cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ. ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Â«Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÂ»
titleType: Subtitle
Creators: name: Ð¡ÐµÐ½Ð¸ÑÐµÐ½ÐºÐ¾Ð², Ð®ÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ ÑÐ±Ð¾ÑÐ½Ð¸Ðº ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹, Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ð¹, Ð¸ ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ² Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ ÑÑÐµÐ´, Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÑÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ ÑÑÐ»Ð¾Ð¶Ð½ÑÑÑÐ¸ÐµÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð´Ð»Ñ ÑÑÐµÐ±Ð½Ð¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÂ», ÑÐ¾ÑÑÐ¾ÑÑÐµÐ¹ Ð¸Ð· ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² Â«ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Â» Ð¸ Â«ÐÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»Ð¾Ð¶Ð½ÑÑ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Â» Ð¸ ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð½ÐµÐ¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½. ÐÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¾Ð±ÑÐµÐ´Ð¸Ð½ÐµÐ½Ñ Ð¿Ð¾Ð´ ÐµÐ´Ð¸Ð½ÑÐ¼ Ð½Ð°Ð·Ð²Ð°Ð½Ð¸ÐµÐ¼ Â«ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ. ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼Â». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Â«Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÂ». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Â«ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ°Â», Â«Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð°Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ Ð¸ Ð´Ð»Ñ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ¾Ð², Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ»Ð¾Ð¶Ð½ÑÑ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼. ÐÐ½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸, Ð² ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸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°.
The Cosmic Near Infrared Background II: Fluctuations
Creators: name: Fernandez, Elizabeth R.
name: Komatsu, Eiichiro
name: Iliev, Ilian T.
name: Shapiro, Paul R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The Near Infrared Background (NIRB) is one of a few methods that can be used to observe the redshifted light from early stars at a redshift of six and above. Fluctuations of the NIRB can provide information on the first structures, such as halos and their surrounding ionized regions in the IGM. We combine, for the first time, N-body simulations, radiative transfer code, and analytic calculations of luminosity of early structures to predict the angular power spectrum (C_l) of fluctuations in the NIRB. We study the effects of various assumptions about the stellar mass, the initial mass spectrum of stars, metallicity, the star formation efficiency (f_*), the escape fraction of ionizing photons (f_esc), and the star formation timescale (t_SF), on the amplitude as well as the shape of C_l. The power spectrum of NIRB fluctuations is maximized when f_* is the largest (as C_l ~ (f_*)^2) and f_esc is the smallest. A significant uncertainty in the predicted amplitude of C_l exists due to our lack of knowledge of t_SF of these galaxies, which is equivalent to our lack of knowledge of the mass-to-light ratio. We do not see a turnover in the NIRB angular power spectrum of the halo contribution and explain this as the effect of high levels of non-linear bias. This is partly due to our choice of the minimum mass of halos contributing to NIRB, and a smaller minimum mass, which has a smaller non-linear bias, may still exhibit a turn over. Therefore, both the amplitude and shape of the NIRB power spectrum provide important information regarding the nature of sources contributing to the cosmic reionization. The angular power spectrum of the IGM, in most cases, is much smaller than the halo angular power spectrum. In addition, low levels of the observed mean background intensity tend to rule out high values of f_* > 0.2.
description: 54 pages, 22 figures, Accepted for publication in ApJ. v2: Comments and references added, along with new figures and a section on fractional anisotropy
The sl(n)-WZNW Fusion Ring: a combinatorial construction and a realisation as quotient of quantum cohomology
Creators: name: Korff, Christian
name: Stroppel, Catharina
Publisher: name: arXiv
Year: 2009
Subjects: subject: Representation Theory (math.RT)
subject: Mathematical Physics (math-ph)
subject: Quantum Algebra (math.QA)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 17B37, 14N35, 17B67, 05E05, 82B23, 81U40

description: A simple, combinatorial construction of the sl(n)-WZNW fusion ring, also known as Verlinde algebra, is given. As a byproduct of the construction one obtains an isomorphism between the fusion ring and a particular quotient of the small quantum cohomology ring of the Grassmannian Gr(k,k+n). We explain how our approach naturally fits into known combinatorial descriptions of the quantum cohomology ring, by establishing what one could call a `Boson-Fermion-correspondence' between the two rings. We also present new recursion formulae for the structure constants of both rings, the fusion coefficients and the Gromov-Witten invariants.
description: 61 pages, 2 eps figures; revised version accepted for publication in Advances in Mathematics: some minor typos removed, rewording of the proof to Corollary 6.9 and figure in Example 8.3 changed
Additional file 6 of Constructing a seventeen-gene signature model for non-obstructive azoospermia based on integrated transcriptome analyses and WGCNA
Creators: name: Chen, Yinwei
name: Yuan, Penghui
name: Gu, Longjie
name: Bai, Jian
name: Ouyang, Song
name: Sun, Taotao
name: Liu, Kang
name: Wang, Zhao
name: Liu, Chang
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 6: Supplementary Table 5. GO enrichment analysis of common DEGs.
Irreversible thermodynamics of dark energy on entropy-corrected apparent horizon
Creators: name: Karami, K.
name: Jamil, Mubasher
name: Sahraei, N.
