cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Schwinger Model Green functions with topological effects
Creators: name: Radozycki, Tomasz
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The fermion propagator and the 4-fermion Green function in the massless QED2 are explicitly found with topological effects taken into account. The corrections due to instanton sectors k=+1,-1, contributing to the propagator, are shown to be just the homogenous terms admitted by the Dyson-Schwinger equation for S. In the case of the 4-fermion function also sectors k=+2,-2 are included into consideration. The quark condensates are then calculated and are shown to satisfy cluster property. The theta-dependence exhibited by the Green functions corresponds to and may be removed by performing certain chiral gauge transformation.
description: 16 pages, in REVTEX
Removal of arsenic from aqueous solution using microflower-like δ-Bi2O3 as adsorbent: adsorption characteristics and mechanisms
Creators: name: Wang, Hongsheng
name: Wang, Sen
name: Zhao, Min
name: Li, Yue
name: Kong, Fanlong
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biophysics
subject: Space Science
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Hematology

description: Arsenic is one of the most common and harmful pollutants in environment, causing serious damage to human health and ecosystems. Herein, the uptake of arsenic by microflower-like δ-Bi2O3 including adsorption equilibrium, kinetics, desorption, the effects of initial pH and interfering ions on removal efficiency were studied in batch experiments, and the adsorption mechanism was also elucidated by Fourier transform infrared spectra and X-ray photoelectron spectroscopy. The results showed that the maximum adsorption capacities of As(III) and As(V) were 115.05 and 33.17 mg g−1, respectively. Simultaneously, the arsenic removal by MF-δ-Bi2O3 could work well in a wide pH range of 4–11 and presented excellent sorption selectivity for arsenic in the presence of competitive anions (NO3
 − and SO4
 2
 −). Furthermore, the adsorbent showed excellent morphological and structural stability after adsorption, which makes it easy to separate from aqueous solution and avoid secondary pollution as much as possible. The ligand exchange between arsenic ions and hydroxyl groups occupying the oxygen vacancies of MF-δ-Bi2O3 was the main adsorption mechanism. All studies in this experiment can led to a new direction for arsenic removal.
Роль минеральных удобрений и агротехнических приемов в формировании продуктивности нового сорта картофеля Евразия
Creators: name: Балакина С.В.
name: Осипов А.И.
Publisher: name: Известия Санкт-Петербургского государственного аграрного университета
Year: 2018
Subjects: КАРТОФЕЛЬ
СОРТ
МИНЕРАЛЬНЫЕ УДОБРЕНИЯ
ГУСТОТА ПОСАДКИ
ПРОДУКТИВНОСТЬ
POTATOES
VARIETY
MINERAL FERTILIZERS
PLANTING DENSITY
PRODUCTIVITY

description: В статье приведены результаты исследования, проведенного в 2015-2017 гг., по изучению влияния агротехнических приемов (применения полного минерального удобрения и густоты посадки) на формирование продуктивности картофеля нового среднераннего нематодоустойчивого сорта Евразия при возделывании на дерново-подзолистой легкосуглинистой среднеокультуренной почве Ленинградской области. Представлены данные хозяйственно-ценных признаков картофеля нового сорта Евразия, а также его характеристика по основным морфологическим признакам. Двухфакторный опыт был заложен методом систематических повторений в четырехкратной повторности. Установлено, что применение минеральных удобрений способствовало значительному повышению продуктивности картофеля сорта Евразия. В среднем за три года внесение различных доз удобрений обеспечило следующий рост урожайности по сравнению с контролем (без удобрений): N30P30K30 -25,4%; N60P60K60 37,1% и N90P90K90 47,5%. Увеличение густоты посадок по своему действию на урожайность оказалось эффективным только при загущении до 55 тыс. шт./га прибавки урожая клубней составили 2,6-5,2 т/га (12,8-17,4%), причем эффект от загущения проявлялся сильнее на удобренных делянках. В среднем за 3 года сорт Евразия сформировал наибольший урожай клубней (35,1 т/га) в посадках с густотой 55 тыс.шт./га и внесением полного минерального удобрения в дозе N90P90K90. Прибавка урожайности от совместного действия дозы N90P90K90 и загущения посадок с 45 до 55 тыс.шт./га составила 14,8 т/га, или 72,9% по отношению к контролю (густота 45 тыс.шт./га, без удобрений). Загущение до 65 тыс.шт./га оказалось малоэффективным приемом, поскольку не обеспечило роста урожайности по сравнению с посадками 55 тыс.шт./га и сопровождалось дополнительным расходом посадочного материала.
