cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Polymer Release out of a Spherical Vesicle through a Pore
Creators: name: Park, Pyeong Jun
name: Sung, Wokyung
Publisher: name: arXiv
Year: 1998
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Translocation of a polymer out of curved surface or membrane is studied via mean first passage time approach. Membrane curvature gives rise to a constraint on polymer conformation, which effectively drives the polymer to the outside of membrane where the available volume of polymer conformational fluctuation is larger. Considering a polymer release out of spherical vesicle, polymer translocation time $τ$ is changed to the scaling behavior $τ\sim L^2$ for $R
description: 14 pages RevTeX, 6 postscript figures, published in Phys. Rev. E 57, 730 (1998)
Self-trapping and stable localized modes in nonlinear photonic crystals
Creators: name: Mingaleev, Serge F.
name: Kivshar, Yuri S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We predict the existence of stable nonlinear localized modes near the band edge of a two-dimensional reduced-symmetry photonic crystal with a Kerr nonlinearity. Employing the technique based on the Green function, we reveal a physical mechanism of the mode stabilization associated with the effective nonlinear dispersion and long-range interaction in the photonic crystals.
description: 4 pages (RevTex) with 5 figures (EPS)
Entropy of gravitons produced in the early Universe
Creators: name: Kiefer, C.
name: Polarski, D.
name: Starobinsky, A. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Gravitons produced from quantum vacuum fluctuations during an inflationary stage in the early Universe have zero entropy as far as they reflect the time evolution (squeezing) of a pure state, their large occupation number notwithstanding. A non-zero entropy of the gravitons (classical gravitational waves (GW) after decoherence) can be obtained through coarse graining. The latter has to be physically justified {\it and} should not contradict observational constraints. We propose two ways of coarse graining for which the fixed temporal phase of each Fourier mode of the GW background still remains observable: one based on quantum entanglement, and another one following from the presence of a secondary GW background. The proposals are shown to be mutually consistent. They lead to the result that the entropy of the primordial GW background is significantly smaller than it was thought earlier. The difference can be ascribed to the information about the regular (inflationary) initial state of the Universe which is stored in this background and which reveals itself, in particular, in the appearance of primordial peaks (acoustic peaks in the case of scalar perturbations) in the multipole spectra of the CMB temperature anisotropy and polarization.
description: 8 pages, REVTEX, final version to match the version to be published in Phys. Rev. D; minor additions in the Introduction, results unchanged
Classical and relativistic evolution of an extra-galactic jet with back-reaction
Creators: name: Zaninetti, Lorenzo
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We consider a turbulent jet which is moving in a Lane--Emden ($n=5$) medium. The conserved quantity is the energy flux, which allows finding, to first order, an analytical expression for the velocity and an approximate trajectory. The conservation of the relativistic flux for the energy allows deriving, to first order, an analytical expression for the velocity, and numerically determining the trajectory. The back-reaction due to the radiative losses for the trajectory is evaluated both in the classical and the relativistic case.
description: 19 pages and 11 figures
Polymer translocation induced by adsorption
Creators: name: Park, Pyeong Jun
name: Sung, Wokyung
Publisher: name: arXiv
Year: 1998
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We study the translocation of a flexible polymer through a pore in a membrane induced by its adsorption on \trans side of the membrane. When temperature $T$ is higher than $T_c$, the adsorption-desorption transition temperature, attractive interaction between polymer and membrane plays little role in affecting polymer conformation, leading to translocation time that scales as $τ\sim L^3$ where $L$ is the polymer contour length. When $T < T_c$, however, the translocation time undergoes a sharp crossover to $τ\sim L^2$ for sufficiently long polymers, following the second order conformational (adsorption) transition. The translocation time is found to exhibit the crossover around $T=T_c'$, which is lower than $T_c$ for polymers shorter than a critical length($N
description: 19 pages RevTeX, 5 postscript figures, to be published in J. Chem. Phys. 108(7), 3013 (1998)
Additional file 3 of Case report: first symptomatic Candidatus Neoehrlichia mikurensis infection in Slovenia
Creators: name: Lenart, Mitja
name: Simoniti, Miha
name: Strašek-Smrdel, Katja
name: Špik, Vesna Cvitković
name: Selič-Kurinčič, Tanja
name: Avšič-Županc, Tatjana
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Ecology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 3: Figure 2. Phylogenetic tree of 16S rDNA gene sequences inferred using Maximum Likelihood method based on the Tamura-Nei model (1). The scale barr indicates the number of base substitutions per site (1516 positions).
muCool: A novel low-energy muon beam for future precision experiments
Creators: name: Belosevic, I.
name: Antognini, A.
name: Bao, Y.
name: Eggenberger, A.
name: Hildebrandt, M.
name: Iwai, R.
name: Kaplan, D. M.
name: Khaw, K. S.
name: Kirch, K.
name: Knecht, A.
name: Papa, A.
name: Petitjean, C.
name: Phillips, T. J.
name: Piegsa, F. M.
name: Ritjoho, N.
