cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A multitrace deformation of ABJM theory
Creators: name: Craps, Ben
name: Hertog, Thomas
name: Turok, Neil
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Motivated by the study of big crunch singularities in asymptotically $AdS_4$ spacetimes, we consider a marginal triple trace deformation of ABJM theory. The deformation corresponds to adding a potential which is unbounded below. In a 't Hooft large N limit, the beta function for the triple trace deformation vanishes, which is consistent with the near-boundary behavior of the bulk fields. At the next order in the 1/N expansion, the triple trace couplings exhibit non-trivial running, which we analyze explicitly in the limit of zero 't Hooft coupling, in which the model reduces to an $O(N)\times O(N)$ vector model with large N. In this limit, we establish the existence of a perturbative UV fixed point, and we comment on possible non-perturbative effects. We also show that the bulk analysis leading to big crunch singularities extends to the $\Zbar_k$ orbifold models dual to ABJM theory.
description: 14 pages, 4 figures; v3. Clarification of precise relation to $O(N)\times O(N)$ model and other minor comments added
title: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ðº Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð²Ð½ÐµÐ°ÑÐ´Ð¸ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ "ÐÐ¾ÑÑÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð±Ð¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸"
title: Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸: 19.04.01 "ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ" ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ (ÑÑÐµÐ¿ÐµÐ½Ñ) Ð²ÑÐ¿ÑÑÐºÐ½Ð¸ÐºÐ° - Ð¼Ð°Ð³Ð¸ÑÑÑ ; Ð½Ð°Ð¸Ð¼ÐµÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐÐÐ 19.04.01_01 "ÐÐ¸Ð¾Ð½Ð°Ð½Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ" ; ÑÐ¾ÑÐ¼Ð° Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ - Ð¾ÑÐ½Ð°Ñ, Ð·Ð°Ð¾ÑÐ½Ð°Ñ
titleType: Subtitle
Creators: name: ÐÑÐ·Ð½ÐµÑÐ¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ

description: ÐÐ¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ â ÑÑÐ¾ Ð½Ð°ÑÐºÐ°, Ð¸Ð·ÑÑÐ°ÑÑÐ°Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ Ð¶Ð¸Ð²ÑÐµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¼Ñ Ð¸Ð»Ð¸ Ð¿ÑÐ¾Ð´ÑÐºÑÑ Ð¸Ñ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ñ. ÐÐ±ÑÐµÐºÑ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ (Ð±Ð¸Ð¾Ð¾Ð±ÑÐµÐºÑ) â ÑÐµÐ½ÑÑÐ°Ð»ÑÐ½ÑÐ¹ Ð¸ Ð¾Ð±ÑÐ·Ð°ÑÐµÐ»ÑÐ½ÑÐ¹ ÑÐ»ÐµÐ¼ÐµÐ½Ñ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°. Ð­ÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð±Ð¸Ð¾Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð² Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð´Ð¾Ð»Ð¶Ð½Ð¾ Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÑÑÑÑ Ð½Ð° Ð·Ð½Ð°Ð½Ð¸Ð¸ ÐµÐ³Ð¾ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð²: Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð°, Ð¼ÐµÑÐ°Ð±Ð¾Ð»Ð¸Ð·Ð¼Ð°, ÑÐµÐ°ÐºÑÐ¸Ð¹ Ð½Ð° ÑÑÑÐµÑÑÐ¾Ð²ÑÐµ ÑÑÐ»Ð¾Ð²Ð¸Ñ ÑÑÐµÐ´Ñ. ÐÐ¾ÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¾ÑÐ²Ð»ÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¹ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÑÐ¾Ð²Ð°ÑÑ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÑ Ð±Ð¸Ð¾Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð¸ ÐºÐ¾ÑÑÐµÐºÑÐ¸ÑÐ¾Ð²Ð°ÑÑ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°. Ð¡Ð¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Ð¾ÑÐ²Ð°ÑÑÐ²Ð°ÐµÑ ÐºÑÑÐ³ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð², ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÑÑÐ°Ð½Ð°Ð²Ð»Ð¸Ð²Ð°ÑÑ Ð½Ð°ÑÑÐ½ÑÐµ ÑÐ²ÑÐ·Ð¸ Ð¼ÐµÐ¶Ð´Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°Ð¼Ð¸: Ð¿Ð¸ÑÐµÐ²Ð°Ñ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ, Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² ÑÐ°ÑÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ, ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¸ÐºÑÐ¾Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ, Ð±Ð¸Ð¾ÑÐ¸Ð¼Ð¸Ñ.
SINAIS E SINTOMAS NA DETECÇÃO PRECOCE DA SEPSE NEONATAL: REVISÃO DE ESCOPO
Creators: name: Gonçalves Borges, Amanda
name: da Silva Moreira, Denis
name: de Lima, Tatiana Albina
Publisher: name: figshare
Year: 2023
Subjects: Neonatology

