cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Participatory constraint analysis regarding the adoption of IPM technologies in pointed gourd cultivation: An empirical study
Creators: name: Chowdhury, Sarthak
name: Ray, Prabuddha
name: Chowdhury, Sarthak
name: Ray, Prabuddha
Publisher: name: Unknown
Year: 2009
Subjects: Research and Development/Tech Change/Emerging Technologies
Research Methods/ Statistical Methods

description: The empirical study revealed that among the various types of constraints (as perceived by the respondents) regarding the adoption of IPM technologies in the Pointed Gourd (Trichosan thes dioica Roxb.) production, the lack of knowledge of the respondents about the Economic Threshold Limit (ETL) concept ranked first closely followed by the lack of knowledge of the respondents regarding the bio-pesticides (under the category of knowledge and information constraints) in second position, the lack of knowledge of the respondents about the Integrated Pest Management (IPM) techniques ranked third position, closely followed by lack of training of the respondents on the proper use of pesticides in the fourth position. The result also showed that among six numbers of different categories of perceived constraints, knowledge and information constraints with a rank score of 2769 enjoyed first rank position, distantly followed by administrative and managerial constraints (with a rank score of 1586) in the second position, technological and communication constraints with a rank score of 1249 in the third position, socio-economic constraint (rank score of 828) in the fourth position.
title: 02_0752
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Jet Propagation in Neutron Star Mergers and GW170817
Creators: name: Hamidani, Hamid
name: Kiuchi, Kenta
name: Ioka, Kunihito
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The gravitational wave event from the binary neutron star (BNS) merger GW170817 and the following multi-messenger observations present strong evidence for i) merger ejecta expanding with substantial velocities and ii) a relativistic jet which had to propagate through the merger ejecta. The ejecta's expansion velocity is not negligible for the jet head motion, which is a fundamental difference from the other systems like collapsars and active galactic nuclei. Here we present an analytic model of the jet propagation in an expanding medium. In particular, we notice a new term in the expression of the breakout time and velocity. In parallel, we perform a series of over a hundred 2D numerical simulations of jet propagation. The BNS merger ejecta is prepared based on numerical relativity simulations of a BNS merger with the highest-resolution to date. We show that our analytic results agree with numerical simulations over a wide parameter space. Then we apply our analytic model to GW170817, and obtain two solid constraints on: i) the central engine luminosity as $L_{iso,0} \sim 3\times10^{49}-2.5\times10^{52}$ erg s$^{-1}$, and on ii) the delay time between the merger and engine activation $t_0-t_m < 1.3$ s. The engine power implies that the apparently-faint \textit{short} gamma-ray burst (\textit{s}GRB) \textit{s}GRB 170817A is similar to typical \textit{s}GRBs if observed on-axis.
description: 28 pages, 10 figures, and 2 tables
Physical and Chemical Structure of the Solar Type Protostar NGC1333-IRAS4
Creators: name: Maret, S.
name: Ceccarelli, C.
name: Caux, E.
name: Tielens, A. G. G. M.
name: Castets, A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Sun like stars are born from the collapse of fragment of molecular clouds. During the first embedded phase (the so called class 0/1), the protostar is surrounded by a collapsing envelope, whose physical and chemical structure would set up the initial conditions of the proto-stellar disk which may eventually form planets. In this contribution, we show how spectroscopic far infrared to millimeter observations can be a powerful diagnostic to derive the chemical and physical structure of the innermost regions of envelopes collapsing around solar type protostars, where disk are believe to form. Our claim is based on the simultaneous modeling of the dynamics, chemistry and radiative transfer in a protostellar envelope. Here we present a study of a class 0 protostar NGC1333-IRAS4, obtained using ISO-LWS observations of water far-infrared lines. We show the derived physical and chemical structure of the protostar, namely the density and temperature profiles, as well as the water abundance across the envelope. Besides, the mass of the central protostar and its accretion rate can be constrained by these observations and modeling, yielding an alternative method to measure these two poorly know parameters.
description: Proceedings of the conference "The Evolution of Galaxies. II- Basic Building Blocks", Ile de la reunion, France, 16-21 October 2001. 2 pages
Kraussia rugulosa
Creators: name: Castro, Peter
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Kraussia
Kraussia rugulosa

description: Kraussia rugulosa (Krauss, 1843)
 Platyonichus rugulosus Krauss, 1843: 26, pl. 1, fig. 5 [type locality: South Africa; type material: status and location unknown].
 Hawaiian Is. records:
 Kraussia rugulosa (Krauss, 1843) — Dana 1852a: 86 [insulas Hawaienses]; 1852b: 302, pl. 19, fig. 1 [Maui]. — Rathbun 1906: 875 [Dana’s record]. — Edmondson 1946: 283, fig. 175 [H.I.].
 Taxonomy. Serène (1972), Ng (1993)
 Geographical distribution. Across Indo-West Pacific region.
