cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Experimental Study of Energy Transfer by Inertial Waves During the Build up of Turbulence in a Rotating System
Creators: name: Kolvin, Itamar
name: Cohen, Kobi
name: Vardi, Yuval
name: Sharon, Eran
Publisher: name: arXiv
Year: 2008
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We study the transition from fluid at rest to turbulence in a rotating water cylinder. We show that the energy, injected at a given height, is transported by inertial wave packets through the fluid volume. These waves propagate at velocities consistent with those calculated from linearized theory, even when they possess large amplitudes. A clear "front" in the temporal evolution of the energy power spectrum is detected, defining a time scale for energy transport at the linear wave speed in the system. Nonlinear energy transfer between modes is governed by a different time scale that can be much longer than the linear one. These observations suggest that the energy distribution and statistics in rotating turbulent fields that are driven by intermittent energy sources may be different from those described by the inverse energy cascade in two-dimensional turbulence.
description: 11 pages, 5 figures
Lattice QCD at finite temperature : present status
Creators: name: Petreczky, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I review recent progress in finite temperature lattice calculations, including calculations of Equation of State, fluctuations of conserved charges and spatial correlation functions. I compare lattice results with the predictions of hadron resonance gas model, resummed perturbation theory and 3-dimensional effective field theory. Comparison of the lattice results for certain ratios with the prediction of AdS/CFT correspondence is also discussed.
description: Invited plenary talk at Quark Matter 2009 Conference, LaTeX, 8 pages, uses elsarticle.cls, corrected typos
Search for massive rare particles with the SLIM experiment
Creators: name: M. Giorgini
Publisher: name: INFN Open Access Repository
Year: 2007

description: The SLIM experiment is a large array of nuclear track detectors located at
the Chacaltaya High Altitude Laboratory (5260 m a.s.l.). The preliminary
results from the analysis of ~383 m^2 exposed for 4.07 y are here reported. The
detector is sensitive to Intermediate Mass Magnetic Monopoles, 10^5 < M_M <
10^12 GeV, and to SQM nuggets and Q-balls, which are possible Dark Matter
candidates.
title: Ð¡Ð²ÑÐ·Ñ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð° Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½ÑÐ¼ ÑÐ¸ÐºÐ»Ð¾Ð¼ (PLM) Ð¿ÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ³Ð½Ð°ÑÑÐµÐ²Ð°, ÐÐºÑ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: 2016
Subjects: PLM
ÑÑÐ½Ð¾Ðº ÑÑÐ´Ð¾Ð²Ð¾Ð¹ ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð¹ Ð°ÑÐ¼Ð°ÑÑÑÑ
Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾Ð´ÑÐºÑ
marine valves market
innovative produkt

description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð±ÑÐ» ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½ÑÐ¼ ÑÐ¸ÐºÐ»Ð¾Ð¼ (PLM) ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð¾ÑÑÐ´Ð° ÑÑÐ´Ð¾Ð²Ð¾Ð¹ ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð¹ Ð°ÑÐ¼Ð°ÑÑÑÑ Ð¸ ÑÐ¾Ð»Ñ Ð¾ÑÐ´ÐµÐ»Ð° Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð° Ð½Ð° ÐºÐ°Ð¶Ð´Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ Ð² Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐµ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° PLM Ð¿ÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð´ÑÐºÑÐ°.
description: In Master's thesis it would be considered the process of the product lifecycle management (PLM) during marine valves series development and the marketing department importance were analyzed at every step of this process. In addition, the economic effect of the PLM process implementation during innovative products development was measured.
The ACS Nearby Galaxy Survey Treasury V. Radial Star Formation History of NGC 300
Creators: name: Gogarten, Stephanie M.
name: Dalcanton, Julianne J.
name: Williams, Benjamin F.
name: Roskar, Rok
name: Holtzman, Jon
name: Seth, Anil C.
name: Dolphin, Andrew
name: Weisz, Daniel
name: Cole, Andrew
name: Debattista, Victor P.
name: Gilbert, Karoline M.
name: Olsen, Knut
name: Skillman, Evan
name: de Jong, Roelof S.
name: Karachentsev, Igor D.
name: Quinn, Thomas R.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present new Hubble Space Telescope (HST) observations of NGC 300 taken as part of the ACS Nearby Galaxy Survey Treasury (ANGST). Individual stars are resolved in these images down to an absolute magnitude of M_F814W = 1.0 (below the red clump). We determine the star formation history of the galaxy in 6 radial bins by comparing our observed color-magnitude diagrams (CMDs) with synthetic CMDs based on theoretical isochrones. We find that the stellar disk out to 5.4 kpc is primarily old, in contrast with the outwardly similar galaxy M33. We determine the scale length as a function of age and find evidence for inside-out growth of the stellar disk: the scale length has increased from 1.1 +/- 0.1 kpc 10 Gyr ago to 1.3 +/- 0.1 kpc at present, indicating a buildup in the fraction of young stars at larger radii. As the scale length of M33 has recently been shown to have increased much more dramatically with time, our results demonstrate that two galaxies with similar sizes and morphologies can have very different histories. With an N-body simulation of a galaxy designed to be similar to NGC 300, we determine that the effects of radial migration should be minimal. We trace the metallicity gradient as a function of time and find a present day metallicity gradient consistent with that seen in previous studies. Consistent results are obtained from archival images covering the same radial extent but differing in placement and filter combination.
description: 18 pages, 18 figures, 4 tables, accepted for publication in ApJ
Chi ha sparato il neutrino cosmico?
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Secondo gli autori è la prima associazione plausibile tra un singolo oggetto extragalattico e un neutrino cosmico, quella pubblicata su Nature Physics riguardo al blazar PKS B1424-418 e il neutrino da record, soprannominato Big Bird, rilevato dall’esperimento IceCube in Antartide il 4 dicembre 2012
Additional file 5 of Single-cell transcriptome analysis and in vitro differentiation of testicular cells reveal novel insights into male sterility of the interspecific hybrid cattle-yak
Creators: name: Mipam, TserangDonko
name: Chen, Xuemei
name: Zhao, Wangsheng
name: Zhang, Peng
name: Chai, Zhixin
name: Yue, Binglin
name: Luo, Hui
name: Wang, Jikun
name: Wang, Haibo
name: Wu, Zhijuan
name: Wang, Jiabo
name: Wang, Mingxiu
name: Wang, Hui
name: Zhang, Ming
name: Wang, Hongying
name: Jing, Kemin
name: Zhong, Jincheng
name: Cai, Xin
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 5: Table S5. Primer sequences for detection of germ cell marker genes during spermatogenic cell proliferation and differentiation between cattle-yak and yak.
title: Wie bleiben gemeinschaftliche Wohnprojekte beständig? : Eine qualitative Analyse der Beständigkeit von gemeinschaftlichen Wohnprojekten in Hinblick auf die nachhaltige Stadtentwicklung
Creators: name: Gies, Dorothee
Publisher: name: Wuppertal Institut für Klima, Umwelt, Energie
Year: 2023
Subjects: subject: 300 Sozialwissenschaften

