cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
An optimised survey strategy for the ERIS/NIX imager: searching for young giant exoplanets and very low mass brown dwarfs using the K-peak custom photometric filter
Creators: name: Dubber, Sophie
name: Biller, Beth
name: Bonavita, Mariangela
name: Allers, Katelyn
name: Fontanive, Clémence
name: Kenworthy, Matthew A.
name: Bonnefoy, Mickaël
name: Taylor, William
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present optimal survey strategies for the upcoming NIX imager, part of the ERIS instrument to be installed on the Very Large Telescope (VLT). We will use a custom 2.2 micron K-peak filter to optimise the efficiency of a future large-scale direct imaging survey, aiming to detect brown dwarfs and giant planets around nearby stars. We use the results of previous large scale imaging surveys (primarily SPHERE SHINE and Gemini GPIES) to inform our choice of targets, as well as improved planet population distributions. We present four possible approaches to optimise survey target lists for the highest yield of detections: i) targeting objects with anomalous proper motion trends, ii) a follow-up survey of dense fields from SPHERE SHINE and Gemini GPIES iii) surveying nearby star-forming regions and iv) targeting newly discovered members of nearby young moving groups. We also compare the predicted performance of NIX to other state-of-the-art direct imaging instruments.
description: 18 pages, 11 figures. Accepted for publication in MNRAS
Walravens, Hartmut und Taube, Manfred: August Hermann Francke und die Westhimalaya-Mission der Herrnhuter Brüdergemeine
Creators: name: Klingner, Martin
Publisher: name: Unitas Fratrum
Year: 1970

description: Unitas Fratrum, Bd. 36 (1994): Unitas Fratrum, Band 36
Arylbismuth (III) carboxylates and sulfinates
Creators: name: Pfeiffer, Jan M.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Mapping the X-ray corona evolution of IRAS 13224-3809 with the power spectral density
Creators: name: Chainakun, Poemwai
name: Luangtip, Wasuthep
name: Jiang, Jiachen
name: Young, Andrew J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We develop the power spectral density (PSD) model to explain the nature of the X-ray variability in IRAS 13224-3809, including the full effects of the X-ray reverberation due to the lamp-post source. We utilize 16 XMM-Newton observations individually as well as group them into three different luminosity bins: low, medium and high. The soft (0.3-1 keV) and hard (1.2-5 keV) PSD spectra are extracted and simultaneously fitted with the model. We find that the corona height changes from h ~ 3 $\ r_{\rm g}$ during the lowest luminosity state to ~ $25 \ r_{\rm g}$ during the highest luminosity state. This provides further evidence that the source height from the reverberation data is significantly larger than what constrained by the spectral analysis. Furthermore, as the corona height increases, the energy spectrum tends to be softer while the observed fractional excess variance, $F_{\rm var}$, reduces. We find that the PSD normalization is strongly correlated with $F_{\rm var}$, and moderately correlated with the PSD bending index. Therefore, the normalization is dependent on accretion rate that controls the intrinsic shape of the PSD. While the intrinsic variability of the disk is manifested by the reverberation signals, the disk and corona may evolve independently. Our results suggest that, during the source height increases, the disk itself generates less overall variability power but more high-frequency variability resulting in the PSD spectrum that flattens out (i.e. the inner disk becomes more active). Using the luminosity-bin data, the hint of Lorentzian component is seen, with the peak appearing at lower frequencies with increasing luminosity.
description: 17 pages, 8 figures, 3 tables, accepted for publication in ApJ
Taxonomy of Operations in the Context of FAIR Digital Objects
Creators: name: Blumenröhr, Nicolas
name: Pfeil, Andreas
name: Jejkal, Thomas
name: Stotzka, Rainer
Publisher: name: Zenodo
Year: 2023
Subjects: FAIR Digital Objects, Operations, Types

description: This document and the accompanying graphic describe a taxonomy of operations that are required in the context of FAIR Digital Objects. It endeavors to provide a foundational guide for users, offering insights into the variety of available operations, their potential categorization, and suggestive placement for additional operations that might be necessary for different use cases.
