cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A classification of near-horizon geometries of extremal vacuum black holes
Creators: name: Kunduri, Hari K.
name: Lucietti, James
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider the near-horizon geometries of extremal, rotating black hole solutions of the vacuum Einstein equations, including a negative cosmological constant, in four and five dimensions. We assume the existence of one rotational symmetry in 4d, two commuting rotational symmetries in 5d and in both cases non-toroidal horizon topology. In 4d we determine the most general near-horizon geometry of such a black hole, and prove it is the same as the near-horizon limit of the extremal Kerr-AdS(4) black hole. In 5d, without a cosmological constant, we determine all possible near-horizon geometries of such black holes. We prove that the only possibilities are one family with a topologically S^1 X S^2 horizon and two distinct families with topologically S^3 horizons. The S^1 X S^2 family contains the near-horizon limit of the boosted extremal Kerr string and the extremal vacuum black ring. The first topologically spherical case is identical to the near-horizon limit of two different black hole solutions: the extremal Myers-Perry black hole and the slowly rotating extremal Kaluza-Klein (KK) black hole. The second topologically spherical case contains the near-horizon limit of the fast rotating extremal KK black hole. Finally, in 5d with a negative cosmological constant, we reduce the problem to solving a sixth-order non-linear ODE of one function. This allows us to recover the near-horizon limit of the known, topologically S^3, extremal rotating AdS(5) black hole. Further, we construct an approximate solution corresponding to the near-horizon geometry of a small, extremal AdS(5) black ring.
description: 45 pages, latex. v2: minor clarifications in section 3. v3: assumption of non-toroidal horizon topology made explicit, improved section 3, references added
CarveMix: A Simple Data Augmentation Method for Brain Lesion Segmentation
Creators: name: Zhang, Xinru
name: Liu, Chenghao
name: Ou, Ni
name: Zeng, Xiangzhu
name: Xiong, Xiaoliang
name: Yu, Yizhou
name: Liu, Zhiwen
name: Ye, Chuyang
Publisher: name: arXiv
Year: 2021
Subjects: subject: Image and Video Processing (eess.IV)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: Brain lesion segmentation provides a valuable tool for clinical diagnosis, and convolutional neural networks (CNNs) have achieved unprecedented success in the task. Data augmentation is a widely used strategy that improves the training of CNNs, and the design of the augmentation method for brain lesion segmentation is still an open problem. In this work, we propose a simple data augmentation approach, dubbed as CarveMix, for CNN-based brain lesion segmentation. Like other "mix"-based methods, such as Mixup and CutMix, CarveMix stochastically combines two existing labeled images to generate new labeled samples. Yet, unlike these augmentation strategies based on image combination, CarveMix is lesion-aware, where the combination is performed with an attention on the lesions and a proper annotation is created for the generated image. Specifically, from one labeled image we carve a region of interest (ROI) according to the lesion location and geometry, and the size of the ROI is sampled from a probability distribution. The carved ROI then replaces the corresponding voxels in a second labeled image, and the annotation of the second image is replaced accordingly as well. In this way, we generate new labeled images for network training and the lesion information is preserved. To evaluate the proposed method, experiments were performed on two brain lesion datasets. The results show that our method improves the segmentation accuracy compared with other simple data augmentation approaches.
description: accepted by MICCAI 2021
Kozai cycles, tidal friction and the dynamical evolution of binary minor planets
Creators: name: Perets, Hagai B.
name: Naoz, Smadar
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In recent years many binary minor planets (BMPs) have been discovered in the Solar system. Many models have been suggested for their formation, but these encounter difficulties explaining their observed characteristics. Here we show that secular perturbations by the Sun (Kozai mechanism) fundamentally change the evolution and the initial distribution of BMPs predicted by such models and lead to unique observational signatures. The Kozai mechanism can lead to a large periodic oscillations in the eccentricity and inclination of highly inclined BMP orbits, where we predict such effects to be observable with current accuracy within a few years (e.g. for the binary asteroid Huenna). In addition, the combined effects of the Kozai mechanism and tidal friction (KCTF) drives BMPs into short period circular orbits. We predict a specific inclination dependent distribution of the separation and eccentricity of BMPs, due to these effects, including a zone of avoidance at the highest inclinations. Specifically the Kozai evolution could explain the recently observed peculiar orbit of the Kuiper belt binary 2001 QW322 . Additionally, the KCTF process could lead to BMPs coalescence and serve as an important route for the formation of irregular shaped single minor planets with large axial tilts.