description: Die Schaffung von bezahlbarem und sozial gerechtem Wohnraum stellt eine zentrale Herausforderung der nachhaltigen Stadtentwicklung dar. Zur Begegnung dieser Herausforderungen spielen innovative Wohnformen wie gemeinschaftliche Wohnprojekte eine bedeutende Rolle, da sie vielfältige soziale Nachhaltigkeitsaspekte aufweisen und dadurch zu einer nachhaltigen Stadtentwicklung beitragen können. In diesem Kontext bleibt die Frage offen, ob die Gemeinschaften in Wohnprojekten nach ihrer Gründung beständig bleiben. Das Ziel der Arbeit war die Beantwortung der folgenden Forschungsfrage: "Wie können gemeinschaftliche Wohnprojekte dauerhaft in Bezug auf ihre Weiterentwicklung bestehen bleiben und somit langfristig eine nachhaltige Stadtentwicklung unterstützen?" 
Zur Beantwortung der Forschungsfrage wurde eine qualitative Studie in Form von narrativen Interviews mit Bewohner:innen gemeinschaftlicher Wohnprojekte durchgeführt. Die Ergebnisse aus Literatur und Praxis konnten acht besonders relevante Faktoren für die Beständigkeit von gemeinschaftlichen Wohnprojekten identifizieren: Soziale Durchmischung, Organisationsstruktur, Gemeinschaftspflege, Vertrauen, Soziales Netzwerk, Kommunikationskultur, gelebte Nachhaltigkeit, Flexibilität und Anpassungsfähigkeit. Diese Faktoren ermöglichen eine nachhaltige und anpassungsfähige Gemeinschaft, welche zu einer nachhaltigen Stadtentwicklung beitragen kann. Dafür sollten gemeinschaftliche Wohnprojekte ihre vorhandenen Potenziale weiterhin ausbauen.
The construction and commissioning of the CMS Silicon Strip Tracker
Creators: name: Sguazzoni, Giacomo
Publisher: name: Giacomo Sguazzoni (for the CMS Silicon Strip Tracker
  Collaboration), in Proceedings of the 34th International Conference in High
  Energy Physics (ICHEP08), Philadelphia, 2008, eConf C080730
Year: 2008

description: As the start up date for LHC approaches, the detectors are readying for data
taking. Here a review will be given on the construction phase with insights
into the various difficulties encountered during the process. An overview will
also be given of the commissioning strategy and results obtained so far.
  The CMS tracker is the largest silicon microstrip detector ever built.
Consisting of three main subsystems, Inner Barrel and Disks, Outer Barrel and
End Caps, it is 5.4m long and is 2.4m in diameter. Total detector surface is an
unprecedented 200m^2 with more than 15000 detector modules.
  The various integration procedures and quality checks implemented are briefly
reviewed. Finally an overview is given of checkout procedures performed at
CERN, after the final underground installation of the detector.
Photometric monitoring of the young star Par 1724 in Orion
Creators: name: Neuhaeuser, R.
name: Koeltzsch, A.
name: Raetz, St.
name: Schmidt, T. O. B.
name: Mugrauer, M.
name: Young, N.
name: Bertoldi, F.
name: Roell, T.
name: Eisenbeiss, T.
name: Hohle, M. M.
name: Vanko, M.
name: Ginski, C.
name: Rammo, W.
name: Moualla, M.
name: Broeg, C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report new photometric observations of the 200000 year old naked weak-line run-away T Tauri star Par 1724, located north of the Trapezium cluster in Orion. We observed in the broad band filters B, V, R, and I using the 90cm Dutch telescope on La Silla, the 80cm Wendelstein telescope, and a 25cm telescope of the University Observatory Jena in Grossschwabhausen near Jena. The photometric data in V and R are consistent with a 5.7 day rotation period due to spots, as observed before between 1960ies and 2000. Also, for the first time, we present evidence for a long-term 9 or 17.5 year cycle in photometric data (V band) of such a young star, a cycle similar to that to of the Sun and other active stars.
description: AN in press (eps or ps files on http://www.astro.uni-jena.de/Observations/gsh/gsh_papers.htm)
Venti stellari estremi da binarie X
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Un team di ricercatori dell’Università di Cambridge ha raccolto dati del telescopio ad alte energie dell’ESA per tre sorgenti ultra-luminose nei raggi X. Lo studio, pubblicato sull’ultimo numero della rivista Nature, mostra che due di queste sorgenti emettono getti a un quarto della velocità della luce
Memoryless Routing in Convex Subdivisions: Random Walks are Optimal
Creators: name: Chen, Dan
name: Devroye, Luc
name: Dujmovic, Vida
name: Morin, Pat
Publisher: name: arXiv
Year: 2009
Subjects: subject: Computational Geometry (cs.CG)
subject: FOS: Computer and information sciences

