cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Extra-tidal structures around the Gaia Sausage candidate globular cluster NGC6779 (M56)
Creators: name: Piatti, Andrés E.
name: Carballo-Bello, Julio A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present results on the stellar density radial profile of the outer regions of NGC6779, a Milky Way globular cluster recently proposed as a candidate member of the Gaia Sausage structure, a merger remnant of a massive dwarf galaxy with the Milky Way. Taking advantage of the Pan-STARRS PS1 public astrometric and photometric catalogue, we built the radial profile for the outermost cluster regions using horizontal branch and main sequence stars, separately, in order to probe for different profile trends because of difference stellar masses. Owing to its relatively close location to the Galactic plane, we have carefully treated the chosen colour-magnitude regions properly correcting them by the amount of interstellar extinction measured along the line-of-side of each star, as well as cleaned them from the variable field star contamination observed across the cluster field. In the region spanning from the tidal to the Jacobi radii the resulting radial profiles show a diffuse extended halo, with an average power law slope of -1. While analysing the relationships between the Galactocentric distance, the half-mass density, the half-light radius, the slope of the radial profile of the outermost regions, the internal dynamical evolutionary stage, among others, we found that NGC6779 shows structural properties similar to those of the remaining Gaia Sausage candidate globular clusters, namely, they are massive clusters (>10^5Mo) in a moderately early dynamical evolutionary stage, with observed extra-tidal structures.
description: 8 pages, 6 figures. Accepted for publication in Monthly Noticies of the Royal Astronomical Society
Signature for local Mixmaster dynamics in U(1) symmetric cosmologies
Creators: name: Berger, Beverly K.
name: Moncrief, Vincent
Publisher: name: arXiv
Year: 2000
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Previous studies \cite{berger98a} have provided strong support for a local, oscillatory approach to the singularity in U(1) symmetric, spatially inhomogeneous vacuum cosmologies on $T^3 \times R$. The description of a vacuum Bianchi type IX, spatially homogeneous Mixmaster cosmology (on $S^3 \times R$) in terms of the variables used to describe the U(1) symmetric cosmologies indicates that the oscillations in the latter are in fact those of local Mixmaster dynamics. One of the variables of the U(1) symmetric models increases only at the end of a Mixmaster era. Such an increase therefore yields a qualitative signature for local Mixmaster dynamics in spatially inhomogeneous cosmologies.
description: 13 pages, uses RevTex, psfig
Additional file 4: of Safety and efficacy of tofacitinib for up to 9.5â years in the treatment of rheumatoid arthritis: final results of a global, open-label, long-term extension study
Creators: name: JĂźrgen Wollenhaupt
name: Eun-Bong Lee
name: Curtis, Jeffrey
name: Silverfield, Joel
name: Ketti Terry
name: Koshika Soma
name: Mojcik, Chris
name: DeMasi, Ryan
name: Strengholt, Sander
name: Kwok, Kenneth
name: Lazariciu, Irina
name: Lisy Wang
name: Cohen, Stanley
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Pharmacology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine

description: Figure S2. All-cause AEs (a) and all-cause AEs leading to discontinuation (b) over time. Baseline qualifying index study data were used for approximately 90% of patients. Database lock: March 2, 2017. AE adverse event, BID twice daily.
Palpita asiaticalis Inoue 1994
Creators: name: Singh, Navneet
name: Ranjan, Rahul
name: Talukdar, Avishek
name: Joshi, Rahul
name: Kirti, Jagbir Singh
name: Chandra, Kailash
name: Mally, Richard
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Crambidae
Palpita
Palpita asiaticalis

description: 934. Palpita asiaticalis Inoue, 1994: 98, figs 3, 4, 11, 12, 14
Type locality: Taiwan
 Distribution. Indian records: India (Zhang & Li 2005b), West and East Himalaya (Sanyal et al. 2018). Global records: China (Guizhou, Yunnan, Taiwan), Vietnam, Thailand, Nepal (Zhang & Li 2005b).
description: Published as part of Singh, Navneet, Ranjan, Rahul, Talukdar, Avishek, Joshi, Rahul, Kirti, Jagbir Singh, Chandra, Kailash & Mally, Richard, 2022, A catalogue of Indian Pyraloidea (Lepidoptera), pp. 1-423 in Zootaxa 5197 (1) on page 323, DOI: 10.11646/zootaxa.5197.1.1, http://zenodo.org/record/7252292
KIC 10001893: A pulsating sdB star with multiple trapped modes
Creators: name: Uzundag, M.
name: Baran, A. S.
name: Østensen, R. H.
name: Reed, M. D.
name: Telting, J. H.