 Habitat. Intertidal, shallow subtidal.
description: Published as part of Castro, Peter, 2011, Catalog of the anomuran and brachyuran crabs (Crustacea: Decapoda: Anomura, Brachyura) of the Hawaiian Islands 2947, pp. 1-154 in Zootaxa 2947 (1) on page 96, DOI: 10.11646/zootaxa.2947.1.1, http://zenodo.org/record/5283044
MOESM1 of Anticholinergic and benzodiazepine medication use and risk of incident dementia: a UK cohort study
Creators: name: Grossi, Carlota
name: Richardson, Kathryn
name: Fox, Chris
name: Maidment, Ian
name: Steel, Nicholas
name: Loke, Yoon
name: Arthur, Antony
name: Phyo Myint
name: Noll Campbell
name: Malaz Boustani
name: Robinson, Louise
name: Brayne, Carol
name: Matthews, Fiona
name: Savva, George
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1. Baseline use and 2-year patterns of use of benzodiazepines and anticholinergics of participants with 10-year follow-up (unweighted percentage).
Nodulation, yield and quality of soybean as influenced by integrated nutrient management
Creators: name: Alam, M.A
name: Siddiqua, A.
name: Chowdhury, M.A.H
name: Prodhan, M.Y
name: Alam, M.A
name: Siddiqua, A.
name: Chowdhury, M.A.H
name: Prodhan, M.Y
Publisher: name: Unknown
Year: 2009
Subjects: Production Economics
Productivity Analysis
Research Methods/ Statistical Methods

description: A field experiment was conducted at the Horticultural Farm of Bangladesh Agricultural University, Mymensingh during the period from November 2007 to March 2008 to study the effect of integrated nutrient management on nodulation and sustainable soybean production. There were significant differences among the different treatment combinations in terms of yield and yield contributing characters. Integrated nutrient management with application of 50% of the recommended doses of urea, TSP, MOP, gypsum and biofertilizer (Bradyrhizobium) at the rate of 1 kg ha-1 significantly increased most of the parameters, such as the highest plant height, number of nodule per plant, nodule dry weight per plant, pods per plant, grains per pod, grain yield, oil and protein contents. Coinoculation of Bradyrhizobium seemed to help reduce the NPKS requirement in soybean cultivation. Overall results indicate that the application of integrated nutrient management of biofertilizer (Bradyrhizobium) with ½ NPKS of the recommended dose would produce the best quality of soybean with higher nodulation and yield.
Fusion reactions in the $^9$Be + $^{197}$Au system above the Coulomb barrier
Creators: name: Li, G. S.
name: Wang, J. G.
name: Lubian, J.
name: Soler, H. O.
name: Fang, Y. D.
name: Liu, M. L.
name: Zhang, N. T.
name: Zhou, X. H.
name: Zhang, Y. H.
name: Gao, B. S.
name: Qiang, Y. H.
name: Guo, S.
name: Wang, S. C.
name: Wang, K. L.
name: Zheng, K. K.
name: Li, R.
name: Zheng, Y.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The cross sections of complete fusion and incomplete fusion for the $ ^{9} $Be + $ ^{197} $Au system, at energies not too much above the Coulomb barrier, were measured for the first time. The online activation followed by offline $γ$-ray spectroscopy method was used for the derivation of the cross sections. A slightly higher value of ICF/TF ratio has been observed, compared to other systems reported in the literature with $ ^{9} $Be beam. The experimental data were compared with coupled channel calculations without taking into account the coupling of the breakup channel, and experimental data of other reaction systems with weakly bound projectiles. A complete fusion suppression of about 40\% was found for the $ ^{9} $Be + $ ^{197} $Au system, at energies above the barrier, whereas the total fusion cross sections are in agreement with the calculations.
GJ 2126 b: A highly eccentric Jovian exoplanet
Creators: name: Schorr, Arbel
name: Binnenfeld, Avraham
name: Zucker, Shay
Publisher: name: arXiv
Year: 2025
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We report the discovery of GJ 2126 b, a highly eccentric (e = 0.85) Jupiter-like planet orbiting its host star every 272.7 days. The planet was detected and characterized using 112 radial velocity (RV) measurements from HARPS (High Accuracy Radial Velocity Planet Searcher), provided by HARPS-RVBank. This planet orbits a low-mass star and ranks among the most eccentric exoplanets discovered, placing it in a unique region of the parameter space of the known exoplanet population. This makes it a valuable addition to the exoplanet demographics, helping to refine our understanding of planetary formation and evolution theories.
description: 7 pages, 5 figures. A&A accepted
Additional file 8 of Divergent airway microbiomes in lung transplant recipients with or without pulmonary infection
Creators: name: Påhlman, Lisa I.
name: Lokeshwaran Manoharan
name: Aspelund, Anna Stjärne
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 8: Table S2. Patient and sample characteristics.
