cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Massive Star Outflows
Creators: name: Shepherd, D. S.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Molecular outflows in the form of wide-angle winds and/or well-collimated jets are associated with young stellar objects of all luminosities. Independent studies have established that the mass outflow rate is proportional to L_bol^0.6 for L_bol = 0.3 to 10^5 L_sun, suggesting that there is a strong link between accretion and outflow for a wide range of source luminosity and there is reasonable evidence that accretion-related processes are responsible for generating massive molecular flows from protostars up to spectral type B0. Beyond L_bol ~ 10^4 L_sun, O stars generate powerful wide-angle, ionized winds that can dramatically affect outflow morphology and even call into question the relationship between outflow and accretion. Recently Beuther & Shepherd (2005) proposed an evolutionary scenario in which massive protostellar flows (up to early B spectral type) begin collimated. Once the star reaches the Main Sequence, ionizing radiation may affect the balance between magnetic and plasma pressure, inducing changes in the flow morphology and energetics. Here I review the properties of outflows from young OB stars, discuss implications and observational tests of this proposed evolutionary scenario, and examine differences between low-mass and massive star formation.
description: To be published in the IAU Symposium 227 conference proceedings: Massive Star Birth: A Crossroads of Astrophysics See http://www.aoc.nrao.edu/~dshepher/science.shtml for a reprint
Additional file 1: of Optimization of late gadolinium enhancement cardiovascular magnetic resonance imaging of post-ablation atrial scar: a cross-over study
Creators: name: Chubb, Henry
name: Shadman Aziz
name: Rashed Karim
name: Sohns, Christian
name: Orod Razeghi
name: Williams, Steven
name: Whitaker, John
name: Harrison, James
name: Chiribiri, Amedeo
name: Schaeffter, Tobias
name: Wright, Matthew
name: OâNeill, Mark
name: Razavi, Reza
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Details of acquisition and analysis techniques. (DOCX 26Â kb)
Supplementary document for Chirp-driven control over fast-slow light effects in epsilon-near-zero metamaterials - 6899594.pdf
Creators: name: Novikov, Vladimir
name: Dotsenko, Andrey
name: Leontiev, Alexey
name: Napolskii, Kirill
name: Murzina, Tatyana
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Uncategorized

description: Preparation procedures of the ENZ metamaterial.
Thermodynamical Detection of Entanglement by Maxwell's Demons
Creators: name: Maruyama, K.
name: Morikoshi, F.
name: Vedral, V.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum correlation, or entanglement, is now believed to be an indispensable physical resource for certain tasks in quantum information processing, for which classically correlated states cannot be useful. Besides information processing, what kind of physical processes can exploit entanglement? In this paper, we show that there is indeed a more basic relationship between entanglement and its usefulness in thermodynamics. We derive an inequality showing that we can extract more work out of a heat bath via entangled systems than via classically correlated ones. We also analyze the work balance of the process as a heat engine, in connection with the Second Law of thermodynamics.
description: 5 pages, 4 figures. v3: a figure added, a few refs added, & typos corrected
title: Characterization of Dielectric Properties of Earth Materials at Low Frequencies
Creators: name: Henrie, Tarrah Dawn
Publisher: name: Utah State University
Year: 1998

description: Sharma and de Lima (1992) have proposed a model based on Fixman's theoretical development of charged macromolecules in external fields (1980). There are three types of charges considered: the fixed surface charges that are covalently bonded, the layer of bound counterions, and the diffuse layer (Fixman, 1980, Lyklema, 1983 ). Figure (1) shows these different layers. Other common theories, such as Schurr's only consider the bound counterions and the diffuse layer. Schurr assumes that the diffuse layer ions can exchange with the electrolyte. A consequence of this assumption is the lack of polarization of the diffuse layer. This leads to an over estimation of the conductivity and permittivity of clay suspensions (Lima 1992). Fixman's model allows polarization of the diffuse layer, shown in figure (2). Fixman's model is different from other models because it accounts for the motion of the ions tangentially and radially in the diffuse layer around a macromolecule. Other models neglect this tangential motion (Lima, 1992)
Additional file 8: of Phylogenomics provides a robust topology of the major cnidarian lineages and insights on the origins of key organismal traits
Creators: name: Kayal, Ehsan
name: Bentlage, Bastian
name: M. Sabrina Pankey
name: Ohdera, Aki
name: Medina, Monica
name: Plachetzki, David
name: Collins, Allen
name: Ryan, Joseph
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Data occupancy mapped onto ML phylogeny for OF-PTP_75tx. (PDF 1352 kb)
Gilovich and Medvec (1994) replications and extensions
Creators: name: Feldman, Gilad
name: Yeung, Siu Kit
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Social and Behavioral Sciences
subject: action
subject: inaction
subject: judgment and decision making
subject: open science
subject: replication
subject: replication and extension
subject: social psychology
subject: temporal pattern

