cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 5: of Glial pathology and retinal neurotoxicity in the anterior visual pathway in experimental autoimmune encephalomyelitis
Creators: name: Jin, Jing
name: Smith, Matthew
name: Kersbergen, Calvin
name: Kam, Tae-In
name: Viswanathan, Mayuri
name: Martin, Kyle
name: Dawson, Ted
name: Dawson, Valina
name: Zack, Donald
name: Whartenby, Katharine
name: Calabresi, Peter
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Neuroscience
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Computational Biology

description: Figure S5. SMI31, MBP and SMI32 staining in the optic nerve of EAE and CFA control mice. a SMI31 and MBP staining in different region of optic nerve of in EAE and CFA control mice at PID16 and PID42, respectively. b SMI32 and MBP staining in different region of optic nerve of EAE and CFA control mice at PID16 and PID42, respectively. CFA group was from control of PID 42. Scale bar =50â Îźm. (PDF 4950 kb)
Soft photon approximation in a laser field
Creators: name: Krachkov, P. A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the present paper, we consider processes involving the emission of soft photons in the presence of a strong laser field. We demonstrate that the matrix element $S$ for a process $\text{i} \rightarrow \text{f} + γ$, with a soft photon $γ$, can be expressed in terms of the matrix element $S_0$ for the process $\text{i} \rightarrow \text{f}$ through a simple multiplicative factor in the integrand over $ϕ$. This approximation enables a result that is exact in the phase and approximate in the prefactor to order $\mathcal{O}(ω/\varepsilon_\text{char})$, where $ω$ is the frequency of the soft photon and $\varepsilon_\text{char}$ is the characteristic energy of the $\text{i}\rightarrow\text{f}$ process.
 We demonstrate several important applications of this soft photon approximation. First, under soft photon approximation we compute the probabilities of nonlinear Compton scattering and photon emission in the superposition of a laser and atomic fields and compare obtained result with the exact one. Second, we demonstrate that the amplitude of $n$ soft photons emission has factorization, which corresponds to the independence of the emission of $n$ soft photons. Third, we use the discussed approximation to prove cancellation of real and virtual infrared divergences for nonlinear Compton scattering and derive the finite radiative corrections.
 The soft photon approximation is a useful tool for investigation of different QED processes in the presence of a strong laser field. Also, it can be widely used for computation of infrared part of radiative correction for some processes.
description: 13 pages, 2 figures
Long-term FRII jet evolution: Clues from three-dimensional simulations
Creators: name: Perucho, Manel
name: Martí, José-María
name: Quilis, Vicent
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a long-term numerical three-dimensional simulation of a relativistic outflow designed to be compared with previous results from axisymmetric, two-dimensional simulations, with existing analytical models and state-of-art observations. We follow the jet evolution from 1~kpc to 200~kpc, using a relativistic gas equation of state and a galactic profile for the ambient medium. We also show results from smaller scale simulations aimed to test convergence and different three-dimensional effects. We conclude that jet propagation can be faster than expected from axisymmetric simulations, covering tens of kiloparsecs in a few million years, until the dentist drill effect produced by the growth of helical instabilities slows down the propagation speed of the jet head. A comparison of key physical parameters of the jet structure as obtained from the simulations with values derived from observations of FRII sources reveals good agreement. Our simulations show that shock heating can play a significant role in the feedback from active galaxies, confirming previous 2D results. A proper description of galactic jets as a relativistic scenario, both dynamical and thermodynamical, reveals an extremely fast and efficient feedback process reheating the ICM, and therefore, with dramatic consequences on the galactic evolution. Our results point towards FRII jets as the source of the energetic electrons observed in radio relics.
description: (1) Universitat de Val\`encia. Accepted for publication in Monthly Notices of the Royal Astronomical Society
Constraints on Disconnected Contributions in $ππ$ Scattering
Creators: name: Acharya, N. Ripunjay
name: Guo, Feng-Kun
name: Meißner, Ulf-G.
name: Seng, Chien-Yeah
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The accuracy of the lattice QCD computation of hadron-hadron scattering at low isospin depends critically on the ability to compute correlation functions with fermionic disconnected Wick contractions. This happens, for instance, in isospin $I=0$ $ππ$ scattering, which receives contributions from rectangular and vacuum types of contractions among other easier calculable ones. Combining Lüscher's formula and partially-quenched chiral perturbation theory, we provide precise theory predictions of the discrete energy levels extracted from specific linear combinations of lattice correlation functions corresponding to various types of contractions. Expressions are provided for extracting the unphysical low-energy constants in the partially-quenched chiral perturbation theory from the energy levels for these contractions. The predictions for the rectangular and vacuum contractions may serve as solid tests of the accuracy for existing and future lattice studies of $ππ$ scattering.
description: Version to appear in JHEP
Magnetically driven superluminal motion from rotating black holes
Creators: name: Fendt, Ch.
