cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ° Ð¼ÐµÑ Ð°Ð½Ð¾Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»ÐµÐ¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð Ð°Ð¶ÐµÐ²Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸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: 2017
Subjects: ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
ÐÐ¸Ð±ÐºÐ¸Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð² Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐµ
Ð¡ÐºÐ»Ð°Ð´ÑÐºÐ¾Ðµ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð¾
Ð¼ÐµÑ Ð°Ð½Ð¾Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ° Ð´ÐµÑÐ°Ð»ÐµÐ¹
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÑÐ°ÑÑÐºÐ¸
Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÑÐ°ÑÑÐºÐ¾Ð²
Ð¼Ð¸ÐºÑÐ¾Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾-ÑÐºÐ»Ð°Ð´ÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ

description: Ð¡Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¸ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð° Ð¼Ð¸ÐºÑÐ¾Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð¹ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾-ÑÐºÐ»Ð°Ð´ÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ (ÐÐ¢Ð¡Ð¡) ÑÑÐ°ÑÑÐºÐ°, ÐºÐ°Ðº ÐµÐµ ÑÐ¾ÑÑÐ°Ð²Ð½Ð¾Ð¹ ÑÐ°ÑÑÐ¸; ÑÐ°ÑÐ°ÐºÑÐµÑÐ½Ð¾Ð¹ Ð½Ð¾Ð¼ÐµÐ½ÐºÐ»Ð°ÑÑÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÐÐ¢Ð¡Ð¡ Ð³Ð¸Ð±ÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ (ÐÐÐ¡) Ð¼ÐµÑÐ°Ð½Ð¾Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸; ÑÐ¾ÑÑÐ°Ð²Ð° Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ°ÑÑÐµÑÐ° Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°ÑÐ¸Ð¸ (ÐÐ) ÐÐÐ¡ Ð¼ÐµÑÐ°Ð½Ð¾Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸.
CO J=1-0 observations of molecular gas interacting with galactic supernova remnants G5.4-1.2, G5.55+0.32 and G5.71-0.08
Creators: name: Liszt, H. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The field just West of the galactic supernova remnant W28 (l=6.4\degr, b=-0.2\degr) harbors 3 of 5 newly-discovered 1720 OH maser spots and two recently-discovered candidate supernova candidates (one of which is a $γ$-ray source), as well as several compact and classical HII regions. Here, we analyze a datacube of CO J=1-0 emission having 1\arcmin and 1 \kms resolution, made with on-the-fly mapping over the region $5\degr \le l \le 6\degr, -1\degr \le b \le 0.5\degr$}. {Extended and often very bright CO emission was detected at the velocities of the 1720 MHz OH masers and around the supernova remnant G5.55+0.32 which lacks a maser. A new bipolar outflow which is marginally resolved at 1\arcmin resolution and strong in CO (12K) was detected at the periphery of G5.55+0.32, coincident with an MSX source; there is also a bright rim of CO just beyond the periphery of the radio remnant. The OH maser near G5.71-0.08 lies on a shell of strongly-emitting molecular gas (up to 20K) . At the -21 \kms velocity of G5.4-1.2, CO covers much of the field but is weak (3 K) and undisturbed near the remnant. The extended molecular gas around the compact H II region and outflow in G5.89-0.39 (W28A2) is shown for the first time.}
description: 6 Pages, 3 figures submitted to A&A 4 May 2009
Sogni voi dite? No signori, realtà, realtà!
Creators: Caterina Boccato
Publisher: name: Media Inaf
Year: 2014

Il 14 ottobre si apre a Padova una mostra organizzata da ASI e INAF che ha come protagonista la sonda Rosetta. Per inaugurarla, un convegno dedicato a Bepi Colombo, matematico padovano a cui l'esplorazione spaziale deve molto
Olimpiadi Astronomia: si parte
Creators: Gaetano Valentini
Publisher: name: Media Inaf
Year: 2014

Sabato prossimo la rappresentativa italiana partirà per la Repubblica del Kyrgyzstan per partecipare alle XIX Olimpiadi Internazionali di Astronomia, che si concluderanno con la cerimonia di premiazione il 20 ottobre. Le tre prove olimpiche (teorica, osservativa e pratica) si effettueranno nella località di Cholpon-Ata, situata a Nord-Est del territorio kirgizo sulle sponde del lago Issyk Kul
Supernova Light Curves Powered by Young Magnetars
Creators: name: Kasen, Daniel
name: Bildsten, Lars
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We show that energy deposited into an expanding supernova remnant by a highly magnetic (B ~ 5 x 10^14 G) neutron star spinning at an initial period of P ~ 2-20 ms can substantially brighten the light curve. For magnetars with parameters in this range, the rotational energy is released on a timescale of days to weeks, which is comparable to the effective diffusion time through the supernova remnant. The late time energy injection can then be radiated without suffering overwhelming adiabatic expansion losses. The magnetar input also produces a central bubble which sweeps ejecta into an internal dense shell, resulting in a prolonged period of nearly constant photospheric velocity in the observed spectra. We derive analytic expressions for the light curve rise time and peak luminosity as a function of B, P and the properties of the supernova ejecta that allow for direct inferences about the underlying magnetar in bright supernovae. We perform numerical radiation hydrodynamical calculations of a few specific instances and compare the resulting light curves to observed events. Magnetar activity is likely to impact more than a few percent of all core collapse supernovae, and may naturally explain some of the brightest events ever seen (e.g., SN 2005ap and SN 2008es) at L > 10^44 ergs/s.
description: 5 pages, submitted to ApJ
title: ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð°ÑÐ²ÐµÑÐ´ÐµÐ²Ð°Ð½Ð¸Ñ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð¼, ÐÑÑÐµÐ¼
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´ÐµÐ½Ð´ÑÐ¸ÑÐ½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ°
ÑÑÐ°ÑÐ¸Ð¾Ð½Ð°ÑÐ½ÑÐ¹ Ð¸ Ð½ÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð°ÑÐ½ÑÐ¹ ÑÐµÐ¶Ð¸Ð¼
ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·
ÑÑÑÑÐºÑÑÑÐ½ÑÐ¹ Ð¿ÐµÑÐµÑ Ð¾Ð´

