cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0157
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
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0157, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0157, 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
Clear and Cloudy Exoplanet Forecasts for JWST: Maps, Retrieved Composition and Constraints on Formation with MIRI and NIRCam
Creators: name: Schlawin, Everett
name: Greene, Thomas P.
name: Line, Michael
name: Fortney, Jonathan J.
name: Rieke, Marcia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The James Webb Space Telescope (JWST) will measure exoplanet transmission and eclipse spectroscopy at un-precedented precisions to better understand planet structure, dynamics, chemistry and formation. These are essential tools on the march towards biosignature searches on potentially habitable planets. We explore a range of exoplanet atmospheric conditions and forecast the expected results with JWST. We take realistic CHIMERA models that match existing Spitzer and HST results and simulate the spectra achievable with the JWST MIRI + NIRCam Guaranteed Time Observations (GTO) survey. We then retrieve atmospheric parameters from these spectra to estimate the precision to which the planets' atmospheric compositions can be measured. We find that emission spectra have well-constrained unimodal solutions but transmission spectra near 10X solar abundance and solar C/O ratios can suffer from bimodal solutions. Broad wavelength coverage as well as higher precision data can resolve bimodal solutions and provide dramatically better atmospheric parameter constraints. We find that metallicities can be measured to within 20% to 170%, which approaches the precisions on Solar System planets, and C/O ratios can be constrained to ~10% to 60%, assuming that observers can leverage short wavelength data to select the correct solution from the bimodal posteriors. These compositional precisions are sufficient to validate or refute predictions from disk formation models on final atmospheric abundances as long as their history is not erased by planet evolution processes. We also show the extent to which eclipse mapping with JWST is possible on our brightest system HD 189733 b.
description: Accepted to The Astronomical Journal, 17 pages
Spectroscopic Constraints on UV Metal Line Emission at z~6-9: The Nature of Lyman-alpha Emitting Galaxies in the Reionization-Era
Creators: name: Mainali, Ramesh
name: Zitrin, Adi
name: Stark, Daniel P.
name: Ellis, Richard S.
name: Richard, Johan
name: Tang, Mengtao
name: Laporte, Nicolas
name: Oesch, Pascal
name: McGreer, Ian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Recent studies have revealed intense UV metal emission lines in a modest sample of z>7 Lyman-alpha emitters, indicating a hard ionizing spectrum is present. If such high ionization features are shown to be common, it may indicate that extreme radiation fields play a role in regulating the visibility of Lyman-alpha in the reionization era. Here we present deep near-infrared spectra of seven galaxies with Lyman-alpha emission at 5.47 photometric targets. In nine sources we do not detect UV metal lines. However in the z=8.683 galaxy EGSY8p7, we detect a 4.6 sigma emission line in the narrow spectral window expected for NV 1243. The feature is unresolved (FWHM<90 km/s) and is likely nebular in origin. A deep H-band spectrum of EGSY8p7 reveals non-detections of CIV, He II, and OIII]. The presence of NV requires a substantial flux of photons above 77 eV, pointing to a hard ionizing spectrum powered by an AGN or fast radiative shocks. Regardless of its origin, the intense radiation field of EGSY8p7 may aid the transmission of Lyman-alpha through what is likely a partially neutral IGM. With this new detection, five of thirteen known Lyman-alpha emitters at z>7 have now been shown to have intense UV line emission, suggesting that extreme radiation fields are commonplace among the Lyman-alpha population. Future observations with JWST will eventually clarify the origin of these features and explain their role in the visibility of Lyman-alpha in the reionization era.
description: 15 pages, 3 tables and 7 figures. Accepted for publication in MNRAS
Additional file 1 of The prostate-specific membrane antigen holds potential as a vascular target for endogenous radiotherapy with [177Lu]Lu-PSMA-I&T for triple-negative breast cancer
Creators: name: Heesch, Amelie
name: Florea, Alexandru
name: Maurer, Jochen
name: Habib, Pardes
name: Werth, Laura S.
name: Hansen, Thomas
name: Stickeler, Elmar
name: Sahnoun, Sabri E. M.
name: Mottaghy, Felix M.
name: Morgenroth, Agnieszka
Publisher: name: figshare
Year: 2024
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1. Supplementary information. Supplementary figures S1–S11.
