cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Protected edge modes without symmetry
Creators: name: Levin, Michael
Publisher: name: arXiv
Year: 2013
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We discuss the question of when a gapped 2D electron system without any symmetry has a protected gapless edge mode. While it is well known that systems with a nonzero thermal Hall conductance, $K_H \neq 0$, support such modes, here we show that robust modes can also occur when $K_H = 0$ -- if the system has quasiparticles with fractional statistics. We show that some types of fractional statistics are compatible with a gapped edge, while others are fundamentally incompatible. More generally, we give a criterion for when an electron system with abelian statistics and $K_H = 0$ can support a gapped edge: we show that a gapped edge is possible if and only if there exists a subset of quasiparticle types $M$ such that (1) all the quasiparticles in $M$ have trivial mutual statistics, and (2) every quasiparticle that is not in $M$ has nontrivial mutual statistics with at least one quasiparticle in $M$. We derive this criterion using three different approaches: a microscopic analysis of the edge, a general argument based on braiding statistics, and finally a conformal field theory approach that uses constraints from modular invariance. We also discuss the analogous result for 2D boson systems.
description: 17 pages, 9 figures, added appendix E on bosonic case, as well as appendix A2-A3 and appendix D
Additional file 5 of Two-year trajectory of functional recovery and quality of life in post-intensive care syndrome: a multicenter prospective observational study on mechanically ventilated patients with coronavirus disease-19
Creators: name: Hatakeyama, Junji
name: Nakamura, Kensuke
name: Inoue, Shigeaki
name: Liu, Keibun
name: Yamakawa, Kazuma
name: Nishida, Takeshi
name: Ohshimo, Shinichiro
name: Hashimoto, Satoru
name: Kanda, Naoki
name: Aso, Shotaro
name: Suganuma, Shinya
name: Maruyama, Shuhei
name: Ogata, Yoshitaka
name: Takasu, Akira
name: Kawakami, Daisuke
name: Shimizu, Hiroaki
name: Hayakawa, Katsura
name: Yoshida, Takeshi
name: Oshima, Taku
name: Fuchigami, Tatsuya
name: Yawata, Hironori
name: Oe, Kyoji
name: Kawauchi, Akira
name: Yamagata, Hidehiro
name: Harada, Masahiro
name: Sato, Yuichi
name: Nakamura, Tomoyuki
name: Sugiki, Kei
name: Hakozaki, Takahiro
name: Beppu, Satoru
name: Anraku, Masaki
name: Kato, Noboru
name: Iwashita, Tomomi
name: Kamijo, Hiroshi
name: Kitagawa, Yuichiro
name: Nagashima, Michio
name: Nishimaki, Hirona
name: Tokuda, Kentaro
name: Nishida, Osamu
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Mental Health

description: Supplementary Material 5.
The magnetic and crystal structures of Sr2IrO4: A neutron diffraction study
Creators: name: Ye, Feng
name: Chi, Songxue
name: Chakoumakos, Bryan C.
name: Fernandez-Baca, Jaime A.
name: Qi, Tongfei
name: Cao, G.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report a single-crystal neutron diffraction study of the layered $\rm Sr_2IrO_4$. This work unambiguously determines the magnetic structure of the system and reveals that the spin orientation rigidly tracks the staggered rotation of the $\rm IrO_6$ octahedra in $\rm Sr_2IrO_4$. The long-range antiferromagnetic order has a canted spin configuration with an ordered moment of 0.208(3) $μ_B$/Ir site within the basal plane; a detailed examination of the spin canting yields 0.202(3) and 0.049(2) $μ_B$/site for the a axis and the b axis, respectively. It is intriguing that forbidden nuclear reflections of space group $I4_1/acd$ are also observed in a wide temperature range from 4 K to 600 K, which suggests a reduced crystal structure symmetry. This neutron-scattering work provides a direct, well-refined experimental characterization of the magnetic and crystal structures that are crucial to the understanding of the unconventional magnetism exhibited in this unusual magnetic insulator.
description: the version appeared in PRB
Additional file 1 of Evaluation of clinical value and potential mechanism of MTFR2 in lung adenocarcinoma via bioinformatics
Creators: name: Chen, Cheng
name: Tang, Yang
name: Qu, Wen-Dong
name: Han, Xu
name: Zuo, Jie-Bin
name: Cai, Qing-Yong
name: Xu, Gang
name: Song, Yong-Xiang
name: Ke, Xi-Xian
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Table S1. Co-expressed gene of MTFR2.
From Creative Coding to Digital Humans:
Creators: name: Syed, Raqi
name: Echevarria, Areito
name: Jagers, Lucy
name: Shi, Ripley
name: Trewavas, Brock
name: Matich, Phil
name: Zhang, Junqi
name: Lee, Jared
Publisher: name: Open Access Victoria University of Wellington | Te Herenga Waka
Year: 2021
Subjects: Uncategorized

