cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Inflation from superstrings
Creators: name: De la Macorra, A.
name: Lola, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the possibility of obtaining inflationary solutions of the slow roll type from a low energy Lagrangian coming from superstrings. The advantage of such an approach is that in these theories the scalar potential has only one free parameter (the Planck scale) and therefore no unnatural fine tuning may be accommodated. We find that in any viable scheme the dilaton and the moduli fields have to be stabilized and that before this happens, no other field may be used as the inflaton. Then inflation may occur due to chiral matter fields. Demanding that the potential terms associated with the chiral fields do not spoil the dilaton and moduli minimization leads to severe constraints on the magnitude of the density fluctuations.
description: 22 pages, no figures, latex file We have corrected the magnitude of the density fluctuations, which become smaller than the COBE ones. Some references have also been added, and a few misprints corrected
Ultracold Rydberg Molecules
Creators: name: Shaffer, J. P.
name: Rittenhouse, S. T.
name: Sadeghpour, H. R
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Ultracold Rydberg molecules have been extensively studied both theoretically and ex-perimentally. Here the authors review the recent realizations of various ultralong-range Rydberg molecules and macrodimers, and explore their potential for current and future applications in spectroscopy, few- and many-body interactions and quantum information processing.
Fermions, differential forms and doubled geometry
Creators: name: Krasnov, Kirill
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We show that all fermions of one generation of the Standard Model (SM) can be elegantly described by a single fixed parity (say even) inhomogeneous real-valued differential form in seven dimensions. In this formalism the full kinetic term of the SM fermionic Lagrangian is reproduced as the appropriate dimensional reduction of (Psi, D Psi) where Psi is a general even degree differential form in R^7, the inner product is as described in the main text, and D is essentially an appropriately interpreted exterior derivative operator. The new formalism is based on geometric constructions originating in the subjects of generalised geometry and double field theory.
description: 40 pages, no figures
Additional file 1 of Transcriptomic comparison sheds new light on regulatory networks for dimorphic flower development in response to photoperiod in Viola prionantha
Creators: name: Li, Qiaoxia
name: Li, Kunpeng
name: Zhang, Zhengrong
name: Li, Jigang
name: Wang, Bo
name: Zhang, Zuoming
name: Zhu, Yuanyuan
name: Pan, Chaochao
name: Sun, Kun
name: He, Chaoying
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Supplementary Figures. (Figures S1–S11 in one PDF file)
MOESM2 of Positive cofactor 4 (PC4) contributes to the regulation of replication-dependent canonical histone gene expression
Creators: name: Brzek, Aleksandra
name: Cichocka, Marlena
name: Dolata, Jakub
name: Juzwa, Wojciech
name: Schümperli, Daniel
name: Raczynska, Katarzyna
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 2: Figure S1. HeLa cell lines with PC4 overexpression and inducible knockdown of PC4. (A, C) RT-qPCR was performed using primers designed to amplify PC4 mRNA in control cells and cells with PC4 overexpression (PC4 OE) (A) or PC4 knockdown (PC4 KD) (C). Error bars indicate standard deviations (SD) of three biological replicates. P-values were calculated on relative level of expression values using Student’s T-test, and statistical significance is represented as follows: *P ≤ 0.05. (B, D). Western blots followed by immunodetection with anti-actin and anti-PC4 antibodies were performed using protein extract isolated from wild type HeLa cells (HeLa), PC4 OE cells (B) and PC4 KD cells with (dox+) or without (dox−) doxycycline treatment (D).
Explicit symplectic integrator for particle tracking in s-dependent static electric and magnetic fields with curved reference trajectory
Creators: name: Wolski, Andrzej
name: Herrod, Alex
Publisher: name: arXiv
Year: 2018
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: We describe a method for symplectic tracking of charged particles through static electric and magnetic fields. The method can be applied to cases where the fields have a dependence on longitudinal as well as transverse position, and where the reference trajectory may have non-zero curvature. Application of the method requires analytical expressions for the scalar and vector potentials: we show how suitable expressions, in the form of series analogous to multipole expansions, can be constructed from numerical field data, allowing the method to be used in cases where only numerical field data are available.
description: 17 pages
A Model of Low-lying States in Strongly Interacting Electroweak Symmetry-Breaking Sector
Creators: name: Han, T.
name: Huang, Z.
name: Hung, P. Q.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is proposed that, in a strongly-interacting electroweak sector, besides the Goldstone bosons, the coexistence of a scalar state ($H$) and vector resonances such as $A_1$ [$I^G(J^P)=1^-(1^+$)], $V$ [$1^+(1^-)$] and $ω_H^{}$ [$0^-(1^-)$] is required by the proper Regge behavior of the forward scattering amplitudes. This is a consequence of the following well-motivated assumptions: (a). Adler-Weisberger-type sum rules and the superconvergence relations for scattering amplitudes hold in this strongly interacting sector; (b). the sum rules at $t=0$ are saturated by a minimal set of low-lying states with appropriate quantum numbers. It therefore suggests that a complete description should include all these resonances. These states may lead to distinctive experimental signatures at future colliders.
