cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Local Orthogonality provides better upper bound for Hardy's nonlocality
Creators: name: Das, Subhadipa
name: Banik, Manik
name: Gazi, Md. Rajjak
name: Rai, Ashutosh
name: Kunkri, Samir
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The amount of nonlocality in quantum theory is limited compared to that allowed in generalized no-signaling theory [Found. Phys. 24, 379 (1994)]. This feature, for example, gets manifested in the amount of Bell inequality violation as well as in the degree of success probability of Hardy's (Cabello's) nonlocality argument. Physical principles like information causality and macroscopic locality have been proposed for analyzing restricted nonlocality in quantum mechanics---viz. explaining the Cirel'son bound. However, these principles are not that much successful in explaining the maximum success probability of Hardy's as well as Cabello's argument in quantum theory. Here we show that, a newly proposed physical principle namely Local Orthogonality does better by providing a tighter upper bound on the success probability for Hardy's nonlocality. This bound is relatively closer to the corresponding quantum value compared to the bounds achieved from other principles.
description: 7 pages (2 columns); Accepted in Phys. Rev. A
Additional file 2 of Enhancing beliefs and implementation of evidence-based practice among undergraduate nurses using a multi-component educational programme: a pre–post study
Creators: name: Pereira, Filipa
name: Lehmann-Wellig, Brigitte
name: Verloo, Henk
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Molecular Biology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Supplementary Material 2
Another look at the dayside spectra of WASP-43b and HD 209458b: are there scattering clouds?
Creators: name: Taylor, Jake
name: Parmentier, Vivien
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The search for clouds on the dayside of hot Jupiters has been disadvantaged due to hot Jupiters having a limited number of high quality space-based observations. To date, retrieval studies have found no evidence for grey clouds on the dayside, however none of these studies explored the impact of scattering clouds. In this study we reanalyse the dayside emission spectrum of the hot Jupiter WASP-43b considering the different Spitzer data in the literature. We find that, in 2 of the 4 data sets explored, retrieving with a model that contains a scattering cloud is favoured over a cloud free model by a confidence of 3.13 - 3.36 $σ$. The other 2 data sets finds no evidence for scattering clouds. We find that the retrieved H$_2$O abundance is consistent regardless of the Spitzer data used and is consistent with literature values. We perform the same analysis for the hot Jupiter HD 209458b and find no evidence for dayside clouds, consistent with previous studies.
description: 7 pages, 6 figures. Accepted for publication with MNRAS
Magnetic fields & rotation periods of M dwarfs from SPIRou spectra
Creators: name: Donati, J. -F.
name: Lehmann, L. T.
name: Cristofari, P. I.
name: Fouqué, P.
name: Moutou, C.
name: Charpentier, P.
name: Ould-Elhkim, M.
name: Carmona, A.
name: Delfosse, X.
name: Artigau, E.
name: Alencar, S. H. P.
name: Cadieux, C.
name: Arnold, L.
name: Petit, P.
name: Morin, J.
name: Forveille, T.
name: Cloutier, R.
name: Doyon, R.
name: Hébrard, G.
name: collaboration, the SLS
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present near-infrared spectropolarimetric observations of a sample of 43 weakly- to moderately-active M dwarfs, carried with SPIRou at the Canada-France-Hawaii Telescope in the framework of the SPIRou Legacy Survey from early 2019 to mid 2022. We use the 6700 circularly polarised spectra collected for this sample to investigate the longitudinal magnetic field and its temporal variations for all sample stars, from which we diagnose, through quasi-periodic Gaussian process regression, the periodic modulation and longer-term fluctuations of the longitudinal field. We detect the large-scale field for 40 of our 43 sample stars, and infer a reliable or tentative rotation period for 38 of them, using a Bayesian framework to diagnose the confidence level at which each rotation period is detected. We find rotation periods ranging from 14 to over 60d for the early-M dwarfs, and from 70 to 200d for most mid- and late-M dwarfs (potentially up to 430d for one of them). We also find that the strength of the detected large-scale fields does not decrease with increasing period or Rossby number for the slowly rotating dwarfs of our sample as it does for higher-mass, more active stars, suggesting that these magnetic fields may be generated through a different dynamo regime than those of more rapidly rotating stars. We also show that the large-scale fields of most sample stars evolve on long timescales, with some of them globally switching sign as stars progress on their putative magnetic cycles.
description: MNRAS, in press (25 pages, 15 figures, 3 tables)
Constraining the SMEFT with a differential cross section measurement of $tWZ$ production at the HL-LHC
Creators: name: Keaveney, James
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A prospective measurement of the differential cross section of \tWZ production with respect to the transverse momentum of the \PZ boson using a general-purpose detector at the High-Luminosity Large Hadron Collider (HL-LHC) is described. The response of a general-purpose detector at the HL-LHC is simulated and used to estimate the uncertainties and covariances of the differential cross section measurement. Constraints on the Standard Model Effective Field Theory (SMEFT) enabled by the measurement are estimated. A parametric model of the differential cross section in the SMEFT is constructed and is used to determine the expected posterior probability function of six SMEFT Wilson coefficients and the expected 95\% Bayesian credible intervals for each coefficient and pair of coefficients. The intervals suggest that for all coefficients, the measurement will provide competitive but weaker constraints than those derived from other \mbox{HL-LHC} measurements involving top quarks and \PZ bosons. However, as the measurement is simultaneously sensitive to to a unique set of SMEFT coefficients, it will provide a useful input to a global SMEFT analysis that considers many operators.
