cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
End of Fieldwork Report: Archaeological Testing at AZ AA:12:130 (ASM) for the Effluent Pipe Outfall Realignment, Pima County Landfill, Pima County, Arizona
Creators: name: System User
Publisher: name: SWCA, Inc. Environmental Consultants
Year: 1997
Subjects: subject: Tucson Basin
valueUri: https://core.tdar.org/browse/geographic-keyword/2758/tucson-basin
subject: Pima (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/7353/pima-county
subject: Arizona (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/79515/arizona-state-territory
subject: Middle Archaic
valueUri: https://core.tdar.org/browse/temporal-keyword/3094/middle-archaic
subject: Hohokam
valueUri: https://core.tdar.org/browse/culture-keyword/21/hohokam
subject: Huhugam
valueUri: https://core.tdar.org/browse/culture-keyword/8166/huhugam
subject: AZ AA:12:130 (ASM)
valueUri: https://core.tdar.org/browse/site-name/102827/az-aa12130-asm
subject: Sheet Midden
valueUri: https://core.tdar.org/browse/site-type/349/sheet-midden
subject: Pit
valueUri: https://core.tdar.org/browse/site-type/355/pit
subject: Firepit
valueUri: https://core.tdar.org/browse/site-type/871/firepit
subject: Midden
valueUri: https://core.tdar.org/browse/site-type/347/midden
subject: Ceramic
valueUri: https://core.tdar.org/browse/material-type/1/ceramic
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Data Recovery / Excavation
valueUri: https://core.tdar.org/browse/investigation-type/5/data-recovery-excavation
subject: Research Design / Data Recovery Plan
valueUri: https://core.tdar.org/browse/investigation-type/9/research-design-data-recovery-plan
subject: Site Evaluation / Testing
valueUri: https://core.tdar.org/browse/investigation-type/10/site-evaluation-testing

description: Archaeologists from SWCA, Inc., Environmental Consultants, conducted test excavations at site AZ AA:12:130 (ASM) on November 21 and 22, 1996. These excavations consisted of five backhoe trenches long the centerline of a planned effluent pipe outfall realignment for Pima County Waste Water Management. This document summarizes the results of archaeological testing on the segment of the pipeline that crosses the plotted location of a known Middle Archaic site. Four features were identified during testing.
Growth Kinetics in Systems with Local Symmetry
Creators: name: Liu, Fong
Publisher: name: arXiv
Year: 1993
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The phase transition kinetics of Ising gauge models are investigated. Despite the absence of a local order parameter, relevant topological excitations that control the ordering kinetics can be identified. Dynamical scaling holds in the approach to equilibrium, and the growth of typical length scale is characteristic of a new universality class with $L(t)\sim \left(t/\ln t\right)^{1/2}$. We suggest that the asymptotic kinetics of the 2D Ising gauge model is dual to that of the 2D annihilating random walks, a process also known as the diffusion-reaction $A+A\to \hbox{inert}$.
description: 10 pages in Tex, 2 Postscript figures appended, NSF-ITP-93-40
Machine learning and genomics: precision medicine vs. patient privacy
Creators: name: Azencott, Chloé-Agathe
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: Machine learning can have major societal impact in computational biology applications. In particular, it plays a central role in the development of precision medicine, whereby treatment is tailored to the clinical or genetic features of the patient. However, these advances require collecting and sharing among researchers large amounts of genomic data, which generates much concern about privacy. Researchers, study participants and governing bodies should be aware of the ways in which the privacy of participants might be compromised, as well as of the large body of research on technical solutions to these issues. We review how breaches in patient privacy can occur, present recent developments in computational data protection, and discuss how they can be combined with legal and ethical perspectives to provide secure frameworks for genomic data sharing.
description: 13 pages, submitted to Philosophical Transactions A
Statistical analysis of Ni nanowires breaking processes: a numerical simulation study
Creators: name: García-Mochales, P.
name: Paredes, R.
name: Peláez, S.
name: Serena, P. A.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A statistical analysis of the breaking behavior of Ni nanowires is presented. Using molecular dynamic simulations, we have determined the time evolution of both the nanowire atomic structure and its minimum cross section (Sm(t)). Accumulating thousands of independent breaking events, Sm histograms are built and used to study the influence of the temperature, the crystalline stretching direction and the initial nanowire size. The proportion of monomers, dimers and more complex structures at the latest stages of the breaking process are calculated, finding important differences among results obtained for different nanowire orientations and sizes. Three main cases have been observed. (A) [111] stretching direction and large nanowire sizes: the wire evolves from more complex structures to monomers and dimers prior its rupture; well ordered structures is presented during the breaking process. (B) Large nanowires stretched along the [100] and [110] directions: the system mainly breaks from complex structures (low probability of finding monomers and dimers), having disordered regions during their breakage; at room temperature, a huge histogram peak around Sm=5 appears, showing the presence of long staggered pentagonal Ni wires with ...-5-1-5-... structure. (C) Initial wire size is small: strong size effects independently on the temperature and stretching direction. Finally, the local structure around monomers and dimmers do not depend on the stretching direction. These configurations differ from those usually chosen in static studies of conductance.
