cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Uniformly hot nightside temperatures on short-period gas giants
Creators: name: Keating, Dylan
name: Cowan, Nicolas B.
name: Dang, Lisa
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Short-period gas giants (hot Jupiters) on circular orbits are expected to be tidally locked into synchronous rotation, with permanent daysides that face their host stars, and permanent nightsides that face the darkness of space. Thermal flux from the nightside of several hot Jupiters has been measured, meaning energy is transported from day to night in some fashion. However, it is not clear exactly what the physical information from these detections reveals about the atmospheric dynamics of hot Jupiters. Here we show that the nightside effective temperatures of a sample of 12 hot Jupiters are clustered around 1100 K, with a slight upward trend as a function of stellar irradiation. The clustering is not predicted by cloud-free atmospheric circulation models. This result can be explained if most hot Jupiters have nightside clouds that are optically thick to outgoing longwave radiation and hence radiate at the cloud-top temperature, and progressively disperse for planets receiving greater incident flux. Phase curve observations at a greater range of wavelengths are crucial to determining the extent of cloud coverage, as well as the cloud composition on hot Jupiter nightsides.
description: 18 pages, 3 figures. Submitted August 13th, 2018, accepted for publication July 5th 2019. Added a second, parallel analysis. Interpretation of results unchanged from previous version. Updated main text to reflect the published version, and removed a sentence in the Methods that misquoted Beatty+ 2019
HST Imaging of the Host Galaxies of High Redshift Radio-Loud Quasars
Creators: name: Lehnert, Matthew D.
name: van Breugel, Wil J. M.
name: Heckman, Timothy M.
name: Miley, George K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present rest-frame UV and Ly-alpha images of spatially-resolved structures around five high-redshift radio-loud quasars obtained with the WFPC2 camera on the Hubble Space Telescope. We find that all five quasars are extended and this "fuzz" contains ~5-40% of the total continuum flux and 15-65% of the Ly-alpha flux within a radius of about 1.5 arcsec. The rest-frame UV luminosities of the hosts are log lambda P_lambda = 11.9 to 12.5 solar luminosities (assuming no internal dust extinction), comparable to the luminous radio galaxies at similar redshifts and a factor 10 higher than both radio-quiet field galaxies at z~2-3 and the most UV-luminous low redshift starburst galaxies. The Ly-alpha luminosities of the hosts are (in the log) approximately 44.3-44.9 erg/s which are also similar to the those of luminous high redshift radio galaxies and considerably larger than the Ly-alpha luminosities of high redshift field galaxies. To generate the Ly-alpha luminosities of the hosts would require roughly a few percent of the total observed ionizing luminosity of the quasar. We find good alignment between the extended Ly-alpha and the radio sources, strong evidence for jet-cloud interactions in two cases, again resembling radio galaxies, and what is possibly the most luminous radio-UV synchrotron jet in one of the hosts at z=2.110.
description: 36 pages (latex, aas macros), 3 figures (3 gif and 10 postscript files), accepted for publication in the the Astrophysical Journal Supplement Series
The Gaia-ESO Survey: kinematical and dynamical study of four young open clusters
Creators: name: Bravi, L.
name: Zari, E.
name: Sacco, G. G.
name: Randich, S.
name: Jeffries, R. D.
name: Jackson, R. J.
name: Franciosini, E.
name: Moraux, E.
name: López-Santiago, J.
name: Pancino, E.
name: Spina, L.
name: Wright, N.
name: Jiménez-Esteban, F. M.
name: Klutsch, A.
name: Roccatagliata, V.
name: Gilmore, G.
name: Bragaglia, A.
name: Flaccomio, E.
name: Francois, P.
name: Koposov, S. E.
name: Bayo, A.
name: Carraro, G.
name: Costado, M. T.
name: Damiani, F.
name: Frasca, A.
name: Hourihane, A.
name: Jofré, P.
name: Lardo, C.
name: Lewis, J.
name: Magrini, L.
name: Morbidelli, L.
name: Prisinzano, L.
name: Sousa, S. G.
name: Worley, C. C.
