cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Degenerate Zeeman Ground States in the Single-Excitation Regime
Creators: name: Sutherland, R. T.
name: Robicheaux, F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: In this work, we demonstrate the importance of considering correlations between degenerate Zeeman sublevels that develop in dense atomic ensembles. In order to do this, we develop a set of equations capable of simulating large numbers of atoms while still incorporating correlations between degenerate Zeeman sublevels. This set of equations is exact in the single-photon limit, and may be interpreted as a generalization of the coupled harmonic oscillator equations typically used the literature. Using these equations, we demonstrate that in sufficiently dense systems, correlations between Zeeman sublevels can cause non-trivial differences in the photon scattering lineshape in arrays and clouds of atoms.
A bias in optical observations of high redshift luminous infrared galaxies
Creators: name: Charmandaris, V.
name: Floc'h, E. Le
name: Mirabel, I. F.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present evidence for the dramatically different morphology between the rest frame UV and 7micron mid-IR emission of VV114 and Arp299, two nearby (z~0) violently interacting infrared luminous galaxies (LIRGs). Nearly all LIRGs are interacting systems and it is currently accepted that they dominate the IR emission at z>1. Luminous IR galaxies located at z=1-2 could easily be detected as unresolved sources in deep optical/near-IR ground based surveys, as well as in upcoming 24micron surveys with the Space Infrared Telescope Facility. We demonstrate that the spatial resolution of these surveys will result in blending of the emission from unresolved interacting components. An increased scatter will thus be introduced in the observed optical to mid-IR colors of these galaxies, leading to a systematic underestimation of their dust content.
description: To appear in the Astrophysical Journal Letters (4 pages 1 figure)
Additional file 6: of Characterization of phenotypic variation and genome aberrations observed among Phytophthora ramorum isolates from diverse hosts
Creators: name: Elliott, Marianne
name: Yuzon, Jennifer
name: Mathu Malar C
name: Tripathy, Sucheta
name: Bui, Mai
name: Chastagner, Gary
name: Coats, Katie
name: Rizzo, David
name: Garbelotto, Matteo
name: Kasuga, Takao
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biotechnology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified

description: Diverse CCNVs revealed by BIC-seq analysis (upper graph for each panel) and a read-depth analysis for heterozygous allele ratios using 10 Kb long non-overlapping sliding window (lower graph). A concatenated view of the 30 largest scaffolds with the total length of 30Â MB, which corresponding to approximately a half of the total genome of Phytophthora ramorum, are shown. Scaffolds numbers for large CCNV regions are indicated with pink bars, and those for copy number neutral LOH are shown with blue bars. Scales show log (base 2) fold difference between sample isolates and reference isolates for BIC-seq analysis and log (base 2) ratios of alleles of sample isolates for the heterozygous allele ratio analysis. At each heterozygous locus, a read count ratio (more-abundant allele/less-abundant allele) was calculated. A) A re-isolate 9D1 from a log of coast live oak showing a small copy number change at scaffold 9 in comparison to its original isolate Pr-1556 (wt, bay) used as a reference. 9D1 is likely a heterokaryon (HK) carrying trisomic (3Ă CCNV) and euploid nuclei. B) Pr-16 carries trisomy and cnLOH aberrations. C) MK516a carries cnLOH. D) BS2014â 584 shows a complicated patter indicating it carries a mixture of trisomic and monosomic nuclei. E) Pr-140.7 is a complicated monosomic heterokaryon. F) Pr-140.9 is monosomic at scaffold 9. G) Pr-106 is a normal euploid. H) Pr-486 is a trisomy at scaffold 10. Numbers of short segmental CNVs are also seen. I) and J) Both re-isolates Pr-745#4 and Pr-1556#7#1 carry complicated mixtures of monosomic and trisomic nuclei. K) BS96 from California bay is trisomic at scaffold 9. L) Pr-218 from Rhamnus cathartica is trisomic at scaffold 10. M) Pr-102, the sequence isolate (Tyler et al..., [17]) is trisomic at scaffold 10. N) a re-isolate Pr-745#3 is trisomic. O) Pr-455 from Osmorhiza berteroi shows cnLOH at several scaffolds. P) Pr-472 from Choisya ternate is trisomic. (PDF 3465 kb)
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00537
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
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: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172), f. 00537, 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
Ongoing Mass Transfer in the Interacting Galaxy Pair NGC 1409/10
Creators: name: Keel, W. C.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I present two-band HST STIS imaging, and WIYN spectral mapping, of ongoing mass transfer in the interacting galaxy pair NGC 1409/10 (where NGC 1410 is the Seyfert galaxy also catalogued as III Zw 55). Archival snapshot WFPC2 imaging from the survey by Malkan et al. showed a dust feature stretching between the galaxies, apparently being captured by NGC 1409. The new images allow estimates of the mass being transferred and rate of transfer. An absorption lane typically 0.25" (100 pc) wide with a representative optical depth tau_B = 0.2 cuts across the spiral structure of NGC 1410, crosses the 7-kpc projected space between the nuclei, wraps in front of and, at the limits of detection, behind NGC 1409, and becomes a denser (tau_B = 0.4) polar feature around the core of NGC 1409. Combination of extinction data in two passbands allows a crude three-dimensional recovery of the dust structure, supporting the front/back geometry derived from colors and extinction estimates. The whole feature contains of order $10^6$ solar masses in dust, implying about 2x10^7 solar masses of gas, requiring a mass transfer rate averaging ~1 solar mass per year unless we are particularly unlucky in viewing angle. Curiously, this demonstrable case of mass transfer seems to be independent of the occurrence of a Seyfert nucleus, since the Seyfert galaxy in this pair is the donor of the material. Likewise, the recipient shows no signs of recent star formation from incoming gas, although NGC 1410 has numerous luminous young star clusters and widespread H-alpha emission.