description: No description supplied
Additional file 2 of Evaluation of clinical value and potential mechanism of MTFR2 in lung adenocarcinoma via bioinformatics
Creators: name: Chen, Cheng
name: Tang, Yang
name: Qu, Wen-Dong
name: Han, Xu
name: Zuo, Jie-Bin
name: Cai, Qing-Yong
name: Xu, Gang
name: Song, Yong-Xiang
name: Ke, Xi-Xian
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: Table S2. GO analysis of MTFR2 co-expressed genes.
The effects of the small t properties of hadronic scattering amplitude on the determination its real part
Creators: name: Selyugin, O. V.
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Taking into account the different forms of the Coulomb-hadron interference phase and the possible spin-flip contribution the new analysis of the experimental data of the proton-antiproton elastic scattering at $3.8 < p_L <6.0 \ $GeV/c and small momentum transfer is carried out. It is shown that the size of the spin-flip amplitude can be determined from the form of the differential cross sections at small $t$, and the deviation of $ρ(s,t)$ obtained from the examined experimental data of the $p\bar{p}$ scattering from the analysis \cite{Kroll}, based on the dispersion relations, is conserved in all xamined assumptions. The analysis of the proton-proton elastic scattering at $9 < p_L < 70 \ $GeV/c also shows the impact of the examined effects on the form of the differential cross sections.
description: 13 pages, 3 figures
Θέματα Γεωμετρικής Μιγαδικής Ανάλυσης
Creators: name: Ζάρβαλης, Κωνσταντίνος Α.
Publisher: name: Aristotle University of Thessaloniki
Year: 2022
Subjects: Ημιομάδες ολόμορφων συναρτήσεων
Αρμονικό μέτρο
Μη-εφαπτομενική σύγκλιση
Υπερβολική απόσταση
Semigroups of holomorphic functions
Harmonic measure
Non-tangential convergence
Hyperbolic distance

description: Σκοπός της παρούσης διατριβής ήταν η μελέτη ορισμένων γεωμετρικών προβλημάτων που αφορούν τον ευρύτερο τομέα της Μιγαδικής Ανάλυσης. Κεντρικό άξονα της διατριβής αποτέλεσαν οι ημιομάδες ολόμορφων συναρτήσεων. Παρουσιάσαμε τις βασικές έννοιες και ιδιότητες που αφορούν τις ημιομάδες και προχωρήσαμε στην κατηγοριοποίησή τους. Στη συνέχεια, εξετάσαμε κατά πόσον οι παραβολικές ημιομάδες θετικού υπερβολικού βήματος ικανοποιούν μία συνθήκη σχετική με την εφαπτομενική ταχύτητα των τροχιών τους. Έπειτα, ασχοληθήκαμε με την προς τα πίσω τροχιά ενός συμπαγούς συνόλου μέσω μιας ημιομάδας, μελετώντας την ασυμπτωτική συμπεριφορά κάποιων ποσοτήτων της Θεωρίας Δυναμικού, όπως το αρμονικό μέτρο. Τέλος, αναζητήσαμε μία ικανή και αναγκαία συνθήκη έτσι ώστε μία ακολουθία σε έναν τυχαία απλά συνεκτικό τόπο να συγκλίνει προς κάποιο συνοριακό σημείο του τόπου υπό ένα αρχικά δοθέν σύνολο γωνιών.
description: The aim of the present thesis was the study of several geometric problems concerning the broad area of Complex Analysis. The main axis around which the thesis unfolded was the field of semigroups of holomorphic functions. We presented the basic notions and properties with regard to semigroups and proceeded to their classification. Next, we examined whether parabolic semigroups of positive hyperbolic step satisfy a condition relevant to the tangential speed of their orbits. Then, we worked with the backward orbit of a compact set under a semigroup by studying the asymptotic behavior of certain quantities of Potential Theory, such as harmonic measure. Finally, we searched for a necessary and sufficient condition in order for a sequence in an arbitrary simply connected domain to converge to some boundary point of the domain by a given set of angles.
Strong suppression of superconductivity by divalent Ytterbium Kondo-holes in CeCoIn_5
Creators: name: Shimozawa, M.
name: Watashige, T.
name: Yasumoto, S.
name: Mizukami, Y.
name: Nakamura, M.
name: Shishido, H.
name: Goh, S. K.
name: Terashima, T.
name: Shibauchi, T.
name: Matsuda, Y.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: To study the nature of partially substituted Yb-ions in a Ce-based Kondo lattice, we fabricated high quality Ce_{1-x}Yb_xCoIn_5 epitaxial thin films using molecular beam epitaxy. We find that the Yb-substitution leads to a linear decrease of the unit cell volume, indicating that Yb-ions are divalent forming Kondo-holes in Ce_{1-x}Yb_xCoIn_5, and leads to a strong suppression of the superconductivity and Kondo coherence. These results, combined with the measurements of Hall effect, indicate that Yb-ions act as nonmagnetic impurity scatters in the coherent Kondo lattice without serious suppression of the antiferromagnetic fluctuations. These are in stark contrast to previous studies performed using bulk single crystals, which claim the importance of valence fluctuations of Yb-ions. The present work also highlights the suitability of epitaxial films in the study of the impurity effect on the Kondo lattice.
description: 5 pages, 4 figures
Rare regions of the Susceptible Infected Susceptible model on Barabási-Albert networks
Creators: name: Ódor, Géza
Publisher: name: arXiv
Year: 2013
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: I extend a previous work to Susceptible-Infected-Susceptible (SIS) models on weighted Barabási-Albert scale-free networks. Numerical evidence is provided that phases with slow, power-law dynamics emerge as the consequence of quenched disorder and tree topologies studied previously with the Contact Process. I compare simulation results with spectral analysis of the networks and show that the quenched mean-field (QMF) approximation provides a reliable, relatively fast method to explore activity clustering. This suggests that QMF can be used for describing rare-region effects due to network inhomogeneities. Finite size study of the QMF shows the expected disappearance of the epidemic threshold $λ_c$ in the thermodynamic limit and an inverse participation ratio $\sim 0.25$, meaning localization in case of disassortative weight scheme. Contrary, for the multiplicative weights and the unweighted trees this value vanishes in the thermodynamic limit, suggesting only weak rare region effects in agreement with the dynamical simulations. Strong corrections to the mean-field behavior in case of disassortative weights explains the concave shape of the order parameter $ρ(λ)$ at the transition point. Application of this method to other models may reveal interesting rare-region effects, Griffiths Phases as the consequence of quenched topological heterogeneities.
description: 6 pages, 4 figures, 1 table, accepted version to appear in PRE
"Direct" observations of ice shelf basal melt rates (WP3 EO Workshop)
Creators: name: Nicholls, Keith
Publisher: name: Zenodo
Year: 2023