description: Objective: To map the scientific evidence on the main signs and symptoms in neonates with sepsis and which early detection strategies are used in the context of the Intensive Care Unit (ICU). Method: This is a scoping review, which will be conducted in accordance with the JBI methodology. The research will include five databases, covering studies published in any language and with a time limit between 2016 and the moment of the research. This review will consider all primary and secondary studies, gray literature and clinical guidelines that address the topic. Titles and abstracts will be selected by two independent reviewers for evaluation according to the inclusion criteria, followed by a full-text review and data extraction. Any disagreements will be discussed with a third reviewer. Data will be extracted using an extraction tool, developed by the reviewers and presented in a tabular format, accompanied by a narrative summary describing how the results relate to the purpose and question of the review. Results: We hope to identify the main signs and symptoms present and early detection strategies in neonatal sepsis. Conclusion: It is expected that the present study can contribute to the identification of relevant scientific evidence, which will make it possible to update the criteria for early recognition of signs and symptoms of newborns with sepsis, supporting the nursing team's performance for centralized, humanized and effective assistance. to this population.
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð²ÐµÐ¹Ð²Ð»ÐµÑ-Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ñ ÑÐ¶Ð°ÑÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÐºÐ¾ÑÐ¸Ð½Ð°, ÐÐ°Ð»ÐµÑ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: Ð²ÐµÐ¹Ð²Ð»ÐµÑ
Ð´Ð¸ÑÐºÑÐµÑÐ½Ð¾Ðµ Ð²ÐµÐ¹Ð²Ð»ÐµÑ-Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¸ÑÑÐ¾Ð²Ð¾Ðµ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ðµ
ÑÐ¶Ð°ÑÐ¸Ðµ Ñ Ð¿Ð¾ÑÐµÑÑÐ¼Ð¸
Ð²ÐµÐ¹Ð²Ð»ÐµÑ Ñ Ð°Ð°ÑÐ°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¾Ð±Ð·Ð¾Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¶Ð°ÑÐ¸Ñ ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ñ Ð¿Ð¾ÑÐµÑÑÐ¼Ð¸ Ð¸ Ð±ÐµÐ· Ð¿Ð¾ÑÐµÑÑ. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ Ð²ÐµÐ¹Ð²Ð»ÐµÑ-Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÐ½Ð¸Ð¼Ð¾ÑÑÑ Ð²ÐµÐ¹Ð²Ð»ÐµÑ-Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº Ð·Ð°Ð´Ð°ÑÐµ ÑÐ¶Ð°ÑÐ¸Ñ ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð¼ÐµÑÐ¾Ð´ ÑÐ¶Ð°ÑÐ¸Ñ ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ñ Ð¿Ð¾ÑÐµÑÑÐ¼Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð²ÐµÐ¹Ð²Ð»ÐµÑ-Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿Ð»Ð°Ð½ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼ÐµÑÐ¾Ð´Ð° Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐ¼Ð¸ ÑÐ¸Ð¿Ð°Ð¼Ð¸ Ð²ÐµÐ¹Ð²Ð»ÐµÑ-ÑÑÐ½ÐºÑÐ¸Ð¹. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð².
Jejunal diverticulosis
Creators: name: Toirkens, Johannes
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Abdomen
subject: CT
subject: Diagnostic procedure
subject: Diverticula

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 67 years
description: Clinical History: A 67-year-old man had progressive abdominal complaints, which were non-specific and eventually caused substantial weight loss. Thirty minutes after eating he suffered from severe pain and sometimes cramp attacks in his upper abdomen. His previous medical ... Final Diagnosis: Jejunal diverticulosis
Orion parte da Torino
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2015

Un pezzo d'Italia per la navetta Orion della NASA. E' l'oggetto rappresentato dall'immagine: l’unità STA (Structural Test Article) riproduce esattamente quella che sarà la struttura di volo del Modulo di Servizio di Orion nella missione del  2018
GMRT dice addio alla radiogalassia morente
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

GMRT è il più grande radiotelescopio al mondo che lavora sulle basse frequenze, anche se fra qualche anno il primato verrà preso dallo Square Kilometre Array. J021659-044920 presenta emissioni radio molto potenti e che da un capo all'altro misurano ben 4 milioni di anni luce: si tratta di una radiogalassia gigante molto rara
On the mystery of the absence of a spin-orbit gap in scanning tunneling microscopy spectra of germanene
Creators: name: Castenmiller, Carolien
name: Zandvliet, Harold J. W.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Germanene, the germanium analogue of graphene, shares many properties with its carbon counterpart. Both materials are two-dimensional materials that host Dirac fermions. There are, however, also a few important differences between these two materials: (1) graphene has a planar honeycomb lattice, whereas germanene's honeycomb lattice is buckled and (2) the spin-orbit gap in germanene is predicted to be about three orders of magnitude larger than the spin-orbit gap in graphene (24 meV for germanene versus 20 $μ$eV for graphene). Surprisingly, scanning tunneling spectra recorded on germanene layers synthesized on different substrates do not show any sign of the presence of a spin-orbit gap in germanene. To date the exact origin of the absence of this spin-orbit gap in the scanning tunneling spectra of germanene has remained a mystery. In this work we show that the absence of the spin-orbit can be explained by germanene's exceptionally low work function of only 3.8 eV. The difference in work function between germanene and the scanning tunneling microscopy tip (the work functions of most commonly used STM tips are in the range of 4.5 to 5.5 eV) gives rise to an electric field in the tunnel junction. This electric field results in a strong suppression of the size of the spin-orbit gap.
description: 8 pages, 2 figures
Il Simposio sul futuro dello spazio
Creators: Livia Giacomini
Publisher: name: Media Inaf
Year: 2015

Nella città brasiliana di Foz Do Iguacu si svolge in questi giorni il secondo Simposio del COSPAR, il Comitato per la Ricerca sullo Spazio, fondato nel lontano 1958. L'argomento, l'acqua e la vita nell’Universo. Il commento di Pietro Ubertini, direttore INAF-IAPS.
title: ÐÐ°Ð»Ð¾ÑÑÐ°Ð¶Ð½ÑÐ¹ Ð¶Ð¸Ð»Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ, ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ°Ñ Ð¾Ð±Ð»Ð°ÑÑÑ
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: ÐÑÐ»Ð°Ð²Ð¾Ð², Ð¡Ð°Ð»Ð¼Ð°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Ð¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
Ð¶Ð¸Ð»Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ

description: Ð Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÑ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÑ ÑÐµÑÐµÐ½Ð¸ÑÑ Ð±ÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿Ð¾ÑÑÐ°Ð¶Ð½ÑÐµ Ð¿Ð»Ð°Ð½Ñ Ð·Ð´Ð°Ð½Ð¸Ñ: Ð¿Ð»Ð°Ð½ 1-Ð³Ð¾, 2-Ð³Ð¾, 3-Ð³Ð¾, ÑÐ°Ð·ÑÐµÐ·Ñ Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°ÑÐ°Ð´Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½ÑÑ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÐ»ÐºÐ¾Ð³Ð¾ Ð·Ð°Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð»Ð¸ÑÑ Ð¿ÐµÑÐµÐºÑÑÑÐ¸Ñ, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐµÐ¿Ð»Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐ¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð¸ ÑÐ°ÑÑÐµÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾ÑÐ¾Ð¿Ð»ÐµÐ½Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐ¹ ÑÑÑÐ¾Ð¹Ð³ÐµÐ½Ð¿Ð»Ð°Ð½ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ Ð¿Ð»Ð°Ð½ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð½Ð° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÐµ Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð·Ð´Ð°Ð½Ð¸Ð¹ Ð¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹, Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½ÑÑ Ð¸ Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹. Ð¡Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð°Ñ ÑÐ¼ÐµÑÐ° Ð½Ð° Ð¾Ð±ÑÐµÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð¸ Ð¾Ð±ÑÐµÐºÑÐ½Ð°Ñ ÑÐ¼ÐµÑÐ°. ÐÐ¿Ð¸ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾ÑÑÐ°Ð½Ðµ ÑÑÑÐ´Ð°, ÑÐµÑÐ½Ð¸ÐºÐ¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ðµ ÑÐ°Ð±Ð¾Ñ, Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¿Ð¾Ð¶Ð°ÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÐµ.
Non li vediamo, ma ci sono
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Una giovane stella distante 450 anni luce da noi è ancora avvolta da un disco di gas e polveri che sembra mostrare indizi di formazione planetaria. Lo conferma un recente studio teorico di un team guidato da ricercatori dell'Università di Milano. Ulteriori indagini con il telescopio LBT non hanno però evidenziato la presenza di protopianeti di grande massa attorno ad HL Tauri. Leonardo Testi (ESO-INAF): «E' molto probabile che i pianeti che cerchiamo siano piccoli, e dunque non ancora rilevabili con la strumentazione attuale»
Glioblastoma multiforme with leptomeningeal dissemination
Creators: name: Silva, Guilherme
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Neuroradiology brain
subject: MR
subject: Imaging sequences
subject: Neoplasia

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 48 years
description: Clinical History: Inaugural generalized seizure in a patient with previous contact (months) with a tuberculosis-infected person. At the time, blood work analyses revealed a MantouxÃ¢ÂÂs test turning positive and interferon-gamma release assay positive, but no clinical evide... Final Diagnosis: Glioblastoma multiforme
Hamiltonian formulation of f(Riemann) theories of gravity
Creators: name: Deruelle, Nathalie
name: Sasaki, Misao
name: Sendouda, Yuuiti
name: Yamauchi, Daisuke
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present a canonical formulation of gravity theories whose Lagrangian is an arbitrary function of the Riemann tensor. Our approach allows a unified treatment of various subcases and an easy identification of the degrees of freedom of the theory.
description: 12 pages, REVTeX 4
Viaggi nel tempo, indietro non si torna
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Uno studio italiano guidato dall'Istituto dei sistemi complessi del CNR ha trovato la prova sperimentale che la freccia del tempo non può essere invertita, neppure in sistemi quantistici. I risultati sono pubblicati su Scientific Reports
title: ÐÐ´Ð°Ð¿ÑÐ¸Ð²Ð½Ð¾-Ð¸Ð³ÑÐ¾Ð²Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð¾ÐµÐ½Ð½ÑÑ ÑÐµÑÐµÐ¹ Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð±Ð¾Ð½ÐµÐ½ÑÑÐºÐ¾Ð³Ð¾ Ð´Ð¾ÑÑÑÐ¿Ð°
Creators: name: ÐÐ´Ð¾ÐµÐ²ÑÐºÐ¸Ð¹, Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐ°Ð»ÑÐºÐ°, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2017
Subjects: ÐÐ¾ÐµÐ½Ð½Ð°Ñ ÑÐ²ÑÐ·Ñ
ÐÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð°Ñ ÑÐ²ÑÐ·Ñ
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description: Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÐºÑÑÐ²Ð°ÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð°Ð´Ð°Ð¿ÑÐ¸Ð²Ð½Ð¾-Ð¸Ð³ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾ÐµÐ½Ð½ÑÑ ÑÐµÑÐµÐ¹ Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð±Ð¾Ð½ÐµÐ½ÑÑÐºÐ¾Ð³Ð¾ Ð´Ð¾ÑÑÑÐ¿Ð°, ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÑÑÑÐ¸Ñ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ (Ð¸Ð»Ð¸) ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ½Ð¾ÑÑÐ¸ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð²Ð½ÐµÑÐ½ÐµÐ¹ ÑÑÐµÐ´Ñ. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÐºÐ°Ð½Ð¾Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ ÑÐ¸Ð½ÑÐµÐ·Ð° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸ ÑÐµÑÐµÐ¹ Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð±Ð¾Ð½ÐµÐ½ÑÑÐºÐ¾Ð³Ð¾ Ð´Ð¾ÑÑÑÐ¿Ð° ÐºÐ°Ðº Ð·Ð°Ð´Ð°Ñ Ð´Ð²ÑÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ¹ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ; Ð¼ÐµÑÐ¾Ð´Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ ÑÐ¸Ð½ÑÐµÐ·Ð° Â«ÑÐµÑÐµÐ· Ð°Ð½Ð°Ð»Ð¸Ð·Â» Ð¿ÐµÑÐµÐ±Ð¸ÑÐ°ÐµÐ¼ÑÑ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ; ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ ÑÐ¸Ð½ÑÐµÐ·Ð° Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð°Ð¼Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐµÑÐµÐ¹ Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð±Ð¾Ð½ÐµÐ½ÑÑÐºÐ¾Ð³Ð¾ Ð´Ð¾ÑÑÑÐ¿Ð°, Ð³Ð°ÑÐ°Ð½ÑÐ¸ÑÑÑÑÐ¸Ñ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ ÑÐ¸Ð½ÑÐµÐ·Ð° Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð°Ð¼Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ, ÑÐ·Ð»Ð¾Ð²ÑÑ Ð¸ ÑÐ¾Ð¿Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð¾Ð´ÑÐ»ÐµÐ¹ ÑÐµÑÐµÐ¹ Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð±Ð¾Ð½ÐµÐ½ÑÑÐºÐ¾Ð³Ð¾ Ð´Ð¾ÑÑÑÐ¿Ð°. ÐÐ»Ñ Ð½Ð°ÑÑÐ½ÑÑ Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð², ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÐ¸ÑÑÑ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ, ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÑÑÑÐ¸Ñ Ð² ÑÐ»Ð¾Ð¶Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð²Ð½ÐµÑÐ½ÐµÐ¹ ÑÑÐµÐ´Ñ.
CaSSIS, il telescopio svizzero dal cuore italiano
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

