cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Gamma Factory at CERN -- novel research tools made of light
Creators: name: Placzek, W.
name: Abramov, A.
name: Alden, S. E.
name: Fernandez, R. Alemany
name: Antsiferov, P. S.
name: Apyan, A.
name: Bartosik, H.
name: Bessonov, E. G.
name: Biancacci, N.
name: Bieron, J.
name: Bogacz, A.
name: Bosco, A.
name: Bruce, R.
name: Budker, D.
name: Cassou, K.
name: Castelli, F.
name: Chaikovska, I.
name: Curatolo, C.
name: Czodrowski, P.
name: Derevianko, A.
name: Dupraz, K.
name: Dutheil, Y.
name: Dzierzega, K.
name: Fedosseev, V.
name: Martinez, N. Fuster
name: Gibson, S. M.
name: Goddard, B.
name: Gorzawski, A.
name: Hirlander, S.
name: Jowett, J.
name: Kersevan, R.
name: Kowalska, M.
name: Krasny, M. W.
name: Kroeger, F.
name: Lamont, M.
name: Lefevre, T.
name: Manglunki, D.
name: Marsh, B.
name: Martens, A.
name: Molson, J.
name: Nutarelli, D.
name: Nevay, L. J.
name: Petrenko, A.
name: Petrillo, V.
name: Radaelli, S.
name: Pustelny, S.
name: Rochester, S.
name: Sapinski, M.
name: Schaumann, M.
name: Serafini, L.
name: Shevelko, V. P.
name: Stoehlker, T.
name: Surzhikov, A.
name: Tolstikhina, I.
name: Velotti, F.
name: Weber, G.
name: Wu, Y. K.
name: Yin-Vallgren, C.
name: Zanetti, M.
name: Zimmermann, F.
name: Zolotorev, M. S.
name: Zomer, F.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: We discuss the possibility of creating novel research tools by producing and storing highly relativistic beams of highly ionised atoms in the CERN accelerator complex, and by exciting their atomic degrees of freedom with lasers to produce high-energy photon beams. Intensity of such photon beams would be by several orders of magnitude higher than offered by the presently operating light sources, in the particularly interesting gamma-ray energy domain of 0.1-400 MeV. In this energy range, the high-intensity photon beams can be used to produce secondary beams of polarised electrons, polarised positrons, polarised muons, neutrinos, neutrons and radioactive ions. New research opportunities in a wide domain of fundamental and applied physics can be opened by the Gamma Factory scientific programme based on the above primary and secondary beams.
description: 12 pages; presented by W. Placzek at the XXV Cracow Epiphany Conference on Advances in Heavy Ion Physics, 8-11 January 2019, Cracow, Poland
title: Braunschweigisches Jahrbuch Band 43. 1962
Creators: name: :None
Publisher: name: Waisenhaus-Buchdruckerei
Year: 1962
Subjects: subject: Brunsvicensien der Universitätsbibliothek Braunschweig
subject: Braunschweigisches Jahrbuch
subject: 90

description: Jahrbücher für Landesgeschichte des Braunschweigischen Geschichtsvereins, vol. 43. 1962
Additional file 1: of Influence of seasonal variation on reported filarial attacks among people living with lymphedema in Ghana
Creators: name: Kwarteng, Alexander
name: Yarhands Arthur
name: Yamba, John
name: Sylverken, Augustina
name: Kini, Priscilla
name: Ahuno, Samuel
name: Owusu-Dabo, Ellis
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Study questionnaires. The reported incidence of filarial attacks among lymphedema patients in the study communities were assessed using the structured questionnaire. The questionnaire was based on authorsâ own constructs. (DOCX 93 kb)
Megarhabda Viswajyothi & Clark 2022, gen. nov.
Creators: name: Viswajyothi, Keezhpattillam
name: Clark, Shawn M.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Megarhabda