description: This presentation was held at the OCEAN:ICE This presentation was held at the OCEAN:ICE WP3 EO Workshop exploring Antarctic fluxes in observations and climate and ice sheet models. The workshop took place in Copenhagen, Denmark from the 23rd to 24th of May in 2023. Keith Nicholls delivered this presentation on May 23rd, 2023 during Session 1 of the workshop, Antarctic surface datasets from in-situ and Earth Observations.
The distinguishable cluster approximation
Creators: name: Kats, Daniel
name: Manby, Frederick R.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: A new method that accurately describes strongly correlated states and captures dynamical correlation is presented. It is derived as a modification of coupled-cluster theory with single and double excitations (CCSD) through consideration of particle distinguishability between dissociated fragments, whilst retaining the key desirable properties of particle-hole symmetry, size extensivity, invariance to rotations within the occupied and virtual spaces, and exactness for two-electron subsystems. The resulting method called the distinguishable cluster approximation, smoothly dissociates difficult cases such as the nitrogen molecule, with the modest N^6 computational cost of CCSD. Even for molecules near their equilibrium geometries, the new model outperforms CCSD. It also accurately describes the massively correlated states encountered when dissociating hydrogen lattices, a proxy for the metal-insulator transition, and the fully dissociated system is treated exactly.
13CO and C18O J=2-1 mapping of the environment of the Class 0 protostellar core SMM 3 in Orion B9
Creators: name: Miettinen, Oskari
Publisher: name: arXiv
Year: 2012
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We attempt to achieve a better understanding of the gas distribution and velocity field around the deeply embedded Class 0 protostar SMM 3 in the Orion B9 star-forming region. Using the APEX 12-m telescope, we mapped the line emission from the J=2-1 rotational transition of two CO isotopologues, 13CO and C18O, over a 4' x 4' region around Orion B9/SMM 3. Both the 13CO and C18O lines exhibit two well separated velocity components at about 1.3 and 8.7 km/s. The emission of both CO isotopologues is more widely distributed than the submillimetre dust continuum emission as probed by LABOCA. The LABOCA 870-micron peak position of SMM 3 is devoid of strong CO isotopologue emission, which is consistent with our earlier detection of strong CO depletion in the source. No signatures of a large-scale outflow were found towards SMM 3. The 13CO and C18O emission seen at ~1.3 km/s is concentrated into a single clump-like feature at the eastern part of the map. The peak H2 column density towards a C18O maximum of the low-velocity component is estimated to be ~10^22 cm-2. A velocity gradient was found across both the 13CO and C18O maps. Interestingly, SMM 3 lies on the border of this velocity gradient. The 13CO and C18O emission at ~1.3 km/s is likely to originate from the "low-velocity part" of Orion B. Our analysis suggests that it contains high density gas, which conforms to our earlier detection of deuterated species at similarly low radial velocities. The sharp velocity gradient in the region might represent a shock front resulting from the feedback from the nearby expanding HII region NGC 2024. The formation of SMM 3, and possibly of the other members of Orion B9, might have been triggered by this feedback.
description: 11 pages, 9 figures, and 2 tables. Accepted for publication in Astronomy and Astrophysics
Stellar haloes of simulated Milky Way-like galaxies: Chemical and kinematic properties
Creators: name: Tissera, P. B.
name: Scannapieco, C.
name: Beers, T.
name: Carollo, D.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the chemical and kinematic properties of the diffuse stellar haloes of six simulated Milky Way-like galaxies from the Aquarius Project. Binding energy criteria are adopted to defined two dynamically distinct stellar populations: the diffuse inner and outer haloes, which comprise different stellar sub-populations with particular chemical and kinematic characteristics. Our simulated inner- and outer-halo stellar populations have received contributions from debris stars (formed in sub-galactic systems while they were outside the virial radius of the main progenitor galaxies) and endo-debris stars (those formed in gas-rich sub-galactic systems inside the dark matter haloes). The inner haloes possess an additional contribution from disc-heated stars in the range $\sim 3 - 30 %$, with a mean of $\sim 20% $. Disc-heated stars might exhibit signatures of kinematical support, in particular among the youngest ones. Endo-debris plus disc-heated stars define the so-called \insitu stellar populations. In both the inner- and outer-halo stellar populations, we detect contributions from stars with moderate to low [$α$/Fe] ratios, mainly associated with the endo-debris or disc-heated sub-populations. The observed abundance gradients in the inner-halo regions are influenced by both the level of chemical enrichment and the relative contributions from each stellar sub-population. Steeper abundance gradients in the inner-halo regions are related to contributions from the disc-heated and endo-debris stars, which tend to be found at lower binding energies than debris stars. (Abridged).
description: 12 pages, 6 figures. Accepted version. To appear in MNRAS
Additional file 1 of The risk factors of thrombus formation and the effect of catheter ablation on repetitive thrombus formation in patients with atrial fibrillation: a single center retrospective study in China
Creators: name: Liu, Huiyu
name: Lin, Mingjie
name: Han, Wenqiang
name: Ge, Junye
name: Maduray, Kellina
name: Zhong, Jingquan
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Computational Biology