description: 5 pages, 2 figures. Appendix removed (to appear in another paper), added and corrected observational data. Results strengthened. Submitted to ApJL
Additional file 4 of Intrathecal interleukin-6 levels are associated with progressive disease and clinical severity in multiple sclerosis
Creators: name: Itorralba, Justine
name: Brand-Arzamendi, Koroboshka
name: Saab, Georges
name: Muccilli, Alexandra
name: Schneider, Raphael
Publisher: name: figshare
Year: 2025
Subjects: subject: Biochemistry
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Neuroscience
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Supplementary Material 4
title: Frontmatter, Table of Contents, Preface, Workshop Organization
Creators: name: Chiba, Yuki
name: Escobar, Santiago
name: Nishida, Naoki
name: Sabel, David
name: Schmidt-Schauß, Manfred
Publisher: name: Schloss Dagstuhl – Leibniz-Zentrum für Informatik
Year: 2015
Subjects: subject: Frontmatter
subject: Table of Contents
subject: Preface
subject: Workshop Organization

description: Frontmatter, Table of Contents, Preface, Workshop Organization
description: OASIcs, Vol. 46, 2nd International Workshop on Rewriting Techniques for Program Transformations and Evaluation (WPTE 2015), pages i-xvi
Additional file 1 of Fall sensors, home emergency system, and social service for ≥ 75-year-olds living at home - a matched control intervention study
Creators: name: Zoellick, Jan C.
name: Lech, Sonia
name: O’Sullivan, Julie L.
name: Jansen, Eva
name: Supplieth, Juliana
name: Kuhnert, Ronny
name: Grittner, Ulrike
name: Schuster, Johanna
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Supplementary Material 1
Explicit Baker-Campbell-Hausdorff-Dynkin formula for Spacetime via Geometric Algebra
Creators: name: Wilson, Joseph
name: Visser, Matt
Publisher: name: arXiv
Year: 2021
Subjects: subject: Mathematical Physics (math-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present a compact Baker-Campbell-Hausdorff-Dynkin formula for the composition of Lorentz transformations $e^{σ_i}$ in the spin representation (a.k.a. Lorentz rotors) in terms of their generators $σ_i$: $$ \ln(e^{σ_1}e^{σ_2}) = \tanh^{-1}\left(\frac{ \tanh σ_1 + \tanh σ_2 + \frac12[\tanh σ_1, \tanh σ_2] }{ 1 + \frac12\{\tanh σ_1, \tanh σ_2\} }\right) $$ This formula is general to geometric algebras (a.k.a. real Clifford algebras) of dimension $\leq 4$, naturally generalising Rodrigues' formula for rotations in $\mathbb{R}^3$. In particular, it applies to Lorentz rotors within the framework of Hestenes' spacetime algebra, and provides an efficient method for composing Lorentz generators. Computer implementations are possible with a complex $2\times2$ matrix representation realised by the Pauli spin matrices. The formula is applied to the composition of relativistic $3$-velocities yielding simple expressions for the resulting boost and the concomitant Wigner angle.
description: 21 pages, no figures
Additional file 2 of Fall sensors, home emergency system, and social service for ≥ 75-year-olds living at home - a matched control intervention study
Creators: name: Zoellick, Jan C.
name: Lech, Sonia
name: O’Sullivan, Julie L.
name: Jansen, Eva
name: Supplieth, Juliana
name: Kuhnert, Ronny
name: Grittner, Ulrike
name: Schuster, Johanna
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Supplementary Material 2
Miller House, Apaquogue Road
Creators: name: Weber, Harvey A.
Publisher: name: Unknown
Year: 1970
Subjects: Photographs
Photos
Historic buildings
East Hampton
Structures
Dwellings
Miller Family

description: These images show the Miller-Poor House and the detail on the Metal gate on the property. This image was taken by photographer Harvey A. Weber (1917-1991) and is part of the East Hampton’s Heritage Photo Collection.
description: Images within East Hampton Heritage Photo Collection seem to have been taken or collected in relation to the East Hampton Heritage project, but not all of them were included in the final publication. Several photographer are included in this collection.
Vibrational spectroscopy of H2+: precise evaluation of the Zeeman effect
Creators: name: Karr, Jean-Philippe
name: Korobov, Vladimir
name: Hilico, Laurent
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present an accurate computation of the g-factors of the hyperfine states of the hydrogen molecular ion H2+. The results are in good agreement with previous experiments, and can be tested further by rf spectroscopy. Their implication for high-precision two-photon vibrational spectroscopy of H2+ is also discussed. It is found that the most intense hyperfine components of two-photon lines benefit from a very small Zeeman splitting.
