cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
ПОСТТЕХНОГЕННАЯ ЦИВИЛИЗАЦИЯ: ОТ ТЕОРИИ К ПРАКТИКЕ
Creators: name: Вадим Михайлович Маслов
Publisher: name: Революция и эволюция: модели развития в науке, культуре, обществе
Year: 2019
Subjects: техногенная цивилизация
посттехногенная цивилизация
теория
практика
СМИ
общественное мнение
социально ответственный университет

description: Современное общественное развитие требует дальнейшего осмысления техногенного феномена. В теории техногенной цивилизации анализируется техногенное как таковое. Цель техногенного: преобразование всего наличного в рациональное, управляемое, искусственное, техногенное. Техника из средства становится целью. Человек (как био-социальное существо) преодолевается по двум направлениям: постчеловеческому (появляются техно-социальные су-щества) и вне-человеческому (появляется искусственный интеллект). Сохранение человеческо-го видится либо на путях отхода, либо контроля развитых форм техногенного. Контроль по-стчеловеческих и внечеловеческих тенденций и итогов суть формирования посттехногенной цивилизации. Теория посттехногенной цивилизации суть теории главной цели современного человечества. Современность требует активизации философской практики формирования по-сттехногенной цивилизации. Ведущая философская практика утверждения посттехногенной цивилизации должна выступить в роли ведущего СМИ. Философская посттехногенная практи-ка, опираясь на наличные логико-риторические, методологические, эвристические знания и умения, способна отстоять посттехногенную истину в любой полемике. В идеале, необходимо, чтобы все обучающееся (будущие представители всех профессий) приобщались к посттехно-генному тестированию своей деятельности, обеспечивая начало формирования и дальнейшее функционирование посттехногенной цивилизации. Такого качества университет будущего можно обозначить как социально ответственный университет.
Decay of a Thermofield-Double State in Chaotic Quantum Systems
Creators: name: del Campo, Adolfo
name: Vilaplana, Javier Molina
name: Santos, Lea F.
name: Sonner, Julian
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Scrambling in interacting quantum systems out of equilibrium is particularly effective in the chaotic regime. Under time evolution, initially localized information is said to be scrambled as it spreads throughout the entire system. This spreading can be analyzed with the spectral form factor, which is defined in terms of the analytic continuation of the partition function. The latter is equivalent to the survival probability of a thermofield double state under unitary dynamics. Using random matrices from the Gaussian unitary ensemble (GUE) as Hamiltonians for the time evolution, we obtain exact analytical expressions at finite $N$ for the survival probability. Numerical simulations of the survival probability with matrices taken from the Gaussian orthogonal ensemble (GOE) are also provided. The GOE is more suitable for our comparison with numerical results obtained with a disordered spin chain with local interactions. Common features between the random matrix and the realistic disordered model in the chaotic regime are identified. The differences that emerge as the spin model approaches a many-body localized phase are also discussed.
description: 12 pages, 4 figures
Shear-free gravitational collapse is strongly censored
Creators: name: Goncalves, Sergio M. C. V.
Publisher: name: arXiv
Year: 2003
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider spherically symmetric spacetimes with matter whose timelike flow is assumed to be shear-free. A number of results on the formation and visibility of spacetime singularities is proven, with the main one being that shear-free collapse cannot admit locally naked singularities (which implies absence of globally naked singularities). We conjecture that shear is a necessary condition for the occurrence of locally naked singularities in generic gravitational collapse.
description: 6 pages, revtex4; accepted for publication in Phys. Rev. D Rapid Comm
УНИВЕРСАЛЬНЫЙ ЭВОЛЮЦИОНИЗМ И КОНВЕРГЕНЦИЯ ИЛИ ПОЛИОНТИЗМ И КОЭВОЛЮЦИЯ
Creators: name: Владимир Александрович Кутырев
name: Владимир Владимирович Слюсарев
Publisher: name: Революция и эволюция: модели развития в науке, культуре, обществе
Year: 2019
Subjects: конвегенция
коэволюция
антропоконсерватизм
онтология
синегретика
технонаука

description: В данной статье авторы предпринимают попытку проследить параллели между двумя оппозициями: революцией и эволюцией с одной стороны, и коэволюцией и самоорганизацией – с другой. Прежде всего, отмечается, что противопоставление революции и эволюции в со-временной социальной реальности является недостаточно актуальным и несколько устарев-шим. Современный мир тяготит к стиранию границ между размеренным эволюционным разви-тием и резкими революционными изменениями, превращаются в непроходящую революцию. Именно такой представляется происходящая сейчас Четвертая промышленная революция. По-добная реализация революционной эволюции близко граничит с концепцией самоорганиции – столь же универсальна и всеобъемлющая. Именно универсальный, революционной эволюцио-низм является фундаментальной основой конвергенции, трансформирующейся в бесцельный новационно-технологический трансгресс. Человек выносится «за скобки», становясь устарев-шим, стремится к своей «ненужности в мире». В качестве альтернативы конвергенции, развен-чивающей человека, авторами предлагается обратиться к концепции коэволюции как модели «коммуникативной онтологии». В противовес постоянному противопоставлению и взаимо-борьбе различных онтологий, на которой основывается идея прогресса, предлагается концепт полионтизма – коммуникации и взаимообмена разных подходов мироописания. Авторами вы-двигается предположение о том, что именно полионтическая коэволюционная парадигма мо-жет стать эффективным способом сохранения традиционного пространства жизненного мира человека.