On the Density Probability Function of Galactic Gas. I. Numerical Simulations and the Significance of the Polytropic Index
Creators: name: Scalo, J.
name: Vazquez-Semadeni, E.
name: Chappell, D.
name: Passot, T.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the form of the one-point probability distribution function (pdf) for the density field of the interstellar medium using numerical simulations that successively reduce the number of physical processes included. Two-dimensional simulations of self-gravitating supersonic MHD and hydrodynamic turbulence, and of decaying Burgers turbulence, produce in all cases filamentary density structures and a power-law density pdf with logarithmic slope around -1.7. This suggests that the functional form of the pdf and the general filamentary morphology are the signature of the nonlinear advection operator. These results do not support previous claims that the pdf is lognormal. A series of 1D simulations of forced supersonic polytropic turbulence is used to resolve the discrepancy. They suggest that the pdf is lognormal only for effective polytropic indices $γ=1$ (or nearly lognormal for $γ\not=1$ if the Mach number is sufficiently small), while power laws develop at high densities if $γ<1$. We evaluate the polytropic index for conditions relevant to the cool interstellar medium using published cooling functions and different heating sources, finding that a lognormal pdf may occur at densities between 10$^3$ and at least 10$^4$ cm$^{-3}$. Several applications are examined. First, we question a recent derivation of the IMF from the density pdf by Padoan, Nordlund & Jones because a) the pdf does not contain spatial information, and b) their derivation produces the most massive stars in the voids of the density distribution. Second, we illustrate how a distribution of ambient densities can alter the predicted form of the size distribution of expanding shells. Finally, a brief comparison is made with the density pdfs found in cosmological simulations.
description: Submitted to ApJ. 23 pages, 15 postscript figures
Additional file 6: of The arrhythmogenic cardiotoxicity of the quinoline and structurally related antimalarial drugs: a systematic review
Creators: name: Haeusler, Ilsa
name: Chan, Xin
name: GuĂŠrin, Philippe
name: White, Nicholas
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Number of studies conducted in each region, for each drug. (DOCX 14 kb)
Additional file 5: of The arrhythmogenic cardiotoxicity of the quinoline and structurally related antimalarial drugs: a systematic review
Creators: name: Haeusler, Ilsa
name: Chan, Xin
name: GuĂŠrin, Philippe
name: White, Nicholas
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: Computational Biology

description: List of references included in the review. (DOCX 28 kb)
A Significant Over-Luminosity in the Transiting Brown Dwarf CWW 89Ab
Creators: name: Beatty, Thomas G.
name: Morley, Caroline V.
name: Curtis, Jason L.
name: Burrows, Adam
name: Davenport, James R. A.
name: Montet, Benjamin T.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We observed eclipses of the transiting brown dwarf CWW 89Ab at 3.6um and 4.5um using Spitzer/IRAC. The CWW 89 binary system is a member of the $3.0\pm0.25$ Gyr-old open cluster Ruprecht 147, and is composed of a Sun-like primary and an early M-dwarf secondary separated by a projected distance of 25 AU. CWW 89Ab has a radius of $0.937\pm0.042$ RJ and a mass of $36.5\pm0.1$ MJ, and is on a 5.3 day orbit about CWW 89A with a non-zero eccentricity of $e=0.19$ (Curtis et al. 2016). We strongly detect the eclipses of CWW 89Ab in both Spitzer channels as $δ_{3.6}=1147\pm213$ ppm and $δ_{4.5}=1097\pm225$ ppm after correcting for the dilution from CWW 89B. After accounting for the irradiation that CWW 89Ab receives from its host star, these measurements imply that the brown dwarf has an internal luminosity of $\log(\mathrm{L_{bol}/\mathrm{L}_\odot})=-4.19\pm0.14$. This is 16 times, or $9.3\,σ$, higher than model predictions given the known mass, radius, and age of CWW 89Ab. As we discuss, this over-luminosity is not explainable by an inaccurate age determination, additional stellar heating, nor tidal heating. Instead, we suggest that the anomalous luminosity of CWW 89Ab is caused by a dayside temperature inversion -- though a significant error in the evolutionary models is also a possibility. Importantly, a temperature inversion would require a super-stellar C/O ratio in CWW 89Ab's atmosphere. If this is indeed the case, it implies that CWW 89Ab is a 36.5 MJ object that formed via core accretion processes. Finally, we use our measurement of CWW 89Ab's orbital eccentricity, improved via these observations, to constrain the tidal quality factors of the brown dwarf and the host star CWW 89A to be $Q_{BD}>10^{4.15}$ and $Q_*>10^{9}$, respectively.
description: 19 pages, 12 figures. AJ in press. Updated based on comments received
MAKTABGACHA TA`LIM MUASSASALARIDA TAHSIL OLAYOTGAN BOLALAR UCHUN O`YINLAR ORQALI INGLIZ TILINI O`QITISH METODLARI
Creators: name: Xushboqova, Jamila
name: Urinova, Tursunoy
Publisher: name: Zenodo
Year: 2024

description: So'nggi bir necha yil ichida chet tilini o'rganish o'z-o'zini rivojlantirish usuli emas, balki zaruratga aylandi.  Chet tili nafaqat maktab va oliy o‘quv yurtlarida, balki ko‘plab qo‘shimcha maktabgacha ta’lim muassasalarida ham ta’limning majburiy tarkibiy qismiga aylandi.  Jamiyatda chet tiliga bo'lgan talab, bir tomondan, ota-onalarning til nafaqat zamonaviy shaxsni tarbiyalash omili, balki uning jamiyatdagi ijtimoiy va moddiy farovonligining asosi ekanligini tushunish -  boshqa tarafdan.  Bu moment chet tilini erta o'rganishni ayniqsa mashhur va dolzarb qiladi.  Agar 20 yil oldin bilim til faqat ba'zi sohalarda ishlash uchun kerak edi, endi kamida bitta chet tilini o'zlashtirish kerak edi.
