cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Ratios of 15N/12C and 4He/12C inclusive electroproduction cross sections in the nucleon resonance region
Creators: name: CLAS Collaboration
name: Bosted, P. E.
name: Fersch, R.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The (W,Q2)-dependence of the ratio of inclusive electron scattering cross sections for 15N/12C was determined in the kinematic range 0.8
description: 13 pages, 2 figures. Significantly shortened version. Results unchanged. Small additions for Phys. Rev. C
title: Au pied du Mont-Tendre
title: Au pied du Mont-Tendre
titleType: AlternativeTitle
Creators: name: Besson, Adrien
name: Besson, François
Publisher: name: François Besson
Year: 0

description: Volume 1: "la contrée d'Apples suivi de quelques notes sur le village de Pampigny" ; Volume 2: "et... un peu au-delà avec l'histoire véritable du Diable de Mollens" ; Volume 3: sans titre spécifique ; Volume 4: sans titre spécifique. Texte repris en format WORD par François Besson à partir des éditions originales de 1938, 1939 et 1943. Couvertures originales des Editions La Concorde.
Estamos como queremos, o los monstruos en acción
Creators: name: Julio, Cortázar
name: Cortázar, Julio
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: Literatura
Literatura argentina
Política
Boom

description: Notas: Pocas correcciones.
description: Source: Num.Ref. : JC-CAR-21.035
description: Source: Localización del archivo: Centre de Recherches Latino-Américaines (CRLA–Archivos, ITEM UMR8132). MSHS - Bât. A5, 1er étage 5 rue Théodore Lefebvre - TSA21103. 86073 Poitiers cedex 9.
description: Bibliographic citation: Cortázar, Julio, « Julio Cortázar: Estamos como queremos, o los monstruos en acción », Crisis, núm. 11 (Marzo 1974), p. 40-44.
ОРОЛ ДЕНГИЗИ ҚУРИШИ ОҚИБАТЛАРИНИ ЮМШАТИШДА ЖЎХОРИ ЭКИНИНИНГ ЎРНИ
Creators: name: Телляев, Р.Ш.
name: Маматкулов, И.И.
Publisher: name: Zenodo
Year: 2024

description: Мақолада, кўп йиллик тадқиқотлар натижасида глобал иқлим ўзгариши, Орол денгизи қуриши оқибатида, шўрланиш, ҳаво ҳароратини ортиши, мунтазам қурғоқчилик шароитида ушбу ҳолатга бардошли бўлган жўхори-sorgum дон жўхорининг “Массино” нави уруғларни униш даражаси  ўрганилиб, натижда Оролбўйи ҳамда шу ҳолатга яқин бўлган ҳудудларида жўхори экинини экиб, тўлиқ кўчатлар олишга эришишнинг илмий асослари бўйича маълумотлар келтирилган.
Spacetime Dependent Lagrangians and Electrogravity Duality
Creators: name: Gangopadhyay, Debashis
name: Bhattacharyya, R.
name: Singh, L. P.
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We apply the spacetime dependent lagrangian formalism [1] to the action in general relativity. We obtain a Barriola-Vilenkin type monopole solution by exploiting theelectrogravity duality of the vacuum Einstein equations and using a modified definition of empty space. An {\it upper bound} is obtained on the monopole mass ${\tt M}$, ${\tt M}\leq e^{(1-α)/α}/(1-α)^{2}{\tt G}$ where $α= 2k $ is the global monopole charge. Keywords: global monopole, electrogravity duality, holographic principle. PACS: 11.15.-q, 11.27.+d, 14.80.Hv, 04.
description: 4 pages, latex
title: Notice sur la famille Besson et la Maison de Fermens
title: Notice sur la famille Besson et la Maison de Fermens
titleType: AlternativeTitle
Creators: name: Besson, Adrien
name: Besson, François
Publisher: name: François Besson
Year: 0