description: 18 pages, 13 figures
Real soliton lattices of KP-II and desingularization of spectral curves: the Gr^{TP}(2,4) case
Creators: name: Abenda, Simonetta
name: Grinevich, Petr G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences
subject: 35Q53, 58F07

description: We apply the general construction developed in references [4,5] to the first non-trivial case of Gr^{TP}(2,4). In particular, we construct finite-gap KP-II real quasiperiodic solutions in the form of soliton lattice corresponding to a smooth genus 4 M-curve, which is a desingularization of a reducible rational M-curve for soliton data in Gr^{TP}(2,4).
description: 20 pages, several figures. Minor corrections
Michelson-Morley Experiments: at the crossroads of Relativity, Cosmology and Quantum Physics
Creators: name: Consoli, Maurizio
name: Pluchino, Alessandro
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: Quantum nonlocality would naturally fit into a version of relativity with a preferred reference system. However, acceptance of this idea has traditionally required experimental evidence. Namely, detecting in laboratory a small angular dependence of the velocity of light correlated to the cosmic motion of the Earth. Here, we summarize a new theoretical framework where the tiny, irregular residuals observed so far, from Michelson-Morley to current experiments of laser interferometry, can indeed be understood in terms of the Earth motion in the Cosmic Microwave Background observed directly with satellites in space. Our results, challenging the usual null interpretation, emphasize the central role of 'ether-drift' experiments for Relativity, Cosmology and Quantum Physics.
description: 60 pages, 25 figures and 3 tables
Dynamical Coupled-Channels Model Analysis of π-N Scattering and Electromagnetic Pion Production Reactions
Creators: name: Julia-Diaz, B.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The ability of the coupled-channels model (MSL) developed in recently in Ref. \cite{msl} to account simultaneously for the $πN$ scattering data and the $π$ photoproduction reactions on the nucleon is presented. An accurate description of $πN$ scattering has been obtained. A preliminary description of $π$ photoproduction is also discussed.
description: Invited talk. 11th International Conference on Meson-Nucleon Physics and the Structure of the Nucleon, Sept. 10th-14th 2007 (MENU 2007), Juelich, Germany
Pre-perihelion Monitoring of Interstellar Comet 2I/Borisov
Creators: name: Prodan, George P.
name: Popescu, Marcel
name: Licandro, Javier
name: Akhlaghi, Mohammad
name: de León, Julia
name: Tatsumi, Eri
name: Pastrav, Bogdan Adrian
name: Hibbert, Jacob M.
name: Văduvescu, Ovidiu
name: Simion, Nicolae Gabriel
name: Pallé, Enric
name: Narita, Norio
name: Fukui, Akihiko
name: Murgas, Felipe
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The discovery of interstellar comet 2I/Borisov offered the unique opportunity to obtain a detailed analysis of an object coming from another planetary system, and leaving behind material in our interplanetary space. We continuously observed 2I/Borisov between October 3 and December 13, 2019 using the 1.52-m Telescopio Carlos Sánchez equipped with MuSCAT2 instrument, and the 2.54-m Isaac Newton Telescope with Wide Field Camera. We characterize its morphology and spectro-photometric features using the data gathered during this extended campaign. Simultaneous imaging in four bands ($g$, $r$, $i$, and $z_s$) reveals a homogeneous composition and a reddish hue, resembling Solar System comets, and as well a diffuse profile exhibiting familiar cometary traits. We discern a stationary trend fluctuating around a constant activity level throughout October and November 2019. Subsequently, a reduction in activity is observed in December. Dust production and mass loss calculations indicate approximately an average of 4 kg/s before perihelion, while after perihelion the net mass loss is about 0.6 kg/s. Our simulations indicate the most probable size of coma dust particles should be in the range 200-250 nm, and the terminal speed around 300 m/s. The spectrum acquired with the 4.2-m William Herschel Telescope shows the presence of a strong CN line for which we find a gas production rate of $1.2 \times 10^{24}~s^{-1}$. We also detected NH$_2$ and OI bands. The ratio between NH$_2$ and CN productions is $\log (NH_2/CN) =-0.2$. Overall, this observing campaign provides a new understanding of 2I/Borisov's unique characteristics and activity patterns.
description: accepted to MNRAS on 12th Feb 2024
Measuring the viewing angle of GW170817 with electromagnetic and gravitational waves
Creators: name: Finstad, Daniel
name: De, Soumi
name: Brown, Duncan A.