Additional file 1 of Phylogenetic signal from rearrangements in 18 Anopheles species by joint scaffolding extant and ancestral genomes
Creators: name: Anselmetti, Yoann
name: Duchemin, Wandrille
name: Tannier, Eric
name: Chauve, Cedric
name: SĂ¨Verine BĂŠrard
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Evolutionary Biology
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Supplementary text. (PDF 181 kb)
Comment on "Thermal Effects on the Casimir Force in the 0.1-5 micrometer Range"
Creators: name: Lamoreaux, Steve K.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In a recent paper (M. Bostrom and Bo E. Sernelius, Phys. Rev. Lett. 84, 4757 (2000)) the combined effect of finite conductivity and finite temperature on the Casimir force is analyzed, and significant deviations from other theoretical results and a recent experiment are obtained. In this Comment, I show that the extrapolation to zero frequency is incorrect because the authors have neglected that the wavenumber and frequency of the electromagentic mode must simultaneously appraoch zero
description: Final version (two previous versions, first was partly incorrect) Rejected by PRL!
Vortices in the Co-orbital Region of an Embedded Protoplanet
Creators: name: Koller, Josef
name: Li, Hui
name: Lin, Douglas N. C.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present global 2-D inviscid disk simulations with an embedded planet, emphasizing the non-linear dynamics in its co-orbital region. We find that the potential vorticity of the flow in this region is not conserved due to the presence of two spiral shocks produced by the planet. As the system evolves, the potential vorticity profile develops extrema (inflection points) which eventually render the flow unstable. Vortices are produced in association with the potential vorticity minima. Born in the separatrix region, these vortices experience close-encounters with the planet, consequently exerting strong torques on the planet. The existence of these vortices have important implications on understanding the migration rates of low mass planets.
description: 5 pages, 4 figures. accepted for publication in ApJL
Additional file 2 of Comparison of endotracheal aspirate and bronchoalveolar lavage fluid metagenomic next-generation sequencing in severe pneumonia: a nested, matched case–control study
Creators: name: Bao, Renren
name: Mei, Qing
name: Yang, Tianjun
name: Zhang, Lei
name: Zhu, Chunyan
name: Fan, Xiaoqin
name: Wang, Yinzhong
name: Tong, Fei
name: He, Yuxi
name: Fang, Xiaowei
name: Geng, Shike
name: Yang, Yu
name: Sheng, Ximei
name: Pan, Aijun
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Table S2. The protocols and primers of real-time quantitative PCR for detecting 17 pathogens.
КОЛЛЕКЦИОНЕРЫ РЕВОЛЮЦИЙ
Creators: name: Нина Михайловна Малиновская
Publisher: name: Революция и эволюция: модели развития в науке, культуре, обществе
Year: 2019
Subjects: гуманитарно-технологическая революция; информационно-коммуникационные революции; формы организации совместной деятельности; типы профес-сионализма

description: В первой части статьи показано, как термин «революция» превращается из предиката синтетического суждения об отдельном событии в категориальное понятие социальной фило-софии, философии истории и методологии, в содержании которого раскрывается сущность глобальных социальных трансформаций. Коренные изменения форм человеческой деятельно-сти и социальных отношений, обозначенные исследователями в разное время как революции, складываются в общую картину развивающегося социального мира. Построена классификация информационно-коммуникационных революций (ИКР), в ко-торой появление философии, абстрактной математики и логики рассматривается как ИКР «Oсевого времени» – середины I тысячелетия до н.э. Автор привлекает эвристические, прогностические и методические возможности поня-тия «революция» к поиску ответа на вопрос, можно ли противостоять нарастающей в ходе чет-вертой промышленной революции «деколлективизации». С этой целью прослеживается связь ИКР и профессиональных революций с эволюцией типов совместной деятельности, выделен-ных и исследованных отечественными учеными. Перечислены пять императивов совместно-творческой деятельности. Обоснована взаимосвязь форм организации совместной деятельно-сти и типов профессионализма. Отмечен практический характер проблемы перехода к совместно-творческой деятельно-сти.
