cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A wide-field photometric survey for extratidal tails around five metal-poor globular clusters in the Galactic halo
Creators: name: Chun, Sang-Hyun
name: Kim, Jae-Woo
name: Sohn, Sangmo T.
name: Park, Jang-Hyun
name: Han, Wonyong
name: Kim, Ho-Il
name: Lee, Young-Wook
name: Lee, Myung Gyoon
name: Lee, Sang-Gak
name: Sohn, Young-Jong
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Wide-field deep gri images obtained with the Megacam of the Canada-France-Hawaii Telescope (CFHT) are used to investigate the spatial configuration of stars around five metal-poor globular cluster M15, M30, M53, NGC 5053, and NGC 5466, in a field-of-view ~3 degree. Applying a mask filtering algorithm to the color-magnitude diagrams of the observed stars, we sorted cluster's member star candidates that are used to examine the characteristics of the spatial stellar distribution surrounding the target clusters. The smoothed surface density maps and the overlaid isodensity contours indicate that all of the five metal-poor globular clusters exhibit strong evidence of extratidal overdensity features over their tidal radii, in the form of extended tidal tails around the clusters. The orientations of the observed extratidal features show signatures of tidal tails tracing the clusters' orbits, inferred from their proper motions, and effects of dynamical interactions with the Galaxy. Our findings include detections of a tidal bridge-like feature and an envelope structure around the pair of globular clusters M53 and NGC 5053. The observed radial surface density profiles of target clusters have a deviation from theoretical King models, for which the profiles show a break at 0.5~0.7r_t, extending the overdensity features out to 1.5~2r_t. Both radial surface density profiles for different angular sections and azimuthal number density profiles confirm the overdensity features of tidal tails around the five metal-poor globular clusters. Our results add further observational evidence that the observed metal-poor halo globular clusters originate from an accreted satellite system, indicative of the merging scenario of the formation of the Galactic halo.
description: 69 pages, 21 figures, accepted for publication in the Astronomical Journal
A Comparison of Goal-Oriented Guided Mental Imagery versus Goal Setting Interventions for Increasing Physical Activity Levels in Young, Inactive Adults with Overweight or Obesity: A Pilot Randomised Controlled Trial
Creators: name: Anandam, Tharushini
Publisher: name: Swinburne
Year: 2025

description: The research examines the effectiveness of goal-oriented guided imagery in increasing physical activity levels among inactive adults with overweight or obesity. A six-week exercise program compared the impacts of guided imagery and SMART goal-setting on exercise adherence, motivation, enjoyment, and muscular endurance. Results showed that goal oriented guided imagery improved adherence to resistance training, motivation, and enjoyment, with higher use of motivational and cognitive imagery. These findings suggest that goal-oriented guided imagery may be a effectivie strategy to enhance physical activity participation, potentially promoting healthier lifestyles in individuals with overweight or obesity.
Improving tactical and strategic cave-pit interaction subsidence forecasting through performance monitoring
Creators: name: Lalang, Marthen Pitherson Cahyadi
Publisher: name: University of British Columbia
Year: 2024

description: The Grasberg Block Cave (GBC) mine represents a transition from open-pit to underground mining to extract deeper resources. However, this transition requires the management of caving-induced surface subsidence and interactions between the cave and overlying open pit that could impact critical infrastructure located on surface in proximity to the open pit. Forecasting when and how these impacts will occur is currently carried out using advanced 3-D numerical modeling. However, this can be challenging, given the potential for uncertainty to cause predictions to not align with subsequent ground responses. To overcome this challenge, performance monitoring must be integrated with numerical models to track and validate forecasts and manage geological, parameter, and model uncertainties. This thesis develops a spatial and temporal framework to analyze subsidence caused by cave-pit interactions. Spatially, this uses LIDAR, which was highly effective at capturing the boundary of the fracture zone that develops during progressive cave breakthrough. Cross-correlation between monitoring data and numerical modeling helps to provide additional detection and insights into emerging slope deformation mechanisms developing in response to block caving. Temporally, adaptive learning provided an excellent tool for capturing the survivability of an area of interest before it collapses, and inverse velocity shows robust agreement in validating the results. In conclusion, this study highlights the importance of performance monitoring to bridge the gap between the value that numerical modeling forecasts can provide and the need to manage uncertainty and risk to protect critical mine infrastructure and assets. While numerical modeling is helpful for long-term strategic projections, the results presented in this thesis demonstrate that empirical trends based on monitoring data offer flexible supplementary prediction updates for short-term and intermittent periods.
Spectral signatures of critical charge and spin fluctuations in cuprates
Creators: name: Grilli, M.
name: Caprara, S.
name: Di Castro, C.
name: Enss, T.
name: Hackl, R.
name: Muschler, B.
name: Prestel, W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We discuss how Raman spectra of high temperature superconducting cuprates are affected by nearly-critical spin and charge collective modes, which are coupled to charge carriers near a stripe quantum critical point. We find that specific fingerprints of nearly-critical collective modes can be observed and that the selectivity of Raman spectroscopy in momentum space may be exploited to distinguish the spin and charge contribution. We apply our results to discuss the spectra of high-T_c superconducting cuprates finding that the collective modes should have masses with substantial temperature dependence in agreement with their nearly critical character. Moreover spin modes have larger masses and are more diffusive than charge modes indicating that in stripes the charge is nearly ordered, while spin modes are strongly overdamped and fluctuating with high frequency.
description: 6 pages and 3 figures, invited paper to the conference SCES 08, Buzios/Rio, Brazil
Coulomb gauge confinement in the heavy quark limit
Creators: name: Popovici, C.