name: Quick, B. K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: KIC 10001893 is a V1093 Her type pulsating subdwarf-B star, which was observed extensively by the Kepler spacecraft. It was a part of the survey searching for compact pulsators in the Kepler field of view. An amplitude spectrum of the star demonstrates a rich content of g-modes between 102 and 496 μHz as well as a few p-modes above 2000 μHz. In total, we found 110 frequencies. The g-mode region contains 104 frequencies, while the p-mode region contains just six, altogether indicating the hybrid nature of KIC 10001893. The main goal of our analysis was to identify the detected modes and to find some features, which will significantly help modeling of the star. We found no multiplets, which points at a pole-on orientation, however, we defined modal degrees and relative radial orders using asymptotic period spacing. Eventually, we assigned 32 dipole l = 1 and 18 quadrupole l = 2 modes. The most remarkable feature we found are trapped modes, which are clearly seen in a reduce period diagram. It is the first time that three trapped modes are detected in one pulsating sdB star. Since the more trapped modes we find, the better sounding of the stellar interior we can do, this feature provides important constraints on the physical structure of the star. Mode trapping is likely caused by the He-H transition region and therefore it provides crucial constraints for making realistic theoretical models of hot subdwarfs.
Quantization of Gravity: Yet Another Way
Creators: name: Kanatchikov, I. V.
Publisher: name: arXiv
Year: 1999
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Recently proposed quantization in field theory based on an analogue of Hamiltonian formulation which treats space and time on equal footing (the so-called De Donder-Weyl theory) is applied to General Relativity in metric variables. We formulate a covariant analogue of the Schroedinger equation for the wave function of space-time and metric variables and a supplementary ``bootstrap condition'' which enables us to incorporate classical metric geometry as an approximate notion - a result of quantum averaging - in the self-consistent with the underlying quantum dynamics way. In this sense an independence of an arbitrarily chosen metric background is ensured.
description: 8 pages, LaTeX2e. Based on author's talks at the XV Workshop on Geometrical Methods in Physics (Bialowieza, Poland, 1998) and XXXI Symposium on Mathematical Physics (Torun, Poland, 1999). To appear in Rep. Math. Phys. (2000)
A constrained Potts antiferromagnet model with an interface representation
Creators: name: Burton,, J. K.
name: Henley, C. L.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We define a four-state Potts model ensemble on the square lattice, with the constraints that neighboring spins must have different values, and that no plaquette may contain all four states. The spin configurations may be mapped into those of a 2-dimensional interface in a 2+5 dimensional space. If this interface is in a Gaussian rough phase (as is the case for most other models with such a mapping), then the spin correlations are critical and their exponents can be related to the stiffness governing the interface fluctuations. Results of our Monte Carlo simulations show height fluctuations with an anomalous dependence on wavevector, intermediate between the behaviors expected in a rough phase and in a smooth phase; we argue that the smooth phase (which would imply long-range spin order) is the best interpretation.
description: 61 pages, LaTeX. Submitted to J. Phys. A
A new coumarin from Murraya alata activates TRPV1 channel
Creators: name: Lyu, Hai-Ning
name: Wei, Ning-Ning
name: Tu, Peng-Fei
name: Wang, KeWei
name: Jiang, Yong
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified

description: One new coumarin, muralatin R, was isolated from the leaves of Murraya alata Drake (Rutaceae). Its structure was elucidated by extensive analysis of the NMR and MS data, along with the specific rotation comparison. Muralatin R was found to be capable of activating the transient receptor potential vanilloid 1 (TRPV1) channel through desensitization mechanism. The results supply reference for clarification of the therapeutic basis and mechanism of action of Murraya plants for treating psychogenic pain or somatoform pain disorders.
LHC-friendly minimal freeze-in models
Creators: name: Bélanger, G.
name: Desai, N.
name: Goudelis, A.
name: Harz, J.
name: Lessa, A.
name: No, J. M.
name: Pukhov, A.
name: Sekmen, S.
name: Sengupta, D.
name: Zaldivar, B.
name: Zurita, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We propose simple freeze-in models where the observed dark matter abundance is explained via the decay of an electrically charged and/or coloured parent particle into Feebly Interacting Massive Particles (FIMP). The parent particle is long-lived and yields a wide variety of LHC signatures depending on its lifetime and quantum numbers. We assess the current constraints and future high luminosity reach of these scenarios at the LHC from searches for heavy stable charged particles, disappearing tracks, displaced vertices and displaced leptons. We show that the LHC constitutes a powerful probe of freeze-in dark matter and can further provide interesting insights on the validity of vanilla baryogenesis and leptogenesis scenarios.
Non-linear evolution and parton distributions at LHC and THERA energies
Creators: name: Lublinsky, M.
name: Gotsman, E.
name: Levin, E.
name: Maor, U.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We suggest a new procedure for extrapolating the parton distributions from HERA energies to higher energies at THERA and LHC. The procedure suggested consists of two steps: first, we solve the non-linear evolution equation which includes the higher twists contributions, however this equation is deficient due to the low ($log(1/x)$) accuracy of our calculations. Second, we introduce a correcting function for which we write a DGLAP type linear evolution equation. We show that this correcting function is small in the whole kinematic region and decreases at low $x$. The nonlinear evolution equation is solved numerically and first estimates for the saturation scale, as well as for the value of the gluon density at THERA and LHC energies are made. We show that non-linear effects lead to damping of the gluon density by a factor of $2 ÷3$ at $x \approx 10^{-7}$.