Phenomenology of Doubly Special Relativity
Creators: name: Amelino-Camelia, Giovanni
name: Kowalski-Glikman, Jerzy
name: Mandanici, Gianluca
name: Procaccini, Andrea
Publisher: name: arXiv
Year: 2003
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Investigations of the possibility that some novel ``quantum" properties of spacetime might induce a modification dispersion relation focused at first on scenarios with Planck-scale violations of Lorentz symmetry. More recently several studies have considered the possibility of a ``doubly special relativity", in which the modification of the dispersion relation emerges from a framework with both the Planck scale and the speed-of-light scale as characteristic scales of a deformation of the Lorentz transformations. For the schemes with broken Lorentz symmetry at the Planck scale there is a large literature on the derivation of experimental limits. We provide here a corresponding analysis for the doubly-special-relativity framework. We find that the analyses of photon stability, synchrotron radiation, and threshold conditions for particle production in collision processes, the three contexts which are considered as most promising for constraining the broken-Lorentz-symmetry scenario, cannot provide significant constraints on doubly-special-relativity parameter space. However, certain types of analyses of gamma-ray bursts are sensitive to the symmetry deformation. A key element of our study is an observation that removes a possible sign ambiguity for the doubly-special-relativity framework. This result also allows us to characterize more sharply the differences between the doubly-special-relativity framework and the framework of k-Poincare Hopf algebras, two frameworks which are often confused with each other in the literature.
description: 22 pages, LaTex
Novel solid state vacuum quartz encapsulated growth of p-Terphenyl: the parent High Tc Oraganic Superconductor (HTOS)
Creators: name: Maheshwari, P. K.
name: Meena, R. S.
name: Gahtori, Bhasker
name: Goyal, Reena
name: Sultana, Rabia
name: Rani, Poonam
name: Awana, V. P. S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report an easy and versatile route for the synthesis of the parent phase of newest superconducting wonder material i.e. p-Terphenyl. Doped p-terphenyl has recently shown superconductivity with transition temperature as high as 120K. For crystal growth, the commercially available p-Terphenyl powder is pelletized, encapsulated in evacuated (10-4 Torr) quartz tube and subjected to high temperature (260C) melt followed by slow cooling at 5C/hour. Simple temperature controlled heating furnace is used during the process. The obtained crystal is one piece, shiny and plate like. Single crystal surface XRD (X-ray Diffraction) showed unidirectional (00l) lines, indicating that the crystal is grown along c-direction. Powder XRD of the specimen showed that as grown p-Terphenyl is crystallized in monoclinic structure with space group P21/a space group, having lattice parameters a = 8.08(2) A, b = 5.62(5) A and c= 13.58(3) A. Scanning electron microscopy (SEM) pictures of the crystal showed clear layered slab like growth without any visible contamination from oxygen. Characteristic reported Raman active modes related to C-C-C bending, C-H bending, C-C stretching and C-H stretching vibrations are seen clearly for the studied p-Terphenyl crystal. The physical properties of crystal are yet underway. The short letter reports an easy and versatile crystal growth method for obtaining quality p-terphenyl. The same growth method may probably be applied to doped p-terphenyl and to subsequently achieve superconductivity to the tune of as high 120K for the newest superconductivity wonder i.e., High Tc Oraganic Superconductor (HTOS).
description: 7 Pages including Figs: Short note on easy synthesis of p-Terphenyl-HTOS
No Sun-like dynamo on the active star $ζ$ Andromedae from starspot asymmetry
Creators: name: Roettenbacher, Rachael M.
name: Monnier, John D.
name: Korhonen, Heidi
name: Aarnio, Alicia N.
name: Baron, Fabien
name: Che, Xiao
name: Harmon, Robert O.
name: Kovari, Zsolt
name: Kraus, Stefan
name: Schaefer, Gail H.
name: Torres, Guillermo
name: Zhao, Ming
name: Brummelaar, Theo A. ten
name: Sturmann, Judit
name: Sturmann, Laszlo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Sunspots are cool areas caused by strong surface magnetic fields inhibiting convection. Moreover, strong magnetic fields can alter the average atmospheric structure, degrading our ability to measure stellar masses and ages. Stars more active than the Sun have more and stronger dark spots than in the solar case, including on the rotational pole itself. Doppler imaging, which has so far produced the most detailed images of surface structures on other stars than the Sun, cannot always distinguish the hemisphere in which the starspots are located, especially in the equatorial region and if the data quality is not optimal. This leads to problems in investigating the north-south distribution of starspot active latitudes (those latitudes with more spot activity), which are crucial constraints of dynamo theory. Polar spots, inferred only from Doppler tomography, could plausibly be observational artifacts, casting some doubt on their very existence. Here we report imaging of the old, magnetically-active star $ζ$ Andromedae using long-baseline infrared interferometry. In our data, a dark polar spot is seen in each of two epochs, while lower-latitude spot structures in both hemispheres do not persist between observations revealing global starspot asymmetries. The north-south symmetry of active latitudes observed on the Sun is absent on $ζ$ And, which hosts global spot patterns that cannot be produced by solar-type dynamos.
