cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Collective Dipole Oscillations in Atomic Nuclei and Small Metal Particles
Creators: name: Bhalerao, R. S.
name: Barma, M.
Publisher: name: arXiv
Year: 1993
Subjects: subject: Nuclear Theory (nucl-th)
subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: (The systematics of photon absorption cross sections in nuclei and small metal particles are examined as a function of the number of constituent fermions $A$. It is pointed out that the shell-structure-linked oscillations in the full width at half maximum (FWHM) of the photoneutron cross section in nuclei, earlier recognized for $A > 63$, in fact persist down to the lightest nuclei. Averaging over the oscillations or focusing on the lower envelope of the oscillating curve (magic nuclei), the FWHM is seen to generally decrease with increasing $A$, consistent with $A^{-1/3}$, a dependence which was earlier known to hold in metal particle systems. If the FWHMs are scaled by the respective Fermi energies and the inverse radii by the Fermi wave vectors, the two data sets become comparable in magnitude. A schematic theoretical description of the systematics is presented.)
description: 21 pages, 2 figs. (not included), TIFR/TH/92-47
Plakkaten classificeren met de computer?
Creators: name: Romein, Christel Annemieke
Publisher: name: Zenodo
Year: 2019
Subjects: digital scholarship
KB Lab
Digital Humanities
Computational linguistics
Entangled Histories
Police Ordinances

description: Researcher-in-residence Annemieke Romein is op zoek naar vroegmoderne regelgeving in plakkaatboeken (±1500-1800): regels tegen bijvoorbeeld bedelaars, over veiligheid, en ter stimulering van de economie. Met KB-collega’s onderzoekt zij of, en zo ja, hoe een computerprogramma dit werk kan overnemen. Kan een computer teksten herkennen die regelgeving bevatten, en onderscheid maken tussen regelgeving rond religie, dijkwezen etc.?
description: {"references": ["https://www.kb.nl/blogs/digitale-geesteswetenschappen/plakkaten-classificeren-met-de-computer"]}
Influence of augmented humans in online interactions during voting events
Creators: name: Stella, Massimo
name: Cristoforetti, Marco
name: De Domenico, Manlio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Computers and Society (cs.CY)
subject: Social and Information Networks (cs.SI)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: The advent of the digital era provided a fertile ground for the development of virtual societies, complex systems influencing real-world dynamics. Understanding online human behavior and its relevance beyond the digital boundaries is still an open challenge. Here we show that online social interactions during a massive voting event can be used to build an accurate map of real-world political parties and electoral ranks. We provide evidence that information flow and collective attention are often driven by a special class of highly influential users, that we name "augmented humans", who exploit thousands of automated agents, also known as bots, for enhancing their online influence. We show that augmented humans generate deep information cascades, to the same extent of news media and other broadcasters, while they uniformly infiltrate across the full range of identified groups. Digital augmentation represents the cyber-physical counterpart of the human desire to acquire power within social systems.
description: 11 pages
Additional file 3: of Mutant p53 gain of function induces HER2 over-expression in cancer cells
Creators: name: A. Román-Rosales
name: E. García-Villa
name: L. Herrera
name: P. Gariglio
name: J. Díaz-Chávez
Publisher: name: figshare
Year: 2018
Subjects: Biochemistry
Cell Biology
Molecular Biology
Cancer
Hematology

description: Figure S1. Wild-type p53 expression inversely correlates with HER2 mRNA levels. HeLa (A) and Saos-2 (B) cell lines were transiently transfected with wtp53, while MCF-7 cell line (C) was transiently transfected with shp53, as indicated in Materials and Methods. Cells were processed to determine HER2 mRNA levels by RT-qPCR. These experiments were performed by triplicate and data are shown as the mean ± SEM. Statistical analysis was performed with t-student test by comparing the results obtained in: wtp53 vs empty vector transfected HeLa and Saos-2 cells; or shp53 vs scramble transfected MCF-7 cells: * p
String Motion in Fivebrane Geometry
Creators: name: Khuri, Ramzi R.
name: La, HoSeong
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The classical motion of a test string in the transverse space of two types of heterotic fivebrane sources is fully analyzed, for arbitrary instanton scale size. The singular case is treated as a special case and does not arise in the continuous limit of zero instanton size. We find that the orbits are either circular or open, which is a solitonic analogy with the motion of an electron around a magnetic monopole, although the system we consider is quantitatively different. We emphasize that at long distance this geometry does not satisfy the inverse square law, but satisfies the inverse cubic law. If the fivebrane exists in nature and this structure survives after any proper compactification, this last result can be used to test classical ``stringy'' effects.