description: A memoryless routing algorithm is one in which the decision about the next edge on the route to a vertex t for a packet currently located at vertex v is made based only on the coordinates of v, t, and the neighbourhood, N(v), of v. The current paper explores the limitations of such algorithms by showing that, for any (randomized) memoryless routing algorithm A, there exists a convex subdivision on which A takes Omega(n^2) expected time to route a message between some pair of vertices. Since this lower bound is matched by a random walk, this result implies that the geometric information available in convex subdivisions is not helpful for this class of routing algorithms. The current paper also shows the existence of triangulations for which the Random-Compass algorithm proposed by Bose etal (2002,2004) requires 2^{Ω(n)} time to route between some pair of vertices.
description: 11 pages, 6 figures
Heavy ions and parton saturation from RHIC to LHC
Creators: name: Dainese, Andrea
Publisher: name: INFN Open Access Repository
Year: 2008

description: The phenomenology of gluon saturation at small parton momentum fraction,
Bjorken-x, in the proton and in the nucleus is introduced. The
experimentally-accessible kinematic domains at the nucleus-nucleus colliders
RHIC and LHC are discussed. Finally, the saturation hints emerging from
measurements at RHIC and the perspectives for LHC are described.
Generalized Fisher information matrix in nonextensive systems with spatial correlation
Creators: name: Hasegawa, Hideo
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: By using the $q$-Gaussian distribution derived by the maximum entropy method for spatially-correlated $N$-unit nonextensive systems, we have calculated the generalized Fisher information matrix of $g_{θ_n θ_m}$ for $(θ_1, θ_2, θ_3) = (μ_q, σ_q^2$, $s$), where $μ_q$, $σ_q^2$ and $s$ denote the mean, variance and degree of spatial correlation, respectively, for a given entropic index $q$. It has been shown from the Cramér-Rao theorem that (1) an accuracy of an unbiased estimate of $μ_q$ is improved (degraded) by a negative (positive) correlation $s$, (2) that of $σ_q^2$ is worsen with increasing $s$, and (3) that of $s$ is much improved for $s \simeq -1/(N-1)$ or $s \simeq 1.0$ though it is worst at $s = (N-2)/2(N-1)$. Our calculation provides a clear insight to the long-standing controversy whether the spatial correlation is beneficial or detrimental to decoding in neuronal ensembles. We discuss also a calculation of the $q$-Gaussian distribution, applying the superstatistics to the Langevin model subjected to spatially-correlated inputs.
description: 18 pages, 3 figures: revised version accepted in Phys. Rev. E
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð³Ð°Ð·Ð¾Ð¼Ð°Ð·ÑÑÐ½Ð¾Ð¹ ÐÐ­Ð¡ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 4Ñ 500 Ð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Ð²Ð°Ð½Ð¾Ð², ÐÐ¼Ð¸ÑÑ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: 2018
Subjects: ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ñ
ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ðµ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ðµ
Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾Ñ
ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾Ñ
ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾.

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸. ÐÑÐ±ÑÐ°Ð½Ð° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐ¾ÐºÐ¸ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ. ÐÑÐ±ÑÐ°Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ Ð¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð³Ð»Ð°Ð²Ð½Ð°Ñ ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÑÑÐµÐ¼Ð° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´.
The York Map and the Role of Non-Inertial Frames in the Geometrical View
  of the Gravitational Field
Creators: name: Lusanna, Luca
Publisher: name: INFN Open Access Repository
Year: 2007

description: The role of non-inertial frames in a class of models of general relativity is
clarified by means of Dirac's theory of constraints. The identification of a
York canonical basis allows to give the interpretation of the gauge variables
as generalized inertial effects and to identify the Dirac observables of the
gravitational field with generalized tidal effects. York time is the gauge
variable controlling the clock synchronization convention. Differently from
special relativity, the instantaneous 3-spaces are dynamically determined.
The thermal decomposition of cyclobutane at low pressures
Creators: name: Ogawa, Rosalind
Publisher: name: University of British Columbia
Year: 2011

