cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Central Haemangioma of Mandible
Creators: name: Chaurasia, Akhilanand
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Head and neck
subject: CT
subject: Conventional radiography
subject: Diagnostic procedure
subject: Haemangioma

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 17 years
description: Clinical History: A 17 year old female complaining of a swelling involving the right side of her lower jaw. The swelling was progressively increasing in size and causing facial asymmetry.The patient also reported exfoliation of the right canine and 1st premolar spontaneous... Final Diagnosis: Central Hemangioma of Mandible
Chimeras in a Network of Three Oscillator Populations with Varying Network Topology
Creators: name: Martens, Erik Andreas
Publisher: name: arXiv
Year: 2010
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: We study a network of three populations of coupled phase oscillators with identical frequencies. The populations interact nonlocally, in the sense that all oscillators are coupled to one another, but more weakly to those in neighboring populations than to those in their own population. Using this system as a model system, we discuss for the first time the influence of network topology on the existence of so called chimera states. In this context, the network with three populations represents an interesting case because the populations may either be connected as a triangle, or as a chain, thereby representing the simplest discrete network of either a ring or a line segment of oscillator populations. We introduce a special parameter that allows us to study the effect of breaking the triangular network structure, and to vary the network symmetry continuously such that it becomes more and more chain-like. By showing that chimera states only exist for a bounded set of parameter values we demonstrate that their existence depends strongly on the underlying network structures. We conclude that chimeras exist on networks with a chain-like character, which indicates that it might be possible to observe chimeras on a continuous line segment of oscillators.
description: 9 pages, 4 figures
title: ÐÐ±ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸Ð½ÑÐµÑÐ¿ÑÐµÑÐ°ÑÐ¸Ð¸ ÑÐ½Ð¸Ð²ÐµÑÑÐ°Ð»ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑÐ½ÑÑ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¾Ð² Ð½Ð° ÑÑÐ¾ÐºÐµ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ·ÑÐºÐ°
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»ÐµÐºÑÐµÐµÐ²Ð°, 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: Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ
Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¹ ÑÐ·ÑÐº
ÑÐ½Ð¸Ð²ÐµÑÑÐ°Ð»ÑÐ½ÑÐµ ÐºÑÐ»ÑÑÑÑÐ½ÑÐµ ÐºÐ¾Ð½ÑÐµÐ¿ÑÑ
ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐµÑÐ¿ÑÐµÑÐ°ÑÐ¸Ð¸ ÑÐ½Ð¸Ð²ÐµÑÑÐ°Ð»ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑÐ½ÑÑ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¾Ð². ÐÐ»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÑÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÑ Ð°Ð²ÑÐ¾ÑÐ°Ð¼Ð¸ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ñ Ð² ÑÐµÐ±Ñ 3 Ð³ÑÑÐ¿Ð¿Ñ. ÐÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ðµ Ð´Ð°Ð½Ð½ÑÑ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð²ÑÑÐ¸Ñ ÑÑÐ¿ÐµÑ ÑÑÐµÐ½Ð¸ÐºÐ¾Ð² Ð² Ð¼ÐµÐ¶ÐºÑÐ»ÑÑÑÑÐ½Ð¾Ð¼ Ð¾Ð±ÑÐµÐ½Ð¸Ð¸, Ð¸ Ð¿Ð¾Ð¼Ð¾Ð¶ÐµÑ Ð¸Ð·Ð±ÐµÐ¶Ð°ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹ Ð¼ÐµÐ¶ÐºÑÐ»ÑÑÑÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ°.
Magnetic anisotropy and low-energy spin dynamics in the van der Waals compounds Mn$_{2}$P$_{2}$S$_{6}$ and MnNiP$_{2}$S$_{6}$
Creators: name: Abraham, J. J.
name: Senyk, Y.
name: Shemerliuk, Y.
name: Selter, S.
name: Aswartham, S.
name: Büchner, B.
name: Kataev, V.
name: Alfonsov, A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report the detailed high-field and high-frequency electron spin resonance (HF-ESR) spectroscopic study of the single-crystalline van der Waals compounds Mn$_{2}$P$_{2}$S$_{6}$ and MnNiP$_{2}$S$_{6}$. Analysis of magnetic excitations shows that in comparison to Mn$_{2}$P$_{2}$S$_{6}$ increasing the Ni content yields a larger magnon gap in the ordered state and a larger g-factor value and its anisotropy in the paramagnetic state. The studied compounds are found to be strongly anisotropic having each the unique ground state and type of magnetic order. Stronger deviation of the g-factor from the free electron value in the samples containing Ni suggests that the anisotropy of the exchange is an important contributor to the stabilization of a certain type of magnetic order with particular anisotropy. At temperatures above the magnetic order, we have analyzed the spin-spin correlations resulting in a development of slowly fluctuating short-range order. They are much stronger pronounced in MnNiP$_{2}$S$_{6}$ compared to Mn$_{2}$P$_{2}$S$_{6}$. The enhanced spin fluctuations in MnNiP$_{2}$S$_{6}$ are attributed to the competition of different types of magnetic order. Finally, the analysis of the temperature dependent critical behavior of the magnon gaps below the ordering temperature in Mn$_{2}$P$_{2}$S$_{6}$ suggests that the character of the spin wave excitations in this compound undergoes a field induced crossover from a 3D-like towards 2D XY regime.
Disintegration of Long-Period Comet C/2021 A1 (Leonard)
Creators: name: Jewitt, David
name: Kim, Yoonyoung
name: Mattiazzo, Michael
name: mutchler, Max
name: Li, Jing
name: Agarwal, Jessica
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present imaging observations of the disintegrating long-period comet C/2021 A1 (Leonard). High resolution observations with Hubble Space Telescope show no evidence for surviving fragments, and place a 3 sigma upper limit to their possible radius about 60 m (albedo 0.1 assumed). In contrast, wide field observations from the Swan Hill Observatory, Australia, show an extensive debris cloud, the cross-section and estimated mass of which are consistent with complete disintegration of the nucleus near mid- December 2021 (at about 0.8 au). Two methods give the pre-disruption nucleus radius, r = 0.6+/-0.2 km. Tidal, collisional, sublimation and pressure-confined explosion models provide implausible explanations of the disintegration. However, rotational instability driven by outgassing torques has a very short timescale (of order 0.1 year) given the orbit and size of the C/2021 A1 nucleus, and offers the most plausible mechanism for the disruption. Initial rotational breakup is accelerated by the exposure and strong sublimation of previously buried volatiles, leading to catastrophic destruction of the nucleus.
description: 35 pages, 7 figures
Impact of chemical short-range order on radiation damage in Fe-Ni-Cr alloys
Creators: name: Arkoub, Hamdy
name: Jin, Miaomiao
Publisher: name: arXiv
Year: 2023
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: Chemical short-range order (CSRO), a form of nanoscale special atom arrangement, has been found to significantly alter material properties such as dislocation motion and defect dynamics in various alloys. Here, we use Fe-Ni-Cr alloys to demonstrate how CSRO affects defect properties and radiation behavior, based on extensive molecular dynamics simulations. Statistically significant results are obtained regarding radiation-induced defect propensity, defect clustering, and chemical mixing as a function of dose for three CSRO levels. The perfect random solution as an energetically unfavorable state (negative stacking fault energy) shows the strongest tendency to enable diffusion, while a high CSRO degree scenario generally reduces the effective defect diffusivity due to trapping effects, leading to distinct defect dynamics. Notably, in the high-CSRO scenario, interstitial clusters are Cr-rich and interstitial loops preferentially reside in/near the Cr-rich CSRO domains. It is also identified that CSRO is dynamically evolving in a decreasing or increasing manner upon continuous irradiation, reaching a steady-state value. These new understandings suggest the importance of incorporating the effect of CSRO in investigating radiation-driven microstructural evolution.
description: 6 figures
title: ÐÐ¸Ð·Ð½ÐµÑ-ÑÐµÐ½ÑÑ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÑÑÑÐºÑÑÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÑÐµÐºÐ»ÐµÐ½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¦Ð¾Ð³ÑÐ¶Ð°Ð²ÑÐ»Ð°Ð½, ÐÐ¾Ñ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: 2016
Subjects: ÑÑÑÑÐºÑÑÑÐ½Ð¾Ðµ Ð¾ÑÑÐµÐºÐ»ÐµÐ½Ð¸Ðµ
ÑÑÑÑÐºÑÑÑÐ½ÑÐ¹ ÑÐ¸Ð»Ð¸ÐºÐ¾Ð½Ð¾Ð²ÑÐ¹ Ð³ÐµÑÐ¼ÐµÑÐ¸Ðº
Ð½Ð°ÐºÐ»Ð¾Ð½Ð½Ð¾Ðµ Ð¾ÑÑÐµÐºÐ»ÐµÐ½Ð¸Ðµ
structure glazing
structural silicone sealent
sloped glazing