Generic emergence of objectivity of observables in infinite dimensions
Creators: name: Knott, Paul A.
name: Tufarelli, Tommaso
name: Piani, Marco
name: Adesso, Gerardo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: Quantum Darwinism posits that information becomes objective whenever multiple observers indirectly probe a quantum system by each measuring a fraction of the environment. It was recently shown that objectivity of observables emerges generically from the mathematical structure of quantum mechanics, whenever the system of interest has finite dimensions and the number of environment fragments is large [F. G. S. L. Brandão, M. Piani, and P. Horodecki, Nature Commun. 6, 7908 (2015)]. Despite the importance of this result, it necessarily excludes many practical systems of interest that are infinite-dimensional, including harmonic oscillators. Extending the study of Quantum Darwinism to infinite dimensions is a nontrivial task: we tackle it here by using a modified diamond norm, suitable to quantify the distinguishability of channels in infinite dimensions. We prove two theorems that bound the emergence of objectivity, first for finite energy systems, and then for systems that can only be prepared in states with an exponential energy cut-off. We show that the latter class of states includes any bounded-energy subset of single-mode Gaussian states.
description: 15 pages, 3 figures
Концепция создания производства добавок для обогащения витаминами хлебобулочных изделий школ и больниц
Creators: name: Кудряшов В. Л.
Publisher: name: Пищевая индустрия
Year: 2019
Subjects: ВИТАМИНЫ
ОБОГАЩЕНИЕ ХЛЕБА
РАСТИТЕЛЬНОЕ СЫРЬЕ
ВТОРИЧНОЕ СЫРЬЕ
ПИЩЕВЫЕ ДОБАВКИ
БАРОМЕМБРАННЫЕ ПРОЦЕССЫ

description: Обоснована целесообразность обогащения витаминами и микроэлементами хлеба для школ и больниц. Приведены состав и количество ингредиентов для обогащения хлеба, перечень рекомендуемого растительного и вторичного сырья и концепция создания производств натуральных пищевых добавок.
Official Report to the Amerind Foundation, Covering a Preliminary Study of the Casas Grandes and the Valley of the Caves in the Sierra Madres, Chihuahua, Mexico, May 13-18, 1957
Creators: name: Chambers, George W.
Publisher: name: The Amerind Foundation, Inc.
Year: 1957
Subjects: subject: Chihuahua (Mexico : State)
valueUri: https://core.tdar.org/browse/geographic-keyword/49578/chihuahua-mexico-state
subject: Sierra Madres
valueUri: https://core.tdar.org/browse/geographic-keyword/85353/sierra-madres
subject: Casas Grandes
valueUri: https://core.tdar.org/browse/site-name/279/casas-grandes
subject: Town / City
valueUri: https://core.tdar.org/browse/site-type/255/town-city
subject: Domestic Structure or Architectural Complex
valueUri: https://core.tdar.org/browse/site-type/251/domestic-structure-or-architectural-complex
subject: Settlements
valueUri: https://core.tdar.org/browse/site-type/252/settlements
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey
subject: Heritage Management
valueUri: https://core.tdar.org/browse/investigation-type/24/heritage-management

description: Official report made by George W. Chambers to the Amerind Foundation covering trips made to the Casas Grandes and the Valley of the Caves in the Sierra Madres, Chihuahua, Mexico. This trip was made after an invitation of Dr. Charles C. Di Peso, Director of the Amerind Foundation, who made the expedition for the primary purpose of continuing arrangements preparatory to the proposed excavation and restoration of Casas Grandes in cooperation with the Mexican Government. The secondary purpose was to visit the Valley of the Caves described by Carl Lumholtz in 1890. The third purpose was to investigate highway routes and conditions between the Casas Grandes site and the Amerind headquarters at Dragoon, Arizona, check living conditions for his family, airport facilities, communications and labor pool.
Мясные продукты, обогащенные эссенциальными микроэлементами
Creators: name: Касьянов Г. И.
name: Мишкевич Э. Ю.
name: Магомедов А. М.
Publisher: name: Пищевая индустрия
Year: 2019

description: Актуальность выполняемых авторами исследований обусловлена рядом отличительных факторов: недостаточностью научно-практической информации о роли эссенциальных микроэлементов при производстве мясорастительных продуктов; наличием пробелов в рекомендациях по обогащению продуктов неорганическими формами микроэлементов, которые могут пагубно влиять на здоровье человека; увеличением числа заболеваний, связанных с дефицитом микроэлементов в организме человека и животных; потребностью в осмыслении существующей на сегодняшний день ситуации со снижением дефицита незаменимых микронутриентов в питании человека, животных, птиц и рыб.
mother / me
Creators: name: Swartzel, Joseph
Publisher: name: Carnegie Mellon University
Year: 2018
Subjects: Art

description: mother / me is a visual exploration and analysis of the biological and constructed maternal realms of artist Gray Swartzel’s life. Orienting and navigating childhood influences, Swartzel explains his desire to use Craigslist to seek out surrogates, or mother figures. Interrogating his queer body within the psychological space between himself and his biological and surrogate mothers, he challenges and interrogates conceptions of the nuclear family, critiquing heteronormative assumptions of family. Swartzel tasks himself as an agent to inspect family as a social construct within a larger Lacanian orientation, while seeking out the objet petit a, or cause of desire in such relationships. He details the influences of early twentieth century glamour photography and maternal theory and outlines how they manifest in performances of the self. mother / me is an experiment to investigate the queer relationship between camp and the twenty-first century dandy through the collaboration of a mother and a child to construct visual images.
