cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Why is it so Cold in Here?: Explaining the Cold Temperatures Retrieved from Transmission Spectra of Exoplanet Atmospheres
Creators: name: MacDonald, Ryan J.
name: Goyal, Jayesh M.
name: Lewis, Nikole K.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Transmission spectroscopy is a powerful technique widely used to probe exoplanet terminators. Atmospheric retrievals of transmission spectra are enabling comparative studies of exoplanet atmospheres. However, the atmospheric properties inferred by retrieval techniques display a significant anomaly: most retrieved temperatures are far colder than expected. In some cases, retrieved temperatures are ~1000 K colder than T_eq. Here, we provide an explanation for this conundrum. We demonstrate that erroneously cold temperatures result when 1D atmospheric models are applied to spectra of planets with differing morning-evening terminator compositions. Despite providing an acceptable fit, 1D retrieval techniques artificially tune atmospheric parameters away from terminator-averaged properties. Retrieved temperature profiles are hundreds of degrees cooler and have weaker temperature gradients than reality. Retrieved abundances are mostly biased by > 1$σ$ and sometimes by > 3$σ$, with the most extreme biases for ultra-hot Jupiters. When morning-evening compositional differences manifest for prominent opacity sources, H$_2$O abundances retrieved by 1D models can be biased by over an order of magnitude. Finally, we demonstrate that these biases provide an explanation for the cold retrieved temperatures reported for WASP-17b and WASP-12b. To overcome biases associated with 1D atmospheric models, there is an urgent need to develop multidimensional retrieval techniques.
description: 16 pages, 4 figures. Accepted for publication in ApJL
The myth of impoverished signal : dispelling the spoken-language fallacy for emoticons in online communication
Creators: name: Baron, Naomi S.
Publisher: name: American University (Washington, D.C.)
Year: 2023
Subjects: classificationCode: 47
subject: Language, communication and culture

description: A version of this chapter appeared in 2009 in Jane Vincent and Leopoldina Fortunati, eds., Electronic Emotion: The Mediation of Emotion via Information and Communication Technologies. Oxford, UK: Peter Lang, pp. 107-135.
The myth of impoverished signal : dispelling the spoken-language fallacy for emoticons in online communication
Creators: name: Baron, Naomi S.
Publisher: name: American University
Year: 2023

description: A version of this chapter appeared in 2009 in Jane Vincent and Leopoldina Fortunati, eds., Electronic Emotion: The Mediation of Emotion via Information and Communication Technologies. Oxford, UK: Peter Lang, pp. 107-135.
title: Идентификация и фальсификация товаров. Идентификация и фальсификация текстильных товаров
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2019

description: В учебном пособии даны краткие теоретические сведения по изучаемым темам курса «Идентификация и фальсификация товаров». Приведены основные термины и определения; рассмотрены методы и способы идентификации, признаки фальсификации продукции, изложены требования к качеству продукции, регламентируемые в соответствующих технических регламентах и стандартах. К каждой теме даны методические указания к выполнению лабораторных работ. Рекомендуется для студентов, обучающихся по направлению 27.03.01 «Стандартизация и метрология».
title: A Bayesian Space-Time Dynamic Linear Model for Radioactivity Deposition after a Nuclear Accident
Creators: name: De, Swarup
Publisher: name: The Open University
Year: 2009

description: A three-stage Hierarchical Bayesian Space-Time (HBST) model, an extension of the class of dynamic linear models to space, is proposed for the ground contamination levels (GCL) and related uncertainties caused by polluting discharges in the environment. The model should allow updating the distribution of GCL in time and space as new data in the form of measurements and expert judgements become available to give real-time estimates of deposition levels. An application of the HBST model is proposed for the statistical modelling of radioactivity deposition after a nuclear accident. It explicitly handles uncertainties associated with (i) predictions of depositions from a long-range atmospheric dispersal model, (ii) in-situ gamma ray measurements and (iii) spatial interpolations. Unlike existing environmental statistical models, the HBST model also accounts for an established food chain contamination model called ECOSYS for which it provides data assimilation capabilities. The HBST model permits a fast implementation and full probabilistic inference for the parameters, interpolation and forecasts. Three distinct formulations of the HBST model were applied to assimilate real data of radioactivity deposition from the Chernobyl accident in southern Germany. Two of those formulations differ on the functional form of their spatial covariance matrices while the third, a normal inverse-Wishart model, allows the spatial covariances to "learn" from the data within the usual Bayesian paradigm. The later is shown to outperform the former models both in short and medium term forecasting as well as in a predictive interpolation test that took some measurements as out-of-sample.
title: Идентификация и фальсификация товаров. Идентификация и фальсификация товаров легкой промышленности
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2020