name: Zaggia, S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Context. The origin and dynamical evolution of star clusters is an important topic in stellar astrophysics. Several models have been proposed to understand the formation of bound and unbound clusters and their evolution, and these can be tested by examining the kinematical and dynamical properties of clusters over a wide range of ages and masses. Aims. We use the Gaia-ESO Survey products to study four open clusters (IC 2602, IC 2391, IC 4665, and NGC 2547) that lie in the age range between 20 and 50 Myr. Methods. We employ the gravity index $γ$ and the equivalent width of the lithium line at 6708 $Å$, together with effective temperature $\rm{T_{eff}}$, and the metallicity of the stars in order to discard observed contaminant stars. Then, we derive the cluster radial velocity dispersions $σ_c$, the total cluster mass $\rm{M}_{tot}$, and the half mass radius $r_{hm}$. Using the $Gaia$-DR1 TGAS catalogue, we independently derive the intrinsic velocity dispersion of the clusters from the astrometric parameters of cluster members. Results. The intrinsic radial velocity dispersions derived by the spectroscopic data are larger than those derived from the TGAS data, possibly due to the different masses of the considered stars. Using $\rm{M}_{tot}$ and $r_{hm}$ we derive the virial velocity dispersion $σ_{vir}$ and we find that three out of four clusters are supervirial. This result is in agreement with the hypothesis that these clusters are dispersing, as predicted by the "residual gas expulsion" scenario. However, recent simulations show that the virial ratio of young star clusters may be overestimated if it is determined using the global velocity dispersion, since the clusters are not fully relaxed.
description: 14 pages, 6 figures
Fig. S4: Biotite Mg/Mg+Fe+Mn vs Mn diagram of P2 ash layers. Chemical and petrographic fingerprinting of volcanic ashes as a tool for high-resolution stratigraphy of the upper Miocene Pisco Formation (Peru)
Creators: name: Bosio, Giulia
name: Gioncada, Anna
name: Malinverno, Elisa
name: Celma, Claudio Di
name: Villa, Igor M.
name: Cataldi, Giuseppe
name: Gariboldi, Karen
name: Collareta, Alberto
name: Urbina, Mario
name: Bianucci, Giovanni
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. S4: Biotite Mg/Mg+Fe+Mn vs Mn diagram of P2 ash layers.
On the Unsolvability of Bosonic Quantum Fields
Creators: name: Aglietti, U. G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences
subject: 81T25

description: Two general unsolvability arguments for interacting bosonic quantum field theories are presented, based on Dyson-Schwinger equations on the lattice and cardinality considerations. The first argument is related to the fact that, on a lattice of size N, the system of lattice Dyson-Schwinger equations closes on a basis of "primitive correlators" which is finite, but grows exponentially with N. By properly defining the continuum limit, one finds for N -> infinity a countably-infinite basis of the primitive correlators. The second argument is that any conceivable exact analytic calculation of the primitive correlators involves, in the continuum limit, a linear system of coupled partial differential equations on an infinite number of unknown functions, namely the primitive correlators, evolving with respect to an infinite number of independent variables.
description: LaTex file, 81 pages, 17 figures
Additional file 1 of Evaluation of factors that predict the success rate of trial of labor after the cesarean section
Creators: name: Mi, Yang
name: Qu, Pengfei
name: Guo, Na
name: Bai, Ruimiao
name: Gao, Jiayi
name: Ma, Zhengfeei
name: He, Yiping
name: Wang, Caili
name: Luo, Xiaoqin
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Mathematical Sciences not elsewhere classified
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Table S1. The AUCs of the ROC curves for the nomogram and variables from the logistic regression model in the training set and validation set
Accretion in the Early Kuiper Belt II. Fragmentation
Creators: name: Kenyon, Scott J.
name: Luu, Jane X.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe new planetesimal accretion calculations in the Kuiper Belt that include fragmentation and velocity evolution. All models produce two power law cumulative size distributions, N_C propto r^{-q}, with q = 2.5 for radii less than 0.3-3 km and q = 3 for radii exceeding 1-3 km. The power law indices are nearly independent of the initial mass in the annulus, the initial eccentricity of the planetesimal swarm, and the initial size distribution of the planetesimal swarm. The transition between the two power laws moves to larger radii as the initial eccentricity increases. The maximum size of objects depends on their intrinsic tensile strength; Pluto formation requires a strength exceeding 300 erg per gram. Our models yield formation timescales for Pluto-sized objects of 30-40 Myr for a minimum mass solar nebula. The production of several `Plutos' and more than 10^5 50 km radius Kuiper Belt objects leaves most of the initial mass in 0.1-10 km radius objects that can be collisionally depleted over the age of the solar system. These results resolve the puzzle of large Kuiper Belt objects in a small mass Kuiper Belt.