name: Berger, Edo
name: Biwer, Christopher M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The joint detection of gravitational waves (GWs) and electromagnetic (EM) radiation from the binary neutron star merger GW170817 ushered in a new era of multi-messenger astronomy. Joint GW-EM observations can be used to measure the parameters of the binary with better precision than either observation alone. Here, we use joint GW-EM observations to measure the viewing angle of GW170817, the angle between the binary's angular momentum and the line of sight. We combine a direct measurement of the distance to the host galaxy of GW170817 (NGC 4993) of $40.7\pm 2.36$ Mpc with the Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo GW data and find that the viewing angle is $32^{+10}_{-13}\,\pm 1.7$ degrees (90% confidence, statistical, and systematic errors). We place a conservative lower limit on the viewing angle of $\ge 13^\circ$, which is robust to the choice of prior. This measurement provides a constraint on models of the prompt $γ$-ray and radio/X-ray afterglow emission associated with the merger; for example, it is consistent with the off-axis viewing angle inferred for a structured jet model. We provide for the first time the full posterior samples from Bayesian parameter estimation of LIGO/Virgo data to enable further analysis by the community.
description: 7 pages, 3 figures
MPEC 2024-U87 : 2024 UZ1
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 UZ1

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
A Uniformly Selected Sample of Low-Mass Black Holes in Seyfert 1 Galaxies. II. The SDSS DR7 Sample
Creators: name: Liu, He-Yang
name: Yuan, Weimin
name: Dong, Xiao-Bo
name: Zhou, Hongyan
name: Liu, Wen-Juan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A new sample of 204 low-mass black holes (LMBHs) in active galactic nuclei (AGNs) is presented with black hole masses in the range of (1-20) * 10^5 M_sun. The AGNs are selected from a systematic search among galaxies in the Seventh Data Release (DR 7) of the Sloan Digital Sky Survey (SDSS), and careful analyses of their optical spectra and precise measurement of spectral parameters. Combining them with our previous sample selected from the SDSS DR 4 makes it the largest LMBH sample so far, totaling over 500 objects. Some of the statistical properties of the combined LMBH AGN sample are briefly discussed, in the context of exploring the low-mass end of the AGN population. Their X-ray luminosities follow the extension of the previously known correlation with the [O III] luminosity. The effective optical-to-X-ray spectral indices α_OX, albeit with a large scatter, are broadly consistent with the extension of the relation with the near-UV luminosity L_2500Å. Interestingly, a correlation of α_OX with black hole mass is also found in the sense that α_OX is statistically flatter (stronger X-ray relative to optical) for lower black hole mass. Only 26 objects, mostly radio loud, were detected in radio at 20 cm in the FIRST survey, giving a radio loud fraction of 4%. The host galaxies of LMBHs have stellar masses in the range of 10^8.8-10^12.4 M_sun and optical colors typical of Sbc spirals. They are dominated by young stellar populations that seem to have undergone a continuous star formation history.
description: 5 tables, 16 figures, ApJS accepted
Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
Creators: name: Scholz-Diaz, Laura
name: Martin-Navarro, Ignacio
name: Falcon-Barroso, Jesus
name: Lyubenova, Mariya
name: van de Ven, Glenn
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In the standard cosmological model, the assembly of galaxies is primarily driven by the growth of their host dark matter halos. At the center of these halos, however, baryonic processes take over, leading to the plethora of observed galaxy properties. The coupling between baryonic and dark matter physics is central to our understanding of galaxies and yet, it remains a challenge for theoretical models and observations. Here, we demonstrate that measured ages, metallicities, stellar angular momentum, morphology and star formation rates, correlate with both stellar and halo mass. Using dynamical modeling, we find that at fixed stellar mass, CALIFA galaxies become younger, more metal-poor and rotationally supported, have higher star formation rates and later-type morphologies as their total mass increases, with independent stellar and total masses measurements. These results indicate that the formation of galaxies and thus their baryonic properties do not vary with stellar mass alone, with halo mass also playing an important role.
description: 14 pages, 5 Figures. Accepted in Nature Astronomy
FARG'ONA VODIYSINING IQLIM SHAROITI
Creators: name: Tursunova, Diyoraxon
Publisher: name: Zenodo
Year: 2025

description: Farg'ona vodiysining O'rta Osiyo kontekstidagi ahamiyatini belgilaydi. Unda vodiyning iqlim sharoitini tushunish, ularning qishloq xo‘jaligi, suv resurslari va mintaqaviy taraqqiyotga qanday ta’sir qilishini ko‘rib chiqish maqsadi belgilangan. Inson va atrof-muhit o'rtasidagi o'zaro munosabatlarni shakllantirishda iqlimning roli ham tanishtiriladi.