name: Watson, P.
name: Reinhardt, H.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The relationship between the nonperturbative Green's functions of Yang-Mills theory and the confinement potential is investigated. By rewriting the generating functional of quantum chromodynamics in terms of a heavy quark mass expansion in Coulomb gauge, restricting to leading order in this expansion and considering only the two-point functions of the Yang-Mills sector, the rainbow-ladder approximation to the gap and Bethe-Salpeter equations is shown to be exact in this case and an analytic, nonperturbative solution is presented. It is found that there is a direct connection between the string tension and the temporal gluon propagator. Further, it is shown that for the 4-point quark correlation functions, only confined bound states of color-singlet quark-antiquark (meson) and quark-quark (baryon) pairs exist.
description: 22 pages, 6 figures
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title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ±Ð»Ð°Ð¼ÑÐºÐ°Ñ, ÐÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¼Ð°ÑÐ³Ð°Ð½ÑÐµÐ²Ð°Ñ ÑÐ½ÑÐµÑÐ°Ð»Ð¾Ð¿Ð°ÑÐ¸Ñ
Ð½ÐµÐ¹ÑÐ¾Ð²Ð¾ÑÐ¿Ð°Ð»ÐµÐ½Ð¸Ðµ
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description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ð¹ Ð¸Ð½ÑÐ¾ÐºÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸ÑÐ¼Ð¸ Ð¼Ð°ÑÐ³Ð°Ð½ÑÐ° Ð¿ÑÐ¸ Ð¸Ñ Ð¿Ð¾Ð¿Ð°Ð´Ð°Ð½Ð¸Ð¸ Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¼ Ð² ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ðµ, Ð¿ÑÐµÐ²ÑÑÐ°ÑÑÐµÐ¼ Ð´Ð¾Ð¿ÑÑÑÐ¸Ð¼ÑÑ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ñ. Ð¦ÐµÐ»Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð¾ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·Ð¾Ð²Ð°ÑÑ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ñ ÑÑÐ¾Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸Ð½ÑÐ¾ÐºÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÐºÑÑÑ ÑÐ»Ð¾ÑÐ¸Ð´Ð¾Ð¼ Ð¼Ð°ÑÐ³Ð°Ð½ÑÐ° Ð¿ÑÐ¸ Ð¸Ð½ÑÑÐ°Ð½Ð°Ð·Ð°Ð»ÑÐ½Ð¾Ð¼ ÑÐ¿Ð¾ÑÐ¾Ð±Ðµ ÐµÐ³Ð¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ. ÐÐºÐ°Ð·Ð°Ð»Ð¾ÑÑ, ÑÑÐ¾ Ð¸Ð½ÑÑÐ°Ð½Ð°Ð·Ð°Ð»ÑÐ½Ð¾Ðµ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ ÑÐ»Ð¾ÑÐ¸Ð´Ð° Ð¼Ð°ÑÐ³Ð°Ð½ÑÐ° Ð² ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ð¸ 50 Ð¼Ð³/Ð¼Ð» Ð½Ð° Ð¿ÑÐ¾ÑÑÐ¶ÐµÐ½Ð¸Ð¸ 90 Ð´Ð½ÐµÐ¹ Ð²ÑÐ·ÑÐ²Ð°ÐµÑ Ñ ÐºÑÑÑ: ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÑÑ ÑÐµÐ»Ð°; Ð½Ð°ÑÑÑÐµÐ½Ð¸Ðµ Ð¿Ð¾ÑÐ¾Ð´ÐºÐ¸ Ð¸ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸; Ð½Ð°ÐºÐ¾Ð¿Ð»ÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐ³Ð°Ð½ÑÐ° Ð² Ð¦ÐÐ¡, Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ Ð² ÑÑÑÐ¸Ð°ÑÑÐ¼Ðµ; ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÑÑÐ¾Ð²Ð½Ñ Ð´Ð¾ÑÐ°Ð¼Ð¸Ð½Ð° Ð² ÑÑÑÐ¸Ð°ÑÑÐ¼Ðµ; ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð½ÐµÐ¹ÑÐ¾Ð²Ð¾ÑÐ¿Ð°Ð»ÐµÐ½Ð¸Ñ Ð¸ Ð½ÐµÐ¹ÑÐ¾Ð´ÐµÐ³ÐµÐ½ÐµÑÐ°ÑÐ¸Ð¸ Ð² ÑÑÑÐ¸Ð°ÑÑÐ¼Ðµ Ð¸ Ð³Ð¸Ð¿Ð¿Ð¾ÐºÐ°Ð¼Ð¿Ðµ; Ð½Ð°ÑÑÑÐµÐ½Ð¸Ðµ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼ÐµÑÐ°Ð±Ð¾Ð»Ð¸Ð·Ð¼Ð°; ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð²Ð¾ÑÐ¿Ð°Ð»ÐµÐ½Ð¸Ñ Ð½Ð° Ð¿ÐµÑÐ¸ÑÐµÑÐ¸Ð¸. Ð¢Ð°ÐºÐ¸Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼, Ð¸Ð½ÑÑÐ°Ð½Ð°Ð·Ð°Ð»ÑÐ½Ð¾Ðµ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ ÑÐ»Ð¾ÑÐ¸Ð´Ð° Ð¼Ð°ÑÐ³Ð°Ð½ÑÐ° Ð² Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð¹ Ð´Ð¾Ð·Ðµ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸Ñ Ðº ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¸Ð¿Ð¸ÑÐ½ÑÑ Ð¿ÑÐ¾ÑÐ²Ð»ÐµÐ½Ð¸Ð¹ Ð¼Ð°ÑÐ³Ð°Ð½ÑÐµÐ²Ð¾Ð¹ ÑÐ½ÑÐµÑÐ°Ð»Ð¾Ð¿Ð°ÑÐ¸Ð¸ Ñ ÐºÑÑÑ Ð¸ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð´Ð»Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ Ð¿Ð°ÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸.