description: Ð¢ÐµÐ¼Ð° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - âÐÐ¸Ð·Ð½ÐµÑ ÑÐµÐ½ÑÑ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÑÑÑÐºÑÑÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÑÐµÐºÐ»ÐµÐ½Ð¸Ñâ. Ð Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐ°ÑÑÐµÑÑ ÑÐ²Ð¾Ð² ÑÑÑÑÐºÑÑÑÐ½Ð¾Ð³Ð¾ ÑÐ¸Ð»Ð¸ÐºÐ¾Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð³ÐµÑÐ¼ÐµÑÐ¸ÐºÐ° Ð² ÑÑÑÑÐºÑÑÑÐ½Ð¾Ð¼ Ð¾ÑÑÐµÐºÐ»ÐµÐ½Ð¸Ð¸, Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½ Ð³ÑÐ°ÑÐ¸Ðº Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐ²Ð¾Ð² ÑÐ¸Ð»Ð¸ÐºÐ¾Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð³ÐµÑÐ¼ÐµÑÐ¸ÐºÐ° Ð¾Ñ ÑÐ³Ð»Ð° ÑÐ°ÑÐ°Ð´Ð¾Ð². Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¿ÑÐ¾ÐµÐºÑÐ½Ð°Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ Ð½Ð° Ð²Ð¾Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¾Ð±ÑÐµÐºÑÐ° Ð¿Ð¾Ð°Ð´ÑÐµÑÑ: Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³, ÐÑÐ¸Ð¼Ð¾ÑÑÐºÐ¸Ð¹ ÑÐ°Ð¹Ð¾Ð½, ÑÐ». ÐÐ¿ÑÐ¸ÐºÐ¾Ð², 31 ÐºÐ¾ÑÐ¿ÑÑ 2, Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÐÐ¾ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð¿ÑÐ°Ð²Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð Ð¤ Ð¾Ñ 16 ÑÐµÐ²ÑÐ°Ð»Ñ 2008 Ð³. â 87 Â«Ð ÑÐ¾ÑÑÐ°Ð²ÐµÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ½Ð¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÑ Ðº Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸ÑÂ».
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ ÑÐ²Ð°ÑÐºÐ¸ Ð¿Ð¾Ð´ Ð²Ð¾Ð´Ð¾Ð¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ³Ð»Ð¾Ð², Ð Ð°Ð¼Ð¸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: 2016
Subjects: Ð¿Ð¾Ð´Ð²Ð¾Ð´Ð½Ð°Ñ ÑÐ²Ð°ÑÐºÐ°
Ð³Ð¸Ð¿ÐµÑÐ±Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ²Ð°ÑÐºÐ°
Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ Ð¿Ð¾Ð´Ð²Ð¾Ð´Ð½Ð°Ñ ÑÐ²Ð°ÑÐºÐ°
ÐºÐµÑÑÐ¾Ð½
Ð¿Ð¾Ð´Ð²Ð¾Ð´Ð½Ð°Ñ ÐºÐ°Ð¼ÐµÑÐ°
underwater welding
hyperbaric welding
mechanized underwater welding
caisson
underwater camera