description: 9 pages, 3 figures
Als Beweis der Dankbarkeit überreichen die Frankfurter Jungfrauen eine von ihnen verfertigte Germania einem hohen Paare um sie von denselben mit Füssen tretten zu lassen; [1849]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Vorlageform der Veröffentlichungsangabe: Verlag von R. Baist in Rödelheim
Discovery of the shell structure via break radii in the outer halo of the Milky Way
Creators: name: Ye, Dashuang
name: Du, Cuihua
name: Shi, Jianrong
name: Ma, Jun
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Based on the \textit{Gaia} DR3 RR Lyrae catalog, we use two methods to fit the density profiles with an improved broken power law, and find that there are two break radii coinciding with the two apocenter pile-ups of high-eccentricity Gaia-Sausage-Enceladus (GSE) merger. Also, there is a break caused by the Sagittarius (Sgr) stream. Combining the positions of all breaks, we briefly analyze the metallicity and its dispersion as a function of $r$ as well as its distribution in cylindrical coordinates. For the clean sample, the $z\text{-to-}x$ ellipsoid axial ratio $q$ in $36\,{\rm kpc}\,\textless\,r\,\textless\,96\,{\rm kpc}$ becomes much smaller than that of the inner halo $(r\,\textless\,36\,{\rm kpc})$, while the major axis has a large uncertainty in the region of $36-66\,{\rm kpc}$ and the one in the region of $66-96\,{\rm kpc}$ is obviously different from that dominated by the Hercules-Aquila Cloud (HAC) and the Virgo Overdensity (VOD) in the inner halo, which indicates that there is an over-density structure distributed at low zenithal angles. Finally, we found that the over-density structure in the outer halo ($r\,\textgreater\,50\,{\rm kpc}$) is shell-shaped and relatively metal-rich compared to the outer background halo. We conclude that the shells could be the apocenter pile-ups of the high-eccentricity GSE merger, which is supported by previous numerical simulations.
description: 16 pages, 14 Figures, accepted for publication in MNRAS
Additional file 1 of Low occupational physical activity is associated with incident type 2 diabetes in overweight and obese individuals: a population-based cohort study
Creators: name: Syrjälä, Maria Brännholm
name: Smidt, Melony Fortuin-de
name: Bergman, Frida
name: Nordendahl, Maria
name: Otten, Julia
name: Renklint, Rebecka
name: Rolandsson, Olov
name: Wahlström, Viktoria
name: Wennberg, Patrik
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Science Policy
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified

description: Supplementary Material 1.
Lepton flavor violation in the Higgs sector and the role of hadronic tau-lepton decays
Creators: name: Celis, Alejandro
name: Cirigliano, Vincenzo
name: Passemar, Emilie
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It has been pointed out recently that current low-energy constraints still allow for sizable flavor-changing decay rates of the 125 GeV boson into leptons, h -> tau ell (ell= e, mu). In this work we discuss the role of hadronic tau-lepton decays in probing lepton flavor violating couplings in the Higgs sector. At low energy, the effective Higgs coupling to gluons induced by heavy quarks contributes to hadronic tau decays, establishing a direct connection with the relevant process at the LHC, pp (gg)-> h -> tau ell. Semileptonic transitions like tau -> ell pi pi are sensitive to flavor-changing scalar couplings while decays such as tau -> ell eta(') probe pseudoscalar couplings, thus providing a useful low-energy handle to disentangle possible Higgs flavor violating signals at the LHC. As part of our analysis, we provide an appropriate description of all the relevant hadronic matrix elements needed to describe Higgs-mediated tau -> ell pi pi transitions, improving over previous treatments in the literature.
description: 33 pages, 9 figures, 6 tables
title: Wie die 3 Schneider Schleswig Holstein Deutschland vereinigen; [1849?]
title: Wie die drei Schneider Schleswig Holstein Deutschland vereinigen
titleType: Subtitle
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Vorlageform der Veröffentlichungsangabe: gedr. v. Ed. Gust. May in Frankfurt aM
Evolution of extortion in structured populations
Creators: name: Szolnoki, Attila
name: Perc, Matjaz
Publisher: name: arXiv
Year: 2014
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Computer Science and Game Theory (cs.GT)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences

description: Extortion strategies can dominate any opponent in an iterated prisoner's dilemma game. But if players are able to adopt the strategies performing better, extortion becomes widespread and evolutionary unstable. It may sometimes act as a catalyst for the evolution of cooperation, and it can also emerge in interactions between two populations, yet it is not the evolutionary stable outcome. Here we revisit these results in the realm of spatial games. We find that pairwise imitation and birth-death dynamics return known evolutionary outcomes. Myopic best response strategy updating, on the other hand, reveals new counterintuitive solutions. Defectors and extortioners coarsen spontaneously, which allows cooperators to prevail even at prohibitively high temptations to defect. Here extortion strategies play the role of a Trojan horse. They may emerge among defectors by chance, and once they do, cooperators become viable as well. These results are independent of the interaction topology, and they highlight the importance of coarsening, checkerboard ordering, and best response updating in evolutionary games.
