cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
From regular black holes to horizonless objects: quasi-normal modes, instabilities and spectroscopy
Creators: name: Franzin, Edgardo
name: Liberati, Stefano
name: Vellucci, Vania
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study gravitational and test-field perturbations for the two possible families of spherically symmetric black-hole mimickers that smoothly interpolate between regular black holes and horizonless compact objects accordingly to the value of a regularization parameter. One family can be described by the Bardeen-like metrics, and the other by the Simpson-Visser metric. We compute the spectrum of quasi-normal modes (QNMs) of these spacetimes enlightening a common misunderstanding regarding this computation present in the recent literature. In both families, we observe long-living modes for values of the regularization parameter corresponding to ultracompact, horizonless configurations. Such modes appear to be associated with the presence of a stable photon sphere and are indicative of potential non-linear instabilities. In general, the QNM spectra of both families display deviations from the standard spectrum of GR singular BHs. In order to address the future detectability of such deviations in the gravitational-wave ringdown signal, we perform a preliminary study, finding that third generation ground-based detectors might be sensible to macroscopic values of the regularization parameter.
Additional file 1 of Serum homocysteine is associated with tubular interstitial lesions at the early stage of IgA nephropathy
Creators: name: Li, Zizhen
name: Han, Qianqian
name: Ye, Hongbo
name: Li, Jiajia
name: Wei, Xiaona
name: Zhang, Rui
name: Huang, Qiuyan
name: Xu, Yanchun
name: Liu, Guanxian
name: Li, Bin
name: Yang, Qiongqiong
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer

description: Additional file 1: Supplement Table 1. Clinicopathologic characteristics comparison in the subgroup of IgAN patients with eGFR≥90 ml/min/1.73 m2. Supplement Table 2. Correlations between Hcy and clinicopathologic parameters in the subgroup of IgAN patients with eGFR≥90 ml/min/1.73 m2. Supplement Table 3. Clinicopathologic features as factors of elevated Hcy by univariate and multivariate logistic regression analysis in whole populations with "Enter" method. Supplement Table 4. Clinicopathologic features as factors of elevated Hcy by univariate and multivariate logistic regression analysis in patients with eGFR≥90 ml/min/1.73 m2 with "Enter" method.
Massless BPS-Saturated States on the Two-Torus Moduli Sub-Space of Heterotic String
Creators: name: Chan, Kwan-Leung
name: Cvetic, Mirjam
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Within a four-dimensional, toroidally compactified heterotic string, we identify (quantized) charge vectors of electrically charged BPS-saturated states (along with the tower of SL(2,Z) related dyonic states), which preserve 1/2 of N=4 supersymmetry and become massless along the hyper-surfaces of enhanced gauge symmetry of the two-torus moduli sub-space. In addition, we identify charge vectors of the dyonic BPS-saturated states (along with the tower of SL(2,Z) related states), which preserve 1/4 of N=4 supersymmetry, and become massless at two points with the maximal gauge symmetry enhancement.
description: 7 pages, uses RevTeX (minor typos corrected, to appear in Phys. Lett. B)
Additional file 1: of Identifying individuals with chronic pain after knee replacement: a population-cohort, cluster-analysis of Oxford knee scores in 128,145 patients from the English National Health Service
Creators: name: Pinedo-Villanueva, Rafael
name: Khalid, Sara
name: Wylde, Vikki
name: Gooberman-Hill, Rachael
name: Soni, Anushka
name: Judge, Andrew
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology

description: Pain component subscale items of the Oxford Knee Score. Description of the items from the Oxford Knee Score included in the Pain component subscale showing their respective scoring categories. (DOCX 13 kb)
Diffusion of large particles through small pores: from entropic to enthalpic transport
Creators: name: Bodrenko, I. V.
name: Salis, S.
name: Acosta-Gutierrez, S.
name: Ceccarelli, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present an implicit statistical model for the steric effect on the potential of mean force (PMF) of a molecule diffusing through a flexible nanochannel of varying size. The average cross sectional area profile of the channel and the average minimal projection area of the molecule are the two major quantities determining the steric part of the PMF barrier for the translocation of the particle in the case of a small rigid particle and a large rigid channel. In this case, the description is reduced to the Fick-Jacobs model and the PMF is completely entropic. However, the flexibility of channel's cross section and that of molecule's size play crucial role when a large molecule goes through a narrow channel. The PMF profile changes its statictical nature and becomes enthalpic. We treat the flexibility in terms of the equilibrium fluctuations of the pore and of the molecule, independently. For the case of gaussian fluctuations, we derived simple analytical expressions for the steric barrier.
description: 7 pages, 1 figure
Musca radicum Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca radicum

description: Musca radicum [spec. nov.]