description: ÐÑÐ¾ÑÐµÑÑ Ð¿ÐµÑÐ²Ð¸ÑÐ½Ð¾Ð¹ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° ÑÐ²ÐµÑÐ´ÑÑ ÑÐµÐ». Ð¤Ð¾ÑÐ¼Ð¸ÑÑÑÑÐ°ÑÑÑ Ð¼Ð°ÐºÑÐ¾ÑÑÑÑÐºÑÑÑÐ° Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑÑÑ ÑÐºÐ¾ÑÐ¾ÑÑÑÑ Ð¾ÑÐ»Ð°Ð¶Ð´ÐµÐ½Ð¸Ñ, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¾Ð¼ Ð¸ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾Ð¼ Ð¿ÑÐ¸Ð¼ÐµÑÐµÐ¹. Ð Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¼ ÑÐ¾ÑÐ¼Ð° ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð² Ð½Ð°Ð¿Ð¾Ð¼Ð¸Ð½Ð°ÐµÑ ÑÐ°Ð·Ð²ÐµÑÐ²Ð»ÐµÐ½Ð½ÑÐµ, Ð´ÑÐµÐ²Ð¾Ð²Ð¸Ð´Ð½ÑÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿Ð¾Ð»ÑÑÐ¸Ð»Ð¸ Ð½Ð°Ð·Ð²Ð°Ð½Ð¸Ðµ Ð´ÐµÐ½Ð´ÑÐ¸ÑÐ¾Ð². ÐÐµÐ½Ð´ÑÐ¸ÑÐ½Ð¾Ðµ ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ½Ð¾ Ð´Ð»Ñ Ð¼Ð°ÐºÑÐ¾- Ð¸ Ð¼Ð¸ÐºÑÐ¾ - ÑÑÑÑÐºÑÑÑÑ Ð»Ð¸ÑÐ¾Ð³Ð¾ Ð¼ÐµÑÐ°Ð»Ð»Ð° Ð¸ Ð¾Ð½Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ, ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð´ÑÑÐ³Ð¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° ÑÐ»Ð¸ÑÐºÐ¾Ð² Ð¸ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº. ÐÐ´Ð½Ð°ÐºÐ¾ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°ÑÐ¸ ÑÑÑÑÐºÑÑÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´ÑÑÐ¾Ð¸Ñ Ð²ÑÑÑÐ½Ð¸ÑÑ ÑÐµÐ»ÑÐ¹ ÑÑÐ´ Ð¼Ð°Ð»Ð¾Ð¸Ð·ÑÑÐµÐ½Ð½ÑÑ Ð´Ð¾ ÑÐ¸Ñ Ð¿Ð¾Ñ ÑÑÐ¾ÑÐ¾Ð½ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸ - ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð¿ÐµÑÐµÑÐ¾Ð´Ð° Ð´ÐµÐ½Ð´ÑÐ¸ÑÐ½Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÑ Ð¾Ñ ÑÑÐ¾Ð»Ð±ÑÐ°ÑÐ¾Ð¹ Ðº ÑÐ°Ð²Ð½Ð¾Ð¾ÑÐ½Ð¾Ð¹ Ð¼Ð¾ÑÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸.
Some No-go Theorems for String Duals of Non-relativistic Lifshitz-like Theories
Creators: name: Li, Wei
name: Nishioka, Tatsuma
name: Takayanagi, Tadashi
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study possibilities of string theory embeddings of the gravity duals for non-relativistic Lifshitz-like theories with anisotropic scale invariance. We search classical solutions in type IIA and eleven-dimensional supergravities which are expected to be dual to (2+1)-dimensional Lifshitz-like theories. Under reasonable ansaetze, we prove that such gravity duals in the supergravities are not possible. We also discuss a possible physical reason behind this.
description: 18 pages, Latex, flux conditions clarified (v2), brief summary of results added (v3)
The Blaimore formation of southern Saskatchewan
Creators: name: Rousell, Don Herbert
Publisher: name: University of British Columbia
Year: 2012

description: Rocks of the Lower Cretaceous Blairmore formation extend over the whole of southern Saskatchewan. Along outcrop areas in western Manitoba, the Blairmore has undergone erosional truncation. Equivalent beds are found over almost the entire western interior plains of Canada and the United States. in southern Saskatchewan and adjacent western Manitoba the formation consists principally of fine to coarse quartzose sandstone, shale, salt and pepper sandstone, lignite, clay ironstone, kaolinite shale, and various mixtures of shaly sandstone and sandy shale. The Blairmore of the area is divided into five areal units and related to adjacent, more thoroughly studied areas. The divisions are: Mannville, Kootenai, Dakota, Swan River, and Ashville areas. The stratigraphy of each area is described and environment and source areas discussed. Oil in commercial quantities has been found in the Blairmore formation. The most likely areas of future exploration are suggested.
Reionizzazione? Chiedi alle galassie vicine
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2014

Una galassia in piena fase di formazione stellare nell'universo vicino potrebbe avere molte caratteristiche in comune con quelle primordiali che avrebbero permesso la reionizzazione dell'universo circa tredici miliardi di anni fa. Il commento di Eros Vanzella (INAF)
title: Ð£ÑÐµÑ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð°
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¾Ð»Ð¾Ð²ÑÐ¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸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: ÑÑÐµÑ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·
ÐºÐ°Ð¿Ð¸ÑÐ°Ð»

