cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Transition Density and Pressure at the Inner Edge of Neutron Star Crusts
Creators: name: Xu, Jun
name: Ko, Che Ming
name: Chen, Lie-Wen
name: Li, Bao-an
name: Ma, Hong-Ru
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Using the nuclear symmetry energy that has been recently constrained by the isospin diffusion data in intermediate-energy heavy ion collisions, we have studied the transition density and pressure at the inner edge of neutron star crusts, and they are found to be 0.040 fm$^{-3}$ $\leq ρ_{t}\leq 0.065$ fm$^{-3}$ and 0.01 MeV/fm$^{3}$ $\leq P_{t}\leq 0.26$ MeV/fm$^{3}$, respectively, in both the dynamical and thermodynamical approaches. We have also found that the widely used parabolic approximation to the equation of state of asymmetric nuclear matter gives significantly higher values of core-crust transition density and pressure, especially for stiff symmetry energies. With these newly determined transition density and pressure, we have obtained an improved relation between the mass and radius of neutron stars.
description: 7 pages, 3 figures, proceeding of "The International Workshop on Nuclear Dynamics in Heavy-Ion Reactions and the Symmetry Energy (IWND2009)"
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 Â«ÐÐ¸Ð¾Ð¾ÑÐ³Ð°Ð½Ð¸ÑÐµÑÐºÐ°Ñ Ñ Ð¸Ð¼Ð¸ÑÂ»
title: Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸: 19.03.01 "ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ", 19.03.04 "Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ"; ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ (ÑÑÐµÐ¿ÐµÐ½Ñ) Ð²ÑÐ¿ÑÑÐºÐ½Ð¸ÐºÐ° - Ð±Ð°ÐºÐ°Ð»Ð°Ð²Ñ; ÑÐ¾ÑÐ¼Ð° Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ - Ð¾ÑÐ½Ð°Ñ, Ð¾ÑÐ½Ð¾-Ð·Ð°Ð¾ÑÐ½Ð°Ñ, Ð·Ð°Ð¾ÑÐ½Ð°Ñ
titleType: Subtitle
Creators: name: ÐÐ¾Ð¿Ð¾Ð²Ð°, ÐÐ°ÑÐ¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: ÐÑÐ³Ð°Ð½Ð¸ÑÐµÑÐºÐ°Ñ Ñ Ð¸Ð¼Ð¸Ñ
ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°
Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ

description: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¤ÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Â«Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² 19.03.01 Â«ÐÐ¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ» Ð¸ 19.03.04 Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸ÑÂ» Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÐ¸Ð¾Ð¾ÑÐ³Ð°Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð¼Ð¸ÑÂ» Ð¾ÑÐ½Ð¾Ð¹, Ð¾ÑÐ½Ð¾-Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¸ Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð£ÐÐ¡Ð 19.00.00 Â«ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â».
Ð¡Ð¾Ð´ÐµÑÐ¶Ð°Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ Ð¾Ð²Ð»Ð°Ð´ÐµÑÑ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐ¼Ð¸ Ð·Ð½Ð°Ð½Ð¸ÑÐ¼Ð¸, Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¼Ð¸ ÑÐ¼ÐµÐ½Ð¸ÑÐ¼Ð¸ Ð¸ Ð½Ð°Ð²ÑÐºÐ°Ð¼Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¾Ð¿ÑÑÐ¾Ð¼ ÑÐ²Ð¾ÑÑÐµÑÐºÐ¾Ð¹ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ñ Ð½Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹:
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Additional file 2 of The direct and mediating effect of social support on health-related quality of life during pregnancy among Australian women
Creators: name: Bedaso, Asres
name: Adams, Jon
name: Peng, Wenbo
name: Sibbritt, David
Publisher: name: figshare
Year: 2023
Subjects: subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÑÐ°ÑÐ°ÐºÑÐ½ÑÑ ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¨Ð¸Ð»Ð¸Ð½Ð°, ÐÐ°Ñ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: 2017
Subjects: ÐºÐ¾Ð½ÑÑÐ°ÑÐ°ÐºÑÐ½ÑÐµ ÑÐ¾Ð²Ð°ÑÑ
ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ
Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð°Ñ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑ
ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ðµ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð¾
ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ ÑÐµÐµÑÑÑ

description: Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð²Ð²Ð¾Ð·Ð¸Ð¼ÑÑ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÑÑ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ñ ÐºÐ¾Ð½ÑÑÐ°ÑÐ°ÐºÑÐ½ÑÑ ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð°Ñ Ð±Ð°Ð·Ð°, ÑÐµÐ³ÑÐ»Ð¸ÑÑÑÑÐ°Ñ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð² Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¸ ÑÐ¾Ð²Ð°ÑÐ¾Ð², ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð¾Ð±ÑÐµÐºÑÑ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÐ¸, Ð¸Ð·ÑÑÐµÐ½Ñ Ð¼ÐµÑÑ, Ð¿ÑÐ¸Ð½Ð¸Ð¼Ð°ÐµÐ¼ÑÐµ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¾ÑÐ³Ð°Ð½Ð°Ð¼Ð¸ Ð´Ð»Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÑÐ°ÑÐ°ÐºÑÐ½ÑÑ ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¼ÐµÑ, ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐµÑÐµ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¾Ð² Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÑÐ°ÑÐ°ÐºÑÐ½ÑÑ ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð¿ÑÐ¸ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ð¸ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ.
