cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Entropy of the Randall-Sundrum brane world with the generalized uncertainty principle
Creators: name: Kim, Wontae
name: Kim, Yong-Wan
name: Park, Young-Jai
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: By introducing the generalized uncertainty principle, we calculate the entropy of the bulk scalar field on the Randall-Sundrum brane background without any cutoff. We obtain the entropy of the massive scalar field proportional to the horizon area. Here, we observe that the mass contribution to the entropy exists in contrast to all previous results, which is independent of the mass of the scalar field, of the usual black hole cases with the generalized uncertainty principle.
description: 12 pages. The improved version published in Phys. Rev. D
Antonina pretiosa Ferris 1953
Creators: name: Matsunaga, Janis N.
name: Howarth, Francis G.
name: Kumashiro, Bernarr R.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pseudococcidae
Antonina
Antonina pretiosa

description: Antonina pretiosa Ferris   New island record
 Collection records: MAUI, Kula, 3.VII.2010, ex. Bambusa sp. stems, coll. E. Rezents, det. J.N. Matsunaga, 26.VII.2010. Vouchers at HDOA.
description: Published as part of Matsunaga, Janis N., Howarth, Francis G. & Kumashiro, Bernarr R., 2019, New State Records and Additions to the Alien Terrestrial Arthropod Fauna in the Hawaiian Islands, pp. 1-71 in Proceedings of the Hawaiian Entomological Society 51 (1) on page 10, DOI: 10.5281/zenodo.10832895
Timing properties and spectral states in Aquila X-1
Creators: name: Reig, P.
name: van Straaten, S.
name: van der Klis, M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have analyzed five X-ray outbursts of the neutron-star soft X-ray transient Aql X-1 and investigated the timing properties of the source in correlation with its spectral states as defined by different positions in the color-color and hardness-intensity diagrams. The hard color and the source count rate serve as the distinguishing parameters giving rise to three spectral states: a low-intensity hard state, an intermediate state and a high-intensity soft state. These states are respectively identified with the extreme island, island and banana states that characterize the atoll sources. The large amount of data analyzed allowed us to perform for the first time a detailed timing analysis of the extreme island state. Differences in the aperiodic variability between the rise and the decay of the X-ray outbursts are found in this state: at the same place in the color-color diagram, during the rise the source exhibits more power at low frequencies (< 1 Hz), whereas during the decay the source is more variable at high frequencies (> 100 Hz). The very-low frequency noise that characterizes the banana-state power spectra below 1 Hz cannot be described in terms of a single power law but a two-component model is required. In two outbursts a new 6-10 Hz QPO has been discovered and tentatively identified with the normal/flaring branch-like oscillation observed only at the highest inferred mass accretion rates. We have compared the spectral and timing properties of Aql X-1 with those of other atoll and Z sources. Our results argue against a unification scheme for these two types of neutron-star X-ray binaries.
description: 24 pages, 4 tables, 9 figures, accepted for publication in ApJ
Additional file 1 of A meta-analysis of the medium- and long-term effects of laparoscopic sleeve gastrectomy and laparoscopic Roux-en-Y gastric bypass
Creators: name: Gu, Lihu
name: Huang, Xiaojing
name: Li, Shengnan
name: Mao, Danyi
name: Shen, Zefeng
name: Khadaroo, Parikshit Asutosh
name: Ng, Derry Minyao
name: Chen, Ping
Publisher: name: figshare
Year: 2020
Subjects: Medicine
Biological Sciences not elsewhere classified
Science Policy

description: Additional file 1 Table S1 Quality assessment of studies included.
Supplementary Figure S3 from ROM mapping of ligamentous constraints on avian hip mobility: implications for extinct ornithodirans
Creators: name: Armita R. Manafzadeh
name: Padian, Kevin
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences
subject: 110601 Biomechanics
subject: FOS: Health sciences

