cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Simple model for transport phenomena : Microscopic construction of Maxwell Demon like engine
Creators: name: Chaudhuri, Jyotipratim Ray
name: Chattopadhyay, Sudip
name: Banik, Suman Kumar
Publisher: name: arXiv
Year: 2007
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present a microscopic Hamiltonian framework to develop Maxwell demon like engine. Our model consists of a equilibrium thermal bath and a non-equilibrium bath; latter generated by driving with an external stationary, Gaussian noise. The engine we develop, can be considered as a device to extract work by modifying internal fluctuations. Our theoretical analysis focusses on finding the essential ingredients necessary for generating fluctuation induced transport under non-equilibrium condition. An important outcome of our model is that the net motion occurs when the non-linear bath is modulated by the external noise, creating the non-zero effective temperature even when the temperature of both the baths are same.
description: 6 pages, RevTex4
Tunable Fault Tolerance via Test and Reconfiguration
Creators: name: Blanton, Shawn
name: Goldstein, Seth C.
name: Schmit, Herman
Publisher: name: Carnegie Mellon University
Year: 2005
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: The advent of reconfigurable hardware as a computing medium creates a multi-dimensional design space where trade-offs between power, speed, cost, and reliability are now possible. Dynamic reconfiguration allows these trade-offs to be made on-line to adapt to various environmental changes. Furthermore, the cost of designing reliable circuits is greatly reduced since varying levels of reliability can be added to any circuit, even if it was not originally designed to run reliably, either at the time of application start-up or during application execution.
Additional file 3 of Inference about time-dependent prognostic accuracy measures in the presence of competing risks
Creators: name: Rajib Dey
name: Sebastiani, Giada
name: Saha-Chaudhuri, Paramita
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer

description: this file includes description files for using r code provided in Additional file 2 for estimating cause-specific aUC(t) using cWMR and cFPL estimators.
Oracle inequalities for the stochastic differential equations
Creators: name: Pchelintsev, Evgeny
name: Pergamenshchikov, Serguei
Publisher: name: arXiv
Year: 2017
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics
subject: 62G08, 62G05

description: This paper is a survey of recent results on the adaptive robust non parametric methods for the continuous time regression model with the semi - martingale noises with jumps. The noises are modeled by the Lévy processes, the Ornstein -- Uhlenbeck processes and semi-Markov processes. We represent the general model selection method and the sharp oracle inequalities methods which provide the robust efficient estimation in the adaptive setting. Moreover, we present the recent results on the improved model selection methods for the nonparametric estimation problems.
description: arXiv admin note: substantial text overlap with arXiv:1710.03111, arXiv:1611.07378
A further look at particle annihilation in dark matter caustics
Creators: name: Natarajan, Aravind
name: Sikivie, Pierre
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Dark matter caustics are small scale, high density structures believed to exist in galaxies like ours. If the dark matter consists of Weakly Interacting Massive Particles, these caustics may be detected by means of the gamma rays produced by dark matter particle annihilation. We discuss particle annihilation in outer and inner caustics and provide sky maps of the expected gamma ray distribution.
description: Minor changes, Introduction expanded, references added, accepted for publication in Phys. Rev. D
An Envelope Disrupted by a Quadrupolar Outflow in the Pre-Planetary Nebula IRAS19475+3119
Creators: name: Hsu, Ming-Chien
name: Lee, Chin-Fei
Publisher: name: arXiv
Year: 2011
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: IRAS 19475+3119 is a quadrupolar pre-planetary nebula (PPN), with two bipolar lobes, one in the east-west (E-W) direction and one in the southeast-northwest (SE-NW) direction. We have observed it in CO J=2-1 with the Submillimeter Array at ~ 1" resolution. The E-W bipolar lobe is known to trace a bipolar outflow and it is detected at high velocity. The SE-NW bipolar lobe appears at low velocity, and could trace a bipolar outflow moving in the plane of the sky. Two compact clumps are seen at low velocity around the common waist of the two bipolar lobes, spatially coincident with the two emission peaks in the NIR, tracing dense envelope material. They are found to trace the two limb-brightened edges of a slowly expanding torus-like circumstellar envelope produced in the late AGB phase. This torus-like envelope originally could be either a torus or a spherical shell, and it appears as it is now because of the two pairs of cavities along the two bipolar lobes. Thus, the envelope appears to be disrupted by the two bipolar outflows in the PPN phase.