description: Please see pre-registration directory for pre-registration documents and Qualtrics survey, with simulated datasets and planned data analysis code.
Observation of the Decay B0 => rho+ rho- and Measurement of the Branching Fraction and Polarization
Creators: name: The BABAR Collaboration
name: Aubert, B.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We have observed the rare decay B0 => rho+ rho- in a sample of 89 million BB pairs recorded with the BABAR detector. The number of observed events is 88 +23-21 +-9, with a significance of 5.1 standard deviations with systematic uncertainties included. The branching fraction and the longitudinal polarization are measured to be BR(B0 => rho+ rho-) = (25 +7-6 +5-6)*10^{-6} and Gamma_L/Gamma = 0.98 +0.02-0.08 +-0.03, respectively.
description: 8 pages, 3 postscript figues, submitted to Phys. Rev. D (Rapid Communications)
Spin and Center of mass comparison between the PN approach and the asymptotic formulation
Creators: name: Kozameh, C. N
name: Nieva, J. I.
name: Quiroga, Gonzalo D
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this work we analyse the similarities and differences between the equations of motion for the center of mass and intrinsic angular momentum for isolated sources of gravitational radiation obtained by two different formulations. One approach is based on the asymptotic formulation of the GR whereas the other relies on Post- Newtonian methods. Several conclusions are obtained which could be useful for further developments in both approaches.
Wigner Distribution Function Approach to Dissipative Problems in Quantum Mechanics with emphasis on Decoherence and Measurement Theory
Creators: name: O'Connell, R. F.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We first review the usefulness of the Wigner distribution functions (WDF), associated with Lindblad and pre-master equations, for analyzing a host of problems in Quantum Optics where dissipation plays a major role, an arena where weak coupling and long-time approximations are valid. However, we also show their limitations for the discussion of decoherence, which is generally a short-time phenomenon with decay rates typically much smaller than typical dissipative decay rates. We discuss two approaches to the problem both of which use a quantum Langevin equation (QLE) as a starting-point: (a) use of a reduced WDF but in the context of an exact master equation (b) use of a WDF for the complete system corresponding to entanglement at all times.
Renormalization of the superfluid density in the two-dimensional BCS-BEC crossover
Creators: name: Bighin, G.
name: Salasnich, L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We analyze the theoretical derivation of the beyond-mean-field equation of state for a two-dimensional gas of dilute, ultracold alkali-metal atoms in the Bardeen-Cooper-Schrieffer (BCS) to Bose-Einstein condensate (BEC) crossover. We show that at zero temperature our theory -- considering Gaussian fluctuations on top of the mean-field equation of state -- is in very good agreement with experimental data. Subsequently, we investigate the superfluid density at finite temperature and its renormalization due to the proliferation of vortex-antivortex pairs. By doing so, we determine the Berezinskii-Kosterlitz-Thouless (BKT) critical temperature -- at which the renormalized superfluid density jumps to zero -- as a function of the inter-atomic potential strength. We find that the Nelson-Kosterlitz criterion overestimates the BKT temperature with respect to the renormalization group equations, this effect being particularly relevant in the intermediate regime of the crossover.
description: 9 pages, 3 figures, presented to the International Conference "Electron correlation in superconductors and nanostructures", 17-20 August 2017, Odessa (Ukraine). To be published in the Proceedings
Recovering Solar Toroidal Field Dynamics From Sunspot Location Patterns
Creators: name: Norton, Aimee A.
name: Gilman, Peter A.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyze both Kitt Peak magnetogram data and MDI continuum intensity sunspot data to search for the following solar toroidal band properties: width in latitude and the existence of a tipping instability (longitudinal m=1 mode) for any time during the solar cycle. To determine the extent which we can recover the toroidal field dynamics, we forward model artificially generated sunspot distributions from subsurface toroidal fields we assigned certain properties. We analyzed two sunspot distribution parameters using MDI and model data: the average latitudinal separation of sunspot pairs as a function of longitudinal separation, and the number of sunspot pairs creating a given angle with respect to the E-W direction. A toroidal band of 10 degrees width with a constant tipping of 5 degrees best fits MDI data early in the solar cycle. A toroidal band of 20 degrees width with a tipping amplitude decreasing in time from 5 to 0 degrees best fits MDI data late in the solar cycle. Model data generated by untipped toroidal bands cannot fit MDI high latitude data and can fit only one parameter at low latitudes. Tipped toroidal bands satisfy chi squared criteria at both high and low latitudes. We conclude this is evidence to reject the null hypothesis - that toroidal bands in the solar tachocline do not experience a tipping instability - in favor of the hypothesis that the toroidal band experiences an m=1 tipping instability. Our finding that the band widens from ~10 degrees early in the solar cycle to ~20 degrees late in the solar cycle may be explained in theory by magnetic drag spreading the toroidal band due to altered flow along the tipped field lines.
description: This paper is accepted to Astrophysical Journal, September 2005 issue
title: Cartogramme de publicité et de vente de primeurs marocaines en 1935 [en France]
title: Cartogramme de publicité et de vente de primeurs marocaines en 1935 [en France]
Creators: name: :Unkn
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Exportation
subject: Echanges
subject: Publicité
subject: Primeurs

