cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Uncertainty Relations for Joint Localizability and Joint Measurability in Finite-Dimensional Systems
Creators: name: Miyadera, Takayuki
Publisher: name: arXiv
Year: 2011
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Two quantities quantifying uncertainty relations are examined. In J.Math.Phys. 48, 082103 (2007), Busch and Pearson investigated the limitation on joint localizability and joint measurement of position and momentum by introducing overall width and error bar width. In this paper, we show a simple relationship between these quantities for finite-dimensional systems. Our result indicates that if there is a bound on joint localizability, it is possible to obtain a similar bound on joint measurability. For finite-dimensional systems, uncertainty relations for a pair of general projection-valued measures are obtained as by-products.
description: 10 pages. To appear in Journal of Mathematical Physics
title: Ð¡Ð¸ÑÑÐµÐ¼Ð½Ð¾Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð±Ð»Ð¾ÐºÐ° Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ð¹ Ð´Ð»Ñ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½ÑÑ Ð¼Ð°Ð½ÐµÐ²ÑÐ¾Ð²ÑÑ Ð»Ð¾ÐºÐ¾Ð¼Ð¾ÑÐ¸Ð²Ð¾Ð²
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
title: System software for the obstacle detection unit for unmanned shunting locomotives
Creators: name: Ð¢Ð¾Ð¼Ð¸Ð»Ð¸Ð½, ÐÐ»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2021
Subjects: linux
linux kernel
systemd
docker
preseed
Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð²ÑÑÐµÑÐ½ÐµÐ½Ð¸Ñ
preemption models

description: Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»Ñ Adlink PIS-5500 Ð´Ð»Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾Ð¹ Ð¸Ð½ÑÐµÐ³ÑÐ°ÑÐ¸Ð¸ (continuous integration) Ð¸ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²ÐµÑÑÑÐ²Ð°Ð½Ð¸Ñ (continuous deployment) ÑÐµÑÐ²Ð¸ÑÐ¾Ð², Ð¾ÑÐ²ÐµÑÐ°ÑÑÐ¸Ñ Ð·Ð° Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ð¹ Ð½Ð° Ð¶ÐµÐ»ÐµÐ·Ð½Ð¾Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð¹ ÐºÐ¾Ð»ÐµÐµ. Ð ÑÐ¾Ð´Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» ÑÐµÑÐµÐ½ ÑÑÐ´ Ð·Ð°Ð´Ð°Ñ, ÐºÐ¾ÑÐ¾ÑÑÐ¹ ÑÐ²ÑÐ·Ð°Ð½ Ñ Ð²ÑÐ±Ð¾ÑÐ¾Ð¼ Ð´Ð¸ÑÑÑÐ¸Ð±ÑÑÐ¸Ð²Ð°, Ð²ÑÐ±Ð¾ÑÐ¾Ð¼ Ð²ÐµÑÑÐ¸Ð¸ ÑÐ´ÑÐ° Linux Ð¸ ÐµÐ³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð²ÑÑÐµÑÐ½ÐµÐ½Ð¸Ñ, ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ð¸ Ð·Ð°ÑÐ¸ÑÐµÐ½Ð½Ð¾Ð¹ ÑÐ°Ð¹Ð»Ð¾Ð²Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ, ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ð¸ Ð¸Ð·Ð¾Ð»Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¾ÐºÑÑÐ¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð·Ð°Ð¿ÑÑÐºÐ° ÑÐµÑÐ²Ð¸ÑÐ¾Ð² Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð²ÑÐµÑ ÑÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð½Ð°ÑÐºÐ¾Ð»ÑÐºÐ¾ ÑÑÐ¾ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾Ð»Ð½Ð¾ÑÑÑÑ Ð½Ð°ÑÑÑÐ¾ÐµÐ½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð±ÐµÐ· Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÑ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½ÑÑ Ð¸Ð½ÑÐµÐ³ÑÐ°ÑÐ¸Ñ Ð¸ ÑÐ°Ð·Ð²ÐµÑÑÑÐ²Ð°Ð½Ð¸Ðµ ÑÐµÑÐ²Ð¸ÑÐ¾Ð².
description: The purpose of this work is to prepare the Adlink PIS-5500 computer for continuous integration and continuous deployment of services responsible for detecting obstacles on the railway track. In the course of the work, a number of tasks were solved, which is related to the choice of the distribution package, the choice of the Linux kernel version and its preemption model, the creation of a secure file system, the creation of an isolated environment for running services, and the automation of all these processes, as far as possible. The result is a fully configured system that allows for seamless integration and deployment of services.