PHARMACY STUDENTS' WELL-BEING: UNDERSTANDING THE ROLE OF PERSONALITY FACTORS
Creators: name: Pharm.D., Alumnus
name: Emily R., Sheaffer
name: Katherine, McNutt
Publisher: name: ZAP journals
Year: 2024
Subjects: Myers-Briggs Type Indicator
Personality Assessment
Psychological Types
Workplace Dynamics
Interpersonal Relationships

description: The Myers-Briggs Type Indicator (MBTI) stands as a widely utilized assessment tool designed for the categorization of individuals based on distinct personality traits and overarching psychological types. Comprising a set of over one hundred questions, participants are prompted to respond rapidly, offering the initial thoughts that come to mind. The resultant categorization assigns participants traits denoting their preference for introversion (I) or extroversion (E), sensing (S) or intuition (N), thinking (T) or feeling (F), and judging (J) or perceiving (P). The amalgamation of these traits yields a comprehensive personality profile, enabling insights into how individuals navigate both challenging situations and their day-to-day lives.

Upon completion of the assessment, participants receive a unique combination of traits, fostering in-depth inferences regarding their personality dynamics. This study focuses on the implications of the Myers-Briggs Type Indicator in unraveling individual characteristics and behavior, emphasizing its utility in deciphering how individuals interact and comprehend one another, particularly within the context of the workplace. By delving into the nuanced traits and types assigned by the MBTI, this research aims to contribute to a deeper understanding of the impact of personality on interpersonal relationships and professional dynamics
Reaction γπ\to ππin a confined quark model
Creators: name: Ivanov, M. A.
name: Mizutani, T.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A confined quark model study in a couple of chirally anomalous processes is presented in comparison with effective meson Lagrangian approaches of various kind. The processes considered are π^0 \to γγand γ\to π^+ π^- π^0 (or the equivalent πγ\to ππ) for which there is a well-known low energy theorem relating the latter amplitude with the former one by a very simple algebraic relation in the zero energy (or chiral, or soft pion) limit. Our quark model naturally generates the so-called contact term in the amplitude for the second process, but with the opposite sign to what effective chiral meson models indicate. A reinterpretation of our vector pole contribution restores the consistency, however. While the first reaction is observed to serve in it calibrating various models, it is found difficult, based upon the quality of the existing data in the second reaction, to single out the best model, which appears indispensable for testing the validity of the above low energy theorem. Thus the proposed experiments and their analyses should aim at attaining an optimal accuracy.
description: We added more discussion on the contact term and pole contrbution to the \gamma \pi \to \pi \pi reaction. 27 pages, latex, 7 figures are available on request from mizutanit@vtinte.phys.vt.edu, to be published in Phys.Rev.D
Additional file 3 of Implications of cardiac markers in risk-stratification and management for COVID-19 patients
Creators: name: Li, Pengping
name: Wu, Wei
name: Zhang, Tingting
name: Wang, Ziyu
name: Li, Jie
name: Zhu, Mengyan
name: Liang, Yuan
name: You, Wenhua
name: Li, Kening
name: Ding, Rong
name: Huang, Bin
name: Wu, Lingxiang
name: Duan, Weiwei
name: Han, Yi
name: Li, Xuesong
name: Tang, Xin
name: Wang, Xin
name: Shen, Han
name: Wang, Qianghu
name: Yan, Hong
name: Xia, Xinyi
name: Ji, Yong
name: Chen, Hongshan
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Additional file 3: Figure S2. Median levels of the cardiac markers on the first day after admission for four groups of patients (non-survivors with CAD, survivors with CAD, non-survivors without CAD, survivors without CAD). The dotted line shows the upper reference limit of the corresponding marker.
Multi-component dark matter from a hidden gauged SU(3)
Creators: name: Poulin, Alexandre
name: Godfrey, Stephen
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study Dark Matter (DM) phenomenology with multiple DM species consisting of both scalar and vector DM particles. More specifically, we study the Hidden Gauged SU(3) model of Arcadi {\it et al}. Before proceeding to the Hidden Gauged SU(3) model, we study the relic abundances of simplified multi-species DM scenarios to gain some insights when multiple species and interactions are included. In the Hidden Gauged SU(3) model, because of the large parameter space, we restrict ourselves to three representative benchmark points, each with multiple DM species. The relic densities for the benchmark points were found using a program developed to solve the coupled Boltzmann equations for an arbitrary number of interacting DM species with two particles in the final state. For each case, we varied the mass of the DM particles and then found the value of the dark SU(3) gauge coupling that gives the correct relic density. We found that in some regions of the parameter space, the DM would be difficult to observe in direct detection experiments while easier to observe in indirect detection experiments and vice versa, so that complementary measurements could help pinpoint the details of the Hidden Gauged SU(3) model. Important to this, is that even for moderate changes in input parameter values, the relative relic density of each species can change significantly resulting in large changes in the observability of multi-species DM by direct or indirect detection.