name: Greiner, J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have investigated magnetically driven superluminal jets originating from rotating black holes. The stationary, general relativistic, magnetohydrodynamic wind equation along collimating magnetic flux surfaces has been solved numerically. In particular, we apply our results to the Galactic superluminal sources GRS 1915+105 and GRO 1655-40. Our results show that the observed speed of more than 0.9 c can be achieved in general by magnetohydrodynamic acceleration. The velocity distribution along the magnetic field has a saturating profile. Further, we find that highly relativistic speeds can be reached also for jets not emerging from a region close to the black hole, if the flow magnetization is sufficiently large. The plasma temperature rapidly decreases from about 10**10 K at the foot point of the jet to about 10**6 K at a distance of 5000 gravitational radii from the source. Temperature and the mass density follow a power law distribution with the radius.
description: Astron. and Astroph., accepted, 15 pages, full ps-paper at http://www.aip.de/~cfendt
Peak effect in CeRu$_2$:history dependence and supercooling
Creators: name: Roy, S. B.
name: Chaddah, P.
name: Chaudhary, Sujeet
Publisher: name: arXiv
Year: 2000
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We present experimental results on single crystal CeRu$_2$ showing that the extent of history dependence of peak-effect depends on the path followed in the space of field (H) and temperature (T). The (H,T) regime over which history effect is observed is larger if the vortex lattice is prepared by lowering T from above T$_C$ in constant H i.e. by field cooling. We compare this history effect with the very recently reported history dependence of peak-effect in detwinned single crystals of YBaCuO, highlighting the similarities and differences. We discuss the possibility of a first order vortex solid-solid transition in CeRu$_2$ within the realm of recent theoretical developments in the field of vortex matter.
description: 21 pages, 5 figures; submitted to Phys. Rev. B on 9th Feb. 2000
Guiding drones by information gain
Creators: name: van Hove, Alouette
name: Aalstad, Kristoffer
name: Pirk, Norbert
Publisher: name: arXiv
Year: 2024
Subjects: subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: The accurate estimation of locations and emission rates of gas sources is crucial across various domains, including environmental monitoring and greenhouse gas emission analysis. This study investigates two drone sampling strategies for inferring source term parameters of gas plumes from atmospheric measurements. Both strategies are guided by the goal of maximizing information gain attained from observations at sequential locations. Our research compares the myopic approach of infotaxis to a far-sighted navigation strategy trained through deep reinforcement learning. We demonstrate the superior performance of deep reinforcement learning over infotaxis in environments with non-isotropic gas plumes.
description: To be published in Proceedings of Machine Learning Research (Proceedings of the 5th Northern Lights Deep Learning Conference (NLDL))
$\bar{B}^{(\ast)} \bar{B}^{(\ast)}$ interactions in chiral effective field theory
Creators: name: Wang, Bo
name: Liu, Zhan-Wei
name: Liu, Xiang
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this work, the intermeson interactions of double-beauty $\bar{B}\bar{B}$, $\bar{B}\bar{B}^\ast$, and $\bar{B}^\ast\bar{B}^\ast$ systems have been studied with heavy meson chiral effective field theory. The effective potentials are calculated with Weinberg's scheme up to one-loop level. At the leading order, four body contact interactions and one pion exchange contributions are considered. In addition to two pion exchange diagrams, we include the one-loop chiral corrections to contact terms and one pion exchange diagrams at the next-to-leading order. The behaviours of effective potentials both in momentum space and coordinate space are investigated and discussed extensively. We notice the contact terms play important roles in determining the characteristics of the total potentials. Only the potentials in $I(J^P)=0(1^+)$ $\bar{B}\bar{B}^\ast$ and $\bar{B}^\ast\bar{B}^\ast$ systems are attractive, and the corresponding binding energies in these two channels are solved to be $ΔE_{\bar{B}\bar{B}^\ast}\simeq -12.6^{+9.2}_{-12.9}$ MeV and $ΔE_{\bar{B}^\ast\bar{B}^\ast}\simeq -23.8^{+16.3}_{-21.5}$ MeV, respectively. The masses of $0(1^+)$ $\bar{B}\bar{B}^\ast$ and $\bar{B}^\ast\bar{B}^\ast$ states lie above the threshold of their electromagnetic decay modes $\bar{B}\bar{B}γ$ and $\bar{B}\bar{B}γγ$, and thus they can be reconstructable via electromagnetic interactions. Our calculation not only provides some useful information to explore exotic doubly-bottomed molecular states for future experiments, but also is helpful for the extrapolations of Lattice QCD simulations.
description: 24 pages, 19 figures, 3 tables
Lithium and mass loss in massive AGB stars in the Large Magellanic Clouds
Creators: name: Ventura, P.
name: D'Antona, F.
