cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Gibbula Harzhauser, 2021, s.l.
Creators: name: Harzhauser, Mathias
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Archaeogastropoda
Trochidae
Gibbula

description: Gibbula s.l. carasiensis (Jekelius, 1944) †
Middle Miocene (Sarmatian): Central Paratethys Sea (Hungary).
(Jekelius 1944)
description: Published as part of Harzhauser, Mathias, 2021, The Cainozoic to present-day record of Circum-Mediterranean, NE Atlantic and North Sea Cantharidinae and Trochinae (Trochoidea, Gastropoda) - a synopsis, pp. 1-81 in Zootaxa 4902 (1) on page 36, DOI: 10.11646/zootaxa.4902.1.1, http://zenodo.org/record/4419088
Force generation in confined active fluids: The role of microstructure
Creators: name: Paul, Shuvojit
name: Jayaram, Ashreya
name: Narinder, N
name: Speck, Thomas
name: Bechinger, Clemens
Publisher: name: arXiv
Year: 2022
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Applied Physics (physics.app-ph)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: We experimentally determine the force exerted by a bath of active particles onto a passive probe as a function of its distance to a wall and compare it to the measured averaged density distribution of active particles around the probe. Within the framework of an active stress, we demonstrate that both quantities are - up to a factor - directly related to each other. Our results are in excellent agreement with a minimal numerical model and confirm a general and system-independent relationship between the microstructure of active particles and transmitted forces.
description: Accepted for the publication in Physical Review Letters, see https://journals.aps.org/prl/accepted/8b078YcbZb419475998267a260895e617cab4a01e
$\mathcal{N}=2$ resonant superalgebra for supergravity
Creators: name: Durka, Remigiusz
name: Graczyk, Krzysztof M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present new superalgebra for $\mathcal{N}=2$ $D=3,4$ supergravity theory endowed with the $U(1)$ generator. The superalgebra is rooted in the so-called Soroka-Soroka algebra and spanned by the Lorentz $J_{ab}$ and Lorentz-like $Z_{ab}$, translation $P_a$ and $T$ generators, as well as two supercharges $Q^I_α$. It is the only possible realization for a given generator content. We construct a corresponding 3D Chern-Simons supergravity realization of the superalgebra and discuss its relevance.
description: 12 pages, to appear in Phys. Lett. B
Benchmark tests of transmission spectroscopy using transiting white dwarfs
Creators: name: Jiang, Chengzi
name: Chen, Guo
name: Pallé, Enric
name: Parviainen, Hannu
name: Murgas, Felipe
name: Ma, Yuehua
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Ground-based transit observations are affected by both telluric absorption and instrumental systematics. To account for these effects, a better understanding of the impact of different data analyses is needed to improve the accuracy of the retrieved transmission spectra. We propose validating ground-based low-resolution transmission spectroscopy using transiting white dwarfs. The advantage here is that we know beforehand what the final transmission spectrum should be: a featureless flat spectrum. We analyzed two transiting white dwarfs analogous to hot Jupiters. We used various noise models to account for the systematic noise in their spectroscopic light curves following common procedures of transmission spectroscopy analyses. We compared the derived transmission spectra with the broadband transit depth to determine whether there are any artificial offsets or spectral features arising from light-curve fitting. The results show a strong model dependence, and the transmission spectra exhibit considerable discrepancies when they are computed with different noise models, different reference stars, and different common-mode removal methods. Nonetheless, we can still derive relatively accurate transmission spectra based on a Bayesian model comparison. With current ground-based instrumentation, the systematics in transit light curves can easily contaminate a transmission spectrum, introducing a general offset or some spurious spectral features and thus leading to a biased interpretation on the planetary atmosphere. Therefore, it is necessary to determine the dependence of results on the adopted noise model through model comparison. The model inferences should be examined through multiple observations and different instruments. (Abridged)
description: Accepted for pulication in A&A, 18 pages, 9 figures
Relativistic QFT from a Bohmian perspective: A proof of concept
Creators: name: Nikolic, Hrvoje
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Since Bohmian mechanics is explicitly nonlocal, it is widely believed that it is very hard, if not impossible, to make Bohmian mechanics compatible with relativistic quantum field theory (QFT). I explain, in simple terms, that it is not hard at all to construct a Bohmian theory that lacks Lorentz covariance, but makes the same measurable predictions as relativistic QFT. All one has to do is to construct a Bohmian theory that makes the same measurable predictions as QFT in one Lorentz frame, because then standard relativistic QFT itself guarantees that those predictions are Lorentz invariant. I first explain this in general terms, then I describe a simple Bohmian model that makes the same measurable predictions as the Standard Model of elementary particles, after which I give some hints towards a more fundamental theory beyond Standard Model. Finally, I present a short story telling how my views of fundamental physics in general, and of Bohmian mechanics in particular, evolved over time.
description: 19 pages, version accepted for publication in Found. Phys
Lithium depletion boundary, stellar associations, and Gaia
Creators: name: Galindo-Guil, F. J.
name: Barrado, D.
name: Bouy, H.
name: Olivares, J.
name: Bayo, A.
name: Morales-Calderón, M.
name: Huélamo, N.
name: Sarro, L. M.
name: Rivière-Marichalar, P.
name: Stoev, H.
name: Montesinos, B.
name: Stauffer, J. R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences
subject: 85