description: 21 pages, 5 figures, 3 tables. We made major revisions to section 3 by changing the points considered and the discussion about those points; also fixed some typos
Negative Energy, Superluminosity and Holography
Creators: name: Polchinski, Joseph
name: Susskind, Leonard
name: Toumbas, Nicolaos
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The holographic connection between large $N$ Super Yang Mills theory and gravity in anti deSitter space requires unfamiliar behavior of the SYM theory in the limit that the curvature of the AdS geometry becomes small. The paradoxical behavior includes superluminal oscillations and negative energy density. These effects typically occur in the SYM description of events which take place far from the boundary of AdS when the signal from the event arrives at the boundary. The paradoxes can be resolved by assuming a very rich collection of hidden degrees of freedom of the SYM theory which store information but give rise to no local energy density. These degrees of freedom, called precursors, are needed to make possible sudden apparently acausal energy momentum flows. Such behavior would be impossible in classical field theory as a consequence of the positivity of the energy density. However we show that these effects are not only allowed in quantum field theory but that we can model them in free quantum field theory.
description: Expanded version replacing earlier hep-th/9902182
title: Der Fachausschuss-Bericht Nr. 42 "Soda" als Grundlage von Lieferbedingungen für Glasschmelzsoda
Creators: name: (:Unkn) Unknown
Publisher: name: Frankfurt, M. : Hüttentechnische Vereinigung der Deutschen Glasindustrie
Year: 1937
Subjects: subject: 660

description: [no abstract available]
The Mass and Mass-to-Light Ratio for Clusters of Galaxies at Large Radii
Creators: name: Vedel, H.
name: Hartwick, F. D. A.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We construct models describing the velocity field in the infall regions of clusters. The velocity field is the superposition of a systematic component and a "noise" component accounting for the effects of small scale substructure and observational errors. This procedure results in models which resemble the observations (redshifts and angular separations of galaxies surrounding clusters) quite well. We demonstrate, on simulated data, that it is possible to estimate correctly the parameters of the systematic velocity component, knowledge of which allows determination of the mass profile of a cluster. To avoid systematic effects when analyzing real data, observations from a number of clusters should be combined. In the absence of sufficient data on other clusters we illustrate the method by applying it only to the Coma cluster. This results in mass estimates near the virial radius as well as at the turn around radius.
description: Accepted for publication in ApJ., 36 pages, incl figures
Additional file 2: of Human papillomavirus infection: protocol for a randomised controlled trial of imiquimod cream (5%) versus podophyllotoxin cream (0.15%), in combination with quadrivalent human papillomavirus or control vaccination in the treatment and prevention of recurrence of anogenital warts (HIPvac trial)
Creators: name: Murray, Macey
name: Meadows, Jade
name: DorĂŠ, Caroline
name: Copas, Andrew
name: Haddow, Lewis
name: Lacey, Charles
name: Jit, Mark
name: Soldan, Kate
name: Bennett, Kate
name: Tetlow, Michelle
name: Nathan, Mayura
name: Gilson, Richard
Publisher: name: figshare
Year: 2018
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Effective contraception. (DOCX 27 kb)
Emergent c-axis magnetic helix in manganite-nickelate superlattices
Creators: name: Fabbris, G.
name: Jaouen, N.
name: Meyers, D.
name: Feng, J.
name: Hoffman, J. D.
name: Sutarto, R.
name: Chiuzbaian, S. G.
name: Bhattacharya, A.
name: Dean, M. P. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The nature of the magnetic order in (La2/3Sr1/3MnO3)9/(LaNiO3)3 superlattices is investigated using x-ray resonant magnetic reflectometry. We observe a new c-axis magnetic helix state in the (LaNiO3)3 layers that had never been reported in nickelates, and which mediates the ~130deg magnetic coupling between the ferromagnetic (La2/3Sr1/3MnO3)9 layers, illustrating the power of x-rays for discovering the magnetic state of complex oxide interfaces. Resonant inelastic x-ray scattering and x-ray absorption spectroscopy show that Ni-O ligand hole states from bulk LaNiO3 are mostly filled due to interfacial electron transfer from Mn, driving the Ni orbitals closer to an atomic-like 3d8 configuration. We discuss the constraints imposed by this electronic configuration to the microscopic origin of the observed magnetic structure. The presence of a magnetic helix in (La2/3Sr1/3MnO3)9/(LaNiO3)3 is crucial for modeling the potential spintronic functionality of this system and may be important for designing emergent magnetism in novel devices in general.
description: 7 pages, 5 figures
title: „Schleuser-Merkel“: Wie Anzeigen und Verdächtigungen den politischen Diskurs bedrohen
Creators: name: Morawitz-Bardenheuer, Jan
Publisher: name: Fachinformationsdienst für internationale und interdisziplinäre Rechtsforschung
Year: 2018
Subjects: subject: 340

description: JuWissBlog
Resonant Slepton Production in Hadron-Hadron Collisions
Creators: name: Dreiner, Herbi
name: Richardson, Peter
name: Seymour, Mike
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the resonant production of sleptons via R-parity violation in hadron-hadron collisions followed by supersymmetric gauge decays of the sleptons. We look at decay modes which lead to the production of a like-sign dilepton pair. The dominant production mechanism giving this signature is the resonant production of a charged slepton followed by a decay to a charged lepton and a neutralino which then decays via R-parity violation. The discovery potential of this process at Run II of the Tevatron and the LHC is investigated using the HERWIG Monte Carlo event generator. We include the backgrounds from the MSSM. We conclude with a discussion of the possibility of extracting the lightest neutralino and slepton masses.
