cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
High-resolution near-infrared imaging of the Orion 114-426 silhouette disk
Creators: name: McCaughrean, Mark J.
name: Chen, Hua
name: Bally, John
name: Erickson, Ed
name: Thompson, Rodger
name: Rieke, Marcia
name: Schneider, Glenn
name: Stolovy, Susan
name: Young, Erick
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the first high-resolution near-infrared images of the edge-on silhouette circumstellar disk, Orion 114-426, made using NICMOS on the Hubble Space Telescope. Images taken against the bright nebular background of the ionized hydrogen Pa$α$ line at 1.87 micron show the major axis of the disk to be approximately 20% smaller than at 0.6 micron, from which we deduce the structure of the edge of the disk. Continuum images of diffuse polar lobes above and below the plane of the disk show a morphology and evolution with wavelength consistent with predictions for reflection nebulae in a diffuse envelope with large polar cavities, surrounding a thin, massless, Keplerian disk, centered on an otherwise hidden central star. We make use of our observations and reasonable assumptions about the underlying disk structure to show that the disk mass is at least 10 earth masses and plausibly $\geq 5\times 10^{-4}$ solar masses.
description: 11 pages, 3 EPS figures, 1 EPS table, LaTeX (using AASTeX, psfig.sty). To appear in the special NICMOS/STIS ERO edition of The Astrophysical Journal (Letters), January 1998
Neutrino-electron processes in a strongly magnetized thermal plasma
Creators: name: Hardy, Stephen J.
name: Thoma, Markus H.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present a new method of calculating the rate of neutrino-electron interactions in a strong magnetic field based on finite temperature field theory. Using this method, in which the effect of the magnetic field on the electron states is taken into account exactly, we calculate the rates of all of the lowest order neutrino-electron interactions in a plasma. As an example of the use of this technique, we explicitly calculate the rate at which neutrinos and antineutrinos annihilate in a highly magnetized plasma, and compare that to the rate in an unmagnetized plasma. The most important channel for energy deposition is the gyromagnetic absorption of a neutrino-antineutrino pair on an electron or positron in the plasma ($ν\barν e^\pm\leftrightarrow e^\pm$). Our results show that the rate of annihilation increases with the magnetic field strength once it reaches a certain critical value, which is dependent on the incident neutrino energies and the ambient temperature of the plasma. It is also shown that the annihilation rates are strongly dependent on the angle between the incident particles and the direction of the magnetic field. If sufficiently strong fields exist in the regions surrounding the core of a type II supernovae or in the central engines of gamma ray bursts, these processes will lead to more efficient plasma heating mechanism than in an unmagnetized medium, and moreover, one which is intrinsically anisotropic.
description: 17 pages, 8 figures, minor corrections, references added, to be published in Phys. Rev. D
Additional file 3: of Comparative genomics reveals the distinct evolutionary trajectories of the robust and complex coral lineages
Creators: name: Ying, Hua
name: Cooke, Ira
name: Sprungala, Susanne
name: Weiwen Wang
name: Hayward, David
name: Yurong Tang
name: Huttley, Gavin
name: Ball, Eldon
name: ForĂŞt, Sylvain
name: Miller, David
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Figure S1. GC content of de novo assembled transcripts before and after PSyTrans treatment. Figure S2. GC content of mitochondrial genomes. Figure S3. Consensus phylogenetic trees estimated from GN model with node support. Figure S4. Comparison of consensus phylogenetic trees for the eight cnidarian species which are the focus of comparative analyses, estimated from the GN (A) and AA (B) models. Figure S5. Phylogenetic relationships amongst HOX-related genes in corals and anemones. Figure S6. Heatmap showing relative counts of genes that displayed significant differences between corals and sea anemones. Figure S7. Heatmap showing relative counts of genes that displayed significant differences between complex and robust corals. Figure S8. Phylogenetic relationships of HSP20 genes in corals and anemones (A) and arrangement of HSP20 genes in Porites lutea (B). Figure S9. Organisation of membrane associated carbonic anhydrase genes in Porites lutea. Figure S10. Alignment of ATP phosphoribosyltransferase (K00765) proteins. Figure S11. Phylogenetic tree of Imidazoleglycerol-phosphate dehydratase (K01693) proteins. Figure S12. Alignment of Imidazoleglycerol-phosphate dehydratase (K01693) protein sequences. (PDF 10350 kb)
Modular Invariants, Graphs and $α$-Induction for Nets of Subfactors. III
Creators: name: Böckenhauer, J.