description: 23 pages, 8 figures
Spontaneous emergence of self-replication in chemical reaction systems
Creators: name: Liu, Yu
name: Sumpter, David
Publisher: name: arXiv
Year: 2018
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Molecular Networks (q-bio.MN)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: Explaining the origin of life requires us to explain how self-replication arises. To be specific, how can a self-replicating entity develop spontaneously from a chemical reaction system in which no reaction is self-replicating? Previously proposed mathematical models either supply an explicit framework for a minimal living system or only consider catalyzed reactions, and thus fail to provide a comprehensive theory. We set up a general model for chemical reaction systems that properly accounts for energetics, kinetics and the conservation law. We find that (1) some systems are collectively-catalytic where reactants are transformed into end products with the assistance of intermediates (as in the citric acid cycle), while some others are self-replicating where different parts replicate each other and the system self-replicates as a whole (as in the formose reaction); (2) many alternative chemical universes often contain one or more such systems; (3) it is possible to construct a self-replicating system where the entropy of some parts spontaneously decreases, in a manner similar to that discussed by Schrödinger; (4) complex self-replicating molecules can emerge spontaneously and relatively easily from simple chemical reaction systems through a sequence of transitions. Together these results start to explain the origins of prebiotic evolution.
description: Supplementary Information (SI) attached. It is the pdf file "Supplementary.pdf" listed under "Ancillary files"
iSHELL PRV Follow-up of TESS Candidates
Creators: name: Mohammd, El Mufti
Publisher: name: Zenodo
Year: 2021
Subjects: precise near infrared (NIR) radial velocities (RVs)

description: We present our program of obtaining precise near infrared (NIR) radial velocities (RVs) with the R ~ 80,000 iSHELL spectrograph on the NASA Infrared Telescope Facility (IRTF) using a methane isotopolgue absorption gas cell in the calibration unit. Observing cool low mass stars provides a “Habitable Zone'' shortcut through their lower mass, effective temperature, and larger reflex velocities from orbiting bodies. It is advantageous to observe these stars at NIR wavelengths where they emit the bulk of their bolometric luminosity and are most quiescent from rotationally modulated stellar activity. Our RV pipeline (pychell) extracts RVs by forward modeling the observed spectra, where the stellar template is derived iteratively using the target observations themselves through averaging barycenter-shifted residuals. With iSHELL, we have aided in the confirmation of seven TOI systems (K and M dwarfs) with notably small semi-amplitudes [3-15 m/s]. We further highlight results from our multi-year monitoring of AU Mic with a variety of facilities (incl. iSHELL) where we are able to robustly detect planets with semi-amplitudes more than an order of magnitude below the stellar-activity level. 
Achieving buildability and robustness in precast concrete structures
Creators: name: Riedel, Kamil
Publisher: name: Imperial College London
Year: 2022

description: This research develops guidance on the rational assessment of structural robustness in precast concrete framing systems. The procedure evaluates first the behaviour of the local connections, followed by the global performance. The joint assessment is applied to two precast concrete framed building systems developed by Laing O'Rourke, namely, the M-Frame and the D-Frame. The robustness performance of the whole structure was done for the D-Frame system only. The M-Frame incorporates a beam-to-beam moment resisting connection which is designed to be stronger than the connected members. The connection consists of top and bottom connector plates, which are welded to vertical dowel bars which are embedded in the connected beams. Satisfactory behaviour of the connection was established through laboratory testing. Procedures are developed for the design and micro-modelling of the connection. The thesis defines this type of connection as "strong" since the flexural strength of the connection exceeds that of the connected beams. This characteristic makes it equivalent to a monolithic beam. The beams of the D-Frame are connected at a half-lapped joint, which was initially designed to meet the tie-based rules for robustness. The connection is defined as "weak" since following column removal, deformations are controlled by joint opening, with the connected precast members remaining relatively straight. Flexural continuity was initially provided by top and bottom plates, but preliminary analysis showed the joint to lack ductility. An alternative connection was developed in which continuity of flexural reinforcement across the joint is achieved using bespoke brackets. Laboratory testing showed that the extension of the connected bars can be controlled by debonding the bars to either side of the bespoke brackets. Localised failure by the bar bending was identified. A component-based model is developed to capture the response of the joint. Performance-based analysis of the whole D-Frame system is carried out. Sudden column removal is chosen as a threat-independent damaging event. The pseudo-static resistance is used as a measure of structural robustness. This was done at different structural idealisation levels to identify the contribution of individual members. The evaluation of different half-lapped joint connections was done for an individual damaged beam. The bracketed connector exhibited the highest performance. Spatial effects were then considered by modelling the entire floor system in 3D. It is shown that the proposed D-Frame system can arrest the progression of the damage under sudden column loss. Further optimisation of the system and connections is recommended.
Additional file 2 of Exploring the influence of socio-cultural factors and environmental resources on the health related quality of life of children and adolescents after congenital heart disease surgery: parental perspectives from a low middle income country
Creators: name: Ladak, Laila A.
name: Gallagher, Robyn
name: Hasan, Babar S.
name: Awais, Khadija
name: Abdullah, Ahmed
name: Gullick, Janice
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 2. Consolidated criteria for reporting qualitative studies (COREQ): 32-item checklist.