name: Mazzitelli, I.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The aim of this work is to use full evolutionary models to derive observational constraints on the mass loss rate of the upper Asymptotic Giant Branch (AGB) stars. The observations used to constrain the models are the relative number of luminous Lithium rich AGBs in the Magellanic Clouds and the s-process enhancement of the same sample. We find that we can put lower and upper limits to the mass loss rate during the AGB phase. The mass loss calibation obtained in this work implies that massive AGBs do not contribute significantly to the lithium enrichment of the interstellar medium.
description: 12 pages, 10 figures
The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxies
Creators: name: González-Otero, Mauro
name: Padilla-Torres, Carmen P.
name: González-Serrano, J. Ignacio
name: Cepa, Jordi
name: García, Ana María Pérez
name: González, J. Jesús
name: Benítez, Erika
name: Bongiovanni, Ángel
name: Cerviño, Miguel
name: Cruz-González, Irene
name: Gallego, Jesús
name: Herrera-Endoqui, Martín
name: Ibarra-Medel, Héctor J.
name: Krongold, Yair
name: Lara-López, Maritza A.
name: Nadolny, Jakub
name: Negrete, C. Alenka
name: Pérez-Martínez, Ricardo
name: Povic, Mirjana
name: Sánchez-Portal, Miguel
name: de Diego, Bernabé Cedrés José A.
name: Hernández-Toledo, Héctor
name: Martínez, Rocío Navarro
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Methods. We performed measurements of the \MgII, \MgI, \FeIIa, \FeIIb, and \FeIIc\ spectral lines present in the spectra of the selected sample to determine the EW and velocity of the flows observed in the star-forming galaxies. Subsequently, we conducted $10^7$ bootstrap simulations using Spearman's rank correlation coefficient ($ρ_s$) to explore correlations with galaxy properties. Furthermore, we calculated the covering factor, gas density, and optical depth for the measured \ion{Fe}{II} doublets.
 Results. Our analysis revealed strong correlations between the EW of \ion{Mg}{II} lines and both $M_{*}$ ($ρ_s=0.43$, 4.5$σ$) and SFR ($ρ_s=0.42$, 4.4$σ$). For the \ion{Fe}{II} lines, we observed strong correlations between the EW and SFR ($ρ_s\sim0.65$, $>3.9σ$), with a weaker correlation for $M_{*}$ ($ρ_s\sim0.35$, $>1.9σ$). No notable correlations were found between velocity measurements of \ion{Mg}{II} line and $M_{*}$, SFR, or sSFR of the objects ($ρ_s\sim0.1)$. However, a negative strong correlation was found between the velocity of the \ion{Fe}{II} lines and the SFR of the galaxies ($ρ_s\sim-0.45$, $\sim3σ$). Our results align with previous studies but studying FIR-selected objects. Finally, we detected a candidate \textit{loitering outflow}, a recently discovered subtype of FeLoBAL quasar, at redshift of $z=1.4399$, exhibiting emission in \ion{C}{III}] and low line velocities ($|v|\lesssim$ 200 km/s).
description: 25 pages, 31 figures
Estimated Number of Days' Supply of Food and Beverages in Warehouses at Wholesale, 1963: A Civil Defense Study
Creators: name: Van Dress, Michael G.
name: Van Dress, Michael G.
Publisher: name: Unknown
Year: 1963
Subjects: Agricultural and Food Policy
Food Consumption/Nutrition/Food Safety
Food Security and Poverty
Research Methods/ Statistical Methods

description: Excerpts from the report: The Office of Civil Defense is charged with the responsibility of developing an overall preparedness program designed to cope with a civil defense emergency. Of particular concern is the number of days that the population can be fed from existing food inventories in the event of an emergency, and the geographical distribution of this supply within the United States. In this connection, the Office of Civil Defense requested the Department of Agriculture to provide technical assistance and guidance in assessing the supply and geographical distribution of food and nonconcentrated fluids within warehouses at the wholesale level of distribution. This report examines the supply of food and nonconcentrated beverages available in warehouses at the wholesale level of distribution. Stocks of food are shown by type of storability and by food group for civil defense regions and for establishments by kind of business. The per capita days' supply is shown also for Standard Metropolitan Statistical Areas.
Li$_2$VO(Si,Ge)O$_4$, a prototype of a two-dimensional frustrated quantum Heisenberg antiferromagnet
Creators: name: Melzi, R.
name: Carretta, P.
name: Lascialfari, A.
name: Mambrini, M.
name: Troyer, M.
name: Millet, P.
name: Mila, F.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: NMR and magnetization measurements in Li$_2$VOSiO$_4$ and Li$_2$VOGeO$_4$ are reported. The analysis of the susceptibility shows that both compounds are two-dimensional $S=1/2$ Heisenberg antiferromagnets on a square lattice with a sizeable frustration induced by the competition between the superexchange couplings $J_1$ along the sides of the square and $J_2$ along the diagonal. Li$_2$VOSiO$_4$ undergoes a low-temperature phase transition to a collinear order, as theoretically predicted for $J_2/J_1 > 0.5$. Just above the magnetic transition the degeneracy between the two collinear ground states is lifted by the onset of a structural distortion.