name: Stoykov, A.
name: Taqqu, D.
name: Wichmann, G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: Experiments with muons ($μ^{+}$) and muonium atoms ($μ^{+}e^{-}$) offer several promising possibilities for testing fundamental symmetries. Examples of such experiments include search for muon electric dipole moment, measurement of muon $g-2$ and experiments with muonium from laser spectroscopy to gravity experiments. These experiments require high quality muon beams with small transverse size and high intensity at low energy. At the Paul Scherrer Institute, Switzerland, we are developing a novel device that reduces the phase space of a standard $μ^{+}$ beam by a factor of $10^{10}$ with $10^{-3}$ efficiency. The phase space compression is achieved by stopping a standard $μ^{+}$ beam in a cryogenic helium gas. The stopped $μ^{+}$ are manipulated into a small spot with complex electric and magnetic fields in combination with gas density gradients. From here, the muons are extracted into the vacuum and into a field-free region. Various aspects of this compression scheme have been demonstrated. In this article the current status will be reported.
description: 8 pages, 5 figures, TCP 2018 conference proceedings
Observing Microscopic Transitions from Macroscopic Bursts: Instability-Mediated Resetting in the Incoherent Regime of the $D$-dimensional Generalized Kuramoto Model
Creators: name: Chandra, Sarthak
name: Ott, Edward
Publisher: name: arXiv
Year: 2019
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Chaotic Dynamics (nlin.CD)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: We consider a recently introduced $D$-dimensional generalized Kuramoto model for many $(N\gg 1)$ interacting agents in which the agent states are $D$-dimensional unit vectors. It was previously shown that, for even $D$, similar to the original Kuramoto model ($D=2$), there exists a continuous dynamical phase transition from incoherence to coherence of the time asymptotic attracting state as the coupling parameter $K$ increases through a critical value $K_c^{(+)}>0$. We consider this transition from the point of view of the stability of an incoherent state, i.e., where the $N\to\infty$ distribution function is time-independent and the macroscopic order parameter is zero. In contrast with $D=2$, for even $D>2$ there is an infinity of possible incoherent equilibria, each of which becomes unstable with increasing $K$ at a different point $K=K_c$. We show that there are incoherent equilibria for all $K_c$ within the range $(K_c^{(+)}/2)\leq K_c \leq K_c^{(+)}$. How can the possible instability of incoherent states arising at $K=K_cK_c^{(+)}$? We find, for a given incoherent equilibrium, that, if $K$ is rapidly increased from $K
description: 15 pages, 6 figures
Additional file 2 of Case report: first symptomatic Candidatus Neoehrlichia mikurensis infection in Slovenia
Creators: name: Lenart, Mitja
name: Simoniti, Miha
name: Strašek-Smrdel, Katja
name: Špik, Vesna Cvitković
name: Selič-Kurinčič, Tanja
name: Avšič-Županc, Tatjana
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Ecology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2: Figure 1. Phylogenetic tree of operon groEL sequences inferred using Maximum Likelihood method based on the Tamura-Nei model (1). The scale barr indicates the number of base substitutions per site (1766 positions).
Relativistic Diskoseismology. II. Analytical Results for C-modes
Creators: name: Silbergleit, Alexander S.
name: Wagoner, Robert V.
name: Ortega-Rodriguez, Manuel
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We first briefly review how we investigate the modes of oscillation trapped within the inner region of accretion disks by the strong-field gravitational properties of a black hole (or a compact, weakly-magnetized neutron star). Then we focus on the `corrugation'(c)-modes, nearly incompressible perturbations of the inner disk. The fundamental c-modes have eigenfrequencies (ordered by radial mode number) which correspond to the Lense-Thirring frequency, evaluated at the outer trapping radius of the mode, in the slow rotation limit. This trapping radius is a decreasing function of the black hole angular momentum, so a significant portion of the disk is modulated only for slowly rotating black holes. The eigenfrequencies are thus strongly increasing functions of black hole angular momentum. The dependence of the eigenfrequencies on the speed of sound within (or the luminosity) within the disk is very weak, except for slowly rotating black holes.
description: Submitted to The Astrophysical Journal. 33 pages, 5 figures
Additional file 1 of Case report: first symptomatic Candidatus Neoehrlichia mikurensis infection in Slovenia
Creators: name: Lenart, Mitja
name: Simoniti, Miha
name: Strašek-Smrdel, Katja
name: Špik, Vesna Cvitković
name: Selič-Kurinčič, Tanja
name: Avšič-Županc, Tatjana
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Ecology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1: Table 1. Primers and their sequences for PCRs and sequencing.
Neurocysticercosis: Are the Criteria Diagnostic Enough?