description: Stellar ages are key to improving our understanding of different astrophysical phenomena. However, many techniques to estimate stellar ages are highly model-dependent. The lithium depletion boundary (LDB), based on the presence or absence of lithium in low-mass stars, can be used to derive ages in stellar associations of between 20 and 500~Ma. The purpose of this work is to revise former LDB ages in stellar associations in a consistent way, taking advantage of the homogeneous \textit{Gaia} parallaxes as well as bolometric luminosity estimations that do not rely on monochromatic bolometric corrections. We studied nine open clusters and three moving groups characterised by a previous determination of the LDB age. We gathered all the available information from our data and the literature: membership, distances, photometric data, reddening, metallicity, and surface gravity. We re-assigned membership and calculated bolometric luminosities and effective temperatures using distances derived from Gaia DR2 and multi-wavelength photometry for individual objects around the former LDB. We located the LDB using a homogeneous method for all the stellar associations. Finally, we estimated the age by comparing it with different evolutionary models. We located the LDB for the twelve stellar associations and derived their ages using several theoretical evolutionary models. We compared the LDB ages among them, along with data obtained with other techniques, such as isochrone fitting, ultimately finding some discrepancies among the various approaches. Finally, we remark that the 32 Ori MG is likely to be composed of at least two populations of different ages.
description: 78 pages, accepted by A&A
Correlated driving-and-dissipation equation for non-Condon spectroscopy with the Herzberg-Teller vibronic coupling
Creators: name: Fang, Jie
name: Chen, Zi-Hao
name: Wang, Yao
name: Xu, Rui-Xue
name: Yan, YiJing
Publisher: name: arXiv
Year: 2022
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Correlated driving-and-dissipation equation (CODDE) is an optimized complete second-order quantum dissipation approach, which is originally concerned with the reduced system dynamics only. However, one can actually extract the hybridized bath dynamics from CODDE with the aid of dissipaton-equation-of-motion theory, a statistical quasi-particle quantum dissipation formalism. Treated as an one{dissipaton theory, CODDE is successfully extended to deal with the Herzberg-Teller vibronic couplings in dipole-field interactions. Demonstrations will be carried out on the non-Condon spectroscopies of a model dimer system.
description: 6 pages, 2 figures
Passing Voice to the Voiceless: An assessment of Wenzhounese Endangerment Level and a Text-to-Speech System for Language Preservation
Creators: name: Chen, Kimball
Publisher: name: Stanford Digital Repository
Year: 2024
Subjects: Language endangerment, Language preservation, Text-to-Speech, Machine learning

description: This thesis examines the current endangerment level of Wenzhounese, a Chinese dialect spoken in the Wenzhou region of China, and explores the potential of a Text-to-Speech (TTS) system as a tool for language preservation. The study employs UNESCO's language vitality assessment framework to conduct a comprehensive survey of Wenzhounese speakers, assessing factors such as intergenerational transmission, absolute number of speakers, and community attitudes. The findings suggest that while Wenzhounese is not immediately endangered, it faces significant challenges in intergenerational transmission and usage across diverse domains, placing it at risk of future endangerment. To explore innovative solutions for language preservation, the thesis develops a TTS system for Wenzhounese by fine-tuning a pre-trained Tacotron 2 model. Despite limitations in training data and the nascent stage of Wenzhounese TTS technology, the results demonstrate the feasibility of creating a functioning TTS system for the language. The Mean Opinion Score (MOS) evaluation of the synthesized speech highlights the need for further refinement and improvement.
Bethe Salpeter Equation Spectra for Very Large Systems
Creators: name: Bradbury, Nadine
name: Nguyen, Minh
name: Caram, Justin R
name: Neuhauser, Daniel
Publisher: name: arXiv
Year: 2022
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We present a highly efficient method for the extraction of optical properties of very large molecules via the Bethe-Salpeter equation. The crutch of this approach is the calculation of the action of the effective Coulombic interaction, $W$, through a stochastic TD Hartree propagation, which uses only 10 stochastic orbitals rather than propagating the full sea of occupied states. This leads to a scaling that is at most cubic in system size, with trivial MPI parallelization. We apply this new method to calculate the spectra and electronic density of the dominant excitons of a carbon-nanohoop bound fullerene system with 520 electrons, using less than 4000 core hours.
description: 6 pages, 3 figures, communication
Gibbula Harzhauser, 2021, s.l.
Creators: name: Harzhauser, Mathias
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Archaeogastropoda
Trochidae
Gibbula