Publisher: name: arXiv
Year: 2010
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the irreversible (non-equilibrium) thermodynamics of FRW universe containing only dark energy. Using the modified entropy-area relation which is motivated from the loop quantum gravity, we calculate the entropy-corrected form of the apparent horizon of FRW universe.
description: 9 pages, to be published in Physica Scripta
The unified theory of chirped-pulse oscillators
Creators: name: Kalashnikov, Vladimir L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: A completely analytical theory of chirped-pulse oscillators is presented. The theory is based on an approximate integration of the generalized nonlinear complex Ginzburg-Landau equation. The obtained parametric space of a chirped-pulse oscillator allows easy tracing the characteristics of both solid-state and fiber oscillators operating in the positive dispersion regime.
description: 12 pages; 9 figures; Conference EOO/SPIE 2009, Prague, Czech Republic; the mathematical apparatus is presented in detail in http://info.tuwien.ac.at/kalashnikov/NCGLE1.html, http://info.tuwien.ac.at/kalashnikov/NCGLE2.html and http://info.tuwien.ac.at/kalashnikov/genNCGLE.html
Diffusive Nested Sampling
Creators: name: Brewer, Brendon J.
name: Pártay, Livia B.
name: Csányi, Gábor
Publisher: name: arXiv
Year: 2009
Subjects: subject: Computation (stat.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: We introduce a general Monte Carlo method based on Nested Sampling (NS), for sampling complex probability distributions and estimating the normalising constant. The method uses one or more particles, which explore a mixture of nested probability distributions, each successive distribution occupying ~e^-1 times the enclosed prior mass of the previous distribution. While NS technically requires independent generation of particles, Markov Chain Monte Carlo (MCMC) exploration fits naturally into this technique. We illustrate the new method on a test problem and find that it can achieve four times the accuracy of classic MCMC-based Nested Sampling, for the same computational effort; equivalent to a factor of 16 speedup. An additional benefit is that more samples and a more accurate evidence value can be obtained simply by continuing the run for longer, as in standard MCMC.
description: Accepted for publication in Statistics and Computing. C++ code available at http://lindor.physics.ucsb.edu/DNest
title: ÐÑÐ°ÑÐµÐ²Ð°Ð½Ð¸Ðµ Ð·Ð½Ð°Ð½Ð¸Ð¹. ÐÐ¾ ÑÑÑÐ°Ð½Ð¸ÑÐ°Ð¼ ÑÑÐµÐ±Ð½Ð¸ÐºÐ¾Ð² ÑÐ¸Ð·Ð¸ÐºÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð¼Ð¾ÑÐ½Ð¾Ð², ÐÐ¾Ð½ÑÑÐ°Ð½ÑÐ¸Ð½
Publisher: name: Ð¡ÐÐ±ÐÐ¢Ð£
Year: 1996
Subjects: Ð¤Ð¸Ð·Ð¸ÐºÐ°

description: ÐÐ°Ð¶Ð½ÐµÐ¹ÑÐ¸Ð¼Ð¸ ÐºÐ°ÑÐµÑÑÐ²Ð°Ð¼Ð¸ Ð»Ð¸ÑÐ½Ð¾ÑÑÐ¸, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ¸Ð¼Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÑ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°, ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÑÐµÐ¼Ð»ÐµÐ½Ð¸Ðµ Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ Ðº Ð½Ð°ÑÑÐ½Ð¾Ð¼Ñ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ, Ð¾ÑÐ²ÑÐ°ÑÐµÐ½Ð¸Ðµ Ðº Ð½ÐµÐ¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ. Ð¢Ð°ÐºÐ¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¼Ð¾Ð³ÑÑ ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°ÑÑÑÑ Ð² ÑÐ¾Ð·Ð½Ð°Ð½Ð¸Ð¸ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸. Ð­ÑÐ¾ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾, ÐµÑÐ»Ð¸ ÑÑÐµÐ±Ð½ÑÐµ ÑÐµÐºÑÑÑ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ñ Ð¾Ñ ÑÑÑÐ½Ð¾ÑÑÐ½ÑÑ Ð¾ÑÐ¸Ð±Ð¾Ðº, Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾ÑÐµÑÐ¸Ð¹ Ð¸ Ð¿ÑÐ¾Ð±ÐµÐ»Ð¾Ð², Ð° ÑÐ·ÑÐº Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¸Ð·ÑÑÐ°ÐµÐ¼Ð¾Ð¹ Ð¾Ð±ÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐµÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸. Ð ÑÐ¾Ð¶Ð°Ð»ÐµÐ½Ð¸Ñ, Ð´ÐµÐ¹ÑÑÐ²Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð´Ð°Ð»ÐµÐºÐ° Ð¾Ñ Ð¸Ð´ÐµÐ°Ð»Ð°. ÐÐ¾ÑÑÐ¾Ð¼Ñ Ð¸ Ð°Ð²ÑÐ¾ÑÐ°Ð¼, Ð¸ ÑÐ¸ÑÐ°ÑÐµÐ»ÑÐ¼ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ ÑÑÐ¸ÑÑÑÑ Ð¿ÑÐµÐ¾Ð´Ð¾Ð»ÐµÐ²Ð°ÑÑ Ð´ÐµÑÐµÐºÑÑ ÑÐµÐºÑÑÐ¾Ð². ÐÐ¾ÑÐºÐ¾Ð»ÑÐºÑ ÑÑÐ¸ÑÐ°ÐµÑÑÑ, ÑÑÐ¾ ÑÐ¸Ð·Ð¸ÐºÐ° ÑÐ»ÑÐ¶Ð¸Ñ ÑÑÐ°Ð»Ð¾Ð½Ð¾Ð¼ ÑÑÑÐ¾Ð³Ð¾ÑÑÐ¸ Ð´Ð»Ñ Ð´ÑÑÐ³Ð¸Ñ ÐµÑÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°ÑÐº, Ð² ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ¸Ð±Ð¾ÑÐ½ÑÐµ ÑÐµÐºÑÑÑ Ð² ÑÑÐµÐ±Ð½Ð¸ÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ¸ Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ Ð¸Ñ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ, Ð¸ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ Ð¿ÑÐµÐ´ÑÐ¿ÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ. ÐÐ½Ð°Ð»Ð¸Ð· Ð²ÐµÐ´ÐµÑÑÑ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ð¹ ÑÐµÑ Ð³ÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½ÑÑ Ð½Ð°ÑÐº, Ð¿ÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¼ÑÑÐ»ÐµÐ½Ð¸Ðµ Ð¸ ÑÐ·ÑÐº ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°. ÐÐ½ÑÐ¼Ð¸ ÑÐ»Ð¾Ð²Ð°Ð¼Ð¸, ÐºÐ½Ð¸Ð³Ð° ÑÑÐ°ÐºÑÑÐµÑ Ð¾ ÐºÑÐ»ÑÑÑÑÐµ Ð¼ÑÑÐ»ÐµÐ½Ð¸Ñ Ð¸ ÑÐ·ÑÐºÐ°. ÐÐ»Ñ ÑÑÐ°ÑÑÐµÐºÐ»Ð°ÑÑÐ½Ð¸ÐºÐ¾Ð², Ð°Ð±Ð¸ÑÑÑÐ¸ÐµÐ½ÑÐ¾Ð², Ð¸Ñ ÑÐ¾Ð´Ð¸ÑÐµÐ»ÐµÐ¹, ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹, Ð°Ð²ÑÐ¾ÑÐ¾Ð² ÑÑÐµÐ±Ð½Ð¸ÐºÐ¾Ð² Ð¸ ÑÐµÐ´Ð°ÐºÑÐ¾ÑÐ¾Ð².
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 ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Challenges of Forecasting the Long-Run Economic Consequences of Pandemics for Selected sub-Saharan Economies
Creators: name: Kangami, Divine Ngenyeh
name: Kangami, Divine Ngenyeh
Publisher: name: Unknown
Year: 2021
Subjects: subject: International Relations/Trade
subject: Labor and Human Capital
subject: Forecasting
subject: Economic Consequences of Pandemics
subject: Sub-Saharan Economies

description: As the global economy continues to wrestle with the recent COVID-19 pandemic, the effect of the pandemic continues to negatively affect economies and markets’ supply and demand trends. The significant decrease in trade and increase in unemployment rates across the globe are indicators of the widespread economic slump. This paper aims to illuminate the long-term effects of the ensuing COVID-19 pandemic by studying the effect of historical catastrophes that also had negative and long-lasting effects in the societies and contexts in West Africa. A desk review and analysis of the challenges encountered in forecasting the long-term effects of pandemics was undertaken to highlight some of the macroeconomic effects of pandemics. One of the takeaways from this critical analysis was that Economists face challenges when forecasting long-run effects across contexts and scenarios. The paper concludes by identifying some of the essential behavioral changes and the role that regional blocs could play in cushioning economies in their regions and mitigating for dangerous levels of economic ruin bought about by future pandemics.
Survey Protocol
Creators: name: Rimpa Basu Achari
name: Tapesh Bhattacharyya
name: Indranil Mallick
name: Chakraborty, Santam
name: Arunsingh, Moses
name: Sanjoy Chatterjee
Publisher: name: OSF Registries
Year: 2022
Subjects: Clinical Trials
India
Randomized Controlled Trials
Research Funding
Survey

description: Protocol for the survey
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¹ÑÐ°Ð¿ÐµÑÑÐ½, ÐÑÐ½Ðµ
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: ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð°Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ðµ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ðµ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÐÐÐ Â«Ð­Ð¹Ñ ÑÐ½Ð´ Ð­Ð¼ Ð¥ÐµÐ½Ð½ÐµÑ ÑÐ½Ð´ ÐÐ°ÑÑÐ¸ÑÂ». 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 ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Â«Ð­Ð¹Ñ ÑÐ½Ð´ Ð­Ð¼ Ð¥ÐµÐ½Ð½ÐµÑ ÑÐ½Ð´ ÐÐ°ÑÑÐ¸ÑÂ». ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«Ð­Ð¹Ñ ÑÐ½Ð´ Ð­Ð¼ Ð¥ÐµÐ½Ð½ÐµÑ ÑÐ½Ð´ ÐÐ°ÑÑÐ¸ÑÂ», ÐµÐµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ ÑÐºÑÐ¿ÐµÑÑÐ½Ð¾Ð³Ð¾ Ð¾Ð¿ÑÐ¾ÑÐ°, Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð². ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑ 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ÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Additional file 8 of Constructing a seventeen-gene signature model for non-obstructive azoospermia based on integrated transcriptome analyses and WGCNA
Creators: name: Chen, Yinwei
name: Yuan, Penghui
name: Gu, Longjie
name: Bai, Jian
name: Ouyang, Song
name: Sun, Taotao
name: Liu, Kang
name: Wang, Zhao
name: Liu, Chang
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 8: Supplementary Table 7. Clinical characteristics of patients with NOA and OA.