Parental information for the adopted child : a descriptive study of relationships between adoptive parents and adopted children between the ages of six and ten, based on Children's Aid Society of Vancouver cases, 1947-1957
Creators: name: Taylor, Audrey Rothnie
Publisher: name: University of British Columbia
Year: 2012

description: Because of the growing recognition that early, continuous and warm relationships are essential for a child's healthy development, it is important that children be placed in their adoptive home as early as possible and that the home be well chosen. But information about the origins of an adopted child is specially significant in several ways. The purpose of this thesis is to explore the subject of how adoptive parents tell their child he is adopted, and to assess their feelings and attitudes on this topic. For exploratory purposes, seven adoptive homes were selected from the files of the Children's Aid Society of Vancouver for study. The adoptions had been completed from five to nine years ago. Each child had been placed in his adoptive home as an infant under 5 months of age. All adoptive parents were interviewed, also the natural parents' file and adoption home files were studied. The study includes a brief description of the adoptive parents, their home, the child, and his adjustment in the home. The subject of telling the child he is adopted is focussed particularly on (a) method of giving the information; (b) time of introduction of the subject; (c) the child's reaction; and (d) questions asked by the child. The analysis of the material obtained indicates that these adoptive parents accepted as their responsibility telling their child he was adopted. Typically, the simple facts of how he came to live with them were told to the child as soon as he was old enough to understand. However, none of the children in the group studied had asked any questions about their natural parents, and all parents signified that they would wait until their child asked specific questions. This suggests that adoptive parents have difficulties in accepting natural parents, and their main area of concern is how and when to tell their child about them. It is indicated that adoption workers should give more guidance to adoptive parents before and after placement in this area, and that adoptive parents should be encouraged to return to the agency for help if needed.
Tra telescopi ed esopianeti
Creators: Dal nostro inviato Marco Galliani
Publisher: name: Media Inaf
Year: 2015

A Honolulu, nella sede del convegno promosso dalla International Astronomical Union, abbiamo incontrato Judith Provencal  e Michael Montgomery per parlarci del progetto Whole Earth Telescope. Lisa Kaltenegger invece ci ha raccontato lo stato dell'arte nella ricerca dei pianeti extrasolari e il suo entusiasmo di essere la prima a votare per il concorso NameExoWorlds
Prospects for top-prime quark discovery at the Tevatron
Creators: name: Dobrescu, Bogdan A.
name: Kong, Kyoungchul
name: Mahbubani, Rakhi
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show that a top-prime quark as heavy as 600 GeV can be discovered at the Tevatron, provided it is resonantly pair-produced via a vector color octet. If the top-prime originates from a vectorlike quark, then the production of a single top-prime in association with a top may also be observable, even through its decay into a Higgs boson and a top. A color octet with mass of about 1 TeV, which decays into a top-prime pair, may account for the CDF excess of semileptonic (Wj)(Wj) events.
description: 22 pages, 6 ps figures. v2: Note added about the new D0 search for (Wb)(Wb) resonances; section 4.1 expanded; single-top constraint updated in section 2; references added
Binaries of massive black holes in rotating clusters: Dynamics, gravitational waves, detection and the role of eccentricity
Creators: name: Amaro-Seoane, Pau
name: Eichhorn, Christoph
name: Porter, Edward K.