Creators: name: Rodriguez-Leyva, Ildefonso
name: Orozco-Narvaez, Alejandro
name: Mayorga, Adriana Patricia Martínez
Publisher: name: Zenodo
Year: 2021
Subjects: Neurocysticercosis
central nervous system
epilepsy
helminthes

description: Neurocysticercosis (NCC) is a common disease produced by helminths (larval form of Taenia Solium) in the Central Nervous System (CNS). It is one of the common causes of epilepsy in the world. Without aggressive treatment, it continues to be associated with high mortality, with intracranial hypertension, and a lack of seizure control. This chapter reviews several cases of patients with secondary epilepsy who meet the diagnostic criteria for NCC and compares 2001 and 2016 diagnostic criteria: one of the cases with a definitive diagnosis, and the rest with a probable diagnosis. This problem is common for residents of regions where cysticercosis is an endemic zone, like in Mexico. Most patients presented clinical courses and image studies highly suggestive of NCC and positive ELISA testing for cysticerci in CSF. We emphasize the importance of ruling out the differential diagnosis, especially in endemic areas, questioning the use of ELISA in the CSF testing for cysticerci antibodies seems to be not enough, and advise caution when interpreting cystic lesions as having a discernible scolex because potential mimics are not infrequent.
Logarithmic density relaxation in compaction of granular materials
Creators: name: Peng, Gongwen
name: Ohta, Takao
Publisher: name: arXiv
Year: 1997
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: On the basis of physical considerations we propose a one-dimensional discrete lattice model for the density relaxation of granular materials under tapping. Solving the difference equation numerically, we find a logarithmic time-dependence of the density relaxation. This is in agreement with experimental results of Knight et al. [Phys. Rev. E 51, 3957(1995)]. The origin of this anomalous relaxation is elucidated analytically by solving the equation of its continuum version asymptotically in time.
description: 12 pages, RevTex, 5 figures in postscript
BARWIENIE BETONU - PRAKTYCZNE WSKAZÓWKI cz 1.pdf
Creators: name: Kurpinski, Konrad
Publisher: name: figshare
Year: 2020
Subjects: subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: Produkowane w Polsce i importowane pigmenty stosowane w produkcji betonu barwionego są wysokoprocentowymi tlenkami żelaza. Są to substancje bezwonne, nietoksyczne i niepalne. Cechują się wysoką jakością w zakresie intensywności barwienia, zdolnością krycia i łatwością rozprowadzania w suchych mieszankach. Oferta rynkowa pigmentów jest bardzo bogata. Pigmenty dostępne są w postaci płynnej, granulatu lub proszku. Możliwe jest stosowanie pigmentów organicznych lub nieorganicznych.
Ferramenta da Psicanálise: Análise de Processos de Transtorno de Personalidade Narcisista
Creators: name: Brandl, Edenilson
Publisher: name: Zenodo
Year: 2024
Subjects: Ferramenta da Psicanálise
Análise de Processos de Transtorno de Personalidade Narcisista
Psicanálise
Enciclopédia da Conscienciologia

description: Definologia: A análise de processos de transtorno de personalidade narcisista é uma ferramenta da psicanálise voltada para a compreensão dos mecanismos psíquicos, dinâmicas inconscientes e manifestações comportamentais característicos do transtorno de personalidade narcisista, visando identificar suas origens, sintomatologia e possíveis estratégias terapêuticas.
Spanish varieties in the classroom - Questionnaire to teachers
Creators: name: Gutierrez, Mara Fuertes
Publisher: name: The Open University
Year: 2019
Subjects: subject: 200308 Iberian Languages
subject: FOS: Languages and literature
subject: 200406 Language in Time and Space (incl. Historical Linguistics, Dialectology)
subject: 200405 Language in Culture and Society (Sociolinguistics)
subject: 200401 Applied Linguistics and Educational Linguistics
subject: Linguistics

description: Data collection instrument (questionnaire) used to collect responses from Spanish language lecturers and teachers on their beliefs and everyday practices related to which linguistic varieties should be taught to non-native students of Spanish
Eclipsing Spotted Giant Star With K2 and Historical Photometry
Creators: name: Oláh, K.
name: Rappaport, S.
name: Borkovits, T.
name: Jacobs, T.
name: Latham, D.
name: Bieryla, A.
name: Bíró, I. B.
name: Bartus, J.
name: Kővári, Zs.
name: Vida, K.
name: Vanderburg, A.
name: LaCourse, D.
name: Csányi, I.
name: Bakos, G. Á.
name: Bhatti, W.
name: Csubry, Z.
name: Hartman, J.
name: Omohundro, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. Stars can maintain their observable magnetic activity from the PMS to the tip of the red giant branch. However, the number of known active giants is much lower than active stars on the main sequence since on the giant branch the stars spend only about 10% of their main sequence lifetime. Due to their rapid evolution it is difficult to estimate the stellar parameters of giant stars. A possibility for obtaining more reliable stellar parameters of an active giant arises when it is a member of an eclipsing binary system. Aims. We have discovered EPIC 211759736, an active spotted giant star in an eclipsing binary system during the Kepler K2 Campaign 5. The eclipsing nature allows us to much better constrain the stellar parameters than in most cases of active giant stars. Method. We have combined the K2 data with archival HATNet and DASCH photometry, new spectroscopic radial velocity measurements, and a set of follow-up ground-based BVRI photometric observations, to find the binary system parameters as well as robust spot models for the giant at two different epochs. Results. We determined the physical parameters of both stellar components and provide a description of the rotational and long-term activity of the primary component. The temperatures and luminosities of both components were examined in the context of the HR diagram. We find that both the primary and the secondary components deviate from the evolutionary tracks corresponding to their masses in the sense that the stars appear in the diagram at lower masses than their true masses. Conclusions. We further evaluate the proposition that active giants have masses that are found to be generally higher by traditional methods than are indicated by stellar evolution tracks in the HR diagram. A possible reason for this discrepancy could be a strong magnetic field, since we see greater differences in more active stars.