description: 17 pages
Rotation and Macroturbulence in Metal-poor Field Red Giant and Red Horizontal Branch Stars
Creators: name: Carney, Bruce W.
name: Gray, David F.
name: Yong, David
name: Latham, David W.
name: Manset, N.
name: Zelman, R.
name: Laird, John B.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results for rotational velocities, Vrot sin i, and macroturbulence dispersion, zeta(RT), for 12 metal-poor field red giant branch stars and 7 metal-poor field red horizontal branch stars. The results are based on Fourier transform analyses of absorption line profiles from high-resolution (R ~ 120,000), high-S/N (~ 215 per pixel) spectra obtained with the Gecko spectrograph at CFHT. We find that the zeta(RT) values for the metal-poor RGB stars are very similar to those for metal-rich disk giants studied earlier by Gray and his collaborators. Six of the RGB stars have small rotational values, less than 2.0 km/sec, while five show significant rotation, over 3 km/sec. The fraction of rapidly rotating RHB stars is somewhat lower than found among BHB stars. We devise two empirical methods to translate the line-broadening results obtained by Carney et al. (2003, 2008) into Vrot sin i for all the RGB and RHB stars they studied. Binning the RGB stars by luminosity, we find that most metal-poor field RGB stars show no detectable sign, on average, of rotation. However, the most luminous stars, with M(V) <= -1.5, do show net rotation, with mean values of 2 to 4 km/sec, depending on the algorithm employed, and these stars also show signs of radial velocity jitter and mass loss.
description: accepted for publication in the Astronomical Journal
Cubes3D: Neural Network based Optical Flow in Omnidirectional Image Scenes
Creators: name: Apitzsch, André
name: Seidel, Roman
name: Hirtz, Gangolf
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Optical flow estimation with convolutional neural networks (CNNs) has recently solved various tasks of computer vision successfully. In this paper we adapt a state-of-the-art approach for optical flow estimation to omnidirectional images. We investigate CNN architectures to determine high motion variations caused by the geometry of fish-eye images. Further we determine the qualitative influence of texture on the non-rigid object to the motion vectors. For evaluation of the results we create ground truth motion fields synthetically. The ground truth contains cubes with static background. We test variations of pre-trained FlowNet 2.0 architectures by indicating common error metrics. We generate competitive results for the motion of the foreground with inhomogeneous texture on the moving object.
description: ICPRAI 2018
Evaluating the isolation effect of the soil-rubber mixture (SRM) around buried pipes during ground vibrations
Creators: name: Izadifar, MohammadAli
name: Mousavi, Hossein
name: Zadehmohamad, Mehdi
name: Hosseini, Seyed Majdeddin Mir Mohammad
Publisher: name: figshare
Year: 2021
Subjects: subject: 90501 Civil Geotechnical Engineering
subject: FOS: Civil engineering

description: Lifelines and buried pipeline systems in seismic areas should be designed to resist dynamic and static loads and provide safety and serviceability, especially during ground vibrations. Taking advantage of recycled material such as crumb rubber in the material around the pipe for optimizing the buried pipe system behavior could be an appropriate method if it would improve the performance of the buried pipelines under critical situations. The current study evaluates the effect of using soil-rubber mixture (SRM) around the buried pipes to absorb the vibration energy, protect the pipe, and reduce pipes' deformation. Results represent that the optimum dimension of area for using SRM around the pipe, which will reduce the pipe deformation and simultaneously makes the design economical, is a square by the dimension of three times the diameter of a circular pipe, through which the pipe is placed in the middle. Moreover, the results have shown that SRM is more effective in pipe protection and reducing pipe deformation than the other parameters.
Terrestrial planet formation during giant planet formation and giant planet migration I: The first 5 million years
Creators: name: Brasser, R.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Terrestrial planet formation (TPF) is a difficult problem that has vexed researchers for decades. Numerical models are only partially successful at reproducing the orbital architecture of the inner planets, but have generally not considered the effect of the growth of the giant planets. I dynamically model TPF as the gas giants Jupiter and Saturn are growing using GENGA. The evolution of the masses, radii and orbital elements of the gas giants are precomputed and read and interpolated within GENGA. The terrestrial planets are formed by planetesimal accretion from tens of thousands of self-gravitating planetesimals spread between 0.5 au and 8.5 au. The total mass of the inner planetesimal disc and outer disc are typically 2 and 3 Earth masses respectively, and the composition of the planetesimals changes from non-carbonaceous-like to carbonaceous-like at a prescribed distance, ranging from 2 au to 5 au. After 5 Myr of evolution approximately 10% to 25% of the mass of planetesimals in the Jupiter-Saturn region is implanted in the inner solar system, which is more than what cosmochemical models predict. The implantation initially sets up a composition gradient in the inner solar system, with the fraction of outer solar system material increasing with increasing distance to the Sun. The planetesimals that remain in the inner solar system have a mixed composition. The growth of the gas giants scatters planetesimals in their vicinity into the inner solar system, which changes the isotopic composition of the terrestrial planets. The planetesimal disc in the vicinity of the gas giants may not have been very massive, ~1 ME. The inner planetesimal disc may not have extended much farther than 2 au otherwise embryos do not grow fast enough to produce Mars analogues. This could mean that the region of the current asteroid belt never contained much mass to begin with.
