cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Playing catch-up in building an open research commons
Creators: name: Bourne, Philip E.
name: Bonazzi, Vivien
name: Brand, Amy
name: Carroll, Bonnie
name: Foster, Ian
name: Guha, Ramanathan V.
name: Hanisch, Robert
name: Keller, Sallie Ann
name: Kennedy, Mary Lee
name: Kirkpatrick, Christine
name: Mons, Barend
name: Nusser, Sarah M.
name: Stebbins, Michael
name: Strawn, George
name: Szalay, Alex
Publisher: name: arXiv
Year: 2022
Subjects: subject: Digital Libraries (cs.DL)
subject: General Literature (cs.GL)
subject: FOS: Computer and information sciences

description: On August 2, 2021 a group of concerned scientists and US funding agency and federal government officials met for an informal discussion to explore the value and need for a well-coordinated US Open Research Commons (ORC); an interoperable collection of data and compute resources within both the public and private sectors which are easy to use and accessible to all.
description: 3 pages on the AAS template
Changes in the Na D$_1$ Absorption Components of $η$ Carinae Provide Clues on the Location of the Dissipating Central Occulter
Creators: name: Pickett, Connor S.
name: Richardson, Noel D.
name: Gull, Theodore
name: Hillier, D. John
name: Hartman, Henrik
name: Ibrahim, Nour
name: Lane, Alexis M.
name: Strawn, Emily
name: Damineli, Augusto
name: Moffat, Anthony F. J.
name: Navarete, Felipe
name: Weigelt, Gerd
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Na D absorption doublet in the spectrum of $η$ Carinae is complex, with multiple absorption features associated with the Great Eruption (1840s), the Lesser Eruption (1890s), and interstellar clouds. The velocity profile is further complicated by the P Cygni profile originating in the system's stellar winds and blending with the He I $λ$5876 profile. The Na D profile contains a multitude of absorption components, including those at velocities of $-$145 km s$^{-1}$, $-$168 km s$^{-1}$, and $+$87 km s$^{-1}$ that we concentrate on in this analysis. Ground-based spectra recorded from 2008 to 2021 show significant variability of the $-$145 km s$^{-1}$ absorption throughout long-term observations. In the high ionization phases of $η$ Carinae prior to the 2020 periastron passage, this feature disappeared completely but briefly reappeared across the 2020 periastron, along with a second absorption at $-$168 km s$^{-1}$. Over the past few decades, $η$ Car has been gradually brightening demonstrated to be caused by a dissipating occulter. The decreasing absorption of the $-$145 km s$^{-1}$ component, coupled with similar trends seen in absorptions of ultraviolet resonant lines, indicate that this central occulter was possibly a large clump associated with the Little Homunculus or another clump between the Little Homunculus and the star. We also report on a foreground absorption component at $+$87 km s$^{-1}$. Comparison of Na D absorption in the spectra of nearby systems demonstrates that this red-shifted component likely originates in an extended foreground structure consistent with a previous ultraviolet spectral survey in the Carina Nebula.
description: 8 figures, 13 pages plus online data, accepted to ApJ
Supplementary document for Multi-frequency self-injection locking of a FSR-tunable multimode laser diode - 6671392.pdf
Creators: name: Danilin, Andrei
name: Lobanov, Valery
name: Koptyaev, Sergey
name: Chermoshentsev, Dmitry
name: Bilenko, Igor
Publisher: name: Optica Publishing Group
Year: 2023
Subjects: Uncategorized

description: Supplementary Material document, which reveals details of phase noise measurements and laser tuning.
title: Quartierspiegel Alt-Wiedikon 2024
Creators: name: (:Unkn) Unknown
Publisher: name: Zentralbibliothek Zürich
Year: 2024
Subjects: subject: 314 Allgemeine Statistiken zu Europa
subject: 710 Städtebau, Raumplanung, Landschaftsgestaltung
subject: 949 Geschichte anderer Teile Europas
subject: Zürich-Wiedikon
subject: Quartier
subject: Amtliche Statistik
subject: Bevölkerungsstatistik

description: Aus dem einstigen Haufendorf Wiedikon entwickelte sich im 19. und 20. Jahrhundert einer der bevölkerungsreichsten Stadtkreise Zürichs. Alt-Wiedikon ist eines seiner drei Quartiere. Während das Ortsmuseum im «Haus zum Eselsschrei» aus dem Jahr 1594 einen Blick in die Vergangenheit gestattet, weisen Bauten wie die «Sihlcity» in die Zukunft.
EVALUATION OF CHEDDAR AND COTTAGE CHEESE PRODUCTION FROM DOE AND EWE MILK
Creators: name: Bezaye Taye Teshome
Publisher: name: Zenodo
Year: 2010

