cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð±Ð¾ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð²Ð¾Ð´Ñ Ð¿ÑÐ¾ÐµÐºÑÐ° ÐÐ­Ð¡ Ð¥Ð°Ð½Ñ Ð¸ÐºÐ¸Ð²Ð¸-1
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Ð¾Ð¿ÑÐµÑÐ¸Ð½ÑÐºÐ¸Ð¹, 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°ÑÑ-2006
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Ð²Ð²ÑÑ-1200
Ð°ÑÑ Ñ Ð°Ð½Ñ Ð¸ÐºÐ¸Ð²Ð¸-1

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð±Ð¾ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾ÐµÐºÑÐ° ÐÐ­Ð¡ Ð¥Ð°Ð½ÑÐ¸ÐºÐ¸Ð²Ð¸-1 Ð¸ Ð²ÑÐ½ÐµÑÐµÐ½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÐµÑ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÐÐ­Ð¡ Ð¥Ð°Ð½ÑÐ¸ÐºÐ¸Ð²Ð¸-1. ÐÑÑÐ¸ÑÐ»ÐµÐ½Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð¾Ð±ÑÑÐ¼Ñ ÑÐ°ÑÑÐ²Ð¾ÑÐ° Ð±Ð¾ÑÐ½Ð¾Ð¹ ÐºÐ¸ÑÐ»Ð¾ÑÑ Ð²ÑÑÐ¾ÐºÐ¾Ð¹ Ð¸ Ð½Ð¸Ð·ÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ð¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ°ÑÑÑÑÐ¾Ð² Ð²ÑÐ½ÐµÑÐµÐ½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð±Ð¾ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð²Ð¾Ð´Ñ.
MMS a caccia delle riconnessioni magnetiche
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

A distanza di nove mesi dal lancio della Magnetospheric MultiScale Mission della NASA, sono stati presentati al convegno autunnale della American Geophysical Union a San Francisco che si è concluso nello scorso fine settimana i primi risultati scientifici della missione
Controlled entanglement source for quantum cryptography
Creators: name: Zeng, Qiang
name: Wang, Haoyang
name: Yuan, Huihong
name: Fan, Yuanbin
name: Zhou, Lai
name: Gao, Yuanfei
name: Ma, Haiqiang
name: Yuan, Zhiliang
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Quantum entanglement has become an essential resource in quantum information processing. Existing works employ entangled quantum states to perform various tasks, while little attention is paid to the control of the resource. In this work, we propose a simple protocol to upgrade an entanglement source with access control through phase randomization at the optical pump. The enhanced source can effectively control all users in utilizing the entanglement resource to implement quantum cryptography. In addition, we show this control can act as a practical countermeasure against memory attack on device-independent quantum key distribution at a negligible cost. To demonstrate the feasibility of our protocol, we implement an experimental setup using just off-the-shelf components and characterize its performance accordingly.
description: 9 pages, 7 figures, comments are welcome! Looking forward to collaborations!
Dynamical 3-Space Predicts Hotter Early Universe: Resolves CMB-BBN Li7 and He4 Abundance Anomalies
Creators: name: Cahill, Reginald T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: The observed abundances of Li7 and He4 are significantly inconsistent with the predictions from Big Bang Nucleosynthesis (BBN) when using the LCDM cosmological model together with the value for Omega_Bh^2 = 0.0224 +/- 0.0009 from WMAP CMB fluctuations, with the value from BBN required to fit observed abundances being 0.009
description: 8 pages 2 figures
Additional file 5: of Genome-wide identification and characterization of the 14â 3-3 family in Vitis vinifera L. during berry development and cold- and heat-stress response
Creators: name: Cheng, Cheng
name: Wang, Yi
name: Chai, Fengmei
name: Li, Shaohua
name: Xin, Haiping
name: Liang, Zhenchang
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: The primer sequence for qRT-PCR. (DOC 31 kb)
Phase Field Simulation of Liquid Filling on Grooved Surfaces for Complete, Partial and Pseudo-partial Wetting Cases
Creators: name: Oktasendra, Fandi
name: Jusufi, Arben
name: Konicek, Andrew R.
name: Yeganeh, Mohsen S.
name: Panter, Jack R.