description: Gibbula s.l. curvilineata (Sinzow, 1877) †
Middle-late Miocene (Bessarabian): Eastern Paratethys Sea (Ukraine).
(Anistratenko & Anistratenko 2012)
description: Published as part of Harzhauser, Mathias, 2021, The Cainozoic to present-day record of Circum-Mediterranean, NE Atlantic and North Sea Cantharidinae and Trochinae (Trochoidea, Gastropoda) - a synopsis, pp. 1-81 in Zootaxa 4902 (1) on page 36, DOI: 10.11646/zootaxa.4902.1.1, http://zenodo.org/record/4419088
Gibbula cremenensis Risso 1826, s.l.
Creators: name: Harzhauser, Mathias
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Archaeogastropoda
Trochidae
Gibbula

description: Gibbula s.l. cremenensis (Andrzejowski, 1830) †
= Trochus angulatus Eichwald, 1829 (non J. de C. Sowerby, 1823)
= Trochus subbalatro Kolesnikov, 1935
= Gibbula angulata spirocarinata Papp, 1954
Middle Miocene (Sarmatian): Central Paratethys Sea (Austria, Slovakia, Hungary).
Middle-late Miocene (Volhynian): Eastern Paratethys Sea (Poland, Moldova, Ukraine, Russia). (Sladkovskaya 2017)
description: Published as part of Harzhauser, Mathias, 2021, The Cainozoic to present-day record of Circum-Mediterranean, NE Atlantic and North Sea Cantharidinae and Trochinae (Trochoidea, Gastropoda) - a synopsis, pp. 1-81 in Zootaxa 4902 (1) on page 36, DOI: 10.11646/zootaxa.4902.1.1, http://zenodo.org/record/4419088
Variance of the Casimir force in an ideal Bose gas
Creators: name: Napiórkowski, Marek
name: Pruszczyk, Marcin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We consider an ideal Bose gas enclosed in a $d$-dimensional slab of thickness $D$. Using the grand canonical ensemble we calculate the variance of the thermal Casimir force acting on the slab's walls. The variance evaluated per unit wall area is shown to decay like $ Δ_{var}/D$ for large $D$. The amplitude $ Δ_{var}$ is a non-universal function of two scaling variables $λ/ ξ$ and $D/ ξ$, where $λ$ is the thermal de Broglie wavelength and $ξ$ is the bulk correlation length. It can be expressed via the bulk pressure, the Casimir force per unit wall area, and its derivative with respect to chemical potential. For thermodynamic states corresponding to the presence of the Bose-Einstein condensate the amplitude $ Δ_{var}$ retains its non-universal character while the ratio of the mean standard deviation and the Casimir force takes the scaling form $(D/L)^{\frac{d-1}{2}}\, (D/λ)^{d/2}$, where $L$ is the linear size of the wall.
description: 9 pages, no figures
Measuring precise radial velocities on individual spectral lines. III. Dependence of stellar activity signal on line formation temperature
Creators: name: Moulla, K. Al
name: Dumusque, X.
name: Cretignier, M.
name: Zhao, Y.
name: Valenti, J. A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Context. To enable radial velocity (RV) precision on the order of ~0.1 m/s required for the detection of Earth-like exoplanets orbiting solar-type stars, the main obstacle lies in mitigating the impact of stellar activity. Aims. This study investigates the dependence of derived RVs with respect to the formation temperature of spectral line segments. Methods. Using spectral synthesis, we compute for each observed wavelength point of unblended spectral lines the stellar temperature below which 50% of the emergent flux originates. We can then construct RV time series for different temperature ranges, using template matching. Results. With HARPS-N solar data and HARPS $α$ Cen B measurements, we demonstrate on time intervals of prominent stellar activity that the activity-induced RV signal has different amplitude and periodicity depending on the temperature range considered. We compare the solar measurements with simulated contributions from active surface regions seen in simultaneous images, and find that the suppression of convective motion is the dominant effect. Conclusions. From a carefully selected set of spectral lines, we are able to measure the RV impact of stellar activity at various stellar temperatures ranges. We are able to strongly correlate the effect of convective suppression with spectral line segments formed in hotter temperature ranges. At cooler temperatures, the derived RVs exhibit oppositely directed variations compared to the average RV time series and stronger anti-correlations with chromospheric emission.
description: Accepted for publication in A&A
Bilateral optic pathway  glioma in Neurofibromatosis type1
Creators: name: Hota, Paramita
Publisher: name: EURORAD
Year: 2018
Subjects: subject: Musculoskeletal spine
subject: Neuroradiology brain
subject: Neuroradiology spine
subject: MR
subject: Colonography MR
subject: Comparative studies
subject: Neoplasia

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 2 years
description: Clinical History: Worsening of vision and headache in a two years old male child. On clinical examination multiple neurofibromas over the body, axillary freckling and 6 cafe au lait spots were noted hence the patient was referred to our department with suspicion of neurofi... Final Diagnosis: Bilateral optic pathway glioma with cervicomedullary glioma in neurofibromatosis 1
Violations of Quark-Hadron Duality in Low-Energy Determinations of $α_s$
Creators: name: Pich, Antonio
name: Rodríguez-Sánchez, Antonio
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Using the spectral functions measured in $τ$ decays, we investigate the actual numerical impact of duality violations on the extraction of the strong coupling. These effects are tiny in the standard $α_s(m_τ^2)$ determinations from integrated distributions of the hadronic spectrum with pinched weights, or from the total $τ$ hadronic width. The pinched-weight factors suppress very efficiently the violations of duality, making their numerical effects negligible in comparison with the larger perturbative uncertainties. However, combined fits of $α_s$ and duality-violation parameters, performed with non-protected weights, are subject to large systematic errors associated with the assumed modelling of duality-violation effects. These uncertainties have not been taken into account in the published analyses, based on specific models of quark-hadron duality.
description: 39 pages, 8 figures. References added. Published version
MPEC 2025-A110 : 2024 YB26
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2025
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 YB26

