cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Importance truncation for the in-medium similarity renormalization group
Creators: name: Hoppe, J.
name: Tichai, A.
name: Heinz, M.
name: Hebeler, K.
name: Schwenk, A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Ab initio nuclear many-body frameworks require extensive computational resources, especially when targeting heavier nuclei. Importance-truncation (IT) techniques allow to significantly reduce the dimensionality of the problem by neglecting unimportant contributions to the solution of the many-body problem. In this work, we apply IT methods to the nonperturbative in-medium similarity renormalization group (IMSRG) approach and investigate the induced errors for ground-state energies in different mass regimes based on different nuclear Hamiltonians. We study various importance measures, which define the IT selection, and identify two measures that perform best, resulting in only small errors to the full IMSRG(2) calculations even for sizable compression ratios. The neglected contributions are accounted for in a perturbative way and serve as an estimate of the IT-induced error. Overall we find that the IT-IMSRG(2) performs well across all systems considered, while the largest compression ratios for a given error can be achieved when using soft Hamiltonians and for large single-particle bases.
description: 14 pages, 9 figures, published version
Orders of Vanishing and U(1) Charges in F-theory
Creators: name: Raghuram, Nikhil
name: Turner, Andrew P.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Many interesting questions about F-theory models, including several concerning the F-theory swampland, involve massless matter charged under U(1) gauge symmetries. It is therefore important to better understand the geometric properties of F-theory models realizing various U(1) charges. We propose that, for F-theory models described by elliptic fibrations in Weierstrass form, the U(1) charge of light matter is encoded in the orders of vanishing of the section components corresponding to the U(1) gauge symmetry. We give specific equations relating the U(1) charges to the orders of vanishing that seem to hold for both U(1)-charged singlets and for matter additionally charged under a simply-laced nonabelian gauge algebra. Our formulas correctly describe properties of F-theory models in the prior literature, and we give an argument that they should describe the orders of vanishing for arbitrarily high U(1) charges. They also resemble formulas for the $p$-adic valuations of elliptic divisibility sequences developed by Stange [arXiv:1108.3051]. These proposals could serve as a U(1) analogue of the Katz-Vafa method, allowing one to determine U(1) charges without resolution. Additionally, they predict geometric information about F-theory models with general U(1) charges, which may be useful for exploring the F-theory landscape and swampland.
description: 112 pages with appendices; v2: references added
Iniciando Con Arduino
Creators: name: Nuñez, Luis Fernando Salas
Publisher: name: figshare
Year: 2017
Subjects: subject: 90604 Microelectronics and Integrated Circuits
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: ¿Que es Arduino?Arduino es una plataforma de desarrollo de computación física de código abierto, basada en una placa con un sencillo microcontrolador Atmel AVR y un entorno de desarrollo para crear software (programas) para la placa (Tomado de la página oficial de ARDUINO http: // arduino .cc / es / Guía / Introducción ).
El lenguaje de programación de Arduino es una implementación de Cableado, una plataforma de computación física parecida, que se basa en la programación, un entorno de programación multimedia. Aunque también se puede programar en otros lenguajes de programación como Java, C, C ++, Matlab, Visual Basic, entre otros.
El software se puede conseguir en forma gratuita y fácil de usar, no tiene ninguna restricción.
A Twist In The Story
Creators: name: RODRIGUES, TENSING CARLOS
Publisher: name: figshare
Year: 2017
Subjects: subject: Ethnic Studies
subject: History
subject: Anthropology
subject: FOS: Sociology
subject: Archaeology
subject: Geography
subject: Sociology

description: Here we let our imagination fly to connect to the other Kuśasthaḷī (Kuṭṭhāḷæ or Cortalim), at the mouth of river Zuari in Goa. I propose that a group of kshatriya, fleeing from the rising sea, travelled by sea to Goa coast, and found a place that not only looked very much like the homeland they had left behind, but was promising – fertile land, lush vegetation and plenty of water; and a safe harbour. In keeping with the nostalgic practice we find common in history, they named the place Kuśasthaḷī. They occupied several villages around – Sāṁkhavāḷæ (Sancoale), naming it after Shankhodhar (also called Bet Dwarka) that they had left behind; Kēḷaśī (Quelossim); Loṭli (Loutulim); etc. This contradicts what we have come to believe up to now : that the brāhman fleeing from the drying Sarasvatī settled Kuśasthaḷī (along with the neighbouring villages) naming it after their homeland. But that would be inconsistent with history : Kuśasthaḷī in Kāṭhīyāvāḍa was never a brāhman settlement, being the capital of kshatriya king Revata; the folk history that Arcamone reports to his superiors in Rome, categorically states that fifteen villages in Salcete were yielded by the kshatriya to the incoming brāhman, meaning thereby that they were already occupied by the kshatriya before the brāhman reached there. [Who Are Chadd’ddi, 01 Jan 17] There is one hitch, however : the submergence of Kuśasthaḷī seems to have occurred around 7,500 BCE; but the upliftment of the Konkan coast could have happened much later; it is difficult to take a call either way. [Tying The Knots, 09 Apr 17]
Growth of Chromobacterium violaceum on R2A and Tryptic Soy Agar
Creators: name: Ng, Wenfa
Publisher: name: figshare
Year: 2017
Subjects: subject: Biotechnology
subject: Microbiology
subject: FOS: Biological sciences
subject: Biochemistry
subject: Cell Biology

description: Chromobacterium violaceum (ATCC 12472), a Gram-negative, rod-shaped bacterium capable of synthesizing hydrogen cyanide, was cultivated on R2A and Tryptic Soy Agar (TSA) at 30 oC for understanding the relative growth performance of the bacterium on different agars. Experiment results revealed that C. violaceum could grow well on both agars with the generation of small, round, purple colonies. Such morphology was similar to those obtained during growth of C. violaceum on LB Lennox agar. However, amount of purple violacein pigment secreted was significantly higher during growth on TSA agar compared to R2A agar. Swarming motility was not observed on both agars during growth of C. violaceum. Overall, relatively high cell density of C. violaceum could be supported by R2A and TSA agar, but TSA would be a more preferable growth medium for the bacterium if violacein production is a subject of study.