Social and emotional problems in rheumatoid arthritis, -- a study of a group of Vancouver cases
Creators: name: Mickelson, Harvey Paul
Publisher: name: University of British Columbia
Year: 2012

description: The purpose of this study is to examine the aspects of arthritis as a social welfare problem as well as a health problem, and to show (a) that the social and emotional components of the disease have a significant bearing on the "treatability" of the patient; (b) that casework, community organization and public welfare must be involved in an adequate treatment programme. The broader implications of the problem are indicated by statistics from national surveys and other related studies. But the essential material is derived from a study of cases. These include thirty hospital cases, of which twenty three were interviewed one or more times, and seven were taken from social histories in which sufficient data were available. Thirty replies were received from a special questionnaire sent to the homes of a second group of patients. The study shows that (1) each of the patients had an average of 3-1 socio-emotional problems significantly related to onset or recurrence (2) the disease created additional personal and family problems which are classified and discussed in detail, all of which prevented the patient from getting or benefiting from adequate treatment; (3) there are gaps in present treatment and rehabilitation programmes which must be filled, and (4) medical social work has an important role to play in assisting diagnosis, treatment and rehabilitation. It is hoped that this study of the social aspects of rheumatoid arthritis will clarify the role that social work must play in an adequate treatment programme, indicate the kinds of further research which would be valuable in this area and point up the need for a much broader perspective on the whole problem.
Stability of the directly imaged multiplanet system HR 8799: resonance and masses
Creators: name: Fabrycky, Daniel C.
name: Murray-Clay, Ruth A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A new era of directly imaged extrasolar planets has produced a three-planet system (Marois et al. 2008), where the masses of the planets have been estimated by untested cooling models. We point out that the nominal circular, face-on orbits of the planets lead to a dynamical instability in ~10^5 yr, a factor of at least 100 shorter than the estimated age of the star. Reduced planetary masses produce stability only for unreasonably small planets (
description: 16 pages; 15 figures; 4 tables. Accepted to ApJ. New version gives more attention to the upper mass limit for a double resonance. A new section allows for arbitrary eccentricities, orientations, and mutual inclinations
title: ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸ÑÐ¼Ð¸ Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ"Ð¡Ð¢Ð -Ð¢ÐµÐ»ÐµÐºÐ¾Ð¼"
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð®Ð¼Ð°ÑÐµÐ², ÐÐ¸ÐºÑÐ¾Ñ
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¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð·Ð°Ð´Ð°Ð½Ð¸Ðµ
ÑÑÐµÑ
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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 Â«Ð¡Ð¢Ð -Ð¢ÐµÐ»ÐµÐºÐ¾Ð¼Â», ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð² Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸ÐµÐ¹, Ð²ÐµÐ´ÑÑÐµÐ¹ Ð±Ð¸Ð·Ð½ÐµÑ Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð¿Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ñ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. 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 Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸ÑÐ¼Ð¸ Ð² ÐÐÐ Â«Ð¡Ð¢Ð -Ð¢ÐµÐ»ÐµÐºÐ¾Ð¼Â» Ð·Ð° ÑÑÐµÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ ÑÐµÐºÑÑÐµÐ³Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸ÑÐ¼Ð¸. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐµ ÑÐµÑÐµÐ½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸ÑÐ¼Ð¸ Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð½Ð¾Ð²Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ 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 ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ, Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð½Ð¾Ð¹ Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² ÐÐÐ Â«Ð¡Ð¢Ð -Ð¢ÐµÐ»ÐµÐºÐ¾Ð¼Â» Ð¿Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸ÑÐ¼Ð¸. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¡Ð£ÐÐ Ð²ÑÐ±ÑÐ°Ð½Ð° ÑÑÐµÐ´Ð° MS SQL Server, Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÑÐµÐ´Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð²ÑÐ±ÑÐ°Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Microsoft Visual Studio Ð½Ð° Ð±Ð°Ð·Ðµ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ .Net. ÑÐ·ÑÐº Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ - C#.
title: Ð ÑÐ¸ÑÐºÐ°Ñ Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð³Ð°Ð·Ð¾ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐÐ¢ÐÐ ÐÐ£Ð ÐÐÐÐÂ»)
Creators: name: ÐÐ¾ÑÐ¾Ð½Ð¾Ð²Ð°, Ð¡.
name: Ð¡ÑÐµÐ¿Ð°Ð½Ð¾Ð², Ð.
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ñ", 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 (Ð ÐÐ¡ÐâÐ­â2018) (2018; 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: 2018

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÐºÐ¾Ð², Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ðµ Ð² ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐµ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð³Ð°Ð·Ð¾ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐÐÐ Â«ÐÐµÑÐµÑÐ±ÑÑÐ³ÐÐ°Ð·Â».