CaSSIS, il telescopio svizzero con il contributo italiano parte alla volta di Marte. Disegnato e realizzato all’Università di Berna, in Svizzera, partirà lunedì 9 Novembre alla volta di Cannes, in Francia, dove sarà integrato nella missione ESA ExoMars Trace Gas Orbiter (TGO), nella sede di Thales-Alenia Space
CodeFill: Multi-token Code Completion by Jointly Learning from Structure and Naming Sequences
Creators: name: Izadi, Maliheh
name: Gismondi, Roberta
name: Gousios, Georgios
Publisher: name: arXiv
Year: 2022
Subjects: subject: Software Engineering (cs.SE)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Code completion is an essential feature of IDEs, yet current autocompleters are restricted to either grammar-based or NLP-based single token completions. Both approaches have significant drawbacks: grammar-based autocompletion is restricted in dynamically-typed language environments, whereas NLP-based autocompleters struggle to understand the semantics of the programming language and the developer's code context. In this work, we present CodeFill, a language model for autocompletion that combines learned structure and naming information. Using a parallel Transformer architecture and multi-task learning, CodeFill consumes sequences of source code token names and their equivalent AST token types. Uniquely, CodeFill is trained both for single-token and multi-token (statement) prediction, which enables it to learn long-range dependencies among grammatical and naming elements. We train CodeFill on two datasets, consisting of 29M and 425M lines of code, respectively. To make the evaluation more realistic, we develop a method to automatically infer points in the source code at which completion matters. We compare CodeFill against four baselines and two state-of-the-art models, GPT-C and TravTrans+.CodeFill surpasses all baselines in single token prediction (MRR: 70.9% vs. 66.2% and 67.8%) and outperforms the state of the art for multi-token prediction (ROUGE-L: 63.7% vs. 52.4% and 59.2%, for n=4 tokens). We publicly release our source code and datasets.
description: To appear in the proceedings of the 44th International Conference on Software Engineering (ICSE 2022)
Malt lymphoma of the lacrimal gland in a patient with Sjogren syndrome.
Creators: name: Zikou, Anastasia
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Neuroradiology brain
subject: MR
subject: Diagnostic procedure
subject: Lymphoma

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 73 years
description: Clinical History: A 73-year old male with known SjogrenÃ¢ÂÂs syndrome (S.S) presented as an outpatient at the rheumatology department of our hospital with left upper eyelid edema and ptosis. Clinical examination revealed a unilateral enlargement of the left  lacrimal gland. Final Diagnosis: Malt lymphoma of the lacrimal gland.
KIC 8462852: mondo alieno o anomalia?
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Un sistema stellare che presenta un oscuramento del disco solare superiore al 20 percento e per giunta aperiodico. Al momento nessun segnale radio “intenzionale” è stato rilevato dall’Allen Telescope Array del SETI Institute, ma il pensiero di trovare una civiltà aliena tecnologicamente evoluta è sempre intrigante
SPH Simulations of Abrasive Processes at a Microscopic Scale
Creators: name: Nutto, Christian
Publisher: name: SMN - The ScienceMedia Network
Year: 2015
Subjects: subject: Engineering
subject: Mechanical engineering
subject: FOS: Mechanical engineering
subject: 1
subject: 6

description: We present the development of smoothed particle hydrodynamics (SPH) simulations for the investigation of the industrial application of abrasive flow machining (AFM). This process cannot be observed in-situ in experiments and therefore demands for numerical simulations at a grain-size process scale.
There are only a few numerical models available for the AFM process, which are strongly simplified. In order to optimize the machining, an explicit approach of including individual grains in the abrasive suspension is essential. These grains are simulated by individual clusters of SPH particles, which are integrated in time by a rigid body solver.
For the correct force transmission between the suspended abrasive particle and the workpiece, a realistic representation of the stress in the fluid model of the suspension is necessary. Therefore, the rheology of the fluids, containing the abrasive grains, has been experimentally characterized. Since the tested
suspensions show a viscoelastic behavior, we have employed a viscoelastic fluid model and have used experimentally gathered data for the calibration of the applied numerical model. The abrasive process on a workpiece and the removal of material from its surface is modeled by the Johnson-Cook ductile flow stress model in combination with a strain-based failure criterion.
We show that the particle method can reproduce key aspects for the simulation of the process of abrasive flow machining. By the application of the Johnson-Cook model, we are able to determine wear contacts between solid materials on a microscopic scale.
Increase in teen smoking in Ireland in 2019 for the first time in 25 years
Creators: name: Sunday, Salome
name: Hanafin, Joan
name: Clancy, Luke
Publisher: name: Zenodo
Year: 2021
Subjects: Teens
smoking
e-cigarette use

