cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ°Ð¹Ð¾Ð½Ð½Ð¾Ð¹ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð³. Ð¢ÑÑÐ°ÐµÐ² Ð¿ÑÐ¸ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐµ ÐÐÐ£-Ð¢Ð­Ð¡ 52 ÐÐÐ¢
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ÑÐ°ÑÐ¸Ð»ÑÐ½Ð¸ÐºÐ¾Ð²Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ°ÑÐ¾Ð³Ð°Ð·Ð¾Ð²ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸
Ð¢ÐµÐ¿Ð»Ð¾Ð²ÑÐµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸
ÐÐ¾ÑÐ»Ñ-ÑÑÐ¸Ð»Ð¸Ð·Ð°ÑÐ¾ÑÑ
ÐÑÐ°Ð´Ð¸ÑÐ½Ð¸ Ð²ÐµÐ½ÑÐ¸Ð»ÑÑÐ¾ÑÐ½ÑÐµ
ÐÐ¾Ð´Ð° Ð¿Ð¸ÑÐ°ÑÐµÐ»ÑÐ½Ð°Ñ
Ð¢ÐµÐ¿Ð»Ð¾Ð²Ð°Ñ ÑÐ½ÐµÑÐ³Ð¸Ñ

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð¹Ð¾Ð½Ð½Ð¾Ð¹ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð³. Ð¢ÑÑÐ°ÐµÐ² Ð² ÐÐÐ£-Ð¢Ð­Ð¡ 52 ÐÐÑ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÑÐµÐ¼Ñ Ð¸ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°Ð±Ð¾ÑÑ ÑÐ°Ð¹Ð¾Ð½Ð½Ð¾Ð¹ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹, Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð° ÑÐµÐ¿Ð»Ð¾Ð²Ð°Ñ ÑÑÐµÐ¼Ð° ÑÐ½ÐµÑÐ³Ð¾Ð±Ð»Ð¾ÐºÐ° Ð²Ð²Ð¾Ð´Ð¸Ð¼Ð¾Ð¹ ÑÑÐ°Ð½ÑÐ¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð³Ð¾ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð°Ñ ÑÐ°Ð±Ð¾ÑÑ Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ Ð½Ð°ÑÑÐ¶Ð½Ð¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÑÑÐ°, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð´Ð»Ñ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ Ð¼ÐµÑÑÑÐ°, Ð³Ð¾Ð´Ð¾Ð²Ð°Ñ Ð²ÑÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸, Ð³Ð¾Ð´Ð¾Ð²Ð¾Ð¹ ÑÐ°ÑÑÐ¾Ð´ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð°. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°ÑÑÐµÑÐ½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÐÐÐ£-Ð¢Ð­Ð¡ 52 ÐÐÑ.
DeCoR: Defy Knowledge Forgetting by Predicting Earlier Audio Codes
Creators: name: Jiang, Xilin
name: Li, Yinghao Aaron
name: Mesgarani, Nima
Publisher: name: arXiv
Year: 2023
Subjects: subject: Audio and Speech Processing (eess.AS)
subject: Machine Learning (cs.LG)
subject: Sound (cs.SD)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: Lifelong audio feature extraction involves learning new sound classes incrementally, which is essential for adapting to new data distributions over time. However, optimizing the model only on new data can lead to catastrophic forgetting of previously learned tasks, which undermines the model's ability to perform well over the long term. This paper introduces a new approach to continual audio representation learning called DeCoR. Unlike other methods that store previous data, features, or models, DeCoR indirectly distills knowledge from an earlier model to the latest by predicting quantization indices from a delayed codebook. We demonstrate that DeCoR improves acoustic scene classification accuracy and integrates well with continual self-supervised representation learning. Our approach introduces minimal storage and computation overhead, making it a lightweight and efficient solution for continual learning.
description: INTERSPEECH 2023
title: ÐÐµÐ¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸Ð»Ð¸ÐºÐ°ÑÐ½ÑÑ ÑÑÐµÐºÐ¾Ð» Ð²ÑÑÐµ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ ÑÑÐµÐºÐ»Ð¾Ð²Ð°Ð½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð ÐµÑÐµÑ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: Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ
Ð´ÐµÐ¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ
ÑÐ¸Ð»Ð¸ÐºÐ°ÑÐ½ÑÐµ ÑÑÐµÐºÐ»Ð°
Ð½Ð¸Ð·ÐºÐ¾ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½ÑÐ¹ Ð¿Ð¸Ðº

description: ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¹ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÑÑÑÑ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ñ ÑÐµÐ»Ð°ÐºÑÐ°ÑÐ¸Ð¸ Ð·Ð°ÑÑÐ´Ð° Ð¿ÑÐ¸ Ð´ÐµÐ¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸Ð»Ð¸ÐºÐ°ÑÐ½ÑÑ ÑÑÐµÐºÐ¾Ð» Ð²ÑÑÐµ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ ÑÑÐµÐºÐ»Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ°Ð±Ð¾ÑÑ [1] Ð±ÑÐ»Ð¾ ÑÐ´ÐµÐ»Ð°Ð½Ð¾ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¾ ÑÐ¾Ð¼, ÑÑÐ¾ Ð½Ð¸Ð·ÐºÐ¾ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½ÑÐ¹ Ð¿Ð¸Ðº Ð½Ð° ÑÐ¿ÐµÐºÑÑÐµ Ð¢Ð¡Ð¢Ð (ÑÐµÑÐ¼Ð¾ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ ÑÐ¾Ðº Ð´ÐµÐ¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸) Ð¾Ð±ÑÑÐ»Ð¾Ð²Ð»ÐµÐ½ Ð´ÑÐµÐ¹ÑÐ¾Ð¼ Ð´Ð²ÑÑÐ²Ð°Ð»ÐµÐ½ÑÐ½ÑÑ ÐºÐ°ÑÐ¸Ð¾Ð½Ð¾Ð², Ð° Ð²ÑÑÐ¾ÐºÐ¾ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½ÑÐµ Ð¿Ð¸ÐºÐ¸ - Ð´ÑÐµÐ¹ÑÐ¾Ð¼ Ð¾Ð´Ð½Ð¾Ð²Ð°Ð»ÐµÐ½ÑÐ½ÑÑ ÐºÐ°ÑÐ¸Ð¾Ð½Ð¾Ð². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¼Ð½Ð¾Ð³Ð¾ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸Ð»Ð¸ÐºÐ°ÑÐ½Ð¾Ð³Ð¾ ÑÑÐµÐºÐ»Ð° Menzel Ð¿ÑÐ¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. ÐÐ¾Ð»ÑÑÐµÐ½Ñ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÐºÑÐ¸Ð²ÑÐµ - Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ ÑÐ¾ÐºÐ° Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð´ÐµÐ¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð´ÐµÐ¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÐºÑÐ¸Ð²ÑÐµ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð²ÑÐµÑ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð±ÑÐ» ÑÐ´ÐµÐ»Ð°Ð½ Ð²ÑÐ²Ð¾Ð´ Ð¾ ÑÐ¾Ð¼, ÑÑÐ¾ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÑ ÐºÐ¾ÑÐ²ÐµÐ½Ð½Ð¾ Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ´Ð¸Ð»Ð¸ Ð¸Ð·Ð½Ð°ÑÐ°Ð»ÑÐ½Ð¾Ðµ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ.