description: revised version, to appear in Modern Physics Letters A; file also available via anonymous ftp at ftp://ucdhep.ucdavis.edu/han/sews/lowlying.ps
Analytic Structure of Amplitudes in Gauge Theories with Confinement
Creators: name: Oehme, Reinhard
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: For gauge theories with confinement, the analytic structure of amplitudes is explored. It is shown that the analytic properties of physical amplitudes are the same as those obtained on the basis of an effective theory involving only the composite, physical fields. The corresponding proofs of dispersion relations remain valid. Anomalous thresholds are considered. They are related to the composite structure of particles. It is shown, that there are no such thresholds in physical amplitudes which are associated with confined constituents, like quarks and gluons in QCD. Unphysical amplitudes are considered briefly, using propagator functions as an example. For general, covariant, linear gauges, it is shown that these functions must have singularities at finite, real points, which may be associated with confined states.
description: Invited talk presented at the Conference on New Problems in the General Theory of Fields and Particles of the International Congress of Mathematical Physics, La Sorbonne, Paris, July 1994. 33 pages, Latex, 4 figures (not included)
MOESM1 of Using decision methods to examine the potential impact of intersectoral action programs
Creators: name: Wanrudee Isaranuwatchai
name: Bayoumi, Ahmed
name: Renahy, Emilie
name: Cheff, Rebecca
name: OâCampo, Patricia
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer

description: Additional file 1. Search strategy for this study.
title: 01_1659
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Resolving the polarized dust emission of the disk around the massive star powering the HH~80-81 radio jet
Creators: name: Girart, J. M.
name: Fernandez-Lopez, M.
name: Li, Z. -Y.
name: Yang, H.
name: Estalella, R.
name: Anglada, G.
name: Añez-Lopez, N.
name: Busquet, G.
name: Carrasco-Gonzalez, C.
name: Curiel, S.
name: Galvan-Madrid, R.
name: Gomez, J. F.
name: de Gregorio-Monsalvo, I.
name: Jimenez-Serra, I.
name: Krasnopolsky, R.
name: Marti, J.
name: Osorio, M.
name: Padovani, M.
name: Rao, R.
name: Rodriguez, L. F.
name: Torrelles, J. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Here we present deep (16 mumJy), very high (40 mas) angular resolution 1.14 mm, polarimetric, Atacama Large Millimeter/submillimeter Array (ALMA) observations towards the massive protostar driving the HH 80-81 radio jet. The observations clearly resolve the disk oriented perpendicular to the radio jet, with a radius of ~0.171 arcsec (~291 au at 1.7 kpc distance). The continuum brightness temperature, the intensity profile, and the polarization properties clearly indicate that the disk is optically thick for a radius of R<170 au. The linear polarization of the dust emission is detected almost all along the disk and its properties suggest that dust polarization is produced mainly by self-scattering. However, the polarization pattern presents a clear differentiation between the inner (optically thick) part of the disk and the outer (optically thin) region of the disk, with a sharp transition that occurs at a radius of 0.1 arcsec (~170 au). The polarization characteristics of the inner disk suggest that dust settling has not occurred yet with a maximum dust grain size between 50 and 500 mum. The outer part of the disk has a clear azimuthal pattern but with a significantly higher polarization fraction compared to the inner disk. This pattern is broadly consistent with self-scattering of a radiation field that is beamed radially outward, as expected in the optically thin outer region, although contribution from non-spherical grains aligned with respect to the radiative flux cannot be excluded.
description: Accepted for publication in the Astrophysical Journal Letters
The Structure and Dynamics of the Sub-parsec Scale Jet in M87 Based on 50 VLBA Observations Over 17 Years at 43 GHz
Creators: name: Walker, R. Craig
name: Hardee, Phillip E.
name: Davies, Frederick B.
name: Ly, Chun
name: Junor, William
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The central radio source in M87 provides the best opportunity to study jet formation because it has a large angular size for the gravitational radius of the black hole and has a bright jet that is well resolved by VLBI observations. We present intensive monitoring observations from 2007 and 2008, plus roughly annual observations that span 17 years, all made with the the Very Long Baseline Array at 43 GHz with a resolution of about 30 by 60 Rs. Our high-dynamic-range images clearly show the wide-opening-angle structure and the counter-jet. The jet and counter-jet are nearly symmetric in the inner 1.5 milli-arcseconds (mas; 0.12 pc in projection) with both being edge brightened. Both show deviations from parabolic shape in the form of an initial rapid expansion and subsequent contraction followed by further rapid expansion and, beyond the visible counter-jet, subsequent collimation. Proper motions and counter-jet/jet intensity ratios both indicate acceleration from apparent speeds of $\lesssim 0.5c$ to $\gtrsim 2c$ in the inner about 2 mas and suggest a helical flow. The jet displays a sideways shift with an approximately 8 to 10 year quasi-periodicity. The shift propagates outwards non-ballistically and significantly more slowly than the flow speed revealed by the fastest moving components. Polarization data show a systematic structure with magnetic field vectors that suggest a toroidal field close to the core.