description: Submitted to Astronomy and Astrophysics; changes are expected
Angular two-point correlation functions for cosmological gamma-ray burst model
Creators: name: Kobayashi, Shiho
name: Sasaki, Shin
name: Suto, Yasushi
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compute the angular two-point correlation functions of the gamma-ray bursts at cosmological distances. Since the gamma-ray burst emission mechanism is not yet established, we simply assume that the gamma-ray burst sources are associated with high-redshift galaxies in some way. Then on the basis of several simple models for the evolution of galaxy spatial correlations, we calculate the amplitude of angular two-point correlation functions on scales appropriate for the Compton Gamma Ray Observatory data. we find that in most cases the predicted correlations are difficult to detect with the current data rate and the angular resolution, but models in which the bursts preferentially occur at relatively low redshift ($z \simlt 0.5$) predict correlation amplitudes on $θ\sim 5^\circ$ which will be marginally detectable with the Gamma Ray Observatory data in several years. If future observations detect a signal of angular correlations, it will imply useful information on the correlation of galaxies at high redshifts provided that the gamma-ray bursts are cosmological.
description: 16 pages
Additional file 3: of Stable isotope informed genome-resolved metagenomics reveals that Saccharibacteria utilize microbially-processed plant-derived carbon
Creators: name: Starr, Evan
name: Shengjing Shi
name: Blazewicz, Steven
name: Probst, Alexander
name: Herman, Donald
name: Firestone, Mary
name: Banfield, Jillian
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Figure S1. Plot of GC skew (black) and cumulative GC skew (green, window 1000 bp, slide of 10 bp) of the T. rhizospherense genome. The plot shows the predicted locations of the origin (red line, 1201 bp) and terminus (blue line, 757,370 bp) of replication. The form of the plot is as expected for a correctly assembled, circularized genome that undergoes bi-directional replication from a single origin. (PDF 69 kb)
Duality-Invariant Gaugino Condensation and One-Loop Corrected Kahler Potentials in String Theory
Creators: name: Lüst, Dieter
name: Muñoz, Carlos
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The duality-invariant gaugino condensation with or without massive matter fields is re-analysed, taking into account the dependence of the string threshold corrections on the moduli fields and recent results concerning one-loop corrected Kähler potentials. The scalar potential of the theory for a generic superpotential is also calculated.
description: 18 pages
Coarse-Grained Simulation of DNA using LAMMPS
Creators: name: Henrich, Oliver
name: Gutierrez-Fosado, Yair Augusto
name: Curk, Tine
name: Ouldridge, Thomas E.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Biological Physics (physics.bio-ph)
subject: Computational Physics (physics.comp-ph)
subject: Biomolecules (q-bio.BM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: During the last decade coarse-grained nucleotide models have emerged that allow us to DNA and RNA on unprecedented time and length scales. Among them is oxDNA, a coarse-grained, sequence-specific model that captures the hybridisation transition of DNA and many structural properties of single- and double-stranded DNA. oxDNA was previously only available as standalone software, but has now been implemented into the popular LAMMPS molecular dynamics code. This article describes the new implementation and analyses its parallel performance. Practical applications are presented that focus on single-stranded DNA, an area of research which has been so far under-investigated. The LAMMPS implementation of oxDNA lowers the entry barrier for using the oxDNA model significantly, facilitates future code development and interfacing with existing LAMMPS functionality as well as other coarse-grained and atomistic DNA models.
description: 16 pages, 13 figures, EPJE topical issue on Advances in Computational Methods for Soft Matter Systems
ROSAT Observations of the Flare Star CC Eri
Creators: name: Pan, H. C.