description: Cartographie
description: BESM-carto_1936-13-p224_13-13
description: 224
description: 13
description: Bulletin économique et social du Maroc
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/1/81818
description: Coverage: Maroc
description: Coverage: XXe siècle
description: Temporal: XXe siècle
description: Bibliographic citation: « Cartogramme de publicité et de vente de primeurs marocaines en 1935 [en France] », In Bulletin économique et social du Maroc (BESM), n° 13, 1936
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/
Additional file 3 of BoostMEC: predicting CRISPR-Cas9 cleavage efficiency through boosting models
Creators: name: Zarate, Oscar A.
name: Yang, Yiben
name: Wang, Xiaozhong
name: Wang, Ji-Ping
Publisher: name: figshare
Year: 2022
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified

description: Additional file 3: This file contains a visual representation of BoostMEC’s second regression tree (tree_index = 1).
MOESM6 of Structural patterns of selection and diversity for Plasmodium vivax antigens DBP and AMA1
Creators: name: Guy, Andrew
name: Vashti Irani
name: Richards, Jack
name: Ramsland, Paul
Publisher: name: figshare
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Marine Biology
subject: Science Policy

description: Additional file 6. Spatially-derived Tajimaâ s D for PvDBP across multiple populations.
Semantic publishing: biodiversity data liberation, linking and FAIRness
Creators: name: BiCKL consortium
Publisher: name: Zenodo
Year: 2023

description: The workshop (September 14-15, 2023, HEG Geneva, Switzerland) is an opportunity to discuss why and to demonstrate how to publish semantically enhanced and linked publications. It will be a mixture of presentations, discussions and technical/practical sessions on implementing workflows. 

 

Topics that will be covered:

The current status of semantic publishing, how we can use it to provide enhanced data for addressing the current biodiversity crisis. 

How natural history institutions can use semantic publishing and data outputs to help build their research strategies. 

Showcase the exciting new semantic publishing tools currently in place  and the status quo of moving from Open Access to Open Access FAIR data.

Linking between publications and collection-related data. 

Linking external data resources and the role of publications as the seeds for building knowledge graphs (BiCIKL). 

Hands on technical session on how the different semantic publishing tools and workflow work: Arpha, Métotaxa, Plazi workflow

Expected results/outcomes

Increase practical understanding on how to implement semantic publishing workflows.

Establishing possible ways to collaborate in further development of semantic publishing and providing innovative tools and support mechanisms (e.g. capacity building, recommendations, guidelines).  

Awareness of the benefits and opportunities of semantic publishing for publishers.