description: 4 pages, 4 figures
An optical transmission spectrum for the ultra-hot Jupiter WASP-121b measured with the Hubble Space Telescope
Creators: name: Evans, Thomas M.
name: Sing, David K.
name: Goyal, Jayesh
name: Nikolov, Nikolay
name: Marley, Mark S.
name: Zahnle, Kevin
name: Henry, Gregory W.
name: Barstow, Joanna K.
name: Alam, Munazza K.
name: Sanz-Forcada, Jorge
name: Kataria, Tiffany
name: Lewis, Nikole K.
name: Lavvas, Panayotis
name: Ballester, Gilda E.
name: Ben-Jaffel, Lotfi
name: Blumenthal, Sarah D.
name: Bourrier, Vincent
name: Drummond, Benjamin
name: Munoz, Antonio Garcia
name: Lopez-Morales, Mercedes
name: Tremblin, Pascal
name: Ehrenreich, David
name: Wakeford, Hannah R.
name: Buchhave, Lars A.
name: Etangs, Alain Lecavelier des
name: Hebrard, Eric
name: Williamson, Michael H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present an atmospheric transmission spectrum for the ultra-hot Jupiter WASP-121b, measured using the Space Telescope Imaging Spectrograph (STIS) onboard the Hubble Space Telescope (HST). Across the 0.47-1 micron wavelength range, the data imply an atmospheric opacity comparable to - and in some spectroscopic channels exceeding - that previously measured at near-infrared wavelengths (1.15-1.65 micron). Wavelength-dependent variations in the opacity rule out a gray cloud deck at a confidence level of 3.8-sigma and may instead be explained by VO spectral bands. We find a cloud-free model assuming chemical equilibrium for a temperature of 1500K and metal enrichment of 10-30x solar matches these data well. Using a free-chemistry retrieval analysis, we estimate a VO abundance of -6.6(-0.3,+0.2) dex. We find no evidence for TiO and place a 3-sigma upper limit of -7.9 dex on its abundance, suggesting TiO may have condensed from the gas phase at the day-night limb. The opacity rises steeply at the shortest wavelengths, increasing by approximately five pressure scale heights from 0.47 to 0.3 micron in wavelength. If this feature is caused by Rayleigh scattering due to uniformly-distributed aerosols, it would imply an unphysically high temperature of 6810+/-1530K. One alternative explanation for the short-wavelength rise is absorption due to SH (mercapto radical), which has been predicted as an important product of non-equilibrium chemistry in hot Jupiter atmospheres. Irrespective of the identity of the NUV absorber, it likely captures a significant amount of incident stellar radiation at low pressures, thus playing a significant role in the overall energy budget, thermal structure, and circulation of the atmosphere.
description: Accepted for publication in The Astronomical Journal
Optical study of the metal-nonmetal transition in NiS
Creators: name: Okamura, H.
name: Naitoh, J.
name: Nanba, N.
name: Matoba, M.
name: Nishioka, M.
name: Anzai, S.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Optical reflectivity study has been made on the hexagonal (NiAs-type) Ni_{1-d}S in order to probe its electronic properties, in particular those associated with the metal-nonmetal transition in this compound. Samples with d=0.005 and 0.02 are studied, which have transition temperatures Tt=246 K and 161 K, respectively. A pronounced dip appears in the reflectivity spectra upon the transition, and the optical conductivity spectra show that the electronic structure below Tt is similar to that of a carrier-doped semiconductor with an energy gap of ~ 0.15 eV. The optical spectra indicate that the gap becomes larger with decreasing temperature, and it becomes smaller as d increases. It is also found that the overall spectrum including the violet region can be described based on a charge-transfer-type semiconductor, consistent with recent photoemission results.