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Starbursts with suppressed velocity dispersion revealed in a forming cluster at z=2.51
Creators: name: Xiao, Mengyuan
name: Wang, Tao
name: Elbaz, David
name: Iono, Daisuke
name: Lu, Xing
name: Bing, Longji
name: Daddi, Emanuele
name: Magnelli, Benjamin
name: Gómez-Guijarro, Carlos
name: Bournaud, Frederic
name: Gu, Qiusheng
name: Jin, Shuowen
name: Valentino, Francesco
name: Zanella, Anita
name: Gobat, Raphael
name: Martin, Sergio
name: Brammer, Gabriel
name: Kohno, Kotaro
name: Schreiber, Corentin
name: Ciesla, Laure
name: Yu, Xiaoling
name: Okumura, Koryo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: One of the most prominent features of galaxy clusters is the presence of a dominant population of massive ellipticals in their cores. Stellar archaeology suggests that these gigantic beasts assembled most of their stars in the early Universe via starbursts. However, the role of dense environments and their detailed physical mechanisms in triggering starburst activities remain unknown. Here we report spatially resolved Atacama Large Millimeter/submillimeter Array (ALMA) observations of the CO $J= 3-2$ emission line, with a resolution of about 2.5 kiloparsecs, toward a forming galaxy cluster core with starburst galaxies at $z=2.51$. In contrast to starburst galaxies in the field often associated with galaxy mergers or highly turbulent gaseous disks, our observations show that the two starbursts in the cluster exhibit dynamically cold (rotation-dominated) gas-rich disks. Their gas disks have extremely low velocity dispersion ($σ_{\mathrm{0}} \sim 20-30$ km s$^{-1}$), which is three times lower than their field counterparts at similar redshifts. The high gas fraction and suppressed velocity dispersion yield gravitationally unstable gas disks, which enables highly efficient star formation. The suppressed velocity dispersion, likely induced by the accretion of corotating and coplanar cold gas, might serve as an essential avenue to trigger starbursts in massive halos at high redshifts.
description: 19 pages, 14 figures, 3 tables. Accepted for publication in A&A
Evaluation of a validated assessment tool of technical skill competency for high risk, low volume procedures.
Creators: name: Smith, Tameka
Publisher: name: Oregon Health and Science University
Year: 2024
Subjects: subject: Central Venous Catheters
subject: Hematemesis
subject: Curriculum
subject: Simulation Training
subject: Critical Care
subject: procedural training
subject: skill competency
subject: critical care fellowship

description: Critical care medicine is an environment that requires a wide skill set of medical knowledge and procedural skills. Trainees in critical care medicine along with future credentialing bodies have an expectation that proficiency in procedure skills are obtained during their training. Simulation training has been used in critical care training typically as task trainers or human patient simulators, which has been shown to be more effective in a recent meta-analysis1. This can easily be accomplished with the more common procedures such as central venous catheters, arterial line catheters, paracenteses, and intubations. Certain procedures are less common in many clinical environments but still require proficiency should the clinical situation arise. We are currently creating a curriculum that provides a simulation for the pulmonary and critical care trainees to review and practice the skills required for less common procedures such as placement of a Blakemore or Minnesota tube for management of hematemesis from gastric or variceal varices, and placement of transvenous pacers.
Gibbula feneoniana Harzhauser, 2021, s.l.
Creators: name: Harzhauser, Mathias
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Archaeogastropoda
Trochidae
Gibbula
Gibbula feneoniana