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ ÑÐ´ÐµÐ»Ð°Ð½ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÐ¹ Ð¾Ð±Ð·Ð¾Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð¿Ð¾Ð´Ð²Ð¾Ð´Ð½Ð¾Ð¹ ÑÐ²Ð°ÑÐºÐ¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ðµ Ð¿ÑÐ¸ ÑÑÐ¾Ð¼. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ ÑÐ²Ð°ÑÐ¾ÑÐ½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐ¸ ÑÑÐ¾Ð¼. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸.
The Massive Progenitor of the Type II-Linear SN 2009kr
Creators: name: Elias-Rosa, N.
name: Van Dyk, S. D.
name: Li, W.
name: Miller, A. A.
name: Silverman, J. M.
name: Ganeshalingam, M.
name: Boden, A. F.
name: Kasliwal, M. M.
name: Vinko, J.
name: Cuillandre, J. -C.
name: Filippenko, A. V.
name: Steele, T. N.
name: Bloom, J. S.
name: Griffith, C. V.
name: Kleiserand, I. K. W.
name: Foley, R. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present early-time photometric and spectroscopic observations of supernova (SN) 2009kr in NGC 1832. We find that its properties to date support its classification as Type II-linear (SN II-L), a relatively rare subclass of core-collapse supernovae (SNe). We have also identified a candidate for the SN progenitor star through comparison of pre-explosion, archival images taken with WFPC2 onboard the Hubble Space Telescope (HST) with SN images obtained using adaptive optics (AO) plus NIRC2 on the 10-m Keck-II telescope. Although the host galaxy's substantial distance (~26 Mpc) results in large uncertainties in the relative astrometry, we find that if this candidate is indeed the progenitor, it is a highly luminous (M_V = -7.8 mag) yellow supergiant with initial mass ~18-24 M_sun. This would be the first time that a SN II-L progenitor has been directly identified. Its mass may be a bridge between the upper initial mass limit for the more common Type II-plateau SNe (SNe II-P) and the inferred initial mass estimate for one Type II-narrow SN (SN IIn).
description: Accepted for publication in The Astrophysical Journal Letters
Recent Trend of Nanotechnology Applications to Improve Bio-accessibility of Lycopene by Nanocarrier: A Review
Creators: name: Alam, Mohammad Anwar Ul
name: Khatun, Mhamuda
name: Alam, Mohammad Arif Ul
Publisher: name: arXiv
Year: 2023
Subjects: subject: Biomolecules (q-bio.BM)
subject: FOS: Biological sciences

description: Lycopene, rich in red, yellow, or orange-colored fruits and vegetables, is the most potent antioxidant among the other carotenoids available in human blood plasma. It is evident that regular lycopene intake can prevent chronic diseases like cardiovascular diseases, type-2 diabetes, hypertension, kidney diseases and cancer. However, thermal processing, light, oxygen, and enzymes in gastrointestinal tract (GIT) compromise the bioaccessibility and bioavailability of lycopene ingested through diet. Nanoencapsulation provides a potential platform to prevent lycopene from light, air oxygen, thermal processing and enzymatic activity of the human digestive system. Physicochemical properties evidenced to be the potential indicator for determining the bioaccessibility of encapsulated bioactive compounds like lycopene. By manipulating the size or hydrodynamic diameter, zeta potential value or stability, polydispersity index or homogeneity and functional activity or retention of antioxidant properties observed to be the most prominent physicochemical properties to evaluate beneficial effect of implementation of nanotechnology on bioaccessibility study. Moreover, the molecular mechanism of the bioavailability of nanoparticles is not yet to be understood due to lack of comprehensive design to identify nanoparticles' behaviors if ingested through oral route as functional food ingredients. This review paper aims to study and leverage existing techniques about how nanotechnology can be used and verified to identify the bioaccessibility of lycopene before using it as a functional food ingredient for therapeutic treatments.
Core-mantle interactions for Mercury
Creators: name: Noyelles, B.
name: Dufey, J.
name: Lemaitre, A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Mercury is the target of two space missions: MESSENGER (NASA) which orbit insertion is planned for March 2011, and ESA/JAXA BepiColombo, that should be launched in 2014. Their instruments will observe the surface of the planet with a high accuracy (about 1 arcsec for BepiColombo), what motivates studying its rotation. Mercury is assumed to be composed of a rigid mantle and an at least partially molten core. We here study the influence of the core-mantle interactions on the rotation perturbed by the solar gravitational interaction, by modeling the core as an ellipsoidal cavity filled with inviscid fluid of constant uniform density and vorticity. We use both analytical (Lie transforms) and numerical tools to study this rotation, with different shapes of the core. We express in particular the proper frequencies of the system, because they characterize the response of Mercury to the different solicitations, due to the orbital motion of Mercury around the Sun. We show that, contrary to its size, the shape of the core cannot be determined from observations of either longitudinal or polar motions. However, we highlight the strong influence of a resonance between the proper frequency of the core and the spin of Mercury that raises the velocity field inside the core. We show that the key parameter is the polar flattening of the core. This effect cannot be directly derived from observations of the surface of Mercury, but we cannot exclude the possibility of an indirect detection by measuring the magnetic field.
description: MNRAS, in press
title: Ð Ð°Ð·ÑÐµÐ¼Ð½ÑÐµ Ð¸ Ð½ÐµÑÐ°Ð·ÑÐµÐ¼Ð½ÑÐµ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ
title: Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÐºÑÑÑÑ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÑÑÐµÐ½Ð¸Ñ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¾Ð², ÐÐµÐ¾Ð½Ð¸Ð´
Publisher: name: ÐÐÐ Ð¸Ð¼. Ð. Ð. ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð°
Year: 1981
Subjects: Ð§ÐµÑÑÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ

description: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÐ¸Ñ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ Ð²ÑÑÐµÑÑÐ¸Ð²Ð°Ð½Ð¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ° "ÐÐ°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÐµÑÑÐµÐ½Ð¸Ðµ". Ð ÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ñ Ðº Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ ÐºÐ°ÑÐµÐ´ÑÐ¾Ð¹ Â«ÐÐ°ÑÐµÑÑÐ°ÑÐµÐ»ÑÐ½Ð°Ñ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÂ» Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð¼Ð¸ÑÑÐ¸ÐµÐ¹ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¾-Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°.
Secondary metabolite arsenal of an opportunistic pathogenic fungus
Creators: name: Bignell, Elaine
name: Cairns, Timothy C.
name: Throckmorton, Kurt
name: Nierman, William C.
name: Keller, Nancy P.
Publisher: name: Technische Universität Berlin
Year: 2016
Subjects: subject: 570 Biowissenschaften; Biologie
subject: Aspergillus fumigatus
subject: secondary metabolism
subject: gene cluster
subject: fungal infection

description: Aspergillus fumigatus is a versatile fungus able to successfully exploit diverse environments from mammalian lungs to agricultural waste products. Among its many fitness attributes are dozens of genetic loci containing biosynthetic gene clusters (BGCs) producing bioactive small molecules (often referred to as secondary metabolites or natural products) that provide growth advantages to the fungus dependent on environment. Here we summarize the current knowledge of these BGCs—18 of which can be named to product—their expression profiles in vivo, and which BGCs may enhance virulence of this opportunistic human pathogen. Furthermore, we find extensive evidence for the presence of many of these BGCs, or similar BGCs, in distantly related genera including the emerging pathogen Pseudogymnoascus destructans, the causative agent of white-nose syndrome in bats, and suggest such BGCs may be predictive of pathogenic potential in other fungi.
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð°: ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ
Creators: name: ÐÐºÑÐµÐ¿Ð¸Ð»Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: Ð§ÑÐ´Ð¸Ð½Ð¾Ð²ÑÐºÐ¸Ñ, ÐÐ³Ð¾ÑÑ
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð² Ð¸Ð½ÑÐµÑÐµÑÐ°Ñ  ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ", Ð¼ÐµÐ¶Ð²ÑÐ·Ð¾Ð²ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2019; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019

description: Ð¡ÑÐ°ÑÑÑ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼ÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² ÑÐ¸ÑÑÐ¾Ð²ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð´ÑÑÐ¸Ðµ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð³Ð¾ÑÐ¾Ð²Ð½Ð¾ÑÑÑ Ðº Ð½Ð¸Ð¼ Ð½Ð°ÑÐµÐ¹ ÑÑÑÐ°Ð½Ñ. ÐÐ¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑÑÑ ÑÐ²ÑÐ·Ñ Ð¼ÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¼ÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸ Ð½Ð° Ð¾Ð±ÑÐµÑÑÐ²Ð¾ Ð² ÑÐµÐ»Ð¾Ð¼.
A silver bullet in a golden age of functional genomics: the impact of Agrobacterium-mediated transformation of fungi
Creators: name: Idnurm, Alexander
name: Bailey, Andy M.
name: Cairns, Timothy C.
name: Elliott, Candace E.
name: Foster, Gary D.
name: Ianiri, Giuseppe
name: Jeon, Junhyun
Publisher: name: Technische Universität Berlin
Year: 2017
Subjects: subject: 570 Biowissenschaften; Biologie
subject: functional genomics
subject: mycota
subject: pathogenicity genes
subject: Rhizobium radiobacter
subject: transfer DNA

description: The implementation of Agrobacterium tumefaciens as a transformation tool revolutionized approaches to discover and understand gene functions in a large number of fungal species. A. tumefaciens mediated transformation (AtMT) is one of the most transformative technologies for research on fungi developed in the last 20 years, a development arguably only surpassed by the impact of genomics. AtMT has been widely applied in forward genetics, whereby generation of strain libraries using random T-DNA insertional mutagenesis, combined with phenotypic screening, has enabled the genetic basis of many processes to be elucidated. Alternatively, AtMT has been fundamental for reverse genetics, where mutant isolates are generated with targeted gene deletions or disruptions, enabling gene functional roles to be determined. When combined with concomitant advances in genomics, both forward and reverse approaches using AtMT have enabled complex fungal phenotypes to be dissected at the molecular and genetic level. Additionally, in several cases AtMT has paved the way for the development of new species to act as models for specific areas of fungal biology, particularly in plant pathogenic ascomycetes and in a number of basidiomycete species. Despite its impact, the implementation of AtMT has been uneven in the fungi. This review provides insight into the dynamics of expansion of new research tools into a large research community and across multiple organisms. As such, AtMT in the fungi, beyond the demonstrated and continuing power for gene discovery and as a facile transformation tool, provides a model to understand how other technologies that are just being pioneered, e.g. CRISPR/Cas, may play roles in fungi and other eukaryotic species.
The nature of HI absorbers in GRB afterglows: clues from hydrodynamic simulations
Creators: name: Pontzen, Andrew
name: Deason, Alis
name: Governato, Fabio
name: Pettini, Max
name: Wadsley, James
name: Quinn, Thomas
name: Brooks, Alyson
name: Bellovary, Jillian
name: Fynbo, Johan P. U.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In recent work, we have shown that it is possible to link quantitatively many aspects of damped Lyman alpha (DLA) absorbers in the spectra of quasars to high resolution simulations of galaxy formation. Using runs from the same series of hydrodynamic numerical studies, we consider the expected properties of Lyman alpha absorbers seen in the spectra of high redshift (z>2) gamma ray burst afterglows (GRB-DLAs). If GRBs are associated with the death of massive stars, their afterglows provide insights into otherwise unprobed regions of protogalactic objects, but detailed physical interpretations are currently embryonic. We find that median impact parameters (measured from the potential minimum) are approximately 1 kpc for GRBs compared with 4 kpc for QSO-DLAs. However, an equally important difference is that GRB-DLAs are predominantly associated with halos of mass 10^1010^19 cm^-2, but they somewhat underpredict the incidence of low column densities N_HI<10^19 cm^-2. Line-of-sight neutral gas metallicities predicted by our simulations (10^-2 < Z/Z_sol < 1) are consistent with the modest observational constraints. Because of large internal dispersions in gas metallicities, this agreement is not significantly compromised by imposing a cut-off on the metallicity of stars able to launch GRBs (Z_star
description: Typos fixed; minor clarifications. 13 pages, 7 figures, accepted for publication in MNRAS
title: Ð¡Ð¸ÑÑÐµÐ¼Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ Ð¼Ð¾Ð´ÑÐ»ÐµÐ¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ½Ð¸Ñ, 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: 2016
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¼ÐµÑÐ¾Ð´Ñ