description: 5 two-column pages, 4 figures; accepted for publication in Physical Review E
Competitive Stress, Social Confidence, and Coping Strategies of students during Socio-Cultural and Arts competitions
Creators: name: Bayangan, Esmerlyn
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 520599
subject: Social and personality psychology not elsewhere classified

description: The specific objectives of this study involve identifying anxiety and stress levels among student participants, assessing their confidence levels, and discerning the coping strategies employed to effectively manage these pressures. Utilizing a structured questionnaire within a descriptive research framework, the study gathered data based on students' experiences in sociocultural and art competitions.
title: Der Kaiserschnitt; [1848]
title: Doctor: Hier mein lieber guter Michel, bringe ich dir wieder ein Söhnchen. Michel: Ich muss Ihnen gesteh'n Herr Doctor, dass es mir diesmal weit lieber wäre, wenn mich meine Germania mit einem Mädel beschenkt hätte, die ich nicht anders als Republik hätte taufen lassen, denn böse Jungen hab' ich schon genug gehabt u. bin sie endlich müde. ...
titleType: Subtitle
Creators: name: Stern, S.
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: No. XXI
A chemical nano-reactor based on a levitated nanoparticle in vacuum
Creators: name: Ricci, Francesco
name: Cuairan, Marc T.
name: Schell, Andreas W.
name: Hebestreit, Erik
name: Rica, Raul A.
name: Meyer, Nadine
name: Quidant, Romain
Publisher: name: arXiv
Year: 2021
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Classical Physics (physics.class-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: A single levitated nanoparticle is used as a nano-reactor for studying surface chemistry at the nanoscale. Optical levitation under controlled pressure, surrounding gas composition, and humidity provides extreme control over the nanoparticle, including dynamics, charge, and surface chemistry. Using a single nanoparticle avoids ensemble averages and allows to study how the presence of silanol groups at its surface affects the adsorption and desorption of water from the background gas with unprecedented real time, spatial, and temporal resolution. Here, we demonstrate the unique potential of this versatile platform by studying the Zhuravlev model in silica particles. In contrast to standard methods, our system allowed the first observation of an abrupt and irreversible change in scattering cross section, mass, and mechanical eigenfrequency during the dehydroxylation process, indicating changes in density, refractive index and volume.
Economic Survey of Oil Palm Products’ Processing and Marketing in Kogi State, Nigeria
Creators: name: Onoja, Anthony Ojonimi
name: Ogali, T. U.
Publisher: name: Columbia University
Year: 2014
Subjects: Palm oil industry
Oil palm--Economic aspects
Palm oil industry--Marketing
Palm oil industry--Finance
Oil palm
Agriculture
Commerce

description: This study was designed to ascertain the level of profitability and inherent problems derivable from oil palm products’ processing and marketing in Kogi State of Nigeria. Primary data used for the study was obtained through the use of structured questionnaire and oral interviews. From the six agricultural Zones in Kogi State a total sample size of 60 was finally drawn to form the sampling frame from 3 Agricultural Zones. Descriptive statistics were used to attain objectives 1 and 3; while objective 2 was attained by the use of gross margin analysis. Majority of the farmers obtained their Fresh Fruit Bunches for processing from the village or open market (50%); oil palm processing and marketing is profitable business in the area with a gross margin of ₦603,320.00K and gross margin ratio of 2.72 from an average enterprise; problems identified in the enterprises included fluctuating prices, lack of basic infrastructure and inputs such as capital and processing machines. The study recommended the need for government to hasten the supply of rural infrastructure, reduce taxes and let processors/marketers be encouraged to form cooperatives so as to access credit.
Star Cluster Classification using Deep Transfer Learning with PHANGS-HST
Creators: name: Hannon, Stephen
name: Whitmore, Bradley C.
name: Lee, Janice C.
name: Thilker, David A.
name: Deger, Sinan
name: Huerta, E. A.
name: Wei, Wei
name: Mobasher, Bahram
name: Klessen, Ralf
name: Boquien, Mederic
name: Dale, Daniel A.
name: Chevance, Melanie
name: Grasha, Kathryn
name: Sanchez-Blazquez, Patricia
name: Williams, Thomas
name: Scheuermann, Fabian
name: Groves, Brent
name: Kim, Hwihyun
name: Kruijssen, J. M. Diederick
name: Team, the PHANGS-HST
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Currently available star cluster catalogues from HST imaging of nearby galaxies heavily rely on visual inspection and classification of candidate clusters. The time-consuming nature of this process has limited the production of reliable catalogues and thus also post-observation analysis. To address this problem, deep transfer learning has recently been used to create neural network models which accurately classify star cluster morphologies at production scale for nearby spiral galaxies (D < 20 Mpc). Here, we use HST UV-optical imaging of over 20,000 sources in 23 galaxies from the Physics at High Angular Resolution in Nearby GalaxieS (PHANGS) survey to train and evaluate two new sets of models: i) distance-dependent models, based on cluster candidates binned by galaxy distance (9-12 Mpc, 14-18 Mpc, 18-24 Mpc), and ii) distance-independent models, based on the combined sample of candidates from all galaxies. We find that the overall accuracy of both sets of models is comparable to previous automated star cluster classification studies (~60-80 per cent) and show improvement by a factor of two in classifying asymmetric and multi-peaked clusters from PHANGS-HST. Somewhat surprisingly, while we observe a weak negative correlation between model accuracy and galactic distance, we find that training separate models for the three distance bins does not significantly improve classification accuracy. We also evaluate model accuracy as a function of cluster properties such as brightness, colour, and SED-fit age. Based on the success of these experiments, our models will provide classifications for the full set of PHANGS-HST candidate clusters (N ~ 200,000) for public release.