Gauge invariant determination of charged hadron masses
Creators: name: Hansen, Martin
name: Lucini, Biagio
name: Patella, Agostino
name: Tantalo, Nazario
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: In this paper we show, for the first time, that charged-hadron masses can be calculated on the lattice without relying on gauge fixing at any stage of the calculations. In our simulations we follow a recent proposal and formulate full QCD+QED on a finite volume, without spoiling locality, by imposing C-periodic boundary conditions in the spatial directions. Electrically charged states are interpolated with a class of operators, originally suggested by Dirac and built as functionals of the photon field, that are invariant under local gauge transformations. We show that the quality of the numerical signal of charged-hadron masses is the same as in the neutral sector and that charged-neutral mass splittings can be calculated with satisfactory accuracy in this setup. We also discuss how to describe states of charged hadrons with real photons in a fully gauge-invariant way by providing a first evidence that the proposed strategy can be numerically viable.
description: 17 pages, 3 figures, 1 table, accepted for publication in JHEP
Results of Archaeological Testing at Site AZ T:8:157 (ASM), Phoenix, Maricopa County, Arizona
Creators: name: Sorrell, Daniel H.
name: Phillips, Bruce G.
name: Bryce, William
Publisher: name: EcoPlan Associates, Inc.
Year: 2008
Subjects: subject: Sonoran Desertscrub Biotic Community
valueUri: https://core.tdar.org/browse/geographic-keyword/82928/sonoran-desertscrub-biotic-community
subject: Northern Periphery
valueUri: https://core.tdar.org/browse/geographic-keyword/83716/northern-periphery
subject: Lower Colorado River Subdivision
valueUri: https://core.tdar.org/browse/geographic-keyword/83829/lower-colorado-river-subdivision
subject: Phoenix Basin
valueUri: https://core.tdar.org/browse/geographic-keyword/27/phoenix-basin
subject: Maricopa (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3900/maricopa-county
subject: Hohokam
valueUri: https://core.tdar.org/browse/culture-keyword/21/hohokam
subject: AZ T:8:157 (ASM)
valueUri: https://core.tdar.org/browse/site-name/106010/az-t8157-asm
subject: Ceramic
valueUri: https://core.tdar.org/browse/material-type/1/ceramic
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Fire Cracked Rock
valueUri: https://core.tdar.org/browse/material-type/5/fire-cracked-rock
subject: Data Recovery / Excavation
valueUri: https://core.tdar.org/browse/investigation-type/5/data-recovery-excavation
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey
subject: Site Evaluation / Testing
valueUri: https://core.tdar.org/browse/investigation-type/10/site-evaluation-testing
subject: Systematic Survey
valueUri: https://core.tdar.org/browse/investigation-type/12/systematic-survey

description: The project area is located within the Phoenix Basin, part of the Basin and Range physiographic province (Chronic 2002). The Federal Highway Administration (FHWA) and the Arizona Department of Transportation (ADOT) intend to construct a new traffic interchange (TI) in the City of Phoenix, Maricopa County, Arizona. The new TI is part of a larger ADOT project that ultimately will increase the traffic capacity and allow access to the freeway as urban development continues to expand in the area. Archaeological site AZ T:8:157 (ASM) was identified as a scatter of aboriginal artifacts dating to between AD 200-1500 during a survey that included the current area of potential effects (APE). Those researchers (DeMaagd and others 2002:62) recommended that the site would require testing to determine its eligibility for inclusion in the National Register of Historic Places (National Register). EcoPlan Associates, Inc. (EcoPlan), as a subconsultant to ADOT’s pre-design consultant, PB, was tasked with preparation and implementation of a work plan for archaeological testing and, if warranted, subsequent data recovery, at site AZ T:8:157 (ASM) (Phillips 2006). Archaeological testing at site AZ T:8:157 (ASM) occurred on 22 May and 26 May 2006. This report presents the results of our investigations.
The Least Action Method, CDM and $Ω$
Creators: name: Dunn, A. M.
name: Laflamme, Raymond
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Peebles has suggested an interesting method to trace back in time positions of galaxies called the least action method. This method applied on the Local Group galaxies seems to indicate that we live in an $Ω\approx 0.1$ Universe. We have studied a CDM N-body simulation with $Ω=0.2$ and $H=50 kms^{-1}/Mpc$ and compare trajectories traced back from the Least Action Principle and the center of mass of the particle forming CDM halos. We show that the agreement between these set of trajectories is at best qualitative. We also show that the line of sight peculiar velocities are underestimated. This discrepancy is due to orphans, CDM particles which do not end up in halos. By varying the density parameter $Ω$ in the least action principle we show that using this method we would underestimate the density of the Universe by a factor of 4-5.
description: 8 pages, Plain Tex, 3 figures
S2 Table
Creators: name: Piri, Reza
name: Seyed-Moayed Alavian
name: Behzad, Mohammad Naghavi
name: Pilevari, Shamim
name: Mohajer, Aida Salman
Publisher: name: figshare
Year: 2018
Subjects: Biomarkers

description: PRISMA checklist for the systematic review and meta-analysis of early prediction of pre-eclampsia using fetal-placental axis biomarkers.