Ranibizumab: A Review in Retinopathy of Prematurity
Creators: name: Lee, Arnold
name: Shirley, Matt
Publisher: name: Adis Journals
Year: 2021
Subjects: subject: Medicine
subject: 111301 Ophthalmology
subject: FOS: Clinical medicine

description: Compliance with Ethical Standards Funding The preparation of this review was not supported by any external funding. Authorship and Conflict of interest Arnold Lee and Matt Shirley are salaried employees of Adis International Ltd/Springer Nature, are responsible for the article content and declare no relevant conflicts of interest. All authors contributed to the review and are responsible for the article content. Ethics approval, Consent to participate, Consent to publish, Availability of data and material, Code availability not applicable
Additional information about this Adis Drug Review can be found here

Abstract  Ranibizumab (Lucentis®) is a monoclonal antibody fragment targeted against VEGF-A that is the first approved anti-VEGF agent for the treatment of retinopathy of prematurity (ROP). In the pivotal, randomized, phase III RAINBOW trial in infants with ROP, the majority of intravitreal ranibizumab recipients experienced treatment success at 24 weeks, with a numerically greater treatment success rate in the ranibizumab 0.2 mg (80% of patients) than laser therapy (66%) group without reaching statistical significance for superiority. Long-term effects on vision following ranibizumab treatment are not yet known, but interim analyses from the RAINBOW extension study do not show evidence of degraded vision. Adverse reactions to ranibizumab in pediatric patients were consistent with the known safety profile in adults, with most adverse reactions attributed to the intravitreal injection procedure. Furthermore, systemic VEGF suppression was not observed in clinical trials, which is congruent with the rapid systemic clearance of ranibizumab. Overall, ranibizumab is an effective and generally well tolerated treatment for ROP and is not associated with systemic VEGF suppression. Although results for its long-term effects on vision are not yet available, ranibizumab is a promising alternative option to laser therapy for treating ROP.

© Springer Nature Switzerland AG 2021
Entropic characterization of Separability in Gaussian states
Creators: name: Shenoy, Sudha
name: Devi, A. R. Usha
name: Rajagopal, A. K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We explore separability of bipartite divisions of mixed Gaussian states based on the positivity of the Abe-Rajagopal (AR) q-conditional entropy. The AR q-conditional entropic characterization provide more stringent restrictions on separability (in the limit q tending to infinity) than that obtained from the corresponding von Neumann conditional entropy (q = 1 case)--similar to the situation in finite dimensional states. Effectiveness of this approach, in relation to the results obtained by partial transpose criterion, is explicitly analyzed in three illustrative examples of two-mode Gaussian states of physical significance.
description: 4 pages, 3 figures; Brief version of the earlier paper; Journal references added
Gyrokinetic simulation of entropy cascade in two-dimensional electrostatic turbulence
Creators: name: Tatsuno, T.
name: Barnes, M.
name: Cowley, S. C.
name: Dorland, W.
name: Howes, G. G.
name: Numata, R.
name: Plunk, G. G.
name: Schekochihin, A. A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Computational Physics (physics.comp-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Two-dimensional electrostatic turbulence in magnetized weakly-collisional plasmas exhibits a cascade of entropy in phase space [Phys. Rev. Lett. 103, 015003 (2009)]. At scales smaller than the gyroradius, this cascade is characterized by the dimensionless ratio D of the collision time to the eddy turnover time measured at the scale of the thermal Larmor radius. When D >> 1, a broad spectrum of fluctuations at sub-Larmor scales is found in both position and velocity space. The distribution function develops structure as a function of v_{perp}, the velocity coordinate perpendicular to the local magnetic field. The cascade shows a local-scale nonlinear interaction in both position and velocity spaces, and Kolmogorov's scaling theory can be extended into phase space.
description: 8 pages, 10 figures, Conference paper presented at 2009 Asia-Pacific Plasma Theory Conference. Ver.2 includes corrected typos & updated references
Extracting the hydrodynamic resistance of droplets from their behavior in microchannel networks
Creators: name: Labrot, Vincent
name: Schindler, Michael
name: Guillot, Pierre
name: Colin, Annie
name: Joanicot, Mathieu
Publisher: name: arXiv
Year: 2009
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The overall traffic of droplets in a network of microfluidic channels is strongly influenced by the liquid properties of the moving droplets. In particular, the effective hydrodynamic resistance of individual droplets plays a key role in their global behavior. We here propose two simple and low-cost experimental methods for measuring this parameter by analyzing the dynamics of a regular sequence of droplets injected into an "asymmetric loop" network. The choice of a droplet taking either route through the loop is influenced by the presence of previous droplets which modulate the hydrodynamic resistance of the branches they are sitting in. We propose to extract the effective resistance of a droplet from easily observable time series, namely from the choices the droplets make at junctions and from the inter-droplet distances. This becomes possible when utilizing a recently proposed theoretical model, based on a number of simplifying assumptions. We here present several sets of measurements of the hydrodynamic resistance of droplets, expressed in terms of a "resistance length". The aim is twofold, (1) to reveal its dependence on a number of parameters, such as the viscosity, the volume of droplets, their velocity as well as the spacing between them. At the same time (2), by using a standard measurement technique, we compare the limitations of the proposed methods. As an important result of this comparison we obtain the range of validity of the simplifying assumptions made in the theoretical model.