WISDOM Project -- XV. Giant Molecular Clouds in the Central Region of the Barred Spiral Galaxy NGC 5806
Creators: name: Choi, Woorak
name: Liu, Lijie
name: Bureau, Martin
name: Cappellari, Michele
name: Davis, Timothy A.
name: Gensior, Jindra
name: Liang, Fu-Heng
name: Lu, Anan
name: Williams, Thomas G.
name: Chung, Aeree
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present high spatial resolution ($\approx24$ pc) Atacama Large Millimeter/sub-millimeter Array $^{12}$CO(2-1) observations of the central region of the nearby barred spiral galaxy NGC 5806. NGC 5806 has a highly structured molecular gas distribution with a clear nucleus, a nuclear ring and offset dust lanes. We identify $170$ spatially- and spectrally-resolved giant molecular clouds (GMCs). These clouds have comparable sizes ($R_{\mathrm{c}}$) and larger gas masses, observed linewidths ($σ_{\mathrm{obs,los}}$) and gas mass surface densities than those of clouds in the Milky Way disc. The size -- linewidth relation of the clouds is one of the steepest reported so far ($σ_{\mathrm{obs,los}}\propto R_{\mathrm{c}}^{1.20}$), the clouds are on average only marginally bound (with a mean virial parameter $\langleα_{\mathrm{vir}}\rangle\approx2$), and high velocity dispersions are observed in the nuclear ring. These behaviours are likely due to bar-driven gas shocks and inflows along the offset dust lanes, and we infer an inflow velocity of $\approx120$ kms$^{-1}$ and a total molecular gas mass inflow rate of $\approx5$ M$_\odot$ yr$^{-1}$ into the nuclear ring. The observed internal velocity gradients of the clouds are consistent with internal turbulence. The number of clouds in the nuclear ring decreases with azimuthal angle downstream from the dust lanes without clear variation of cloud properties. This is likely due to the estimated short lifetime of the clouds ($\approx6$ Myr), which appears to be mainly regulated by cloud-cloud collision and/or shear processes. Overall, it thus seems that the presence of the large-scale bar and gas inflows to the centre of NGC 5806 affect cloud properties.
description: Accepted for publication in MNRAS, 20 pages, 16 figures
Learning from failure : development and discussion of a database of structural failures
Creators: name: Epp, Peter Yvon
Publisher: name: University of British Columbia
Year: 2022

description: This thesis presents and examines a database of structural failures, including bridges, buildings, and telecommunication towers. In addition to the database, a novelty of this work is the comparison of observed failure probabilities with target reliability index values in design codes. The study aims to improve the safety of future construction by exposing and understanding past structural failures. A labelling system is established to categorize and provide a basis for the future documentation of failures. The 275 failures in the database are collected from a search of newspaper articles, case studies, and the Imhof (2021) database of bridge failures. The scope of structural failures in this research considers partial and total collapse. The focus of the database is unexpected failures; therefore, failures due to vandalism, terrorism, or earthquakes are not considered. Earthquakes are excluded from the natural hazards considered because substantial damage is often expected during design-level ground shaking. Other natural hazards, such as ice accumulation, wind, and flooding, are considered. The majority of the failures that are considered in the database occurred in the United States; those account for 41% of the failures. Several insights are obtained from the total database. For instance, the most significant cause of failure for bridges is natural hazards, accounting for 29% of the failures. That is followed by 20% design errors and 15% failures caused by collisions. The most significant causes of failure for buildings are construction errors (24%), design errors (20%), and natural hazards (15%). The most significant failure causes for telecommunication towers are natural hazards (61%) and negligent maintenance errors (26%). The failures that occur during maintenance operations are primarily associated with the removal of structural members without adequate temporary support. The bridge superstructure type with the most failures is beam bridges. In the United States, truss bridges are apparently associated with the largest probability of failure. That failure probability corresponds to a reliability index of 3.1, which is inferior to the lifetime target reliability index of 3.5 from CSA S6.1.19.
Additional file 2 of Galectin-1 expression in the serum and placenta of pregnant women with fetal growth restriction and its significance
Creators: name: Jin, Xiao-Xiao
name: Ying, Xiang
name: Dong, Min-Yue
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2. The expression of Glaectin-1 in FGR group (n=3 per group).
Compact Steep Spectrum Radio Sources with Enhanced Star Formation are Smaller than $10\,$kpc
Creators: name: Gordon, Yjan A.
name: O'Dea, Christopher P.
name: Baum, Stefi A.
name: Bechtol, Keith
name: Duggal, Chetna
name: Ferguson, Peter S.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Compact Steep Spectrum (CSS) radio sources are active galactic nuclei that have radio jets propagating only on galactic scales, defined as having projected linear sizes (LS) of up to $20\,$kpc. CSS sources are generally hosted by massive early-type galaxies with little on-going star formation, however a small fraction are known to have enhanced star formation. Using archival data from the Faint Images of the Radio Sky at Twenty cm survey, the Very Large Array Sky Survey and the Sloan Digital Sky Survey we identify a volume-limited sample of $166$ CSS sources at $z<0.2$ with $L_{1.4\,\text{GHz}}>10^{24}\,\text{W}\,\text{Hz}^{-1}$. Comparing the star formation rates and linear sizes of these CSS sources, we find that the $\approx14\,\%$ of CSS sources with specific star formation rates above $0.01\,\text{Gyr}^{-1}$ all have $\text{LS}<10\,$kpc. We discuss the possible mechanisms driving this result, concluding that it is likely the excess star formation in these sources occurred in multiple bursts and ceased prior to the AGN jet being triggered.