Threshold temperature for pairwise and many-particle thermal entanglement in the isotropic Heisenberg model
Creators: name: Wang, Xiaoguang
Publisher: name: arXiv
Year: 2002
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We study the threshold temperature for pairwise thermal entanglement in the spin-1/2 isotropic Heisenberg model up to 11 spins and find that the threshold temperature for odd and even number of qubits approaches the thermal dynamical limit from below and above, respectively. The threshold temperature in the thermodynamical limit is estimated. We investigate the many-particle entanglement in both ground states and thermal states of the system, and find that the thermal state in the four-qubit model is four-particle entangled before a threshold temperature.
description: 4 pages with 1 fig. More discussions on many-particle ground-state and thermal entanglement in the multiqubit Heisenberg model from 2 to 11 qubits are added
Expansible thermal gelling foam aerosol for vaginal drug delivery
Creators: name: Mei, Liling
name: Chen, Jintian
name: Yu, Siqin
name: Huang, Ying
name: Xie, Yecheng
name: Wang, Hui
name: Pan, Xin
name: Wu, Chuanbin
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Astronomical and Space Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Vaginal delivery of antimicrobial drugs is the most effective method for the local treatment of the vaginal infections. However, current vaginal drug delivery systems (VDDS), including gel, lotion, aerosol and cream, are suffering from low penetration in the deep vaginal rugae and easy elimination by self-cleaning of vaginal canal. To address these issues, a foam aerosol based on the thermal transformation was designed to improve penetration efficiency and achieve the extended retention. The expansible thermal gelling foam aerosol (ETGFA) consisting of thermal sensitive matrix, silver nanoparticle, adhesive agent and propellant, was optimized by evaluations of precursor viscosity, foam expansion, thermal gelation, gel adhesiveness, antimicrobial effects and tissue irritation. The ETGFA would penetrate to the deep vaginal rugae to cover the infectious sites by foam expansion. Drug leakage was intended to be avoided by the thermal gelation at physiological temperature before foam collapse. The gel could be retained in the vaginal canal for extended time due to its superior adhesiveness when compared to the commercial gel Asimi®. The ETGFA provided extended drug release for over 4 h and maintained effective drug concentrations at the infectious sites. The ETGFA containing silver nanoparticles showed dose-dependent antimicrobial effects on the vaginal floras and irritation reduction to the vaginal tissues. The results demonstrated that the ETGFA could overcome the limitations of conventional dosage forms, including poor drug penetration, carrier retention and patient compliance and satisfied the requirements for vaginal drug delivery.
MOESM1 of What has changed HIV and syphilis infection among men who have sex with men (MSM) in Southwest China: a comparison of prevalence and behavioural characteristics (2013â 2017)
Creators: name: Yangchang Zhang
name: Guohui Wu
name: Rongrong Lu
name: Wanyuan Xia
name: Hu, Ling
name: Xiong, Yang
name: Junhao Xie
name: Qiuhua Yu
name: Mengliang Ye
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
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: Additional file 1. The questionnaire for men sex with men: This structured questionnaire includes socio-demographic data and characteristics of sexual behaviors among MSM.
Optimization of Agrobacterium tumefaciens mediated genetic transformation protocol for aromatic rice
Creators: name: Hossain, M.R
name: Hassan, L.
name: Patwary, A.K
name: Ferdous, M.J
name: Hossain, M.R
name: Hassan, L.
name: Patwary, A.K
name: Ferdous, M.J
Publisher: name: Unknown
Year: 2009
Subjects: Research and Development/Tech Change/Emerging Technologies
Research Methods/ Statistical Methods

description: A rapid, efficient and reproducible genetic transformation protocol was optimized for four aromatic rice varieties by using the established plant regeneration protocol. Mature embryos were inoculated with Agrobacterium tumefaciens strain EHA105 carrying a binary vector pIG121-Hm with GUS (reporter gene) and hpt (hygromycin resistance) gene and the transformation experiment was performed by optimizing two important parameters viz. infection times and co-cultivation periods. The highest response to GUS assay was showed by Kalizira (70% GUS positive) followed by Pusa Basmati 1 (66.67%) when the explants were inoculated for 25 minutes and co-cultivated for three days. Twenty five minutes infection time (9.44%) and three day co- cultivation period (8.06%) were found effective for percentage of transgenic shoot regeneration. The highest percentage of putative transgenic shoots was regenerated by variety Kalizira (33.33%) followed by Pusa Basmati 1 (20.0%) and Radhunipagol (13.33%). Among the varieties, Kalizira produced the highest percentage (60%) of rooted shoots. Kalizira also showed the highest survival rate in growth chamber (75%) and in field condition (60%). The performance of Tulsimala was poor for almost all the cases.
