cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
NACRE II: an update of the NACRE compilation of charged-particle-induced thermonuclear reaction rates for nuclei with mass number $A < 16$
Creators: name: Xu, Yi
name: Takahashi, Kohji
name: Goriely, Stephane
name: Arnould, Marcel
name: Ohta, Masahisa
name: Utsunomiya, Hiroaki
Publisher: name: arXiv
Year: 2013
Subjects: subject: Nuclear Theory (nucl-th)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: An update of the NACRE compilation [Angulo et al., Nucl. Phys. A 656 (1999) 3] is presented. This new compilation, referred to as NACRE II, reports thermonuclear reaction rates for 34 charged-particle induced, two-body exoergic reactions on nuclides with mass number $A<16$, of which fifteen are particle-transfer reactions and the rest radiative capture reactions. When compared with NACRE, NACRE II features in particular (1) the addition to the experimental data collected in NACRE of those reported later, preferentially in the major journals of the field by early 2013, and (2) the adoption of potential models as the primary tool for extrapolation to very low energies of astrophysical $S$-factors, with a systematic evaluation of uncertainties. As in NACRE, the rates are presented in tabular form for temperatures in the $10^{6}$ $\simeq\leq$ T $\leq$ $10^{10}$ K range. Along with the 'adopted' rates, their low and high limits are provided. The new rates are available in electronic form as part of the Brussels Library (BRUSLIB) of nuclear data. The NACRE II rates also supersede the previous NACRE rates in the Nuclear Network Generator (NETGEN) for astrophysics. [http://www.astro.ulb.ac.be/databases.html.]
description: 86 figures
Microtus thomasi
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Microtus
Microtus thomasi

description: Microtus thomasi (Barrett-Hamilton, 1903). Ann. Mag. Nat. Hist., ser. 7, 11:306. TYPE LOCALITY: Yugoslavia, Montenegro, Vranici. DISTRIBUTION: From S coastal Yugoslavia into Greece (including Evvoia Isl); see map in Niethammer (1982k). SYNONYMS: atticus. COMMENTS: Subgenus Terricola, duodecimcostatus species group sensu Chaline et al. (1988) or a member of its own species group sensu Zagorodnyuk (1990). Reviewed by Corbet (1978c) and Niethammer (1982k); chromosomal information summarized by Zima and Krâl (1984a).
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 530, DOI: 10.5281/zenodo.7353098
description: {"references": ["Niethammer, J. 1982 k. Microtus thomasi Barrett-Hamilton, 1903 -- Balkan-Kurzohrmaus. Pp. 485 - 490, in Handbuch der Saugetiere Europas (J. Niethammer and F. Krapp, eds.). Akademische Verlagsgesellschaft (Wiesbaden), 2 / I: 1 - 649.", "Zagorodnyuk, I. V. 1990. Kariotipicheskaya izmenchivost' i sistematika serykh polevok (Rodentia, Arvicolini). Soobshchenie 1. Vidovoi sostav i khromosomnye chisla [Karyotypic variability and systematics of the gray voles (Rodentia, Arvicolini). Communication 1. Species composition and chromosomal numbers]. Vestnik Zoologii, 2: 26 - 37 (in Russian).", "Corbet, G. B. 1978 c. The mammals of the Palaearctic region: A taxonomic review. British Museum (Natural History), London, 314 pp.", "Zima, J., and B. Kral. 1984 a. Karyotypes of European mammals. II. Acta Scientiarum Naturalium, Academiae Scientarium Bohemoslovacae (Brno), 18 (8): 1 - 62."]}
Tuning of quantum interference in top-gated graphene on SiC
Creators: name: Iagallo, Andrea
name: Tanabe, Shinichi
name: Roddaro, Stefano
name: Takamura, Makoto
name: Hibino, Hiroki
name: Heun, Stefan
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We report on quantum-interference measurements in top-gated Hall bars of monolayer graphene epitaxially grown on the Si face of SiC, in which the transition from negative to positive magnetoresistance was achieved varying temperature and charge density. We perform a systematic study of the quantum corrections to the magnetoresistance due to quantum interference of quasiparticles and electron-electron interaction. We analyze the contribution of the different scattering mechanisms affecting the magnetotransport in the $-2.0 \times 10^{10}$ cm$^{-2}$ to $3.75 \times 10^{11}$ cm$^{-2}$ density region and find a significant influence of the charge density on the intravalley scattering time. Furthermore, we observe a modulation of the electron-electron interaction with charge density not accounted for by present theory. Our results clarify the role of quantum transport in SiC-based devices, which will be relevant in the development of a graphene-based technology for coherent electronics.