description: Published in Nature, 33 pages, 8 figures, 5 tables
К СОЦИАЛЬНОЙ НОРМЕ СТАНОВЛЕНИЯ ЧЕЛОВЕКА В КУЛЬТУРЕ
Creators: name: Елена Борисовна Бабошина
Publisher: name: Революция и эволюция: модели развития в науке, культуре, обществе
Year: 2019
Subjects: норма
становление
человек
культура
ценность
смысл

description: Автор представляет подход к социальной норме в становлении человека как результату выбора в дилемме сущего и сущности, подчеркивая одновременность индивидуального и соци-ального пространства выбора. Понятие «норма» определяется с онтологических и социально-антропологических позиций, что способствует восприятию социально-культурной реальности как ценностного и целостного мира человека. По мнению автора, понимание социальной нор-мы становления человека в ее развитии как следствия восприятия ситуации выбора либо как осознания вневременной ценности человека в отношении к дилемме «нормативность – вне-нормативность» показывает разное качество развития нормы как идеи социального порядка. Таким образом, автор полемизирует с ограничением понимания нормы только как исторически сложившегося феномена и на этой основе почти не подверженного ценностному сомнению. В социально-философском и антропологическом обосновании подхода к социальной норме ав-тор считает важным учет аксиологического взаимодействия ценности, нормы и смысла в изу-чении нормы становления человека в культуре. Подход помогает открытию горизонтов ценно-стно-смысловой (духовной) идентификации в современном обществе вопреки нормам потреб-ления как культурного отчуждения человека от себя и других.
Gravitational Waves from Hyper-Accretion onto Nascent Black Holes
Creators: name: Araya-Gochez, Rafael Angel
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We examine the possibility that hyper-accretion onto newly born, black holes occurs in highly intermittent, non-asymmetric fashion favorable to gravitational wave emission in a neutrino cooled disk. This picture of near-hole accretion is motivated by magneto-rotationally induced, ultra-relativistic disk dynamics in the region of the flow bounded from below by the marginally bound geodesic radius. For high spin values, a largely coherent magnetic field in this region has the dynamical implication of compact mass segregation at the displacement nodes of the non-axisymmetric, MRI modes. When neutrino stress competes favorably for the disk dynamical structure, the matter clumps may be rather dense and sufficiently long-lived to excite the Quasi-Normal Ringing (a.k.a. QNR) modes of the Kerr geometry upon their in-fall. We find that such accretion flow may drive bar-like, quadrupole (l,m=2,2) modes in nearly resonant fashion for spin parameters $a \geq .9$. The ensuing build up in strain amplitude of the undamped oscillations warrants a brisk rate of energy deposition into gravitational waves. A detectability assessment for the LIGO interferometers through the match filtering technique is given by integrating the energy flux over a one second epoch of resonant hyper-accretion at $1 \msun \sec^{-1}$. Thus, a $15 \msun$ Kerr black hole spinning at $a \simeq .98$ ($f_{\rm QNR} \simeq 1677$ Hz), and located at 27 Mpc (e.g., GRB980425), will deliver a characteristic strain amplitude, $h_{\rm char} \simeq 2.2_{-21}$, large enough to be detectable by LIGO II. If resonant hyper-accretion were sustainable for a longer period (or at higher rates) possibly associated with a second broad hump in a GRB light-curve, these objects could be detected by LIGO I at very low redshifts.
description: 12 pages, 4 figures, M.N.R.A.S. submission
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00325
Creators: name: de la Côte-d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes
subject: LaMOP

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00325, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Analytic Expression for Exact Ground State Energy Based on an Operator Method for a Class of Anharmonic Potentials
Creators: name: Kwek, L. C.
name: Liu, Yong
name: Oh, C. H.
name: Wang, Xiang-Bin
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A general procedure based on shift operators is formulated to deal with anharmonic potentials. It is possible to extract the ground state energy analytically using our method provided certain consistency relations are satisfied. Analytic expressions for the exact ground state energy have also been derived specifically for a large class of the one-dimensional oscillator with cubic-quartic anharmonic terms. Our analytical results can be used to check the accuracy of existing numerical methods, for instance the method of state-dependent diagonalization. Our results also agree with the asymptotic behavior in the divergent pertubative expansion of quartic harmonic oscillator.