M. antennis setariis pilosa, abdomine cinereo: linea dorsali cingulisque quatuor nigris.
Habitat in radicibus Raphani. Rolander.
Similis M. domesticae, sed dimidio minor, angustior.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 596, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Evaluating author name disambiguation for digital libraries: A case of DBLP
Creators: name: Kim, Jinseok
Publisher: name: arXiv
Year: 2018
Subjects: subject: Digital Libraries (cs.DL)
subject: Information Retrieval (cs.IR)
subject: FOS: Computer and information sciences

description: Author name ambiguity in a digital library may affect the findings of research that mines authorship data of the library. This study evaluates author name disambiguation in DBLP, a widely used but insufficiently evaluated digital library for its disambiguation performance. In doing so, this study takes a triangulation approach that author name disambiguation for a digital library can be better evaluated when its performance is assessed on multiple labeled datasets with comparison to baselines. Tested on three types of labeled data containing 5,000 ~ 700K disambiguated names and 6M pairs of disambiguated names, DBLP is shown to assign author names quite accurately to distinct authors, resulting in pairwise precision, recall, and F1 measures around 0.90 or above overall. DBLP's author name disambiguation performs well even on large ambiguous name blocks but deficiently on distinguishing authors with the same names. When compared to other disambiguation algorithms, DBLP's disambiguation performance is quite competitive, possibly due to its hybrid disambiguation approach combining algorithmic disambiguation and manual error correction. A discussion follows on strengths and weaknesses of labeled datasets used in this study for future efforts to evaluate author name disambiguation on a digital library scale.
description: Scientometrics (2018)
Evolution of a Primordial Black Hole Population
Creators: name: Custodio, P. S.
name: Horvath, J. E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We reconsider in this work the effects of an energy absorption term in the evolution of primordial black holes (hereafter PBHs) in the several epochs of the Universe. A critical mass is introduced as a boundary between the accreting and evaporating regimes of the PBHs. We show that the growth of PBHs is negligible in the Radiation-dominated Era due to scarcity of energy density supply from the expanding background, in agreement with a previous analysis by Carr and Hawking, but that nevertheless the absorption term is large enough for black holes above the critical mass to preclude their evaporation until the universe has cooled sufficiently. The effects of PBH motion are also discussed: the Doppler effect may give rise to energy accretion in black-holes with large peculiar motions relative to background. We discuss how cosmological constraints are modified by the introduction of the critical mass since that PBHs above it do not disturb the CMBR. We show that there is a large range of admissible masses for PBHs above the critical mass but well below the cosmological horizon. Finally we outline a minimal kinetic formalism, solved in some limiting cases, to deal with more complicated cases of PBH populations
description: RevTex file, 8 pp., 3 .ps figures available upon request from foton@andromeda.iagusp.usp.br
Experimental measurement of the quality factor of a Fabry-Pérot open-cavity axion haloscope
Creators: name: Hernández-Cabrera, Juan F.
name: De Miguel, Javier
name: Hernández-Suárez, E.
name: Joven-Álvarez, Enrique
name: Lorenzo-Hernández, H.
name: Otani, Chiko
name: Rapado-Tamarit, Miguel A.
name: Rubiño-Martín, J. Alberto
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The axion is a hypothetical boson arising from the most natural solution to the problem of charge and parity symmetry in the strong nuclear force. Moreover, this pseudoscalar emerges as a dark matter candidate in a parameter space extending several decades in mass. The Dark-photons \& Axion-Like particles Interferometer (DALI) is a proposal to search for axion dark matter in a range that remains under-examined. Currently in a design and prototyping phase, this haloscope is a multilayer Fabry-Pérot interferometer. A proof-of-principle experiment is performed to observe the resonance in a prototype. The test unveils a quality factor per open cavity of a few hundred over a bandwidth of the order of dozens of megahertz. The result elucidates a physics potential to find the, so far elusive, axion, in a sector which can simultaneously solve the symmetry problem in the strong interaction and the enigma of dark matter.
description: 5 pages, 6 figures
Interaction-induced time-symmetry breaking in driven quantum oscillators
Creators: name: Dykman, M. I.
name: Bruder, Christoph
name: Lörch, Niels
name: Zhang, Yaxing
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study parametrically driven quantum oscillators and show that, even for weak coupling between the oscillators, they can exhibit various many-body states with broken time-translation symmetry. In the quantum-coherent regime, the symmetry breaking occurs via a nonequilibrium quantum phase transition. For dissipative oscillators, the main effect of the weak coupling is to make the switching rate of an oscillator between its period-2 states dependent on the states of other oscillators. This allows mapping the oscillators onto a system of coupled spins. Away from the bifurcation parameter values where the period-2 states emerge, the stationary state corresponds to having a microscopic current in the spin system, in the presence of disorder. In the vicinity of the bifurcation point or for identical oscillators, the stationary state can be mapped on that of the Ising model with an effective temperature $\propto \hbar$, for low temperature. Closer to the bifurcation point the coupling can not be considered weak and the system maps onto coupled overdamped Brownian particles performing quantum diffusion in a potential landscape.