A Comprehensive Study on Torchvision Pre-trained Models for Fine-grained Inter-species Classification
Creators: name: Albardi, Feras
name: Kabir, H M Dipu
name: Bhuiyan, Md Mahbub Islam
name: Kebria, Parham M.
name: Khosravi, Abbas
name: Nahavandi, Saeid
Publisher: name: arXiv
Year: 2021
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: This study aims to explore different pre-trained models offered in the Torchvision package which is available in the PyTorch library. And investigate their effectiveness on fine-grained images classification. Transfer Learning is an effective method of achieving extremely good performance with insufficient training data. In many real-world situations, people cannot collect sufficient data required to train a deep neural network model efficiently. Transfer Learning models are pre-trained on a large data set, and can bring a good performance on smaller datasets with significantly lower training time. Torchvision package offers us many models to apply the Transfer Learning on smaller datasets. Therefore, researchers may need a guideline for the selection of a good model. We investigate Torchvision pre-trained models on four different data sets: 10 Monkey Species, 225 Bird Species, Fruits 360, and Oxford 102 Flowers. These data sets have images of different resolutions, class numbers, and different achievable accuracies. We also apply their usual fully-connected layer and the Spinal fully-connected layer to investigate the effectiveness of SpinalNet. The Spinal fully-connected layer brings better performance in most situations. We apply the same augmentation for different models for the same data set for a fair comparison. This paper may help future Computer Vision researchers in choosing a proper Transfer Learning model.
description: Accepted
Additional file 1 of Refractory autoimmune cytopenia in children, possible role for sirolimus treatment
Creators: name: Elhady, Marwa Abd
name: Fadeel, Samar Hasan Abd El
name: Galal, Nermeen M.
name: Meshaal, Safa
name: Mohammed, Eman Abdel-Raouf
Publisher: name: figshare
Year: 2025
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 1: Tables S1–S4
Strong magnetic fields: neutron stars with an extended inner crust
Creators: name: Pais, Helena
name: Bertolino, Bruno
name: Fang, Jianjun
name: Wang, Xiaopeng
name: Providência, Constança
Publisher: name: arXiv
Year: 2021
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Using relativistic mean-field models, the formation of clusterized matter, as the one expected to exist in the inner crust of neutron stars, is determined under the effect of strong magnetic fields. As already predicted from a calculation of the unstable modes resulting from density fluctuations at subsaturation densities, we confirm in the present work that for magnetic field intensities of the order of $\approx 5 \times 10^{16}$ G to $5 \times 10^{17}$ G, pasta phases may occur for densities well above the zero-field crust-core transition density. This confirms that the extension of the crust may be larger than expected. It is also verified that the equilibrium structure of the clusterized matter is very sensitive to the intensity of the magnetic fields. As a result, the decay of the magnetic field may give rise to internal stresses which may result on the yield and fracture of the inner crust lattice.
description: 9 pages, 4 figures, accepted for publication in the EPJ A Topical Issue "The QCD Phase Diagram in Strong Magnetic Fields"
Temperature microstructure in Howe Sound
Creators: name: Bilodeau, Laurent Ernest
Publisher: name: University of British Columbia
Year: 2010

description: Temperature microstructure observations obtained in Howe Sound are presented and related to their oceanographic context, In some instances, two free-falling probes have been launched simultaneously with separations of 10 to 20 m at the surface in an attempt to look at the lateral extent of temperature microstructure features. Patches of temperature gradient variance were found where the gradient presented peak values of both signs at smaller scales. These patches were usually observed by one probe only and seem to extend laterally over less than 20 m. In other instances the peak gradient values took mostly the same sign within a given patch. Such patches were usually detected by both probes, indicating that their horizontal extent is significantly larger than 20 m. These types of temperature microstructure are also discussed in terms of mechanisms that could provide an explanation for their existence. In Howe Sound's Inner Basin, the Deep Water occasionally receives large influxes of water from the Strait of Georgia. Otherwise, it stays essentially trapped behind a 75 m deep sill and becomes more homogeneous with time. A model is presented which relates the rate at which temperature becomes homogeneous to temperature gradient variance and the molecular coefficient of heat diffusion. Other parts of the water column are discussed in terms of the Osborn-Cox (1972) model of vertical heat transport.
Electroweak scale seesaw and heavy Dirac neutrino signals at LHC
Creators: name: del Aguila, F.
name: Aguilar-Saavedra, J. A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Models of type I seesaw can be implemented at the electroweak scale in a natural way provided that the heavy neutrino singlets are quasi-Dirac particles. In such case, their contribution to light neutrino masses has the suppression of a small lepton number violating parameter, so that light neutrino masses can arise naturally even if the seesaw scale is low and the heavy neutrino mixing is large. We implement the same mechanism with fermionic triplets in type III seesaw, deriving the interactions of the new quasi-Dirac neutrinos and heavy charged leptons with the SM fermions. We then study the observability of heavy Dirac neutrino singlets (seesaw I) and triplets (seesaw III) at LHC. Contrarily to common wisdom, we find that heavy Dirac neutrino singlets with a mass around 100 GeV are observable at the 5 sigma level with a luminosity of 13 fb^-1. Indeed, in the final state with three charged leptons l+- l+- l-+, not previously considered, Dirac neutrino signals can be relatively large and backgrounds are small. In the triplet case, heavy neutrinos can be discovered with a luminosity of 1.5 fb^-1 for a mass of 300 GeV in the same channel.