description: TobaccoFree Research Institute Ireland
description: Funded by Royal City of Dublin Hospital Trust (RCDHT) Grant No. 184
title: ÐÐ±ÑÑÐµÐ½Ð¸Ðµ Ð±Ð¾ÑÐ° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸Ð³ÑÐ¾ÐºÐ¾Ð² Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐµÑ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ÐµÑÑÐµÑÐµÐ½Ñ, 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: 2018
Subjects: Ð¸Ð³ÑÐ¾Ð²Ð¾Ð¹ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑ
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description: ÐÐ°Ð½Ð½Ð°Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¹ Ð¸Ð³ÑÑ Ð² Ð¶Ð°Ð½ÑÐµ Â«Shoot 'em upÂ» (Ð°Ð½Ð³Ð». Ð¿ÐµÑÐµÑÑÑÐµÐ»ÑÐ¹ Ð¸Ñ Ð²ÑÐµÑ) Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ¹ Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸Ð³ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÐ°. ÐÐ±ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð´Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸Ð³ÑÐ¾ÐºÐ°.
ÐÐ»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð±ÑÐ»Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ ÑÐ·ÑÐº Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Python, Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Pygame, Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð½Ð°Ñ Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÑ Ð¸Ð³Ñ, Ð¸ TensorFlow Ð´Ð»Ñ Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ.
Size-consistent variational approaches to non-local pseudopotentials: standard and lattice regularized diffusion Monte Carlo methods revisited
Creators: name: Casula, Michele
name: Moroni, Saverio
name: Sorella, Sandro
name: Filippi, Claudia
Publisher: name: arXiv
Year: 2010
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We propose improved versions of the standard diffusion Monte Carlo (DMC) and the lattice regularized diffusion Monte Carlo (LRDMC) algorithms. For the DMC method, we refine a scheme recently devised to treat non-local pseudopotential in a variational way. We show that such scheme --when applied to large enough systems-- maintains its effectiveness only at correspondingly small enough time-steps, and we present two simple upgrades of the method which guarantee the variational property in a size-consistent manner. For the LRDMC method, which is size-consistent and variational by construction, we enhance the computational efficiency by introducing (i) an improved definition of the effective lattice Hamiltonian which remains size-consistent and entails a small lattice-space error with a known leading term, and (ii) a new randomization method for the positions of the lattice knots which requires a single lattice-space.
description: 10 pages, 4 figures, submitted to the Journal of Chemical Physics
title: FedMentalCare: Towards Privacy-Preserving Fine-Tuned LLMs to Analyze Mental Health Status Using Federated Learning Framework
Creators: name: Sarwar, S. M.
Publisher: name: Maryland Shared Open Access Repository
Year: 2025

description: With the increasing prevalence of mental health conditions worldwide, AI-powered chatbots and conversational agents have emerged as accessible tools to support mental health. However, deploying Large Language Models (LLMs) in mental healthcare applications raises significant privacy concerns, especially regarding regulations like HIPAA and GDPR. In this work, we propose FedMentalCare, a privacy-preserving framework that leverages Federated Learning (FL) combined with Low-Rank Adaptation (LoRA) to fine-tune LLMs for mental health analysis. We investigate the performance impact of varying client data volumes and model architectures (e.g., MobileBERT and MiniLM) in FL environments. Our framework demonstrates a scalable, privacy-aware approach for deploying LLMs in real-world mental healthcare scenarios, addressing data security and computational efficiency challenges.
A polynomial computer
Creators: name: Ruegg, Frank Arthur
Publisher: name: University of British Columbia
Year: 2012

description: A computer for solving polynomial equations, performing Fourier synthesis, and displaying system functions is a valuable asset to an electrical laboratory. A number of successful computers have been built for such purposes but each has its limitations. The design of a versatile and precise instrument superior to existing computers is the purpose of this study. Using a voltage analogue of the function, this computer is designed for the solution of 20th - degree polynomials with real coefficients, 10th - degree polynomials with complex coefficients, and Fourier synthesis of either even or odd functions to the 20th harmonic or mixed functions to the 10th harmonic. Provision is made for the addition of circuits which will plot the magnitudes and angles of the polynomial or will form combinations of two 10th-degree polynomials. The computer, using servo phase-shifters harmonically geared in pairs and excited with a two-phase, 400-cps carrier, generates a polynomial term by term in exponential form. The coefficients and radial components of the terms are obtained by the use of precision potentiometers. The terms are summed by operational amplifiers which, mounted as a separate unit, can be removed from the computer for other analogue computations. The radial and angular components of the independent variable, p, of the polynomial may be constant or linear functions of time. The display consists of a long-persistence cathode-ray-tube on which the zeros of a polynomial are automatically plotted. For greater accuracy, zero positions may be determined manually by using a null indicator. Fourier synthesis can be performed with minor changes in the output circuit. The periodic function may be displayed continuously or point by point. The major part of the computer, the phase-shifter unit, has been built and most of the other components partially assembled. Completion and testing of the computer will be part of a further project.
Supernovae gemelle
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Le supernovae di tipo Ia hanno luminosità simili, una proprietà che viene utilizzata dagli astronomi per studiare l’espansione dell’Universo. Oggi, uno studio basato su un campione di quasi 50 supernovae, guidato dal team SNfactory, presenta un nuovo metodo che permette di identificare coppie di oggetti dagli spettri confrontabili e da cui è possibile misurare le distanze cosmologiche con una accuratezza migliore. I risultati sono riportati su ApJ
Some ideas about quantitative convergence of collision models to their mean field limit
Creators: name: Peyre, Remi
Publisher: name: arXiv
Year: 2009
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 82C31; 60K35