Angular systematics-free cosmological analysis of galaxy clustering in configuration space
Creators: name: Paviot, Romain
name: de la Torre, Sylvain
name: de Mattia, Arnaud
name: Zhao, Cheng
name: Bautista, Julian
name: Burtin, Etienne
name: Dawson, Kyle
name: Escoffier, Stéphanie
name: Jullo, Eric
name: Raichoor, Anand
name: Ross, Ashley J.
name: Rossi, Graziano
Publisher: name: arXiv
Year: 2021
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Galaxy redshift surveys are subject to incompleteness and inhomogeneous sampling due to the various constraints inherent to spectroscopic observations. This can introduce systematic errors on the summary statistics of interest, which need to be mitigated in cosmological analysis to achieve high accuracy. Standard practices involve applying weighting schemes based on completeness estimates across the survey footprint, possibly supplemented with additional weighting schemes accounting for density-dependent effects. In this work, we concentrate on pure angular systematics and describe an alternative approach consisting in analysing the galaxy two-point correlation function where angular modes are nulled. By construction, this procedure removes all possible known and unknown sources of angular observational systematics, but also part of the cosmological signal.We use a modified Landy-Szalay estimator for the two-point correlation function that relies on an additional random catalogue where angular positions are randomly drawn from the galaxy catalogue, and provide an analytical model to describe this modified statistic. We test the model by performing an analysis of the full anisotropic clustering in mock catalogues of luminous red and emission-line galaxies at 0.43 < z < 1.1. We find that the model fully accounts for the modified correlation function in redshift space, without introducing new nuisance parameters. The derived cosmological parameters from the analysis of baryon acoustic oscillations and redshift-space distortions display slightly larger statistical uncertainties, mostly for the growth rate of structure parameter fs8 that exhibits a 50% statistical error increase, but free from angular systematic error.
description: 16 pages, submitted to MNRAS
Effects of Incipient Pairing on Non-equilibrium Quasiparticle Transport in Fermi Liquids
Creators: name: Lin, Wei-Ting
name: Sauls, J. A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The low temperature properties of a wide range of many-fermion systems are well understood within the framework of Landau's theory of Fermi liquids. The low-energy physics of these systems is governed by interacting fermionic quasiparticles with momenta and energies near a Fermi surface in momentum space. Nonequilibrium properties are described by a kinetic equation for the distribution function for quasiparticles proposed by Landau. Quasiparticle interactions with other quasiparticles, phonons or impurities lead to internal forces acting on a distribution of nonequilibrium quasiparticles, as well as collision processes that ultimately limit the transport of mass, heat, charge and magnetization, as well as limit the coherence times of quasiparticles. For Fermi liquids that are close to a second order phase transition, e.g. Fermi liquids that undergo a superfluid transition, \emph{incipient} Cooper pairs - long-lived fluctuations of the ordered phase - provide a new channel for scattering quasiparticles, as well as corrections to internal forces acting on the distribution of nonequilibrium quasiparticles. We develop the theory of quasiparticle transport for Fermi liquids in the vicinity of a BCS-type superfluid transition starting from Keldysh's field theory for non-equilibrium, strongly interacting fermions. The leading corrections to Fermi liquid theory for non-equilibrium quasiparticle transport near a Cooper instability arise from the virtual emission and absorption of incipient Cooper pairs. Our theory is applicable to quasiparticle transport in superconductors, nuclear matter and the low temperature phases of liquid $^3$He. As an implementation of the theory we calculate the pairing fluctuation corrections to the attenuation of zero sound in liquid $^3$He near the superfluid transition and demonstrate quantitative agreement with experimental results.
description: 22 pages, 8 Figures
Manifestations of Spinodal Decomposition into Dilute Pd$_{1-x}$Fe$_{x}$ "Phases" in Iron-Implanted Palladium Films: FMR Study
Creators: name: Gumarov, A. I.
name: Yanilkin, I. V.
name: Rodionov, A. A.
name: Gabbasov, B. F.
name: Yusupov, R. V.
name: Aliyev, M. N.
name: Khaibullin, R. I.