description: Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ±Ð¾ÑÐºÐ¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ Ð¼Ð¾Ð´ÑÐ»ÐµÐ¹ Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ ÑÑÐµÐ±ÑÐµÐ¼ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸Ñ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ½Ð°Ð»Ð¸Ð· Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð» Ð²ÑÑÐ²Ð¸ÑÑ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐ¸Ðµ Ð´Ð»Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÑÐµÐ½Ð´ Ð´Ð»Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð±ÑÐ» Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½ 16-ÑÐ¸ ÑÐ°Ð·ÑÑÐ´Ð½ÑÐ¹ Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑ PIC24HJ64GP206. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¿ÐµÑÐ°ÑÐ½Ð°Ñ Ð¿Ð»Ð°ÑÐ° Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¼ Ð¿Ð°ÐºÐµÑÐµ P-CAD 2004 (Ñ Ð½Ð°ÑÐ°Ð»Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¸Ð°Ð»ÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°, Ð·Ð°ÑÐµÐ¼ Ð¿Ð¾ÑÐ»Ðµ ÑÑÐ°ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð¾Ð»ÑÑÐ¸Ð»Ð¸ ÑÐ°Ð·Ð²Ð¾Ð´ÐºÑ Ð¿ÐµÑÐ°ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑ). ÐÑÐ»Ð¾ ÑÐ¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¸ÑÐ¿ÑÐ°Ð²Ð½Ð¾Ð³Ð¾ Ð¸ Ð½ÐµÐ¸ÑÐ¿ÑÐ°Ð²Ð½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐ´Ð²Ð¸Ð³Ð°ÐµÑÑÑ Ð³Ð¸Ð¿Ð¾ÑÐµÐ·Ð° Ð¾ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾Ð¹ Ð½ÐµÐ¸ÑÐ¿ÑÐ°Ð²Ð½Ð¾ÑÑÐ¸, Ð¸ Ð·Ð°ÑÐµÐ¼ Ð³Ð¸Ð¿Ð¾ÑÐµÐ·Ð° Ð¿ÑÐ¾Ð²ÐµÑÑÐµÑÑÑ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸ÑÐ¼Ð¸
Stochastic model of optical variability of BL Lacertae
Creators: name: Blinov, D. A.
name: Hagen-Thorn, V. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use optical photometric and polarimetric data of BL Lacertae that cover a period of 22 years to study the variability of the source. The long-term observations are employed for establishing parameters of a stochastic model consisting of the radiation from a steady polarized source and a number of variable components with different polarization parameters, proposed by Hagen-Thorn et al. earlier. We infer parameters of the model from the observations using numerical simulations based on a Monte Carlo method, with values of each model parameter selected from a Gaussian distribution. We determine the best set of model parameters by comparing model distributions to the observational ones using the chi-square criterion. We show that the observed photometric and polarimetric variability can be explained within a model with a steady source of high polarization, ~40%, and with direction of polarization parallel to the parsec scale jet, along with 10+-5 sources of variable polarization.
description: 4 pages, 10 figures, published by Astronomy and Astrophysics; v2: typos corrected
Genially : se démarquer avec un CV infographique créatif
Creators: name: BRETON Virginie
name: BARATIN Aude
Publisher: name: Zenodo
Year: 2025

description: Vous trouverez :

- Le déroulé formateur de la formation Genially : se démarquer avec un CV infographique créatif

- Le support de présentation Genially de l'atelier avec les exercices et les liens des modèles de CV.
Appendix 2 Raw data for CD013121
Creators: name: Gurusamy, Kurinchi
Publisher: name: Zenodo
Year: 2021

description: This is raw data for the Cochrane review: “Primary prevention of variceal bleeding in people with oesophageal varices due to liver cirrhosis: a network meta-analysis” (DOI: 10.1002/14651858.CD013121)
Genially : se démarquer avec un CV infographique créatif
Creators: name: BRETON Virginie
name: BARATIN Aude
Publisher: name: Zenodo
Year: 2024

description: Vous trouverez :

- Le déroulé formateur de la formation Genially : se démarquer avec un CV infographique créatif

- Le support de présentation Genially de l'atelier avec les exercices et les liens des modèles de CV.
title: Ð¢Ð¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ Ñ Ð°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ²Ð¾ÑÐ¾Ð³Ð°, ÑÐµÐ°Ð»Ð¸Ð·ÑÐµÐ¼Ð¾Ð³Ð¾ Ð² ÑÐ¾Ð·Ð½Ð¸ÑÐ½ÑÑ ÑÐ¾ÑÐ³Ð¾Ð²ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ±Ð°ÑÐ¾Ð², Ð Ð°Ñ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: ÑÐ²Ð¾ÑÐ¾Ð³
Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð°
Ð¾ÑÐ³Ð°Ð½Ð¾Ð»ÐµÐ¿ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ²Ð¾ÑÐ¾Ð³Ð°
ÑÐ¸Ð·Ð¸ÐºÐ¾-Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ²Ð¾ÑÐ¾Ð³Ð°