name: Jordan, C.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The flare/spotted spectroscopic binary star CC Eri was observed with the Position Sensitive Proportional Counter (PSPC) on the X-ray satellite ROSAT on 1990 July 9-11 and 1992 January 26-27. During the observations, the source was variable on time scales from a few minutes to several hours, with the X-ray (0.2-2 keV) luminosity in the range $\sim 2.5-6.8\times 10^{29} erg s^{-1}$. An X-ray flare-like event, which has a one hour characteristic rise time and a two hour decay time, was observed from CC Eri on 1990 July 10 16:14-21:34 (UT). The X-ray spectrum of the source can be described by current thermal plasma codes with two temperature components or with a continuous temperature distribution. The spectral results show that plasma at $Te\sim 10^{7}$ K exists in the corona of CC Eri. The variations in the observed source flux and spectra can be reproduced by a flare, adopting a magnetic reconnection model. Comparisons with an unheated model, late in the flare, suggest that the area and volume of the flare are substantially larger than in a solar two ribbon flare, while the electron pressure is similar. The emission measure and temperature of the non-flaring emission, interpreted as the average corona, lead to an electron pressure similar to that in a well-developed solar active region. Rotational modulation of a spot related active region requires an unphysically large X-ray flux in a concentrated area.
description: 14 pages, compressed and uuencoded postscript file, to be published in MNRAS
Additional file 2: of Mutant p53 gain of function induces HER2 over-expression in cancer cells
Creators: name: A. Román-Rosales
name: E. García-Villa
name: L. Herrera
name: P. Gariglio
name: J. Díaz-Chávez
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: 60506 Virology

description: Table S2. The sequences of the primers used for HER2 promoter analysis. (PDF 336 kb)
Dynamical reconstruction of the $Λ$CDM model in the scalar-tensor representation of $f\left(Q,T\right)$ gravity
Creators: name: Kaczmarek, Adam Z.
name: Rosa, João Luís
name: Szczȩśniak, Dominik
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Motivated by the growing interest in the nonmetricity-matter couplings, we develop the scalar-tensor formulation of recently introduced $f(Q,T)$ gravity, where $Q$ is the nonmetricity and $T$ is the trace of the energy-momentum tensor. The main properties of the scalar-tensor formalism for the Friedmann-Lema{\^ i}tre-Robertson-Walker (FLRW) Universe are discussed, and we introduce an appropriate set of dynamical variables to analyze the cosmic evolution of the scalar-tensor $f(Q,T)$ cosmology as a dynamical system. By considering two distinct cosmic fluids, namely matter and radiation, we have demonstrated that the cosmological phase space exhibits the typical curvature-dominated, radiation-dominated, matter-dominated, and exponentially accelerated fixed points. Furthermore, under an appropriate set of initial conditions compatible with the current observations from the Planck satellite, our analysis shows that the scalar-tensor $f(Q,T)$ successfully yields models indistinguishable from the $Λ$CDM cosmology and compatible with the weak-field solar system dynamics, without the inclusion of a cosmological constant $Λ$. Thus, the theory introduced herein may be regarded as a suitable candidate to describe the cosmological dynamics of the Universe.
description: 13 pages, 2 figures, 1 table
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 795
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 795, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 795, 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
MOESM5 of Development of in vitro enteroids derived from bovine small intestinal crypts
Creators: name: Hamilton, Carly
name: Young, Rachel
name: Siddharth Jayaraman
name: Anuj Sehgal
name: Paxton, Edith
name: Thomson, Sarah
name: Katzer, Frank
name: Hope, Jayne
name: Innes, Elisabeth
name: Morrison, Liam
name: Mabbott, Neil
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 5. Comparison of stress-related gene expression in bovine enteroid cultures. Table comparing the relative expression level of a range of stress-related genes [13] in the enteroid cultures during serial subsequent rounds of passage. P0, freshly prepared enteroids; P1, passage 1 enteroids, etc.
Effect of grid resolution on large eddy simulation of wall-bounded turbulence
Creators: name: Rezaeiravesh, Saleh
name: Liefvendahl, Mattias
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The effect of grid resolution on large eddy simulation (LES) of wall-bounded turbulent flow is investigated. A channel flow simulation campaign involving systematic variation of the streamwise ($Δx$) and spanwise ($Δz$) grid resolution is used for this purpose. The main friction-velocity based Reynolds number investigated is 300. Near the walls, the grid cell size is determined by the frictional scaling, $Δx^+$ and $Δz^+$, and strongly anisotropic cells, with first $Δy^+ \sim 1$, thus aiming for wall-resolving LES. Results are compared to direct numerical simulations (DNS) and several quality measures are investigated, including the error in the predicted mean friction velocity and the error in cross-channel profiles of flow statistics. To reduce the total number of channel flow simulations, techniques from the framework of uncertainty quantification (UQ) are employed. In particular, generalized polynomial chaos expansion (gPCE) is used to create meta models for the errors over the allowed parameter ranges. The differing behavior of the different quality measures is demonstrated and analyzed. It is shown that friction velocity, and profiles of velocity and the Reynolds stress tensor, are most sensitive to $Δz^+$, while the error in the turbulent kinetic energy is mostly influenced by $Δx^+$. Recommendations for grid resolution requirements are given, together with quantification of the resulting predictive accuracy. The sensitivity of the results to subgrid-scale (SGS) model and varying Reynolds number is also investigated. All simulations are carried out with second-order accurate finite-volume based solver. The choice of numerical methods and SGS model is expected to influence the conclusions, but it is emphasized that the proposed methodology, involving gPCE, can be applied to other modeling approaches as well.