description: 45 pages, 29 figures
"KOMPETENTSIYA" FENOMENINING ILMIY TALQINI VA TALABALARDA IJTIMOIY FAOL FUQAROLIK KOMPETENTLIKNI RIVOJLANTIRISHNING IJTIMOIY AHAMIYATI
Creators: name: Teshayev, Azizbek
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqolada kompentsiyaning ilmiy ta’rifi va ijtimoiy mas’uliyatli fuqarolarni tarbiyalashdagi ahamiyati, xususan, uning ijtimoiy ahamiyati va talabalarga ta’siriga e’tibor qaratilib, ijtimoiy kompetentsiyani rivojlantirishda ta'limning rolini o'rganish, takomillashtirish bo'yicha samarali strategiyalarni o'rganish hamda uni targ'ib qilishdagi muammolarni, imkoniyatlarni hal qilish orqali talabalarda ijtimoiy faol fuqarolik kompetentsiyani tarbiyalashning muhimligi haqida fikr yuritilgan.
Additional file 4 of Whole-genome sequencing of phenotypically distinct inflammatory breast cancers reveals similar genomic alterations to non-inflammatory breast cancers
Creators: name: Li, Xiaotong
name: Kumar, Sushant
name: Harmanci, Arif
name: Li, Shantao
name: Kitchen, Robert R.
name: Zhang, Yan
name: Wali, Vikram B.
name: Reddy, Sangeetha M.
name: Woodward, Wendy A.
name: Reuben, James M.
name: Rozowsky, Joel
name: Hatzis, Christos
name: Ueno, Naoto T.
name: Krishnamurthy, Savitri
name: Pusztai, Lajos
name: Gerstein, Mark
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4: Fig. S1-S10. Supplementary Fig. S1-S10.
The Dynamics of D-3-brane Dyons and Toric Hyper-Kähler manifolds
Creators: name: Papadopoulos, G.
name: Gutowski, J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We find the dyonic worldvolume solitons due to parallel (p,q) strings ending on a D-3-brane. These solutions preserve 1/4 of bulk supersymmetry. Then we investigate the scattering of well-separated dyons and find that their moduli space is a toric hyper-Kähler manifold. In addition, we present the worldvolume solitons of the D-3-brane which are related by duality to the M-theory configuration of two orthogonal membranes ending on a M-5-brane. We show that these solitons preserve 1/8 of supersymmetry and compute their effective action.
description: 25 pages, phyzzx
Tunneling spectroscopy between one-dimensional helical conductors
Creators: name: Braunecker, Bernd
name: Simon, Pascal
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We theoretically investigate the tunneling spectroscopy of a system of two parallel one-dimensional helical conductors in the interacting, Luttinger liquid regime. We calculate the non-linear differential conductance as a function of the voltage bias between the conductors and the orbital momentum shift induced on tunneling electrons by an orthogonal magnetic field. We show that the conductance map exhibits an interference pattern which is characteristic to the interacting helical liquid. This can be contrasted with the different interference pattern from tunneling between regular Luttinger liquids which is governed by the spin-charge separation of the elementary collective excitations.
description: 9 pages, 6 figures, final version
Superconformal Symmetry and Correlation Functions
Creators: name: Park, Jeong-Hyuck
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Four-dimensional N-extended superconformal symmetry and correlation functions of quasi-primary superfields are studied within the superspace formalism. A superconformal Killing equation is derived and its solutions are classified in terms of supertranslations, dilations, Lorentz transformations, R-symmetry transformations and special superconformal transformations. In general, due to the invariance under supertranslations and special superconformal transformations, superconformally invariant n-point functions reduce to one unspecified (n-2)-point function which must transform homogeneously under the remaining rigid transformations, i.e. dilations, Lorentz transformations and R-symmetry transformations. Based on this result, we are able to identify all the superconformal invariants and obtain the general form of n-point functions for scalar superfields. In particular, as a byproduct, a selection rule for correlation functions is derived, the existence of which in N=4 super Yang-Mills theory was previously predicted in the context of AdS/CFT correspondence. Superconformally covariant differential operators are also discussed.
description: 1+56 pages, No figure, LaTeX. Reference Added, Selection Rule Generalized, Typos. To be published in Nucl. Phys. B 559: 455, 1999
Additional file 2: of Effects of green tea extract on overweight and obese women with high levels of low density-lipoprotein-cholesterol (LDL-C): a randomised, double-blind, and cross-over placebo-controlled clinical trial
Creators: name: Lin-Huang Huang
name: Liu, Chia-Yu
name: Wang, Li-Yu
name: Chien-Jung Huang
name: Chung-Hua Hsu
Publisher: name: figshare
Year: 2018
Subjects: subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: This is the raw data that was gathered in the clinical trial and was used to establish the data base of this study. (DOC 219 kb)
Radiative Corrections to the Z-b-(anti-b) and Z-tau-(anti-tau) Vertices in a Realistic One-Family Extended Technicolor Model
Creators: name: Yue, Chong-Xing
name: Kuang, Yu-Ping
name: Lu, Gong-Ru
name: Wan, Ling-De
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In a realistic effective one-family extended technicolor(ETC) model without exact custodial symmetry, we calculate the one-loop corrections to the Z-b-(anti-b) and Z-tau-(anti-tau)vertices from the sideways and diagonal ETC bosons exchange. The result shows that both the Z-->b+anti-b partial width (and the branching ratio) and the tau polarization asymmetry parameter A_tau are enhanced by the corrections and are in agreement with the present experimental data.