description: 4 pages, 4 figs, submitted to Solid State Commun. Fig.2 corrected
Additional file 2 of MaGIC: a machine learning tool set and web application for monoallelic gene inference from chromatin
Creators: name: Vinogradova, Svetlana
name: Sachit Saksena
name: Ward, Henry
name: SĂŠbastien Vigneau
name: Gimelbrant, Alexander
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Hematology

description: Table S2. The generalized linear model performance evaluated on mouse B-lymphoid clonal cell lines (B-lymph), mouse embryonic fibroblasts (MEF) and mouse neural progenitor cells (NPC). (PDF 310 kb)
Jahn-Teller driven quadrupolar ordering and spin-orbital dimer formation in GaNb$_{4}$Se$_{8}$
Creators: name: Yang, Tsung-Han
name: Chang, Tieyan
name: Chen, Yu-Sheng
name: Plumb, K. W.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The lacunar spinel GaNb$_4$Se$_8$ is a tetrahedral cluster Mott insulator where spin-orbit coupling on molecular orbitals and Jahn-Teller energy scales are competitive. GaNb$_4$Se$_8$ undergoes a structural and anti-polar ordering transition at T$_Q$ = 50 K that corresponds to a quadrupolar ordering of molecular orbitals on Nb$_4$ clusters. A second transition occurs at T$_M$ = 29 K, where local distortions on the Nb$_4$ clusters rearrange. We present a single crystal x-ray diffraction investigation these phase transitions and solve the crystal structure in the intermediate T$_M$ < T < T$_Q$ and low T < T$_M$ temperature phases. The intermediate phase is a primitive cubic P2$_1$3 structure with a staggered arrangement of Nb4 cluster distortions. A symmetry mode analysis reveals that the transition at TQ is continuous and described by a single Jahn-Teller active amplitude mode. In the low temperature phase, the symmetry of Nb$_4$ clusters is further reduced and the unit cell doubles into an orthorhombic P2$_1$2$_1$2$_1$ space group. Nb$_4$ clusters rearrange through this transition to form a staggered arrangement of intercluster dimers, suggesting a valence bond solid magnetic state.
Real-time Impurity Solver Using Grassmann Time-Evolving Matrix Product Operators
Creators: name: Chen, Ruofan
name: Xu, Xiansong
name: Guo, Chu
Publisher: name: arXiv
Year: 2024
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: An emergent and promising tensor-network-based impurity solver is to represent the path integral as a matrix product state, where the bath is analytically integrated out using Feynman-Vernon influence functional. Here we present an approach to calculate the equilibrium impurity spectral function based on the recently proposed Grassmann time-evolving matrix product operators method. The central idea is to perform a quench from a separable impurity-bath initial state as in the non-equilibrium scenario. The retarded Green's function $G(t+t_0, t'+t_0)$ is then calculated after an equilibration time $t_0$ such that the impurity and bath are approximately in thermal equilibrium. There are two major advantages of this method. First, since we focus on real-time dynamics, we do not need to perform the numerically ill-posed analytic continuation in the continuous-time quantum Monte Carlo case that relies on imaginary-time evolution. Second, the entanglement growth of the matrix product states in real-time calculations is observed to be much slower than that in imaginary-time calculations, leading to a significant improvement in numerical efficiency. The accuracy of this method is demonstrated in the single-orbital Anderson impurity model and benchmarked against the continuous-time quantum Monte Carlo method.
description: 9 pages, 6 figures
Inventory of Food Products and Beverages in Warehouses at Wholesale, 1962
Creators: name: Van Dress, Michael G.
name: Van Dress, Michael G.
Publisher: name: Unknown
Year: 1964
Subjects: Agricultural and Food Policy
Food Consumption/Nutrition/Food Safety
Food Security and Poverty
Research Methods/ Statistical Methods

description: Excerpts from the report: This supplement provides a special tabulation of wholesale food and beverage inventory data. The data were collected in conjunction with a civil defense study conducted in 1962. Findings of the original study are reported in Marketing Research Report No. 632 “Estimated Number of Days' Supply of Food and Beverages in Warehouses at Wholesale." The amount of individual food products available and their locations in the channel of distribution are of interest and importance, however, not only to defense officials in planning emergency feeding programs, but also to members of the food trade. For this reason, inventory data in this supplement are presented in pounds rather than in number of days' supply. They are listed for major food groups by wholesaler's kind of business and type of operation and for individual food product.
description: Supplement to Marketing Research Report No. 632: "Estimated Number of Days' Supply of Food and Beverages in Warehouses at Wholesale."
Additional file 22 of Transcriptomic analysis of paternal behaviors in prairie voles
Creators: name: Duclot, Florian
name: Liu, Yan
name: Saland, Samantha K.
name: Wang, Zuoxin
name: Kabbaj, Mohamed
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 22. Structure-specific associations of gene coexpression modules with parental behaviors. The correlation of each co-expression module from the weighted gene coexpression network analysis with behavioral traits (behaviors scored during parental behavior test and phenotype status) is depicted for each structure. The correlation value is detailed alongside its corresponding p-value in parentheses. Note that within each structure, only modules with at least one significant association are depicted. MPOA: medial preoptic area, NAc: nucleus accumbens, LS: lateral septum.