Growing correlations and aging of an elastic line in a random potential
Creators: name: Iguain, José Luis
name: Bustingorry, Sebastian
name: Kolton, Alejandro B.
name: Cugliandolo, Leticia F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We study the thermally assisted relaxation of a directed elastic line in a two dimensional quenched random potential by solving numerically the Edwards-Wilkinson equation and the Monte Carlo dynamics of a solid-on-solid lattice model. We show that the aging dynamics is governed by a growing correlation length displaying two regimes: an initial thermally dominated power-law growth which crosses over, at a static temperature-dependent correlation length $L_T \sim T^3$, to a logarithmic growth consistent with an algebraic growth of barriers. We present a scaling arguments to deal with the crossover-induced geometrical and dynamical effects. This analysis allows to explain why the results of most numerical studies so far have been described with effective power-laws and also permits to determine the observed anomalous temperature-dependence of the characteristic growth exponents. We argue that a similar mechanism should be at work in other disordered systems. We generalize the Family-Vicsek stationary scaling law to describe the roughness by incorporating the waiting-time dependence or age of the initial configuration. The analysis of the two-time linear response and correlation functions shows that a well-defined effective temperature exists in the power-law regime. Finally, we discuss the relevance of our results for the slow dynamics of vortex glasses in High-Tc superconductors.
description: 18 pages, 15 figures, submitted for publication
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ¾ÑÐ¿ÑÑÂ»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð Ð°ÑÑÐºÐ°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: 2016
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð½Ð°Ð»Ð°Ð´ÐºÐ°
Ð±Ð°Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
technological process
operating adjustment
basing

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ¾ÑÐ¿ÑÑÐ° Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¾Ð±ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÑÑÐµÐ³Ð¾ ÑÐµÐ½ÑÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÑÐ°Ð½Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¸ ÑÑÐµÐ·ÐµÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ðµ. Ð Ð¿Ð¾ÑÑÐ½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð·Ð°Ð¿Ð¸ÑÐºÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ, Ð·Ð°Ð¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð°Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ.
description: Graduate work is designed housing technology manufacturing process using a machining center. Designs of machine tools for milling operations and control and measuring device. The explanatory memorandum made ââtechnological and economic calculations, fill out the required technical documentation.
JADES: Detecting [OIII]$λ4363$ Emitters and Testing Strong Line Calibrations in the High-$z$ Universe with Ultra-deep JWST/NIRSpec Spectroscopy up to $z \sim 9.5$
Creators: name: Laseter, Isaac H.
name: Maseda, Michael V.
name: Curti, Mirko
name: Maiolino, Roberto
name: D'Eugenio, Francesco
name: Cameron, Alex J.
name: Looser, Tobias J.
name: Arribas, Santiago
name: Baker, William M.
name: Bhatawdekar, Rachana
name: Boyett, Kristan
name: Bunker, Andrew J.
name: Carniani, Stefano
name: Charlot, Stephane
name: Chevallard, Jacopo
name: Curtis-lake, Emma
name: Egami, Eiichi
name: Eisenstein, Daniel J.
name: Hainline, Kevin
name: Hausen, Ryan
name: Ji, Zhiyuan
name: Kumari, Nimisha
name: Perna, Michele
name: Rawle, Tim
name: Rix, Hans-Walter
name: Robertson, Brant
name: Del Pino, Bruno Rodríguez
name: Sandles, Lester
name: Scholtz, Jan
name: Smit, Renske
name: Tacchella, Sandro
name: Übler, Hannah
name: Williams, Christina C.
name: Willott, Chris
name: Witstok, Joris
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present 10 novel [OIII]$λ4363$ auroral line detections up to $z\sim 9.5$ measured from ultra-deep JWST/NIRSpec MSA spectroscopy from the JWST Advanced Deep Extragalactic Survey (JADES). We leverage the deepest spectroscopic observations yet taken with NIRSpec to determine electron temperatures and oxygen abundances using the direct T$_e$ method. We directly compare against a suite of locally calibrated strong-line diagnostics and recent high-$z$ calibrations. We find the calibrations fail to simultaneously match our JADES sample, thus warranting a self-consistent revision of these calibrations for the high-$z$ Universe. We find weak dependence between R2 and O3O2 with metallicity, thus suggesting these line-ratios are ineffective in the high-$z$ Universe as metallicity diagnostics and degeneracy breakers. We find R3 and R23 still correlate with metallicity, but we find tentative flattening of these diagnostics, thus suggesting future difficulties when applying these strong-line ratios as metallicity indicators in the high-$z$ Universe. We also propose and test an alternative diagnostic based on a different combination of R3 and R2 with a higher dynamic range. We find a reasonably good agreement (median offset of 0.002 dex, median absolute offset of 0.13 dex) with the JWST sample at low metallicity. Our sample demonstrates higher ionization/excitation ratios than local galaxies with rest-frame EWs(H$β$) $\approx 200 -300$ Angstroms. However, we find the median rest-frame EWs(H$β$) of our sample to be $\sim 2\text{x}$ less than the galaxies used for the local calibrations. This EW discrepancy combined with the high ionization of our galaxies does not present a clear description of [OIII]$λ4363$ production in the high-$z$ Universe, thus warranting a much deeper examination into the factors affecting production.