description: Accepted for publication in Astronomy and Astrophysics
Additional file 1: of Utilizing a low-carbohydrate/high-protein diet to improve metabolic health in individuals with spinal cord injury (DISH): study protocol for a randomized controlled trial
Creators: name: Yarar-Fisher, Ceren
name: Li, Jia
name: McLain, Amie
name: Gower, Barbara
name: Oster, Robert
name: Morrow, Casey
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: SPIRIT checklist. (DOC 128 kb)
Antheua tricolor Walker 1855
Creators: name: Mbata, Keith J.
name: Prins, Jurate De
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Notodontidae
Antheua
Antheua tricolor

description: Antheua tricolor Walker, 1855a
COMMON NAME(S): Tricoloured Frill.
SYNONYM(S): Antheua varia Walker, 1855a.
IUCN STATUS: Not Evaluated (NE).
DISTRIBUTION: Botswana, Burkina Faso, Democratic Republic of Congo, Ethiopia, Gambia, Kenya, Malawi, Mozambique, Namibia, Sierra Leone, South Africa, Sudan, Tanzania, Zambia, Zimbabwe.
LOCALITY IN ZAMBIA: Petauke in Eastern Province.
LARVAL HOSTPLANT(S): Larval foodplants include various species of grasses (Poaceae) including Pennisetum purpureum Schumach., and a yet to be identified Cyperaceae species, Carex sp.
SOURCES: African Moths 2019; Catalogue of Life 2017; De Prins & De Prins 2022; Pinhey 1975.
Genus Eutimia Wallengren, 1858
description: Published as part of Mbata, Keith J. & Prins, Jurate De, 2023, Annotated checklist of moths of Zambia (Insecta: Lepidoptera), pp. 1-503 in Zootaxa 5354 (1) on page 268, DOI: 10.11646/zootaxa.5354.1.1, http://zenodo.org/record/10130434
Additional file 1 of Real-time automatic uncertainty estimation of coseismic single rectangular fault model using GNSS data
Creators: name: Ohno, Keitaro
name: Ohta, Yusaku
name: Kawamoto, Satoshi
name: Abe, Satoshi
name: Hino, Ryota
name: Koshimura, Shunichi
name: Musa, Akihiro
name: Kobayashi, Hiroaki
Publisher: name: figshare
Year: 2021
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Additional file 1: Table S1. Fault parameters of 60 simulated earthquakes. Figure S1. Computation times required for the “RUNE” algorithm ( $$1.1\times {10}^{6}$$ 1.1 × 10 6 steps per chain using eight parallel chains). Figure S2. All marginal PDFs for the 2016 Kumamoto earthquake (60 s after the origin time). Figure S3. All marginal PDFs for the 2019 Yamagata-Oki earthquake. Figure S4. Map of 60 simulated earthquakes. Figure S5. Marginal PDFs between VR and Mw. Figure S6. Expected seafloor crustal deformation based on the estimated coseismic fault model.
Scalar GW detection with a hollow spherical antenna
Creators: name: Coccia, E.
name: Fucito, F.
name: Lobo, J. A.
name: Salvino, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the response and cross sections for the absorption of GW energy in a Jordan-Brans-Dicke theory by a resonant mass detector shaped as a hollow sphere.
description: latex file, 9 pages
Structure elucidation of a new terpenylated coumarin with the combination of CASE algorithms and DFT/NMR approach
Creators: name: Lv, Tian-Ming
name: Guo, Rui
name: Yan, Zhi-Yang
name: Du, Ye-Qing
name: Lin, Bin
name: Huang, Xiao-Xiao
name: Song, Shao-Jiang
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Physical Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Hematology

description: One new terpenylated coumarin ailanthuscoumarin was isolated from the root barks of Ailanthus altissima (Mill.) Swingle. The high oxidation of the compound led to the difficulty of structure elucidation by 2D-NMR spectra. Its structure was determined with the aid of computer-assisted structure elucidation (CASE) expert systems and Gauge-independent atomic orbital (GIAO) NMR calculations. The absolute configuration of ailanthuscoumarin was determined by the comparison between the experimental and calculated electronic circular dichroism (ECD) spectra. The anti-hepatoma activity of ailanthuscoumarin against two human hepatoma cells (Hep3B, HepG2) was also reported.