name: Tagirov, L. R.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Palladium-iron alloys produced by high-dose implantation of iron ions into epitaxial palladium films were investigated with the ferromagnetic resonance (FMR) and vibrating sample magnetometry (VSM) techniques. The samples reveal distinct multiple FMR responses depending on the dose of iron ion implantation. The post-implantation annealing at 770 K does not bring the implanted films to a homogeneous solid solution state, as might be expected from the Pd-Fe phase diagram. On the contrary, the system approaches a stable state composed of several magnetic phases. FMR spectra exhibit an angular behavior specific for a stack of interacting magnetic layers. This observation, correlated with the magnetometry data, indicates that the palladium-iron binary alloy has a previously unknown tendency towards spinodal decomposition into isostructural phases with well-defined iron concentrations and, accordingly, with different temperatures of ferromagnetic ordering and saturation magnetizations.
description: 14 pages, 6 figures, 36 references
Using biochemical and isotopic tracers to characterise organic matter sources and their incorporation into estuarine food webs (Rufiji delta, Tanzania)
Creators: name: Dativa Shilla
name: Joyanto Routh
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: Biochemistry
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry

description: Fatty acid biomarkers and stable isotope signatures were used to identify the sources of particulate and sedimentary organic matter and its input into the food web through the dominant consumer within the mangrove-dominated Rufiji estuary, Tanzania. Specific fatty acids were used to identify the preferred basal sources of dominant fauna (i.e. filter feeder bivalves, snails, crabs, shrimps, and three fish species), and their presence in the water and sediment samples in the estuary. Both fatty acid and stable isotope results revealed that food web in the Rufiji estuary depended on a variety of carbon sources (mangroves, allochthonous terrestrial inputs, macroalgae, and phytoplankton), contributing to a different degree into the diets of primary consumers and members of near-shore fish, but none of them were obligatory for the survival of these species. The δ15N values of major primary producers and consumers/predators revealed a trend for δ15N enrichment with increasing trophic level. The ratio of docosahexaenoic acid to eicosapentaenoic acid (DHA:EPA) decreased from pelagic to benthic feeding fish. This indicated that fish with different feeding modes derived their fatty acids from different primary sources of nutrition, and suggested that the DHA:EPA ratio may be a useful indicator of feeding mode.
शिव र शिव का मुख्य शिक्षाहरू
Creators: name: Timalsina, Staneshwar
Publisher: name: Zenodo
Year: 2022
Subjects: Guhyakālī
Kubjika
amnaya
Kaula
timalsina
Divine Mother
consciousness
krama
Kula
Īśāna
shakta upāya
Saundaryalahari
Mālinīvijayottaratantra
Chandi
advaita vedanta
sthaneshwar timalsina
vimarsha-foundation
Sarvamnaya
Abhinavagupta
vedanta
Kali
Devi Mahatmya
trika
Spanda
Shiva Sutra
Tantra
mahadeva
saivadvaita
shakti
sarvamnaya-oral-tradition-archive
Vasugupta
Tripura Rahasya
sarvamnaya
anava upaya
agama
Sadāśiva
Camunda
Shiva
Bhairava
yantra
Mahakali
tripura
Tantric philosophy
Shaiva
tantraloka
Durga
shambhava
Kashmir Shaivism
Tripurasundari

description: शिव को हुन् र शिवका मुख्य शिक्षाहरू के हुन्?
A short introduction of Shiva and his teachings in Nepali by Dr. Sthaneshwar Timalsina, Professor at San Diego State University, California.

Original YouTube video: https://www.youtube.com/watch?v=gDCGTq2H4A0

This presentation is part of the Sarvāmnāya Oral Tradition Archive.
Vimarsha Foundation. (2025). The Sarvāmnāya Oral Tradition Archive [Data set]. Zenodo. https://doi.org/10.5281/zenodo.15188107
title: La consommation de substances psychoactives chez les élèves de 11 à 15 ans en Suisse
title: situation en 2018 et évolution depuis 2002
titleType: Subtitle
title: La consommation de substances psychoactives chez les élèves de 11 à 15 ans en Suisse
titleType: AlternativeTitle
Creators: name: Kretschmann, Andrea
Publisher: name: Addiction Info Suisse
Year: 2019

description: Feuille-info basée sur les données de l'étude HBSC 2018
Nodal gaps from local interactions in Sr$_2$RuO$_4$
Creators: name: Ramires, Aline
Publisher: name: arXiv
Year: 2021
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Sr$_2$RuO$_4$ has been under intensive scrutiny over the past years after new NMR measurements unveiled that the superconducting state might be a spin singlet. One of the best order parameter candidates in light of these new experiments is a chiral d-wave state with $d_{xz}+id_{yz}$ symmetry. This order parameter has been overlooked given the strong two-dimensional character of the normal state electronic structure. Recently, a phenomenological proposal based on local interactions with a three-dimensional electronic structure showed that a chiral d-wave state can be stable in Sr$_2$RuO$_4$ once momentum-dependent spin-orbit coupling is properly taken into account. Here we discuss the origin of the nodes and dips in this order parameter as inherited from the normal state Hamiltonian, showing that a nodal gap can emerge out of purely local interactions and connect the presence of nodes with the superconducting fitness measure.
description: 6 pages, 1 figure. To appear in Journal of Physics: Conference Series (IOP), associated with the SCES 2020/2021 conference
Iniciando Con Arduino - Luis Fernado Salas Nuñez.pdf
Creators: name: Nuñez, Luis Fernando Salas
Publisher: name: figshare
Year: 2017
Subjects: subject: 90604 Microelectronics and Integrated Circuits
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: ¿Que es Arduino?Arduino es una plataforma de desarrollo de computación física de código abierto, basada en una placa con un sencillo microcontrolador Atmel AVR y un entorno de desarrollo para crear software (programas) para la placa (Tomado de la página oficial de ARDUINO http: // arduino .cc / es / Guía / Introducción ).