Comment on ``Magnetoresistance Anomalies in Antiferromagnetic YBa$_2$Cu$_3$O$_{6+x}$: Fingerprints of Charged Stripes''
Creators: name: Janossy, Andras
name: Simon, Ferenc
name: Feher, Titusz
Publisher: name: arXiv
Year: 2000
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: In a recent Letter Ando et al (cond-mat/9905071) discovered an anomalous magnetoresistance(MR) in hole doped antiferromagnetic YBa$_2$Cu$_3$O$_{6+x}$, which they attributed to charged stripes, i.e., to segregation of holes into lines. In this Comment we show that the experiments, albeit being interesting, do not prove the existence of stripes. In our view the anomalous behavior is due to an (a,b) plane anisotropy of the resistivity in the bulk and to a magnetic field dependent antiferromagnetic (AF) domain structure. It is unlikely that domain walls are charged stripes.
description: 1 page, Accepted to PRL, Reply exists by authors of original paper
Sub-Kelvin Lateral Thermal Transport in Diffusive Graphene
Creators: name: Draelos, A. W.
name: Silverman, A.
name: Eniwaye, B.
name: Arnault, E. G.
name: Ke, C. T.
name: Wei, M. T.
name: Vlassiouk, I.
name: Borzenets, I. V.
name: Amet, F.
name: Finkelstein, G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In this work, we report on hot carrier diffusion in graphene across large enough length scales that the carriers are not thermalized across the crystal. The carriers are injected into graphene at one site and their thermal transport is studied as a function of applied power and distance from the heating source, up to tens of micrometers away. Superconducting contacts prevent out-diffusion of hot carriers to isolate the electron-phonon coupling as the sole channel for thermal relaxation. As local thermometers, we use the amplitude of the Universal Conductance Fluctuations, which varies monotonically as a function of temperature. By measuring the electron temperature simultaneously along the length we observe a thermal gradient which results from the competition between electron-phonon cooling and lateral heat flow.
Additional file 1: of Urban metagenomics uncover antibiotic resistance reservoirs in coastal beach and sewage waters
Creators: name: Fresia, Pablo
name: Antelo, Verónica
name: Salazar, Cecilia
name: Giménez, Matías
name: D’Alessandro, Bruno
name: Afshinnekoo, Ebrahim
name: Mason, Christopher
name: Gastón Gonnet
name: Iraola, Gregorio
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Supplementary figures. (PDF 426 kb)
Multi-Task Learning for Front-End Text Processing in TTS
Creators: name: Kang, Wonjune
name: Wang, Yun
name: Zhang, Shun
name: Hinsvark, Arthur
name: He, Qing
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: We propose a multi-task learning (MTL) model for jointly performing three tasks that are commonly solved in a text-to-speech (TTS) front-end: text normalization (TN), part-of-speech (POS) tagging, and homograph disambiguation (HD). Our framework utilizes a tree-like structure with a trunk that learns shared representations, followed by separate task-specific heads. We further incorporate a pre-trained language model to utilize its built-in lexical and contextual knowledge, and study how to best use its embeddings so as to most effectively benefit our multi-task model. Through task-wise ablations, we show that our full model trained on all three tasks achieves the strongest overall performance compared to models trained on individual or sub-combinations of tasks, confirming the advantages of our MTL framework. Finally, we introduce a new HD dataset containing a balanced number of sentences in diverse contexts for a variety of homographs and their pronunciations. We demonstrate that incorporating this dataset into training significantly improves HD performance over only using a commonly used, but imbalanced, pre-existing dataset.
description: ICASSP 2024
Multiplicative Bell Inequalities
Creators: name: Te'eni, Amit
name: Peled, Bar Y.
name: Carmi, Avishy
name: Cohen, Eliahu
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Bell inequalities are important tools in contrasting classical and quantum behaviors. To date, most Bell inequalities are linear combinations of statistical correlations between remote parties. Nevertheless, finding the classical and quantum mechanical (Tsirelson) bounds for a given Bell inequality in a general scenario is a difficult task which rarely leads to closed-form solutions. Here we introduce a new class of Bell inequalities based on products of correlators that alleviate these issues. Each such Bell inequality is associated with a unique coordination game. In the simplest case, Alice and Bob, each having two random variables, attempt to maximize the area of a rectangle and the rectangle's area is represented by a certain parameter. This parameter, which is a function of the correlations between their random variables, is shown to be a Bell parameter, i.e. the achievable bound using only classical correlations is strictly smaller than the achievable bound using non-local quantum correlations We continue by generalizing to the case in which Alice and Bob, each having now n random variables, wish to maximize a certain volume in n-dimensional space. We term this parameter a multiplicative Bell parameter and prove its Tsirelson bound. Finally, we investigate the case of local hidden variables and show that for any deterministic strategy of one of the players the Bell parameter is a harmonic function whose maximum approaches the Tsirelson bound as the number of measurement devices increases. Some theoretical and experimental implications of these results are discussed.
description: Revised version, accepted to Phys. Rev. A
Pew Research Center: American Trends Panel Wave 33
Creators: name: Pew Research Center
Publisher: name: Roper Center for Public Opinion Research
Year: 2019

description: Things that will/will not happen in next 50 years (6); heard about National Aeronautics and Space Administration (NASA) (1); NASA priorities (9); space station (1); humans vs. robots in space (1); U.S. as world leader in space exploration (1); space exploration by private companies (6); space exploration by NASA (1); interest in orbiting Earth (3); local pollution (2); local land development (1); U.S. energy production (1); expanding sources of energy (6); U.S. energy policy priorities (5); increasing reliance on renewable energy sources (1); cutting back on environmental regulations (1); government actions to protect environment (5); climate change (19); preventing school shootings (5).