description: Texte repris en format WORD à partir de l’édition originale de 1949
Electron fractionalization for two-dimensional Dirac fermions
Creators: name: Chamon, Claudio
name: Hou, Chang-Yu
name: Jackiw, Roman
name: Mudry, Christopher
name: Pi, So-Young
name: Semenoff, Gordon
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Fermion-number fractionalization without breaking of time-reversal symmetry was recently demonstrated for a field theory in $(2+1)$-dimensional space and time that describes the couplings between massive Dirac fermions, a complex-valued Higgs field carrying an axial gauge charge of 2, and a U(1) axial gauge field. Charge fractionalization occurs whenever the Higgs field either supports vortices by itself, or when these vortices are accompanied by half-vortices in the axial gauge field. The fractional charge is computed by three different techniques. A formula for the fractional charge is given as a function of a parameter in the Dirac Hamiltonian that breaks the spectral energy-reflection symmetry. In the presence of a charge $\pm1$ vortex in the Higgs field only, the fractional charge varies continuously and thus can take irrational values. The simultaneous presence of a half-vortex in the axial gauge field and a charge $\pm1$ vortex in the Higgs field re-rationalizes the fractional charge to the value 1/2.
description: 18 pages, 2 figures
Stellar populations of galaxies in the ALHAMBRA survey up to $z \sim 1$. III. The stellar content of the quiescent galaxy population during the last $8$ Gyr
Creators: name: Díaz-García, L. A.
name: Cenarro, A. J.
name: López-Sanjuan, C.
name: Ferreras, I.
name: Fernández-Soto, A.
name: Delgado, R. M. González
name: Márquez, I.
name: Masegosa, J.
name: Roman, I. San
name: Viironen, K.
name: Bonoli, S.
name: Cerviño, M.
name: Moles, M.
name: Cristóbal-Hornillos, D.
name: Alfaro, E.
name: Aparicio-Villegas, T.
name: Benítez, N.
name: Broadhurst, T.
name: Cabrera-Caño, J.
name: Castander, F. J.
name: Cepa, J.
name: Husillos, C.
name: Infante, L.
name: Aguerri, J. A. L.
name: Martínez, V. J.
name: Molino, A.
name: del Olmo, A.
name: Perea, J.
name: Prada, F.
name: Quintana, J. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We aim at constraining the stellar population properties of quiescent galaxies. These properties reveal how these galaxies evolved and assembled since $z\sim1$ up to the present time. Combining the ALHAMBRA multi-filter photo-spectra with the SED-fitting code MUFFIT, we build a complete catalogue of quiescent galaxies via the dust-corrected stellar mass vs colour diagram. This catalogue includes stellar population properties, such as age, metallicity, extinction, stellar mass and photometric redshift, retrieved from the analysis of composited populations based on two independent sets of SSP models. We develop and apply a novel methodology to provide, for the first time, the analytic probability distribution functions (PDFs) of mass-weighted age, metallicity, and extinction of quiescent galaxies as a function of redshift and stellar mass. We adopt different star formation histories to discard potential systematics in the analysis. The number density of quiescent galaxies is found to increase since $z\sim1$, with a more substantial variation at lower mass. Quiescent galaxies feature extinction $A_V<0.6$, with median values in the range $A_V = 0.15\mathrm{-}0.3$. At increasing stellar mass, quiescent galaxies are older and more metal rich since $z\sim1$. A detailed analysis of the PDFs reveals that the evolution of quiescent galaxies is not compatible with passive evolution and a slight decrease is hinted at median metallicity $0.1\mathrm{-}0.2$~dex. The intrinsic dispersion of the age and metallicity PDFs show a dependence with stellar mass and/or redshift. These results are consistent with both sets of SSP models and the alternative SFH assumptions explored. Consequently, the quiescent population must undergo an evolutive pathway including mergers and/or remnants of star formation to reconcile the observed trends, where the `progenitor' bias should also be taken into account.
description: 27 pages, 8 figures, 9 tables, accepted for publication in A&A
Additional file 1: of Speech-guided breathing retraining in asthma: a randomised controlled crossover trial in real-life outpatient settings
Creators: name: Bonin, Dietrich Von
name: Klein, Sabine
name: WĂźrker, Jana
name: Streit, Eva
name: Avianus, Oliver
name: Grah, Christian
name: JĂśrg Salomon
name: Wolf, Ursula
Publisher: name: figshare
Year: 2018
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: CONSORT 2010 checklist of information to include when reporting a randomised trial. (PDF 57Â kb)
Precision Calculation of Inflation Correlators at One Loop
Creators: name: Wang, Lian-Tao
name: Xianyu, Zhong-Zhi
name: Zhong, Yi-Ming
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We initiate a systematic study of precision calculation of the inflation correlators at the 1-loop level, starting in this paper with bosonic 1-loop bispectrum with chemical-potential enhancement. Such 1-loop processes could lead to important cosmological collider observables but are notoriously difficult to compute due to the lack of symmetries. We attack the problem from a direct numerical approach based on the real-time Schwinger-Keldysh formalism and show full numerical results for arbitrary kinematics containing both the oscillatory "signals" and the "backgrounds". Our results show that, while the non-oscillatory part can be one to two orders of magnitude larger, the oscillatory signal can be separated out by applying appropriate high-pass filters. We have also compared the result with analytic estimates typically adopted in the literature. While the amplitude is comparable, there is a non-negligible deviation in the frequency of the oscillatory part away from the extreme squeezed limit.