$L^p$ norms of higher rank eigenfunctions and bounds for spherical functions
Creators: name: Marshall, Simon
Publisher: name: arXiv
Year: 2011
Subjects: subject: Analysis of PDEs (math.AP)
subject: Number Theory (math.NT)
subject: Representation Theory (math.RT)
subject: FOS: Mathematics
subject: 22E30, 35P20

description: We prove almost sharp upper bounds for the $L^p$ norms of eigenfunctions of the full ring of invariant differential operators on a compact locally symmetric space, as well as their restrictions to maximal flat subspaces. Our proof combines techniques from semiclassical analysis with harmonic theory on reductive groups, and makes use of new asymptotic bounds for spherical functions that are of independent interest.
description: 57 pages, 1 figure. Substantially revised, and close to the published version
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00218
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/2017
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00218, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Exotic Exoplanets: Using NASA Exoplanet Archive data and Equilibrium Chemistry to predict an exoplanetary atmosphere with non-spontaneous syntheses of important basic molecules
Creators: name: Kalra, Archit
Publisher: name: Zenodo
Year: 2021
Subjects: Exoplanets
spontaneous reactions
equilibrium chemistry

description: Although some reactions such as the synthesis of water and carbon dioxide are spontaneous on Earth, there are a large number of exoplanets with atmospheres in which these reactions are nonspontaneous, indicating that they may not normally exist in the atmospheric composition of the exoplanet. Inversely, some reactions such as the synthesis of nitrogen dioxide are nonspontaneous on Earth, but may be spontaneous on an exoplanet. Here I use basic equilibrium chemistry to describe some attributes of possible exoplanets in which methane synthesis is nonspontaneous, in which case carbon may exist as graphite, as well as in an exoplanet with spontaneous ammonia synthesis, in which case important atmospheric processes may differ depending on how nitrogen interacts with other species present in the exoplanetary atmosphere. I cross-reference the average temperatures at which the reactions would have a standard Gibbs Free Energy of formation of 0 kJ/mol with the available equilibrium temperature data for discovered exoplanets and identify possible locations where the discussed reactions may be spontaneous or nonspontaneous.
On marginally outer trapped surfaces in stationary and static spacetimes
Creators: name: Carrasco, Alberto
name: Mars, Marc
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this paper we prove that for any spacelike hypersurface containing an untrapped barrier in a stationary spacetime satisfying the null energy condition, any marginally outer trapped surface cannot lie in the exterior region where the stationary Killing vector is timelike. In the static case we prove that any marginally outer trapped surface cannot penetrate into the exterior region where the static Killing vector is timelike. In fact, we prove these result at an initial data level, without even assuming existence of a spacetime. The proof relies on a powerful theorem by Andersson and Metzger on existence of an outermost marginally outer trapped surface.
description: 22 pages, 3 figures; 1 reference added, 1 figure changed, other minor changes
Matter-gravity interaction in a multiply warped braneworld,
Creators: name: Mukhopadhyaya, Biswarup
name: Sen, Somasri
name: SenGupta, Soumitra
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The role of a bulk graviton in predicting the signature of extra dimensions through collider-based experiments is explored in the context of a multiply warped spacetime. In particular it is shown that in a doubly warped braneworld model, the presence of the sixth dimension, results in enhanced concentration of graviton Kaluza Klein (KK) modes compared to that obtained in the usual 5-dimensional Randall-Sundrum model. Also, the couplings of these massive graviton KK modes with the matter fields on the visible brane turn out to be appreciably larger than that in the corresponding 5- dimensional model. The significance of these results are discussed in the context of KK graviton search at the Large Hadron Collider (LHC).
description: 13 pages, 2 tables
Additional file 1 of Exploring the influence of socio-cultural factors and environmental resources on the health related quality of life of children and adolescents after congenital heart disease surgery: parental perspectives from a low middle income country
Creators: name: Ladak, Laila A.
name: Gallagher, Robyn
name: Hasan, Babar S.
name: Awais, Khadija
name: Abdullah, Ahmed
name: Gullick, Janice
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 1. Semi structured interview guide for the parents.