description: The positions of the ligament fibers modeled in our dynamic ligament fiber simulation, displayed on a right hip in the pose (FE°, ABAD°, LAR°) = (90, 25, 20). Views are: (a) anterolateral, (b) ventral, and (c) posterior. Magenta indicates a fiber of the pubofemoral ligament, cyan indicates a ventral fiber of the ischiofemoral ligament, and orange indicates a caudal fiber of the ischiofemoral ligament.
A Class of topological nodal rings and its realization in carbon networks
Creators: name: Gao, Yan
name: Chen, Yuanping
name: Xie, Yuee
name: Chang, Po-Yao
name: Cohen, Marvin L.
name: Zhang, Shengbai
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Chemical Physics (physics.chem-ph)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: Topological nodal rings can be classified into three types according to the slopes in their energy dispersion. The first two are made of type-I and II nodal points, respectively, while the third is made of both. In carbon networks, all three types can exist. Under strain, phase transitions from a topological metal to a semiconductor, take place, and at the transition points, these nodal rings shrink into type-I, II, and III semi-Dirac points. These topological features exhibit diverse electron-hole pocket patterns and Landau levels, which give rise to exotic transport properties.
MCMC Exploration of Supermassive Black Hole Binary Inspirals
Creators: name: Cornish, Neil J.
name: Porter, Edward K.
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The Laser Interferometer Space Antenna will be able to detect the inspiral and merger of Super Massive Black Hole Binaries (SMBHBs) anywhere in the Universe. Standard matched filtering techniques can be used to detect and characterize these systems. Markov Chain Monte Carlo (MCMC) methods are ideally suited to this and other LISA data analysis problems as they are able to efficiently handle models with large dimensions. Here we compare the posterior parameter distributions derived by an MCMC algorithm with the distributions predicted by the Fisher information matrix. We find excellent agreement for the extrinsic parameters, while the Fisher matrix slightly overestimates errors in the intrinsic parameters.
description: Submitted to CQG as a GWDAW-10 Conference Proceedings, 9 pages, 5 figures, Published Version
Horridipamera inconspicua
Creators: name: Matsunaga, Janis N.
name: Howarth, Francis G.
name: Kumashiro, Bernarr R.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Rhyparochromidae
Horridipamera
Horridipamera inconspicua