The effect of the redox state on the insulin receptor in rat liver plasma membrane
Creators: name: Scher, Barbara Eva.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
The MC-QTAIM: A framework for extending the atoms in molecules analysis beyond purely electronic systems
Creators: name: Shahbazian, Shant
Publisher: name: arXiv
Year: 2021
Subjects: subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: Nuclear Theory (nucl-th)
subject: Chemical Physics (physics.chem-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The quantum theory of atoms in molecules, QTAIM, is employed to identify AIM and quantify their interactions through the partitioning of molecule into atomic basins in the real space and it is confined only to the purely electronic systems composed of electrons as quantum particles and the nuclei as clamped point charges. The extended version of the QTAIM, called the multi-component QTAIM, MC-QTAIM, bypasses this border and makes it possible to identify AIM and quantify their interactions in systems composed of multiple quantum particles that electrons may or may not be one of their components opening a new door for the analysis of the exotic AIM and bonds. In this contribution, two conjectures, called Bader conjecture, BC, and extended Bader conjecture, EBC, are proposed as the cornerstones of the real-space partitioning of a molecule into atomic basins within the context of the QTAIM and the MC-QTAIM, respectively. A literature survey on various few-body quantum systems composed of quarks, nucleons, and elementary particles like muons and positrons is also done unraveling the fact that in all these diverse systems there are unambiguous cases of clusterizations. These clustered systems, irrespective to their components, behave as if they are molecules composed of some kind of atoms, instead of being an amorphous mixture of quantum particles. In the case of the muonic and the positronic molecules computational studies reveal that the AIM structures of these systems are well-captured by the EBC. Beyond identifying atomic basins, both QTAIM and MC-QTAIM attribute properties to AIM, which is their share from the molecular expectation values of quantum observables. It is demonstrated that not only the share from the average value of an observable may be attributed to an atomic basin, but also the fluctuation of each basin property is also quantifiable.
description: This is a polished version of v2 draft
Scalar Curvature and Intrinsic Flat Convergence
Creators: name: Sormani, Christina
Publisher: name: arXiv
Year: 2016
Subjects: subject: Metric Geometry (math.MG)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: Herein we present open problems and survey examples and theorems concerning sequences of Riemannian manifolds with uniform lower bounds on scalar curvature and their limit spaces. Examples of Gromov and of Ilmanen which naturally ought to have certain limit spaces do not converge with respect to smooth or Gromov-Hausdorff convergence. Thus we focus here on the notion of Intrinsic Flat convergence, developed jointly with Wenger. This notion has been applied successfully to study sequences that arise in General Relativity. Gromov has suggested it should be applied in other settings as well. We first review intrinsic flat convergence, its properties, and its compactness theorems, before presenting the applications and the open problems.
description: 53 pages, 4 figures, Geometric Analysis on Riemannian and singular metric spaces, Lake Como School of Advnaced Studies, 11-15 July 2016, v2: minor fixes as requested by referee, to appear as a chapter in the deGruyter book series on PDE and Measure Theory edited by Gigli
Boundary effects on convection in a fluid layer subjected to underside heating
Creators: name: Yannios, Nicholas.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
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Swift J0503.7-2819: A Short-Period Asynchronous Polar or Stream-Fed Intermediate Polar
Creators: name: Halpern, J. P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We analyze a 7.4 hr XMM-Newton light curve of the cataclysmic variable Swift J0503.7-2819, previously classified using optical periods as an intermediate polar (IP) with an orbital period of 0.0567 days. A photometric signal at 975 s, previously suggested to be the spin period, is not present in X-rays and is readily understood as a quasi-periodic oscillation. The X-ray light curve instead shows clear behavior of a highly asynchronous polar (AP) or stream-fed IP. It can be described by either of two scenarios: one which switches between one-pole and two-pole accretion, and another in which accretion alternates fully between two poles. The spin periods in these two models are 0.0455 days and 0.0505 days, respectively. The spin frequency $ω$ is thus either 24% faster or 12% faster than the orbital frequency $Ω$, and the corresponding beat period between spin and orbit is 0.231 days or 0.462 days. Brief absorption events seen in light curve are spaced in a way that may favor the longer spin and beat periods. These periods are confirmed and refined using data from the Transiting Exoplanet Survey Satellite (TESS) and the Asteroid Terrestrial-impact Last Alert System (ATLAS). The short beat cycle of Swift J0503.7-2819 makes it well-suited to resolving this common dilemma, which amounts to deciding whether the main signal in the power spectrum is $ω$ or $2ω-Ω$.
description: 10 pages, 3 figures, to appear in The Astrophysical Journal
On the structure observed in the in-flight ${}^{3}\text{He} ( K^{-} , \, Λp ) n$ reaction at J-PARC
Creators: name: Sekihara, Takayasu
name: Oset, Eulogio
name: Ramos, Angels
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A theoretical investigation is done to clarify the origin of the peak structure observed near the $K^{-} p p$ threshold in the in-flight ${}^{3}\text{He} ( K^{-}, \, Λp ) n$ reaction of the J-PARC E15 experiment, which could be a signal of the lightest kaonic nuclei, that is, the $\bar{K} N N (I=1/2)$ state. For the investigation, we evaluate the $Λp$ invariant mass spectrum assuming two possible scenarios to interpret the experimental peak. One assumes that the $Λ(1405)$ resonance is generated after the emission of an energetic neutron from the absorption of the initial $K^-$, not forming a bound state with the remaining proton. This uncorrelated $Λ(1405) p$ system subsequently decays into the final $Λp$. The other scenario implies that, after the emission of the energetic neutron, a $\bar{K} N N$ bound state is formed, decaying eventually into a $Λp$ pair. Our results show that the experimental signal observed in the in-flight ${}^{3}\text{He} ( K^{-} , \, Λp ) n$ reaction at J-PARC is qualitatively well reproduced by the assumption that a $\bar{K} N N$ bound state is generated in the reaction, definitely discarding the interpretation in terms of an uncorrelated $Λ(1405) p$ state.