Supersymmetric, cold and lukewarm black holes in cosmological Einstein-Maxwell theory
Creators: name: Romans, L. J.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In flat space, the extreme Reissner-Nordstrøm (RN) black hole is distinguished by its coldness (vanishing Hawking temperature) and its supersymmetry. We examine RN solutions to Einstein-Maxwell theory with a cosmological constant $Λ$, classifying the cold black holes and, for positive $Λ$, the ``lukewarm" black holes at the same temperature as the de Sitter thermal background. For negative $Λ$, we classify the supersymmetric solutions within the context of $N=2$ gauged supergravity. One finds supersymmetric analogues of flat-space extreme RN black holes, which for nonzero $Λ$ differ from the cold black holes. In addition, there is an exotic class of supersymmetric solutions which cannot be continued to flat space, since the magnetic charge becomes infinite in that limit.
description: (18 pp., plain tex)
DBNets: A publicly available deep learning tool to measure the masses of young planets in dusty protoplanetary discs
Creators: name: Ruzza, Alessandro
name: Lodato, Giuseppe
name: Rosotti, Giovanni Pietro
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Machine Learning (cs.LG)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Current methods to characterize embedded planets in protoplanetary disc observations are severely limited either in their ability to fully account for the observed complex physics or in their computational and time costs. To address this shortcoming, we developed DBNets: a deep learning tool, based on convolutional neural networks, that analyses substructures observed in the dust continuum emission of protoplanetary discs to quickly infer the mass of allegedly embedded planets. We focussed on developing a method to reliably quantify not only the planet mass, but also the associated uncertainty introduced by our modelling and adopted techniques. Our tests gave promising results achieving an 87% reduction of the log Mp mean squared error with respect to an analytical formula fitted on the same data (DBNets metrics: lmse 0.016, r2-score 97%). With the goal of providing the final user of DBNets with all the tools needed to interpret their measurements and decide on their significance, we extensively tested our tool on out-of-distribution data. We found that DBNets can identify inputs strongly outside its training scope returning an uncertainty above a specific threshold and we thus provided a rejection criterion that helps determine the significance of the results obtained. Additionally, we outlined some limitations of our tool: it can be reliably applied only on discs observed with inclinations below approximately 60°, in the optically thin regime, with a resolution 8 times better than the gap radial location and with a signal-to-noise ratio higher than approximately ten. Finally, we applied DBNets to 33 actual observations of protoplanetary discs measuring the mass of 48 proposed planets and comparing our results with the available literature. We confirmed that most of the observed gaps imply planets in the sub-Jupiter regime. DBNets is publicly available at dbnets.fisica.unimi.it.
RETURN To an Address of the Legislative Assembly for copies of the following papers referring to the "Chinese Regulation Act, 1884;" a copy of the Attorney-General's report to His Honour the Lieutenant-Governor; copies of all Orders in Council and Rules and Regulations; copies of all letters or telegrams received or sent by any member of the Government; the names and date of appointment of Chinese Collectors.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
Excitons and Dark Fermions as Origins of Mott Gap, Pseudogap and Superconductivity in Cuprate Superconductors --- General Idea and Basic Concept Based on Gap Physics
Creators: name: Imada, Masatoshi
name: Suzuki, Takafumi J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Theory of doped Mott insulators is revisited in the light of recent understanding on the singular self-energy structure of the single-particle Green's function. The unique pole structure in the self-energy induces the high-temperature superconductivity in the anomalous part, while it generates Mott gap and pseudogap in the normal part. Here, we elucidate that fractionalization of electrons, which is exactly hold in the Mott insulator in the atomic limit, more generally produces the emergent Mott-gap fermion and dark (hidden) fermions. It does not require any spontaneous symmetry breaking. The two gaps are the consequences of the hybridization of these two fermions with quasiparticles. We further propose that the Mott-gap fermion and dark fermions are the fermionic component of Frenkel- and Wannier-type excitons, respectively, which coexist in the doped Mott insulator. The Bose-Einstein condensation of the Frenkel-type excitons allowed without spontaneous symmetry breaking holds a key for understanding the unique pole structure and the pseudogap through the instantaneous hybridization between the fractionalized quasiparticle and the dark fermion in analogy with the Mott gap. We argue that the high-$T_{\rm c}$ superconductivity is ascribed to the dipole attraction of the Wannier-type excitons. The gap formation mechanism is compared with that caused by conventional spontaneous symmetry breaking known over condensed matter and elementary particle physics including quantum chromodynamics. We propose a theoretical framework and discuss experimental tests to analyze this idea and concept.
description: 15 pages including 6 figures
B_s and B_d mixing in full lattice QCD using NRQCD b quarks
Creators: name: Gamiz, Elvira
name: Davies, Christine T. H.
name: Lepage, G. Peter
name: Shigemitsu, Junko
name: Wingate, Matthew
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We give a progress report on studies of B_s and B_d mixing with valence NRQCD b quarks and asqtad light quarks on the MILC configurations including the effect of 2+1 flavours of sea quarks. We explore methods for reducing statistical and systematic errors in the ratio ξ= f_{B_s}\sqrt{B_{B_s}}/f_{B_d}\sqrt{B_{B_d}}.