description: LaTeX 19 pages, 22 PS figures. Enlarged discussion and added a reference. Final version to appear in PLB
Additional file 1 of Novel spectrophotometric methods for concurrent assessment of duloxetine and avanafil in their binary mixture using derivative spectroscopy: greenness-blueness evaluation
Creators: name: Elhamdy, Hadeer A.
name: Derayea, Sayed M.
name: El-Din, Khalid M. Badr
name: Oraby, Mohamed
Publisher: name: figshare
Year: 2025
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
Additional file 1 of The Chinese version of the autonomy preference index for advanced cancer patients: a study on cultural adaptation based on cognitive interview
Creators: name: Yan, Chao
name: Li, Yonghong
name: Ai, Ji
name: Yang, Shenghuan
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Supplementary Material 1
Nathaniel Huntting House, Details on Post
Creators: name: Weber, Harvey A.
Publisher: name: Unknown
Year: 1970
Subjects: Photographs
Photos
Historic buildings
East Hampton
Structures
Dwellings
Miller Family
Huntting, Nathaniel, 1675-1753
Wood carving
Woodwork

description: This image shows the detail work on a wooden post in the Nathaniel Huntting House, located at 94 Main Street. This image was taken by photographer Harvey A. Weber (1917-1991) and is part of the East Hampton’s Heritage Photo Collection.
description: Images within East Hampton Heritage Photo Collection seem to have been taken or collected in relation to the East Hampton Heritage project, but not all of them were included in the final publication. Several photographer are included in this collection.
title: Frontmatter, Table of Contents, Preface, Workshop Organization
Creators: name: Schmidt-Schauß, Manfred
name: Sakai, Masahiko
name: Sabel, David
name: Chiba, Yuki
Publisher: name: Schloss Dagstuhl – Leibniz-Zentrum für Informatik
Year: 2014
Subjects: subject: Frontmatter
subject: Table of Contents
subject: Preface
subject: Workshop Organization

description: Frontmatter, Table of Contents, Preface, Workshop Organization
description: OASIcs, Vol. 40, First International Workshop on Rewriting Techniques for Program Transformations and Evaluation, pages i-xv
Additional file 1 of Barriers, facilitators, needs, and preferences in seeking information regarding cervical cancer prevention programs among Turkish, Moroccan, and Syrian immigrant women: a scoping review
Creators: name: Veeravagu, Tharsini
name: Hamdiui, Nora
name: Stein, Mart L.
name: Crutzen, Rik
name: Timen, Aura
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
Alcune notti nel Wollo tra gli adepti di culti di possessione
Creators: name: Budriesi, Laura
Publisher: name: Dipartimento delle Arti - Alma Mater Studiorum - Università di Bologna
Year: 2014

description: Abstract – IT
I culti di possessione in Etiopia, legati alle credenze tradizionali e praticati in confraternite di fedeli che si appoggiano alla religione cristiano-ortodossa e all’islam sono esperienze multiformi, antiche e ben radicate in tutto il paese ma di difficile accesso agli studiosi occidentali per via del loro carattere esoterico, dovuto anche alla condanna del clero ortodosso e al rapporto ambiguo col potere statale. L’autrice si rifà alla sua esperienza sul campo condotta tra il 2008 e il 2009, compiuta in alcuni villaggi del Wollo, negli altopiani del nord. Il saggio cerca di restituire sensazioni ed emozioni provate a caldo nelle notti trascorse ad assistere alle cerimonie di possessione (hadra) presso l’abitazione del guaritore noto come Alì, fondendole con la riflessione avviata a partire dalla traduzione successiva dei materiali. Alcuni frammenti di dialoghi tra il bale-zar e i suoi adepti/pazienti sono riportati e inseriti nella cornice della struttura performativa delle cerimonie per delineare le voci e i ruoli degli attori coinvolti, umani e non.

Abstract – EN
The possession cults in Ethiopia, linked to traditional beliefs and practiced in brotherhoods of believers who lean to the Christian Orthodox religion and Islam are multifaceted experiences, both ancient and well-established throughout the country but are difficult to access by Western scholars due to their esoteric character, the disapproval of the Orthodox clergy and the ambiguous relationship with the state power. The author draws on her experience in the field conducted between 2008 and 2009, carried out in some villages of Wollo, in the northern highlands. The essay manages to convey feelings and emotions experienced in person while attending the ceremonies of possession (hadra) at the home of the healer known as Ali, together with the later study of the recording of the event. Some fragments of the dialogues between the bale-zar and his followers / patients are reported and included in the text, to outline the roles and voices of the actors involved – human or otherwise – in the performative structure of the ceremonies.
description: Antropologia e Teatro. Rivista di Studi, No 5 (2014)
Information Security Analysis in the Passenger-Autonomous Vehicle Interaction
Creators: name: Bakhtina, Mariia
name: Matulevičius, Raimundas
Publisher: name: arXiv
Year: 2021
Subjects: subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: Autonomous vehicles (AV) are becoming a part of humans' everyday life. There are numerous pilot projects of driverless public buses; some car manufacturers deliver their premium-level automobiles with advanced self-driving features. Thus, assuring the security of a Passenger-Autonomous Vehicle interaction arises as an important research topic, as along with opportunities, new cybersecurity risks and challenges occur that potentially may threaten Passenger's privacy and safety on the roads. This study proposes an approach of the security requirements elicitation based on the developed threat model. Thus, information security risk management helps to fulfil one of the principles needed to protect data privacy - information security. We demonstrate the process of security requirements elicitation to mitigate arising security risks. The findings of the paper are case-oriented and are based on the literature review. They are applicable for AV system implementation used by ride-hailing service providers that enable supervisory AV control.