description: Genus Megarhabda gen. nov.
urn:lsid:zoobank.org:act: 1A56949E-BD82-4D21-969D-0374649544B6
Type species
Trirhabda obscurovittata Jacoby, 1886, by present designation.
Diagnosis
This genus is quite different from Trirhabda LeConte, 1865 (the genus in which the single named species of Megarhabda gen. nov. was previously placed). Among other things, the pronotum of Megarhabda is very short (about 2.5 times as broad as long). In this respect, the new genus is similar to Derospidea, but differs in the larger pronotal depressions and the more broadly explanate lateral pronotal margins (Fig. 192). See the following key for additional diagnostic characters.
Etymology
The genus name ‘ Megarhabda ’ suggests a relationship to Trirhabda, but with unusually large size. It should be treated as a female noun.
Remarks
This genus includes a single named species, M. obscurovittata (Jacoby, 1886), which occurs from Guatemala to Panama, but an undescribed species from Guatemala and Mexico also belongs here. See Fig. 14 for a habitus photograph.
description: Published as part of Viswajyothi, Keezhpattillam & Clark, Shawn M., 2022, New World genera of Galerucinae Latreille, 1802 (tribes Galerucini Latreille, 1802, Metacyclini Chapuis, 1875, and Luperini Gistel, 1848): an annotated list and identification key (Coleoptera: Chrysomelidae), pp. 1-102 in European Journal of Taxonomy 842 on pages 5-6, DOI: 10.5852/ejt.2022.842.1945, http://zenodo.org/record/7222499
Exact solution of a many body problem with nearest and next-nearest neighbour interactions
Creators: name: Basu-Mallick, B.
name: Kundu, Anjan
Publisher: name: arXiv
Year: 2000
Subjects: subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Recently a partially solvable many-body problem with nearest and next-nearest neighbour interactions is proposed [cond-mat/9904121]. We show that by adding a suitably chosen momentum dependent nearest neighbour interaction, such a model can be converted into an integrable system with Lax operator formulation and related conserved quantities. We also solve the eigenvalue problem for the model exactly and as a byproduct obtain some identities involving associated Laguerre polynomials.
description: Latex, 6 pages, no figure
On the statistics of resonances and non-orthogonal eigenfunctions in a model for single-channel chaotic scattering
Creators: name: Fyodorov, Y. V.
name: Mehlig, B.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We describe analytical and numerical results on the statistical properties of complex eigenvalues and the corresponding non-orthogonal eigenvectors for non-Hermitian random matrices modeling one-channel quantum-chaotic scattering in systems with broken time-reversal invariance.
description: 4 pages, 2 figures
title: Braunschweigisches Jahrbuch Band 44. 1963
Creators: name: :None
Publisher: name: Waisenhaus-Buchdruckerei
Year: 1963
Subjects: subject: Brunsvicensien der Universitätsbibliothek Braunschweig
subject: Braunschweigisches Jahrbuch
subject: 90

description: Jahrbücher für Landesgeschichte des Braunschweigischen Geschichtsvereins, vol. 44. 1963
Stochastic Hysteresis and Resonance in a Kinetic Ising System
Creators: name: Sides, S. W.
name: Rikvold, P. A.
name: Novotny, M. A.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Chaotic Dynamics (nlin.CD)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study hysteresis for a two-dimensional, spin-1/2, nearest-neighbor, kinetic Ising ferromagnet in an oscillating field, using Monte Carlo simulations and analytical theory. Attention is focused on small systems and weak field amplitudes at a temperature below $T_{c}$. For these restricted parameters, the magnetization switches through random nucleation of a single droplet of spins aligned with the applied field. We analyze the stochastic hysteresis observed in this parameter regime, using time-dependent nucleation theory and the theory of variable-rate Markov processes. The theory enables us to accurately predict the results of extensive Monte Carlo simulations, without the use of any adjustable parameters. The stochastic response is qualitatively different from what is observed, either in mean-field models or in simulations of larger spatially extended systems. We consider the frequency dependence of the probability density for the hysteresis-loop area and show that its average slowly crosses over to a logarithmic decay with frequency and amplitude for asymptotically low frequencies. Both the average loop area and the residence-time distributions for the magnetization show evidence of stochastic resonance. We also demonstrate a connection between the residence-time distributions and the power spectral densities of the magnetization time series. In addition to their significance for the interpretation of recent experiments in condensed-matter physics, including studies of switching in ferromagnetic and ferroelectric nanoparticles and ultrathin films, our results are relevant to the general theory of periodically driven arrays of coupled, bistable systems with stochastic noise.
description: 35 pages. Submitted to Phys. Rev. E Minor revisions to the text and updated references
Additional file 1 of Photoluminescent carbon dots (PCDs) from sour apple: a biocompatible nanomaterial for preventing UHMWPE wear-particle induced osteolysis via modulating Chemerin/ChemR23 and SIRT1 signaling pathway and its bioimaging application
Creators: name: Li, Xiang
name: Lu, Yang
name: Li, Jiarui
name: Zhou, Shengji
name: Wang, Yuxin
name: Li, Liangping
name: Zhao, Fengchao
Publisher: name: figshare
Year: 2022
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Fig. S1. Phytochemical analysis of sour apple peel extract using GC-MS analysis. Fig. S2 XRD spectrum of sour apple peel extract. Fig. S3. C1s XPS spectrum of as-prepared PCDs. Fig. S4 N1s XPS spectrum of as-prepared PCDs. Fig. S5 O1s XPS spectrum of as-prepared PCDs. Fig. S6 Graph representing the cell viability of BMMs in the presence of different concentrations of PCDs. The cell viability was measured by CCK-8 assay. Values are presented as means ± SD from three independent experiments. * = P < 0.05 compared to control. Fig. S7 Graph representing the DPPH scavenging activity, which reveals the antioxidant property of synthesized PCDs. Values are presented as means ± SD from three independent experiments. * = P < 0.05 compared to control. Fig. S8 Graph representing the scavenging activity of PCDs on other biological ROS radicals such as H2O2, •OH, and O2•− radicals. Values are presented as means ± SD from three independent experiments. * = P < 0.05 compared to control. Fig. S9 The expression of pro-inflammatory cytokines (TNF-α, IL-1β, and IL-6) in BMMs that treated with PCDs before being stimulated with UHMWPE for 3 days. Values are presented as means ± SD from three independent experiments. * = P < 0.05 compared to control; # = P < 0.05 compared to UHMWPE-treated group. Table S1 Sequences of primers used in the present study.
Available options for the determination of ultra trace elements in pristine environments
Creators: name: Hua, Timothy
Publisher: name: The University of British Columbia
Year: 2010