Identification of cultivable heat tolerant wheat genotypes suitable for Patuakhali district in Bangladesh
Creators: name: Haque, M.Z
name: Hasan, M.M
name: Rajib, M.M.R
name: Haque, M.Z
name: Hasan, M.M
name: Rajib, M.M.R
Publisher: name: Unknown
Year: 2009
Subjects: Research and Development/Tech Change/Emerging Technologies
Research Methods/ Statistical Methods

description: Fifteen wheat genotypes namely Agrani, Prodip, Bijoy, CB 69, Sourav, Sufi, BAW 1064, Gourab, Kanchan Shatabdi, CB 30, Sonora, CB 24, CB34, and Protiva were sown under optimum (Nov. 30) and late (Dec. 30) sowing times to evaluate their performances at high temperature depending on cell membrane thermostability and some morpho-physiological characters. Based on cell membrane thermostability test four genotypes showed the longest heat killing time and were separated as heat tolerant (HT). Four genotypes showed the shortest heat killing time and were separated as heat sensitive (HS). The remaining seven genotypes required time in between those two were separated as intermediate heat tolerant (IHT) genotypes. Lower contribution of photosynthate stem reserves (PSR) to grain in HT genotypes finally contributed to its less affected 1000-grain weight as well as yield. These results suggest that greater cell membrane thermostability supported the minimal changes in some physiological characters of HT ganotypes which ultimately increased the wheat yield under short winter warmer condition.
Liomera bella
Creators: name: Castro, Peter
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Xanthidae
Liomera
Liomera bella

description: Liomera bella (Dana, 1852)
 Actaeodes bellus Dana, 1852a: 78 [type localities: insulas Samoenses … Wakes; type material presumed lost].
 Hawaiian Is. records:
 Carpilodes vaillantianus (A. Milne-Edwards, 1862) — Rathbun 1906: 843 [O‘ahu, H. I., Laysan] — Edmondson 1923a: 1552 [Kure Atoll]; 1925: 53 [O‘ahu, Kure Atoll, Pearl and Hermes Reef, Lisianski, Laysan, French Frigate Shoals, Johnston Atoll]. — Pesta 1933: 280 [H.I.].
 Carpilodes bellus (Dana, 1852) — Edmondson 1946: 291, fig. 177 f [H.I.]; 1962a: 249, fig. 8f [H.I.]. — Buitendijk 1960: 257, fig. 2b [Hawai‘i].
 Liomere [sic] bella (Dana, 1852) — Amerson & Shelton 1976: 76 [Johnston Atoll].
 Liomera (Liomera) bella (Dana, 1852): Titgen 1987: 108 [Laysan].
 Liomera bella (Dana, 1852) — DeFelice et al. 1998: 16 [Midway Is.]. — Coles, DeFelice & Eldredge 1999: 159 [O‘ahu] [also as Carpilodes bellus]; 2002a: 270, 333 [O‘ahu]; 2002b: 138, 224 [O‘ahu]. — Coles et al. 2001: 52 [Johnston Atoll]. — Godwin & Bolick 2006: 39, 49 [Moloka‘i]. — Hoover 2006: 279, color photograph [O‘ahu].
 Taxonomy. Serène (1984)
 Geographical distribution. Across Indo-West Pacific region.
 Habitat. Intertidal, shallow subtidal.
description: Published as part of Castro, Peter, 2011, Catalog of the anomuran and brachyuran crabs (Crustacea: Decapoda: Anomura, Brachyura) of the Hawaiian Islands 2947, pp. 1-154 in Zootaxa 2947 (1) on page 97, DOI: 10.11646/zootaxa.2947.1.1, http://zenodo.org/record/5283044
How do Fermi liquids get heavy and die?
Creators: name: Coleman, P.
name: Pepin, C.
name: Si, Q.
name: Ramazashvili, R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We discuss non-Fermi liquid and quantum critical behavior in heavy fermion materials, focussing on the mechanism by which the electron mass appears to diverge at the quantum critical point. We ask whether the basic mechanism for the transformation involves electron diffraction off a quantum critical spin density wave, or whether a break-down in the composite nature of the heavy electron takes place at the quantum critical point. We show that the Hall constant changes continously in the first scenario, but may ``jump'' discontinuously at a quantum critical point where the composite character of the electron quasiparticles changes.
description: Revised version with many new references added. To appear as a topical review in Journal of Physics: Condensed Matter Physics. Two column version http://www.physics.rutgers.edu/~coleman/online/questions.ps.gz
The Galactic Halo Contribution to the Dispersion Measure of Extragalactic Fast Radio Bursts
Creators: name: Yamasaki, Shotaro
name: Totani, Tomonori
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A new model of the Milky Way (MW) halo component of the dispersion measure (DM) for extragalactic sources, such as fast radio bursts (FRBs), is presented in light of recent diffuse X-ray observations. In addition to the spherical component of isothermal gas ($kT\sim0.3$ keV) in hydrostatic equilibrium with the Galactic gravitational potential, our model includes a disk-like non-spherical hot gas component to reproduce the directional dependence of the observed X-ray emission measure (EM). The total gas mass ($1.2\times10^{11}\,M_{\odot}$) is dominated by the spherical component, and is consistent with the total baryon mass of the MW expected from the dark matter mass and the cosmic baryon-to-dark-matter ratio. Our model predicts a mean halo DM of $43\:\,{\rm pc\:cm^{-3}}$, with a full range of $30$-$245\:\,{\rm pc\:cm^{-3}}$ over the whole sky. The large scatter seen in the X-ray EM data implies a $\sim0.2$ dex (rms) fluctuation of the MW halo DM. We provide an analytic formula to estimate the MW halo DM of our model along any line of sight, which can be easily used to compute the total MW component of DM toward extragalactic sources, in combination with existing DM models of the warm ionized medium associated with the Galactic disk.