Exploring Home Rule Authority: An Assessment of the Impetuses Behind Broad Grants of Local Power
Creators: name: Lloyd, Katherine J.
Publisher: name: IUPUI University Library
Year: 2010
Subjects: subject: home rule
subject: Municipal home rule
subject: Home rule

description: Indiana University-Purdue University Indianapolis (IUPUI)
description: This study is a comparative examination of factors related to a state’s likelihood of granting its local governments broad home rule authority or broad local governing discretion. Six factors are assessed: percentage of a state’s residents living in urban areas, state’s heterogeneity, per capita income, region, age of state, and dominant political culture. Binary, logistic regression analysis is used to determine logistic odds of a state’s granting structural and broad functional home rule authority given the posited factors. Results showed no significant relationships between variables.
The Redshift Search Receiver Observations of 12CO J=1-->0 in 29 Ultraluminous Infrared Galaxies
Creators: name: Chung, Aeree
name: Narayanan, Gopal
name: Yun, Min S.
name: Heyer, Mark
name: Erickson, Neal R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present 12CO J=1-->0 observations of ultraluminous infrared galaxies (ULIRGs) obtained using the Redshift Search Receiver (RSR) on the 14-m telescope of the Five College Radio Astronomy Observatory. The RSR is a novel, dual-beam, dual-polarization receiver equipped with an ultra-wideband spectrometer backend that is being built as a facility receiver for the Large Millimeter Telescope. Our sample consists of 29 ULIRGs in the redshift range of 0.04-0.11, including 10 objects with no prior 12CO measurements. We have detected 27 systems (a detection rate of 93%), including 9 ULIRGs that are detected in CO for the first time. Our study has increased the number of local ULIRGs with CO measurements by ~15%. The CO line luminosity L'_CO, correlates well with far-infrared luminosity L_FIR, following the general trend of other local ULIRGs. However, compared to previous surveys we probe deeper into the low CO luminosity end of ULIRG population as a single study by including a number of CO faint objects in the sample. As a result, we find 1) a smoother transition between the ULIRG population and local QSOs in L_FIR-L'_CO ("star formation efficiency") space, and 2) a broader range of L_FIR/L'_CO flux ratio (~60--1000 L_sun/[K km/s/pc^2]) than previously reported. In our new survey, we also have found a small number of ULIRGs with extreme L_FIR/L'_CO which had been known to be rare. The mid-IR color and radio-excess of 56 local ULIRGs as a function of FIR-to-CO flux ratio is examined and compared with those of spirals/starburst galaxies and low-z QSOs. In this paper, using a large sample of local ULIRGs we explore the origin of their current power source and potential evolution to QSOs.
description: 16 pages, 12 figures; accepted for publication in the Astronomical Journal
Higher order QED in high mass e+ e- pairs production at RHIC
Creators: name: Baltz, Anthony J.
name: Nystrand, Joakim
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Lowest order and higher order QED calculations have been carried out for the RHIC high mass e+ e- pairs observed by PHENIX with single ZDC triggers. The lowest order QED results for the experimental acceptance are about two standard deviations larger than the PHENIX data. Corresponding higher order QED calculations are within one standard deviation of the data.
description: 2 pages
Using Surrogate Models to Speed up the Creation of Aerodynamic Databases in CEASIOMpy
Creators: name: Jungo, Aidan
name: Riolo, Vivien
name: Vos, Jan
Publisher: name: Zenodo
Year: 2020
Subjects: EWADE2020
CEASIOM
aerodynamics

description: CEASIOMpy is an open source conceptual aircraft design environment. CEASIOMpy can be used to set up complex design and optimization workflows, both for conventional and unconventional configurations. CEASIOMpy provides tools for various disciplines in aircraft design, amongst others: Geometry and meshes, weight and balance, aerodynamics, structures, mission analysis, stability analysis. CEASIOMpy uses the open-standard format CPACS. Workflows can be set up with the open-source environment RCE. Both CPACS and RCE are actively developed by the German Aerospace Center DLR. Follow the links below to learn how get started or how to contribute to the project. CEASIOMpy uses surrogate models to speed up the creation of aerodynamic databases.