description: Horridipamera inconspicua (Dallas)
 NEW STATE RECORD
 Horridipamera inconspicua is widespread in the tropics from the Ethiopian Region to South Asia and Japan. It is sometimes abundant in its preferred habitat, which is early successional disturbed grassland mixed with Euphorbiaceae weeds. Its hosts are unknown, but it presumably prefers grass seeds (Slater and Zheng, 1984).
 Collection records: HAWAII, Laupahoehoe, 27.X.2008, ex. mixed lawn grass (bermuda, manienie, seashore paspalum, Tiffton), coll. Art Hollinger; Laupahoehoe, 7.VII.2009, ex. Euphorbia hirta, coll. R. Hamasaki, det. T.J. Henry, 18.V.2011; Laupahoehoe, 7.X. 2009, on patio floor-attracted to light, coll. R. Hamasaki. Vouchers at HDOA.
description: Published as part of Matsunaga, Janis N., Howarth, Francis G. & Kumashiro, Bernarr R., 2019, New State Records and Additions to the Alien Terrestrial Arthropod Fauna in the Hawaiian Islands, pp. 1-71 in Proceedings of the Hawaiian Entomological Society 51 (1) on page 11, DOI: 10.5281/zenodo.10832895
Evaluation of Automatic Video Captioning Using Direct Assessment
Creators: name: Graham, Yvette
name: Awad, George
name: Smeaton, Alan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: We present Direct Assessment, a method for manually assessing the quality of automatically-generated captions for video. Evaluating the accuracy of video captions is particularly difficult because for any given video clip there is no definitive ground truth or correct answer against which to measure. Automatic metrics for comparing automatic video captions against a manual caption such as BLEU and METEOR, drawn from techniques used in evaluating machine translation, were used in the TRECVid video captioning task in 2016 but these are shown to have weaknesses. The work presented here brings human assessment into the evaluation by crowdsourcing how well a caption describes a video. We automatically degrade the quality of some sample captions which are assessed manually and from this we are able to rate the quality of the human assessors, a factor we take into account in the evaluation. Using data from the TRECVid video-to-text task in 2016, we show how our direct assessment method is replicable and robust and should scale to where there many caption-generation techniques to be evaluated.
description: 26 pages, 8 figures
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Cart. 193 (11 H 78), f. 0075r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0075r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0075r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Casimir-Lifshitz Force for Nonreciprocal Media and Applications to Photonic Topological Insulators
Creators: name: Fuchs, Sebastian
name: Lindel, Frieder
name: Krems, Roman V.
name: Hanson, George W.
name: Antezza, Mauro
name: Buhmann, Stefan Yoshi
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Based on the theory of macroscopic quantum electrodynamics, we generalize the expression of the Casimir force for nonreciprocal media. The essential ingredient of this result is the Green's tensor between two nonreciprocal semi-infinite slabs including a reflexion matrix with four coefficients that mixes optical polarizations. This Green's tensor does not obey Lorentz's reciprocity and thus violates time-reversal symmetry. The general result for the Casimir force is analyzed in the retarded and nonretarded limits, concentrating on the influences arising from reflections with or without change of polarization. In a second step we apply our general result to a photonic topological insulator whose nonreciprocity stems from an anisotropic permittivity tensor, namely InSb. We show that there is a regime for the distance between the slabs where the magnitude of the Casimir force is tunable by an external magnetic field. Furthermore the strength of this tuning depends on the orientation of the magnetic field with respect to the slab surfaces.
description: 14 pages, 9 figures
Evolution of the polarization of the optical afterglow of the gamma-ray burst GRB 030329
Creators: name: Greiner, J.
name: Klose, S.
name: Reinsch, K.
name: Schmid, H. M.
name: Sari, R.
name: Hartmann, D. H.
name: Kouveliotou, C.
name: Rau, A.
name: Palazzi, E.
name: Straubmeier, C.
name: Stecklum, B.
name: Zharikov, S.
name: Tovmassian, G.
name: Barnbantner, O.
name: Ries, C.
name: Jehin, E.
name: Henden, A.
name: Kaas, A. A.
name: Grav, T.
name: Hjorth, J.
name: Pedersen, H.
name: Wijers, R. A. M. J.
name: Kaufer, A.
name: Park, H. -S.
name: Williams, G.
name: Reimer, O.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report 31 polarimetric observations of the afterglow of GRB 030329 with high signal-to-noise and high sampling frequency. We establish the polarization light curve, detect sustained polarization at the percent level, and find significant variability of polarization degree and angle. The data imply that the afterglow magnetic field has small coherence length and is mostly random, probably generated by turbulence.
description: Nature 426 (13. Nov. 2003), 2 figures
JASPER: Joint Optimization of Scaling, Placement, and Routing of Virtual Network Services
Creators: name: Dräxler, Sevil
name: Karl, Holger
name: Mann, Zoltán Ádám
Publisher: name: arXiv
Year: 2017
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: To adapt to continuously changing workloads in networks, components of the running network services may need to be replicated (scaling the network service) and allocated to physical resources (placement) dynamically, also necessitating dynamic re-routing of flows between service components. In this paper, we propose JASPER, a fully automated approach to jointly optimizing scaling, placement, and routing for complex network services, consisting of multiple (virtualized) components. JASPER handles multiple network services that share the same substrate network; services can be dynamically added or removed and dynamic workload changes are handled. Our approach lets service designers specify their services on a high level of abstraction using service templates. From the service templates and a description of the substrate network, JASPER automatically makes scaling, placement and routing decisions, enabling quick reaction to changes. We formalize the problem, analyze its complexity, and develop two algorithms to solve it. Extensive empirical results show the applicability and effectiveness of the proposed approach.
Spin orientation of supermassive black holes in active galaxies
Creators: name: Kollatschny, W.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Accretion of gas onto a central supermassive black hole is generally accepted to be the source of the emitted energy in active galactic nuclei.The broad emission lines we observe in their optical spectra are probably formed in the wind of an accretion disk at distances of light days to light years from the central black hole. The variable fraction of the emission lines originates at typical distances of only 1 to 50 light days from the central supermassive black hole. We derived a central black hole mass of M_orbital = 1.8 +/-0.4 x 10^7 M_sun in the Seyfert galaxy Mrk110 assuming the broad emission lines are generated in gas clouds orbiting within an accretion disk. This figure depends on the inclination angle of the accretion disk. Here we report on the detection of gravitational redshifted emission in the variable fraction of the broad emission lines. We derive a central black hole mass of M_grav = 14.0 +/-3.0 x 10^7 M_sun. These measurements are independent on the orientation of the accretion disk. The comparison of both black hole mass estimates allows to determine the projection of the central accretion disk angle i to 21 +/-5 deg. in Mrk110 and therefore the orientation of the spin axis of the central black hole.
description: 4 pages, 6 figures, in press in Astronomy and Astrophysics Letters
Supplementary Figure S2 from ROM mapping of ligamentous constraints on avian hip mobility: implications for extinct ornithodirans
Creators: name: Armita R. Manafzadeh
name: Padian, Kevin
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences
subject: 110601 Biomechanics
subject: FOS: Health sciences

description: Additional views of the ROM map comparison of “osteological” (grey) and “ligamentous” (teal) mobilities from the following (azimuth°, elevation°) viewpoints: (a) (30, 15), (b) (0, 0), (c) (90, 0), and (d) (0, 90).
Supplementary Method S2 from ROM mapping of ligamentous constraints on avian hip mobility: implications for extinct ornithodirans
Creators: name: Armita R. Manafzadeh
name: Padian, Kevin
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences
subject: 110601 Biomechanics
subject: FOS: Health sciences