Radiation-dominated bouncing model with slow contraction and inflation
Creators: name: Molinari, Piero A. P.
name: Delgado, Paola C. M.
name: Pinheiro, Rodrigo F.
name: Pinto-Neto, Nelson
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: A very simple non-singular inflationary model is presented where the unique matter content is a radiation fluid. The model slowly contracts from a very large, almost empty and flat spacetime and realizes a bounce. It is then launched to a quasi-de Sitter inflationary expansion with more than sixty e-folds, which smoothly changes to the usual classical, decelerated radiation-dominated expansion before nucleosynthesis. The initial contracting and final expanding phases are classical, but the intermediate bounce and inflationary phases are induced by quantum cosmological effects emerging from a Gaussian wave function quickly moving in configuration space. During this quantum era, a huge number of photons is created. The scale factor describing all this rich evolution is a surprisingly simple analytic function of conformal time. The cosmological scalar perturbations arising from quantum vacuum fluctuations in the far past of the model present an almost scale invariant spectrum with an amplitude compatible with observations for reasonable values of the free parameters of the model.
description: 14 pages, 5 figures
Musca lateralis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca lateralis

description: Musca lateralis [spec. nov.]
M. antennis setariis pilosa nigricans, abdominis lateribus ferrugineis.
Habitat in Europa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 597, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Integration Measure and Spectral Flow in the Critical N=2 String
Creators: name: Lechtenfeld, Olaf
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: I present the moduli space of the (2+2)-dimensional critical closed fermionic string with two world-sheet supersymmetries. The integration of fermionic and Maxwell moduli in the presence of punctures yields the string measure for n-point amplitudes at arbitrary genus and instanton number. Generalized picture-changing and spectral-flow operators emerge, connecting different instanton sectors. Tree and loop amplitudes are computed.
description: Talk at 29th Ahrenshoop Symposium in Buckow 1995, 6 pages, espcrc2.sty
Strangelet spectra from type II supernovae
Creators: name: Vucetich, H.
name: Horvath, J. E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study in this work the fate of strangelets injected as a contamination in the tail of a "strange matter-driven" supernova shock. A simple model for the fragmentation and braking of the strangelets when they pass through the expanding oxygen shell is presented and solved to understand the reprocessing of this component. We find that the escaping spectrum is a scaled-down version of the one injected at the base of the oxygen shell. The supernova source is likely to produce low-energy particles of $A \sim 100-1000$ quite independently of the initial conditions. However, it is difficult that ultrarrelativistic strangelets (such as the hypothetical Centauro primaries) can have an origin in those explosive events.
description: RevTex file, 5 pp., no figures
Numerical Computation of the Effective Potential and Renormalization
Creators: name: Palma, G.
name: Vergara, L.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We present a novel way to compute the one-loop ring-improved effective potential numerically, which avoids the spurious appearence of complex expressions and at the same time is free from the renormalization ambiguities of the self-consistent approaches, based on the direct application of Schwinger-Dyson type equations to the masses.
description: 8 pages, LATEX, 2 postscript figures available. e-mail : gpalma@lauca.usach.cl , submitted to Mod. Phys. Letter A
Introducing the Condor Array Telescope: IV. A possible nova super-remnant surrounding the putative recurrent nova KT Eridani
Creators: name: Shara, Michael M.
name: Lanzetta, Kenneth M.
name: Garland, James T.
name: Gromoll, Stefan
name: Valls-Gabaud, David
name: Walter, Frederick M.
name: Webb, John K.
name: Kniazev, Alexei
name: Townsend, Lee
name: Darnley, Matthew J.
name: Healy-Kalesh, Michael
name: Corral-Santana, Jesus
name: Schmidtobreick, Linda
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Just 10 recurrent novae (RNe) - which erupt repeatedly on timescales shorter than one century - are known in our Galaxy. The most extreme RN known (located in the Andromeda galaxy), M31N 2008-12a, undergoes a nova eruption every year, and is surrounded by a vast nova "super-remnant", 134 pc in extent. Simulations predict that all RNe should be surrounded by similar vast shells, but previous searches have failed to detect them. KT Eri has recently been suggested to be a RN, and we have used the Condor Array Telescope to image its environs through multiple narrowband filters. We report the existence of a large ($\sim$ 50 pc diameter), H$\,α$-bright shell centered on KT Eri, exactly as predicted. This strongly supports the claim that KT Eri is the 11th Galactic recurrent nova, and only the second nova known to be surrounded by a super-remnant. SALT spectra of the super-remnant demonstrate that its velocity width is consistent with that of M31-2008-12a.
