cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
[CAD] TJOE_Teia_2021_Circular_Group_Calculator_FINAL_Model.FCStd [TJOE / Luis Teia 2021]
Creators: name: Teia, Luis
Publisher: name: figshare
Year: 2021
Subjects: classificationCode: 401799
subject: Mechanical engineering not elsewhere classified
classificationCode: 401402
subject: CAD/CAM systems
classificationCode: 400903
subject: Digital processor architectures
classificationCode: 469999
subject: Other information and computing sciences not elsewhere classified

description: The following file is the final 3D model (in FreeCAD Version 0.18) of a novel calculator design published in The Journal of Open Engineering / Luis Teia 2021 -->> https://www.tjoe.org/pub/ur4nm2o5/release/3
Try the calculator for free by downloading it at Google Apps here :Pink Theme - https://play.google.com/store/apps/details?id=com.tool.KreisCalculatorNextGenPinkTheme
Day Theme - https://play.google.com/store/apps/details?id=com.tool.KreisCalculatorNextGenDayThemeNight Theme - https://play.google.com/store/apps/details?id=com.tool.KreisCalculatorNextGenNightTheme
FreeCAD software available for free download here : https://www.freecadweb.org/
A promotional video providing an insight into this new calculator technology is available here -->> https://figshare.com/articles/media/_VIDEO_New_Circular_Group_Calculator_-_Promotion_TJOE_Luis_Teia_2021_/14766411
Enjoy!
------------------------------------------------------------------------------------------ABSTRACT
Next generation calculators need to be efficient in all its design aspects. Current advanced computation calculators lack an efficient human-machine interface, with its unchanged traditional design traced back to the early 1960’s electro-mechanical commercialized solutions. The present article highlights how the perceived safety of “designing by tradition” can actually prevent evolution, and proposes - in a logical and argumentative way - a new layout based on the circular group approach, which derives from various already successful and working systems operating in society. Numerical comparison of the time spent in computing between the classical matrix calculator layout and the new circular group approach have shown that substantial time-saving can be achieved, in addition to the calculation acceleration effect imparted by aligning the highly organized calculator design with the intuitive nature of the mind of the user. Ultimately, the importance of such an advancement is appreciated when considering the compounding time-saving effect on the millions of users that will spend hours operating calculators in the years to come.
Isolate record for VAFB-ISO-242
Creators: name: McClure, Maggie
Year: 1986
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-242. The artifacts are two small gray-and-tan banded Monterey chert interior flakes, approximately 2 cm in length and 1 cm in width; no cortex on either.
Double or nothing: a Kolmogorov extension theorem for multitime (bi)probabilities in quantum mechanics
Creators: name: Lonigro, Davide
name: Sakuldee, Fattah
name: Cywiński, Łukasz
name: Chruściński, Dariusz
name: Szańkowski, Piotr
Publisher: name: arXiv
Year: 2024
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The multitime probability distributions obtained by repeatedly probing a quantum system via the measurement of an observable generally violate Kolmogorov's consistency property. Therefore, one cannot interpret such distributions as the result of the sampling of a single trajectory. We show that, nonetheless, they do result from the sampling of one pair of trajectories. In this sense, rather than give up on trajectories, quantum mechanics requires to double down on them. To this purpose, we prove a generalization of the Kolmogorov extension theorem that applies to families of complex-valued bi-probability distributions (that is, defined on pairs of elements of the original sample spaces), and we employ this result in the quantum mechanical scenario. We also discuss the relation of our results with the quantum comb formalism.
description: Accepted in Quantum
Isolate record for VAFB-ISO-231
Creators: name: Holloway, Corinne
Year: 1996
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-231. The artifact is a large Monterey chert biface thinning flake.
Isolate record for VAFB-ISO-215
Creators: name: Holloway, Corinne
Year: 1991
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-215. The artifact is a gray and white mottled Monterey chert flake with a pronounced bulb, small platform, and possible edge damage/use wear.