description: The study was aimed to produce cheddar and cottage cheese from doe and ewe milk. The sources of milk were from Arsi Negele and Kofele areas of Oromiya region. Cheddar cheeses were made from whole doe, whole ewe milk and their mixtures contained ratio of 25, 50 and 75% of doe and ewe milk using standard procedure for cheddar cheese processing technology. The proximate, microbiological, Physico-chemical, sensory analysis and yield calculation of the cheeses were made at chemical Engineering laboratory, Holleta agricultural research center, Ethiopian health and nutrition research institute.The proximate analysis result showed that cheeses made from 100% doe milk had the lowest moisture content (27.77%) and highest fat content (54.80%) but a lower yield (0.66kg/5kg of whole milk) compared to cheeses made from 100% ewe milk (35.29%, 30.1%, 0.88kg/5kg of whole milk respectively). Other mix ratios had intermediate values between the two specious of cheese (p<0.05). No significant differences in the values of protein, total solid and lactose content of sampled cheeses were found. Microbiological results showed that all cheeses made were within the limit range for acceptable conditions for consumers (< 1* 104 cfu/g). Physico – chemical analysis result showed that whole ewe milk had highest viscosity of all cheeses (3.04mPas). Three main stage of cheddar cheese making was considered for pH measurement. These stages were ripening, cooking and cheddaring.
(Mirabilia Romae vel potius) Historia et descriptio urbis Romae. Add.: Indulgentiae ecclesiarum principalium urbis Romae; 1489
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliografischer Nachweis: HR 11193; Sander 4542; Schudt 2; IGI 6448; Sajó-Soltész 2290; GW M23566
Detection of weak ubiquitous impulsive nonthermal emissions from the solar corona
Creators: name: Sharma, Rohit
name: Oberoi, Divya
name: Battaglia, Marina
name: Krucker, Sam
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: A ubiquitous presence of weak energy releases is one of the most promising hypotheses to explain coronal heating, referred to as the nanoflare hypothesis. The accelerated electrons associated with such weak heating events are also expected to give rise to coherent impulsive emission via plasma instabilities in the meterwave radio band, making this a promising spectral window to look for their presence. Recently \citet{Mondal2020b} reported the presence of weak impulsive emissions from quiet Sun regions which seem to meet the requirements of being radio counterparts of the hypothesized nanoflares. Detection of such low-contrast weak emission from the quiet Sun is challenging and, given their implications, it is important to confirm their presence. In this work, using data from the Murchison Widefield Array, we explore the use of an independent robust approach for their detection by separating the dominant slowly varying component of emission from the weak impulsive one in the visibility domain. We detect milli-SFU level bursts taking place all over the Sun and characterize their brightness temperatures, distributions, morphologies, durations and association with features seen in EUV images. We also attempt to constraint the energies of the nonthermal particles using inputs from the FORWARD coronal model along with some reasonable assumptions and find them to lie in the sub-pico flare ($\sim 10^{19}-10^{21}$ ergs) range. In the process, we also discover perhaps the weakest type III radio burst and another one that shows clear signatures of weakest quasi-periodic pulsations.
description: 16 pages, 14 figures Accepted in ApJ (7th August 2022)
Diurnale Cartusianum; [um 1495]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliografischer Nachweis: C 2017; Boh (LB) 605; Pr 5717; BMC V 590; GW 8512
Parthenice Catharinaria Fratris Baptistae Mantuani; [ca. 1502]
Creators: name: Baptista Mantuanus
name: Badius Ascensius, Jodocus
name: Franciscus A Monte Politiano
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Bibliografischer Nachweis: Goff B73; H 2376; Moreau I 89: 121; Renouard, Imprimeurs V 14; Polain (B) 480; Olivar 59 (Anm.); Hunt 4693; GW III Sp.348a.
The polluted atmosphere of the white dwarf NLTT 25792 and the diversity of circumstellar environments
Creators: name: Vennes, S.
name: Kawka, A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present an analysis of X-Shooter spectra of the polluted, hydrogen-rich white dwarf NLTT 25792. The spectra show strong lines of calcium (Ca H&K, near-infrared calcium triplet, and Ca I 4226 and numerous lines of iron along with magnesium and aluminum lines from which we draw the abundance pattern. Moreover, the photospheric Ca H&K lines are possibly blended with a circumstellar component shifted by -20 km/s relative to the photosphere. A comparison with a sample of four white dwarfs with similar parameters show considerable variations in their abundance patterns, particularly in the calcium to magnesium abundance ratio that varies by a factor of five within this sample. The observed variations, even after accounting for diffusion effects, imply similar variations in the putative accretion source. Also, we find that silicon and sodium are significantly underabundant in the atmosphere of NLTT 25792, a fact that may offer some clues on the nature of the accretion source.
description: Accepted for publication in ApJ
Nannosciurus Trouessart 1880
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Nannosciurus

description: Nannosciurus Trouessart, 1880. Le Naturaliste, p. 292. COMMENT: Formerly included the species now placed in Exilisciurus; see Moore, 1958, Am. Mus. Novit., 1914:1-5. ISIS NUMBER: 5301410002020000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 357, DOI: 10.5281/zenodo.7353023
description: {"references": ["Moore, J. C. 1958. New genera of East Indian squirrels. American Museum Novitates, 1914: 1 - 5."]}
title: Les déterminants du soutien au financement de la protection sociale : une étude sur les données du baromètre DREES  (LIEPP Working Paper, n°149)
Creators: name: Baudoin, Florian
name: Guillaud, Elvire
name: Zemmour, Michaël
Publisher: name: Sciences Po - LIEPP
Year: 2023
Subjects: classificationCode: 5
subject: FOS: Social sciences

