cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Using Heavy Quark Fragmentation into Heavy Hadrons to Determine QCD Parameters and Test Heavy Quark Symmetry
Creators: name: Randall, L.
name: Rius, N.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a detailed analysis of the use of heavy quark fragmentation into heavy hadrons for testing the heavy quark effective theory through comparison of the measured fragmentation parameters of the $c$ and $b$ quarks. Our analysis is entirely model independent. We interpret the known perturbative evolution in a way useful for exploiting heavy quark symmetry at low energy. We first show consistency with perturbative QCD scaling for measurements done solely with $c$ quarks. We then apply the perturbative analysis and the heavy quark expansion to relate measurements from ARGUS and LEP. We place bounds on a nonperturbative quark mass suppressed parameter, and compare the values for the $b$ and $c$ quarks. We find consistency with the heavy quark expansion but fairly sizable QCD uncertainties. We also suggest that one might reduce the systematic uncertainty in the result by not extrapolating to low $z$.
description: 26 pages in LaTeX, with 9 PostScript figures included (using epsf macros). MIT-CTP-2257
EFFECTS OF PROPRIOCEPTIVE TRAINING WITH PNF STRETCHING ON SELECTED MOTOR FITNESS COMPONENTS AMONG INTER-COLLEGIATE LEVEL FIELD HOCKEY PLAYERS
Creators: name: S. Nagaraj* & Dr. V. Saminathan**
Publisher: name: Zenodo
Year: 2025

description: The purpose of the study was to investigate effects of proprioceptive training with PNF stretching on selected motor fitness components among inter-collegiate level field hockey players. In this study, a total of thirty players were randomly selected from SRMV Maruthi College of Physical Education, Coimbatore, with ages ranging between 18 and 23 years. The participants were divided into two groups of fifteen each and assigned as control group and experimental group. The experimental treatment was applied only to the experimental group for a period of six weeks, while the control group did not receive any intervention. The proprioceptive training combined with PNF stretching was conducted thrice a week. After six weeks, the final performance of both the control and experimental groups was assessed. The significant differences between the pre-test and post-test scores of the experimental and control groups were determined using a dependent t-test. The level of significance was set at 0.05 for a degree of freedom of 1 and 14. The results indicated that the experimental group showed significant improvement in the selected motor fitness components.
Trochus perversus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Trochidae
Trochus
Trochus perversus

description: Trochus perversus [spec. nov.]
T. testa imperforata turrita glabra, anfractibus serie duplici excavato-punctatis.
Habitat in M. Mediterraneo.
Testa parva, anfractibus cylindricis duplici serie excavato punctatis, praeter margines anfractuum etiam crenato punctata. Apertura quadrata, columella basi prominula, at non in canalem evidentem. Color fere corneus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 760, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 2 of Weight change and risk of cardiovascular disease among adults with type 2 diabetes: more than 14 years of follow-up in the Tehran Lipid and Glucose Study
Creators: name: Moazzeni, Seyyed Saeed
name: Hizomi Arani, Reyhane
name: Deravi, Niloofar
name: Hasheminia, Mitra
name: Khalili, Davood
name: Azizi, Fereidoun
name: Hadaegh, Farzad
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Computational Biology

description: Additional file 2: Table S2. Multivariable hazard ratios (HR) and 95% confidence intervals (CI) of association between weight change categories and incident CVD with imputed baseline missing data for covariates (number: 1104 participants): Tehran Lipid and Glucose Study, Iran, 1999–2018.
Molecular Gas in the Powerful Radio Nucleus of the Ultraluminous Infrared Galaxy PKS 1345+12
Creators: name: Evans, A. S.
name: Kim, D. -C.
name: Mazzarella, J. M.
name: Scoville, N. Z.
name: Sanders, D. B.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Millimeter CO(1-0) interferometry and high resolution, Hubble Space Telescope (HST) 1.1, 1.6, and 2.2 micron imaging of the radio compact galaxy PKS 1345+12 are presented. With an infrared luminosity of 2x10^{12} L_sun, PKS 1345+12 is a prime candidate for studying the link between the ultraluminous infrared galaxy phenomenon and radio galaxies. These new observations probe the molecular gas distribution and obscured nuclear regions of PKS 1345+12 and provide morphological support for the idea that the radio activity in powerful radio galaxies is triggered by the merger of gas rich galaxies. Two nuclei separated by 2" (4.0 kpc) are observed in the near-infrared; the extended southeastern nucleus has colors consistent with reddened starlight, and the compact northwestern nucleus has extremely red colors indicative of an optical quasar with a warm dust component. Further, the molecular gas, 3mm continuum, and radio emission are coincident with the redder nucleus, confirming that the northwestern nucleus is the site of the AGN and that the molecular gas is the likely fuel source.
description: LaTex, 5 pages with 1 postscript and 1 jpg figure, ApJ Letters, in press (August 20, 1999)
Effects of unconventional breakup modes on incomplete fusion of weakly bound nuclei
Creators: name: Diaz-Torres, Alexis
name: Quraishi, Daanish
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The incomplete fusion dynamics of $^6$Li + $^{209}$Bi collisions at energies above the Coulomb barrier is investigated. The classical dynamical model implemented in the {\sc platypus} code is used to understand and quantify the impact of both $^6$Li resonance states and transfer-triggered breakup modes (involving short-lived projectile-like nuclei such as $^8$Be and $^5$Li) on the formation of incomplete fusion products. Model calculations explain the experimental incomplete-fusion excitation function fairly well, indicating that (i) delayed direct breakup of $^6$Li reduces the incomplete fusion cross-sections, and (ii) the neutron-stripping channel practically determines those cross-sections.
description: Accepted in Physical Review C
Additional file 1: of Recent trends, risk factors, and disparities in low birth weight in California, 2005–2014: a retrospective study
Creators: name: Anura Ratnasiri
name: Parry, Steven
name: Arief, Vivi
name: DeLacy, Ian
name: Halliday, Laura
name: DiLibero, Ralph
name: Basford, Kaye
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Science Policy