description: 11 pages, 9 figures, 1 table, 2 hot gas halo components, accepted for publication in ApJ; v2
Productivity and Resource Use Efficiency of Boro Rice Production
Creators: name: Majumder, M.K
name: Mozumdar, L.
name: Roy, P.C
name: Majumder, M.K
name: Mozumdar, L.
name: Roy, P.C
Publisher: name: Unknown
Year: 2008
Subjects: Production Economics
Productivity Analysis

description: This study was attempted to measure and compare resource use efficiency and relative productivity of farming under different tenure conditions in an area of Bhola district. A random sampling technique was used in the study. Sample farmers were classified as owner, crop share tenant and cash tenant farmers. A total of 90 samples, 30 from each class were selected on the basis of random sampling technique. The study explored the difference in the efficiency and productivity among owner, cash tenant and crop share tenant. Total cash expenses as well as total gross costs for producing HYV Boro rice was highest in owner farms and lowest in crop share tenant's farm. When individual inputs were concerned it was observed that expenses on human labor shared a major portion of expenses in the production of HYV Boro rice where owner operators used more hired labor in compare to other groups. However, the cash tenant farmers were more efficient than owner and crop share tenant farmers. Due to poor resource base the crop share tenants were unable to invest on modern farm inputs. It may be mentioned that in Bangladesh the predominant tenancy arrangement is share cropping, which is an inefficient form of tenure arrangement in compare to cash tenancy.
Nonrelativistic energies and predissociation widths of quasibound states in the Li$dμ$ molecular ions
Creators: name: Korobov, V. I.
name: Eskin, A. V.
name: Martynenko, F. A.
name: Sukhorukova, O. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Muonic molecular ions $^6$Li$^{3+}dμ$ and $^7$Li$^{3+}dμ$ are studied numerically. Using the complex coordinate rotation method we found six rotational states (three for each isotope), which are resonant states with the life-time of an order of picoseconds. These molecular systems may be of interest for studying low-energy fusion reactions. A key quantity, $|Ψ(0)|^2$, the wave function squared at the coalescence point of the nuclei is calculated for $S$ states for both isotopes with a precision better than 3\%.
Can Van Hove singularities be observed in relativistic heavy-ion collisions ?
Creators: name: Mustafa, Munshi G.
name: Thoma, Markus H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Based on general arguments the in-medium quark propagator in a quark-gluon plasma leads to a quark dispersion relation consisting of two branches, of which one exhibits a minimum at some finite momentum. This results in a vanishing group velocity for collective quark modes. Important quantities such as the production rate of low mass lepton pairs and mesonic correlators depend inversely on this group velocity. Therefore these quantities, which follow from self energy diagrams containing a quark loop, are strongly affected by Van Hove singularities (peaks and gaps). If these sharp structures could be observed in relativistic heavy-ion collisions it would reveal the physical picture of the QGP as a gas of quasiparticles.
description: 12 pages including nine figures and style files, invited talk given at the ICPAQGP-2001, November 26-30, 2001, Jaipur, India
Additional file 9 of Divergent airway microbiomes in lung transplant recipients with or without pulmonary infection
Creators: name: Påhlman, Lisa I.
name: Lokeshwaran Manoharan
name: Aspelund, Anna Stjärne
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 9: Table S3. Enrichment analysis for samples collected during infection.
Specifying Object Attributes and Relations in Interactive Scene Generation
Creators: name: Ashual, Oron
name: Wolf, Lior
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: We introduce a method for the generation of images from an input scene graph. The method separates between a layout embedding and an appearance embedding. The dual embedding leads to generated images that better match the scene graph, have higher visual quality, and support more complex scene graphs. In addition, the embedding scheme supports multiple and diverse output images per scene graph, which can be further controlled by the user. We demonstrate two modes of per-object control: (i) importing elements from other images, and (ii) navigation in the object space, by selecting an appearance archetype. Our code is publicly available at https://www.github.com/ashual/scene_generation
description: Best Paper Honorable Mention in ICCV 2019
Liomera pallida
Creators: name: Castro, Peter
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Xanthidae
Liomera
Liomera pallida

description: Liomera pallida (Borradaile, 1900)
 Carpiliodes [sic] pallidus Borradaile, 1900: 586, pl. 40, fig. 3 [type locality: Rotuma (Fiji); syntypes: UMZC]. Hawaiian Is. record:
 Carpilodes pallidus Borradaile, 1900 — Edmondson 1951: 228, fig. 28 [O‘ahu].