description: to appear in the Astronomical Journal (July 1999); 54 pages including 7 tables and 13 figures
Witnessing Opto-Mechanical Entanglement with Photon-Counting
Creators: name: Ho, Melvyn
name: Oudot, Enky
name: Bancal, Jean-Daniel
name: Sangouard, Nicolas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The ability to coherently control mechanical systems with optical fields has made great strides over the past decade, and now includes the use of photon counting techniques to detect the non-classical nature of mechanical states. These techniques may soon be used to perform an opto-mechanical Bell test, hence highlighting the potential of cavity opto-mechanics for device-independent quantum information processing. Here, we propose a witness which reveals opto-mechanical entanglement without any constraint on the global detection efficiencies in a setup allowing one to test a Bell inequality. While our witness relies on a well-defined description and correct experimental calibration of the measurements, it does not need a detailed knowledge of the functioning of the opto-mechanical system. A feasibility study including dominant sources of noise and loss shows that it can readily be used to reveal opto-mechanical entanglement in present-day experiments with photonic crystal nanobeam resonators.
description: 5+7 pages, 4 figures
Fig. S6: Biotite total vs K+Na+Ca diagram of P2 ash layers. Chemical and petrographic fingerprinting of volcanic ashes as a tool for high-resolution stratigraphy of the upper Miocene Pisco Formation (Peru)
Creators: name: Bosio, Giulia
name: Gioncada, Anna
name: Malinverno, Elisa
name: Celma, Claudio Di
name: Villa, Igor M.
name: Cataldi, Giuseppe
name: Gariboldi, Karen
name: Collareta, Alberto
name: Urbina, Mario
name: Bianucci, Giovanni
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. S6: Biotite total vs K+Na+Ca diagram of P2 ash layers.
Podura viridis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Entognatha
Collembola
Poduridae
Podura
Podura viridis

description: Podura viridis [spec. nov.]
P. subglobosa viridis. Fn svec. 1172.
Habitat in Europae plantis.
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 608, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Experimental signature of Quantum Darwinism in photonic cluster states
Creators: name: Ciampini, Mario A.
name: Pinna, Giorgia
name: Mataloni, Paolo
name: Paternostro, Mauro
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We report on an experimental assessment of the emergence of Quantum Darwinism (QD) from engineered open-system dynamics. We use a photonic hyperentangled source of graph states to address the effects that correlations among the elements of a multi-party environment have on the establishment of objective reality ensuing the quantum-to-classical transition. Besides embodying one of the first experimental efforts towards the characterization of QD, our work illustrates the non-trivial consequences that multipartite entanglement and, in turn, the possibility of having environment-to-system back-action have on the features of the QD framework.
description: 5 pages, 5 figures, Revtex4-1
Electron-electron interactions in one- and three-dimensional mesoscopic disordered rings: a perturbative approach
Creators: name: Ramin, Michel
name: Reulet, Bertrand
name: Bouchiat, Helene
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We have computed persistent currents in a disordered mesoscopic ring in the presence of small electron-electron interactions, treated in first order perturbation theory. We have investigated both a contact (Hubbard) and a nearest neighbour interaction in 1D and 3D. Our results show that a repulsive Hubbard interaction produces a paramagnetic contribution to the average current (whatever the dimension) and increases the value of the typical current. On the other hand, a nearest neighbour repulsive interaction results in a diamagnetic contribution in 1D and paramagnetic one in 3D, and tends to decrease the value of the typical current in any dimension. Our study is based on numerical simulations on the Anderson model and is justified analytically in the presence of very weak disorder. We have also investigated the influence of the amount of disorder and of the statistical (canonical or grand-canonical) ensemble.
description: 7 pages in REVTEX, 4 figures
Two Neutron Star SXT in Quiescence: 4U 2129+47 and EXO 0748-676
Creators: name: Garcia, Michael R.
name: Callanan, Paul J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on x-ray observations of two soft x-ray transients containing neutron stars, 4U 2129+47 and EXO 0748-676. Our emphasis is on the quiescent properties of these sources. The x-ray spectrum and lightcurve of the eclipsing Low-Mass X-ray Binary (LMXB) 4U 2129+47 was measured with the ROSAT PSPC during its current quiescent state. The quiescent x-ray luminosity of ~ 10**32.7 ergs/s and blackbody temperature of kT ~ 0.21 keV are similar to other quiescent LMXB. The quiescent x-ray light curve appears to show orbital modulation, but the statistics are insufficient to distinguish between a v-shaped partial eclipse (as seen in the high state) or a total, square wave eclipse. The similarity in the luminosity and temperature to other (non-eclipsing) quiescent LMXB implies that the vertical structure in the disk which blocked our direct view of the neutron star in the high state has collapsed, and the neutron star is seen directly. EXO 0748-676 was serendipitously observed with the Einstein IPC in quiescence before it was discovered as a bright transient with EXOSAT. Our re-analysis of this quiescent observation finds L_x ~ 10**34.0 ergs/s, and blackbody temperature of kT ~ 0.22 keV, again similar to other LMXBs in quiescence.