description: http://EWADE.AircraftDesign.org --- http://Presentations2020.AircraftDesign.org
title: ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ°ÑÑÐ½Ð¾Ðµ Ð¿Ð°ÑÑÐ½ÐµÑÑÑÐ²Ð¾ ÐºÐ°Ðº Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð° Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸ Ð¡ÐµÐ²ÐµÑÐ½Ð°Ñ ÐÑÐµÑÐ¸Ñ-ÐÐ»Ð°Ð½Ð¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Â«ÐÐ£Ð ÐÐÐ£ÐÂ»)
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ°Ð½Ð¸ÐµÐ²Ð°, ÐÐ¸Ð°Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½Ð¾Ðµ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð¾
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ¥ Ð Ð¡Ð-ÐÐ»Ð°Ð½Ð¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Â«ÐÐ£Ð ÐÐÐ£ÐÂ». Ð¦ÐµÐ»ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÐÐÐ¥ Ð Ð¡Ð-ÐÐ»Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ°ÑÑÐ½Ð¾Ð³Ð¾ Ð¿Ð°ÑÑÐ½ÐµÑÑÑÐ²Ð°. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¾ÑÑÐ°ÑÐ»Ð¸ ÐÐÐ¥ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸ Ð¡ÐµÐ²ÐµÑÐ½Ð°Ñ ÐÑÐµÑÐ¸Ñ-ÐÐ»Ð°Ð½Ð¸Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐÐÐ¥ Ð² Ð Ð¡Ð-ÐÐ»Ð°Ð½Ð¸Ñ. Ð Ð¸ÑÐ¾Ð³Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÑÐ´ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÐµÑÐ¾Ð¹ ÐÐÐ¥ Ð¿ÑÑÐµÐ¼ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð½Ð° Ð±Ð°Ð·Ðµ ÐÐ¸Ð½Ð¸ÑÑÐµÑÑÑÐ²Ð° ÐÐÐ¥, ÑÐ¾Ð¿Ð»Ð¸Ð²Ð° Ð¸ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð Ð¡Ð-Ð ÐÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¡Ð¾Ð²ÐµÑÐ° Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ°ÑÑÐ½Ð¾Ð³Ð¾ Ð¿Ð°ÑÑÐ½ÐµÑÑÑÐ²Ð° Ð² ÐÐÐ¥ ÑÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸, ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¤Ð¾Ð½Ð´Ð° Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐÐÐ¥ Ð Ð¡Ð-Ð, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÐÐ§Ð.
Continuous self-similar evaporation of a rotating cosmic string loop
Creators: name: Anderson, Malcolm
Publisher: name: arXiv
Year: 2008
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: A solution of the linearized Einstein and Nambu-Goto equations is constructed which describes the evaporation of a certain type of rotating cosmic string - the Allen-Casper-Ottewill loop - under the action of its own self-gravity. The solution evaporates self-similarly, and radiates away all its mass-energy and momentum in a finite time. Furthermore, the corresponding weak-field metric can be matched to a remnant Minkowski spacetime at all points on the future light cone of the final evaporation point of the loop.
description: 80 pages, 13 figures. Accepted for publication in Classical and Quantum Gravity
12nm Finfet aging characterization through wear-out sensor design
Creators: name: Rendon, Mateo Jose
Publisher: name: University of British Columbia
Year: 2024

description: Reliability in electronics is becoming increasingly crucial as semiconductor markets diversify, economic and policy trends point to sustainability, and transistors scale into more aging-sensitive devices. This thesis studies the wear-out mechanisms at the center of device aging and failure in advanced technology nodes by creating a testing platform for characterization across several circuit design variables. We start with the physical explanations and device effects of bias temperature instability (BTI), hot-carrier injection (HCI), electromigration (EM), and time dependent dielectric breakdown (TDDB). Then, a survey on state-of-the-art wear-out mitigation techniques reveals that developing aging mechanisms sensors aids academia and industry alike by serving as tools for model characterization and monitors for dynamic on-silicon aging relief. Therefore, the core of this thesis presents four wear-out sensor designs by recollecting learnings from similar literature approaches, detailing their circuit topologies, and discussing the specifics of their implementation in a 12nmLP FinFET technology. The experimental methodology includes the tapeout of a test platform chip featuring over 150 sensor variants to verify the topologies. Additionally, we introduce a firmware-based dual PCB solution capable of automatically measuring the sensor outputs while replicating accelerated aging testing industry standards. After presenting initial measurements, we perform a 1000-hour 125°C stress test to estimate the test platform’s 10-year aging. The first 600-hour experimental results verify the developed sensors and provide insights on how transistor type, size, threshold voltage, and power supply impact BTI, HCI, EM, and soft and hard-breakdown TDDB in the 12nm FinFET technology.
A General Formula for Black Hole Gravitational Wave Kicks
Creators: name: van Meter, James R.
name: Miller, M. Coleman
name: Baker, John G.
name: Boggs, William D.
name: Kelly, Bernard J.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Although the gravitational wave kick velocity in the orbital plane of coalescing black holes has been understood for some time, apparently conflicting formulae have been proposed for the dominant out-of-plane kick, each a good fit to different data sets. This is important to resolve because it is only the out-of-plane kicks that can reach more than 500 km/s and can thus eject merged remnants from galaxies. Using a different ansatz for the out-of-plane kick, we show that we can fit almost all existing data to better than 5 %. This is good enough for any astrophysical calculation, and shows that the previous apparent conflict was only because the two data sets explored different aspects of the kick parameter space.
description: 14 pages.