Dark matter - electron interactions in materials beyond the dark photon model
Creators: name: Catena, Riccardo
name: Cole, Daniel
name: Emken, Timon
name: Matas, Marek
name: Spaldin, Nicola
name: Tarantino, Walter
name: Urdshals, Einar
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The search for sub-GeV dark matter (DM) particles via electronic transitions in underground detectors attracted much theoretical and experimental interest in the past few years. A still open question in this field is whether experimental results can in general be interpreted in a framework where the response of detector materials to an external DM probe is described by a single ionisation or crystal form factor, as expected for the so-called dark photon model. Here, ionisation and crystal form factors are examples of material response functions: interaction-specific integrals of the initial and final state electron wave functions. In this work, we address this question through a systematic classification of the material response functions induced by a wide range of models for spin-0, spin-1/2 and spin-1 DM. We find several examples for which an accurate description of the electronic transition rate at DM direct detection experiments requires material response functions that go beyond those expected for the dark photon model. This concretely illustrates the limitations of a framework that is entirely based on the standard ionisation and crystal form factors, and points towards the need for the general response-function-based formalism we pushed forward recently [1,2]. For the models that require non-standard atomic and crystal response functions, we use the response functions of [1,2] to calculate the DM-induced electronic transition rate in atomic and crystal detectors, and to present 90% confidence level exclusion limits on the strength of the DM-electron interaction from the null results reported by XENON10, XENON1T, EDELWEISS and SENSEI.
description: 35 pages, 6 figures
Self-Organized Cooperative Criticality in Coupled Complex Systems
Creators: name: Liu, Lei
name: Hu, Fei
Publisher: name: arXiv
Year: 2013
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We show that the coupled complex systems can evolve into a new kind of self-organized critical state where each subsystem is not critical, however, they cooperate to be critical. This criticality is different from the classical BTW criticality where the single system itself evolves into a critical state. We also find that the outflows can be accumulated in the coupled systems. This will lead to the emergency of spatiotemporal intermittency in the critical state.
Mixed Gauginos Sending Mixed Messages to the LHC
Creators: name: Kribs, Graham D.
name: Raj, Nirmal
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Supersymmetric models with a Dirac gluino have been shown to be considerably less constrained from LHC searches than models with a Majorana gluino. In this paper, we generalize this discussion to models with a "Mixed Gluino", that acquires both Dirac and Majorana masses, as well as models in which electroweak gauginos contribute to squark production. Our primary interest is the degree of suppression of the cross section for first generation squarks compared with a gluino with a pure Majorana mass. We find that not all Majorana masses are alike -- a Majorana mass for the gluino can suppress the squark production cross section, whereas a Majorana mass for the adjoint fermion partner leads to an increased cross section, compared with a pure Dirac gluino. In the presence of electroweak gauginos, squark production can increase by at most a factor of a few above the pure Dirac gluino case when the electroweak gauginos have purely Majorana masses near to the squark masses. This unusual set of gaugino masses is interesting since the usual Higgs quartic coupling would not be suppressed. When the electroweak gaugino masses are much lighter than the squarks, there is a negligible change to the squark production cross section. We explain both of these cases in detail by considering the various subprocesses for squark production at the LHC. Continued searches for squark production with cross sections much smaller than expected in the MSSM are absolutely warranted, and we suggest new simplified models to fully characterize the collider constraints.
description: 20 pages
An Evolution and Eruption of the Coronal Magnetic Field through a Data-Driven MHD Simulation
Creators: name: Inoue, Satoshi
name: Hayashi, Keiji
name: Miyoshi, Takahiro
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a newly developed data-driven magnetohydrodynamics (MHD) simulation code under a zero-beta approximation based on a method proposed by Hayashi et al. 2018 and 2019. Although many data-driven MHD simulations have been developed and conducted, there are not many studies on how accurately those simulations can reproduce the phenomena observed in the solar corona. In this study, we investigated the performance of our data-driven simulation quantitatively using ground-truth data. The ground-truth data was produced by an MHD simulation in which the magnetic field is twisted by the sunspot motions. A magnetic flux rope (MFR) is created by the cancellation of the magnetic flux at the polarity inversion line due to the converging flow on the sunspot, which eventually leads the eruption of the MFR. We attempted to reproduce these dynamics using the data-driven MHD simulation. The coronal magnetic fields are driven by the electric fields, which are obtained from a time-series of the photospheric magnetic field that is extracted from the ground-truth data, on the surface. As a result, the data-driven simulation could capture the subsequent MHD processes, the twisted coronal magnetic field and formation of the MFR, and also its eruption. We report these results and compare with the ground-truth data, and discuss how to improve the accuracy and optimize numerical method.
description: Accepted for publication in ApJ
Comparative risk of infection of medications used for type 2 diabetes
Creators: name: Zapata-Bravo, Estefania
name: Douros, Antonios
name: Yu, Oriana Hoi Yun
name: Filion, Kristian B.
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Glucose-lowering drugs pose a potential infection risk among individuals with type 2 diabetes. The U.S. Food and Drug Administration has issued safety warnings regarding increased risks of urinary tract infections (UTIs) and genital infections with sodium-glucose cotransporter 2 (SGLT2) inhibitors. However, the infection risk associated with other glucose-lowering drugs remains unclear. We conducted a PubMed database search to review the infection risk of glucose-lowering drugs, focusing on meta-analysis of randomized controlled trials. We described the infection risks associated with SGLT2 inhibitors, dipeptidyl peptidase-4 (DPP-4) inhibitors, glucose-like peptide-1 receptor agonists, metformin, and thiazolidinediones, covering infections of the genitourinary, respiratory, and gastrointestinal systems, including skin and soft tissue infections (SSTIs). SGLT2 inhibitors are associated with a higher genital infection risk, while their UTI risk remains inconclusive. DPP-4 inhibitors could be a treatment option for those intolerant to SGLT2 inhibitors, given their lower genital infection risk compared to placebo. Uncertainty persists regarding the risks of respiratory infections, gastroenteritis, and SSTIs with SGLT2 inhibitors. Limited evidence is available regarding the impact of DPP-4 inhibitors on respiratory infections. Additional research is needed to determine the comparative infection risk of other glucose-lowering drugs.