description: 28 pages, 13 figures
Local politicians’ support for different types of citizen participation processes
Creators: name: Wagenaar, Charlotte
name: Sipma, Take
name: Van Ham, Carolien
name: De Blok, Lisanne
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Political Science
subject: FOS: Political science
subject: Social and Behavioral Sciences

description: In this research project, we investigate the role of design conditions (RQ1) and politicians’ characteristics (RQ2) in explaining local politicians’ support for different citizen participation processes using a conjoint experimental design. In the first study, we evaluate to what extent 4 design conditions (initiating actor, participation mode, political uptake, and topic) affect local politicians’ support for citizen participation processes. In the second study, we investigate heterogeneity in politicians’ support for citizen participation by focusing on politicians’ characteristics. Here, in contrast to our baseline assumption in study 1, we seek to explain why some politicians do support different processes of citizen participation. We evaluate the relative influence of opposition or coalition position, political ideology, politicians’ perceptions of citizens, and satisfaction with the functioning of local democracy, on politicians’ support for different types of citizen participation. The conjoint experiment will field in an online survey amongst all local council members, mayors and aldermen in the Netherlands on January 29, 2024. At the time of this pre-registration, the data collection has not yet started.
The dynamical behavior of the Extended Holographic Dark Energy with Hubble Horizon
Creators: name: Liu, Jie
name: Gong, Yungui
name: Chen, Ximing
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The extended holographic dark energy model with the Hubble horizon as the infrared cutoff avoids the problem of the circular reasoning of the holographic dark energy model. Unfortunately, it is hit with the no-go theorem. In this paper, we consider the extended holographic dark energy model with a potential, $V(ϕ)$, for the Brans-Dicke scalar field. With the addition of a potential for the Brans-Dicke scalar field, the extended holographic dark energy model using the Hubble horizon as the infrared cutoff is a viable dark energy model, and the model has the dark energy dominated attractor solution.
description: 12 pages, 7 figures; minor corrections, PRD in press
Transferable empirical pseudopotenials from machine learning
Creators: name: Kim, Rokyeon
name: Son, Young-Woo
Publisher: name: arXiv
Year: 2023
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: Machine learning is used to generate empirical pseudopotentials that characterize the local screened interactions in the Kohn-Sham Hamiltonian. Our approach incorporates momentum-range-separated rotation-covariant descriptors to capture crystal symmetries as well as crucial directional information of bonds, thus realizing accurate descriptions of anisotropic solids. Trained empirical potentials are shown to be versatile and transferable such that the calculated energy bands and wave functions without cumbersome self-consistency reproduce conventional ab initio results even for semiconductors with defects, thus fostering faster and faithful data-driven materials researches.
description: 10 pages, 9 figures, 3 tables
Taming Reversible Halftoning via Predictive Luminance
Creators: name: Lau, Cheuk-Kit
name: Xia, Menghan
name: Wong, Tien-Tsin
Publisher: name: arXiv
Year: 2023
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Image and Video Processing (eess.IV)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Traditional halftoning usually drops colors when dithering images with binary dots, which makes it difficult to recover the original color information. We proposed a novel halftoning technique that converts a color image into a binary halftone with full restorability to its original version. Our novel base halftoning technique consists of two convolutional neural networks (CNNs) to produce the reversible halftone patterns, and a noise incentive block (NIB) to mitigate the flatness degradation issue of CNNs. Furthermore, to tackle the conflicts between the blue-noise quality and restoration accuracy in our novel base method, we proposed a predictor-embedded approach to offload predictable information from the network, which in our case is the luminance information resembling from the halftone pattern. Such an approach allows the network to gain more flexibility to produce halftones with better blue-noise quality without compromising the restoration quality. Detailed studies on the multiple-stage training method and loss weightings have been conducted. We have compared our predictor-embedded method and our novel method regarding spectrum analysis on halftone, halftone accuracy, restoration accuracy, and the data embedding studies. Our entropy evaluation evidences our halftone contains less encoding information than our novel base method. The experiments show our predictor-embedded method gains more flexibility to improve the blue-noise quality of halftones and maintains a comparable restoration quality with a higher tolerance for disturbances.
description: published in IEEE Transactions on Visualization and Computer Graphics
A Simple UV-Completion of QED in 5D
Creators: name: Iengo, Roberto
name: Serone, Marco
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We construct a Lifshitz-like version of five-dimensional (5D) QED which is UV - completed and reduces at low energies to ordinary 5D QED. The UV quantum behaviour of this theory is very smooth. In particular, the gauge coupling constant is finite at all energy scales and at all orders in perturbation theory. We study the IR properties of this theory, when compactified on a circle, and compare the one-loop energy dependence of the coupling in the Lifshitz theory with that coming from the standard 5D QED effective field theory. The range of validity of the 5D effective field theory is found to agree with the more conservative version of Naive Dimensional Analysis.
description: 24 pages, 7 figures; v2: Minor improvements, matches journal version
DFT2kp: effective kp models from ab-initio data
Creators: name: Cassiano, João Victor V.
name: Araújo, Augusto L.