The Galactic potential and the asymmetric distribution of hypervelocity stars
Creators: name: Perets, Hagai B.
name: Wu, Xufen
name: Zhao, HongSheng
name: Famaey, Benoit
name: Gentile, Gianfranco
name: Alexander, Tal
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In recent years several hypervelocity stars (HVSs) have been observed in the halo of our Galaxy. Such HVSs have possibly been ejected from the Galactic center and then propagated in the Galactic potential up to their current position. The recent survey for candidate HVSs show an asymmetry in the kinematics of candidate HVSs (position and velocity vectors), where more outgoing stars than ingoing stars (i.e. positive Galactocentric velocities vs. negative ones) are observed. We show that such kinematic asymmetry, which is likely due to the finite lifetime of the stars and Galactic potential structure, could be used in a novel method to probe and constrain the Galactic potential, identify the stellar type of the stars in the survey and estimate the number of HVSs. Kinematics-independent identification of the stellar types of the stars in such surveys (e.g. spectroscopic identification) could further improve these results. We find that the observed asymmetry between ingoing and outgoing stars favors specific Galactic potential models. It also implies a lower limit of ~54+-8 main sequence HVSs in the survey sample (>=648+-96 in the Galaxy), assuming that all of the main sequence stars in the survey originate from the Galactic center. The other stars in the survey are likely to be hot blue horizontal branch stars born in the halo rather than stars ejected from the Galactic center.
description: 7 pages, 3 figures. Added an appendix. Accepted to ApJ
Additional file 2 of Barriers, facilitators, needs, and preferences in seeking information regarding cervical cancer prevention programs among Turkish, Moroccan, and Syrian immigrant women: a scoping review
Creators: name: Veeravagu, Tharsini
name: Hamdiui, Nora
name: Stein, Mart L.
name: Crutzen, Rik
name: Timen, Aura
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 2
The Lagrangian-averaged model for magnetohydrodynamics turbulence and the absence of bottleneck
Creators: name: Graham, Jonathan Pietarila
name: Mininni, Pablo D.
name: Pouquet, Annick
Publisher: name: arXiv
Year: 2008
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Astrophysics (astro-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We demonstrate that, for the case of quasi-equipartition between the velocity and the magnetic field, the Lagrangian-averaged magnetohydrodynamics alpha-model (LAMHD) reproduces well both the large-scale and small-scale properties of turbulent flows; in particular, it displays no increased (super-filter) bottleneck effect with its ensuing enhanced energy spectrum at the onset of the sub-filter-scales. This is in contrast to the case of the neutral fluid in which the Lagrangian-averaged Navier-Stokes alpha-model is somewhat limited in its applications because of the formation of spatial regions with no internal degrees of freedom and subsequent contamination of super-filter-scale spectral properties. No such regions are found in LAMHD, making this method capable of large reductions in required numerical degrees of freedom; specifically, we find a reduction factor of 200 when compared to a direct numerical simulation on a large grid of 1536^3 points at the same Reynolds number.
description: 22 pages, 9 figures; accepted Phys.Rev.E
Mapping the Dark Side with DEIMOS: Globular Clusters, X-ray Gas, and Dark Matter in the NGC 1407 Group
Creators: name: Romanowsky, Aaron J.
name: Strader, Jay
name: Spitler, Lee R.
name: Johnson, Ria
name: Brodie, Jean P.
name: Forbes, Duncan A.