description: À l’aide du baromètre d’opinion de la DREES, nous étudions la soutenabilité politique du financement de la protection sociale en France depuis 20 ans. Dans une première analyse méthodologique, nous montrons l’influence de la formulation des questions sur les opinions exprimées et mesurons l’importance du biais de statu quo dans les réponses exprimées en niveau. À la lumière de ces éléments, nous exploitons dans la suite de l’article les variations d’opinions entre individus et au fil du temps pour dégager un certain nombre de résultats robustes. Les assurances maladie et retraite, dont le financement est affecté et la couverture quasi universelle, sont celles qui sont le plus fortement soutenues. Au niveau individuel, le soutien au financement d’une prestation est d’autant plus fort qu’on est concerné (directement ou indirectement) par le risque couvert et qu’on y est éligible. Dans un contexte général pourtant marqué par la défiance vis-à-vis de l’impôt, nous n’observons pas de signe d’une « révolte des cotisants ». Au contraire, l’opposition à la baisse conjointe des prélèvements et des prestations est de plus en plus large. De plus, les épisodes de hausse des cotisations identifiés sur les vingt dernières années ne provoquent pas de changement d’opinion chez les assurés, tant que ces hausses sont graduelles et concernent des prestations auxquelles ils sont éligibles.
Light bending in radiation background
Creators: name: Kim, Jin Young
name: Lee, Taekoon
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We consider the velocity shift of light in presence of radiation emitted by a black body. Within geometric optics formalism we calculate the bending angle of a light ray when there is a gradient in the energy density. We model the bending for two simplified cases. The bending angle is proportional to the inverse square power of the impact parameter ($\propto 1/b^2$) when the dilution of energy density is spherically symmetric. The bending angle is inversely proportional to the impact parameter ($\propto 1/b$) when the energy density dilutes cylindrically. Assuming that a neutron star is an isothermal black body, we estimate the order of magnitude for such bending angle and compare it with the bending angle by magnetic field.
description: 8 pages, no figure
Strength and geometry of the large-scale fossil magnetic field in the accretion disks
Creators: name: Khaibrakhmanov, Sergey
Publisher: name: Zenodo
Year: 2020

description: We investigate the large-scale fossil magnetic field in the accretion disks of young stars [1,2]. We elaborate an MHD modification of Shakura and Sunyaev’s model [3]. In addition to the equations of Shakura and Sunyaev, we solve the equations of thermal and collisional ionization taking into account main ionization and recombination mechanisms, as well as dust grain evaporation. Induction equation is solved taking into account Ohmic dissipation, magnetic ambipolar diffusion, the Hall effect, and magnetic buoyancy. Analytical solution and numerical simulations of the model equations show that the magnetic buoyancy prevents runaway generation of the toroidal magnetic field, and magnetic field has quasi-azimuthal geometry in the innermost region of the disk. Magnetic field has quasi-poloidal geometry inside the `dead’ zone due to Ohmic dissipation. Ambipolar diffusion operates in the outer part of the disk, and magnetic field is quasi-radial or -azimuthal depending on the ionization rate and recombinations efficiency in this region. The Hall effect influences magnetic field geometry near the boundaries of the `dead’ zone. In the case of classical T Tauri star, magnetic field strength is of 10-300 G near the inner edge of the disk, 0.01 G at typical radial distance r=3 au inside the `dead’ zone, and it approaches interstellar value near the outer edge of the disk. Magnetic plasma beta is not constant over the disk, ranging from 100-1000 at the inner edge to 10^4-^5 inside the `dead’ zone and 1-10 at the outer edge. We compare our results with contemporary observational data on the magnetic field in the protoplanetary disks and show that the model predictions agree with the observations. The work is supported by Russian Science Foundation (project 19-72-10012).
Relativistic calculations of charge transfer probabilities in U92+ - U91+(1s) collisions using the basis set of cubic Hermite splines
Creators: name: Maltsev, I. A.
name: Deyneka, G. B.
name: Tupitsyn, I. I.
name: Shabaev, V. M.
name: Kozhedub, Y. S.
name: Plunien, G.
name: Stoehlker, Th.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: A new approach for solving the time-dependent two-center Dirac equation is presented. The method is based on using the finite basis set of cubic Hermite splines on a two-dimensional lattice. The Dirac equation is treated in rotating reference frame. The collision of U92+ (as a projectile) and U91+ (as a target) is considered at energy E_lab=6 MeV/u. The charge transfer probabilities are calculated for different values of the impact parameter. The obtained results are compared with the previous calculations [I. I. Tupitsyn et al., Phys. Rev. A 82, 042701 (2010)], where a method based on atomic-like Dirac-Sturm orbitals was employed. This work can provide a new tool for investigation of quantum electrodynamics effects in heavy-ion collisions near the supercritical regime.
Nannosciurus melanotis
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Nannosciurus
Nannosciurus melanotis