Detection and measure of genuine tripartite entanglement with partial transposition and realignment of density matrices
Creators: name: Li, Ming
name: Wang, Jing
name: Shen, Shuqian
name: Chen, Zhihua
name: Fei, Shao-Ming
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: It is challenging task to detect and measure genuine multipartite entanglement. We investigate the problem by considering the average based positive partial transposition(PPT) criterion and the realignment criterion. Sufficient conditions for detecting genuine tripartite entanglement are presented. We also derive lower bounds for the genuine tripartite entanglement concurrence with respect to the conditions. While the PPT criterion and the realignment criterion are powerful for detecting bipartite entanglement and for providing lower bounds of bipartite concurrences, our results give an effective operational way to detect and measure the genuine tripartite entanglement.
description: 10 pages, 2 figures
Additional file 1 of Perceived stress and diet quality in women of reproductive age: a systematic review and meta-analysis
Creators: name: Khaled, Karim
name: Tsofliou, Fotini
name: Hundley, Vanora
name: Helmreich, Rebecca
name: Orouba Almilaji
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Table 1. Search strategy.
Tunable Fault Tolerance for Runtime Reconfigurable Architectures
Creators: name: Sinha, Steven K.
name: Kamarchik, Peter M.
name: Goldstein, Seth C.
Publisher: name: Carnegie Mellon University
Year: 1988
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Fault tolerance is becoming an increasingly important issue, especially in mission-critical applications where data integrity is a paramount concern. Performance, however, remains a large driving force in the market place. Runtime reconfigurable hardware architectures have the power to balance fault tolerance with performance, allowing the amount of fault tolerance to be tuned at run-time. This paper describes a new built-in self-test designed to run on, and take advantage of, runtime reconfigurable architectures using the PipeRench architecture as a model. In addition, this paper introduces a new metric by which a user can set the desired fault tolerance of a runtime reconfigurable device
Allesfitter in the Cloud: An All-in-One Classroom and Outreach Tool for Fitting TESS Data and More
Creators: name: Van Duzer, Aidan
name: Günther, Maximilian N.
name: Guerrero, Natalia
name: Daylan, Tansu
Publisher: name: Zenodo
Year: 2021
Subjects: Data Analysis Techniques
Allesfitter
Exoplanets
Teaching Tool

description: Inspiring the next generation of astronomers is an essential element of the TESS mission. However, in classroom or outreach settings, limited computing tools and programming knowledge can pose barriers to hands-on experiences. Allesfitter, a software package to analyze and model data from TESS and other missions, can provide an inclusive educational tool to engage students and public audiences. By hosting and running Allesfitter in the cloud in an easy-to-use Jupyter Notebook graphical interface, learners can model TESS light curves without prior coding knowledge or software installation, unveiling real astronomical events such as exoplanet transits or binary systems. A learner’s individual experience of modeling state-of-the-art TESS data, coupled with an instructor’s guidance, gives a compelling, visual insight into the exciting world of astronomy. Expanding Allesfitter’s usage into the classroom can help inspire a new generation to engage with public data from TESS and other missions.
Entanglement of charge transfer, hole doping, exchange interaction and octahedron tilting angle and their influence on the conductivity of La1-xSrxFe0.75Ni0.25O3-δ: A combination of x-ray spectroscopy and diffraction
Creators: name: Erat, Selma
name: Braun, Artur
name: Piamonteze, Cinthia
name: Liu, Zhi
name: Ovalle, Alejandro
name: Schindler, Hansjürgen
name: Graule, Thomas
name: Gauckler, Ludwig J.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Substitution of La by Sr in the 25% Ni doped charge transfer insulator LaFeO3 creates structural changes that inflect the electrical conductivity caused by small polaron hopping via exchange interactions and charge transfer. The substitution forms electron holes and a structural crossover from orthorhombic to rhombohedral symmetry, and then to cubic symmetry. The structural crossover is accompanied by a crossover from Fe3+-O2--Fe3+ superexchange interaction to Fe3+-O2--Fe4+ double exchange interaction, as evidenced by a considerable increase of conductivity. These interactions and charge transfer mechanism depend on superexchange angle, which approaches 180° upon increasing Sr concentration, leading an increased overlap between the O (2p) and Fe/Ni (3d) orbitals.
Additional file 1 of Prevalence of healthcare-associated infections and antimicrobial use among inpatients in a tertiary hospital in Fiji: a point prevalence survey
Creators: name: M. J. Loftus
name: S. J. Curtis
name: R. Naidu
name: A. C. Cheng
name: A. W. J. Jenney
name: B. G. Mitchell
name: P. L. Russo
name: E. Rafai
name: A. Y. Peleg
name: Stewardson, A. J.
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology

description: Additional file 1: Table S1. Summary of major differences in study protocol compared to ECDC protocol. Table S2. Additional questions to identify patients with clinician diagnosis of HAI that failed to meet ECDC criteria.