name: Kusumaatmaja, Halim
Publisher: name: arXiv
Year: 2023
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We develop and harness a phase field simulation method to study liquid filling on grooved surfaces. We consider both short-range and long-range liquid-solid interactions, with the latter including purely attractive and repulsive interactions, as well as those with short-range attraction and long-range repulsion. This allows us to capture complete, partial and pseudo-partial wetting states, demonstrating complex disjoining pressure profiles over the full range of possible contact angles as previously proposed in the literature. Applying the simulation method to study liquid filling on grooved surfaces, we compare the filling transition for the three different classes of wetting states as we vary the pressure difference between the liquid and gas phases. The filling and emptying transition is reversible for the complete wetting case, while significant hysteresis is observed for the partial and pseudo-partial cases. In agreement with previous studies, we also show that the critical pressure for the filling transition follows the Kelvin equation for the complete and partial wetting scenarios. Finally, we find the filling transition can display a number of distinct morphological pathways for the pseudo-partial wetting cases, as we demonstrate here for varying groove dimensions.
description: 11 pages, 6 figures, accepted in the Journal of Chemical Physics
Buchi neri extra large
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Fino a che punto può crescere un buco nero supermassiccio? E’ la domanda a cui ha tentato di rispondere un professore dell’Università di Leicester in uno studio, riportato su Monthly Notices Letters of the Royal Astronomical Society, in cui viene suggerito che tali oggetti possono raggiungere, in linea di principio, 50 miliardi di masse solari prima che il gas circostante si trasformi in stelle
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title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
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Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐµÐ³ÑÐ»Ð¸ÑÑÐµÐ¼ÑÐµ Ð¿ÐµÑÐµÑÐµÑÐµÐ½Ð¸Ñ
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title: ÐÐ½Ð°Ð»Ð¸Ð· Ð²Ð½ÐµÑÐ½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð²Ð¸Ð½ÑÐ¸Ð¸ Ð¡ÑÑÑÐ°Ð½Ñ ÐÐÐ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÑÐ¾Ð´ÑÐºÑ intel ChengDuÂ» )
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§Ð¶Ñ 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: 2018
Subjects: ÐÐ¸ÑÐ°Ð¹
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title: Ð Ð¾Ð»Ñ ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð½ÑÐ°Ð²ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½Ð¾ÑÐ¼, Ð² Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ð¸ ÑÐ¾Ð±Ð»ÑÐ´ÐµÐ½Ð¸Ñ Ð·Ð°Ð¿ÑÐµÑÐ¾Ð², Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹, ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð½ÑÑ Ð² ÑÐµÐ»ÑÑ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÐºÐ¾ÑÑÑÐ¿ÑÐ¸Ð¸
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Ð»Ð°Ð·ÑÑÐ¸Ð½, Ð¤Ð¸Ð»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: 2018
Subjects: ÐºÐ¾ÑÑÑÐ¿ÑÐ¸Ñ
ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð¾ÑÐ¼Ñ
Ð½ÑÐ°Ð²ÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð½Ð¾ÑÐ¼Ñ
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Anno della Luce verso la chiusura
Creators: Ginevra Trinchieri e Il comitato INAF/SAIt per IYL2015
Publisher: name: Media Inaf
Year: 2015

Proclamato il 20 dicembre 2013 dall’Assemblea Generale delle Nazioni Unite, in collaborazione con l’UNESCO e un gran numero di soggetti scientifici, tra cui anche la Società Astronomica Italiana e l’Istituto Nazionale di Astrofisica
Early excess emission in Type Ia supernovae from the interaction between supernova ejecta and their circumstellar wind
Creators: name: Moriya, Takashi J.
name: Mazzali, Paolo A.
name: Ashall, Chris
name: Pian, Elena
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The effects of the interaction between Type Ia supernova ejecta and their circumstellar wind on the photometric properties of Type Ia supernovae are investigated. We assume that a hydrogen-rich, dense, and extended circumstellar matter (CSM) is formed by the steady mass loss of their progenitor systems. The CSM density is assumed to be proportional to r^{-2}. When the mass-loss rate is above 1e-4 Msun/yr with a wind velocity of 100 km/s, CSM interaction results in an early flux excess in optical light-curves within 4 days of explosion. In these cases, the optical colour quickly evolves to the blue. The ultraviolet flux below 3000 A is found to have a persistent flux excess compared to Type Ia supernovae as long as CSM interaction continues. Type Ia supernovae with progenitor mass-loss rates between 1e-4 and 1e-3 Msun/yr may not have a CSM that is dense enough to affect spectra to make them Type Ia-CSM, but they may still result in Type Ia supernovae with an early optical flux excess. Because they have a persistent ultraviolet flux excess, ultraviolet light curves around the luminosity peak would be significantly different from those with a low-density CSM.
