publisher: name: Royal College of Surgeons in Ireland
Year: 2019
Subjects: Uncategorized

description: The traditional form of surgical skills training and recent changes in health care have created challenges in keeping up the standards in skills training of future surgeons. The structured development of simulation training might help tackle these challenges. The main aim of this thesis was to explore whether basic surgical skills acquired using proficiency-based simulation training in superficial femoral artery (SFA) angioplasty and saphenofemoral junction (SFJ) dissection translate to real-world performance. Four studies were performed. In the first study, a procedure-specific checklist for SFA angioplasty was developed and validated using the Vascular Intervention Simulation Trainer (VIST) simulator. In the second study, the impact of an assistant on the technical skills of the primary operator performing SFA angioplasties on the VIST simulator was assessed. The first and the second studies were essential to study the transfer of endovascular skills after proficiency-based simulation training in SFA angioplasty to the interventional suite (third study). The fourth study describes the transfer of open vascular surgical skills after proficiency-based bench model simulation training in SFJ dissection to the operating room (OR). Simulation-trained trainees scored higher than the controls on the procedural checklist developed (86.80 ± 5.36 vs. 67.60 ± 6.02 P = 0.001) and a global rating scale (37.20 ± 4.09 vs. 24.40 ± 5.32 P = 0.003) when performing SFA angioplasty on patients. Similarly, bench model simulation-trained trainees scored higher than the controls on procedural (30.33 ± 2.07 vs. 18 ± 2.19 P < 0.001) and global (28.33 ± 1.86 vs. 18.50 ± 4.04 P < 0.001) rating scales when performing SFJ dissection on patients. Basic surgical skills acquired using proficiency-based simulation training in SFA angioplasty and SFJ dissection do translate to real world performance. Structured proficiency-based simulation training in SFA angioplasty and SFJ dissection should be incorporated into surgical training programs.
Collapse of a Circular Loop of Cosmic String
Creators: name: Garfinkle, David
name: Duncan, G. Comer
Publisher: name: arXiv
Year: 1993
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the collapse of a circular loop of cosmic string. The gravitational field of the string is treated using the weak field approximation. The gravitational radiation from the loop is evaluated numerically. The memtric of the loop near the point of collapse is found analytically.
description: 15 pages
Compact Lattice QED and the Coulomb Potential
Creators: name: Srivstava, Y. N.
name: Widom, A.
name: Friedman, M. H.
name: Panella, O.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The potential energy of a static charge distribution on a lattice is rigorously computed in the standard compact quantum electrodynamic model. The method used follows closely that of Weyl for ordinary quantum electrodynamics in continuous space-time. The potential energy of the static charge distribution is independent of temperature and can be calculated from the lattice version of Poisson's equation. It is the usual Coulomb potential.
description: 6 pages, includes one figure in Topdrawer, NUB 3054/92
Chapter 4 - Solving a problem they did not know they had. Tailoring participatory action research to deal with latent environmental problems: can Saba overcome the inertia?
Creators: name: Vaas, J.
Publisher: name: Zenodo
Year: 2019

description: Chapter 4 of the dissertation "Widely resented yet neglected: latent environmental problems. The case of an invasive alien vine on Saba and Statia", by Jetske Vaas, Utrecht University, December 2019. This chapter has been accepted by Regional Environmental Change as: Vaas, J., P.P.J. Driessen, M.
 Giezen, F. van Laerhoven, M.J. Wassen. Solving a problem they did not know they had. Tailoring
 participatory action research to deal with latent environmental problems: can Saba overcome the
 inertia?
Additional file 17 of Comparative functional genomics analysis of cytochrome P450 gene superfamily in wheat and maize
Creators: name: Li, Yixuan
name: Wei, Kaifa
Publisher: name: figshare
Year: 2020
Subjects: Biophysics
Biochemistry
Space Science
Medicine
Environmental Sciences not elsewhere classified
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Developmental Biology
Virology

description: Additional file 17: Figure S13. Validation of structures A. Stereo chemical quality of the structures assessed by Ramachandran plot using RAMPAGE server. B. Amino acid environment assessed by ERRAT using UCLA-DOE Institute for Genomics and Proteomics Server. C. Superposition of 4LXJ, TaCYP51G3_2D and ZmCYP51G35; Superposition of 2RCH, TaCYP74A98_4A and ZmCYP74A39; c. Superposition of 2X2N, TaCYP97A59_6B and ZmCYP97A16.
title: AN, Registre des écrous du Châtelet, Y5266, f. p1000779
Creators: name: Claustre, Julie
name: Nationales, Archives
name: Archives Nationales
name: Claustre, Julie
name: ArchivesNationales/J.CLAUSTRE/H.REGAZZI/2020
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: Châtelet
subject: registre