description: 27 pages, The following article has been accepted by Physics of Fluids. After it is published, it will be found at https://aip.scitation.org/journal/phf. Copyright 2018 Saleh Rezaeiravesh and Mattias Liefvendahl. This article is distributed under a Creative Commons Attribution (CC-BY-NC-ND 4.0) License
Haldane gap in the quasi one-dimensional nonlinear $σ$-model
Creators: name: Senechal, D.
Publisher: name: arXiv
Year: 1993
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: This work studies the appearance of a Haldane gap in quasi one-dimensional antiferromagnets in the long wavelength limit, via the nonlinear $σ$-model. The mapping from the three-dimensional, integer spin Heisenberg model to the nonlinear $σ$-model is explained, taking into account two antiferromagnetic couplings: one along the chain axis ($J$) and one along the perpendicular planes ($J_\bot$) of a cubic lattice. An implicit equation for the Haldane gap is derived, as a function of temperature and coupling ratio $J_\bot/J$. Solutions to these equations show the existence of a critical coupling ratio beyond which a gap exists only above a transition temperature $T_N$. The cut-off dependence of these results is discussed.
description: 14 pages (RevTeX 3.0), 3 PostScript figures appended (printing instructions included)
Symmetry-protected coherent relaxation of open quantum systems
Creators: name: van Caspel, Moos
name: Gritsev, Vladimir
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We compute the effect of Markovian bulk dephasing noise on the staggered magnetization of the spin-1/2 XXZ Heisenberg chain, as the system evolves after a Néel quench. For sufficiently weak system-bath coupling, the unitary dynamics are found to be preserved up to a single exponential damping factor. This is a consequence of the interplay between $\mathbb{PT}$ symmetry and weak symmetries, which strengthens previous predictions for $\mathbb{PT}$-symmetric Liouvillian dynamics. Requirements are a non-degenerate $\mathbb{PT}$-symmetric generator of time evolution $\hat{\mathcal{L}}$, a weak parity symmetry and an observable that is anti-symmetric under this parity transformation. The spectrum of $\hat{\mathcal{L}}$ then splits up into symmetry sectors, yielding the same decay rate for all modes that contribute to the observable's time evolution. This phenomenon may be realized in trapped ion experiments and has possible implications for the control of decoherence in out-of-equilibrium many-body systems.
description: 9 pages, 3 figures. Added discussion at end of section III
Additional file 1: of Mutant p53 gain of function induces HER2 over-expression in cancer cells
Creators: name: A. Román-Rosales
name: E. García-Villa
name: L. Herrera
name: P. Gariglio
name: J. Díaz-Chávez
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Developmental Biology
subject: Cancer
subject: 60506 Virology

description: Table S1. The sequences of the primers used for HER2 and p53 analysis. (PDF 339 kb)
Effective action for the Yukawa model in curved spacetime
Creators: name: Toms, David J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the one-loop renormalization of a real scalar field interacting with a Dirac spinor field in curved spacetime. A general Yukawa interaction is considered which includes both a scalar and a pseudoscalar coupling. The scalar field is assumed to be non-minimally coupled to the gravitational field and to have a general quartic self-interaction potential. All of the one-loop renormalization group functions are evaluated and in the special case where there is no mass scale present in the classical theory (apart from the fields) we evaluate the one-loop effective action up to and including order $R^2$ in the curvature. In the case where the fermion is massive we include a chiral term in $γ_5$ and we show that although the $γ_5$ term can be removed by a redefinition of the spinor field an anomaly in the effective action arises that is related to the familiar axial current anomaly.
description: 28 pages
BAYON ISHLARINING METODIK TAVSIFI VA TA'LIMDAGI MAQSADI
Creators: name: Kabulov, Inamjan
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqolamizda biz umumiy oʻrta ta’lim maktablarida ijodiy yozma ishlarning turlari va ta’limdagi maqsadi haqida va oʻquvchilarning yozma savodxonligini rivojlantirishda yozma ishlarning, jumladan bayon ishlarining ahamiyatini va metodik tavsifini yoritib berishga harakat qildik.