Additional file 6: of Glial pathology and retinal neurotoxicity in the anterior visual pathway in experimental autoimmune encephalomyelitis
Creators: name: Jin, Jing
name: Smith, Matthew
name: Kersbergen, Calvin
name: Kam, Tae-In
name: Viswanathan, Mayuri
name: Martin, Kyle
name: Dawson, Ted
name: Dawson, Valina
name: Zack, Donald
name: Whartenby, Katharine
name: Calabresi, Peter
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Neuroscience
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Mental Health

description: Figure S6. GFAP and IBA1 staining in the optic nerve of EAE and CFA control mice. a GFAP and IBA1 staining in different region of optic nerve of in EAE and CFA control mice at PID16 and PID42, respectively. b IBA1 and iNOS staining in different region of optic nerve of EAE and CFA control mice at PID16 and PID42, respectively. CFA group was from control of PID 42. Scale bar =50â Îźm. (PDF 5320 kb)
Incremental SWAP Operator for Entanglement Entropy: Application for Exponential Observables in Quantum Monte Carlo Simulation
Creators: name: Zhou, Xuan
name: Meng, Zi Yang
name: Qi, Yang
name: Da Liao, Yuan
Publisher: name: arXiv
Year: 2024
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We propose a new method to efficiently compute the entanglement entropy (EE) of quantum many-body systems. Our approach, called the incremental SWAP operator method , combines the simplicity of the SWAP operator used in projector quantum Monte Carlo simulations with recent advances in precisely computing exponential observables using incremental algorithms. We apply this technique to obtain accurate EE data at reduced computational cost for 1d and 2d antiferromagnetic Heisenberg models with different bipartition schemes. Using the computed EE data, we extract the area law coefficient, universal logarithmic corrections from Goldstone modes, and the geometric constant, finding quantitative agreement with analytical predictions. Moreover, for the first time in an unbiased numerical simulation of 2d antiferromagnetic Heisenberg model, we successfully obtain reliable universal logarithmic corrections from sharp corners that match expected theoretical values. The consistency between our numerical results and theoretical calculations demonstrates the power of our approach for accessing challenging universal entanglement properties. The extensions of our method to other quantum spin/boson models and the interacting fermion models, are outlined.
Preis- und Musterbüchlein
Creators: name: Basler Bandfabrik vorm. Trüdinger & Cons
Publisher: name: [s.n.]
Year: 1868

description: Deutsch, Französisch
description: Verzeichnung=Description=Inventaire 2014 ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Sebastian Preher
Could We Detect Molecular Oxygen in the Atmosphere of a Transiting Extra-Solar Earth-Like Planet?
Creators: name: Webb, John K.
name: Wormleaton, Imma
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Although the extra-solar planets discovered so far are of the giant, gaseous, type, the increased sensitivity of future surveys will result in the discovery of lower mass planets. The detection of O2 in the atmosphere of a rocky extra-solar planet would be a potential indicator of a life. In this paper we address the specific issue of whether we would be able to detect the O2 A-band absorption feature in the atmosphere of a planet similar to the Earth, if it were in orbit around a nearby star. Our method is empirical, in that we use observations of the Earth's O2 A-band, with a simple geometric modification for a transiting extra-solar planet, allowing for limb-darkening of the host star. We simulate the spectrum of the host star with the superposed O2 A-band absorption of the transiting planet, assuming a spectral resolution of 7 km/s (typical of current echelle spectrographs), for a range of spectral signal-to-noise ratios. The main result is that we could reliably detect the O2 A-band of the transiting planet for host stars with radii 0.3 solar or less. However, using existing instrumentation and 8m telescopes, this requires target M stars with m(V) of approximately 10 or brighter for integration times of about 10 hours or less. The number of such stars over the sky is small. Larger aperture telescopes and/or improved instrumentation efficiency would enable surveys of M stars down to m(V) = 13 and greatly improve the chances of discovering life elsewhere.