Companilactobacillus heilongjiangensis HEILONGJIANGENSIS 2020, COMB. NOV.
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Companilactobacillus
Companilactobacillus heilongjiangensis

description: DESCRIPTIONOF COMPANILACTOBACILLUS HEILONGJIANGENSIS COMB. NOV.
Companilactobacillus heilongjiangensis (hei.long.ji.ang.en’sis. N.L. masc. adj. heilongjiangensis pertainingto Heilongjiang, a river flowing through the province of China where the bacterium was isolated).
Basonym: Lactobacillus heilongjiangensis Gu et al. 2013, 4098 VP
Hexoses and disaccharides but not pentoses are fermented [130]. The genome size is 2.79 Mbp. The mol% G+C content of DNAis 37.5.
Isolated from fermented vegetables and type I sourdough.
Thetypestrainis S4-3 T =LMG 26166 T =DSM 28069 T =NCIMB 14701 T.
Genome sequence accession number: CP012559.
16S RNA gene sequence accession number: JF411966.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2805, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Perturbation theory with dispersion and higher cumulants: framework and linear theory
Creators: name: Garny, Mathias
name: Laxhuber, Dominik
name: Scoccimarro, Roman
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The standard perturbation theory (SPT) approach to gravitational clustering is based on a fluid approximation of the underlying Vlasov-Poisson dynamics, taking only the zeroth and first cumulant of the phase-space distribution function into account (density and velocity fields). This assumption breaks down when dark matter particle orbits cross and leads to well-known problems, e.g. an anomalously large backreaction of small-scale modes onto larger scales that compromises predictivity. We extend SPT by incorporating second and higher cumulants generated by orbit crossing. For collisionless matter, their equations of motion are completely fixed by the Vlasov-Poisson system, and thus we refer to this approach as Vlasov Perturbation Theory (VPT). Even cumulants develop a background value, and they enter the hierarchy of coupled equations for the fluctuations. The background values are in turn sourced by power spectra of the fluctuations. The latter can be brought into a form that is formally analogous to SPT, but with an extended set of variables and linear as well as non-linear terms, that we derive explicitly. In this paper, we focus on linear solutions, which are far richer than in SPT, showing that modes that cross the dispersion scale set by the second cumulant are highly suppressed. We derive stability conditions on the background values of even cumulants from the requirement that exponential instabilities be absent. We also compute the expected magnitude of averaged higher cumulants for various halo models and show that they satisfy the stability conditions. Finally, we derive self-consistent solutions of perturbations and background values for a scaling universe and study the convergence of the cumulant expansion. The VPT framework provides a conceptually straightforward and deterministic extension of SPT that accounts for the decoupling of small-scale modes.
description: 31 pages + appendices, 10 figures
Production of J/psi+eta(c) vs. J/psi+J/psi at the LHC: Impact of Real alpha_s^5 corrections
Creators: name: Lansberg, Jean-Philippe
name: Shao, Hua-Sheng
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 proceed for the first time to the evaluation of the Born cross section for J/psi+eta(c) production, namely via g+g -> J/psi+eta(c)+g, and show that it has a harder P_T spectrum than the J/psi-pair yield at Born level. If one stuck to a comparison at Born level, one would conclude that J/psi+eta(c) production would surpass that of J/psi+J/psi at large P_T. This is nonetheless not the case since J/psi-pair production, as for single J/psi, receives leading-P_T contributions at higher orders in alpha_s. We also present the first evaluation of these leading-P_T next-to-leading order contributions. These are indeed significant for increasing P_T and are of essential relevance for comparison with forthcoming data. We also compute kinematic correlations relevant for double-parton-scattering studies. Finally, we evaluate the polarisation of a J/psi accompanied either by a eta(c) or a J/psi and another light parton. These results may be of great help to understand the polarisation of quarkonia produced at high energies.