name: Junior, Paulo E. Faria
name: Ferreira, Gerson J.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The $\mathbf{k}\cdot\mathbf{p}$ method, combined with group theory, is an efficient approach to obtain the low energy effective Hamiltonians of crystalline materials. Although the Hamiltonian coefficients are written as matrix elements of the generalized momentum operator $\mathbfπ=\mathbf{p}+\mathbf{p}_{\rm SOC}$ (including spin-orbit coupling corrections), their numerical values must be determined from outside sources, such as experiments or ab initio methods. Here, we develop a code to explicitly calculate the Kane (linear in crystal momentum) and Luttinger (quadratic in crystal momentum) parameters of $\mathbf{k}\cdot\mathbf{p}$ effective Hamiltonians directly from ab initio wavefunctions provided by Quantum ESPRESSO. Additionally, the code analyzes the symmetry transformations of the wavefunctions to optimize the final Hamiltonian. This is an optional step in the code, where it numerically finds the unitary transformation $U$ that rotates the basis towards an optimal symmetry-adapted representation informed by the user. Throughout the paper, we present the methodology in detail and illustrate the capabilities of the code applying it to a selection of relevant materials. Particularly, we show a "hands-on" example of how to run the code for graphene (with and without spin-orbit coupling). The code is open source and available at https://gitlab.com/dft2kp/dft2kp.
description: 28 pages, 8 figures
The chemical abundance analysis of normal early A- and late B-type stars
Creators: name: Fossati, L.
name: Ryabchikova, T.
name: Bagnulo, S.
name: Alecian, E.
name: Grunhut, J.
name: Kochukhov, O.
name: Wade, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Modern spectroscopy of early-type stars often aims at studying complex physical phenomena. Comparatively less attention is paid to identifying and studying the "normal" A- and B-type stars and testing how the basic atomic parameters and standard spectral analysis allow one to fit the observations. We wish to stablish whether the chemical composition of the solar photosphere can be regarded as a reference for early A- and late B-type stars. We have obtained optical high-resolution, high signal-to-noise ratio spectra of three slowly rotating early-type stars (HD 145788, 21 Peg and pi Cet) that show no obvious sign of chemical peculiarity, and performed a very accurate LTE abundance analysis of up to 38 ions of 26 elements (for 21 Peg), using a vast amount of spectral lines visible in the spectral region covered by our spectra. We provide an exhaustive description of the abundance characteristics of the three analysed stars with a critical review of the line parameters used to derive the abundances. We compiled a table of atomic data for more than 1100 measured lines that may be used in the future as a reference. The abundances we obtained for He, C, Al, S, V, Cr, Mn, Fe, Ni, Sr, Y, and Zr are compatible with the solar ones derived with recent 3D radiative-hydrodynamical simulations of the solar photosphere. The abundances of the remaining studied elements show some degree of discrepancy compared to the solar photosphere. Those of N, Na, Mg, Si, Ca, Ti, and Nd may well be ascribed to non-LTE effects; for P, Cl, Sc and Co, non-LTE effects are totally unknown; O, Ne, Ar, and Ba show discrepancies that cannot be ascribed to non-LTE effects. The discrepancies obtained for O (in two stars) and Ne agree with very recent non-LTE abundance analysis of early B-type stars in the solar neighbourhood.
description: Accepted for publication on Astronomy and Astrophysics
title: ÐÑÐ¾ÐµÐºÑ Ð¼Ð½Ð¾Ð³Ð¾ÐºÐ²Ð°ÑÑÐ¸ÑÐ½Ð¾Ð³Ð¾ 5-ÑÐ¸ ÑÑÐ°Ð¶Ð½Ð¾Ð³Ð¾ Ð¶Ð¸Ð»Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð Ð¾Ð´Ð¸Ð¾Ð½Ð¾Ð², ÐÐ°ÐºÑÐ¸Ð¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¶Ð¸Ð»Ð¾Ð¹ Ð´Ð¾Ð¼
Ð¿ÑÐ¾ÐµÐºÑ
ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾

description: ÐÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼ÑÐ¹ Ð¶Ð¸Ð»Ð¾Ð¹ Ð´Ð¾Ð¼ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½ Ð² ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸, ÐÑÐµÐ²Ð¾Ð»Ð¾Ð¶ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ, Ð Ð¾Ð¼Ð°Ð½Ð¾Ð²ÑÐºÐ¾Ð¼ ÑÐµÐ»ÑÑÐºÐ¾Ð¼ Ð¿Ð¾ÑÐµÐ»ÐµÐ½Ð¸Ð¸, Ð¿Ð¾Ñ. Ð Ð¾Ð¼Ð°Ð½Ð¾Ð²ÐºÐ°, Ð´Ð¾Ð¼ â33.ÐÐµÑÑÐ¾ Ð¿Ð¾Ð´ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾ Ð¶Ð¸Ð»Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð° ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾ Ð¾Ñ Ð·Ð°ÑÑÑÐ¾Ð¹ÐºÐ¸. ÐÐ´Ð°Ð½Ð¸Ðµ Ð¶Ð¸Ð»Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð° Ð² Ð¿Ð»Ð°Ð½Ðµ Ð¸Ð¼ÐµÐµÑ Ð²Ð¸Ð´ Ð- Ð¾Ð±ÑÐ°Ð·Ð½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ, Ñ Ð³Ð°Ð±Ð°ÑÐ¸ÑÐ½ÑÐ¼Ð¸ ÑÐ°Ð·Ð¼ÐµÑÐ°Ð¼Ð¸ Ð² Ð¾ÑÑÑ: (1 -10*)-15Ð¼; (Ð-Ð­) - 43; (1-41) -82; (Ð-Ð) - 15 Ð¼. ÐÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²ÐµÐ½Ð½Ð°Ñ ÑÑÐµÐ¼Ð° Ð·Ð´Ð°Ð½Ð¸Ñ - Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÐ¹ Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½ÑÐ¹ ÐºÐ°ÑÐºÐ°Ñ, ÑÐ¾ÑÑÐ¾ÑÑÐ¸Ð¹ Ð¸Ð· ÐºÐ¾Ð»Ð¾Ð½Ð½ ÑÐµÑÐµÐ½Ð¸ÐµÐ¼ 350*350Ð¼Ð¼, ÑÑÐµÐ½ Ð¿Ð¾Ð´Ð²Ð°Ð»Ð°, Ð»ÐµÑÑÐ½Ð¸ÑÐ½Ð¾-Ð»Ð¸ÑÑÐ¾Ð²ÑÐµ ÑÐ·Ð»Ñ ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÐ²Ð»ÑÑÑÑÑ ÑÐ´ÑÐ°Ð¼Ð¸ Ð¶ÐµÑÑÐºÐ¾ÑÑÐ¸ Ð·Ð´Ð°Ð½Ð¸Ð¹, Ð¼ÐµÐ¶Ð´ÑÑÑÐ°Ð¶Ð½ÑÑ Ð¿ÐµÑÐµÐºÑÑÑÐ¸Ð¹ Ð¸ Ð¿Ð¾ÐºÑÑÑÐ¸Ñ ÑÐ¾Ð»ÑÐ¸Ð½Ð¾Ð¹ 180Ð¼Ð¼. Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½Ñ Ð·Ð´Ð°Ð½Ð¸Ñ Ð·Ð°Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð² Ð²Ð¸Ð´Ðµ Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½Ð¾Ð¹ Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½Ð¾Ð¹ Ð¿Ð»Ð¸ÑÑ Ð¸Ð· Ð±ÐµÑÐ¾Ð½Ð° ÐºÐ»Ð°ÑÑÐ° Ð-30 ÑÐ¾Ð»ÑÐ¸Ð½Ð¾Ð¹ 600Ð¼Ð¼. Ð¡ÑÐµÐ½Ñ Ð¿Ð¾Ð´Ð²Ð°Ð»Ð° - Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½ÑÐµ Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÐµ Ð¸Ð· Ð±ÐµÑÐ¾Ð½Ð° ÐºÐ»Ð°ÑÑÐ° Ð-25. Ð¡Ð±Ð¾ÑÐ½ÑÐµ Ð»ÐµÑÑÐ½Ð¸ÑÐ½ÑÐµ Ð¼Ð°ÑÑÐ¸ Ð¸ Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½ÑÐµ Ð¶/Ð± Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÐ¸. ÐÐ°ÑÑÐ¶Ð½ÑÐµ ÑÑÐµÐ½Ñ - Ð¸Ð· Ð³Ð°Ð·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÑ Ð±Ð»Ð¾ÐºÐ¾Ð² Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÑÑ 400 ÐºÐ³/Ð¼3 ÑÐ¾Ð»ÑÐ¸Ð½Ð¾Ð¹ - 250Ð¼Ð¼. ÐÑÐ¾Ð²Ð»Ñ Ð¿Ð»Ð¾ÑÐºÐ°Ñ Ñ 2-Ñ-ÑÐ»Ð¾Ð¹Ð½ÑÐ¼ Ð½Ð°Ð¿Ð»Ð°Ð²Ð»ÑÐµÐ¼ÑÐ¼ Ð¿Ð¾ÐºÑÑÑÐ¸ÐµÐ¼ Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ð¼ Ð²Ð¾Ð´Ð¾ÑÑÐ¾ÐºÐ¾Ð¼. Ð¦Ð²ÐµÑÐ¾Ð²Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ ÑÐ°ÑÐ°Ð´Ð¾Ð² Ð²ÑÐ´ÐµÑÐ¶Ð°Ð½Ð° Ð² ÐºÐ¾Ð½ÑÑÐ°ÑÑÐ½Ð¾Ð¹ Ð³Ð°Ð¼Ð¼Ðµ. ÐÐ»Ð¾ÑÐºÐ¾ÑÑÐ¸ ÑÑÐµÐ½ Ð¾Ð±Ð»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÐ¼ Ð»Ð¸ÑÐµÐ²ÑÐ¼ ÐºÑÐ°ÑÐ½ÑÐ¼ ÐºÐ¸ÑÐ¿Ð¸ÑÐ¾Ð¼ Ð¸ Ð¾ÑÑÑÐºÐ°ÑÑÑÐµÐ½Ñ Ñ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÑÐµÐ¹ Ð¾ÐºÑÐ°ÑÐºÐ¾Ð¹ Ð² Ð±ÐµÐ»ÑÐ¹ Ð¸ ÑÐµÐ¼Ð½Ð¾-ÑÐµÑÑÐ¹ ÑÐ²ÐµÑÐ°. ÐÑÐ´ÐµÐ»Ð¾ÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¾ÑÐ²ÐµÑÐ°ÑÑ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ð¼ ÑÐ°Ð½Ð¸ÑÐ°ÑÐ½ÑÐ¼ Ð¸ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð¿Ð¾Ð¶Ð°ÑÐ½ÑÐ¼ Ð½Ð¾ÑÐ¼Ð°Ð¼. ÐÐ°Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½Ð°Ñ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ½Ð°Ñ Ð¿Ð»Ð¸ÑÐ° ÑÐ¾Ð»ÑÐ¸Ð½Ð¾Ð¹ 600 Ð¼Ð¼. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ±Ð¾Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¸ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½ÑÑ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº.
Classifying irreducible fixed points of five scalar fields in perturbation theory
Creators: name: Rong, Junchen
name: Rychkov, Slava
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Classifying perturbative fixed points near upper critical dimensions plays an important role in understanding the space of conformal field theories and critical phases of matter. In this work, we consider perturbative fixed points of $N=5$ scalar bosons coupled with quartic interactions preserving an arbitrary subgroup $G\subset {\rm O}(5)$. We perform an exhaustive algorithmic search over the symmetry groups $G$ which are irreducible and satisfy the Landau condition, so that the fixed point can be reached by fine-tuning a single mass term and there is no need to tune the cubic couplings. We also impose stability of the RG flow in the space of quartic couplings, and reality. We thus prove that there exist no new stable fixed points in $d=4-ε$ dimensions beyond the two known ones: namely the ${\rm O}(5)$ invariant fixed point and the Cubic(5) fixed point. This work is a continuation of the classification of such fixed points with $N=4$ scalars by Toledano, Michel, Toledano, and Brézin in 1985.