 Taxonomy. Serène (1984)
 Geographical distribution. Across Indo-West Pacific region.
 Habitat. Intertidal, shallow subtidal to 91 m.
description: Published as part of Castro, Peter, 2011, Catalog of the anomuran and brachyuran crabs (Crustacea: Decapoda: Anomura, Brachyura) of the Hawaiian Islands 2947, pp. 1-154 in Zootaxa 2947 (1) on page 98, DOI: 10.11646/zootaxa.2947.1.1, http://zenodo.org/record/5283044
Quintessential brane cosmology
Creators: name: Kunze, K. E.
name: Vazquez-Mozo, M. A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study a class of braneworlds where the cosmological evolution arises as the result of the movement of a three-brane in a five-dimensional static dilatonic bulk, with and without reflection symmetry. The resulting four-dimensional Friedmann equation includes a term which, for a certain range of the parameters, effectively works as a quintessence component, producing an acceleration of the universe at late times. Using current observations and bounds derived from big-bang nucleosynthesis we estimate the parameters that characterize the model.
description: 29 pages. LaTeX. 5 postscript figures included. v2 typos corrected and references added. Final version to appear in Phys.Rev.D
The Banach-Mazur compactum is the Alexandroff compactification of a Hilbert cube manifold
Creators: name: Ageev, Sergei M.
name: Bogatyi, Semeon A.
name: Repovš, Dušan
Publisher: name: arXiv
Year: 2002
Subjects: subject: Geometric Topology (math.GT)
subject: General Topology (math.GN)
subject: FOS: Mathematics
subject: 57S10, 54C55

description: We prove that for every $n>2$, the Banach-Mazur compactum Q(n) is the compactification of a Hilbert cube manifold by the Euclidean point. For $n=2$ this result was proved earlier.
Additional file 1 of Can a ‘rewards-for-exercise app’ increase physical activity, subjective well-being and sleep quality? An open-label single-arm trial among university staff with low to moderate physical activity levels
Creators: name: Lemola, Sakari
name: Gkiouleka, Anna
name: Brieze Read
name: Realo, Anu
name: Lukasz Walasek
name: Tang, Nicole K. Y.
name: Elliott, Mark T.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Science Policy

description: Additional file 1: Table S1. List of products available from retail outlets in the University campus offered as rewards on the in-app local marketplace. Table S2. Intention to Treat Analysis’ Results.
ANN4EOR: Artificial Neural Network for Enhanced Oil Recovery Screening
Creators: name: Yohanes Nuwara
Publisher: name: Zenodo
Year: 2020
Subjects: neural-network
enhanced-oil-recovery
python

description: This is a mini-project that I took part in Machine Learning for Physicist summer training program with Prof. Dr. Florian Marquardt from Max Planck Institute for the Science of Light, Erlangen, Germany, on August 4, 2020. Due to COVID-19 pandemic, this presentation was brought virtually. As an engineer, I brought this project to investigate the performance of Neural Network to screen EOR methods on 245 synthetic datasets comprising field observations of oil viscosity, gravity, reservoir temperature, and so on. I generated datasets using random technique, 245 dummy field observations, each containing 6 reservoir fluid and rock parameters. These datasets are the my train datasets. These 6 parameters are the input features for the NN. The datasets are labeled with each of 7 EOR methods. I generated as well, another 50 dummy field observations, without label. These datasets are the my test datasets, for prediction. 2 hidden layers with 100 and 50 hidden neurons are used, with Adam optimizer and Categorical Cross-entropy loss function.
Evaluating the Potential of Quantum Machine Learning in Cybersecurity: A Case-Study on PCA-based Intrusion Detection Systems
Creators: name: Bellante, Armando
name: Fioravanti, Tommaso
name: Carminati, Michele
name: Zanero, Stefano
name: Luongo, Alessandro
Publisher: name: arXiv
Year: 2025
Subjects: subject: Quantum Physics (quant-ph)
subject: Cryptography and Security (cs.CR)
subject: Machine Learning (cs.LG)
subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Quantum computing promises to revolutionize our understanding of the limits of computation, and its implications in cryptography have long been evident. Today, cryptographers are actively devising post-quantum solutions to counter the threats posed by quantum-enabled adversaries. Meanwhile, quantum scientists are innovating quantum protocols to empower defenders. However, the broader impact of quantum computing and quantum machine learning (QML) on other cybersecurity domains still needs to be explored. In this work, we investigate the potential impact of QML on cybersecurity applications of traditional ML. First, we explore the potential advantages of quantum computing in machine learning problems specifically related to cybersecurity. Then, we describe a methodology to quantify the future impact of fault-tolerant QML algorithms on real-world problems. As a case study, we apply our approach to standard methods and datasets in network intrusion detection, one of the most studied applications of machine learning in cybersecurity. Our results provide insight into the conditions for obtaining a quantum advantage and the need for future quantum hardware and software advancements.