name: Spurzem, Rainer
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The dynamical evolution of binaries of intermediate-massive black holes (IMBHs, massive black holes with a mass ranging between $10^2$ and $10^4 M_{\odot}$) in stellar clusters has recently received an increasing amount of attention. This is at least partially due to the fact that if the binary is hard enough to evolve to the phase at which it will start emitting gravitational waves (GWs) efficiently, there is a good probability that it will be detectable by future space-borne detectors like LISA. We study this evolution in the presence of rotation in the cluster. The eccentricity is strongly connected to the initial IMBHs velocities, and values of $\sim 0.7$ up to 0.9 are reached for low initial velocities, while almost circular orbits result if the initial velocities are increased. A Monte Carlo study indicates that these sources will be detectable by a detector such as LISA with median signal to noise ratios of between 10 and 20 over a three year period, although some events had signal to noise ratios of 300 or greater. Furthermore, one should also be able to estimate the chirp-mass with median fractional errors of $10^{-4}$, reduced mass on the order of $10^{-3}$ and luminosity distance on the order of $10^{-1}$. Finally, these sources will have a median angular resolution in the LISA detector of about 3 square degrees, putting events firmly in the field of view of future electromagnetic detectors such as LSST.
description: 20 pages, 12 figs, abstract abridged. Minor changes. Accepted for publication in MNRAS
title: ÐÑÐµÐ½ÐºÐ° Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÐºÐ¾Ð² Ð¿ÑÐ¸ Ð¾ÑÐ²Ð¾ÐµÐ½Ð¸Ð¸ Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²ÑÑ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ð¹ ÐÑÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ³Ð¸Ð¾Ð½Ð°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐµÑÐºÑÐ»Ð¾Ð²Ð°, Ð¡ÑÑÑ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: 2017
Subjects: ÐÐµÑÑÑÐ½ÑÐµ Ð¸ Ð³Ð°Ð·Ð¾Ð²ÑÐµ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ
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Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÐºÐ¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐ»Ð¾Ð²Ð½Ð¾Ðµ Ð½ÐµÑÑÑÐ½Ð¾Ðµ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ðµ Ð½Ð° Ð°ÑÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¼ ÑÐµÐ»ÑÑÐµ Ð Ð¾ÑÑÐ¸Ð¸ (ÐÐµÑÐ¾ÑÑÐºÐ¾Ðµ Ð¼Ð¾ÑÐµ). Ð¦ÐµÐ»ÑÑ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾ÑÐµÐ½ÐºÐ° Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÐºÐ¾Ð² Ð¿ÑÐ¸ Ð¾ÑÐ²Ð¾ÐµÐ½Ð¸Ð¸ Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²ÑÑ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ð¹ ÐÑÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ³Ð¸Ð¾Ð½Ð°. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð²Ð½ÐµÑÐ½Ð¸Ñ Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÐºÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð°ÑÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸Ðº Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÐºÐ¾Ð², Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐ°Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¸Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð² Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¸ Ð°ÑÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð². ÐÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ°. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÑÐ°Ð²ÐºÐ° Ð´Ð¸ÑÐºÐ¾Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ¸ÑÑÐ°Ñ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð½Ð°Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°, ÑÑÐ¾Ðº Ð¾ÐºÑÐ¿Ð°ÐµÐ¼Ð¾ÑÑÐ¸, Ð¸Ð½Ð´ÐµÐºÑ Ð´Ð¾ÑÐ¾Ð´Ð½Ð¾ÑÑÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÐºÐ°ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÐºÐ¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð²ÑÑÐ²Ð¸Ð²ÑÐ¸Ð¹ ÐºÐ»ÑÑÐµÐ²ÑÐµ ÑÐ°ÐºÑÐ¾ÑÑ, Ð²Ð»Ð¸ÑÑÑÐ¸Ðµ Ð½Ð° ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°.