description: The thermal decomposition of cyclobutane is a homogeneous,unimolecular reaction;ethylene being the only product.The rate law :- K = 10¹⁵•³ e⁻⁶¹’⁰⁰⁰[symbol omitted] sec.⁻¹ was found to be obeyed in the pressure region 10 to 40 mm. and temperature range 398° to 450°C. Cyclobutane undergoes a wall reaction to form propylene and 1-butene. The high pressure rate constant falls off at low pressures and reaches a limiting low pressure rate when activation is maintained by collision with the walls of the reactor. The low pressure limiting rate decreases as the size of the reactor increases. The fall off curves gave best agreement with values of the Slater parameter, n, between 5 and 8, and values of the Kassel parameter, s, between 3 and 7. It was concluded that the ring vibrations are of major importance in the dissociation, and that the C—H bond vibrations are relatively unimportant. No evidence for a tetramethylene biradical intermediate was found. The reaction mechanism probably involves the simultaneous splitting of two opposite C—C bonds.
The fast declining Type Ia supernova 2003gs, and evidence for a significant dispersion in near-infrared absolute magnitudes of fast decliners at maximum light
Creators: name: Krisciunas, Kevin
name: Marion, G. H.
name: Suntzeff, Nicholas B.
name: Blanc, Guillaume
name: Bufano, Filomena
name: Candia, Pablo
name: Cartier, Regis
name: Elias-Rosa, Nancy
name: Espinoza, Juan
name: Gonzalez, David
name: Gonzalez, Luis
name: Gonzalez, Sergio
name: Gooding, Samuel D.
name: Hamuy, Mario
name: Knox, Ethan A.
name: Milne, Peter A.
name: Morrell, Nidia
name: Phillips, Mark M.
name: Stritzinger, Maximillian
name: Thomas-Osip, Joanna
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We obtained optical photometry of SN 2003gs on 49 nights, from 2 to 494 days after T(B_max). We also obtained near-IR photometry on 21 nights. SN 2003gs was the first fast declining Type Ia SN that has been well observed since SN 1999by. While it was subluminous in optical bands compared to more slowly declining Type Ia SNe, it was not subluminous at maximum light in the near-IR bands. There appears to be a bimodal distribution in the near-IR absolute magnitudes of Type Ia SNe at maximum light. Those that peak in the near-IR after T(B_max) are subluminous in the all bands. Those that peak in the near-IR prior to T(B_max), such as SN 2003gs, have effectively the same near-IR absolute magnitudes at maximum light regardless of the decline rate Delta m_15(B). Near-IR spectral evidence suggests that opacities in the outer layers of SN 2003gs are reduced much earlier than for normal Type Ia SNe. That may allow gamma rays that power the luminosity to escape more rapidly and accelerate the decline rate. This conclusion is consistent with the photometric behavior of SN 2003gs in the IR, which indicates a faster than normal decline from approximately normal peak brightness.
description: 41 pages, 13 figures, to be published in the December, 2009, issue of the Astronomical Journal
title: ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð³ÑÐ°ÑÐ¸ÐºÐµ. Ð§. 3
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐºÐ¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: ÐÐ¾ÑÐºÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
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: 2022
Subjects: ÐÐ½Ð¶ÐµÐ½ÐµÑÐ½Ð°Ñ Ð³ÑÐ°ÑÐ¸ÐºÐ°
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
ÐÐ°ÑÐ¸Ð½Ð½Ð°Ñ Ð³ÑÐ°ÑÐ¸ÐºÐ°
ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð·Ð°ÐºÑÐµÐ¿Ð¸ÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð½Ð°Ð½Ð¸Ñ ÐºÑÑÑÐ° Â«ÐÐ½Ð¶ÐµÐ½ÐµÑÐ½Ð°Ñ Ð³ÑÐ°ÑÐ¸ÐºÐ°Â», Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ Ð¾ÑÐ²Ð¾Ð¸ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐÐÐÐÐÐ¡-3D V18 Ð¸ ÑÑÐ°ÑÑÐµ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐµÐ¹, ÑÐ¾ÑÐ¼Ð¸ÑÑÑÑÑÑ Ð½Ð°Ð²ÑÐºÐ¸ ÑÑÐµÐ½Ð¸Ñ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸ Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸, Ð¸Ð·ÑÑÐ°ÑÑÑÑ ÐºÐ¾Ð¼Ð°Ð½Ð´Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¡ÐÐÐ . ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ ÐºÑÑÑÐ° Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ÐµÐ¼Ð¾Ð² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð´ÑÑÐ³Ð¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸.
Beam-Beam Interaction in Novel, Very High Luminosity Parameter Regimes
Creators: name: Zobov, Mikhail
Publisher: name: INFN Open Access Repository
Year: 2010

description: In order to achieve luminosities significantly higher than in existing
machines, future storage-ring based colliders will need to operate in novel
parameter regimes combining ultra-low emittance, large Piwinski angle and high
bunch charge; implementation of techniques such as a "crab waist" will add
further challenges. Understanding the beam-beam interaction in these situations
will be essential for the design of future very high luminosity colliders.
Recent developments in modeling tools for studying beam-beam effects, capable
of investigating the relevant regimes, will be discussed and examples,
including tests with crab waist collisions in DAFNE, will be presented.
title: Ð¡Ð¾ÑÑÐ¾ÑÐ½Ð¸Ðµ, Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð§ÐµÑÐµÐ½ÐºÐ¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
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: 2016
Subjects: Ð¼Ð°Ð»ÑÐ¹ Ð±Ð¸Ð·Ð½ÐµÑ
Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ° Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ°
Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ°
Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ
the prospects for small business
small business
peculiarities of small business