HI 2334+26: An Extended HI Cloud near Abell 2634
Creators: name: Giovanelli, Riccardo
name: Scodeggio, Marco
name: Solanes, Jose` M.
name: Haynes, Martha P.
name: Arce, Hector
name: Sakai, Shoko
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the serendipitous discovery of a large HI cloud with an associated HI mass of $6(\pm1.5)\times 10^9 h^{-2}$ M$_\odot$ and a heliocentric velocity 8800 \kms, located near the periphery of the cluster of galaxies Abell 2634. Its velocity field appears to be very quiescent, as no gradients in the peak velocity are seen over its extent of 143$ h^{-1}$ by 103$ h^{-1}$ kpc. The distribution of gas is poorly resolved spatially, and it is thus difficult at this time to ascertain the nature of the cloud. At least two relatively small, actively star--forming galaxies appear to be embedded in the HI gas, which may (a) be an extended gaseous envelope surrounding one or both galaxies, (b) have been spread over a large region by a severe episode of tidal disruption or (c) have been affected by the ram pressure resulting from its motion through the intracluster gas of A2634.
description: 12 pages plus 2 tables (AAS LaTeX macro v3.0), 4 figures not included. To appear in the AJ
Rotating Charged Black Hole Solution in Heterotic String Theory
Creators: name: Sen, Ashoke
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct a solution of the classical equations of motion arising in the low energy effective field theory for heterotic string theory. This solution describes a black hole in four dimensions carrying mass $M$, charge $Q$ and angular momentum $J$. The extremal limit of the solution is discussed.
description: 9 pages
A Simple Worldsheet Black Hole
Creators: name: Dubovsky, Sergei
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study worldsheet theory of confining strings in two-dimensional massive adjoint QCD. Similarly to confining strings in higher dimensions this theory exhibits a non-trivial $S$-matrix surviving even in the strict planar limit. In the process of two-particle scattering a zigzag is formed on the worldsheet. It leads to an interesting non-locality and exhibits some properties of a quantum black hole. Ordinarily, identical quantum particles do not carry identity. On the worldsheet they acquire off-shell identity due to strings attached. Identity implies complementarity. We discuss similarities and differences of the worldsheet scattering with the $T\bar{T}$ deformation. We also propose a promising candidate for a supersymmetric model with integrable confining strings.
description: 30 pages, 8 figures; v2: refs updated, typos corrected, several comments added
Electron energy loss spectroscopy determination of Ti oxidation state at the (001) LaAlO3/SrTiO3 interface as a function of LaAlO3 growth conditions
Creators: name: Maurice, Jean-Luc
name: Herranz, Gervasi
name: Colliex, Christian
name: Devos, Isabelle
name: Carrétéro, Cécile
name: Barthelemy, Agnès
name: Bouzehouane, Karim
name: Fusil, Stéphane
name: Imhoff, Dominique
name: Jacquet, Éric
name: Jomard, François
name: Ballutaud, Dominique
name: Basletic, Mario
Publisher: name: arXiv
Year: 2007
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: At the (001) interface between the two band-insulators LaAlO3 and SrTiO3, a high-mobility electron gas may appear, which has been the object of numerous works over the last four years. Its origin is a subject of debate between the interface polarity and unintended doping. Here we use electron energy loss 'spectrum images', recorded in cross-section in a scanning transmission electron microscope, to analyse the Ti3+ ratio, characteristic of extra electrons. We find an interface concentration of Ti3+ that depends on growth conditions.
description: 6 pages
An Overabundance of Black Hole X-Ray Binaries in the Galactic Center from Tidal Captures
Creators: name: Generozov, A.
name: Stone, N. C.
name: Metzger, B. D.