description: 13 pages, 3 figures, Submitted to AJ
Large-Scale Power Spectrum and Cosmological Parameters from SFI Peculiar Velocities
Creators: name: Freudling, Wolfram
name: Zehavi, Idit
name: da Costa, Luiz N.
name: Dekel, Avishai
name: Eldar, Amiram
name: Giovanelli, Riccardo
name: Haynes, Martha P.
name: Salzer, John J.
name: Wegner, Gary
name: Zaroubi, Saleem
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We estimate the power spectrum of mass density fluctuations from peculiar velocities of galaxies by applying an improved maximum-likelihood technique to the new all-sky SFI catalog. Parametric models are used for the power spectrum and the errors, and the free parameters are determined by assuming Gaussian velocity fields and errors and maximizing the probability of the data given the model. It has been applied to generalized CDM models with and without COBE normalization. The method has been carefully tested using artificial SFI catalogs. The most likely distance errors are found to be similar to the original error estimates in the SFI data. The general result that is not very sensitive to the prior model used is a relatively high amplitude of the power spectrum. For example, at k=0.1 h/Mpc we find P(k)Ω^{1.2}=(4.4+/-1.7)X10^3 (Mpc/h)^3. An integral over the power spectrum yields σ_8Ω^{0.6}=0.82+/-0.12. Model-dependent constraints on the cosmological parameters are obtained for families of CDM models. For example, for COBE-normalized ΛCDM models (scalar fluctuations only), the maximum-likelihood result can be approximated by Ωn^{2} h_{60}^{1.3} =0.58+/-0.11. The formal random errors quoted correspond to the 90% confidence level. The total uncertainty, including systematic errors associated with nonlinear effects, may be larger by a factor of ~2. These results are in agreement with an application of a similar method to other data (Mark III).
description: 35 pages, 11 figures. To appear in the Astrophysical Journal
Podura atra Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Entognatha
Collembola
Poduridae
Podura
Podura atra

description: Podura atra [spec. nov.]
P. subglobosa atra, antennis longitudine corporis apice albis. Fn. svec. 1173.
Habitat in Europae plantis.
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 608, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Superconducting Coherence in a Vortex Line Liquid; Simulations with Finite λ
Creators: name: Chen, Tao
name: Teitel, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We carry out simulations of a lattice London superconductor in a magnetic field B, with a finite magnetic penetration length λ. We find that superconducting coherence parallel to B persists into the vortex line liquid. We argue that the length scale relevant to this effect is Λ=ϕ_0^2/8πT_m.
description: 11 pages, RevTex, 3 figures (available upon request to stte@pas.rochester.edu)
Poiseuille flow of soft polycrystals in 2D rough channels
Creators: name: Sarkar, Tanmoy
name: Chaudhuri, Pinaki
name: Sain, Anirban
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Polycrystals are partially ordered solids where crystalline order extends over mesoscopic length scales, namely, the grain size. We study the Poisuielle flow of such materials in a rough channel. In general, similar to yield stress fluids, three distinct dynamical states, namely, flowing, stick-slip and jammed can be observed, with a yield threshold dependent on channel width. Importantly, the interplay between the finite channel width, and the intrinsic ordering scale (the grain size) leads to new type of spatiotemporal heterogeneity. In wide channels, although the average flow profile remains plug like, at the underlying granular level, there is vigorous grain remodelling activity resulting from the velocity heterogeneity among the grains. As the channel width approaches typical grain size, the flowing polycrystalline state breaks up into a spatially heterogeneous mixture of flowing liquid like patches and chunks of nearly static grains. Despite these static grains, the average velocity still shows a parabolic profile, dominated by the moving liquid like patches. However, the solid-liquid front moves at nearly constant speed in the opposite direction of the external drive.
Podura fusca Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Entognatha
Collembola
Poduridae
Podura
Podura fusca

description: Podura fusca [spec. nov.]
P. globosa fusca nitida, antennis longis: articulis plurimis. Fn. svec. 1174.
Act. Stockh. 1743. p. 296. t. 7.
Habitat in Europae terrestribus.
Mutilla 220 qvum aptera, hunc ordinem secundum alas intraret, sed character ordinis Hymenopterorum affinibus eam sociat.