El lenguaje de programación de Arduino es una implementación de Cableado, una plataforma de computación física parecida, que se basa en la programación, un entorno de programación multimedia. Aunque también se puede programar en otros lenguajes de programación como Java, C, C ++, Matlab, Visual Basic, entre otros.
El software se puede conseguir en forma gratuita y fácil de usar, no tiene ninguna restricción.
Rapid growth of seed black holes during early bulge formation
Creators: name: Inayoshi, Kohei
name: Nakatani, Riouhei
name: Toyouchi, Daisuke
name: Hosokawa, Takashi
name: Kuiper, Rolf
name: Onoue, Masafusa
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study the early growth of massive seed black holes (BHs) via accretion in protogalactic nuclei where the stellar bulge component is assembled, performing axisymmetric two-dimensional radiation hydrodynamical simulations. We find that when a seed BH with $M_\bullet \sim 10^5~M_\odot$ is embedded in dense metal-poor gas ($Z=0.01~Z_\odot$) with a density of $\gtrsim 100~{\rm cm}^{-3}$ and bulge stars with a total mass of $M_\star \gtrsim 100~M_\bullet$, a massive gaseous disk feeds the BH efficiently at rates of $\gtrsim 0.3-1~M_\odot~{\rm yr}^{-1}$ and the BH mass increases nearly tenfold within $\sim 2$ Myr. This rapid accretion phase lasts until a good fraction of the gas bounded within the bulge accretes onto the BH, although the feeding rate is regulated owing to strong outflows driven by ionizing radiation emitted from the accreting BH. The transient growing mode can be triggered for seed BHs formed in massive dark-matter halos with masses of $\gtrsim 10^9~M_\odot$ at $z\sim 15-20$ (the virial temperature is $T_{\rm vir}\simeq 10^5~{\rm K}$). The host halos are heavier and rarer than those of typical first galaxies, but are more likely to end up in quasar hosts by $z\simeq 6$. This mechanism naturally yields a mass ratio of $M_\bullet/M_\star >0.01$ higher than the value seen in the local universe and the existence of such overmassive BHs provides us a unique opportunity of detecting highly accreting seed BHs at $z\sim 15$ with AB magnitude of $m_{\rm AB} \sim26 - 29$ mag at $2~μ{\rm m}$ (rest-frame 10 eV) by the upcoming observations by the James Webb Space Telescope and Nancy Grace Roman Space Telescope.
description: 28 pages, 11 figures, accepted for publication to ApJ. Movies of the simulation are available at https://www.youtube.com/playlist?list=PLqDrKvxmu0l4fyJ74u5ZYyQ8PmwuNZA32
Bayesian vs Frequentist: Comparing Bayesian model selection with a frequentist approach using the iterative smoothing method
Creators: name: Koo, Hanwool
name: Keeley, Ryan E.
name: Shafieloo, Arman
name: L'Huillier, Benjamin
Publisher: name: arXiv
Year: 2021
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We have developed a frequentist approach for model selection which determines the consistency between any cosmological model and the data using the distribution of likelihoods from the iterative smoothing method. Using this approach, we have shown how confidently we can conclude whether the data support any given model without comparison to a different one. In this current work, we compare our approach with the conventional Bayesian approach based on the estimation of the Bayesian evidence using nested sampling. We use simulated future Roman (formerly WFIRST)-like type Ia supernovae data in our analysis. We discuss the limits of the Bayesian approach for model selection and show how our proposed frequentist approach can perform better in the falsification of individual models. Namely, if the true model is among the candidates being tested in the Bayesian approach, that approach can select the correct model. If all of the options are false, then the Bayesian approach will select merely the least incorrect one. Our approach is designed for such a case and we can conclude that all of the models are false.