title: ÐÐ»Ð¸ÑÐ½Ð¸Ðµ Fintech-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð½Ð° Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ·Ð½ÐµÑÐ¾Ð², ÐÐ½ÑÐ¾Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ð¹ Ð±Ð°Ð½Ðº
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ Ð±Ð°Ð½ÐºÐ¾Ð² Ð¿Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ñ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½Ð¾Ð²ÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð², ÑÑÐ»ÑÐ³ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹. Ð¦ÐµÐ»Ñ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð² Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð½Ð¾Ð²ÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð½Ð° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ Ð±Ð°Ð½ÐºÐ¾Ð². Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð½Ð¾Ð²ÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑÑÑ Ð² Ð´Ð²ÑÑ Ð²ÐµÐºÑÐ¾ÑÐ°Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ: ÐºÐ°Ðº ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ, ÑÐµÐ¼ ÑÐ°Ð¼ÑÐ¼ Ð¾Ð½Ð¸ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑ ÐºÐ¾Ð½ÐºÑÑÐ¸ÑÑÑÑÐµÐµ Ð·Ð²ÐµÐ½Ð¾ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ Ð±Ð°Ð½ÐºÐ°Ð¼; Ð¸ ÐºÐ°Ðº ÐºÐ°ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¾ÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÐ¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹, ÑÐµÐ¼ ÑÐ°Ð¼ÑÐ¼, Ð½Ð¾Ð²ÑÐµ ÑÐ¸Â¬Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð²Ð½ÐµÐ´ÑÑÑÑÑÑ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÑÐ¾Ð²ÐµÐ´ÑÐ½Ð½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð»Ð¾, ÑÑÐ¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð±Ð°Ð½ÐºÐ¸ ÑÑÑÐµÐ¼ÑÑÑÑ Ðº ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ñ Ñ FinTech-Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸ Ð´Ð»Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¼Ð¾Ð´ÐµÐ»Ð¸, Ð´ÐµÐ»Ð°Ñ ÐµÑ Ð±Ð¾Ð»ÐµÐµ Ð³Ð¸Ð±ÐºÐ¾Ð¹ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð² ÑÐ»Ð¾Ð¶Ð¸Ð²ÑÐµÐ¹ÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸. Ð¢Ð°ÐºÐ¸Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼, Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð¹ Ð¾Ð¿ÑÑ Ð¿Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð²Ð½Ð¸Ð¼Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¸Ð½Ð´ÑÑÑÑÐ¸Ð¸ Ð±Ð°Ð½ÐºÐ°Ð¼Ð¸. Ð Ð´ÑÑÐ³Ð¾Ð¼ ÑÐ»ÑÑÐ°Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ, ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ðµ Ð½Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¼ ÑÑÐ½ÐºÐµ, Ð¼Ð¾Ð³ÑÑ Ð´Ð¾ÑÑÐ¸ÑÑ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ Ð¸ ÑÑÐµÑÐ½Ð¸ÑÑ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð±Ð°Ð½ÐºÐ¸, Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÑÑ ÐºÐ»Ð¸ÐµÐ½ÑÐ°Ð¼ Ð±Ð¾Ð»ÐµÐµ ÑÐ´Ð¾Ð±Ð½ÑÐµ Ð¸ Ð±ÑÑÑÑÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÑ Ð¸ ÑÑÐ»ÑÐ³Ð¸.
P.Oxy. LVI 3825. Homer, Iliad 1. 61-86, 98-120, 204?, 229-52
Creators: name: Oxyrhynchus Papyri
Publisher: name: University of Oxford
Year: 2022
Subjects: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
Semileptonic decays of the standard Higgs boson
Creators: name: Dobrescu, Bogdan A.
name: Lykken, Joseph D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The Higgs boson decay into a pair of real or virtual W bosons, with one of them decaying leptonically, is predicted within the Standard Model to have the largest branching fraction of all Higgs decays that involve an isolated electron or muon, for M_h > 120 GeV. We compute analytically the fully-differential width for this h -> l νjj decay at tree level, and then explore some multi-dimensional cuts that preserve the region of large signal. Future searches for semileptonic decays at the Tevatron and LHC, employing fully-differential information as outlined here, may be essential for ruling out or in the Higgs boson and for characterizing a Higgs signal.
description: 17 pages, 5 .eps figures
Recent results on two-photon physics at BABAR
Creators: name: Druzhinin, V. P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present measurements of the gamma gamma* --> pi0 transition form factor for the momentum transfer range Q^2=4-40 GeV^2 and the gamma gamma* --> eta_c transition form factor for the range Q^2=2-50 GeV^2. The results of the measurement of the eta_c mass, total and two-photon widths are also presented.
description: 6 pages, 6 figures; added two references. To appear in the proceedings of the 2009 Europhysics Conference on High Energy Physics, July 16-22, 2009, Krakow, Poland
title: ÐÐ½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¹ Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°: ÑÑÑÑÐ¾ÑÑÑÐ²Ð¾ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð½ÐµÑÐ¾ÑÐ¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ
title: University internalization tools: tutoring and non-formal education programs
Creators: name: ÐÑÐ°ÑÐ½Ð¾ÑÐµÐºÐ¾Ð², ÐÐ¸ÐºÑÐ¾Ñ
name: "ÐÐ½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐµ ÑÑÑÐ´ÐµÐ½ÑÑ Ð² Ð²ÑÐ·Ð°Ñ  Ð Ð¤: ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ, Ð¿ÑÐ¸ÐµÐ¼Ð° Ð¸ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸", Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ (2021; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
ÑÑÑÑÐ¾ÑÑ
Ð½Ð°Ð´Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð½Ð°Ð²ÑÐºÐ¸
Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ ÑÑÑÐ´ÐµÐ½ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÑ
Ð½ÐµÑÐ¾ÑÐ¼Ð°Ð»ÑÐ½Ð¾Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ

description: ÐÐ²ÑÐ¾Ñ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑ Ð¿ÑÐ¾ÑÐµÑÑ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¹ Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°. ÐÐ²ÑÐ¾Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÑ ÑÑÑÑÐ¾ÑÑÐºÐ¾Ðµ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÐºÐ°Ðº Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÐºÐ¸Ñ Ð½Ð°Ð´Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð½Ð°Ð²ÑÐºÐ¾Ð², ÐºÐ°Ðº Ð»Ð¸Ð´ÐµÑÑÑÐ²Ð¾ Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ðº Ð¼ÐµÐ¶ÐºÑÐ»ÑÑÑÑÐ½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸. ÐÑÑÐ³Ð¸Ð¼ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð¼ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð½Ð°Ð´Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð½Ð°Ð²ÑÐºÐ¾Ð² ÑÐ²Ð»ÑÑÑÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ ÑÑÑÐ´ÐµÐ½ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÑ, Ð¿ÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¸Ð½ÑÐµÐ³ÑÐ°ÑÐ¸Ð¸ ÑÐ¾ÑÐ¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð½ÐµÑÐ¾ÑÐ¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ.
description: The author examines the process of internal internationalization of the university. The author analyzes the tutor movement as a mechanism for
the formation of such soft skills as leadership and the ability for intercultural
communication. Another mechanism for the development of soft skills is
international student projects, in the implementation of which the possibilities of integrating formal and non-formal education are used.