description: Accepted for publication in ApJL. 9 pages, 5 figures
A new limit on the Ultra-High-Energy Cosmic-Ray flux with the Westerbork Synthesis Radio Telescope
Creators: name: ter Veen, S.
name: Buitink, S.
name: Falcke, H.
name: James, C. W.
name: Mevius, M.
name: Scholten, O.
name: Singh, K.
name: Stappers, B.
name: de Vries, K. D.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A particle cascade (shower) in a dielectric, for example as initiated by an ultra-high energy cosmic ray, will have an excess of electrons which will emit coherent Čerenkov radiation, known as the Askaryan effect. In this work we study the case in which such a particle shower occurs in a medium just below its surface. We show, for the first time, that the radiation transmitted through the surface is independent of the depth of the shower below the surface when observed from far away, apart from trivial absorption effects. As a direct application we use the recent results of the NuMoon project, where a limit on the neutrino flux for energies above $10^{22}$\,eV was set using the Westerbork Synthesis Radio Telescope by measuring pulsed radio emission from the Moon, to set a limit on the flux of ultra-high-energy cosmic rays.
description: Accepted for publication in Phys. Rev. D
Additional file 1: of miR-296-5p suppresses EMT of hepatocellular carcinoma via attenuating NRG1/ERBB2/ERBB3 signaling
Creators: name: Shi, Dong-Min
name: Li, Li-Xin
name: Bian, Xin-Yu
name: Shi, Xue-Jiang
name: Lu, Li-Li
name: Zhou, Hong-Xin
name: Pan, Ting-Jia
name: Zhou, Jian
name: Fan, Jia
name: Wu, Wei-Zhong
Publisher: name: figshare
Year: 2018
Subjects: Biological Sciences not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer

description: Table S1. HCC cell lines with different metastatic potentials. (DOCX 20 kb)
Magnetic field measurement from the Davis-Chandrasekhar-Fermi method employed with Atomic Alignment
Creators: name: Pavaskar, Parth
name: Yan, Huirong
name: Cho, Jungyeon
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The Davis-Chandrasekhar-Fermi (DCF) method is widely employed to estimate the mean magnetic field strength in astrophysical plasmas. In this study, we present a numerical investigation using the DCF method in conjunction with a promising new diagnostic tool for studying magnetic fields: the polarization of spectral lines resulting from the atomic alignment effect. We obtain synthetic spectro-polarimetry observations from 3D magnetohydrodynamic (MHD) turbulence simulations and estimate the mean magnetic field projected onto the plane of the sky using the DCF method with GSA polarization maps and a modification to account for the driving scale of turbulence. We also compare the method to the classical DCF approach using dust polarization observations. Our observations indicate that the modified DCF method correctly estimates the plane-of-sky projected magnetic field strengths for sub-Alfvénic turbulence using a newly proposed correction factor of $ξ' \in 0.35 - 0.75$. We find that the field strengths are accurately obtained for all magnetic field inclination and azimuth angles. We also observe a minimum threshold for the mean magnetic field inclination angle with respect to the line of sight, $θ_B \sim 16^\circ$, for the method. The magnetic field dispersion traced by the polarization from the spectral lines is comparable in accuracy to dust polarization, while mitigating some of the uncertainties associated with dust observations. The measurements of the DCF observables from the same atomic/ionic line targets ensure the same origin for the magnetic field and velocity fluctuations and offer a possibility of tracing the 3D direction of the magnetic field.
description: Accepted MNRAS, 11 pages, 9 figures, 2 tables
Constraining the Origin of Mars via Simulations of Multi-Stage Core Formation
Creators: name: Nathan, Gabriel
name: Rubie, David C.
name: Jacobson, Seth A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: It remains an elusive goal to simultaneously model the astrophysics of Solar System accretion while reproducing the mantle chemistry of more than one inner terrestrial planet. Here, we used a multistage core-mantle differentiation model based on Rubie et al. (2011,2015) to track the formation and composition of Earth and Mars in various Grand Tack formation simulations. Prior studies showed that in order to recreate Earth's mantle composition, it must grow first from reduced (Fe-metal rich and O-poor) building blocks and then from increasingly oxidized (FeO rich) material. This accretion chemistry occurs when an oxidation gradient exists across the disk so that the innermost solids are reduced and increasingly oxidized material is found at greater heliocentric distances. For a suite of Grand Tack simulations, we investigated whether Earth and Mars can be simultaneously produced by the same oxidation gradient. Our model did not find an oxidation gradient that simultaneously reproduces the mantle composition of Earth and Mars. Due to its small mass and rapid formation, the formation history of Mars-like planets is very stochastic which decreases the likelihood of compatibility with an Earth-producing oxidation gradient in any given realization. To reconcile the accretion history and ideal chemistry of the Mars-like planet with the oxidation gradient of an Earth-producing disk, we determined where in the Earth-producing disk Mars must have formed. We find that the FeO-rich composition of the Martian mantle requires that Mars' building blocks must originate exterior to 1.0 astronomical units (AU).