description: There are many key factors that require consideration when trying to successfully determine elemental concentrations at ultra-low levels. Some of these processes include: sample collection, preservation, preparation and the consideration of the choice of instrumental technique for analysis. These all must be taken into account in order to ensure the highest quality and accuracy of the resulting data. This paper will discuss some of the options available for advanced contamination control as well as analytical techniques available for reporting extremely low detection limits. Instrumentation such as high resolution inductively coupled plasma mass spectrometry (HR-ICPMS) and hydride generation atomic fluorescence spectrometry (HG-AFS) will be discussed. High resolution ICPMS coupled with a clean working environment and procedures has shown through experimental data that for baseline monitoring work, where samples are relatively free of interferences, that extremely low detection limits are accurately achievable to the low parts per trillion levels for many elements including, cadmium, arsenic and selenium. The versatility of high resolution ICPMS has also been extended to biological and seawater testing along with numerous other applications. Hydride generation AFS has also been demonstrated to be capable of accurate measurements to the low parts per trillion levels for selenium and arsenic. This technology also has the added benefit of being able to measure to these levels in the presence of high chloride concentrations.
The case for two-dimensional galaxy-galaxy lensing
Creators: name: Dvornik, Andrej
name: Zoutendijk, Sebastiaan L.
name: Hoekstra, Henk
name: Kuijken, Konrad
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We revisit the performance and biases of the two-dimensional approach to galaxy-galaxy lensing. This method exploits the information for the actual positions and ellipticities of source galaxies, rather than using only the ensemble properties of statistically equivalent samples. We compare the performance of this method with the traditionally used one-dimensional tangential shear signal on a set of mock data that resemble the current state-of-the-art weak lensing surveys. We find that under idealised circumstances the confidence regions of joint constraints for the amplitude and scale parameters of the NFW model in the two-dimensional analysis can be more than three times tighter than the one-dimensional results. Moreover, this improvement depends on the lens number density and it is larger for higher densities. We compare the method against the results from the hydrodynamical EAGLE simulation in order to test for possible biases that might arise due to lens galaxies being missed, and find that the method is able to return unbiased estimates of halo masses when compared to the true properties of the EAGLE galaxies. Because of its advantage in high galaxy density areas, the method is especially suitable for studying the properties of satellite galaxies in clusters of galaxies.
description: 9 pages, 7 figures, accepted for publication in A&A
Additional file 1: of The STELLAR trial protocol: a prospective multicentre trial for Richterâ s syndrome consisting of a randomised trial investigation CHOP-R with or without acalabrutinib for newly diagnosed RS and a single-arm platform study for evaluation of novel agents in relapsed disease
Creators: name: Appleby, Niamh
name: Eyre, Toby
name: Cabes, Maite
name: Jackson, Aimee
name: Boucher, Rebecca
name: Yates, Francesca
name: Fox, Sonia
name: Rawstron, Andrew
name: Hillmen, Peter
name: Schuh, Anna
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 60506 Virology

description: Table S1. Power calculations (posterior probability) for Platform Cohort 1: Progressive RS following chemo-immunotherapy. (DOCX 15 kb)
Asplenium theciferum Mett.
Creators: name: Zhou, Ya-Dong
name: Mwachala, Geoffrey
name: Hu, Guang-Wan
name: Wang, Qing-Feng
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Aspleniaceae
Asplenium
Asplenium theciferum

description: Asplenium theciferum (Kunth) Mett.  —
Habit: Fern.
Habitat: LMWF, BZ; up to 2 800 m. Distribution: II.
 Voucher: Naro Moru Track, 18 Jun. 2010, Kamau 486 (EA, BM).
 References: Fries et al. (1924b), Schelpe (1951), Bussmann (1993, 1994, 2006), Bussmann & Beck (1995a, 1999), Agnew (2013).
description: Published as part of Zhou, Ya-Dong, Mwachala, Geoffrey, Hu, Guang-Wan & Wang, Qing-Feng, 2022, Annotated checklist of the vascular plants of Mount Kenya, East Africa, pp. 1-108 in Phytotaxa 546 (1) on page 18, DOI: 10.11646/phytotaxa.546.1.1, http://zenodo.org/record/6550464
title: Braunschweigisches Jahrbuch Band 45. 1964
Creators: name: :None
Publisher: name: Waisenhaus-Buchdruckerei
Year: 1965
Subjects: subject: Brunsvicensien der Universitätsbibliothek Braunschweig
subject: Braunschweigisches Jahrbuch
subject: 90