description: 12 pages, 8 figures
Quantum Spin Dynamics in a Normal Bose Gas with Spin-orbit Coupling
Creators: name: Tang, Wai Ho
name: Zhang, Shizhong
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: In this Letter, we investigate spin dynamics of a two-component Bose gas with spin-orbit coupling realised in cold atom experiments. We derive coupled hydrodynamic equations for number and spin densities as well as their associated currents. Specialising to quasi-one-dimensional situation, we obtain analytic solutions of the spin helix structure and its dynamics in both adiabatic and diabatic regimes. In the adiabatic regime, the transverse spin decays parabolically in the short-time limit and exponentially in the long time limit, depending on initial polarisation. In contrast, in the diabatic regime, transverse spin density and current oscillate in a way similar to the charge-current oscillation in an undamped LC circuit. The effects of Rabi coupling on the short-time spin dynamics is also discussed. Finally, using realistic experimental parameters for $^{87}$Rb, we show that the time scales for spin dynamics is of order of milliseconds to a few seconds and can be observed experimentally.
description: 6+6 pages, 3 figures
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00135
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173), f. 00135, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Phase-dependent chiral transport and effective non-Hermitian dynamics in a bosonic Kitaev-Majorana chain
Creators: name: McDonald, Alexander
name: Pereg-Barnea, T.
name: Clerk, A. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study a 1D chain of non-interacting bosonic cavities which are subject to nearest-neighbour parametric driving. With a suitable choice of drive phases, this model is strongly analogous to the celebrated Kitaev chain model of a 1D p-wave superconductor. The system exhibits phase-dependent chirality: photons propagate and are amplified in a direction that is determined by the phase of the initial drive or excitation. Further, we find a drastic sensitivity to boundary conditions: for a range of parameters, the boundary-less system has only delocalized, dynamically unstable modes, while a finite open chain is described by localized, dynamically stable modes. While our model is described by a Hermitian Hamiltonian, we show that it has a surprising connection to non-Hermitian asymmetric-hopping models.
description: 12 pages, 7 figures
Bosonic Fields in the String-like Defect Model
Creators: name: Oda, Ichiro
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study localization of bosonic bulk fields on a string-like defect with codimension 2 in a general space-time dimension in detail. We show that in cases of spin 0 scalar and spin 1 vector fields there are an infinite number of massless Kaluza-Klein (KK) states which are degenerate with respect to the radial quantum number, but only the massless zero mode state among them is coupled to fermion on the string-like defect. It is also commented on interesting extensions of the model at hand to various directions such as 'little' superstring theory, conformal field theory and a supersymmetric construction.
description: 17 pages, LaTex 2e, revised version (to appear in Phys. Rev. D)
Solar chemical composition in the hot gas of cool-core ellipticals, groups, and clusters of galaxies
Creators: name: Mernier, François
name: Werner, Norbert
name: de Plaa, Jelle
name: Kaastra, Jelle S.
name: Raassen, Anton J. J.
name: Gu, Liyi
name: Mao, Junjie
name: Urdampilleta, Igone
name: Simionescu, Aurora
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The hot intracluster medium (ICM) pervading galaxy clusters and groups is rich in metals, which were synthesised by billions of supernovae and have accumulated in cluster gravitational wells for several Gyrs. Since the products of both Type Ia and core-collapse supernovae - expected to explode over different time scales - are found in the ICM, constraining accurately the chemical composition these hot atmospheres can provide invaluable information on the history of the enrichment of large-scale structures. Recently, Hitomi observations reported solar abundance ratios in the core of the Perseus cluster, in tension with previous XMM-Newton measurements obtained for 44 cool-core clusters, groups, and massive ellipticals (the CHEERS sample). In this work, we revisit the CHEERS results by using an updated version of the spectral code used to fit the data (SPEXACT v3), the same as was used to obtain the Hitomi measurements. Despite limitations in the spectral resolution, the average Cr/Fe and Ni/Fe ratios are now found to be remarkably consistent with unity and in excellent agreement with the Hitomi results. Our updated measurements suggest that the solar composition of the ICM of Perseus is a very common feature in nearby cool-core systems.
description: 6 pages, 4 figures, accepted for publication in MNRAS Letters
Defect-influenced particle advection in highly confined liquid crystal flows
Creators: name: Lesniewska, Magdalena
name: Mottram, Nigel
name: Henrich, Oliver
Publisher: name: arXiv
Year: 2023
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We study the morphology of the Saturn ring defect and director structure around a colloidal particle with normal anchoring conditions and within the flow of the nematic host phase through a rectangular duct of comparable size to the particle. The changes in the defect structures and director profile influence the advection behaviour of the particle, which we compare to that in a simple Newtonian host phase. These effects lead to a non-monotonous dependence of the differential velocity of particle and fluid, also known as retardation ratio, on the Ericksen number.