description: Table S1. Recorded births and percentage of births according to maternal characteristics and perinatal health behaviors in California for the period 2005–2014. Table S2. Likelihood of low birth weight listed as adjusted odds ratios (95% confidence intervals) for maternal age for each maternal race and ethnic group, after accounting for confounding effects in California for the period 2005–2014. Table S3. Likelihood of low birth weight listed as adjusted odds ratios (95% confidence intervals) for maternal education for each maternal race and ethnic group, after accounting for confounding effects in California for the period 2005–2014. (DOCX 52 kb)
Diffusion of Elements in the Interstellar Medium in Early-Type Galaxies
Creators: name: Medvedev, P.
name: Sazonov, S.
name: Gilfanov, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We consider the role of diffusion in the redistribution of elements in the hot interstellar medium (ISM) of early-type galaxies. It is well known that gravitational sedimentation can affect significantly the abundances of helium and heavy elements in the intracluster gas of massive galaxy clusters. The self-similarity of the temperature profiles and tight mass--temperature relation of relaxed cool-core clusters suggest that the maximum effect of sedimentation take place in the most massive virialized objects in the Universe. However, Chandra and XMM-Newton observations demonstrate more complex scaling relations between the masses of early-type galaxies and other parameters, such as the ISM temperature and gas mass fraction. An important fact is that early-type galaxies can show both decreasing and increasing radial temperature profiles. We have calculated the diffusion based on the observed gas density and temperature distributions for 13 early-type galaxies that belonging to the different environments and cover a wide range of X-ray luminosities. To estimate the maximum effect of sedimentation and thermal diffusion, we have solved the full set of Burgers' equations for a non-magnetized ISM plasma. The results obtained demonstrate a considerable increase of the He/H ratio within one effective radius for all galaxies of our sample. For galaxies with a flat or declining radial temperature profile the average increase of the helium abundance is 60\% in one billion years of diffusion. The revealed effect can introduce a significant bias in the metal abundance measurements based on X-ray spectroscopy and can affect the evolution of stars that could be formed from a gas with a high helium abundance.
description: 15 pages, 9 figures, 3 tables, published in Astronomy Letters, 2017, Volume 43, Issue 5, pp.285-303
The extended minimal geometric deformation of SU($N$) dark glueball condensates
Creators: name: Fernandes-Silva, A.
name: Ferreira-Martins, A. J.
name: da Rocha, R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The extended minimal geometric deformation (EMGD) procedure, in the holographic membrane paradigm, is employed to model stellar distributions that arise upon self-interacting scalar glueball dark matter condensation. Such scalar glueballs are SU($N$) Yang-Mills hidden sectors beyond the Standard Model. Then, corrections to the gravitational wave radiation, emitted by SU($N$) EMGD dark glueball stars mergers, are derived, and their respective spectra are studied in the EMGD framework, due to a phenomenological brane tension with finite value. The bulk Weyl fluid that drives the EMGD is then proposed to be experimentally detected by enhanced windows at the eLISA and LIGO.
description: 9 pages, 7 figures
Commensurate Scale Relations in Quantum Chromodynamics
Creators: name: Brodsky, Stanley J.
name: Lu, Hung Jung
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We use the BLM method to show that perturbatively-calculable observables in QCD can be related to each other without renormalization scale or scheme ambiguity. We define and study the commensurate scale relations. We show that the commensurate scales satisfy the renormalization group transitivity rule which ensures that predictions in PQCD are independent of the choice of an intermediate renormalization scheme. We generalize the BLM procedure to higher order. The application of this procedure to relate known physical observables in QCD gives surprisingly simple results. In particular, the annihilation ratio $R_{e^+e^-}$ and the Bjorken sum rule for polarized electroproduction are related through simple coefficients, which reinforces the idea of a hidden symmetry between these two observables.
description: 35 pages (RevTeX), one PostScript figure included at the end. SLAC-PUB-6481, UMD Preprint #94-135
Scheme for the protective measurement of a single photon using a tunable quantum Zeno effect
Creators: name: Schlosshauer, Maximilian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: This paper presents a proof-of-principle scheme for the protective measurement of a single photon. In this scheme, the photon is looped arbitrarily many times through an optical stage that implements a weak measurement of a polarization observable followed by a strong measurement protecting the state. The ability of this scheme to realize a large number of such interaction-protection steps means that the uncertainty in the measurement result can be drastically reduced while maintaining a sufficient probability for the photon to survive the measurement.
description: 5 pages, 1 figure
Air Showers and Geomagnetic Field
Creators: name: Cillis, A.
name: Sciutto, S. J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The influence of the geomagnetic field on the development of air showers is studied. The well known International Geomagnetic Reference Field was included in the AIRES air shower simulation program as an auxiliary tool to allow calculating very accurate estimations of the geomagnetic field given the geographic coordinates, altitude above sea level and date of a given event. Our simulations indicate that the geomagnetic deflections alter significantly some shower observables like, for example, the lateral distribution of muons in the case of events with large zenith angles (larger than 75 degrees). On the other hand, such alterations seem not to be important for smaller zenith angles. Global observables like total numbers of particles or longitudinal development parameters do not present appreciable dependences on the geomagnetic deflections for all the cases that were studied.
description: 16 pages, 9 figures. Corrected some typos
Trochus punctatus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Trochidae
Trochus
Trochus punctatus