description: Jahrbücher für Landesgeschichte des Braunschweigischen Geschichtsvereins, vol. 45. 1964
Highest weight representations of $U_q(\hat{sl}(2|1))$ and correlation functions of the q-deformed supersymmetric t-J model
Creators: name: Yang, Wen-Li
name: Zhang, Yao-Zhong
Publisher: name: arXiv
Year: 1998
Subjects: subject: Quantum Algebra (math.QA)
subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We re-examine the level-one irreducible highest weight representations of the quantum affine superalgebra $U_q(\hat{sl}(2|1))$ and derive the characters and supercharacters associated with these representations. We calculate the exchange relations of the vertex operators and find that these vertex operators satisfy the graded Faddeev-Zamolodchikov algebra. We give an integral expression of the correlation functions of the q-deformed supersymmetric t-J model and derive the difference equations which they satisfy.
description: Some misprints corrected; RevTex 18 pages
Additional file 12 of Genome-wide identification and expression profiling of odorant receptor genes in the malaria vector Anopheles sinensis
Creators: name: He, Zhengbo
name: Yu, Zhengrong
name: He, Xingfei
name: Hao, Youjin
name: Qiao, Liang
name: Luo, Shihui
name: Zhang, Jingjing
name: Chen, Bin
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 12: Table S7. Statistical table of chemosensory genes in different expression levels.
Asplenium uhligii Hieron.
Creators: name: Zhou, Ya-Dong
name: Mwachala, Geoffrey
name: Hu, Guang-Wan
name: Wang, Qing-Feng
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Aspleniaceae
Asplenium
Asplenium uhligii

description: Asplenium uhligii Hieron.  —
Habit: Fern.
Habitat: BZ, UMF, HZ, AZ; 2 600–4 200 m. Distribution: II.
 Voucher: Sirimon Track, Alt. 2 742 m, 17 Jul. 2014, CPG 28378 (HIB, PE).
 References: Fries et al. (1924b), Schelpe (1951), Bussmann (1994), Bussmann & Beck (1995a), Beentje (2008a), Agnew (2013).
description: Published as part of Zhou, Ya-Dong, Mwachala, Geoffrey, Hu, Guang-Wan & Wang, Qing-Feng, 2022, Annotated checklist of the vascular plants of Mount Kenya, East Africa, pp. 1-108 in Phytotaxa 546 (1) on page 18, DOI: 10.11646/phytotaxa.546.1.1, http://zenodo.org/record/6550464
Gravitational wave energy budget in strongly supercooled phase transitions
Creators: name: Ellis, John
name: Lewicki, Marek
name: No, José Miguel
name: Vaskonen, Ville
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We derive efficiency factors for the production of gravitational waves through bubble collisions and plasma-related sources in strong phase transitions, and find the conditions under which the bubble collisions can contribute significantly to the signal. We use lattice simulations to clarify the dependence of the colliding bubbles on their initial state. We illustrate our findings in two examples, the Standard Model with an extra $|H|^6$ interaction and a classically scale-invariant $U(1)_{\rm B-L}$ extension of the Standard Model. The contribution to the GW spectrum from bubble collisions is found to be negligible in the $|H|^6$ model, whereas it can play an important role in parts of the parameter space in the scale-invariant $U(1)_{\rm B-L}$ model. In both cases the sound-wave period is much shorter than a Hubble time, suggesting a significant amplification of the turbulence-sourced signal. We find, however, that the peak of the plasma-sourced spectrum is still produced by sound waves with the slower-falling turbulence contribution becoming important off-peak.
description: published version
Has cosmological dark matter been observed?
Creators: name: Salgado, Marcelo
name: Sudarsky, Daniel
name: Quevedo, Hernando
Publisher: name: arXiv
Year: 1996
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: There are many indications that ordinary matter represents only a tiny fraction of the matter content of the Universe, with the remainder assumed to consist of some different type of matter, which, for various reasons must be nonluminous (dark matter). Among these indications are the inflationary scenarios which predicts that the average energy density of the Universe coincides with the so called critical value (for which the expansion never stops but the rate of expansion approaches zero at very late times). At the same time it is known (from the predictions of Big Bang nucleosynthesis on the abundances of the light elements, other than Helium) that the baryonic energy density (ordinary matter) must represent ($1.5\pm 0.5)h^{-2}$ \% (where $h$ is the Hubble constant in units of 100 km s$^{-1}$Mpc$^{-1}$) of this critical value \cite{Copi,OstStein}. We present here evidence supporting the model in which the rest of the energy density corresponds to a scalar field, which can be observed, however indirectly, in the oscillation of the effective gravitational constant, and manifests itself in the known periodicity of the number distribution of galaxies \cite{Broad,Szalay}. We analyze this model numerically and show that, the requirement that the model satisfy the bounds of light element abundances in the Universe, as predicted by Big Bang nucleosynthesis, yields a specific value for the red-shift-galactic-count oscillation amplitude compatible with that required to explain the oscillations described above \cite{hill,CritStein}, and, furthermore, yields a value for the age of the Universe compatible with standard bounds \cite{OstStein}.
description: Latex file 15 pages with no figures. Please contact M.Salgado for figures. This paper was submitted the 4 June as a letter for publication in Nature
title: Braunschweigisches Jahrbuch Band 46. 1965
Creators: name: :None
Publisher: name: Braunschweigischer Geschichtsverein
Year: 1965
Subjects: subject: Brunsvicensien der Universitätsbibliothek Braunschweig
subject: Braunschweigisches Jahrbuch
subject: 90