description: Gibbula s.l. feneoniana (d’Orbigny, 1844) †
= Trochus praefeneonianus Kolesnikov, 1935
Middle-late Miocene (Volhynian, Bessarabian): Eastern Paratethys Sea (Moldova, Ukraine, Russia). (Sladkovskaya 2017)
description: Published as part of Harzhauser, Mathias, 2021, The Cainozoic to present-day record of Circum-Mediterranean, NE Atlantic and North Sea Cantharidinae and Trochinae (Trochoidea, Gastropoda) - a synopsis, pp. 1-81 in Zootaxa 4902 (1) on page 36, DOI: 10.11646/zootaxa.4902.1.1, http://zenodo.org/record/4419088
Quantum state inference from coarse-grained descriptions: analysis and an application to quantum thermodynamics
Creators: name: Vallejos, Raúl O.
name: Correia, Pedro Silva
name: Obando, Paola Concha
name: O'Neill, Nina Machado
name: Tacla, Alexandre Baron
name: de Melo, Fernando
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The characterization of physical systems relies on the observable properties which are measured, and how such measurements are performed. Here we analyze two ways of assigning a description to a quantum system assuming that we only have access to coarse-grained properties. More specifically, we compare the Maximum Entropy Principle method, with the Bayesian-inspired recently proposed Average Assignment Map method [P. S. Correia et al, Phys. Rev. A 103, 052210 (2021)]. Despite the fact that the assigned descriptions by both methods respect the measured constraints, and that they share the same conceptual foundations, the descriptions differ in scenarios that go beyond the traditional system-environment structure. The Average Assignment Map is thus shown to be a more sensible choice for the ever more prevalent scenario of complex quantum systems. We discuss the physics behind such a difference, and further exploit it in a quantum thermodynamics process.
description: 14+5 pages, 9+2 figures. Comments are welcome
Re-Evaluating Computational Models Of Semantic Cognition
Creators: name: Guest, Olivia
Publisher: name: Zenodo
Year: 2014

description: Several computational models of the semantic cognitive system have been developed. This thesis considers four such models: the hub-and-spoke, the conceptual structure, the modality-specific, and the conceptual topography model. These models account for both generalised and category-specific semantic impairments. The models encapsulate different, and partially mutually exclusive, theoretical positions, but still account for similar, if not overlapping, semantic impairments. However, no single theory explains the full spectrum of both healthy and impaired semantic cognition. In order to better understand the space of theories and their inter-relations, this thesis reports results from (re)implementing the four theories and attempting to simulate both types of semantic impairment within each implementation. These four implementations shed light on the various computational and modelling assumptions and implications of each theoretical position. Compatibilities (and incompatibilities) between each theory (and model) are also discussed. It is additionally argued that some assumptions within each account, even though superficially different, are shared, and, conversely, some seemingly minor or background assumptions are centrally important. Examples of the latter include: limiting attention within any model to just two input modalities; evaluating model and patient behaviour with non-naturalistic semantic tasks; ignoring input from executive and affective systems; or (within the hub-and-spoke model) appealing to emergent properties of the implementation.
YOG'DA ERUVCHI VITAMINLARNING HAYVONLAR ORGANIZMIGA TA'SIRI.
Creators: name: Babayeva Sh. Samarqand davlat veterinariya meditsinasi, chorvachilik va biotexnologiyalar universiteti
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqolada yog‘da eruvchi har xil vitaminlarninghayvonlar organizmiga ijobiy ta’siri, mahsuldorlikni oshirishga samarasi haqidabayon etilgan.
Enhanced $d$-$p$ hybridization intertwined with anomalous ground state formation in van der Waals-coupled magnetic metal Fe$_5$GeTe$_2$
Creators: name: Yamagami, K.
name: Fujisawa, Y.
name: Pardo-Almanza, M.
name: Smith, B. R. M.
name: Sumida, K.
name: Takeda, Y.
name: Okada, Y.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Fe$_5$GeTe$_2$ is a van der Waals (vdW)-coupled unconventional ferromagnetic metal with a high Curie temperature ($T_C$) exceeding 300 K. The formation of an anomalous ground state significantly below $T_C$ has received considerable attention, resulting in increased interest in understanding the spin-polarized electronic state evolution near the Fermi energy ($E_F$) as a function of temperature. Despite recent extensive studies, a microscopic understanding of the spin-polarized electronic structure around $E_F$ has not yet been established owing to the intrinsic complexity of both the crystal and band structures. In this study, we investigate the temperature dependence of element-specific soft X-ray magnetic circular dichroism (XMCD). A systematic temperature evolution in the XMCD signal from both magnetic Fe and its ligand Te is clearly observed. More importantly, the enhancement in the hybridization between the Fe 3$d$ and Te 5$p$ states in the zero-magnetic field limit is revealed, and we discuss its implications on the possible emergence of an exotic magnetic ground state in Fe$_5$GeTe$_2$.
description: 12 pages, 4 figures
On the solidity parameter in canopy flows
Creators: name: Monti, Alessandro
name: Nicholas, Shane
name: Omidyeganeh, Mohammad
name: Pinelli, Alfredo
name: Rosti, Marco E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We have performed high-fidelity simulations of turbulent open-channel flows over submerged rigid canopies made of cylindrical filaments of fixed length $l=0.25H$ ($H$ being the domain depth) mounted on the wall with an angle of inclination $θ$. The inclination is the free parameter that sets the density of the canopy by varying its frontal area. The density of the canopy, based on the solidity parameter $λ$, is a widely accepted criterion defining the ongoing canopy flow regime, with low values ($λ\ll 0.1$) indicating the sparse regime, and higher values ($λ> 0.1$) the dense regime. All the numerical predictions have been obtained considering the same nominal bulk Reynolds number (i.e. $Re_b=U_b H/ν= 6000$). We consider nine configurations of canopies, with $θ$ varying symmetrically around $0°$ in the range $θ\in [\pm 78.5°]$, where positive angles define canopies inclined in the flow direction (with the grain) and $θ=0°$ corresponds to the wall-normally mounted canopy. The study compares canopies with identical solidity obtained inclining the filaments in opposite angles and assesses the efficacy of the solidity as a representative parameter. It is found that when the canopy is inclined, the actual flow regime differs substantially from the one of a straight canopy that shares the same solidity indicating that criteria solely based on this parameter are not robust. Finally, a new phenomenological model describing the interaction between the coherent structures populating the canopy region and the outer flow is given.
Breathing of dissipative light bullets of nonlinear polarization mode in Kerr resonators
Creators: name: Gopalakrishnan, S. S.
name: Tlidi, M.
name: Taki, M.
name: Panajotov, K.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We demonstrate the existence of breathing dissipative light bullets in a birefringent optical resonator filled with Kerr media. The propagation of light inside the cavity for each polarized component, which is coupled by cross-phase modulation, is described by the coupled Lugiato-Lefever equations. The space-time dynamics of breathing light bullets are described using Stokes parameters and frequency spectra.
description: 4
Simple, fast, and accurate method for detection of human mycotic keratitis.
Creators: name: El-Badry, Anwer
name: Mahmoud, Yehia
name: Abul-Souod, Soad
name: El-Shorbagy, M. Sameh
Publisher: name: Egyptian Society of Botany
Year: 2013