description: 19 pages, 28 figures
Trends in Demand, Growth, and Breadth in Scientific Computing Training Delivered by a High-Performance Computing Center
Creators: name: van Zon, Ramses
name: Ponce, Marcelo
name: Spence, Erik
name: Gruner, Daniel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computers and Society (cs.CY)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences

description: We analyze the changes in the training and educational efforts of the SciNet HPC Consortium, a Canadian academic High Performance Computing center, in the areas of Scientific Computing and High-Performance Computing, over the last six years. Initially, SciNet offered isolated training events on how to use HPC systems and write parallel code, but the training program now consists of a broad range of workshops and courses that users can take toward certificates in scientific computing, data science, or high-performance computing. Using data on enrollment, attendence, and certificate numbers from SciNet's education website, used by almost 1800 users so far, we extract trends on the growth, demand, and breadth of SciNet's training program. Among the results are a steady overall growth, a sharp and steady increase in the demand for data science training, and a wider participation of 'non-traditional' computing disciplines, which has motivated an increasingly broad spectrum of training offerings. Of interest is also that many of the training initiatives have evolved into courses that can be taken as part of the graduate curriculum at the University of Toronto.
description: Presented at the Fifth Workshop on Best Practices for Enhancing HPC Training and Education (BPHTE18) @ SC18
Orphanostigma fulvistriga Swinhoe 1894
Creators: name: Singh, Navneet
name: Ranjan, Rahul
name: Talukdar, Avishek
name: Joshi, Rahul
name: Kirti, Jagbir Singh
name: Chandra, Kailash
name: Mally, Richard
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Crambidae
Orphanostigma
Orphanostigma fulvistriga

description: 916. Orphanostigma fulvistriga Swinhoe, 1894c: 206
Type locality: India, Meghalaya, Shillong
Distribution. Indian records: Shillong (Gupta 1994). Global records: unknown.
description: Published as part of Singh, Navneet, Ranjan, Rahul, Talukdar, Avishek, Joshi, Rahul, Kirti, Jagbir Singh, Chandra, Kailash & Mally, Richard, 2022, A catalogue of Indian Pyraloidea (Lepidoptera), pp. 1-423 in Zootaxa 5197 (1) on page 320, DOI: 10.11646/zootaxa.5197.1.1, http://zenodo.org/record/7252292
Shape of Mixed Micelles: Cylinders or Spheres? Theoretical Analysis
Creators: name: Kozlov, M. M.
name: Lichtenberg, D.
name: Andelman, D.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Biological Physics (physics.bio-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We develop a theoretical model for the solubilization of phospholipid bilayers by micelle-forming surfactants. Cylindrical micelles, disc-like micelles and spherical micelles are considered as alternative resultant structures. The main question addressed is what kind of micelles can be expected under various thermodynamical conditions. Our analysis is based on a theoretical model that accounts for Helfrich energy of curvature of amphiphile monolayers and for the entropy of mixing of lipids and surfactants in mixed aggregates. We conclude that for usual values of the elastic parameters of amphiphile monolayers cylindrical micelles are the most probable aggregates resulting from micellization of phospholipid by surfactants. This conclusion is consistent with available experimental data. Conditions of formation of disc-like and spherical micelles are also determined.
description: 21 pages, plain tex
Additional file 3: of Safety and efficacy of tofacitinib for up to 9.5â years in the treatment of rheumatoid arthritis: final results of a global, open-label, long-term extension study
Creators: name: JĂźrgen Wollenhaupt
name: Eun-Bong Lee
name: Curtis, Jeffrey
name: Silverfield, Joel
name: Ketti Terry
name: Koshika Soma
name: Mojcik, Chris
name: DeMasi, Ryan
name: Strengholt, Sander
name: Kwok, Kenneth
name: Lazariciu, Irina
name: Lisy Wang
name: Cohen, Stanley
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine

description: Table S2. Patient baseline demographic and disease characteristics.
Non-minimally coupled scalar fields in homogeneous universes
Creators: name: Alberghi, G. L.
name: Casadio, R.
name: Gruppuso, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The equations governing the evolution of non-minimally coupled scalar matter and the scale factor of a Robertson-Walker universe are derived from a minisuperspace action. As for the minimally coupled case, it is shown that the entire semiclassical dynamics can be retrieved from the Wheeler-DeWitt equation via the Born-Oppenheimer reduction, which properly yields the (time-time component of the) covariantly conserved energy-momentum tensor of the scalar field as the source term for gravity. However, for a generic coupling, the expectation value of the operator which evolves the matter state in time is not equal to the source term in the semiclassical Einstein equation for the scale factor of the universe and the difference between these two quantities is related to the squeezing and quantum fluctuations of the matter state. We also argue that matter quantum fluctuations become relevant in an intermediate regime between quantum gravity and semiclassical gravity and study several cases in detail.
description: REVTeX, 24 pages, 12 EPS figures included. Accepted for publication in Phys. Rev. D
Hund's metal regimes and orbital selective Mott transitions in three band systems
Creators: name: Facio, Jorge I.