description: 27 pages, 9 figures. Accepted for the Astronomical Journal, March 2004
title: Topographie de l'industrie de la tannerie à Fès
title: Topographie de l'industrie de la tannerie à Fès
Creators: name: :Unkn
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Tannerie

description: 219
description: 9
description: Bulletin économique et social du Maroc
description: Cartographie
description: BESM-carto_1935-09-p219_09-11
description: Source: Maison méditerranéenne des sciences de l'homme, Cité numérique de la Méditerranée (Cinumed), Bibliothèque nationale du Royaume du Maroc (BNRM)
description: Source: Bulletin économique et social du Maroc
description: Source: Bulletin économique et social du Maroc (BESM) > BESM (Cartographie)
description: Relation: https://cinumed.mmsh.univ-aix.fr/idurl/1/81980
description: Coverage: Maroc
description: Coverage: Fès
description: Coverage: XXe siècle
description: Temporal: XXe siècle
description: Bibliographic citation: « Topographie de l'industrie de la tannerie à Fès », In Bulletin économique et social du Maroc (BESM), n° 9, 1935
description: Provenance: Maison méditerranéenne des sciences de l'homme, Cité numérique de la Méditerranée (Cinumed), Bibliothèque nationale du Royaume du Maroc (BNRM)
description: Provenance: https://cinumed.mmsh.univ-aix.fr/
Effects of attending a writing retreat on doctoral candidates' psychological health and sense of scientific community
Creators: name: Vincent, Cynthia
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Education
subject: Higher Education
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: This experimental research project aims to examine the effects of participating in a writing retreat on the psychological health and sense of scientific community of doctoral students.
Additional file 1 of Comorbidity between depression and anxiety: assessing the role of bridge mental states in dynamic psychological networks
Creators: name: Groen, Robin N.
name: Ryan, Oisín
name: Wigman, Johanna T. W.
name: Riese, Harriëtte
name: Penninx, Brenda W. J. H.
name: Giltay, Erik J.
name: Wichers, Marieke
name: Hartman, Catharina A.
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health

description: Additional file 1.
Every finite non-solvable group admits an Oriented Regular Representation
Creators: name: Morris, Joy
name: Spiga, Pablo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Combinatorics (math.CO)
subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: 05C25, 05C20, 20B25

description: In this paper we give a partial answer to a 1980 question of Lazslo Babai: "Which [finite] groups admit an oriented graph as a DRR?" That is, which finite groups admit an oriented regular representation (ORR)? We show that every finite non-solvable group admits an ORR, and provide a tool that may prove useful in showing that some families of finite solvable groups admit ORRs. We also completely characterize all finite groups that can be generated by at most three elements, according to whether or not they admit ORRs.
description: 37 pages. This is the first in a series of 3 papers that completely answer the 1980 question of Babai
Quantum random walks with history dependence
Creators: name: Flitney, Adrian P.
name: Abbott, Derek
name: Johnson, Neil F.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We introduce a multi-coin discrete quantum random walk where the amplitude for a coin flip depends upon previous tosses. Although the corresponding classical random walk is unbiased, a bias can be introduced into the quantum walk by varying the history dependence. By mixing the biased random walk with an unbiased one, the direction of the bias can be reversed leading to a new quantum version of Parrondo's paradox.
description: 8 pages, 6 figures, RevTeX
A gravito-electromagnetic analogy based on tidal tensors
Creators: name: Costa, L. Filipe
name: Herdeiro, Carlos A. R.