name: Evans, D. E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we further develop the theory of $α$-induction for nets of subfactors, in particular in view of the system of sectors obtained by mixing the two kinds of induction arising from the two choices of braiding. We construct a relative braiding between the irreducible subsectors of the two ``chiral'' induced systems, providing a proper braiding on their intersection. We also express the principal and dual principal graphs of the local subfactors in terms of the induced sector systems. This extended theory is again applied to conformal or orbifold embeddings of SU(n) WZW models. A simple formula for the corresponding modular invariant matrix is established in terms of the two inductions, and we show that it holds if and only if the sets of irreducible subsectors of the two chiral induced systems intersect minimally on the set of marked vertices i.e. on the ``physical spectrum'' of the embedding theory, or if and only if the canonical endomorphism sector of the conformal or orbifold inclusion subfactor is in the full induced system. We can prove either condition for all simple current extensions of SU(n) and many conformal inclusions, covering in particular all type I modular invariants of SU(2) and SU(3), and we conjecture that it holds also for any other conformal inclusion of SU(n) as well. As a by-product of our calculations, the dual principal graph for the conformal inclusion $SU(3)_5 \subset SU(6)_1$ is computed for the first time.
description: 59 pages, latex2e; final version, minor changes
Renormalization group improvement of the effective potential in massive $ϕ^4$ theory
Creators: name: Chung, J. -M.
name: Chung, B. K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Using the method of renormalization group, we improve the two-loop effective potential of the massive $ϕ^4$ theory to obtain the next-next-to-leading logarithm correction in the $\bar{MS}$ scheme. Our result well reproduces the next-next-to-leading logarithm parts of the ordinary loop expansion result known up to the four-loop order.
description: 15 pages, 1 eps figure, RevTeX
Streamlines of the Mean Stellar Motions in Elliptical Galaxies
Creators: name: Anderson, R. F.
name: Statler, Thomas S.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The stellar velocity fields of elliptical galaxies hold clues to their dynamical structure and origin. The construction of velocity field models is greatly simplified by assuming an approximate geometrical form for the streamlines of the mean stellar motions. We test the conjecture that confocal streamlines are a valid approximation for realistic triaxial systems. We numerically integrate orbits in Schwarzschild's logarithmic potential, and fit confocal streamlines to their mean velocity fields by minimizing the RMS magnitude of the cross product between the velocity vectors and the streamlines. We find that most orbits at a given energy can be fitted by nearly identical confocal systems. There are statistically significant differences between the streamline parameters obtained for different orbit families, but the differences are small. The fitted parameters reproduce, to high accuracy, the boundary between short axis and outer long axis tubes, which is a direct measure of the triaxiality of the potential. These results strongly support efforts to obtain accurate statistical measurements of triaxiality from kinematic observations and reasonably simple velocity field models.
description: 15 pages, 4 EPS figures included in paper. Latex, uses AASTeX v4.0. To appear in Astrophys. J
Additional file 2: of Educating patient-centered, systems-aware physicians: a qualitative analysis of medical student perceptions of value-added clinical systems learning roles
Creators: name: Gonzalo, Jed
name: Wolpaw, Daniel
name: Graaf, Deanna
name: Thompson, Britta
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Appendix 2. In-Depth Interview Protocol. (DOCX 19 kb)
Neutron to Dark Matter Decay in Neutron Stars
Creators: name: Motta, T. F.
name: Guichon, P. A. M.
name: Thomas, A. W.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Recent proposals have suggested that a previously unknown decay mode of the neutron into a dark matter particle could solve the long lasting measurement problem of the neutron decay width. We show that, if the dark particle in neutron decay is the major component of the dark matter in the universe, this proposal is in disagreement with modern astro-physical data concerning neutron star masses.
description: Invited talk presented at the Conference on Particles and Cosmology at NTU Singapore, March 2018
Gravitational mass of composite systems
Creators: name: Zych, Magdalena
name: Rudnicki, Łukasz
name: Pikovski, Igor
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The equivalence principle in combination with the special relativistic equivalence between mass and energy, $E=mc^2$, is one of the cornerstones of general relativity. However, for composite systems a long-standing result in general relativity asserts that the passive gravitational mass is not simply equal to the total energy. This seeming anomaly is supported by all explicit derivations of the dynamics of bound systems, and is only avoided after time-averaging. Here we rectify this misconception and derive from first principles the correct gravitational mass of a generic bound system in an external gravitational field. Our results clarify a lasting conundrum in general relativity and show how the weak and strong equivalence principles naturally manifest themselves for composite systems. The results are crucial for describing new effects due to the quantization of the interaction between gravity and composite systems.
description: To appear in Phys. Rev. D (accepted version; 7 pages, 1 figure)
Engytatus nicotianae
Creators: name: Usinger, Robert L.
Publisher: name: Bernice P. Bishop Museum, Bulletin 189
Year: 1946
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Engytatus
Engytatus nicotianae

description: 68. Engytatus nicotianae (Koningsberger) (fig. 17, a, b).
Leptoterna nicotianae Koningsberger, Mededeel. Lands Plantent. 64: 32, pl. 4, fig. 8, 1903.
Cyrtopeltis (?) nicotianae Kirkaldy, Linn. Soc. N. S. Wales, Proc. 33: 377, 1908. New synonymy.
Dicyphus nicotianae, Fulmek, Deli Proefstation, Bull. 25: 2, 1925.