description: 12 pages, 3 figures, 3 tables
The Bhaṁḍārī Militia
Creators: name: RODRIGUES, TENSING CARLOS
Publisher: name: figshare
Year: 2017
Subjects: subject: History
subject: Anthropology
subject: FOS: Sociology
subject: Archaeology
subject: Geography
subject: Sociology

description: It is difficult to define the bhaṁḍārī identity very clearly; they seem to have adopted different occupations at different times at different places; and seem to have been bracketed in narrow categories based on those occupations – different categories at different times at different places. What makes the discovery of their authentic identity even more difficult is the clouds created around it by political exigencies over the last half a century. For that reason any post-Independence information can only make our task difficult. We will have to take our search to 15th and 16th century. Perhaps some early Portuguese documents could be of help; those that record the gāṁvakārī system for instance. But we will need to go even beyond that point of time to answer the question : Who are bhaṁḍārī ? We need to fit the community in our basic ethnic triad of brāmhaṇa, kshatriya and vaḍukar – the three jana based on their geographical origin; and the multiplicity of jana that emerged from the encounters between these. It may be difficult; but definitely it is not impossible. The vast treasure of resources on the pre-history of the Deccan is yet unexplored; only the tip of it has been studied. The excavations by Sankalia, Ansari and Dhavalikar in Inamgaon is just the beginning. We have seen how our roots are more than obvious in these chalcolithic settlements. [Driven By The Drought, 05 Feb 17] Another promising line of investigation is the study of the deities and temples, and the traditions that envelop them. These hold within them a rich source of information about the people associated with them. The studies by Sontheimer and Shulman have inspired many historians now to follow that route. [Sontheimer, 1989 : Pastoral Deities In Western India; Shulman, 1980 : Tamil Temple Myths] We have already seen how useful this approach has been for us to unravel the kshatriya identity in the Deccan. [The Dhangar Dynasties Of Deccan, 13 Aug 17; The Yādavarāyā, 27 Aug 17; To The Ramparts Of Pratāpagaḍa, 03 Sep 17]
Supplementary material: Analog Backpropagation Learning Circuits for Memristive Crossbar Neural Networks
Creators: name: James, Alex Pappachen
name: Krestinskaya, Olga
name: Salama, Khaled Nabil
Publisher: name: figshare
Year: 2017
Subjects: subject: 100705 Nanoelectronics
subject: FOS: Nanotechnology
subject: 90604 Microelectronics and Integrated Circuits
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Supplementary material
Additional file 1 of Influence of benzene exposure, fat content, and their interactions on erythroid-related hematologic parameters in petrochemical workers: a cross-sectional study
Creators: name: Zhang, Xue
name: Deng, Qifei
name: He, Zhini
name: Li, Jie
name: Ma, Xiaoju
name: Zhang, Zhaorui
name: Wu, Dehua
name: Xing, Xiumei
name: Peng, Jing
name: Guo, Hongyu
name: Huang, Ming
name: Chen, Liping
name: Dang, Shanfeng
name: Zhu, Yanqun
name: Zhang, Zhengbao
name: Yang, Boyi
name: Wang, Hailan
name: Chen, Wen
name: Xiao, Yongmei
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Hematology
subject: Computational Biology
subject: Cardiology

description: Additional file 1: Table S1. Associations of urinary SPMA with erythroid-related hematologic parameters in different groups of gender, smoking status and drinking status. Table S2. Associations of BF% with erythroid-related hematologic parameters in different groups of smoking status and drinking status. Table S3. Associations of plasma TC levels with erythroid-related hematologic parameters in different groups of gender, smoking status and drinking status. Table S4. Associations of plasma TG levels with erythroid-related hematologic parameters in different groups of gender, smoking status and drinking status. Table S5. Associations of fatty liver occurrence with erythroid-related hematologic parameters in different groups of gender, smoking status and drinking status. Table S6. Associations of urinary SPMA with erythroid-related hematologic parameters in different fat content categories.
Primordial neutrino asymmetry evolution with full mean-field effects and collisions
Creators: name: Froustey, Julien
name: Pitrou, Cyril
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Neutrino oscillations and mean-field effects considerably enrich the phenomenology of neutrino evolution in the early Universe. Taking into account these effects, most notably the neutrino self-interaction mean-field contribution, we revisit the problem of the evolution of primordial neutrino asymmetries including for the first time the complete expression for collisions, which describe scattering and annihilations with electrons/positrons and reactions among (anti)neutrinos. We show that a generalisation of the adiabatic transfer of averaged oscillations (ATAO) scheme, a numerical method previously developed without neutrino degeneracy and based on the large separation of time scales in this problem, is sufficient to reach the same accuracy as the full quantum kinetic equation integration, but is notably faster. This approximation highlights the physics of synchronous oscillations at play in the evolution of neutrino chemical potentials, especially in the particular case with only two-neutrino mixing. In particular, it allows to understand what controls the beginning and the amplitude of oscillations, but also why there is a subsequent regime of collective oscillations with larger frequencies. We also find that it is very important to use the full collision term instead of relying on damping-like approximations, in order not to overestimate how collisions reduce these synchronous oscillations. Finally we study qualitatively how mixing parameters affect the final neutrino configuration, and in particular we show that the CP-violating Dirac phase cannot substantially affect the final $N_{\rm eff}$ nor the final electronic (anti)-neutrino spectrum, and thus should not affect cosmological observables.