description: 27 pages, 18 EPS figures, version accepted for publication in PTEP, discussions on numerical results improved
Clues to the nature of ultra diffuse galaxies from estimated galaxy velocity dispersions
Creators: name: Zaritsky, Dennis
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We describe how to estimate the velocity dispersions of ultra diffuse galaxies, UDGs, using a previously defined galaxy scaling relationship. The method is accurate for the two UDGs with spectroscopically measured dispersions, as well as for ultra compact galaxies, ultra faint galaxies, and stellar systems with little or no dark matter. This universality means that the relationship can be applied without further knowledge or prejudice regarding the structure of a galaxy. We then estimate the velocity dispersions of UDGs drawn from two published samples and examine the distribution of total masses. We find, in agreement with the previous studies of two individual UDGs, that these systems are dark matter dominated systems, and that they span a range of at least $10^{10} < M_{200}/M_\odot < 10^{12} $. These galaxies are not, as an entire class, either all dwarfs or all failed $L_*$ galaxies. Estimates of the velocity dispersions can also help identify interesting subsets of UDGs, such as those that are likely to have the largest mass-to-light ratios, for subsequent spectroscopic study.
description: 4 pages, accepted for publication in MNRAS Letters (typographical error in Equation 1 corrected)
The Galactic Center Molecular Cloud Survey. I. A Steep Linewidth-Size Relation & Suppression of Star Formation
Creators: name: Kauffmann, Jens
name: Pillai, Thushara
name: Zhang, Qizhou
name: Menten, Karl M.
name: Goldsmith, Paul F.
name: Lu, Xing
name: Guzmán, Andrés E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Central Molecular Zone (CMZ; inner $\sim{}200~\rm{}pc$) of the Milky Way is a star formation (SF) environment with very extreme physical properties. Exploration of SF in this region is important because (i) this region allows us to test models of star formation under exceptional conditions, and (ii) the CMZ clouds might be suitable to serve as templates to understand the physics of starburst galaxies in the nearby and the distant universe. For this reason we launched the Galactic Center Molecular Cloud Survey (GCMS), the first systematic study that resolves all major CMZ clouds at interferometer angular resolution (i.e., a few arc seconds). Here we present initial results based on observations with the Submillimeter Array (SMA) and the Atacama Pathfinder Experiment (APEX). Our study is complemented by dust emission data from the Herschel Space Telescope and a comprehensive literature survey of CMZ star formation activity. Our research reveals (i) an unusually steep linewidth-size relation, $σ(v)\propto{}r_{\rm{}eff}^{0.66\pm{}0.18}$, down to velocity dispersions $\sim{}0.6~\rm{}km\,s^{-1}$ at 0.1 pc scale. This scaling law potentially results from the decay of gas motions to transonic velocities in strong shocks. The data also show that, relative to dense gas in the solar neighborhood, (ii) star formation is suppressed by factors $\gtrsim{}10$ in individual CMZ clouds. This observation encourages exploration of processes that can suppress SF inside dense clouds for a significant period of time.
description: accepted to Astronomy & Astrophysics
Quasi-perpendicular shock acceleration and TDE radio flares
Creators: name: Xu, Siyao
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Delayed radio flares of optical tidal disruption events (TDEs) indicate the existence of non-relativistic outflows accompanying TDEs. The interaction of TDE outflows with the surrounding circumnuclear medium creates quasi-perpendicular shocks in the presence of toroidal magnetic fields. Because of the large shock obliquity and large outflow velocity, we find that the shock acceleration induced by TDE outflows generally leads to a steep particle energy spectrum, with the power-law index significantly larger than the "universal" index for a parallel shock. The measured synchrotron spectral indices of recently detected TDE radio flares are consistent with our theoretical expectation. It suggests that the particle acceleration at quasi-perpendicular shocks can be the general acceleration mechanism accounting for the delayed radio emission of TDEs.
description: 8 pages, 5 figures; accepted for publication in The Astrophysical Journal
Full elasticity tensor from thermal diffuse scattering
Creators: name: Wehinger, Björn
name: Mirone, Alessandro
name: Bosak, Alexeï
name: Krisch, Michael
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We present a method for the precise determination of the full elasticity tensor from a single crystal diffraction experiment using monochromatic X-rays. For the two benchmark systems calcite and magnesium oxide we show that the measurement of thermal diffuse scattering in the proximity of Bragg reflections provides accurate values of the complete set of elastic constants. This approach allows for a reliable and model free determination of the elastic properties and can be performed together with crystal structure investigation in the same experiment.