One specimen, Piti, May 2, and two specimens, Piti, April 30, on Nicotiana, Usinger; seven specimens, Yona, May 12, on Nicotiana, Usinger.
I follow Fulmek in assuming that this is the species described by Koningsberger from Java, though the length is given as 4 mm. in the original description, whereas my series is uniformly about 3.5 mm. E. nicotianae may be separated from tenuis, aside from the distinctive male terminalia, by the dark dorsal pubescence, and by the third antenna! segment which is pale even at the base.
Judging from the damaged female types, Kirkaldy's Cyrtopeltis (?) nicotianae from Fiji belongs here. Whether Froggatt's Dicyphus tabaci (Agric. Gaz. N. S. Wales 31: 715-716, figs., 1920) from Australia belongs here or elsewhere is impossible for me to determine from the brief description. I have seen nicotianae from Noumea, New Caledonia, on Datura, F. X. Williams.
description: Published as part of Usinger, Robert L., 1946, Hemiptera Heteroptera of Guam, pp. 11-103 in Insects of Guam II, Honolulu, Hawaii :Bernice P. Bishop Museum, Bulletin 189 on pages 72-73, DOI: 10.5281/zenodo.5173934
Calibrating the metallicity of M dwarfs in wide physical binaries with F-, G-, and K- primaries - I: High-resolution spectroscopy with HERMES: stellar parameters, abundances, and kinematics
Creators: name: Montes, D.
name: González-Peinado, R.
name: Tabernero, H. M.
name: Caballero, J. A.
name: Marfil, E.
name: Alonso-Floriano, F. J.
name: Cortés-Contreras, M.
name: Hernández, J. I. González
name: Klutsch, A.
name: Moreno-Jódar, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We investigated almost 500 stars distributed among 193 binary or multiple systems made of late-F, G-, or early-K primaries and late-K or M dwarf companion candidates. For all of them, we compiled or measured coordinates, J-band magnitudes, spectral types, distances, and proper motions.With these data, we established a sample of 192 physically bound systems. In parallel, we carried out observations with HERMES/Mercator and obtained high resolution spectra for the 192 primaries and five secondaries. We used these spectra and the automatic StePar code for deriving precise stellar atmospheric parameters: Teff, log g, Vmicro, and chemical abundances for 13 atomic species, including [Fe/H]. After computing Galactocentric space velocities for all the primary stars, we performed a kinematic analysis and classified them in different Galactic populations and stellar kinematic groups of very different ages, which match our own metallicity determinations and isochronal age estimations. In particular, we identified three systems in the halo and 33 systems in the young Local Association, Ursa Major and Castor moving groups, and IC 2391 and Hyades Superclusters. We finally studied the exoplanet-metallicity relation in our 193 primaries and made a list 13 M-dwarf companions with very high metallicity that can be the targets of new dedicated exoplanet surveys. All in all, our dataset will be of great help for future works on the accurate determination of metallicity of M dwarfs.
description: accepted for publication in MNRAS, 49 pages, 11 figures and 10 tables
Additional file 1: of Time-varying predatory behavior is primary predictor of fine-scale movement of wildland-urban cougars
Creators: name: Buderman, Frances
name: Mevin Hooten
name: Alldredge, Mathew
name: Hanks, Ephraim
name: Ivan, Jacob
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Continuous-Time Markov Chain Model Details. Provides additional details on the CTMC model specification. (PDF 133 kb)
Prediction of astrometric microlensing events from Gaia DR2 proper motions
Creators: name: Klüter, J.
name: Bastian, U.
name: Demleitner, M.
name: Wambsganss, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Context: Astrometric gravitational microlensing is an excellent tool to determine the mass of stellar objects. Using precise astrometric measurements of the lensed position of a background source in combination with accurate predictions of the positions of the lens and the unlensed source it is possible to determine the mass of the lens with an accuracy of a few percent. Aims: Making use of the recently published Gaia Data Release 2 (DR2) catalogue, we want to predict astrometric microlensing events caused by foreground stars with high proper motion passing a background source in the coming decades. Methods: We selected roughly 148 000 high-proper-motion stars from Gaia DR2 with $μ_{tot} > 150\,\mathrm{mas/yr}$ as potential lenses. We then searched for background sources close to their paths. Using the astrometric parameters of Gaia DR2, we calculated the future positions of source and lens. With a nested-intervals algorithm we determined the date and separation of the closest approach. Using Gaia DR2 photometry we determined an approximate mass of the lens, which we used to calculate the expected microlensing effects. Results: We predict 3914 microlensing events caused by 2875 different lenses between 2010 and 2065, with expected shifts larger than $0.1\,\mathrm{mas}$ between the lensed and unlensed positions of the source. Of those, 513 events are expected to happen between 2014.5 - 2026.5 and might be measured by Gaia. For 127 events we also expect a magnification between $1\,\mathrm{mmag}$ and $3\,\mathrm{mag}$.