The Megamaser Cosmology Project. X. High Resolution Maps and Mass Constraint for SMBHs
Creators: name: Zhao, W.
name: Braatz, J. A.
name: Condon, J. J.
name: Lo, K. Y.
name: Reid, M. J.
name: Henkel, C.
name: Pesce, D. W.
name: Greene, J. E.
name: Gao, F.
name: Kuo, C. Y.
name: Impellizzeri, C. M. V.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present high resolution (sub-mas) VLBI maps of nuclear H2O megamasers for seven galaxies. In UGC6093, the well-aligned systemic masers and high-velocity masers originate in an edge-on, flat disk and we determine the mass of the central SMBH to be M_SMBH = 2.58*10^7Msun(+-7%). For J1346+5228, the distribution of masers is consistent with a disk, but the faint high-velocity masers are only marginally detected, and we constrain the mass of the SMBH to be in the range 1.5-2.0*10^7Msun. The origin of the masers in Mrk1210 is less clear, as the systemic and high-velocity masers are misaligned and show a disorganized velocity structure. We present one possible model in which the masers originate in a tilted, warped disk, but we do not rule out the possibility of other explanations including outflow masers. In NGC6926, we detect a set of redshifted masers, clustered within a pc of each other, and a single blueshifted maser about 4.4pc away, an offset that would be unusually large for a maser disk system. Nevertheless, if it is a disk system, we estimate the enclosed mass to be M_SMBH<4.8*10^7 Msun . For NGC5793, we detect redshifted masers spaced about 1.4pc from a clustered set of blueshifted features. The orientation of the structure supports a disk scenario as suggested by Hagiwara et al.(2001). We estimate the enclosed mass to be M SMBH<1.3*10^7 Msun. For NGC2824 and J0350-0127, the masers may be associated with pc or sub-pc scale jets or outflows.
description: Accepted by ApJ
Additional file 5 of Perceived stress and diet quality in women of reproductive age: a systematic review and meta-analysis
Creators: name: Khaled, Karim
name: Tsofliou, Fotini
name: Hundley, Vanora
name: Helmreich, Rebecca
name: Orouba Almilaji
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 5: Table 4. Data values extracted from the included studies on food intake and frequency of consumption: ↑ (increase), ↓ (decrease), <= > (no association).
Channel coding for Tb/s wireless communications: insights into code design and implementation
Creators: name: Douillard, Catherine
Publisher: name: Zenodo
Year: 2019
Subjects: Channel coding
Tb/s wireless communication

description: A presentation on "Channel coding for Tb/s wireless communications: insights into code design and implementation", which was given at the International Symposium on Ubiquitous Networking - UNet'19 in Limoges, France
The electromagnetic form factors of $Λ$ hyperon in $e^+e^-\rightarrow \barΛΛ$
Creators: name: Yang, Yongliang
name: Lu, Zhun
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the electromagnetic form factors of $Λ$ hyperon in the timelike region using the recent experimental data in the exclusive production of $\barΛ Λ$ pair in electron-position annihilation. We present a pQCD inspired parametrization of $G_E(s)$ and $G_M(s)$ with only two parameters, and we consider a suppression mechanism of the electric form factor $G_E(s)$ compared to the magnetic form factor $G_M(s)$. The parameters are determined through fitting our parametrization to the effective form factor data in the reaction $e^+e^-\rightarrow \barΛΛ$. Except the threshold region, our parametrization can reproduce satisfactorily the known behavior of the existing data from the BarBar, DM2 and BESIII Collaborations. We also predict the double spin polarization observables $A_{xx}$, $A_{yy}$ and $A_{zz}$ in $e^+e^-\rightarrow \barΛΛ$.
description: 5 pages, 3 figures
Additional file 2 of Perceived stress and diet quality in women of reproductive age: a systematic review and meta-analysis
Creators: name: Khaled, Karim
name: Tsofliou, Fotini
name: Hundley, Vanora
name: Helmreich, Rebecca
name: Orouba Almilaji
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2.
Spin Frustration and Magnetic Exchange in Cobalt Aluminum Oxide Spinels
Creators: name: Tristan, N.
name: Zestrea, V.
name: Behr, G.
name: Klingeler, R.
name: Buechner, B.
name: von Nidda, H. A. Krug
name: Loidl, A.
name: Tsurkan, V.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We report on x-ray diffraction, magnetic susceptibility, electron- spin resonance and heat- capacity studies of Co[Al_1-xCo_x]_2O_4 for Co concentrations 0 10 indicates the presence of strong spin frustration at least for x < 0.6. The frustration mechanism is attributed to competing nearest neighbor and next-nearest neighbor superexchange interactions between the A-site Co^2+ ions.