Additional file 9 of Successful implementation of a longitudinal skill-based teaching curriculum for residents
Creators: name: Rowat, Jane
name: Johnson, Krista
name: Antes, Lisa
name: White, Katherine
name: Rosenbaum, Marcy
name: Suneja, Manish
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences

description: Additional file 9: Supplemental Table 9. AAMC graduation questionnaire: “Residents provide effective teaching during clerkship.”
A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
Creators: name: Armendariz-Picon, C.
name: Mukhanov, V.
name: Steinhardt, Paul J.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Increasing evidence suggests that most of the energy density of the universe consists of a dark energy component with negative pressure, a ``cosmological constant" that causes the cosmic expansion to accelerate. In this paper, we address the puzzle of why this component comes to dominate the universe only recently rather than at some much earlier epoch. We present a class of theories based on an evolving scalar field where the explanation is based entirely on internal dynamical properties of the solutions. In the theories we consider, the dynamics causes the scalar field to lock automatically into a negative pressure state at the onset of matter-domination such that the present epoch is the earliest possible time, consistent with nucleosynthesis restrictions, when it can start to dominate.
description: 5 pages, 3 figures
“Requests” and “offers” in orangutans and human infants
Creators: name: Rossano, Federico
name: Liebal, Katja
Publisher: name: Freie Universität Berlin
Year: 2014
Subjects: subject: orangutans
subject: humans
subject: sharing
subject: 100 Philosophie und Psychologie::150 Psychologie::155 Differentielle Psychologie, Entwicklungspsychologie

description: This paper presents two pilot studies of sharing situations in orangutans and human infants. We report on the communicative behaviors that elicit food transfers, the contingencies associated with gesture selection and the (relative) success in obtaining food. We focus on the sequential unfolding of these interactional projects, on the timing between an initial action and the responsive move, and on the semiotic features that allow a participant to recognize (a) when a request has been produced, (b) when it has been unsuccessful and, (c) in the absence of success, when to pursue it further. We claim that the infrastructure for sequentially organized, cooperative social interaction and the capacity to selectively produce communicative actions predates language evolution and is, at least to some degree, shared with other primates.
Near Infrared spectroscopic indices for unresolved stellar populations. I. Template galaxy spectra
Creators: name: Francois, P.
name: Morelli, L.
name: Pizzella, A.
name: Ivanov, V. D.
name: Coccato, L.
name: Cesetti, M.
name: Corsini, E. M.
name: Bonta, E. Dalla
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A new generation of spectral synthesis models has been developed in the recent years, but there is no matching -- in terms of quality and resolution -- set of template galaxy spectra for testing and refining the new models. Our main goal is to find and calibrate new near-infrared spectral indices along the Hubble sequence of galaxies which will be used to obtain additional constraints to the population analysis based on medium resolution integrated spectra of galaxies. Spectra of previously studied and well understood galaxies with relatively simple stellar populations (e.g., ellipticals or bulge dominated galaxies) are needed to provide a baseline data set for spectral synthesis models. X-Shooter spectra spanning the optical and infrared wavelength (350-2400\,nm) of bright nearby elliptical galaxies with resolving power $ R\sim$4000-5400 were obtained. Heliocentric systemic velocity, velocity dispersion and Mg, Fe and \Hb\ line-strength indices are presented. We present a library of very high quality spectra of galaxies covering a large range of age, metallicity and morphological type. Such as a dataset of spectra will be crucial to address important questions of the modern investigation concerning galaxy formation and evolution.
description: accepted for publication in A&A (25 pages , 10 figures)
Tirathaba irrufatella Ragonot & Hampson 1901
Creators: name: Singh, Navneet
name: Ranjan, Rahul
name: Talukdar, Avishek
name: Joshi, Rahul
name: Kirti, Jagbir Singh
name: Chandra, Kailash
name: Mally, Richard
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Pyralidae
Tirathaba
Tirathaba irrufatella

description: 106. Tirathaba irrufatella Ragonot & Hampson, 1901: 462
Type locality: Japan
Distribution. Indian records: Khasis (Hampson 1903a). Global records: Japan (Hampson 1903a).
description: Published as part of Singh, Navneet, Ranjan, Rahul, Talukdar, Avishek, Joshi, Rahul, Kirti, Jagbir Singh, Chandra, Kailash & Mally, Richard, 2022, A catalogue of Indian Pyraloidea (Lepidoptera), pp. 1-423 in Zootaxa 5197 (1) on page 65, DOI: 10.11646/zootaxa.5197.1.1, http://zenodo.org/record/7252292
Additional file 1 of Trehalose in pine wood nematode participates in DJ3 formation and confers resistance to low-temperature stress
Creators: name: Chen, Qiaoli
name: Zhang, Ruizhi
name: Li, Danlei
name: Wang, Feng
name: Jiang, Shengwei
name: Wang, Jianan
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Cluster Dendrogram. Figure S2.KEGG enrichment analyses of genes in the magenta module. Figure S3.Signal peptide analysis. Figure S4. KEGG enrichment analyses of Bx-tpsand Bx-tpp coexpressed genes. Table S1. Primers used in cloning encoding sequence. Table S2.Target sequences for siRNA. Table S3.Primers used in RT-qPCR. Table S4. Statistical analysis of the RNA sequencing data. Table S5. Alignment results of trehalose metabolism related genes in pine wood nematode. Table S6. Expression of trehalose metabolism related genes after RNAi treatment. Table S7. Expression of trehalose metabolism related genes after RNAi treatment. Table S8. Selected genes in the magenta module with high weight value (>0.2) to Bx-tps or Bx-tpp.Table S9. KEGG enrichment for genes highly related to Bx-tps1 andBx-tps2. Table S10. Gene annotation result.