description: 7 pages, talk at The XXV International Symposium on Lattice Field Theory, July 30 - August 4 2007, Regensburg,
Galactic Chemical Evolution: Hydrogen Through Zinc
Creators: name: Timmes, by F. X.
name: Woosley, S. E.
name: Weaver, Thomas A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the output from a grid of 60 Type II supernova models (Woosley \& Weaver 1994) of varying mass (11 $\ltaprx$ M/M\sun $\ltaprx$ 40) and metallicity (0, 10$^{-4}$, 0.01, 0.1, and 1 Z\sol), the chemical evolution of 76 stable isotopes, from hydrogen to zinc, is calculated. The chemical evolution calculation employs a simple dynamical model for the Galaxy (infall with a 4 billion year $e$-folding time scale onto a exponential disk and 1/r$^2$ bulge), and standard evolution parameters, such as a Salpeter initial mass function and a quadratic Schmidt star formation rate. The theoretical results are compared in detail with observed stellar abundances in stars with metallicities in the range -3.0 $\ltaprx$ [Fe/H] $\ltaprx$ 0.0 dex. While our discussion focuses on the solar neighborhood where there are the most observations, the supernovae rates, an intrinsically Galactic quantity, are also discussed.
description: 114 pages including 39 figures, uuencoded gzipped postscript; accepted ApJ Supp
RETURN To an Order of the House for a copy of the report of Mr. Lee in reference to a proposed road to connect the Spallumcheen waggon road at Salmon Arm with the Canadian Pacific Railway; the report of Mr. Neil Black in reference to construction of a waggon road from the present Nicola road to Granite Creek; also Mr. A. Stevensons' report in reference to construction of a waggon road from Lytton to Foster's Bar.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
Nematicity and magnetism in LaFeAsO single crystals probed by $^{75}$As nuclear magnetic resonance
Creators: name: Ok, J. M.
name: Baek, S. -H.
name: Efremov, D. V.
name: Kappenberger, R.
name: Aswartham, S.
name: Kim, J. S.
name: Brink, J. van den
name: Büchner, B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report a $^{75}$As nuclear magnetic resonance study in LaFeAsO single crystals, which undergoes nematic and antiferromagnetic transitions at $T_\text{nem}\sim 156$ K and $T_N \sim 138$ K, respectively. Below $T_\text{nem}$, the $^{75}$As spectrum splits sharply into two for an external magnetic field parallel to the orthorhombic $a$ or $b$ axis in the FeAs planes. Our analysis of the data demonstrates that the NMR line splitting arises from an electronically driven rotational symmetry breaking. The $^{75}$As spin-lattice relaxation rate as a function of temperature shows that spin fluctuations are strongly enhanced just below $T_\text{nem}$. These NMR findings indicate that nematic order promotes spin fluctuations in magnetically ordered LaFeAsO, as observed in non-magnetic and superconducting FeSe. We conclude that the origin of nematicity is identical in both FeSe and LaFeAsO regardless of whether or not a long range magnetic order develops in the nematic state.
description: 5 pages, 4 figures, published as a rapid communication in PRB
title: Fascicule de Notices sur la carte pédologique de reconnaissance des grands groupes de sols de La Réunion
Creators: name: Riquier, Jean
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2017
Subjects: subject: pédologie
subject: sable
subject: sol
subject: alluvion
subject: formation superficielle
subject: classification des sols
subject: lithosol
subject: sol brunifié
subject: sol ferrallitique
subject: sol hydromorphe
subject: sol lythochrome
subject: sol à voune et mascareignite
subject: évolution du sol

description: Un fascicule de notices publié, en 1960, par l'Office de la recherche scientifique et technique outre-mer (ORSTOM) et l'Institut de Recherche Scientifique de Madagascar et écrit par Jean Riquier fournit des explications.
description: Relation: http://www.nakala.fr/data/11280/7e9926af
description: Relation: http://www.nakala.fr/data/11280/dbf1bab3
description: Relation: http://www.nakala.fr/data/11280/dc2228f9
description: Coverage: La Réunion
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0543
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0543, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0543, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Anatomy of the hyper-runaway star LP 40-365 with Gaia
Creators: name: Raddi, R.
name: Hollands, M. A.
name: Gaensicke, B. T.
name: Townsley, D. M.
name: Hermes, J. J.
name: Fusillo, N. P. Gentile
name: Koester, D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: LP 40-365 (aka GD 492) is a nearby low-luminosity hyper-runaway star with an extremely unusual atmospheric composition, which has been proposed as the remnant of a white dwarf that survived a subluminous Type Ia supernova (SN Ia) in a single-degenerate scenario. Adopting the Gaia Data Release (DR2) parallax, 1.58 +/- 0.03 mas, we estimate a radius of 0.18 +/- 0.01 Rsun, confirming LP 40-365 as a subluminous star that is ~ 15 times larger than a typical white dwarf and is compatible with the SN Ia remnant scenario. We present an updated kinematic analysis, making use of the Gaia parallax and proper motion, and confirm that Lp 40-365 is leaving the Milky Way at about 1.5 times the escape velocity of the Solar neighbourhood with a rest-frame velocity of 852 +/- 10 km/s. Integrating the past trajectories of LP 40-365, we confirm it crossed the Galactic disc 5.0 +/- 0.3 Myr ago in the direction of Carina, likely coming from beneath the plane. Finally, we estimate that LP 40-365 was ejected from its progenitor binary with a velocity of at least 600 km/s, which is compatible with theoretical predictions for close binaries containing a white dwarf and a helium-star donor.