description: Trochus punctatus [spec. nov.]
T. testa imperforata turrita, anfractibus serie triplici punctorum prominentium.
Habitat in Europa australi.
Testa magnitudine praecedentis s. Hordei, ferruginea undique punctis obtusis eminentibus obtecta, in singulo anfractu serie triplici, quarum intermedia minor est. Apertura quadrata cum columella prominula, vix manifeste canaliculata.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 760, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1 of Clinical phenotypes and prognostic factors of adult-onset Still’s disease: data from a large inpatient cohort
Creators: name: Li, Rui
name: Liu, Xiaolei
name: Chen, Guangliang
name: Tang, Guo
name: Chen, Xiaoxiang
name: Liu, Xuesong
name: Wang, Juan
name: Lu, Liangjing
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1: Supplementary Figure 1. Flow chart of patient selection, clustering and follow-up. Supplementary Figure 2. Visualization of the three-subgroup model. Each dot represents a patient, and each colour represents a cluster. Supplementary Table 1. Comparison of second-line treatments used in different clusters of AOSD patients. Supplementary Table 2. Comparison of the prognosis of the three distinct AOSD patient clusters. Supplementary Table 3. Survival of the three subgroups patients. Supplementary Table 4. Raw data of patients completed follow-up.
Investigating particle emissions and aerosol dynamics from a consumer fused deposition modeling 3D printer with a lognormal moment aerosol model
Creators: name: Zhang, Qian
name: Sharma, Girish
name: P. S. Wong, Jenny
name: Davis, Aika Y.
name: Black, Marilyn S.
name: Biswas, Pratim
name: Weber, Rodney J.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences

description: Particle emissions from consumer-fused deposition modeling 3D printers have been reported previously; however, the complex processes leading to observed aerosols have not been investigated. We measured particle concentrations and size distributions between 7 nm and 25 μm emitted from a 3D printer under different conditions in an emission test chamber. The experimental data was combined with a moment lognormal aerosol dynamic model to better understand particle formation and subsequent evolution mechanisms. The model was based on particles being formed from nucleation of unknown semivolatile compounds emitted from the heated filament during printing, which evolve due to condensation of emitted vapors and coagulation, all within a small volume near the printer extruder nozzle. The model captured observed steady state particle number size distribution parameters (total number, geometric mean diameter and geometric standard deviation) with errors nominally within 20%. Model solutions provided a range of vapor generation rates, saturation vapor pressures and vapor condensation factors consistent with measured steady state particle concentrations and size distributions. Vapor generation rate was a crucial factor that was linked to printer extruder temperature and largely accounted for differences between filament material and brands. For the unknown condensing vapor species, saturation vapor pressures were in the range of 10−3 to 10−1 Pa. The model suggests particles could be removed by design of collection surfaces near the extruder tip. Copyright © 2018 American Association for Aerosol Research
Additional file 2: of Functional insights into the infective larval stage of Anisakis simplex s.s., Anisakis pegreffii and their hybrids based on gene expression patterns
Creators: name: C. Llorens
name: S. Arcos
name: L. Robertson
name: R. Ramos
name: R. Futami
name: B. Soriano
name: S. Ciordia
name: M. Careche
name: M. González-Muñoz
name: Y. Jiménez-Ruiz
name: N. Carballeda-Sangiao
name: I. Moneo
name: J. Albar
name: M. Blaxter
name: A. Navas
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: List of species and specimen used in the phylogenetic tree of Additional file 1. Code of the voucher specimen and accession number for mitochondrial gene COII (*: sequences obtained from GenBank). Labeled are the specimens selected for RNA sequencing (first number, population; second number specimen). A. simplex s.s. – A. pegreffii refers to hybrids haplotype according Abollo et al. [23]. (DOCX 47 kb)
Additional file 4: of Breast cancer patients suggestive of Li-Fraumeni syndrome: mutational spectrum, candidate genes, and unexplained heredity
Creators: name: Penkert, Judith
name: Schmidt, Gunnar
name: Hofmann, Winfried
name: Schubert, Stephanie
name: Schieck, Maximilian
name: Auber, Bernd
name: Ripperger, Tim
name: Hackmann, Karl
name: Sturm, Marc
name: Prokisch, Holger
name: Hille-Betz, Ursula
name: Mark, Dorothea
name: Illig, Thomas
name: Schlegelberger, Brigitte
name: Steinemann, Doris
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: 60506 Virology

description: Total list of TP53 (NM_000546.5) variants detected via NGS-based sequencing (entire list of all detected TP53 variants in our collective). (DOCX 35Â kb)
An LTE effective temperature scale for red supergiants in the Magellanic clouds
Creators: name: Tabernero, H. M.
name: Dorda, R.
name: Negueruela, I.
name: Gonzalez-Fernandez, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a self-consistent study of cool supergiants (CSGs) belonging to the Magellanic clouds. We calculated stellar atmospheric parameters using LTE KURUCZ and MARCS atmospheric models for more than 400 individual targets by fitting a careful selection of weak metallic lines. We explore the existence of a T eff scale and its implications in two different metallicity environments (each Magellanic cloud). Critical and in-depth tests have been performed to assess the reliability of our stellar parameters (i.e. internal error budget, NLTE systematics). In addition, several Montercarlo tests have been carried out to infer the significance of the Teff scale found. Our findingspoint towards a unique Teff scale that seems to be independent of the environment.
description: Accepted for publication in MNRAS
Additional file 3 of Weight change and risk of cardiovascular disease among adults with type 2 diabetes: more than 14 years of follow-up in the Tehran Lipid and Glucose Study
Creators: name: Moazzeni, Seyyed Saeed
name: Hizomi Arani, Reyhane
name: Deravi, Niloofar
name: Hasheminia, Mitra
name: Khalili, Davood
name: Azizi, Fereidoun
name: Hadaegh, Farzad
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Computational Biology

description: Additional file 3: Table S3. Multivariable hazard ratios (HR) and 95% confidence intervals (CI) of association between weight change categories and incident CHD with imputed baseline missing data for covariates (number: 1104 participants): Tehran Lipid and Glucose Study, Iran, 1999–2018.
Additional file 3 of Benchmarking hybrid assembly approaches for genomic analyses of bacterial pathogens using Illumina and Oxford Nanopore sequencing
Creators: name: Chen, Zhao
name: Erickson, David L.
name: Meng, Jianghong
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Table S3. Thirty strains of Pseudomonas aeruginosa.
Trochus striatellus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Trochidae
Trochus
Trochus striatellus