Awareness why semantic publishing is important for biological science in mitigating biodiversity decline.
The five-loop Beta function for a general gauge group and anomalous dimensions beyond Feynman gauge
Creators: name: Luthe, Thomas
name: Maier, Andreas
name: Marquard, Peter
name: Schroder, York
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We focus on a non-abelian gauge field coupled to a single (but general) representation of a family of Nf fermions. By using the same machinery that had allowed us to evaluate the sub-leading large-Nf term of the five-loop Beta function earlier, we here report on a confirmation of the all-Nf result that has in the meantime been published by another group. Furthermore, in order to push forward the 5-loop renormalization program regarding gauge parameter dependence, we present the linear terms of the complete set of anomalous dimensions, in an expansion in the covariant gauge parameter around the Feynman gauge.
description: 17 pages, 2 ancillary files files available with the source. v2: journal version, reference added
The all-sky distribution of 511 keV electron-positron annihilation emission
Creators: name: Knödlseder, J.
name: Jean, P.
name: Lonjou, V.
name: Weidenspointner, G.
name: Guessoum, N.
name: Gillard, W.
name: Skinner, G.
name: von Ballmoos, P.
name: Vedrenne, G.
name: Roques, J. -P.
name: Schanne, S.
name: Teegarden, B.
name: Schönfelder, V.
name: Winkler, C.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a map of 511 keV electron-positron annihilation emission, based on data accumulated with the SPI spectrometer aboard ESA's INTEGRAL gamma-ray observatory, that covers approximately 95% of the celestial sphere. 511 keV line emission is significantly detected towards the galactic bulge region and, at a very low level, from the galactic disk. The bulge emission is highly symmetric and is centred on the galactic centre with an extension of 8 deg. The emission is equally well described by models that represent the stellar bulge or halo populations. The disk morphology is only weakly constrained by the present data, being compatible with both the distribution of young and old stellar populations. The 511 keV line flux from the bulge and disk components is 1.05e-3 ph cm-2 s-1 and 0.7e-3 ph cm-2 s-1, respectively, corresponding to a bulge-to-disk flux ratio in the range 1-3. Assuming a positronium fraction of 0.93 this translates into annihilation rates of 1.5e43 s-1 and 3e42 s-1, respectively. The ratio of the bulge luminosity to that of the disk is in the range 3-9. We find no evidence for a point-like source in addition to the diffuse emission, down to a typical flux limit of 1e-4 ph cm-2 s-1. We also find no evidence for the positive latitude enhancement that has been reported from OSSE measurements; our 3 sigma upper flux limit for this feature is 1.5e-4 ph cm-2 s-1. The disk emission can be attributed to the beta+ decay of the radioactive species 26Al and 44Ti. The bulge emission arises from a different source which has only a weak or no disk component. We suggest that Type Ia supernovae and/or low-mass X-ray binaries are the prime candidates for the source of the galactic bulge positrons. Light dark matter annihilation could also explain the observed 511 keV bulge emission characteristics.
description: accepted for publication in A&A
Generating carrier-envelope-phase stabilized few-cycle pulses from a free-electron laser oscillator
Creators: name: Hajima, Ryoichi
name: Nagai, Ryoji
Publisher: name: arXiv
Year: 2017
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: We propose a scheme to generate carrier-envelope-phase (CEP) stabilized few-cycle optical pulses from a free-electron laser oscillator. The CEP stabilization is realized by continuous injection of CEP-stabilized seed pulses from an external laser to the FEL oscillator whose cavity length is perfectly synchronized to the electron bunch repetition. Such CEP-stabilized few-cycle FEL pulses will be an efficient driver for exploring high-harmonic generation at energies 1-10~keV for attosecond and zeptosecond science, broad-band x-ray optical frequency combs and coherent control of chemical reaction.
description: 14 pages, 5 figures
Additional file 4: of Brazilian propolis ethanol extract and its component kaempferol induce myeloid-derived suppressor cells from macrophages of mice in vivo and in vitro
Creators: name: Kitamura, Hiroshi
name: Saito, Natsuko
name: Fujimoto, Junpei
name: Ken-Ichi Nakashima
name: Fujikura, Daisuke
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Gating processes of FACS analysis. (PDF 516Â kb)
Searches for supersymmetric particles in e+e- collisions up to 208 GeV and interpretation of the results within the MSSM
Creators: name: The DELPHI Collaboration
name: Abdallah, J.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: DELPHI data collected at centre-of-mass energies up to 208 GeV have been analysed to search for charginos, neutralinos and sfermions in the framework of the Minimal Supersymmetric Standard Model (MSSM) with R-parity conservation. No evidence for a signal was found in any of the channels. The results of each search were used to derive limits on production cross-sections and particle masses. In addition, the combined result of all searches excludes regions in the parameter space of the constrained MSSM, leading to limits on the mass of the Lightest Supersymmetric Particle and other supersymmetric particles.
description: 103 pages, 44 figures, Accepted by Eur. Phys. J. C; a version with higher resolution figures 15, 16, 21, 23, 24, 28, 35 and 37 can be found at http://delphiwww.cern.ch/~pubxx/www/delsec/papers/public/paper0302.ps.gz