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð°ÑÐ¿ÐµÐºÑÐ¾Ð² ÐºÐ°ÑÐ°ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² Ð¡Ð°Ð½ÐºÑ - ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ. Ð ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² Ð²Ð¸Ð´Ðµ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½Ð¾Ð³Ð¾ Ð¸ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð¿ÑÑÐ°, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ¾Ð»Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ð¸ ÑÐµÐ³Ð¸Ð¾Ð½Ð°, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ. ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ: Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ°, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ°.
description: This work represents a study of the theoretical aspects of tangent condition of the problems and prospects of small business development in Saint - Petersburg. In the theoretical part reviewed the history of the formation of small businesses in the form of foreign and domestic experience, discussed the role of small business in the development of the region, peculiarities of small business in St. Petersburg. Practical part of the work presents the analysis of prospects of development of small business, the analysis of sources of small business financing and recommendations for the development of the system of state support of small business.
Additional file 1 of Single-cell transcriptome analysis and in vitro differentiation of testicular cells reveal novel insights into male sterility of the interspecific hybrid cattle-yak
Creators: name: Mipam, TserangDonko
name: Chen, Xuemei
name: Zhao, Wangsheng
name: Zhang, Peng
name: Chai, Zhixin
name: Yue, Binglin
name: Luo, Hui
name: Wang, Jikun
name: Wang, Haibo
name: Wu, Zhijuan
name: Wang, Jiabo
name: Wang, Mingxiu
name: Wang, Hui
name: Zhang, Ming
name: Wang, Hongying
name: Jing, Kemin
name: Zhong, Jincheng
name: Cai, Xin
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Table S1. Statistics of cell numbers, scRNA sequencing and transcriptome alignment.
title: Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸. ÐÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ñ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð·Ð°ÑÑÐ°Ñ Ð¸ Ð´ÐµÐ»ÐµÐ¶Ð° Ð´Ð¾Ñ Ð¾Ð´Ð° Ð² Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÑÐ¸ÑÐ¼Ðµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐ·ÑÐ¼ÐµÐ½ÐºÐ¾Ð², ÐÐ°Ð»ÐµÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐÐ£
Year: 2002
Subjects: ÐÑÐ¸Ð½ÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ð¹

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸Â» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµÂ». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ - ÑÐ³Ð°Ð»Ð¸ÑÐ°ÑÐ¸Ð·Ð¼, ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ÑÑÑ, Ð¼Ð¾Ð½Ð¾ÑÐ¾Ð½Ð½Ð¾ÑÑÑ, ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÑÐ¸Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¾Ð² ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½ ÑÑÐ´ Ð¿ÑÐ¾ÑÐµÐ´ÑÑ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð·Ð°ÑÑÐ°Ñ Ð¸ Ð´Ð¾ÑÐ¾Ð´Ð° Ð¼ÐµÐ¶Ð´Ñ Ð°Ð³ÐµÐ½ÑÐ°Ð¼Ð¸ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÑÐ¸ÑÐ¼Ñ, Ð¿ÑÐµÑÐ»ÐµÐ´ÑÑÑÐ¸Ð¼Ð¸ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð²ÑÐ³Ð¾Ð´Ñ, Ð½Ð¾ Ð¸ Ð¾Ð±ÑÐµÐ´Ð¸Ð½ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¾Ð±ÑÐ¸Ð¼Ð¸ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐ¼Ð¸ Ð¸Ð½ÑÐµÑÐµÑÐ°Ð¼Ð¸. ÐÑÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿ÑÐ¾Ð¸Ð»Ð»ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ð¼Ð¸ Ð¸Ð· ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¾Ð±Ð»Ð°ÑÑÐµÐ¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸. ÐÑÐ½Ð¾Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾Ð¹ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ Ð¿ÑÐ¾ÑÐµÐ´ÑÑ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐµÑÐ²ÐµÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ° ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸Â» Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸.
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°.
Angular momentum-mass inequality for axisymmetric black holes
Creators: name: Dain, Sergio
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In these notes we describe recent results concerning the inequality $m\geq \sqrt{|J|}$ for axially symmetric black holes.
description: 7 pages, 1 figure
Il lato gamma della Luna
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

L'Astronomy Picture of the Day della NASA di oggi è un'immagine della Luna ai raggi gamma, costruita con i dati rilevati nei primi sette anni di operatività e osservazioni (2008-2015) dal Large Area Telescope a bordo di Fermi, l'osservatorio spaziale della NASA dedicato allo studio della radiazione gamma di alta e altissima energia, cui l’Italia collabora con ASI, INAF e INFN
title: Ð­ÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¾ÑÑ Ð¾Ð´Ð¾Ð²
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ÐµÑÑÑÐ¾Ð²Ð°, ÐÑÐµÐ½Ð¸Ñ
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¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ°Ð±Ð¾ÑÑ
Ð¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÐµ Ð¾ÑÑ Ð¾Ð´Ñ
ÑÑÐ¸Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
Ð²ÑÐ¾ÑÐ¸ÑÐ½Ð¾Ðµ ÑÑÑÑÐµ