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We propose a new approach to a physical analogy between General Relativity and Electromagnetism, based on tidal tensors of both theories. Using this approach we write a covariant form for the gravitational analogues of the Maxwell equations. The following realisations of the analogy are given. The first one matches linearised gravitational tidal tensors to exact electromagnetic tidal tensors in Minkwoski spacetime. The second one matches exact magnetic gravitational tidal tensors for ultra-stationary metrics to exact magnetic tidal tensors of electromagnetism in curved spaces. In the third we show that our approach leads to two-step exact derivation of the Papapetrou force on a gyroscope. We then establish a new proof for a class of tensor identities that define invariants of the type $\vec{E}^2-\vec{B}^2$ and $\vec{E}\cdot\vec{B}$, and we exhibit the invariants built from tidal tensors in both gravity and electromagnetism. We contrast our approach with the two gravito-electromagnetic analogies commonly found in the literature, and argue that it sheds light on the debate about the limit of validity of one of the analogies, and clarifies issues concerning the physical interpretation of the other.
description: 30 pages, LaTeX; v2. 38 pages, Major rewritting including: i) a new realisation of the proposed analogy giving a simple derivation of the Papapetrou equation for a spinning particle; ii) an appendix with a derivation of the generalised worldline deviation equation; iii) a detailed discussion of main results; iv) more references; v) typos corrected
Additional file 2 of Comorbidity between depression and anxiety: assessing the role of bridge mental states in dynamic psychological networks
Creators: name: Groen, Robin N.
name: Ryan, Oisín
name: Wigman, Johanna T. W.
name: Riese, Harriëtte
name: Penninx, Brenda W. J. H.
name: Giltay, Erik J.
name: Wichers, Marieke
name: Hartman, Catharina A.
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health

description: Additional file 2.
Additional file 5: of Characterization of phenotypic variation and genome aberrations observed among Phytophthora ramorum isolates from diverse hosts
Creators: name: Elliott, Marianne
name: Yuzon, Jennifer
name: Mathu Malar C
name: Tripathy, Sucheta
name: Bui, Mai
name: Chastagner, Gary
name: Coats, Katie
name: Rizzo, David
name: Garbelotto, Matteo
name: Kasuga, Takao
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Allele sizes for the 15 multilocus genotypes (MLGs) identified in 30 Washington State isolates of P. ramorum. (PDF 48 kb)
Supplementary document for Highly efficient visible and near-IR photon pair generation with thin-film lithium niobate - 6829149.pdf
Creators: name: Harper, Nathan
name: Hwang, Emily
name: Sekine, Ryoto
name: Ledezma, Luis
name: Perez, Christian
name: Marandi, Alireza
name: Cushing, Scott
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Uncategorized

description: Supplemental document with additional details on the SPDC background theory, coincidence raw data and detection probabilities, multimode pump theory, and theoretical Michelson interferogram.
The Magnetized Universe
Creators: name: Giovannini, Massimo
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Cosmology, high-energy physics and astrophysics are converging on the study of large-scale magnetic fields. While the experimental evidence for the existence of large-scale magnetization in galaxies, clusters and superclusters is rather compelling, the origin of the phenomenon remains puzzling especially in light of the most recent observations. The purpose of the present review is to describe the physical motivations and some of the open theoretical problems related to the existence of large-scale magnetic fields.
description: 147 pages, 10 included figures. Few corrected typos and added references
High-Energy Emission from Presupernovae
Creators: name: Kryvdyk, Volodymyr
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The non-thermal emission in the magnetospheres of presupernova collapsing stars with initial dipole magnetic fields and a certain initial energy distribution of the charged particles in a magnetosphere is considered. The analysis of particle dynamics and its emission in the stellar magnetosphere under collapse show that the collapsing stars can be the powerful sources of a non-thermal radiation produced by the interaction of charged particles with the magnetic field. The radiation flux grows with decreasing stellar radius. This flux can be observed in the form of radiation burst with duration equal to the stellar collapse time. The radiation flux depends on the distance to the stars, the particle spectrum and magnetic field in the magnetosphere. The radiation flux is calculated for various collapsing stars with initial dipole magnetic fields and an initial power series, relativistic Maxwell, and Boltzmann particle energy distribution in the magnetosphere. This radiation can be observed by means of modern astronomical instruments.