description: 16 pages, 10 figures
Propagation-invariant vortex Airy beam whose singular point follows its main lobe
Creators: name: Suzuki, Masato
name: Yamane, Keisaku
name: Omatsu, Takashige
name: Morita, Ryuji
Publisher: name: arXiv
Year: 2021
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We propose and demonstrate a novel vortex Airy beam which is a superposition of an Airy beam and its laterally sheared beam with a $π/2$ phase shift. This new-type of vortex Airy beam exhibits stable propagation dynamics, wherein its singular point closely follows its main lobe, unlike conventional vortex Airy beams. Notably, the orbital angular mode purity of this new vortex Airy beam is up to 10% better than that of a conventional vortex Airy beam. We anticipate that this new type of vortex Airy beam, which combines the characteristics of an optical vortex and a diffraction-free Airy beam, will facilitate new directions in applications such as microscopy, material processing and nonlinear optics.
Galaxy Cluster Baryon Fractions Revisited
Creators: name: Gonzalez, Anthony H.
name: Sivanandam, Suresh
name: Zabludoff, Ann I.
name: Zaritsky, Dennis
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We measure the baryons contained in both the stellar and hot gas components for twelve galaxy clusters and groups at z~0.1 with M=1-5e14 Msun. This paper improves upon our previous work through the addition of XMM data, enabling measurements of the total mass and masses of each major baryonic component --- ICM, intracluster stars, and stars in galaxies --- for each system. We recover a relation for the stellar mass versus halo mass consistent with our previous result. We confirm that the partitioning of baryons between the stellar and hot gas components is a strong function of M500; the fractions of total mass in stars and X-ray gas within r500 scale as M500^-0.45 and M500^0.26, respectively. We also confirm that the combination of the BCG and intracluster stars is an increasingly important contributor to the stellar baryon budget in lower halo masses. We find a weak, but statistically significant, dependence of the total baryon fraction upon halo mass, scaling as M500^0.16. For M500>2e14, the total baryon fractions within r500 are on average 18% (7%) below the Universal value from the WMAP7 (Planck) analysis. For Planck, the difference between the Universal value and cluster baryon fractions is less than the systematic uncertainties associated with M500. The total baryon fractions exhibit significant scatter, particularly at M500<2e14 Msun where they range from 60-90% (65-100%) of the Universal value for WMAP7 (Planck). The ratio of the stellar-to-gas mass within r500, a measure of star formation efficiency, strongly decreases with M500. The fact that this relation remains tight at low mass implies that the larger scatter in the total baryon fractions at these masses arises from either true scatter in the total baryon content or observational scatter in M500, rather than late-time physical processes such as redistribution of gas to beyond r500. (abridged)
description: 20 pages, Accepted to The Astrophysical Journal
title: Deutschland. Dänemark.; [1848]
title: Die vom Abgeord. Bassermann beispielweise angeführte Demarcations-Linien zwischen Dänemark und Deutschland : (72te. Sitzung.)
titleType: Subtitle
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: No. XXVII
An incompressible 2D didactic model with singularity and explicit solutions of the 2D Boussinesq equations
Creators: name: Chae, Dongho
name: Constantin, Peter
name: Wu, Jiahong
Publisher: name: arXiv
Year: 2014
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35Q35, 35B65, 76D03

description: We give an example of a well posed, finite energy, 2D incompressible active scalar equation with the same scaling as the surface quasi-geostrophic equation and prove that it can produce finite time singularities. In spite of its simplicity, this seems to be the first such example. Further, we construct explicit solutions of the 2D Boussinesq equations whose gradients grow exponentially in time for all time. In addition, we introduce a variant of the 2D Boussinesq equations which is perhaps a more faithful companion of the 3D axisymmetric Euler equations than the usual 2D Boussinesq equations.
description: 9 pages; simplified a solution formula in section 4 and added a sentence on the time growth rate in the solution
Applications of neutron activation spectroscopy
Creators: name: Silarski, M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Medical Physics (physics.med-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Since the discovery in 1932, neutrons became a basis of many methods used not only in research, but also in industry and engineering. Among others, the exceptional role in the modern nuclear engineering is played by the neutron activation spectroscopy, based on the interaction of neutron flux with atomic nuclei. In this article we shortly describe application of this method in medicine and detection of hazardous substances.
description: Presented at Symposium on applied nuclear physics and innovative technologies, Cracow, 03-06 June 2013
U-spin analysis of CP violation in $B^- $ decays into three charged light pseudoscalar mesons
Creators: name: Xu, Dong
name: Li, Guan-Nan
name: He, Xiao-Gang
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We carry out a $U$-spin symmetry analysis for CP violation in $B^- $ decays into three light $π^-π^-π^+$, $π^- K^-K^+$, $K^-K^-K^+$ and $K^- π^-π^+$ mesons. We clarify some subtle points in constructing decay amplitudes with $U=0$ formed by the two negatively charged light mesons in the final states. $U$-spin conserving momentum independent and momentum dependent decay amplitudes, and $U$-spin violating decay amplitudes due to quark mass difference are constructed.