description: 28 pages + appendices and references, 11 figures, 1 table. v2 as published in JHEP
Scaffold hopping for designing of potent and selective CYP1B1 inhibitors to overcome docetaxel resistance: synthesis and evaluation
Creators: name: Raju, Baddipadige
name: Narendra, Gera
name: Verma, Himanshu
name: Kumar, Manoj
name: Sapra, Bharti
name: Kaur, Gurleen
name: Jain, Subheet Kumar
name: Chary, Padakanti Sandeep
name: Mehra, Neelesh Kumar
name: Silakari, Om
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Biochemistry
subject: Space Science
subject: Cell Biology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Cytochrome P450 1B1, a tumor-specific overexpressed enzyme, significantly impairs the pharmacokinetics of several commonly used anticancer drugs including docetaxel, paclitaxel and cisplatin, leading to the problem of resistance to these drugs. Currently, there is no CYP1B1 inhibition-based adjuvant therapy available to treat this resistance problem. Hence, in the current study, exhaustive in-silico studies including scaffold hopping followed by molecular docking, three-dimensional quantitative structure-activity relationships (3D-QSAR), molecular dynamics and free energy perturbation studies were carried out to identify potent and selective CYP1B1 inhibitors. Initially, scaffold hopping analysis was performed against a well-reported potent and selective CYP1B1 inhibitor (i.e. compound 3n). A total of 200 scaffolds were identified along with their shape and field similarity scores. The top three scaffolds were further selected on the basis of these scores and their synthesis feasibility to design some potent and selective CYP1B1 inhibitors using the aforementioned in-silico techniques. Designed molecules were further synthesized to evaluate their CYP1B1 inhibitory activity and docetaxel resistance reversal potential against CYP1B1 overexpressed drug resistance MCF-7 cell line. In-vitro results indicated that compounds 2a, 2c and 2d manifested IC50 values for CYP1B1 ranging from 0.075, 0.092 to 0.088 μM with at least 10-fold selectivity. At low micromolar concentrations, compounds 1e, 1f, 2a and 2d exhibited promising cytotoxic effects in the docetaxel-resistant CYP1B1 overexpressed MCF-7 cell line. In particular, compound 2a is most effective in reversing the resistance with IC50 of 29.0 ± 3.6 μM. All of these discoveries could pave the way for the development of adjuvant therapy capable of overcoming CYP1B1-mediated resistance.
Neutrino Properties with Ground-Based Millimeter-Wavelength Line Intensity Mapping
Creators: name: Dizgah, Azadeh Moradinezhad
name: Keating, Garrett K.
name: Karkare, Kirit S.
name: Crites, Abigail
name: Choudhury, Shouvik Roy
Publisher: name: arXiv
Year: 2021
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Line intensity mapping (LIM) is emerging as a powerful technique to map the cosmic large-scale structure and to probe cosmology over a wide range of redshifts and spatial scales. We perform Fisher forecasts to determine the optimal design of wide-field ground-based mm-wavelength LIM surveys for constraining properties of neutrinos and light relics. We consider measuring the auto-power spectra of several CO rotational lines (from J=2-1 to J=6-5) and the [CII] fine-structure line in the redshift range of $0.25
description: v2 matches the published article, with number of spectrometer-hours in caption of table 3 edited
The Herschel-ATLAS: magnifications and physical sizes of $500\,μ$m-selected strongly lensed galaxies
Creators: name: Enia, A.
name: Negrello, M.
name: Gurwell, M.
name: Dye, S.
name: Rodighiero, G.
name: Massardi, M.
name: De Zotti, G.
name: Franceschini, A.
name: Cooray, A.
name: van der Werf, P.
name: Birkinshaw, M.
name: Michałowski, M. J.
name: Oteo, I.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We perform lens modelling and source reconstruction of Submillimeter Array (SMA) data for a sample of 12 strongly lensed galaxies selected at 500$μ$m in the Herschel Astrophysical Terahertz Large Area Survey H-ATLAS. A previous analysis of the same dataset used a single Sèrsic profile to model the light distribution of each background galaxy. Here we model the source brightness distribution with an adaptive pixel scale scheme, extended to work in the Fourier visibility space of interferometry. We also present new SMA observations for seven other candidate lensed galaxies from the H-ATLAS sample. Our derived lens model parameters are in general consistent with previous findings. However, our estimated magnification factors, ranging from 3 to 10, are lower. The discrepancies are observed in particular where the reconstructed source hints at the presence of multiple knots of emission. We define an effective radius of the reconstructed sources based on the area in the source plane where emission is detected above 5$σ$. We also fit the reconstructed source surface brightness with an elliptical Gaussian model. We derive a median value $r_{eff}\,\sim 1.77\,$kpc and a median Gaussian full width at half maximum $\sim1.47\,$kpc. After correction for magnification, our sources have intrinsic star formation rates SFR$\,\sim900-3500\,M_{\odot}yr^{-1}$, resulting in a median star formation rate surface density $Σ_{SFR}\sim132\,M_{\odot}$ yr$^{-1}$ kpc$^{-2}$ (or $\sim 218\,M_{\odot}$ yr$^{-1}$ kpc$^{-2}$ for the Gaussian fit). This is consistent with what observed for other star forming galaxies at similar redshifts, and is significantly below the Eddington limit for a radiation pressure regulated starburst.
description: 19 pages, 8 figures, accepted for publication in MNRAS
THE RELATIONSHIP BETWEEN ECONOMIC GROWTH AND INTERNATIONAL TRADE
Creators: name: Hodan, Yusuf Ahmed
Publisher: name: Zenodo
Year: 2025
Subjects: RELATIONSHIP BETWEEN ECONOMIC GROWTH
INTERNATIONAL TRADE