description: 4 page
Additional file 13 of Increased intratumoral mast cells foster immune suppression and gastric cancer progression through TNF-Îą-PD-L1 pathway
Creators: name: Lv, Yipin
name: Zhao, Yongliang
name: Wang, Xianhua
name: Chen, Na
name: Mao, Fangyuan
name: Teng, Yongsheng
name: Wang, Tingting
name: Peng, Liusheng
name: Zhang, Jinyu
name: Cheng, Ping
name: Liu, Yugang
name: Kong, Hui
name: Chen, Weisan
name: Hao, Chuanjie
name: Han, Bin
name: Ma, Qiang
name: Zou, Quanming
name: Chen, Jun
name: Zhuang, Yuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
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: Virology

description: Table S6. Primer and probe sequences for real-time PCR analysis. (DOCX 20 kb)
Additional file 4: of Characterization of phenotypic variation and genome aberrations observed among Phytophthora ramorum isolates from diverse hosts
Creators: name: Elliott, Marianne
name: Yuzon, Jennifer
name: Mathu Malar C
name: Tripathy, Sucheta
name: Bui, Mai
name: Chastagner, Gary
name: Coats, Katie
name: Rizzo, David
name: Garbelotto, Matteo
name: Kasuga, Takao
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified

description: Mean values for irregularity index and relative lesion area of Phytophthora ramorum isolates identified in K-means analysis. Isolates in Cluster 3 were significantly different from those in Clusters 1 and 2. Bars with different letters are significantly different at pÂ
A mathematical bridge between discretized gauge theories in quantum physics and approximate reasoning in pairwise comparisons
Creators: name: Magnot, Jean-Pierre
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Physics (math-ph)
subject: Information Theory (cs.IT)
subject: Differential Geometry (math.DG)
subject: Logic (math.LO)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: 03F25, 70S15, 81T13

description: We describe a mathematical link between aspects of information theory, called pairwise comparisons, and discretized gauge theories. The link is made by the notion of holonomy along the edges of a simplex. This correspondance leads to open questions in both field.
Merger of black hole-neutron star binaries: nonspinning black hole case
Creators: name: Shibata, Masaru
name: Uryu, Koji
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We perform a simulation for merger of a black hole (BH)-neutron star (NS) binary in full general relativity preparing a quasicircular state as initial condition. The BH is modeled by a moving puncture with no spin and the NS by the $Γ$-law equation of state with $Γ=2$. Corotating velocity field is assumed for the NS. The mass of the BH and the rest-mass of the NS are chosen to be $\approx 3.2 M_{\odot}$ and $\approx 1.4 M_{\odot}$ with relatively large radius of the NS $\approx 14$ km. The NS is tidally disrupted near the innermost stable orbit but $\sim 80%$ of the material is swallowed into the BH with small disk mass $\sim 0.3M_{\odot}$ even for such small BH mass $\sim 3M_{\odot}$. The result indicates that the system of a BH and a massive disk of $\sim M_{\odot}$ is not formed from nonspinning BH-NS binaries, although a disk of mass $\sim 0.1M_{\odot}$ is a possible outcome.
description: 5 pages. Phys. Rev. D 74, 121503 (R) (2006)
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0709
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Archives Départementales De La Côte-D'Or
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0709, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0709, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Additional file 14 of Increased intratumoral mast cells foster immune suppression and gastric cancer progression through TNF-Îą-PD-L1 pathway
Creators: name: Lv, Yipin
name: Zhao, Yongliang
name: Wang, Xianhua
name: Chen, Na
name: Mao, Fangyuan
name: Teng, Yongsheng
name: Wang, Tingting
name: Peng, Liusheng
name: Zhang, Jinyu
name: Cheng, Ping
name: Liu, Yugang
name: Kong, Hui
name: Chen, Weisan
name: Hao, Chuanjie
name: Han, Bin
name: Ma, Qiang
name: Zou, Quanming
name: Chen, Jun
name: Zhuang, Yuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
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: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Materials and Methods. (DOCX 63 kb)
Collective Atomic Recoil Lasing Including Friction and Diffusion Effects
Creators: name: Robb, G. R. M.
name: Piovella, N.
name: Ferraro, A.
name: Bonifacio, R.
name: Courteille, Ph. W.