description: 5 pages, 11 figures, LaTeX. v2: matches the PRL version (3 typos corrected and title changed)
Perturbation theory with dispersion and higher cumulants: non-linear regime
Creators: name: Garny, Mathias
name: Laxhuber, Dominik
name: Scoccimarro, Roman
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present non-linear solutions of Vlasov Perturbation Theory (VPT), describing gravitational clustering of collisionless dark matter with dispersion and higher cumulants induced by orbit crossing. We show that VPT can be cast into a form that is formally analogous to standard perturbation theory (SPT), but including additional perturbation variables, non-linear interactions, and a more complex propagation. VPT non-linear kernels have a crucial decoupling property: for fixed total momentum, the kernels becomes strongly suppressed when any of the individual momenta cross the dispersion scale into the non-linear regime. This screening of UV modes allows us to compute non-linear corrections to power spectra even for cosmologies with very blue power-law input spectra, for which SPT diverges. We compare predictions for the density and velocity divergence power spectra as well as the bispectrum at one-loop order to N-body results in a scaling universe with spectral indices $-1\leq n_s\leq +2$. We find a good agreement up to the non-linear scale for all cases, with a reach that increases with the spectral index $n_s$. We discuss the generation of vorticity as well as vector and tensor modes of the velocity dispersion, showing that neglecting vorticity when including dispersion would lead to a violation of momentum conservation. We verify momentum conservation when including vorticity, and compute the vorticity power spectrum at two-loop order, necessary to recover the correct large-scale limit with slope $n_w=2$. Comparing to our N-body measurements confirms the cross-over from $k^4$ to $k^2$ scaling on large scales. Our results provide a proof-of-principle that perturbative techniques for dark matter clustering can be systematically improved based on the known underlying collisionless dynamics.
description: 37 pages + appendices, 23 figures
A one-dimensional ultracold medium of extreme optical depth
Creators: name: Blatt, Frank
name: Halfmann, Thomas
name: Peters, Thorsten
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: Atomic Physics (physics.atom-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We report on the preparation of a one-dimensional ultracold medium in a hollow-core photonic crystal fiber, reaching an effective optical depth of 1000(150). We achieved this extreme optical depth by transferring atoms from a magneto-optical trap into a far-detuned optical dipole trap inside the hollow-core fiber, yielding up to 2.5(3)$\times$10$^5$ atoms inside the core with a loading efficiency of $2.5(6)~\%$. The preparation of an ultracold medium of such huge optical depth paves the way towards new applications in quantum optics and nonlinear optics.
FAIR approach in  low frequency radioastronomy
Creators: name: Cecconi, Baptiste
Publisher: name: Zenodo
Year: 2023

description: The Open Science paradigm and the FAIR principles (Findable, Accessible, Interoperable, Reusable) is aiming to foster scientific return, and reinforce the trust in science production. We present how the MASER (Measuring, Analysing and Simulating Emissions in the Radio range) implements Open Science through a series of existing solutions that have been put together, only adding new pieces where needed.
The MASER service is a "science ready" and "open science" toolbox dedicated to time-domain low frequency radioastronomy, which data products mostly covers Solar and planetary observations. The principal data product in this domain is a "dynamic spectrum", i.e., a series of consecutive spectra with the same observing configuration. The observed physical phenomena are related to plasma instabilities and energetic particles in magnetized plasma. Hence low frequency radio astronomy is a remote sensing tool for plasma diagnostics. 
MASER covers four community needs:1. Discovering data products,2. Exploring data collections before downloading TB's of files,3. Annotating and then storing and sharing annotations on radio dynamic spectra,4. Accessing data in Python.
MASER solutions are based on IVOA protocols for data discovery, on IHDEA tools for data exploration, and on a dedicated format developed by MASER for the temporal-spectral annotations. The service also proposes a data repository for sharing data collections, catalogues and associated documentation, as well as supplementary materials associated to papers. Each collection is managed through a Data Management Plan, which purpose is two-fold: supporting the provider for managing the collection content; and supporting the data centre for resource management. Each product of the repository is citable with a DOI, and the landing page contains web semantics annotations (using schema.org).
Microtus townsendii
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Microtus
Microtus townsendii

description: Microtus townsendii (Bachman, 1839). J. Acad. Nat. Sci. Philadelphia, 8:60. TYPE LOCALITY: USA, Oregon, Multnomah Co., Wappatoo (Sauvie) Island, lower Columbia River near mouth of Willamette River (as located by Bailey, 1900:46). DISTRIBUTION: Pacific northwest, from extreme SW British Columbia, Canada, to NW California, USA, including Vancouver and neighboring islands. SYNONYMS: cowani, cummingi, laingi, occidentalis, pugeti, tetramerus. COMMENTS: Subgenus Mynomes, pennsylvanicus species group sensu Zagorodnyuk (1990). Broadly allied with M. pennsylvanicus and M. nwntanus (Anderson, 1959; Hooper and Hart, 1962; Modi, 1987), though precise cladistic picture unresolved. See Comely and Verts (1988, Mammalian Species, 325).
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 530, DOI: 10.5281/zenodo.7353098
description: {"references": ["Bailey, V. E. 1900. Revision of American voles of the genus Microtus. North American Fauna, 17: 1 - 88.", "Zagorodnyuk, I. V. 1990. Kariotipicheskaya izmenchivost' i sistematika serykh polevok (Rodentia, Arvicolini). Soobshchenie 1. Vidovoi sostav i khromosomnye chisla [Karyotypic variability and systematics of the gray voles (Rodentia, Arvicolini). Communication 1. Species composition and chromosomal numbers]. Vestnik Zoologii, 2: 26 - 37 (in Russian).", "Anderson, S. 1959. Distribution, variation, and relationships of the montane vole, Microtus montanus. University of Kansas Publications, Museum of Natural History, 9: 415 - 511.", "Hooper, E. T., and B. S. Hart. 1962. A synopsis of Recent North American microtine rodents. Miscellaneous Publications, Museum of Zoology, University of Michigan, 120: 1 - 68.", "Modi, W. S. 1987. Phylogenetic analyses of chromosomal banding patterns among the Nearctic Arvicolidae (Mammalia: Rodentia). Systematic Zoology, 36: 109 - 136.", "Verts, B. J., and G. L. Kirkland, Jr. 1988. Perognathus parvus. Mammalian Species, 318: 1 - 8."]}
title: Saliniteitsgradiënt in het Schelde-estuarium: deelrapport 2. Scenario analyse numerieke modellering
Creators: name: Smolders, Sven
name: Kaptein, Steven
Publisher: name: Flanders Hydraulics
Year: 2024

description: Title : WL Rapporten. Waterbouwkundig Laboratorium: Antwerpen.