Additional file 2: of COSUTI: a protocol for the development of a core outcome set (COS) for interventions for the treatment of uncomplicated urinary tract infection (UTI) in adults
Creators: name: Duane, Sinead
name: Vellinga, Akke
name: Murphy, Andrew
name: Cormican, Martin
name: Smyth, Andrew
name: Healy, Patricia
name: Moore, Michael
name: Little, Paul
name: Devane, Declan
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: PubMed search queries for the systematic review. (DOCX 17 kb)
BHPWAVE: An adiabatic gravitational waveform model for compact objects undergoing quasi-circular inspirals into rotating massive black holes
Creators: name: Nasipak, Zachary
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present {bhpwave}: a new Python-based, open-source tool for generating the gravitational waveforms of stellar-mass compact objects undergoing quasi-circular inspirals into rotating massive black holes. These binaries, known as extreme-mass-ratio inspirals (EMRIs), are exciting mHz gravitational wave sources for future space-based detectors such as the Laser Interferometer Space Antenna (LISA). Relativistic models of EMRI gravitational wave signals are necessary to unlock the full scientific potential of mHz detectors, yet few open-source EMRI waveform models exist. Thus we built {bhpwave}, which uses the adiabatic approximation from black hole perturbation theory to rapidly construct gravitational waveforms based on the leading-order inspiral dynamics of the binary. In this work, we present the theoretical and numerical foundations underpinning {bhpwave}. We also demonstrate how {bhpwave} can be used to assess the impact of EMRI modeling errors on LISA gravitational wave data analysis. In particular, we find that for retrograde orbits and slowly-spinning black holes we can mismodel the gravitational wave phasing by as much as $\sim 10$ radians without significantly biasing EMRI parameter estimation.
description: 24 pages, 17 figures, 2 tables
Oral history interview with Renee A. Schwartz, 2003
Publisher: name: Columbia University
Year: 2021
Subjects: Women lawyers

description: Family: Immigrant parents, furrier union; Brooklyn College: BA, Political Science, 1953, Phi Beta Kappa; Columbia University Law School: LLB, 1955, faculty, curriculum, Law Review, Rosenberg Note, Legislative Drafting Research Fund; Hays, Sklar, Epstein & Herzberg: 1955-1989, Partner 1965-1989, public utility regulation, conjunctional billing, New York City Housing Authority, Transit Authority, matrimonials, equitable distribution, publishing, general corporate, libel; Kronish, Lieb, Weiner & Hellman: Partner 1990; I Have A Dream Foundation pro bono
A forecast of the sensitivity of the DALI Experiment to Galactic axion dark matter
Creators: name: Cabrera, Juan F. Hernández
name: De Miguel, Javier
name: Álvarez, Enrique Joven
name: Hernández-Suárez, E.
name: Rubiiño-Martín, J. Alberto
name: Otani, Chiko
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The axion is a long-postulated boson that can simultaneously solve two fundamental problems of modern physics: the charge-parity symmetry problem in the strong interaction and the enigma of dark matter. In this work we estimate, by means of Monte Carlo simulations, the sensitivity of the Dark-photons$\&$Axion-Like particles Interferometer (DALI), a new-generation Fabry-Pérot haloscope proposed to probe axion dark matter in the 25-250 $μ$eV band.
description: As accepted by Symmetry
Effective Star Formation Rates for Cosmological Applications
Creators: name: Spaans, Marco
name: Carollo, Marcella
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Effective star formation rates in tabular form are computed which yield a prescription for the star formation activity in model galaxies as a function of ambient density, metallicity, and stellar feedback. The effects of supernova explosions on the thermal balance of the Interstellar Medium (ISM) and the presence of a multi-phase ISM are explicitly included. The resulting grid of models can be implemented easily in N-body codes for the computation of star formation processes in merging galaxies and cosmological simulations.