description: В учебном пособии даны краткие теоретические сведения по изучаемым темам курса «Идентификация и фальсификация товаров». Приведены основные термины и определения; рассмотрены методы и способы идентификации, признаки фальсификации продукции, изложены требования к качеству продукции, регламентируемые в соответствующих технических регламентах и стандартах. В каждой теме даны методические указания к выполнению лабораторных работ. Рекомендуется для студентов, обучающихся по направлению 27.03.01 «Стандартизация и метрология».
Age-chemical abundance structure of the Galaxy I: Evidence for a late accretion event in the outer disc at z ~ 0.6
Creators: name: Lian, Jianhui
name: Thomas, Daniel
name: Maraston, Claudia
name: Zamora, Olga
name: Tayar, Jamie
name: Pan, Kaike
name: Tissera, Patricia
name: Fernández-Trincado, José G.
name: Garcia-Hernandez, Domingo Anibal
Publisher: name: arXiv
Year: 2020
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigate the age-chemical abundance structure of the outer Galactic disc at a galactocentric distance of r > 10 kpc as recently revealed by the SDSS/APOGEE survey. Two sequences are present in the [alpha/Fe]-[Fe/H] plane with systematically different stellar ages. Surprisingly, the young sequence is less metal-rich, suggesting a recent dilution process by additional gas accretion. As the stars with the lowest iron abundance in the younger sequence also show an enhancement in alpha-element abundance, the gas accretion event must have involved a burst of star formation. In order to explain these observations, we construct a chemical evolution model. In this model we include a relatively short episode of gas accretion at late times on top of an underlying secular accretion over long timescales. Our model is successful at reproducing the observed distribution of stars in the three dimensional space of [alpha/Fe]-[Fe/H]-Age in the outer disc. We find that a late-time accretion with a delay of 8.2 Gyr and a timescale of 0.7 Gyr best fits the observed data, in particular the presence of the young, metal-poor sequence. Our best-fit model further implies that the amount of accreted gas in the late-time accretion event needs to be about three times the local gas reservoir in the outer disc at the time of accretion in order to sufficiently dilute the metal abundance. Given this large fraction, we interpret the late-time accretion event as a minor merger presumably with a gas-rich dwarf galaxy with a mass M_* < 10^9 M_Sun and a gas fraction of ~ 75 per cent.
description: 17 pages, 11 figures, accepted for publication in MNRAS
Hamiltonian BRST and Batalin-Vilkovisky formalisms for second quantization of gauge theories
Creators: name: Barnich, Glenn
name: Grigoriev, Maxim
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Gauge theories that have been first quantized using the Hamiltonian BRST operator formalism are described as classical Hamiltonian BRST systems with a BRST charge of the form _{even} and with natural ghost and parity degrees for all fields. The associated proper solution of the classical Batalin-Vilkovisky master equation is constructed from first principles. Both of these formulations can be used as starting points for second quantization. In the case of time reparametrization invariant systems, the relation to the standard _{odd} master action is established.
description: 25 pages, LaTeX
Charges of Monopole Operators in $\widehat{ADE}$ Chern-Simons Quiver Gauge Theories
Creators: name: Patra, Moumita
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We compute R-charges of the BPS-monopole operators in $\mathcal{N} = 3$ $\widehat{ADE}$ Chern-Simons quiver gauge theories, along the lines of the work of Benna, Klebanov and Klose in \cite{bkk}. These theories have a weakly coupled UV completion in terms of $\mathcal{N}=3$ supersymmetric Chern-Simons Yang-Mills theories. In the UV limit the monopole operators are well approximated by classical solutions. We construct classical BPS and anti-BPS monopole solutions to these theories which preserve $\frac{1}{3}$ supersymmetry all along the RG flow. We compute the $SU(2)_R$ charges in these backgrounds and show that the smallest possible value of quantised $SU(2)_R$ charge is zero in each quiver theory.
description: 72 pages, 6 figures. This article supersedes arXiv:1809.10731
title: Иностранный язык (английский). Интерактивные занятия
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2019

description: Учебное издание соответствует содержанию дисциплины Б1.Б.3 Иностранный язык (английский) направлений подготовки 42.03.02 Журналистика, 42.03.03 Издательское дело профиль Книгоиздательское дело, дисциплины Б1.Б.4 Иностранный язык (английский) направления подготовки 42.03.01 Реклама и связи с общественностью профиль Реклама и связи с общественностью в коммерческой сфере.
Higher-order Alexander invariants of plane algebraic curves
Creators: name: Leidy, Constance
name: Maxim, Laurentiu
Publisher: name: arXiv
Year: 2005
Subjects: subject: Algebraic Topology (math.AT)
subject: Algebraic Geometry (math.AG)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 32S20, 32S05, 14J70, , 14F17, 57M25, 57M27