description: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ Ð¾ÑÑÐ¾Ð´Ð¾Ð² ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¸Ð½Ð´ÑÑÑÑÐ¸Ð¸, ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ð¼ Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ñ ÑÑÐµÑÐ¾Ð¼ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¼Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¼ÑÑÐ¾ÑÐ° Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð²ÑÐ¾ÑÐ¸ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÑ. Ð ÑÐ²ÑÐ·Ð¸ Ñ ÑÑÐ¸Ð¼ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÑÐ¸Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¼ÑÑÐ¾ÑÐ°, Ð²ÑÑÐ²Ð»ÑÑÑÑÑ Ð¸Ñ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð¸ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸. ÐÐ·ÑÑÐµÐ½Ð¸Ðµ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¾ÑÑÐ¾Ð´Ð¾Ð² ÑÐ°Ð·Ð³ÑÐ°Ð½Ð¸ÑÐ¸Ð²Ð°ÐµÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÐ¼ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°Ð¼, ÑÑÐµÐ¿ÐµÐ½ÑÐ¼ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð½Ð° Ð¾ÐºÑÑÐ¶Ð°ÑÑÑÑ ÑÑÐµÐ´Ñ Ð¸ Ð´ÑÑÐ³Ð¸Ð¼ ÐºÑÐ¸ÑÐµÑÐ¸ÑÐ¼. Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ñ Ñ Ð¾ÑÑÐ¾Ð´Ð°Ð¼Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÑÑÐµÐ±ÑÐµÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐµÐ³Ð¾ ÑÐµÐ¼Ð¿Ð°Ð¼ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¾ÑÑÐ°ÑÐ»Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸ÑÐ¼ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð°, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð½Ð° ÑÐ»ÑÑÑÐµÐ½Ð¸Ðµ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸.
Perché non siamo soli nell’Universo
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

È praticamente ovvio che esistano altre forme di vita. Lo dice uno studio appena pubblicato su Astrobiology e che prova a ridisegnare i limiti all’unicum di una civiltà sviluppata come quella umana all’interno della Galassia e dell’Universo. Risultato: è già accaduto miliardi di volte
59Co and 75As NMR Investigation of the Lightly Doped Ba[Fe(1-x)Co(x)]2As2 (x =0.02, 0.04)
Creators: name: Ning, F. L.
name: Ahilan, K.
name: Imai, T.
name: Sefat, A. S.
name: Jin, R.
name: McGuire, M. A.
name: Sales, B. C.
name: Mandrus, D.
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 investigate the electronic properties of Ba[Fe(1-x)Co(x)]2As2 (x =0.02, 0.04) in the lightly electron-doped regime by 59Co and 75As NMR. We demonstrate that Co doping significantly suppresses the magnetic ordering temperature to the SDW state, T_{SDW}. Furthermore, ordered moments below T_{SDW} exhibit large distribution. Strong spin fluctuations remain even below T_{SDW}, persisting all the way down to 4.2 K. We find no signature of additional freezing of spin degrees of freedom unlike the case of the lightly hole-doped stripe phase of the cuprates.
description: 4 figures are changed to color online. 4 pages
JWST: un gioiello di specchio
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

Il James Webb Space Telescope, destinato a diventare il successore scientifico del beneamato telescopio spaziale Hubble, presto entrerà nelle fasi di test in vista del lancio, previsto per il 2018. A Greenbelt, Maryland, nella camera pulita del Goddard Space Flight Center's della NASA gli ingegneri hanno scoperto l’enorme specchio primario del telescopio, formato da 18 specchi più piccoli, tutti ricoperti di un sottile strato d’oro. Sarà lo specchio più grande fino ad ora lanciato nello spazio
Metallicity of low-mass stars in Orion
Creators: name: D'Orazi, V.
name: Randich, S.
name: Flaccomio, E.
name: Palla, F.
name: Sacco, G. G.
name: Pallavicini, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Determining the metal content of low-mass members of young associations provides a tool that addresses different issues, such as triggered star formation or the link between the metal-rich nature of planet-host stars and the early phases of planet formation. The Orion complex is a well known example of possible triggered star formation and is known to host a rich variety of proto-planetary disks around its low-mass stars. Available metallicity measurements yield discrepant results. We analyzed FLAMES/UVES and Giraffe spectra of low-mass members of three groups/clusters belonging to the Orion association. Our goal is the homogeneous determination of the metallicity of the sample stars, which allows us to look for [Fe/H] differences between the three regions and for the possible presence of metal-rich stars. Nine members of the ONC and one star each in the $λ$ Ori cluster and OB1b subgroup were analyzed. After the veiling determination, we retrieved the metallicity by means of equivalent widths and/or spectral synthesis using MOOG. We obtain an average metallicity for the ONC [Fe/H]=-0.01\pm 0.04. No metal-rich stars were detected and the dispersion within our sample is consistent with measurement uncertainties. The metallicity of the $λ$ Ori member is also solar, while the OB1b star has an [Fe/H] significantly below the ONC average. If confirmed by additional [Fe/H] determinations in the OB1b subgroup, this result would support the triggered star formation and the self-enrichment scenario for the Orion complex.
description: 13 pages, accepted for publication in A&A
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ¾ÑÐ¿ÑÑÂ»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ½Ð¸ÑÐ¾Ð², ÐÐ¸ÑÐ°Ð¸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: 2016
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
ÑÑÐ°Ð½Ð¾ÑÐ½Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐµÐ¶ÑÑÐ¸Ð¹ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ
ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ
Ð¿ÑÐ¸Ð¿ÑÑÐº Ð½Ð° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÑ
ÑÑÐ°Ð½Ð¾ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ðµ
ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ðµ
technological progress
machine tools
cutting tools
cutting conditions
allowance for processing
machine tool accessories
control and measuring device