description: 8 pages, 8 figures, accepted by Monthly Notices of the Royal Astronomical Society
Type I planet migration in nearly laminar disks - long term behavior
Creators: name: Yu, Cong
name: Li, Hui
name: Li, Shengtai
name: Lubow, S. H.
name: Lin, D. N. C.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We carry out 2-D high resolution numerical simulations of type I planet migration with different disk viscosities. We find that the planet migration is strongly dependent on disk viscosities. Two kinds of density wave damping mechanisms are discussed. Accordingly, the angular momentum transport can be either viscosity dominated or shock dominated, depending on the disk viscosities. The long term migration behavior is different as well. Influences of the Rossby vortex instability on planet migration are also discussed. In addition, we investigate very weak shock generation in inviscid disks by small mass planets and compare the results with prior analytic results.
description: Accepted for publication in ApJ
title: PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð½ÐµÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹ Ð² ÑÑÐµÑÐµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð½ÐµÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð¤Ð¾Ð½Ð´Ð° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¼Ð¾ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÐ°)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÑÐ¾Ð»Ð±Ð¾Ð²Ð°Ñ, ÐÐ»Ð°Ð´Ð»ÐµÐ½Ð°
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: PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð½ÐµÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
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ÑÑÐµÑÐ° ÑÑÐ»ÑÐ³
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° ÑÑÑÐ½Ð¾ÑÑÑ PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½ÐµÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹ Ð² ÑÑÐµÑÐµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼. ÐÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½ÐµÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹, ÐºÐ°Ðº Â«ÑÐ¿Ð¾Ð½ÑÐ¾ÑÐ¸Ð½Ð³Â», Â«ÑÐ°Ð½Ð´ÑÐ°Ð¹Ð·Ð¸Ð½Ð³Â», Â«ÐºÑÐ°ÑÐ´ÑÐ°Ð½Ð´Ð¸Ð½Ð³Â». ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ SWOT-Ð°Ð½Ð°Ð»Ð¸Ð· Ð¤Ð¾Ð½Â­Ð´Ð°, Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ°Ð¹ÑÐ° Â«Ð­ÐÐ²Ð°ÑÐ¾ÑÂ», ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Â«Ð­ÐÐ²Ð°ÑÐ¾ÑÂ», Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ»ÐµÐ²Ð¾Ð¹ Ð°ÑÐ´Ð¸ÑÐ¾ÑÐ¸Ð¸ Ð¤Ð¾Ð½Ð´Ð°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Ð¿Ð¾ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ ÑÑÐ»ÑÐ³ Ð½ÐµÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð¤Ð¾Ð½Ð´Ð° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¼Ð¾ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÐ° (Ð½Ð° Ð±Ð°Ð·Ðµ ÑÑÐµÐ½Ð¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«Ð­ÐÐ²Ð°ÑÐ¾ÑÂ»).