description: LaTeX with six figure (gif) files; Submitted to Phys. Rev. A
Additional file 5: of Patient-directed self-management of pain (PaDSMaP) compared to treatment as usual following total knee replacement; a randomised controlled trial
Creators: name: Deane, Katherine
name: Gray, Richard
name: Balls, Paula
name: Darrah, Clare
name: Swift, Louise
name: Clark, Alan
name: Barton, Garry
name: Morris, Sophie
name: Butters, Sue
name: Bullough, Angela
name: Flaherty, Helen
name: Talbot, Barbara
name: Sanders, Mark
name: Donell, Simon
Publisher: name: figshare
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences

description: Training pamphlets for the PaDSMaP study. (PDF 1589 kb)
Galactic Point Sources of TeV Antineutrinos
Creators: name: Anchordoqui, Luis A.
name: Goldberg, Haim
name: Halzen, Francis
name: Weiler, Thomas J.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: High energy cosmic ray experiments have identified an excess from the region of the Galactic Plane in a limited energy range around $10^{18}$ eV (EeV). This is very suggestive of neutrons as candidate primaries, because the directional signal requires relatively-stable neutral primaries, and time-dilated neutrons can reach Earth from typical Galactic distances when the neutron energy exceeds an EeV. We here point out that if the Galactic messengers are neutrons, then those with energies below an EeV will decay in flight, providing a flux of cosmic antineutrinos above a TeV which is {\it observable} at a kilometer-scale neutrino observatory. The expected event rate per year above 1 TeV in a detector such as IceCube, for example, is 20 antineutrino showers (all flavors) and a $1^\circ$ directional signal of 4 $\bar ν_μ$ events. A measurement of this flux can serve to identify the first extraterrestrial point source of TeV antineutrinos.
description: matches published version
Moduli of quantum Riemannian geometries on <= 4 points
Creators: name: Majid, S.
name: Raineri, E.
Publisher: name: arXiv
Year: 2003
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We classify parallelizable noncommutative manifold structures on finite sets of small size in the general formalism of framed quantum manifolds and vielbeins introduced previously. The full moduli space is found for $\le 3$ points, and a restricted moduli space for 4 points. The topological part of the moduli space is found for $\le 9$ points based on the known atlas of regular graphs. We also discuss aspects of the quantum theory defined by functional integration.
description: 34 pages ams-latex, 4 figures
ТЕЛЕСНОСТЬ И ТЕЛЕСНАЯ ОСОЗНАННОСТЬ: ЕСТЬ ЛИ ЗНАК РАВЕНСТВА?
Creators: name: Наталья Николаевна Булыга
Publisher: name: Революция и эволюция: модели развития в науке, культуре, обществе
Year: 2019
Subjects: тело
телесность
сознание тела
сознание — тело
телесная осознанность
осознанность тела

description: В настоящее время тема телесности рассматривается в философии достаточно широко и затрагивает онтологические, антропологические, культурологические и другие аспекты. Пово-дом для рассмотрения вопроса о том, как соотносится телесность и телесная осознанность ста-ла книга «Сознание тела: философия осознанности и сомаэстетики» Ричарда Шустермана — американского философа-прагматика, внесшего вклад в эстетику как философскую дисципли-ну и развивающуюся область под названием сомаэстетика. Данную книгу в переводе на рус-ский язык найти не удалось, имеется лишь её англоязычное издание. Обзор русскоязычной литературы и статей привел к пониманию, что в текстах в основ-ном используются слова «тело», «телесность». Поставлена проблема «сознание-тело». Замече-но, что термин «телесная осознанность» в философии широко не употребляется и существует, в основном, в психологической литературе. В свою очередь, в указанной выше книге Р. Шус-термана используется именно термин «сознание тела». Попробуем разобраться в нюансах тер-минов и того, какую смысловую нагрузку они несут.
ТЕОРЕТИЧЕСКИЕ ОСНОВАНИЯ БЛАГОПОЛУЧНОГО ПУТИ ЖИЗНИ ЧЕЛОВЕКА
Creators: name: Сергей Анатольевич Ермаков
Publisher: name: Революция и эволюция: модели развития в науке, культуре, обществе
Year: 2019
Subjects: человек
путь жизни
благополучный путь
добродетель
динамика жизни
реальность
объективность
субъективность

description: В статье рассматривается вопрос о необходимости поиска теоретических оснований для построения благополучного пути жизни человека. При этом индивидуальный путь жизни чело-века полагается как реальность, присущая и данная субъекту, формируемая им (и/или другими) под воздействием природной, социальной и духовной среды и являющаяся частью бытия. В связи с этим обращается внимание на то, что путь жизни человека есть объективно-субъективная реальность, включающая в себя био-социо-духовные начала, которые пребывают в непрерывной динамике. Знание этого аспекта помогает человеку представить свой путь жиз-ни как целостное динамичное образование. Вместе с тем в статье указывается на роль субъек-тивного фактора в построении благополучной жизни. Как человек ведет себя в конкретных жизненных ситуациях, таким и выстраивается его жизненный путь. По мнению автора, благо-получный путь жизни напрямую связан с позитивной направленностью индивидуального бы-тия человека. Насколько человек сможет сохранить свое тело в здоровом состоянии, поддер-живать его жизненную активность, насколько он сможет включиться в систему родственных отношений с возможностью их воспроизводства, повысить свой социальный статус нацелен-ный на благобытие, в котором такие ценности, как добро, красота, вера и любовь являются до-минирующими в человеческом мироощущении, настолько человек и сможет обрести свой бла-гополучный путь жизни. Для реализации этого предлагается избегать негативных моментов в своем существовании и тяготеть ко всему доброму, принуждать себя к добродетели, стремить-ся всегда делать лучшее из возможного, возрастать в добродетели.