Studies on the biology of the common armyworm mythimna convecta (Walker)
Creators: name: Smith, Andrew Mark.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Cell-free DNA in the Cerebrospinal Fluid under Emotional Stress
Creators: name: Mariia Zharova
name: Umriukhin, Pavel
name: Veiko, Natalia
Publisher: name: International Student’s Journal of Medicine
Year: 2016
Subjects: Stress Resistance
Rat
Open Field
Motor Activity Index

description: Background: Cell free circulating DNA (cfDNA) in blood is known to be a tumor marker however there is no information about its concentration in cerebrospinal fluid (CSF) in control and in emotional stress (ES). The aim of the study was to determine level of cfDNA in CSF of rats with different resistance to stress before and after ES. Methods: A total of 19 male Wistar rats weighing 200-220 g were included in this study. All rats were divided into 2 groups depending on the motor activity: active (prognostically resistant to ES) – 9, animals predisposed to ES (passive) – 10. CSF samples were collected twice by puncture of the cisterna magna of the brain before and after stress in the interval of 10 days. CfDNA was detected by phenol method. Statistical data analysis was performed with SPSS 16 for Windows. Results: Tendency to higher level of cfDNA in active rats compared with other groups has been found in our experiments. All animals statistically significant were divided into two groups: with high and low concentration of cfDNA in CSF. 70% animals with high level of cfDNA in CSF were active rats and 30% passive. After stress the concentration of cfDNA in active animals demonstrated a tendency to decrease, while the passive on the contrary, to increase after ES. Furthermore, the inverse correlation between the change of cfDNA and volume of CSF aliquot was identified. Conclusion: We have proved the presence of cfDNA in rats` CSF. cfDNA concentrations differ in active and passive rats. It`s level decreases in active rats and increases in passive after ES. The higher concentration of cfDNA in active rats possibly related to the low activity of endonuclease compared with passive animals. This data can be compared with similar data from earlier studies of cfDNA in serum.Volume of CSF changes in active and passive rats differently: in active, it increases in passive decreases after ES. We cannot explain this phenomenon. Therefore, to clarify these issues and to determine the source of cfDNA in CSF further studies are needed.
Consciousness of natural numbers
Creators: name: Khripkov, Alexander Ivanovich
Publisher: name: Zenodo
Year: 2023
Subjects: Number theory, number structure, natural numbers, number series, number order, number function, number event, number field, degree of movement, number reorientation, numerical data, data base, scientific programs, artificial intelligence, number integration, number values, degree of freedom, paradoxes of numbers, fundamental data, unity of numbers. functional connection, phases of functions, sequences of functions, order of functions, limits of functions, functional transitions, tensor functions, mathematical physics, mathematical genetics, nuclear functions, neutrinos, quantum.

description: The main reason for the content of this material is that mathematics is not an applied science. In turn, any scientific discipline that uses mathematical reasoning is a philosophical or experimental technical application that defines all sorts of criteria for perceiving real nature. Pay attention to the main perception by the "observer" of only the external reflection of the surrounding world. Mathematics, in this case, provides the possibility of perceiving the compatibility of the inner and outer Worlds, when the unit is not equal to one: [1 ≠ 1]
Niche evolution and diversification in Middle Eastern stream salamanders (Paradactylodon): vulnerability to future climate change
Creators: name: Vaissi, Somaye
name: Heshmatzad, Pouria
name: Hernandez, Axel
Publisher: name: Brill Online
Year: 2023
Subjects: classificationCode: 310399
subject: Ecology not elsewhere classified

description: The relict genus Paradactylodon is narrowly distributed in temperate forests throughout the Middle East region, including P. mustersi in Afghanistan, P. persicus, and P. gorganensis in northwestern and northeastern Iran. Recent phylogenetic analyses suggest that the Iranian Paradactylodon populations may belong to a single species, P. persicus. In this study, we addressed how climatic niche conservatism and/or niche divergence may have affected the evolution of all Paradactylodon species using ecological niche models and multivariate niche analyses to identify niche overlap and assess equivalency and similarity tests. We also used an ensemble of ten algorithms to predict Paradactylodon species distributions for recent (1970-2000) and future (2081-2100) climate conditions. The results show that future climate change may cause the loss of 80 to 97% of these species' suitable habitat, especially at lower elevations. The niche divergence hypothesis was supported by the results of niche equivalency tests on P. persicus vs. P. gorganensis (and vice versa) with moderate overlap (D = 0.23, I = 0.41) and P. persicus vs. P. mustersi (and vice versa) with little overlap (D = 0.05, I = 0.06). Meanwhile, the niche similarity test for the niche conservatism hypothesis revealed significant results for P. persicus vs. P. gorganensis, P. mustersi vs. P. persicus, and P. persicus + P. gorganensis (as a single species) vs. P. mustersi. Due to these complex evolutionary ecological patterns and allopatric distributions, we recommend that P. gorganensis be considered a valid subspecies.