name: Cornaglia, Pablo S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We analyze the electronic properties of interacting crystal field split three band systems. Using a rotationally invariant slave boson approach we analyze the behavior of the electronic mass renormalization as a function of the intralevel repulsion $U$, the Hund's coupling $J$, the crystal field splitting, and the number of electrons per site $n$. We first focus on the case in which two of the bands are identical and the levels of the third one are shifted by $Δ>0$ with respect to the former. We find an increasing quasiparticle mass differentiation between the bands, for system away from half-filling ($n=3$), as the Hubbard interaction $U$ is increased. This leads to orbital selective Mott transitions where either the higher energy band (for $4>n>3$) or the lower energy degenerate bands ($2
description: 12 pages, 8 figures
O'ZBEKISTONDA BIZNES MUHITINI YAXSHILASH VA INVESTITSION LOYIHALARDAN FOYDALANISH JARAYONLARINI TAKOMILLASHTIRISH
Creators: name: Xaqqulova, Rano
Publisher: name: Zenodo
Year: 2024

description: Mazkur maqolada O'zbekistonda biznes muhitini yaxshilash va investitsion loyihalardan foydalanish jarayonlarini takomillashtirish boʻyicha bir qancha muammolar va ularning mumkin boʻlgan yechimlari atroflicha koʻrib chiqiladi. Bundan tashqari, respublikamiz iqtisodiyotining turli sohalarida biznes muhitini yaxshilash va investitsion loyihalardan foydalanish mexanizmlari haqida batafsil bayon etilgan.
Attenuation of polarization echoes in NMR: A study of the emergence of dynamical irreversibility in many-body quantum systems
Creators: name: Levstein, Patricia R.
name: Usaj, Gonzalo
name: Pastawski, Horacio M.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The reversal of the time evolution of the local polarization in an interacting spin system involves a sign change of the effective dipolar Hamiltonian which refocuses the 'spin diffusion' process generating a polarization echo. Here, the attenuation of these echo amplitudes as a function of evolution time is presented for cymantrene and ferrocene polycrystalline samples, involving one and two five spin rings per molecule respectively. We calculate the fraction of polarization which is not refocused because only the secular part of the dipolar Hamiltonian is inverted. The results indicate that, as long as the spin dynamics is restricted to a single ring, the non-inverted part of the Hamiltonian is notable by itself to explain the whole decay of the polarization echoes. A cross over from exponential (cymantrene) to Gaussian (ferrocene) attenuation is experimentally observed. This is attributed to an increase of the relative importance of the spin dynamics, as compared with irreversible interactions, which favors dynamical irreversibility.
description: 6 pages in Revtex, 11 Postscript figures. Final version
Palpita albiantennalis Kirti 1992
Creators: name: Singh, Navneet
name: Ranjan, Rahul
name: Talukdar, Avishek
name: Joshi, Rahul
name: Kirti, Jagbir Singh
name: Chandra, Kailash
name: Mally, Richard
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Crambidae
Palpita
Palpita albiantennalis

description: 931. Palpita albiantennalis Kirti, 1992: 39, figs 1–3, 8
Type locality: Deomali, Tirap, Arunachal Pradesh
Distribution. Indian records: Arunachal Pradesh, Assam (Kirti 1992). Global Records: Not known.
description: Published as part of Singh, Navneet, Ranjan, Rahul, Talukdar, Avishek, Joshi, Rahul, Kirti, Jagbir Singh, Chandra, Kailash & Mally, Richard, 2022, A catalogue of Indian Pyraloidea (Lepidoptera), pp. 1-423 in Zootaxa 5197 (1) on page 323, DOI: 10.11646/zootaxa.5197.1.1, http://zenodo.org/record/7252292
Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors
Creators: name: Müller, B.
name: Tauris, T. M.
name: Heger, A.
name: Banerjee, P.
name: Qian, Y. -Z.
name: Powell, J.
name: Chan, C.
name: Gay, D. W.
name: Langer, N.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a suite of seven 3D supernova simulations of non-rotating low-mass progenitors using multi-group neutrino transport. Our simulations cover single star progenitors with zero-age main sequence masses between $9.6 M_\odot$ and $12.5 M_\odot$ and (ultra)stripped-envelope progenitors with initial helium core masses between $2.8 M_\odot$ and $3.5 M_\odot$. We find explosion energies between $0.1\,\mathrm{Bethe}$ and $0.4\,\mathrm{Bethe}$, which are still rising by the end of the simulations. Although less energetic than typical events, our models are compatible with observations of less energetic explosions of low-mass progenitors. In six of our models, the mass outflow rate already exceeds the accretion rate onto the proto-neutron star, and the mass and angular momentum of the compact remnant have closely approached their final value, barring the possibility of later fallback. While the proto-neutron star is still accelerated by the gravitational tug of the asymmetric ejecta, the acceleration can be extrapolated to obtain estimates for the final kick velocity. We obtain gravitational neutron star masses between $1.22 M_\odot$ and $1.44 M_\odot$, kick velocities between $11\, \mathrm{km}\, \mathrm{s}^{-1}$ and $695\, \mathrm{km}\, \mathrm{s}^{-1}$, and spin periods from $20\, \mathrm{ms}$ to $2.7\,\mathrm{s}$, which suggests that typical neutron star birth properties can be naturally obtained in the neutrino-driven paradigm. We find a loose correlation between the explosion energy and the kick velocity. There is no indication of spin-kick alignment, but a correlation between the kick velocity and the neutron star angular momentum, which needs to be investigated further as a potential point of tension between models and observations.