name: Ponman, Trevor
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: NGC 1407 is the central elliptical in a nearby evolved galaxy group apparently destined to become a cluster core. We use the kinematics of globular clusters to probe the dynamics and mass profile of the group's center, out to 60 kpc (~10 R_eff) -- the most extended data set to date around an early-type galaxy. This sample consists of 172 GC velocities, most of them newly obtained using Keck/DEIMOS, with a few additional objects identified as DGTOs or as IGCs. We find weak rotation in the GC system's outer parts, with the metal-poor and metal-rich GCs misaligned. The RMS velocity profile declines rapidly to a radius of ~20 kpc, and then becomes flat or rising to ~60 kpc. There is evidence that the GC orbits have a tangential bias that is strongest for the metal-poor GCs -- possibly contradicting theoretical expectations. We construct cosmologically-motivated galaxy+dark halo dynamical models and infer a mass within 60 kpc of ~3x10^12 M_Sun, extrapolating to a virial mass of ~6x10^13 M_Sun for a typical LCDM halo -- in agreement with results from group galaxy kinematics. We present an independent Chandra-based analysis, whose relatively high mass at ~20 kpc disagrees strongly with the GC-based result unless the GCs are assumed to have a peculiar orbit distribution, and we discuss some general comparisons between X-ray and optical results. The group's B-band mass-to-light ratio of ~800 is extreme even for a rich galaxy cluster, much less a poor group -- placing it among the most dark matter dominated systems in the universe, and also suggesting a massive reservoir of baryons lurking in an unseen phase, in addition to the nonbaryonic dark matter. We compare the kinematical and mass properties of the NGC 1407 group to other nearby groups and clusters, and discuss some implications of this system for structure formation.
description: 34 pages, 27 figures, accepted by The Astronomical Journal. Minor revisions, and significant improvements to kinematics analysis of Sec. 5.1. PDF version with optimized formatting at http://www.ucolick.org/~romanow/res.html
Resonance Recombination Model and Quark Distribution Functions in the Quark-Gluon Plasma
Creators: name: Ravagli, L.
name: van Hees, H.
name: Rapp, R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We investigate the consequences of space-momentum correlations in quark phase-space distributions for coalescence processes at the hadronization transition. Thus far it has been proved difficult to reconcile such correlations with the empirically observed constituent quark number scaling (CQNS) at the Relativistic Heavy-Ion Collider (RHIC). To address this problem we combine our earlier developed quark recombination model with quark phase-space distributions computed from relativistic Langevin simulations in an expanding Quark-Gluon Plasma (QGP). Hadronization is based on resonance formation within a Boltzmann equation which recovers thermal equilibrium and obeys energy conservation in the quark-coalescence process, while the fireball background is adjusted to hydrodynamic simulations of semi-central Au-Au collisions at RHIC. To facilitate the applicability of the Langevin process, we focus on strange and charm quarks. Their interactions in the QGP are modeled using leading-order perturbative QCD augmented by effective Lagrangians with resonances which smoothly merge into hadronic states formed at T_c. The interaction strength is adjusted to reproduce the empirical saturation value for the quark-elliptic flow, v_{2,q}^{sat}~7-8%. The resulting phi and J/ψelliptic flow recover CQNS over a large range in transverse momentum (p_T) within a few percent. As a function of transverse kinetic energy, both the quark spectra from the Langevin simulations and the meson spectra generated via resonance recombination recover CQNS from zero to at least 3 GeV.
description: 10 pages, 6 figures; v2: modified title, light-quark results taken out, version accepted for publication in PRC
Atmospheric circulation of hot Jupiters: Coupled radiative-dynamical general circulation model simulations of HD 189733b and HD 209458b
Creators: name: Showman, Adam P.
name: Fortney, Jonathan J.
name: Lian, Yuan
name: Marley, Mark S.
name: Freedman, Richard S.
name: Knutson, Heather A.
name: Charbonneau, David
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present global, three-dimensional numerical simulations of HD 189733b and HD 209458b that couple the atmospheric dynamics to a realistic representation of non-gray cloud-free radiative transfer. The model, which we call the Substellar and Planetary Atmospheric Radiation and Circulation (SPARC) model, adopts the MITgcm for the dynamics and uses the radiative model of McKay, Marley, Fortney, and collaborators for the radiation. Like earlier work with simplified forcing, our simulations develop a broad eastward equatorial jet, mean westward flow at higher latitudes, and substantial flow over the poles at low pressure. For HD 189733b, our simulations without TiO and VO opacity can explain the broad features of the observed 8 and 24-micron light curves, including the modest day-night flux variation and the fact that the planet/star flux ratio peaks before the secondary eclipse. Our simulations also provide reasonable matches to the Spitzer secondary-eclipse depths at 4.5, 5.8, 8, 16, and 24 microns and the groundbased upper limit at 2.2 microns. However, we substantially underpredict the 3.6-micron secondary-eclipse depth, suggesting that our simulations are too cold in the 0.1-1 bar region. Predicted temporal variability in secondary-eclipse depths is ~1% at Spitzer bandpasses, consistent with recent observational upper limits at 8 microns. We also show that nonsynchronous rotation can significantly alter the jet structure. For HD 209458b, we include TiO and VO opacity; these simulations develop a hot (>2000 K) dayside stratosphere. Despite this stratosphere, we do not reproduce current Spitzer photometry of this planet. Light curves in Spitzer bandpasses show modest phase variation and satisfy the observational upper limit on day-night phase variation at 8 microns. (abridged)
description: 20 pages (emulate-apj format), 21 figures, final version now published in ApJ. Includes expanded discussion of radiative-transfer methods and two new figures
Additional file 3 of o8G-modified circKIAA1797 promotes lung cancer development by inhibiting cuproptosis
Creators: name: Xu, Haotian
name: Zhao, Qingyun
name: Cai, Dunyu
name: Chen, Xingcai
name: Zhou, Xiaodong
name: Gao, Yihong
name: Wu, Jiaxi
name: Yuan, Shengyi
name: Li, Deqing
name: Zhang, Ruirui
name: Peng, Wenyi
name: Li, Gang
name: Nan, Aruo
Publisher: name: figshare
Year: 2025
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 3
Silver-enhanced lateral flow immunoassay for highly-sensitive detection of potato leafroll virus
Creators: name: Panferov, Vasily G.