description: The current study mainly designed for rapid detection of mycotic keratitis in patients. Ordinary culturing of infection swap was time consuming. SCAR-PCR-based DNA amplification was conducted by using a highly specific primer pairing for detection of fungal chitin synthase gene conserved region, for all samples expected to be infected with fungi; specially by using the primer pairing probability (Forward primer: 5'- TAC AAG CTT ACT ATG TAT AAT GAG GAT -3'+ Reverse primer: 5'- TTA CTC GAG CTT ATA CTC AAA ATT TTG -3'). The obtained results confirmed that this method gave more accurate, time-saving, as positive visualization of fungal genome was achieved only after 1 day of work, while ordinary cultures consumed about 4 to 14 days to visualize the fungal growth.
An Energy Conserving Mechanism for Temporal Metasurfaces
Creators: name: Deshmukh, Kshiteej J.
name: Milton, Graeme W.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Classical Physics (physics.class-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Changing the microstructure properties of a space-time metamaterial while a wave is propagating through it, in general requires addition or removal of energy, which can be of exponential form depending on the type of modulation. This limits the realization and application of space-time metamaterials. We resolve this issue by introducing a novel mechanism of conserving energy at temporal metasurfaces in a non-linear setting. The idea is first demonstrated by considering a wave-packet propagating in a discrete medium of 1-d chain of springs and masses, where using our energy conserving mechanism we show that the spring stiffness can be incremented at several time interfaces and the energy will still be conserved. We then consider an interesting application of time-reversed imaging in 1-d and 2-d spring-mass systems with a wave packet traveling in the homogenized regime. Our numerical simulations show that, in 1-d, when the wave packet hits the time-interface two sets of waves are generated, one traveling forward in time and the other traveling backward. The time-reversed waves re-converge at the location of the source and we observe its regeneration. In 2-d, we use more complicated initial shapes and, even then, we observe regeneration of the original image or source. Thus, we achieve time-reversed imaging with conservation of energy in a non-linear system. The energy conserving mechanism can be easily extended to continuum media.
description: 6 pages, 4 figures
Discovery of optical and infrared accretion disc wind signatures in the black hole candidate MAXI J1348-630
Creators: name: Panizo-Espinar, G.
name: Padilla, M. Armas
name: Muñoz-Darias, T.
name: Koljonen, K. I. I.
name: Cúneo, V. A.
name: Sánchez-Sierras, J.
name: Sánchez, D. Mata
name: Casares, J.
name: Corral-Santana, J.
name: Fender, R. P.
name: Jiménez-Ibarra, F.
name: Ponti, G.
name: Steeghs, D.
name: Torres, M. A. P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: MAXI J1348-630 is a low mass X-ray binary discovered in 2019 during a bright outburst. During this event, the system sampled both hard and soft states following the standard evolution. We present multi-epoch optical and near-infrared spectroscopy obtained with X-shooter at the Very Large Telescope. Our dataset includes spectra taken during the brightest phases of the outburst as well as the decay towards quiescence. We study the evolution of the main emission lines, paying special attention to the presence of features commonly associated with accretion disc winds, such as blue-shifted absorptions, broad emission line wings and flat-top profiles. We find broad emission line wings in H-alpha during the hard-to-soft transition and blue-shifted absorption troughs at ~-500 km/s in H-beta, HeI-5876, H-alpha and Pa-beta during the bright soft-intermediate state. In addition, flat-top profiles are seen throughout the outburst. We interpret these observables as signatures of a cold (i.e. optical to infrared) accretion disc wind present in the system. We discuss the properties of the wind and compare them with those seen in other X-ray transients. In particular, the wind velocity that we observe is low when compared to those of other systems, which might be a direct consequence of the relatively low binary inclination, as suggested by several observables. This study strengthen the hypothesis that cold winds are a common feature in low mass X-ray binaries and that they can also be detected in low inclination objects via high-quality optical and infrared spectroscopy.
description: Accepted for publication in A&A
A general stability-driven approach for the refinement of multi-planet systems
Creators: name: Stalport, M.
name: Delisle, J. -B.
name: Udry, S.
name: Matthews, E. C.
name: Bourrier, V.
name: Leleu, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: Over the past years, the amount of detected multi-planet systems significantly grew, an important sub-class of which being the compact configurations. A precise knowledge of them is crucial to understand the conditions with which planetary systems form and evolve. However, observations often leave these systems with large uncertainties, notably on the orbital eccentricities. This is especially prominent for systems with low-mass planets detected with Radial Velocities (RV), the amount of which is more and more important in the exoplanet population. It is becoming a common approach to refine these parameters with the help of orbital stability arguments. Such dynamical techniques can be computationally expensive. In this work we use an alternative procedure faster by orders of magnitude than classical N-body integration approaches. We couple a reliable exploration of the parameter space with the precision of the Numerical Analysis of Fundamental Frequencies (NAFF, Laskar 1990) fast chaos indicator. We also propose a general procedure to calibrate the NAFF indicator on any multi-planet system without additional computational cost. This calibration strategy is illustrated on HD 45364, in addition to yet-unpublished measurements obtained with the HARPS and CORALIE high-resolution spectrographs. We validate the calibration approach on HD 202696. We test the performances of this stability-driven approach on two systems with different architectures. First we study HD 37124, a 3-planet system composed of planets in the Jovian regime. Then, we analyse HD 215152, a compact system of four low-mass planets. We demonstrate the potential of the NAFF stability-driven approach to refine the orbital parameters and planetary masses. We stress the importance of undertaking systematic global dynamical analyses on every new multi-planet system discovered.
description: 14 pages, 14 figures. Accepted for publication in A&A
MPEC 2025-A111 : 2024 YC26
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2025
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 YC26