description: Automatically Checking for Mesh Model Interpenetration in Maya
Quantization of strings and branes coupled to BF theory
Creators: name: Baez, John C.
name: Perez, Alejandro
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: BF theory is a topological theory that can be seen as a natural generalization of 3-dimensional gravity to arbitrary dimensions. Here we show that the coupling to point particles that is natural in three dimensions generalizes in a direct way to BF theory in d dimensions coupled to (d-3)-branes. In the resulting model, the connection is flat except along the membrane world-sheet, where it has a conical singularity whose strength is proportional to the membrane tension. As a step towards canonically quantizing these models, we show that a basis of kinematical states is given by `membrane spin networks', which are spin networks equipped with extra data where their edges end on a brane.
Supplementary Figure S4 from ROM mapping of ligamentous constraints on avian hip mobility: implications for extinct ornithodirans
Creators: name: Armita R. Manafzadeh
name: Padian, Kevin
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences
subject: 110601 Biomechanics
subject: FOS: Health sciences

description: Scatterplots demonstrating relationship between the following simulated ligament fiber recruitment values and hip joint rotations, including correlation coefficients: (a) pubofemoral and FE, (b) pubofemoral and ABAD, (c) pubofemoral and LAR, (d) caudal ischiofemoral and FE, (e) caudal ischiofemoral and ABAD, (f) caudal ischiofemoral and LAR, (g) ventral ischiofemoral and FE, (h) ventral ischiofemoral and ABAD, and (i) ventral ischiofemoral and LAR.
Josephiella Matsunaga & Howarth & Kumashiro 2019, n. sp.
Creators: name: Matsunaga, Janis N.
name: Howarth, Francis G.
name: Kumashiro, Bernarr R.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Agaonidae
Josephiella

description: Josephiella n. sp. A (apparently undescribed)
 NEW STATE RECORD
 An agaonid wasp new to science was discovered causing galls on the stems of Ficus microcarpa. Terminal stems of affected trees appeared unhealthy with a sparse foliar canopy. Initial observers of this damage were under the assumption that the same species which causes leaf galling on F. microcarpa (Josephiella microcarpae) was also causing the galling on stems of the same plant. However, closer examination of the stem-galling wasps showed that while both the leaf-galler and the stem-galler are morphologically similar in many ways, this in fact may be a different species. Both leaf and stem-gallers can be found on the same plant. Jean-Yves Rasplus, co-author of the leaf-galling J. microcarpae, agreed that this could be an undescribed species and is currently working on its species description.
 Subsequent to the initial discovery of this stem-galler on Oahu in 2012, infested F. microcarpa were quickly noted on Hawaii and Maui. In May, 2016, galled F. microcarpa stems with exit holes were collected from Molokai and in July, 2017, from Kauai. However, material from these islands were too old and no adults could be recovered. Therefore, we do not list the collection data below, and in the list of new species we noted a question mark next to these islands until the adults are confirmed. Josephiella n. sp. A, along with Josephiella microcarpae, lobate lac scale (Paratarchardina pseudolobata), and other ficus-feeding species has contributed to the weakening of large banyan trees on Oahu.
 Collection records: OAHU, Manoa, 13.VII.2012, ex. Ficus microcarpa stems, coll. D. Hulbert, det. J.-Y. Rasplus, 6.X.2012.
 HAWAII, Hilo, 30.VII.2012, ex. F. microcarpa stems, coll. C. Hirayama, L. Larish & S. Chun, det. B. Kumashiro, VIII.2012.
 MAUI, Wailuku, 6.VIII.2012, ex. F. microcarpa stems, coll. M. Fukada, VIII.2012. Vouchers at HDOA.
description: Published as part of Matsunaga, Janis N., Howarth, Francis G. & Kumashiro, Bernarr R., 2019, New State Records and Additions to the Alien Terrestrial Arthropod Fauna in the Hawaiian Islands, pp. 1-71 in Proceedings of the Hawaiian Entomological Society 51 (1) on pages 11-12, DOI: 10.5281/zenodo.10832895
Transversality of smooth definable maps in O-minimal structures
Creators: name: Nguyen, Nhan
name: Trivedi, Saurabh
Publisher: name: arXiv
Year: 2017
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics

description: We present a definable smooth version of the Thom transversality theorem. We show further that the set of non-transverse definable smooth maps is nowhere dense in the definable smooth topology. Finally, we prove a definable version of a theorem of Trotman which says that the Whitney $(a)$-regularity of a stratification is necessary and sufficient for the stability of transversality.
description: 17 pages
Inhomogeneous spacetimes as a dark energy model
Creators: name: Garfinkle, David
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Tolman-Bondi inhomogeneous spacetimes are used as a cosmological model for type Ia supernova data. It is found that with certain parameter choices the model fits the data as well as the standard $Λ$CDM cosmology does.
description: 9 pages, 6 figures, Added References
QCD at finite isospin chemical potential
Creators: name: Brandt, Bastian B.
name: Endrodi, Gergely
name: Schmalzbauer, Sebastian
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We investigate the properties of QCD at finite isospin chemical potential at zero and non-zero temperatures. This theory is not affected by the sign problem and can be simulated using Monte-Carlo techniques. With increasing isospin chemical potential and temperatures below the deconfinement transition the system changes into a phase where charged pions condense, accompanied by an accumulation of low modes of the Dirac operator. The simulations are enabled by the introduction of a pionic source into the action, acting as an infrared regulator for the theory, and physical results are obtained by removing the regulator via an extrapolation. We present an update of our study concerning the associated phase diagram using 2+1 flavours of staggered fermions with physical quark masses and the comparison to Taylor expansion. We also present first results for our determination of the equation of state at finite isospin chemical potential and give an example for a cosmological application. The results can also be used to gain information about QCD at small baryon chemical potentials using reweighting with respect to the pionic source parameter and the chemical potential and we present first steps in this direction.
description: 16 pages, 10 figures, Proceedings of the 35th International Symposium on Lattice Field Theory, Granada, Spain
Quantum Computation Relative to Oracles
Creators: name: Tamon, Christino
name: Yamakami, Tomoyuki
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: This paper has been withdrawn by Christino Tamon and Tomoyuki Yamakami because of errors of the main theorems. An erratum appeared in the Proceedings of the UMC 2000 Conference published by Springer.
description: This paper has been withdrawn by Christino Tamon and Tomoyuki Yamakami because of errors of the main theorems. An erratum appeared in the Proceedings of the UMC 2000 Conference published by Springer
Supplementary Figure S1 from ROM mapping of ligamentous constraints on avian hip mobility: implications for extinct ornithodirans
Creators: name: Armita R. Manafzadeh
name: Padian, Kevin
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences
subject: 110601 Biomechanics
subject: FOS: Health sciences

description: Alpha shapes computed for each of the six hips studied, viewed from an (azimuth°, elevation°) viewpoint of (210, 15) in the same subset of joint pose space: (a) QROM01 left, (b) QROM01 right, (c) QROM02 left, (d) QROM02 right, (e) QROM03 left, (f) QROM03 right, and (g) all six alpha shapes overlaid.
Encarsia cubensis Gahan 1931
Creators: name: Matsunaga, Janis N.
name: Howarth, Francis G.
name: Kumashiro, Bernarr R.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Aphelinidae
Encarsia
Encarsia cubensis

description: Encarsia cubensis Gahan
 NEW STATE RECORD
 Specimens of Encarsia cubensis were first reared from Aleurotrachelus trachoides (Hemiptera: Aleyrodidae) infesting pepper plant (Capsicum sp.) foliage in Hilo in 2008. E. cubensis is a parasitoid of various whitefly species, including A. trachoides and Aleurothrixis floccosus (Noyes 2014), two economically important pests in Hawaii.
 Collection records: HAWAII, Hilo, Waiakea Uka, 21.V.2008, ex. Aleurotrachelus trachoides on Capsicum sp. foliage, coll. S. Matayoshi, det. G.A. Evans, 21.X.2008; Hilo, Waiakea Uka, 28.IX.2009, ex. A. trachoides on Capsicum sp., coll. S. Matayoshi. OAHU, Makiki, 17.IV.2009, ex. prob. A. trachoides, coll. D. Oishi, C. Young & M. Lee, det. W. Nagamine, IV.2009. Vouchers at HDOA.
description: Published as part of Matsunaga, Janis N., Howarth, Francis G. & Kumashiro, Bernarr R., 2019, New State Records and Additions to the Alien Terrestrial Arthropod Fauna in the Hawaiian Islands, pp. 1-71 in Proceedings of the Hawaiian Entomological Society 51 (1) on page 12, DOI: 10.5281/zenodo.10832895
How vortices and shocks provide for a flux loop in two-dimensional compressible turbulence
Creators: name: Falkovich, Gregory
name: Kritsuk, Alexei G.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Chaotic Dynamics (nlin.CD)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: Large-scale turbulence in fluid layers and other quasi-two-dimensional compressible systems consists of planar vortices and waves. Separately, wave turbulence usually produces a direct energy cascade, while solenoidal planar turbulence transports energy to large scales by an inverse cascade. Here, we consider turbulence at finite Mach numbers when the interaction between acoustic waves and vortices is substantial. We employ solenoidal pumping at intermediate scales and show how both direct and inverse energy cascades are formed starting from the pumping scale. We show that there is an inverse cascade of kinetic energy up to a scale $\ell$, where a typical velocity reaches the speed of sound; this creates shock waves, which provide for a compensating direct cascade. When the system size is less than $\ell$, the steady state contains a system-size pair of long-living condensate vortices connected by a system of shocks. Thus turbulence in fluid layers processes energy via a loop: Most energy first goes to large scales via vortices and is then transported by waves to small-scale dissipation.
description: 11 pages, 7 figures
Supplementary document for Unveiling osteosarcoma responses to DAPT combined with cisplatin by using confocal Raman microscopy - 5386651.pdf
Creators: name: Li, Jie
name: Li, Jing
name: Wang, Haifeng
name: Qin, Jie
name: Zeng, Haishan
name: wang, kaige
name: wang, shuang
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Uncategorized