description: Jahrbücher für Landesgeschichte des Braunschweigischen Geschichtsvereins, vol. 46. 1965
Additional file 1: of Developing national strategies for reaching men with HIV testing services in Tanzania: results from the male catch-up plan
Creators: name: Donaldson Conserve
name: Jumanne Issango
name: Kilale, Andrew
name: Njau, Bernard
name: Nhigula, Patrick
name: Memiah, Peter
name: Mbita, Gaspar
name: Choko, Augustine T.
name: Akeen Hamilton
name: King, Gary
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Interview guide. (DOC 42 kb)
Organizational and Individual Factors Associated with Job Satisfaction and Burnout of Community Social Service Workers
Creators: Martin, Ursula
Publisher: name: Columbia University
Year: 1991
Subjects: subject: Social service
subject: Psychology
subject: FOS: Psychology

description: Job satisfaction and burnout are important areas of study because of the social and economic effects of job satisfaction and the damaging physical/psychological impacts of burnout. 200 family/children and psychiatric workers of seven social service organizations were surveyed in the spring of 1990. Instruments used were the Minnesota Satisfaction Questionnaire, the Maslach Burnout Inventory, and the Staff Burnout Scale for Health Professionals. Reported levels of job satisfaction and burnout are within normal limits. Psychiatric and family/children workers report equal job satisfaction levels, but the latter group reports significantly higher burnout levels. Both groups are particularly satisfied with the amount of praise delivered by supervisors and are reportedly dissatisfied with salary levels and promotional opportunities. Praise delivered by supervisors, promotional opportunities, and salary satisfaction are strongly associated with job satisfaction levels of both groups. Correlates of burnout for psychiatric workers are dissatisfaction with amount of praise delivered by supervisors and dissatisfaction with salary; correlates for family/children workers are limited social services employment and dissatisfaction with amount of praise. Findings have practical implications for social service administrators and practitioners. Correlates of satisfaction and burnout can be altered in order to maintain employee satisfaction and reduce burnout, absenteeism and turnover.
title: Braunschweigisches Jahrbuch Band 47. 1966
Creators: name: :None
Publisher: name: Braunschweigischer Geschichtsverein
Year: 1966
Subjects: subject: Brunsvicensien der Universitätsbibliothek Braunschweig
subject: Braunschweigisches Jahrbuch
subject: 90

description: Jahrbücher für Landesgeschichte des Braunschweigischen Geschichtsvereins, vol. 47. 1966
The gentle monster PDS 456: the kpc scale molecular outflow and its implications for QSO feedback
Creators: name: Bischetti, M.
name: Piconcelli, E.
name: Feruglio, C.
name: Fiore, F.
name: Carniani, S.
name: Brusa, M.
name: Cicone, C.
name: Vignali, C.
name: Bongiorno, A.
name: Cresci, G.
name: Mainieri, V.
name: Maiolino, R.
name: Marconi, A.
name: Nardini, E.
name: Zappacosta, L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report on the first ALMA observation of the CO(3$-$2) and rest-frame ~340 GHz continuum emission in PDS 456, which is the most luminous, radio-quiet QSO in the local Universe ($z$~0.18), with a bolometric luminosity $L_{\rm Bol}\sim10^{47}$ erg s$^{-1}$. ALMA angular resolution allowed us to map scales as small as ~700 pc. The molecular gas reservoir, traced by the core of the very bright CO(3$-$2) emission line, is distributed in a compact rotating disk, with size of ~1.3 kpc, seen close to face-on ($i$~25 deg). Fast CO(3$-$2) emission in the velocity range $v\in[-1000,+500]$ km s$^{-1}$ is also present. Specifically, we detect several blue-shifted clumps out to ~5 kpc from the nucleus, in addition to a compact ($R\lesssim1.2$ kpc), broad emission component. These components reveal a galaxy-wide molecular outflow, with a total mass $M_{\rm mol}^{\rm out}\sim2.5\times10^8$ $M_{\odot}$ and a mass outflow rate $\dot{M}_{\rm mol}\sim290$ $M_{\odot}$ yr$^{-1}$. The corresponding depletion time is ~8 Myr, shorter than the rate at which the molecular gas is converted into stars, indicating that the detected outflow is potentially able to quench star-formation in the host. The momentum flux of the molecular outflow normalised to the radiative momentum output (i.e. $L_{\rm Bol}/c$) is $\lesssim1$, comparable to that of the X-ray ultra-fast outflow (UFO) detected in PDS 456. This is at odds with the expectations for an energy-conserving expansion suggested for most of the large-scale outflows detected in low-luminosity AGN so far. We suggest three possible scenarios that may explain this observation: (i) in very luminous AGN such as our target the molecular gas phase is tracing only a fraction of the total outflowing mass; (ii) a small coupling between the shocked gas by the UFO and the host-galaxy ISM (iii) AGN radiation pressure may play an important role in driving the outflow.
description: Accepted in A&A
Filling Length in Finitely Presentable Groups
Creators: name: Gersten, S.
name: Riley, T.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Group Theory (math.GR)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 20F06 (Primary), 20F05, 20F65, 57M07 (Secondary)