name: Ostriker, J. P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: A large population of X-ray binaries (XRBs) was recently discovered within the central parsec of the Galaxy by Hailey et al. While the presence of compact objects on this scale due to radial mass segregation is, in itself, unsurprising, the fraction of binaries would naively be expected to be small because of how easily primordial binaries are dissociated in the dynamically hot environment of the nuclear star cluster (NSC). We propose that the formation of XRBs in the central parsec is dominated by the tidal capture of stars by black holes (BHs) and neutron stars (NSs). We model the time-dependent radial density profiles of stars and compact objects in the NSC with a Fokker-Planck approach, using the present-day stellar population and rate of in situ massive star (and thus compact object) formation as observational constraints. Of the ~10,000-40,000 BHs that accumulate in the central parsec over the age of the Galaxy, we predict that ~60 - 200 currently exist as BH-XRBs formed from tidal capture, consistent with the population seen by Hailey et al. A somewhat lower number of tidal capture NS-XRBs is also predicted. We also use our observationally calibrated models for the NSC to predict rates of other exotic dynamical processes, such as the tidal disruption of stars by the central supermassive black hole (~0.0001 per year at z=0).
description: 18 pages, 15 figures, 4 tables + Appendices. Accepted to MNRAS
Museum Visitor Engagement Through Resonant, Rich and Interactive Experiences
Creators: name: Templeton, Cheryl A.
Publisher: name: Carnegie Mellon University
Year: 2011
Subjects: Design

description: Museums are vast resources, but much of their information is inaccessible to visitors. Typical labels for artifacts provide few details, making it difficult for non-expert visitors to learn about an artifact, and to find its relevance to other artifacts or to themselves. Although museums have developed interpretive aids such as brochures and audio guides, these are limited and do not offer visitors the possibility to explore artifacts both broadly and deeply as they go through an exhibition. Visitors often have questions that go unanswered or pass through an exhibition without being engaged. As visitors all have their own personal interests and preferences, it would be difficult to offer a usable version of any current interpretive aid that includes all of the information, stories, and related content that each visitor would like. Personal mobile devices provide a platform for interactivity and access to an unlimited amount of information, presentation of rich media, and flexibility for customized experiences both inside the museum and beyond. To bridge the gap between museum collection information and visitor engagement, I propose a framework for increasing engagement through resonant, rich, and interactive experiences mediated by a personal mobile guide, and present a case study and functional prototype mobile guide for the Hall of Architecture at the Carnegie Museum of Art.
The Mouse Pulsar Wind Nebula
Creators: name: Klingler, Noel
name: Kargaltsev, Oleg
name: Pavlov, George G.
name: Ng, C. -Y.
name: Beniamini, Paz
name: Volkov, Igor
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The young energetic pulsar J1747-2958 ($τ=26$ kyr, $\dot{E}=2.5\times 10^{36}$ erg s$^{-1}$) powers the Mouse pulsar wind nebula (PWN), famous for its spectacular tail spanning 45$"$ in X-rays and 12$'$ in radio ($d\sim5$ kpc). We present the results of Chandra observations of the PWN and the analysis of archival lower-frequency data. The Chandra HRC image reveals a point-like source at the pulsar position, $\approx$1$'$ behind the bow shock apex of the PWN. The flattened appearance of the compact nebula is consistent with an equatorial outflow deformed by the ram pressure, implying that the angle between the pulsar's spin axis and line of sight is $\sim70^\circ$ (in agreement with the radio and $γ$-ray pulse profiles). The spatially-resolved spectroscopy with Chandra ACIS shows that the power-law (PL) spectrum steepens from $Γ=1.65\pm0.02$ to $3.0\pm0.1$ over the 45$'$ extent of the X-ray tail. However, the tail's X-ray spectrum integrated over its 45$"$ length fits a single absorbed PL with $Γ=2.09\pm0.03$. We also found the Mouse PWN in 150 MHz GMRT data, and a possible counterpart in 24 ${\rm μ}$m Spitzer data. The multiwavelength data suggest that, at low frequencies, the spectrum of the X-ray-emitting tail region can be described by a broken PL with at least one turnover between radio and X-rays. This is consistent with synchrotron cooling of electrons injected at the termination shock (with an SED slope of 2.2) in an equipartition magnetic field $B\sim200$ ${\rm μG}$ and a bulk flow speed $v\sim4000$ km s$^{-1}$.