Compressive Data Aggregation on Mobile Wireless Sensor Networks for Sensing in Bike Races
Creators: name: Du, Wei
name: Gorce, Jean-Marie
name: Risset, Tanguy
name: Lauzier, Matthieu
name: Fraboulet, Antoine
Publisher: name: arXiv
Year: 2016
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: -This paper presents an efficient approach to data collection in mobile wireless sensor networks, with the specific application of sensing in bike races. Recent sensor technology permits to track GPS position of each bike. Because of the inherent correlation between bike positions in a bike race, a simple GPS log is inefficient. The idea presented in this work is to aggregate GPS data at sensors using compressive sensing techniques. We enforce, in addition to signal sparsity, a spatial prior on biker motion because of the group behaviour (peloton) in bike races. The spatial prior is modeled by a graphical model and the data aggregation problem is solved, with both the sparsity and the spatial prior, by belief propagation. We validate our approach on a bike race simulator using trajectories of motorbikes in a real bike race, the "crit{é}rium du dauphin{é} 20XX" .
[Halle (Saale), Universitäts- und Landesbibliothek Sachsen-Anhalt, Morbio 14 (23)]
Creators: name: Micherius Ferrarius
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1283
Subjects: subject: Sonstige weltliche Aussteller
subject: Notarsurkunde
subject: Urkunde
subject: 090

description: Micherius Ferrarius, Sohn des verstorbenen Albertus Ferrarius de Uglono, und weitere genannte Personen, alle wohnhaft an der porta Ticinensis in Mailand, verpflichten sich gegenüber Continus de Uboldo, genannt Turronus, wohnhaft ebendort, zur Haftung für einen erhaltenen Geldbetrag.
[Halle (Saale), Universitäts- und Landesbibliothek Sachsen-Anhalt, Morbio 28 (19)]
Creators: name: Zygmunt August, II.
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1553
Subjects: subject: Herrscherurkunde
subject: Urkunde
subject: 090

description: Sigismund II. August, König von Polen und Großfürst von Litauen, verleiht Carolus Antonius Gambaloyta aus Mailand für seinen Dienst an der Königin das Recht, ein genau beschriebenes Wappen zu führen.
Extrapancreatic effects of gliclazide (diamicron)
Creators: name: Hoich, Robert Ivan.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
[Halle (Saale), Universitäts- und Landesbibliothek Sachsen-Anhalt, Morbio 28 (3)]
Creators: name: Avalos, Innigo D
name: Alberus, Paulus
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1592
Subjects: subject: Sonstige geistliche Aussteller
subject: Urkunde
subject: 090

description: Innigo [d'Avalos], Bischof von Porto-Santa Rufina, Kardinal von Aragon und protector der Erzbruderschaft Sanctorum Duodecim Apostolorum de Urbe, und Paulus Alberus, Erzbischof von Ragusa und Prior der genannten Erzbruderschaft, sowie weitere Offiziale der Erzbruderschaft sichern der Bruderschaft Sanctissimi Sacramenti Corporis Christi der Kirche St. Laurentii in Bergamo die Aufnahme in ihren Schutz zu.
Oficina de Processo de Trabalho do Enfermeiro no Hospital Materno Infantil
Creators: name: Martins, Vanessa Naffitali de Souza
name: Casagrande, Vanessa
name: Silva, Luís Carlos de Paula
name: Braccialli, Luzmarina Aparecida Doretto
Publisher: name: Zenodo
Year: 2023
Subjects: enfermeiros; enfermagem; cuidados de enfermagem; serviços de enfermagem; fluxo de trabalho.

description: Considerando os processos de trabalho do enfermeiro há necessidade de maior compreensão desse e uma reconstrução dos processos de trabalho no Hospital Materno Infantil (HMI) para melhoria do cuidado em enfermagem e em saúde. Para tanto, esta oficina é proposta para promover discussões da temática e capacitação dos profissionais.
[Halle (Saale), Universitäts- und Landesbibliothek Sachsen-Anhalt, Morbio 28 (6)]
Creators: name: Julius, II.
name: Michiel, Giovanni
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1493
Subjects: subject: Ablassurkunde
subject: Urkunde
subject: 090

description: Verschiedene genannte Kardinäle gewähren im Namen Papst Alexanders VI. allen, die die Kapelle St. Hieronymi in der Kirche St. Petri in Bozzolo im Bistum Cremona besuchen, einen 100 Tage währenden Ablass, wenn sie die Kapelle am Tag der Apostel Petrus und Paulus von der ersten bis zur zweiten Vesper besuchen.