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ñ Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð½Ñ Ð¸ ÐµÐ³Ð¾ ÐºÐ¾Ð½ÑÑÐ¼ÐµÑÑ
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°Ð¾ Ð¡ÑÑÑÑÐ½
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¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ°Ð½Ñ
Ð¸Ð½ÑÑÐ°ÑÑÑÑÐºÑÑÑÐ½ÑÐµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸
Ð°Ð·Ð¸Ð°ÑÑÐºÐ¸Ðµ Ð±Ð°Ð½ÐºÐ¸

description: Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ: ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð½ÑÐ½ÐµÑÐ½ÐµÐ¹ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸ Ð² ÐºÑÐµÐ´Ð¸ÑÐ½Ð¾ Ð´ÐµÐ½ÐµÐ¶Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐµ Ð¸ Ð´ÐµÐ½ÐµÐ¶Ð½Ð¾Ð¼ Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ð¸ ÐÐ¸ÑÐ°Ñ, Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð½Ñ, Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ ÑÑÑÐ´Ð½Ð¾ÑÑÐµÐ¹ Ð¸ Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ð¹, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¸ Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð½Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÑÐµÐ¹ Ð¸ ÑÑÐµÐ´ÑÑÐ² Ð¿ÑÐµÐ¾Ð´Ð¾Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ð¹ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÑÐµÐ¼ ÑÑÐºÐ¾ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ°. ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð»Ð¾ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ ÑÐ»ÑÑÑÐ¸ÑÑ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð½Ñ, ÑÑÐ¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð»Ð¾ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð². ÐÐ¾Ð»ÑÑÐ¾Ðµ Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾ÐºÐ°Ð·Ð°Ð»Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Â«ÑÑÐ¾Ð¹Ð½Ð¾Ð³Ð¾ Ð¿Ð°ÑÐ°Ð´Ð¾ÐºÑÐ°Â» Ð² ÐÐ¸ÑÐ°Ðµ. ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐ¿ÐµÑÐ½Ð¾ ÑÐµÐ°Ð»Ð¸Ð·ÑÑÑÑÑ Ð² ÐÐ·Ð¸Ð°ÑÑÐºÐ¾Ð¼ Ð±Ð°Ð½ÐºÐµ Ð¸Ð½ÑÑÐ°ÑÑÑÑÐºÑÑÑÐ½ÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ (ÐÐÐÐ) Ð¸ Ð¿ÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Â«ÐÐ´Ð¸Ð½ Ð¿Ð¾ÑÑ Ð¸ Ð¾Ð´Ð¸Ð½ Ð¿ÑÑÑÂ».
Continuous-variable quantum information processing with squeezed states of light
Creators: name: Yonezawa, Hidehiro
name: Furusawa, Akira
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate experiments of continuous-variable quantum information processing based on the teleportation scheme. Quantum teleportation, which is realized by a two-mode squeezed vacuum state and measurement-and-feedforward, is considered as an elementary quantum circuit as well as quantum communication. By modifying ancilla states or measurement-and-feedforwards, we can realize various quantum circuits which suffice for universal quantum computation. In order to realize the teleportation-based computation we improve the level of squeezing, and fidelity of teleportation. With a high-fidelity teleporter we demonstrate some advanced teleportation experiments, i.e., teleportation of a squeezed state and sequential teleportation of a coherent state. Moreover, as an example of the teleportation-based computation, we build a QND interaction gate which is a continuous-variable analog of a CNOT gate. A QND interaction gate is constructed only with ancillary squeezed vacuum states and measurement-and-feedforwards. We also create continuous-variable four mode cluster type entanglement for further application, namely, one-way quantum computation.
description: submitted to Optics and Spectroscopy special issue for ICQO'2008
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð½ÑÐ°Ð¹Ð·Ð¸Ð½Ð³Ð° Ð² ÑÑÑÐ¸Ð·Ð¼Ðµ, ÐºÐ°Ðº ÑÐ¿Ð¾ÑÐ¾Ð±Ð° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾Ð³Ð¾ Ð¸ ÑÐ¸Ð²Ð¸Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° ÑÑÑÐ¸Ð·Ð¼Ð° Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¾ÑÐµÐµÐ²Ð°, ÐÐ½Ð½Ð°
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ÑÐ°Ð½ÑÐ°Ð¹Ð·Ð¸Ð½Ð³
ÑÑÐ°Ð½ÑÐ¸Ð·Ð°
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ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½Ð¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐ°Ð½ÑÐ°Ð¹Ð·Ð¸Ð½Ð³ Ð² ÑÑÑÐ¸ÑÑÑÐºÐ¾Ð¹ ÑÑÐµÑÐµ Ð Ð¤.