Сравнение показателей динамики накопления ртути и кадмия овсом из почвы
Creators: name: Ефремова М.А.
name: Митрофанов В.В.
Publisher: name: Известия Санкт-Петербургского государственного аграрного университета
Year: 2018
Subjects: РТУТЬ
КАДМИЙ
ЛОГИСТИЧЕСКАЯ ФУНКЦИЯ РОСТА
УДЕЛЬНАЯ СКОРОСТЬ РОСТА ОВСА
УДЕЛЬНАЯ СКОРОСТЬ ВЫНОСА ЭЛЕМЕНТОВ РАСТЕНИЯМИ ИЗ ПОЧВЫ
MERCURY
CADMIUM
THE LOGISTIC FUNCTION OF GROWTH
THE SPECIFIC GROWTH RATE OF OATS
THE SPECIFIC RATE OF REMOVAL OF ELEMENTS BY PLANTS FROM THE SOIL

description: В процессе вегетационного опыта овес выращивали на дисперсном минеральном техногенно образованном почвенном грунте со слабощелочной реакцией среды, искусственно загрязненном кадмием и ртутью. Проведено сравнение показателей динамики накопления ртути и кадмия овсом из почвогрунта. Показатели динамики получены в процессе постановки вегетационного опыта с помощью логистической функции, лежащей в основе математической модели динамики накопления элементов растениями, предложенной В.Ф. Дричко. Доступность Cd растениям овса из почвогрунта в экспоненциальный период роста культуры (фаза проростков, начало кущения) больше, чем Hg при одинаковой степени загрязнения почвенной среды тяжелыми металлами, удельная скорость выноса Cd овсом из почвогрунта в этот период в 5 раз больше, чем Hg. Концентрация Cd в растениях на протяжении всего жизненного цикла овса значительно превышала концентрацию Hg. Максимальный вынос ртути овсом из почвогрунта составил 0,01% от общего содержания элемента в почве, кадмия 0,45%. Показатель максимального выноса Cd овсом из почвогрунта в 50 раз выше, чем аналогичный показатель выноса Hg.In the process of vegetative experience, oats were grown on dispersed mineral technogenically formed soil with a slightly alkaline reaction of the medium artificially contaminated with cadmium and mercury. The dynamic parameters of mercury and cadmium accumulation by oats from soil are compared. The dynamics indicators were obtained during the process of setting up the vegetation experience with the help of the logistic function underlying the mathematical model of the dynamics of elements accumulation by plants proposed by V.F. Drichko. The availability of Cd to oat plants from the soil during the exponential growth period of the crop (the seedling phase, the start of tillering) is larger than Hg with the same degree of contamination of the soil environment with heavy metals, the specific rate of Cd removal from oats from the soil during this period is 5 times greater than Hg. The concentration of Cd in plants throughout the life cycle of oats was significantly higher than the concentration of Hg. The maximum removal of mercury from oats from soil was 0.01% of the total element content in the soil, cadmium 0.45%. The indicator of maximum removal of Cd from oats from the soil is 50 times higher than the similar value of Hg removal.
Formation of Large Scale Coronal Loops Interconnecting Two Active Regions Through Gradual Magnetic Reconnection and Associated Heating Process
Creators: name: Du, Guohui
name: Chen, Yao
name: Zhu, Chunming
name: Liu, Chang
name: Ge, Lili
name: Wang, Bing
name: Li, Chuanyang
name: Wang, Haimin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Coronal loops interconnecting two active regions, called as interconnecting loops (ILs), are prominent large-scale structures in the solar atmosphere. They carry a significant amount of magnetic flux, therefore are considered to be an important element of the solar dynamo process. Earlier observations show that eruptions of ILs are an important source of CMEs. It is generally believed that ILs are formed through magnetic reconnection in the high corona (>150-200"), and several scenarios have been proposed to explain their brightening in soft X-rays (SXRs). Yet, the detailed IL formation process has not been fully explored and the associated energy release in the corona still remains unresolved. Here we report the complete formation process of a set of ILs connecting two nearby active regions, with successive observations by STEREO-A on the far side of the Sun and SDO and Hinode on the Earth side. We conclude that ILs are formed by gradual reconnection high in the corona, in line with earlier postulations. In addition, we show evidence supporting that ILs become brightened in SXRs and EUVs through heating at or close to the reconnection site in the corona (i.e., through direct heating process of reconnection), a process that has been largely overlooked in earlier studies on ILs
description: 10 figures
title: Sechs Fragen an… Prof. Dr. em. Udo Steiner, Richter am Bundesverfassungsgericht a.D.: Interview im Rahmen der 58. Assistententagung Öffentliches Recht in Regensburg
Creators: name: Schröter, Nico
Publisher: name: Fachinformationsdienst für internationale und interdisziplinäre Rechtsforschung
Year: 2018
Subjects: subject: 340

description: JuWissBlog
ChipNet: Real-Time LiDAR Processing for Drivable Region Segmentation on an FPGA
Creators: name: Lyu, Yecheng
name: Bai, Lin
name: Huang, Xinming
Publisher: name: arXiv
Year: 2018
Subjects: subject: Signal Processing (eess.SP)
subject: Image and Video Processing (eess.IV)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: This paper presents a field-programmable gate array (FPGA) design of a segmentation algorithm based on convolutional neural network (CNN) that can process light detection and ranging (LiDAR) data in real-time. For autonomous vehicles, drivable region segmentation is an essential step that sets up the static constraints for planning tasks. Traditional drivable region segmentation algorithms are mostly developed on camera data, so their performance is susceptible to the light conditions and the qualities of road markings. LiDAR sensors can obtain the 3D geometry information of the vehicle surroundings with high precision. However, it is a computational challenge to process a large amount of LiDAR data in real-time. In this paper, a convolutional neural network model is proposed and trained to perform semantic segmentation using data from the LiDAR sensor. An efficient hardware architecture is proposed and implemented on an FPGA that can process each LiDAR scan in 17.59 ms, which is much faster than the previous works. Evaluated using Ford and KITTI road detection benchmarks, the proposed solution achieves both high accuracy in performance and real-time processing in speed.