description: We define new higher-order Alexander modules $\mathcal{A}_n(C)$ and higher-order degrees $δ_n(C)$ which are invariants of the algebraic planar curve $C$. These come from analyzing the module structure of the homology of certain solvable covers of the complement of the curve $C$. These invariants are in the spirit of those developed by T. Cochran in \cite{C} and S. Harvey in \cite{H} and \cite{Har}, which were used to study knots, 3-manifolds, and finitely presented groups, respectively. We show that for curves in general position at infinity, the higher-order degrees are finite. This provides new obstructions on the type of groups that can arise as fundamental groups of complements to affine curves in general position at infinity.
description: a new section 'Examples' is added
title: Иностранный язык (английский язык). Перевод и разговорная речь
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2019

description: Учебное издание соответствует содержанию дисциплины Б1.Б.3 Иностранный язык направления подготовки 15.03.02 Технологические машины и оборудование профиль Полиграфические машины и автоматизированные комплексы.
title: Иностранный язык (английский язык): профессионально-ориентированная лексика
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2019

description: Учебное издание соответствует содержанию дисциплины Б1.Б.4 Иностранный язык направления подготовки 09.03.02 Информационные системы и технологии профиль Информационные технологии в дизайне, направления подготовки 09.03.02 Информационные системы и технологии профиль Информационные технологии в медиаиндустрии.
High-energy neutrinos as observational signature of massive black hole formation
Creators: name: Berezinsky, Veniamin S.
name: Dokuchaev, Vyacheslav I.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe the formation of a seed massive black hole (MBH) inside a supermassive star (SMS) in a distant galactic nucleus. The short-lived SMS is naturally formed due to collision destructions of normal stars in the evolving galactic nucleus. The neutron stars (NSs) and stellar-mass black holes form a compact self-gravitating subsystem deep inside a SMS. This subsystem is short-lived in comparison with a host SMS and collapses finally into the MBH. Just before gravitational collapse of compact subsystem the frequent NS collisions are accompanied by the generation of numerous ultra-relativistic fireballs. A combined ram pressure of multiple coexisting fireballs produces a quasi-stationary rarefied cavity in the central part of SMS. The protons are accelerated in the fireballs and by relativistic shocks in the cavity. All secondary particles, produced in collisions, except the high-energy neutrinos are absorbed in the SMS interiors. An estimated high-energy neutrino signal from this hidden source can be detected by the neutrino telescope with an effective area 1 km^2 providing the evidence for MBH formation in a distant galactic nucleus. A corresponding lifetime of this high-energy hidden neutrino source is ~0.1-1 yr.
description: 8 pages
Constraining VLBI-optical offsets in high redshift galaxies using strong gravitational lensing
Creators: name: Spingola, C.
name: Barnacka, A.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a multi-wavelength analysis of two highly magnified strong gravitationally lensed galaxies, CLASS B0712+472 and CLASS B1608+656, at redshifts $1.34$ and $1.394$, respectively, using new VLBI and archival HST observations. We reconstruct the positions of the radio and optical emissions with their uncertainties using Monte Carlo sampling. We find that in CLASS B0712+472 the optical and radio emissions are co-spatial within $2\pm5$ mas ($17\pm 42$ pc at redshift of 1.34). But, in CLASS B1608+656, we reconstruct an optical-radio offset of $25\pm16$ mas ($214\pm137$ pc at redshift of 1.394), the smallest offset measured for an AGN at such high redshift. The spectral features indicate that CLASS B1608+656 is a post-merger galaxy, which, in combination with the optical-VLBI offset reported here, makes CLASS B1608+656 a promising candidate for a high-$z$ offset-AGN. Furthermore, the milliarcsecond angular resolution of the VLBI observations combined with the precise lens models allow us to spatially locate the radio emission at $0.05$ mas precision ($0.4$ pc) in CLASS B0712+472, and $0.009$ mas precision ($0.08$ pc) in CLASS B1608+656. The search for optical-radio offsets in high redshift galaxies will be eased by the upcoming synoptic all-sky surveys, including E-ELT and SKA, which are expected to find $\sim 10^5$ strongly lensed galaxies, opening an era of large strong lensing samples observed at high angular resolution.
description: 16 pages, 7 figures; accepted for publication in MNRAS
X-Ray and Infrared Observations of Embedded Young Stars in L1630
Creators: name: Simon, T.
name: Andrews, S. M.
name: Rayner, J. T.
name: Drake, S. A.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The HH 24-26 star-forming region within the L1630 dark cloud in Orion contains a remarkable collection of rare Class 0 and Class I protostars, collimated molecular and ionized jets, and a luminous but spatially unresolved ASCA X-ray source. To study the X-ray properties of the embedded protostar population of that region, we have obtained a deep X-ray image with the ACIS-S camera on board the Chandra X-Ray Observatory. A number of H-alpha emission-line objects were detected in the areas surrounding HH 24-26, of which the weak-line T Tauri star SSV 61 was the brightest source, at a steady luminosity of 10^31.9 erg/s (0.3-10 keV). Two Class I protostars aligned with optical jets in HH 24, SSV 63E and SSV 63W, were also detected, as was the continuum radio source SSV 63NE, which is very likely an extreme Class I or Class 0 object. We observed no X rays from the Class 0 protostars HH 24-MMS and HH 25-MMS, nor any from regions of the cloud bounded by HH 25 and HH 26, at a 2-sigma upper limit of 10^30.0 erg/s. HH 26-IR, the Class I object thought to be the origin of the HH 26 flow, was not detected. Near-infrared spectroscopy obtained at the NASA IRTF reveals 3 micron ice bands in the spectra of SSV 59, 63E, 63W, and HH 26-IR, and 2.3 micron CO overtone absorption bands for SSV 61. SSV 60, which lies astride one end of the great arc of nebulosity forming HH 25, exhibits a deep infrared ice band and CO absorption, but is not an X-ray source, and is most likely a distant background giant of late spectral type.
description: to appear in ApJ. 32 pages, 8 figures. High-resolution figures available at http://www.ifa.hawaii.edu/~andrews/L1630.ps
ANRS - François Dabis
Creators: name: Leibowitch, Jacques (1942-2020)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: 1 fichier (2 pages).
description: created: start=2019-08-05;end=2019-11-13
title: Иностранный язык (английский язык). Сборник упражнений по переводу и разговорной речи
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2019