description: Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð°Ñ Ð±Ð°Ð·Ð° Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð°. ÐÑÐ¾ÑÐ°Ñ Ð³Ð»Ð°Ð²Ð° ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÑÑ ÑÐ°Ð±Ð¾ÑÑ, ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð°, Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð°, Ð°Ð½Ð°Ð»Ð¸Ð· Ð½Ð°Ð»Ð¸ÑÐ¸Ñ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ, ÑÐµÐ·ÐµÑÐ²Ñ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð° Ð¿Ð¾ ÐÐÐ Â«ÐÐ°Ð»ÑÐ¸Ð¹ÑÐºÐ°Ñ ÐÐ¾Ð¼Ð¿Ð°Ð½Ð¸ÑÂ». Ð¢ÑÐµÑÑÑ Ð³Ð»Ð°Ð²Ð° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð° Ð¸ÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð¼ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾-Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐ°Ð»ÑÐ¸Ð½Ð³Ð° Ð² Ð¸Ð½ÑÐµÑÐµÑÐ°Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 08.00.05 "Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð¾Ð¼ (ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸ÑÐ¼Ð¸)"
titleType: Subtitle
Creators: name: ÐÐ°Ð»ÐµÐ±Ð½Ð¸ÐºÐ¾Ð²Ð°, 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: 2020
Subjects: ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¹ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»
Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾-Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ ÐºÐ¾Ð½ÑÐ°Ð»ÑÐ¸Ð½Ð³
Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¸

description: ÐÐ¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾-Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐ°Ð»ÑÐ¸Ð½Ð³Ð° Ð² ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð¼ Ð² Ð¸Ð½ÑÐµÑÐµÑÐ°Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¾Ð»Ð¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹ Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð¼. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾-Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐ°Ð»ÑÐ¸Ð½Ð³Ð° Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½ Ð½Ð°Ð±Ð¾Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð², Ð²ÑÐ¾Ð´ÑÑÐ¸Ñ Ð² Ð½ÐµÐ³Ð¾.Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÑÐ¾Ð²Ð½ÐµÐ¹ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¸ÑÑÐµÐ¼Ð° Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð²ÑÑÐµÑÐ¿Ð¾Ð¼ÑÐ½ÑÑÑÑ ÑÑÐ¾Ð²Ð½ÐµÐ¹. ÐÐ°ÑÑÑÑ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿Ð¾ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐ¼ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼.
The Lyapunov Characteristic Exponents and their computation
Creators: name: Skokos, Charalampos
Publisher: name: arXiv
Year: 2008
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: Astrophysics (astro-ph)
subject: Mathematical Physics (math-ph)
subject: Dynamical Systems (math.DS)
subject: Numerical Analysis (math.NA)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We present a survey of the theory of the Lyapunov Characteristic Exponents (LCEs) for dynamical systems, as well as of the numerical techniques developed for the computation of the maximal, of few and of all of them. After some historical notes on the first attempts for the numerical evaluation of LCEs, we discuss in detail the multiplicative ergodic theorem of Oseledec \cite{O_68}, which provides the theoretical basis for the computation of the LCEs. Then, we analyze the algorithm for the computation of the maximal LCE, whose value has been extensively used as an indicator of chaos, and the algorithm of the so--called `standard method', developed by Benettin et al. \cite{BGGS_80b}, for the computation of many LCEs. We also consider different discrete and continuous methods for computing the LCEs based on the QR or the singular value decomposition techniques. Although, we are mainly interested in finite--dimensional conservative systems, i. e. autonomous Hamiltonian systems and symplectic maps, we also briefly refer to the evaluation of LCEs of dissipative systems and time series. The relation of two chaos detection techniques, namely the fast Lyapunov indicator (FLI) and the generalized alignment index (GALI), to the computation of the LCEs is also discussed.
description: 74 pages, 8 figures, accepted for publication in Lecture Notes in Physics
LHC: due nuove particelle
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2014

Nome scientifico DS3*(2860)– e DS1*(2860)– per le due particelle rilevate dall’esperimento LHCb nel gigantesco laboratorio sotterraneo del Large Hadron Collider al CERN di Ginevra: tre volte più massicce dei comuni protoni e con proprietà mai osservate prima
Demystifying ionic and electronic transport in prominent oxide ion and proton conducting ceramic electrolytes: Ce0.8Sm0.2O2 and BaCe0.7Zr0.1Y0.1Yb0.1O3-δ
Creators: name: Bello, Idris Temitope
name: Ni, Meng
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Biophysics
subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Developmental Biology

description: The development and performance of ceramic electrochemical cells (CECs) depend critically on choosing ceramic electrolytes with optimal ionic and electronic transport properties. In this study, we compare the structural, morphological, and transport characteristics of two representative ceramic electrolytes, oxide ion conducting Ce0.8Sm0.2O2 (SDC) and proton conducting BaCe0.7Zr0.1Y0.1Yb0.1O3-δ (BCZYYb). We demonstrate that SDC exhibits higher bulk conductivity but lower open-circuit voltage due to its higher electron density and larger crystallite size. In contrast, BCZYYb possesses higher proton conduction, lower activation energy (0.35–0.38 eV), and higher open-circuit voltage due to its lower electron density and smaller crystallite size with more grain boundaries. BCZYYb shows enhanced proton conductivity in humidified atmospheres due to the hydration of oxygen vacancies, making it more suitable for low-temperature CEC applications. These insights into ceramic electrolyte conduction mechanisms and microstructure-property relationships can guide the optimization of CECs for energy applications.
Il volto scavato di Lutetia
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2014

Uno studio pubblicato questa settimana sulla rivista Planetary and Space Science ricostruisce le sembianze, ovvero la forma, dell’asteroide Lutetia. Lo studio è stato realizzato grazie ai dati raccolti durante il passaggio della sonda Rosetta vicino all’asteroide e dalla “messa a sistema” di queste immagini con le osservazioni effettuate da terra
title: Ð Ð°ÑÑÐµÑ Ð´Ð²ÑÑ Ð·Ð²ÐµÐ½Ð½Ð¾Ð¹ ÑÑÑÐ¿ÐµÐ½Ð¸ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð¶ÑÑÐ¾Ð², Ð®ÑÐ¸Ð¹
name: Ð¢ÑÑÐ¸Ð½Ð°, ÐÑÐ¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2014
Subjects: ÐÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÑ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½ÑÐµ