Ferromagnetism in a Hubbard model for an atomic quantum wire: a realization of flat-band magnetism from even-membered rings
Creators: name: Arita, R.
name: Kuroki, K.
name: Aoki, H.
name: Yajima, A.
name: Tsukada, M.
name: Watanabe, S.
name: Ichimura, M.
name: Onogi, T.
name: Hashizume, T.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We have examined a Hubbard model on a chain of squares, which was proposed by Yajima et al as a model of an atomic quantum wire As/Si(100), to show that the flat-band ferromagnetism according to a kind of Mielke-Tasaki mechanism should be realized for an appropriate band filling in such a non-frustrated lattice. Reflecting the fact that the flat band is not a bottom one, the ferromagnetism vanishes, rather than intensified, as the Hubbard U is increased. The exact diagonalization method is used to show that the critical value of U is in a realistic range. We also discussed the robustness of the magnetism against the degradation of the flatness of the band.
description: misleading terms and expressions are corrected, 4 pages, RevTex, 5 figures in Postscript, to be published in Phys. Rev. B (rapid communication)
Additional file 8 of Successful implementation of a longitudinal skill-based teaching curriculum for residents
Creators: name: Rowat, Jane
name: Johnson, Krista
name: Antes, Lisa
name: White, Katherine
name: Rosenbaum, Marcy
name: Suneja, Manish
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences

description: Additional file 8: Supplemental Table 8A. Confidence score after first year of participation in curriculum by program year. Supplemental Table 8B. Confidence score after second year of participation in curriculum by program year.
Fluctuation induced first order phase transition in thin films of type I superconductors
Creators: name: Folk, R.
name: Shopova, D. V.
name: Uzunov, D. I.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The effect of fluctuation induced weakly first order phase transition known for three dimensional (3D) type I superconductors appears in a modified and strongly enhanced variant in thin (quasi-2D) superconducting films. The unusual thermodynamic properties of this new type of first order phase transitions and the possibility for an experimental verification of the effect are established and discussed.
The XXL Survey: XXVII. The 3XLSS point source catalogue
Creators: name: Chiappetti, L.
name: Fotopoulou, S.
name: Lidman, C.
name: Faccioli, L.
name: Pacaud, F.
name: Elyiv, A.
name: Paltani, S.
name: Pierre, M.
name: Plionis, M.
name: Adami, C.
name: Alis, S.
name: Altieri, B.
name: Baldry, I.
name: Bolzonella, M.
name: Bongiorno, A.
name: Brown, M.
name: Driver, S.
name: Elmer, E.
name: Franzetti, P.
name: Grootes, M.
name: Guglielmo, V.
name: Iovino, A.
name: Koulouridis, E.
name: Lefevre, J. P.
name: Liske, J.
name: Maurogordato, S.
name: Melnyk, O.
name: Owers, M.
name: Poggianti, B.
name: Polletta, M.
name: Pompei, E.
name: Ponman, T.
name: Robotham, A.
name: Sadibekova, T.
name: Tuffs, R.
name: Valtchanov, I.
name: Vignali, C.
name: Wagner, G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the version of the point source catalogue of the XXL Survey that was used, in part, in the first series of XXL papers. In this paper we release, in our database in Milan and at CDS: (i) the X-ray source catalogue with 26056 objects in two areas of 25 deg2; (ii) the associated multiwavelength catalogues with candidate counterparts of the X-ray sources in the infrared, near-infrared, optical, and ultraviolet (plus spectroscopic redshift when available); and (iii) a catalogue of spectroscopic redshifts recently obtained in the southern XXL area. We also present the basic properties of the X-ray point sources and their counterparts. Other catalogues described in the second series of XXL papers will be released contextually, and will constitute the second XXL data release.
description: 19 pages, 11 figures, part of A&A Special Issue "The XXL Survey: second series" https://www.aanda.org/component/toc/?task=topic&id=927
Properties of cosmologies with dynamical pseudo Nambu-Goldstone bosons
Creators: name: Ng, S. C. C.