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A Practical Walk-on-Boundary Method for Boundary Value Problems
Creators: name: Sugimoto, Ryusuke
name: Chen, Terry
name: Jiang, Yiti
name: Batty, Christopher
name: Hachisuka, Toshiya
Publisher: name: arXiv
Year: 2023
Subjects: subject: Graphics (cs.GR)
subject: Numerical Analysis (math.NA)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: We introduce the walk-on-boundary (WoB) method for solving boundary value problems to computer graphics. WoB is a grid-free Monte Carlo solver for certain classes of second order partial differential equations. A similar Monte Carlo solver, the walk-on-spheres (WoS) method, has been recently popularized in computer graphics due to its advantages over traditional spatial discretization-based alternatives. We show that WoB's intrinsic properties yield further advantages beyond those of WoS. Unlike WoS, WoB naturally supports various boundary conditions (Dirichlet, Neumann, Robin, and mixed) for both interior and exterior domains. WoB builds upon boundary integral formulations, and it is mathematically more similar to light transport simulation in rendering than the random walk formulation of WoS. This similarity between WoB and rendering allows us to implement WoB on top of Monte Carlo ray tracing, and to incorporate advanced rendering techniques (e.g., bidirectional estimators with multiple importance sampling, the virtual point lights method, and Markov chain Monte Carlo) into WoB. WoB does not suffer from the intrinsic bias of WoS near the boundary and can estimate solutions precisely on the boundary. Our numerical results highlight the advantages of WoB over WoS as an attractive alternative to solve boundary value problems based on Monte Carlo.
description: Accepted to ACM SIGGRAPH North America 2023 / Transactions on Graphics. See https://rsugimoto.net/WoBforBVPsProject/ for updates, including the reference implementation
Revising the observable consequences of slow-roll inflation
Creators: name: Agullo, Ivan
name: Navarro-Salas, Jose
name: Olmo, Gonzalo J.
name: Parker, Leonard
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the generation of primordial perturbations in a (single-field) slow-roll inflationary universe. In momentum space, these (Gaussian) perturbations are characterized by a zero mean and a non-zero variance $Δ^2(k, t)$. However, in position space the variance diverges in the ultraviolet. The requirement of a finite variance in position space forces one to regularize $Δ^2(k, t)$. This can (and should) be achieved by proper renormalization in an expanding universe in a unique way. This affects the predicted scalar and tensorial power spectra (evaluated when the modes acquire classical properties) for wavelengths that today are at observable scales. As a consequence, the imprint of slow-roll inflation on the CMB anisotropies is significantly altered. We find a non-trivial change in the consistency condition that relates the tensor-to-scalar ratio $r$ to the spectral indices. For instance, an exact scale-invariant tensorial power spectrum, $n_t=0$, is now compatible with a non-zero ratio $r\approx 0.12\pm0.06$, which is forbidden by the standard prediction ($r=-8n_t$). The influence of relic gravitational waves on the CMB may soon come within the range of planned measurements, offering a non-trivial test of the new predictions.
description: 24 pages
A Tech Hybrid-Recommendation Engine and Personalized Notification: An integrated tool to assist users through Recommendations (Project ATHENA)
Creators: name: Lecaros, Lordjette Leigh M.
name: Khan, Concepcion L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Information Retrieval (cs.IR)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Project ATHENA aims to develop an application to address information overload, primarily focused on Recommendation Systems (RSs) with the personalization and user experience design of a modern system. Two machine learning (ML) algorithms were used: (1) TF-IDF for Content-based filtering (CBF); (2) Classification with Matrix Factorization- Singular Value Decomposition(SVD) applied with Collaborative filtering (CF) and mean (normalization) for prediction accuracy of the CF. Data sampling in academic Research and Development of Philippine Council for Agriculture, Aquatic, and Natural Resources Research and Development (PCAARRD) e-Library and Project SARAI publications plus simulated data used as training sets to generate a recommendation of items that uses the three RS filtering (CF, CBF, and personalized version of item recommendations). Series of Testing and TAM performed and discussed. Findings allow users to engage in online information and quickly evaluate retrieved items produced by the application. Compatibility-testing (CoT) shows the application is compatible with all major browsers and mobile-friendly. Performance-testing (PT) recommended v-parameter specs and TAM evaluations results indicate strongly associated with overall positive feedback, thoroughly enough to address the information-overload problem as the core of the paper. A modular architecture presented addressing the information overload, primarily focused on RSs with the personalization and design of modern systems. Developers utilized Two ML algorithms and prototyped a simplified version of the architecture. Series of testing (CoT and PT) and evaluations with TAM were performed and discussed. Project ATHENA added a UX feature design of a modern system.