description: 20 pages, 7 figures, Accepted for publication at ICARUS 04/2023
Critical comment on the recent microscopic black hole search at the LHC
Creators: name: Park, Seong Chan
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Recently the CMS collaboration at the LHC reported "the first direct limit on black hole production at a particle accelerator" using a data sample corresponding to an integrated luminosity of 35/pb of pp-collision at a center of mass energy of 7 TeV. Even though the result has a strong impact on future searches, the interpretation lacks enough theoretical support. In this letter, we show that the parameter range which was considered by the CMS collaboration is actually out of the validity range of semi-classical black hole picture so that the Monte-Carlo simulation result which was crucially used in the analysis still needs further solid scientific basis.
description: 5 pages, 3 figures, version to appear in PLB
Erinnerung an Frau Margaretha Hagenbach-Bischoff, geboren den 7. Juni 1842, gestorben den 21. März 1887
Creators: name: Lindner, August
Publisher: name: Schweighausersche Buchdruckerei
Year: 1887
Subjects: subject: 920 Biografien, Genealogie, Insignien
subject: Nachruf
subject: Hagenbach-Bischoff, Margaretha

description: Enthält: Leichenrede gehalten von Herrn Pfarrer August Lindner den 23. März 1887; Choräle, gesungen von einem Freundeschor.
Orbital precession of stars in the Galactic center
Creators: name: Capuzzo-Dolcetta, Roberto
name: Bordoni, Matteo Sadun
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The region around the center of our Galaxy is very dense of stars. The kinematics of inner moving stars in the Galaxy (the so called S-stars) has been deeply studied by different research groups leading to the conclusion of the existence of a very compact object (Sgr A$^*$, likely a supermassive black hole) responsible for their high speed. Here we start from the observational evidence of orbital apsidal line precession for the S2 (also called S0-2) star to investigate on a theoretical side what level of quality in such regime of relatively strong gravitational field is reached in the orbit angular precession determination when using a direct orbital integration of the star motion subjected to an acceleration computed in the post-Newtonian (PN) scheme up to different orders. This approach, although approximated and limited to particle speed not exceeding $\sim \ 0.3 c$, allows the inclusion of various effects, like that of a possible spin of the central massive object. Our results show that the inclusion of PN terms above the standard 1PN term (the one corresponding to the classic Einstein-Schwarzschild estimate of pericenter advance) is compulsory to determine angular precession at sufficient level of accuracy for those penetrating stars that would allow to pick contemporary the value of the mass and of the spin of a rotating (Kerr-like) super massive black hole (SMBH). We discuss how future observational data, together with a proper modelization, could allow the determination of both mass and spin of the SMBH of our Galaxy.
description: 12 pages, 8 figures, 7 tables. Submitted to Monthly Notices of the Royal Astronomical Society
Additional file 2: of miR-296-5p suppresses EMT of hepatocellular carcinoma via attenuating NRG1/ERBB2/ERBB3 signaling
Creators: name: Shi, Dong-Min
name: Li, Li-Xin
name: Bian, Xin-Yu
name: Shi, Xue-Jiang
name: Lu, Li-Li
name: Zhou, Hong-Xin
name: Pan, Ting-Jia
name: Zhou, Jian
name: Fan, Jia
name: Wu, Wei-Zhong
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Table S2. Sequence of primers for Real-time PCR. (DOC 34 kb)
Exponential galaxy discs as the quasi-stationary distribution in a Markov chain model simulating stellar scattering
Creators: name: Wu, Jian
name: Struck, Curtis
name: Elmegreen, Bruce G.
name: D'Onghia, Elena
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Previous models have shown that stochastic scattering of stars in a two-dimensional galaxy disc can generate a time-independent surface density distribution that is an exponential divided by radius when a constant inward scattering bias is present. Here we show, using a Markov chain model, that similar profiles result from an outward scattering bias, although the disc surface density decreases slowly with time because of a net stellar outflow. The trend towards a near-exponential surface profile is robust, as it exists even if the scattering intensity has moderate radial and time dependences, subject to some limitations on the scattering rates discussed in the text. The exponential scale length of the pseudo-equilibrium disc depends on the scattering bias, the scattering length, and the size of the disc where scattering is important.
description: 18 pages, 20 figures
Exotic dynamically generated baryons with C$=-$1
Creators: name: Gamermann, D.
name: García-Recio, C.
name: Nieves, J.
name: Salcedo, L. L.
name: Tolos, L.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We follow a model based on the SU(8) symmetry for the interaction of mesons with baryons. The model treats on an equal footing the pseudo-scalars and the vector mesons, as required by heavy quark symmetry. The T-matrix calculated within an unitary scheme in coupled channels has poles which are interpreted as baryonic resonances.