Volume : 19_081_2
Issue :
Pagination : VII, 37 + 5 p. bijl.
Companilactobacillus huachuanensis HUACHUANENSIS 2020, COMB. NOV.
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Companilactobacillus
Companilactobacillus huachuanensis

description: DESCRIPTIONOF COMPANILACTOBACILLUS HUACHUANENSIS COMB. NOV.
Companilactobacillus huachuanensis (hua.chuan.eńsis. N.L. masc. adj. huachuanensis pertainingto Huachuan County, a county in the Heilongjiang province of China).
Basonym: Lactobacillus huachuanensis Fu and Gu 2019, 2812 VP
The physiological properties of C. huachuanensis are comparable to C. heilongjiangensis [131]. The genome size is 3.02 Mbp. The mol% G+C content of DNA is 36.4.
Isolatedfromfermented Chinesecabbage.
Thetypestrainis 395–6.2 T =CCM 8927 T =NCIMB15188 T =L MG31179 T.
Genome sequence accession number: BJDF00000000.
16S RNA gene sequence accession number: LC438522.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2805, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Condensation Under Controlled Cooling: A Simulation Study
Creators: name: Pal, Barnana
Publisher: name: arXiv
Year: 2013
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The formation, growth, structure and cluster size distribution (CSD) properties in a two-dimensional system of particles interacting with Lennard-Jones (LJ) potential under controlled cooling condition have been studied using Monte-Carlo (MC) method considering modified Metropolis algorithm to introduce realistic thermal motion of the particles. The system, initially at relatively higher temperature Ti, undergoes temperature reduction following exponential law with decay constant a to a lower temperature Tf and subsequently reaches equilibrium. The equilibrium phase configuration depends strongly on the number density c of particles and a. The root mean square particle displacement in the final equilibrium phase shows maximum value for a = ac ~ 10-3 for all c. The CSD properties obtained at a = 10-3 shows a sharp peak in the lower cluster size region for low c. The peak shifts towards higher cluster size for lower a. The CSD fits well with a modified Gamma distribution function. All of the particles in the system form a single cluster when c is larger than a critical value cc (~0.5). A compact well-defined ordered structure is obtained for c > cc and a << ac.
A sub-Neptune transiting the young field star HD 18599 at 40 pc
Creators: name: de Leon, Jerome P.
name: Livingston, John H.
name: Jenkins, James S.
name: Vines, Jose I.
name: Wittenmyer, Robert A.
name: Clark, Jake T.
name: Winn, Joshua I. M.
name: Addison, Brett
name: Ballard, Sarah
name: Bayliss, Daniel
name: Beichman, Charles
name: Benneke, Björn
name: Berardo, David Anthony
name: Bowler, Brendan P.
name: Brown, Tim
name: Bryant, Edward M.
name: Christiansen, Jessie
name: Ciardi, David
name: Collins, Karen A.
name: Collins, Kevin I.
name: Crossfield, Ian
name: Deming, Drake
name: Dragomir, Diana
name: Dressing, Courtney D.
name: Fukui, Akihiko
name: Gan, Tianjun
name: Giacalone, Steven
name: Gill, Samuel
name: Alvarez, Erica Gonz\' alez
name: Hesse, Katharine
name: Horner, Jonathan
name: Howell, Steve B.
name: Jenkins, Jon M.
name: Kane, Stephen R.
name: Kendall, Alicia
name: Kielkopf, John F.
name: Kreidberg, Laura
name: Latham, David W.
name: Liu, Huigen
name: Lund, Michael B.
name: Matson, Rachel
name: Matthews, Elisabeth
name: Mengel, Matthew W.
name: Morales, Farisa
name: Mori, Mayuko
name: Narita, Norio
name: Nishiumi, Taku
name: Okumura, Jack
name: Plavchan, Peter
name: Quinn, Sam
name: Rabus, Markus
name: Ricker, George
name: Rudat, Alexander
name: Schlieder, Joshua
name: Schwarz, Richard P.
name: Seager, Sara
name: Shporer, Avi
name: Smith, Alexis M. S.
name: Sphorer, Avi
name: Stassun, Keivan
name: Tamura, Motohide
name: Tan, Thiam Guan
name: Tinney, C. G.
name: Vanderspek, Roland
name: Gorjian, Varoujan
name: Werner, Michael W.
name: West, Richard G.