description: 16 pages, 11 figures, accepted for publication in ApJ
The Effects of Laser and Electron Beam Spot Size in Additive Manufacturing Processes
Creators: name: Francis, Zachary Ryan
Publisher: name: Carnegie Mellon University
Year: 2017
Subjects: subject: Mechanical Engineering
subject: FOS: Mechanical engineering

description: In this work, melt pool size in process mapped in power-velocity space for multiple processes and alloys. In the electron beam wire feed and laser powder feed processes, melt pool dimensions are then related to microstructure in the Ti-6Al-4V alloy. In the electron beam wire feed process, work by previous authors that related prior beta grain size to melt pool area is extended and a control scheme is suggested. In the laser powder feed process, in situ thermal imaging is used to monitor melt pool length. Real time melt pool length measurements are used in feedback control to manipulate the resulting microstructure. In laser and electron beam direct metal additive manufacturing, characteristics of the individual melt pool and the resulting final parts are a product of a variety of process parameters. Laser or electron beam spot size is an important input parameter that can affect the size and shape of a melt pool, and has a direct influence on the formation of lack-of-fusion and keyholing porosity. In this work, models are developed to gain a better understanding of the effects of spot size across different alloys and processes. Models are validated through experiments that also span multiple processes and alloys. Methods to expand the usable processing space are demonstrated in the ProX 200 laser powder bed fusion process. In depth knowledge of process parameters can reduce the occurrence of porosity and flaws throughout processing space and allow for the increased use of non-standard parameter sets. Knowledge of the effects of spot size and other process parameters can enable an operator to expand the usable processing space while avoiding the formation of some types of flaws. Based on simulation and experimental results, regions where potential problems may occur are identified and process parameter based solutions are suggested. Methods to expand the usable processing space are demonstrated in the ProX 200 laser powder bed fusion process. In depth knowledge of process parameters can reduce the occurrence of porosity and flaws throughout processing space and allow for the increased use of non-standard parameter sets.
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00118
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes
subject: LaMOP

description: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172), f. 00118, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
The Stellar-to-Halo mass relation over thee last 12 Gyr
Creators: name: Girelli, Giacomo
Publisher: name: Zenodo
Year: 2019

description: Understanding how galaxy properties are linked to the dark matter halos they reside in, and how they co-evolve is a powerful tool to constrain the processes related to galaxy formation. The stellar-to-halo mass relation (SHMR) and its evolution over the history of the Universe provides insights on galaxy formation models and allows to assign galaxy masses to halos in N-body dark matter simulations. We use a statistical approach to link the observed galaxy stellar mass functions on the COSMOS field to dark matter halo mass functions from the DUSTGRAIN simulation and from a theoretical parametrization from z=0 to z=4. We also propose an empirical model to describe the evolution of the stellar-to-halo mass relation as a function of redshift. We calculate the star-formation efficiency (SFE) of galaxies and compare results with previous works and semi-analytical models. In addition, we test the robustness of the model from z=0 up to z>4 by applying it to N-body dark matter simulations and comparing with observations.
Quench Dynamics Across Topological Quantum Phase Transitions
Creators: name: Liou, Shiuan-Fan
name: Yang, Kun
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study the dynamics of systems quenched through topological quantum phase transitions and investigate the behavior of the bulk and edge excitations with various quench rates. Specifically, we consider the Haldane model and checkerboard model in slow quench processes with distinct band-touching structures leading to topology changes. The generation of bulk excitations is found to obey the power-law relation Kibble-Zurek and Landau-Zener theories predict. However, an anti-Kibble-Zurek behavior is observed in the edge excitations. The mechanism of excitation generation on edge states is revealed, which explains the anti-Kibble-Zurek behavior.
description: 7 pages, 7 figures
Quantum Group and Magnetic Translations. Bethe-Ansatz Solution for Bloch Electrons in a Magnetic Field
Creators: name: Wiegmann, P. B
name: Zabrodin, A. V.
Publisher: name: arXiv
Year: 1993
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We present a new approach to the problem of Bloch electrons in magnetic field,\\ by making explicit a natural relation between magnetic translations and the\\quantum group $U_{q}(sl_2)$. The approach allows to express the spectrum and\\\ the Bloch function as solutions of the Bethe-Ansatz equations typical for com\\pletely integrable quantum systems
description: 9 pages, Revtex
Hubbard model physics in transition metal dichalcogenide moiré bands
Creators: name: Wu, Fengcheng
name: Lovorn, Timothy
name: Tutuc, Emanuel
name: MacDonald, A. H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Flexible long period moir\' e superlattices form in two-dimensional van der Waals crystals containing layers that differ slightly in lattice constant or orientation. In this Letter we show theoretically that isolated flat moir\' e bands described by generalized triangular lattice Hubbard models are present in twisted transition metal dichalcogenide heterobilayers. The hopping and interaction strength parameters of the Hubbard model can be tuned by varying the twist angle and the three-dimensional dielectric environment. When the flat moiré bands are partially filled, candidate many-body ground states at some special filling factors include spin-liquid states, quantum anomalous Hall insulators and chiral $d$-wave superconductors.