description: Trochus striatellus [spec. nov.]
T. testa turrita imperforata: striis longitudinalibus parallelis obliquatis.
Habitat in M. Mediterraneo.
Testa admodum parva, subulata, alba, apice violacea.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 760, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Probing the density dependence of the symmetry energy by nucleon flow
Creators: name: Fan, Xiao-Hua
name: Yong, Gao-Chan
name: Zuo, Wei
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: In the framework of the isospin-dependent Boltzmann-Uehling-Uhlenbeck transport model, sensitive regions of some nucleon observables to the nuclear symmetry energy are studied. It is found that the symmetry energy sensitive observable n/p ratio in the $^{132}$Sn+$^{124}$Sn reaction at 0.3 GeV/nucleon in fact just probes the density-dependent symmetry energy below the density of $1.5ρ_0$ and effectively probes the density-dependent symmetry energy around or somewhat below the saturation density. Nucleon elliptic flow can probe the symmetry energy from the low-density region to the high-density region when changing the incident beam energies from 0.3 to 0.6 GeV/nucleon in the semi-central $^{132}$Sn+$^{124}$Sn reaction. And nucleon transverse and elliptic flows in the semi-central $^{197}$Au+$^{197}$Au reaction at 0.6 GeV/nucleon are more sensitive to the high-density behavior of the nuclear symmetry energy. One thus concludes that nucleon observables in the heavy reaction system and with higher incident beam energy are more suitable to be used to probe the high-density behavior of the symmetry energy. The present study may help one to get more specific information about the density-dependent symmetry energy from nucleon flow observable in heavy-ion collisions at intermediate energies.
description: 5 pages, 6 figures
Electroweak corrections to the $H\to t\bar{t}$ decay rate
Creators: name: Chen, Xiao-Xi
name: Ma, Wen-Gan
name: Liu, Yao-Yang
name: Sun, La-Zhen
name: Chang, Chao-Hsi
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The electroweak corrections at one-loop level to the process $H\rightarrow t{\bar t}$ are calculated, especially the fresh top mass value announced recently by CDF is concerned. For $M_H < 1. TeV$ where a perturbative calculation is valid, the corrections themselves would gain a few to 20 percent increment in the decay width as the Higgs mass $M_H$ is increasing within the region, but they are in opposite direction to the QCD ones. If the electroweak and QCD corrections are concerned in the meantime, the resultant decay width of the mode yields a reduction about a few percent of the tree level one.
description: 18, a new version#
Additional file 3: of Breast cancer patients suggestive of Li-Fraumeni syndrome: mutational spectrum, candidate genes, and unexplained heredity
Creators: name: Penkert, Judith
name: Schmidt, Gunnar
name: Hofmann, Winfried
name: Schubert, Stephanie
name: Schieck, Maximilian
name: Auber, Bernd
name: Ripperger, Tim
name: Hackmann, Karl
name: Sturm, Marc
name: Prokisch, Holger
name: Hille-Betz, Ursula
name: Mark, Dorothea
name: Illig, Thomas
name: Schlegelberger, Brigitte
name: Steinemann, Doris
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: 60506 Virology
subject: Computational Biology

description: Pedigrees of investigated families with (likely) pathogenic variants (pedigrees of all families of carriers of pathogenic or likely pathogenic variants in our cohort, including age of onset of malignant disease). (DOCX 692Â kb)
Galactic Fountains and Galactic Winds
Creators: name: Breitschwerdt, Dieter
name: Komossa, Stefanie
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The development of galactic fountain theories is reviewed with special emphasis on the different approaches and concepts that have been used in the past. In particular the outstanding contribution of Franz Kahn to our physical understanding is appreciated. It is argued that galactic outflows represent an essential phase during galaxy evolution. The dynamics of the outflow imprints its signature on the emission spectra of soft X-rays, which may well be observable with AXAF and XMM. Finally, some remarks about winds in starburst galaxies and AGN are made.
description: 12 pages; contribution to the proceedings of "Astrophysical Dynamics" (Evora, April 1999; in honour of Franz Kahn), D. Berry, D. Breitschwerdt, A. da Costa, J. Dyson (eds); to appear in Ap&SS
Multiple-target robust design with multiple functional outputs
Creators: name: Jiang, Fan
name: Tan, Matthias Hwai Yong
name: Tsui, Kwok-Leung
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Robust Parameter Design (RPD) is a quality improvement method to mitigate the effect of input noise on system output quality via adjustment of control and signal factors. This article considers RPD with multiple functional outputs and multiple target functions based on a time-consuming nonlinear simulator, which is a challenging problem rarely studied in the literature. The Joseph–Wu formulation of multi-target RPD as an optimization problem is extended to accommodate multiple functional outputs and use of a Gaussian Process (GP) emulator for the outputs. Due to computational demands in emulator fitting and expected loss function estimation posed by this big-data problem, a separable GP model is used. The separable regression and prior covariance functions, and the Cartesian product structure of the data are exploited to derive computationally efficient formulas for the posterior means of expected loss criteria for optimizing signal and control factors, and to develop a fast Monte Carlo procedure for building credible intervals for the criteria. Our approach is applied to an example on RPD of a coronary stent for treating narrowed arteries, which allows the optimal signal and control factor settings to be estimated efficiently. Supplementary materials are available for this article. Go to the publisher’s online edition of IISE Transactions, datasets, additional tables, detailed proofs, etc.
Stabilization of the arrival time of a relativistic electron beam to the 50 fs level
Creators: name: Roberts, J.
name: Skowronski, P.
name: Burrows, P. N.
name: Christian, G. B.
name: Corsini, R.
name: Ghigo, A.
name: Marcellini, F.
name: Perry, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: We report the results of a low-latency beam phase feed-forward system built to stabilize the arrival time of a relativistic electron beam. The system was operated at the Compact Linear Collider (CLIC) Test Facility (CTF3) at CERN where the beam arrival time was stabilized to approximately 50 fs. The system latency was 350 ns and the correction bandwidth >23 MHz. The system meets the requirements for CLIC.
description: 5 pages, 9 figures, 1 table
Dynamical Stability of Witten Rings
Creators: name: Martin, X.
name: Peter, P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The dynamical stability of cosmic rings, or vortons, is investigated for the particular equation of state given by the Witten bosonic model. It is found that there exists a finite range of the state parameter for which the vorton states are actually stable against dynamical perturbations. Inclusion of the electromagnetic self action into the equation of state slightly shrinks the stability region but otherwise yields no qualitative difference. If the Witten bosonic model represents a good approximation for more realistic string models, then the cosmological vorton excess problem can only be solved by assuming either that strings are formed at low energy scales or that some quantum instability may develop at a sufficient rate.
description: 11 pages, LaTeX-ReVTeX (v.3), 2 figures available upon request, DAMTP R-94/19
Turbo obtusatus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Turbinidae
Turbo
Turbo obtusatus