name: Safenkova, Irina V.
name: Byzova, Nadezhda A.
name: Varitsev, Yuri A.
name: Zherdev, Anatoly V.
name: Dzantiev, Boris B.
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Rapid non-laboratory screening of plants for pathogenic viruses crucially influences crop yields in modern agricultural technologies. The aim of this study was to develop a highly-sensitive lateral flow immunoassay (LFIA) for rapid detection of potato leafroll virus (PLRV), an infectious agent of one of the most widespread potato diseases. The proposed LFIA combines the formation of sandwich immune complexes with gold nanoparticles (GNP) as labels and silver enhancement. The enhancement stage was realized using mixture of silver lactate and hydroquinone and subsequent addition of chloride-containing buffer to stop silver reduction. LFIA with silver enhancement was 15 times more sensitive (detection limit 0.2 ng/mL; 15 min) compared with conventional LFIA (detection limit 3 ng/mL; 10 min). The enhanced LFIA detected PLRV in leaves’ extracts of infected potato in dilutions higher than enzyme-linked immunosorbent assay.
title: Front Matter, Table of Contents, Preface, Organization
Creators: name: Italiano, Giuseppe F.
name: Schmidt, Marie
Publisher: name: Schloss Dagstuhl – Leibniz-Zentrum für Informatik
Year: 2015
Subjects: subject: Front Matter
subject: Table of Contents
subject: Preface
subject: Organization

description: Front Matter, Table of Contents, Preface, Organization
description: OASIcs, Vol. 48, 15th Workshop on Algorithmic Approaches for Transportation Modelling, Optimization, and Systems (ATMOS 2015), pages i-x
Comprehensive diagnostic synthesis on Open Access and Open Data in Angola
Creators: name: United Nations Educational, Scientific and Cultural Organization
name: Ministério Do Ensino Superior, Ciência
name: Redalyc-Universidad Autónoma Del Estado De México
name: AmeliCA
name: Universidade Óscar Ribas
Publisher: name: Zenodo
Year: 2022
Subjects: Open Access
Angola
Africa
Open Data
publishing policies
internationalization

description: Work derived from the collaborative project among Redalyc UAEM, AmeliCA, MESCTI and U. Óscar Ribas funded by UNESCO for the development of an Open Access strategy in Angola. Vol. 10 of 38
Quantum Error Correction and Holographic Information from Bilocal Holography
Creators: name: Koch, Robert de Mello
name: Gandote, Eunice
name: Tahiridimbisoa, Nirina Hasina
name: Van Zyl, Hendrik J. R.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Bilocal holography is a constructive approach to the higher spin theory holographically dual to $O(N)$ vector models. In contrast to other approaches to bulk reconstruction, bilocal holography does not take input from the dual gravitational theory. The resulting map is a complete bulk/boundary mapping in that it maps the complete set of $O(N)$ invariant degrees of freedom in the CFT, to the complete set of higher spin degrees of freedom. After restricting to a suitable code subspace we demonstrate that bilocal holography naturally reproduces the quantum error correcting properties of holography and it gives a robust bulk (entanglement wedge) reconstruction. A gauge invariant entangled pair of CFT degrees of freedom are naturally smeared over a semicircle in the bulk spacetime, which is highly suggestive of bit threads. Finally, we argue that finite $N$ relations in the CFT, when interpreted in the dual AdS spacetime, can provide relations between degrees of freedom located near the boundary and degrees of freedom deep in the bulk.
description: 31 pages, 6 figures
A novel variable antibody fragment dimerized by the dHLX peptide with enhanced affinity against amantadine compared to its corresponding scFv antibody
Creators: name: Xie, Sanlei
name: Wen, Kai
name: Peng, Tao
name: Wang, Jianyi
name: Yao, Kai
name: Jiang, Haiyang
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Amantadine (AMA) is an illegally used antiviral drug in the poultry industry, it is necessary to establish a fast, accurate and time-saving detection method for poultry food. The antibody-based immunoassay can achieve fast and accurate requirements. We developed a recombinant antibody-based specificity immunoassay for AMA. In the recombinant antibody, the heavy chain variable region (VH) is connected covalently with the light chain variable region (VL) by the artificial linker. Here, two recombinant antibodies’ single-chain variable fragment (scFv) and scFv-dHLX were constructed and functionally expressed in the periplasm of Escherichia coli. The helix-turn-helix peptide was utilized to dimerize VH and VL similar to the IgG counterpart. The ScFv-dHLX protein showed a higher binding ability and affinity resulting in improvement of in vitro affinity activity over its corresponding scFv. Our results not only indicated scFv-dHLX as an alternative for scFv in analytical application, but also offered a novel and efficient hetero-dimerization pattern of VH and VL leading to enhanced affinity.