description: 49 pages, 25 figures (one double). 4 tables, 3 animations. Accepted for publication in the Astrophysical Journal. The animations are provided in the ancillary files
INFORMATSION TEXNOLOGIYALAR ASOSIDA YUQORI MALAKALI, ZAMONAVIY XOTIN-QIZLARNI TAYYORLASHNING DOLZARB MUAMMOLARI
Creators: name: Sobirova, Nigina
name: Maxmudova, Shaxlo
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqolada hozirgi kunda xotin-qizlarga berilyotgan keng imkoniyatlar, shart-sharoitlar hamda  informatsion texnologiyalar asosida yuqori malakali, zamonaviy xotin-qizlarni tayyorlashning dolzarb muammolari haqida fikr yuritiladi. Jamiyatda xotin-qizlarning  o‘rni beqiyosdir. Har bir sohada talab qilinayotgan zamonaviy axborot texnologiylarni bilish xotin-qizlarning ish faoliyatlarida o‘z ta’sirini o‘tkazmoqda. Nafaqat ilm-fan balki iqtisodiy-siyosiy jabhalarni rivojlantirishda  informatsion texnologiyalar asosida yuqori malakali kadrlarni tayyorlash bugungi kunning muhim masalalaridan biri hisoblanadi. Aynan shu sohada qilingan ishlar to‘g‘risida maqolamizda atroflicha yoritilgan.
Evidence of energy and charge sign dependence of the recovery time for the December 2006 Forbush event measured by the PAMELA experiment
Creators: name: Munini, R.
name: Boezio, M.
name: Bruno, A.
name: Christian, E. C.
name: de Nolfo, G. A.
name: Di Felice, V.
name: Martucci, M.
name: Merge, M.
name: Richardson, I. G.
name: Ryan, J. M.
name: Stochaj, S.
name: Adriani, O.
name: Barbarino, G. C.
name: Bazilevskaya, G. A.
name: Bellotti, R.
name: Bongi, M.
name: Bonvicini, V.
name: Bottai, S.
name: Cafagna, F.
name: Campana, D.
name: Carlson, P.
name: Casolino, M.
name: Castellini, G.
name: De Santis, C.
name: Galper, A. M.
name: Karelin, A. V.
name: Koldashov, S. V.
name: Koldobskiy, S.
name: Krutkov, S. Y.
name: Kvashnin, A. N.
name: Leonov, A.
name: Malakhov, V.
name: Marcelli, L.
name: Mayorov, A. G.
name: Menn, W.
name: Mikhailov, V. V.
name: Mocchiutti, E.
name: Monaco, A.
name: Mori, N.
name: Osteria, G.
name: Panico, B.
name: Papini, P.
name: Pearce, M.
name: Picozza, P.
name: Ricci, M.
name: Ricciarini, S. B.
name: Simon, M.
name: Sparvoli, R.
name: Spillantini, P.
name: Stozhkov, Y. I.
name: Vacchi, A.
name: Vannuccini, E.
name: Vasilyev, G.
name: Voronov, S. A.
name: Yurkin, Y. T.
name: Zampa, G.
name: Zampa, N.
name: Potgieter, M. S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: New results on the short-term galactic cosmic ray (GCR) intensity variation (Forbush decrease) in December 2006 measured by the PAMELA instrument are presented. Forbush decreases are sudden suppressions of the GCR intensities which are associated with the passage of interplanetary transients such as shocks and interplanetary coronal mass ejections (ICMEs). Most of the past measurements of this phenomenon were carried out with ground-based detectors such as neutron monitors or muon telescopes. These techniques allow only the indirect detection of the overall GCR intensity over an integrated energy range. For the first time, thanks to the unique features of the PAMELA magnetic spectrometer, the Forbush decrease commencing on 2006 December 14, following a CME at the Sun on 2006 December 13 was studied in a wide rigidity range (0.4 - 20 GV) and for different species of GCRs detected directly in space. The daily averaged GCR proton intensity was used to investigate the rigidity dependence of the amplitude and the recovery time of the Forbush decrease. Additionally, for the first time, the temporal variations in the helium and electron intensities during a Forbush decrease were studied. Interestingly, the temporal evolutions of the helium and proton intensities during the Forbush decrease were found in good agreement, while the low rigidity electrons (< 2 GV) displayed a faster recovery. This difference in the electron recovery is interpreted as a charge-sign dependence introduced by drift motions experienced by the GCRs during their propagation through the heliosphere.