description: Nannosciurus melanotis (Muller, 1844). In Temminck, Verhandl. Nat. Gesch. Nederland Overz. Bezitt., ZooL, pp. 87, 98. TYPE LOCALITY: Indonesia, Java. DISTRIBUTION: Sumatra; Java; Borneo; adjacent small islands. ISIS NUMBER: 5301410002020002001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 357, DOI: 10.5281/zenodo.7353023
Using river locks to teach hydrodynamic concepts
Creators: name: Carvalho-Santos, Vagson L.
name: Mendes, Thales C.
name: Silva, Enisvaldo C.
name: Rios, Márcio L.
name: Silva, Anderson A P
Publisher: name: arXiv
Year: 2013
Subjects: subject: Physics Education (physics.ed-ph)
subject: FOS: Physical sciences

description: In this work, the use of a river lock as a non-formal setting for teaching Q2 hydrodynamical concepts is proposed. In particular, we describe the operation of a river lock situated at the Sobradinho dam, on the São Francisco River (Brazil). A model to represent and to analyse the dynamics of river lock operation is presented and we derive the dynamical equations for the rising of the water column as an example to understand the Euler equation. Furthermore, with this activity, we enable the integration of content initially introduced in the classroom with practical applications, thereby allowing the association of physical themes to content relevant in disciplines such as history and geography. In addition, experiences of this kind enable teachers to talk about the environmental and social impacts caused by the construction of a dam and, consequently, a crossover of concepts has been made possible, leading to more meaningful learning for the students.
description: 14 pages, 4 firgures, To appear in the European Journal of Physics
Paraxerus Forsyth Major 1893
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Paraxerus

description: Paraxerus Forsyth Major, 1893. Proc. Zool. Soc. Lond., 1893:189. COMMENT: Includes Aethosciurus (with the exception of ruwenzorii, here included in Heliosciurus) and Tamiscus; see Moore, 1959, Bull. Am. Mus. Nat. Hist., 118:153-206. ISIS NUMBER: 5301410002021000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 357, DOI: 10.5281/zenodo.7353023
description: {"references": ["Moore, J. C. 1959. Relationships among the living squirrels of the Sciurinae. Bulletin of the American Museum of Natural History, 118 (4): 157 - 206."]}
Sub-Gaussian heat kernel estimates and quasi Riesz transforms for $1\leq p\leq 2$
Creators: name: Chen, Li
Publisher: name: arXiv
Year: 2014
Subjects: subject: Analysis of PDEs (math.AP)
subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics

description: On a complete non-compact Riemannian manifold $M$, we prove that a so-called quasi Riesz transform is always $L^p$ bounded for $1
description: Final version, published in Publ. Mat., 2015
Modelling the Natural History of Rare Diseases Using Disparate Data Sources: pplication to Patients with Duchenne Muscular Dystrophy
Creators: name: Broomfield, Jonathan
Publisher: name: University of Leicester
Year: 2024

description: A health technology assessment compares the costs and effects of two or more treatments for a disease. Generally, these will be the standard of care against a novel treatment. The disease in question will often have a number of key phases that a patient progresses through, with different treatment plans, resource requirements and quality of life at each stage. These stages can be represented by a multi-state model. To compare treatments in progressive diseases, a baseline model (termed the natural history) is estimated to represent the progression made by a typical patient under current standard of care, to which different treatments can be compared. Constructing these models for rare diseases can be problematic, since evidence sources are typically much sparser, meaning data from more than one study may need to be combined to fully model disease progression from diagnosis through to death. This thesis investigates and extends current methodology for modelling the natural history of rare progressive diseases using multiple sources of data, which are likely to be heterogeneous. Electronic health records are also evaluated as a potential source of natural history data. Data from a motivating example of Duchenne Muscular Dystrophy, a rare and progressive neuromuscular disease, is used throughout. Lastly, the identified methods are applied to an economic context, with a simulated cost-effectiveness analysis comparing these methods to a previous model framework and highlighting the importance of appropriate model selection to health technology assessments and decision making.
Fratris Baptiste Mantani Carmelit[a]e Theologi de morte Colle viri prestantissimi et amicorum optimi ad Joa[n]em Baptistam Refrigerium Bononiensem; [ca. 1500]
Creators: name: Baptista Mantuanus
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Bibliografischer Nachweis: Goff B57; R 58; Camp-Kron 226a; ILC 324; Nijhoff u. Kronenberg 189; IDL 635; Schlechter-Ries 194; GW 3269
Large-scale simulations with chiral symmetry
Creators: name: The JLQCD Collaboration
name: Kaneko, T.
name: Aoki, S.
name: Cossu, G.
name: Fukaya, H.
name: Hashimoto, S.
name: Noaki, J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We carry out a comparative study among five-dimensional formulations of chirally symmetric fermions about the algorithmic performance, chiral symmetry violation and topological tunneling to find a computationally inexpensive formulation with good chiral symmetry. With our choice of the lattice action, we have launched large-scale simulations on fine lattices aiming at a precision study of light and heavy quark physics. We report on the comparative study, current status of the large-scale simulations, and preliminary results on the residual quark mass and auto-correlation.
description: 7 pages, talk presented at the 31st International Symposium on Lattice Field Theory (Lattice 2013), 29 July - 3 August 2013, Mainz, Germany
title: Les trois dimensions de la contributivité dans les assurances sociales contemporaines (LIEPP Working Paper, n°148)
Creators: name: Guillaud, Elvire
name: Zemmour, Michaël
Publisher: name: Sciences Po - LIEPP
Year: 2023
Subjects: classificationCode: 5
subject: FOS: Social sciences