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title: Ð¡ÐµÑÐ²Ð¸Ñ-Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ðµ Ð³ÑÐ¸Ð´-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð´Ð»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ Ð±Ð¸Ð¾Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÐ¾Ð·Ð´Ð¾Ð², 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: 2017
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°
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ÐÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ Ð½Ð° Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¼Ð°ÑÐ¸Ð½Ð°Ñ
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾ÐºÑÑÐ¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð´Ð¾ÑÑÑÐ¿Ð° Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ðº ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ðµ. ÐÐ°Ð½Ð½Ð¾Ðµ Ð¾ÐºÑÑÐ¶ÐµÐ½Ð¸Ðµ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð±ÑÐ¸Ð¼ ÑÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð´Ð»Ñ Ð½ÐµÐ±Ð¾Ð»ÑÑÐ¸Ñ ÑÐµÑÐµÐ¹ Ð¸ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ ÐºÐ°Ðº Ð² Ð½Ð°ÑÑÐ½ÑÑ, ÑÐ°Ðº Ð¸ Ð² ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ ÑÐµÐ»ÑÑ. Ð Ð±Ð¸Ð¾Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐµ ÑÑÑÐµÑÑÐ²ÑÐµÑ Ð±Ð¾Ð»ÑÑÐ¾Ðµ ÑÐ¸ÑÐ»Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² ÐºÐ¾Ð¼Ð°Ð½Ð´Ð½Ð¾Ð¹ ÑÑÑÐ¾ÐºÐ¸, ÑÐºÐ¾ÑÐ¾ÑÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¼Ð¾Ð¶Ð½Ð¾ ÑÐ²ÐµÐ»Ð¸ÑÐ¸ÑÑ Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÑ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ð¹. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, ÑÑÑÐµÑÑÐ²ÑÐµÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð·Ð°Ð¿ÑÑÐºÐ° Ð±Ð¾Ð»ÑÑÐ¾Ð³Ð¾ ÑÐ¸ÑÐ»Ð° Ð¾Ð´Ð½Ð¾ÑÐ¸Ð¿Ð½ÑÑ Ð·Ð°Ð´Ð°Ñ. ÐÐ»Ñ ÑÑÐ¸Ñ ÑÐµÐ»ÐµÐ¹ Ð¾ÑÐ»Ð¸ÑÐ½Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¸Ñ Ð³ÑÐ¸Ð´ - Ð¾Ð´Ð¸Ð½ Ð¸Ð· Ð²Ð¸Ð´Ð¾Ð² ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¸Ð·ÑÑÐµÐ½Ð° Ð¿ÑÐµÐ´Ð¼ÐµÑÐ½Ð°Ñ Ð¾Ð±Ð»Ð°ÑÑÑ; ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð²Ð°Ð¶Ð½ÑÐµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÑ. ÐÑÐ¸Ð´ÑÐ¼Ð°Ð½Ð° Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ°, Ð¿Ð¾Ð»Ð½Ð¾ÑÑÑÑ ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÑÑÑÐ°Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼. Ð ÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½ web-ÑÐµÑÐ²Ð¸Ñ, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐµ Ð¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ð¹ ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ñ Ð³ÑÐ¸Ð´-ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹. ÐÐ»Ñ Ð¿ÑÐ¸Ð¼ÐµÑÐ° ÑÐ°Ð±Ð¾ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ²Ð¸ÑÐ° ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½ ÐºÐ»Ð¸ÐµÐ½ÑÑÐºÐ¸Ð¹ Ð¸Ð½ÑÐµÑÑÐµÐ¹Ñ Ð´Ð»Ñ ÑÐµÐ¼ÐµÐ¹ÑÑÐ²Ð° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ BLAST. ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼, ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð² ÑÑÐ¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°Ñ, ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð´Ð½Ð¸Ð¼ Ð¸Ð· ÑÐ°Ð¼ÑÑ Ð²Ð¾ÑÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð² Ð·Ð°Ð´Ð°ÑÐ°Ñ Ð±Ð¸Ð¾Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ¸. Ð¡Ð¾Ð·Ð´Ð°Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð¾ÑÐ²ÐµÑÐ°ÐµÑ Ð²ÑÐµÐ¼ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ Ð·Ð°ÐºÐ°Ð·ÑÐ¸ÐºÐ°, ÐºÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, Ð¼Ð°ÑÑÑÐ°Ð±Ð¸ÑÑÐµÐ¼Ð°, Ð¿ÑÐ°ÐºÑÐ¸ÑÐ½Ð°, ÑÐ½Ð¸Ð²ÐµÑÑÐ°Ð»ÑÐ½Ð° Ð¸ Ð¾ÑÐ»Ð¸ÑÐ½Ð¾ ÑÐµÐ±Ñ Ð¿Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑ Ð¿ÑÐ¸ Ð±Ð¾Ð»ÑÑÐ¾Ð¼ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ðµ Ð·Ð°Ð¿ÑÐ¾ÑÐ¾Ð² Ð² ÑÐ¸ÑÑÐµÐ¼Ñ.
Bouncing cosmology from nonlinear dark energy with two cosmological constants
Creators: name: Burkmar, Molly
name: Bruni, Marco
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We explore the dynamics of FLRW cosmologies which consist of dark matter, radiation and dark energy with a quadratic equation of state. Standard cosmological singularities arise due to energy conditions which are violated by dark energy, therefore we focus our analysis on non-singular bouncing and cyclic cosmologies, in particular focusing on the possibility of closed models always having a bounce for any initial conditions. We analyse the range of dynamical behaviour admitted by the system, and find a class of closed models that admit a non-singular bounce, with early- and late-time accelerated expansion connected by a decelerating phase. In all cases, we find the bouncing models are only relevant when dark matter and radiation appear at a certain energy scale, and so require a period such as reheating. We then investigate imposing an upper bound on the dark matter and radiation, such that their energy densities cannot become infinite. We find that bounces are always the general closed model, and a class of models exist with early- and late-time acceleration, connected by a decelerating phase. We also consider parameter values for the dark energy component, such that the discrepancy between the observed value of $Λ$ and the theoretical estimates of the contributions to the effective cosmological constant expected from quantum field theory would be explained. However, we find that the class of models left does not allow for an early- and late-time accelerated expansion, connected by a decelerating period where large-scale structure could form. Nonetheless, our qualitative analysis serves as a basis for the construction of more realistic models with realistic quantitative behaviour.
description: 26 pages, 21 figures. Updated version to reflect changes made for publication
Systematic analysis of the impacts of symmetry energy parameters on neutron star properties
Creators: name: Patra, N. K.
name: Venneti, Anagh
name: Imam, Sk Md Adil
name: Mukherjee, Arunava