description: We consider a stochastic $N$-particle model for the spatially homogeneous Boltzmann evolution and prove its convergence to the associated Boltzmann equation when $N\to \infty$. For any time $T>0$ we bound the distance between the empirical measure of the particle system and the measure given by the Boltzmann evolution in some homogeneous negative Sobolev space. The control we get is Gaussian, i.e. we prove that the distance is bigger than $x N^{-1/2}$ with a probability of type $O(e^{-x^2})$. The two main ingredients are first a control of fluctuations due to the discrete nature of collisions, secondly a Lipschitz continuity for the Boltzmann collision kernel. The latter condition, in our present setting, is only satisfied for Maxwellian models. Numerical computations tend to show that our results are useful in practice.
description: 27 pages, references added and style improved
Hubble si dà all’archeologia galattica
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Le incredibili capacità osservative di Hubble ci regalano uno sguardo così profondo e dettagliato del bulge della Via Lattea da permetterci di individuare un’intera popolazione di nane bianche al suo interno. Un team internazionale di astronomi ha presentato i propri risultati in un articolo apparso su The Astrophysical Journal, ricostruendo la storia della nostra galassia nelle sue prime fasi di vita
Sources of experimental errors in the observation of nanoscale magnetism
Creators: name: Garcia, M. A.
name: Pinel, E. Fernandez
name: de la Venta, J
name: Quesada, A.
name: Bouzas, V.
name: Fernandez, J. F.
name: Romero, J. J.
name: Gonzalez, M. S. Martin
name: Costa-Kramer, J. L.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: It has been recently reported that some non-magnetic materials in bulk state, exhibit magnetic behavior at the nanscale due to surface and size effects. The experimental observation of these effects is based on the measurement of very small magnetic signals. Thus, some spurious effects that are not critical for bulk materials with large magnetic signals may become important when measuring small signals (typically below 0.0001 emu). Here, we summarize some sources of these small magnetic signals that should be considered when studying this new nanomagnetism
description: 16 pages, 10 figures
Spiking Cochlea with System-level Local Automatic Gain Control
Creators: name: Kiselev, Ilya
name: Gao, Chang
name: Liu, Shih-Chii
Publisher: name: arXiv
Year: 2022
Subjects: subject: Signal Processing (eess.SP)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: Sound (cs.SD)
subject: Systems and Control (eess.SY)
subject: Audio and Speech Processing (eess.AS)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: Including local automatic gain control (AGC) circuitry into a silicon cochlea design has been challenging because of transistor mismatch and model complexity. To address this, we present an alternative system-level algorithm that implements channel-specific AGC in a silicon spiking cochlea by measuring the output spike activity of individual channels. The bandpass filter gain of a channel is adapted dynamically to the input amplitude so that the average output spike rate stays within a defined range. Because this AGC mechanism only needs counting and adding operations, it can be implemented at low hardware cost in a future design. We evaluate the impact of the local AGC algorithm on a classification task where the input signal varies over 32 dB input range. Two classifier types receiving cochlea spike features were tested on a speech versus noise classification task. The logistic regression classifier achieves an average of 6% improvement and 40.8% relative improvement in accuracy when the AGC is enabled. The deep neural network classifier shows a similar improvement for the AGC case and achieves a higher mean accuracy of 96% compared to the best accuracy of 91% from the logistic regression classifier.
description: Accepted for publication at the IEEE Transactions on Circuits and Systems I - Regular Papers, 2022
Sorvolando l’atmosfera marziana
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Nuovi indizi emergono dagli ultimi dati raccolti dalla missione della NASA MAVEN che è stata concepita per studiare gli strati superiori dell’atmosfera, della ionosfera e della magnetosfera marziana. In quattro articoli, pubblicati sulla rivista Science, vengono presentati una serie di risultati che tra gli altri fanno luce sulle possibili correlazioni tra l'attività solare e il magnetismo residuo del pianeta rosso
title: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²ÑÐ¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð¼
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ²ÑÑÐ¸Ð³Ð½ÐµÐµÐ²Ð°, 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: ÑÐ¾ÑÐ³Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑ
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description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ½ÐºÐ° ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¾ ÑÐ»Ð¾Ð¶Ð¸Ð²ÑÐµÐµÑÑ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð½Ð° ÑÑÐ½ÐºÐµ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð° Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐµÐ³Ð¼ÐµÐ½ÑÐ¾Ð² ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð²ÑÐ±Ð¾Ñ Ð½Ð°Ð¸Ð»ÑÑÑÐµÐ³Ð¾ Ð¸ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·ÐµÐ¼ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ° ÐºÐ°Ðº ÑÑÐ»Ð¾Ð²Ð½Ð¾ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð³Ð¾. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·ÐµÐ¼ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ°, Ð¸ÑÑÐ¾Ð´Ñ Ð¸Ð· ÐµÐ³Ð¾ Ð¼ÐµÑÑÐ¾Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ, ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð Ð¤, ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÑÑÐµÑÑÐ²Ð¸Ð¼Ð¾ÑÑÐ¸, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÑÐµÑÑÐ²Ð¸Ð¼Ð¾ÑÑÐ¸. ÐÐ°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÐ¹ Ð²Ð°ÑÐ¸Ð°Ð½Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·ÐµÐ¼ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ° ÐºÐ°Ðº ÑÑÐ»Ð¾Ð²Ð½Ð¾ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð±ÑÐ» Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½ Ð¿ÑÑÐµÐ¼ ÑÐ°ÑÑÐµÑÐ° ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð·ÐµÐ¼ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ°, Ð¼Ð°ÐºÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð´Ð¾ÑÑÐ¸Ð³Ð½ÑÑÐ° Ð¿ÑÐ¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾-Ð¾ÑÐ¸ÑÐ½Ð¾Ð¹ ÑÑÐ½ÐºÑÐ¸Ð¸.
Storia dell’universo in 11 equazioni
Creators: Elisabetta Andreina Brunelli
Publisher: name: Media Inaf
Year: 2015