Ionization Distributions in Outflows of Active Galaxies: Universal Trends and Prospect of Future XRISM Observations
Creators: name: Keshet, Noa
name: Behar, Ehud
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The physics behind the ionization structure of outflows from black holes is yet to be fully understood. Using archival observations with the Chandra\HETG gratings over the past two decades, we measured an absorption measure distribution for a sample of outflows in nine active galaxies (AGNs), namely the dependence of outflow column density, $N_H$, on the ionization parameter, $ξ$. The slope of $\log(N_H)$ vs. $\logξ$ is found to be between 0.00 and 0.72. We find an anti-correlation between the log of total column density of the outflow and the log of AGN luminosity, and none with the black hole mass and accretion efficiency. A major improvement in the diagnostics of AGN outflows will potentially occur with the launch of the XRISM/Resolve spectrometer. We study the ability of Resolve to reveal the outflow ionization structure by constructing the absorption measure distribution from simulated Resolve spectra, utilizing its superior resolution and effective area. Resolve constrains the column density as well as HETG, but with much shorter observations.
description: To be published in ApJ
Comparative Dynamical Study of a Bound Entangled State
Creators: name: Sinha, Suprabhat
Publisher: name: arXiv
Year: 2021
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The bound entangled state carries noisy entanglement and it is very hard to distill but the usefulness of bound entangled states has been depicted in different applications. This article represents a comparative dynamical study of an open quantum system for one of the bound entangled states proposed by Bennett et al. The study is conducted under the influence of Heisenberg, bi-linear bi-quadratic and Dzyaloshinskii-Moriya (DM) interaction. During the study, an auxiliary qutrit interacts with one of the qutrits of the selected two qutrit bound entangled state through different interactions. The computable cross-norm or realignment (CCNR) criterion has been used to detect the bound entanglement of the state and the negativity has been applied to measure the free entanglement. From this three-fold study it is observed that, although the auxiliary qutrit plays a significant role during the interaction, the probability amplitude of the qutrit does not affect the open quantum system. Further, it is found that the Dzyaloshinskii-Moriya (DM) interaction performs better to activate the chosen bound entangled state among all the interactions.
description: 9 pages, 3 figures
Upper Bound on the Gluino Mass in Supersymmetric Models with Extra Matters
Creators: name: Moroi, Takeo
name: Yanagida, Tsutomu T.
name: Yokozaki, Norimi
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We discuss the upper bound on the gluino mass in supersymmetric models with vector-like extra matters. In order to realize the observed Higgs mass of 125 GeV, the gluino mass is bounded from above in supersymmetric models. With the existence of the vector-like extra matters at around TeV, we show that such an upper bound on the gluino mass is significantly reduced compared to the case of minimal supersymmetric standard model. This is due to the fact that radiatively generated stop masses as well the stop trilinear coupling are enhanced in the presence of the vector-like multiplets. In a wide range of parameter space of the model with extra matters, the gluino is required to be lighter than $\sim 3$ TeV, which is likely to be within the reach of forthcoming LHC experiment.
description: 16 pages, 6 figures; references added
Uncertainty aware anomaly detection to predict errant beam pulses in the SNS accelerator
Creators: name: Blokland, Willem
name: Ramuhalli, Pradeep
name: Peters, Charles
name: Yucesan, Yigit
name: Zhukov, Alexander
name: Schram, Malachi
name: Rajput, Kishansingh
name: Jeske, Torri
Publisher: name: arXiv
Year: 2021
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: Machine Learning (cs.LG)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: High-power particle accelerators are complex machines with thousands of pieces of equipmentthat are frequently running at the cutting edge of technology. In order to improve the day-to-dayoperations and maximize the delivery of the science, new analytical techniques are being exploredfor anomaly detection, classification, and prognostications. As such, we describe the applicationof an uncertainty aware Machine Learning method, the Siamese neural network model, to predictupcoming errant beam pulses using the data from a single monitoring device. By predicting theupcoming failure, we can stop the accelerator before damage occurs. We describe the acceleratoroperation, related Machine Learning research, the prediction performance required to abort beamwhile maintaining operations, the monitoring device and its data, and the Siamese method andits results. These results show that the researched method can be applied to improve acceleratoroperations.
description: 11 pages, 15 figures, for PR-AB
Non-solar abundance ratios trends of dEs in Fornax Cluster using newly defined high resolution indices
Creators: name: Şen, Şeyda
name: Peletier, Reynier F.