name: Wright, Duncan
name: Zhang, Hui
name: Zhou, George
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Transiting exoplanets orbiting young nearby stars are ideal laboratories for testing theories of planet formation and evolution. However, to date only a handful of stars with age <1 Gyr have been found to host transiting exoplanets. Here we present the discovery and validation of a sub-Neptune around HD 18599, a young (300 Myr), nearby (d=40 pc) K star. We validate the transiting planet candidate as a bona fide planet using data from the TESS, Spitzer, and Gaia missions, ground-based photometry from IRSF, LCO, PEST, and NGTS, speckle imaging from Gemini, and spectroscopy from CHIRON, NRES, FEROS, and Minerva-Australis. The planet has an orbital period of 4.13 d, and a radius of 2.7Rearth. The RV data yields a 3-sigma mass upper limit of 30.5Mearth which is explained by either a massive companion or the large observed jitter typical for a young star. The brightness of the host star (V~9 mag) makes it conducive to detailed characterization via Doppler mass measurement which will provide a rare view into the interior structure of young planets.
description: submitted to MNRAS
Modeling and estimation of multi-source clustering in crime and security data
Creators: name: Mohler, George
Publisher: name: arXiv
Year: 2013
Subjects: subject: Applications (stat.AP)
subject: FOS: Computer and information sciences

description: While the presence of clustering in crime and security event data is well established, the mechanism(s) by which clustering arises is not fully understood. Both contagion models and history independent correlation models are applied, but not simultaneously. In an attempt to disentangle contagion from other types of correlation, we consider a Hawkes process with background rate driven by a log Gaussian Cox process. Our inference methodology is an efficient Metropolis adjusted Langevin algorithm for filtering of the intensity and estimation of the model parameters. We apply the methodology to property and violent crime data from Chicago, terrorist attack data from Northern Ireland and Israel, and civilian casualty data from Iraq. For each data set we quantify the uncertainty in the levels of contagion vs. history independent correlation.
description: Published in at http://dx.doi.org/10.1214/13-AOAS647 the Annals of Applied Statistics (http://www.imstat.org/aoas/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Topological phase transition in commensurate multi-frequency Floquet Su-Schrieffer-Heeger model
Creators: name: Olin, Sam
name: Lee, Wei-Cheng
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Recently, Floquet systems have attracted a great deal of interest as they offer unprecedented ability to engineer topological states through the tuning of an external time-periodic drive. Consequentially, seeking new driving protocols that allow for more exotic topological phases and transitions becomes imperative for the Floquet engineer. In this paper, we study the Su-Schrieffer-Heeger model driven by two time-dependent periodic sources with commensurate frequencies and an amplitude modulation. Imposing more than one driving frequency allows us to realize even more exotic topological phases resulting from new couplings appearing in the Fourier space representation. Moreover, we find an experimentally practical method for sweeping the system through a topological phase transition by varying the amplitude mixture of the commensurate sources. We employ the local Chern marker, a real space representation of the Chern number, to simulate topological phase diagrams of the two-drive Floquet Hamiltonian in a variety of driving cases.
description: 8 pages, 9 figures
title: Αναδυόμενες τάσεις στην παραγωγή υδροηλεκτρικής ενέργειας: Εξερεύνηση τεχνολογιών ροής ποταμού, αντλησοταμίευσης και θαλάσσιας ενέργειας για βιώσιμη παραγωγή ενέργειας
Creators: name: Μαρκακης Μιχαηλ
Publisher: name: Technical University of Crete
Year: 2024

description: Η παρούσα διατριβή διερευνά το εξελισσόμενο τοπίο των ανανεώσιμων πηγών ενέργειας, εστιάζοντας ειδικά στις εξελίξεις και την ενσωμάτωση των υδροηλεκτρικών και θαλάσσιων ενεργειακών συστημάτων στο παγκόσμιο ενεργειακό πλέγμα. Η μελέτη εμβαθύνει στις τεχνολογικές καινοτομίες, τις περιβαλλοντικές επιπτώσεις και την οικονομική βιωσιμότητα αυτών των ανανεώσιμων πηγών, παρέχοντας μια ολοκληρωμένη ανάλυση του ρόλου τους στην αειφόρο ενεργειακή ανάπτυξη. Η υδροηλεκτρική ενέργεια, μια καθιερωμένη πηγή, συνεχίζει να επεκτείνει την αποδοτικότητά της μέσω τεχνολογικών αναβαθμίσεων και της ενσωμάτωσης με άλλες ανανεώσιμες πηγές ενέργειας, ιδίως σε υβριδικά συστήματα. Η θαλάσσια ενέργεια, συμπεριλαμβανομένης της παλιρροιακής και της κυματικής ενέργειας, αν και λιγότερο ανεπτυγμένη, παρουσιάζει σημαντικές δυνατότητες λόγω της προβλέψιμης φύσης της και των τεράστιων ανεκμετάλλευτων πόρων της.