title: The Short-Term Effects of Grade 1 and 2 Joint Mobilizations on Subject Pain Range of Motion and Muscle Activity in the Pathological Lumbar Spine
Creators: name: Hanrahan, Sean
Publisher: name: Old Dominion University
publisherIdentifier: https://ror.org/04zjtrb98
publisherIdentifierScheme: ROR
Year: 2003

description: The purpose of this study was to examine the short-term effects of Grades 1 and 2 posteroanterior joint mobilizations (JM) at the pathological lumbar spine on subject pain, range of motion (ROM), and muscle force. All subjects were determined to have sustained mechanical dysfunction of the lumbar spine of less than 48 hours as assessed through a standardized evaluation. Subjects were randomly assigned to a group; the control group received ice and stretching while the experimental group received JM in addition to ice and stretching. The JM's were performed at 3 consecutive lumbar segments surrounding the area of greatest discomfort. The oscillatory treatment was administered for 30 seconds with a 30 second resting period, and Grade 1 JM' s were utilized initially followed by Grade 2 JM's, for a total of six 30-second treatments. Data collection consisted of (1) pain assessment through the McGill Pain Questionnaire (MPQ), and a visual analog scale (VAS) in lumbar neutral, flexion, and extension, (2) ROM through the double inclinometer method at the LI and L5 spinous processes, and (3) muscle force with a hand-held dynamometer during maximal voluntary contraction. Data collection was undertaken immediately prior to and following the administration of JM's or no treatment, as well as 24 hours after the initial measurements. The MPQ was only completed initially and at 24 hours post-treatment. All subjects were intercollegiate athletes who continued participation during data collection. All JM treatment sessions were performed manually by a certified athletic trainer in the clinical setting. Various analyses were computed (2 x 2 ANOVA's, 2 x 3 ANOVA's and non parametric statistics) for all dependent measures. All subjects had decreased values for the MPQ over time, but no difference was found between treatment groups. However, when each subscale was evaluated, the experimental group had a significantly decreased sensory subscale following the treatment. Muscle force increased for both groups over time. A Tukey HSD Post Hoc comparison revealed significantly higher force values over time for those treated with the JM's. Friedman testing showed significant decreases in VAS scoring during lumbar neutral and flexion after JM. There were no significant differences between the groups for ROM. JM's for pain are a useful component in the treatment of acute mechanical dysfunctions in the lumbar spine. Further research should investigate other segments of the spine and the utilization of this technique.
On O(N)-Symmetric Gauged $ϕ^6{}_{2+1}$ Theory with Chern-Simons Term
Creators: name: Park, S. H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I investigate the effects of the Chern-Simons coupling on high-energy behavior in $2+1$ dimensional U(1) gauged $η(ϕ^\daggerϕ)^3$ theory with a Chern-Simons term. The effective potential and the $β$ function for $η$ are calculated to the next-to-leading order of the $1/N$ expansion as functions of $θ$ (the Chern-Simons coupling). For all $θ$, the theory is found to be driven to instability region at high momenta. It is briefly discussed on radiative corrections to $θ$.
description: 9 pages, LaTex file
Gravitational wave sources from inspiralling globular clusters in the Galactic Centre and similar environments
Creators: name: Sedda, Manuel Arca
name: Gualandris, Alessia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We model the inspiral of globular clusters (GCs) towards a galactic nucleus harboring a supermassive black hole (SMBH), a leading scenario for the formation of nuclear star clusters. We consider the case of GCs containing either an intermediate-mass black hole (IMBH) or a population of stellar mass black holes (BHs), and study the formation of gravitational wave (GW) sources. We perform direct summation $N$-body simulations of the infall of GCs with different orbital eccentricities in the live background of a galaxy with either a shallow or steep density profile. We find that the GC acts as an efficient carrier for the IMBH, facilitating the formation of a bound pair. The hardening and evolution of the binary depends sensitively on the galaxy's density profile. If the host galaxy has a shallow profile the hardening is too slow to allow for coalescence within a Hubble time, unless the initial cluster orbit is highly eccentric. If the galaxy hosts a nuclear star cluster, the hardening leads to coalescence by emission of GWs within $3-4$ Gyr. In this case, we find a IMBH-SMBH merger rate of $Γ_{\rm IMBH-SMBH} = 2.8\times 10^{-3}$ yr$^{-1}$ Gpc$^{-3}$. If the GC hosts a population of stellar BHs, these are deposited close enough to the SMBH to form extreme-mass-ratio-inspirals with a merger rate of $Γ_{\rm EMRI} = 0.25$ yr$^{-1}$ Gpc$^{-3}$. Finally, the SMBH tidal field can boost the coalescence of stellar black hole binaries delivered from the infalling GCs. The merger rate for this merging channel is $Γ_{\rm BHB} = 0.4-4$ yr$^{-1}$ Gpc$^{-3}$.