description: La notion de contributivité est centrale dans les réflexions autour de la protection sociale mais son sens et sa définition varient selon les contextes. Nous faisons tout d’abord un inventaire raisonné des usages du terme de contributivité dans le champ des politiques publiques et dans la littérature économique. Très présente dans les réformes récentes des retraites ou de l’assurance chômage, la notion de contributivité structure également de longue date les controverses quant à la répartition du financement de la protection sociale entre État et cotisations. Dans le champ de la science économique, la contributivité est souvent associée hâtivement à la neutralité actuarielle avec laquelle elle ne se confond pourtant pas. Dans un second temps, nous proposons une définition positive et graduelle de la contributivité, qui peut désigner la notion d’affectation des recettes, l’affiliation des assurés et les prestations dites « contributives ». Les prestations contributives sont des prestations de remplacement du revenu d’activité, réservées aux salariés affiliés et financées par des ressources affectées. Économiquement, le montant des prestations contributives n’est pas, même approximativement, proportionnel aux cotisations versées, que l’on raisonne de manière statique ou sur le cycle de vie. En revanche, le montant des droits à prestation croît avec le revenu salarial et donc avec les cotisations versées. Ces différentes dimensions de la contributivité déterminent directement la soutenabilité politique du financement de la protection sociale. En particulier, l’affiliation des assurés à des caisses d’assurance sociale dont les recettes sont affectées est associée à un haut niveau de soutien à la protection sociale.
STUDIES ON DEVELOPMENT OF CLEANER BEAMHOUSE PROCESS, EXTRACTION AND CHARACTERIZATION OF COLLAGEN FROM FLESHING WASTES
Creators: name: DEMISSIE TSEGAW
Publisher: name: Zenodo
Year: 2018

description: The study presents the development of cleaner beamhouse processes to facilitate the extraction of collagen from fleshing waste. 0.8% offer level of alkali protease in soaking process is observed to be optimum for opening up the fibre texture of the hide, and to provide good yield of fleshing waste. In addition to this, complete removal of hair is still an issue of concern for unhairing using enzymes. CLRI had developed a novel protease for unhairing and the effectiveness of this protease for unhairing in the presence of lipase as co-enzymes was study and presented in this thesis. Experimental results indicated that 1% lipase followed by 4% protease treatment improved the unhairing efficacy. The enzymatically dehaired hide was further analyse by SEM, and the complete removal of hair in the experimental process (1% lipase followed by 4% protease) is further established. The reduction in pollution load parameters viz., BOD, COD, TOC, TDS and TSS is 89.375%, 88.57%, 85.79%, 47.37% and 48.57%, respectively with reference to conventional unhairing process. The leathers processed from optimized soaking and unhairing system showed comparable strength characteristics with reference to leather processed with chemical unhairing system. Hence a total bio-based beamhouse processing in leather manufacture was feasible. Fleshing from conventional lime and green fleshing wastes were used for the extraction of collagen, which is high value protein that can be used for a wide range of applications viz., tissue engineering, cosmetic, food, and wound healing and pharmacy application.
Paraxerus alexandri
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Paraxerus
Paraxerus alexandri

description: Paraxerus alexandri (Thomas and Wroughton, 1907). Ann. Mag. Nat. Hist., ser. 7, 19: 376. TYPE LOCALITY: Zaire, Gudima, River Iri, Upper Welle. DISTRIBUTION: N.E. Zaire, Uganda. ISIS NUMBER: 5301410002021001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 357, DOI: 10.5281/zenodo.7353023
Qusinormal oscillations and late-time tail of massless scalar perturbations of a magnetized black hole in Rastall gravity
Creators: name: Shao, Cai-Ying
name: Tan, Yu-Jie
name: Shao, Cheng-Gang
name: Lin, Kai
name: Qian, Wei-Liang
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this paper, we study the quasinormal mode and late-time tail of charged massless scalar perturbations of a black hole in the generalized Rastall gravity. The black hole metric in question is spherically symmetric, accompanied by a power-Maxwell field surrounded by a quintessence fluid. It is shown that the massless scalar field, when {\it dressed up} with the magnetic field, acquires an effective mass which, in turn, significantly affects the properties of the resultant quasinormal oscillations and late-time tails. To be specific, the quasinormal frequencies become distorted and might even be unstable for particular spacetime configurations. Also, the exponent of the usual power-law tail is modified in accordance with the modification in the structure of the branch cut of the retarded Green's function. In particular, as the effective mass is generated dynamically due to the presence of the magnetic field, one may consider a process through which the field is gradually removed from the spacetime configuration. In this context, while the quasinormal oscillations converge to the case of massless perturbations, we argue that the properties of resultant late-time tails do not fall back to their massless counterpart. The relevant features are investigated by numerical and analytic approaches.
description: Accepted for publication on CPC, doi: 10.1088/1674-1137/ac7855
Tractatus De Sphera; 1493
Creators: name: Johannes De Sacrobosco
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2010