Un modello in grado di render conto dell’energia oscura, e di riprodurre le tappe fondamentali dell’evoluzione dell’universo, partendo dalle equazioni di Einstein, Yang-Mills e Higgs. Lo ha messo punto un ricercatore dell’Università di Trento, Massimiliano Rinaldi
A general strong law of large numbers for additive arithmetic functions
Creators: name: Berkes, Istvan
name: Weber, Michel
Publisher: name: arXiv
Year: 2009
Subjects: subject: Number Theory (math.NT)
subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 11A25, 60F15

description: Let $f(n)$ be a strongly additive complex valued arithmetic function. Under mild conditions on $f$, we prove the following weighted strong law of large numbers: if $ X,X_1,X_2,... $ is any sequence of integrable i.i.d. random variables, then $$ \lim_{N\to \infty} {\sum_{n=1}^N f(n) X_n \over\sum_{n=1}^N f(n)} \buildrel{a.s.}\over{=} \E X . $$
Pianeti nascosti? Magari è solo un’illusione
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Le regioni scure nei dischi ci sembrano vuote perché in realtà potrebbero essere realmente vuote, visto che le particelle più grandi si aggregano formando oggetti più densi (non per forza pianeti) e le particelle più piccole spariscono
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¸ÑÐº-Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°
Creators: name: ÐÐ¾ÑÐµÐ·Ð¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2008
Subjects: ÐÐ¾Ð´Ð½ÑÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑ
Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
ÑÐ¸ÑÐºÐ¸

description: Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð¾Ð²Ð¾Ð¹ Ð¿Ð°ÑÐ°Ð´Ð¸Ð³Ð¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð½Ð° Ð²Ð¾Ð´Ð½Ð¾Ð¼ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐµ. ÐÐ±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÑÑÑÑ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¹ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÑÐº-Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÑ Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°. ÐÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¸ÑÐº-Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð² Ð·Ð¾Ð½Ðµ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÐ´Ð¾ÑÐ¾Ð´Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. ÐÐ½Ð¸Ð³Ð° Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð° ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°Ð¼ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð° ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐµ, Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÐ¼, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐµÐ¼ Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸Ð¼ÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸ÐµÐ¼ Ð½Ð¾Ð²ÐµÐ¹ÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°.
title: Fiducial Confidence Intervals for Agreement Measures Among Raters Under a Generalized Linear Mixed Effects Model
Creators: name: Sahu, Soumya
name: Mathew, Thomas
name: Bhaumik, Dulal K.
Publisher: name: Maryland Shared Open Access Repository
Year: 2025
Subjects: subject: Statistics - Methodology
subject: Statistics - Applications

description: A generalization of the classical concordance correlation coefficient (CCC) is considered under a three-level design where multiple raters rate every subject over time, and each rater is rating every subject multiple times at each measuring time point. The ratings can be discrete or continuous. A methodology is developed for the interval estimation of the CCC based on a suitable linearization of the model along with an adaptation of the fiducial inference approach. The resulting confidence intervals have satisfactory coverage probabilities and shorter expected widths compared to the interval based on Fisher Z-transformation, even under moderate sample sizes. Two real applications available in the literature are discussed. The first application is based on a clinical trial to determine if various treatments are more effective than a placebo for treating knee pain associated with osteoarthritis. The CCC was used to assess agreement among the manual measurements of the joint space widths on plain radiographs by two raters, and the computer-generated measurements of digitalized radiographs. The second example is on a corticospinal tractography, and the CCC was once again applied in order to evaluate the agreement between a well-trained technologist and a neuroradiologist regarding the measurements of fiber number in both the right and left corticospinal tracts. Other relevant applications of our general approach are highlighted in many areas including artificial intelligence.
Electronic transport properties of a tilted graphene pn junction
Creators: name: Low, Tony
name: Appenzeller, Joerg
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Spatial manipulation of current flow in graphene could be achieved through the use of a tilted pn junction. We show through numerical simulation that a pseudo-Hall effect (i.e. non-equilibrium charge and current density accumulating along one of the sides of a graphene ribbon) can be observed under these conditions. The tilt angle and the pn transition length are two key parameters in tuning the strength of this effect. This phenomenon can be explained using classical trajectory via ray analysis, and is therefore relatively robust against disorder. Lastly, we propose and simulate a three terminal device that allows direct experimental access to the proposed effect.
description: 7 pages, 7 figures
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð²ÑÐºÑÐ°ÑÐ½ÑÑ ÑÑÑÐ±Ð¸Ð½ Ð´Ð»Ñ Ð¼Ð°Ð»ÑÑ ÐÐ­Ð¡
title: Research and design of cross flow water turbines for small HPP
Creators: name: ÐÐ±ÑÐµÑÐµÐ½Ð¾Ð², ÐÐ°Ð»ÐµÐ½ÑÐ¸Ð½
name: Ð¦Ð°Ð»Ð¾Ð², Ð¦Ð²ÐµÑÐ°Ð½
name: "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°. Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2020; 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: 2020
Subjects: ÐÐ¸Ð´ÑÐ¾ÑÑÑÐ±Ð¸Ð½Ñ
ÐÐ¸Ð´ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¾Ð¿ÑÑ ÐºÐ°ÑÐµÐ´ÑÑ Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð¸ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð°ÑÐ¸Ð½ Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° Ð¡Ð¾ÑÐ¸Ð¸ (ÐÐ¾Ð»Ð³Ð°ÑÐ¸Ñ) Ð² Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð´Ð²ÑÐºÑÐ°ÑÐ½ÑÑ Ð³Ð¸Ð´ÑÐ¾ÑÑÑÐ±Ð¸Ð½. ÐÐ¿Ð¸ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð´Ð»Ñ ÑÐ¸Ð½ÑÐµÐ·Ð° ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿ÑÐ¾ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð´Ð²ÑÐºÑÐ°ÑÐ½ÑÑ ÑÑÑÐ±Ð¸Ð½. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÑ Ð¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ (Ð¼Ð¾Ð´ÐµÐ»ÑÐ½ÑÑ Ð¸ Ð¿Ð¾Ð»ÐµÐ²ÑÑ) Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ ÑÑÑÐ±Ð¸Ð½ ÑÑÐ¾Ð³Ð¾ ÑÐ¸Ð¿Ð°. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼ÑÑ ÑÑÑÐ±Ð¸Ð½ Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÐºÐ¾Ð½ÐºÑÐµÑÐ½ÑÐµ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¼Ð°Ð»ÑÑ ÐÐ­Ð¡ Ð² ÐÐ¾Ð»Ð³Ð°ÑÐ¸Ð¸.
description: This paper presents the experience of the Hydroaerodynamics and hydraulic machinery department of the Technical university of Sofia (Bulgaria) in the research and design of cross flow water turbines. The methods and computer programs used for the synthesis of the elements of the flow part of the cross flow turbines are described. Results of numerical and experimental (model and field) studies of turbines of this type are presented. The peculiarities of the elements of the designed turbines are analyzed and specific examples of their used in small hydropower plants in Bulgaria are shown.
THE 0¹⁶(p,૪)F¹⁷ REACTION
Creators: name: Robertson, Lyle Purmal
Publisher: name: University of British Columbia
Year: 2012