description: Supplemental Document
Cosmology: a bird's eye view
Creators: name: Coley, Alan A.
name: Hervik, Sigbjorn
name: Lim, Woei Chet
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this essay we discuss the difference in views of the Universe as seen by two different observers. While one of the observers follows a geodesic congruence defined by the geometry of the cosmological model, the other observer follows the fluid flow lines of a perfect fluid with a linear equation of state. We point out that the information these observers collect regarding the state of the Universe can be radically different; while one observes a non-inflating ever-expanding ever-lasting universe, the other observer can experience a dynamical behaviour reminiscent to that of quintessence or even that of a phantom cosmology leading to a 'big rip' singularity within finite time (but without the need for exotic forms of matter).
description: 5 pages; received an honorable mention in the Gravity Research Foundation Essay Competition, 2006
Ellipticity dependence of high-harmonic generation in solids: unraveling the interplay between intraband and interband dynamics
Creators: name: Tancogne-Dejean, Nicolas
name: Mücke, Oliver D.
name: Kärtner, Franz X.
name: Rubio, Angel
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The strong ellipticity dependence of high-harmonic generation in gases enables numerous experimental techniques that are nowadays routinely used, for instance, to create isolated attosecond pulses. Extending such techniques to high-harmonic generation in solids requires a fundamental understanding of the microscopic mechanism of the high-harmonic generation. Here, using extensive first-principles simulations within a time-dependent density-functional framework, we show how intraband and interband mechanisms are strongly and differently affected by the ellipticity of the driving laser field. The complex interplay between intraband and interband effects can be used to tune and improve harmonic emission in solids. In particular, we show that the energy cutoff of the high-harmonic plateau can be increased by as much as 30\% using a finite ellipticity of the driving field, opening a new avenue for better understanding and control of HHG in solids based on ellipticity. Also, we demonstrate the possibility to generate, from a single circularly polarized driving field, circularly polarized harmonics with alternating helicity. Our work shows that ellipticity provides an additional knob to experimentally control high-order harmonic generation in solids.
Local decay of $C_0$-semigroups with a possible singularity of logarithmic type at zero
Creators: name: Stahn, Reinhard
Publisher: name: arXiv
Year: 2017
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 40E05 (47D06, 35B40)

description: We prove decay rates for a vector-valued function $f$ of a non-negative real variable with bounded weak derivative, under rather general conditions on the Laplace transform $\hat{f}$. This generalizes results of Batty-Duyckaerts (2008) and other authors in later publications. Besides the possibility of $\hat{f}$ having a singularity of logarithmic type at zero, one novelty in our paper is that we assume $\hat{f}$ to extend to a domain to the left of the imaginary axis, depending on a non-decreasing function $M$ and satisfying a growth assumption with respect to a different non-decreasing function $K$. The decay rate is expressed in terms of $M$ and $K$. We prove that the obtained decay rates are essentially optimal for a very large class of functions $M$ and $K$. Finally we explain in detail how our main result improves known decay rates for the local energy of waves on exterior domains.
description: 37 pages. This is a significantly enhanced version of my paper "A quantified Tauberian theorem and local decay of C0-semigroups" submitted to arxiv in May 2017
Supplementary Method S1 from ROM mapping of ligamentous constraints on avian hip mobility: implications for extinct ornithodirans
Creators: name: Armita R. Manafzadeh
name: Padian, Kevin
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences
subject: 110601 Biomechanics
subject: FOS: Health sciences

description: Systematically Sampling Joint Poses in Maya
Encarsia diaspidicola Silvestri
Creators: name: Matsunaga, Janis N.
name: Howarth, Francis G.
name: Kumashiro, Bernarr R.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Aphelinidae
Encarsia
Encarsia diaspidicola