description: 51 pages, 17 figures
The impact of natal kicks on galactic r-process enrichment by neutron star mergers
Creators: name: van de Voort, Freeke
name: Pakmor, Rüdiger
name: Bieri, Rebekka
name: Grand, Robert J. J.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We study galactic enrichment with rapid neutron capture (r-process) elements in cosmological, magnetohydrodynamical simulations of a Milky Way-mass galaxy. We include a variety of enrichment models, based on either neutron star mergers or a rare class of core-collapse supernova as sole r-process sources. For the first time in cosmological simulations, we implement neutron star natal kicks on-the-fly to study their impact. With kicks, neutron star mergers are more likely to occur outside the galaxy disc, but how far the binaries travel before merging also depends on the kick velocity distribution and shape of the delay time distribution for neutron star mergers. In our fiducial model, the median r-process abundance ratio is somewhat lower and the trend with metallicity is slightly steeper when kicks are included. In a model 'optimized' to better match observations, with a higher rate of early neutron star mergers, the median r-process abundances are fairly unaffected by kicks. In both models, the scatter in r-process abundances is much larger with natal kicks, especially at low metallicity, giving rise to more r-process enhanced stars. We experimented with a range of kick velocities and find that with lower velocities, the scatter is reduced, but still larger than without natal kicks. We discuss the possibility that the observed scatter in r-process abundances is predominantly caused by natal kicks removing the r-process sources far from their birth sites, making enrichment more inhomogeneous, rather than the usual interpretation that the scatter is set by the rarity of its production source.
description: Accepted for publication in MNRAS. Revised version: minor changes
(Re)Solving Reionization with Lyα: How Bright Lyα Emitters account for the $z\approx2-8$ Cosmic Ionizing Background
Creators: name: Matthee, Jorryt
name: Naidu, Rohan P.
name: Pezzulli, Gabriele
name: Gronke, Max
name: Sobral, David
name: Oesch, Pascal A.
name: Hayes, Matthew
name: Erb, Dawn
name: Schaerer, Daniel
name: Amorín, Ricardo
name: Tacchella, Sandro
name: Paulino-Afonso, Ana
name: Llerena, Mario
name: Calhau, João
name: Röttgering, Huub
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV luminosity functions. Here we introduce an emissivity framework based on Ly$α$ emitters (LAEs), which naturally hones in on the subset of galaxies responsible for the ionizing background due to the intimate connection between the production and escape of Ly$α$ and LyC photons. Using constraints on the escape fractions of bright LAEs ($L_{\rm{Lyα}}>0.2 L^{*}$) at $z\approx2$ obtained from resolved Ly$α$ profiles, and arguing for their redshift-invariance, we show that: (i) quasars and LAEs together reproduce the relatively flat emissivity at $z\approx2-6$, which is non-trivial given the strong evolution in both the star-formation density and quasar number density at these epochs and (ii) LAEs produce late and rapid reionization between $z\approx6-9$ under plausible assumptions. Within this framework, the $>10\times$ rise in the UV population-averaged $f_{\rm{esc}}$ between $z\approx3-7$ naturally arises due to the same phenomena that drive the growing Ly$α$ emitter fraction with redshift. Generally, a LAE dominated emissivity yields a peak in the distribution of the ionizing budget with UV luminosity as reported in latest simulations. Using our adopted parameters ($f_{\rm{esc}}=50\%$, $ξ_{\rm{ion}}=10^{25.9}$ Hz erg$^{-1}$ for half the bright LAEs), a highly ionizing minority of galaxies with $M_{\rm UV}
description: Accepted for publication in MNRAS. Figure 2 shows the main result -- the comoving emissivity due to bright LAEs. Our fiducial model is based on results presented in our companion paper -- Naidu & Matthee et al. 2022, arXiv: 2110.11961
The open citations revolution
Creators: name: Peroni, Silvio
Publisher: name: figshare
Year: 2017
Subjects: subject: Library and Information Studies
subject: FOS: Media and communications

description: Citations are the primary tool to acknowledge others' prior work on a particular topic. They enable one to find key publications within a particular field, and are used also for research purposes – e.g. people working in Bibliometrics, Informetrics, and Scientometrics use them for analysing the complex relationships that exist within huge networks of citations of scholarly works. In addition, citation data are important for the assessment of the quality of research by means of metrics and indicators calculated from citation databases. However, the cruel reality is that citations have been locked up in close silos for years, and often they can only be accessed by paying significant subscription fees.

But the scenario is quickly changing. In the past years, several initiatives (I4OC, OpenCitations, WikiCite, LORC, etc.) have started to promote the availability of open citation data. In this talk I will introduce some of the main significative efforts in the area, focussing on the way Semantic Publishing technologies have been used and adopted for enabling a FAIR publication of open citation data.