description: Abstract

Economic growth and international trade are two important factors that have a significant impact on the development and prosperity of countries. Over the years, there has been a growing interest in understanding and determining the relationship between economic growth and international trade. International trade refers to the exchange of goods and services between different countries, which promotes specialization, competition and economies of scale.
Rigorous derivation of the hydrodynamical equations for rotating superfluids
Creators: name: Liu, Hailiang
name: Sparber, Christof
Publisher: name: arXiv
Year: 2007
Subjects: subject: Analysis of PDEs (math.AP)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 81Q20, 76A25, 35Q55

description: Using a modified WKB approach, we present a rigorous semi-classical analysis for solutions of nonlinear Schroedinger equations with rotational forcing. This yields a rigorous justification for the hydrodynamical system of rotating superfluids. In particular it is shown that global-in-time semi-classical convergence holds whenever the limiting hydrodynamical system has global smooth solutions and we also discuss the semi-classical dynamics of several physical quantities describing rotating superfluids.
description: to appear in Math. Mod. Methods Appl. Sci
MPEC 2024-U99 : 2024 UM2
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 UM2

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Can accelerated expansion of the universe be due to spacetime vorticity?
Creators: name: Mirza, Babur M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present here a general relativistic mechanism for accelerated cosmic expansion and the Hubble's constant. It is shown that spacetime vorticity coupled to the magnetic field density in galaxies causes the galaxies to recede from one another at a rate equal to the Hubble's constant. We therefore predict an oscillatory universe, with zero curvature, without assuming violation of Newtonian gravity at large distances or invoking dark energy/dark matter hypotheses. The value of the Hubble's constant, along with the scale of expansion, as well as the high isotropy of CMB radiation are deduced from the model.
description: To appear in Mod. Phys. Lett. A
Investigation of natural compounds as methyltransferase inhibitors against dengue virus: an in silico approach
Creators: name: Imran, Mohd
name: Abida
name: Alotaibi, Nawaf M.
name: Thabet, Hamdy Khamees
name: Alruwaili, Jamal Alhameedi
name: Eltaib, Lina
name: Alshehri, Ahmed
name: Kamal, Mehnaz
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences

description: The global challenge posed by Dengue virus (DENV) infection persists, exacerbated by the absence of specific antiviral therapies. The viral methyltransferase (MTase) enzyme, crucial for viral RNA methylation and immune system evasion, has emerged as a promising drug target for combating Dengue fever. In this study, a comprehensive exploration of natural compounds derived from the COCONUT database was conducted, selecting 224 compounds based on their structural similarity to the native substrate of the MTase enzyme, S-adenosyl-L-methionine (SAM). Employing virtual screening techniques, four natural compounds (CNP0307160, CNP0082902, CNP0449158, and CNP0296775) with acceptable docking scores were selected for further re-docking after geometry optimization by the DFT method. Re-docking analyses unveiled significant interactions, including hydrogen bonds and hydrophobic interactions, between these selected ligands and the MTase protein. To gain deeper insights into the dynamic stability of these complexes, we conducted molecular dynamics simulations which showed lower RMSD values for CNP0307160, CNP0082902, and CNP0296775 when compared to the reference molecule. Furthermore, we assessed the structural and dynamic stability of the protein-ligand complexes through free binding energy calculations and Principal Component Analysis (PCA) of the simulation trajectories. In these analyses, the CNP0296775 compound exhibited promising results compared to the other three compounds. The cumulative findings of these investigations underscore the potential of CNP0296775 as a strong inhibitor of DENV MTase, thus offering a promising starting point for its further experimental validation and optimization.
title: Ultraluminous X-ray source 1E 0953.8+6918 (M81 X-9): an intermediate-mass black hole candidate and its environs
Creators: name: Wang, QD
Publisher: name: University of Massachusetts Amherst
Year: 2002
Subjects: subject: * binaries: general; * ISM: bubbles; * galaxies: individual: M81; * X-rays: galaxies
subject: Astrophysics and Astronomy

description: This is the pre-published version harvested from ArXiv. The published version is located at http://onlinelibrary.wiley.com/doi/10.1046/j.1365-8711.2002.05317.x/abstract
description: We present a ROSAT and ASCA study of the Einstein source X-9 and its relation to a shock-heated shell-like optical nebula in a tidal arm of the M81 group of interacting galaxies. Our ASCA observation of the source shows a flat and featureless X-ray spectrum well described by a multicolour disc blackbody model. The source most likely represents an optically thick accretion disc around an intermediate-mass black hole (M∼102 M⊙) in its high/soft state, similar to other variable ultraluminous X-ray sources observed in nearby disc galaxies. Using constraints derived from both the innermost stable orbit around a black hole and the Eddington luminosity, we find that the black hole is fast-rotating and that its mass is between ∼80 M⊙–1.5×102 M⊙. The inferred bolometric luminosity of the accretion disc is ∼(1.1×1040 erg s−1)/(cos i). Furthermore, we find that the optical nebula is very energetic and may contain large amounts of hot gas, accounting for a soft X-ray component as indicated by archival ROSAT PSPC data. The nebula is apparently associated with X-9; the latter may be powering the former and/or they could be formed in the same event (e.g. a hypernova). Such a connection, if confirmed, could have strong implications for understanding both the birth of intermediate-mass black holes and the formation of energetic interstellar structures.
A polynomial oracle-time algorithm for convex integer minimization
Creators: name: Hemmecke, Raymond
name: Onn, Shmuel
name: Weismantel, Robert
Publisher: name: arXiv
Year: 2007
Subjects: subject: Optimization and Control (math.OC)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 90C05; 90C10; 90C15; 90C20; 90C25; 90C30