description: 11 Pages, 14 figures, 2 tables, Accepted for publication in A&A
Spatially Resolved STIS Spectroscopy of SN 1987A: Evidence for Shock Interaction with Circumstellar Gas
Creators: name: Sonneborn, G.
name: Pun, C. S. J.
name: Kimble, R. A.
name: Gull, T. R.
name: Lundqvist, P.
name: McCray, R.
name: Plait, P.
name: Boggess, A.
name: Bowers, C. W.
name: Danks, A. C.
name: Grady, J.
name: Heap, S. R.
name: Kraemer, S.
name: Lindler, D.
name: Loiacono, J.
name: Maran, S. P.
name: Moos, H. W.
name: Woodgate, B. E.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Visual and ultraviolet spatially resolved (~ 0."1) spectra of SN 1987A obtained on days 3715 and 3743 with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope show that the high-velocity SN debris is colliding with circumstellar gas. Very broad Ly-alpha emission with velocities extending to ~ +/- 20,000 km/s originates inside the inner circumstellar ring and appears to fill most of the surface area within 0."67 +/- 0."03 (0.14 pc at a distance of 50 kpc) of the ring's center. The observed Ly-alpha flux from the shocked ejecta is (1.85 +/- 0.53) 10^{-13} erg/cm2/s and (1.25 +/- 0.51) 10^{-12} erg/cm2/s after correcting for extinction. A spatially unresolved blue-shifted emission feature was discovered in H-alpha (and other lines) on the inner ring at p.a. 31 +/- 8 degree. The H-alpha emission extends to -250 km/s with no corresponding red-shifted emission. This highly localized interaction appears to be the initial contact of the supernova blast wave with an inward protrusion of the inner ring. The broad Ly-alpha emission and the `hot spot' are separate interaction phemonena associated with the reverse and forward shocks, respectively. We also find that the size of the inner ring in forbidden lines of oxygen has a dependence on ionization potential, in agreement with photoionization models of the ring.
description: 11 pages (LaTeX, aaspp4.sty), 8 figures, accepted for publication in the Astrophysical Journal Letters HST Second Servicing Mission special issue
Computation and Numerical Simulation of Focused Undulator Radiation for Optical Stochastic Cooling
Creators: name: Andorf, Matthew
name: Lebedev, Valeri
name: Jarvis, Jonathan
name: Piot, Philippe
Publisher: name: arXiv
Year: 2018
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: Optical stochastic cooling (OSC) is a promising technique for the cooling of dense particle beams. Its operation at optical frequencies enables obtaining a much larger bandwidth compared to the wellknown microwave-based stochastic cooling. In the OSC undulator radiation generated by a particle in an upstream \pickup" undulator is amplified and focused at the location of a downstream "kicker" undulator. Inside the kicker, a particle interacts with its own radiation field from the pickup. The resulting interaction produces a longitudinal kick with its value depending on the particles momentum which, when correctly phased, yields to longitudinal cooling. The horizontal cooling is achieved by introducing a coupling between longitudinal and horizontal degrees of freedom. Vertical cooling is achieved by coupling between horizontal and vertical motions in the ring. In this paper, we present formulae for computation of the corrective kick and validate them against numerical simulations performed using a wave-optics computer program.
description: 9 pages, 7 figures
ENTREPRENEURIAL JOURNEY: OVERCOMING CHALLENGES IN RECENT IMMIGRANT-OWNED SMALL BUSINESSES
Creators: name: Anderson, Robert Mitchell
Publisher: name: ZAP journals
Year: 2024
Subjects: Small Businesses
Recent Immigrants
Entrepreneurship
Challenges
Canadian Economy

description: Small businesses play a pivotal role in any economy, stimulating growth by offering goods and services and generating employment opportunities. In Canada, these enterprises have been responsible for a substantial share of job creation in the past decade, with a significant portion originating from firms employing fewer than five individuals. Moreover, the demographic landscape of Canadian entrepreneurs is evolving, with an increasing number of recent immigrants becoming small business owners. Over the years, Canada has welcomed a significant influx of immigrants, many of whom have transitioned into low-wage occupations or embarked on entrepreneurial ventures that contribute to the nation's social and economic well-being. This study focuses on recent immigrants, defined as those who have arrived in Canada within the last decade. These newcomers have ventured into a variety of small businesses, such as convenience stores, dry cleaning services, taxi companies, and beauty salons. Some sectors, like dry cleaning and convenience stores, are particularly characterized by immigrant ownership due to lower entry barriers. While anecdotal evidence has hinted at the challenges faced by recent immigrant entrepreneurs, a comprehensive and systematic exploration of these hurdles is essential. The research project's objective is to identify and prioritize the key challenges confronting small businesses owned by recent immigrants, offering a rigorous analysis of the obstacles they encounter. This study seeks to present a thorough and well-defined list of the significant challenges faced by recent immigrant small business owners, contributing valuable insights to the existing research literature.