description: 11 pages, 11 figures
The contribution of supernova remnants to the galactic cosmic ray spectrum
Creators: name: Caprioli, D.
name: Amato, E.
name: Blasi, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The supernova paradigm for the origin of galactic cosmic rays has been deeply affected by the development of the non-linear theory of particle acceleration at shock waves. Here we discuss the implications of applying such theory to the calculation of the spectrum of cosmic rays at Earth as accelerated in supernova remnants and propagating in the Galaxy. The spectrum is calculated taking into account the dynamical reaction of the accelerated particles on the shock, the generation of magnetic turbulence which enhances the scattering near the shock, and the dynamical reaction of the amplified field on the plasma. Most important, the spectrum of cosmic rays at Earth is calculated taking into account the flux of particles escaping from upstream during the Sedov-Taylor phase and the adiabatically decompressed particles confined in the expanding shell and escaping at later times. We show how the spectrum obtained in this way is well described by a power law in momentum with spectral index close to -4, despite the concave shape of the instantaneous spectra of accelerated particles. On the other hand we also show how the shape of the spectrum is sensible to details of the acceleration process and environment which are and will probably remain very poorly known.
description: 19 pages, 8 figures, published version (references updated)
title: Wheat-Gold Currency How To Make Large-Scale Grain Storage Possible
Creators: name: Garrett, David L.
Publisher: name: Utah State University
Year: 2012

description: The United States has a National Oil Reserve but no food reserve. Just as the oil reserve is designed to buffer unforeseen disruptions in the critical supply, the nation should also have a food reserve for at least the same purpose. The United States and other developed nations have little or no food reserve beyond the typical demands between growing seasons. Marvelous production achievements in agriculture beginning in the early 1960s and known as the “Green Revolution” are now leveling off. Food production, suffering from such negative side effects as reduced water tables, is being outstripped by population growth (Bourne, 2009). In 2006 through 2008 the US and world drawdown of wheat and other grain stocks, together with agricultural events such as droughts in various parts of the world, caused grain reserves to hit historically low levels. The resulting lack of supply created significant disruptions, including record high prices (Figure 1) (Good and Li, 2010, USDA - Foreign Agricultural Service, 2011), countries refusing to export, riots, and famine (CNN.com, 2008). The need for higher world grain stocks seems clear. Higher grain stocks should result in lower price volatility and higher food security in Utah, the US, the UK, and internationally.
title: La philosophie pour enfants et son influence sur les représentations des émotions de colère et de peur chez l’enfant
title: La philosophie pour enfants et son influence sur les représentations des émotions de colère et de peur chez l’enfant
titleType: AlternativeTitle
Creators: name: Cuénoud, Natacha
name: Guignard, Amandine
Publisher: name: Unknown
Year: 0
Subjects: subject: émotions
subject: philosophie avec les enfants
subject: représentations sociales
subject: verbalisation
subject: compréhension
subject: identification

description: Dans le cadre de ce mémoire professionnel, nous souhaitons estimer si la pratique de la philosophie avec les enfants permet de faire évoluer leurs représentations relatives aux émotions de colère et de peur. En effet, nous voyons dans la philosophie pour enfants un moyen concret et cohérent de donner du sens à la vie en mettant à la disposition des enfants un espace au sein duquel il leur est possible de poser des questions et de tenter d’y apporter des réponses grâce à la discussion entre pairs et, par extension, la co-construction du savoir. Notre recherche ambitionne de répondre aux questions de recherche suivantes : Quelles sont les représentations initiales d’enfants de six et sept ans des émotions de colère et de peur ? Ces représentations tendent-elles à évoluer grâce à l’utilisation de la philosophie pour enfants (PPE) ? Cette recherche a été menée dans une classe de 3H du canton de Vaud. Des prétests ont été effectués auprès de 21 élèves n’ayant encore jamais travaillé la thématique des émotions en classe. Par la suite, des discussions à visée philosophique ont été conduites. Les résultats qui ont émergé de l’analyse attestent d’une meilleure compréhension des émotions de colère et de peur chez les enfants. Par ailleurs, une analyse détaillée par la réalisation de posttests n’a malheureusement pas pu être effectuée en raison de la crise sanitaire COVID-19. Nous avons néanmoins pu relever une nette amélioration quant à la compréhension et la verbalisation des émotions et une réelle plus-value de ces ateliers de philosophie.
Odds of observing the multiverse
Creators: name: Dahlen, Alex
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Eternal inflation predicts our observable universe lies within a bubble (or pocket universe) embedded in a volume of inflating space. The interior of the bubble undergoes inflation and standard cosmology, while the bubble walls expand outward and collide with other neighboring bubbles. The collisions provide either an opportunity to make a direct observation of the multiverse or, if they produce unacceptable anisotropy, a threat to inflationary theory. The probability of an observer in our bubble detecting the effects of collisions has an absolute upper bound set by the odds of being in the part of our bubble that lies in the forward light-cone of a collision; in the case of collisions with bubbles of identical vacua, this bound given by the bubble nucleation rate times ($H_{\rm{O}}/H_{\rm{I}})^2$, where $H_{\rm{O}}$ is the Hubble scale outside the bubbles and $H_{\rm{I}}$ is the scale of the second round of inflation that occurs inside our bubble. Similar results were obtained by Freigovel \emph{et al.} using a different method for the case of collisions with bubbles of much larger cosmological constant; here it is shown to hold in the case of collisions with identical bubbles as well. A significant error in a previous draft was corrected in order to arrive at this result.
description: 21 pages, 12 figures; a significant error was corrected
The metanephros of the bird
Creators: name: Clayton, Blanche-P.