description: Учебное издание соответствует содержанию дисциплины Б1.Б.4 Иностранный язык направления подготовки 09.03.01 Информатика и вычислительная техника профиль Автоматизированные системы обработки информации и управления, направления подготовки 09.03.02 Информационные системы и технологии профиль Информационные технологии в дизайне, профиль Информационные технологии в медиаиндустрии.
Absolute anomalies in (2+1)D symmetry-enriched topological states and exact (3+1)D constructions
Creators: name: Bulmash, Daniel
name: Barkeshli, Maissam
Publisher: name: arXiv
Year: 2020
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Algebra (math.QA)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Certain patterns of symmetry fractionalization in (2+1)D topologically ordered phases of matter can be anomalous, which means that they possess an obstruction to being realized in purely (2+1)D. In this paper we demonstrate how to compute the anomaly for symmetry-enriched topological (SET) states of bosons in complete generality. We demonstrate how, given any unitary modular tensor category (UMTC) and symmetry fractionalization class for a global symmetry group $G$, one can define a (3+1)D topologically invariant path integral in terms of a state sum for a $G$ symmetry-protected topological (SPT) state. We present an exactly solvable Hamiltonian for the system and demonstrate explicitly a (2+1)D $G$ symmetric surface termination that hosts deconfined anyon excitations described by the given UMTC and symmetry fractionalization class. We present concrete algorithms that can be used to compute anomaly indicators in general. Our approach applies to general symmetry groups, including anyon-permuting and anti-unitary symmetries. In addition to providing a general way to compute the anomaly, our result also shows, by explicit construction, that every symmetry fractionalization class for any UMTC can be realized at the surface of a (3+1)D SPT state. As a byproduct, this construction also provides a way of explicitly seeing how the algebraic data that defines symmetry fractionalization in general arises in the context of exactly solvable models. In the case of unitary orientation-preserving symmetries, our results can also be viewed as providing a method to compute the $\mathcal{H}^4(G, U(1))$ obstruction that arises in the theory of $G$-crossed braided tensor categories, for which no general method has been presented to date.
description: 39+18 pages, 20+13 figures
The random 2-SAT partition function
Creators: name: Achlioptas, Dimitris
name: Coja-Oghlan, Amin
name: Hahn-Klimroth, Max
name: Lee, Joon
name: Müller, Noela
name: Penschuck, Manuel
name: Zhou, Guangyan
Publisher: name: arXiv
Year: 2020
Subjects: subject: Probability (math.PR)
subject: Discrete Mathematics (cs.DM)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 05C80, 60C05, 68Q87

description: We show that throughout the satisfiable phase the normalised number of satisfying assignments of a random $2$-SAT formula converges in probability to an expression predicted by the cavity method from statistical physics. The proof is based on showing that the Belief Propagation algorithm renders the correct marginal probability that a variable is set to `true' under a uniformly random satisfying assignment.
Transverse phase-locking in fully frustrated Josephson junction arrays: a new type of fractional giant steps
Creators: name: Marconi, Veronica
name: Kolton, Alejandro
name: Dominguez, Daniel
name: Gronbech-Jensen, Niels
Publisher: name: arXiv
Year: 2003
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We study, analytically and numerically, phase locking of driven vortex lattices in fully-frustrated Josephson junction arrays at zero temperature. We consider the case when an ac current is applied {\it perpendicular} to a dc current. We observe phase locking, steps in the current-voltage characteristics, with a dependence on external ac-drive amplitude and frequency qualitatively different from the Shapiro steps, observed when the ac and dc currents are applied in parallel. Further, the critical current increases with increasing transverse ac-drive amplitude, while it decreases for longitudinal ac-drive. The critical current and the phase-locked current step width, increase quadratically with (small) amplitudes of the ac-drive. For larger amplitudes of the transverse ac-signal, we find windows where the critical current is hysteretic, and windows where phase locking is suppressed due to dynamical instabilities. We characterize the dynamical states around the phase-locking interference condition in the $IV$ curve with voltage noise, Lyapunov exponents and Poincaré sections. We find that zero temperature phase-locking behavior in large fully frustrated arrays is well described by an effective four plaquette model.
description: 12 pages, 11 figures
Guided Disentangled Representation Learning from Audio data for Transfer Learning
Creators: name: Haque, Kazi
Publisher: name: University of Southern Queensland
Year: 2024
Subjects: Machine Learning
Deep Learning
Generative Adversarial Neural Networks
Convolutional Neural Networks
Guided Representation Learning
TransferLearning