description: In this paper we consider the solution of certain convex integer minimization problems via greedy augmentation procedures. We show that a greedy augmentation procedure that employs only directions from certain Graver bases needs only polynomially many augmentation steps to solve the given problem. We extend these results to convex $N$-fold integer minimization problems and to convex 2-stage stochastic integer minimization problems. Finally, we present some applications of convex $N$-fold integer minimization problems for which our approach provides polynomial time solution algorithms.
description: 19 pages, 1 figure
Additional file 3: of The impact of telehealth remote patient monitoring on glycemic control in type 2 diabetes: a systematic review and meta-analysis of systematic reviews of randomised controlled trials
Creators: name: Puikwan Lee
name: Greenfield, Geva
name: Pappas, Yannis
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Excluded references. (DOCX 119 kb)
Dip-coating of bidisperse particulate suspensions
Creators: name: Jeong, Deok-Hoon
name: Lee, Michael Ka Ho
name: Thiévenaz, Virgile
name: Bazant, Martin Z.
name: Sauret, A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Dip-coating consists in withdrawing a substrate from a bath to coat it with a thin liquid layer. This process is well-understood for homogeneous fluids, but heterogeneities such as particles dispersed in the liquid lead to more complex situations. Indeed, particles introduce a new length scale, their size, in addition to the thickness of the coating film. Recent studies have shown that at first order, the thickness of the coating film for monodisperse particles can be captured by an effective capillary number based on the viscosity of the suspension, providing that the film is thicker than the particle diameter. However, suspensions involved in most practical applications are polydisperse, characterized by a wide range of particle sizes, introducing additional length scales. In this study, we investigate the dip coating of suspensions having a bimodal size distribution of particles. We show that the effective viscosity approach is still valid in the regime where the coating film is thicker than the diameter of the largest particles, although bidisperse suspensions are less viscous than monodisperse suspensions of the same solid fraction. We also characterize the intermediate regime that consists of a heterogeneous coating layer and where the composition of the film is different from the composition of the bath. A model to predict the probability of entraining the particles in the liquid film depending on their sizes is proposed and captures our measurements. In this regime, corresponding to a specific range of withdrawal velocities, capillarity filters the large particles out of the film.
Measurement of the Proton Asymmetry Parameter C in Neutron Beta Decay
Creators: name: Schumann, M.
name: Kreuz, M.
name: Deissenroth, M.
name: Glueck, F.
name: Krempel, J.
name: Maerkisch, B.
name: Mund, D.
name: Petoukhov, A.
name: Soldner, T.
name: Abele, H.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The proton asymmetry parameter C in neutron decay describes the correlation between neutron spin and proton momentum. In this Letter, the first measurement of this quantity is presented. The result C=-0.2377(26) agrees with the Standard Model expectation. The coefficient C provides an additional parameter for new and improved Standard Model tests. From a differential analysis of the same data (assuming the Standard Model), we obtain lambda=-1.275(16) as ratio of axial-vector and vector coupling constant.
description: 4 pages, 2 figures
Orthogonality for Quantum Latin Isometry Squares
Creators: name: Musto, Benjamin
name: Vicary, Jamie
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Goyeneche et al recently proposed a notion of orthogonality for quantum Latin squares, and showed that orthogonal quantum Latin squares yield quantum codes. We give a simplified characterization of orthogonality for quantum Latin squares, which we show is equivalent to the existing notion. We use this simplified characterization to give an upper bound for the number of mutually orthogonal quantum Latin squares of a given size, and to give the first examples of orthogonal quantum Latin squares that do not arise from ordinary Latin squares. We then discuss quantum Latin isometry squares, generalizations of quantum Latin squares recently introduced by Benoist and Nechita, and define a new orthogonality property for these objects, showing that it also allows the construction of quantum codes. We give a new characterization of unitary error bases using these structures.
description: In Proceedings QPL 2018, arXiv:1901.09476
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0749
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: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0749, 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. 0749, 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
Unveiling fructose and glucose binding to human serum albumin: fluorescence measurements and docking, molecular dynamics and quantum biochemistry computations
Creators: name: Hadad, André
name: França, Victor L. B.
name: Crisostomo, Marcos William
name: Brunaldi, Kellen
name: Carvalho, Hernandes F.
name: Freire, Valder N.
Publisher: name: Taylor & Francis
Year: 2024
Subjects: Biophysics
Biochemistry
Physical Sciences not elsewhere classified
Medicine
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Computational Biology