Direct measurement of the nonconservative force field generated by optical tweezers
Creators: name: Wu, Pinyu
name: Huang, Rongxin
name: Tischer, Christian
name: Jonas, Alexandr
name: Florin, Ernst-Ludwig
Publisher: name: arXiv
Year: 2009
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The force field of optical tweezers is commonly assumed to be conservative, neglecting the complex action of the scattering force. Using a novel method that extracts local forces from trajectories of an optically trapped particle, we measure the three dimensional force field experienced by a Rayleigh particle with 10 nm spatial resolution and femtonewton precision in force. We find that the force field is nonconservative with the nonconservative component increasing radially away from the optical axis, in agreement with the Gaussian beam model of the optical trap. Together with thermal position fluctuations of the trapped particle, the presence of the nonconservative force can cause a complex flux of energy into the optical trap depending on the experimental conditions.
Quantum Non-Magnetic state near Metal-Insulator Transition - a Possible Candidate of Spin Liquid State
Creators: name: Sun, Gao-Yong
name: Kou, Su-Peng
Publisher: name: arXiv
Year: 2008
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: In this paper, based on the formulation of an O(3) non-linear sigma model, we study the two-dimensional Pi-flux Hubbard model at half-filling. A quantum non-magnetic insulator is explored near the metal-insulator transition that may be a possible candidate of the spin liquid state. Such quantum non-magnetic insulator on square lattice is not induced by frustrations. Instead, it originates from quantum spin fluctuations with relatively small effective spin moments. In the strong-coupling limit, our results of the spin velocity and spin order parameter agree with results obtained from earlier calculations.
description: 6 pages, 6 figures, Version of publication in EPL, removing the contents of honeycomb lattice and adding some contents of square lattice
P.Oxy. LVI 3826. Homer, Iliad 4. 517-22, 5. 1-4, 31-45, 62-75
Creators: name: Oxyrhynchus Papyri
Publisher: name: University of Oxford
Year: 2022
Subjects: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
title: ÐÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ð¸ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÐºÐ° Ð²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¢Ð¾Ð½ÐºÐ¾Ð½Ð¾Ð³Ð¾Ð², ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2015
Subjects: ÐÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ð¸ Ð²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸, ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸, Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÐºÐ° Ð²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ. ÐÑÐ½Ð¾Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð² Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð´ÑÐ³Ð¾Ð³Ð°ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¼ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°Ð¼ Ð¸ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð½ÑÐ¼ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð°Ð¼ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÐºÐ° Ð²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¾ÑÐºÑÑÑÑÑ Ð¸ Ð·Ð°ÐºÑÑÑÑÑ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÑÑÑÐ¾Ð¹ÑÑÐ² Ð¸ ÑÐ»ÐµÐ³Ð°Ð·Ð¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÑ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÑÑÑÐ¾Ð¹ÑÑÐ², ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°Ð¼ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹, Ð¼ÐµÑÐ¾Ð´Ð°Ð¼ Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¸Ñ Ð¾ÑÐºÐ»ÑÑÐ°ÑÑÐµÐ¹ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸. Ð Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸ÑÑ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÐºÑÑÑÐ¾Ð²ÑÑ ÑÐ°Ð±Ð¾Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑÂ» Ð¿Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² 140400.62 Â«Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ° Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Â» Ð¸ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ¾Ð²Â» Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 140400.68 Â«Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ° Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Â». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ñ, Ð·Ð°Ð½ÑÑÐ¾Ð¼Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼Ð¸, ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸ÐµÐ¹ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÐºÐ° Ð²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
A Scoping Review of The Evidence on Pharmacological and Non-Pharmacological Interventions For Idiopathic Hypersomnia
Creators: name: Saini, Vishal
name: Saini, Shivani
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Medicine and Health Sciences

description: This scoping review aimed to thoroughly examine the current management methods for idiopathic hypersomnia (IH) to address gaps in understanding and treatment strategies. This study provides valuable insights for optimizing patient care and improving diagnostic approaches by analyzing existing research on pharmacological and non-pharmacological interventions for IH.