High energy scattering amplitudes in matrix string theory
Creators: name: Wynter, Thomas
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: High energy fixed angle scattering is studied in matrix string theory. The saddle point world sheet configurations, which give the dominant contributions to the string theory amplitude, are taken as classical backgrounds in matrix string theory. A one loop fluctuation analysis about the classical background is performed. An exact treatment of the fermionic and bosonic zero modes is shown to lead to all of the expected structure of the scattering amplitude. The ten dimensional Lorentz invariant kinematical structure is obtained from the fermion zero modes, and the correct factor of the string coupling constant is obtained from the abelian gauge field zero modes. Up to a numerical factor we reproduce, from matrix string theory, the high energy limit of the tree level, four graviton scattering amplitude.
description: harvmac.tex, 55 pages, typos corrected, includes 2 figures. First part of section 3 expanded to give a clearer discussion of the justification for using a one loop calculation. Two paragraphs added to the end of section 8.1 discussing the non-Lorentz invariant factor $c$ equn 8.9. It is pointed out that the same factor occurs in string theory where it combines with the determinant to give a Lorentz Invaraint result. Other minor changes. Final version to appear in Nucl. Phys B
Anomalous effects of velocity rescaling algorithms: the flying ice cube effect revisited
Creators: name: Braun, Efrem
name: Moosavi, S. Mohamad
name: Smit, Berend
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The flying ice cube effect is a molecular dynamics simulation artifact in which the use of velocity rescaling thermostats sometimes causes the violation of the equipartition theorem, affecting both structural and dynamic properties. The reason for this artifact and the conditions under which it occurs have not been fully understood. Since the flying ice cube effect was first demonstrated, a new velocity rescaling algorithm (the CSVR thermostat) has been developed and become popular without its effects on the equipartition theorem being truly known. Meanwhile, use of the simple velocity rescaling and Berendsen thermostat algorithms has not abated but has actually continued to grow. Here, we have calculated the partitioning of the kinetic energy between translational, rotational, and vibrational modes in simulations of diatomic molecules to explicitly determine whether the equipartition theorem is violated under different thermostats and while rescaling velocities to different kinetic energy distributions. We have found that the underlying cause of the flying ice cube effect is a violation of balance leading to systematic redistributions of kinetic energy under simple velocity rescaling and the Berendsen thermostat. When velocities are instead rescaled to the canonical ensemble's kinetic energy distribution, as is done with the CSVR thermostat, the equipartition theorem is not violated, and we show that the CSVR thermostat satisfies detailed balance. The critical necessity for molecular dynamics practitioners to abandon the use of popular yet incorrect velocity rescaling algorithms is underscored with an example demonstrating that the main result of a highly-cited study is entirely due to artifacts resulting from the study's use of the Berendsen thermostat.
description: 32 pages, 13 figures; typos fixed
Coulomb corrections for Bose-Einstein correlations in whole momentum transfer region: Proposal of seamless fitting
Creators: name: Mizoguchi, M. Biyajima T.
name: Osada, T.
name: Wilk, G.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We applied an improved Coulomb correction method developed by us recently to data on identical KK-pairs production in S + Pb and p + Pb reactions at 200 GeV/c obtained by NA44 Collaboration. To analyse the whole range of the momentum transfers measured the method of "seamless fitting" has been proposed and used together with the asymptotic expansion formula for the Coulomb wave function. We found that such Coulomb corrections lead sometimes to different than previously reported (by NA44 Collaboration) interaction region and strongly influence the long range correlations.
description: LaTex file, 6 pages, hard copies of 5 figures available on request to minoru44@jpnyitp.bitnet or wilk@fuw.edu.pl (one new Fig. 5 added)
Additional file 1 of Exogenous IL-25 ameliorates airway neutrophilia via suppressing macrophage M1 polarization and the expression of IL-12 and IL-23 in asthma
Creators: name: Chang, Chenli
name: Chen, Gongqi
name: Wu, Wenliang
name: Chen, Dian
name: Chen, Shengchong
name: Gao, Jiali
name: Feng, Yuchen
name: Zhen, Guohua
Publisher: name: figshare
Year: 2023
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 1: Figure S1
“Purtroppo non abbiamo trovato molto tra le carte della nostra cara amica Gertrud Bing che si potrebbe salvare” Testo e contesto di Ernst Gombrich, Lettera a Delio Cantimori, 29 ottobre 1964
Creators: name: Centanni, Monica;
Publisher: name: La Rivista di Engramma
Year: 2020
Subjects: Ernst H Gombrich
Delio Cantimori
Gertrud Bing
Aby Warburg
Scuola Normale Superiore di Pisa Archive
The Warburg Institute Archive

description: In this paper, we present the edition of an unpublished letter from Ernst H. Gombrich to Delio Cantimori, dated 29 October 1964, kept in the Archive of the Scuola Normale Superiore in Pisa. The document, compared with other sources preserved in The Warburg Institute Archive, previously unpublished and recently made public in a volume printed in France by Philippe Despoix and Martin Treml, sheds new light on the genesis of the Intellectual Biography by Ernst H. Gombrich (London 1970) and on the role, hitherto unknown and denied by Gombrich himself, that Gertrud Bing played in the biography of Aby Warburg.
PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics
Creators: name: Edwards, Faber
name: Kendall, Emily
name: Hotchkiss, Shaun
name: Easther, Richard
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: PyUltraLight simulates the dynamics of ultralight dark matter in a non-expanding background. PyUltraLight can describe the evolution of several interacting ultralight dark matter halos or one or more halos orbiting a central, fixed Newtonian potential, the latter scenario corresponding to dwarf galaxies orbiting a massive central galaxy. We verify PyUltraLight by showing that it reproduces qualitative dynamical features of previously published simulations and demonstrate that it has excellent energy-conservation properties. PyUltraLight is implemented in a Python-based Jupyter notebook, solving the Schrodinger-Poisson equation governing ultralight scalar field dark matter dynamics in the non-relativistic regime using a symmetrised split-step pseudospectral algorithm. The notebook interface makes it simple to specify simulation parameters and visualise the resulting output but performance-critical routines are managed via calls to computationally efficient compiled libraries. PyUltraLight runs on standard desktop hardware with support for shared memory mutlithreading and is available on GitHub.
description: available at: https://github.com/auckland-cosmo/PyUltraLight
Phanera kockiana var. angustifolia Bandyop., P. P. Ghoshal & M. K. Pathak
Creators: name: Mackinder, Barbara A.
name: Clark, Ruth
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Fabales
Fabaceae
Phanera
Phanera kockiana
Phanera kockiana var. angustifolia (k. larsen & s.s. larsen) bandyop., p.p. ghoshal & m.k. pathak

description: b. Phanera kockiana var. angustifolia (K. Larsen & S.S. Larsen) Bandyop., P.P. Ghoshal & M.K. Pathak, Bangladesh J. Pl. Taxon. 19(1): 57. 2012.
Bauhinia kockiana var. angustifolia K. Larsen & S.S. Larsen, Nordic J. Bot. 13(6): 664. 1993.
DISTRIBUTION. Sarawak and Sabah [Bario, 4.ix.1985, fl., Dayang Awa S. 51084 (K)].
description: Published as part of Mackinder, Barbara A. & Clark, Ruth, 2014, A synopsis of the Asian and Australasian genus Phanera Lour. (Cercideae: Caesalpinioideae: Leguminosae) including 19 new combinations, pp. 49-68 in Phytotaxa 166 (1) on page 58, DOI: 10.11646/phytotaxa.166.1.3, http://zenodo.org/record/5138206
Publishing in the Hands of Librarians and Academics - Three Perspectives
Creators: name: Chatterji, Promita
name: Dublin, Yvonne
name: Griffin, Kevin
Publisher: name: Zenodo
Year: 2019
Subjects: Open access, library-led publishing,

description: Institution-led publishing today can take many forms. As sophisticated technologies become more user-friendly, an increasing number of digital publishing platforms are emerging. Librarians and academics are often the new vanguard in this evolving landscape. During this session, each of the panelists will present their current activities and explain how they are collaborating in order to further the cause of university-led and academic led-publishing. Yvonne Desmond, a library administrator, will describe how her library is managing an entire open access publishing program the covers a range of disciplines. She will talk about publishing strategy, managing contributors and stakeholders, and communicating successes and milestones. Kevin Griffin, an academic at the same institution, will describe how he publishes his own peer-reviewed journal-managing submissions, handling peer review, assigning content to issues, tracking readership and reporting to stakeholders. He will provide an overview of how he launched the journal and how he has made inroads within his discipline. Promita Chatterji, a technologist, will suggest what traits make for a flexible, secure, usable, and scalable publishing platform, as well as how the most successful platforms seamlessly integrate with institutional repositories.
Thermodynamics of Schwarzschild-(Anti-)de Sitter Black Holes with account of quantum corrections
Creators: name: Nojiri, Shin'ichi
name: Odintsov, Sergei D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss the quantum corrections to thermodynamics (and geometry) of S(A)dS BHs using large $N$ one-loop anomaly induced effective action for dilaton coupled matter (scalars and spinors). It is found the temperature, mass and entropy with account of quantum effects for multiply horizon SdS BH and SAdS BH what also gives the corresponding expressions for their limits: Schwarzschild and de Sitter spaces. In the last case one can talk about quantum correction to entropy of expanding Universe. The anomaly induced action under discussion corresponds to 4d formulation (s-wave approximation, 4d quantum matter is minimal one) as well as 2d formulation (complete effective action, 2d quantum matter is dilaton coupled one). Hence, most of results are given for the same gravitational background with interpretation as 4d quantum corrected BH or 2d quantum corrected dilatonic BH. Quantum aspects of thermodynamics of 4d 't Hooft BH model are also considered.