description: Additional file 1: Table S1. Baseline clinical and demographic characteristics and thrombus resolution management. Table S2. Catheter ablation procedure and outcomes. Table S3. TEE and brain MRI results, post-CA in 27 patients.
SUSY into Darkness: Heavy Scalars in the CMSSM
Creators: name: Mayes, Van E.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: A survey of the mSUGRA/CMSSM parameter space is presented. The viable regions of the parameter space which satisfy all experimental constraints are identified and discussed. These constraints include a 124-127 GeV mass for the lightest CP-even Higgs and the correct relic density for cold dark matter (CDM). The superpartner spectra corresponding to these regions fall within the well-known hyperbolic branch (HB) and are found to possess sub-TeV neutralinos and charginos, with mixed Bino/Higgsino LSP's with 200-800 GeV masses. In addition, the models possess ~3-4 TeV gluino masses and heavy squarks and sleptons with masses heavier than the gluino mass. Spectra with a Higgs mass near 125 GeV and a relic density 0.109 < Ωh^2 < 0.123 are found to require EWFT at around the one-percent level, while those spectra with a much lower relic density require EWFT of only a few percent. Moreover, the SI neutralino-proton direct detection cross-sections are found to be below or within the XENON100 2-sigma limits and should be experimentally accessible now or in the near future. Finally, it is pointed-out that the supersymmetry breaking soft terms corresponding to these regions of the mSUGRA/CMSSM parameter space (m_0 proportional to m_{1/2} with m_0^2 >> m_{1/2}^2 and A_0 = -m_{1/2}) may be obtained from general flux-induced soft terms in Type IIB flux compactifications with D3 branes.
description: 17 pages, 6 figures. V2 References added. V3 minor corrections and references added
Older than you think: Using U-Pb calcite geochronology to better constrain basin-bounding fault reactivation, Inner Moray Firth Basin, W North Sea
Creators: name: Tamas, A.
name: Holdsworth, R. E.
name: Tamas, D. M.
name: Dempsey, E. D.
name: Hardman, K.
name: Bird, A.
name: Roberts, N. M. V.
name: Lee, J.
name: Underhill, J. R.
name: McCarthy, D.
name: McCaffrey, K. J. W.
name: Selby, D.
Publisher: name: Geological Society of London
Year: 2023
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Appendix D. Additional thin section microphotographs of HD1 sample showing repeated cycles of syntaxial grain growth.
Europäisches Finanzrecht: Stand - Methoden - Perspektiven
Creators: name: Kube/ Reimer, Hanno/ Ekkehart
Publisher: name: Heidelberger Beiträge zum Finanz- und Steuerrecht
Year: 2017

description: Heidelberger Beiträge zum Finanz- und Steuerrecht, Bd. 6 (2017)
Additional file 1 of Phytochrome-mediated shade avoidance responses impact the structure and composition of the bacterial phyllosphere microbiome of Arabidopsis
Creators: name: O’Rourke, James A.
name: Vincent, Stacey A.
name: Williams, Isabel E. I.
name: Gascoyne, Eleanor L.
name: Devlin, Paul F.
Publisher: name: figshare
Year: 2025
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Supplementary Material 1: Additional file 1. Spectra of light conditions used. Spectra of light conditions used in the analysis of the effect of simulated shade on the phyllosphere microbiome. W: white light, PAR 55 µmol m− 2 s− 1, R: FR 3.84; W + FR: white light supplemented with additional far red light, PAR 55 µmol m− 2 s− 1, R: FR 0.28.
Halo Modification of a Supernova Neutronization Neutrino Burst
Creators: name: Cherry, John F.
name: Carlson, J.
name: Friedland, Alexander
name: Fuller, George M.
name: Vlasenko, Alexey
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We give the first self-consistent calculation of the effect of the scattered neutrino halo on flavor evolution in supernovae. Our example case is an O-Ne-Mg core collapse supernova neutronization neutrino burst. We find that the addition of the halo neutrinos produces qualitative and quantitative changes in the final flavor states of neutrinos. We also find that the halo neutrinos produce a novel distortion of the neutrino flavor swap. Our results provide strong motivation for tackling the full multidimensional and composition-dependent aspects of this problem in the future.
description: 14 pages, 13 figures, 1 table
God may not play dice, but human observers surely do
Creators: name: de Bianchi, Massimiliano Sassoli
Publisher: name: arXiv
Year: 2012
Subjects: subject: Quantum Physics (quant-ph)
subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: We investigate indeterminism in physical observations. For this, we introduce a distinction between genuinely indeterministic (creation-1 and discovery-1) observational processes, and fully deterministic (creation-2 and discovery-2) observational processes, which we analyze by drawing a parallel between the localization properties of microscopic entities, like electrons, and the lateralization properties of macroscopic entities, like simple elastic bands. We show that by removing the randomness incorporated in certain of our observational processes, acquiring over them a better control, we also alter these processes in such a radical way that in the end they do not correspond anymore to the observation of the same property. We thus conclude that a certain amount of indeterminism must be accepted and welcomed in our physical observations, as we cannot get rid of it without also diminishing our discriminative power. We also provide in our analysis some elements of clarification regarding the non-spatial nature of microscopic entities, which we illustrate by using an analogy with the process of objectification of human concepts. Finally, the important notion of relational properties is properly defined, and the role played by indeterminism in their characterization clarified.
A simple global representation for second-order normal forms of Hamiltonian systems relative to periodic flows
Creators: name: Avendaño-Camacho, M.
name: Vallejo, J. A.
name: Vorobjev, Yu.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mathematical Physics (math-ph)
subject: Differential Geometry (math.DG)
subject: Dynamical Systems (math.DS)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 53D17, 53-04 (Primary) 70F15 (Secondary)