description: Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÑ ÑÐ°ÑÑÐµÑÐ° Ð¾Ð±ÑÐµÐ¹ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾Ð¼ÑÑÂ­Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ°: Ð²ÑÐ±Ð¾Ñ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° ÑÑÑÐ¿ÐµÐ½ÐµÐ¹, ÐºÐ¾Ð»Ð¸ÑÐµÂ­ÑÑÐ²Ð° Ð³Ð°Ð·Ð¾Ð¾ÑÐ»Ð°Ð´Ð¸ÑÐµÐ»ÐµÐ¹. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ°ÑÑÐµÑÐ° ÑÐµÑÐµÐ½Ð¸Ñ Ð² Ð¼ÐµÑÐ¸Ð´Ð¸Ð¾Â­Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¸ ÑÐ°Ð´Ð¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐºÐ¾ÑÑÑÑ ÑÐ°Ð±Ð¾ÑÐµÐ³Ð¾ ÐºÐ¾Ð»ÐµÑÐ° Ð¸ Ð»Ð¾Ð¿Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð´Ð¸ÑÑÑÐ·Ð¾ÑÐ° ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ°. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð³Ð°Ð·Ð° Ð² Ð´Ð²ÑÑÐ·Ð²ÐµÐ½Ð½Ð¾Ð¹ ÑÑÑÐ¿ÐµÐ½Ð¸ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿ÑÐµÑÂ­ÑÐ¾ÑÐ°. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»ÑÐ¼ Â«ÐÐ°ÐºÑÑÐ¼Ð½Ð°Ñ Ð¸ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ½Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ°Â» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾Â­ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² 151000 Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÂ», Â«ÐÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ½ÑÐµ Ð¸ ÑÐ¾Ð»Ð¾Ð´Ð¸Ð»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸Â» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Â­Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² 141100 Â«Ð­Ð½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ», Ð° ÑÐ°Ðº Ð¶Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð°ÑÑÐ½ÑÑ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² 05.04.06 Â«ÐÐ°ÐºÑÑÐ¼Ð½Ð°Ñ, ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ½Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ° Ð¸ Ð¿Ð½ÐµÐ²Ð¼Ð¾ÑÐ¸ÑÑÐµÐ¼ÑÂ».
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°.
Homogeneous comparison of planet candidates imaged directly until 2008
Creators: name: Schmidt, T. O. B.
name: Neuhäuser, R.
name: Seifahrt, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a compilation of the planet candidates currently known from direct imaging. We have gathered available data from the literature and derive the luminosity of all candidates in a homogeneous way using a bolometric correction, the distances and the K band magnitudes of the objects. In a final step we find the masses of the candidates from a comparison of the luminosity or, if not available, an absolute brightness and several well known hot-start evolutionary models.
description: 4 pages, 1 figure, Proceedings of the 2nd Subaru International Conference on Exoplanets and Disks: Their Formation and Diversity, Keauhou - Hawaii - USA, 9-12 March 2009; 2nd version: Several typos corrected
The shape of nearby Open Clusters
Creators: name: Tarricq, Yoann
name: Casamiquela, Laia
name: Soubiran, Caroline
Publisher: name: Zenodo
Year: 2019
Subjects: open clusters, solar neighborhood

description: We use new memberships from Gaia DR2 to investigate the shape of the nearest open clusters. We investigate their 2D distribution projected on the sky and fit two gaussians components on the central part and external envelope. For open clusters closer than 200 pc from the Sun, we fit 3D ellipsoids on the spatial distribution of the members. We look for correlations of the spatial properties with age and galactic environment.
De Rham theory of exploded manifolds
Creators: name: Parker, Brett
Publisher: name: arXiv
Year: 2010
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics

description: This paper extends de Rham theory of smooth manifolds to exploded manifolds. Included are versions of Stokes' theorem, De Rham cohomology, Poincare duality, and integration along the fiber. The resulting cohomology theory is used to define Gromov Witten invariants of exploded manifolds in a separate paper.
description: 57 pages. v4: Post-publication update fixing an error in the computation of compactly supported cohomology of a coordinate chart. An additional assumption that a polytope was simplicial at infinity was required. As a consequence, this additional assumption is also required for the integration pairing to be a perfect pairing. See Appendix for further details
Nucleus-nucleus reaction cross-sections for deformed nuclei
Creators: name: Hassan, M. Y. M.
name: Farag, M. Y. H.
name: Abul-Magd, A. Y.
name: Nassar, T. E. I.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Reaction cross-sections are calculated using the Coulomb modified Glauber model for deformed target nuclei. The deformed nuclear matter density of the target is expanded into multipoles of order k = 0,2,4.The reaction cross-sections between some spherical and deformed nuclei are studied at energy range (10-1000 MeV/nucleon). The most significant effects in the intermediate energy range are the Coulomb field and in-medium effect that modified the trajectory of the incident beams. Introducing the deformation effect beside the Coulomb field and in-medium effect improves the agreement with the experimental data and two empirical parameterizations in the case of not finding experimental data. Moreover it is indicated that the enhancement of the reaction cross-sections is attributed with fixed orientation in deformed nuclei.
description: 17 pages, 7 pages
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¿ÑÐ¸Ð±Ð¾ÑÐµ Ð£ÐÐ-1000
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Ð°Ð´Ð°Ð»Ð¸ÐµÐ², 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: 2018
Subjects: ÐÐ°Ð»Ð¸Ð±ÑÐ¾Ð²ÐºÐ°
ÐÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¸ Ð¿ÑÐ¸Ð±Ð¾ÑÑ
Ð¤ÑÐµÐ·ÐµÑÐ½ÑÐµ ÑÑÐ°Ð½ÐºÐ¸ Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼
ÐÐµÑÑ Ð´Ð»Ð¸Ð½Ñ ÐºÐ¾Ð½ÑÐµÐ²ÑÐµ