name: Vazdekis, Alexandre
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We perform a detailed study of the stellar populations in a sample of massive Fornax dwarf galaxies using a set of newly defined line indices. Using data from the Integral field spectroscopic data, we study abundance ratios of eight dEs with stellar mass ranging from 10$^8$ to 10$^{9.5}$ M$_\odot$ in the Fornax cluster. We present the definitions of a new set of high-resolution Lick-style indices to be used for stellar population studies of unresolved small stellar systems. We identify 23 absorption features and continuum regions, mainly dominated by 12 elements (Na, Ca, Sc, Ti, V, Cr, Mn, Fe, Ni, Y, Ba and Nd) in the wavelength range 4700 - 5400 Å and characterise them as a function of age, metallicity and alpha element abundance ratios. We analyse eight dEs and interpret the line strengths, measured in our new high resolution system of indices, with the aid of stellar population models with high enough spectral resolution. We obtain abundance ratio proxies for a number of elements that have never been studied before for dwarf ellipticals outside the Local Group. These proxies represent relative deviations from predicted index-strengths of base stellar population models built-up following the abundance pattern of The Galaxy. The abundance proxy trend results are compared to abundance ratios from resolved stars in the Local Group, and indices from integrated light of larger early-type galaxies. We find that all our dwarfs show a pattern of abundance ratios consistent with the disk of the Milky Way, indicative of slow formation in comparison to their high mass counterparts.
description: Accepted for publication in MNRAS, 31 pages, 30 figures
Flash vacuum pyrolysis of aryl prop-2-ynoates and attempted synthesis of dimethylpropadienethione
Creators: name: Anderson, Mark Robert.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
[Halle (Saale), Universitäts- und Landesbibliothek Sachsen-Anhalt, Morbio 28 (1)]
Creators: name: Johannes
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1343
Subjects: subject: Sammelindulgenz
subject: Urkunde
subject: 090

description: Johannes, Erzbischof von Edessa, und weitere genannte Geistliche gewähren der Congregatio Beatae Mariae Virginis ac Beati Cyri Confessoris in Pavia Sündenablass.
Features and impact of dysphagia, dysphonia and laryngeal hypersensitivity in whiplash associated disorder – a qualitative study
Creators: name: Stone, Danielle B.
name: Rebbeck, Trudy
name: Ward, Elizabeth C.
name: Elliott, James E.
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
classificationCode: 69999
subject: Biological Sciences not elsewhere classified
subject: Cancer
classificationCode: 111714
subject: Mental Health

description: Investigation into dysphagia, dysphonia and laryngeal hypersensitivity after whiplash is limited, offering minimal insight into specific features and impact. This study aimed to explore these symptoms. A qualitative interpretive description design was used. Eleven participants with chronic Whiplash Associated Disorder and self-reported swallowing, voice and/or throat-related problems completed baseline symptom questionnaires and were offered a videofluroscopic swallow study to investigate baseline swallowing biomechanics. Semi-structured interviews were conducted to explore features of swallowing, voice and laryngeal sensory complaints and analysed using thematic analysis. There were high baseline levels of self-reported neck, pain- and throat-related disability and psychological distress. There was no evidence of baseline deficits in swallow biomechanics. Thematic analysis revealed 5 themes: (1) A range of features of dysphagia and dysphonia exist after whiplash with varied clinical course; (2) Activity and participation in swallow and voice activities have changed; (3) There are psychological and emotional impacts; (4) Features of laryngeal hypersensitivity co-exist and (5) There are barriers to management. Swallow, voice and laryngeal sensory problems after whiplash were described, with impacts on quality of life and barriers to management. These insights broaden understanding of post-whiplash sequalae, indicating the need for better detection.Implications for rehabilitationDysphagia, dysphonia and laryngeal hypersensitivity are under-recognised consequences of whiplash.Individuals presenting with dysphagia, dysphonia and laryngeal sensory symptoms after whiplash experience significant implications to wellbeing, activity and participation.Improved understanding of these symptoms may facilitate better detection and subsequent referral to speech-language pathology.Greater understanding into the functional and psychosocial implications of these symptoms may guide more effective post-whiplash assessments and informed rehabilitation. Dysphagia, dysphonia and laryngeal hypersensitivity are under-recognised consequences of whiplash. Individuals presenting with dysphagia, dysphonia and laryngeal sensory symptoms after whiplash experience significant implications to wellbeing, activity and participation. Improved understanding of these symptoms may facilitate better detection and subsequent referral to speech-language pathology. Greater understanding into the functional and psychosocial implications of these symptoms may guide more effective post-whiplash assessments and informed rehabilitation.
An Exact, Time-dependent Analytical Solution for the Magnetic Field in the Inner Heliosheath
Creators: name: Röken, Christian
name: Kleimann, Jens
name: Fichtner, Horst
Publisher: name: arXiv
Year: 2021
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: We derive an exact, time-dependent analytical magnetic field solution for the inner heliosheath, which satisfies both the induction equation of ideal magnetohydrodynamics in the limit of infinite electric conductivity and the magnetic divergence constraint. To this end, we assume that the magnetic field is frozen into a plasma flow resembling the characteristic interaction of the solar wind with the local interstellar medium. Furthermore, we make use of the ideal Ohm's law for the magnetic vector potential and the electric scalar potential. By employing a suitable gauge condition that relates the potentials and working with a characteristic coordinate representation, we thus obtain an inhomogeneous first-order system of ordinary differential equations for the magnetic vector potential. Then, using the general solution of this system, we compute the magnetic field via the magnetic curl relation. Finally, we analyze the well-posedness of the corresponding Dirichlet-type initial-boundary value problem, specify compatibility conditions for the initial-boundary values, and outline the implementation of initial-boundary conditions.