The Chern-Simons Source as a Conformal Family and Its Vertex Operators
Creators: name: Balachandran, A. P.
name: Bimonte, G.
name: Gupta, K. S.
name: Stern, A.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In a previous work, a straightforward canonical approach to the source-free quantum Chern-Simons dynamics was developed. It makes use of neither gauge conditions nor functional integrals and needs only ideas known from QCD and quantum gravity. It gives Witten's conformal edge states in a simple way when the spatial slice is a disc. Here we extend the formalism by including sources as well. The quantum states of a source with a fixed spatial location are shown to be those of a conformal family, a result also discovered first by Witten. The internal states of a source are not thus associated with just a single ray of a Hilbert space. Vertex operators for both abelian and nonabelian sources are constructed. The regularized abelian Wilson line is proved to be a vertex operator. We also argue in favor of a similar nonabelian result. The spin-statistics theorem is established for Chern-Simons dynamics even though the sources are not described by relativistic quantum fields. The proof employs geometrical methods which we find are strikingly transparent and pleasing. It is based on the research of European physicists about ``fields localized on cones.''
RETURN To an Address of the Legislative Assembly, praying for a return of all moneys received, during the years 1875, 1876, 1877, from leases of Timber Lands in this Province, giving the names of said Lessees; the number of acres held by each respectively ; and where such lands are located.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
The comparative effect of FUV, EUV and X-ray disc photoevaporation on gas giant separations
Creators: name: Jennings, Jeff
name: Ercolano, Barbara
name: Rosotti, Giovanni P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Gas giants' early ($\lesssim 5$ Myr) orbital evolution occurs in a disc losing mass in part to photoevaporation driven by high energy irradiance from the host star. This process may ultimately overcome viscous accretion to disperse the disc and halt migrating giants by starving their orbits of gas, imprinting on giant planet separations in evolved systems. Inversion of this distribution could then give insight into whether stellar FUV, EUV or X-ray flux dominates photoevaporation, constraining planet formation and disc evolution models. We use a 1D hydrodynamic code in population syntheses for gas giants undergoing Type II migration in a viscously evolving disc subject to either a primarily FUV, EUV or X-ray flux from a pre-solar T Tauri star. The photoevaporative mass loss profile's unique peak location and width in each energetic regime produces characteristic features in the distribution of giant separations: a severe dearth of $\lesssim$ 2 M$_{\rm J}$ planets interior to 5 AU in the FUV scenario, a sharp concentration of $\lesssim$ 3 M$_{\rm J}$ planets between $\approx 1.5 - 2$ AU in the EUV case, and a relative abundance of $\approx 2 - 3.5$ M$_{\rm J}$ giants interior to 0.5 AU in the X-ray model. These features do not resemble the observational sample of gas giants with mass constraints, though our results do show some weaker qualitative similarities. We thus assess how the differing photoevaporative profiles interact with migrating giants and address the effects of large model uncertainties as a step to better connect disc models with trends in the exoplanet population.
description: 12 pages, 3 figures, accepted to MNRAS
ColaCare: Enhancing Electronic Health Record Modeling through Large Language Model-Driven Multi-Agent Collaboration
Creators: name: Wang, Zixiang
name: Zhu, Yinghao
name: Zhao, Huiya
name: Zheng, Xiaochen
name: Sui, Dehao
name: Wang, Tianlong
name: Tang, Wen
name: Wang, Yasha
name: Harrison, Ewen
name: Pan, Chengwei
name: Gao, Junyi
name: Ma, Liantao
Publisher: name: arXiv
Year: 2024
Subjects: subject: Machine Learning (cs.LG)
subject: Artificial Intelligence (cs.AI)
subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: We introduce ColaCare, a framework that enhances Electronic Health Record (EHR) modeling through multi-agent collaboration driven by Large Language Models (LLMs). Our approach seamlessly integrates domain-specific expert models with LLMs to bridge the gap between structured EHR data and text-based reasoning. Inspired by the Multidisciplinary Team (MDT) approach used in clinical settings, ColaCare employs two types of agents: DoctorAgents and a MetaAgent, which collaboratively analyze patient data. Expert models process and generate predictions from numerical EHR data, while LLM agents produce reasoning references and decision-making reports within the MDT-driven collaborative consultation framework. The MetaAgent orchestrates the discussion, facilitating consultations and evidence-based debates among DoctorAgents, simulating diverse expertise in clinical decision-making. We additionally incorporate the Merck Manual of Diagnosis and Therapy (MSD) medical guideline within a retrieval-augmented generation (RAG) module for medical evidence support, addressing the challenge of knowledge currency. Extensive experiments conducted on three EHR datasets demonstrate ColaCare's superior performance in clinical mortality outcome and readmission prediction tasks, underscoring its potential to revolutionize clinical decision support systems and advance personalized precision medicine. All code, case studies and a questionnaire are available at the project website: https://colacare.netlify.app.