name: Wiltshire, D. L.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study observational constraints on cosmological models with a quintessence field in the form of a dynamical pseudo Nambu-Goldstone boson. After reviewing the properties of the solutions, from a dynamical systems phase space analysis, we consider the constraints on parameter values imposed by luminosity distances from the 60 Type Ia supernovae published by Perlmutter et al., and also from gravitational lensing statistics of distant quasars. In the case of the Type Ia supernovae we explicitly allow for the possibility of evolution of the peak luminosities of the supernovae sources, using simple empirical models which have been recently discussed in the literature. We find weak evidence to suggest that the models with supernovae evolution fit the data better in the context of the quintessence models in question. If source evolution is a reality then the greatest challenge facing these models is the tension between current value of the expansion age, H_0 t_0, and the fraction of the critical energy density, Omega_{phi0}, corresponding to the scalar field. Nonetheless there are ranges of the free parameters which fit all available cosmological data.
description: 22 pages, RevTeX, 13 figures, epsf. v3: References added, plus a few sentences to clarify some small points; v4: Typos fixed
Statistical outliers in random laser emission
Creators: name: Tommasi, Federico
name: Fini, Lorenzo
name: Ignesti, Emilio
name: Lepri, Stefano
name: Martelli, Fabrizio
name: Cavalieri, Stefano
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We provide theoretical and experimental evidence of statistical outliers in random laser emission that are not accounted for by the, now established, power-law tailed (Lévy) distribution. Such outliers manifest themselves as single, large isolated spikes over an otherwise smooth background. A statistical test convincingly shows that their probability is larger than the one extrapolated from lower-intensity events. To compare with experimental data, we introduced the anomaly parameter that allows for an identification of such rare events from experimental spectral measurements and that agrees as well with the simulations of our Monte Carlo model. A possible interpretation in terms of Black Swans or Dragon Kings, large events having a different generation mechanism from their peers, is discussed.
Chemical network reduction in protoplanetary disks
Creators: name: Xu, Rui
name: Bai, Xue-Ning
name: Öberg, Karin
name: Zhang, Hao
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Protoplanetary disks (PPDs) are characterized by different kinds of gas dynamics and chemistry, which are coupled via ionization, heating and cooling processes, as well as advective and turbulent transport. However, directly coupling gas dynamics with time-dependent chemistry is prohibitively computationally expensive when using comprehensive chemical reaction networks. In this paper, we evaluate the utility of a species-based network reduction method in different disk environments to produce small chemical networks that reproduce the abundances of major species found in large gas-phase chemistry networks. We find that the method works very well in disk midplane and surfaces regions, where approximately 20-30 gas phase species, connected by $\sim$50-60 gas phase reactions, are sufficient to reproduce the targeted ionization fraction and chemical abundances. Most species of the reduced networks, including major carriers of oxygen, carbon and nitrogen, also have similar abundances in the reduced and complete network models. Our results may serve as an initial effort for future hydrodynamic/magnetohydrodynamic simulations of PPDs incorporating time-dependent chemistry in appropriate regions. Accurately modeling the abundances of major species at intermediate disk heights, however, will require much more extended network incorporating gas-grain chemistry and are left for future studies.
description: accepted for publication in ApJ
Comorta atricostella Ragonot 1888
Creators: name: Singh, Navneet
name: Ranjan, Rahul
name: Talukdar, Avishek
name: Joshi, Rahul
name: Kirti, Jagbir Singh
name: Chandra, Kailash
name: Mally, Richard
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Pyralidae
Comorta
Comorta atricostella

description: 166. Comorta atricostella Ragonot, 1888: 48
Type locality: Indes orientales [East Indies]
Distribution. Indian records: Iles Andaman (Ragonot 1888). Global records: Indes orientales (Ragonot 1888), Bathurst (Ragonot 1888).
  Genus Copamyntis Meyrick, 1934: 495
 Type species: Elegia alectryonura Meyrick, 1932, by original designation
 = Compamyntis (misspell.) (Roesler & Küppers 1979)
description: Published as part of Singh, Navneet, Ranjan, Rahul, Talukdar, Avishek, Joshi, Rahul, Kirti, Jagbir Singh, Chandra, Kailash & Mally, Richard, 2022, A catalogue of Indian Pyraloidea (Lepidoptera), pp. 1-423 in Zootaxa 5197 (1) on page 79, DOI: 10.11646/zootaxa.5197.1.1, http://zenodo.org/record/7252292
Additional file 1: of Genetic assessment of inbred chicken lines indicates genomic signatures of resistance to Marekâ s disease
Creators: name: Xu, Lingyang
name: He, Yanghua
name: Ding, Yi
name: Liu, George
name: Zhang, Huanmin
name: Cheng, Hans
name: Taylor, Robert
name: Song, Jiuzhou
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Figure S1. Histogram plot of MD incidence (%) rate. MD resistance in chickens is generally evaluated with MD incidence (induced gross tumors by MDV) and survival day post MDV challenge, and the extent of resistance is dependent of the virulence of challenge viruses and other factors. Figure S2. Barplot show the call rate for 30 chickens on Affymetrix chicken SNP genotyping array. X axis represent the call rate values, and Y axis represents the chicken individuals. Figure S3. Frequency distribution in autosomes for a total of 527,021 SNPs on the Affymetrix chicken SNP genotyping array. Figure S4. Frequency distribution in autosomes for 155,216 SNPs on the Affymetrix chicken SNP genotyping array. Figure S5. Comparison of ROH regions among three groups, line 63, line 72, lines RCS (C, L, M, N, S, X). The overlap length of ROH was indicated in kb. (DOCX 35 kb)
Nonminimally coupled Weyl gravity
Creators: name: Gomes, Cláudio
name: Bertolami, Orfeu
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Weyl gravity in the presence of a non-minimal matter-curvature coupling is presented. Some properties arising from the non-metricity give rise to a second order theory whose vacuum is compatible with a cosmological constant, under conditions on the vector field.