description: 18 pages, 14 figures. Submitted to MNRAS
Additional file 1 of Ki-67 can be used for further classification of triple negative breast cancer into two subtypes with different response and prognosis
Creators: name: Bhumsuk Keam
name: Seock-Ah Im
name: Kyung-Hun Lee
name: Sae-Won Han
name: Do-Youn Oh
name: Kim, Jee Hyun
name: Se-Hoon Lee
name: Wonshik Han
name: Kim, Dong-Wan
name: Tae-You Kim
name: Park, In Ae
name: Noh, Dong-Young
name: Heo, Dae Seog
name: Yung-Jue Bang
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1: Supplementary Table S1. Univariate and multivariate Cox regression analysis of factors associated with overall survival in triple negative breast cancer. (DOC 40 KB)
Interfaces of Modulated Phases
Creators: name: Netz, R. R.
name: Andelman, D.
name: Schick, M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Numerically minimizing a continuous free-energy functional which yields several modulated phases, we obtain the order-parameter profiles and interfacial free energies of symmetric and non-symmetric tilt boundaries within the lamellar phase, and of interfaces between coexisting lamellar, hexagonal, and disordered phases. Our findings agree well with chevron, omega, and T-junction tilt-boundary morphologies observed in diblock copolymers and magnetic garnet films.
description: 4 pages
Low power commissioning of an innovative laser beam circulator for inverse Compton scattering Gamma-ray source
Creators: name: Ndiaye, Cheikh Fall
name: Cassou, Kevin
name: Cornebise, Patrick
name: Dupraz, Kevin
name: Douillet, Denis
name: Barillec, Titouan Le
name: Magueur, Christopher
name: Martens, Aurelien
name: Nutarelli, Daniele
name: Peinaud, Yann
name: Thiebault, Alice
name: Williams, Themis
name: Zomer, Fabian
name: Beaugerard, Nicolas
name: Lacrampe, Bastien
name: Rocipon, Hervé
name: Alesini, David
name: Cardelli, Fabio
name: Falone, Antonio
name: Franzini, Giovanni
name: Gallo, Alessandro
name: Piersanti, Luca
name: Petinacci, Valerio
name: Pioli, Stefano
name: Variola, Alessandro
name: Mostacci, Andrea
name: Serafini, L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: We report on the optical commissioning of the high power laser beam circulator (LBC) for the high brightness Compton γ-ray source Extreme Light Infrastructure for Nuclear Physics. Tests aiming at demonstrating the optical performances of the LBC have been realized with a low-power pulsed laser-beam system and without electron beam. We show that, with the developed alignment and synchronization methods coming from the LBC design study presented in the Dupraz et al. paper [1], the LBC enhances the laser-beam power available at the interaction point (IP) by a factor in excess of 25. This corresponds to a potential of bringing the average laser-beam power in excess of 1 kW when the LBC is injected with the interaction point laser-beam pulse energy of 400 mJ at 100 Hz.
description: 26 pages, 37 figures
Achaea echo Walker 1858
Creators: name: Mbata, Keith J.
name: Prins, Jurate De
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Achaea
Achaea echo

description: Achaea echo Walker 1858c
COMMON NAME(S): Echo moth.
SYNONYM(S): Achaea mariaca Pl ̂tz, 1880.
IUCN STATUS: Not Evaluated (NE).
DISTRIBUTION: Burundi, Democratic Republic of Congo, Eritrea, Eswatini, Ethiopia, Ghana, Kenya, Madagascar, Mozambique, Nigeria, Réunion, Sierra Leone, South Africa, Tanzania, Zambia, Zimbabwe.
LOCALITY IN ZAMBIA: ‘Lusaka’, in Lusaka Province.
LARVAL HOSTPLANT(S): Unknown.