name: Zimmermann, C.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We extend the Collective Atomic Recoil Lasing (CARL) model including the effects of friction and diffusion forces acting on the atoms due to the presence of optical molasses fields. The results from this model are consistent with those from a recent experiment by Kruse et al. [Phys. Rev. Lett. 91, 183601 (2003)]. In particular, we obtain a threshold condition above which collective backscattering occurs. Using a nonlinear analysis we show that the backscattered field and the bunching evolve to a steady-state, in contrast to the non-stationary behaviour of the standard CARL model. For a proper choice of the parameters, this steady-state can be superfluorescent.
description: 4 pages, 4 figures, submitted to PRA
Magnetization spin dynamics in a (LuBi)3Fe5O12 (BLIG) epitaxial film
Creators: name: Malathi, M.
name: Venkat, G.
name: Arora, A.
name: Syvorotka, I. I.
name: Sivasubramanian, V.
name: Prabhakar, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Bismuth substituted lutetium iron garnet (BLIG) films exhibit larger Faraday rotation, and have a higher Curie temperature than yttrium iron garnet. We have observed magnetic stripe domains and measured domain widths of 1.4 μμm using Fourier domain polarization microscopy, Faraday rotation experiments yield a coercive field of 5 Oe. These characterizations form the basis of micromagnetic simulations that allow us to estimate and compare spin wave excitations in BLIG films. We observed that these films support thermal magnons with a precessional frequency of 7 GHz with a line width of 400 MHz. Further, we studied the dependence of precessional frequency on the externally applied magnetic field. Brillouin light scattering experiments and precession frequencies predicted by simulations show similar trend with increasing field.
description: Journal of Magnetism and Magnetic Materials, 2017
The Ellis group conjecture and variants of definable amenability
Creators: name: Jagiella, Grzegorz
Publisher: name: arXiv
Year: 2017
Subjects: subject: Logic (math.LO)
subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: 03C99, 54H20, 03C64

description: We consider definable topological dynamics for $NIP$ groups admitting certain decompositions in terms of specific classes of definably amenable groups. For such a group, we find a description of the Ellis group of its universal definable flow. This description shows that the Ellis group is of bounded size. Under additional assumptions, it is shown to be independent of the model, proving a conjecture proposed by Newelski. Finally we apply the results to new classes of groups definable in o-minimal structures, generalizing all of the previous results for this setting.
Dredge-up and envelope burning in intermediate mass giants of very low metallicity
Creators: name: Herwig, Falk
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (abbreviated) The evolution of intermediate mass stars at very low metallicity during their final thermal pulse asymptotic giant branch phase is studied in detail. As representative examples models with initial masses of 4Msun and 5Msun with a metallicity of Z=0.0001 ([Fe/H] ~ -2.3) are discussed. The 1D stellar structure and evolution model includes time- and depth dependent overshooting motivated by hydrodynamical simulations, as well as a full nuclear network and time-dependent mixing. Particular attention is given to high time and space resolution to avoid numerical artefacts related to third dredge-up and hot-bottom burning predictions. The model calculations predict very efficient third dredge-up which mixes the envelope with the entire intershell layer or a large fraction thereof, and in some cases penetrates into the C/O core below the He-shell. In all cases primary oxygen is mixed into the envelope. The models predict efficient envelope burning during the interpulse phase. Depending on the envelope burning temperature, oxygen is destroyed to varying degrees. The combined effect of dredge-up and envelope burning does not lead to any significant oxygen depletion in any of the cases considered in this study. The large dredge-up efficiency in our model is closely related to the particular properties of the H-shell during the dredge-up phase in low-metallicity very metal poor stars, which is followed here over many thermal pulses. During the dredge-up phase, the temperature just below the convective boundary is large enough for protons to burn vigorously when they are brought into the C-rich environment below the convection boundary by the time- and depth dependent overshooting. H-burning luminosities of 10^5 to ~2* 10^6L_sun are generated. [...]
Mode change of a gamma-ray pulsar, PSR J2021+4026
Creators: name: Zhao, J.
name: Ng, C. W.
name: Lin, L. C. C.
name: Takata, J.
name: Cai, Y.
name: Hu, C. P.
name: Yen, D. C. C.
name: Tam, P. H. T.
name: Hui, C. Y.
name: Kong, A. K. H.