description: 15 pages
Additional file 2: of Genome-wide identification and characterization of the 14â 3-3 family in Vitis vinifera L. during berry development and cold- and heat-stress response
Creators: name: Cheng, Cheng
name: Wang, Yi
name: Chai, Fengmei
name: Li, Shaohua
name: Xin, Haiping
name: Liang, Zhenchang
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: The organs presented in Fig. 6 from published data GSE36128. (DOC 63 kb)
Una serata dedicata a Margherita Hack
Creators: Francesca Brunetti
Publisher: name: Media Inaf
Year: 2015

Arcetri, Donna Ginevra, Margherita, il telescopio e un quarto di Luna è il titolo dell’evento dedicato a Margherita Hack che si terrà sabato 19 dicembre al Teatro del Cielo dell’INAF - Osservatorio Astrofisico di Arcetri. Protagonista la cantante Donna Ginevra Di Marco
Additional file 1 of Sensitivity and specificity of self-reported psychiatric diagnoses amongst patients treated for opioid use disorder
Creators: name: Leung, Kelly
name: Xu, Emily
name: Rosic, Tea
name: Worster, Andrew
name: Thabane, Lehana
name: Samaan, Zainab
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Science Policy
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Mental Health

description: Additional file 1: Appendix A. Paired contingency tables comparing results of self-reported diagnosis to MINI diagnosis.
Projectable Horava-Lifshitz gravity in a nutshell
Creators: name: Weinfurtner, Silke
name: Sotiriou, Thomas P.
name: Visser, Matt
Publisher: name: arXiv
Year: 2010
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Approximately one year ago Horava proposed a power-counting renormalizable theory of gravity which abandons local Lorentz invariance. The proposal has been received with growing interest and resulted in various different versions of Horava-Lifshitz gravity theories, involving a colourful potpourri of new terminology. In this proceedings contribution we first motivate and briefly overview the various different approaches, clarifying their differences and similarities. We then focus on a model referred to as projectable Horava-Lifshitz gravity and summarize the key results regarding its viability.
description: 8 pages, no figures, to appear in the proceedings of First Mediterranean Conference on Classical and Quantum Gravity Conference (MCCQG), Kolymbari (Crete, Greece), September 14-18, 2009
L’esosfera lunare svelata da LADEE
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Uno studio recente, apparso ieri sulle pagine di Science, mostra che l’abbondanza di sodio e potassio nell’esosfera lunare dipende dalla sua esposizione al Sole, dalla presenza di sciami meteorici e dalla composizione della superficie. I dati sono stati raccolti dalla sonda spaziale Lunar Atmosphere and Dust Environment Explorer della NASA tra l’ottobre 2013 e l’aprile 2014
Some optimum properties and applications of Stein's test
Creators: name: Knight, William Rixford
Publisher: name: University of British Columbia
Year: 2012

description: Stein's test tests the homogeneity of means of a set of normal distributions with the homoscedasticity property by means of a sequential sampling prodecure in two stages, the results of the first sample determining the size of the second. By means of this procedure a test the power of which is independent of the variance is possible. Certain extensions of Stein's test are obtained. Some optimum properties for such two stage sequential procedures are proposed, and it is shown that the tests satisfying these optimum properties are essentially the same as Stein's test.
CT color perfusion for the localization of parathyroid glands preoperatively-a novel tool in difficult diagnostic cases.
Creators: name: Myschetzky, Peter
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Head and neck
subject: CT
subject: Computer Applications-Detection, diagnosis
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 61 years
description: Clinical History: A 61-year-old obese female patient with hypocalcaemia (1.34mmol/l: nl range 1.18-1.32) and a high PTH level (9.4pmol/l: nl range 1.18-8.43) was referred from our ENT clinic for CT evaluation. This patient had recently had a Tc-99m-MIBI-SPECT (MIBI-SPECT) ... Final Diagnosis: Primary hyperparathyroidism gland localization
Perineal dermoid cyst
Creators: name: Woussen, Sofie
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Pelvis
subject: MR
subject: Ultrasound
subject: Diagnostic procedure
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 32 years
description: Clinical History: A 32-year-old male patient presented with a right-sided gluteal mass. His past medical history was unremarkable. On rectal examination there was right-sided fullness. Final Diagnosis: Dermoid cyst
The âdouble panda signâ and central pontine signal changes in Wilsonâs disease.
Creators: name: Zikou, Anastasia
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Neuroradiology brain
subject: MR
subject: Diagnostic procedure
subject: Metabolic disorders

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 28 years
description: Clinical History: Female patient of 28 years of age was admitted to the hospital for hand tremor, ataxia, slurred speech and bipolar disorder. Few years after, her younger sister presented to the emergency department with the same symptoms. Brain-MRI was conducted in both ... Final Diagnosis: Wilson disease.