description: 5 pages. Proceedings for Chiral10 workshop, Valencia, June 21-24 2010
Additional file 1 of A doctor-nurse-patient mobile health management system effectively controls blood glucose in chinese patients with type 2 diabetes mellitus: a prospective study
Creators: name: Tan, Xiaoqing
name: Qi, Zonghai
name: Chen, Ling
name: Li, Dongmin
name: Cai, Xiangyin
name: Song, Yi
name: Liu, Yajie
Publisher: name: figshare
Year: 2023
Subjects: Space Science
Medicine
Biotechnology
Biological Sciences not elsewhere classified
Science Policy
Mental Health
Computational Biology

description: Additional file 1.
title: Ð¢ÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ Ð¶Ð°ÑÐ¾Ð¿ÑÐ¾ÑÐ½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð½Ð¸ÐºÐµÐ»Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
title: Thermodynamic modeling of crystallization of high-temperature nickel-based casting alloys
Creators: name: ÐÐ°Ð»Ð¸Ð¼Ð¾Ð², Ð¢Ð¸Ð¼ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2021
Subjects: Ð¶Ð°ÑÐ¾Ð¿ÑÐ¾ÑÐ½ÑÐµ ÑÐ¿Ð»Ð°Ð²Ñ
Ð¶Ð°ÑÐ¾Ð¿ÑÐ¾ÑÐ½ÑÐµ ÑÐ¿Ð»Ð°Ð²Ñ Ð½Ð° Ð½Ð¸ÐºÐµÐ»ÐµÐ²Ð¾Ð¹ Ð¾ÑÐ½Ð¾Ð²Ðµ
ÑÑÐ¿ÐµÑÑÐ¿Ð»Ð°Ð²Ñ
ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
ÑÑÑÑÐºÑÑÑÐ°
high-temperature alloys
high-temperature alloys Ni-based
superalloys
thermodynamic modeling
crystallization
structure

description: Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¾ÑÐµÑÑÑ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ Ð¶Ð°ÑÐ¾Ð¿ÑÐ¾ÑÐ½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð½Ð¸ÐºÐµÐ»Ñ Ð¼ÐµÑÐ¾Ð´Ð°Ð¼Ð¸ ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ»Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ñ Ð¸ Ð¸Ð·ÑÑÐµÐ½Ñ Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð½Ð¸ÐºÐµÐ»Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ Ð¶Ð°ÑÐ¾Ð¿ÑÐ¾ÑÐ½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð². ÐÐ»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÐ¾Ð²Ð½Ñ Ð¶Ð°ÑÐ¾Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð²ÑÐ±Ð¾Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð° ÑÐ¿Ð»Ð°Ð²Ð° ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐµÐ¹ Ð¿Ð¾ Ð²ÑÐ±Ð¾ÑÑ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð°, ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÑÑÑÐµÐ³Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐ¼ ÐºÑÐ¸ÑÐµÑÐ¸ÑÐ¼ Ð¶Ð°ÑÐ¾Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸. ÐÐ°Ð½Ð½ÑÑ Ð·Ð°Ð´Ð°ÑÑ Ð¼Ð¾Ð¶Ð½Ð¾ ÑÐµÑÐ¸ÑÑ Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐµÑÐµ Ð½Ð° ÑÑÐ°Ð¿Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ¿Ð»Ð°Ð²Ð°.
description: As a result of the study, the processes of crystallization of cast heat-resistant alloys based on nickel by the methods of thermodynamic modeling were investigated. State diagrams of various Ni-based systems were constructed and studied. Thermodynamic modeling of crystallization processes of cast heat-resistant alloys has been carried out. To determine the level of heat resistance, optimization criteria were selected. It is shown that a reasonable choice of the optimal alloy composition is an optimization problem for the choice of a chemical composition that meets the developed criteria for high-temperature strength. This problem can be solved using thermodynamic modeling methods at the stage of alloy development.
Additional file 3 of Galectin-1 expression in the serum and placenta of pregnant women with fetal growth restriction and its significance
Creators: name: Jin, Xiao-Xiao
name: Ying, Xiang
name: Dong, Min-Yue
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 3. A western blot analysis of GAPDH expression in control patients (n=3 per group).
General Electric Quarterly Survey 72-04, Versions I & II, Prof, & Manag., I & II, College Student
Creators: name: Electric, General
Publisher: name: Roper Center for Public Opinion Research
Year: 2022

description: Adult sample: Most interesting concern (1); local community interests (1); US-Vietnam settlement (1); race relations (1); future race relations (1); companies helping race relations (1); price controls (1); wage controls (1); unaffordable purchases (1); government activity changes (12); defense spending (7); company regulations (1); national issues discussion (2); importance of economic competition (3); pollution (5); large companies effects (1); best job aspects (1); switching employers (3); future career goals (1); length of residency (1); housing aspects (2); housing satisfaction (1); previous housing (1); housing improvements (3); moving away (2); activity danger levels (6); performances seen (4); income change (1); price changes (1); inflation responsibility (2). College Student sample: Most interesting concern (1); US-Vietnam settlement (1); race relations (1); future race relations (1); companies helping race relations (1); unaffordable purchases (1); government activity changes (6); defense spending (7); national issues discussion (2); air pollution (5); large companies effects (1); activity danger levels (6); college attended (2); class year (1); major (1); degree (1); preferred career (2); academic standing (2).