description: Computers & Security (2025): 104341
QuTiBench: Benchmarking Neural Networks on Heterogeneous Hardware
Creators: name: Blott, Michaela
name: Halder, Lisa
name: Leeser, Miriam
name: Doyle, Linda
Publisher: name: arXiv
Year: 2019
Subjects: subject: Hardware Architecture (cs.AR)
subject: FOS: Computer and information sciences

description: Neural Networks have become one of the most successful universal machine learning algorithms. They play a key role in enabling machine vision and speech recognition for example. Their computational complexity is enormous and comes along with equally challenging memory requirements, which limits deployment in particular within energy constrained, embedded environments. In order to address these implementation challenges, a broad spectrum of new customized and heterogeneous hardware architectures have emerged, often accompanied with co-designed algorithms to extract maximum benefit out of the hardware. Furthermore, numerous optimization techniques are being explored for neural networks to reduce compute and memory requirements while maintaining accuracy. This results in an abundance of algorithmic and architectural choices, some of which fit specific use cases better than others. For system level designers, there is currently no good way to compare the variety of hardware, algorithm and optimization options. While there are many benchmarking efforts in this field, they cover only subsections of the embedded design space. None of the existing benchmarks support essential algorithmic optimizations such as quantization, an important technique to stay on chip, or specialized heterogeneous hardware architectures. We propose a novel benchmark suite, QuTiBench, that addresses this need. QuTiBench is a novel multi-tiered benchmarking methodology that supports algorithmic optimizations such as quantization and helps system developers understand the benefits and limitations of these novel compute architectures in regard to specific neural networks and will help drive future innovation. We invite the community to contribute to QuTiBench in order to support the full spectrum of choices in implementing machine learning systems.
The Formation of Close Binary Systems by Dynamical Interactions and Orbital Decay
Creators: name: Bate, Matthew R.
name: Bonnell, Ian A.
name: Bromm, Volker
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from the first hydrodynamical star formation calculation to demonstrate that close binary stellar systems (separations $\lsim 10$ AU) need not be formed directly by fragmentation. Instead, a high frequency of close binaries can be produced through a combination of dynamical interactions in unstable multiple systems and the orbital decay of initially wider binaries. Orbital decay may occur due to gas accretion and/or the interaction of a binary with its circumbinary disc. These three mechanisms avoid the problems associated with the fragmentation of optically-thick gas to form close systems directly. They also result in a preference for close binaries to have roughly equal-mass components because dynamical exchange interactions and the accretion of gas with high specific angular momentum drive mass ratios towards unity. Furthermore, due to the importance of dynamical interactions, we find that stars with greater masses ought to have a higher frequency of close companions, and that many close binaries ought to have wide companions. These properties are in good agreement with the results of observational surveys.
description: Published in MNRAS, 10 pages, 6 figures (5 degraded). Paper with high-resolution figures and animations available from http://www.astro.ex.ac.uk/people/mbate
Spatial distribution of photoelectrons participating in formation of x-ray absorption spectra
Creators: name: Sipr, Ondrej
Publisher: name: arXiv
Year: 2002
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Interpretation of x-ray absorption near-edge structure (XANES) experiments is often done via analyzing the role of particular atoms in the formation of specific peaks in the calculated spectrum. Typically, this is achieved by calculating the spectrum for a series of trial structures where various atoms are moved and/or removed. A more quantitative approach is presented here, based on comparing the probabilities that a XANES photoelectron of a given energy can be found near particular atoms. Such a photoelectron probability density can be consistently defined as a sum over squares of wave functions which describe participating photoelectron diffraction processes, weighted by their normalized cross sections. A fine structure in the energy dependence of these probabilities can be extracted and compared to XANES spectrum. As an illustration of this novel technique, we analyze the photoelectron probability density at the Ti K pre-edge of TiS2 and at the Ti K-edge of rutile TiO2.