Functions holomorphic along holomorphic vector fields
Creators: name: Kim, Kang-Tae
name: Poletsky, Evgeny
name: Schmalz, Gerd
Publisher: name: arXiv
Year: 2008
Subjects: subject: Complex Variables (math.CV)
subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 32A99, 35A20, 35F99

description: The main result of the paper is the following generalization of Forelli's theorem: Suppose F is a holomorphic vector field with singular point at p, such that F is linearizable at p and the matrix is diagonalizable with the eigenvalues whose ratios are positive reals. Then any function $ϕ$ that has an asymptotic Taylor expansion at p and is holomorphic along the complex integral curves of F is holomorphic in a neighborhood of p. We also present an example to show that the requirement for ratios of the eigenvalues to be positive reals is necessary.
Il mistero della silice su Marte
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Il rover della NASA sta analizzando le rocce del Monte Sharp per capire i processi che hanno portato alla sedimentazione della silice sul Pianeta rosso. Dal 2014 Curiosity studia l'evoluzione geologica del Monte Sharp. Sette mesi fa è arrivato a "Marias Pass", dove la ChemCam ha rilevato abbondante silice in alcune rocce. Una vera e propria sorpresa per il team del JPL
Euclid: via libera alla costruzione
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2015

Euclid, la missione dell’ESA dedicata allo studio dell’universo oscuro, ha superato la Preliminary Design Review: il satellite e la sua strumentazione scientifica possono quindi essere costruiti. Una buona notizia per i ricercatori italiani
Cosmology with interaction in the dark sector
Creators: name: Costa, F. E. M.
name: Barboza, E. M.
name: Alcaniz, J. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Unless some unknown symmetry in Nature prevents or suppresses a non-minimal coupling in the dark sector, the dark energy field may interact with the pressureless component of dark matter. In this paper, we investigate some cosmological consequences of a general model of interacting dark matter-dark energy characterized by a dimensionless parameter $ε$. We derive a coupled scalar field version for this general class of scenarios and carry out a joint statistical analysis involving SNe Ia data ({Legacy} and {Constitution} sets), measurements of baryon acoustic oscillation peak at $z = 0.20$ (2dFGRS) and $z = 0.35$ (SDSS), and measurements of the Hubble evolution $H(z)$. For the specific case of vacuum decay ($w = -1$), we find that, although physically forbidden, a transfer of energy from dark matter to dark energy is favored by the data.
description: 5 pages, 5 figures, LaTeX
Il risveglio della forza stellare
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Nel complesso della nube molecolare di Orione, una giovane stella in fase di formazione sta lanciando nello spazio due spettacolari getti di materia, che ricordano le spade laser di Guerre Stellari. Le immagini ottenute dal telescopio spaziale Hubble hanno permesso di osservare questi particolari oggetti, noti come Herbig-Haro, avvolti dal gas e dalla polvere a cui gli astronomi danno la caccia
title: ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¸Ð²Ð¾Ð´ Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ¸. ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ¸Ð»Ð¸ÑÐµÐ»Ð¸, ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÑ ÐµÐ¼Ñ, Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿ ÑÐ°Ð±Ð¾ÑÑ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐ¾Ð´Ð½ÐµÐ², ÐÐ°Ð²ÐµÐ»
name: ÐÐ°Ð¹ÑÐ¼Ð°Ð½, ÐÐ°ÑÐ°Ð»Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2006
Subjects: ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ
Ð£ÑÐ¸Ð»Ð¸ÑÐµÐ»Ð¸ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ

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¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 150802 Â«ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ, Ð³Ð¸Ð´ÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ Ð¸ Ð³Ð¸Ð´ÑÐ¾Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ°Â», Ð° ÑÐ°ÐºÐ¶Ðµ 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¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 552700 Â«Ð­Ð½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ» (Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¸Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ 552704 Â«ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð³Ð¸Ð´ÑÐ¾Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð°Ð³ÑÐµÐ³Ð°ÑÑÂ» Ð¸ 552705 Â«Ð¡Ð¸ÑÑÐµÐ¼Ñ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¾Ð²Â»). ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÑÐµÐ¼Ñ Ð´Ð²ÑÑÐºÐ°ÑÐºÐ°Ð´Ð½ÑÑ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐ»ÐµÐºÑÑÐ¾Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ¸Ð»Ð¸ÑÐµÐ»ÐµÐ¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¸ Ð´Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ ÐºÐ°ÑÐµÐ´ÑÑ Ð³Ð¸Ð´ÑÐ¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¡ÐÐ±ÐÐÐ£ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ¾Ð² Â«ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¸Ð²Ð¾Ð´ Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ¸Â», Â«ÐÐ¸Ð½Ð°Ð¼Ð¸ÐºÐ° Ð¸ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð³Ð¸Ð´ÑÐ¾Ð¿Ð½ÐµÐ²Ð¼Ð¾ÑÐ¸ÑÑÐµÐ¼Â», Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ¾Ð²ÑÑ Ð¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð². ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð´ÑÑÐ³Ð¸Ñ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ð¼ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¸Ð²Ð¾Ð´.