The RL/LLM Taxonomy Tree: Reviewing Synergies Between Reinforcement Learning and Large Language Models
Creators: name: Pternea, Moschoula
name: Singh, Prerna
name: Chakraborty, Abir
name: Oruganti, Yagna
name: Milletari, Mirco
name: Bapat, Sayli
name: Jiang, Kebei
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computation and Language (cs.CL)
subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: In this work, we review research studies that combine Reinforcement Learning (RL) and Large Language Models (LLMs), two areas that owe their momentum to the development of deep neural networks. We propose a novel taxonomy of three main classes based on the way that the two model types interact with each other. The first class, RL4LLM, includes studies where RL is leveraged to improve the performance of LLMs on tasks related to Natural Language Processing. L4LLM is divided into two sub-categories depending on whether RL is used to directly fine-tune an existing LLM or to improve the prompt of the LLM. In the second class, LLM4RL, an LLM assists the training of an RL model that performs a task that is not inherently related to natural language. We further break down LLM4RL based on the component of the RL training framework that the LLM assists or replaces, namely reward shaping, goal generation, and policy function. Finally, in the third class, RL+LLM, an LLM and an RL agent are embedded in a common planning framework without either of them contributing to training or fine-tuning of the other. We further branch this class to distinguish between studies with and without natural language feedback. We use this taxonomy to explore the motivations behind the synergy of LLMs and RL and explain the reasons for its success, while pinpointing potential shortcomings and areas where further research is needed, as well as alternative methodologies that serve the same goal.
description: 30 pages (including bibliography), 1 figure, 7 tables
Isolate record for VAFB-ISO-217
Creators: name: Holloway, Corinne
Year: 1993
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-217. The artifact is a unifacially worked Monterey chert flake, broken in two pieces, probably form recent grading or traffic along the road.
Isolate record for VAFB-ISO-212
Creators: name: Holloway, Corinne
Year: 1991
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-212. The artifact is a brown and white finely banded Monterey chert flake with cortex on platform.
The Populations of Carina. I. Decoding the Color--Magnitude Diagram
Creators: name: Norris, John E.
name: Yong, David
name: Venn, Kim A.
name: Dotter, Aaron
name: Casagrande, Luca
name: Gilmore, Gerard
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigate the color-magnitude diagram (CMD) of the Carina dwarf spheroidal galaxy using data of Stetson et al. (2011) and synthetic CMDs based on isochrones of Dotter et al. (2008), in terms of the parameters [Fe/H], age, and [alpha/Fe], for the cases when (i) [alpha/Fe] is held constant and (ii) [alpha/Fe] is varied. The data are well described by four basic epochs of star formation, having [Fe/H] = -1.85, -1.5, -1.2, and ~-1.15 and ages ~13, 7, ~3.5, and ~1.5 Gyr, respectively (for [alpha/Fe] = 0.1 (constant [alpha/Fe]) and [alpha/Fe] = 0.2, 0.1, -0.2, -0.2 (variable [alpha/Fe])), with small spreads in [Fe/H] and age of order 0.1 dex and 1 - 3 Gyr. Within an elliptical radius 13.1 arcmin, the mass fractions of the populations, at their times of formation, were (in decreasing age order) 0.34, 0.39, 0.23, and 0.04. This formalism reproduces five observed CMD features (two distinct subgiant branches of old and intermediate-age populations, two younger, main-sequence components, and the small color dispersion on the red giant branch (RGB)). The parameters of the youngest population are less certain than those of the others, and given it is less centrally concentrated it may not be directly related to them. High-resolution spectroscopically analyzed RGB samples appear statistically incomplete compared with those selected using radial velocity, which contain bluer stars comprising ~5 - 10% of the samples. We conjecture these objects may, at least in part, be members of the youngest population. We use the CMD simulations to obtain insight into the population structure of Carina's upper RGB.
description: Accepted by ApJS
Isolate record for VAFB-ISO-218
Creators: name: Holloway, Corinne
Year: 1991
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-218. The artifact is a large Monterey chert flake, black banded in color and possibly utilized on lateral margins. Measuring 40 cm by 60 cm.
Isolate record for VAFB-ISO-239
Creators: name: McClure, Maggie
Year: 1993
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-239. The artifact is a black Monterey chert biface fragment.