description: Vorlageform des Erscheinungsvermerks: Georgivs. Mittelhvs. - Kolophon: ... Anno incarnatio[n]is. M.cccc.xciii. me[n]sis dece[m]br.
Reconciliation of MOND and Dark Matter theory
Creators: name: Chan, Man Ho
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: I show that Modified Newtonian Dynamics (MOND) is equivalent to assuming an isothermal dark matter density profile, with its density related to the enclosed total baryonic mass. This density profile can be deduced by physical laws if a dark matter core exists and if the baryonic component is spherically-symmetric, isotropic and isothermal. All the usual predictions of MOND, as well as the universal constant $a_0$, can be derived in this model. Since the effects of baryonic matter are larger in galaxies than in galaxy clusters, this result may explain why MOND appears to work well for galaxies but poorly for clusters. As a consequence of the results presented here, MOND can be regarded as a misinterpretation of a particular dark matter density profile.
description: Accepted by Physical Review D
Paraxerus boehmi
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Paraxerus
Paraxerus boehmi

description: Paraxerus boehmi (Reichenow, 1886). Zool. Anz., 9:315. TYPE LOCALITY: S. Zaire, Marungu. DISTRIBUTION: E. and C. Africa. COMMENT: Includes antoniae, emini, and vulcanorum; see Amtmann, 1975, Part 6.1: 10. ISIS NUMBER: 5301410002021003001 as P. boehmi. 5301410002021002001 as P. antoniae. 5301410002021006001 as P. emini. 5301410002021012001 as P. vulcanorum.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 357, DOI: 10.5281/zenodo.7353023
description: {"references": ["Amtmann, E. 1975. Family Sciuridae. Part 6. 1. Pp. 1 - 12, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.) [issued 10 Dec 1975]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Plasmonic polarons induced by alkali-atom deposition in hafnium disulfide (1$T$-HfS$_2$)
Creators: name: Emeis, Christoph
name: Mahatha, Sanjoy Kr
name: Rohlf, Sebastian
name: Rossnagel, Kai
name: Caruso, Fabio
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2023

description: We combine ab-initio calculations based on many-body perturbation theory and the cumulant expansion with angle-resolved photoemission spectroscopy (ARPES) to quantify the electron-plasmon interaction in the highly-doped semiconducting transition metal dichalcogenide 1$T$-HfS$_2$. ARPES reveals the emergence of satellite spectral features in the vicinity of quasiparticle excitations at the bottom of the conduction band, suggesting coupling to bosonic excitations with a characteristic energy of 200 meV. Our first-principles calculations of the photoemission spectral function reveal that these features can be ascribed to electronic coupling to carrier plasmons (doping-induced collective charge-density fluctuations). We further show that reduced screening at the surface enhances the electron-plasmon interaction and is primarily responsible for the emergence of plasmonic polarons.
Vitae et sententiae philosophorum; [um 1509]
Creators: name: Diogenes Laertius
name: Traversarius, Ambrosius
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliograph. Nachweis: Goff D226; H 6197?; Aquilon p. 91; Frasson-Cochet 106; Moreau I 317: 68; Richard 191; Sajó-Soltész p. 367; Günt (L) 2256; Walsh 3631b; BMC (Fr) p. 135; GW VII Sp.436a
Risk Assessment using Practical and Innovative Diagnostic Tools for Type II Diabetes Mellitus in Low-Middle Income Countries and High Income Countries: A Rapid Review Protocol
Creators: name: Shivika Marwaha
name: Gowshal, Matthew
name: Griphin Chirambo
name: Andersson, Bo
name: Mawkin, Mala
name: Taylor-Robinson, Simon
name: Henn, Patrick
name: Gallagher, Joe
name: Carroll, Christopher
name: O'Donoghue, John
Publisher: name: figshare
Year: 2020
Subjects: subject: 110107 Metabolic Medicine
subject: FOS: Clinical medicine
subject: Medicine
subject: 111716 Preventive Medicine
subject: FOS: Health sciences