title: Ð¢ÐµÐ¾ÑÐ¸Ñ, ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð´Ð°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼
title: Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
titleType: Subtitle
Creators: name: ÐÑÐ½ÐºÐ¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐºÑÐµÐ½Ð¾Ð², ÐÐµÐ¾Ð½Ð¸Ð´
name: ÐÑÐ¾ÑÑÐ¾ÑÐ¾Ð²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2014
Subjects: ÐÐµÑÐ°Ð»Ð»Ð¾Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ° Ð´Ð°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼

description: ÐÑÐ°ÐºÑÐ¸ÐºÑÐ¼ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð¢ÐµÐ¾ÑÐ¸Ñ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð´Ð°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼Â» Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 150700.62 Â«ÐÐ°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ», Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«ÐÑÐ¾ÑÐµÑÑÑ Ð¸ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼Â», 151900.62.01 Â«ÐÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Â», ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÑÂ». Ð¦ÐµÐ»Ñ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼Ð° - Ð¿Ð¾Ð¼Ð¾ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¾Ð²Ð»Ð°Ð´ÐµÑÑ Ð½Ð°Ð²ÑÐºÐ°Ð¼Ð¸ Ð¸ Ð¿Ð¾Ð»ÑÑÐ¸ÑÑ Ð·Ð½Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð´Ð°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÐºÐ°Ðº ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ, ÑÐ°Ðº Ð¸ Ð½Ð°ÑÐºÐ¾ÐµÐ¼ÐºÐ¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, Ð¿Ð¾Ð»ÑÑÐ¸Ð²ÑÐ¸Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð² Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ: Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½Ð¾Ðµ Ð´ÐµÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ, ÑÑÐ°Ð¼Ð¿Ð¾Ð²ÐºÐ° ÑÐ»Ð°ÑÑÐ¸ÑÐ½ÑÐ¼Ð¸ ÑÑÐµÐ´Ð°Ð¼Ð¸ Ð¸ Ð´Ñ. Ð Ð°Ð±Ð¾ÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÑÑ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² Ð´Ð»Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ Ð´Ð°Ð½Ð½ÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÑÐµÑÑÐµÐ³Ð¾ Ð¸ ÑÐµÑÐ²ÐµÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ¾Ð² ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ð¸, Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ° Ð¡ÐÐ±ÐÐÐ£.
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title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð¸Ñ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ (ÐÐ° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "Ð¢Ð°Ð¹Ð½Ð°Ñ ÐºÐ¾Ð¼Ð½Ð°ÑÐ°")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÐµÑÐµÐ´ÑÐº, ÐÐ°ÑÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð·Ð°ÑÑÐ°Ñ
ÑÑÐµÑ ÑÐ°ÑÑ Ð¾Ð´Ð¾Ð²
Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ° Ð´Ð¾Ñ Ð¾Ð´Ð¾Ð²
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ

description: Ð Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¾Ð±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«Ð¢Ð°Ð¹Ð½Ð°Ñ ÐºÐ¾Ð¼Ð½Ð°ÑÐ°Â». Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÑÑÑÐºÑÑÑÑ Ð´Ð¾ÑÐ¾Ð´Ð¾Ð² Ð¸ ÑÐ°ÑÑÐ¾Ð´Ð¾Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÐ¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ Ð²ÑÐµÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð±ÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð½Ð° ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐ¾Ð´Ð¾Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ¸Ðµ ÑÐ¾ÑÑ Ð²ÑÑÑÑÐºÐ¸. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ Ð¼ÐµÑ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸, Ð° ÑÐ°Ðº Ð¶Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸.
Bose-Einstein Condensation of $^{88}$Sr Through Sympathetic Cooling with $^{87}$Sr
Creators: name: Mickelson, P. G.
name: de Escobar, Y. N. Martinez
name: Yan, M.
name: DeSalvo, B. J.
name: Killian, T. C.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We report Bose-Einstein condensation of $^{88}$Sr, which has a small, negative s-wave scattering length ($a_{88}=-2$\,$a_0$). We overcome the poor evaporative cooling characteristics of this isotope by sympathetic cooling with $^{87}$Sr atoms. $^{87}$Sr is effective in this role in spite of the fact that it is a fermion because of the large ground state degeneracy arising from a nuclear spin of $I=9/2$, which reduces the impact of Pauli blocking of collisions. We observe a limited number of atoms in the condensate ($N_{max}\approx 10^4$) that is consistent with the value of $a_{88}$ and the optical dipole trap parameters.
description: 4 pages, 4 figures
title: ÐÑÐ±Ð¾Ñ Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð² Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿ÑÐ°ÑÑÐµÐ¹ Ð² Ð°Ð²ÑÐ¾ÑÐµÑÐ²Ð¸Ñ ÐÐÐ Â«ÐÐµÐ»Ð¸Ð½Ð³ÐµÐ½ ÐÐ¾Ð´Ð¶Ð¸ÑÑÐ¸ÐºÑÂ»
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ·ÑÐ¼Ð¸Ð½Ð°, ÐÐ°ÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð°Ð²ÑÐ¾ÑÐµÑÐ²Ð¸ÑÑ
Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð·Ð°Ð¿ÑÐ°ÑÑÐ¸
Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð²ÑÐ±Ð¾Ñ Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð² Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿ÑÐ°ÑÑÐµÐ¹ Ð² Ð°Ð²ÑÐ¾ÑÐµÑÐ²Ð¸Ñ ÐÐÐ Â«ÐÐµÐ»Ð¸Ð½Ð³ÐµÐ½ÐÐ¾Ð´Ð¶Ð¸ÑÑÐ¸ÐºÑÂ». Ð ÑÐµÐ»ÑÑ Ð²ÑÐ±Ð¾ÑÐ° Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð² Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿ÑÐ°ÑÑÐµÐ¹ Ð² Ð°Ð²ÑÐ¾ÑÐµÑÐ²Ð¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾ Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð² Ðº Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ¿Ð¾ÑÐºÐ¸ Ð¿Ð¾ÑÑÐ°Ð²Ð¾Ðº. ÐÑÐ±ÑÐ°Ð½ Ð¼ÐµÑÐ¾Ð´ Ð´Ð»Ñ Ð²ÑÐ±Ð¾ÑÐ° Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð². ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¼ÐµÑÑÐ¾ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸ Ð²ÑÐ±Ð¾ÑÐ° Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð² Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ¿Ð¾ÑÐºÐ¸ Ð¿Ð¾ÑÑÐ°Ð²Ð¾Ðº Ð¸ ÑÑÑÐµÑÑÐ²ÑÑÑÑÑ ÑÑÑÑÐºÑÑÑÐ° ÐºÐ°Ð½Ð°Ð»Ð° ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ. ÐÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð° ÑÐµÐºÑÑÐ°Ñ Ð¿ÑÐ¾ÑÐµÐ´ÑÑÐ° Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð².