description: 23 pages LaTex, uses aasps, Accepted by ApJ
Unusual double-peak specific heat and spin freezing in a spin-2 triangular lattice antiferromagnet FeAl$_{2}$Se$_{4}$
Creators: name: Li, Kunkun
name: Jin, Shifeng
name: Guo, Jiangang
name: Xu, Yanping
name: Su, Yixi
name: Feng, Erxi
name: Liu, Yu
name: Zhou, Shengqiang
name: Ying, Tianping
name: Li, Shiyan
name: Wang, Ziqiang
name: Chen, Gang
name: Chen, Xiaolong
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report the properties of a triangular lattice iron-chalcogenide antiferromagnet FeAl$_{2}$Se$_{4}$. The spin susceptibility reveals a significant antiferromagnetic interaction with a Curie-Weiss temperature Θ$_{CW}$ ~ -200K and a spin-2 local moment. Despite a large spin and a large |Θ$_{CW}$|, the low-temperature behaviors are incompatible with conventional classical magnets. No long-range order is detected down to 0.4K. Similar to the well-known spin-1 magnet NiGa$_{2}$S$_{4}$, the specific heat of FeAl$_{2}$Se$_{4}$ exhibits an unusual double-peak structure and a T$^{2}$ power law at low temperatures, which are attributed to the underlying quadrupolar spin correlations and the Halperin-Saslow modes, respectively. The spin freezing occurs at ~ 14K, below which the relaxation dynamics is probed by the ac susceptibility. Our results are consistent with the early theory for the spin-1 system with Heisenberg and biquadratic spin interactions. We argue that the early proposal of the quadrupolar correlation and gauge glass dynamics may be well extended to FeAl$_{2}$Se$_{4}$. Our results provide useful insights about the magnetic properties of frustrated quantum magnets with high spins.
description: 7 pages, 4 figures
Universality of random-site percolation thresholds for two-dimensional complex non-compact neighborhoods
Creators: name: Malarz, Krzysztof
Publisher: name: arXiv
Year: 2023
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The phenomenon of percolation is one of the core topics in statistical mechanics. It allows one to study the phase transition known in real physical systems only in a purely geometrical way. In this paper, we determine thresholds $p_c$ for random site percolation in triangular and honeycomb lattices for all available neighborhoods containing sites from the sixth coordination zone. The results obtained (together with the percolation thresholds gathered from the literature also for other complex neighborhoods and also for a square lattice) show the power-law dependence $p_c\propto(ζ/K)^{-γ}$ with $γ=0.526(11)$, $0.5439(63)$ and $0.5932(47)$, for honeycomb, square, and triangular lattice, respectively, and $p_c\proptoζ^{-γ}$ with $γ=0.5546(67)$ independently on the underlying lattice. The index $ζ=\sum_i z_i r_i$ stands for an average coordination number weighted by distance, that is, depending on the coordination zone number $i$, the neighborhood coordination number $z_i$ and the distance $r_i$ to sites in $i$-th coordination zone from the central site. The number $K$ indicates lattice connectivity, that is, $K=3$, 4 and 6 for the honeycomb, square and triangular lattice, respectively.
description: 21 pages (with Supplemental Material), 8 figures, 2 tables, 2 procedures
Anomalies, D-flatness and Small Instantons
Creators: name: Leigh, R. G.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Recently, Witten has proposed a mechanism for symmetry enhancement in $SO(32)$ heterotic string theory, where the singularity obtained by shrinking an instanton to zero size is resolved by the appearance of an $Sp(1)$ gauge symmetry. In this short letter, we consider spacetime constraints from anomaly cancellation in six dimensions and D-flatness and demonstrate a subtlety which arises in the moduli space when many instantons are shrunk to zero size.
description: 8 pages, harvmac
Revisited nuclear magnetic dipole and electric quadrupole moments of polonium isotopes
Creators: name: Skripnikov, Leonid V.
name: Barzakh, Anatoly E.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Nuclear Theory (nucl-th)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We revisited the electronic structure parameters used to interpret the hyperfine structure of neutral polonium. We used a computational scheme that treats relativistic and high-order electronic correlation effects within the coupled cluster with single, double, triple and perturbative quadruple excitations CCSDT(Q) method, as well as estimate the contribution of quantum electrodynamics and finite nuclear size effects. A systematic study of the uncertainty is carried out. This allowed us to obtain significantly refined values for the nuclear magnetic dipole and electric quadrupole moments of a wide range of odd-mass polonium isotopes. For $^{205}$Po and $^{207}$Po we extracted both the magnetic moment and the nuclear magnetization distribution parameter in a nuclear model-independent way. To assess the accuracy of the calculations, we also computed the ionization potential (IP), excitation energies (EE) of the $6p^4~{}^1D_2$ and $6p^3 7s^1~{}^5S_2$ electronic states and the electronic $g_J$ factor in the same theoretical framework. A good agreement of the theory and experiment for IP, EEs and $g_J$ confirms the reliability of the computational scheme and uncertainty estimation for the Po electromagnetic moments. We identify the $6p^4~{}^1D_2$ electronic level as a potentially promising state for further studies of the nuclear moments of polonium isotopes.
title: Физика в задачах. Макросистемы
title: Учебное пособие
titleType: Subtitle
Creators: name: Паршаков А.Н.