Concurrent Pigeon Paramyxovirus-1 and Acinetobacter Baumannii Infection in A Fatal Case of Pneumonia
Creators: name: Zou, Xiaohui
name: Suo, Lijun
name: Wang, Yiming
name: Cao, Hongyun
name: Mu, Shengrui
name: Wu, Chao
name: Yan, Lizhen
name: Qi, Xiaowei
name: Lu, Jianwei
name: Lu, Binghuai
name: Fan, Yanyan
name: Li, Hui
name: Huang, Lixue
name: Ren, Lili
name: Liu, Bo
name: Cao, Bin
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Pigeon paramyxovirus type 1 (PPMV-1) is an antigenic variant of avian paramyxovirus type 1 (APMV-1), which mainly infects pigeons. PPMV-1 genotype VI is the dominant genotype infecting pigeons in China. Human infection of avian paramyxovirus was rarely reported and usually developed mild symptoms such as conjunctivitis. We here detected PPMV-1 in the lower respiratory sample from a fatal case with severe pneumonia; this patient aged 64 years presented cough, fever, and hemoptysis for 8 days and was admitted to hospital on Dec 26, 2020. He developed acute respiratory distress syndrome and sepsis in the following days and died of multiple organ failure on Jan 7, 2021. Sputum and blood culture reported multidrug resistant Acinetobacter baumannii (ABA) for samples collected on day 22 and 19 post illness, respectively. However, clinical metagenomic sequencing further reported PPMV-1 besides ABA in the bronchoalveolar lavage fluid. The PPMV-1 genome showed 99.21% identity with a Chinese strain and belonged to VI genotype by BLAST analysis. Multiple basic amino acids were observed at the cleavage site of F protein (113RKKRF117), which indicated high virulence of this PPMV-1 strain to poultry. The patient had a close contact with pigeons before his illness and PPMV-1 nucleic acid was detected from the pigeon feather. PPMV antibody was also detected in the patient serum 20 days after illness. In conclusion, concurrent PPMV-1 genotype VI.2.1.1.2.2 and ABA infection was identified in a fatal pneumonia case and cross-species transmission of PPMV-1 may occurred between infected pigeons and human.
Study of the Impact of the Big Data Era on Accounting and Auditing
Creators: name: Sun, Yuxiang
name: Li, Jingyi
name: Lu, Mengdie
name: Guo, Zongying
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Finance (q-fin.GN)
subject: FOS: Economics and business

description: Big data revolutionizes accounting and auditing, offering deep insights but also introducing challenges like data privacy and security. With data from IoT, social media, and transactions, traditional practices are evolving. Professionals must adapt to these changes, utilizing AI and machine learning for efficient data analysis and anomaly detection. Key to overcoming these challenges are enhanced analytics tools, continuous learning, and industry collaboration. By addressing these areas, the accounting and auditing fields can harness big data's potential while ensuring accuracy, transparency, and integrity in financial reporting. Keywords: Big Data, Accounting, Audit, Data Privacy, AI, Machine Learning, Transparency.
description: 4 pages
The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
Creators: name: Scicluna, P.
name: Kemper, F.
name: McDonald, I.
name: Srinivasan, S.
name: Trejo, A.
name: Wallström, S. H. J.
name: Wouterloot, J. G. A.
name: Cami, J.
name: Greaves, J.
name: He, Jinhua
name: Hoai, D. T.
name: Kim, Hyosun
name: Jones, O. C.
name: Shinnaga, H.
name: Clark, C. J. R.
name: Dharmawardena, T.
name: Holland, W.
name: Imai, H.
name: van Loon, J. Th.
name: Menten, K. M.
name: Wesson, R.
name: Chawner, H.
name: Feng, S.
name: Goldman, S.
name: Liu, F. C.
name: MacIsaac, H.
name: Tang, J.
name: Zeegers, S.
name: Amada, K.
name: Antoniou, V.
name: Bemis, A.
name: Boyer, M. L.
name: Chapman, S.
name: Chen, X.
name: Cho, S. -H.
name: Cui, L.
name: Dell'Agli, F.
name: Friberg, P.
name: Fukaya, S.
name: Gomez, H.
name: Gong, Y.
name: Hadjara, M.
name: Haswell, C.
name: Hirano, N.
name: Hony, S.
name: Izumiura, H.
name: Jeste, M.
name: Jiang, X.
name: Kaminski, T.
name: Keaveney, N.
name: Kim, J.
name: Kraemer, K. E.
name: Kuan, Y. -J.
name: Lagadec, E.
name: Lee, C. F.
name: Li, D.
name: Liu, S. -Y.
name: Liu, T.
name: de Looze, I.
name: Lykou, F.
name: Maraston, C.
name: Marshall, J. P.
name: Matsuura, M.
name: Min, C.
name: Otsuka, M.
name: Oyadomari, M.
name: Parsons, H.
name: Patel, N. A.
name: Peeters, E.
name: Pham, T. A.
name: Qiu, J.
name: Randall, S.
name: Rau, G.
name: Redman, M. P.
name: Richards, A. M. S.
name: Serjeant, S.
name: Shi, C.
name: Sloan, G. C.
name: Smith, M. W. L.
name: Suh, K. -W.
name: Toalá, J. A.
name: Uttenthaler, S.
name: Ventura, P.
name: Wang, B.
name: Yamamura, I.
name: Yang, T.
name: Yun, Y.
name: Zhang, F.
name: Zhang, Y.
name: Zhao, G.
name: Zhu, M.
name: Zijlstra, A. A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of $\sim$850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO $J = $ (2$-$1) and (3$-$2) rotational lines, and the sub-mm continuum, using the James Clark Maxwell Telescope and Atacama Pathfinder Experiment. NESS consists of five tiers, based on distances and dust-production rate (DPR). We define a new metric for estimating the distances to evolved stars and compare its results to \emph{Gaia} EDR3. Replicating other studies, the most-evolved, highly enshrouded objects in the Galactic Plane dominate the dust returned by our sources, and we initially estimate a total DPR of $4.7\times 10^{-5}$ M$_\odot$ yr$^{-1}$ from our sample. Our sub-mm fluxes are systematically higher and spectral indices are typically shallower than dust models typically predict. The 450/850 $μ$m spectral indices are consistent with the blackbody Rayleigh--Jeans regime, suggesting a large fraction of evolved stars have unexpectedly large envelopes of cold dust.
description: 20 pages, 13 figures, 5 tables, accepted for publications in MNRAS
water-hexane-xfer.gif
Creators: name: Karnes, John
name: Benjamin, Ilan
Publisher: name: figshare
Year: 2017
Subjects: subject: 30799 Theoretical and Computational Chemistry not elsewhere classified
subject: FOS: Chemical sciences
subject: 30699 Physical Chemistry not elsewhere classified
subject: Computational Chemistry

description: Transfer of a water molecule from bulk aqueous phase to an adjacent liquid hexane phase. The transferring water is represented by its Van der Waals surface for clarity.