description: 5+2 pages, 4+1 figures
Beyond the Standard Model at the LHC and Beyond
Creators: name: Ellis, John
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Many of the open questions beyond the Standard Model will be addressed by the LHC, including the origin of mass, supersymmetry, dark matter and the possibility of large extra dimensions. A linear e+ e- collider (LC) with sufficient centre-of-mass energy would add considerable value to the capabilities of the LHC.
description: 12 pages, 8 figures, Contribution to the Proceedings of the 13th International Symposium on Particles, Strings and Cosmology, PASCOS-07
Attractor Behaviour in Multifield Inflation
Creators: name: Carrilho, Pedro
name: Mulryne, David
name: Ronayne, John
name: Tenkanen, Tommi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study multifield inflation in scenarios where the fields are coupled non-minimally to gravity via $ξ_I(ϕ^I)^n g^{μν}R_{μν}$, where $ξ_I$ are coupling constants, $ϕ^I$ the fields driving inflation, $g_{μν}$ the space-time metric, $R_{μν}$ the Ricci tensor, and $n>0$. We consider the so-called $α$-attractor models in two formulations of gravity: in the usual metric case where $R_{μν}=R_{μν}(g_{μν})$, and in the Palatini formulation where $R_{μν}$ is an independent variable. As the main result, we show that, regardless of the underlying theory of gravity, the field-space curvature in the Einstein frame has no influence on the inflationary dynamics at the limit of large $ξ_I$, and one effectively retains the single-field case. However, the gravity formulation does play an important role: in the metric case the result means that multifield models approach the single-field $α$-attractor limit, whereas in the Palatini case the attractor behaviour is lost also in the case of multifield inflation. We discuss what this means for distinguishing between different models of inflation.
description: 20 pages, 6 figures. Typos corrected and references added. This is an author-created, un-copyedited version of an article published in JCAP. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at https://iopscience.iop.org/article/10.1088/1475-7516/2018/06/032/pdf
RETURN To an Address to His Honour the Lieutenant-Governor, praying him to cause to be sent down to the House a Return showing the results of the revised census in each enumerator's division, with a statement showing in which of the new Electoral Districts, or Ridings of Districts, each enumerator's division was.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2014

Abstract
The Ice Cap Zone: A Unique Habitable Zone for Ocean Worlds
Creators: name: Ramirez, Ramses M.
name: Levi, Amit
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Traditional definitions of the habitable zone assume that habitable planets contain a carbonate-silicate cycle that regulates CO2 between the atmosphere, surface, and the interior. Such theories have been used to cast doubt on the habitability of ocean worlds. However, Levi et al (2017) have recently proposed a mechanism by which CO2 is mobilized between the atmosphere and the interior of an ocean world. At high enough CO2 pressures, sea ice can become enriched in CO2 clathrates and sink after a threshold density is achieved. The presence of subpolar sea ice is of great importance for habitability in ocean worlds. It may moderate the climate and is fundamental in current theories of life formation in diluted environments. Here, we model the Levi et al. mechanism and use latitudinally-dependent non-grey energy balance and single-column radiative-convective climate models and find that this mechanism may be sustained on ocean worlds that rotate at least 3 times faster than the Earth. We calculate the circumstellar region in which this cycle may operate for G-M-stars (Teff = 2,600 to 5,800 K), extending from about 1.23 to 1.65, 0.69 to 0.954, 0.38 to 0.528 AU, 0.219 to 0.308 AU, 0.146 to 0.206 AU, and 0.0428 to 0.0617 AU for G2, K2, M0, M3, M5, and M8 stars, respectively. However, unless planets are very young and not tidally locked, our mechanism would be unlikely to apply to stars cooler than a ~M3. We predict C/O ratios for our atmospheres (about 0.5) that can be verified by the JWST mission.