description: ACM TheWebConf 2025 Conference (WWW 2025) Research Track
Primordial Black Hole Mergers as Probes of Dark Matter in Galactic Center
Creators: name: Ding, Qianhang
name: He, Minxi
name: Takhistov, Volodymyr
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Primordial black holes (PBHs) from the early Universe that can contribute to dark matter (DM) abundance have been linked to gravitational wave observations. Super-massive black holes (SMBHs) at the centers of galaxies are expected to modify distribution of DM in their vicinity, and can result in highly concentrated DM spikes. We revisit PBH merger rates in the presence of DM spikes, tracking their history. We find novel peaked structure in the redshift-evolution of PBH merger rates at low redshifts around $z \sim 5$. These effects are generic and are present for distinct PBH mass functions and spike profiles, and also can be linked to peaked structure in redshift evolution of star formation rate. Redshift evolution characteristics of PBH merger rates can be distinguished from astrophysical black hole contributions and observable with gravitational waves, enabling them to serve as probes of DM in galactic centers.
description: 20 pages, 14 figures
RETURN To an Address of the Legislative Assembly for a Return of the telegrams from Mr. T.L. Stahlschmidt, dated respectively as follows :--June 30th, cable message; July 3rd, cable message; August 9th, cable message; September 25th, cable message ; and October 2nd, cable message.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
A large amplitude flaring dMe star in the 1978 October 6B $γ$-ray burst error box
Creators: name: Greiner, J.
name: Motch, C.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Spectroscopic observations provide evidence that the optical transient object observed in 1966 on archival plates of Sonneberg Observatory is a B=18.5 dMe star. For an assumed flare duration of 40 min. (or longer) the flare amplitude was $\bigtriangleup$m$_{B}$ $\approx$ 5.2 mag. If the recorded event was belonging to the class of 'fast' flares its amplitude could have reached 7-9 mag.. We estimate a lower limit for the optical flare energy release of 10$^{35}$ (d/100 pc)$^2$ erg/s. We discuss the positional coincidence of this large amplitude flaring star with the error box of the $γ$-ray burst 1978 October 6B and conclude that the flare star is probably not related to the $γ$-ray burst. The fact that no other optical flare was found from this object restricts their frequency to be less than 7$\times$10$^{-4}$ h$^{-1}$ for amplitudes (in B) greater than 4.5 mag. Nevertheless, large amplitude flares constitute a serious background problem for the wide field search for possible optical counterparts of $γ$-ray bursters.
description: 6 p., LATEX with A\&A macro l-aa, MPE Prep. 295
MOESM3 of Development of in vitro enteroids derived from bovine small intestinal crypts
Creators: name: Hamilton, Carly
name: Young, Rachel
name: Siddharth Jayaraman
name: Anuj Sehgal
name: Paxton, Edith
name: Thomson, Sarah
name: Katzer, Frank
name: Hope, Jayne
name: Innes, Elisabeth
name: Morrison, Liam
name: Mabbott, Neil
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 20199 Astronomical and Space Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology

description: Additional file 3. Mean expression profiles of the genes in each of the largest 50 co-expression clusters. Individual mean expression profiles of the genes in each of the largest 50 co-expression clusters derived from the network graph. The x axis shows the samples ordered as follows: C, isolated intestinal crypts; P0, freshly prepared enteroids; P1, passage 1 enteroids, etc. The y axis shows the mean expression intensity (transcripts/million reads, TPM) for the cluster.