Holography for Heavy Ions Collisions at LHC and NICA
Creators: name: Aref'eva, I. Ya.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: This is a contribution for the Proceedings of 5th International Conference on New Frontiers in Physics (ICNFP 2016), held at Crete, 6-14 July 2016. Our goal is to obtain phenomenologically reliable insights for the physics of the quark-gluon plasma (QGP) from the holography. I briefly review how in the holographic setup one can describe the QGP formation in heavy ion collisions and how to get quantitatively the main characteristics of the QGP formation -- the total multiplicity and the thermalization time. To fit the experimental form of dependence of total multiplicity on energy, obtained at LHC, we have to deal with a special anisotropic holographic model, related with the Lifshitz-type background. Our conjecture is that this Lifshitz-type background with non-zero chemical potential can be used to describe future data expected from NICA. In particular, we present the results of calculations of the holographic confinement/deconfinement phase transition in the $(μ,T)$ (chemical potential, temperature) plane in this anisotropic background and show the dependence of the transition line on the orientation of the quark pair. This dependence leads to a non-sharp character of physical confinement/deconfinement phase in the $(μ,T)$-plane. We use the bottom-up soft wall approach incorporating quark confinement deforming factor and vector field providing the non-zero chemical potential. In this model we also estimate the holographic photon production.
description: 24 pages, 16 figures,Summary of the talks presented at 5th International Conference on New Frontiers in Physics (ICNFP 2016), held at Crete, 6-14 July 2016; Meeting of the working group on "Theory of Hadronic Matter under Extreme Conditions" 31 Oct -3 Nov 2016, Dubna and the seminar "Holography for NICA", MIAN, Moscow, 23 Dec 2016
S6W1
Creators: name: Aebig, Adam
Year: 2024
Subjects: subject: Mesoamerica
valueUri: https://core.tdar.org/browse/geographic-keyword/61/mesoamerica
subject: Basin of Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/3/basin-of-mexico
subject: Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/134/mexico
subject: Mexico (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/326/mexico-state-territory
subject: United Mexican States (Country)
valueUri: https://core.tdar.org/browse/geographic-keyword/438/united-mexican-states-country
subject: Central Mexico, Teotihuacan Valley
valueUri: https://core.tdar.org/browse/geographic-keyword/7/central-mexico-teotihuacan-valley
subject: Central Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/135/central-mexico
subject: Teotihuacan Valley
valueUri: https://core.tdar.org/browse/geographic-keyword/154/teotihuacan-valley
subject: Teotihuacan
valueUri: https://core.tdar.org/browse/geographic-keyword/202/teotihuacan
subject: Valley of Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/44/valley-of-mexico
subject: Classic Period
valueUri: https://core.tdar.org/browse/temporal-keyword/125/classic-period
subject: Terminal Formative
valueUri: https://core.tdar.org/browse/temporal-keyword/67/terminal-formative
subject: Teotihuacan Period
valueUri: https://core.tdar.org/browse/temporal-keyword/7765/teotihuacan-period
subject: Early Classic
valueUri: https://core.tdar.org/browse/temporal-keyword/5560/early-classic
subject: Teotihuacan
valueUri: https://core.tdar.org/browse/culture-keyword/7527/teotihuacan
subject: Teotihuacano
valueUri: https://core.tdar.org/browse/culture-keyword/9224/teotihuacano
subject: Teotihuacan
valueUri: https://core.tdar.org/browse/site-name/92/teotihuacan
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: Systematic Survey
valueUri: https://core.tdar.org/browse/investigation-type/12/systematic-survey

description: Site Survey Form For Square S6W1
Revisiting the role of cosmic-ray driven Alfvén waves in pre-existing magnetohydrodynamic turbulence. I. Turbulent damping rates and feedback on background fluctuations
Creators: name: Cerri, Silvio Sergio
Publisher: name: arXiv
Year: 2024