description: Turbo obtusatus [spec. nov.]
T. testa subrotunda laevi: superne ventricosiore obtusissima, margine columnari plano.
Habitat in O. Septentrionali.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 761, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Gravitationally unstable condensations revealed by ALMA in the TUKH122 prestellar core in the Orion A cloud
Creators: name: Ohashi, Satoshi
name: Sanhueza, Patricio
name: Sakai, Nami
name: Kandori, Ryo
name: Choi, Minho
name: Hirota, Tomoya
name: Luong, Quang Nguyen
name: Tatematsu, Ken'ichi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have investigated the TUKH122 prestellar core in the Orion A cloud using ALMA 3 mm dust continuum, N$_2$H$^+$ ($J=1-0$), and CH$_3$OH ($J_K=2_K-1_K$) molecular line observations. Previous studies showed that TUKH122 is likely on the verge of star formation because the turbulence is almost dissipated and chemically evolved among other starless cores in the Orion A cloud. By combining ALMA 12-m and ACA data, we recover extended emission with a resolution of $\sim5"$ corresponding to 0.01 pc and identify 6 condensations with a mass range of $0.1-0.4$ $M_\odot$ and a radius of $\lesssim0.01$ pc. These condensations are gravitationally bound following a virial analysis and are embedded in the filament including the elongated core with a mass of $\sim29$ $M_\odot$ and a radial density profile of $r^{-1.6}$ derived by {\it Herschel}. The separation of these condensations is $\sim0.035$ pc, consistent with the thermal jeans length at a density of $4.4\times10^5$ cm$^{-3}$. This density is similar to the central part of the core. We also find a tendency that the N$_2$H$^+$ molecule seems to deplete at the dust peak condensation. This condensation may be beginning to collapse because the linewidth becomes broader. Therefore, the fragmentation still occurs in the prestellar core by thermal Jeans instability and multiple stars are formed within the TUKH122 prestellar core. The CH$_3$OH emission shows a large shell-like distribution and surrounds these condensations, suggesting that the CH$_3$OH molecule formed on dust grains is released into gas phase by non-thermal desorption such as photoevaporation caused by cosmic-ray induced UV radiation.
description: 13 pages, 14 figures, 2 tables, accepted for publication in ApJ
A case devoid of bias: ORS voids vs. IRAS voids
Creators: name: El-Ad, Hagai
name: Piran, Tsvi
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a comparison between the voids in two nearly all sky redshift surveys: the ORS and the IRAS 1.2 Jy. While the galaxies in these surveys are selected differently and their populations are known to be biased relative to each other, the two void distributions are similar. We compare the spatial distribution of the two void populations and demonstrate the correlation between them. The voids also agree with regard to the overall void statistics -- a filling factor of ~0.45 of the volume, an average void diameter ~45/h Mpc and an average galaxy underdensity in the voids of approximately -0.9. Our measurements of the underdensities of the voids in the two surveys enable us to estimate the relative bias in the voids between optical and IRAS samples. We find b(opt) / b(IRAS) ~ 1, showing that on average there is little -- or no -- biasing between the two void populations.
description: Submitted to MNRAS; 6 pages, MN LaTeX file using epsfig, 3 tables, 3 PS figures. Complete gzipped version is available at http://merger.fiz.huji.ac.il/~eladh
Comparing Clinical Judgment with MySurgeryRisk Algorithm for Preoperative Risk Assessment: A Pilot Study
Creators: name: Brennan, Meghan
name: Puri, Sahil
name: Ozrazgat-Baslanti, Tezcan
name: Bhat, Rajendra
name: Feng, Zheng
name: Momcilovic, Petar
name: Li, Xiaolin
name: Wang, Daisy Zhe
name: Bihorac, Azra
Publisher: name: arXiv
Year: 2018
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: Background: Major postoperative complications are associated with increased short and long-term mortality, increased healthcare cost, and adverse long-term consequences. The large amount of data contained in the electronic health record (EHR) creates barriers for physicians to recognize patients most at risk. We hypothesize, if presented in an optimal format, information from data-driven predictive risk algorithms for postoperative complications can improve physician risk assessment. Methods: Prospective, non-randomized, interventional pilot study of twenty perioperative physicians at a quarterly academic medical center. Using 150 clinical cases we compared physicians' risk assessment before and after interaction with MySurgeryRisk, a validated machine-learning algorithm predicting preoperative risk for six major postoperative complications using EHR data. Results: The area under the curve (AUC) of MySurgeryRisk algorithm ranged between 0.73 and 0.85 and was significantly higher than physicians' risk assessments (AUC between 0.47 and 0.69) for all postoperative complications except cardiovascular complications. The AUC for repeated physician's risk assessment improved by 2% to 5% for all complications with the exception of thirty-day mortality. Physicians' risk assessment for acute kidney injury and intensive care unit admission longer than 48 hours significantly improved after knowledge exchange, resulting in net reclassification improvement of 12.4% and 16%, respectively. Conclusions: The validated MySurgeryRisk algorithm predicted postoperative complications with equal or higher accuracy than pilot cohort of physicians using available clinical preoperative data. The interaction with algorithm significantly improved physicians' risk assessment.
description: 21 pages, 4 tables
Turbo neritoides Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Turbinidae
Turbo
Turbo neritoides