description: The global prevalence of non-communicable diseases including diabetes has doubled since 1980 and T2DM is of particular concern in Low-Middle Income Countries due to a lack of risk assessment and diagnostic tools available in these settings. The primary objectives of this study are to identify existing T2DM weighted risk scores in LMICs and HICs. This will allow us to identify which health parameters determine weighted risk scores as well as, the contrast in parameters collected in LMICs and HICs. Moreover, we aim to identify gaps in the treatment guidelines issued by LMICs as compared to regulations issued by international organisations. This will give us the opportunity to assess the parameters currently taken into account in developing weighted risk scores and whether new variables such as body image could be taken into consideration.
Somnia Danielis, seu Interpretationes; 1500
Creators: name: Daniel Prophet
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliografischer Nachweis: Hélin 27; IBP 1833; SI 1289; Klebs 319.37; Coll (U) 468; GW 7935
LEGAL AID AND JUSTICE EFFICIENCY IN NIGERIA: A STUDY ON THE IMPACT OF THE NIGERIAN LEGAL AID COUNCIL
Creators: name: Chinedu, Paul Okorie
Publisher: name: AYDEN JOURNAL
Year: 2024
Subjects: Access to Justice, Legal aid, Legal Aid Council, Quick dispensation of justice, Justice in Nigeria.

description: Objectives:  Various Nigerian constitutions have guaranteed citizens' right to access to justice over time. When taken literally, access to justice refers to a person's ability to go to a court of law to air his grievances against another person or the government. Access to justice encompasses more than just access to a court of law; it also includes citizens' equitable access to political order and available resources in a particular community. Despite the constitution's provision for citizens' access to justice, a number of factors conspire to prevent this from happening in Nigeria. The Legal aid council is a body responsible for guaranteeing access to justice and quick dispensation of justice especially for the poor and other indigent citizens. The objective of this paper is to review the impacts of the legal aid council on access to justice in Nigeria. The paper commenced with reviewing the relevant key terms. The paper adopted a doctrinal research method. It was revealed among others that inequality in the distribution of the nation’s wealth coupled with the poor structure of the legal aid council and other justice administration agencies over the years contributed to delays in access to justice in Nigeria. It was based on the foregoing that recommendations were made
Towards a gravitational self force-informed effective-one-body waveform model for nonprecessing, eccentric, large-mass-ratio inspirals
Creators: name: Nagar, Alessandro
name: Albanesi, Simone
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Building upon several recent advances in the development of effective-one-body models for spin-aligned eccentric binaries with individual masses $(m_1,m_2)$ we introduce a new EOB waveform model that aims at describing inspiralling binaries in the large mass-ratio regime, $m_1\gg m_2$. The model exploits the current state-of-the-art TEOBResumS-Dali model for eccentric binaries, but the standard EOB potentials $(A,\bar{D},Q)$, informed by Numerical Relativity (NR) simulations, are replaced with the corresponding functions that are linear in the symmetric mass ratio $ν\equiv m_1 m_2/(m_1+m_2)^2$ taken at 8.5PN accuracy. To improve their strong-field behavior, these functions are: (i) suitably factorized and resummed using Padé approximants and (ii) additionally effectively informed to state-of-the-art numerical results obtained by gravitational self-force theory (GSF). For simplicity, the spin-sector of the model is taken to be the one of TEOBResumS-Dali, though removing the NR-informed spin-orbit effective corrections. We propose the current GSF-informed EOB framework as a conceptually complete analytical tool to generate waveforms for eccentric Extreme (and Intermediate) Mass Ratio Inspirals for future gravitational wave detectors.
description: 11 pages, 8 figures. Submitted to Phys. Rev. D
Paraxerus cepapi
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Paraxerus
Paraxerus cepapi

description: Paraxerus cepapi (A. Smith, 1836). Rept. Exped. Expl. C. Afr...., p. 43. TYPE LOCALITY: South Africa, W. Transvaal, Rustenberg Dist., Marico River. DISTRIBUTION: S. Angola to S. Tanzania to Transvaal (South Africa). ISIS NUMBER: 5301410002021005001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 357, DOI: 10.5281/zenodo.7353023
Tricritical curve of massive chiral Gross-Neveu model with isospin
Creators: name: Thies, Michael
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We reconsider the two-flavor version of the massive, chiral Gross-Neveu model in 1+1 dimensions. Its phase diagram as a function of baryon chemical potential, isospin chemical potential and temperature has previously been explored. We recapitulate the results, adding the missing tricritical curves. They can be determined exactly by extending the standard stability analysis, using fourth order almost degenerate perturbation theory. Results for three different bare masses are presented and discussed.
description: 9 pages, 16 figures
Orbital dynamics landscape near the most distant known trans-Neptunian objects
Creators: name: Volk, Kathryn
name: Malhotra, Renu
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The most distant known trans-Neptunian objects (perihelion distance above 38 au and semimajor axis above 150 au) are of interest for their potential to reveal past, external, or present but unseen perturbers. Realizing this potential requires understanding how the known planets influence their orbital dynamics. We use a recently-developed Poincare mapping approach for orbital phase space studies of the circular planar restricted three body problem, which we have extended to the case of the three-dimensional restricted problem with $N$ planetary perturbers. With this approach, we explore the dynamical landscape of the 23 most distant TNOs under the perturbations of the known giant planets. We find that, counter to common expectations, almost none of these TNOs are far removed from Neptune's resonances. Nearly half (11) of these TNOs have orbits consistent with stable libration in Neptune's resonances; in particular, the orbits of TNOs 148209 and 474640 overlap with Neptune's 20:1 and 36:1 resonances, respectively. Five objects can be ruled currently non-resonant, despite their large orbital uncertainties, because our mapping approach determines the resonance boundaries in angular phase space in addition to semimajor axis. Only three objects are in orbital regions not appreciably affected by resonances: Sedna, 2012 VP113 and 2015 KG163. Our analysis also demonstrates that Neptune's resonances impart a modest (few percent) non-uniformity in the longitude of perihelion distribution of the currently observable distant TNOs. While not large enough to explain the observed clustering, this small dynamical sculpting of the perihelion longitudes could become relevant for future, larger TNO datasets.
description: accepted for publication in ApJ
Self-duality and associated parallel or cocalibrated ${\mathrm{G}}_2$ structures
Creators: name: Albuquerque, Rui
Publisher: name: arXiv
Year: 2014
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: Primary: 53C25, 53C38, Secondary: 53C20, 53C28, 53C29