Publisher: name: University of British Columbia
Year: 2012

description: Certain investigations were undertaken on the kidneys of various birds using that of the domestic fowl, as a type; and, where possible, comparing the results with those reported for other classes of animals. The vascular system was considered, to establish the statement of Spanner (1924), that the bird kidney possesses a renal portal system. Embryological, histological, and anatomical evidence, were brought forward in favour of this venous arrangement. The histology was examined with different techniques. In this connection, a comparative examination of fixation fluids was undertaken, as difficulty was experienced in the histological examination of bird kidney tissue. The histological results indicated some degree of glomerular degeneration and an Increase in proximal tubule development as compared to that of the mammal. Cytological studies were carried out on mitochondria and the Golgi apparatus. The mitochondria of the domestic fowl, and the pigeon, showed great concentration in the cells of the proximal tubule. The Golgi apparatus was investigated in the fowl; and showed a development in the cells of the proximal segment of the nephron, in excess of that in the mammal. The conclusion deduced from both these cytological studies, indicated an increase in activity of the proximal segment in the bird, over that of the mammal. A histochemical test using alkaline phosphatase, was performed, to decide whether the reported glomerular degeneration in the bird is such that glucose elimination is reduced or absent. Alkaline phosphatase is an enzyme stated to assist in the reabsorption of glucose eliminated by glomerular filtration. The results were compared with those of the classes possessing good glomerular development. It was noted that the avian kidney shows considerable evidence of alkaline phosphatase activity. Two conclusions are reached: (1) That the bird kidney shows definite evidence of tubular activity. (2) That in spite of apparent signs of degeneration, the glomerulus in the avian kidney functions comparably to that of the mammal.
The Left-Right SU(3)(L)xSU(3)(R)xU(1)(X) Model with Light, keV and Heavy Neutrinos
Creators: name: Dias, Alex G.
name: Pires, C. A. de S.
name: da Silva, P. S. Rodrigues
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We construct a full left-right model for the electroweak interactions based on the $SU(3)_{L}\otimes SU(3)_{R}\otimes U(1)_{X}$ gauge symmetry. The fermion content of the model is such that anomaly cancellation restricts the number of families to be a multiple of three. One of the most important features of the model is the joint presence of three light active neutrinos, three additional neutrinos at keV mass scale, and six heavy ones with masses around\textbf{$10^{11}$} GeV. They form a well-motivated part of the spectrum in the sense they address challenging problems related to neutrino oscillation, warm dark matter, and baryogenesis through leptogenesis.
description: 11 pages. Small corrections and typos fixed. Accepted for publication in PRD
title: ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð½Ð°Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð½Ð° Ð¿ÑÐ¾ÑÐµÑÑÑ Ð¿Ð»Ð°Ð²ÐºÐ¸ Ð»ÑÐ´Ð° Ð½Ð° Ð¿ÑÐ¾Ð²Ð¾Ð´Ð°Ñ Ð¸ ÑÑÐ¾ÑÐ°Ñ Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÑ Ð»Ð¸Ð½Ð¸Ð¹
title: Ð°Ð²ÑÐ¾ÑÐµÑ. Ð´Ð¸Ñ. â¦ ÐºÐ°Ð½Ð´. ÑÐµÑ Ð½. Ð½Ð°ÑÐº: 05.09.05
titleType: Subtitle
Creators: name: ÐÐ¾Ð½ÑÐ°ÑÐ¾Ð², ÐÐ°Ð»ÐµÑÐ¸Ð¹
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: 2019
Subjects: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð»Ð¸Ð½Ð¸Ð¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÐµ
ÐÑÐ¿ÑÑÐ¼Ð¸ÑÐµÐ»Ð¸ Ð²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ
ÐÐ°Ð·ÐµÐ¼Ð»ÑÑÑÐ¸Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°
ÐÑÑÐ¾ÐºÐ¸Ðµ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ (ÑÐ»ÐµÐºÑÑ.)
Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð»Ð¸Ð½Ð¸Ð¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¿Ð»Ð°Ð²ÐºÐ¸ Ð»ÑÐ´Ð° Ð½Ð° Ð¿ÑÐ¾Ð²Ð¾Ð´Ð°Ñ Ð¸ Ð³ÑÐ¾Ð·Ð¾Ð·Ð°ÑÐ¸ÑÐ½ÑÑ ÑÑÐ¾ÑÐ°Ñ Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÑ Ð»Ð¸Ð½Ð¸Ð¹. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐºÑÐ¿ÑÐµÑÑ-Ð¼ÐµÑÐ¾Ð´ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°ÑÐ¸ ÑÐ¸Ð½ÑÐµÐ·Ð° Ð´Ð»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÐµÐ¼Ñ Ð·Ð°Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð·ÐµÐ¼Ð»ÑÑÑÐµÐ³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¿Ð¾ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÐ¼ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°Ð¼. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÑÐ¿Ð¾ÑÐ¾Ð± ÑÑÐµÑÐ° Ð²ÑÑÑÐ¸Ñ Ð³Ð°ÑÐ¼Ð¾Ð½Ð¸Ðº Ð¿ÑÐ¸ Ð¾ÑÐµÐ½ÐºÐµ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð³Ð¾ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÐ¾ÐºÐ° Ð¿Ð»Ð°Ð²ÐºÐ¸.