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Gibbula Harzhauser, 2021, s.l.
Creators: name: Harzhauser, Mathias
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Archaeogastropoda
Trochidae
Gibbula

description: Gibbula s.l. gracilitesta (Papp, 1954) †
Middle Miocene (Sarmatian): Central Paratethys Sea (Austria).
(Papp 1954)
description: Published as part of Harzhauser, Mathias, 2021, The Cainozoic to present-day record of Circum-Mediterranean, NE Atlantic and North Sea Cantharidinae and Trochinae (Trochoidea, Gastropoda) - a synopsis, pp. 1-81 in Zootaxa 4902 (1) on page 36, DOI: 10.11646/zootaxa.4902.1.1, http://zenodo.org/record/4419088
Gibbula gradespira Risso 1826, s.l.
Creators: name: Harzhauser, Mathias
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Archaeogastropoda
Trochidae
Gibbula

description: Gibbula s.l. gradespira (Švagrovský, 1957) †
= Calliostoma gradespira misslense Švagrovský, 1957
Middle Miocene (Sarmatian): Central Paratethys Sea (Slovakia).
(Švagrovský 1971)
description: Published as part of Harzhauser, Mathias, 2021, The Cainozoic to present-day record of Circum-Mediterranean, NE Atlantic and North Sea Cantharidinae and Trochinae (Trochoidea, Gastropoda) - a synopsis, pp. 1-81 in Zootaxa 4902 (1) on page 36, DOI: 10.11646/zootaxa.4902.1.1, http://zenodo.org/record/4419088
Gibbula Harzhauser, 2021, s.l.
Creators: name: Harzhauser, Mathias
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Archaeogastropoda
Trochidae
Gibbula

description: Gibbula s.l. guttenbergi (Hilber, 1897) †
Middle Miocene (Sarmatian): Central Paratethys Sea (Austria, Slovakia).
(Švagrovský 1971)
description: Published as part of Harzhauser, Mathias, 2021, The Cainozoic to present-day record of Circum-Mediterranean, NE Atlantic and North Sea Cantharidinae and Trochinae (Trochoidea, Gastropoda) - a synopsis, pp. 1-81 in Zootaxa 4902 (1) on page 36, DOI: 10.11646/zootaxa.4902.1.1, http://zenodo.org/record/4419088
Tunneling Gravimetry
Creators: name: Schach, Patrik
name: Friedrich, Alexander
name: Williams, Jason R.
name: Schleich, Wolfgang P.
name: Giese, Enno
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We examine the prospects of utilizing matter-wave Fabry-Pérot interferometers for enhanced inertial sensing applications. Our study explores such tunneling-based sensors for the measurement of accelerations in two configurations: (a) a transmission setup, where the initial wave packet is transmitted through the cavity and (b) an out-tunneling scheme with intra-cavity generated initial states lacking a classical counterpart. We perform numerical simulations of the complete dynamics of the quantum wave packet, investigate the tunneling through a matter-wave cavity formed by realistic optical potentials and determine the impact of interactions between atoms. As a consequence we estimate the prospective sensitivities to inertial forces for both proposed configurations and show their feasibility for serving as inertial sensors.
description: 19 pages, 9 figures, 1 table
Gibbula Harzhauser, 2021, s.l.
Creators: name: Harzhauser, Mathias
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Archaeogastropoda
Trochidae
Gibbula