description: This research examines the interaction between human serum albumin (HSA) and various sugar forms (β-D-fructofuranose (FRC), α-D-glucopyranose (GLC), Keto-D-fructose (FRO), Aldehydo-D-glucose (GLO), and modified Aldehydo-D-glucose (GLOm)) using fluorescent spectroscopy, molecular docking simulations, molecular dynamics, protein conformational clusters (EnGens), molecular fractionation with conjugate caps (MFCC) and quantum biochemistry analysis. We analyze molecular and quantum aspects, uncovering interaction energies between sugar atoms and amino acids. Total interaction energy considers protein fragmentation, energetic decomposition, and interaction energy from a bottom-up perspective. Molecular dynamics reveal that unmodified Aldehydo-D-glucose (GLO) escapes HSA binding sites, explaining gradual glycation. We pioneer studying HSA’s binding mechanism with glucose and fructose in a 1:1 ratio using long molecular dynamics simulations. Results suggest the transitional GLOm form has a higher Sudlow I site propensity than unmodified glucose, crucial for K195 glycation. FRO and GLOm interaction tendencies move toward a deeper FA7 cavity, near its center. This approach effectively elucidates small molecule binding mechanisms, consistent with previous experimental results.
On the role of density fluctuations in the core turbulent transport of Wendelstein 7-X
Creators: name: Carralero, D.
name: Estrada, T.
name: Maragkoudakis, E.
name: Windisch, T.
name: Alonso, J. A.
name: Velasco, J. L.
name: Ford, O.
name: Jakubowski, M.
name: Lazerson, S.
name: Beurskens, M.
name: Bozhenkov, S.
name: Calvo, I.
name: Damm, H.
name: Fuchert, G.
name: García-Regaña, J. M.
name: Höfel, U.
name: Marushchenko, N.
name: Pablant, N.
name: Sánchez, E.
name: Smith, H. M.
name: Pasch, E.
name: Stange, T.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: A recent characterization of core turbulence carried out with a Doppler reflectometer in the optimized stellarator Wendelstein 7-X (W7-X) found that discharges achieving high ion temperatures at the core featured an ITG-like suppression of density fluctuations driven by a reduction of the gradient ratio $η_i = L_n/L_{T_i}$ [D. Carralero et al., Nucl. Fusion, 2021]. In order to confirm the role of ITG turbulence in this process, we set out to establish experimentally the relation between core density fluctuations, turbulent heat flux and global confinement. With this aim, we consider the scenarios found in the previous work and carry out power balance analysis for a number of representative ones, including some featuring high ion temperature. As well, we evaluate the global energy confinement time and discuss it in the context of the ISS04 inter-stellarator scaling. We find that, when turbulence is suppressed as a result of a reduction of $η_i$, there is a reduction of ion turbulent transport, and global performance is improved as a result. This is consistent with ITG turbulence limiting the ion temperature at the core of W7-X. In contrast, when turbulence is reduced following a decrease in collisionality, no changes are observed in transport or confinement. This could be explained by ITG modes being combined with TEM turbulence when the later is destabilized at low collisionalities.
description: Submitted to PPCF, 47th EPS special issue
IMPROPER DIET CAUSES DISEASE.
Creators: name: Alimova, Dilrabo
name: Panjieva, O`gilshad
Publisher: name: Zenodo
Year: 2024