Note on group irregularity strength of disconnected graphs
Creators: name: Anholcer, Marcin
name: Cichacz, Sylwia
name: Jura, Rafal
name: Marczyk, Antoni
Publisher: name: arXiv
Year: 2017
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: We investigate the \textit{group irregularity strength} ($s_g(G)$) of graphs, i.e. the smallest value of $s$ such that taking any Abelian group $\gr$ of order $s$, there exists a function $f:E(G)\rightarrow \gr$ such that the sums of edge labels at every vertex are distinct. So far it was not known if $s_g(G)$ is bounded for disconnected graphs. In the paper we we present some upper bound for all graphs. Moreover we give the exact values and bounds on $s_g(G)$ for disconnected graphs without a star as a component.
description: arXiv admin note: substantial text overlap with arXiv:1209.0200
Additional file 3: of A systematic review comparing neurodevelopmental outcome in term infants with hypoxic and vascular brain injury with and without seizures
Creators: name: T. De Haan
name: J. Langeslag
name: J. Van Der Lee
name: A. Van Kaam
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: Data extraction form. (DOC 72Â kb)
Convective Dynamos and the Minimum X-ray Flux in Main Sequence Stars
Creators: name: Bercik, D. J.
name: FIsher, G. H.
name: Johns-Krull, C. M.
name: Abbett, W. P.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The objective of this paper is to investigate whether a convective dynamo can account quantitatively for the observed lower limit of X-ray surface flux in solar-type main sequence stars. Our approach is to use 3D numerical simulations of a turbulent dynamo driven by convection to characterize the dynamic behavior, magnetic field strengths, and filling factors in a non-rotating stratified medium, and to predict these magnetic properties at the surface of cool stars. We use simple applications of stellar structure theory for the convective envelopes of main-sequence stars to scale our simulations to the outer layers of stars in the F0--M0 spectral range, which allows us to estimate the unsigned magnetic flux on the surface of non-rotating reference stars. With these estimates we use the recent results of \citet{Pevtsov03} to predict the level of X-ray emission from such a turbulent dynamo, and find that our results compare well with observed lower limits of surface X-ray flux. If we scale our predicted X-ray fluxes to \ion{Mg}{2} fluxes we also find good agreement with the observed lower limit of chromospheric emission in K dwarfs. This suggests that dynamo action from a convecting, non-rotating plasma is a viable alternative to acoustic heating models as an explanation for the basal emission level seen in chromospheric, transition region, and coronal diagnostics from late-type stars.
description: ApJ, accepted, 30 pages with 7 figures
Is Einsteinian no-signalling violated in Bell Tests?
Creators: name: Kupczynski, Marian
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: Relativistic invariance is a physical law verified in several domains of physics. The impossibility of faster than light influences is not questioned by quantum theory. In quantum electrodynamics, in quantum field theory and in the standard model relativistic invariance is incorporated by construction. Quantum mechanics predicts strong long range correlations between outcomes of spin projection measurements performed in distant laboratories. In spite of these strong correlations marginal probability distributions should not depend on what was measured in the other laboratory what is called shortly: non-signalling. In several experiments, performed to test various Bell-type inequalities, some unexplained dependence of empirical marginal probability distributions on distant settings was observed . In this paper we demonstrate how a particular identification and selection procedure of paired distant outcomes is the most probable cause for this apparent violation of no-signalling principle. Thus this unexpected setting dependence does not prove the existence of superluminal influences and Einsteinian no-signalling principle has to be tested differently in dedicated experiments. We propose a detailed protocol telling how such experiments should be designed in order to be conclusive. We also explain how magical quantum correlations may be explained in a locally causal way.
description: 26 pages,2 figures, 23 equations, 107 references. It is a revised version in which some misprints were corrected and 4 references added. The paper was accepted for publication and will be published soon
Search for SUSY in Gauge Mediated and Anomaly Mediated Supersymmetry Breaking Models
Creators: name: Nunnemann, Thomas
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: In this note, recent results on the search for Gauge Mediated Supersymmetry Breaking (GMSB) and Anomaly Mediated Supersymmetry Breaking (AMSB) at the LEP and Tevatron colliders are summarized. We report on DZERO's search for GMSB in di-photon events with large missing transverse energy and discuss the sensitivity of similar searches based on future Tevatron integrated luminosities.
description: 3 pages, 4 pages, talk presented at the International Europhysics Conference on High Energy Physics EPS, July 17th-23rd 2003, Aachen, Germany
MOESM5 of Structural patterns of selection and diversity for Plasmodium vivax antigens DBP and AMA1
Creators: name: Guy, Andrew
name: Vashti Irani
name: Richards, Jack
name: Ramsland, Paul
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Science Policy
subject: 60506 Virology