description: ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ¾ÑÐ¿ÑÑÂ». Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐ»Ð¸ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸, ÑÑÐµÐ±ÑÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ Ð² Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ. ÐÑÐ±ÑÐ°Ð½ Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¸ÑÑÐ¾Ð´Ð½Ð¾Ð¹ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ, ÑÐµÐ¶ÑÑÐ¸Ð¹ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¸ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ ÑÑÐ°Ð½Ð¾ÑÐ½Ð¾Ðµ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð½Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ.
description: Analyzed the purpose of the part ""Case ". Formulated goals and objectives to be addressed in the Capstone project. Selected and justified the method of producing metal blanks, hardware, cutting tools. Designed special machine tools and measuring devices. Proposed technological process of machining of the workpiece. The calculated cutting conditions and made the rationing process works.
Titano: oceano di metano purissimo
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

Avrebbero scommesso su un gigantesco bacino di etano. E invece, dopo aver controllato e ricontrollato i dati raccolti dalla sonda NASA Cassini, gli scienziati hanno dovuto ammettere che il Ligeia Mare è costituito da metano purissimo. Ma i conti non tornano
Amide hydrolysis in vitamin B12
Creators: name: Raleigh, James Arthur
Publisher: name: University of British Columbia
Year: 2011

description: Six alicyclic amides which simulate the steric environment of the amide groupings in vitamin B12 have been prepared and their rates of alkaline hydrolysis compared on the basis of second order apparent rate constants. In addition, vitamin B12b, a simple derivative of vitamin B12, has been prepared and hydrolyzed under the same conditions as for the model compounds.
Civil society, social capital and the churches: HIV/AIDS in Papua New Guinea
Creators: name: Luker, Vicki
Publisher: name: Canberra, ACT: State, Society and Governance in Melanesia (SSGM) Program, The Australian National University
Year: 2004
Subjects: social capital
churches
HIV/AIDS care and prevention
Papua New Guinea
civil society

description: The churches are crucial actors in the response to Papua New Guineas growing problem with HIV/AIDS, but often they excite ambivalence. While several have led the way in supporting people affected by HIV, Christianity tends to be identified with teachings about sexuality and an opposition to condoms that many people involved with prevention deplore. In this paper I try to move beyond the glib assessment that the churches are bad at prevention, good at care. I frame HIV/AIDS in terms of development, and broadly conceptualise the activities that can affect the course and impacts of the epidemic. Without venturing far into theoretical debates surrounding civil society and social capital, I use these concepts or ideas associated with them - to think about the churches. Although they are major institutions in PNG and other Pacific Island countries, very little secular analysis of their contemporary social capacities and roles is available. Finally, I reflect upon the future roles of the churches in response to HIV/AIDS. These parting thoughts have some bearing on general issues concerning the role of churches in development.
A new light boson from MAGIC observations?
Creators: name: Roncadelli, Marco
name: De Angelis, Alessandro
name: Mansutti, Oriana
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Recent detection of blazar 3C279 by MAGIC has confirmed previous indications by H.E.S.S. that the Universe is more transparent to very-high-energy gamma rays than currently thought. This circumstance can be reconciled with observations of nearby blazars provided that photon oscillations into a very light Axion-Like Particle occur in extragalactic magnetic fields. The emerging "DARMA scenario" can be tested in the near future by the satellite-borne Fermi LAT detector as well as by the ground-based Imaging Atmospheric Cherenkov Telescopes H.E.S.S., MAGIC, CANGAROO III, VERITAS and by the Extensive Air Shower arrays ARGO-YBJ and MILAGRO.
description: 4 pages, 1 figure, Proceeding of the "Neutrino Oscillation Workshop", Conca Specchiulla, Otranto, Italy, 6-12 September 2008
title: ÐÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐºÐ°Ñ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ° Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐµÐ¿Ð¾Ð²Ð° , ÐÐ»ÑÐ³Ð°
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´ÐµÑÑÐºÐ°Ñ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ° Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸
ÐºÐ½Ð¸Ð¶ÐºÐ°-ÐºÐ°ÑÑÐ¸Ð½ÐºÐ°
Ð¸Ð»Ð»ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÑÐ´Ð½Ð¾ÑÑÐ¸ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð°