name: Agrawal, B. K.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The impacts of various symmetry energy parameters on the properties of neutron stars (NSs) have been recently investigated, and the outcomes are at variance, as summarized in Table III of Phys. Rev. D 106, 063005 (2022). We have systematically analyzed the correlations of slope and curvature parameters of symmetry energy at the saturation density ($ρ_0=0.16 \text{fm}^{-3}$) with the tidal deformability and stellar radius of non-spinning neutron stars in the mass range of $1.2 - 1.6 M_\odot$ using a large set of minimally constrained equations of state (EoSs). The EoSs at low densities correspond to the nucleonic matter and are constrained by empirical ranges of a few low-order nuclear matter parameters from the finite nuclei data and the pure neutron matter EoS from chiral effective field theory. The EoSs at high densities ($ρ> 1.5 - 2ρ_0$) are obtained by a parametric form for the speed of sound that satisfies the causality condition. Several factors affecting the correlations between the NS properties and the individual symmetry energy parameters usually encountered in the literature are considered. These correlations are quite sensitive to the choice of the distributions of symmetry energy parameters and their interdependence. But, variations of NS properties with the pressure of $β-$ equilibrated matter at twice the saturation density remain quite robust which maybe due to the fact that the pressure depends on the combination of multiple nuclear matter parameters that describe the symmetric nuclear matter as well as the density dependence of the symmetry energy. Our results are practically insensitive to the behavior of EoS at high densities.
description: 14 pages, 8 figures, 4 tables (Published in PRC)
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ½Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð³Ð½Ð°Ð»Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÑÐ°Ð¼Ð²Ð°Ñ Ð¸ ÑÑÐ¾Ð»Ð»ÐµÐ¹Ð±ÑÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¯Ð¼ÑÐ¸ÐºÐ¾Ð², ÐÑÑÑ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Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ°
ÑÑÐ¾Ð»Ð»ÐµÐ¹Ð±ÑÑ
ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð³Ð½Ð°Ð»Ð°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð´Ð»Ñ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÑ ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð² Ñ Ð¿ÐµÐ´Ð°Ð»ÐµÐ¹ Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ ÑÑÐ¾Ð»Ð»ÐµÐ¹Ð±ÑÑÐ° Ð¸Ð»Ð¸ Ñ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° ÑÑÐ°Ð¼Ð²Ð°Ñ Ð² ÐºÐ¾Ð´ ÐÑÐµÑ, Ð¿ÑÐ¸Ð³Ð¾Ð´Ð½ÑÐ¹ Ð´Ð»Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÐ³Ð¾Ð²ÑÐ¼ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¾Ð¼. ÐÐ±ÐµÑÐ¿ÐµÑÐµÐ½Ð° Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¿ÐµÑÐµÐ¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð´Ð»Ñ Ð¿Ð¾Ð´ÑÑÑÐ¾Ð¹ÐºÐ¸ Ð¿Ð¾Ð´ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ¾Ð² Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ.
title: Ð¡Ð¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¡Ð¸Ð½ÑÑÐ·ÑÐ½-Ð£Ð¹Ð³ÑÑÑÐºÐ¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° ÐÐÐ Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ Ð¸ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸ÑÑÑÐºÐ¸Ðµ Ð½Ð°ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð² Ð½ÐµÐ¼
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»ÑÐºÐµÐ²Ð¸Ñ, Ð¤ÐµÐ´Ð¾Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐÐ
ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸Ð·Ð¼
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° ÐÐ¸ÑÐ°Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð° Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð², Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð¾ÑÐ¸ÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð², Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ ÑÑÐµÐ½ÑÑ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¡Ð½ÑÑÐ·ÑÐ½-Ð£Ð¹Ð³ÑÑÑÐºÐ¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° ÐÐ¸ÑÐ°Ñ Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ. ÐÐ¾Ð´ÑÐ¾Ð±Ð½Ð¾ ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸, ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ð°, ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°, ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÑÑ.
Chain Routing: A new routing framework for the Internet based on complete orders
Creators: name: Arjona-Villicaña, P. David
name: Constantinou, Costas C.
name: Stepanenko, Alexander S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: A new framework to perform routing at the Autonomous System level is proposed in this paper. This mechanism, called Chain Routing, uses complete orders as its main topological unit. Since complete orders are acyclic digraphs that possess a known topology, it is possible to define an acyclic structure to route packets between a group of Autonomous Systems. The adoption of complete orders also allows easy identification and avoidance of persistent route oscillations, eliminates the possibility of developing transient loops in paths, and provides a structure that facilitates the implementation of traffic engineering. Moreover, by combining Chain Routing with other mechanisms that implement complete orders in time, we suggest that it is possible to design a new routing protocol which could be more reliable and stable than BGP's current implementation. Although Chain Routing will require an increase of the message overhead and greater coordination between network administrators, the rewards in stability and resilience should more than compensate for this effort.
description: Submitted to Computer Networks
New representations of pi and Dirac delta using the nonextensive-statistical-mechanics q-exponential function
Creators: name: Jauregui, M.
name: Tsallis, C.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mathematical Physics (math-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We present a generalization of the representation in plane waves of Dirac delta, $δ(x)=(1/2π)\int_{-\infty}^\infty e^{-ikx}\,dk$, namely $δ(x)=(2-q)/(2π)\int_{-\infty}^\infty e_q^{-ikx}\,dk$, using the nonextensive-statistical-mechanics $q$-exponential function, $e_q^{ix}\equiv[1+(1-q)ix]^{1/(1-q)}$ with $e_1^{ix}\equiv e^{ix}$, being $x$ any real number, for real values of $q$ within the interval $[1,2[$. Concomitantly with the development of these new representations of Dirac delta, we also present two new families of representations of the transcendental number $π$. Incidentally, we remark that the $q$-plane wave form which emerges, namely $e_q^{ikx}$, is normalizable for $1
description: 13 pages, 6 figures. Accepted for publication in the Journal of Mathematical Physics. Some misprints have been eliminated
Towards classifier visualisation in 3D source space
Creators: name: Krol, Laurens R.
name: Mousavi, Mahta
name: De Sa, Virginia
name: Zander, Thorsten O.
Publisher: name: Technische Universität Berlin
Year: 2019
Subjects: subject: 153 Kognitive Prozesse, Intelligenz
subject: 004 Datenverarbeitung; Informatik
subject: scalp
subject: brain modeling
subject: electroencephalography
subject: feature extraction
subject: transforms
subject: visualization