Additional file 4 of o8G-modified circKIAA1797 promotes lung cancer development by inhibiting cuproptosis
Creators: name: Xu, Haotian
name: Zhao, Qingyun
name: Cai, Dunyu
name: Chen, Xingcai
name: Zhou, Xiaodong
name: Gao, Yihong
name: Wu, Jiaxi
name: Yuan, Shengyi
name: Li, Deqing
name: Zhang, Ruirui
name: Peng, Wenyi
name: Li, Gang
name: Nan, Aruo
Publisher: name: figshare
Year: 2025
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 4
Building on a Vision: An Analysis of 103 Years of Ideological and Material Development of the University Avenue Church of Christ
Creators: name: Young, Natalie
Publisher: name: The University of Texas at Austin
Year: 2020
Subjects: University Avenue Church of Christ
Church of Christ
Religion
University of Texas
Religious Studies

description: I take a multifaceted approach to addressing the following overarching research question: How does the 103-year-old University Avenue Church of Christ come to function as it does in the present day? To address this question, I analyze tow areas of the church--its ideological and material makeup--in order to show how certain factors shape the church. Part one of this paper deals with the church's ideological development through a presentation of primary sources taken largely from church archives which describe the work of the church, its long and short-term 'vision' for the church coupled with statements about its own identity and doctrinal beliefs. These sources help explain how and why the church is the was it is today. Part Two of this paper deals with the church's material development. Analysis of images and firsthand accounts of the buildings UA has worshiped in helps get an idea of what the church wants to present to the outside world aesthetically but also in iconographic associations that will inevitably be made due to certain choices about what appears materially inside and outside the building.
Tunable bandgaps and flat bands in twisted bilayer biphenylene carbon
Creators: name: Ma, Yabin
name: Ouyang, Tao
name: Chen, Yuanping
name: Xie, Yuee
Publisher: name: arXiv
Year: 2021
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Owing to the interaction between the layers, the twisted bilayer two-dimensional materials exhibit numerous unique optical and electronic properties different from the monolayer counterpart, and have attracted tremendous interests in current physical research community. By means of first-principles and tight-binding model calculations, the electronic properties of twisted bilayer biphenylene carbon are systematically investigated in this paper. The results indicate that the effect of twist will not only leads to a phase transition from semiconductor to metal, but also an adjustable band gap in BPC (0 meV to 120 meV depending on the twist angle). Moreover, unlike the twisted bilayer graphene (TBG), the flat bands in twisted BPC are no longer restricted by "magic angles", i.e., abnormal flat bands could be appeared as well at several specific large angles in addition to the small angles. The charge density of these flat bands possesses different local modes, indicating them might be derived from different stacked modes and host different properties. The exotic physical properties presented in this work foreshow twisted BPC a promising material for the application of terahertz and infrared photodetectors and the exploration of strong correlation.
On the physical oceanography of Burrard Inlet and Indian Arm, British Columbia
Creators: name: Davidson, Laurie Wayne
Publisher: name: University of British Columbia
Year: 2010

description: Measurements of the distributions of temperature, salinity and oxygen in Burrard Inlet and Indian Arm, British Columbia from May 1974 to October 1975 have been analysed to determine features of the large scale circulation in this system. Observations at roughly four-week intervals were supplemented by serial CSTD casts taken over intervals of a few hours, and by 93-day records of near-bottom currents, temperature, and salinity on the Indian Arm sill. Short-term tidal fluctuations in property distributions have been shown to be small compared to seasonal changes. Circulation in the Burrard Inlet - Indian Arm system is basically estuarine: relatively fresh surface waters normally flow down the inlet overlying more saline waters which enter from the Strait of Georgia. Turbulent mixing associated with estuarine and tidal flow through the shallow constrictions at both First and Second Narrows yields surface waters between the narrows which are more saline and cooler than those which would be found in a simpler estuarine environment. In a complementary sense, bottom waters are fresher and warmer. Significant exchange and overturn of deep water in Indian Arm was recorded between October 1974 and April 1975. Intruding waters were shown to have originated west of First Narrows. In one instance exchange of at least 80% of the volume of the Arm, over an interval of 33 days, was inferred from property distributions, compared to exchange estimates of 111% and 74% deduced from the current meter record for the same event. Exchange was shown to be intermittent, with fresh water runoff volume into Indian Arm, tidal mixing (particularly at Second Narrows) and density of Georgia Strait water being identified as some of the controlling factors.