SOURCES: African Moths 2019; De Prins & De Prins 2022.
description: Published as part of Mbata, Keith J. & Prins, Jurate De, 2023, Annotated checklist of moths of Zambia (Insecta: Lepidoptera), pp. 1-503 in Zootaxa 5354 (1) on page 329, DOI: 10.11646/zootaxa.5354.1.1, http://zenodo.org/record/10130434
Comparative transcriptome analysis between a resistant and a susceptible Chinese cabbage in response to Hyaloperonospora brassicae
Creators: name: Zheng, Han
name: Zhang, Yihui
name: Li, Jingjuan
name: He, Lilong
name: Wang, Fengde
name: Bi, Yuping
name: Gao, Jianwei
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mental Health
subject: Plant Biology

description: Downy mildew caused by Hyaloperonosporabrassicae (H. brassicae) leads to up to 90% of the crop yield loss in Chinese cabbage in China. A transcriptome analysis was carried out between a resistant line (13-13, R) and a susceptible line (15-14, S) of Chinese cabbage in response to H. brassicae. The NOISeq method was used to find differentially expressed genes (DEGs) between these two groups and GO and KEGG were carried out to find R genes related to downy mildew response of Chinese cabbage. qRT-PCR was carried out to verify the reliability of RNA-seq expression data. A total of 3,055 DEGs were screened out from 41,020 genes and clustered into 6 groups with distinct expression patterns. A total of 87 candidate DEGs were identified by functional annotation based on GO and KEGG analysis. These candidate genes are involved in plant-pathogen interaction pathway, among which 54 and 33 DEGs were categorized into plant-pathogen interaction proteins and transcription factors, respectively. Proteins encoded by these genes have been reported to play an important role in the pattern-triggered immunity (PTI) and effector-triggered immunity (ETI) processes of disease responses in some model plants, such as Arabidopsis, rice, tobacco, and tomato. However, little is known about the mechanisms of these genes in resistance to downy mildew in Chinese cabbage. Our findings are useful for further characterization of these candidate genes and helpful in breeding resistant strains.
Numerical evolution of Brill waves
Creators: name: Garfinkle, David
name: Duncan, G. Comer
Publisher: name: arXiv
Year: 2000
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We report a numerical evolution of axisymmetric Brill waves. The numerical algorithm has new features, including (i) a method for keeping the metric regular on the axis and (ii) the use of coordinates that bring spatial infinity to the edge of the computational grid. The dependence of the evolved metric on both the amplitude and shape of the initial data is found.
description: added more discussion of results and several references
ECHO-3DHPC: Advance the performance of astrophysics simulations with code modernization
Creators: name: Bugli, Matteo
name: Iapichino, Luigi
name: Baruffa, Fabio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: We present recent developments in the parallelization scheme of ECHO-3DHPC, an efficient astrophysical code used in the modelling of relativistic plasmas. With the help of the Intel Software Development Tools, like Fortran compiler and Profile-Guided Optimization (PGO), Intel MPI library, VTune Amplifier and Inspector we have investigated the performance issues and improved the application scalability and the time to solution. The node-level performance is improved by $2.3 \times$ and, thanks to the improved threading parallelisation, the hybrid MPI-OpenMP version of the code outperforms the MPI-only, thus lowering the MPI communication overhead.
description: 7 pages, 6 figures. Accepted for publication on The Parallel Universe Magazine ( https://software.intel.com/en-us/parallel-universe-magazine )
Palpita palpifulvata Kirti & Rose 1992
Creators: name: Singh, Navneet
name: Ranjan, Rahul
name: Talukdar, Avishek
name: Joshi, Rahul
name: Kirti, Jagbir Singh
name: Chandra, Kailash
name: Mally, Richard
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Crambidae
Palpita
Palpita palpifulvata

description: 948. Palpita palpifulvata Kirti & Rose, 1992: 67, figs 8–11
Type locality Deomali, Tirap, Arunachal Pradesh
Distribution. Indian records: Arunachal Pradesh (Tirap, Deomali), Assam (North Cachar Hills, Jatinga) (Kirti & Rose 1992), South and NE India (Inoue 1996a). Global records: Thailand, Sumatra, Borneo, Philippines (Luzon), Seram? (Inoue 1996a), Kachin, Philippines: Panay Island (Inoue 1999).
description: Published as part of Singh, Navneet, Ranjan, Rahul, Talukdar, Avishek, Joshi, Rahul, Kirti, Jagbir Singh, Chandra, Kailash & Mally, Richard, 2022, A catalogue of Indian Pyraloidea (Lepidoptera), pp. 1-423 in Zootaxa 5197 (1) on pages 325-326, DOI: 10.11646/zootaxa.5197.1.1, http://zenodo.org/record/7252292
Additional file 2: of Safety and efficacy of tofacitinib for up to 9.5 years in the treatment of rheumatoid arthritis: final results of a global, open-label, long-term extension study
Creators: name: Wollenhaupt, Jürgen
name: Eun-Bong Lee
name: Curtis, Jeffrey
name: Silverfield, Joel
name: Ketti Terry
name: Koshika Soma
name: Mojcik, Chris
name: DeMasi, Ryan
name: Strengholt, Sander
name: Kwok, Kenneth
name: Lazariciu, Irina
name: Lisy Wang
name: Cohen, Stanley
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Figure S1. Patient disposition (a) and discontinuation over time (b). aFour patients in the tofacitinib 10 mg BID arm had a missing end-of-study page. bEvaluable for AEs (evaluable for laboratory data: tofacitinib 5 mg BID n = 1118, tofacitinib 10 mg BID n = 3346, and all tofacitinib n = 4464). cTwo patients in the tofacitinib 10 mg BID arm did not have recorded AEs. Safety analysis set: all patients who received at least one dose of study medication; efficacy analysis set: all patients who received at least one dose of study medication and had at least one post-baseline efficacy measurement available. Time to discontinuation: difference between the end-of-study date and first tofacitinib dose date plus 1 day; completers are censored at the end-of-study date. Study discontinuation occurred with the following scenarios: serious infections requiring antimicrobial therapy or hospitalization; opportunistic infections judged to be significant by the investigator; two sequential lymphocyte or neutrophil counts 3 times the ULN with ≥ 1 total bilirubin value > 2 times the ULN, abnormal International Normalized Ratio liver function test, or symptoms consistent with hepatic injury (or elevations > 5 times the ULN regardless); single positive HBcAb and a negative HBsAb; two sequential hemoglobins 30% from baseline; two sequential increases in serum creatinine > 100% of the average baseline/screening values (> 50% for Korea); other serious or severe AEs. Database lock: March 2, 2017. AE adverse event, ALT alanine aminotransferase, AST aspartate aminotransferase, BID twice daily, HBcAb hepatitis B core antibody, HBsAb hepatitis B surface antibody, ULN upper limit of normal.