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÑ Ð´Ð»Ñ ÐºÐ°Ð»Ð¸Ð±ÑÐ¾Ð²ÐºÐ¸ ÐºÐ¾Ð½ÑÐµÐ²ÑÑ Ð¼ÐµÑ Ð´Ð»Ð¸Ð½Ñ, Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸, Ð¿ÑÐ¸Ð±Ð¾Ñ Ð£ÐÐ-1000 Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ¸Ð¸ Â«ÐÐ¸ÐºÑÐ¾Â». ÐÑÑÐ²Ð»ÑÑÑÑÑ ÑÐ°ÐºÑÐ¾ÑÑ, Ð²Ð»Ð¸ÑÑÑÐ¸Ðµ Ð½Ð° ÑÐ¾ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð² Ð´Ð»Ñ ÐºÐ°Ð»Ð¸Ð±ÑÐ¾Ð²ÐºÐ¸ ÐºÐ¾Ð½ÑÐµÐ²ÑÑ Ð¼ÐµÑ Ð´Ð»Ð¸Ð½Ñ. ÐÐ¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð¼ Ð£ÐÐ-1000 ÑÐ°ÑÑÑÐ¸ÑÑÐ²Ð°ÐµÑÑÑ Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÑ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹, Ð´Ð°ÐµÑÑÑ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ°. ÐÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÑÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Ð¿ÑÐ¸Ð±Ð¾ÑÐ°. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ñ Ð´Ð»Ñ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¸Ð±Ð¾ÑÐ° Ð¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ðº Ð·Ð°Ð¿ÑÑÐºÑ Ð¼ÐµÐ»ÐºÐ¾ÑÐµÑÐ¸Ð¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°.
The Smith Cloud: high-velocity accretion and dark-matter confinement
Creators: name: Nichols, M.
name: Bland-Hawthorn, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The Smith Cloud is a massive system of metal-poor neutral and ionized gas M_gas >= 2x10^6 M_sun) that is presently moving at high velocity (V_GSR ~300 km s^-1) with respect to the Galaxy at a distance of 12 kpc from the Sun. The kinematics of the cloud's cometary tail indicates that the gas is in the process of accretion onto the Galaxy, as first discussed by Lockman et al. (2008). Here, we re-investigate the cloud's orbit by considering the possibility that the cloud is confined by a dark matter halo. This is required for the cloud to survive its passage through the Galactic corona. We consider three possible models for the dark matter halo (NFW, Einasto, Burkert) including the effects of tidal disruption and ram-pressure stripping during the cloud's infall onto and passage through the Galactic disk. For the NFW and Einasto dark-matter models, we are able to determine reasonable initial conditions for the Smith Cloud, although this is only marginally possible with the Burkert model. For all three models, the progenitor had an initial (gas+dark matter) mass that was an order of magnitude higher than inferred today. In agreement with Lockman et al. (2008), the cloud appears to have punched through the disk ~70 Myr ago. For our most successful models, the baryon to dark matter ratio is fairly constant during an orbital period but drops by a factor of 2-5 after transiting the disk. The cloud appears to have only marginally survived its transit, and is unlikely to retain its integrity during the next transit ~30 Myr from now.
description: 9 pages, 7 figures. ApJ, accepted
Biologics in the treatment of active Psoriatic arthritis in China: a network meta-analysis and cost-effectiveness analysis
Creators: name: Xie, Ouyang
name: Wu, Meiyu
name: Li, Andong
name: Meng, Kehui
name: Xiang, Heng
name: Tan, Chongqing
name: Peng, Liubao
name: Ge, Yan
name: Wan, Xiaomin
Publisher: name: Taylor & Francis
Year: 2025
Subjects: Medicine
Pharmacology
Biotechnology
Biological Sciences not elsewhere classified
Science Policy

description: Biologics are recommended for use in patients with psoriatic arthritis (PsA) after the failure of conventional systemic disease-modifying anti-rheumatic drugs (csDMARDs). However, compared to csDMARDs, biologics are significantly more expensive. The aim of this study was to evaluate the cost-effectiveness of biologic treatments for active PsA patients who have failed treatment with csDMARDs, from the perspective of the Chinese healthcare system. A discrete event simulation model was constructed to estimate health and economic outcomes of patients. The seven biologics recommended by the Chinese psoriasis treatment guidelines were included in the evaluation. One-way and probabilistic sensitivity analysis were performed to ensure that our results were robust. Our results found that compared to the standard of care (SoC) and all other biologics strategies, secukinumab (SEC) had the highest quality-adjusted life years, and at a willingness-to-pay (WTP) threshold of US $38,161 per QALY, SEC was the most cost-effective option, with an incremental cost-effectiveness ratio of $14,968 per QALY. One-way sensitivity analysis and probabilistic sensitivity analysis confirmed the robust of this result. From the perspective of the Chinese healthcare system, biologics are estimated to be cost-effective compared to SoC. Among these, SEC is the most cost-effective option.
Il crollo di peso della galassia centrale
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2014

Dal movimento delle stelle nell’alone galattico un giovane ricercatore nepalese trapiantato in Australia ha calcolato che nella Via Lattea c’è molta meno materia oscura di quel che si pensava. Il che spiegherebbe anche il mistero delle galassie satelliti mancanti
A comparative study of sex role portrayals in magazine advertisements between Korea and the United States
Creators: name: Cho, Haewon
Publisher: name: The University of Texas at Austin
Year: 1993
Subjects: subject: Sex role in advertising
subject: Korea
subject: United States
subject: Magazine advertising
subject: Cross-cultural studies
subject: Sex role portrayals
subject: Korean culture
subject: American culture
subject: Korean sex roles
subject: American sex roles
subject: Sex role in advertising--Korea
subject: Sex role in advertising--United States
subject: Advertising, Magazine--Korea
subject: Advertising, Magazine--United States
subject: Sex role--Cross-cultural studies
subject: Sex role--Korea
subject: Sex role--United States