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Alfvén waves (AWs) excited by the cosmic-ray (CR) streaming instability (CRSI) are a fundamental ingredient for CR confinement. The effectiveness of self-confinement relies on a balance between CRSI growth rate and damping mechanisms acting on quasi-parallel AWs excited by CRs. One relevant mechanism is the so-called turbulent damping, in which an AW packet injected in pre-existing turbulence undergoes a cascade process due to its nonlinear interaction with fluctuations of the background. The turbulent damping of an AW packet in pre-existing magnetohydrodynamic turbulence is re-examined, revised, and extended to include most-recent theories of MHD turbulence that account for dynamic alignment and reconnection-mediated regime. The case in which the role of feedback of CR-driven AWs on pre-existing turbulence is important will also be discussed. Particular attention is given to the nonlinearity parameter $χ^w$ that estimates the strength of nonlinear interaction between CR-driven AWs and background fluctuations. We point out the difference between $χ^w$ and $χ^z$ that instead describes the strength of nonlinear interactions between pre-existing fluctuations. When $χ^w$ is properly taken into account, one finds that (i) the turbulent damping rate of quasi-parallel AWs in anisotropic turbulence depends on the background-fluctuations' amplitude to the third power, hence is strongly suppressed, and (ii) the dependence on the AW's wavelength (and thus on the CR gyro-radius from which it is excited) is different from what has been previously obtained. Finally, (iii) when dynamic alignment of cascading fluctuations and the possibility of a reconnection-mediated range is included in the picture, the turbulent damping rate exhibits novel regimes and breaks. Finally, a criterion for CR-feedback is derived and simple phenomenological models of CR-modified turbulent scaling are provided.
description: final version after language and layout corrections (19 pages, 3 figures, 2 tables)
Isolate record for VAFB-ISO-253
Creators: name: Holloway, Corinne
Year: 1995
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-253. The artifact is a tan chert core reduction flake.
S3W1
Creators: name: Aebig, Adam
Year: 2024
Subjects: subject: Mesoamerica
valueUri: https://core.tdar.org/browse/geographic-keyword/61/mesoamerica
subject: Basin of Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/3/basin-of-mexico
subject: Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/134/mexico
subject: Mexico (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/326/mexico-state-territory
subject: United Mexican States (Country)
valueUri: https://core.tdar.org/browse/geographic-keyword/438/united-mexican-states-country
subject: Central Mexico, Teotihuacan Valley
valueUri: https://core.tdar.org/browse/geographic-keyword/7/central-mexico-teotihuacan-valley
subject: Central Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/135/central-mexico
subject: Teotihuacan Valley
valueUri: https://core.tdar.org/browse/geographic-keyword/154/teotihuacan-valley
subject: Teotihuacan
valueUri: https://core.tdar.org/browse/geographic-keyword/202/teotihuacan
subject: Valley of Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/44/valley-of-mexico
subject: Classic Period
valueUri: https://core.tdar.org/browse/temporal-keyword/125/classic-period
subject: Terminal Formative
valueUri: https://core.tdar.org/browse/temporal-keyword/67/terminal-formative
subject: Teotihuacan Period
valueUri: https://core.tdar.org/browse/temporal-keyword/7765/teotihuacan-period
subject: Early Classic
valueUri: https://core.tdar.org/browse/temporal-keyword/5560/early-classic
subject: Teotihuacan
valueUri: https://core.tdar.org/browse/culture-keyword/7527/teotihuacan
subject: Teotihuacano
valueUri: https://core.tdar.org/browse/culture-keyword/9224/teotihuacano
subject: Teotihuacan
valueUri: https://core.tdar.org/browse/site-name/92/teotihuacan
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: Systematic Survey
valueUri: https://core.tdar.org/browse/investigation-type/12/systematic-survey

description: Site Survey Form From Square S3W1
title: Banca dati dei diari di scuola e delle autobiografie. Volume 2
Creators: name: Borruso, Francesca
Publisher: name: Roma TrE-Press
Year: 2022

description: Presentazione della banca dati
La Banca dati dei diari di scuola e delle autobiografie consiste in un repertorio elettronico di diari di scuola inediti e di autobiografie inedite redatti da insegnanti tra il 1861 e il 2001 e relativi ad esperienze educative e di insegnamento realizzate nella scuola pubblica o privata italiana.