description: Additional file 5. Spatially-derived nucleotide diversity for PvDBP across multiple populations.
วรรณยุกต์ภาษาไทยของผู้พูดภาษาลัวะ จังหวัดน่าน: การศึกษาทางกลสัทศาสตร์
Creators: name: ชมนาด อินทจามรรักษ์
Publisher: name: คณะศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์
Year: 2019
Subjects: วรรณยุกต์
สัทลักษณะ
ภาษาลัวะ
การออกเสียงภาษาไทย

description: วารสารศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์, 19, 2, 1-21
title: Inventaire des titres de propriété et des actes concernant les droits de l'abbaye de Morimond, Manuscrit n° 1, Bibliothèque municipale de Bourbonne-les-Bains, f.195
Creators: name: Rouzeau, Benoît
name: Rouzeau, Benoît
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cistercien
subject: cartulaire

description: Inventaire des titres de propriété et des actes concernant les droits de l'abbaye de Morimond, Manuscrit n° 1, Bibliothèque municipale de Bourbonne-les-Bains. Numérisation en mode image
description: Relation: https://cisterciensetressources.lamop.fr/
description: Bibliographic citation: Inventaire des titres de propriété et des actes concernant les droits de l'abbaye de Morimond, Manuscrit n° 1, Bibliothèque municipale de Bourbonne-les-Bains, f.195, in Projet Cisterciens et Ressources [Ressource en ligne], https://cisterciensetressources.lamop.fr
description: Inventaire des titres de propriété et des actes concernant les droits de l'abbaye de Morimond, Manuscrit n° 1, Bibliothèque municipale de Bourbonne-les-Bains, f. 195
Information diffusion in interconnected heterogeneous networks
Creators: name: Mahdizadehaghdam, Shahin
name: Wang, Han
name: Krim, Hamid
name: Dai, Liyi
Publisher: name: arXiv
Year: 2017
Subjects: subject: Social and Information Networks (cs.SI)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: In this paper, we are interested in modeling the diffusion of information in a multilayer network using thermodynamic diffusion approach. State of each agent is viewed as a topic mixture represented by a distribution over multiple topics. We have observed and learned diffusion-related thermodynamical patterns in the training data set, and we have used the estimated diffusion structure to predict the future states of the agents. A priori knowledge of a fraction of the state of all agents changes the problem to be a Kalman predictor problem that refines the predicted system state using the error in estimation of the agents. A real world Twitter data set is then used to evaluate and validate our information diffusion model.
description: 5-9 March 2017. arXiv admin note: substantial text overlap with arXiv:1602.04854
Phongsawadan Yonok: The Creation of a Modern Northern Thai Chronicle
Creators: name: Nittayaporn Prompanya
Publisher: name: คณะศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์
Year: 2019
Subjects: Phongsawadan Yonok
creation of the modern
northern Thai chronicle
significant features of modern writing

description: วารสารศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์, 19, 2, 22-52
Incorporating Structured Metacognitive Training into an Undergraduate Human Anatomy Course - Supplemental files
Creators: name: Ruth, Aidan
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 390110
subject: Medicine, nursing and health curriculum and pedagogy
classificationCode: 390113
subject: Science, technology and engineering curriculum and pedagogy

description: These files are supplements to a poster presented at the Anatomy Connected 2024 meeting entitled "Incorporating Structured Metacognitive Training into an Undergraduate Anatomy Classroom." It includes:Metacognitive prompts that designed for undergraduate human anatomy studentsSyllabus from Basic Human Anatomy course
Diverging Entanglement Length in Gapped Quantum Spin Systems
Creators: name: Verstraete, F.
name: Martin-Delgado, M. A.
name: Cirac, J. I.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We prove the existence of gapped quantum Hamiltonians whose ground states exhibit an infinite entanglement length, as opposed to their finite correlation length. Using the concept of entanglement swapping, the localizable entanglement is calculated exactly for valence bond and finitely correlated states, and the existence of the so--called string-order parameter is discussed. We also report on evidence that the ground state of an antiferromagnetic chain can be used as a perfect quantum channel if local measurements on the individual spins can be implemented.
description: 4 pages
Red giant branch stars as probes of stellar populations. II. Properties of the newly discovered globular cluster GLIMPSE-C01
Creators: name: Ivanov, Valentin D.
name: Kurtev, Radostin
name: Borissova, Jordanka
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Deep near infrared photometry of the newly discovered Galactic globular Cluster GLIMPSE-C01 is reported. We derived for the first time the metal abundance of this object from the slope of the RGB: [Fe/H]=-1.61+/-0.14 in the scale of Zinn (as implemented in Harris 1996), [Fe/H]=-1.44+/-0.12 in the scale of Caretta & Gratton (1997), and [Fe/H]=-1.12+/-0.12 in the scale of Ferraro et al. (1999). The tip and the clump of the red giant branch were used to confirm the estimates of Kobulnicky et al. (2005), placing the cluster at D~3.7+/-0.8 kpc, behind A_v~15 mag of visual extinction. The best fit to the radial surface brightness profile with a single-mass King's model (1962) yielded core radius r_c=0.78 arcmin, tidal radius r_t=27 arcmin, and central concentration c=1.54. Finally, we estimate the number of the "missing" globulars in the central region of the Milky Way. Based on the spatial distribution of the known clusters, and assuming radial symmetry around the Galactic center, we conclude that the Milky Way contains at least 10+/-3 undiscovered objects. The distribution of known clusters in the bulge seem to resemble the orientation of the Milky Way bar.
description: A&A accepted; 6 pages, 7 figures (one in jpg format, available upon request from the authors as postscript)
ปัจจัยความสำเร็จของร้านอาหารไทยภายใต้รางวัลมิชลินสตาร์
Creators: name: เจริญชัย เอกมาไพศาล
Publisher: name: คณะศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์
Year: 2019
Subjects: มิชลินสตาร์
ร้านอาหาร
ความสำเร็จ
อาหารไทย
พ่อครัว

description: วารสารศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์, 19, 2, 53-82
Recent Spin Physics at HERA
Creators: name: Ryckbosch, D.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Recent results from the HERMES experiment at HERA are described. The large data set from Run-I has yielded new information on the helicity structure of the nucleon. The data to be taken in Run-II will deal mainly with the transverse spin structure and with exclusive reactions.
description: Talk at the International Workshop on QCD: QCD@Work 2003 - Conversano (Italy) 14-18 June 2003 (eConf C030614)
Queering Confucian influences to better support queer Asian women from international student backgrounds in Australian and New Zealand higher education institutions
Creators: name: KAMAL, RAJA NUR ASHIKIN BINTE RAJA AHMAD
Publisher: name: Monash University
Year: 2024
Subjects: classificationCode: 390407
subject: Inclusive education
classificationCode: 440501
subject: Feminist and queer theory
classificationCode: 470202
subject: Asian cultural studies
classificationCode: 390303
subject: Higher education