description: 14 pages, 6 figures, to appear in Publ. Astron. Soc. Austr
Deep Neural Network with Walsh-Hadamard Transform Layer For Ember Detection during a Wildfire
Creators: name: Pan, Hongyi
name: Chen, Chang
name: Watts, Adam
name: Koyuncu, Erdem
name: Badawi, Diaa
name: Cetin, Ahmet Enis
Publisher: name: University of Illinois at Chicago
Year: 2022

description: No description supplied
Additional file 1 of MaGIC: a machine learning tool set and web application for monoallelic gene inference from chromatin
Creators: name: Vinogradova, Svetlana
name: Sachit Saksena
name: Ward, Henry
name: SĂŠbastien Vigneau
name: Gimelbrant, Alexander
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Hematology

description: Table S1. Modelsâ performances evaluated on an additional human dataset, with MAE and BAE genes identified in monoclonal cell lines derived from GM12878 ([10], Dataset S2). (PDF 26 kb)
One-dimensional fermions with incommensurate hopping close to dimerization
Creators: name: Sen, Diptiman
name: Lal, Siddhartha
Publisher: name: arXiv
Year: 1998
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the spectrum of fermions hopping on a chain with a weak incommensuration close to dimerization; both q, the deviation of the wave number from pi, and delta, the strength of the incommensuration, are small. For free fermions, we use a continuum Dirac theory to show that there are an infinite number of bands which meet at zero energy as q approaches zero. In the limit that the ratio q/delta ---> 0, the number of states lying inside the q = 0 gap is nonzero and equal to 2 delta / pi^2. Thus the limit q ---> 0 differs from q = 0; this can be seen clearly in the behavior of the specific heat at low temperature. For interacting fermions or the XXZ spin-1/2 chain, we use bosonization to argue that similar results hold.
description: Revtex, 9 pages including 2 epsf figures
Chemical Evolution of the Galaxy: the G-dwarf problem and radioactive chronology revisited taking account of the Thick Disk
Creators: name: Pagel, B. E. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Thin and Thick disk metallicities overlap, but alpha(Fe) relations differ; there is also a hiatus in time before the first thin-disk stars, with a minimum metallicity [Fe/H] = -0.6. Thus there are two `G-dwarf' problems. We fit metallicity distribution functions (MDFs) for the two disks derived by Wyse & Gilmore (1995) with analytical models (for O and Mg). The Thick disk fits a simple inflow model with effective yield and final [Mg/H] about the same as for the Thin Disk, excluding continuous mass loss from the former as a source of prompt initial enrichment (PIE) for the latter. The Thin disk has a narrow MDF fitted (rather poorly) with a closed model having PIE from some other source, or more elegantly with a slow infall model similar to the `two-inflow' scenario of Matteucci et al., but with a PIE and a severe break in the age-metallicity relation. Implications for radio-active cosmochronology are investigated.
description: World Scientific LaTeX, 6 pages, 4 Postscript figures To appear in `Cosmic Evolution' Conference at IAp, Paris, honoring Jean Audouze and Jim Truran, 13-17 Nov 2000
Aphodius (Aganocrossus) postpilosus Reitter 1895
Creators: name: Král, David
name: Šípek, Petr
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Aphodiidae
Aphodius
Aphodius postpilosus

description: Aphodius (Aganocrossus) postpilosus Reitter, 1895
 Distribution. Oriental species, widely distributed in China (type locality: Shanghai), recorded also from Japan, Laos, South Korea and Vietnam; from India so far reported only from Sikkim (BORDAT & DELLACASA 1996, DELLACASA & DELLACASA 2006a). First record for the states of Maharashtra and Rajasthan.
description: Published as part of Král, David & Šípek, Petr, 2013, Aphodiinae (Coleoptera: Scarabaeidae) of the Goa, Maharashtra and Rajasthan (India) with description of Aphodius (Gilletianus) rajawatorum sp. nov., pp. 633-648 in Acta Entomologica Musei Nationalis Pragae 53 (2) on page 637, DOI: 10.5281/zenodo.5739687
Analytical approach for the Quartet Condensation Model
Creators: name: Baran, V. V.
name: Delion, D. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Within the Quartet Condensation Model (QCM), the isovector pairing correlations for $N = Z$ nuclei are described with a very high accuracy by a condensate of $α$-like quartets. The usual approach involves cumbersome recurrence relations in order to compute numerically the relevant quantities of the model: the norm of the quartet states and the mean value of the isovector pairing Hamiltonian as functions of the pair mixing amplitudes. We present the final analytical expressions for the above mentioned quantities, for all cases up to four quartets in the valence shell. The analytical QCM expressions were obtained by a straightforward implementation of the SO(5) algebra in the symbolic computer algebra system Cadabra2. The norm of the quartet states and the mean value of the Hamiltonian are polynomial functions of the mixing amplitudes. The numerical implementation of the QCM model is thus made trivial as matter of copying and pasting the presented formulas. We introduce in this work the method of computer aided analytical calculus for a many body setting. In particular, we provide precise and easy to use tools for the description of isovector pairing correlations.
description: 5 pages
Nanometer-scale capacitors
Creators: name: Stepanic, J.
name: Bilalbegovic, G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Molecular dynamics computer simulations which employ the embedded-atom potential show that nanowires of gold exist as multishelled structures. We simulate double-walled gold nanowires and calculate the capacitance of a finite nanometer-size cylindrical capacitor. For the sizes for which multishelled nanowires appear in simulations we find the capacitances below one attofarad.
description: 2 ps and 1 jpg figures