description: 21 pages, 29 figures, 6 tables. Accepted for publication in MNRAS
Carnet nº 4, commencé à Novorossiïsk (p. 46)
Creators: name: Péraire, Lucien
name: CNRS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023

description: created: 1-5-1929
Additional file 2: of Knowledge of HPV and acceptability of HPV vaccine among women in western China: a cross-sectional survey
Creators: name: Junyong He
name: Lixia He
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Biotechnology
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Questionnaire (English). (DOCX 18 kb)
CHANG-ES XI: Circular Polarization in the Cores of Nearby Galaxies
Creators: name: Irwin, Judith A
name: Henriksen, Richard N.
name: Wezgowiec, Marek
name: Damas-Segovia, Ancor
name: Wang, Q. Daniel
name: Krause, Marita
name: Heald, George
name: Dettmar, Ralf-Juergen
name: Li, Jiang-Tao
name: Wiegert, Theresa
name: Stein, Yelena
name: Braun, Timothy T.
name: Im, Jisung
name: Schmidt, Philip
name: Macdonald, Scott
name: Miskolczi, Arpad
name: Merritt, Alison
name: Mora-Partiarroyo, S. C.
name: Saikia, D. J.
name: Sotomayor, Carlos
name: Yang, Yang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We detect 5 galaxies in the CHANG-ES (Continuum Halos in Nearby Galaxies -- an EVLA Survey) sample that show circular polarization (CP) at L-band in our high resolution data sets. Two of the galaxies (NGC~4388 and NGC~4845) show strong Stokes $V/I\,\equiv\,m_C\,\sim\,2$\%, two (NGC~660 and NGC~3628) have values of $m_C\sim \,0.3$\%, and NGC~3079 is a marginal detection at $m_C\sim \,0.2$\%. The two strongest $m_C$ galaxies also have the most luminous X-ray cores and the strongest internal absorption in X-rays. We have expanded on our previous Faraday conversion interpretation and analysis and provide analytical expressions for the expected $V$ signal for a general case in which the cosmic ray electron energy spectral index can take on any value. We provide examples as to how such expressions could be used to estimate magnetic field strengths and the lower energy cutoff for CR electrons. Four out of our detections are {\it resolved}, showing unique structures, including a {\it jet} in NGC~4388 and a CP `conversion disk' in NGC~4845. The conversion disk is inclined to the galactic disk but is perpendicular to a possible outflow direction. Such CP structures have never before been seen in any galaxy to our knowledge. None of the galaxy cores show linear polarization at L-band. Thus CP may provide a unique probe of physical conditions deep into radio AGNs.
description: 30 pages, 4 figures, accepted to MNRAS
High-colour pomerons with a running coupling constant in the Hartree-Fock approximation
Creators: name: Braun, M. A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The Hartree-Fock approximation is applied to study the "high-colour pomerons" in the system of many reggeized gluons with a running QCD coupling constant. It is shown that, contrary to the fixed coupling case, the high-colour pomerons result supercritical, although with a smaller intercept than the multipomeron states.
description: 8 pages, LaTeX, no figures
Semantic Segmentation of Pathological Lung Tissue with Dilated Fully Convolutional Networks
Creators: name: Anthimopoulos, Marios
name: Christodoulidis, Stergios
name: Ebner, Lukas
name: Geiser, Thomas
name: Christe, Andreas
name: Mougiakakou, Stavroula
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Early and accurate diagnosis of interstitial lung diseases (ILDs) is crucial for making treatment decisions, but can be challenging even for experienced radiologists. The diagnostic procedure is based on the detection and recognition of the different ILD pathologies in thoracic CT scans, yet their manifestation often appears similar. In this study, we propose the use of a deep purely convolutional neural network for the semantic segmentation of ILD patterns, as the basic component of a computer aided diagnosis (CAD) system for ILDs. The proposed CNN, which consists of convolutional layers with dilated filters, takes as input a lung CT image of arbitrary size and outputs the corresponding label map. We trained and tested the network on a dataset of 172 sparsely annotated CT scans, within a cross-validation scheme. The training was performed in an end-to-end and semi-supervised fashion, utilizing both labeled and non-labeled image regions. The experimental results show significant performance improvement with respect to the state of the art.