description: In the context of brain-computer interfacing, it is important to investigate what regions of the brain a classifier focuses on. For one, this will clarify to what extent the classifier relies on brain activity, as opposed to undesirable non-cortical signals. More generally, the practice is informative as it allows conclusions to be drawn about the cortical regions-and thus, cortical functions-that contribute to the effect under investigation. In this study, we start to investigate different methods to visualise the regions of interest of classifiers based on windowed means and on common spatial patterns. Specifically, we take individually reconstructed source spaces and transform the classifier filter weights into relevance weights indicating the relative contribution of each source to the classifier. This is visualised across participants in an average brain. By decomposing the classifier weights into separate sources and localising these in the brain, this method provides a tool to evaluate classifiers and test hypotheses.
Transport properties of a 1000-nm HgTe film: the interplay of surface and bulk carriers
Creators: name: Savchenko, M. L.
name: Kozlov, D. A.
name: Mikhailov, N. N.
name: Dvoretsky, S. A.
name: Kvon, Z. D.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We report on systematic study of transport properties of a 1000-nm HgTe film. Unlike to thinner and strained HgTe films, which are known as high-quality three-dimensional (3D) topological insulators, the film under study is much thicker than the limit of pseudomorphic growth of HgTe on a CdTe substrate. Therefore, it is expected to be fully relaxed and has the band structure of bulk HgTe, i.e., a zero gap semiconductor. Nevertheless, since the bands inversion the two-dimensional (2D) topological surface states are still expected to exist. To check this claim we studied classical and quantum transport response of the system. We demonstrate that by tuning the top-gate voltage one can change the electron-dominating transport to the hole one. The highest electron mobility is found to be more than $300 \times 10^3$ cm$^2$/Vs. The system exhibits Shubnikov-de Haas (SdH) oscillations with a complicated pattern and shows up to 5 independent frequencies in corresponding Fourier spectra. They are attributed to the topological surface states, Volkov-Pankratov states and spin-degenerate bulk states in the accumulation layer near the gate. The observed peculiarities of the quantum transport are the strong SdH oscillations of the Hall resistance, and the suppressed oscillatory response of the topological surface states.
Superconductivity above 50K in LnFeAsO1-y (Ln= Nd, Sm, Gd, Tb and Dy) Synthesized by High-pressure Technique
Creators: name: Miyazawa, Kiichi
name: Kihou, Kunihiro
name: Shirage, Parasharam M.
name: Lee, Chul-Ho
name: Kito, Hijiri
name: Eisaki, Hiroshi
name: Iyo, Akira
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We have succeeded in synthesizing single-phase polycrystalline samples of oxygen-deficient oxypnictide superconductors, LnFeAsO1-y (Ln: lanthanide elements) with Ln=La, Ce, Pr, Nd, Sm, Gd, Tb and Dy using high-pressure synthesis technique. It is found out that the synthesis pressure is the most important parameter for synthesizing single-phase samples, in particular for the heavier Ln?s, such as Tb and Dy. The lattice parameters systematically decrease with the atomic number of Ln, reflecting the shrinkage of Ln ionic radius. For the lighter Ln?s (La, Ce, Pr, Nd), Tc increases monotonously with decreasing the lattice parameters from 26K for Ln=La to 54K for Ln=Nd, then stays at the constant value around 53K for the heavier counterpart (Nd, Sm, Gd, Tb and Dy). The results suggest the intimate relationship between the crystal structural parameters and the superconductivity on the one hand, as well as the possible existence of the inherent maximum Tc on the other, which is located around 50 K in the LnFeAsO based materials.
description: 14 pages, 10 figures,Accepted for publication in Journal of the Physical Society of Japan Vol.78No.3
Representing multipliers of the Fourier algebra on non-commutative $L^p$ spaces
Creators: name: Daws, Matthew
Publisher: name: arXiv
Year: 2009
Subjects: subject: Functional Analysis (math.FA)
subject: Operator Algebras (math.OA)
subject: FOS: Mathematics
subject: 3A22, 43A30, 46L51

description: We show that the multiplier algebra of the Fourier algebra on a locally compact group $G$ can be isometrically represented on a direct sum on non-commutative $L^p$ spaces associated to the right von Neumann algebra of $G$. If these spaces are given their canonical Operator space structure, then we get a completely isometric representation of the completely bounded multiplier algebra. We make a careful study of the non-commutative $L^p$ spaces we construct, and show that they are completely isometric to those considered recently by Forrest, Lee and Samei; we improve a result about module homomorphisms. We suggest a definition of a Figa-Talamanca--Herz algebra built out of these non-commutative $L^p$ spaces, say $A_p(\hat G)$. It is shown that $A_2(\hat G)$ is isometric to $L^1(G)$, generalising the abelian situation.
description: 23 pages; added references, fixed typos