description: 37 pages, 4 figures, references updated
Average observational quantities in the timescape cosmology
Creators: name: Wiltshire, David L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We examine the properties of a recently proposed observationally viable alternative to homogeneous cosmology with smooth dark energy, the timescape cosmology. In the timescape model cosmic acceleration is realized as an apparent effect related to the calibration of clocks and rods of observers in bound systems relative to volume-average observers in an inhomogeneous geometry in ordinary general relativity. The model is based on an exact solution to a Buchert average of the Einstein equations with backreaction. The present paper examines a number of observational tests which will enable the timescape model to be distinguished from homogeneous cosmologies with a cosmological constant or other smooth dark energy, in current and future generations of dark energy experiments. Predictions are presented for: comoving distance measures; H(z); the equivalent of the dark energy equation of state, w(z); the Om(z) measure of Sahni, Shafieloo and Starobinsky; the Alcock-Paczynski test; the baryon acoustic oscillation measure, D_v; the inhomogeneity test of Clarkson, Bassett and Lu; and the time drift of cosmological redshifts. Where possible, the predictions are compared to recent independent studies of similar measures in homogeneous cosmologies with dark energy. Three separate tests with indications of results in possible tension with the Lambda CDM model are found to be consistent with the expectations of the timescape cosmology.
description: 22 pages, 12 figures; v2 discussion, references added, matches published version
title: ÐÑÐµÐ½ÐºÐ° ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ Ð¿ÑÐ¸Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "ÐÐ¾Ð¼Ð¿Ð°Ñ Ð¥Ð¾ÑÑÐµÐ»")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð½Ð¾Ð², ÐÐ²Ð°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: Ð¿ÑÐ¾ÐµÐºÑ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð¾ÑÐµÐ½ÐºÐ°
Ñ Ð¾ÑÑÐµÐ»
expancion project
investment project
economic assessment
hostel

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐµÐµ Ð² ÑÑÐµÑÐµ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐ½ÑÑ ÑÑÐ»ÑÐ³ Ð¸Ð¼ÐµÐ½ÑÐµÐ¼Ð¾Ðµ Â«ÐÐ¾Ð¼Ð¿Ð°Ñ Ð¥Ð¾ÑÑÐµÐ»ÑÂ». Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ Ð¿ÑÐ¸Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿ÑÑÐµÐ¼ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐºÐ¸ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ. ÐÑÐ» ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿Ð»Ð°Ð½ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÐµÐ³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð¾ÑÐµÐ½ÐºÐ°, Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ Ð¿ÑÐ¸Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¸ÑÐºÐ¾Ð².
description: The object of research is the company working in a sphere of hotel services with the name âCompass Hostelsâ. The aim of the work - assessment of commercial attractiveness of company's expansion project through the creation of additional point of accommodation. Company expansion plan was developed, it was carried out it's financial assessment, assessment of commercial attractiveness and assessment of a risks.
The ~0.9 mJy sample: A mid-infrared spectroscopic catalog of 150 infrared-luminous, 24 micron selected galaxies at 0.3
Creators: name: Dasyra, Kalliopi M.
name: Yan, Lin
name: Helou, George
name: Sajina, Anna
name: Fadda, Dario
name: Zamojski, Michel
name: Armus, Lee
name: Draine, Bruce
name: Frayer, David
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present a catalog of mid-infrared (MIR) spectra of 150 infrared (IR) luminous galaxies in the Spitzer extragalactic first look survey obtained with IRS on board Spitzer. The sample is selected to be brighter than ~0.9 mJy at 24 micron and it has a z distribution in the range [0.3,3.5] with a peak at z=1. It primarily comprises ultraluminous IR galaxies at z>1 and luminous IR galaxies at z<1, as estimated from their monochromatic 14 micron luminosities. The number of sources with spectra that are dominated by an active galactic nucleus (AGN) continuum is 49, while 39 sources have strong, star-formation related features. For this classification, we used the equivalent width (EW) of the 11.3 micron polycyclic aromatic hydrocarbon (PAH) feature. Several intermediate/high z starbursts have higher PAH EW than local ULIRGs. An increase in the AGN activity is observed with increasing z and luminosity, based on the decreasing EW of PAHs and the increasing [NeIII]/[NeII] ratio. Spectral stacking leads to the detection of the 3.3 micron PAH, the H2 0-0 S(1) and S(3) lines, and the [NeV] line. We observe differences in the flux ratios of PAHs in the stacked spectra of IR-luminous galaxies with z or luminosity, which are not due to extinction effects. When placing the observed galaxies on IR color-color diagrams, we find that the wedge defining AGN comprises most sources with continuum-dominated spectra, but also contains many starbursts. The comparison of the 11.3 micron PAH EW and the H-band effective radius, measured from HST data, indicates that sources with EW>2 micron, are typically more extended than ~3 kpc. However, there is no strong correlation between the MIR spectral type and the near-IR extent of the sources. [Abridged].
description: accepted for publication in the Astrophysical Journal
title: ÐÐ½ÑÑÑÐ¸ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸ ÐºÐ°Ðº Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ HR-Ð±ÑÐµÐ½Ð´Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ°Ð¹Ð´Ð°Ð¼Ð°ÐºÐ¸Ð½Ð°, Ð®Ð»Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð±ÑÐµÐ½Ð´Ñ
Ð²Ð½ÑÑÑÐ¸ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸
Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° ÑÑÑÐ½Ð¾ÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð²Ð½ÑÑÑÐ¸ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸ Ð¸ HR-Ð±ÑÐµÐ½Ð´, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ»Ð¸, Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð´Ð°Ð½Ð½ÑÑ ÑÐ²Ð»ÐµÐ½Ð¸Ð¹. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð²Ð½ÑÑÑÐ¸ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹. ÐÑÐ»Ð¾ Ð¾Ð±Ð¾Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸ ÑÐµÐ»Ð¸ HR-Ð±ÑÐµÐ½Ð´Ð°, Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. ÐÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ HR-Ð±ÑÐµÐ½Ð´Ñ ÐºÑÑÐ¿Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹ Ð² Ð¾ÑÑÐ°ÑÐ»Ð¸. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð° Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð²Ð½ÑÑÑÐ¸ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð½Ð° Ð¿ÑÐµÐ´Ð¼ÐµÑ ÐµÐ³Ð¾ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð²Ð½ÑÑÑÐ¸ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ Ð´Ð»Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
Large Late-time Asphericities in Three Type IIP Supernovae
Creators: name: Chornock, Ryan
name: Filippenko, Alexei V.