description: We study the determination of the second-order normal form for perturbed Hamiltonians $H_ε=H_0 +εH_1 +\frac{ε^2}{2} H_2$, relative to the periodic flow of the unperturbed Hamiltonian $H_0$. The formalism presented here is global, and can be easily implemented in any CAS. We illustrate it by means of two examples: the Hénon-Heiles and the elastic pendulum Hamiltonians.
description: Third version. A more detailed mathematical treatment, the computational part has been relegated to the documentation of the package, which can be downloaded from http://galia.fc.uaslp.mx/~jvallejo/pdynamics.zip
Redshift 6.4 host galaxies of 10^8 solar mass black holes: low star formation rate and dynamical mass
Creators: name: Willott, Chris J.
name: Omont, Alain
name: Bergeron, Jacqueline
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present ALMA observations of rest-frame far-infrared continuum and [CII] line emission in two z=6.4 quasars with black hole masses of ~10^8 M_sun. CFHQS J0210-0456 is detected in the continuum with a 1.2 mm flux of 120+/-35 microJy, whereas CFHQS J2329-0301 is undetected at a similar noise level. J2329-0301 has a star formation rate limit of <40 M_sun/yr, considerably below the typical value at all redshifts for this bolometric luminosity. By comparison with hydro simulations, we speculate that this quasar is observed at a relatively rare phase where quasar feedback has effectively shut down star formation in the host galaxy. [CII] emission is also detected only in J0210-0456. The ratio of [CII] to far-infrared luminosity is similar to that of low redshift galaxies of comparable luminosity, suggesting the previous finding of an offset in the relationships between this ratio and far-infrared luminosity at low- and high-redshift may be partially due to a selection effect from the limited sensitivity of previous observations. The [CII] line of J0210-0456 is relatively narrow (FWHM=189+/-18 km/s), indicating a dynamical mass substantially lower than expected from the local black hole - velocity dispersion correlation. The [CII] line is marginally resolved at 0.7" resolution with the blue and red wings spatially offset by 0.5" (3 kpc) and a smooth velocity gradient of 100 km/s across a scale of 6 kpc, possibly due to rotation of a galaxy-wide disk. These observations are consistent with the idea that stellar mass growth lags black hole accretion for quasars at this epoch with respect to more recent times.
description: 8 pages, 7 figures, ApJ in press, replaced with final version
Burgen in gute Hand / Verkauf u. Kauf - Verpachten
Creators: name: Redaktion, Die
Publisher: name: Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege
Year: 2017

description: -
description: Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege, Bd. 7, Nr. 2 (1966): Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege
Additional file 1 of Sedation, sleep-promotion, and non-verbal and verbal communication techniques in critically ill intubated or tracheostomized patients: results of a survey
Creators: name: Waydhas, Christian
name: Deffner, Teresa
name: Gaschler, Robert
name: Häske, David
name: Hamsen, Uwe
name: Herbstreit, Frank
name: Hierundar, Anke
name: Kumpf, Oliver
name: Rohe, Georg
name: Spiekermann, Aileen
name: Vonderhagen, Sonja
name: Waeschle, Reiner M.
name: Riessen, Reimer
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 1.
Hecke grids and congruences for weakly holomorphic modular forms
Creators: name: Ahlgren, Scott
name: Andersen, Nickolas
Publisher: name: arXiv
Year: 2013
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 11F33