name: Cheng, K. S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: A glitch of a pulsar is known as a sudden increase in the spin frequency and spin-down rate (frequency time derivative), and it can be caused by a sudden rel\ ease of the stress built up in the solid crust of the star or pinned vortices in the superfluid interior. PSR J2021+4026 is the first pulsar that shows a significant change in the gamma-ray flux and pulse profile at the glitch that occurred around 2011 October 16. We report the results of timing and spectral analysis of PSR~J2021+4026 using $\sim$ 8~yr Fermi-LAT data. We find that the pulsar stayed at a high spin-down rate ($\sim 4\%$ higher than the pre-glitch value) and a low gamma-ray state ($\sim 18\%$ lower) for about 3~yr after the glitch. Around 2014 December, the spin-down rate and gamma-ray flux gradually returned to pre-glitch values within a time scale of a few months. The phase-resolved spectra and pulse profiles after the relaxation are also consistent with those before the glitch. The observed long-term evolution of the spin-down rate and the gamma-ray flux indicates that the glitch triggered a mode change in the global magnetosphere. We speculate that the glitch changed the local magnetic field structure around the polar cap and/or the inclination angle of the dipole axis, leading to a change in the electric current circulating in the magnetosphere.
description: 23 pages, 6 figures. Accepted for publication in ApJ
On the possibility of finite quantum Regge calculus
Creators: name: Khatsymovsky, V. M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The arguments were given in a number of our papers that the discrete quantum gravity based on the Regge calculus possesses nonzero vacuum expectation values of the triangulation lengths of the order of Plank scale $10^{-33}cm$. These results are considered paying attention to the form of the path integral measure showing that probability distribution for these linklengths is concentrated at certain nonzero finite values of the order of Plank scale. That is, the theory resembles an ordinary lattice field theory with fixed spacings for which correlators (Green functions) are finite, UV cut off being defined by lattice spacings. The difference with an ordinary lattice theory is that now lattice spacings (linklengths) are themselves dynamical variables, and are concentrated around certain Plank scale values due to {\it dynamical} reasons.
description: 12 pages, plain LaTeX, readability improved, matches version to be published
Additional file 1 of Increased intratumoral mast cells foster immune suppression and gastric cancer progression through TNF-Îą-PD-L1 pathway
Creators: name: Lv, Yipin
name: Zhao, Yongliang
name: Wang, Xianhua
name: Chen, Na
name: Mao, Fangyuan
name: Teng, Yongsheng
name: Wang, Tingting
name: Peng, Liusheng
name: Zhang, Jinyu
name: Cheng, Ping
name: Liu, Yugang
name: Kong, Hui
name: Chen, Weisan
name: Hao, Chuanjie
name: Han, Bin
name: Ma, Qiang
name: Zou, Quanming
name: Chen, Jun
name: Zhuang, Yuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
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: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Table S1. Antibodies and other reagents. (DOCX 29 kb)
Additional file 3: of Characterization of phenotypic variation and genome aberrations observed among Phytophthora ramorum isolates from diverse hosts
Creators: name: Elliott, Marianne
name: Yuzon, Jennifer
name: Mathu Malar C
name: Tripathy, Sucheta
name: Bui, Mai
name: Chastagner, Gary
name: Coats, Katie
name: Rizzo, David
name: Garbelotto, Matteo
name: Kasuga, Takao
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology

description: The maximum and minimum radii within a 45-degree sector of the colony were used to obtain irregularity index as: (43.5â 34.7)/43.5â =â 20.8% (PDF 960 kb)
title: Show and Tell: Eva Canel at the 1893 Columbia World Exhibition in Chicago
Creators: name: Vallejo, Catharina
Publisher: name: Utah State University
Year: 2012

description: Agar Eva Infanzón Canel (1857-1932), a Spanish woman who took the penname of Eva Canel for her professional literary activities, married actor and author Eloy Perillán Buxó at the precocious age of 14 and, after being exiled from Spain for his subversive writing, traveled the theater circuit with him through the Americas. Wherever she stayed for some prolonged period she established cultural magazines, the texts of which she often wrote entirely herself. After her husband’s death in 1889, she earned her living by giving conferences wherever she traveled, and by writing, being one of the first Hispanic women professional journalists. These writings relate mainly to the political and feminist questions of the day and appeared in prestigious venues in Spain and all over the Spanish-American continent—both topics, as Kenmogne and Hooper have indicated, being very daring for a woman of the era. As she was “[a]mante de la tradición por encima de todo” (Simón Palmer 299), one of the first paradoxes of this fascinating figure is the fact that, as Kessel Schwartz has pointed out, she strongly defended the traditional subservient role of women, but lived and worked outside of this role herself (211). Canel also published volumes of short stories, several novels (using the style and stereotypes of romantic sentimentalism “para fustigar los vicios sociales,” says Jean Kenmogne 57), and plays—some of which were performed in Havana, and again although they seem to be an apparent “defence of Spain’s continued spiritual dominance…[they also reveal] a more critical view of the colonial legacy,” says Hooper (9). She also wrote several volumes of travel writing (see Caballer), including a collaborative work on her experiences as (Spanish) war correspondent and secretary of the Spanish Red Cross during the Cuban-Spanish-American war of 1895-1898, in which she strongly supported Spain’s position. She left Cuba in 1898 but returned in 1914 to remain there until her death, always in difficult financial straits. Eva Canel’s omission from serious critical study is compounded by the fact that she lived in many different places and wrote under several different pseudonyms; thus, she has not been recognized as any “national” writer—a circumstance that is hugely ironic, as she was a lifelong, proud Spanish nationalist and conservative monarchist.1 However, given her many “firsts,” her very diverse publications and controversial opinions, it is clear that her work merits more study.