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°.
Nuvole e schiarite attorno al buco nero
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Due telescopi spaziali, XMM-Newton dell’ESA e NuSTAR della NASA hanno osservato il denso anello di polveri e gas che circonda un buco nero super-massivo. Le accurate misure hanno permesso di rivelare per la prima volta che questa enorme struttura di materia a forma di ciambella non è compatta e uniforme, ma presenta una configurazione granulosa. A guidare la ricerca, a cui hanno partecipato anche due ricercatori dell’INAF, Andrea Marinucci, dell’Università Roma Tre e associato INAF
DAMPE: il nuovo cacciatore di materia oscura
Creators: Davide Patitucci
Publisher: name: Media Inaf
Year: 2015

Lanciato a 500 km di quota da una base cinese nel deserto di Gobi all'1:12 della notte, ora italiana, con i suoi quattro strumenti, uno dei quali realizzato a Perugia dall'INFN, DAMPE cercherà la sfuggente materia oscura in fotoni e particelle di origine cosmica che piovono incessantemente sulla Terra
Contact values for disparate-size hard-sphere mixtures
Creators: name: Santos, A.
name: Yuste, S. B.
name: de Haro, M. López
name: Alawneh, M.
name: Henderson, D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: A universality ansatz for the contact values of a multicomponent mixture of additive hard spheres is used to propose new formulae for the case of disparate-size binary mixtures. A comparison with simulation data and with a recent proposal by Alawneh and Henderson for binary mixtures shows reasonably good agreement with the predictions for the contact values of the large-large radial distribution functions. A discussion on the usefulness and limitations of the new proposals is also presented.
description: 12 pages, 10 figures; v2: typo in Eq. (28) corrected
La danza del pianeta gigante
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Grazie alle immagini ad altissima ottenute dal sistema di ottiche adattive del telescopio Magellan un team di astronomi è riuscito ad identificare i componenti di un sistema planetario estremamente peculiare: una stella simile al Sole, una stella nana e un pianeta gigante che “danza” tra le due stelle
Measurement invariance of a direct behavior rating multi item scale across occasions
Creators: name: Gebhardt, Markus
name: DeVries, J. M.
name: Jungjohann, J.
name: Casale, G.
name: Gegenfurtner, Andreas
name: Kuhn, T. J.
Publisher: name: Universität Regensburg
Year: 2019
Subjects: subject: direct behavior rating; test; sensitivity over time; rating; school; classroom behavior; progress monitoring
subject: 370 Erziehung, Schul- und Bildungswesen

description: Direct Behavior Rating (DBR) as a behavioral progress monitoring tool can be designed as longitudinal assessment with only short intervals between measurement points. The reliability of these instruments has been mostly evaluated in observational studies with small samples based on generalizability theory. However, for a standardized use in the pedagogical field, a larger and broader sample is required in order to assess measurement invariance between different participant groups and over time. Therefore, we constructed a DBR, the Questionnaire for Monitoring Behavior in Schools (QMBS) with multiple items to measure the occurrence of specific externalizing and internalizing student classroom behaviors on a Likert scale (1 = never to 7 = always). In a pilot study, two trained raters observed 16 primary education students and rated the student behavior over all items with a satisfactory reliability. In the main study, 108 regular primary school students, 97 regular secondary students, and 14 students in a clinical setting were rated daily over one week (five measurement points). Item response theory (IRT) analyses confirmed the technical adequacy of the instrument and latent growth models demonstrated the instrument’s stability over time. Further development of the instrument and study designs to implement DBRs is discussed.