Additional file 4 of Galectin-1 expression in the serum and placenta of pregnant women with fetal growth restriction and its significance
Creators: name: Jin, Xiao-Xiao
name: Ying, Xiang
name: Dong, Min-Yue
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 4. A western blot analysis of GAPDH expression in FGR group (n=3).
Bahadur Representation for U-Quantiles of Dependent Data
Creators: name: Wendler, Martin
Publisher: name: arXiv
Year: 2010
Subjects: subject: Statistics Theory (math.ST)
subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 62G30, 62G20 (primary), 62M10 (secondary)

description: U-quantiles are applied in robust statistics, like the Hodges-Lehmann estimator of location for example. They have been analyzed in the case of independent random variables with the help of a generalized Bahadur representation. Our main aim is to extend these results to U-quantiles of strongly mixing random variables and functionals of absolutely regular sequences. We obtain the central limit theorem and the law of the iterated logarithm for U-quantiles as straightforward corollaries. Furthermore, we improve the existing result for sample quantiles of mixing data.
Additional file 1 of Galectin-1 expression in the serum and placenta of pregnant women with fetal growth restriction and its significance
Creators: name: Jin, Xiao-Xiao
name: Ying, Xiang
name: Dong, Min-Yue
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1. The expression of Glaectin-1 in control group (n=3).
Finite temperature stability of a trapped dipolar Bose gas
Creators: name: Bisset, R. N.
name: Baillie, D.
name: Blakie, P. B.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We calculate the stability diagram for a trapped normal Bose gas with dipole-dipole interactions. Our study characterizes the roles of trap geometry, temperature, and short-ranged interactions on the stability. We predict a robust double instability feature in oblate trapping geometries arising from the interplay of thermal gas saturation and the anisotropy of the interaction. Our results are relevant to current experiments with polar molecules and will be useful in developing strategies to obtain a polar molecule Bose-Einstein condensate.
description: 5 pages, 2 figures
WASP-131 b with ESPRESSO I: A bloated sub-Saturn on a polar orbit around a differentially rotating solar-type star
Creators: name: Doyle, L.
name: Cegla, H. M.
name: Anderson, D. R.
name: Lendl, M.
name: Bourrier, V.
name: Bryant, E.
name: Vines, J.
name: Allart, R.
name: Bayliss, D.
name: Burleigh, M. R.
name: Buchschacher, N.
name: Casewell, S. L.
name: Hawthorn, F.
name: Jenkins, J. S.
name: Lafarga, M.
name: Moyano, M.
name: Psaridi, A.
name: Roguet-Kern, N.
name: Sosnowska, D.
name: Wheatley, P.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In this paper, we present observations of two high-resolution transit datasets obtained with ESPRESSO of the bloated sub-Saturn planet WASP-131~b. We have simultaneous photometric observations with NGTS and EulerCam. In addition, we utilised photometric lightcurves from {\tess}, WASP, EulerCam and TRAPPIST of multiple transits to fit for the planetary parameters and update the ephemeris. We spatially resolve the stellar surface of WASP-131 utilising the Reloaded Rossiter McLaughlin technique to search for centre-to-limb convective variations, stellar differential rotation, and to determine the star-planet obliquity for the first time. We find WASP-131 is misaligned on a nearly retrograde orbit with a projected obliquity of $λ= 162.4\substack{+1.3 \\ -1.2}^{\circ}$. In addition, we determined a stellar differential rotation shear of $α= 0.61 \pm 0.06$ and disentangled the stellar inclination ($i_* = 40.9\substack{+13.3 \\ -8.5}^{\circ}$) from the projected rotational velocity, resulting in an equatorial velocity of $v_{\rm{eq}} = 7.7\substack{+1.5 \\ -1.3}$~km s$^{-1}$. In turn, we determined the true 3D obliquity of $ψ= 123.7\substack{+12.8 \\ -8.0}^{\circ}$, meaning the planet is on a perpendicular/polar orbit. Therefore, we explored possible mechanisms for the planetary system's formation and evolution. Finally, we searched for centre-to-limb convective variations where there was a null detection, indicating that centre-to-limb convective variations are not prominent in this star or are hidden within red noise.