description: This thesis addresses the underrepresentation of research on queer Asian women from international student backgrounds in Australian and New Zealand Higher Education Institutions (HEIs). It explores how four queer Asian women from international student backgrounds navigate HEIs through the lens of queering Confucianism, which critically evaluates the impact of Confucian values on their migration and HEI experiences. Additionally, interviews with three Diversity, Equity, and Inclusion (DEI) practitioners reveal barriers in supporting these women, including racism and tokenistic initiatives within DEI spaces in HEIs. The research emphasizes the importance of inclusive policies in HEIs.
Ultraviolet, Optical, and X-Ray Observations of the Type Ia Supernova 2005am with Swift
Creators: name: Brown, P. J.
name: Holland, S. T.
name: James, C.
name: Milne, P.
name: Roming, P. W. A.
name: Mason, K. O.
name: Page, K. L.
name: Beardmore, A. P.
name: Burrows, D.
name: Morgan, A.
name: Gronwall, C.
name: Blustin, A. J.
name: Boyd, P.
name: Still, M.
name: Breeveld, A.
name: de Pasquale, M.
name: Hunsberger, S.
name: Ivanushkina, M.
name: Landsman, W.
name: McGowan, K.
name: Poole, T.
name: Rosen, S.
name: Schady, P.
name: Gehrels, N.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present ultraviolet and optical light curves in six broadband filters and grism spectra obtained by Swift's Ultraviolet/Optical Telescope for the Type Ia supernova SN2005am. The data were collected beginning about four days before the B-band maximum, with excellent coverage of the rapid decline phase and later observations extending out to 69 days after the peak. The optical and near UV light curve match well those of SN1992A. The other UV observations constitute the first set of light curves shorter than 2500 Angstroms and allow us to compare the light curve evolution in three UV bands. The UV behavior of this and other low redshift supernovae can be used to constrain theories of progenitor evolution or to interpret optical light curves of high redshift supernovae. Using Swift's X-Ray Telescope, we also report the upper limit to SN2005am's X-ray luminosity to be 1.77 x 10^40 erg s^-1 in the 0.3--10 keV range from 58,117 s of exposure time.
description: 15 pages, including 3 figures and 2 tables, submitted to Astrophysical Journal
Signatures of unresolved binaries in stellar spectra: implications for spectral fitting
Creators: name: El-Badry, Kareem
name: Rix, Hans-Walter
name: Ting, Yuan-Sen
name: Weisz, Daniel R.
name: Bergemann, Maria
name: Cargile, Phillip
name: Conroy, Charlie
name: Eilers, Anna-Christina
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The observable spectrum of an unresolved binary star system is a superposition of two single-star spectra. Even without a detectable velocity offset between the two stellar components, the combined spectrum of a binary system is in general different from that of either component, and fitting it with single-star models may yield inaccurate stellar parameters and abundances. We perform simple experiments with synthetic spectra to investigate the effect of unresolved main-sequence binaries on spectral fitting, modeling spectra similar to those collected by the APOGEE, GALAH, and LAMOST surveys. We find that fitting unresolved binaries with single-star models introduces systematic biases in the derived stellar parameters and abundances that are modest but certainly not negligible, with typical systematic errors of $300\,\rm K$ in $T_{\rm eff}$, 0.1 dex in $\log g$, and 0.1 dex in $[\rm Fe/H]$ for APOGEE-like spectra of solar-type stars. These biases are smaller for spectra at optical wavelengths than in the near-infrared. We show that biases can be corrected by fitting spectra with a binary model, which adds only two labels to the fit and includes single-star models as a special case. Our model provides a promising new method to constrain the Galactic binary population, including systems with single-epoch spectra and no detectable velocity offset between the two stars.
description: Accept to MNRAS with minor revisions since v1. 7 pages, 5 figures
Quantum fluctuations and correlations of spatial scalar or multimode vector solitons in Kerr media
Creators: name: Lantz, Eric
name: Sylvestre, Thibaut
name: Maillote, Herve
name: Treps, Nicolas
name: Fabre, Claude
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We apply the Green's function method to determine the global degree of squeezing and the transverse spatial distribution of quantum fluctuations of solitons in Kerr media. We show that both scalar bright solitons and multimode vector solitons experience strong squeezing on the optimal quadrature. For vector solitons, this squeezing is shown to result from an almost perfect anti-correlation between the fluctuations on the two incoherently-coupled circular polarisations.
การจัดกิจกรรมการเรียนรู้ภาษาฝรั่งเศสเชิงรุกโดยใช้กระบวนการกลุ่ม
Creators: name: สิรจิตต์ เดชอมรชัย
Publisher: name: คณะศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์
Year: 2019
Subjects: การเรียนรู้เชิงรุก
กระบวนการกลุ่ม
ภาษาฝรั่งเศสระดับกลาง
กิจกรรมการเรียนรู้ภาษาฝรั่งเศส