description: Encarsia diaspidicola Silvestri
 NEW STATE RECORD
 Pest calls regarding high infestations of Pseudaulacaspis pentagona attacking papaya trees in Manoa were reported in June, 2012. Samples of the scales were taken and held for emergence of any parasitoids that may be present. Unexpectedly, a species of Encarsia emerged, and was tentatively identified as E. diaspidicola Silvestri, and subsequently confirmed by G.A. Evans. Evans also revisited specimens which were reared from sago palm fronds infested with Aulacapis yasumatsui and other scale insects in 2008. He identified these as E. diaspidicola in 2012.
 This was surprising not only because it would constitute a new record for Hawaii, but because Encarsia diaspidicola was a candidate biological control agent of P. pentagona (Diaspididae) in Hawaii by USDA-ARS-PBARC entomologists, and had not yet been released (Neumann et al. 2010). Shortly after the Oahu discovery, lab-reared E. diaspidicola were released on Hawaii island in papaya fields to control the P. pentagona infestations devastating this crop in Hawaii (Follett et al. 2015).
 Collection records: OAHU, Hawaii Loa Ridge, 3.XI.2008, ex. reared from Cycas revoluta infested with Aulacaspis yasumatsui and possibly other scale insects, coll. J. (Garcia) Matsunaga, det. G.A. Evans, 2012; Manoa, 5.XI.2012, ex. Pseudaulacaspis pentagona, on Carica papaya, coll. W. Nagamine, det. G. A. Evans, 16.II.2013. Vouchers at HDOA.
description: Published as part of Matsunaga, Janis N., Howarth, Francis G. & Kumashiro, Bernarr R., 2019, New State Records and Additions to the Alien Terrestrial Arthropod Fauna in the Hawaiian Islands, pp. 1-71 in Proceedings of the Hawaiian Entomological Society 51 (1) on page 12, DOI: 10.5281/zenodo.10832895
Deuteration of ammonia with D atoms on oxidized partly ASW covered graphite surface
Creators: name: Chaabouni, Henda
name: Minissale, Marco
name: Baouche, Saoud
name: Dulieu, François
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The deuteration of ammonia by D atoms has been investigated experimentally in the sub-monolayer regime on realistic analogues of interstellar dust grain surfaces. About 0.8 monolayer of solid NH3 was deposited on top of an oxidized graphite surface held at 10 K, partly covered with ASW ice. Ammonia ice is subsequently exposed to D atoms for different exposure times using a differentially pumped beam-line. The deuteration experiments of ammonia were carried out by mass spectroscopy and temperature programmed desorption (TPD) technique. The experimental results showed the formation of three isotopologue ammonia species by direct exothermic H-D substitution surface reactions: NH3+D->NH2D+H, NH2D+D->NHD2+H, and NHD2+D->ND3+H. The formation of the deuterated isotopologues NH2D, NHD2, and ND3 at low surface temperature (10 K) is likely to occur through quantum tunneling process on the oxidized graphite surface. A kinetic model taking into account the diffusion of D atoms on the surface is developed to estimate the width and the hight of the activation energy barriers for the successive deuteration reactions of ammonia species by D atoms. Identical control experiments were performed using CH3OH and D atoms. The deuteration process of solid methanol is ruled by H abstraction and D addition mechanism, and is almost five orders of magnitude faster than ammonia deuteration process.
Phase-space picture of resonance creation and avoided crossings
Creators: name: Timberlake, T.
name: Reichl, L. E.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Complex coordinate scaling (CCS) is used to calculate resonance eigenvalues and eigenstates for a system consisting of an inverted Gaussian potential and a monochromatic driving field. Floquet eigenvalues and Husimi distributions of resonance eigenfunctions are calculated using two different versions of CCS. The number of resonance states in this system increases as the strength of the driving field is increased, indicating that this system might have increased stability against ionization when the field strength is very high. We find that the newly created resonance states are scarred on unstable periodic orbits of the classical motion. The behavior of these periodic orbits as the field strength is increased may explain why there are more resonance states at high field strengths than at low field strengths. Close examination of an avoided crossing between resonance states shows that this type of avoided crossing does not delocalize the resonance states, although it may lead to interesting effects at certain field strengths.
description: 11 pages, 11 figures, submitted to PRA
Additional file 1 of Association of three micro-RNA gene polymorphisms with the risk of cervical cancer: a meta-analysis and systematic review
Creators: name: Xu, Jingyu
name: Geng, Junze
name: Zhang, Qiang
name: Fan, Yihua
name: Qi, Zijun
name: Xia, Tian
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1: Table S1: The PRISMA checklist.
Star Formation in Transient Molecular Clouds
Creators: name: Clark, Paul C.
name: Bonnell, Ian A.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a numerical simulation in which star formation proceeds from an initially unbound molecular cloud core. The turbulent motions, which dominate the dynamics, dissipate in shocks leaving a quiescent region which becomes gravitationally bound and collapses to form a small multiple system. Meanwhile, the bulk of the cloud escapes due to its initial supersonic velocities. In this simulation, the process naturally results in a star formation efficiency of 50%. The mass involved in star formation depends on the gas fraction that dissipates sufficient kinetic energy in shocks. Thus, clouds with larger turbulent motions will result in lower star formation efficiencies. This implies that globally unbound, and therefore transient giant molecular clouds (GMCs), can account for the low efficiency of star formation observed in our Galaxy without recourse to magnetic fields or feedback processes. Observations of the dynamic stability in molecular regions suggest that GMCs may not be self-gravitating, supporting the ideas presented in this letter.
description: 5 pages, 3 figures, accepted for MNRAS as a letter
Supplementary Method S3 from ROM mapping of ligamentous constraints on avian hip mobility: implications for extinct ornithodirans
Creators: name: Armita R. Manafzadeh
name: Padian, Kevin
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences
subject: 110601 Biomechanics
subject: FOS: Health sciences