Classification of the core-collapse supernova explosion mechanism with learned dictionaries
Creators: name: Saiz-Pérez, Ainara
name: Torres-Forné, Alejandro
name: Font, José A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Core-collapse supernovae (CCSN) are a prime source of gravitational waves. Estimations of their typical frequencies make them perfect targets for the current network of advanced, ground-based detectors. A successful detection could potentially reveal the underlying explosion mechanism through the analysis of the waveform. This has been illustrated using the SupernovaModel Evidence Extractor (SMEE; Logue et al. (2012)), an algorithm based on principal-component analysis and Bayesian model selection. Here, we present a complementary approach to SMEE based on (supervised) dictionary-learning and show that it is able to reconstruct and classify CCSN signals according to their morphology. Our waveform signals are obtained from (a) two publicly available catalogs built from numerical simulations of neutrino-driven (Mur) and magneto-rotational (Dim) CCSN explosions and (b) from a third 'mock' catalog of simulated sine-Gaussian (SG) waveforms. Those signals are injected into coloured Gaussian noise to simulate the background noise of Advanced LIGO in its broadband configuration and scaled to a freely-specifiable signal-to-noise ratio (SNR). We show that our approach correctly classifies signals from all three dictionaries. In particular, for SNR=15-20, we obtain perfect matches for both Dim and SG signals and about 85% true classifications for Mur signals. These results are comparable to those reported by SMEE for the same CCSN signals when those are injected in only one LIGO detector. We discuss the main limitations of our approach as well as possible improvements.
title: Lettre de Jacques Leibowitch à Jean-Pierre Chaumard
Creators: name: Leibowitch, Jacques
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Source: http://www.calames.abes.fr/pub/ms/Calames-20193111134069922
Quantum Gutzwiller approach for the two-component Bose-Hubbard model
Creators: name: Colussi, V. E.
name: Caleffi, F.
name: Menotti, C.
name: Recati, A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We study the effects of quantum fluctuations in the two-component Bose-Hubbard model generalizing to mixtures the quantum Gutzwiller approach introduced recently in [Phys. Rev. Research 2, 033276 (2020)]. As a basis for our study, we analyze the mean-field ground-state phase diagram and spectrum of elementary excitations, with particular emphasis on the quantum phase transitions of the model. Within the quantum critical regimes, we address both the superfluid transport properties and the linear response dynamics to density and spin probes of direct experimental relevance. Crucially, we find that quantum fluctuations have a dramatic effect on the drag between the superfluid species of the system, particularly in the vicinity of the paired and antipaired phases absent in the usual one-component Bose-Hubbard model. Additionally, we analyse the contributions of quantum corrections to the one-body coherence and density/spin fluctuations from the perspective of the collective modes of the system, providing results for the few-body correlations in all the regimes of the phase diagram.
description: 50 pages, 17 figures
Additional file 1 of Capnodynamic monitoring of lung volume and blood flow in response to increased positive end-expiratory pressure in moderate to severe COVID-19 pneumonia: an observational study
Creators: name: Schulz, Luis
name: Stewart, Antony
name: O’Regan, William
name: McCanny, Peter
name: Austin, Danielle
name: Hallback, Magnus
name: Wallin, Mats
name: Aneman, Anders
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology

description: Additional file 1 STROBE checklist and ECMO cases.
Dimensional reduction of higher derivative heterotic supergravity
Creators: name: Chang, Hao-Yuan
name: Sezgin, Ergin
name: Tanii, Yoshiaki
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Higher derivative couplings of hypermultiplets to $6D, N=(1,0)$ supergravity are obtained from dimensional reduction of 10D heterotic supergravity that includes order $α'$ higher derivative corrections. Reduction on $T^4$ is followed by a consistent truncation. In the resulting action the hyperscalar fields parametrize the coset $SO(4,4)/(SO(4)\times SO(4))$. While the $SO(4,4)$ symmetry is ensured by Sen's construction based on string field theory, its emergence at the field theory level is a nontrivial phenomenon. A number of field redefinitions in the hypermultiplet sector are required to remove several terms that break the $SO(4)\times SO(4)$ down to its $SO(4)$ diagonal subgroup in the action and the supersymmetry transformation rules. Working with the Lorentz Chern-Simons term modified 3-form field strength, where the spin connection has the 3-form field strength as torsion, is shown to simplify considerably the dimensional reduction.
description: 40 pages. References added, appendices improved and typos corrected