Magnetic topological analysis of coronal bright points
Creators: name: Galsgaard, K.
name: Madjarska, M. S.
name: Moreno-Insertis, F.
name: Huang, Z.
name: Wiegelmann, T.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: {We report on the first of a series of studies on coronal bright points investigating the physical mechanism that generates these phenomena.} {The aim of this paper is to understand the magnetic-field structure that hosts the bright points.} {We use longitudinal magnetograms taken by the Solar Optical Telescope with the Narrowband Filter Imager. For a single case, magnetograms from the Helioseismic and Magnetic Imager were added to the analysis. The longitudinal magnetic field component is used to derive the potential magnetic fields of the large regions around the bright points. A magneto-static field extrapolation method is tested to verify the accuracy of the potential field modelling. The three dimensional magnetic fields are investigated for the presence of magnetic null points and their influence on the local magnetic domain.} {In 9 out of 10 cases the bright point resides in areas where the coronal magnetic field contains an opposite polarity intrusion defining a magnetic null point above it. It is found that X-ray bright points reside, in these 9 cases, in a limited part of the projected fan dome area, either fully inside the dome or expanding over a limited area below which typically a dominant flux concentration resides. The 10th bright point is located in a bipolar loop system without an overlying null point.} {All bright points in coronal holes and two out of tree bright points in quiet Sun regions are seen to reside in regions containing a magnetic null point. An yet unidentified process(es) generates the BPs in specific regions of the fan-dome structure. }
description: 14 pages, 9 figures, 10 movies located at http://comp.astro.ku.dk/kg/BP/movies/, Accepted for publication in A&A
Photon antibunching in the fluorescence of individual color centers in diamond
Creators: name: Brouri, Rosa
name: Beveratos, Alexios
name: Poizat, Jean-Philippe
name: Grangier, Philippe
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We have observed photon antibunching in the fluorescence light emitted from a single N-V center in diamond at room temperature. The possibility of generating triggerable single photons with such a solide state system is discussed
description: 4 pages, 4 figures
Additional file 1 of Relationship of caffeine regimen with osteopenia of prematurity in preterm neonates: a cohort retrospective study
Creators: name: Kumar, Manoj
name: Ali, Amin
name: Khan, Muhammad Azeem
name: Sohail, Sadia
name: Saleem, Syed Muzafar
name: Khan, Midhat
name: Naz, Fizzah
name: Khan, Wasif Ahmed
name: Salat, Muhammad Sohail
name: Hussain, Kashif
name: Ambreen, Gul
Publisher: name: figshare
Year: 2022
Subjects: Medicine
Pharmacology
Biological Sciences not elsewhere classified
Developmental Biology
Science Policy

description: Additional file 1.
X-ray Preionisation Powered by Accretion on the First Black Holes. I: a Model for the WMAP Polarisation Measurement
Creators: name: Ricotti, Massimo
name: Ostriker, Jeremiah P.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the possibility that there is a first phase of partial ionisation due to X-rays produced by black hole accretion in small-mass galaxies at redshifts 7
description: MNRAS in press (ref: 2004, MNRAS, 352,547). 16 pages, including 10 figures and 3 tables
Galaxy Cluster Mass Reconstruction Project: III. The impact of dynamical substructure on cluster mass estimates
Creators: name: Old, L.
name: Wojtak, R.
name: Pearce, F. R.
name: Gray, M. E.
name: Mamon, G. A.
name: Sifón, C.
name: Tempel, E.
name: Biviano, A.
name: Yee, H. K. C.
name: de Carvalho, R.
name: Müller, V.
name: Sepp, T.
name: Skibba, R. A.
name: Croton, D.
name: Power, S. P. Bamford C.
name: von der Linden, A.