description: Let $U(p)$ denote the Atkin operator of prime index $p$. Honda and Kaneko proved infinite families of congruences of the form $f|U(p) \equiv 0 \pmod{p}$ for weakly holomorphic modular forms of low weight and level and primes $p$ in certain residue classes, and conjectured the existence of similar congruences modulo higher powers of $p$. Partial results on some of these conjectures were proved recently by Guerzhoy. We construct infinite families of weakly holomorphic modular forms on the Fricke groups $Γ^*(N)$ for $N=1,2,3,4$ and describe explicitly the action of the Hecke algebra on these forms. As a corollary, we obtain strengthened versions of all of the congruences conjectured by Honda and Kaneko.
Teacher Preparation Program Models
Creators: name: States, Jack
name: cleaver, samantha
name: Detrich, Ronnie
Publisher: name: figshare
Year: 2021
Subjects: subject: Education
subject: 130313 Teacher Education and Professional Development of Educators
subject: FOS: Educational sciences

description: Teacher preparation began in the mid-19th century with the normal school, a 2-year course of study that prepared candidates for teaching. This model remained unchanged until the early 20th century, when universities created the undergraduate model, which currently predominates. Teacher candidates are required to spend 4 years obtaining a bachelor’s degree built around a prescribed course of education study. A second relatively recent modification is the 5-year credential model, requiring candidates to obtain a bachelor’s degree before beginning a 5th year of instruction in teaching. The driving force behind the postgraduate model was the belief that teachers were not respected. It was assumed that a post-bachelor’s and/or graduate degree certificate would confer greater esteem on the profession. This model is offered across the country and is mandated for all new teachers in California. A third option, the alternative credential (AC) model, arose as a solution to teacher shortages. The AC model is distinct from the traditional models in that candidates receive formal preparation coursework while already employed in the classroom. Currently, little evidence exists to support the superiority of any one method over the others.
title: Einsatz neuer Medien in der betrieblichen Ausbildung
title: Didaktisches & webdidaktisches Konzept des Forschungsvorhabens "effekt"
titleType: Subtitle
Creators: name: Salzer, Sigrid
name: Möhring-Lotsch, Nadine
name: Müller, Axel
Publisher: name: Otto-von-Guericke-Universtät, Universitätsbibliothek, Magdeburg
Year: 2010

description: Das Projekt "effekt - Verknüpfende Vermittlung von Fach- und Medienkompetenz " ist ein von der Mein Unternehmen gemeinnützigen Gesellschaft mbH initiiertes Forschungsvorhaben im Rahmen des Förderprogramms "Neue Medien in der Bildung" des Bundesministeriums für Bildung und Forschung. Mit dem Projekt soll ein Beitrag zur Erforschung und zum Einsatz digitaler Medien in der beruflichen Ausbildung geleistet werden.  Ziele des Projektes sind die Entwicklung und Erprobung eines mediengestützten Ausbildungskonzeptes, das mit Lern- und Arbeitsaufgaben sowie Aufgaben zur Leistungskontrolle und -bewertung für die betrieblichen Ausbildung in den neu geordneten Berufen Elektroniker/-in für Betriebstechnik (E.ON Avacon AG, MVB GmbH, SWM GmbH) und Fachkraft im Fahrbetrieb (MVB GmbH) ausgestaltet wird.
description: IBBP-Arbeitsbericht, Band 75, 2010
Additional file 2 of Sedation, sleep-promotion, and non-verbal and verbal communication techniques in critically ill intubated or tracheostomized patients: results of a survey
Creators: name: Waydhas, Christian
name: Deffner, Teresa
name: Gaschler, Robert
name: Häske, David
name: Hamsen, Uwe
name: Herbstreit, Frank
name: Hierundar, Anke
name: Kumpf, Oliver
name: Rohe, Georg
name: Spiekermann, Aileen
name: Vonderhagen, Sonja
name: Waeschle, Reiner M.
name: Riessen, Reimer
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 2.
Electron-phonon coupling in the conventional superconductor YNi$_2$B$_2$C at high phonon energies studied by time-of-flight neutron spectroscopy
Creators: name: Weber, F.
name: Rosenkranz, S.
name: Pintschovius, L.
name: Castellan, J. -P.
name: Osborn, R.
name: Reichardt, W.
name: Heid, R.
name: Bohnen, K. -P.
name: Goremychkin, E. A.
name: Kreyssig, A.
name: Hradil, K.
name: Abernathy, D. L.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We report an inelastic neutron scattering investigation of phonons with energies up to 159 meV in the conventional superconductor YNi$_2$B$_2$C. Using the SWEEP mode, a newly developed time-of-flight technique involving the continuous rotation of a single crystal specimen, allowed us to measure a four dimensional volume in (Q,E) space and, thus, determine the dispersion surface and linewidths of the $A_{1g}$ (~ 102 meV) and $A_u$ (~ 159 meV) type phonon modes for the whole Brillouin zone. Despite of having linewidths of $Γ= 10 meV$, $A_{1g}$ modes do not strongly contribute to the total electron-phonon coupling constant $λ$. However, experimental linewidths show a remarkable agreement with ab-initio calculations over the complete phonon energy range demonstrating the accuracy of such calculations in a rare comparison to a comprehensive experimental data set.
description: accepted for publication in PRL
Additional file 1 of Religiosity and spirituality in the prevention and management of depression and anxiety in young people: a systematic review and meta-analysis
Creators: name: Aggarwal, Shilpa
name: Wright, Judith
name: Morgan, Amy
name: Patton, George
name: Reavley, Nicola
Publisher: name: figshare
Year: 2023
Subjects: Medicine
Biotechnology
Biological Sciences not elsewhere classified
Cancer
Science Policy
Mental Health