description: In the field of machine learning, disentangled representation learning seeks to map high-dimensional data into a low-dimensional space where the underlying variational factors are both disentangled and easily separable. This thesis investigates the application of such representations, derived from unlabelled data to tasks where only limited labelled data is available. Specifically, I explore the domain of audio modelling, where the absence of supervision in learning representations from unlabelled data often results in representations that may not be optimally useful for downstream tasks, leading to potential resource wastage. To address this issue, I introduce the Guided Generative Adversarial Neural Network (GGAN), a novel model that utilises a modest amount of labelled data to guide the learning of relevant disentangled representations from a larger corpus of unlabelled data. While the representation learned through GGAN proves beneficial for the task at hand, its generalisation capabilities are limited, restricting the model's application to tasks similar to or closely related to the original one. To overcome this limitation, I propose a second model, the Guided Generative Adversarial Autoencoder (GAAE), which not only learns representations tailored to a specific downstream task but also captures the general attributes of the data, thereby being independent of the particular task. Both GGAN and GAAE are founded on the Generative Adversarial Network (GAN) architecture, leveraging the audio generalisation prowess of GANs for representation learning. Nevertheless, the models eschew working with 1D raw audio waveforms directly, instead utilising 2D spectrograms, a practice that recent research suggests may curtail the models' ultimate performance capabilities, representing a significant gap in the literature. This thesis confronts this issue head-on. Convolutional Neural Networks (CNNs), forming the structural backbone of both GGAN and GAAE, have historically faced challenges in generating raw audio waveforms via adversarial training. A foundational step in surmounting this hurdle involves a thorough examination of CNNs' ability to model raw audio waveforms, such as classification tasks. Moving strategically in this direction, I have proposed two cosine filter-based CNN models: the Cosine Convolution Neural Network (CosCovNN) and the Vector Quantised Cosine Convolutional Neural Network with Memory (VQCCM). These models have not only outclassed traditional CNN architectures but have also set a new benchmark in the field of audio classification.
title: Иностранный язык. Английский язык. Контрольные работы. Самостоятельная работа
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2017