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 608, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: ADCO, Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Cart. 198-01 (11 H 1055), 185 folios, f. 0081
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2019
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0081, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0081, 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
Supplementary table 1 - quality assessment.docx
Creators: name: Campbell, Danielle
Publisher: name: figshare
Year: 2018
Subjects: subject: 111799 Public Health and Health Services not elsewhere classified
subject: FOS: Health sciences

description: For all (n=14) papers included in the review, this table summarises the intervention, study design, sample selection and size, methods, primary and other outcomes, timing of outcome measurements and study quality (assessed using the Mixed Methods Appraisal Tool (MMAT) Version 2011)
Electron-Cyclotron-Maser Observable Modes
Creators: name: Stupp, Amnon
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigated wave amplification through the Electron-Cyclotron-Maser mechanism. We calculated absorption and emission coefficients without any approximations, also taking into account absorption by the ambient thermal plasma. A power-law energy distribution for the fast electrons was used, as is indicated by X-ray and microwave observations. We developed a model for the saturation length and amplification ratio of the maser, scanned a large parameter space, and calculated the absorption and emission coefficients for every frequency and angle. Previous studies concluded that the unobservable Z-mode dominates in the nu_p \~ nu_B region, and that millisecond spikes are produced in the region nu_p / nu_B<0.25. We find that the observable O-mode and X-mode can produce emission in the 0.8
description: 18 pages, 5 figures
Microscopic Analysis of the Non-Dissipative Force on a Line Vortex in Superconductor
Creators: name: Gaitan, Frank
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: A microscopic analysis of the non-dissipative force F_nd acting on a line vortex in a type-II superconductor at T=0 is given. All work assumes a charged BCS superconductor. We first examine the Berry phase induced in the BCS ground state by movement of the vortex and show how this phase enters into the hydrodynamic action S_hyd of the condensate. Appropriate variation of S_hyd gives F_nd and variation of the Berry phase term is seen to contribute the Magnus force of classical hydrodynamics to F_nd. This analysis confirms in detail the arguments of Ao and Thouless within the context of the BCS model. Our Berry phase, in the limit e -> 0, reproduces the Berry phase they obtain for a neutral superfluid. A second independent determination of F_nd is given through a microscopic derivation of the continuity equation for the condensate linear momentum. This yields the acceleration equation for the superflow. The vortex is seen to act as a momentum sink and the rate of momentum loss yields F_nd. Both calculations yield the same F_nd and show that the Magnus force contribution to F_nd is a consequence of the vortex motion and topology.
description: abbrev. version of cond-mat/9408025, 4 pages, RevTex, no figures
Polish metric spaces with fixed distance set
Creators: name: Camerlo, Riccardo
name: Marcone, Alberto
name: Ros, Luca Motto
Publisher: name: arXiv
Year: 2018
Subjects: subject: Logic (math.LO)
subject: FOS: Mathematics
subject: 03E15, 54E50

description: We study Polish spaces for which a set of possible distances $A \subseteq \mathbb{R}^+$ is fixed in advance. We determine, depending on the properties of $A$, the complexity of the collection of all Polish metric spaces with distances in $A$, obtaining also example of sets in some Wadge classes where not many natural examples are known. Moreover we describe the properties that $A$ must have in order that all Polish spaces with distances in that set belong to a given class, such as zero-dimensional, locally compact, etc. These results lead us to give a fairly complete description of the complexity, with respect to Borel reducibility and again depending on the properties of $A$, of the relations of isometry and isometric embeddability between these Polish spaces.
description: changes following the referee report; main results unchanged
Additional file 1 of A consensus and saturated genetic map provides insight into genome anchoring, synteny of Solanaceae and leaf- and fruit-related QTLs in wolfberry (Lycium Linn.)
Creators: name: Zhao, Jianhua
name: Li, Haoxia
name: Xu, Yuhui
name: Yin, Yue
name: Huang, Ting
name: Zhang, Bo
name: Wang, Yajun
name: Li, Yanlong
name: Cao, Youlong
name: An, Wei
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 1: Figure 1. Two genetic map. (A) The high-density genetic map by resequencing; (B) The consensus genetic map.
A Non-Perturbative Definition of the Standard Models
Creators: name: Wang, Juven
name: Wen, Xiao-Gang
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The Standard Models contain chiral fermions coupled to gauge theories. It has been a long-standing problem to give such gauged chiral fermion theories a quantum non-perturbative definition. By classification of quantum anomalies and symmetric invertible topological orders via a mathematical cobordism theorem for differentiable and triangulable manifolds, and the existence of symmetric gapped boundary for the trivial symmetric invertible topological orders, we propose that Spin(10) chiral fermion theories with Weyl fermions in 16-dimensional spinor representations can be defined on a 3+1D lattice, and subsequently dynamically gauged to be a Spin(10) chiral gauge theory. As a result, the Standard Models from the 16n-chiral fermion SO(10) Grand Unification can be defined non-perturbatively via a 3+1D local lattice model of bosons or qubits. Furthermore, we propose that Standard Models from the 15n-chiral fermion SU(5) Grand Unification can also be realized by a 3+1D local lattice model of fermions.