description: Additional file 1: Appendix 1. Search terms for identifying eligible studies. Appendix 2. Region, age, gender, quality distribution of longitudinal and intervention studies. Appendix 3. Risk of bias. Appendix 4. Gender differences in associations between spirituality and religiosity with depression and anxiety. Appendix 5. Race, ethnicity and faith differences in association of spirituality and religiosity with depression and anxiety. Appendix 6. Spirituality/ Religiosity as a moderator between risk factor and depression/anxiety.
Additional file 1 of Weight variability and cardiovascular outcomes: a systematic review and meta-analysis
Creators: name: Massey, Robert J.
name: Siddiqui, Moneeza K.
name: Pearson, Ewan R.
name: Dawed, Adem Y.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy

description: Additional file 1: Appendix S1. Search Strategies. Appendix S2. Description of Emails. Appendix S3. List of Inclusion and Exclusion Criteria. Table S1. Descriptions and Definitions of Weight Variability Metrics. Table S2. Table of Study Characteristics. Table S3. Additional Table of Study Characteristics. Figure S1. Results of Per +1 SD in Weight Variability Analysis. Figure S2. Results of Degree of BMI Variability Analysis. Figure S3. Results of Ethnicity Stratification. Figure S4. Results of Diabetes Status Stratification. Figure S5. Results of Metric of Variability Stratification. Figure S6. Results of Quantile Stratification. Figure S7. Results of Previous Cardiovascular Disease Stratification. Figure S8. Results of adjustment for change in BMI or average BMI stratification. Figure S9. Results of Univariate Meta-Regression by Age. Figure S10. Egger’s Regression and Funnel Plots. Figure S11. Results of Newcastle-Ottawa Bias Analysis. Appendix S4. MOOSE Checklist. Table S4. Newcastle – Ottawa Scale Quality Assessment Results. Appendix S5. Newcastle-Ottawa Quality Assessment Scale.
Additional file 9 of PATH-SURVEYOR: pathway level survival enquiry for immuno-oncology and drug repurposing
Creators: name: Obermayer, Alyssa N.
name: Chang, Darwin
name: Nobles, Gabrielle
name: Teng, Mingxiang
name: Tan, Aik-Choon
name: Wang, Xuefeng
name: Chen, Y. Ann
name: Eschrich, Steven
name: Rodriguez, Paulo C.
name: Grass, G. Daniel
name: Meshinchi, Soheil
name: Tarhini, Ahmad
name: Chen, Dung-tsa
name: Shaw, Timothy I.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Hematology

description: Additional file 9. Supplementary Method.
The Broad Line Region in NGC 4051: An Inflow Illuminated by a 10^5 K Accretion Disk
Creators: name: Devereux, Nick
name: Heaton, Emily
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Adopting a spherically symmetric steady-state ballistic inflow as the kinematic model for the gas distribution responsible for producing the Hα emission line and a central black hole (BH) mass of 1.7 x10^6 M_sun, determined from prior reverberation mapping, leads to the following dimensions for the size of the broad line region (BLR) in NGC 4051; an inner radius ~3 lt-days and a lower limit to the outer radius ~ 475 lt-days. Thus, the previously determined reverberation size for the BLR marks just the inner radius of a much larger volume of ionized gas. The number of ionizing photons required to sustain the Hα emission line luminosity exceeds the number observed to be available from the central AGN by a factor of 3 - 4. Such a large ionizing deficit can be reconciled if the BLR is ionized by a 10^5 K accretion disk that is hidden from direct view by the high opacity of intervening H gas. A new definition is introduced for the ionization parameter that acknowledges the fact that H opacity significantly attenuates the flux of ionizing photons in the large, partially ionized, nebula surrounding the AGN. Collectively, these results have important implications for BH masses estimated using reverberation radii and the structure of the BLR inferred from velocity-delay maps.
description: v2 revised according to referee comments. Accepted for publication in ApJ, 22 April 2013
Die Bronzezeit in Bayern. Stand der Forschungen zur relativen Chronologie
Creators: name: Torbrügge, Walter
Publisher: name: Bericht der Römisch-Germanischen Kommission
Year: 2017