description: 11 pages. IEEE Transactions on Circuits and Systems I: Regular Papers (2018)
Supplementary document for CO2-based hollow-core fiber Raman laser with high-pulse energy at 1.95 µm - 5453097.pdf
Creators: name: Wang, Yazhou
name: Schiess, Olav
name: Correa, Rodrigo Amezcua
name: Markos, Christos
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Uncategorized

description: Supplemental Document
Phanera erythropoda Mackinder & R. Clark 2014, comb. nov.
Creators: name: Mackinder, Barbara A.
name: Clark, Ruth
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Fabales
Fabaceae
Phanera
Phanera erythropoda

description: Phanera erythropoda (Hayata) Mackinder & R. Clark comb. nov.
Bauhinia erythropoda Hayata, Icon. Pl. Formosan. 3: 83. 1913.
Type: China, Hainan, Katsumada 1910 (holotype TI).
DISTRIBUTION. Endemic to China.
description: Published as part of Mackinder, Barbara A. & Clark, Ruth, 2014, A synopsis of the Asian and Australasian genus Phanera Lour. (Cercideae: Caesalpinioideae: Leguminosae) including 19 new combinations, pp. 49-68 in Phytotaxa 166 (1) on page 54, DOI: 10.11646/phytotaxa.166.1.3, http://zenodo.org/record/5138206
Additional file 6: of Using equitable impact sensitive tool (EQUIST) to promote implementation of evidence informed policymaking to improve maternal and child health outcomes: a focus on six West African Countries
Creators: name: Chigozie Uneke
name: Issiaka Sombie
name: Uro-Chukwu, Henry
name: Ermel Johnson
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Molecular Biology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Outcome of EQUSIT Scenario analysis for poorest quintile in Senegal. (PDF 345 kb)
Local stellar kinematics from Hipparcos data
Creators: name: Dehnen, Walter
name: Binney, James
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (shortened) From a kinematically unbiased subsample of the Hipparcos catalogue we have redetermined as a function of colour the kinematics of main-sequence stars. The stars' mean heliocentric velocity nicely follows the asymmetric drift relation, except for stars blueward of B-V=0.1. Extrapolating to zero dispersion yields for the velocity of the Sun w.r.t. the LSR in km/s: U_0=10.00+/-0.36 (radially inwards), V_0=5.23+/-0.62 (in direction of galactic rotation), and W_0=7.17+/-0.38 (vertically upwards). A plot of velocity dispersion vs. colour beautifully shows Parenago's discontinuity: the dispersion is constant for B-V>0.62 and decreases towards bluer colour. We determine the velocity-dispersion tensor sigma^2_ij as function of B-V. The mixed moments involving vertical motion are zero within the errors, while sigma^2_xy is non-zero at about (10km/s)^2 independent of colour. The resulting vertex deviations are about 20 deg for early-type stars and 10+/-4 deg for old-disc stars. The persistence of the vertex deviation to late-type stars implies that the Galactic potential is significantly non-axisymmetric at the solar radius. If spiral arms are responsible for this, they cannot be tightly wound. Except for stars bluer than B-V=0.1 the ratios of the principal velocity dispersions are 2.2 : 1.4 :1, while the absolute values increase with colour from sigma_1=20km/s at B-V=0.2 to sigma_1=38km/s at Parenago's discontinuity and beyond. These ratios imply significant heating of the disc by spiral structure and that R_0/R_d=3 to 3.5, where R_d is the scale length of the disc.
description: 7 pages, LaTeX, mn.sty, 6 postscript figures, submitted to MNRAS
title: ADCO, Cartulaire de Cîteaux pour les possessions de Beaune et du Beaunois (XVe siècle), Cart. 174 (11 H 79), 56 pages, f. 0015
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Cîteaux pour les possessions de Beaune et du Beaunois (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 174 (11 H 79), 56 pages, f. 0015, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Beaune et du Beaunois (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 174 (11 H 79), 56 pages, f. 0015, 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
D=5 Simple Supergravity on AdS_2 \times S^3
Creators: name: Fujii, Akira
name: Kemmoku, Ryuji
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The Kaluza-Klein spectrum of D=5 simple supergravity compactified on S^3 is studied. A classical background solution which preserves maximal supersymmetry is fulfilled by the geometry of AdS_2\times S^3. The physical spectrum of the fluctuations is classified according to SU(1,1|2)\times SU(2) symmetry, which has a very similar structure to that in the case of compactification on AdS_3\times S^2.