description: Цель данного пособия - дать основные рекомендации по изучению программного материала курса английского языка в Санкт-Петербургском государственном университете промышленных технологий и дизайна. Данное пособие включает материалы для аудиторных занятий и самостоятельной работы по дисциплине «Иностранный язык» для бакалавров первого курса заочного отделения. В пособии представлены контрольные работы и краткие справочные материалы по грамматике английского языка. Кроме того, в пособие включены тексты для дополнительного чтения и материалы для самостоятельной работы студентов. Пособие предназначено для студентов первого курса заочной формы обучения по всем направлениям подготовки для получения звания бакалавра Санкт-Петербургского государственного университета промышленных технологий и дизайна.
Universal restrictions to the conversion of heat into work derived from the analysis of the Nernst theorem as a uniform limit
Creators: name: Martin-Olalla, Jose-Maria
name: de Luna, Alfredo Rey
Publisher: name: arXiv
Year: 2003
Subjects: subject: Classical Physics (physics.class-ph)
subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: We revisit the relationship between the Nernst theorem and the Kelvin-Planck statement of the second law. We propose that the exchange of entropy uniformly vanishes as the temperature goes to zero. The analysis of this assumption shows that is equivalent to the fact that the compensation of a Carnot engine scales with the absorbed heat so that the Nernst theorem should be embedded in the statement of the second law. ----- Se analiza la relaci{ó}n entre el teorema de Nernst y el enunciado de Kelvin-Planck del segundo principio de la termodin{á}mica. Se{ñ}alamos el hecho de que el cambio de entrop{\'ı}a tiende uniformemente a cero cuando la temperatura tiende a cero. El an{á}lisis de esta hip{ó}tesis muestra que es equivalente al hecho de que la compensaci{ó}n de una m{á}quina de Carnot escala con el calor absorbido del foco caliente, de forma que el teorema de Nernst puede derivarse del enunciado del segundo principio.
description: 8pp, 4 ff. Original in english. Also available translation into spanish. Twocolumn format. RevTeX
Clusters Have Edges: The Projected Phase SpaceStructure of SDSS redMaPPer Clusters
Creators: name: Tomooka, Paxton
name: Rozo, Eduardo
name: Wagoner, Erika L.
name: Aung, Han
name: Nagai, Daisuke
name: Safonova, Sasha
Publisher: name: arXiv
Year: 2020
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the distribution of line-of-sight velocities of galaxies in the vicinity of SDSS redMaPPer galaxy clusters. Based on their velocities, galaxies can be split into two categories: galaxies that are dynamically associated with the cluster, and random line-of-sight projections. Both the fraction of galaxies associated with the galaxy clusters, and the velocity dispersion of the same, exhibit a sharp feature as a function of radius. The feature occurs at a radial scale $R_{\rm edge} \approx 2.2R_{\rmλ}$, where $R_{\rmλ}$ is the cluster radius assigned by redMaPPer. We refer to $R_{\rm edge}$ as the "edge radius." These results are naturally explained by a model that further splits the galaxies dynamically associated with a galaxy cluster into a component of galaxies orbiting the halo and an infalling galaxy component. The edge radius $R_{\rm edge}$ constitutes a true "cluster edge", in the sense that no orbiting structures exist past this radius. A companion paper (Aung et al. 2020) tests whether the "halo edge" hypothesis holds when investigating the full three-dimensional phase space distribution of dark matter substructures in numerical simulations, and demonstrates that this radius coincides with a suitably defined splashback radius.
description: 10 pages, 5 figures, submitted to MNRAS, companion paper to Aung et al. 2020
Phase Coherence in a Driven Double-Well System
Creators: name: Miyakawa, T.
name: Search, C. P.
name: Meystre, P.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We analyze the dynamics of the molecular field incoherently pumped by the photoassociation of fermionic atoms and coupled by quantum tunnelling in a double-well potential. The relative phase distribution of the molecular modes in each well and their phase coherence are shown to build up owing to quantum mechanical fluctuations starting from the vacuum state. We identify three qualitatively different steady-state phase distributions, depending on the ratio of the molecule-molecule interaction strength to interwell tunnelling, and examine the crossover from a phase-coherent regime to a phase-incoherent regime as this ratio increases.
description: 5 pages, 2 figures
Talk about texting : Attitudes towards mobile phones
Creators: name: Baron, Naomi S.
Publisher: name: American University (Washington, D.C.)
Year: 2023
Subjects: classificationCode: 47
subject: Language, communication and culture

description: More than half the world’s population now has access to mobile phones. While these devices enable spoken communication, many users (especially teenagers and young adults) heavily employ them for sending and receiving written text messages. There is a growing literature on the linguistic features of text messages, but much less is objectively known about user attitudes towards texting (or towards mobile phones in general). Drawing upon data from a cross-cultural mobile phone project involving university students in Sweden, the US, Italy, Japan, and Korea, this study examines user perspectives on mobile communication, with special emphasis on texting functions.
The remnant of neutron star-white dwarf merger and the repeating fast radio bursts
Creators: name: Liu, Xiang
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Fast radio bursts (FRBs) at cosmological distances still hold concealed physical origins. Previously Liu (2018) proposes a scenario that the collision between a neutron star (NS) and a white dwarf (WD) can be one of the progenitors of non-repeating FRBs and notices that the repeating FRBs can also be explained if a magnetar formed after such NS-WD merger. In this paper, we investigate this channel of magnetar formation in more detail. We propose that the NS-WD post-merger, after cooling and angular momentum redistribution, may collapse to either a black hole or a new NS or even remains as a hybrid WDNS, depending on the total mass of the NS and WD. In particular, the newly formed NS can be a magnetar if the core of the WD collapsed into the NS while large quantities of degenerate electrons of the WD compressed to the outer layers of the new NS. A strong magnetic field can be formed by the electrons and positive charges with different angular velocities induced by the differential rotation of the newborn magnetar. Such a magnetar can power the repeating FRBs by the magnetic reconnections due to the crustal movements or starquakes.
description: 8 pages, accepted
title: Revue de presse des articles publiés sur ICCARRE entre janvier 2014 et mars 2015
Creators: name: Leibowitch, Jacques
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Source: http://www.calames.abes.fr/pub/ms/Calames-20193111232830351
description: created: start=2014;end=2015-03
Network-based models for social recommender systems
Creators: name: Godoy-Lorite, Antonia
name: Guimera, Roger
name: Sales-Pardo, Marta
Publisher: name: arXiv
Year: 2020
Subjects: subject: Machine Learning (stat.ML)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Machine Learning (cs.LG)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: With the overwhelming online products available in recent years, there is an increasing need to filter and deliver relevant personalized advice for users. Recommender systems solve this problem by modeling and predicting individual preferences for a great variety of items such as movies, books or research articles. In this chapter, we explore rigorous network-based models that outperform leading approaches for recommendation. The network models we consider are based on the explicit assumption that there are groups of individuals and of items, and that the preferences of an individual for an item are determined only by their group memberships. The accurate prediction of individual user preferences over items can be accomplished by different methodologies, such as Monte Carlo sampling or Expectation-Maximization methods, the latter resulting in a scalable algorithm which is suitable for large datasets.
Additional file 2 of Principal component analysis of adipocytokines and insulin associate with risk factors of cardiovascular diseases
Creators: name: Yarizadeh, Habib
name: Setayesh, Leila
name: Moein Askarpoor
name: Pooyan, Sara
name: Seyedeh Forough Sajjadi
name: Negin Badrooj
name: Roberts, Caroline
name: Mirzaei, Khadijeh
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer

description: Additional file 2: Table S2. Demographic, medical and biomedical characteristics with adherence to two groups of Adipokines patterns.
Additional file 1 of KnowTox: pipeline and case study for confident prediction of potential toxic effects of compounds in early phases of development
Creators: name: Morger, Andrea
name: Mathea, Miriam
name: Achenbach, Janosch H.
name: Wolf, Antje
name: Buesen, Roland
name: Schleifer, Klaus-Juergen
name: Landsiedel, Robert
name: Volkamer, Andrea
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Additional file 1. Additional Tables S1–S5.
Chaotic self-similar wave maps coupled to gravity
Creators: name: Szybka, Sebastian J.
Publisher: name: arXiv
Year: 2003
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We continue our studies of spherically symmetric self-similar solutions in the SU(2) sigma model coupled to gravity. For some values of the coupling constant we present numerical evidence for the chaotic solution and the fractal threshold behavior. We explain this phenomenon in terms of horseshoe-like dynamics and heteroclinic intersections.
description: 25 pages, 17 figures
title: Иностранный язык. Английский язык: практическая грамматика
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2017

description: Учебное издание соответствует содержанию дисциплины Иностранный язык всех направлений подготовки и специальности 54.05.03 Графика.
Crystal and magnetic structure of antiferromagnetic Mn$_{2}$PtPd
Creators: name: Kumar, Vivek
name: Reehuis, Manfred
name: Hoser, Andreas
name: Adler, Peter
name: Felser, Claudia
Publisher: name: arXiv
Year: 2020
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We have investigated the crystal and magnetic structure of Mn${}_{2}$PtPd alloy using powder x-ray and neutron diffraction experiments. This compound is believed to belong to the Heusler family having crystal symmetry $\mathit{I}$4/$\mathit{mmm}$ (TiAl${}_{3}$-type). However, in this work we found that the Pd and Pt atoms are disordered and thus Mn${}_{2}$PtPd crystallizes in the $\mathit{L}$1${}_{0}$ structure having $\mathit{P}$4/$\mathit{mmm}$ symmetry (CuAu-I type) like MnPt and MnPd binary alloys. The lattice constants are $\mathit{a}$ = 2.86 Å and $\mathit{c}$ = 3.62 Å at room temperature. Mn${}_{2}$PtPd has a collinear antiferromagnetic spin structure below the Néel temperature $\mathit{T}$${}_{N}$ = 866 K, where Mn moments of $\mathrm{\sim}$4 $μ$${}_{B}$ lie in the $\mathit{ab}$-plane. We observed a strong change in the lattice parameters near $\mathit{T}$${}_{N}$. The sample exhibits metallic behaviour, where electrical resistivity and carrier concentration are of the order of 10${}^{-5}$ $Ω$ cm and 10${}^{21}$ cm${}^{-3}$, respectively.
Talk about texting : Attitudes towards mobile phones
Creators: name: Baron, Naomi S.
Publisher: name: American University
Year: 2023

description: More than half the world’s population now has access to mobile phones. While these devices enable spoken communication, many users (especially teenagers and young adults) heavily employ them for sending and receiving written text messages. There is a growing literature on the linguistic features of text messages, but much less is objectively known about user attitudes towards texting (or towards mobile phones in general). Drawing upon data from a cross-cultural mobile phone project involving university students in Sweden, the US, Italy, Japan, and Korea, this study examines user perspectives on mobile communication, with special emphasis on texting functions.
Structure of Exotic Nuclei
Creators: name: Dobaczewski, J.
name: Michel, N.
name: Nazarewicz, W.
name: Ploszajczak, M.
name: Stoitsov, M. V.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The progress in the modeling of exotic nuclei with an extreme neutron-to-proton ratio is discussed. Two topics are emphasized: (i) the quest for the universal microscopic nuclear energy density functional and (ii) the progress in the continuum shell model.
description: 10 pages, 2 figures, presented by W. Nazarewicz at the International Symposium on "A New Era of Nuclear Structure Physics", Kurokawa Village (Niigata Pref.), Japan, Nov. 19-22, 2003
title: A word at the limit
Creators: name: Kazarina, Tatiana
Publisher: name: Technology and Language, 2(1), 81-97
Year: 2021
Subjects: Cubo-futurism
“Gilea”
Semiosis
Universe
Creative strategy
Zaum
Suprematism