description: The differential cross section for direct radiative capture of protons by 0¹⁶ has been measured using ice targets of known thickness and 800 kev. protons. The differential cross section for the gamma ray transition to the first excited state in F¹⁷ was found to be (10.4 ± 1.3) x 10⁻⁻³² cm² per steradian at 90° to the incident proton beam direction. At the same energy, the ratio of the differential cross section at 90° for transitions to the ground state to that for transitions to the first excited state in F¹⁷ was found to be o.14 ± 0.03. The energy of the first excited state in F¹⁷ was determined by measuring the energy of the gamma ray from this level to the ground state. This method is difficult because of the presence of positron annihilation radiation of the same energy, within experimental errors, from the decay of F¹⁷. The first excited state energy was also measured by noting the difference between the capture gamma rays to this state and to the ground state. The energy of this level was found to be 0.50 ± 0.01 Mev. in agreement with the results of Marion and Bonner (55) and with earlier results obtained in this laboratory (Warren et. al., (54), An attempt to confirm that the source of the 873 kev. radiation from proton bombardment of natural oxide targets above 1.8 Mev. bombarding energy was the 0¹⁷(p, p',૪)0¹⁷ reaction, was made using separated 0¹⁶ and 0¹⁷ targets. The results were inconclusive due to the small percentage of oxygen that stuck to the targets and to the presence of several contaminants.
SLS: ok su carta al super razzo NASA
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Nonostante intoppi e tagli al bilancio, lo Space Launch System NASA porta a casa l'approvazione a procedere dello Standing Review Board. Quello che gli Stati Uniti hanno sempre presentato come l'erede del programma Apollo e il più potente razzo mai costruito dall'uomo, punta però al raddoppio: da 77 a 143 tonnellate in capacità di sollevamento. Marte è più vicino
Understanding optimal dosage frequency and patient engagement on improving outcomes using digital therapy
Creators: name: Swathi Kiran
name: Gerst, Kyle
name: Godlove, Jason
name: Anantha, Veera
name: Dubas, Emily
Publisher: name: F1000 Research Limited
Year: 2019

description: This poster shows that users that engaged in Constant Therapy for 3x or more per week had significantly greater rates of progress compared to 1x and 2x/week users. Results support the theory that increased treatment dosage frequency results in improved outcomes.
GRB 070518: A Gamma-ray Burst with Optically Dim Luminosity
Creators: name: Xin, L. P.
name: Zheng, W. K.
name: Wang, J.
name: Deng, J. S.
name: Urata, Y.
name: Qiu, Y. L.
name: Huang, K. Y.
name: Hu, J. Y.
name: Wei, J. Y.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present our optical observations of {\em Swift} GRB 070518 afterglow obtained at the 0.8-m Tsinghua University-National Astronomical Observatory of China telescope (TNT) at Xinglong Observatory. Our follow-up observations were performed from 512 sec after the burst trigger. With the upper limit of redshift $\sim$0.7, GRB 070518 is found to be an optically dim burst. The spectra indices $β_{ox}$ of optical to X-ray are slightly larger than 0.5, which implies the burst might be a dark burst. The extinction $A_{V}$ of the host galaxy is 3.2 mag inferred from the X-ray hydrogen column density with Galactic extinction law, and 0.3 mag with SMC extinction law. Also, it is similar to three other low-redshift optically dim bursts, which belong to XRR or XRF, and mid-term duration($T_{90}<10$, except for GRB 070419A, $T_{90}$=116s). Moreover, its $R$ band afterglow flux is well fitted by a single power-law with an index of 0.87. The optical afterglow and the X-ray afterglow in the normal segment might have the same mechanism, as they are consistent with the prediction of the classical external shock model. Besides, GRB 070518 agrees with Amati relation under reasonable assumptions. The Ghirlanda relation is also tested with the burst.
description: 8 pages, 4 figures, MNRAS accepted