description: วารสารศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์, 19, 2, 83-101
Charm-anticharm baryon production asymmetries in photon-nucleon interactions
Creators: name: FOCUS Collaboration
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We report measurements of the charm-anticharm production asymmetries for $Λ_c^+$, $Σ_c^{++}$, $Σ_c^0$, $Σ_c^{++*}$, $Σ_c^{0*}$, and $Λ_c^+(2625)$ baryons from the Fermilab photoproduction experiment FOCUS (E831). These asymmetries are integrated over the region where the spectrometer has good acceptance. In addition, we have obtained results for the photoproduction asymmetries of the $Λ_c$ baryons as functions of $p_L$, $p_T^2$, and $x_F$. The integrated asymmetry for $Λ_c^+$ production, $(σ_{Λ_c^+} - σ_{Λ_c^-}) / (σ_{Λ_c^+} + σ_{Λ_c^-})$, is $0.111 \pm 0.018 \pm 0.012$, significantly different from zero. The asymmetries of the excited states are consistent with the $Λ_c$ asymmetry.
description: 12 pages, 9 figures, 1 table
Jet physics of accreting super-massive black holes in the era of the Fermi Gamma-ray Space Telescope
Creators: name: D'Ammando, Filippo
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The Fermi Gamma-ray Space Telescope with its main instrument on-board, the Large Area Telescope (LAT), opened a new era in the study of high-energy emission from Active Galactic Nuclei (AGN). When combined with contemporaneous ground- and space-based observations, Fermi-LAT achieves its full capability to characterize the jet structure and the emission mechanisms at work in radio-loud AGN with different black hole mass and accretion rate, from flat spectrum radio quasars to narrow-line Seyfert 1 (NLSy1) galaxies. Here, I discuss important findings regarding the blazar population included in the third LAT catalog of AGN and the gamma-ray emitting NLSy1. Moreover, the detection of blazars at redshift beyond three in gamma rays allows us to constrain the growth and evolution of heavy black holes over cosmic time, suggesting that the radio-loud phase may be important for a fast black hole growth in the early Universe. Finally, results on extragalactic objects from the third catalog of hard LAT sources are presented.
description: 9 pages, 2 figures. Proceeding of the conference "Quasars at all cosmic epochs", Padova, 2017 April 2-7. Published on Frontiers in Astronomy and Space Sciences, Volume 4, 53 (2017)
Additional file 6: of Phylogenomics provides a robust topology of the major cnidarian lineages and insights on the origins of key organismal traits
Creators: name: Kayal, Ehsan
name: Bentlage, Bastian
name: M. Sabrina Pankey
name: Ohdera, Aki
name: Medina, Monica
name: Plachetzki, David
name: Collins, Allen
name: Ryan, Joseph
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Data occupancy mapped onto ML phylogeny for AG_62tx. (PDF 3275 kb)
ชุดความคิดว่าด้วย "อาเซียน" ที่นำเสนอผ่านภาษาในหนังสือการ์ตูนเสริมความรู้ชุดรอบรู้อาเซียน
Creators: name: ดีอนา คาซา
Publisher: name: คณะศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์
Year: 2019
Subjects: วาทกรรมวิเคราะห์เชิงวิพากษ์
ภาษากับความคิด
อาเซียน

description: วารสารศิลปศาสตร์ มหาวิทยาลัยธรรมศาสตร์, 19, 2, 102-132
Systematic Errors in Future Weak Lensing Surveys: Requirements and Prospects for Self-Calibration
Creators: name: Huterer, Dragan
name: Takada, Masahiro
name: Bernstein, Gary
name: Jain, Bhuvnesh
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the impact of systematic errors on planned weak lensing surveys and compute the requirements on their contributions so that they are not a dominant source of the cosmological parameter error budget. The generic types of error we consider are multiplicative and additive errors in measurements of shear, as well as photometric redshift errors. In general, more powerful surveys have stronger systematic requirements. For example, for a SNAP-type survey the multiplicative error in shear needs to be smaller than 1%(fsky/0.025)^{-1/2} of the mean shear in any given redshift bin, while the centroids of photometric redshift bins need to be known to better than 0.003(fsky/0.025)^{-1/2}. With about a factor of two degradation in cosmological parameter errors, future surveys can enter a self-calibration regime, where the mean systematic biases are self-consistently determined from the survey and only higher-order moments of the systematics contribute. Interestingly, once the power spectrum measurements are combined with the bispectrum, the self-calibration regime in the variation of the equation of state of dark energy w_a is attained with only a 20-30% error degradation.
description: 20 pages, 9 figures, to be submitted to MNRAS. Comments are welcome