description: Published in the Monthly Notices of the Royal Astronomical Society (31 pages, 7 Figures, 1 Table) https://doi.org/10.1093/mnras/sty761
The Effects of Group Status on Intragroup Behavior: Implications for Group Process and Outcome
Creators: name: Chang, Jin Wook
Publisher: name: Carnegie Mellon University
Year: 2015
Subjects: subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: How does the status of a group influence the behavior of individuals within the group? This dissertation aims to answer this question by investigating the psychological and behavioral implications of membership in high- versus low-status groups, with a primary focus on the impact of membership in a high-status group. I propose that membership in high-status groups leads to self-oriented intragroup behavior, behavior that best suits members’ own interests regardless of the impact on group outcomes. In five studies, I test this idea and examine the psychological mechanism underlying this effect. The first three studies find that membership in a high-status group (a) decreases the resources allocated for the group as members attempt to ensure personal gain; (b) lowers the preference for a competent newcomer who may enhance group outcome but who may jeopardize personal gains; and (c) reduces the amount of voluntary information sharing during group negotiations, hindering group outcomes. The findings also reveal that reducing the conflict between group and personal interests via cooperative incentives encourages group-oriented behavior in high-status groups. The next two studies conceptually replicate these findings focusing on members’ information withholding – self-oriented behavior designed to prevent other in-group members from outperforming them. Specifically, results reveal that high-status group-membership increases intentional withholding of information, which in turn impairs group outcomes. However, this damaging pattern of intragroup behavior triggered by membership in a high-status group is alleviated when group members are led to believe that their group status is at stake. Taken together, this dissertation provides converging evidence that membership in high-status groups increases emphasis on personal interests within the group and that these concerns manifest in intragroup behavior that is distinct from that triggered by membership in low-status groups. The findings illuminate how the status of a group might shape the ways that members interact with other in-group members, as well as document the potential micro- and meso-level mechanisms through which status differences among social groups persist and change.
Strong Coupling Qed Breaks Chiral Symmetry
Creators: name: Semenoff, Gordon
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show that the strong coupling limit of d-dimensional quantum electrodynamics with $2^{d}/2^{[d/2]}$ flavors of fermions can be mapped onto the s=1/2 quantum Heisenberg antiferromagnet in d-1 space dimensions. The staggered Néel order parameter is the expectation value of a mass operator in QED and the spin-waves are pions. We speculate that the chiral symmetry breaking phase transition corresponds to a transition between the flux phase and the conventional Néel ordered phase of an antiferromagnetic t-J model.
description: 11pages
Hydrodynamic Simulations of Galaxy Formation
Creators: name: Thoul, A. A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have developed an accurate, one-dimensional, spherically symmetric, Lagrangian hydrodynamics/gravity code, designed to study the effects of radiative cooling and photo-ionization on the formation of protogalaxies. We examine the ability of collapsing perturbations to cool within the age of the universe. In contrast to some studies based on order-of-magnitude estimates, we find that cooling arguments alone cannot explain the sharp upper cutoff observed in the galaxy luminosity function. We also look at the effect of a photoionizing background on the formation of low-mass galaxies.
description: 4 pages, uuencoded compressed postscript with figures
Statistics of finite scale local Lyapunov exponents in fully developed homogeneous isotropic turbulence
Creators: name: de Divitiis, Nicola
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: The present work analyzes the statistics of finite scale local Lyapunov exponents of pairs of fluid particles trajectories in fully developed incompressible homogeneous isotropic turbulence. According to the hypothesis of fully developed chaos, this statistics is here analyzed assuming that the entropy associated to the fluid kinematic state is maximum. The distribution of the local Lyapunov exponents results to be an unsymmetrical uniform function in a proper interval of variation. From this PDF, we determine the relationship between average and maximum Lyapunov exponents, and the longitudinal velocity correlation function. This link, which in turn leads to the closure of von Kàrmàn-Howarth and Corrsin equations, agrees with results of previous works, supporting the proposed PDF calculation, at least for the purposes of the energy cascade main effect estimation. Furthermore, through the property that the Lyapunov vectors tend to align the direction of the maximum growth rate of trajectories distance, we obtain the link between maximum and average Lyapunov exponents in line with the previous results. To validate the proposed theoretical results, we present different numerical simulations whose results justify the hypotheses of the present analysis.
description: Research article. arXiv admin note: text overlap with arXiv:1706.00972
Characteristic molecular properties of one-electron double quantum rings under magnetic fields
Creators: name: Climente, JI
name: Planelles, J
Publisher: name: arXiv
Year: 2007
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The molecular states of conduction electrons in laterally coupled quantum rings are investigated theoretically. The states are shown to have a distinct magnetic field dependence, which gives rise to periodic fluctuations of the tunnel splitting and ring angular momentum in the vicinity of the ground state crossings. The origin of these effects can be traced back to the Aharonov-Bohm oscillations of the energy levels, along with the quantum mechanical tunneling between the rings. We propose a setup using double quantum rings which shows that Aharonov-Bohm effects can be observed even if the net magnetic flux trapped by the carriers is zero.
description: 16 pages (iopart format), 10 figures, accepted in J.Phys.Cond.Matt
Model reduction for Kuramoto models with complex topologies
Creators: name: Hancock, Edward J.