description: RevTex 12 pages wit no figure
Eigenstates of Thiophosgene Near the Dissociation Threshold -- Deviations From Ergodicity
Creators: name: Keshavamurthy, Srihari
Publisher: name: arXiv
Year: 2013
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: A subset of the highly excited eigenstates of thiophosgene (SCCl$_{2}$) near the dissociation threshold are analyzed using sensitive measures of quantum ergodicity. We find several localized eigenstates, suggesting that the intramolecular vibrational energy flow dynamics is nonstatistical even at such high levels of excitations. The results are consistent with recent observations of sharp spectral features in the stimulated emission spectra of SCCl$_{2}$
description: Accepted manuscript in The Journal of Physical Chemistry A, 10 pages,4 figures
Additional file 3 of Epigenetic timing effects on child developmental outcomes: a longitudinal meta-regression of findings from the Pregnancy And Childhood Epigenetics Consortium
Creators: name: Neumann, Alexander
name: Sammallahti, Sara
name: Cosin-Tomas, Marta
name: Reese, Sarah E.
name: Suderman, Matthew
name: Alemany, Silvia
name: Almqvist, Catarina
name: Andrusaityte, Sandra
name: Arshad, Syed H.
name: Bakermans-Kranenburg, Marian J.
name: Beilin, Lawrence
name: Breton, Carrie
name: Bustamante, Mariona
name: Czamara, Darina
name: Dabelea, Dana
name: Eng, Celeste
name: Eskenazi, Brenda
name: Fuemmeler, Bernard F.
name: Gilliland, Frank D.
name: Grazuleviciene, Regina
name: Håberg, Siri E.
name: Herberth, Gunda
name: Holland, Nina
name: Hough, Amy
name: Hu, Donglei
name: Huen, Karen
name: Hüls, Anke
name: Jarvelin, Marjo-Riitta
name: Jin, Jianping
name: Julvez, Jordi
name: Koletzko, Berthold V.
name: Koppelman, Gerard H.
name: Kull, Inger
name: Lu, Xueling
name: Maitre, Léa
name: Mason, Dan
name: Melén, Erik
name: Merid, Simon K.
name: Molloy, Peter L.
name: Mori, Trevor A.
name: Mulder, Rosa H.
name: Page, Christian M.
name: Richmond, Rebecca C.
name: Röder, Stefan
name: Ross, Jason P.
name: Schellhas, Laura
name: Sebert, Sylvain
name: Sheppard, Dean
name: Snieder, Harold
name: Starling, Anne P.
name: Stein, Dan J.
name: Tindula, Gwen
name: van IJzendoorn, Marinus H.
name: Vonk, Judith
name: Walton, Esther
name: Witonsky, Jonathan
name: Xu, Cheng-Jian
name: Yang, Ivana V.
name: Yousefi, Paul D.
name: Zar, Heather J.
name: Zenclussen, Ana C.
name: Zhang, Hongmei
name: Tiemeier, Henning
name: London, Stephanie J.
name: Felix, Janine F.
name: Cecil, Charlotte
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Biotechnology
subject: Developmental Biology
subject: Cancer
subject: Mental Health

description: Additional file 3. Cohort-specific information.
Early Disc Accretion as the Origin of Abundance Anomalies in Globular Clusters
Creators: name: Bastian, N.
name: Lamers, H. J. G. L. M.
name: de Mink, S. E.
name: Longmore, S. N.
name: Goodwin, S. P.
name: Gieles, M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Globular clusters (GCs), once thought to be well approximated as simple stellar populations (i.e. all stars having the same age and chemical abundance), are now known to host a variety of anomalies, such as multiple discrete (or spreads in) populations in colour-magnitude diagrams and abundance variations in light elements (e.g., Na, O, Al). Multiple models have been put forward to explain the observed anomalies, although all have serious shortcomings (e.g., requiring a non-standard initial mass function of stars and GCs to have been initially 10-100 times more massive than observed today). These models also do not agree with observations of massive stellar clusters forming today, which do not display significant age spreads nor have gas/dust within the cluster. Here we present a model for the formation of GCs, where low mass pre-main sequence (PMS) stars accrete enriched material released from interacting massive binary and rapidly rotating stars onto their circumstellar discs, and ultimately onto the young stars. As was shown in previous studies, the accreted material matches the unusual abundances and patterns observed in GCs. The proposed model does not require multiple generations of star-formation, conforms to known properties of massive clusters forming today, and solves the "mass budget problem" without requiring GCs to have been significantly more massive at birth. Potential caveats to the model as well as model predictions are discussed.
description: 15 pages, 4 figures, MNRAS in press
BGO quenching effect on spectral measurements of cosmic-ray nuclei in DAMPE experiment
Creators: name: Chen, Zhan-Fang
name: Yue, Chuan
name: Jiang, Wei
name: Cui, Ming-Yang
name: Yuan, Qiang
name: Wang, Ying
name: Zhao, Cong
name: Wei, Yi-Feng
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: The Dark Matter Particle Explorer (DAMPE) is a satellite-borne detector designed to measure high energy cosmic-rays and $γ$-rays. As a key sub-detector of DAMPE, the Bismuth Germanium Oxide (BGO) imaging calorimeter is utilized to measure the particle energy with a high resolution. The nonlinear fluorescence response of BGO for large ionization energy deposition, known as the quenching effect, results in an under-estimate of the energy measurement for cosmic-ray nuclei. In this paper, various models are employed to characterize the BGO quenching factors obtained from the experimental data of DAMPE. Applying the proper quenching model in the detector simulation process, we investigate the tuned energy responses for various nuclei and compare the results based on two different simulation softwares, i.e. GEANT4 and FLUKA. The BGO quenching effect results in a decrease of the measured energy by approximately $2.5\%$ ($5.7 \%$) for carbon (iron) at $\sim$10 GeV/n and $<1\%$ above 1 TeV/n, respectively. Accordingly, the correction of the BGO quenching effect leads to an increase of the low-energy flux measurement of cosmic-ray nuclei.