Carnet de notes relatives aux sociétés de farandoles, aux représentations théatrales et aux archives de la marine de Toulon
Creators: name: Lancelot, Francine
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Source: ttp://www.calames.abes.fr/pub/ms/FileId-3413
description: created: ca 1970
Determination of the Coronal and Interplanetary Magnetic-Field Strength and Radial Profiles from the Large-Scale Photospheric Magnetic Fields
Creators: name: Bilenko, Irina A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: A new model has been proposed for magnetic field determination at different distances from the Sun during different solar cycle phases. The model depends on the observed large-scale non-polar photospheric magnetic fields and that measured at polar regions from 55N to 90N and from 55S to 90S,which are the visible manifestations of cyclic changes in the toroidal and poloidal components of the global magnetic field of the Sun. The modeled magnetic field is determined as the superposition of the non-polar and the polar photospheric magnetic field cycle variations. The agreement between the model predictions and magnetic fields derived from direct, in-situ, measurements at different distances from the Sun, obtained by different methods, and at different solar activity phases is quite satisfactory. From a comparison of the magnetic fields as observed and as calculated from the model at 1 AU, it should be concluded that the model magnetic-field variations adequately explains the major features of the IMF Bx component cycle evolution at the Earth's orbit. The model CR-averaged magnetic fields correlate with CR-averaged IMF Bx component at the Earth's orbit with a coefficient of 0.688, and for seven CR-averaged data the correlation reaches 0.808. The model magnetic-field radial profiles were compared with that of the already existing models. In addition, the decrease in the non-polar and polar photospheric magnetic fields has been revealed. Both magnetic fields during solar cycle maxima and that during minima phases decreased from Cycle 21 to Cycle 24. It means that both the toroidal and poloidal components and therefore, the solar global magnetic field decreased from Cycle 21 to Cycle 24.
description: 27 pages, 6 figures, 2 tables
Pain sensitivity increases with sleep disturbance under predictable chronic mild stress in mice
Creators: name: Dalanon, Junhel
Publisher: name: figshare
Year: 2021
Subjects: subject: 119999 Medical and Health Sciences not elsewhere classified
subject: FOS: Other medical sciences
subject: 111699 Medical Physiology not elsewhere classified
subject: FOS: Basic medicine
subject: Medicine
subject: 30405 Molecular Medicine
subject: 110505 Oral Medicine and Pathology
subject: FOS: Clinical medicine

description: Even though it has been well documented that stress can lead to the development of sleep disorders and the intensification of pain, their relationships have not been fully understood. The present study was aimed at investigating the effects of predictable chronic mild stress (PCMS) on sleep–wake states and pain threshold, using the PCMS rearing conditions of mesh wire (MW) and water (W) for 21 days. Exposure to PCMS decreased the amount of non-rapid eye movement (NREM) sleep during the dark phase. Moreover, the chronicity of PCMS decreased slow-wave activity (SWA) during NREM sleep in the MW and W groups in both the light and dark phases. Mechanical and aversively hot thermal hyperalgesia were more intensified in the PCMS groups than the control. Higher plasma corticosterone levels were seen in mice subjected to PCMS, whereas TNF-α expression was found higher in the hypothalamus in the W and the trigeminal ganglion in the MW group. The W group had higher expression levels of IL-6 in the thalamus as well. The PCMS paradigm decreased SWA and may have intensified mechanical and thermal hyperalgesia. The current study also suggests that rearing under PCMS may cause impaired sleep quality and heightened pain sensation to painful mechanical and aversively hot thermal stimuli.
Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
Creators: name: Wang, Ling-Feng
name: Zhang, Xuan-Neng
name: Zhang, Jing-Fei
name: Zhang, Xin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate the impacts of the gravitational-wave (GW) standard siren observation of the Einstein Telescope (ET) on constraining the total neutrino mass. We simulate 1000 GW events that would be observed by the ET in its 10-year observation by taking the standard $Λ$CDM cosmology as a fiducial model. We combine the simulated GW data with other cosmological observations including cosmic microwave background (CMB), baryon acoustic oscillations (BAO), and type Ia supernovae (SN). We consider three mass hierarchy cases for the neutrino mass, i.e., normal hierarchy (NH), inverted hierarchy (IH), and degenerate hierarchy (DH). Using Planck+BAO+SN, we obtain $\sum m_ν<0.175$ eV for the NH case, $\sum m_ν<0.200$ eV for the IH case, and $\sum m_ν<0.136$ eV for the DH case. After considering the GW data, i.e., using Planck+BAO+SN+GW, the constraint results become $\sum m_ν<0.151$ eV for the NH case, $\sum m_ν<0.185$ eV for the IH case, and $\sum m_ν<0.122$ eV for the DH case. We find that the GW data can help reduce the upper limits of $\sum m_ν$ by 13.7%, 7.5%, and 10.3% for the NH, IH, and DH cases, respectively. In addition, we find that the GW data can also help break the degeneracies between $\sum m_ν$ and other parameters. We show that the GW data of the ET could greatly improve the constraint accuracies of cosmological parameters.
description: 8 pages, 4 figures