description: We find a remarkable family of $\mathrm{G}_2$ structures defined on certain principal $\mathrm{SO}(3)$-bundles $P_\pm\longrightarrow M$ associated with any given oriented Riemannian 4-manifold $M$. Such structures are always cocalibrated. The study starts with a recast of the Singer-Thorpe equations of 4-dimensional geometry. These are applied to the Bryant-Salamon cons\-truction of complete $\mathrm{G}_2$-holonomy metrics on the vector bundle of self- or anti-self-dual 2-forms on $M$. We then discover new examples of that special holonomy on disk bundles over ${\cal H}^4$ and ${\cal H}^2_{\mathbb{C}}$, respectively, the real and complex hyperbolic space. Only in the end we present the new $\mathrm{G}_2$ structures on principal bundles.
description: 20 pages; final version, to appear in Annales Academi{\ae} Scientiarum Fennic{\ae}
Cosmic-ray ionization rate in protoplanetary disks with sheared magnetic fields
Creators: name: Fujii, Yuri I.
name: Kimura, Shigeo S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We investigate the effects of magnetic field configurations on the ionization rate by cosmic rays in protoplanetary disks. First, we consider cosmic-ray propagation from the interstellar medium (ISM) to the protoplanetary disks and showed that the cosmic-ray density around the disk should be 2 times lower than the ISM value. Then, we compute the attenuation of cosmic rays in protoplanetary disks. The magnetic fields in the disk are stretched to the azimuthal directions, and cosmic rays need to detour while propagating to the midplane. Our results show that the detouring effectively enhances the column density by about two orders of magnitudes. We employ a typical ionization rate by cosmic rays in diffuse ISM, which is considered too high to be consistent with observations of protoplanetary disks, and find that the cosmic rays are significantly shielded at the midplane. In the case of the disk around IM Lup, the midplane ionization rate is very low for $r\lesssim\,100$ au, while the value is as large as a diffuse ISM in the outer radii. Our results are consistent with the recent ALMA observation that indicates the radial gradient in the cosmic-ray ionization rate. The high ionization rate in the outer radii of disks may activate the magnetorotational instability that was thought to be suppressed due to ambipolar diffusion. These results will have a strong influence on the dynamical and chemical evolutions of protoplanetary disks.
description: The model is updated. Conclusions are unchanged
title: Doctrinale (Partes III u. IV); 19.08.1497
title: (Cum commento valde utili)
titleType: Subtitle
Creators: name: Alexander De Villa Dei
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Bibliografischer Nachweis: C 358; Camp 132; R (Doctr) 130; IDL 220; GW 1205
Conserved Charge Fluctuations in a Chiral Hadronic Model including Hadrons and Quarks
Creators: name: Rau, Philip
name: Steinheimer, Jan
name: Schramm, Stefan
name: Stöcker, Horst
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In this work the susceptibility coefficients of the strange and non-strange quark number of second and fourth order are presented. The results at zero baryonchemical potential are obtained using a well tested chiral effective model including all known hadron degrees of freedom and additionally incorporating quarks and gluons in a PNJL model approach. Quark number susceptibilities are sensitive to the fundamental degrees of freedom in the model and signal the shift from massive hadrons to light quarks at the deconfinement transition by a sharp rise at the critical temperature. Furthermore, all susceptibilities are found to be largely suppressed by repulsive vector field interactions of the particles. In the hadronic sector vector repulsion of baryon resonances restrains fluctuations to a region determined in lattice QCD. However, in the quark sector above $T_c$ even small vector field interactions of quarks quench all fluctuations almost completely. For this reason, vector field interactions for quarks have to vanish in the deconfinement limit.
description: 8 pages, 4 figures