name: Saro, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: With the advent of wide-field cosmological surveys, we are approaching samples of hundreds of thousands of galaxy clusters. While such large numbers will help reduce statistical uncertainties, the control of systematics in cluster masses becomes ever more crucial. Here we examine the effects of an important source of systematic uncertainty in galaxy-based cluster mass estimation techniques: the presence of significant dynamical substructure. Dynamical substructure manifests as dynamically distinct subgroups in phase-space, indicating an 'unrelaxed' state. This issue affects around a quarter of clusters in a generally selected sample. We employ a set of mock clusters whose masses have been measured homogeneously with commonly-used galaxy-based mass estimation techniques (kinematic, richness, caustic, radial methods). We use these to study how the relation between observationally estimated and true cluster mass depends on the presence of substructure, as identified by various popular diagnostics. We find that the scatter for an ensemble of clusters does not increase dramatically for clusters with dynamical substructure. However, we find a systematic bias for all methods, such that clusters with significant substructure have higher measured masses than their relaxed counterparts. This bias depends on cluster mass: the most massive clusters are largely unaffected by the presence of significant substructure, but masses are significantly overestimated for lower mass clusters, by $\sim10\%$ at $10^{14}$ and $\geq20\%$ for $\leq10^{13.5}$. The use of cluster samples with different levels of substructure can, therefore, bias certain cosmological parameters up to a level comparable to the typical uncertainties in current cosmological studies.
description: 14 pages, 8 figures, 3 tables. Submitted to MNRAS
Additional file 1: of Development and validation of the Crohnâ s disease patient-reported outcomes signs and symptoms (CD-PRO/SS) diary
Creators: name: Higgins, Peter
name: Harding, Gale
name: Leidy, Nancy
name: DeBusk, Kendra
name: Patrick, Donald
name: Viswanathan, Hema
name: Fitzgerald, Kristina
name: Donelson, Sarah
name: Marcoli Cyrille
name: Ortmeier, Brian
name: Wilson, Hilary
name: Revicki, Dennis
name: Globe, Gary
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Development and validation of the Crohnâ s Disease Patient-reported Outcomes Signs and Symptoms (CD-PRO/SS) Diary. (DOCX 117 kb)
Pentaquarks in semileptonic $Λ_b$ decays
Creators: name: Zhou, Ping
name: Hsiao, Y. K.
name: Geng, C. Q.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: In terms of ${\cal P}_{c1,c2}={\cal P}_c(4380,4450)^+$ as the hidden charm pentaquark states to consist of $c\bar c uud$, we study the semileptonic $Λ_b\to ({\cal P}_{c1,c2}\to)J/ψp \ell^-\bar ν_\ell$ decays. In our discussion, while the main contribution to $Λ_b\to K^-J/ψp$ is from the non-perturbative process via the doubly charmful $b\to c\bar cs$ transition, we propose that the $Λ_b\to {\cal P}_{c1,c2}\to J/ψp$ transitions are partly contribute to the $Λ_b\to K^-({\cal P}_{c1,c2}\to)J/ψp$ decays, in which the required $c\bar c$ pair is formed by the sea quarks, intrinsic charm, or both. We predict that ${\cal B}(Λ_b\to J/ψp \ell^-\bar ν_\ell)=(2.04^{+4.82}_{-1.57},1.75^{+4.14}_{-1.35})\times 10^{-6}$ for $\ell=(e,μ)$, which are about two orders of magnitude smaller than the observed decay of $Λ_b\to pμ\bar ν_μ$. We also explore the angular correlations for the $J/ψp$ and $\ell^-\bar ν_\ell$ pairs. Our results of the decay branching ratios and angular asymmetries in $Λ_b\to J/ψp \ell^-\bar ν_\ell$, accessible to the ongoing experiments at the LHCb, can be used to improve the understanding of the hidden charm pentaquark states.
description: 11 pages, 3 figures, accepted by Annals of Physics
title: ADCO, Cartulaire de Cîteaux pour la grange et seigneurie d'Ouges (XVe siècle), Cart. 173 (11 H 939), 226 folios, f. 0159
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Cîteaux pour la grange et seigneurie d'Ouges (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 173 (11 H 939), 226 folios, f. 0159, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour la grange et seigneurie d'Ouges (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 173 (11 H 939), 226 folios, f. 0159, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Stability of phantom wormholes
Creators: name: Lobo, Francisco S. N.