description: 14 pages, Latex, 4 figures; some description improved
The McDonagh Sisters
Creators: Barry, Rebecca
Publisher: name: Columbia University
Year: 2013
Subjects: Women in the motion picture industry
Motion pictures
Silent films

description: Isabel, Phyllis, and Paulette McDonagh were sisters, business partners, and creative collaborators who made films in Sydney, Australia, in the 1920s and 1930s. Isabel, the eldest, was the actress and star of all their films under the name Marie Lorraine. Phyllis took on the role of art director, publicist, and producer. Paulette, the youngest of the three, was the writer and director of all their films. The sisters grew up in the upper middle class suburb of Drummoyne in Sydney, Australia. Drummoyne House, the grand family home, was filled with antique furniture and became the movie set and backdrop for many of their films. The home was a hub of bohemia, with traveling theatrical and entertainment people visiting whenever in Sydney.
title: Generation of Mitochondria-Depleted Cell Lines - a Tool for Assessing Mitochondrial Transfer
Creators: name: Osgood, Chris
name: Stacey, M.
name: Wyckoff, C.
Publisher: name: Old Dominion University
publisherIdentifier: https://ror.org/04zjtrb98
publisherIdentifierScheme: ROR
Year: 2024

description:
An overarching goal of current research in our lab is to assess the impact of mitochondrial transfer between cancer cells and their non-cancerous neighbors, focusing on epigenetic and metabolic impacts. Specifically, we are using SW1353 cells, a chondrosarcoma cell line, carrying a mutation in the IDH2 gene which disrupts the TCA cycle and generates an important oncometabolite, D-2-hydroxyglutarate (D2-HG). We will test the impact of transfer of mitochondria from SW1353 to non-cancerous recipients, as well as return trafficking of mitochondria from the non-cancer cell to SW1353’s. A challenge we will face in these experiments arises from the fact that the recipient cells, either SW1353 or non-cancer cells, will contain 100-1,000s of their resident mitochondria. To enhance our ability to detect the impact of mitochondrial transfer, we are developing mitochondria-free cell lines, these are designated as rho0 cell lines. Techniques for targeting mitochondrial for depletion as well as our preliminary results will be presented.
The James Webb Space Telescope North Ecliptic Pole Time-Domain Field -- I: Field Selection of a JWST Community Field for Time-Domain Studies
Creators: name: Jansen, Rolf A.
name: Windhorst, Rogier A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We describe the selection of the James Webb Space Telescope (JWST) North Ecliptic Pole (NEP) Time-Domain Field (TDF), a ~14' diameter field located within JWST's northern Continuous Viewing Zone (CVZ) and centered at (RA, Dec)_J2000 = (17:22:47.896, +65:49:21.54). We demonstrate that this is the only region in the sky where JWST can observe a clean (i.e., free of bright foreground stars and with low Galactic foreground extinction) extragalactic deep survey field of this size at arbitrary cadence or at arbitrary orientation, and without a penalty in terms of a raised Zodiacal background. This will crucially enable a wide range of new and exciting time-domain science, including high redshift transient searches and monitoring (e.g., SNe), variability studies from Active Galactic Nuclei (AGN) to brown dwarf atmospheres, as well as proper motions of possibly extreme scattered Kuiper Belt and Inner Oort Cloud Objects, and of nearby Galactic brown dwarfs, low-mass stars, and ultracool white dwarfs. A JWST/NIRCam+NIRISS GTO program will provide an initial 0.8--5.0micron spectrophotometric characterization to m_AB ~ 28.8+/-0.3 mag of four orthogonal "spokes" within this field. The multi-wavelength (radio through X-ray) context of the field is in hand (ground-based near-UV--visible--near-IR), in progress (VLA 3GHz, VLBA 5GHz, HST UV--visible, Chandra X-ray, IRAM30m 1.3 and 2mm), or scheduled (JCMT 850micron). We welcome and encourage ground- and space-based follow-up of the initial GTO observations and ancillary data, to realize its potential as an ideal JWST time-domain community field.
description: PDFLaTeX, 15 pages with 7 figures (18 panels), minor revision, as accepted for publication in PASP
On the construction of gauge theories from non critical type 0 strings
Creators: name: Ferretti, Gabriele
name: Martelli, Dario
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate Polyakov's proposal of constructing Yang-Mills theories by using non critical type 0 strings. We break conformal invariance by putting the system at finite temperature and find that the entropy of the cosmological solutions for these theories matches that of a gas of weakly interacting Yang-Mills bosons, up to a numerical constant. The computation of the entropy using the effective action approach presents some novelties in that the whole contribution comes from the RR fields. We also find an area law and a mass gap in the theory and show that such behavior persists for $p>4$. We comment on the possible physical meaning of this result.
description: 12 pages LaTeX, V2: reference added, report number changed. V3: minor misprints corrected