description: LaTeX file, 28 pages, some misprints are corrected
COMPARACIÓN DEL LÁSER DIODO Y LÁSER CO2 COMO  INSTRUMENTO DE CORTE EN LABIOPLASTIA DE REDUCCIÖN
Creators: name: Ajakaida, Renaud
Publisher: name: Zenodo
Year: 2024

description: Se realizó un estudio multicéntrico, prospectivo, para comparar el láser diodo 980nm y láser CO2 como instrumento de corte en labio plastia de reducción realizada en consultorios. Participaron 320 pacientes que consultaron principalmente por disconfort e inesteticismo de labios menores entre agosto 2015 hasta septiembre 2018, con edades entre 12 y 58 años. Se efectuaron adecuadas medidas de bioseguridad, previa asepsia y antisepsia, y uso de anestesia local, se efectuó labioplastia a 146 pacientes con Láser diodo 30 w (980 nm) y a 174 pacientes con Láser CO2 15 w, con potencia de 4 w, enio modo continúo para ambos equipos. Se tomaron 50 biopsias de labio al azar para estudio histopatológico. Se hizo síntesis con sutura monofilamento reabsorbible 5-0. Se efectuó seguimiento a 72 h. 7 d, 21 d, 3 m, 1 año y 2 años. En los resultados se halló que la indicación para la labio plastia más frecuente fue disconfort en 80%, seguido por inesteticismo. Los hallazgos histológicos señalaron menor daño térmico con el uso del láser diodo con respecto al láser CO2. Se reportaron complicaciones en el 3% de las pacientes, las cuales fueron, hematoma, dehiscencia de sutura, prurito y granuloma. Se concluyó que, la hipertrofia labial dependiendo del grado afecta enormemente la calidad de vida y autoestima, el instrumento de corte adecuado debe ser el que produzca menos daño a los tejidos. El láser es el instrumento ideal para realizar estas cirugías en oficina, y de ellos el láser diodo se recomienda por producir menos daño térmico, comparado con el láser CO2.
Additional file 1: of Educating patient-centered, systems-aware physicians: a qualitative analysis of medical student perceptions of value-added clinical systems learning roles
Creators: name: Gonzalo, Jed
name: Wolpaw, Daniel
name: Graaf, Deanna
name: Thompson, Britta
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Appendix 1. Patient Navigator Log Questions. (DOCX 19 kb)
Generalized polarizabilities of the proton in a constituent quark model revisited
Creators: name: Pasquini, B.
name: Scherer, S.
name: Drechsel, D.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study low-energy virtual Compton scattering off the proton within the framework of a nonrelativistic constituent quark model. The Compton tensor is divided into two separately gauge-invariant contributions. The first consists of the groundstate propagation in the direct and crossed channels together with an appropriately chosen term to satisfy gauge invariance. The residual part contains the relevant structure information characterized by the so-called generalized polarizabilities. We discuss two different schemes to obtain the generalized polarizabilities from the residual term. Explicit predictions for the generalized polarizabilities are presented for the Isgur-Karl model. Our results are compared with previous predictions in that model as well as other approaches.
description: 38 pages, 7 figures, Latex, using RevTex
Rare b-hadron decays as probe of new physics
Creators: name: Lanfranchi, Gaia
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The unexpected absence of unambiguous signals of New Physics at the TeV scale at the Large Hadron Collider puts today flavour physics at the forefront. In particular rare decays of b-hadrons represent a unique probe to challenge the Standard Model paradigm and test models of New Physics at a scale much higher than that accessible by direct searches. This article reviews the status of the field.
description: 14 pages, 8 figures
Additional file 1: of Comparative genomics reveals the distinct evolutionary trajectories of the robust and complex coral lineages
Creators: name: Ying, Hua
name: Cooke, Ira
name: Sprungala, Susanne
name: Weiwen Wang
name: Hayward, David
name: Yurong Tang
name: Huttley, Gavin
name: Ball, Eldon
name: ForĂŞt, Sylvain
name: Miller, David
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Computational Biology

description: Table S1. Summary of biological data for Galaxea fascicularis, Fungia fungites and Goniastrea aspera. Data from Veron (1986, 2000) unless otherwise noted. (DOCX 510 kb)
Leptogenesis via Varying Weinberg Operator: a Semi-Classical Approach
Creators: name: Pascoli, Silvia
name: Turner, Jessica
name: Zhou, Ye-Ling
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this Letter, we introduce leptogenesis via a varying Weinberg operator from a semi-classical perspective. This mechanism is motivated by the breaking of an underlying symmetry which triggers a phase transition that causes the coupling of the Weinberg operator to become dynamical. Consequently, a lepton anti-lepton asymmetry arises from the interference of the Weinberg operator at two different spacetime points. Using this semi-classical approach, we treat the Higgs as a background field and show a reflection asymmetry between the leptons and anti-leptons is generated in the vicinity of the bubble wall. We solve the equations of motion of the lepton and anti-lepton quasiparticles to obtain the final lepton asymmetry.