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: It has recently been shown that traversable wormholes may be supported by phantom energy. In this work phantom wormhole geometries are modelled by matching an interior traversable wormhole solution, governed by the equation of state $p=ωρ$ with $ω
description: 9 pages, 9 figures, Revtex4. V2: five references added
Squeezing of electromagnetic field in a cavity by electrons in Trojan states
Creators: name: Kochanski, Piotr
name: Bialynicka-Birula, Zofia
name: Bialynicki-Birula, Iwo
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The notion of the Trojan state of a Rydberg electron, introduced by I.Bialynicki-Birula, M.Kaliński, and J.H.Eberly (Phys. Rev. Lett. 73, 1777 (1994)) is extended to the case of the electromagnetic field quantized in acavity. The shape of the electronic wave packet describing the Trojan state is practically the same as in the previously studied externally driven system. The fluctuations of the quantized electromagnetic field around its classical value exhibit strong squeezing. The emergence of Trojan states in the cylindrically symmetrical system is attributed to spontaneous symmetry braking.
description: 9 pages, 8 figures
Additional file 1: of Relationship between occlusal force and falls among community-dwelling elderly in Japan: a cross-sectional correlative study
Creators: name: Eto, Maki
name: Miyauchi, Shinji
Publisher: name: figshare
Year: 2018
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Physical assessment data sheet. (DOCX 17Â kb)
From the self-force problem to the Radiation reaction formula
Creators: name: Mino, Yasushi
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We review a recent theoretical progress in the so-called self-force problem of a general relativistic two-body system. Although a two-body system in Newtonian gravity is a very simple problem, some fundamental issues are involved in relativistic gravity. Besides, because of recent projects for gravitational wave detection, it comes to be possible to see those phenomena directly via gravitational waves, and the self-force problem becomes one of urgent and highly-motivated problems in general relativity. Roughly speaking, there are two approaches to investigate this problem; the so-called post-Newtonian approximation, and a black hole perturbation. In this paper, we review a theoretical progress in the self-force problem using a black hole perturbation. Although the self-force problem seems to be just a problem to calculate a self-force, we discuss that the real problem is to define a gauge invariant concept of a motion in a gauge dependent metric perturbation.
description: a special issue for Classical and Quantum Gravity, a review article of Capra Ranch Meetings
Contemporaneous Imaging Comparisons of the Spotted Giant $σ$ Geminorum Using Interferometric, Spectroscopic, and Photometric Data
Creators: name: Roettenbacher, Rachael M.
name: Monnier, John D.
name: Korhonen, Heidi
name: Harmon, Robert O.
name: Baron, Fabien
name: Hackman, Thomas
name: Henry, Gregory W.
name: Schaefer, Gail H.
name: Strassmeier, Klaus G.
name: Weber, Michael
name: Brummelaar, Theo A. ten
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Nearby, active stars with relatively rapid rotation and large starspot structures offer the opportunity to compare interferometric, spectroscopic, and photometric imaging techniques. In this paper, we image a spotted star with three different methods for the first time. The giant primary star of the RS Canum Venaticorum binary $σ$ Geminorum ($σ$ Gem) was imaged for two epochs of interferometric, high-resolution spectroscopic, and photometric observations. The light curves from the reconstructions show good agreement with the observed light curves, supported by the longitudinally-consistent spot features on the different maps. However, there is strong disagreement in the spot latitudes across the methods.
description: Accepted to ApJ, 19 pages, 16 figures, 5 tables
Environmental Perceptions of College Students during the COVID-19 Pandemic
Creators: name: Kaylor, Sydney
name: Elshorbany, Yasin
name: Collins, Jennifer
name: Rives, Robin
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health
subject: Plant Biology

description: In this study, we investigate the environmental perception changes in college students during the COVID-19 pandemic. During the almost worldwide lockdown between March and December 2020, many students experienced dramatic changes in their socioeconomic life that have affected their well-being, ability to learn, and environmental perceptions. Students were sent home from college campuses, many businesses were shut down, and changes were seen in the environment throughout the world. In many places, lockdown policies lead to improved air, water, and land quality, mainly due to fewer vehicle and anthropogenic emissions. An online survey conducted on students enrolled in the University of South Florida and Florida State University demonstrates that most students have become more environmentally conscious after the COVID-19 lockdown, indicating significant perception changes. The students’ demographic backgrounds played a major role in affecting their perception changes. Furthermore, mass media was found to have affected the student’s perceptions, which demonstrates the important role media plays in directing public opinion, especially among college students and millennia. This study also highlights the environmental issues that underrepresented students face and calls for policies to address them on both educational and socioeconomic levels.
Inflationary potentials yielding constant scalar perturbation spectral indices
Creators: name: Vallinotto, Alberto
name: Copeland, Edmund J.
name: Kolb, Edward W.
name: Liddle, Andrew R.
name: Steer, Daniele A.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We explore the types of slow-roll inflationary potentials that result in scalar perturbations with a constant spectral index, i.e., perturbations that may be described by a single power-law spectrum over all observable scales. We devote particular attention to the type of potentials that result in the Harrison--Zel'dovich spectrum.
description: 8 pages, 3 figures. New general derivation method, structure changed