description: Filling length measures the length of the contracting closed loops in a null-homotopy. The filling length function of Gromov for a finitely presented group measures the filling length as a function of length of edge-loops in the Cayley 2-complex. We give a bound on the filling length function in terms of the log of an isoperimetric function multiplied by a (simultaneously realisable) isodiametric function.
description: 10 pages, 3 figures
Dynamical System Analysis for Steep Potentials
Creators: name: Das, Sudipta
name: Banerjee, Manisha
name: Roy, Nandan
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In this work we have performed the dynamical system analysis for steep(er) exponential potentials considering different values of the steepness index $n$. We have performed the analysis using centre manifold theory as well as by employing numerical method. We have shown that in most of the cases, the higher values of steepness index corresponds to an unstable solution. We have shown that with this steep(er) potentials one can not have a phase transition from dark matter to dark energy in the past.
description: 23 pages, 33 figures, Accepted for publication in JCAP
Amauropelta bergiana Holttum
Creators: name: Zhou, Ya-Dong
name: Mwachala, Geoffrey
name: Hu, Guang-Wan
name: Wang, Qing-Feng
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Thelypteridaceae
Amauropelta
Amauropelta bergiana

description: Amauropelta bergiana (Schltdl.) Holttum  —
Habit: Fern.
Habitat: LMWF, BZ; up to 2 600 m. Distribution: II.
 Voucher: Chogoria Track, Alt. 2 572 m, 22 Jul. 2014, CPG 28575 (EA).
 References: Fries et al. (1924b), Fries & Fries (1948), Bussmann (1993, 1994), Bussmann & Beck (1995a), Verdcourt (2006), Agnew (2013).
description: Published as part of Zhou, Ya-Dong, Mwachala, Geoffrey, Hu, Guang-Wan & Wang, Qing-Feng, 2022, Annotated checklist of the vascular plants of Mount Kenya, East Africa, pp. 1-108 in Phytotaxa 546 (1) on page 18, DOI: 10.11646/phytotaxa.546.1.1, http://zenodo.org/record/6550464
Antiferromagnetic Domain Wall Control via the Surface Spin Flop in Fully Tunable Synthetic Antiferromagnets with Perpendicular Magnetic Anisotropy
Creators: name: Böhm, Benny
name: Fallarino, Lorenzo
name: Pohl, Darius
name: Rellinghaus, Bernd
name: Nielsch, Kornelius
name: Kiselev, Nikolai S.
name: Hellwig, Olav
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Antiferromagnetic (AF) domain walls have recently attracted revived attention, not only in the emerging field of AF spintronics, but also more specifically for offering fast domain wall velocities and dynamic excitations up to the terahertz frequency regime. Here we introduce an approach to nucleate and stabilize an AF domain wall in a synthetic antiferromagnet (SAF). We present experimental and micromagnetic studies of the magnetization reversal in [(Co/Pt)$_{X-1}$/Co/Ir]$_{N-1}$(Co/Pt)$_X$ SAFs, where interface induced perpendicular magnetic anisotropy (PMA) and AF interlayer exchange coupling (IEC) are completely controlled via the individual layer thicknesses within the multilayer stack. By combining strong PMA with even stronger AF IEC, the SAF reveals a collective response to an external magnetic field applied normal to the surface, and we stabilize the characteristic surface spin flop (SSF) state for an even number N of AF-coupled (Co/Pt)$_{X-1}$/Co multilayer blocks. In the SSF state our system provides a well-controlled and fully tunable vertical AF domain wall, easy to integrate as no single crystal substrates are required and with uniform 2D-magnetization in the film plane for further functionalization options, such as for example lateral patterning via lithography.
description: 15 pages, 3 figures
title: Braunschweigisches Jahrbuch Band 48. 1967
Creators: name: :None
Publisher: name: Braunschweigischer Geschichtsverein
Year: 1967
Subjects: subject: Brunsvicensien der Universitätsbibliothek Braunschweig
subject: Braunschweigisches Jahrbuch
subject: 90

description: Jahrbücher für Landesgeschichte des Braunschweigischen Geschichtsvereins, vol. 48. 1967
Miraces Jacoby 1888
Creators: name: Viswajyothi, Keezhpattillam
name: Clark, Shawn M.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Miraces

description: Genus Miraces Jacoby, 1888
Miraces Jacoby, 1888: 611
(type species Miraces aeneipennis Jacoby, 1888, by monotypy).
Halticidea Horn, 1893: 61 (type species Halticidea delata Horn, 1893, by subsequent designation of Wilcox 1965).
Remarks
This genus contains five described species. They are distributed from the southern United States through Guatemala, and in West Indies. Other species, apparently undescribed, occur throughout much of Latin America, including South America. See Fig. 18 for a habitus illustration. See Wilcox (1965) for a key to the species occurring in the United States.
description: Published as part of Viswajyothi, Keezhpattillam & Clark, Shawn M., 2022, New World genera of Galerucinae Latreille, 1802 (tribes Galerucini Latreille, 1802, Metacyclini Chapuis, 1875, and Luperini Gistel, 1848): an annotated list and identification key (Coleoptera: Chrysomelidae), pp. 1-102 in European Journal of Taxonomy 842 on page 6, DOI: 10.5852/ejt.2022.842.1945, http://zenodo.org/record/7222499
Strongly coupled quantum criticality with a Fermi surface in two dimensions: fractionalization of spin and charge collective modes
Creators: name: Sachdev, Subir
name: Morinari, Takao
Publisher: name: arXiv
Year: 2002
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We describe two dimensional models with a metallic Fermi surface which display quantum phase transitions controlled by strongly interacting critical field theories below their upper critical dimension. The primary examples involve transitions with a topological order parameter associated with dislocations in collinear spin density wave ("stripe") correlations: the gapping of the order parameter fluctuations leads to a fractionalization of spin and charge collective modes, and this transition has been proposed as a candidate for the cuprates near optimal doping. The coupling between the order parameter and long-wavelength volume and shape deformations of the Fermi surface is analyzed by the renormalization group, and a runaway flow to a non-perturbative regime is found in most cases. A phenomenological scaling analysis of simple observable properties of possible second order quantum critical points is presented, with results quite similar to those near quantum spin glass transitions and to phenomenological forms proposed by Schroeder et al. (cond-mat/0011002).
description: 16 pages, 4 figures; (v2) additional clarifying remarks
Amauropelta oppositiformis Holttum
Creators: name: Zhou, Ya-Dong
name: Mwachala, Geoffrey
name: Hu, Guang-Wan
name: Wang, Qing-Feng
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Thelypteridaceae
Amauropelta
Amauropelta oppositiformis