description: Journal abstract available on-line at http://link.aps.org/abstract/PRB/v65/e205115
Investigation of the transport and absorption of Angelica sinensis polysaccharide through gastrointestinal tract both in vitro and in vivo
Creators: name: Wang, Kaiping
name: Cheng, Fang
name: Pan, Xianglin
name: Zhou, Tao
name: Liu, Xiqiu
name: Zheng, Ziming
name: Luo, Li
name: Zhang, Yu
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Information Systems not elsewhere classified

description: To investigate the absorption and delivery of ASP in gastrointestinal (GI) tract, cASP was successfully synthesized by chemically modifying with succinic anhydride and then conjugating with a near infrared fluorescent dye Cy5.5. Then, the capacity of oral absorption of cASP was evaluated. The results demonstrated that cASP had low toxicity and no disruption on the integrity of cell membrane. The endocytosis of cASP into the epithelial cells was time- and energy-dependent, which was mediated by macropinocytosis pathway and clathrin- and caveolae (or lipid raft)-related routes. Otherwise, the actin filaments played a relatively weak role at the same time. The transport study illustrated that cASP could penetrate through the epithelial monolayer and mainly mediated by the same routes as that in the endocytosis experiment. Moreover, both in vitro Ussing chamber and in vivo ligated intestinal loops models indicated that cASP could be diffused through the mucus barriers and be absorbed in the whole small intestine. Finally, near-infrared fluorescence imaging presented that cASP could be absorbed and circulated into the blood, then distributed into various organs after oral administration. In conclusion, ASP could be absorbed after oral administration through endocytosis process mainly mediated by macropinocytosis pathway and clathrin- and caveolae (or lipid raft)-related routes, then be absorbed and circulated into blood. This study presents a comprehensive understanding of oral delivery of cASP, which will provide theoretical basis for the clinical application of ASP.
Double-spin cos(phi) Asymmetry in Semi-inclusive Electroproduction
Creators: name: Oganessyan, K. A.
name: Mulders, P. J.
name: De Sanctis, E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the double-spin cos(phi) asymmetry for pion electroproduction in semi-inclusive deep inelastic scattering of longitudinally polarized leptons off longitudinally polarized protons. We estimate the size of the asymmetry in the approximation where all twist-3 interaction-dependent distribution and fragmentation functions are set to zero. In that approximation at HERMES kinematics a sizable negative cos(phi) double-spin asymmetry for pi+ electroproduction is predicted.
description: LaTeX, 5 pages, 2 figures. Minor changes, figure modified. Final version to appear in Phys.Lett. B
РАЗРАБОТКА СТАРТАП-ПРОЕКТОВ НА ОСНОВЕ ИССЛЕДОВАНИЯ ЦИНК-ИОННЫХ АККУМУЛЯТОРОВ НА ВОДНОЙ ОСНОВЕ, МОДИФИЦИРОВАННЫХ ДОБАВКАМИ НИТРОИМИДАЗОЛА
Creators: name: Низамханова, Маликапашша
Publisher: name: Zenodo
Year: 2024

description: Чтобы удовлетворить основные стратегические потребности страны в целях развития «углеродного пика» и «углеродной нейтральности», а также активно разрабатывать новые энергетические системы, мы надеемся решить проблемы дефицита ресурсов литиевых батарей и низкой экологической безопасности. Использование недорогих, высоко безопасных и экологически чистых цинк-ионных аккумуляторов на водной основе является жизнеспособной альтернативой [1,2]. Однако цинковые электроды подвержены таким проблемам, как рост дендритов и реакция выделения водорода в воде, что приводит к неровной поверхности батареи и выходу ее из строя.
Mid-IR Variability and Dust Reverberation Mapping of Low-$z$ Quasars. I. Data, Methods and Basic Results
Creators: name: Lyu, Jianwei
name: Rieke, George H.
name: Smith, Paul S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The continued operation of the Wide-field Infrared Survey Explorer (WISE) combined with several ground-based optical transient surveys (e.g., CRTS, ASAS-SN and PTF) offer an unprecedented opportunity to explore the dust structures in luminous AGNs. We use these data for a mid-IR dust reverberation mapping (RM) study of 87 archetypal Palomar-Green quasars at $z\lesssim0.5$. To cope with various contaminations of the photometry data and the sparse time sampling of the light curves, procedures to combine these datasets and retrieve the dust RM signals have been developed. We find $\sim$70% of the sample (with a completeness correction, up to 95%) have convincing mid-IR time-lags in the WISE W1 ($\sim3.4~μm$) and W2 ($\sim4.5~μm$) bands and they are proportional to the square root of the AGN luminosity. Combined with previous K-band ($\sim2.2~μm$) RM results in the literature, the inferred dust emission size ratios are $R_{K}:R_{W1}:R_{W2}=0.6:1:1.2$. Under simple assumptions, we put preliminary constraints on the projected dust surface density at these bands and reveal the possibly different torus structures among hot-dust-deficient, warm-dust-deficient and normal quasars from the reverberation signals. With multi-epoch Spitzer data and later WISE photometry, we also explore AGN IR variability at 10--24 $μm$ over a 5-year time-scale. Except for blazars and flat-spectrum radio sources, the majority of AGNs have typical variation amplitudes at 24 $μm$ no more than 10% of that in the W1 band, indicating the dust reverberation signals damp out quickly at longer wavelengths. In particular, steep-spectrum radio quasars also lack strong 24 $μm$ variability, consistent with the unification picture of radio-loud AGN.
description: ApJ accepted (35 pages, 21 figures), revised to match the published paper