description: Eating is the basic biological need of life. Food, in turn, provides the energy necessary for the development and regulation of metabolism of the organism, ensures the growth and proper formation of the organism, and health maintenance. Food products should be useful, diverse, nutritious and quantitatively optimal.
The model of interacting spatial permutations and its relation to the Bose gas
Creators: name: Ueltschi, Daniel
Publisher: name: arXiv
Year: 2007
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The model of spatial permutations is related to the Feynman-Kac representation of the Bose gas. The transition to infinite cycles corresponds to Bose-Einstein condensation. We review the general setting and some results, and we derive a multi-body interaction between permutation jumps, that is due to the original interactions between quantum particles.
description: 14 pages
Understanding Type Ia supernovae through their U-band spectra
Creators: name: Nordin, J.
name: Aldering, G.
name: Antilogus, P.
name: Aragon, C.
name: Bailey, S.
name: Baltay, C.
name: Barbary, K.
name: Bongard, S.
name: Boone, K.
name: Brinnel, V.
name: Buton, C.
name: Childress, M.
name: Chotard, N.
name: Copin, Y.
name: Dixon, S.
name: Fagrelius, P.
name: Feindt, U.
name: Fouchez, D.
name: Gangler, E.
name: Hayden, B.
name: Hillebrandt, W.
name: Kim, A.
name: Kowalski, M.
name: Kuesters, D.
name: Leget, P. -F.
name: Lombardo, S.
name: Lin, Q.
name: Pain, R.
name: Pecontal, E.
name: Pereira, R.
name: Perlmutter, S.
name: Rabinowitz, D.
name: Rigault, M.
name: Runge, K.
name: Rubin, D.
name: Saunders, C.
name: Smadja, G.
name: Sofiatti, C.
name: Suzuki, N.
name: Taubenberger, S.
name: Tao, C.
name: Thomas, R. C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. Observations of Type Ia supernovae (SNe Ia) can be used to derive accurate cosmological distances through empirical standardization techniques. Despite this success neither the progenitors of SNe Ia nor the explosion process are fully understood. The U-band region has been less well observed for nearby SNe, due to technical challenges, but is the most readily accessible band for high-redshift SNe. Aims. Using spectrophotometry from the Nearby Supernova Factory, we study the origin and extent of U-band spectroscopic variations in SNe Ia and explore consequences for their standardization and the potential for providing new insights into the explosion process. Methods. We divide the U-band spectrum into four wavelength regions λ(uNi), λ(uTi), λ(uSi) and λ(uCa). Two of these span the Ca H&K λλ 3934, 3969 complex. We employ spectral synthesis using SYNAPPS to associate the two bluer regions with Ni/Co and Ti. Results. (1) The flux of the uTi feature is an extremely sensitive temperature/luminosity indicator, standardizing the SN peak luminosity to 0.116 $\pm$ 0.011 mag RMS. A traditional SALT2.4 fit on the same sample yields a 0.135 mag RMS. Standardization using uTi also reduces the difference in corrected magnitude between SNe originating from different host galaxy environments. (2) Early U-band spectra can be used to probe the Ni+Co distribution in the ejecta, thus offering a rare window into the source of lightcurve power. (3) The uCa flux further improves standardization, yielding a 0.086 $\pm$ 0.010 mag RMS without the need to include an additional intrinsic dispersion to reach χ$^2$/dof $\sim$ 1. This reduction in RMS is partially driven by an improved standardization of Shallow Silicon and 91T-like SNe.
description: 19 pages, 17 figures, accepted for publication in A&A
Lettre de Johann Caspar Hagenbuch à Scipione Maffei, 1747-11
Creators: name: Hagenbuch, Johann Caspar
name: Hagenbuch, Johann Caspar
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2022

description: [lettre en latin]
description: Source: [établissement de conservation] Nîmes, Bibliothèque Carré d'Art [cote] ms. 143, fol. 327-328
description: created: 1747-11-00
X-ray Irradiation-induced Carrier Doping Effects in Organic Dimer-Mott Insulators
Creators: name: Sasaki, T.
name: Oizumi, H.
name: Yoneyama, N.
name: Kobayashi, N.
name: Toyota, N.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We report X-ray irradiation-induced carrier doping effects on the electrical conductivity in the organic dimer-Mott insulators $κ$-(ET)$_{2}$$X$ with $X =$ Cu[N(CN)$_{2}$]Cl and Cu$_{2}$(CN)$_{3}$. For $κ$-(ET)$_{2}$Cu[N(CN)$_{2}$]Cl, we have observed a large decrease of the resistivity by 40 % with the irradiation at 300 K and the metal-like temperature dependence down to about 50 K. The irradiation-induced defects expected at the donor molecule sites might cause a local imbalance of the charge transfer in the crystal. Such molecular defects result in the effective doping of carriers into the half-filled dimer-Mott insulators.
description: 4 pages, 3 figures
Inadequacy of Modal Logic in Quantum Settings
Creators: name: Nurgalieva, Nuriya
name: del Rio, Lídia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Logic in Computer Science (cs.LO)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We test the principles of classical modal logic in fully quantum settings. Modal logic models our reasoning in multi-agent problems, and allows us to solve puzzles like the muddy children paradox. The Frauchiger-Renner thought experiment highlighted fundamental problems in applying classical reasoning when quantum agents are involved; we take it as a guiding example to test the axioms of classical modal logic. In doing so, we find a problem in the original formulation of the Frauchiger-Renner theorem: a missing assumption about unitarity of evolution is necessary to derive a contradiction and prove the theorem. Adding this assumption clarifies how different interpretations of quantum theory fit in, i.e., which properties they violate. Finally, we show how most of the axioms of classical modal logic break down in quantum settings, and attempt to generalize them. Namely, we introduce constructions of trust and context, which highlight the importance of an exact structure of trust relations between agents. We propose a challenge to the community: to find conditions for the validity of trust relations, strong enough to exorcise the paradox and weak enough to still recover classical logic.
description: In Proceedings QPL 2018, arXiv:1901.09476
Additional file 2: of Status of nutrients important in brain function in phenylketonuria: a systematic review and meta-analysis
Creators: name: Parra, Gina Montoya
name: Singh, Rani
name: Cetinyurek-Yavuz, Aysun
name: Kuhn, Mirjam
name: MacDonald, Anita
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Developmental Biology