description: 6 pages, 4 figures, 1 table. Accepted for publication on MNRAS
RETURN To an address of the Legislative Assembly for copies of all Orders in Council and correspondence respecting the sale of lots in 1884 at James Bay, Victoria, stating the number of lots sold and the price sold at ; and, also, respecting the proposed transfer to the Corporation of Victoria of the lands and buildings on Bastion Square, Victoria, now used as the Gaol, Police Barracks and Sheriff's Office.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
Susquehanna River young of the year smallmouth bass myxozoan (Myxobolus inornatus) dataset
Creators: name: Schall, Megan
name: Blazer, Vicki
name: Walsh, Heather
name: Smith, Geoffrey
name: Wertz, Timothy
name: Wagner, Tyler
Publisher: name: figshare
Year: 2018
Subjects: subject: 70499 Fisheries Sciences not elsewhere classified
subject: FOS: Agriculture, forestry and fisheries

description: The enclosed data file include young of the year smallmouth bass data from the Susquehanna River Basin assessing prevalence of a myxozoan parasite (Myxobolus inornatus). The young of the year smallmouth bass were collected during 2013-2016 across the Susquehanna River Basin and at several out of basin sites.
Heavy Mesons Photoproduction in Peripheral AA Collisions
Creators: name: Ducati, M. B. Gay
name: Martins, S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The exclusive photoproduction of the heavy vector mesons $ψ$'s and $Y$'s is investigated in peripheral lead-lead collisions for the energies available at the LHC, $\sqrt{s}=2.76$ TeV and $\sqrt{s}=5.02$ TeV. In order to evaluate the robustness of the light-cone color dipole formalism, previously tested in the ultraperipheral regime. It was calculated the rapidity distribution as well as the nuclear modification factor ($R_{AA}$) for the three centrality classes: 30%-50%, 50%-70% and 70%-90%. The transition from ultraperipheral to peripheral regime was carried out sophisticating the photon flux description and the photonuclear cross section, taking into account the effective interaction area. In our calculations, three scenarios were considered: (scenario 1) the direct application of the usual photon flux and of the photonuclear cross section without any relevant change in relation to the UPC's, (scenario 2) the application of an effective photon flux keeping the photonuclear cross section unchanged and (scenario 3) where it was also considered an effective photonuclear cross section. The results obtained from the three scenarios were compared with the ALICE measurements (only $J/ψ$ at the moment), showing a better agreement with the data in the more complete approach (scenario 3), mainly in the more central regions (30%-50% and 50%-70%) where the incertainty is smaller.
Gutzwiller wavefunction in the three-band Hubbard model: A variational Monte Carlo study
Creators: name: Oguri, A.
name: Asahta, T.
name: Maekawa, S.
Publisher: name: arXiv
Year: 1993
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The Gutzwiller wave function for the three-band Hubbard model on a two dimensional CuO$_2$ plane is studied by using the variational Monte Carlo (VMC) method in the limit $U_d \to \infty$, where $U_d$ is the Coulomb repulsion between holes on a Cu site. The VMC results for the energy and the fraction of $d$-holes are compared with those of the Rice-Ueda type Gutzwiller approximation (GA). The difference between the VMC and the GA results are most pronounced at half-filling, and away from half-filling the two results agree well in both the hole-doped and the electron-doped cases. The doping dependence of the momentum distribution function is also studied.
description: 18 pages (RevTeX), 8 figures (postscript) appended, for remaining 5 figures contact a40954a@nucc.cc.nagoya-u.ac.jp
SOCIO-POLITICAL SITUATION OF UZBEKISTAN IN THE CONTEXT OF ECOLOGICAL GLOBALIZATION
Creators: name: Gulomova, Rukhsora
Publisher: name: Zenodo
Year: 2025

description: Uzbekistan, a landlocked Central Asian country, has been navigating complex socio-political changes over the past few decades, especially since gaining independence from the Soviet Union in 1991. This paper aims to analyze Uzbekistan’s socio-political landscape in the context of ecological globalization, focusing on how environmental issues, global ecological shifts, and international climate policies have impacted the country's political and social dynamics. As Uzbekistan continues its economic reforms and seeks closer integration with global markets, the interplay between its internal development and the broader ecological crisis presents both challenges and opportunities. The analysis will examine policy shifts, environmental movements, and socio-political adjustments made by the government to address climate change, sustainability, and environmental health. In conclusion, this paper offers insights into the complexities of ecological globalization in Uzbekistan, proposing a framework for future socio-political adaptation.