description: 19 pages, 9 figures, 46 references
The Effect of Accretion Environment at Large Radius on Hot Accretion Flows
Creators: name: Yang, Xiao-Hong
name: Bu, De-Fu
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study the effects of accretion environment (gas density, temperature and angular momentum) at large radii ($\sim 10$pc) on luminosity of hot accretion flows. The radiative feedback effects from the accretion flow on the accretion environment are also self-consistently taken into account. We find that the slowly rotating flows at large radii can significantly deviate from Bondi accretion when radiation heating and cooling are considered. We further find that when the temperature of environment gas is low (e.g. $T=2\times 10^7$K), the luminosity of hot accretion flows is high. When the temperature of gas is high (e.g. $T\geq4\times 10^7$K), the luminosity of hot accretion flow significantly deceases. The environment gas density can also significantly influence the luminosity of accretion flows. When density is higher than $\sim 4\times 10^{-22}\text{g} \text{cm}^{-3}$ and temperature is lower than $2\times 10^7$K, hot accretion flow with luminosity lower than $2\%L_{\text{Edd}}$ is not present. Therefore, the pc-scale environment density and temperature are two important parameters to determine the luminosity. The results are also useful for the sub-grid models adopted by the cosmological simulations.
description: Accepted for publication in MNRAS. 7 pages, 4 figures
Exploring Magneto-Meteorology with Ultra-Hot Jupiters Phase Curves from TESS
Creators: name: Jackson, Brian
name: Hindle, A.W.
name: Rogers, T. M.
name: Adams, Elisabeth R.
Publisher: name: Zenodo
Year: 2021
Subjects: Exoplanets
ultra-hot Jupiters
TESS Mission

description: Exoplanetary phase curves, light reflected and emitted by the planet as it orbits its star, have revealed exotic weather on these distant worlds. For example, blistering temperatures (~2000 K) on the cloudless daysides of ultra-hot Jupiters partially ionize the atmospheres, providing the magnetic field a handhold to sculpt weather. The resulting competition between transport of angular momentum, which can produce an equatorial jet, and magnetic stresses, a source of atmospheric drag, can drive the hottest region in the atmosphere back and forth across the sub-stellar point. Recent work using phase curves observed by the Kepler mission has shown that the phasing and amplitude of phase curves may therefore directly constrain the strength of an ultra-hot Jupiter’s magnetic field. Detections of ultra-hot Jupiter phase curves within TESS observations promise to expand the scope of magneto-meteorological studies. In this presentation, we explore the possibilities for constraining magnetic fields with observations of ultra-hot Jupiter phase curves from TESS.
Open/Closed Topological CP1 Sigma Model Revisited
Creators: name: Elitzur, Shmuel
name: Oz, Yaron
name: Rabinovici, Eliezer
name: Walcher, Johannes
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the topological sigma-model on Riemann surfaces with genus g and h holes, and target space CP1. We calculate the correlation functions of bulk and boundary operators, and study the symmetries of the model and its most general deformation. We study the open/closed topological field theory (TFT) correspondence by summing up the boundaries. We argue that this summation can be understood as a renormalization of the closed TFT. We couple the model to topological gravity and derive constitutive relations between the correlation functions of bulk and boundary operators.
description: 25 pages
Substrate limited electron dynamics in graphene
Creators: name: Fratini, S.
name: Guinea, F.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We study the effects of polarizable substrates such as SiO2 and SiC on the carrier dynamics in graphene. We find that the quasiparticle spectrum acquires a finite broadening due to the long-range interaction with the polar modes at the interface between graphene and the substrate. This mechanism results in a density dependent electrical resistivity, that exhibits a sharp increase around room temperature, where it can become the dominant limiting factor of electron transport. The effects are weaker in doped bilayer graphene, due to the more conventional parabolic band dispersion.
description: 4 pages, 3 figs. Corrected for spinor overlap factors
Probabilistic approach to a proliferation and migration dichotomy in the tumor cell invasion
Creators: name: Fedotov, Sergei
name: Iomin, Alexander
Publisher: name: arXiv
Year: 2007
Subjects: subject: Cell Behavior (q-bio.CB)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Biological sciences

description: The proliferation and migration dichotomy of the tumor cell invasion is examined within a two-component continuous time random walk (CTRW) model. The balance equations for the cancer cells of two phenotypes with random switching between cell proliferation and migration are derived. The transport of tumor cells is formulated in terms of the CTRW with an arbitrary waiting time distribution law, while proliferation is modelled by a logistic growth. The overall rate of tumor cell invasion for normal diffusion and subdiffusion is determined.
description: Accepted for publication as a Regular Article in Physical Review E
Disordered resonant media: Self-induced transparency versus light localization
Creators: name: Novitsky, Denis
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We propose a concept of disordered resonant media, which are characterized by random variations of their parameters along the light propagation direction. In particular, a simple model of disorder considered in the paper implies random change of the density of active particles (two-level atoms). Within this model, the effect of disorder on self-induced transparency (SIT) is analyzed using numerical simulations of light pulse propagation through the medium. The transition from the SIT to localization regime is revealed as well as its dependence on the disorder level, atom density, medium thickness, and period of random variations.