description: Sex roles are one facet of cultural characteristics which reflect the norms of a particular society. Culture has a profound effect on people's ways of life, values, and behavior. Cultural characteristics are considered to be particularly important in advertising since advertising tends to reproduce these characteristics in idealized form (Hong, Mudderrisoglu, and Zinkhan, 1987). Recently, cross-cultural researchers were concerned about the content of advertisements and analyzed how cultural differences would be presented in advertising. Many studies support a thesis that cross-cultural differences are reflected in different advertising appeals (Hornick, 1980; Unwin, 1974; Madden, Caballero and Matsukubo, 1986; Hong, Muderrisoglu and Zinkhan, 1987; Mueller, 1987; Tse, Belk and Zhou, 1989; Tansey, Hyman, and Zinkhan, 1990). Therefore, a knowledge of the impact of culture on advertising is critical in international advertising. This study attempts to determine how different sex roles from different cultures are treated in advertising. Content analysis is employed in order to compare the current status of sex role portrayals in magazine advertisements from the United States and Korea. Since the U.S. and Korea have different sex role concepts that reflect different cultures, it is expected that these different roles between the two countries are also reflected in advertising. This cross-cultural study will examine how the cultures of two societies influence portrayals of sex roles in advertising. In addition, this cross-cultural study will help us to understand cultural differences that often function as boundaries in international advertising (Cole and Bruner, 1971)
title: Ð Ð¾Ð±Ð°ÑÑÐ½Ð¾Ðµ Ð¾ÑÐµÐ½Ð¸Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ° Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½ÐµÑÐµÐ³ÑÐ»ÑÑÐ½Ð¾ÑÑ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¥Ð»ÐµÐ±Ð°Ð»Ð¸Ð½Ð°, ÐÐ°ÑÐ°Ð»Ð¸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: 2017
Subjects: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ°
Ð Ð°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ (Ð¼Ð°Ñ.)
ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
Ð¿Ð°ÑÐ°Ð¼ÐµÑÑ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ
ÑÐ¾Ð±Ð°ÑÑÐ½Ð¾ÑÑÑ

description: Ð Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð° Ð¼Ð°ÐºÑÐ¸Ð¼ÑÐ¼Ð° Ð¿ÑÐ°Ð²Ð´Ð¾Ð¿Ð¾Ð´Ð¾Ð±Ð¸Ñ Ð¸ ÐµÐ³Ð¾ Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð¸Ñ Ð² Ð²Ð¸Ð´Ðµ Ð¼ÐµÑÐ¾Ð´Ð° Ð-Ð¾ÑÐµÐ½Ð¾Ðº Ð´Ð»Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ ÑÐ¾Ð±Ð°ÑÑÐ½ÑÑ Ð²ÑÑÐ¾ÐºÐ¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð¾ÑÐµÐ½Ð¾Ðº Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ° Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð² ÑÐ»ÑÑÐ°Ðµ ÑÐ°Ð·ÑÑÐ²Ð½ÑÑ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÐµÐ¹ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ Ð´Ð°Ð½Ð½ÑÑ (ÑÑÐµÑÐµÐ½Ð½ÑÑ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹) - Ð² ÑÑÐ¾Ð¼ ÑÐ»ÑÑÐ°Ðµ Ð¿ÑÑÐ¼Ð¾Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÑÐ¸Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð½ÐµÐ²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾. ÐÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð°Ñ ÑÐµÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð³Ð°ÐµÑÑÑ Ð¿ÑÑÐµÐ¼ ÑÐµÐ³ÑÐ»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð·ÑÑÐ²Ð½ÑÑ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÐµÐ¹, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾, Ð°Ð¿Ð¿ÑÐ¾ÐºÑÐ¸Ð¼Ð°ÑÐ¸Ð¸ ÑÐ°Ð·ÑÑÐ²Ð½ÑÑ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÐµÐ¹ Ð¸Ñ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½ÑÐ¼Ð¸ Ð°Ð½Ð°Ð»Ð¾Ð³Ð°Ð¼Ð¸ Ñ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÑÐ¸Ð¼ Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð² Ð¿ÑÐ¾ÑÐµÐ´ÑÑÐ°Ñ Ð¼ÐµÑÐ¾Ð´Ð° Ð¼Ð°ÐºÑÐ¸Ð¼ÑÐ¼Ð° Ð¿ÑÐ°Ð²Ð´Ð¾Ð¿Ð¾Ð´Ð¾Ð±Ð¸Ñ Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐ¾Ð±Ð°ÑÑÐ½ÑÑ Ð-Ð¾ÑÐµÐ½Ð¾Ðº Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ° Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ. ÐÑÐ¸ ÑÑÐ¾Ð¼ ÑÐ¾Ð±Ð°ÑÑÐ½Ð¾ÑÑÑ Ð¾ÑÐµÐ½Ð¸Ð²Ð°Ð½Ð¸Ñ Ð´Ð¾ÑÑÐ¸Ð³Ð°ÐµÑÑÑ Ð·Ð° ÑÑÐµÑ ÑÑÐµÑÐµÐ½Ð¸Ñ Ð¾ÑÐµÐ½Ð¾ÑÐ½ÑÑ ÑÑÐ½ÐºÑÐ¸Ð¹ Ð-Ð¾ÑÐµÐ½Ð¾Ðº, Ð¿ÑÐ¸ ÑÑÐ¾Ð¼ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÑÑÐµÑÐµÐ½Ð¸Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ Ð¸Ð· ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¼Ð°ÐºÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¸ ÑÐµÐ»Ð¸, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÑÑÑÑ ÑÐ¾Ð±Ð¾Ð¹ ÑÑÐ¼Ð¼Ñ Ð²Ð·Ð°Ð¸Ð¼Ð½Ð¾-Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¾ÑÐµÐ½Ð¾Ðº. Ð­ÑÐ¾Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´ ÑÐµÐ°Ð»Ð¸Ð·ÑÐµÑÑÑ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ ÐÐ°ÑÑÑÐ°, ÐÐ°Ð¿Ð»Ð°ÑÐ° Ð¸ ÐÐ¾ÑÐ¸.
The Hilbert Lagrangian and Isometric Embedding: Tetrad Formulation of Regge-Teitelboim Gravity
Creators: name: Estabrook, Frank B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We discuss Exterior Differential Systems (EDS) for the vacuum gravitational field. These EDS are derived by varying the Hilbert-Einstein Lagrangian, given most elegantly as a Cartan 4-forrm calibrating 4-spaces embedded in ten flat dimensions. In particular we thus formulate with tetrad equations the Regge-Teitelboim dynamics "a la string" (R-T); it arises when variation of the 4-spaces gives the Euler-Lagrange equations of a multicontact field theory. We calculate the Cartan character table of this EDS, showing the field equations to be well posed with no gauge freedom. The Hilbert Lagrangian as usually varied over just the intrinsic curvature structure of a 4-space yields only a subset of this dynamics, viz., solutions satisfying additional conditions constraining them to be Ricci-flat. In the static spherically symmetric case we present a new tetrad embedding in flat six dimensions, which allows reduction of the R-T field equations to a quadrature; the Schwarzschild metric is a special case. As has previously been noted there may be a classical correspondence of R-T theory with the hidden dimensions of brane theory, and perhaps this extended general relativistic dynamics holds in extreme circumstances where it can be interpreted as including a sort of dark or bulk energy, even though no term with a cosmological constant is included in the Lagrangian. As a multicontact system, canonical quantization should be straightforward.
description: 12 pages, 1 figure. Version 2 has modified title and text, reflecting added earlier references. New Introduction
A retrospective observational analysis of the real-world care pathway of people with hereditary transthyretin amyloidosis with polyneuropathy in Italy
Creators: name: Calabria, Silvia
name: Ronconi, Giulia
name: Dondi, Letizia
name: Dondi, Leonardo
name: Dell’Anno, Irene
name: Piccinni, Carlo
name: Esposito, Immacolata
name: Addesi, Alice
name: Gnesi, Marco
name: Cosentino, Nicola
name: D’Amelio, Marco
name: Martini, Nello
name: Maggioni, Aldo Pietro
Publisher: name: Taylor & Francis
Year: 2025
Subjects: subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Mental Health