description: 24 pages. Two columns. v3: Refinement with detailed discussions. Appendices include viewpoints from perturbative local anomalies and non-perturbative global anomalies (e.g. arXiv:1810.00844, SU(2) = Spin(3) $\subset$ Spin(10)), and co/bordism theories (e.g. $\Omega_{D}^{{(\mathrm{Spin}(D) \times \mathrm{Spin}(10))}/{\mathbb{Z}_2^f}}$)
Formation Rates of Black Hole Accretion Disk Gamma-Ray Bursts
Creators: name: Fryer, C. L.
name: Woosley, S. E.
name: Hartmann, D. H.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: While many models have been proposed for GRBs, those currently favored are all based upon the formation of and/or rapid accretion into stellar mass black holes. We present population synthesis calculations of these models using a Monte Carlo approach in which the many uncertain parameters intrinsic to such calculations are varied. We estimate the event rate for each class of model as well as the propagation distance for those having significant delay between formation and burst production, i.e., double neutron star (DNS) mergers and black hole-neutron star (BH/NS) mergers. For reasonable assumptions regarding the many uncertainties in population synthesis, we calculate a daily event rate in the universe for i) merging neutron stars: ~100/day; ii) neutron-star black hole mergers: ~450/day; iii) collapsars: ~10,000/day; iv) helium star black hole mergers: ~1000/day; and v) white dwarf black hole mergers: ~20/day. The range of uncertainty in these numbers however, is very large, typically two to three orders of magnitude. These rates must additionally be multiplied by any relevant beaming factor and sampling fraction (if the entire universal set of models is not being observed). Depending upon the mass of the host galaxy, half of the DNS and BH/NS mergers will happen within 60kpc (for a Milky-Way massed galaxy) to 5Mpc (for a galaxy with negligible mass) from the galactic center. Because of the delay time, neutron star and black hole mergers will happen at a redshift 0.5 to 0.8 times that of the other classes of models. Information is still lacking regarding the hosts of short hard bursts, but we suggest that they are due to DNS and BH/NS mergers and thus will ultimately be determined to lie outside of galaxies and at a closer mean distance than long complex bursts (which we attribute to collapsars).
description: 57 pages total, 23 figures, submitted by ApJ
Existence of ground states for aggregation-diffusion equations
Creators: name: Carrillo, J. A.
name: Delgadino, M. G.
name: Patacchini, F. S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: We analyze free energy functionals for macroscopic models of multi-agent systems interacting via pairwise attractive forces and localized repulsion. The repulsion at the level of the continuous description is modeled by pressure-related terms in the functional making it energetically favorable to spread, while the attraction is modeled through nonlocal forces. We give conditions on general entropies and interaction potentials for which neither ground states nor local minimizers exist. We show that these results are sharp for homogeneous functionals with entropies leading to degenerate diffusions while they are not sharp for fast diffusions. The particular relevant case of linear diffusion is totally clarified giving a sharp condition on the interaction potential under which the corresponding free energy functional has ground states or not.
description: 21 pages
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Cart. 185 (11 H 70), f. 0262r
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0262r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0262r, 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
Binary Classification of Alzheimer Disease using sMRI Imaging modality and Deep Learning
Creators: name: Tufail, Ahsan Bin
name: Zhang, Qiu-Na
name: Ma, Yong-Kui
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences

description: Alzheimer's disease (AD) is an irreversible devastative neurodegenerative disorder associated with progressive impairment of memory and cognitive functions. Its early diagnosis is crucial for the development of possible future treatment option(s). Structural magnetic resonance images (sMRI) plays an important role to help in understanding the anatomical changes related to AD especially in its early stages. Conventional methods require the expertise of domain experts and extract hand-picked features such as gray matter substructures and train a classifier to distinguish AD subjects from healthy subjects. Different from these methods, this paper proposes to construct multiple deep 2D convolutional neural networks (2D-CNNs) to learn the various features from local brain images which are combined to make the final classification for AD diagnosis. The whole brain image was passed through two transfer learning architectures; Inception version 3 and Xception; as well as custom Convolutional Neural Network (CNN) built with the help of separable convolutional layers which can automatically learn the generic features from imaging data for classification. Our study is conducted using cross-sectional T1-weighted structural MRI brain images from Open Access Series of Imaging Studies (OASIS) database to maintain the size and contrast over different MRI scans. Experimental results show that the transfer learning approaches exceed the performance of non-transfer learning based approaches demonstrating the effectiveness of these approaches for the binary AD classification task.