description: The article discusses the reasons for the pronounced interest of cubo-futurists in the possibilities of the poetic word and the nature of their experiments with linguistic material. The author proceeds from the fact that for the artists of the early Russian avant-garde, the laws of language and the system of cultural conventions are an artificially created barrier that protects the sphere of human existence from the surplus of naturally emanating energy. This protects society from shocks, but at the same time deprives it of the opportunity to develop. All the poets of the “Gilea” group saw as their most important task the elimination of this gap between objective reality and the sphere of semiosis, but the most convincing solutions were offered by Vladimir Mayakovsky, Velimir Khlebnikov and Alexei Kruchenykh. The purpose of this article is to characterize the strategies developed by these artists for overcoming the linguistic dogma of the previous culture and to determine the range of possibilities for the future. A structural-semiotic approach to the analysis of avant-garde texts was used. In this way it can be shown that the poetic work with words and the variants proposed by the three authors proceeded in different directions and was in many respects mutually exclusive. While the poetics of Mayakovsky assumed the convergence of words and things, Khlebnikov's experiments were carried out to balance both, and Kruchenykh’s zaum creativity took the word out of any control, except for the author's will. Even if different poets used the same words to denote the genres and types of creativity they discovered, they were talking about dissimilar phenomena. This is demonstrated by comparing the zaum of Khlebnikov with the zaum of Kruchenykh. Each of the creative projects proposed by the three poets was an experiment to identify certain limiting possibilities of the word, therefore, in the work of all three poets it did not lose its meaning.
description: Technology and Language, 2(1), 81-97
Observational Evidence for an Age Dependence of Halo Bias
Creators: name: Yang, Xiaohu
name: Mo, H. J.
name: Bosch, Frank C. van den
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the dependence of the cross-correlation between galaxies and galaxy groups on group properties. Confirming previous results, we find that the correlation strength is stronger for more massive groups, in good agreement with the expected mass dependence of halo bias. We also find, however, that for groups of the same mass, the correlation strength depends on the star formation rate (SFR) of the central galaxy: at fixed mass, the bias of galaxy groups decreases as the SFR of the central galaxy increases. We discuss these findings in light of the recent findings by Gao et al (2005) that halo bias depends on halo formation time, in that halos that assemble earlier are more strongly biased. We also discuss the implication for galaxy formation, and address a possible link to galaxy conformity, the observed correlation between the properties of satellite galaxies and those of their central galaxy.
description: 4 pages, 4 figures, Accepted for publication in ApJ Letters. Figures 3 and 4 replaced. The bias dependence on the central galaxy luminosity is omitted due to its sensitivity to the mass model
title: Инфокоммуникационные системы и сети
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2017

description: Учебное издание соответствует содержанию дисциплины Б1.В.ОД.13 Инфокоммуникационные системы и сети направления подготовки 09.03.02 Информационные системы и технологии профиль Информационные технологии в дизайне, Информационные технологии в медиаиндустрии.
Talking takes too long : gender and cultural patterns in mobile telephony
Creators: name: Campbell, Elise M.
name: Baron, Naomi S.
Publisher: name: American University
Year: 2023

description: The sociolinguistic literature has frequently reported differences in how males and females communicate face-to-face and in writing, and more recently, through information and communication technologies. This article reports on gender patterns identified in a cross- cultural study of mobile phone use by university students in Sweden, the US, Italy, Japan and Korea. Data were analyzed with respect to the purpose of communication, politeness issues, social manipulation and volume of use (along with user complaints about dependency and reachability). Results indicated a number of gendered usage and attitudinal patterns. However, in some cases, cultural variables may prove more explanatory than gender.
Explicit Multi-element Extension of the Spectral Neighbor Analysis Potential for Chemically Complex Systems
Creators: name: Cusentino, Mary Alice
name: Wood, Mitchell A.
name: Thompson, Aidan P.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: A natural extension of the descriptors used in the Spectral Neighbor Analysis Potential (SNAP) method is derived to treat atomic interactions in chemically complex systems. Atomic environment descriptors within SNAP are obtained from a basis function expansion of the weighted density of neighboring atoms. This new formulation instead partitions the neighbor density into partial densities for each chemical element, thus leading to explicit multi-element descriptors. For $N_{elem}$ chemical elements, the number of descriptors increases as $\mathcal{O}(N_{elem}^3)$, while the computational cost of the force calculation as implemented in LAMMPS is limited to $\mathcal{O}(N_{elem}^2)$ and the favorable linear scaling in the number of atoms is retained. We demonstrate these chemically aware descriptors by producing an interatomic potential for indium phosphide capable of capturing high-energy defects that result from radiation damage cascades. This new explicit multi-element SNAP method reproduces the relaxed defect formation energies with substantially greater accuracy than weighted-density SNAP, while retaining accurate representation of the bulk indium phosphide properties.
description: 11 pages, 4 figures