Publisher: name: Ай Пи Ар Медиа
Year: 2019

description: Данное учебное пособие является четвертым выпуском из серии «Физика в задачах» и посвящено рассмотрению основных положений физики макросистем. Молекулярная физика и термодинамика занимают особое место в курсе общей физики в силу особенностей систем, состоящих из гигантского числа частиц — атомов и молекул. Рассмотрены следующие разделы: основы молекулярно-кинетической теории вещества, распределения Максвелла, Больцмана; начала термодинамики и их приложения к практическим задачам; явления переноса — теплопроводность, внутреннее трение и диффузия, разреженные газы. Кроме того, ряд задач посвящен реальным газам, фазовым превращениям и поверхностным явлениям. Подготовлено с учетом требований Федерального государственного образовательного стандарта высшего образования. Предназначено для студентов технических вузов и физических факультетов, изучающих дисциплины «Физика», «Физика макросистем», «Молекулярная физика», а также для преподавателей общей физики. Может быть использовано для более углубленного изучения физики в классах физико-математического профиля школ и лицеев.
A Note on Background Independence in Noncommutative Gauge Theories, Matrix Model and Tachyon Condensation
Creators: name: Seiberg, Nathan
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Using the construction of D-branes with nonzero $B$ field in the matrix model we give a physical interpretation of the known background independence in gauge theories on a noncommutative space. The background independent variables are identified as the degrees of freedom of the underlying matrix model. This clarifies and extends some recent results about the end point of tachyon condensation in D-branes with a $B$ field. We also explain the freedom in the description which is parametrized by a two form $Φ$ from the points of view of the noncommutative geometry on the worldvolume of the branes, and of the first quantized string theory.
description: 16 pages. A section about Phi and references were added
A Comparative Analysis of Contact Models in Trajectory Optimization for Manipulation
Creators: name: Onol, Aykut Ozgun
name: Long, Philip
name: Padir, Taskin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: In this paper, we analyze the effects of contact models on contact-implicit trajectory optimization for manipulation. We consider three different approaches: (1) a contact model that is based on complementarity constraints, (2) a smooth contact model, and our proposed method (3) a variable smooth contact model. We compare these models in simulation in terms of physical accuracy, quality of motions, and computation time. In each case, the optimization process is initialized by setting all torque variables to zero, namely, without a meaningful initial guess. For simulations, we consider a pushing task with varying complexity for a 7 degrees-of-freedom robot arm. Our results demonstrate that the optimization based on the proposed variable smooth contact model provides a good trade-off between the physical fidelity and quality of motions at the cost of increased computation time.
description: 6 pages, 7 figures, 4 tables, IROS 2018 camera-ready version
A-type Stars, the Destroyers of Worlds: The lives and deaths of Jupiters in evolving stellar binaries
Creators: name: Stephan, Alexander P.
name: Naoz, Smadar
name: Gaudi, B. Scott
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Hot Jupiters (HJs), gas giant planets orbiting their host stars with periods on the order of days, commonly occur in the Galaxy, including relatively massive ($1.6-2.4$ $M_\odot$, i.e., A-type main sequence stars) and evolved stars. The majority of A-type main sequence stars have stellar binary companions, which can strongly affect the dynamical evolution of planets around either star. In this work, we investigate the effects of gravitational perturbations by a far away stellar companion on the orbital evolution of gas giant planets orbiting A-type stars, the so-called Eccentric Kozai-Lidov (EKL) mechanism, including the effects of general relativity, post-main sequence stellar evolution, and tides. We find that only $0.15~\%$ of A-type stars will host HJs during their main sequence lifetime. However, we also find a new class of planets, Temporary Hot Jupiters (THJs), that form during the post-main sequence lifetime of about $3.7~\%$ of former A-type main sequence stars. These THJs orbit on periods of tens to a hundred days and only exist for a few $100{,}000$ years before they are engulfed, but they reach similar temperatures as `classical' HJs due to the increased stellar luminosities. THJs' spin-orbit angles will mostly be misaligned. THJ effects on the host stars' evolution could also be observable for longer than a few $100{,}000$ years. Overall, we find that approximately $70~\%$ of all gas giant planets orbiting A-type stars will eventually be destroyed or engulfed by their star, about $25~\%$ during the main sequence lifetime, about $45~\%$ during post-main sequence evolution.