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐµ Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾ -ÑÐ²Ð¾ÑÑÐµÑÑÐ²Ñ Ð´ÐµÑÑÐºÐ¸Ñ Ð¿Ð¸ÑÐ°ÑÐµÐ»ÐµÐ¹ Ð¸ Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¾ÑÐ¾Ð². Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ ÑÑÐ°Ð¿Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´ÐµÑÑÐºÐ¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸, Ð¸Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ Ð²Ð°Ð¶Ð½ÑÐµ Ð¾ÑÐ»Ð¸ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐµÑÑÑ. Ð¢Ð°ÐºÐ¶Ðµ Ð¾ÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ ÑÐ²Ð¾ÑÑÐµÑÑÐ²Ñ ÐºÐ¾Ð½ÐºÑÐµÑÐ½ÑÑ Ð°Ð²ÑÐ¾ÑÐ¾Ð², Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¿Ð¾Ð¿ÑÐ»ÑÑÐ½ÑÑ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð² Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸, Ð½Ð¾ Ð¸ Ð·Ð° ÑÑÐ±ÐµÐ¶Ð¾Ð¼. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÐºÐ¶Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð°Ð²ÑÐ¾ÑÐ°Ð¼-Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¾ÑÐ°Ð¼, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿Ð¸ÑÑÑ ÑÐºÐ°Ð·ÐºÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð»Ð»ÑÑÑÑÐ¸ÑÑÑÑ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð¸ÑÑÑ ÑÐµÐºÑÑ Ð¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑ ÑÐ½Ð¾Ð¼Ñ ÑÐ¸ÑÐ°ÑÐµÐ»Ñ Ð¿Ð¾Ð·Ð½Ð°ÐºÐ¾Ð¼Ð¸ÑÑÑÑ Ñ Ð³ÐµÑÐ¾ÑÐ¼Ð¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿ÐµÑÐµÐ²Ð¾Ð´ÑÐ¸ÐºÐ¾Ð², Ð¸Ð¼ÐµÑÑÐ¸Ñ Ð½ÐµÐ¿Ð¾ÑÑÐµÐ´ÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ðµ Ðº ÑÐ¾Ð¼Ñ, ÐºÐ°Ðº Ð±ÑÐ´ÐµÑ Ð¾ÑÐµÐ½ÐµÐ½Ð¾ ÑÐ¾ Ð¸Ð»Ð¸ Ð¸Ð½Ð¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÐ¼Ð¸ ÑÐ¸ÑÐ°ÑÐµÐ»ÑÐ¼Ð¸.
Echi di luce per misurare dischi protoplanetari
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Un team di ricercatori guidato da Huang Meng, post-doc dell’Università dell’Arizona, è riuscito a misurare per via indiretta la distanza tra una giovane stella e il disco di polveri e gas che la circonda, da cui potrebbero formarsi nuovi pianeti. Con il commento di Davide Fedele (INAF)
Canonical ADM Tetrad Gravity: from Metrological Inertial Gauge Variables
  to Dynamical Tidal Dirac observables
Creators: name: Lusanna, Luca
Publisher: name: INFN Open Access Repository
Year: 2014

description: Dirac constraint theory allows to identify the York canonical basis
(diagonalizing the York-Lichnerowicz approach) in ADM tetrad gravity for
asymptotically Minkowskian space-times without super-translations. This allows
to identify the inertial (gauge) and tidal (physical) degrees of freedom of the
gravitational field and to interpret Ashtekar variables in these space-times.
The use of radar 4-coordinates centered on a time-like observer allows to
connect the 3+1 splittings of space-time with the relativistic metrology used
in atomic physics and astronomy. The asymptotic ADM Poincar\'e group replaces
the Poincar\'e group of particle physics. The general relativistic remnant of
the gauge freedom in clock synchronization is described by the inertial gauge
variable ${}^3K$, the trace of the extrinsic curvature of the non-Euclidean
3-spaces. The theory can be linearized in a Post-Minkowskian way by using the
asymptotic Minkowski metric as an asymptotic background at spatial infinity and
the family of non-harmonic 3-orthogonal Schwinger time gauges allows to
reproduce the known results on gravitational waves in harmonic gauges. It is
shown that the main signatures for the existence of dark matter can be
reinterpreted as an relativistic inertial effect induced by ${}^3K$: while in
the space-time inertial and gravitational masses coincide (equivalence
principle), this is not true in the non-Euclidean 3-spaces (breaking of Newton
equivalence principle), where the inertial mass has extra ${}^3K$-dependent
terms simulating dark matter. Therefore a Post-Minkowskian extension of the
existing Post-Newtonian celestial reference frame is needed.
Corrected Entropy of Friedmann-Robertson-Walker Universe in Tunneling Method
Creators: name: Zhu, Tao
name: Ren, Ji-Rong
name: Li, Ming-Fan
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this paper, we study the thermodynamic quantities of Friedmann-Robertson-Walker (FRW) universe by using the tunneling formalism beyond semiclassical approximation developed by \emph{Banerjee} and \emph{Majhi}\cite{beyond0}. For this we first calculate the corrected Hawking-like temperature on apparent horizon by considering both scalar particle and fermion tunneling. With this corrected Hawking-like temperature, the explicit expressions of the corrected entropy of apparent horizon for various gravity theories including Einstein gravity, Gauss-Bonnet gravity, Lovelock gravity, $f(R)$ gravity and scalar-tensor gravity, are computed. Our results show that the corrected entropy formula for different gravity theories can be written into a general expression (\ref{entropy-final}) of a same form. It is also shown that this expression is also valid for black holes. This might imply that the expression for the corrected entropy derived from tunneling method is independent of gravity theory, spacetime and dimension of the spacetime. Moreover, it is concluded that the basic thermodynamical property that the corrected entropy on apparent horizon is a state function is satisfied by the FRW universe.
description: 25 pages, no figure, and comments are welcome; v2:27 pages, more references added and typoes corrected, accepted for publication in JCAP