description: 7 pages, 8 figures
The Radius Valley as a by-product of Planet Formation: Observational Signatures of the Core-Powered Mass-Loss Mechanism
Creators: name: Gupta, Akash
name: Schlichting, Hilke
Publisher: name: Zenodo
Year: 2021
Subjects: Exoplanets
Atmospheres
Planet formation and evolution
Planet-star interactions
Radius valley

description: Observations have revealed a lack of planets of sizes ~1.5-2.0 Earth radii, i.e. a radius ‘valley’ or ‘gap’ in the size distribution of small, short-period exoplanets. This observation has been typically attributed to atmospheric mass-loss due to photoevaporation. However, in recent work, Ginzburg et al. (2018) and Gupta and Schlichting (2019, 2020) have demonstrated that atmospheric mass-loss, powered by the cooling luminosity of a planet and its host star’s bolometric luminosity, can also explain the origin of this radius valley, even in the absence of photoevaporation or any other process. In my talk, I will describe the key physical processes that drive this core-powered mass-loss mechanism followed by a comparison of our results with observations and the testable predictions we can make for the distribution of planets as a function of planet and host star properties. Finally, I will discuss our latest work where we present lists of planets that could be undergoing considerable atmospheric mass-loss or that might harbor secondary atmospheres abundant with high-molecular weight species, low-density interiors or both, if their evolution is indeed primarily dictated by core-powered mass-loss.
description: {"references": ["Owen & Wu 2013, ApJ, 775, 105", "Fulton et al. 2017, AJ, 154, 109", "Fulton & Petigura, 2018, AJ, 156, 264", "Ginzburg et al. 2018, MNRAS, 476, 759", "Gupta & Schlichting, 2019, MNRAS, 487, 24", "Gupta & Schlichting, 2020, MNRAS, 493, 792", "Gupta & Schlichting, 2021, MNRAS, 504, 4634", "Rogers, Gupta, Owen & Schlichting, 2021, arXiv:2105.03443", "Teske et al. 2020., AJ, 160, 96"]}
Non-binary turbo codes: design, simplified decoding and comparison with SoA codes
Creators: name: Klaimi, Rami
name: Abdel Nour, Charbel
name: Douillard, Catherine
Publisher: name: Zenodo
Year: 2019
Subjects: Non-binary Turbo codes
LDPC
FEC codes

description: A presentation on "Non-binary turbo codes: design, simplified decoding and comparison with SoA codes", which was given at the GdR ISIS workshop in Paris, France
X-rays from young stars - a summary of highlights from the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)
Creators: name: Guedel, M.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) is a survey of the nearest large star-forming region, the Taurus Molecular Cloud (TMC), making use of all instruments on board the XMM-Newton X-ray observatory. The survey, presently still growing, has provided unprecedented spectroscopic results from nearly every observed T Tauri star, and from ~50% of the studied brown dwarfs and protostars. The survey includes the first coherent statistical sample of high-resolution spectra of T Tauri stars, and is accompanied by an U-band/ultraviolet imaging photometric survey of the TMC. XEST led to the discovery of new, systematic X-ray features not possible before with smaller samples, in particular the X-ray soft excess in classical T Tauri stars and the Two-Absorber X-ray (TAX) spectra of jet-driving T Tauri stars. This paper summarizes highlights from XEST and reviews the key role of this large project.
description: 5 pages, 6 figures, accepted for "Astronomische Nachrichten"
Additional file 3 of Perceived stress and diet quality in women of reproductive age: a systematic review and meta-analysis
Creators: name: Khaled, Karim
name: Tsofliou, Fotini
name: Hundley, Vanora
name: Helmreich, Rebecca
name: Orouba Almilaji
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 3 Table 2. Characteristics extracted from the 24 included studies: BS (Breakfast skippers), BE (Breakfast eaters), CS (Cross-Sectional), LG (Longitudinal), y (years), m (months), FFQ (Food Frequency Questionnaire, WFR (Weigh food record), SES (Socioeconomic status), PA (Physical Activity), AM (Anthropometric measures), − (not reported).