description: 13 pages, 4 figures, to be published in Nuclear Inst. and Methods in Physics Research, A
Delicious to Deadly Toxin: Uncovering a Global Culinary Crisis
Creators: name: Gomathy V1* and Ulaganathan Arisekar2
Publisher: name: trends in Agriculture Science
Year: 2023

description: India has vast species diversity and constitutes 10 % of the total fish species in the World. One of the most available species, pufferfish is poisonous to consume despite its nutritional advantage and delicacy worldwide. India is the third largest exporter of frozen pufferfish and China, Japan, and South Korea are the largest consumer for the same. However, these fishes are caught as by-catch due to a lack of domestic demand. Therefore, the development of organized supply and value chains in the domestic and export markets would help to utilize the available resources in India efficiently.
Two-point G$^2$ Hermite interpolation with spirals by inversion of conics: summary
Creators: name: Kurnosenko, Alexey
Publisher: name: arXiv
Year: 2014
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53A04

description: The article completes the research of two-point G$^2$ Hermite interpolation problem with spirals by inversion of conics. A simple algorithm is proposed to construct a family of 4th degree rational spirals, matching given G$^2$ Hermite data. A possibility to reduce the degree to cubic is discussed.
description: 18 pages, 8 figures
Detection of a strong ~2.5 Hz modulation in the Newly Discovered Millisecond Pulsar MAXI J1816-195
Creators: name: Li, P. P.
name: Tao, L.
name: Zhang, L.
name: Bu, Q. C.
name: Qu, J. L.
name: Ji, L.
name: Wang, P. J.
name: Chen, Y. P.
name: Zhang, S.
name: Ma, R. C.
name: Yang, Z. X.
name: Ye, W. T.
name: Zhao, S. J.
name: Zhao, Q. C.
name: Huang, Y.
name: Ma, X.
name: Qiao, E. L.
name: Jia, S. M.
name: Zhang, S. N.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: MAXI J181-195 is a newly discovered accreting millisecond X-ray pulsar that went outburst in June 2022. Through timing analysis with NICER and NuSTAR observations, we find a transient modulation at ~2.5 Hz during the decay period of MAXI J1816-195. The modulation is strongly correlated with a spectral hardening, and its fractional rms amplitude increases with energy. These results suggest that the modulation is likely to be produced in an unstable corona. In addition, the presence of the modulation during thermonuclear bursts indicates that it may originate from a disk-corona where the optical depth is likely the main factor affecting the modulation, rather than temperature. Moreover, we find significant reflection features in the spectra observed simultaneously by NICER and NuSTAR, including a relativistically broadened Fe-K line around 6-7 keV, and a Compton hump in the 10-30 keV energy band. The radius of the inner disc is constrained to be Rin = (1.04-1.23) RISCO based on reflection modeling of the broadband spectra. Assuming that the inner disc is truncated at the magnetosphere radius, we estimate that the magnetic field strength is < 4.67 * 10e8 G.
description: 12 pages, 13 figures
The Effects of Mega-Herbivore Extinctions on Seed Dispersal and Community Structure in An East African Savanna
Creators: name: Bernard, Miranda
name: Kielar, Abraham
name: Booth, Laura
Publisher: name: Columbia University
Year: 2014
Subjects: subject: Herbivores--Ecology
subject: Savanna ecology
subject: Savanna animals
subject: Soil seed banks
subject: Extinction (Biology)--Environmental aspects
subject: Seed dispersal by animals
subject: Sustainability
subject: Africans
subject: Ecology
subject: FOS: Biological sciences

description: Herbivory is a prominent top-down force shaping the landscape of semi-arid savannas in East Africa. Herbivores participate in seed dispersal both by ingesting and defecating the seeds of endozoochorously-dispersed plants and by translocating the seeds of exozoochorously-dispersed plants. In this study, we sought to determine how the extinction of large mammalian herbivores would affect the abundance of five focal species of plants that use fruiting as theira primary dispersal mechanism. We also examined how the absence of large mammalian herbivores affected seed predation by small mammals. We counted the number of individual plants for each of the five species in three short-term (5 yearr. old) exclusion blocks and one long-term (15 yearr. old) exclusion block. We found that total abundance of fleshy-fruited species increaseds as successive levels of large mammalian herbivores weare excluded and as the duration of herbivore exclusion increaseds. Within species, we found that C. orthacantha and S. campylacanthum increased in the absence of herbivores, while O. stricta decreased in the absence of herbivores. B. aegyptiaca and B. albitrunca did not exhibit differences in abundance between different levels of herbivore exclosure. We found that small mammals demonstrated a preference for B. albitrunca and O. stricta seeds, which were consumed primarily by the fringe-tailed gerbil, Gerbilliscus robustus. Understanding the interactions between herbivores and vegetation is vital to conserving understanding how plant communities as well as understanding how they may change in the future, as well as how to conserve them.