description: Amauropelta oppositiformis (C.Chr.) Holttum  —
Habit: Fern.
Habitat: LMWF, BZ; up to 3 000 m. Distribution: II.
 Voucher: Mount Kenya, Alt. 2 286 m, 11 Apr. 1976, Schippers K163 (WAG).
References: Bussmann (1993, 1994), Bussmann & Beck (1995a), Verdcourt (2006), Agnew (2013).
description: Published as part of Zhou, Ya-Dong, Mwachala, Geoffrey, Hu, Guang-Wan & Wang, Qing-Feng, 2022, Annotated checklist of the vascular plants of Mount Kenya, East Africa, pp. 1-108 in Phytotaxa 546 (1) on page 18, DOI: 10.11646/phytotaxa.546.1.1, http://zenodo.org/record/6550464
title: Braunschweigisches Jahrbuch Band 49. 1968
Creators: name: :None
Publisher: name: Braunschweigischer Geschichtsverein
Year: 1968
Subjects: subject: Brunsvicensien der Universitätsbibliothek Braunschweig
subject: Braunschweigisches Jahrbuch
subject: 90

description: Jahrbücher für Landesgeschichte des Braunschweigischen Geschichtsvereins, vol. 49. 1968
Who Are the Liveaboards —A Study in Bristol and Bath (MSc Thesis)
Creators: name: Tuomi, Liisa
Publisher: name: Zenodo
Year: 2006

description: Despite their increasing visibility, people who live on boats have not received an academic study of their lifestyle. A key question pertaining to the phenomenon of living aboard is why people do it and how does society perceive their life style choice.This dissertation is intended to explore the social, cultural and economic circumstances in which 'live-aboards' have evolved. This study assesses how society confronts live-aboards and what is the importance of communal ties and consumerist values in their lives. Semi-structured interviews were conducted with 14 live-aboards around Bristol and Bath. Data from the interviews was supported with field notes. The findings show that besides a lifestyle choice, living aboard can be a consequence of socioeconomic hardship. The findings verify that live-aboards encounter stereotypical thinking and discrimination from the sedentary society. Moreover, live-aboard lifestyle seem to be characterized by a sense of community and rejection of consumerist values. On this basis it is concluded that along with increasing the general awareness of live-aboards their community networks should be further supported.
Additional file 4: of DNA methylation dynamic of bone marrow hematopoietic stem cells after allogeneic transplantation
Creators: name: Trino, Stefania
name: Zoppoli, Pietro
name: Carella, Angelo
name: Laurenzana, Ilaria
name: Weisz, Alessandro
name: Memoli, Domenico
name: Calice, Giovanni
name: Rocca, Francesco La
name: Simeon, Vittorio
name: Savino, Lucia
name: Vecchio, Luigi Del
name: Musto, Pellegrino
name: Caivano, Antonella
name: Luca, Luciana De
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Hematology
subject: Plant Biology

description: Table S3. Hypo- and Hyper-methylated genes deriving from p2 t4 vs all other t4 patients comparisons. (DOC 33 kb)
Chaos Thresholds in finite Fermi systems
Creators: name: Silvestrov, P. G.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Chaotic Dynamics (nlin.CD)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The development of Quantum Chaos in finite interacting Fermi systems is considered. At sufficiently high excitation energy the direct two-particle interaction may mix into an eigen-state the exponentially large number of simple Slater-determinant states. Nevertheless, the transition from Poisson to Wigner-Dyson statistics of energy levels is governed by the effective high order interaction between states very distant in the Fock space. The concrete form of the transition depends on the way one chooses to work out the problem of factorial divergency of the number of Feynman diagrams. In the proposed scheme the change of statistics has a form of narrow phase transition and may happen even below the direct interaction threshold.
description: 9 pages, REVTEX, 2 eps figures. Enlarged version
Christella dentata Brownsey & Jermy
Creators: name: Zhou, Ya-Dong
name: Mwachala, Geoffrey
name: Hu, Guang-Wan
name: Wang, Qing-Feng
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Thelypteridaceae
Christella
Christella dentata