Podura nivalis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Entognatha
Collembola
Poduridae
Podura
Podura nivalis

description: Podura nivalis [spec. nov.]
P. oblonga cinerea signaturis nigris. Fn. svec. 1176.
E. N. C. dec. 2. ann. 3. obs. 197. Pulex nivis.
De Geer Act. Ups. 1740. p. 54. t. 2.
Habitat in Europae nemoribus, Lignis.
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 609, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Victor Frankenstein’s Evil Genius: Plutarch, Brutus’s Vision, and the Absent Revolution
Creators: name: Camilletti, Fabio
Publisher: name: ENTHYMEMA
Year: 2021

description: This essay examines the influence of Plutarch’s Life of Brutus on Mary Shelley’s Frankenstein, arguing that the relationship between Brutus and his «evil genius» provides Shelley with a model for characterizing the pair of Victor Frankenstein and his Creature. By considering the broader context of Plutarch’s reception from the sixteenth through the early nineteenth centuries, and particularly the construction of Brutus as a ghost-seer, a clinical obsessive, or a revolutionary icon, the essay examines the Brutus/Victor parallel as actual and/or symbolic parricides, shedding new light on Shelley’s failed representation of the French Revolution in her novel.
description: ENTHYMEMA, N. 27 (2021)
DMRG Studies of the Spin-Half Heisenberg System with Dimerization and Frustration
Creators: name: Chitra, R.
name: Pati, Swapan K.
name: Krishnamurthy, H. R.
name: Sen, D.
name: Ramasesha, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Using the density matrix renormalization group technique, we study the ground state phase diagram and other low-energy properties of an isotropic antiferromagnetic spin-half chain with both dimerization and frustration, i.e., an alternation $δ$ of the nearest neighbor exchanges and a next-nearest-neighbor exchange $J_2~$. For $δ= 0$, the system is gapless for $J_2 < J_{2c} ~$ and has a gap for $J_2 > J_{2c} ~$ where $J_{2c}~$ is about $0.241$. For $J_2 = J_{2c}$, the gap above the ground state grows as $δ$ to the power $0.667 \pm 0.001$. In the $J_2 - δ$ plane, there is a disorder line $2 J_2 + δ= 1$. To the left of this line, the peak in the static structure factor $S(q)$ is at $q_{max} = π$ (Neel phase), while to the right of the line, $q_{max}$ decreases from $π$ to $π/ 2$ as $J_2$ is increased to large values (spiral phase). For $δ= 1$, the system is equivalent to two coupled chains as on a ladder and it is gapped for all values of the interchain coupling.
description: 17 pages in tex; figures not included; this published version differs significantly from the original, particularly in some numbers
Hematologic parameters in female dogs with carcinoma in benign mixed tumor, stratified as before and after the proposed treatment
Creators: name: Machado, Marília
Publisher: name: figshare
Year: 2018
Subjects: subject: 70709 Veterinary Pathology
subject: FOS: Veterinary sciences

description: Hematologic parameters in female dogs with carcinoma in benign mixed tumor, stratified as before and after the proposed treatment
title: ADCO, Ordre cistercien : comptes (1499-1515) (11 H 1162), f. 00402
Creators: name: de la Côte-d'Or, Archives départementales
name: CBMA/CG21/F.PETOT/2019
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
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: Ordre cistercien : comptes (1499-1515), Archives départementales de la Côte-d'Or, (11 H 1162). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien : comptes (1499-1515), Archives départementales de la Côte-d'Or, (11 H 1162), f. 00402, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Low Luminosity States of the Black Hole Candidate GX 339-4. I. ASCA and Simultaneous Radio/RXTE Observations
Creators: name: Wilms, Joern
name: Nowak, Michael
name: Dove, James B.
name: Fender, Robert P.
name: Di Matteo, Tiziana
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss a series of observations of the black hole candidate GX 339-4 in low luminosity, spectrally hard states. We present spectral analysis of three separate archival Advanced Satellite for Cosmology and Astrophysics (ASCA) data sets and eight separate Rossi X-ray Timing Explorer (RXTE) data sets. Three of the RXTE observations were strictly simultaneous with 843 MHz and 8.3-9.1 GHz radio observations. All of these observations have (3-9 keV) flux approximately < 10^{-9} ergs s^{-1} cm^{-2}. The ASCA data show evidence for an 6.4 keV Fe line with equivalent width 40 eV, as well as evidence for a soft excess that is well-modeled by a power law plus a multicolor blackbody spectrum with peak temperature 150-200 eV. The RXTE data sets also show evidence of an Fe line with equivalent widths 20-140 eV. Reflection models show a hardening of the RXTE spectra with decreasing X-ray flux; however, these models do not exhibit evidence of a correlation between the photon index of the incident power law flux and the solid angle subtended by the reflector. `Sphere+disk' Comptonization models and Advection Dominated Accretion Flow (ADAF) models also provide reasonable descriptions of the RXTE data. The former models yield coronal temperatures in the range 20-50 keV and optical depths of τ~ 3. The model fits to the X-ray data, however, do not simultaneously explain the observed radio properties. The most likely source of the radio flux is synchrotron emission from an extended outflow of size greater than O(10^7 GM/c^2).