Μέθοδοι αναλυτικής των δεδομένων και στατιστικής μηχανικής μάθησης στην ασφάλιση υγείας
Creators: name: Μπουντούλης, Χρήστος
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2022
Subjects: subject: Ασφάλιση υγείας
subject: Αναλυτική των δεδομένων
subject: Μηχανική μάθηση
subject: Ασφαλιστικός κλάδος

description: Σε αυτή την εργασία, γίνεται μία εκτενής περιγραφή σε προβλήματα που εφάπτονται του τομέα της Ασφάλισης Υγείας με τα οποία οι εταιρείες βρίσκονται πολύ συχνά αντιμέτωπες και παρουσιάζονται εφαρμογές που οδηγούν στην ανάληψη στρατηγικών αποφάσεων με τη χρήση μεθόδων αναλυτικής των δεδομένων και στατιστικής μηχανικής μάθησης.
Environmental effects on associations of dwarf galaxies
Creators: name: Yaryura, C. Yamila
name: Abadi, Mario G.
name: Gottlöber, Stefan
name: Libeskind, Noam I.
name: Cora, Sofía A.
name: Ruiz, Andrés N.
name: Vega-Martínez, Cristian A.
name: Yepes, Gustavo
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the properties of associations of dwarf galaxies and their dependence on the environment. Associations of dwarf galaxies are extended systems composed exclusively of dwarf galaxies, considering as dwarf galaxies those galaxies less massive than $M_{\star, \rm max} = 10^{9.0}$ ${\rm M}_{\odot}\,h^{-1}$. We identify these particular systems using a semi-analytical model of galaxy formation coupled to a dark matter only simulation in the $Λ$ Cold Dark Matter cosmological model. To classify the environment, we estimate eigenvalues from the tidal field of the dark matter particle distribution of the simulation. We find that the majority, two thirds, of associations are located in filaments ($ \sim 67$ per cent), followed by walls ($ \sim 26 $ per cent), while only a small fraction of them are in knots ($ \sim 6 $ per cent) and voids ($ \sim 1 $ per cent). Associations located in more dense environments present significantly higher velocity dispersion than those located in less dense environments, evidencing that the environment plays a fundamental role in their dynamical properties. However, this connection between velocity dispersion and the environment depends exclusively on whether the systems are gravitational bound or unbound, given that it disappears when we consider associations of dwarf galaxies that are gravitationally bound. Although less than a dozen observationally detected associations of dwarf galaxies are currently known, our results are predictions on the eve of forthcoming large surveys of galaxies, which will enable these very particular systems to be identified and studied.
description: 13 pages, 9 figures. Accepted for publication in MNRAS
HST/WFC3 Near-Infrared spectroscopy of quenched galaxies at z~1.5 from the WISP Survey: Stellar population properties
Creators: name: Bedregal, A. G.
name: Scarlata, C.
name: Henry, A. L.
name: Atek, H.
name: Rafelski, M.
name: Teplitz, H. I.
name: Dominguez, A.
name: Siana, B.
name: Colbert, J. W.
name: Malkan, M.
name: Ross, N. R.
name: Martin, C. L.
name: Dressler, A.
name: Bridge, C.
name: Hathi, N. P.
name: Masters, D.
name: McCarthy, P. J.
name: Rutkowski, M. J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We combine Hubble Space Telescope (HST) G102 & G141 NIR grism spectroscopy with HST/WFC3-UVIS, HST/WFC3-IR and Spitzer/IRAC[3.6μm] photometry to assemble a sample of massive (log(M_star/M_sun) ~ 11) and quenched galaxies at z~1.5. Our sample of 41 galaxies is the largest with G102+G141 NIR spectroscopy for quenched sources at these redshifts. In contrast to the local Universe, z~1.5 quenched galaxies in the high-mass range have a wide range of stellar population properties. We find their SEDs are well fitted with exponentially decreasing SFHs, and short star-formation time-scales (τ<100Myr). Quenched galaxies also show a wide distribution in ages, between 1-4Gyr. In the (u-r)_0-versus-mass space quenched galaxies have a large spread in rest-frame color at a given mass. Most quenched galaxies populate the z~1.5 red-sequence (RS), but an important fraction of them (32%) have substantially bluer colors. Although with a large spread, we find that the quenched galaxies ON the RS have older median ages (3.1Gyr) than the quenched galaxies OFF the RS (1.5Gyr). We also show that a rejuvenated SED cannot reproduce the observed stacked spectra of (the bluer) quenched galaxies OFF the RS. We derive the upper limit on the fraction of massive galaxies ON the RS at z~1.5 to be <43%. We speculate that the young quenched galaxies OFF the RS are in a transition phase between vigorous star formation at z>2 and the z~1.5 RS. According to their estimated ages, the time required for quenched galaxies OFF the RS to join their counterparts ON the z~1.5 RS is of the order of ~1Gyr.