ROLE OF WOMEN ENHANCING INNOVATION INFRASTRUCTURE FOR ECONOMIC DEVELOPMENT IN UZBEKISTAN: CHALLENGES AND STRATEGIC APPROACHES
Creators: name: Tairova, Zarnigor
name: Aslonov, Muhammad
Publisher: name: Zenodo
Year: 2024

description: This paper explores the critical role of women in enhancing innovation infrastructure to spur economic development in Uzbekistan, while addressing both prevailing challenges and strategic approaches. Despite making up a significant portion of the population and workforce, Uzbek women remain underrepresented in sectors critical to innovation and economic growth, particularly in science, technology, engineering, and mathematics (STEM) fields. This study delves into cultural, educational, economic, and professional obstacles that hinder women’s full participation and leadership in innovation. It discusses strategic approaches, including policy reforms, targeted educational programs, support for women entrepreneurs, and the creation of networks and mentorship opportunities aimed at empowering women. Through qualitative analysis and case studies, this research highlights the transformative potential of women in innovation sectors and proposes a multi-stakeholder implementation framework to overcome gender disparities. The findings underscore the necessity of integrating gender inclusivity into national policies to foster a robust innovation ecosystem that can drive sustainable economic development in Uzbekistan.
Asymmetry of line profiles of stellar oscillations measured by Kepler for ensembles of solar-like oscillators: impact on mode frequencies and dependence on effective temperature
Creators: name: Benomar, O.
name: Goupil, Mjo.
name: Belkacem, K.
name: Appourchaux, T.
name: Nielsen, M. B.
name: Bazot, M.
name: Gizon, L.
name: Hanasoge, S.
name: Sreenivasan, K. R.
name: Marchand, B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Oscillation properties are usually measured by fitting symmetric Lorentzian profiles to the power spectra of Sun-like stars. However the line profiles of solar oscillations have been observed to be asymmetrical for the Sun. The physical origin of this line asymmetry is not fully understood, although it should depend on the depth dependence of the source of wave excitation (convective turbulence) and details of the observable (velocity or intensity). For oscillations of the Sun, it has been shown that neglecting the asymmetry leads to systematic errors in the frequency determination. This could subsequently affects the results of seismic inferences of the solar internal structure. Using light curves from the {\it Kepler} spacecraft we have measured mode asymmetries in 43 stars. We confirm that neglecting the asymmetry leads to systematic errors that can exceed the $1σ$ confidence intervals for seismic observations longer than one year. Therefore, the application of an asymmetric Lorentzian profile is to be favoured to improve the accuracy of the internal stellar structure and stellar fundamental parameters. We also show that the asymmetry changes sign between cool Sun-like stars and hotter stars. This provides the best constraints to date on the location of the excitation sources across the Hertzsprung-Russel diagram.
description: 8 pages, 7 Figures, 1 Table, Accepted to ApJ
Additional file 1: of Assessment of personal exposure to particulate air pollution: the first result of City Health Outlook (CHO) project
Creators: name: Liang, Lu
name: Gong, Peng
name: Cong, Na
name: Li, Zhichao
name: Zhao, Yu
name: Chen, Ying
Publisher: name: figshare
Year: 2019
Subjects: Space Science
Environmental Sciences not elsewhere classified
Chemical Sciences not elsewhere classified
Marine Biology
Science Policy
Computational Biology

description: The validation of TE-STR against TSI aerosol monitor in both chamber-controlled environment and outdoor environment. (DOCX 630 kb)
Synthesis of Unused-wood-derived C-Fe-N Catalysts for Oxygen Reduction Reaction by Heteroatom Doping During Hydrothermal Carbonisation and Subsequent Carbonisation in Nitrogen Atmosphere
Creators: name: Goto, Yasuto
name: Nakayasu, Yuta
name: Abe, Hiroya
name: Katsuyama, Yuto
name: Itoh, Takashi
name: Watanabe, Masaru
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: 91305 Energy Generation, Conversion and Storage Engineering
subject: FOS: Mechanical engineering
subject: 30203 Inorganic Green Chemistry
subject: FOS: Chemical sciences
subject: 30504 Organic Green Chemistry

description: Tables and Raman spactra
MOESM2 of Infection of novel reassortant H1N2 and H3N2 swine influenza A viruses in the guinea pig model
Creators: name: Tapia, Rodrigo
name: García, Victoria
name: Mena, Juan
name: Bucarey, Sergio
name: Medina, Rafael
name: Neira, Víctor
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Evolutionary Biology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Additional file 2. Phylogenetic trees based on HA sequences of subtype H3. Maximum Likelihood method and General Time Reversible model with a variation rate among sites given by gamma distribution with invariant sites (GTR + G + I) were used. Human and swine reference sequences are in black. Chilean IAVs-S sequences are in red, and the node of the selected virus for guinea pig infection is highlighted with a red circle. The closest related sequences to the Chilean H3 IAV-S correspond to human sequences, which are highlighted in blue.