description: 13 pages, 1 figure, details added, minor corrections and improvements
Zero-Point Energy Leakage in Quantum Thermal Bath Molecular Dynamics Simulations
Creators: name: Brieuc, Fabien
name: Bronstein, Yael
name: Dammak, Hichem
name: Depondt, Philippe
name: Finocchi, Fabio
name: Hayoun, Marc
Publisher: name: arXiv
Year: 2016
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The quantum thermal bath (QTB) has been presented as analternative to path-integral-based methods to introduce nuclear quantumeffects in molecular dynamics simulations. The method has proved to beefficient, yielding accurate results for various systems. However, the QTBmethod is prone to zero-point energy leakage (ZPEL) in highly anharmonicsystems. This is a well-known problem in methods based on classicaltrajectories where part of the energy of the high-frequency modes istransferred to the low-frequency modes leading to a wrong energydistribution. In some cases, the ZPEL can have dramatic consequences onthe properties of the system. Thus, we investigate the ZPEL by testing theQTB method on selected systems with increasing complexity in order to studythe conditions and the parameters that influence the leakage. We also analyze the consequences of the ZPEL on the structuraland vibrational properties of the system. We find that the leakage is particularly dependent on the damping coefficient and thatincreasing its value can reduce and, in some cases, completely remove the ZPEL. When using sufficiently high values for thedamping coefficient, the expected energy distribution among the vibrational modes is ensured. In this case, the QTB methodgives very encouraging results. In particular, the structural properties are well-reproduced. The dynamical properties should beregarded with caution although valuable information can still be extracted from the vibrational spectrum, even for large values ofthe damping term.
Ultra-relativistic electron beams deflection by quasi-mosaic crystals
Creators: name: Sushko, Gennady B.
name: Korol, Andrei V.
name: Solov'yov, Andrey V.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: This paper provides an explanation of the key effects behind the deflection of ultra-relativistic electron beams by means of oriented quasi-mosaic Bent Crystals (qmBC). It is demonstrated that accounting for specific geometry of the qmBC and its orientation with respect to a collimated electron beam, its size and emittance is essential for an accurate quantitative description of experimental results on the beam deflection by such crystals. In an exemplary case study a detailed analysis of the recent experiment at the SLAC facility is presented. The methodology developed has enabled to understand the peculiarities in the measured distributions of the deflected electrons. This achievement constitutes an important progress in the efforts towards the practical realization of novel gamma-ray crystal-based light sources and puts new challenges for the theory and experiment in this research area.
description: 6 pages, 4 figures plus Supplemental Material
[Halle (Saale), Universitäts- und Landesbibliothek Sachsen-Anhalt, Morbio 28 (25)]
Creators: name: Santori, Giulio Antonio
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1582
Subjects: subject: Sonstige geistliche Aussteller
subject: Notarsurkunde
subject: Urkunde
subject: 090

description: Giulio Antonio Santòrio, Kardinal von Santa Severina und der Titularkirche San Bartolemeo all'Isola sowie portector der Erzbruderschaft Charitatis in Rom und weitere genannte Geistliche dieser Bruderschaft gewähren den fratres der Bruderschaft Sanctae Mariae de Sole in Lodi einen Ablass für die Verrichtung guter Werke
Different ice shell geometries on Europa and Enceladus due to their different sizes: impacts of ocean heat transport
Creators: name: Kang, Wanying
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: On icy worlds, the ice shell and subsurface ocean form a coupled system -- heat and salinity flux from the ice shell induced by the ice thickness gradient drives circulation in the ocean, and in turn, the heat transport by ocean circulation shapes the ice shell. Therefore, understanding the dependence of the efficiency of ocean heat transport (OHT) on orbital parameters may allow us to predict the ice shell geometry before direct observation is possible, providing useful information for mission design. Inspired by previous works on baroclinic eddies, I first derive scaling laws for the OHT on icy moons, driven by ice topography, and then verify them against high resolution 3D numerical simulations. Using the scaling laws, I am then able to make predictions for the equilibrium ice thickness variation knowing that the ice shell should be close to heat balance. Ice shell on small icy moons (e.g., Enceladus) may develop strong thickness variations between the equator and pole driven by the polar-amplified tidal dissipation in the ice, to the contrary, ice shell on large icy moons (e.g., Europa, Ganymede, Callisto etc.) tends to be flat due to the smoothing effects of the efficient OHT. These predictions are manifested by the different ice evolution pathways simulated for Enceladus and Europa, considering the ice freezing/melting induced by ice dissipation, conductive heat loss and OHT as well as the mass redistribution by ice flow.
description: arXiv admin note: substantial text overlap with arXiv:2203.16625