description: This retrospective observational study described the epidemiology and the burden on the Italian healthcare service (SSN) of patients with polyneuropathy (PN) associated with hereditary transthyretin amyloidosis (ATTRv). From the Fondazione ReS (Ricerca e Salute) administrative healthcare database (~5.5 million inhabitants in 2021), patients were identified as having ATTRv-PN in 2021 if they had received treatments for ATTRv-PN under SSN reimbursement (i.e. tafamidis, patisiran, or inotersen) from 1 January 2014 to 31 December 2021 (index date in 2021). Demographics and comorbidities at the baseline, healthcare resource consumption, and related direct costs reimbursed by the SSN throughout the one-year follow-up were described. In 2021, 36 patients with ATTRv-PN (prevalence: 7.4/1,000,000) were identified (males were 83.3%; patients with ≥2 comorbidities were 61.1%; the mean age was 73 ± 8 years). During follow-up, of patients, 91.7% received drugs for ATTRv-PN; >50% received antiepileptics and acid suppressants; 22.2% were admitted to overnight hospitalizations; 30.6% accessed the emergency department; 97.2% received local outpatient specialist care. The per patient mean annual cost was € 122,017; drugs for ATTRv-PN accounted for 94.7% of the total expenditure. This study of real-world patients with ATTRv-PN showed a high rate of comorbidities, and substantial direct healthcare and economic burdens on the SSN.
Una cabina di regia per la ricerca
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2014

Alla vigilia dell'iter della Legge di Stabilità 2015, la Commissione Istruzione del Senato rilancia sulla Ricerca scientifica italiana e, dopo circa sette mesi di indagini e audizioni a tutto campo, approva all'unanimità una risoluzione da presentare al Governo sugli Enti pubblici di ricerca, proponendo un Piano settennale di rifinanziamento che raggiunga lo 0,7% del Pil entro il 2020
Growth of superconducting single-crystalline (Lu, Ca)Ba2Cu3O7-d whiskers
Creators: name: Deguchi, K.
name: Ogawara, S.
name: Okutsu, T.
name: Nagao, M.
name: Watanabe, T.
name: Mizuguchi, Y.
name: Kubo, Y.
name: Tomioka, F.
name: Ishii, S.
name: Tsuda, S.
name: Yamaguchi, T.
name: Nagasawa, M.
name: Takano, Y.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Single-crystalline (Lu, Ca)Ba2Cu3O7-d (Lu(Ca)123) whiskers have been successfully grown using the Te-doping method. X-ray diffraction patterns of Lu(Ca)123 whiskers showed sharp (0 0 l) peaks corresponding to REBa2Cu3O7-d phase (RE = rare earth elements). Transport measurements showed that the superconducting transition occurred at 83 K in the obtained whiskers.
description: 3 pages, 3 figures, ISS2008
title: ÐÐµÑÐ¾Ð´ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð´Ð¾Ð¼ÐµÑÑÐ¸Ð¸ Ð¿ÑÐ¸ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ð¸ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð±Ð¾ÑÐ° Ð² Ð³Ð°Ð·Ð¾Ð²ÑÑ ÑÑÑÐ±Ð°Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¼Ð¸ÑÐ½Ð¾Ð²Ð°, 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: 2016
Subjects: Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÐ¹ ÑÐ¾Ð±Ð¾Ñ
ÑÐ¾Ð±Ð¾ÑÑ
Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¾Ð½Ð´Ð¾Ð¼ÐµÑÑÐ¸Ñ
Ð³Ð°Ð·Ð¾Ð²ÑÐµ ÑÑÑÐ±Ñ
Ð¼ÐµÑÐ¾Ð´ ÐÑÐºÐ°Ñ-ÐÐ°Ð½Ð°Ð´Ðµ
Ð¼ÐµÑÐ¾Ð´ Ð¤Ð°ÑÐ½ÐµÐ±ÐµÐºÐ°
mobile robot
robots
optical ondometry
gas pipes
Lucas-Canada method
Farnebeka method