Prime divisors of the Lagarias sequence
Creators: name: Moree, Pieter
name: Stevenhagen, Peter
Publisher: name: arXiv
Year: 1999
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: For integer a let us consider the sequence X_a={x_0,x_1,x_2,...} defined by x_0=a, x_1=1 and, for n>=1, x_{n+1}=x_n+x_{n-1}. We say that a prime p divides X_a if p divides at least one term of the sequence. It is easy to see that every prime p divides X_1, the sequence of Fibonacci numbers. Lagarias, using a technique involving the computation of degrees of various Kummerian extensions first employed by Hasse, showed in 1985 that X_2, the set of primes dividing some Lucas number has natural density 2/3 and posed as a challenge finding the density of prime divisors of X_3. In this paper we resolve this challenge, assuming GRH, by showing that the density of X_3 equals 1573727S/1569610, with S the so called Stephens constant. This is the first example of a `non-torsion' second order recurrent sequence with irreducible recurrence relation for which we can determine the associated density of prime divisors.
Role of edge poloidal density asymmetry in tokamak confinement
Creators: name: Aydemir, A. Y.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Mass flows and radial electric field driven by edge poloidal density asymmetries can be used as a highly effective control mechanism for the edge and thus global confinement in tokamaks. The underlying physics can be demonstrated entirely within a simple magnetohydrodynamic equilibrium model, without resorting to sophisticated and usually collisionality-dependent neoclassical physics arguments. As an example, strong dependence of the low to high (LH) transition power threshold on the magnetic topology, an experimental observation still poorly understood, can be easily explained within this framework. Similar arguments indicate that the ITER fueling ports above the midplane might lead to higher input power requirements.
description: 5 pages, 7 figures
CP Violation in $τ\rightarrow 3πν_τ$
Creators: name: Choi, S. Y.
name: Hagiwara, K.
name: Tanabashi, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider CP violating effects in the decays $τ\rightarrow (3π)ν_τ$ where both the ${\rm J}^{\rm P}=1^+$ resonance, $a_1$, and ${\rm J}^{\rm P}=0^-$ resonance, $π^\prime$, can contribute. The interference between the $a_1$ and $π^\prime$ resonances can lead to enhanced CP-violating asymmetries whose magnitudes depend crucially on the $π^\prime$ decay constant, $f_{π^\prime}$. We make an estimate of $f_{π^\prime}$ with a simplified chiral Lagrangian coupled to a massive pseudoscalar field, and we compare the estimates from the non-relativistic quark model and from the QCD sum rule with the estimate from the `mock' meson model. We then estimate quantitatively the size of CP-violating effects in a multi-Higgs-doublet model and scalar-leptoquark models. We find that, while CP-violating effects in the scalar-leptoquark models may require more than $10^{10}$ $τ$ leptons, CP-violating effects from the multi-Higgs-doublet model can be seen at the $2σ$ level with about $10^7$ $τ$ leptons using the chiral Lagrangian estimate of $f_{π^\prime}=(1\sim 5)\times 10^{-3}$ GeV.
description: Latex, 30 pages, 2 figures (not included). Three compressed postscript files of the paper available at ftp://ftp.kek.jp/kek/preprints/TH/TH-419/kekth419.ps.gz, Tau1.ps.gz, Tau2.ps.gz
O'ZBEKISTONDA IT – TEXNOLOGIYALARI SOHASIDA XOTIN-QIZLAR ROLINING RIVOJLANISH BOSQICHLARI
Creators: name: Mavlyanova, Nodira
name: Sodikova, Nigora
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqolada O‘zbekistonda ayollarning axborot texnologiyalari (IT) sohasidagi rolining rivojlanish bosqichlari tahlil qilingan. Tarixiy sharoitdan tortib, zamonaviy tendentsiyalargacha O‘zbekistonda ayollarning IT-sohasida ishtirok etishiga ta’sir etuvchi omillar ko‘rib chiqilmoqda. Mualliflar e’tiborni ayollarning IT kareralarini tanlash va targ‘ib qilishda duch keladigan to‘siqlarga, shuningdek, ularning ishtirokini qo‘llab-quvvatlashga qaratilgan turli tashabbus va dasturlarga qaratadi. Natijada maqolada O‘zbekistonda barqaror rivojlanish va farovonlikka erishish uchun IT sohasida gender tengligi va inklyuzivlik muhimligiga alohida e’tibor qaratilgan.
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0065
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: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0065, 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. 0065, 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
Additional file 3: of Synthesizing existing evidence to design future trials: survey of methodologists from European institutions
Creators: name: Nikolakopoulou, Adriani
name: Trelle, Sven
name: Sutton, Alex
name: Egger, Matthias
name: Salanti, Georgia
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology

description: Full results. (DOCX 45 kb)
Inverse spectral theory for a class of non-compact Hankel operators
Creators: name: Gerard, Patrick
name: Pushnitski, Alexander
Publisher: name: arXiv
Year: 2018
Subjects: subject: Spectral Theory (math.SP)
subject: Complex Variables (math.CV)
subject: FOS: Mathematics
subject: 47B35, 30H10

description: We characterize all bounded Hankel operators $Γ$ such that $Γ^*Γ$ has finite spectrum. We identify spectral data corresponding to such operators and construct inverse spectral theory including the characterization of these spectral data.