description: Registre des écrous du Châtelet, Archives Nationales, Y5266. Numérisation en mode image.
description: Bibliographic citation: Archives Nationales, Registre des écrous du Châtelet, Y5266, f. p1000779
Summing tree graphs at threshold
Creators: name: Brown, Lowell S.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The solution of the classical field equation generates the sum of all tree graphs. We show that the classical equation reduces to an easily solved ordinary differential equation for certain multiparticle threshold amplitudes and compute these amplitudes.
description: 11 pages in RevTex, UW/PT-92-16
Additional file 4: of ETV4 transcription factor and MMP13 metalloprotease are interplaying actors of breast tumorigenesis
Creators: name: Dumortier, Mandy
name: Ladam, Franck
name: Damour, Isabelle
name: Vacher, Sophie
name: BiĂ¨Che, Ivan
name: Marchand, Nathalie
name: Launoit, Yvan De
name: Tulasne, David
name: Chotteau-LeliĂ¨Vre, Anne
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Figure S2. ETS and AP-1 binding sites are highly conserved among mouse, human, and rabbit. Nucleotide sequence comparison of mouse, human, and rat proximal MMP13 promoters. Shaded boxes indicate the conserved ETS and AP-1 binding site sequences. (PDF 46 kb)
Decay of polarized muon at rest as a source of polarized neutrino beam
Creators: name: Ciechanowicz, S.
name: Sobkow, W.
name: Misiaszek, M.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this paper, we indicate the theoretical possibility of using the decay of polarized muons at rest as a source of the transversely polarized electron antineutrino beam. Such a beam can be used to probe new effects beyond standard model. We mean here new tests concerning CP violation, Lorentz structure and chirality structure of the charged current weak interactions. The main goal is to show how the energy and angular distribution of the electron antineutrinos in the muon rest frame depends on the transverse components of the antineutrino beam polarization. Our analysis is model-independent and consistent with the current upper limits on the non-standard couplings. The results are presented in a limit of infinitesimally small mass for all particles produced in the decay.
description: elsart style, 11 pages, 2 eps figures, submitted do publication
High-order Radio Frequency Differentiation via Photonic Signal Processing with an Integrated Micro-resonator Kerr Optical Frequency Comb Source
Creators: name: Xu, Xingyuan
name: Wu, Jiayang
name: Shoeiby, Mehrdad
name: Chu, Sai T.
name: Little, Brent E.
name: Morandotti, Roberto
name: Mitchell, Arnan
name: Moss, David J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: Signal Processing (eess.SP)
subject: Optics (physics.optics)
subject: FOS: Physical sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: We demonstrate the use of integrated micro-resonator based optical frequency comb sources as the basis for transversal filtering functions for microwave and radio frequency photonic filtering and advanced functions.
description: 8 pages, 7 figures, 46 References. arXiv admin note: substantial text overlap with arXiv:1512.01741, arXiv:1512.06301
title: ADCO, Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Cart. 168 (11 H 66), f. 0069r
Creators: name: de la Côte d'Or, Archives départementales
name: Projet CBMA
name: CG21/F.PETOT/2010
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP

description: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 168 (11 H 66), f. 0069r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 168 (11 H 66), f. 0069r, 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
Precision measurements on trapped antihydrogen in the ALPHA experiment
Creators: name: Eriksson, S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Both the 1S-2S transition and the ground state hyperfine spectrum have been observed in trapped antihydrogen. The former constitutes the first observation of resonant interaction of light with an anti-atom, and the latter is the first detailed measurement of a spectral feature in antihydrogen. Due to the narrow intrinsic linewidth of the 1S-2S transition and use of two-photon laser excitation, the transition energy can be precisely determined in both hydrogen and antihydrogen, allowing a direct comparison as a test of fundamental symmetry. The result is consistent with CPT invariance at a relative precision of around \num{2e-10}. This constitutes the most precise measurement of a property of antihydrogen. The hyperfine spectrum of antihydrogen is determined to a relative uncertainty of \num{4e-4}. The excited state and the hyperfine spectroscopy techniques currently both show sensitivity at the few \SI{100}{\kilo\hertz} level on the absolute scale. Here, the most recent work of the ALPHA collaboration on precision spectroscopy of antihydrogen is presented together with an outlook on improving the precision of measurements involving lasers and microwave radiation. Prospects of measuring the Lamb-shift and determining the antiproton charge radius in trapped antihydrogen in the ALPHA-apparatus are presented. Future perspectives of precision measurements of trapped antihydrogen in the ALPHA apparatus when the ELENA facility becomes available to experiments at CERN are discussed.
description: Accepted manuscript
Additional file 2: of Molecular diversity and function of jasmintides from Jasminum sambac
Creators: name: Kumari, Geeta
name: Wong, Ka
name: Serra, Aida
name: Shin, Joon
name: Yoon, Ho
name: Siu Sze
name: Tam, James
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Figure S1. NH/CÎąH fingerprint region of 2D-NOESY spectrum of jS3 recorded in 90% H2O/10% D2O at 298Â K. Sequential connectivity of each amino acid residue are shown by solid lines. (DOCX 4392 kb)
Additional file 1 of Parkinson’s disease with early motor complications: predicting EQ-5D- 3L utilities from PDQ-39 data in the EARLYSTIM trial
Creators: name: Zahra, Mehdi
name: Durand-Zaleski, Isabelle
name: Górecki, Michal
name: Walleser Autiero, Silke
name: Barnett, Gillian
name: Schüpbach, W.
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Mental Health

description: Additional file 1. Mean EQ-5D-3L utilities for France derived from PDQ-39 scores using the algorithms developed by (A) ordinal regression and (B) multinomial regression. EARLYSTIM trial data that were used in this analysis included the scores of the eight subscales of PDQ-39, for 127 BMT patients and 124 dB patients, measured at baseline, five, 12, and 24 month visits in addition to age and gender.
Urban water networks as an alternative source for district heating and emergency heat-wave cooling
Creators: name: Guo, Xiaofeng
name: Hendel, Martin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Urban water networks can contribute to the energy transition of cities by serving as alternatives sources for heating and cooling. Indeed, the thermal energy potential of the urban water cycle is considerable. Paris is taken as an example to present an assessment of the field performance of a district-scale waste water heat recovery system and to explore potential techniques for emergency cold recovery from drinking or non-potable water networks in response to heat-waves. The case heat recovery system was found to provide significant greenhouse gas emission reductions (up to 75%) and limited primary energy savings (around 30%). These limited savings are found to be mainly due to the performance of the heat pump system. Three emergency cold recovery techniques are presented as a response to heat-waves: subway station cooling, ice production for individual cooling, and "heat-wave shelter" cooling in association with pavement-watering. The cold generation potential of each approach is assessed with a special consideration for mains water temperature sanitary limitations. Finally, technical obstacles and perspectives are discussed.
Multiple High-Velocity Emission-Line Systems in the E+S Pair CPG 29
Creators: name: Marziani, P.
name: Keel, W. C.
name: Dultzin--Hacyan, D.
name: Sulentic, J. W.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A detailed study of the mixed-morphology galaxy pair CPG 29 (Arp 119, VV 347) shows spectacular spectroscopic peculiarities in the southern (spiral) component (Mkn 984) including a spatially resolved region, roughly aligned along the minor axis of the galaxy, with multiple emission-line components redshifted by as much as 1300 km s$^{-1}$ with respect to the LINER nucleus. Strong [OI]\l6300 and [SII]ł\l6716,6731 emission suggest shock ionization. The rest of the galaxy's disk is spectroscopically undistinguished, with emission lines characteristic of disk H II regions and, in large part, ordered rotation. We discuss the following four possible explanations for the morphological and spectroscopic peculiarities in the spiral: (1) a super--wind scenario, supported by the high FIR luminosity of the spiral, and by emission line activity similar to that observed in FIR strong galaxies; (2) motion of the spiral through a hot, relatively dense intergalactic medium, possibly associated with the elliptical, that could affect the star formation rate and create a brightened disk rim; (3) a faint companion in direct collision with the disk, at $Δv_r \sim 1000$ \kms, that would straightforwardly explain the existence of the different redshift systems; (4) a pole on collision by the elliptical, that could produce the disturbed morphology and other properties of the spiral. The elliptical/spiral pole--on collision explains the high velocity line emitting regions as tidally stripped gas, and accounts for the presence of gas ionized by moterate velocity shocks. The morphology of Mrk 984 is consistent
description: 40 pp. + 9 figures available upon request, AASTeX, no preprint number