description: 15 Pages, 10 Figures and 4 Tables Accepted for Publication in MNRAS. arXiv admin note: text overlap with arXiv:2207.10127
Periodicity Analysis of the Logistic Map over Ring $\mathbb{Z}_{3^n}$
Creators: name: Lu, Xiaoxiong
name: Xie, Eric Yong
name: Li, Chengqing
Publisher: name: arXiv
Year: 2023
Subjects: subject: Information Theory (cs.IT)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences
subject: 65P20

description: Periodicity analysis of sequences generated by a deterministic system is a long-standing challenge in both theoretical research and engineering applications. To overcome the inevitable degradation of the Logistic map on a finite-precision circuit, its numerical domain is commonly converted from a real number field to a ring or a finite field. This paper studies the period of sequences generated by iterating the Logistic map over ring $\mathbb{Z}_{3^n}$ from the perspective of its associate functional network, where every number in the ring is considered as a node, and the existing mapping relation between any two nodes is regarded as a directed edge. The complete explicit form of the period of the sequences starting from any initial value is given theoretically and verified experimentally. Moreover, conditions on the control parameter and initial value are derived, ensuring the corresponding sequences to achieve the maximum period over the ring. The results can be used as ground truth for dynamical analysis and cryptographical applications of the Logistic map over various domains.
description: 10 pages
Programme - 1st MIDA Spring School, 2-7 March 2020, Catania
Creators: name: Debargue Audrey
name: Galluccio Giulia
name: Buresi Pascal
Publisher: name: Zenodo
Year: 2020
Subjects: ITN MIDA
PROGRAMME
SPRING SCHOOL
Università degli studi di Catania
ISLAM
SOCIAL SCIENCES
GRAPHIC DESIGN

description: 1st MIDA Spring School 2nd March 2020 - 7th March 2020 Università degli studi di Catania Contesting authority: knowledge, power and expressions of selhood
Dynamical Casimir effect on surface waves
Creators: name: Saharian, A. A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We consider the quantum radiation of scalar particles from a surface wave excited on a plane surface of a mirror. It is assumed that the field obeys Dirichlet condition on the boundary of the mirror. In both cases of running and standing surface waves the expression is given for the spectral-angular distribution of the number of the radiated quanta.
description: 7 pages, 3 figures, Talk presented at the International Conference "Electrons, Positrons, Neutrons and X-rays Scattering Under External Influences", Yerevan-Meghri, Armenia, October 26-30, 2009
Stochastic kinetics of a single headed motor protein: dwell time distribution of KIF1A
Creators: name: Garai, Ashok
name: Chowdhury, Debashish
Publisher: name: arXiv
Year: 2010
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Subcellular Processes (q-bio.SC)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: KIF1A, a processive single headed kinesin superfamily motor, hydrolyzes Adenosine triphosphate (ATP) to move along a filamentous track called microtubule. The stochastic movement of KIF1A on the track is characterized by an alternating sequence of pause and translocation. The sum of the durations of pause and the following translocation defines the dwell time. Using the NOSC model (Nishinari et. al. PRL, {\bf 95}, 118101 (2005)) of individual KIF1A, we systematically derive an analytical expression for the dwell time distribution. More detailed information is contained in the probability densities of the "conditional dwell times" $τ_{\pm\pm}$ in between two consecutive steps each of which could be forward (+) or backward (-). We calculate the probability densities $Ξ_{\pm\pm}$ of these four conditional dwell times. However, for the convenience of comparison with experimental data, we also present the two distributions $Ξ_{\pm}^{*}$ of the times of dwell before a forward (+) and a backward (-) step. In principle, our theoretical prediction can be tested by carrying out single-molecule experiments with adequate spatio-temporal resolution.
description: Author-edited final version published in EPL
Statistics of non-linear stochastic dynamical systems under Lévy noises by a convolution quadrature approach
Creators: name: Cottone, Giulio
Publisher: name: arXiv
Year: 2010
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 65R10, 65D32, 60H15, 65C30

description: This paper describes a novel numerical approach to find the statistics of the non-stationary response of scalar non-linear systems excited by Lévy white noises. The proposed numerical procedure relies on the introduction of an integral transform of Wiener-Hopf type into the equation governing the characteristic function. Once this equation is rewritten as partial integro-differential equation, it is then solved by applying the method of convolution quadrature originally proposed by Lubich, here extended to deal with this particular integral transform. The proposed approach is relevant for two reasons: 1) Statistics of systems with several different drift terms can be handled in an efficient way, independently from the kind of white noise; 2) The particular form of Wiener-Hopf integral transform and its numerical evaluation, both introduced in this study, are generalizations of fractional integro-differential operators of potential type and Grünwald-Letnikov fractional derivatives, respectively.
description: 20 pages, 5 figures
Additional file 1 of Generation and Starch Characterization of Non-Transgenic BEI and BEIIb Double Mutant Rice (Oryza sativa) with Ultra-High Level of Resistant Starch
Creators: name: Miura, Satoko
name: Koyama, Nana
name: Crofts, Naoko
name: Hosaka, Yuko
name: Abe, Misato
name: Fujita, Naoko
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
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: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology
subject: 60506 Virology

description: Additional file 1: Table S1. Percentages and average chain length of amylopectin branches analyzed by capillary electrophoresis.