Specific temperature dependence of pseudogap in YBa$_2$Cu$_3$O$_{7-δ}$ nanolayers
Creators: name: Solovjov, A. L.
name: Omelchenko, L. V.
name: Stepanov, V. B.
name: Vovk, R. V.
name: Habermeier, H. -U.
name: Lochmajer, H.
name: Przysłupski, P.
name: Rogacki, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The pseudogap (PG) derived from the analysis of the excess conductivity $σ'(T)$ in superlattices and double-layer films of $YBa_2Cu_3O_{7-δ}$-$PrBa_2Cu_3O_{7-δ}$(YBCO-PrBCO), prepared by pulsed laser deposition, is studied for the first time. The $σ'(T)$ analysis has been performed within the local-pair (LP) model based on the assumption of the paired fermion (LPs) formation in the cuprate high-$T_c$ superconductors (cuprates) below the representative temperature $T^*\gg T_c$ resulting in the PG opening. Within the model, the temperature dependencies of the PG, $Δ^*(T)$, for the samples with different number of the PrBCO layers ($N_{Pr}$) were analyzed in the whole temperature range from $T^*$ down to $T_c$. Near $T_c$, excess conductivity was found to be perfectly described by the Aslamasov-Larkin and Hikami-Larkin (Maki-Thompson term) fluctuation theories, suggesting the presence of superconducting fluctuations in a relatively large (up to 15 K) temperature range above $T_c$. All sample parameters were found to change with increase of $N_{Pr}$, finally resulting in the appearance of the pronounced maximum of $Δ^*(T)$ at high temperatures. The result is most likely due to increasing influence of the intrinsic magnetism of PrBCO ($μ_{Pr}\approx 4\,μ_B$) and suggests the possibility to search in that way the change of interplay between the superconductivity and magnetism in cuprates.
description: 11 pages, 12 figures
Additional file 5: of Genome-wide analysis of the WRKY gene family and their positive responses to phytoplasma invasion in Chinese jujube
Creators: name: Xue, Chaoling
name: Li, Hongtai
name: Liu, Zhiguo
name: Wang, Lili
name: Zhao, Yitong
name: Wei, Ximeng
name: Fang, Hu
name: Liu, Mengjun
name: Zhao, Jin
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: The phylogenetic analysis of Group III WRKYs of Ziziphus jujuba, Arabidopsis thaliana, Pyres Bretschneideri, Persica Prunus and Malus domestica. (DOC 89 kb)
Potential and spin-exchange interaction between Anderson impurities in graphene
Creators: name: Agarwal, M.
name: Mishchenko, E. G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The effective interaction between resonant magnetic Anderson impurities in graphene, mediated by conduction electrons, is studied as a function of the strength of the onsite energy level of the impurities and the amplitude of coupling to conduction electrons. The sign and character of the interaction depend on whether the impurities reside on the same or opposite sublattices. For the same (opposite) sublattice, the potential interaction is attractive (repulsive) in the weak coupling limit with $1/R^3$ dependence on the distance; the interaction reverses sign and becomes repulsive (attractive) in the strong coupling limit and displays $1/R$ behavior. The spin-exchange coupling is ferromagnetic (antiferromagnetic) at both large and small distances, but reverses sign and becomes anti-ferromagnetic (ferromagnetic) for intermediate distances. For opposite sublattices, the effective spin exchange coupling is resonantly enhanced at distances where the energy levels cross the Dirac points.
Sur les paquets d'Arthur des groupes unitaires et quelques conséquences pour les groupes classiques
Creators: name: Moeglin, Colette
name: Renard, David
Publisher: name: arXiv
Year: 2018
Subjects: subject: Representation Theory (math.RT)
subject: FOS: Mathematics
subject: 22E50, 20G05, 11F57

description: We give an explicit construction of Arthur packets for real unitary groups by cohomological and parabolic induction and following an idea communicated to us by P. Trapa, we show that they satisfy the multiplicity one property. In particular, we show the irreducibility of some parabolically induced representations for unitary groups, and use this to give the proof of analogous statements made in our work on Arthur packets of classical groups. Nous donnons une construction explicite des paquets d'Arthur des groupes unitaires réels par induction cohomologique et induction parabolique et en suivant une idée communiquée par P. Trapa, nous établissons la propriété de multiplicité un de ceux-ci. Nous montrons en particulier des résultats d'irréductibilité de certaines induites paraboliques pour les groupes unitaires, ce qui nous permet de compléter les démonstrations d'énoncés analogues annoncés dans nos travaux sur les paquets d'Arthur des groupes classiques.
description: 28 pages, in French