description: Vitamin A levels in PKU patients versus healthy controls. Vitamin A levels in PKU patients versus healthy controls. Abbreviations: LCL, lower confidence limit; REML, restricted maximum likelihood; SD, standard deviation; SMD, standardized mean difference; UCL, upper confidence limit (PDF 271 kb).
Is $Z_{cs}(3982)$ a molecular partner of $Z_c(3900)$ and $Z_c(4020)$ states?
Creators: name: Baru, V.
name: Epelbaum, E.
name: Filin, A. A.
name: Hanhart, C.
name: Nefediev, A. V.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Lattice (hep-lat)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We perform an effective-field-theory-based coupled-channel analysis of the recent BES III data on the $e^+e^-$ annihilation into the final state $K^+(D_s^-D^{*0}+D_s^{*-}D^0)$ in a wide energy range and extract the poles responsible for the formation of the $Z_{cs}(3982)$. We identify two scenarios which provide a similar description of the experimental mass distributions but result in utterly different predictions for the spin partners of the $Z_{cs}(3982)$: although both scenarios are consistent with the $Z_{cs}$ as a $SU(3)$ partner of the $Z_c(3900)$, the $Z_c(4020)$ appears naturally as a spin partner of these states only in one of them (fit 1) while in the other (fit 2) its nature has to be different. Also, the $Z_{cs}(3982)$ has a $J^{P}=1^+$ spin partner near the $\bar D_s^* D^*$ threshold in fit 1, while no such state exists in fit 2. We predict the $\bar{D}_s^*D^*$ invariant mass distribution in the $J^{P}=1^+$ channel for the reaction $e^+e^-\to K^+D_s^{*-}D^{*0}$ and argue that this line shape can be used to distinguish between the two scenarios once data in this channel are available.
description: 21 pages, 6 figures, 4 tables
Nonlinear Phenomena in Canonical Stochastic Quantization
Creators: name: Huffel, Helmuth
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Stochastic quantization provides a connection between quantum field theory and statistical mechanics, with applications especially in gauge field theories. Euclidean quantum field theory is viewed as the equilibrium limit of a statistical system coupled to a thermal reservoir. Nonlinear phenomena in stochastic quantization arise when employing nonlinear Brownian motion as an underlying stochastic process. We discuss a novel formulation of the Higgs mechanism in QED.
description: 8 pages, invited talk at the International Workshop ``Critical Phenomena and Diffusion in Complex Systems'', Dec. 5-7, 2006, Nizhni Novgorod, Russia
The Ando-Hiai inequalities for the solution of the generalized Karcher equation and related results
Creators: name: Yamazaki, Takeaki
Publisher: name: arXiv
Year: 2018
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 47A63, 47A64

description: In this paper, we shall give a concrete relation between the generalized Karcher equation and operator means as its solution. Next, we shall show two types of the Ando-Hiai inequalities for the solution of the generalized Karcher equation. In this discussion, we also give a property of relative operator entropy.
description: 16 pages
title: Type Ia supernova-driven Galactic bulge wind
Creators: name: Tang, S
name: Wang, QD
name: Low, M-MM
name: Joung, MR
Publisher: name: University of Massachusetts Amherst
Year: 2009
Subjects: subject: * hydrodynamics; * ISM: abundances; * ISM: kinematics and dynamics; * ISM: structure; * supernova remnants; * Galaxy: bulge
subject: Astrophysics and Astronomy

description: This is the pre-published version harvested from ArXiv. The published version is located at http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2009.15206.x/abstract
description: Stellar feedback in Galactic bulges plays an essential role in shaping the evolution of galaxies. To quantify this role and facilitate comparisons with X-ray observations, we conduct three-dimensional hydrodynamical simulations with the adaptive mesh refinement code, flash, to investigate the physical properties of hot gas inside a Galactic bulge, similar to that of our Galaxy or M 31. We assume that the dynamical and thermal properties of the hot gas are dominated by mechanical energy input from supernovae (SNe), primarily type Ia, and mass injection from evolved stars as well as iron enrichment from SNe. We study the bulge-wide outflow as well as the SN heating on scales down to ∼4 pc. An embedding scheme that is devised to plant individual supernova remnant (SNR) seeds allows examining, for the first time, the effect of sporadic SNe on the density, temperature and iron ejecta distribution of the hot gas as well as the resultant X-ray morphology and spectrum. We find that the SNe produce a bulge wind with highly filamentary density structures and patchy ejecta. Compared with a one-dimensional (1D) spherical wind model, the non-uniformity of simulated gas density, temperature and metallicity substantially alters the spectral shape and increases the diffuse X-ray luminosity. The differential emission measure as a function of temperature of the simulated gas exhibits a lognormal distribution, with a peak value much lower than that of the corresponding 1D model. The X-ray luminosity depends sensitively on the mass-loss rate from evolved stars. The bulk of the X-ray emission comes from the relatively low-temperature and low-abundance gas shells associated with SN blastwaves. SN ejecta are not well mixed with the ambient medium, at least in the bulge region. These results, at least partly, account for the apparent lack of evidence for iron enrichment in the soft X-ray-emitting gas in Galactic bulges and intermediate-mass elliptical galaxies. The bulge wind helps to explain the ‘missing’ stellar feedback in such galaxies. But the resultant diffuse emission is more than one order of magnitude less than that observed in the Galactic and M 31 bulges, indicating that gas in these bulges is in a subsonic outflow state probably due to additional mass loading to the hot gas and/or due to energy input rate that is substantially lower than the current estimate.