Τα περιβαλλοντικά ζητήματα που σχετίζονται με αυτές τις μορφές ενέργειας εξετάζονται κριτικά, υπογραμμίζοντας την ισορροπία μεταξύ της παραγωγής ενέργειας και της οικολογικής διατήρησης. Η παρούσα διατριβή εξετάζει την εφαρμογή προηγμένων μηχανολογικών λύσεων που αποσκοπούν στην ελαχιστοποίηση του περιβαλλοντικού αποτυπώματος των υδροηλεκτρικών σταθμών και των θαλάσσιων ενεργειακών συστημάτων. Αξιολογείται επίσης η αποτελεσματικότητα των υφιστάμενων κανονιστικών πλαισίων και πολιτικών που προωθούν τη βιώσιμη ανάπτυξη αυτών των τεχνολογιών, προτείνοντας τομείς για την ενίσχυση της πολιτικής ώστε να υποστηριχθεί η περαιτέρω ενσωμάτωση στις εθνικές και διεθνείς ενεργειακές στρατηγικές.
Οι οικονομικές αναλύσεις αποκαλύπτουν ότι, ενώ το αρχικό κόστος παραμένει υψηλό, τα μακροπρόθεσμα οφέλη από την ενσωμάτωση της υδροηλεκτρικής και της θαλάσσιας ενέργειας στα συστήματα ανανεώσιμων πηγών ενέργειας - όπως η σταθερότητα του δικτύου, η διαφοροποίηση του εφοδιασμού και η μείωση των εκπομπών διοξειδίου του άνθρακα - αντισταθμίζουν αυτές τις αρχικές δαπάνες. Η διατριβή προτείνει στρατηγικές συστάσεις για τη μείωση του κόστους μέσω τεχνολογικών καινοτομιών, πολιτικών κινήτρων και αυξημένων επενδύσεων του κυβερνητικού και ιδιωτικού τομέα.
An Explanation for the Different X-ray to Optical Column Densities in the Environments of Gamma Ray Bursts: A Progenitor Embedded in a Dense Medium
Creators: name: Krongold, Yair
name: Prochaska, J. Xavier
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study the > 10 ratios in the X-ray to optical column densities inferred from afterglow spectra of Gamma Ray Bursts due to gas surrounding their progenitors. We present time-evolving photoionization calculations for these afterglows and explore different conditions for their environment. We find that homogenous models of the environment (constant density) predict X-ray columns similar to those found in the optical spectra, with the bulk of the opacity being produced by neutral material at large distances from the burst. This result is independent of gas density or metallicity. Only models assuming a progenitor immersed in a dense (10^(2-4) cm-3) cloud of gas (with radius ~10 pc), with a strong, declining gradient of density for the surrounding interstellar medium are able to account for the large X-ray to optical column density ratios. However, to avoid an unphysical correlation between the size of this cloud, and the size of the ionization front produced by the GRB, the models also require that the circumburst medium is already ionized prior to the burst. The inferred cloud masses are <10^6 M_solar, even if low metallicities in the medium are assumed (Z~0.1 Z_solar). These cloud properties are consistent with those found in giant molecular clouds and our results support a scenario in which the progenitors reside within intense star formation regions of galaxies. Finally, we show that modeling over large samples of GRB afterglows may offer strong constraints on the range of properties in these clouds, and the host galaxy ISM.
description: Accepted for publication in ApJ. Tentatively scheduled for the September 1, 2013, V774-1 issue. 9 figures 28 pages
Microtus transcaspicus Satunin 1905
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Microtus
Microtus transcaspicus

description: Microtus transcaspicus Satunin, 1905. Izv. Kavkas. Mus., 2:57. TYPE LOCALITY: Turkmenistan, Kopet Dag Mtns, Chuli Valley, near Ashkhabad. DISTRIBUTION: S Turkmenistan, N Afghanistan, and N Iran. SYNONYMS: khorkoutensis. COMMENTS: Subgenus Microtus, arvalis species group sensu Zagorodnyuk (1990). Taxonomy reviewed by Gromov and Polyakov (1977), Corbet (1978c), Malygin (1978), Meier et al. (1981), and Meier (1983).
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 531, DOI: 10.5281/zenodo.7353098
description: {"references": ["Zagorodnyuk, I. V. 1990. Kariotipicheskaya izmenchivost' i sistematika serykh polevok (Rodentia, Arvicolini). Soobshchenie 1. Vidovoi sostav i khromosomnye chisla [Karyotypic variability and systematics of the gray voles (Rodentia, Arvicolini). Communication 1. Species composition and chromosomal numbers]. Vestnik Zoologii, 2: 26 - 37 (in Russian).", "Gromov, I. M., and I. Ya. Polyakov. 1977. Fauna SSSR, Mlekopitayushchie, tom 3, vyp. 8 [Fauna of the USSR, vol. 3, pt. 8, Mammals]. Polevki [Voles (Microtinae)]. Nauka, Moscow-Leningrad, 504 pp. (in Russian).", "Corbet, G. B. 1978 c. The mammals of the Palaearctic region: A taxonomic review. British Museum (Natural History), London, 314 pp.", "Malygin, V. M. 1978. [A comparative-morphological analysis of species from the group Microtus arvalis (Rodentia, Cricetidae).] Zoologicheskii Zhurnal, 67: 1062 - 1073 (in Russian)."]}
Signature transition in Einstein-Cartan cosmology
Creators: name: Vakili, Babak
name: Jalalzadeh, Shahram
Publisher: name: arXiv
Year: 2013
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In the context of Einstein-Cartan theory of gravity, we consider a Friedmann-Lemaitre-Robertson-Walker (FLRW) cosmological model with Weyssenhoff perfect fluid. We focus attention on those classical solutions that admit a degenerate metric in which the scale factor has smooth behavior in the transition from a Euclidean to a Lorentzian domain. It is shown that the spin-spin contact interaction enables one to obtain such a signature changing solutions due to the Riemann-Cartan ($U_4$) structure of space-time.
description: 9 pages, typos corrected
Razvoj samostalnog interaktivnog sistema za programiranje industrijskih robota podržanog tehnologijom proširene realnosti (L-IRL XR).