description: 15 pages, 11 figures and appendix. Accepted for publication in ApJ
Influence of rotation on axisymmetric plasma equilibria: double-null DTT scenario
Creators: name: Del Prete, Matteo
name: Montani, Giovanni
Publisher: name: arXiv
Year: 2021
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We study the dependence of some relevant tokamak equilibrium quantities on the toroidal plasma rotation. The Grad-Shafranov equation generalised to the rotating case is analytically solved employing two different representations for the homogenous solution. Using an expression in terms of polynomials, we describe the separatrix shape by a few geometrical parameters, reproducing different plasma scenarios such as double-null and inverse triangularity. In this setting, the introduction of toroidal rotation corresponds to variations on relevant plasma quantities, most notably an enhancement of the poloidal beta. Using a more general expression in terms of Bessel functions, we reconstruct the full plasma boundary of the double-null configuration proposed for the upcoming DTT experiment, demonstrating how said configuration is compatible with different values of the plasma velocity.
description: 7 pages, 6 figures. Submitted to PPCF
Stadler, Arnold: "Die Menschen lügen. Alle" und andere Psalmen
Creators: name: Adam-Cassini, Tina
Publisher: name: Werkstatt Schwule Theologie
Year: 1970

description: Werkstatt Schwule Theologie, Bd. 8 Nr. 1 (2001): Werkstatt Schwule Theologie, Band 8, Heft 1
Geißler, Maximilian; Przyklenk, Andrea: Ich mach mir nichts aus Mädchen
Creators: name: Maurer, Frank
Publisher: name: Werkstatt Schwule Theologie
Year: 1970

description: Werkstatt Schwule Theologie, Bd. 8 Nr. 1 (2001): Werkstatt Schwule Theologie, Band 8, Heft 1
Η επίπτωση των επιδημιών στο ανθρώπινο δυναμικό και την λειτουργία του πλοίου
Creators: name: Πετσίνη, Ελευθερία
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2022
Subjects: subject: Επιδημία
subject: Κορωνοϊός
subject: Επιπτώσεις
subject: Ναυτικός
subject: Αλλαγές πληρωμάτων
subject: Επαναπατρισμός
subject: Αποτελεσματική λειτουργική διαχείριση
subject: Ναυτιλιακές εταιρείες

description: Η παρούσα διπλωματική εργασία έχει ως στόχο να μελετήσει τις επιπτώσεις των επιδημιών στη ναυτιλία και πιο συγκεκριμένα τις επιπτώσεις στο ανθρώπινο δυναμικό και τη λειτουργία του πλοίου. Αφορμή για την εκπόνηση της εργασίας στάθηκε η υγειονομική κρίση που πλήττει όλο τον πλανήτη εδώ κα 2 χρόνια με σοβαρές συνέπειες σε όλους τους τομείς της ζωής. Παρά τις πρωτοφανείς προκλήσεις τα πλοία δεν σταμάτησαν να πλέουν και να διεκπεραιώνουν το έργο τους, τη μεταφορά δηλαδή αγαθών, πράγμα που υποδηλώνει τον σημαντικότατο ρόλο που διαδραματίζει η ναυτιλία για την οικονομική και κοινωνική ανάπτυξη των κρατών που πραγματοποιείται μέσω του διεθνούς εμπορίου. Σκοπός της διπλωματικής είναι να προσεγγίσει και να αναδείξει αφενός τον αντίκτυπο των επιδημιών στους εργαζομένους μιας ναυτιλιακής επιχείρησης αλλά κυρίως στους ναυτικούς που επανδρώνουν τα πλοία με αυταπάρνηση για πολλούς μήνες μη μπορώντας να επιστρέψουν στα σπίτια τους, δημιουργώντας προβλήματα ναυτολόγησης και επαναπατρισμού και αφετέρου τις προκλήσεις που καλείται να διαχειριστεί η επιχείρηση ώστε να βελτιστοποιηθεί η οικονομική και ασφαλή ανάπτυξη του πλοίου στο ευμετάβλητο περιβάλλον με τα πολύπλοκα δεδομένα.
Search of nearby resolved neutron stars among optical sources
Creators: name: Bihain, Gabriel
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Neutron stars are identified as pulsars, X-ray binary components, central objects of supernovae remnants, or isolated thermally emitting sources, and at distances beyond 120 pc. A population extrapolation suggests 10$^3$ objects within that boundary. Potentially, neutron stars could continuously emit gravitational waves at sensitivity reach of present instrumentation. As part of our Search for the Nearest Neutron Stars ``Five Seasons'' project, we search for nearby resolved neutron stars. Based on expected fluxes and magnitudes of thermally cooling neutron stars and pulsars, we selected sources in Gaia DR3. The sources have $G$-band absolute magnitudes $M_G>16$ mag, parallax signal-to-noise ratios greater than two, and colours $G_{BP}-G<0.78$ and $G-G_{RP}<0.91$ mag for power-law emitters of flux $F_ν \propto ν^{-α_ν}$ with spectral indices $α_ν<3$. The photometric region overlaps with that of white dwarfs, in confluence with most known pulsars in binaries having white dwarf companions. We looked for counterparts in gamma-ray, X-ray, ultraviolet, radio, optical, and infrared catalogues. We find about two X-ray-, 15 ultraviolet-, one radio probable counterparts, and at least four sources with power-law profiles at the ultraviolet-optical(-infrared). Because the sources have $G\gtrapprox20$ mag, we rely on Gaia DR3 single-source parameters. We identify possible binaries based on photoastrometric parameters, visual companions, and flux excesses. Some emission components suggest small thermal radii. Source types, neutron star content, and properties require further inquiry.
description: 76 pages, 47 figures, 15 tables. With supplementary material. Monthly Notices of the Royal Astronomical Society, in press