Ciascuna scheda catalografica contiene una serie di informazioni relative al diario o all’autobiografia attraverso le quali è possibile risalire all’autore, alla scuola, all’anno scolastico e alla data di produzione dell’opera, al luogo di conservazione del manoscritto.
La scheda è inoltre corredata da una sinossi e da identificatori semantici e cronologici.
Responsabile intellettuale
Francesca Borruso
Autori delle schede
Francesca Borruso, Maura Di Giacinto, Francesca Davida Pizzigoni, Luca Silvestri
Demonstration of Metaplectic Geometrical Optics for Reduced Modeling of Plasma Waves
Creators: name: Marholt, Rune Højlund
name: Senstius, Mads Givskov
name: Nielsen, Stefan Kragh
Publisher: name: arXiv
Year: 2024
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: The WKB approximation of geometrical optics is widely used in plasma physics, quantum mechanics and reduced wave modeling in general. However, it is well-known that the approximation breaks down at focal and turning points. In this work we present the first unsupervised numerical implementation of the recently developed metaplectic geometrical optics framework, which extends the applicability of geometrical optics beyond the limitations of WKB, such that the wave field remains finite at caustics. The implementation is in 1D and uses a combination of Gauss-Freud quadrature and barycentric rational function inter- and extrapolation to perform an inverse metaplectic transform numerically. The capabilities of the numerical implementation are demonstrated on Airy's and Weber's equation, which both have exact solutions to compare with. Finally, the implementation is applied to the plasma physics problem of linear conversion of X-mode to electron Bernstein waves at the upper hybrid layer and a comparison is made with results from fully kinetic particle-in-cell simulations. In all three applications we find good agreement between the exact results and the new reduced wave modeling paradigm of metaplectic geometrical optics.
description: 18 pages (incl. references), 12 figures
First Detection of Equatorial Dark Dust Lane in a Protostellar Disk at Submillimeter Wavelength
Creators: name: Lee, Chin-Fei
name: Li, Zhi-Yun
name: Ho, Paul. T. P
name: Hirano, Naomi
name: Zhang, Qizhou
name: Shang, Hsien
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In the earliest (so-called "Class 0") phase of sunlike (low-mass) star formation, circumstellar disks are expected to form, feeding the protostars. However, such disks are difficult to resolve spatially because of their small sizes. Moreover, there are theoretical difficulties in producing such disks in the earliest phase, due to the retarding effects of magnetic fields on the rotating, collapsing material (so-called "magnetic braking"). With the Atacama Large Millimeter/submillimeter Array (ALMA), it becomes possible to uncover such disks and study them in detail. HH 212 is a very young protostellar system. With ALMA, we not only detect but also spatially resolve its disk in dust emission at submillimeter wavelength. The disk is nearly edge-on and has a radius of ~ 60 AU. Interestingly, it shows a prominent equatorial dark lane sandwiched between two brighter features, due to relatively low temperature and high optical depth near the disk midplane. For the first time, this dark lane is seen at submillimeter wavelength, producing a "hamburger"-shaped appearance that is reminiscent of the scattered-light image of an edge-on disk in optical and near infrared. Our observations open up an exciting possibility of directly detecting and characterizing small disks around the youngest protostars through high-resolution imaging with ALMA, which provides strong constraints on theories of disk formation.