description: Creating a ROM Map in MATLAB
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00022
Creators: name: de la Côte-d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00022, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Pulse profiles from a pulsar in scalar-tensor gravity
Creators: name: Sotani, Hajime
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The pulse profile from a neutron star in scalar-tensor theory of gravity is examined for several stellar models, where we assume the existence of the antipodal hot spots on the neutron star based on the polar cap model. Then, we find that the pulse profile from the scalarized neutron star in scalar-tensor gravity is almost the same as that in general relativity, i.e., without a scalar field, if the stellar compactness of the both stars is very similar. That is, the existence of the scalar field does not directly change the pulse profile from the neutron star, while the stellar compactness is crucial for determining the pulse shape even in the scalar-tensor gravity. Additionally, we find that the pulse shape from the scalarized neutron star is more or less similar to that from the neutron star with the same mass in general relativity, while the ratio of the minimum amplitude to the maximum amplitude in the pulse profile depend strongly on the coupling constant in scalar-tensor gravity, depending on the angle between the rotational and magnetic axes and the angle between the rotational axis and the direction to the observer. So, the direct observation of the pulse profile together with the additional observation of the stellar mass, one may extract the imprint of the gravitational theory in strong field regime.
description: accepted for publication in PRD
Scalar Metric fluctuations in space time matter inflation
Creators: name: Anabitarte, Mariano
name: Bellini, Mauricio
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the Ponce de Leon background metric, which describes a 5D universe in an apparent vacuum: $\bar{G}_{AB}=0$, we study the effective 4D evolution of both, the inflaton and gauge-invariant scalar metric fluctuations, in the recently introduced model of space time matter inflation.
description: (improved version) Accepted in Physics Letters B
Astrophysical S-factor of the $^{14}\textrm{N(p,}γ\textrm{)}^{15}\textrm{O}$ reaction at 0.4 -- 1.3\,MeV
Creators: name: Wagner, L.
name: Akhmadaliev, S.
name: Anders, M.
name: Bemmerer, D.
name: Caciolli, A.
name: Gohl, St.
name: Grieger, M.
name: Junghans, A.
name: Marta, M.
name: Munnik, F.
name: Reinhardt, T. P.
name: Reinicke, S.
name: Röder, M.
name: Schmidt, K.
name: Schwengner, R.
name: Serfling, M.
name: Takács, M. P.
name: Szücs, T.
name: Vomiero, A.
name: Wagner, A.
name: Zuber, K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The $^{14}\textrm{N(p,}γ\textrm{)}^{15}\textrm{O}$ reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning and thus determines its rate. The precise knowledge of its rate is required to correctly model hydrogen burning in asymptotic giant branch stars. In addition, it is a necessary ingredient for a possible solution of the solar abundance problem by using the solar $^{13}$N and $^{15}$O neutrino fluxes as probes of the carbon and nitrogen abundances in the solar core. After the downward revision of its cross section due to a much lower contribution by one particular transition, capture to the ground state in $^{15}$O, the evaluated total uncertainty is still 8\%, in part due to an unsatisfactory knowledge of the excitation function over a wide energy range. The present work reports precise S-factor data at twelve energies between 0.357-1.292~MeV for the strongest transition, capture to the 6.79~MeV excited state in $^{15}$O, and at ten energies between 0.479-1.202~MeV for the second strongest transition, capture to the ground state in $^{15}$O. An R-matrix fit is performed to estimate the impact of the new data on astrophysical energies. The recently suggested slight enhancement of the 6.79~MeV transition at low energy could not be confirmed. The present extrapolated zero-energy S-factors are $S_{6.79}(0)$~=~1.24$\pm$0.11~keV~barn and $S_{\rm GS}(0)$~=~0.19$\pm$0.05~keV~barn.
description: Submitted to Phys. Rev. C
Characterising a universal cloning machine by maximum-likelihood estimation
Creators: name: Sacchi, Massimiliano F.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We apply a general method for the estimation of completely positive maps to the 1-to-2 universal covariant cloning machine. The method is based on the maximum-likelihood principle, and makes use of random input states, along with random projective measurements on the output clones. The downhill simplex algorithm is applied for the maximisation of the likelihood functional.
description: 5 pages, 2 figures