description: Turbo neritoides [spec. nov.]
T. testa ovata glabra obtusiuscula, margine columnari plano.
Gvalt. test. t. 45. f. F.
Habitat in M. Mediterraneo.
Testa Neritis maxime affinis. Minutus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 761, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1: of m-Power Heart Project - a nurse care coordinator led, mHealth enabled intervention to improve the management of hypertension in India: study protocol for a cluster randomized trial
Creators: name: Venkateshmurthy, Nikhil Srinivasapura
name: Vamadevan Ajay
name: Sailesh Mohan
name: Devraj Jindal
name: Shuchi Anand
name: Kondal, Dimple
name: Tandon, Nikhil
name: Malipeddi Rao
name: Dorairaj Prabhakaran
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Standard Protocol Items: Recommendations for Interventional Trials (SPIRIT) 2013 Checklist: recommended items to address in a clinical trial protocol and related documents*. (DOCX 49 kb)
Non Intercommuting Configurations in the Collisions of Type-I $U(1)$ Cosmic Strings
Creators: name: Bettencourt, L. M. A.
name: Kibble, T. W. B.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that for small relative angle and kinetic energy two type I $U(1)$ strings can form bound states upon collision instead of the more familiar intercommuting configuration. The velocity below which this may happen is estimated as function of the ratio of the coupling constants in the theory, crossing angle and initial kinetic energy.
description: 12 pages,REVTEX, Imperial/TP/93-94/34
Additional file 1 of Association between childhood trauma and medication adherence among patients with major depressive disorder: the moderating role of resilience
Creators: name: Wang, Hongqiong
name: Liao, Yuhua
name: Guo, Lan
name: Zhang, Huimin
name: Zhang, Yingli
name: Lai, Wenjian
name: Teopiz, Kayla M.
name: Song, Weidong
name: Zhu, Dongjian
name: Li, Lingjiang
name: Lu, Ciyong
name: Fan, Beifang
name: McIntyre, Roger S.
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Additional file 1: eTable 1. Baseline sample characteristics between eligible and ineligible participants. eTable 2. Frequencies of responses on the MARS among the suboptimal adherence group (n=234). eFigure 1. The distribution of suboptimal adherence in the low, medium and high resilience group.
Additional file 1 of Medication safety knowledge, attitude, and practice among hospital pharmacists in tertiary care hospitals in Saudi Arabia: a multi-center study
Creators: name: AL-Mutairi, Azizah
name: AlFayyad, Isamme
name: Altannir, Youssef
name: Al-Tannir, Mohamad
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Science Policy
subject: Cancer