description: Gibbula s.l. joannea Hilber, 1897 †
Middle Miocene (Sarmatian): Central Paratethys Sea (Austria, Slovakia).
(Švagrovský 1971)
description: Published as part of Harzhauser, Mathias, 2021, The Cainozoic to present-day record of Circum-Mediterranean, NE Atlantic and North Sea Cantharidinae and Trochinae (Trochoidea, Gastropoda) - a synopsis, pp. 1-81 in Zootaxa 4902 (1) on page 36, DOI: 10.11646/zootaxa.4902.1.1, http://zenodo.org/record/4419088
NIR spectroscopic survey of protostellar jets in the star forming region IC 1396N
Creators: name: Massi, Fabrizio
name: López, Rosario
name: Beltrán, Maria T.
name: Estalella, Robert
name: Girart, Josep M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Abridged. The bright-rimmed cloud IC1396N hosts CO, H$_2$, and Herbig-Haro outflows powered by millimetre compact sources. We aim to characterise the kinematics and physical conditions of the H$_2$ emission features spread over IC1396N, which appear as chains of knots with a jet-like morphology, tracing different H$_2$ outflows, and to obtain further information about (and an identification of) the driving sources. Low-resolution, long-slit near-infrared spectra were acquired with NICS at the TNG, using grisms KB (R~1200), HK and JH (R~500). Several slit pointings and PA were used throughout IC1396N to sample a number of the H$_2$ knots previously detected in deep H$_2$ 2.12 $μ$m images. The knots exhibit rich ro-vibrational spectra of H$_2$, consistent with shock-excited excitation, from which radial velocities and relevant physical conditions of the IC1396N H$_2$ outflows were derived. These also allowed estimating extinction ranges towards several features. [FeII] emission was only detected towards a few knots, which also display unusually large H$_2$ 1-0 S(3)/S(1) flux ratios. The obtained radial velocities confirm that most of the outflows are close to the plane of the sky. Nearby knots in the same chain often display different radial velocities, both blue-shifted and red-shifted, which we interpret as due to ubiquitous jet precession in the driving sources or the development of oblique shocks. One of the chains (strand A) appears as a set of features trailing a leading bow-shock structure consistent with the results of 3-D magneto-hydrodynamical models. Either side of the leading bow-shock (A15) exhibits a different radial velocity, whose possible explanations are discussed in the paper. Our data cannot confirm whether strands A and B have both been originated by the intermediate mass young stellar object BIMA 2.
description: 13 pages, 7 figures, 3 tables in electronic form (only at CDS), accepted by Astronomy & Astrophysics
Gibbula kishineviae Harzhauser, 2021, s.l.
Creators: name: Harzhauser, Mathias
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Archaeogastropoda
Trochidae
Gibbula
Gibbula kishineviae

description: Gibbula s.l. kishineviae (d’Orbigny, 1844) †
= Trochus jeremejewi Sinzow, 1875
Middle-late Miocene (Bessarabian): Eastern Paratethys Sea (Bulgaria, Moldova, Ukraine, Russia). (Sladkovskaya 2017)
description: Published as part of Harzhauser, Mathias, 2021, The Cainozoic to present-day record of Circum-Mediterranean, NE Atlantic and North Sea Cantharidinae and Trochinae (Trochoidea, Gastropoda) - a synopsis, pp. 1-81 in Zootaxa 4902 (1) on page 36, DOI: 10.11646/zootaxa.4902.1.1, http://zenodo.org/record/4419088
Emergence of an island of extreme nuclear isomerism at high excitation near $^{208}$Pb
Creators: name: Wahid, S. G.
name: Tandel, S. K.
name: Suman, Saket
name: Srivastava, P. C.
name: Kumar, Anil
name: Chowdhury, P.
name: Kondev, F. G.
name: Janssens, R. V. F.
name: Carpenter, M. P.
name: Lauritsen, T.
name: Seweryniak, D.
name: Zhu, S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Metastable states with T$_{1/2}$ = 8(2) ms in $^{205}$Bi and T$_{1/2}$ = 0.22(2) ms in $^{204}$Pb, with $\approx $ 8 MeV excitation energy and angular momentum $\ge $ 22 $\hbar $, have been established. These represent, by up to two orders of magnitude, the longest-lived nuclear states above an excitation energy of 7 MeV, ever identified in the nuclear chart. Additionally, the half-life of the 10.17 MeV state in $^{206}$Bi has been determined to be 0.027(2) ms, the next highest value in this highly excited regime. These observations indicate the emergence of an island of extreme nuclear isomerism arising from core-excited configurations at high excitation in the vicinity of the doubly closed-shell nucleus $^{208}$Pb. These results are expected to provide discriminating tests of the effective interactions used in current large-scale shell-model calculations.
description: 17 pages, 5 figures