description: 19 pages, 6 figures, accepted for publication by AJ
Floquet engineering in the presence of optically excited carriers
Creators: name: Conway, Mitchell A.
name: Tollerud, Jonathan O.
name: Vu, Thi-Hai-Yen
name: Watanabe, Kenji
name: Taniguchi, Takashi
name: Fuhrer, Michael S.
name: Edmonds, Mark T.
name: Davis, Jeffrey A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Other Condensed Matter (cond-mat.other)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Floquet engineering provides an optical means to manipulate electronic bandstructures, however, carriers excited by the pump field can lead to an effective heating, and can obscure measurement of the band changes. A recent demonstration of the effects of Floquet engineering on a coherent ensemble of excitons in monolayer WS$_2$ proved particularly sensitive to non-adiabatic effects, while still being able to accurately resolve bandstructure changes. Here, we drive an AC-Stark effect in monolayer WS$_2$ using pulses with constant fluence but varying pulse duration (from 25-235~fs). With shorter pump pulses, the corresponding increase in peak intensity introduces additional carriers via two-photon absorption, leading to additional decoherence and peak broadening (which makes it difficult to resolve the AC-Stark shift). We use multidimensional coherent spectroscopy to create a coherent ensemble of excitons in monolayer WS$_2$ and measure the evolution of the coherence throughout the duration of the Floquet pump pulse. Changes to the amplitude of the macroscopic coherence quantifies the additional broadening. At the same time, the evolution of the average phase allows the instantaneous changes to the bandstructure to be quantified, and is not impacted by the additional broadening. This approach to measuring the evolution of Floquet-Bloch states demonstrates a means to quantify effective heating and non-adiabaticity caused by excited carriers, while at the same time resolving the coherent evolution of the bandstructure.
Peculiar Spin Frequency and Radio Profile Evolution of PSR J1119$-$6127 Following Magnetar-like X-ray Bursts
Creators: name: Dai, S.
name: Johnston, S.
name: Weltevrede, P.
name: Kerr, M.
name: Burgay, M.
name: Esposito, P.
name: Israel, G.
name: Possenti, A.
name: Rea, N.
name: Sarkissian, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the spin frequency and profile evolution of the radio pulsar J1119$-$6127 following magnetar-like X-ray bursts from the system in 2016 July. Using data from the Parkes radio telescope, we observe a smooth and fast spin-down process subsequent to the X-ray bursts resulting in a net change in the pulsar rotational frequency of $Δν\approx-4\times10^{-4}$\,Hz. During the transition, a net spin-down rate increase of $Δ\dotν\approx-1\times10^{-10}$\,Hz\,s$^{-1}$ is observed, followed by a return of $\dotν$ to its original value. In addition, the radio pulsations disappeared after the X-ray bursts and reappeared about two weeks later with the flux density at 1.4\,GHz increased by a factor of five. The flux density then decreased and undershot the normal flux density followed by a slow recovery back to normal. The pulsar's integrated profile underwent dramatic and short-term changes in total intensity, polarization and position angle. Despite the complex evolution, we observe correlations between the spin-down rate, pulse profile shape and radio flux density. Strong single pulses have been detected after the X-ray bursts with their energy distributions evolving with time. The peculiar but smooth spin frequency evolution of PSR~J1119$-$6127 accompanied by systematic pulse profile and flux density changes are most likely to be a result of either reconfiguration of the surface magnetic fields or particle winds triggered by the X-ray bursts. The recovery of spin-down rate and pulse profile to normal provides us the best case to study the connection between high magnetic-field pulsars and magnetars.
description: Accepted for publication in MNRAS on 2018 July 24
Oral history interview with Reuben Benton, 1971
Publisher: name: Columbia University
Year: 2019
Subjects: Journalists
African American press
African American journalists
Advertising--Newspapers
Newspaper publishing--Economic aspects--United States
Journalists--Labor unions--United States
African Americans--Civil rights

description: Benton discusses the Kansas City Call's experience with unionization by the Luggage Workers Union. At the time, The Call was the only unionized black newspaper. Benton describes his role as advertising manager of the paper, including the struggles of gaining white merchants to advertise in The Call. He chronicles how the relationship between the paper and advertisers, both black and white, shifted throughout the years. Benton describes the importance of black papers, primarily how these papers can understand and report on aspects of the black experience differently than white papers.
Musca pluvialis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca pluvialis

description: Musca pluvialis [spec. nov.]
M. antennis setariis pilosa cinerea, thorace maculis quinque nigris, abdomine maculis tridentatis obsoletis.
Fn. svec. 1112.
Habitat in Europa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 597, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206