Abrupt global events in the Earth's history: a physics perspective
Creators: name: Ryskin, Gregory
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: The timeline of the Earth's history reveals quasi-periodicity of the geological record over the last 542 Myr, on timescales close, in the order of magnitude, to 1 Myr. What is the origin of this quasi-periodicity? What is the nature of the global events that define the boundaries of the geological time scale? I propose that a single mechanism is responsible for all three types of such events: mass extinctions, geomagnetic polarity reversals, and sea-level fluctuations. The mechanism is fast, and involves a significant energy release. The mechanism is unlikely to have astronomical causes, both because of the energies involved, and because it acts quasi-periodically. It must then be sought within the Earth itself. And it must be capable of reversing the Earth's magnetic field. The last requirement makes it incompatible with the consensus model of the origin of the geomagnetic field - the hydromagnetic dynamo operating in the Earth's fluid core. In the second part of the paper, I show that a vast amount of seemingly unconnected geophysical and geological data can be understood in a unified way if the source of the Earth's main magnetic field is a ~200-km-thick lithosphere, repeatedly magnetized as a result of methane-driven oceanic eruptions, which produce ocean flow capable of dynamo action. The eruptions are driven by the interplay of buoyancy forces and exsolution of dissolved gas, which accumulates in the oceanic water masses prone to stagnation and anoxia. Polarity reversals, mass extinctions, and sequence boundaries are consequences of these eruptions. Unlike the consensus model of geomagnetism, this scenario is consistent with the paleomagnetic data showing that "directional changes during a [geomagnetic polarity] reversal can be astonishingly fast, possibly occurring as a nearly instantaneous jump from one inclined dipolar state to another in the opposite hemisphere".
description: Final journal version. New title, significant changes. Supersedes v.1
title: INVESTIGATION OF INSTALLATION TORQUE AND TORQUE-TO-CAPACITY RELATIONSHIP OF SCREW-PILES AND HELICAL ANCHORS
Creators: name: Ruberti, Mark
Publisher: name: University of Massachusetts Amherst
Year: 2015
Subjects: subject: Civil Engineering
subject: FOS: Civil engineering
subject: Geotechnical Engineering

description: Installation torque has been used in the design of helical anchors (Screw-Piles) since the late 1960s. KT factors released by the manufacturer relating ultimate capacity of Screw-Piles to installation torque allow engineers to calculate a design installation torque which is necessary to achieve the design capacity in the field. These KT factors have been based on shaft geometry alone (Hoyt and Clemence 1989). Recent full-scale uplift tests in both clay and sand have shown that the traditional methods of analysis for estimating uplift capacity based on microscale tests are not representative of macroscale behavior. A soil wedge does not fully develop in many cases and failure is a result of local bearing capacity in the soil immediately above the lead helix and side resistance along the pipe shaft. The relative contribution of these two components to the uplift capacity depends on the specific geometry of the Screw-Pile, not only the shaft geometry, but also the configuration of the helices, the soil type, and depth of embedment of the helical plate (Lutenegger 2015). Full-scale installations and load tests were performed on anchors of varying lead section geometry, shaft geometry, number of helices, soil type, and depth of embedment. Both direct (TORQ-PIN and Chance Digital Indicator) and indirect (hydraulic pressure) methods were used to monitor torque during installation. The direct methods were used to evaluate the reliability of hydraulic pressure readings and how different combinations of machine, torque head, and operator can affect the torque during installation. This paper will investigate how these factors affect KT and also determine the factors that affect the accuracy of torque measurement in the field.