description: 12 pages
Critical Behavior of Coupled q-state Potts Models under Weak Disorder
Creators: name: Simon, P.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We investigate the effect of weak disorder on different coupled $q$-state Potts models with $q\le 4$ using two loops renormalisation group. This study presents new examples of first order transitions driven by randomness. We found that weak disorder makes the models decouple. Therefore, it appears that no relations emerge, at a perturbation level, between the disordered $q_1\times q_2$-state Potts model and the two disordered $q_1$, $q_2$-state Potts models ($q_1\ne q_2$), despite their central charges are similar according to recent numerical investigations. Nevertheless, when two $q$-state Potts models are considered ($q>2$), the system remains always driven in a strong coupling regime, violating apparently the Imry-Wortis argument.
description: 7 pages + 1 PS figure (Latex)
Self-Averaging, Distribution of Pseudo-Critical Temperatures and Finite Size Scaling in Critical Disordered Systems
Creators: name: Wiseman, S.
name: Domany, E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: The distributions $P(X)$ of singular thermodynamic quantities in an ensemble of quenched random samples of linear size $l$ at the critical point $T_c$ are studied by Monte Carlo in two models. Our results confirm predictions of Aharony and Harris based on Renormalization group considerations. For an Ashkin-Teller model with strong but irrelevant bond randomness we find that the relative squared width, $R_X$, of $P(X)$ is weakly self averaging. $R_X\sim l^{α/ν}$, where $α$ is the specific heat exponent and $ν$ is the correlation length exponent of the pure model fixed point governing the transition. For the site dilute Ising model on a cubic lattice, known to be governed by a random fixed point, we find that $R_X$ tends to a universal constant independent of the amount of dilution (no self averaging). However this constant is different for canonical and grand canonical disorder. We study the distribution of the pseudo-critical temperatures $T_c(i,l)$ of the ensemble defined as the temperatures of the maximum susceptibility of each sample. We find that its variance scales as $(δT_c(l))^2 \sim l^{-2/ν}$ and NOT as $\sim l^{-d}. We find that $R_χ$ is reduced by a factor of $\sim 70$ with respect to $R_χ(T_c)$ by measuring $χ$ of each sample at $T_c(i,l)$. We analyze correlations between the magnetization at criticality $m_i(T_c,l)$ and the pseudo-critical temperature $T_c(i,l)$ in terms of a sample independent finite size scaling function of a sample dependent reduced temperature $(T-T_c(i,l))/T_c$. This function is found to be universal and to behave similarly to pure systems.
description: 31 pages, 17 figures, submitted to Phys. Rev. E
Late-time evolution of the Yang-Mills field in the spherically symmetric gravitational collapse
Creators: name: Cai, Rong-Gen
name: Wang, Anzhong
Publisher: name: arXiv
Year: 1999
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We investigate the late-time evolution of the Yang-Mills field in the self-gravitating backgrounds: Schwarzschild and Reissner-Nordström spacetimes. The late-time power-law tails develop in the three asymptotic regions: the future timelike infinity, the future null infinity and the black hole horizon. In these two backgrounds, however, the late-time evolution has quantitative and qualitative differences. In the Schwarzschild black hole background, the late-time tails of the Yang-Mills field are the same as those of the neutral massless scalar field with multipole moment l=1. The late-time evolution is dominated by the spacetime curvature. When the background is the Reissner-Nordström black hole, the late-time tails have not only a smaller power-law exponent, but also an oscillatory factor. The late-time evolution is dominated by the self-interacting term of the Yang-Mills field. The cause responsible for the differences is revealed.
description: Revtex, 14 pages, no figures
BARWIENIE BETONU - poradnik wykonawcy cz 1.pdf
Creators: name: Kurpinski, Konrad
Publisher: name: figshare
Year: 2019
Subjects: subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: Produkowane w Polsce i importowane pigmenty stosowane w produkcji betonu barwionego są wysokoprocentowymi tlenkami żelaza. Są to substancje bezwonne, nietoksyczne i niepalne. Cechują się wysoką jakością w zakresie intensywności barwienia, zdolnością krycia i łatwością rozprowadzania w suchych mieszankach. Oferta rynkowa pigmentów jest bardzo bogata. Pigmenty dostępne są w postaci płynnej, granulatu lub proszku. Możliwe jest stosowanie pigmentów organicznych lub nieorganicznych.