description: 24 pages, 3 figures
N4W6
Creators: name: Robinson, Galen
Year: 2024
Subjects: subject: Mesoamerica
valueUri: https://core.tdar.org/browse/geographic-keyword/61/mesoamerica
subject: Basin of Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/3/basin-of-mexico
subject: Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/134/mexico
subject: Mexico (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/326/mexico-state-territory
subject: United Mexican States (Country)
valueUri: https://core.tdar.org/browse/geographic-keyword/438/united-mexican-states-country
subject: Central Mexico, Teotihuacan Valley
valueUri: https://core.tdar.org/browse/geographic-keyword/7/central-mexico-teotihuacan-valley
subject: Central Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/135/central-mexico
subject: Teotihuacan Valley
valueUri: https://core.tdar.org/browse/geographic-keyword/154/teotihuacan-valley
subject: Teotihuacan
valueUri: https://core.tdar.org/browse/geographic-keyword/202/teotihuacan
subject: Valley of Mexico
valueUri: https://core.tdar.org/browse/geographic-keyword/44/valley-of-mexico
subject: Classic Period
valueUri: https://core.tdar.org/browse/temporal-keyword/125/classic-period
subject: Terminal Formative
valueUri: https://core.tdar.org/browse/temporal-keyword/67/terminal-formative
subject: Teotihuacan Period
valueUri: https://core.tdar.org/browse/temporal-keyword/7765/teotihuacan-period
subject: Early Classic
valueUri: https://core.tdar.org/browse/temporal-keyword/5560/early-classic
subject: Teotihuacan
valueUri: https://core.tdar.org/browse/culture-keyword/7527/teotihuacan
subject: Teotihuacano
valueUri: https://core.tdar.org/browse/culture-keyword/9224/teotihuacano
subject: Teotihuacan
valueUri: https://core.tdar.org/browse/site-name/92/teotihuacan
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: Systematic Survey
valueUri: https://core.tdar.org/browse/investigation-type/12/systematic-survey

description: Site Surface Report for Square N4W6
Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals
Creators: name: Arredondo, J. Nijaid
name: Klein, Antoine
name: Yunes, Nicolás
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Future gravitational-wave detectors, especially the Laser Interferometer Space Antenna (LISA), will be sensitive to black hole binaries formed in astrophysical environments that promote large eccentricities and spin-induced orbital precession. Approximate models of gravitational waves that include both effects have only recently begun to be developed. The Efficient Fully Precessing Eccentric (EFPE) family is one such model, covering the inspiral stage with small-eccentricity-expanded gravitational-wave amplitudes accurate for initial time eccentricities $e < 0.3$ at 4 years before reaching an orbital frequency of 1 Hz. In this work, we extend this model to cover a larger range of initial eccentricities. The new EFPE for moderate eccentricities (EFPE_ME) model is able to accurately represent the leading-order gravitational-wave amplitudes to $e \leq 0.8$. Comparing the EFPE and the EFPE_ME models in the LISA band, however, reveals that there is no significant difference when the eccentricity at 4 years before merger, $e_0$, is less than or equal to 0.5, as radiation reaction circularizes supermassive black hole binaries too quickly. This suggests that the EFPE model may have a larger regime of validity in eccentricity space than previously thought, making it suitable for some inspiral parameter estimation with LISA data. On the other hand, for systems with $e_0 > 0.5$, the deviations between the models are significant, particularly for binaries with total masses below $10^5\, \mathrm{M}_{\odot}$. This suggests that the EFPE_ME model will be crucial to avoid systematic bias in parameter estimation with LISA in the future, once this model has been hybridized to include the merger and ringdown and the computation of the amplitudes is optimized.
description: 23 pages, 10 figures; matches published version
Isolate record for VAFB-ISO-248
Creators: name: McClure, Maggie
Year: 1994
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-248. The artifact is a dark-brown Monterey chert flake, measuring 5 cm long and 3 cm wide.
Multiple populations along the asymptotic giant branch of the globular cluster M 4
Creators: name: Lardo, C.
name: Salaris, M.
name: Savino, A.
name: Donati, P.
name: Stetson, P. B.
name: Cassisi, S.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Nearly all Galactic globular clusters host stars that display characteristic abundance anti-correlations, like the O-rich/Na-poor pattern typical of field halo stars, together with O-poor/Na-rich additional components. A recent spectroscopic investigation questioned the presence of O-poor/Na-rich stars amongst a sample of asymptotic giant branch stars in the cluster M 4, at variance with the spectroscopic detection of a O-poor/Na-rich component along both the cluster red giant branch and horizontal branch. This is contrary to what is expected from the cluster horizontal branch morphology and horizontal branch stellar evolution models. Here we have investigated this issue by employing the CUBI= (U-B)-(B-I) index, that previous studies have demonstrated to be very effective in separating multiple populations along both the red giant and asymptotic giant branch sequences. We confirm previous results that the RGB is intrinsically broad in the V-CUBI diagram, with the presence of two components which nicely correspond to the two populations identified by high-resolution spectroscopy. We find that AGB stars are distributed over a wide range of CUBI values, in close analogy with what is observed for the RGB, demonstrating that the AGB of M4 also hosts multiple stellar populations.