title: Ð®ÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð² ÐÐ¾Ð»Ð¸ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ð¼ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐµ
title: ÑÐ±Ð¾ÑÐ½Ð¸Ðº ÑÑÐ°ÑÐµÐ¹ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼, 11â13 Ð°Ð¿ÑÐµÐ»Ñ 2019 Ð³Ð¾Ð´Ð°
titleType: Subtitle
Creators: name: "Ð®ÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð² ÐÐ¾Ð»Ð¸ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ð¼ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐµ", Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ (2019; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐ¸Ðµ Ð¾Ð¿ÑÑ Ð²ÑÐ·Ð¾Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹
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Ð¿ÑÐ°Ð²Ð°. ÐÐ¾Ð»ÑÑÐ¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹, Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾-
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ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ Ð½Ð°ÑÑÐ½ÑÑ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð½Ðµ ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹.
Magnetic Fields in Paradigms of Planetary Nebulae and Related MHD Frontiers
Creators: name: Blackman, Eric G.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Many, if not all, post AGB stellar systems swiftly transition from a spherical to a powerful aspherical pre-planetary nebula (pPNE) outflow phase before waning into a PNe. The pPNe outflows require engine rotational energy and a mechanism to extract this energy into collimated outflows. Just radiation and rotation are insufficient but a symbiosis between rotation, differential rotation and large scale magnetic fields remains promising. Present observational evidence for magnetic fields in evolved stars is suggestive of dynamically important magnetic fields, but both theory and observation are rife with research opportunity. I discuss how magnetohydrodynamic outflows might arise in pPNe and PNe and distinguish different between approaches that address shaping vs. those that address both launch and shaping. Scenarios involving dynamos in single stars, binary driven dynamos, or accretion engines cannot be ruled out. One appealing paradigm involves accretion onto the primary post-AGB white dwarf core from a low mass companion whose decaying accretion supply rate owers first the pPNe and then the lower luminosity PNe. Determining observational signatures of different MHD engines is a work in progress. Accretion disk theory and large scale dynamos pose many of their own fundamental challenges, some of which I discuss in a broader context.
description: 10 pages, to appear in the proceedings of IAU Symposium 259: "Cosmic Magnetic Fields:from Planets, to Stars and Galaxies," edited by K.G. Strassmeier, A.G. Kosovichev, J. Beckmann
Association between long-range temporal correlations in functional MRI BOLD signal and the excitatory / inhibitory metabolites ratio
Creators: name: Sochan, Lydia
Publisher: name: University of British Columbia
Year: 2024

description: A 3T multimodal MRI study of healthy adults (n=19; 10 female; 21-54 years) was performed to investigate the potential link between brain activity complexity and excitatory/inhibitory balance. The study objective was to determine if the Hurst exponent (HE) – an estimate of the self-correlation and signal complexity of the blood-oxygen-level-dependent (BOLD) functional MRI (fMRI) signal – is correlated with the excitatory-inhibitory (E/I) ratio in the visual cortex during movie-watching and rest. Findings in this domain have implications for neurological and neuropsychiatric conditions with disrupted E/I balance, such as autism spectrum disorder, schizophrenia, and Alzheimer’s disease. From a methodological perspective, HE is also considerably easier to accurately measure than E/I ratio. If HE can serve as a proxy for E/I, it may serve as a useful clinical biomarker for E/I imbalance. Moreover, E/I has been proposed to serve as a control parameter for brain criticality, which HE is believed to be a measure of. Thus, understanding if HE and E/I are correlated would serve to clarify this relationship. The study collected movie-watching and rest data including functional magnetic resonance imaging (fMRI) – which was used to calculate HE – and magnetic resonance spectroscopy (MRS) – which was used to measure inhibitory and excitatory neurotransmitters – GABA and glutamate, respectively. HE was found to increase with movie compared to rest, while E/I did not change between conditions. HE and E/I were not correlated during either movie or rest. This thesis represents the first attempt to investigate this connection in vivo in humans. We conclude that, at 3T and with our particular methodologies, no association was found in this small sample.
Additional file 2 of Interaction study of Pasteurella multocida with culturable aerobic bacteria isolated from porcine respiratory tracts using coculture in conditioned media
Creators: name: Nonzee Hanchanachai
name: Pramote Chumnanpuen
name: E-Kobon, Teerasak
Publisher: name: figshare
Year: 2021
Subjects: subject: Microbiology
subject: FOS: Biological sciences

description: Additional file 2. Comparison with other published studies. Comparison of bacterial genera isolated from the porcine respiratory tract in other published studies compared to our study.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÑ Ð° Ð¿Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ñ ÐºÑÐ»Ð¸Ð½Ð°ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸Ð· Ð¾Ð²Ð¾ÑÐµÐ¹ Ð´Ð»Ñ ÑÐµÑÐ¸ ÐºÐ°ÑÐµ Ð² Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ²Ð´Ð¾ÐºÐ¸Ð¼Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ ÑÐµÑ
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