Submillimeter spectroscopy and astronomical searches of vinyl mercaptan, C$_2$H$_3$SH
Creators: name: Martin-Drumel, Marie-Aline
name: Lee, Kin Long Kelvin
name: Belloche, Arnaud
name: Zingsheim, Oliver
name: Thorwirth, Sven
name: Mueller, Holger S. P.
name: Lewen, Frank
name: Garrod, Robin T.
name: Menten, Karl M.
name: McCarthy, Michael C.
name: Schlemmer, Stephan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have extended the pure rotational investigation of the two isomers syn and anti vinyl mercaptan to the millimeter domain using a frequency-multiplication spectrometer. The species were produced by a radiofrequency discharge in 1,2-ethanedithiol. Additional transitions have been re-measured in the centimeter band using Fourier-transform microwave spectroscopy to better determine rest frequencies of transitions with low-$J$ and low-$K_a$ values. Experimental investigations were supported by quantum chemical calculations on the energetics of both the [C$_2$,H$_4$,S] and [C$_2$,H$_4$,O] isomeric families. Interstellar searches for both syn and anti vinyl mercaptan as well as vinyl alcohol were performed in the EMoCA (Exploring Molecular Complexity with ALMA) spectral line survey carried out toward Sagittarius (Sgr) B2(N2) with the Atacama Large Millimeter/submillimeter Array (ALMA). Highly accurate experimental frequencies (to better than 100 kHz accuracy) for both syn and anti isomers of vinyl mercaptan have been measured up to 250 GHz; these deviate considerably from predictions based on extrapolation of previous microwave measurements. Reliable frequency predictions of the astronomically most interesting millimeter-wave lines for these two species can now be derived from the best-fit spectroscopic constants. From the energetic investigations, the four lowest singlet isomers of the [C$_2$,H$_4$,S] family are calculated to be nearly isoenergetic, which makes this family a fairly unique test bed for assessing possible reaction pathways. Upper limits for the column density of syn and anti vinyl mercaptan are derived toward the extremely molecule-rich star-forming region Sgr B2(N2) enabling comparison with selected complex organic molecules.
description: 13 pages, 5 figures, 2 tables, 2 appendices. Accepted for publication in A&A 13th of February, 2019
Relaxing LHC constraints on the $W_R$ mass
Creators: name: Frank, Mariana
name: Özdal, Özer
name: Poulose, Poulose
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study mass bounds of the $W_R$ gauge boson in generic left-right symmetric models. Assuming that the gauge bosons couple universally to quarks and leptons, we allow different gauge couplings $g_R \ne g_L$ and mass mixing, $V_{CKM}^L \ne V_{CKM}^R$ in the left and right sectors. Imposing constraints from collider experiments and $K^0$, $B_d$, $B_s$ physics, we investigate scenarios where $W_R$ is lighter, or heavier than the right handed neutrino $ν_R$. In these scenarios, $W_R$ mass bounds can be considerably relaxed, while $Z_R$ mass bounds are much more stringent. In the case where $M_{W_R} \le M_{ν_R}$, the experimental constraints come from $W_R \to tb $ and $W_R \to jj$ channels, while if $M_{W_R} \ge M_{ν_R}$, the dominant constraints come from $W_R \to \ell \ell jj $. The observed (expected) limits in the two-dimensional ($M_{W_R}$, $M_{ν_R}$) mass plane excluded at 95\% confidence level extend to approximately $M_{W_R}$= 3.1 (3.3) TeV in the $ee$ channel and 3.3 (3.4) TeV in the ($μμ$) channel, for a large range of right-handed neutrino masses up to $M_{ν_R}$= 2.1 (2.1) TeV in the $ee$ channel and 2.6 (2.5) in the ($μμ$) channel, representing a significant relaxation of the mass bounds.