description: 6 pages, 4 figures, MNRAS accepted
Eco-evolutionary dynamics of adapting pathogens and host immunity
Creators: name: Barrat-Charlaix, Pierre
name: Neher, Richard A.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Populations and Evolution (q-bio.PE)
subject: FOS: Biological sciences

description: As pathogens spread in a population of hosts, immunity is built up and the pool of susceptible individuals is depleted. This generates selective pressure, to which many human RNA viruses, such as influenza virus or SARS-CoV-2, respond with rapid antigenic evolution and frequent emergence of immune evasive variants. However, the host's immune systems adapt and older immune responses wane, such that escape variants only enjoy a growth advantage for a limited time. If variant growth dynamics and reshaping of host-immunity operate on comparable time scales, viral adaptation is determined by eco-evolutionary interactions that are not captured by models of rapid evolution in a fixed environment. Here, we use a Susceptible/Infected model to describe the interaction between an evolving viral population in a dynamic but immunologically diverse host population. We show that depending on strain cross-immunity, heterogeneity of the host population, and durability of immune responses, escape variants initially grow exponentially, but lose their growth advantage before reaching high frequencies. Their subsequent dynamics follows an anomalous random walk determined by future escape variants and results in variant trajectories that are unpredictable. This model can explain the apparent contradiction between the clearly adaptive nature of antigenic evolution and the quasi-neutral dynamics of high frequency variants observed for influenza viruses.
description: Main text: 30 pages, 4 figures. Appendix: 26 pages, 7 figures
Isolate record for VAFB-ISO-206
Creators: name: Holloway, Corinne
Year: 1990
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-206. The artifact is a secondary Monterey chert flake measuring 14 cm by 6 cm.
Coarse-Grained Incompressible Magnetohydrodynamics: analyzing the turbulent cascades
Creators: name: Aluie, Hussein
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Fluid Dynamics (physics.flu-dyn)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We formulate a coarse-graining approach to the dynamics of magnetohydrodynamic (MHD) fluids at a continuum of length-scales. In this methodology, effective equations are derived for the observable velocity and magnetic fields spatially-averaged at an arbitrary scale of resolution. The microscopic equations for the bare velocity and magnetic fields are renormalized by coarse-graining to yield macroscopic effective equations that contain both a subscale stress and a subscale electromotive force (EMF) generated by nonlinear interaction of eliminated fields and plasma motions. At large coarse-graining length-scales, the direct dissipation of invariants by microscopic mechanisms (such as molecular viscosity and Spitzer resistivity) is shown to be negligible. The balance at large scales is dominated instead by the subscale nonlinear terms, which can transfer invariants across scales, and are interpreted in terms of work concepts for energy and in terms of topological flux-linkage for the two helicities. An important application of this approach is to MHD turbulence, where the coarse-graining length $\ell$ lies in the inertial cascade range. We show that in the case of sufficiently rough velocity and/or magnetic fields, the nonlinear inter-scale transfer need not vanish and can persist to arbitrarily small scales. Although closed expressions are not available for subscale stress and subscale EMF, we derive rigorous upper bounds on the effective dissipation they produce in terms of scaling exponents of the velocity and magnetic fields. These bounds provide exact constraints on phenomenological theories of MHD turbulence in order to allow the nonlinear cascade of energy and cross-helicity. On the other hand, we show that the forward cascade of magnetic helicity to asymptotically small scales is impossible unless 3rd-order moments of either velocity or magnetic field become infinite.