name: Li, Weidong
name: Silverman, Jeffrey M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Type II-plateau supernovae (SNe IIP) are the results of the explosions of red supergiants and are the most common subclass of core-collapse supernovae. Past observations have shown that the outer layers of the ejecta of SNe IIP are largely spherical, but the degree of asphericity increases toward the core. We present evidence for high degrees of asphericity in the inner cores of three recent SNe IIP (SNe 2006my, 2006ov, and 2007aa), as revealed by late-time optical spectropolarimetry. The three objects were all selected to have very low interstellar polarization (ISP), which minimizes the uncertainties in ISP removal and allows us to use the continuum polarization as a tracer of asphericity. The three objects have intrinsic continuum polarizations in the range of 0.83-1.56% in observations taken after the end of the photometric plateau, with the polarization dropping to almost zero at the wavelengths of strong emission lines. Our observations of SN 2007aa at earlier times, taken on the photometric plateau, show contrastingly smaller continuum polarizations (~0.1%). The late-time H-alpha and [O I] line profiles of SN 2006ov provide further evidence for asphericities in the inner ejecta. Such high core polarizations in very ordinary core-collapse supernovae provide further evidence that essentially all core-collapse supernova explosions are highly aspherical, even if the outer parts of the ejecta show only small deviations from spherical symmetry.
description: 15 pages, 13 figures, minor revisions to match published version (2010, ApJ, 713, 1363)
Quantum K theory rings of partial flag manifolds
Creators: name: Gu, W.
name: Mihalcea, L.
name: Sharpe, E.
name: Xu, W.
name: Zhang, H.
name: Zou, H.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we use three-dimensional gauged linear sigma models to make physical predictions for Whitney-type presentations of equivariant quantum K theory rings of partial flag manifolds, as quantum products of universal subbundles and various ratios, extending previous work for Grassmannians. Physically, these arise as OPEs of Wilson lines for certain Chern-Simons levels. We also include a simplified method for computing Chern-Simons levels pertinent to standard quantum K theory.
description: 49 pages, LaTeX; v2: miscellaneous updates
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÐÐ¸ÑÐ¾Ð²ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¼Ð¸ÑÐ½Ð¾Ð²Ð°, 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: 2016
Subjects: ÐÐ¸ÑÐ¾Ð²ÑÐºÐ°Ñ Ð¾Ð±Ð»Ð°ÑÑÑ
Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÐµÐ³Ð¸Ð¾Ð½Ð°
Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ
Ð°ÐºÑÐ¾ÑÑ
ÑÐµÐ»ÐµÐ²Ð°Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°
Ð´Ð¾ÑÐ¾Ð¶Ð½Ð°Ñ ÐºÐ°ÑÑÐ°
Kirov region
foreign economic activity of the region
motoring map
foreign economic strategy
actors
target complex program

description: Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ: Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ, Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð¸ ÐºÑÐµÐ´Ð¸ÑÐ½Ð¾-Ð²Ð°Ð»ÑÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° ÐÐ¸ÑÐ¾Ð²ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. ÐÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Â«ÐÐ¾ÑÐ¾Ð¶Ð½Ð°Ñ ÐºÐ°ÑÑÐ°Â».
description: In this work, were analyzed: foreign economic activity, investment and credit-monetary policy of the Kirov region. Developed a model of the development of economic activities and a Road map.
Unparticle-Higgs Mixing: MSW Resonances, See-saw Mechanism and Spinodal Instabilities
Creators: name: Boyanovsky, D.
name: Holman, R.
name: Hutasoit, Jimmy A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Motivated by slow-roll inflationary cosmology we study a scalar unparticle weakly coupled to a Higgs field in the broken symmetry phase. The mixing between the unparticle and the Higgs field results in a seesaw type matrix and the mixing angles feature a Mikheyev-Smirnov-Wolfenstein (MSW) effect as a consequence of the unparticle field being noncanonical. We find two (MSW) resonances for small and large spacelike momenta. The unparticlelike mode features a nearly flat potential with spinodal instabilities and a large expectation value. An effective potential for the unparticlelike field is generated from the Higgs potential, but with couplings suppressed by a large power of the small seesaw ratio. The dispersion relation for the Higgs-like mode features an imaginary part even at "tree level" as a consequence of the fact that the unparticle field describes a multiparticle continuum. Mixed unparticle-Higgs propagators reveal the possibility of oscillations, albeit with short coherence lengths. The results are generalized to the case in which the unparticle features a mass gap, in which case a low energy MSW resonance may occur for lightlike momenta depending on the scales. Unparticle-Higgs mixing leads to an effective unparticle potential of the new-inflation form. Slow-roll variables are suppressed by seesaw ratios and the anomalous dimensions and favor a red spectrum of scalar perturbations consistent with cosmic microwave background data.
description: 22 pages, 1 figure, RevTeX; v.2: a section on inflation added and references added
Possible $J^{PC} = 0^{--}$ Charmonium-like State
Creators: name: Chen, Wei
name: Zhu, Shi-Lin
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the possible charmonium-like states with $J^{PC}=0^{--}, 0^{-+}$ using the tetraquark interpolating currents with the QCD sum rules approach. The extracted masses are around 4.5 GeV for the $0^{--}$ charmonium-like states and 4.6 GeV for the $0^{-+}$ charmonium-like states while their bottomonium-like analogues lie around 10.6 GeV. We also discuss the possible decay, production and the experiment search of the $0^{--}$ charmonium-like state.
description: 12 pages, 10 figures, 3 tables
Ninguna comida del día es prescindible: hay que conseguir que los niños las hagan todas: reparte sus comidas, 5 al día
Creators: name: Loria-Kohen, Viviana
Publisher: name: Zenodo
Year: 2009

description: Revista de divulgación: Mi Pediatra. Editorial ICM. Se destaca la importancia de todas las comidas durante la edad infantil.