description: Additional file 1.
Additional file 1: of Associations and prognostic significance of diffuse myocardial fibrosis by cardiovascular magnetic resonance in heart failure with preserved ejection fraction
Creators: name: Roy, Clotilde
name: Slimani, Alisson
name: Meester, Christophe De
name: Amzulescu, Mihaela
name: Pasquet, Agnes
name: Vancraeynest, David
name: Beauloye, Christophe
name: Jean-Louis Vanoverschelde
name: Gerber, Bernhard
name: Anne-Catherine Pouleur
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer

description: Risk score. (DOCX 62 kb)
Research and Implementation of Global Path Planning for Unmanned Surface Vehicle Based on Electronic Chart
Creators: name: Wang, Yanlong
name: Liang, Xu
name: Li, Baoan
name: Yu, Xuemin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: Unmanned Surface Vehicle (USV) is a new type of intelligent surface craft, and global path planning is the key technology of USV research, which can reflect the intelligent level of USV. In order to solve the problem of global path planning of USV, this paper proposes an improved A* algorithm for sailing cost optimization based on electronic charts. This paper uses the S-57 electronic chart to realize the establishment of the octree grid environment model, and proposes an improved A* algorithm based on sailing safety weight, pilot quantity and path curve smoothing to ensure the safety of the route, reduce the planning time, and improve path smoothness. The simulation results show that the environmental model construction method and the improved A* algorithm can generate safe and reasonable global path.
description: 7 pages, 3 figures, conference
Turbo littoreus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Turbinidae
Turbo
Turbo littoreus

description: Turbo littoreus [spec. nov.]
T. testa subovata acuta striata, margine columnari plano.
It. wgoth. 169, 199. t. 5. f. 3.
List. angl. 162. t. 3. f. 9.
Gvalt. test. t. 45. f. G.
Habitat in O. Europaeo, frequens ad littora Norvegiae.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 761, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The History of the Comic Supernova Rate Derived from the Evolution of the Host Galaxies
Creators: name: Kobayashi, Chiaki
name: Tsujimoto, Takuji
name: Nomoto, Ken'ichi
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We make a prediction of the cosmic supernova rate history as a composite of the supernova rates in spiral and elliptical galaxies. We include the metallicity effect on the evolution of Type Ia supernova (SN Ia) progenitors, and construct detailed models for the evolutions of spiral and elliptical galaxies in clusters and field to meet the latest observational constraints. In the cluster environment, the synthesized cosmic star formation rate (SFR) has an excess at $z \gtsim 3$ corresponding to the early star burst in ellipticals and a shallower slope from the present to the peak at the redshift of $z \sim 1.4$ compared with Madau's plot. In the field environment, we assume that ellipticals form over a wide range of redshifts as $1 \ltsim z \ltsim 4$. The synthesized cosmic SFR has a broad peak around $z \sim 3$, which is in good agreement with the observed one. The resultant cosmic SFRs lead to the following predictions for the cosmic SN Ia rate: 1) The SN Ia rate in spirals has a break at $z \sim 2$ due to the low-metallicity inhibition of SNe Ia, regardless of clusters or field. 2) At high redshifts, the SN Ia rate has a strong peak around $z \sim 3$ in clusters, whereas in field much lower rate is expected, reflecting the difference in the formation epochs of ellipticals.
description: 19 pages LaTeX, 10 PostScript figures, To appear in the Astrophysical Journal
The cosmological light-cone effect on the power spectrum of galaxies and quasars in wide-field redshift surveys
Creators: name: Yamamoto, Kazuhiro
name: Nishioka, Hiroaki
name: Suto, Yasushi
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine observational consequences of the cosmological light-cone effect on the power spectrum of the distribution of galaxies and quasars from upcoming redshift surveys. First we derive an expression for the power spectrum of cosmological objects in real space on a light cone, $P^{\rm LC}_{\rm R,lin}(k)$, which is exact in linear theory of density perturbations. Next we incorporate corrections for the nonlinear density evolution and redshift-space distortion in the formula in a phenomenological manner which is consistent with recent numerical simulations. On the basis of this formula, we predict the power spectrum of galaxies and quasars on the light cone for future redshift surveys taking account of the selection function properly. We demonstrate that this formula provides a reliable and useful method to compute the power spectrum on the light cone given an evolution model of bias.
description: 18 pages, 3 figures, to be published in the Astrophysical Journal