Observing gravitational wave bursts in pulsar timing measurements
Creators: name: Pshirkov, M. S.
name: Baskaran, D.
name: Postnov, K. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We propose a novel method for observing the gravitational wave signature of super-massive black hole (SMBH) mergers. This method is based on detection of a specific type of gravitational waves, namely gravitational wave burst with memory (BWM), using pulsar timing. We study the unique signature produced by BWM in anomalous pulsar timing residuals. We show that the present day pulsar timing precision allows one to detect BWM due to SMBH mergers from distances up to 1 Gpc (for case of equal mass 10^8 Msun SMBH). Improvements in precision of pulsar timing together with the increase in number of observed pulsars should eventually lead to detection of a BWM signal due to SMBH merger, thereby making the proposed technique complementary to the capabilities of the planned LISA mission.
description: 9 pages, 1 figure, generally matches the MNRAS version
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
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ÐµÐ»ÑÐ½Ð¸ÐºÐ¾Ð², ÐÐ»ÐµÐ³
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¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹
Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«Ð¡Ð¾ Ð²ÐºÑÑÐ¾Ð¼Â».
Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ â Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾- ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. ÐÐ·ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð´Ð»Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¸ Ð¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "Ð¡Ð¾ Ð²ÐºÑÑÐ¾Ð¼".
ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ ÑÐ°ÑÑÐµÑ Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸.
title: Planning, Acting, and Learning in Incomplete Domains
Creators: name: Weber, Christopher H.
Publisher: name: Utah State University
Year: 2012

description: The engineering of complete planning domain descriptions is often very costly because of human error or lack of domain knowledge. Learning complete domain descriptions is also very challenging because many features are irrelevant to achieving the goals and data may be scarce. Given incomplete knowledge of their actions, agents can ignore the incompleteness, plan around it, ask questions of a domain expert, or learn through trial and error.
Our agent Goalie learns about the preconditions and effects of its incompletely-specified actions by monitoring the environment state. In conjunction with the plan failure explanations generated by its planner DeFault, Goalie diagnoses past and future action failures. DeFault computes failure explanations for each action and state in the plan and counts the number of incomplete domain interpretations wherein failure will occur. The questionasking strategies employed by our extended Goalie agent using these conjunctive normal form-based plan failure explanations are goal-directed and attempt to approach always successful execution while asking the fewest questions possible. In sum, Goalie: i) interleaves acting, planning, and question-asking; ii) synthesizes plans that avoid execution failure due to ignorance of the domain model; iii) uses these plans to identify relevant (goal-directed) questions; iv) passively learns about the domain model during execution to improve later replanning attempts; v) and employs various targeted (goal-directed) strategies to ask questions (actively learn).
Our planner DeFault is the first reason about a domain's incompleteness to avoid potential plan failure. We show that DeFault performs best by counting prime implicants (failure diagnoses) rather than propositional models. Further, we show that by reasoning about incompleteness in planning (as opposed to ignoring it), Goalie fails and replans less often, and executes fewer actions. Finally, we show that goal-directed knowledge acquisition - prioritizing questions based on plan failure diagnoses - leads to fewer questions, lower overall planning and replanning time, and higher success rates than approaches that naively ask many questions or learn by trial and error.
title: Ð¡Ð¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÐ»ÑÐµÐ², ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
name: ÐÐ°ÑÐ¸Ð±Ð¸Ð½, ÐÐ°Ð²ÐµÐ»
name: ÐÐ°Ð³ÑÑÐ´ÑÐºÐ°Ñ, ÐÐ°ÑÐ°Ð»Ð¸Ñ
Publisher: name: [Ð¡ÐÐ±ÐÐ¢Ð£]
Year: 1995
Subjects: Ð¡ÑÐ´Ð¾Ð¿Ð¾Ð´ÑÐµÐ¼Ð½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð° Ð¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ
Ð¨Ð»ÑÐ·Ñ ÑÑÐ´Ð¾Ñ Ð¾Ð´Ð½ÑÐµ

description: ÐÐ°Ð½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¸ Ð²Ð¾Ð´Ð½Ð¾ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð² Ð Ð¾ÑÑÐ¸Ð¸. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÑÐ´Ð¾Ð¿ÑÐ¾Ð¿ÑÑÐºÐ½ÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹, ÑÐ°ÐºÐ¸Ñ, ÐºÐ°Ðº ÑÐ»ÑÐ·Ñ Ð¸ ÑÑÐ´Ð¾Ð¿Ð¾Ð´ÑÐµÐ¼Ð½Ð¸ÐºÐ¸. ÐÑÐ²ÐµÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ°ÑÑÐµÑÐ° Ð¸
ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°.
ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ "ÐÐ¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ", "ÐÐ¸Ð´ÑÐ¾Ð¼ÐµÐ»Ð¸Ð¾ÑÐ°ÑÐ¸Ñ", "ÐÐ¸Ð´ÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°":
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 ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.