description: 7 pages, 1 figure, comments and refs added, published version
Evidence for a Disk-Jet Interaction in the Microquasar GRS 1915+105
Creators: name: Eikenberry, S. S.
name: Matthews, K.
name: Morgan, E. H.
name: Remillard, R. A.
name: Nelson, R. W.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report simultaneous X-ray and infrared (IR) observations of the Galactic microquasar GRS1915+105 using XTE and the Palomar 200-inch telescope on August 13-15, 1997 UTC. During the last two nights, the microquasar GRS 1915+105 exhibited quasi-regular X-ray/infrared (IR) flares with a spacing of $\sim 30$ minutes. While the physical mechanism triggering the flares is currently unknown, the one-to-one correspondence and consistent time offset between the X-ray and IR flares establish a close link between the two. At late times in the flares the X-ray and IR bands appear to ``decouple'', with the X-ray band showing large-amplitude fast oscillations while the IR shows a much smoother, more symmetrical decline. In at least three cases, the IR flare has returned to near its minimum while the X-rays continue in the elevated oscillatory state, ruling out thermal reprocessing of the X-ray flux as the source of IR flare. Furthermore, observations of similar IR and radio flares by Fender et al. (1997) imply that the source of the IR flux in such flares is synchrotron emission. The common rise and subsequent decoupling of the X-ray and IR flux and probable synchrotron origin of the IR emission is consistent with a scenario wherein the IR flux originates in a relativistic plasma which has been ejected from the inner accretion disk. In that case, these simultaneous X-ray/IR flares from a black-hole/relativistic-jet system are the first clear observational evidence linking of the time-dependent interaction of the jet and the inner disk in decades of quasar and microquasar studies.
description: 15 pages, incl. 3 figures. To appear in ApJ Letters
Confining Properties of Abelian(-Projected) Theories
Creators: name: Antonov, Dmitri
name: Ebert, Dietmar
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Representations of the Abelian-projected SU(2)- and SU(3)-gluodynamics in terms of the magnetic monopole currents are derived. Besides the quadratic part, the obtained effective actions contain interactions of these currents with the world-sheets of electric strings in 4D or electric vortex lines in 3D. Next, we illustrate that 3D compact QED is a small gauge boson mass limit of 3D Abelian Higgs model with external monopoles and give a physical interpretation to the confining string theory as the integral over the monopole densities. Finally, we derive the bilocal field strength correlator in the weak-field limit of 3D compact QED, which turns out to be in line with the one predicted by the Stochastic Vacuum Model.
description: 18 pages, LaTeX2e, no figures
title: Nach der Debatte um die Einsetzung einer Kommission zum Einsatz der Streitkräfte im Ausland: Vorschläge zur Novellierung des Wehrverfassungsrechts
Creators: name: Daum, Oliver
Publisher: name: Fachinformationsdienst für internationale und interdisziplinäre Rechtsforschung
Year: 2014
Subjects: subject: 340

description: JuWissBlog
Non-asymptotic assisted distillation of quantum coherence
Creators: name: Regula, Bartosz
name: Lami, Ludovico
name: Streltsov, Alexander
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We characterize the operational task of environment-assisted distillation of quantum coherence under different sets of free operations when only a finite supply of copies of a given state is available. We first evaluate the one-shot assisted distillable coherence exactly, and introduce a semidefinite programming bound on it in terms of a smooth entropic quantity. We prove the bound to be tight for all systems in dimensions 2 and 3, which allows us to obtain computable expressions for the one-shot rate of distillation, establish an analytical expression for the best achievable fidelity of assisted distillation for any finite number of copies, and fully solve the problem of asymptotic zero-error assisted distillation for qubit and qutrit systems. Our characterization shows that all relevant sets of free operations in the resource theory of coherence have exactly the same power in the task of one-shot assisted coherence distillation, and furthermore resolves a conjecture regarding the additivity of coherence of assistance in dimension 3.
description: 8 pages, 3 figures; v2: added comparison with unassisted distillation
Density-driven correlations in many-electron ensembles: theory and application for excited states
Creators: name: Gould, Tim
name: Pittalis, Stefano
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Density functional theory can be extended to excited states by means of a unified variational approach for passive state ensembles. This extension overcomes the restriction of the typical density functional approach to ground states, and offers useful formal and demonstrated practical benefits. The correlation energy functional in the generalized case acquires higher complexity than its ground state counterpart, however. Little is known about its internal structure nor how to effectively approximate it in general. Here we show that such a functional can be broken down into natural components, including what we call "state-" and "density-driven" correlations, with the former amenable to conventional approximations, and the latter being a unique feature of ensembles. Such a decomposition, summarised in eq. (6), provides us with a pathway to general approximations that are able to routinely handle low-lying excited states. The importance of density-driven correlations is demonstrated, an approximation for them is introduced and shown to be useful.