description: 18 pages, 16 figures
Additional file 5: of Assessment of direct and indirect associations between children active school travel and environmental, household and child factors using structural equation modelling
Creators: name: Ikeda, Erika
name: Hinckson, Erica
name: Witten, Karen
name: Smith, Melody
Publisher: name: figshare
Year: 2019
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Unstandardised estimated coefficients of the structural equation model of children’s active travel to school. Root mean square error of approximation (RMSEA) = 0.04, comparative fit index (CFI) = 0.94, Tucker-Lewis index (TLI) = 0.92. (DOCX 606 kb)
False Vacuum Decay With Gravity in Non-Thin-Wall Limit
Creators: name: Gen, Uchida
name: Sasaki, Misao
Publisher: name: arXiv
Year: 1999
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider a wave-function approach to the false vacuum decay with gravity and present a new method to calculate the tunneling amplitude under the WKB approximation. The result agrees with the one obtained by the Euclidean path-integral method, but gives a much clearer interpretation of an instanton (Euclidean bounce solution) that dominates the path integral. In particular, our method is fully capable of dealing with the case of a thick wall with the radius of the bubble comparable to the radius of the instanton, thus surpassing the path-integral method whose use can be justified only in the thin-wall and small bubble radius limit. The calculation is done by matching two WKB wave functions, one with the final state and another with the initial state, with the wave function in the region where the scale factor of the metric is sufficiently small compared with the inverse of the typical energy scale of the field potential at the tunneling. The relation of the boundary condition on our wave function for the false vacuum decay with Hartle-Hawking's no-boundary boundary condition and Vilenkin's tunneling boundary condition on the wave function of the universe is also discussed.
description: 11 pages, 5 figures, submitted to PRD
title: Profitability and play in urban satirical pamphlets, 1575–1625
Creators: name: Hasler, Rebecca Louise
Publisher: name: University of St Andrews
publisherIdentifier: https://ror.org/02wn5qz54
publisherIdentifierScheme: ROR
Year: 2018

description: This thesis reconstructs the genre of urban satirical pamphleteering. It contends that the pamphlets of Robert Greene, Thomas Nashe, Thomas Dekker, Thomas Middleton, and Barnaby Rich are stylistically and generically akin. Writing in a relatively undefined form, these pamphleteers share an interest in describing contemporary London, and employ an experimental style characterised by its satirical energy. In addition, they negotiate a series of tensions between profitability and play. In the early modern period, ‘profit’ was variously conceived as financial, moral, or rooted in public service. Pamphleteers attempted to reconcile these senses of profitability. At the same time, they produced playful works that are self-consciously mocking, that incorporate alternative perspectives, and that are generically hybrid. To varying degrees, urban satirical pamphlets can be defined in relation to the concepts of profitability and play. Chapter One introduces the concept of moral profitability through an examination of Elizabethan moralistic pamphlets. In particular, it analyses the anxious response to profitability contained in Philip Stubbes’s Anatomie of Abuses (1583). Chapter Two argues that Greene disrupted appeals to totalising profitability, and instead demonstrated the alternative potential of play. Chapter Three examines Nashe’s notoriously evasive pamphlets, contending that he embraced play in response to the potential profitlessness of pamphleteering. Chapter Four argues that although Dekker and Middleton rejected absolutist notions of profitability, their pamphlets redirect stylistic play towards compassionate social commentary. Finally, Chapter Five explores Rich’s relocation of moralistic conventions in pamphlets that are presented as both honest and mocking. Taken as a whole, this thesis re-evaluates the style and genre of urban satirical pamphleteering. It reveals that this frequently overlooked literary form was deeply invested in defining and critiquing the purpose of literature.
Explicit relations and criteria for eclipses, transits and occultations
Creators: name: Veras, Dimitri
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Solar system, exoplanet and stellar science rely on transits, eclipses and occultations for dynamical and physical insight. Often, the geometry of these configurations are modelled by assuming a particular viewpoint. Here, instead, I derive user-friendly formulae from first principles independent of viewpoint and in three dimensions. I generalise the results of Veras & Breedt (2017) by (i) characterising three-body systems which are in transit but are not necessarily perfectly aligned, and by (ii) incorporating motion. For a given snapshot in time, I derive explicit criteria to determine whether a system is in or out of transit, if an eclipse is total or annular, and expressions for the size of the shadow, including their extreme values and a condition for engulfment. These results are exact. For orbital motion, I instead obtain approximate results. By assuming fixed orbits, I derive a single implicit algebraic relation which can be solved to obtain the frequency and duration of transit events -- including ingresses and egresses -- for combinations of moons, planets and stars on arbitrarily inclined circular orbits; the eccentric case requires the solution of Kepler's equation but remains algebraic. I prove that a transit shadow -- whether umbral, antumbral or penumbral -- takes the shape of a parabolic cylinder, and finally present geometric constraints on Earth-based observers hoping to detect a three-body syzygy (or perfect alignment) -- either in extrasolar systems or within the solar system -- potentially as a double annular eclipse.
description: Accepted for publication in MNRAS