The Gaia-ESO Survey: Empirical estimates of stellar ages from lithium equivalent widths (EAGLES)
Creators: name: Jeffries, R. D.
name: Jackson, R. J.
name: Wright, Nicholas J.
name: Weaver, G.
name: Gilmore, G.
name: Randich, S.
name: Bragaglia, A.
name: Korn, A. J.
name: Smiljanic, R.
name: Biazzo, K.
name: Casey, A. R.
name: Frasca, A.
name: Gonneau, A.
name: Guiglion, G.
name: Morbidelli, L.
name: Prisinzano, L.
name: Sacco, G. G.
name: Tautvaišienė, G.
name: Worley, C. C.
name: Zaggia, S.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present an empirical model of age-dependent photospheric lithium depletion, calibrated using a large, homogeneously-analysed sample of 6200 stars in 52 open clusters, with ages from 2--6000 Myr and $-0.3<{\rm [Fe/H}]<0.2$, observed in the Gaia-ESO spectroscopic survey. The model is used to obtain age estimates and posterior age probability distributions from measurements of the Li I 6708A equivalent width for individual (pre) main sequence stars with $3000 < T_{\rm eff}/{\rm K} <6500$, a domain where age determination from the HR diagram is either insensitive or highly model-dependent. In the best cases, precisions of 0.1 dex in log age are achievable; even higher precision can be obtained for coeval groups and associations where the individual age probabilities of their members can be combined. The method is validated on a sample of exoplanet-hosting young stars, finding agreement with claimed young ages for some, but not others. We obtain better than 10 per cent precision in age, and excellent agreement with published ages, for seven well-studied young moving groups. The derived ages for young clusters ($<1$ Gyr) in our sample are also in good agreement with their training ages, and consistent with several published, model-insensitive lithium depletion boundary ages. For older clusters there remain systematic age errors that could be as large as a factor of two. There is no evidence to link these errors to any strong systematic metallicity dependence of (pre) main sequence lithium depletion, at least in the range $-0.29 < {\rm [Fe/H]} < 0.18$. Our methods and model are provided as software -- "Empirical AGes from Lithium Equivalent widthS" (EAGLES).
description: Accepted for publication in Monthly Notices of the Royal Astronomical Society. Code available at https://github.com/robdjeff/eagles
Beating in electronic transport through quantum dot based devices
Creators: name: Trocha, Piotr
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Electronic transport through a two-level system driven by external electric field and coupled to (magnetic or non-magnetic) electron reservoirs is considered theoretically. The basic transport characteristics such as current and tunnel magnetoresistance (TMR) are calculated in the weak coupling approximation by the use of rate equation connected with Green function formalism and slave-boson approach. The time dependent phenomenon is considered in the gradient expansion approximation. The results show that coherent beats pattern can be observed both in current and TMR. The proposed system consisting of two quantum dots attached to external leads, in which the dots' levels can be tuned independently, can be realized experimentally to test this well known physical phenomenon. Finally, we also indicate possible practical applications of such device.
description: 9 pages, 9 figures
ALMACAL X: Constraints on molecular gas in the low-redshift circumgalactic medium
Creators: name: Klitsch, Anne
name: Davis, Timothy A.
name: Hamanowicz, Aleksandra
name: van de Voort, Freeke
name: Péroux, Céline
name: Zwaan, Martin A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Despite its crucial role in galaxy evolution, the complex circumgalactic medium (CGM) remains underexplored. Although it is known to be multi-phase, the importance of the molecular gas phase to the total CGM mass budget is, to date, unconstrained. We present the first constraints on the molecular gas covering fraction in the CGM of low-redshift galaxies, using measurements of CO column densities along sightlines towards mm-bright background quasars with intervening galaxies. We do not detect molecular absorption against the background quasars. For the individual, low-redshift, 'normal' galaxy haloes probed here, we can therefore rule out the presence of an extremely molecular gas-rich CGM, as recently reported in high-redshift protoclusters and around luminous active galactic nuclei. We also set statistical limits on the volume filling factor of molecular material in the CGM as a whole, and as a function of radius. ISM-like molecular clouds of ~30 pc in radius with column densities of N(CO) >~ 10^16 cm^-2 have volume filling factors of less than 0.2 per cent. Large-scale smooth gas reservoirs are ruled out much more stringently. The development of this technique in the future will allow deeper constraining limits to be set on the importance (or unimportance) of molecular gas in the CGM.
description: 5 pages, 5 figures, accepted for publication in MNRAS
Potts q-color field theory and scaling random cluster model
Creators: name: Delfino, Gesualdo
name: Viti, Jacopo
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study structural properties of the q-color Potts field theory which, for real values of q, describes the scaling limit of the random cluster model. We show that the number of independent n-point Potts spin correlators coincides with that of independent n-point cluster connectivities and is given by generalized Bell numbers. Only a subset of these spin correlators enters the determination of the Potts magnetic properties for q integer. The structure of the operator product expansion of the spin fields for generic q is also identified. For the two-dimensional case, we analyze the duality relation between spin and kink field correlators, both for the bulk and boundary cases, obtaining in particular a sum rule for the kink-kink elastic scattering amplitudes.
description: 27 pages; 6 figures. Published version, some comments and references added