name: Gottwald, Georg A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: Synchronisation of coupled oscillators is a ubiquitous phenomenon, occurring in topics ranging from biology and physics, to social networks and technology. A fundamental and long-time goal in the study of synchronisation has been to find low-order descriptions of complex oscillator networks and their collective dynamics. However, for the Kuramoto model - the most widely used model of coupled oscillators - this goal has remained surprisingly challenging, in particular for finite-size networks. Here, we propose a model reduction framework that effectively captures synchronisation behaviour in complex network topologies. This framework generalises a collective coordinates approach for all-to-all networks [Gottwald (2015) Chaos 25, 053111] by incorporating the graph Laplacian matrix in the collective coordinates. We first derive low dimensional evolution equations for both clustered and non-clustered oscillator networks. We then demonstrate in numerical simulations for Erdos-Renyi (ER) networks that the collective coordinates capture the synchronisation behaviour in both finite-size networks as well as in the thermodynamic limit, even in the presence of interacting clusters.
Half-Integral Spin-Singlet Quantum Hall Effect
Creators: name: Belkhir, L.
name: Wu, X. G.
name: Jain, J. K.
Publisher: name: arXiv
Year: 1993
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We provide numerical evidence that the ground state of a short range interaction model at $ν=1/2$ is incompressible and spin-singlet for a wide range of repulsive interactions. Furthermore it is accurately described by a trial wave function studied earlier. For the Coulomb interaction we find that this wave function provides a good description of the lowest lying spin-singlet state, and propose that fractional quantum Hall effect would occur at $ν=1/2$ if this state became the global ground state.
description: Latex 13 pages, 3 figures upon request
Vapor-liquid equilibrium and equation of state of two-dimensional fluids from a discrete perturbation theory
Creators: name: Trejos, V. M.
name: Santos, A.
name: Gámez, F.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The interest in the description of the properties of fluids of restricted dimensionality is growing for theoretical and practical reasons. In this work, we have firstly developed an analytical expression for the Helmholtz free energy of the two-dimensional square-well fluid in the Barker--Henderson framework. This equation of state is based on an approximate analytical radial distribution function for $d$-dimensional hard-sphere fluids ($1\leq d\leq 3$) and is validated against existing and new simulation results. The so-obtained equation of state is implemented in a discrete perturbation theory able to account for general potential shapes. The prototypical Lennard-Jones and Yukawa fluids are tested in its two-dimensional version against available and new simulation data with semi-quantitative agreement.
description: 9 pages, 6 figures; v2: new references added
Intersections forms and the geometry of lattice Chern-Simons theory
Creators: name: Eliezer, David
name: Semenoff, Gordon
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show that it is possible to formulate Abelian Chern-Simons theory on a lattice as a topological field theory. We discuss the relationship between gauge invariance of the Chern-Simons lattice action and the topological interpretation of the canonical structure. We show that these theories are exactly solvable and have the same degrees of freedom as the analogous continuum theories.
description: 14 pages
Ultra-Low Frequency Gravitational Radiation from Massive Black Hole Binaries
Creators: name: Rajagopal, Mohan
name: Romani, Roger W.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: For massive black hole binaries produced in galactic mergers, we examine the possibility of inspiral induced by interaction with field stars. We model the evolution of such binaries for a range of galaxy core and binary parameters, using numerical results from the literature to compute the binary's energy and angular momentum loss rates due to stellar encounters and including the effect of back-action on the field stars. We find that only a small fraction of binary systems can merge within a Hubble time via unassisted stellar dynamics. External perturbations may, however, cause efficient inspiral. Averaging over a population of central black holes and galaxy mergers, we compute the expected background of gravitational radiation with periods Pw ~ 1-10 yr. Comparison with sensitivities from millisecond pulsar timing suggests that the strongest sources may be detectable with modest improvements to present experiments.
description: To appear in Ap.J., June 1995; corrections to merger frequency formulae, updated figures; latex, 15 pages with 5 eps figures. POSTSCRIPT VERSION at http://geminga.stanford.edu/users/mohan/bhgw_pp.ps
Many-body methods for nuclear systems at subnuclear densities
Creators: name: Sedrakian, Armen
name: Clark, John W.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: This article provides a concise review of selected topics in the many-body physics of low density nuclear systems. The discussion includes the condensation of alpha particles in supernova envelopes, formation of three-body bound states and the BEC-BCS crossover in dilute nuclear matter, and neutrino production in $S$-wave paired superfluid neutron matter.
description: 10 pages, 3 figures. Talk given by AS at "Recent Progress in Many-Body Theories 14", Barcelona, 2007. To be published by World Sci., eds. G.E. Astrakharchik, J. Boronat, and F. Mazzanti