title: ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±Ð¾Ð»ÑÑÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ñ Ð¸ÐµÑÐ°ÑÑ Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÑÐºÑÑÑÐ¾Ð¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð»Ð¾ÑÐ¸Ð½Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: IT-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ
ÑÐ°Ð´Ð¸Ð°Ð»ÑÐ½Ð¾Ðµ Ð´ÐµÑÐµÐ²Ð¾
Ð³Ð¸Ð¿ÐµÑÐ±Ð¾Ð»Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð¾
Ð¸Ð½ÑÐ¾Ð³ÑÐ°ÑÐ¸ÐºÐ°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð·Ð°Ð´Ð°ÑÐ° Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±Ð¾Ð»ÑÑÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¸ÐµÑÐ°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÑÐºÑÑÑÑ. ÐÐ·ÑÑÐµÐ½ Ð¼ÐµÑÐ¾Ð´ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ Ð¸ÐµÑÐ°ÑÑÐ¸Ð¹ Ð² Ð²Ð¸Ð´Ðµ ÑÐ°Ð´Ð¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð´ÐµÑÐµÐ²Ð°. ÐÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð³Ð¸Ð¿ÐµÑÐ±Ð¾Ð»Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð° Ð¸ Ð¼ÐµÑÐ¾Ð´ ÐµÐ³Ð¾ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ Ð½Ð° Ð¿Ð»Ð¾ÑÐºÐ¾ÑÑÑ Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÐÑÐ°Ð½ÐºÐ°ÑÐµ. ÐÐ° ÑÐ·ÑÐºÐµ JavaScript Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð¾ Ð´Ð²Ð° Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð°: Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐ°Ð´Ð¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð³Ð¸Ð¿ÐµÑÐ±Ð¾Ð»Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð´ÐµÑÐµÐ²Ð°. ÐÐ¾Ð»ÑÑÐµÐ½Ð½ÑÐµ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ Ð½Ð° ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¾Ð±ÑÐµÐ¼Ð°Ñ Ð´Ð°Ð½Ð½ÑÑ, Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐµÐ³Ð¾ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÑÐ¸Ñ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹.
Discovery and Characterization of Transiting SuperEarths Using an All-Sky Transit Survey and Follow-up by the James Webb Space Telescope
Creators: name: Deming, D.
name: Seager, S.
name: Winn, J.
name: Miller-Ricci, E.
name: Clampin, M.
name: Lindler, D.
name: Greene, T.
name: Charbonneau, D.
name: Laughlin, G.
name: Ricker, G.
name: Latham, D.
name: Ennico, K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Doppler and transit surveys are finding extrasolar planets of ever smaller mass and radius, and are now sampling the domain of superEarths (1-3 Earth radii). Recent results from the Doppler surveys suggest that discovery of a transiting superEarth in the habitable zone of a lower main sequence star may be possible. We evaluate the prospects for an all-sky transit survey targeted to the brightest stars, that would find the most favorable cases for photometric and spectroscopic characterization using the James Webb Space Telescope (JWST). We use the proposed Transiting Exoplanet Survey Satellite (TESS) as representative of an all-sky survey. We couple the simulated TESS yield to a sensitivity model for the MIRI and NIRSpec instruments on JWST. We focus on the TESS planets with radii between Earth and Neptune. Our simulations consider secondary eclipse filter photometry using JWST/MIRI, comparing the 11- and 15-micron bands to measure CO2 absorption in superEarths, as well as JWST/NIRSpec spectroscopy of water absorption from 1.7-3.0 microns, and CO2 absorption at 4.3-microns. We project that TESS will discover about eight nearby habitable transiting superEarths. The principal sources of uncertainty in the prospects for JWST characterization of habitable superEarths are superEarth frequency and the nature of superEarth atmospheres. Based on our estimates of these uncertainties, we project that JWST will be able to measure the temperature, and identify molecular absorptions (water, CO2) in one to four nearby habitable TESS superEarths.
description: accepted for PASP; added discussion and figure for habitable planets; abridged Abstract
OActive project Data Management Plan introduction
Creators: name: Gondikas, Andreas
name: Katsavou, Ioanna
Publisher: name: Zenodo
Year: 2019
Subjects: Data Management Plan (DMP)
FAIR DATA
metadata
open access
repositories
data generating procedures
Publications

description: During the DMP training Axia has provided information on data and metadata that should be collected, the choise of publishing vs patenting, the importance of publishing in open access journals, the data management plan principles, and why data shoud be F.A.I.R.
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¢ÑÑÑÐ¸Ð½Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÑÑÑÑÑ
Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð±ÑÐ´Ð¶ÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ°ÑÐºÑÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ, ÑÑÑÐ½Ð¾ÑÑÑ Ð¸ ÑÐ¾Ð»Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±ÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÐµÐ¼. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ "ÐÐ°Ð»ÑÑÐ¿ÐµÑÑÑÑÐ¾Ð¹". Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸, Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸, ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸, Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÑÐºÑÑÑÑ Ð°ÐºÑÐ¸Ð²Ð¾Ð² Ð¸ Ð¿Ð°ÑÑÐ¸Ð²Ð¾Ð². ÐÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐºÑÑÐµÐ¹ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸ Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
Large scale structure of the Universe
Creators: name: Einasto, Jaan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: A short overview is given on the development of our present paradigm of the large scale structure of the Universe with emphasis on the role of Ya. B. Zeldovich. Next we use the Sloan Digital Sky Survey data and show that the distribution of phases of density waves of various scale in the present-day Universe are correlated. Using numerical simulations of structure evolution we show that the skeleton of the cosmic web was present already in an early stage of the evolution of structure. The positions of maxima and minima of density waves (their phases) are the more stable, the larger is the wavelength. The birth of the first generation of stars occured most probably in the central regions of rich proto-superclusters where the density was highest in the early Universe.
description: 10 pages, 9 figures; The Sun, the Stars, the Universe and General Relativity, International conference in honor of Ya. B. Zeldovich 95th Anniversary, April 20 - 23, 2009, Minsk; Eds. R. Ruffini, G. Vereshchagin