description: 18 pages in latex emulateapj.sty. Accepted for publication in the Astrophysical Journal
NV-Metamaterial: Tunable Quantum Hyperbolic Metamaterial Using Nitrogen-Vacancy Centers in Diamond
Creators: name: Ai, Qing
name: Li, Peng-Bo
name: Qin, Wei
name: Sun, C. P.
name: Nori, Franco
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Optics (physics.optics)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We show that nitrogen-vacancy (NV) centers in diamond can produce a novel quantum hyperbolic metamaterial. We demonstrate that a hyperbolic dispersion relation in diamond with NV centers can be engineered and dynamically tuned by applying a magnetic field. This quantum hyperbolic metamaterial with a tunable window for the negative refraction allows for the construction of a superlens beyond the diffraction limit. In addition to subwavelength imaging, this NV-metamaterial can be used in spontaneous emission enhancement, heat transport and acoustics, analogue cosmology, and lifetime engineering. Therefore, our proposal interlinks the two hotspot fields, i.e., NV centers and metamaterials.
description: 7+16 pages, 2+4 figures
Serum biochemical parameters in female dogs with carcinoma in benign mixed tumor, stratified as before and after the proposed treatment
Creators: name: Machado, Marília
Publisher: name: figshare
Year: 2018
Subjects: subject: 70709 Veterinary Pathology
subject: FOS: Veterinary sciences

description: Serum biochemical parameters in female dogs with carcinoma in benign mixed tumor, stratified as before and after the proposed treatment
Additional file 1 of ALG3 contributes to stemness and radioresistance through regulating glycosylation of TGF-β receptor II in breast cancer
Creators: name: Sun, Xiaoqing
name: He, Zhenyu
name: Guo, Ling
name: Wang, Caiqin
name: Lin, Chuyong
name: Ye, Liping
name: Wang, Xiaoqing
name: Li, Yue
name: Yang, Meisongzhu
name: Liu, Sailan
name: Hua, Xin
name: Wen, Wen
name: Lin, Chao
name: Long, Zhiqing
name: Zhang, Wenwen
name: Li, Han
name: Jian, Yunting
name: Zhu, Ziyuan
name: Wu, Xianqiu
name: Lin, Huanxin
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Cell Biology
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 1: Supplementary Figure 1. (A) The distribution of patients with different tumor type and TP53 status was as shown (left); mRNA expression of ALG3 in subgroup with mutant p53 or wild-type p53 was as shown (right) Each bar represents the mean ± SD of the group. (B) TCGA dataset indicates ALG3 hyper-expresses in basal-like and HER2 positive cell lines. Each bar represents the mean ± SD of the group. (C) TCGA dataset indicates ALG3 tends to be overexpressed in cell lines with TP53 mutation, but not BRCA mutation. Each bar represents the mean ± SD of the group. (D) The correlation between relative RNA expression of ALG3 and the ratio of gray-scale (gray value of the target protein band / gray value of the-tubulin band) was shown. (E) TCGA dataset indicates gene gain or amplification contributes to ALG3 overexpression. Each bar represents the mean ± SD of the group. All data were analyzed by Student’s t-test. “ns” no significance, *P < 0.05, **P < 0.01, *** P < 0.001.
Large-$U$ limit of a Hubbard model in a magnetic field: chiral spin interactions and paramagnetism
Creators: name: Sen, Diptiman
name: Chitra, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We consider the large-$U$ limit of the one-band Hubbard model at half-filling on a non-bipartite two-dimensional lattice. An external magnetic field can induce a three-spin chiral interaction at order $1 / U^2 ~$. We discuss situations in which, at low temperatures, the chiral term may have a larger effect than the Pauli coupling of electron spins to a magnetic field. We present a model which explicitly demonstrates this. The ground state is a singlet with a gap; hence the spin susceptibility is zero while the chiral susceptibility is finite and paramagnetic.
description: 12 pages, plain TeX, one figure available on request, to appear in Phys. Rev. B
Carnet nº 2, commencé à Vienne (p. 39)
Creators: name: Péraire, Lucien
name: CNRS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023

description: created: 18-9-1928