description: [nicht vorhanden / not available]
description: Bericht der Römisch-Germanischen Kommission, Bd. 40 (1959): Bericht der Römisch-Germanischen Kommission
Time persistency of floating particle clusters in free-surface turbulence
Creators: name: Lovecchio, Salvatore
name: Marchioli, Cristian
name: Soldati, Alfredo
Publisher: name: arXiv
Year: 2013
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We study the dispersion of light particles floating on a flat shear-free surface of an open channel in which the flow is turbulent. This configuration mimics the motion of buoyant matter (e.g. phytoplankton, pollutants or nutrients) in water bodies when surface waves and ripples are smooth or absent. We perform direct numerical simulation of turbulence coupled with Lagrangian particle tracking, considering different values of the shear Reynolds number (Reτ = 171 and 509) and of the Stokes number (0.06 < St < 1 in viscous units). Results show that particle buoyancy induces clusters that evolve towards a long-term fractal distribution in a time much longer than the Lagrangian integral fluid time scale, indicating that such clusters over-live the surface turbulent structures which produced them. We quantify cluster dynamics, crucial when modeling dispersion in free-surface flow turbulence, via the time evolution of the cluster correlation dimension.
How reliable is Zeeman Doppler Imaging without simultaneous temperature reconstruction?
Creators: name: Rosén, Lisa
name: Kochukhov, Oleg
Publisher: name: arXiv
Year: 2012
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Aims: The goal of this study is to perform numerical tests of Zeeman Doppler Imaging (ZDI) to asses whether correct reconstruction of magnetic fields is at all possible without taking temperature into account for stars in which magnetic and temperature inhomogeneities are spatially correlated. Methods: We used a modern ZDI code employing a physically realistic treatment of the polarized radiative transfer in all four Stokes parameters. We generated artificial observations of isolated magnetic spots and of magnetic features coinciding with cool temperature spots and then reconstructed magnetic and temperature distributions from these data. Results: Using Stokes I and V for simultaneous magnetic and temperature mapping for the star with a homogeneous temperature distribution yields magnetic field strengths underestimated by typically 10-15% relative to their true values. When temperature is kept constant and Stokes I is not used for magnetic mapping, the underestimation is 30-60%. At the same time, the strength of magnetic field inside cool spots is underestimated by as much as 80-95% and the spot geometry is also poorly reconstructed when temperature variations are ignored. On the other hand, the inversion quality is greatly improved when temperature variations are accounted for in magnetic mapping. When using all four Stokes parameters the reconstructed field strength inside cool spots is underestimated by 30-40% but the spot geometry can be recovered very accurately compared to the experiments with circular polarization alone. Conclusions: Reliable magnetic field reconstruction for a star with high-contrast temperature spots is essentially impossible if temperature inhomogeneities are ignored. A physically realistic line profile modeling method, which simultaneously accounts for both types of inhomogeneities, is required for meaningful ZDI of cool active stars.
A Higher Dimensional Potential Model Approach in the Study of Isgur-Wise Function for Heavy-Light Mesons
Creators: name: Roy, Sabyasachi
name: Choudhury, D. K.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Nambu-Goto action of bosonic string predicts the quark-antiquark potential to be $ V (r) = \fracγ{r} + σr +μ_0 $. The coefficient$ γ= - \frac{π(d-2)}{24} $ is the universal Lüscher coefficient of the Lüscher term $ \fracγ{r}$, which depends upon the space-time dimension `d'. We take linear term in potential as parent and Lüscher term as perturbation for the generation of wave function for meson in d space-time dimension.The wave function comes out in terms of Airy's infinite polynomial series. With this wave function in higher dimension, we then study the Isgur-Wise function for heavy-light mesons and its derivatives.
description: Accepted in Physica Scripta
Burgen und Schlösser Heft 1963/I
Creators: name: Redaktion, Die
Publisher: name: Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege
Year: 2017

description: -
description: Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege, Bd. 4, Nr. 1 (1963): Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege
Differential Higgs+jet production in bottom quark annihilation and gluon fusion
Creators: name: Wiesemann, Marius
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present recent developments concerning Higgs production in bottom quark annihilation and gluon fusion. For bottom quark annihilation, we show the transverse momentum distribution of the associated jets. Furthermore, we discuss the distribution of events into n-jet bins for n=0 and n>0 at NNLO and NLO, respectively. For gluon fusion, the quality of the heavy-top limit for differential quantities at O(α_s^4) is studied by taking into account higher order terms in the 1/m_{top} expansion.
description: 4 pages, 7 figures. Contribution to the proceedings of QCD12 - 16th International Conference in Quantum ChromoDynamics, 2-6th July 2012 (Montpellier - France)
Testing modified gravity with Planck: the case of coupled dark energy
Creators: name: Pettorino, Valeria
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The Planck collaboration has recently published maps of the Cosmic Microwave Background (CMB) radiation, in good agreement with a LCDM model, a fit especially valid for multipoles l > 40. We explore here the possibility that dark energy is dynamical and gravitational attraction between dark matter particles is effectively different from the standard one in General Relativity: this is the case of coupled dark energy models, where dark matter particles feel the presence of a fifth force, larger than gravity by a factor beta^2. We investigate constraints on the strength of the coupling beta in view of Planck data. Interestingly, we show that a non-zero coupling is compatible with data and find a likelihood peak at beta = 0.036 \pm 0.016 (Planck + WP + BAO) (compatible with zero at 2sigma). The significance of the peak increases to beta = 0.066 \pm 0.018 (Planck + WP + HST) (around 3.6sigma) when Planck is combined to Hubble Space Telescope data. This peak comes mostly from the small difference between the Hubble parameter determined with CMB measurements and the one coming from astrophysics measurements. In this sense, future observations and further tests of current observations are needed to determine whether the discrepancy is due to systematics in any of the datasets. Our aim here is not to claim new physics but rather to show how Planck data can be used to provide information on dynamical dark energy and modified gravity, allowing us to test the strength of an effective fifth force between dark matter particles with precision smaller than 2%.
description: 10 pages, 4 figures
Zu einigen Schwertscheiden aus La Tène
Creators: name: Navarro, José Maria De
Publisher: name: Bericht der Römisch-Germanischen Kommission
Year: 2017

description: [nicht vorhanden / not available]
description: Bericht der Römisch-Germanischen Kommission, Bd. 40 (1959): Bericht der Römisch-Germanischen Kommission