Additional file 3 of Increased intratumoral mast cells foster immune suppression and gastric cancer progression through TNF-Îą-PD-L1 pathway
Creators: name: Lv, Yipin
name: Zhao, Yongliang
name: Wang, Xianhua
name: Chen, Na
name: Mao, Fangyuan
name: Teng, Yongsheng
name: Wang, Tingting
name: Peng, Liusheng
name: Zhang, Jinyu
name: Cheng, Ping
name: Liu, Yugang
name: Kong, Hui
name: Chen, Weisan
name: Hao, Chuanjie
name: Han, Bin
name: Ma, Qiang
name: Zou, Quanming
name: Chen, Jun
name: Zhuang, Yuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
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: Developmental Biology
subject: Science Policy

description: Table S3. Univariate and multivariate analyses of factors associated with survival. (DOCX 20 kb)
Towards Accurate Binary Convolutional Neural Network
Creators: name: Lin, Xiaofan
name: Zhao, Cong
name: Pan, Wei
Publisher: name: arXiv
Year: 2017
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: We introduce a novel scheme to train binary convolutional neural networks (CNNs) -- CNNs with weights and activations constrained to {-1,+1} at run-time. It has been known that using binary weights and activations drastically reduce memory size and accesses, and can replace arithmetic operations with more efficient bitwise operations, leading to much faster test-time inference and lower power consumption. However, previous works on binarizing CNNs usually result in severe prediction accuracy degradation. In this paper, we address this issue with two major innovations: (1) approximating full-precision weights with the linear combination of multiple binary weight bases; (2) employing multiple binary activations to alleviate information loss. The implementation of the resulting binary CNN, denoted as ABC-Net, is shown to achieve much closer performance to its full-precision counterpart, and even reach the comparable prediction accuracy on ImageNet and forest trail datasets, given adequate binary weight bases and activations.
Fault-Tolerant Logical Gate Networks for CSS Codes
Creators: name: Steane, Andrew M.
name: Ibinson, Ben
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Fault-tolerant logical operations for qubits encoded by CSS codes are discussed, with emphasis on methods that apply to codes of high rate, encoding k qubits per block with k>1. It is shown that the logical qubits within a given block can be prepared by a single recovery operation in any state whose stabilizer generator separates into X and Z parts. Optimized methods to move logical qubits around and to achieve controlled-not and Toffoli gates are discussed. It is found that the number of time-steps required to complete a fault-tolerant quantum computation is the same when k>1 as when k=1.
description: 13 pages, 16 figures. The material in the appendix was included in a previous quant-ph eprint, but not yet published; it has been corrected and clarified. The rest is new. Replacement version: various small corrections and clarifications
Rosette nebula globules: Seahorse giving birth to a star
Creators: name: Mäkelä, M. M.
name: Haikala, L. K.
name: Gahm, G. F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The Rosette Nebula is an HII region ionized mainly by the stellar cluster NGC 2244. Elephant trunks, globules, and globulettes are seen at the interface where the HII region and the surrounding molecular shell meet. We have observed a field in the northwestern part of the Rosette Nebula where we study the small globules protruding from the shell. Our aim is to measure their properties and study their star formation history in continuation of our earlier study of the features of the region. We imaged the region in broadband near-infrared (NIR) JsHKs filters and narrowband H2 1-0 S(1), P$β$, and continuum filters using the SOFI camera at the ESO/NTT. The imaging was used to study the stellar population and surface brightness, create visual extinction maps, and locate star formation. Mid-infrared (MIR) Spitzer IRAC and WISE and optical NOT images were used to further study the star formation and the structure of the globules. The NIR and MIR observations indicate an outflow, which is confirmed with CO observations made with APEX. The globules have mean number densities of ~$4.6\times10^4 \rm cm^{-3}$. P$β$ is seen in absorption in the cores of the globules where we measure visual extinctions of 11-16 mag. The shell and the globules have bright rims in the observed bands. In the Ks band 20 to 40% of the emission is due to fluorescent emission in the 2.12 $μ$m H2 line similar to the tiny dense globulettes we studied earlier in a nearby region. We identify several stellar NIR excess candidates and four of them are also detected in the Spitzer IRAC 8.0 $μ$m image and studied further. We find an outflow with a cavity wall bright in the 2.124 $μ$m H2 line and at 8.0 $μ$m in one of the globules. The outflow originates from a Class I young stellar object (YSO) embedded deep inside the globule. An H$α$ image suggests the YSO drives a possible parsec-scale outflow. (abridged)
description: 20 pages, 19 figures, accepted for publication in Astronomy and Astrophysics, figures reduced for astro-ph