The statistics of multi-planet systems
Creators: name: Tremaine, Scott
name: Dong, Subo
Publisher: name: arXiv
Year: 2011
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We describe statistical methods for measuring the exoplanet multiplicity function - the fraction of host stars containing a given number of planets - from transit and radial-velocity surveys. The analysis is based on the approximation of separability - that the distribution of planetary parameters in an n-planet system is the product of identical 1-planet distributions. We review the evidence that separability is a valid approximation for exoplanets. We show how to relate the observable multiplicity function in surveys with similar host-star populations but different sensitivities. We also show how to correct for geometrical selection effects to derive the multiplicity function from transit surveys if the distribution of relative inclinations is known. Applying these tools to the Kepler transit survey and radial-velocity surveys, we find that (i) the Kepler data alone do not constrain the mean inclination of multi-planet systems; even spherical distributions are allowed by the data but only if a small fraction of host stars contain large planet populations (> 30); (ii) comparing the Kepler and radial-velocity surveys shows that the mean inclination of multi-planet systems lies in the range 0-5 degrees; (iii) the multiplicity function of the Kepler planets is not well-determined by the present data.
description: 34 pages, 10 figures
Cosmological Parameter Estimation Using the Genus Amplitude - Application to Mock Galaxy Catalogs
Creators: name: Appleby, Stephen
name: Park, Changbom
name: Hong, Sungwook E.
name: Kim, Juhan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the topology of the matter density field in two dimensional slices, and consider how we can use the amplitude $A$ of the genus for cosmological parameter estimation. Using the latest Horizon Run 4 simulation data, we calculate the genus of the smoothed density field constructed from lightcone mock galaxy catalogs. Information can be extracted from the amplitude of the genus by considering both its redshift evolution and magnitude. The constancy of the genus amplitude with redshift can be used as a standard population, from which we derive constraints on the equation of state of dark energy $w_{\rm de}$ - by measuring $A$ at $z \sim 0.1$ and $z \sim 1$, we can place an order $Δw_{\rm de} \sim {\cal O}(15\%)$ constraint on $w_{\rm de}$. By comparing $A$ to its Gaussian expectation value we can potentially derive an additional stringent constraint on the matter density $ΔΩ_{\rm mat} \sim 0.01$. We discuss the primary sources of contamination associated with the two measurements - redshift space distortion and shot noise. With accurate knowledge of galaxy bias, we can successfully remove the effect of redshift space distortion, and the combined effect of shot noise and non-linear gravitational evolution is suppressed by smoothing over suitably large scales $R_{\rm G} \ge 15 {\rm Mpc}/h$. Without knowledge of the bias, we discuss how joint measurements of the two and three dimensional genus can be used to constrain the growth factor $β= f/b$. The method can be applied optimally to redshift slices of a galaxy distribution generated using the drop-off technique.
description: Published 01/2018. 15 pages, 10 figures
A Cluster Randomized Field Trial to Improve Social Norms for Behavior Change: Findings from the RANI Project in Odisha, India (Difference-in-difference analysis)
Creators: name: Rimal, Rajiv
name: Yilma, Hagere
name: Sedlander, Erica
name: Mohanty, Satyanarayan
name: Patro, Lipika
name: Pant, Ichhya
name: Khuntia, Srimant Kumar
name: Swain, Minati
name: Behera, Satyaranjan
Publisher: name: figshare
Year: 2021
Subjects: subject: 111712 Health Promotion
subject: FOS: Health sciences

description: In-depth explanation of difference-in-difference analyses in the Reduction of Anemia through Normative Innovations (RANI) Project's midterm findings
PDF dependence of Higgs cross sections at the Tevatron and LHC: response to recent criticism
Creators: name: Thorne, R. S.
name: Watt, G.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We respond to some criticism questioning the validity of the current Standard Model Higgs exclusion limits at the Tevatron, due to the significant dependence of the dominant production cross section from gluon-gluon fusion on the choice of parton distribution functions (PDFs) and the strong coupling (alpha_S). We demonstrate the ability of the Tevatron jet data to discriminate between different high-x gluon distributions, performing a detailed quantitative comparison to show that fits not explicitly including these data fail to give a good description. In this context we emphasise the importance of the consistent treatment of luminosity uncertainties. We comment on the values of alpha_S obtained from fitting deep-inelastic scattering data, particularly the fixed-target NMC data, and we show that jet data are needed for stability. We conclude that the Higgs cross-section uncertainties due to PDFs and alpha_S currently used by the Tevatron and LHC experiments are not significantly underestimated, contrary to some recent claims.
description: 44 pages, 19 figures. v2: version published in JHEP (paragraph added at bottom of p.15)
Diagnostic of electron temperature from bremsstrahlung in overdense targets
Creators: name: Hernández, Guillermo
name: Fernández, Francisco
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Models for characterization of laser-accelerated electron via its produced bremsstrahlung are provided for both thin and thick targets. An effective temperature functional is proposed to overcome the so-called cold and hot "temperatures" in the emission spectra, which are shown not to describe the underlying electron energy distribution. In contrast, this functional allows for identifying the real effect of a hot electron component. A false "heating" effect due to added noise is also exposed. The models are shown to be in good agreement with Monte Carlo simulations, as well as in good agreement with other experimental methods when applied to experimental data.