description: Christella dentata (Forssk.) Brownsey & Jermy  —
Habit: Fern.
Habitat: LMWF; up to 2 300 m. Distribution: I.
 Voucher: Meru Forest, Alt. 2 234 m, 7 Aug. 2015, SAJIT 003197 (HIB).
References: Bussmann (1994), Bussmann & Beck (1995a), Agnew (2013).
description: Published as part of Zhou, Ya-Dong, Mwachala, Geoffrey, Hu, Guang-Wan & Wang, Qing-Feng, 2022, Annotated checklist of the vascular plants of Mount Kenya, East Africa, pp. 1-108 in Phytotaxa 546 (1) on page 18, DOI: 10.11646/phytotaxa.546.1.1, http://zenodo.org/record/6550464
Thermal expansion coefficient and lattice anharmonicity of cubic boron arsenide
Creators: name: Chen, Xi
name: Li, Chunhua
name: Tian, Fei
name: Gamage, Geethal Amila
name: Sullivan, Sean
name: Zhou, Jianshi
name: Broido, David
name: Ren, Zhifeng
name: Shi, Li
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Recent measurements of an unusual high thermal conductivity of around 1000 W m-1 K-1 at room temperature in cubic boron arsenide (BAs) confirm predictions from theory and suggest potential applications of this semiconductor compound for thermal management applications. Knowledge of the thermal expansion coefficient and Grüneisen parameter of a material contributes both to the fundamental understanding of its lattice anharmonicity and to assessing its utility as a thermal-management material. However, previous theoretical calculations of the thermal expansion coefficient and Grüneisen parameter of BAs yield inconsistent results. Here we report the linear thermal expansion coefficient of BAs obtained from the X-ray diffraction measurements from 300 K to 773 K. The measurement results are in good agreement with our ab initio calculations that account for atomic interactions up to fifth nearest neighbours. With the measured thermal expansion coefficient and specific heat, a Grüneisen parameter of BAs of 0.84 +/- 0.09 is obtained at 300 K, in excellent agreement with the value of 0.82 calculated from first principles and much lower than prior theoretical results. Our results confirm that BAs exhibits a better thermal expansion coefficient match with commonly used semiconductors than other high-thermal conductivity materials such as diamond and cubic boron nitride.
Models for Covid-19 underreporting
Creators: name: Perez-Reche, Francisco
Publisher: name: figshare
Year: 2021
Subjects: subject: 10202 Biological Mathematics
subject: FOS: Mathematics
subject: 80204 Mathematical Software
subject: FOS: Computer and information sciences
subject: 10299 Applied Mathematics not elsewhere classified

description: Mathematica notebook and data for the article "Importance of untested infectious individuals for interventions to suppress COVID-19"
Circumgalactic Pressure Profiles Indicate Precipitation-Limited Atmospheres for $M_* \sim 10^9$$-$$10^{11.5}\,M_\odot$
Creators: name: Voit, G. M.
name: Donahue, M.
name: Zahedy, F.
name: Chen, H. -W.
name: Werk, J.
name: Bryan, G. L.
name: O'Shea, B. W.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Cosmic gas cycles in and out of galaxies, but outside of galaxies it is difficult to observe except for the absorption lines that circumgalactic clouds leave in the spectra of background quasars. Using photoionization modeling of those lines to determine cloud pressures, we find that galaxies are surrounded by extended atmospheres that confine the clouds and have a radial pressure profile that depends on galaxy mass. Motivated by observations of the universe's most massive galaxies, we compare those pressure measurements with models predicting the critical pressure at which cooler clouds start to precipitate out of the hot atmosphere and rain toward the center. We find excellent agreement, implying that the precipitation limit applies to galaxies over a wide mass range.
description: Accepted to ApJ Letters (8 pages, 4 figures)
Some spherical uniqueness theorems for multiple trigonometric series
Creators: name: Ash, J. Marshall
name: Wang, Gang
Publisher: name: arXiv
Year: 2000
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 42B05;42B99

description: We prove that if a multiple trigonometric series is spherically Abel summable everywhere to an everywhere finite function $f(x)$ which is bounded below by an integrable function, then the series is the Fourier series of $f(x)$ if the coefficients of the multiple trigonometric series satisfy a mild growth condition. As a consequence, we show that if a multiple trigonometric series is spherically convergent everywhere to an everywhere finite integrable function $f(x)$, then the series is the Fourier series of $f(x)$. We also show that a singleton is a set of uniqueness. These results are generalizations of a recent theorem of J. Bourgain and some results of V. Shapiro.
description: 33 pages
Probing tachyon kinks in Newton-Cartan background
Creators: name: Roychowdhury, Dibakar
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper, we perform a systematic analysis of tachyon condensation over string Newton-Cartan (NC) geometry by probing the background with non BPS $ Dp $ brane. We construct the \textit{finite} tachyon effective action for NC geometry and explore the dynamics associated with the tachyon kink on the world-volume of the non BPS $ Dp $ brane. We show that under certain specific assumptions, the spatial dependent tachyon condensation leads to an emerging BPS $ D(p-1) $ brane dynamics over NC background. We further compute the strees energy tensor and show the equivalence between two different $ Dp $ brane configurations in the NC limit.
description: typos fixed, version to appear in PLB