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¼ÐµÑÐ¾Ð´ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð´Ð¾Ð¼ÐµÑÑÐ¸Ð¸, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÐ¸Ð¹ÑÑ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÐ¼ ÑÐ¾Ð±Ð¾ÑÐ¾Ð¼ Ð¿ÑÐ¸ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ð¸ Ð¿Ð¾ ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ñ. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð²ÑÐ±Ð¾Ñ Ð¼ÐµÑÐ¾Ð´Ð° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾ÐºÐ° Ð´Ð»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÐµÐ´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÐºÐ°ÑÑÑ Ð¿ÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð´Ð¾Ð¼ÐµÑÑÐ¸Ð¸ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÐ¼ ÑÐ¾Ð±Ð¾ÑÐ¾Ð¼, Ð´Ð²Ð¸Ð¶ÑÑÐ¸Ð¼ÑÑ Ð¿Ð¾ ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾ÐºÐ° Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ñ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð±Ð¾ÑÐ°, Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ ÐºÐ°ÑÑÑ Ð¸ ÑÑÐµÑÐ¼ÐµÑÐ½ÑÑ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ñ Ð²Ð¸Ð´ÐµÐ¾ÐºÐ°Ð¼ÐµÑÑ Ð² ÑÐµÐ¶Ð¸Ð¼Ðµ ÑÐµÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð¸.
description: The object of research is the method of optical odometry using by the mobile robot while moving through the pipeline. The purpose - to choose the method of estimating the optical flow in order to determine the motion and built the map while implementing the method of optical odometry to the mobile robot moving through the pipeline. Developed optical flow algorithms provide a definition of movement of the mobile robot, the construction of maps and three-dimensional reconstruction of the space on the basis of data obtained from the camera in real time.
Norm optimization problem for linear operators in classical Banach spaces
Creators: name: Pellegrino, Daniel
name: Teixeira, Eduardo V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 46B20

description: The main result of the paper shows that, for 1
description: 12 pages
Tandem Coding and Cryptography on Wiretap Channels: EXIT Chart Analysis
Creators: name: Harrison, Willie K
name: McLaughlin, Steven W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Information Theory (cs.IT)
subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: Traditional cryptography assumes an eavesdropper receives an error-free copy of the transmitted ciphertext. Wyner's wiretap channel model recognizes that at the physical layer both the intended receiver and the passive eavesdropper inevitably receive an error-prone version of the transmitted message which must be corrected prior to decryption. This paper considers the implications of using both channel and cryptographic codes under the wiretap channel model in a way that enhances the \emph{information-theoretic} security for the friendly parties by keeping the information transfer to the eavesdropper small. We consider a secret-key cryptographic system with a linear feedback shift register (LFSR)-based keystream generator and observe the mutual information between an LFSR-generated sequence and the received noise-corrupted ciphertext sequence under a known-plaintext scenario. The effectiveness of a noniterative fast correlation attack, which reduces the search time in a brute-force attack, is shown to be correlated with this mutual information. For an iterative fast correlation attack on this cryptographic system, it is shown that an EXIT chart and mutual information are very good predictors of decoding success and failure by a passive eavesdropper.
description: 11 pages, 5 figures, accepted at 2009 IEEE International Symposium on Information Theory (ISIT 2009)
Spuntino stellare per un vorace buco nero
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2014

Gli astronomi hanno scoperto che questo buco nero, a 12 milioni di anni luce dalla Terra, è estremamente vorace tanto da poter consumare la stella a cui attorno orbita (20 volte più massiccia del Sole) in solo un milione di anni
Redshift Evolution in Black Hole-Bulge Relations: Testing CIV-based Black Hole Masses
Creators: name: Greene, Jenny E.
name: Peng, Chien Y.
name: Ludwig, Randi R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We re-examine claims of redshift evolution in black hole-bulge scaling relations based on lensed quasars. In particular, we refine the black hole mass estimates using measurements of Balmer lines from near-infrared spectroscopy obtained with Triplespec at Apache Point Observatory. In support of previous work, we find a large scatter between Balmer and UV line widths, both MgII 2796, 2803 and CIV 1548, 1550. There is tentative evidence that CIII] 1909, despite being a blend of multiple transitions, may correlate well with MgII, although a larger sample is needed for a real calibration. Most importantly, we find no systematic changes in the estimated BH masses for the lensed sample based on Balmer lines, providing additional support to the interpretation that black holes were overly massive compared to their host galaxies at high redshift.
description: 15 pages, 9 figures, Accepted for publication in ApJ
Structural alignment using the generalized Euclidean distance between conformations
Creators: name: Mohazab, Ali R.
name: Plotkin, Steven S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Biomolecules (q-bio.BM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: The usual Euclidean distance may be generalized to extended objects such as polymers or membranes. Here, this distance is used for the first time as a cost function to align structures. We examined the alignment of extended strands to idealized beta-hairpins of various sizes using several cost functions, including RMSD, MRSD, and the minimal distance. We find that using minimal distance as a cost function typically results in an aligned structure that is globally different than that given by an RMSD-based alignment
description: Accepted in IJQC
title: Polyurethane Nanocapsules Incorporating Epigallocatechin Gallate, A Green Tea Extract
Creators: name: Ale, Temitope
name: Ghunney, Nhyira
name: Pandala, Narendra
name: Tucker, Budd
name: McFadden, Kassandra
name: Hutcheson, Jack
name: Lavik, Erin
Publisher: name: Wiley
Year: 2025
Subjects: subject: traumas
subject: repairs
subject: polymers
subject: regenerations
subject: brain injuries
subject: nanomaterials

description: Explosions cause 79% of combat-related injuries, often leading to traumatic brain injury (TBI) and hemorrhage. Epigallocatechin gallate (EGCG), a green tea polyphenol, aids neuroprotection and wound healing. In this work, we sought to investigate the fabrication and characterization of polyurethane nanocapsules encapsulating EGCG, demonstrating controlled, on-demand release, and highlighting their potential for targeted therapeutic delivery in trauma care.
Prima pietra per ESS
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2014

Cerimonia di posa della prima pietra della European Spallation Source (ESS) nel cantiere di Lund in Svezia per  l’avvio dei lavori di realizzazione di quella che sarà la più potente sorgente di neutroni al mondo