description: 33 pages, 2 figures, to appear in the special issue "Focus on Turbulence in Astrophysical and Laboratory Plasmas" of the New Journal of Physics
Clustering of primordial black holes from quantum diffusion during inflation
Creators: name: Animali, Chiara
name: Vennin, Vincent
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study how large fluctuations are spatially correlated in the presence of quantum diffusion during inflation. This is done by computing real-space correlation functions in the stochastic-$δN$ formalism. We first derive an exact description of physical distances as measured by a local observer at the end of inflation, improving on previous works. Our approach is based on recursive algorithmic methods that consistently include volume-weighting effects. We then propose a "large-volume'' approximation under which calculations can be done using first-passage time analysis only, and from which a new formula for the power spectrum in stochastic inflation is derived. We then study the full two-point statistics of the curvature perturbation. Due to the presence of exponential tails, we find that the joint distribution of large fluctuations is of the form $P(ζ_{R_1}, ζ_{R_2}) = F(R_1,R_2,r) P(ζ_{R_1})P( ζ_{R_2})$, where $ζ_{R_1}$ and $ζ_{R_2}$ denote the curvature perturbation coarse-grained at radii $R_1$ and $R_2$, around two spatial points distant by $r$. This implies that, on the tail, the reduced correlation function, defined as $P(ζ_{R_1}>ζ_{\rm{c}}, ζ_{R_2}>ζ_{\rm{c}})/[P(ζ_{R_1}>ζ_{\rm{c}}) P(ζ_{R_2}>ζ_{\rm{c}})]-1$, is independent of the threshold value $ζ_{\rm{c}}$. This contrasts with Gaussian statistics where the same quantity strongly decays with $ζ_{\rm{c}}$, and shows the existence of a universal clustering profile for all structures forming in the exponential tails. Structures forming in the intermediate (i.e. not yet exponential) tails may feature different, model-dependent behaviours.
description: 52 pages, 14 figures. Discussion around Eq.(3.6) expanded, a few minor changes and typos fixed. Some references added. Matches published version in JCAP
Isolate record for VAFB-ISO-247
Creators: name: McClure, Maggie
Year: 1991
Subjects: subject: Santa Barbara (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/3486/santa-barbara-county
subject: Vandenberg Air Force Base (VAFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85469/vandenberg-air-force-base-vafb
subject: Vandenberg Space Force Base (VSFB)
valueUri: https://core.tdar.org/browse/geographic-keyword/85584/vandenberg-space-force-base-vsfb
subject: California (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/1484/california-state-territory
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Chert
valueUri: https://core.tdar.org/browse/material-type/213/chert
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey

description: This document is the isolated find record for VAFB-ISO-247. The artifact is a primary flake of gray-blue-brown Monterey chert.
$1/N$-expansion for the critical temperature of the Bose gas
Creators: name: Hryhorchak, Orest
name: Pastukhov, Volodymyr
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We revised the large-$N$ expansion for a three-dimensional Bose system with short-range repulsion in normal phase. Particularly, for the model potential that is characterised only by the $s$-wave scattering length $a$ the full numerical calculations of the critical temperature in the $1/N$-approximation as a function of the gas parameter $an^{1/3}$ are performed. Additionally to the well-known result in the dilute limit we estimated analytically the leading-order strong-coupling behavior of the Bose-Einstein condensation transition temperature. It is shown that the critical temperature shift of the non-ideal Bose gas grows at small $an^{1/3}$, reaches some maximal value and then falls down becoming negative.
description: 6 pages, 3 figures
Correlations between Abelian Monopoles and center vortices
Creators: name: Nejad, Seyed Mohsen Hosseini
name: Deldar, Sedigheh
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the correlations between center vortices and Abelian monopoles for SU($3$) gauge group. Combining fractional fluxes of monopoles, center vortex fluxes are constructed in the thick center vortex model. Calculating the potentials induced by fractional fluxes constructing the center vortex flux in a thick center vortex-like model and comparing with the potential induced by center vortices, we observe an attraction between fractional fluxes of monopoles constructing the center vortex flux. We conclude that the center vortex flux is stable, as expected. In addition, we show that adding a contribution of the monopole-antimonopole pairs in the potentials induced by center vortices ruins the Casimir scaling at intermediate regime.
description: 11 pages, 11 figures, Version accepted for publication in Nucl. Phys. B