The Weingarten Model a la Polyakov
Creators: name: Dalley, S.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The Weingarten lattice gauge model of Nambu-Goto strings is generalised to allow for fluctuations of an intrinsic worldsheet metric through a dynamical quadrilation. The continuum limit is taken for $c\leq1$ matter, reproducing the results of hermitian matrix models to all orders in the genus expansion. For the compact $c=1$ case the vortices are Wilson lines, whose exclusion leads to the theory of non-interacting fermions. As a by-product of the analysis one finds the critical behaviour of SOS and vertex models coupled to 2D quantum gravity.
description: 16 pages (5 illustrations not included)
Higher-order nonequilibrium term: Effective power density quantifying evolution towards or away from local thermodynamic equilibrium
Creators: name: Barbhuiya, M. Hasan
name: Cassak, Paul A.
name: Adhikari, Subash
name: Parashar, Tulasi N.
name: Liang, Haoming
name: Argall, Matthew R.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: A common approach to assess the nature of energy conversion in a classical fluid or plasma is to compare power densities of the various possible energy conversion mechanisms. A forefront research area is quantifying energy conversion for systems that are not in local thermodynamic equilibrium (LTE), as is common in a number of fluid and plasma systems. Here, we introduce the ``higher-order non-equilibrium term'' (HORNET) effective power density that quantifies the rate of change of departure of a phase space density from LTE. It has dimensions of power density, which allows for quantitative comparisons with standard power densities. We employ particle-in-cell simulations to calculate HORNET during two processes, namely magnetic reconnection and decaying kinetic turbulence in collisionless magnetized plasmas, that inherently produce non-LTE effects. We investigate the spatial variation of HORNET and the time evolution of its spatial average. By comparing HORNET with power densities describing changes to the internal energy (pressure dilatation, $\rm{Pi-D}$, and divergence of the vector heat flux density), we find that HORNET can be a significant fraction of these other measures (8\% and 35\% for electrons and ions, respectively, for reconnection; up to 67\% for both electrons and ions for turbulence), meaning evolution of the system towards or away from LTE can be dynamically important. Applications to numerous plasma phenomena are discussed.
description: 19 pages (including references), 7 figures
EXPERIMENTAL RESULTS OF GRAIN GRINDING DEVICE
Creators: name: Karshiev, Fakhridin
Publisher: name: Zenodo
Year: 2024

description: The article provides information on the scientific and technical solutions of providing grain feed grinding technologies and technical means in animal husbandry and the results obtained in the preparation of grain feed in animal husbandry. It is known that feeding livestock by grinding grains and mixing them with soft fodder is one of the main factors of increasing their productivity. Today, one of the urgent tasks is the development of a device for grinding and mixing feed intended for individual use by farmers, personal assistants and farmers.
RETURN To an Order of the House for a return of the names of all persons who applied to purchase lands at Port Simpson in 1879 or 1883; the dates and particulars of the respective applications; the dates of instructions for surveys; to whom issued; the dates of surveys; copies of publication (if any) of same; the dates of acceptance of surveys; and the dates of the issue of Crown grants, and to who issued; together with copies of all correspondence in relation to the matter.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
RETURN To an Address of the Legislative Assembly for copies of the following papers referring to an "Act to prevent the immigration of Chinese," 47 Vic., chap. 3, 1884, and an "Act to prevent the immigration of Chinese," 48 Vic., chap. 13, 1885 :--Copies of the Attorney-General's report to His Honour the Lieutenant-Governor ; copies of all Orders in Council, letters or telegrams received or sent by any member of the Government ; the amount of revenue received under either of the above Acts.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
Vortex rings in fragmentation regions in heavy-ion collisions at $\sqrt{s_{NN}}=$ 39 GeV
Creators: name: Ivanov, Yu. B.
name: Soldatov, A. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Vorticity generated in heavy-ion collisions at energy of $\sqrt{s_{NN}}=$ 39 GeV is studied. Simulations are performed within a model of the three-fluid dynamics. A peculiar structure consisting of two vortex rings is found: one ring in the target fragmentation region and another one in the projectile fragmentation region. These rings are also formed in central collisions. The matter rotation is opposite in this two rings. These vortex rings are already formed at the early stage of the collision together with primordial fragmentation regions. The average vorticity, responsible for the global polarization of the observed $Λ$ and $\barΛ$, is also studied. In the semi-central collisions the average vorticity in the midrapidity region turns out to be more than an order of magnitude lower than the total one. The total vorticity is dominated by the contributions of the fragmentation regions and is produced because of asymmetry of the vortex rings in noncentral collisions. This suggests that in semi-central collisions the global polarization in the fragmentation regions should be at least an order of magnitude higher than that observed by the STAR collaboration in the midrapidity. This polarization should be asymmetrical in the reaction plain and correlate with the corresponding directed flow.
description: 10 pages, 7 figures, version published in Phys. Rev. C