Creators: name: A. Dević
name: J. Vidaković
name: N. Živković
Publisher: name: Zenodo
Year: 2024

description: Razvoj samostalnog interaktivnog sistema za programiranje industrijskih robota podržanog tehnologijom proširene realnosti (L-IRL XR). (2024). U procesu recenziranja.
Inflaton as a pseudo-Nambu-Goldstone boson
Creators: name: Kitazawa, Noriaki
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In the realistic model of cosmic inflation the inflaton potential should be flat and stable under quantum corrections. It is natural to imagine that there is some symmetry behind and an idea of the inflaton as a Nambu-Goldstone boson of spontaneous breaking of some symmetry has been examined. We give a general formulation of this idea using the non-linear realization of Nambu-Goldstone boson in low-energy effective theory with some explicit symmetry breaking to generate non-trivial potential. The potential is naturally a simple function, typically the mass term of inflaton, and the scenario of "warm inflation" should necessarily be applied under the present observational constraints. We investigate the generation mechanism of necessary thermal dissipation term in inflaton field equation for "warm inflation" without large thermal corrections to inflaton potential. A simple numerical analysis is given to investigate the viability of this scenario.
description: 11 pages
Conversion of Legal Agreements into Smart Legal Contracts using NLP
Creators: name: Chen, Eason
name: Roche, Niall
name: Tseng, Yuen-Hsien
name: Hernandez, Walter
name: Shangguan, Jiangbo
name: Moore, Alastair
Publisher: name: arXiv
Year: 2022
Subjects: subject: Computers and Society (cs.CY)
subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences
subject: I.7
subject: 68T50

description: A Smart Legal Contract (SLC) is a specialized digital agreement comprising natural language and computable components. The Accord Project provides an open-source SLC framework containing three main modules: Cicero, Concerto, and Ergo. Currently, we need lawyers, programmers, and clients to work together with great effort to create a usable SLC using the Accord Project. This paper proposes a pipeline to automate the SLC creation process with several Natural Language Processing (NLP) models to convert law contracts to the Accord Project's Concerto model. After evaluating the proposed pipeline, we discovered that our NER pipeline accurately detects CiceroMark from Accord Project template text with an accuracy of 0.8. Additionally, our Question Answering method can extract one-third of the Concerto variables from the template text. We also delve into some limitations and possible future research for the proposed pipeline. Finally, we describe a web interface enabling users to build SLCs. This interface leverages the proposed pipeline to convert text documents to Smart Legal Contracts by using NLP models.
description: 7 pages, Companion Proceedings of the ACM Web Conference 2023 (WWW '23 Companion), April 30-May 4, 2023, Austin, TX, USA
Microtus umbrosus Merriam 1898
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Microtus
Microtus umbrosus

description: Microtus umbrosus Merriam, 1898. Proc. Biol. Soc. Washington, 12:107. TYPE LOCALITY: Mexico, Oaxaca, Mt. Zempoaltepec, 8200 ft. DISTRIBUTION: Known only from Mt. Zempoaltepec. COMMENTS: Type species and sole member of Orthriomys, a taxon typically identified as a subgenus of Microtus (Anderson, 1959; Bailey, 1900; Hall and Cockrum, 1953; Zagorodnyuk, 1990). Martin (1974:61) suggested that this species "may eventually" be included in Neodon.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 531, DOI: 10.5281/zenodo.7353098
description: {"references": ["Anderson, S. 1959. Distribution, variation, and relationships of the montane vole, Microtus montanus. University of Kansas Publications, Museum of Natural History, 9: 415 - 511.", "Bailey, V. E. 1900. Revision of American voles of the genus Microtus. North American Fauna, 17: 1 - 88.", "Hall, E. R., and E. L. Cockrum. 1953. A synopsis of the North American microtine rodents. University of Kansas Publications, Museum of Natural History, 5: 373 - 498.", "Zagorodnyuk, I. V. 1990. Kariotipicheskaya izmenchivost' i sistematika serykh polevok (Rodentia, Arvicolini). Soobshchenie 1. Vidovoi sostav i khromosomnye chisla [Karyotypic variability and systematics of the gray voles (Rodentia, Arvicolini). Communication 1. Species composition and chromosomal numbers]. Vestnik Zoologii, 2: 26 - 37 (in Russian).", "Martin, R. A. 1974. Fossil mammals from the Coleman IIA Fauna, Sumter County. Pp. 35 - 99, in Pleistocene mammals of Florida (S. D. Webb, ed.). The University Presses of Florida, Gainesville, 270 pp."]}