title: Ð Ð°ÑÑÐµÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¸ Ð¾ÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ Jupiter Ð² ÐÐ°ÑÐµÐ½ÑÐµÐ²Ð¾Ð¼ Ð¼Ð¾ÑÐµ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ´Ð¸Ð½Ð¾ÐºÐ¾Ð²Ð°, ÐÐ°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: 2017
Subjects: Ð¼Ð¾ÑÑÐºÐ°Ñ Ð±ÑÑÐ¾Ð²Ð°Ñ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ð°
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description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: Ð¼Ð¾ÑÑÐºÐ°Ñ Ð±ÑÑÐ¾Ð²Ð°Ñ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ð°. Ð¦ÐµÐ»Ð¸ ÑÐ°Ð±Ð¾ÑÑ: ÑÐ°ÑÑÑÐ¸ÑÐ°ÑÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ Ð¼Ð¾ÑÑÐºÐ¾Ð¹ Ð±ÑÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ Ñ ÑÑÐµÑÐ¾Ð¼ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð½Ð¾ÑÐ¼Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ Ð² ÑÐµÑÐµÐ½Ð¸Ð¸ Ð²ÑÐµÐ³Ð¾ ÑÑÐ¾ÐºÐ° ÑÐ»ÑÐ¶Ð±Ñ; ÑÐ°ÑÑÑÐ¸ÑÐ°ÑÑ Ð¾ÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ Ð¿ÑÐ¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ¸ÑÐ¾Ð²ÐºÐµ. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð¼Ð¾ÑÑÐºÐ¾Ð¹ Ð±ÑÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ Ð½Ð° Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð²Ð½ÐµÑÐ½Ð¸Ñ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº; Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð¿ÑÐ¾Ð²ÐµÑÐºÐ° ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð½Ð° Ð¾Ð¿ÑÐ¾ÐºÐ¸Ð´ÑÐ²Ð°Ð½Ð¸Ðµ Ð¸ Ð¿Ð»Ð¾ÑÐºÐ¸Ð¹ ÑÐ´Ð²Ð¸Ð³; ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð° Ð¾ÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð² ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ð¼ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¸. ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¿Ð¾ÑÑÐ½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð·Ð°Ð¿Ð¸ÑÐºÑ Ð¾Ð±ÑÐµÐ¼Ð¾Ð¼ 95 ÑÑÑÐ°Ð½Ð¸ÑÐ°, Ð²ÐºÐ»ÑÑÐ°Ñ 11 Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¸Ð¹, ÑÐ¿Ð¸ÑÐ¾Ðº Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð¸Ð· 23 Ð½Ð°Ð¸Ð¼ÐµÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¸ 7 Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ñ Ð² ÑÐµÐ±Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¸ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÑÑÐ½ÐµÐ½Ð¸Ñ.
The Wouthuysen-Field effect in a clumpy intergalactic medium
Creators: name: Higgins, Jonathan
name: Meiksin, Avery
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that, due to the high optical depth of the intergalactic medium to Lyman-alpha photons before the Epoch of Reionization, the Lyman-alpha scattering rate responsible for the Wouthuysen-Field effect from an isolated source will be negligible unless (1) there is sufficient time for the scattering photons to establish a steady state, or (2) the scattering gas is undergoing internal expansion or has a peculiar motion of tens to hundreds of km/s away from the source. We present steady-state solutions in the radiative diffusion approximation for the radiation field trapped in a clump of gas and show that this may result in an enhancement, by a factor of up to 10^6, of the strength of the Wouthuysen-Field effect over that obtained from the free-streaming limit. Solutions to the time-dependent diffusion equation, however, suggest that the timescales required to reach such a steady state will generally exceed the source lifetimes. In the presence of internal expansion, a steady state may be established as photons are redshifted into the red wing, and significant enhancement in the scattering rate may again be produced. Alternatively, a substantial scattering rate may arise in systems with a peculiar motion away from the source that redshifts the received radiation into the resonance line centre. As a consequence, at epochs z<30, when collisional decoupling is small except in dense regions, and prior to the establishment of any large-scale diffuse radiation field of resonance line photons, the 21cm signature from the Intergalactic Medium produced by the Wouthuysen-Field effect will in general trace the peculiar velocity field of the gas in addition to its density structure.
description: 11 pages, 7 figures. Accepted for publication in MNRAS
title: International Service Learning 3.0: Using Technology to Improve Outcomes and Sustainability
Creators: name: Vandarakis, Anthony
Publisher: name: World Academy of Science, Engineering and Technology
Year: 2020

description: Today’s International Service Learning practices require an update: modern technologies, fresh educational frameworks, and a new operating system to accountably prosper. This paper describes a model of International Service Learning (ISL), which combines current technological hardware, electronic platforms, and asynchronous communications that are grounded in inclusive pedagogy. This model builds on the work around collaborative field trip learning, extending the reach to international partnerships across continents. Mobile technology, 21st century skills and summitbasecamp modeling intersect to support novel forms of learning that tread lightly on fragile natural ecosystems, affirm local reciprocal partnership in projects, and protect traveling participants from common yet avoidable cultural pitfalls.
L’inquinamento luminoso visto dallo spazio
Creators: Dal nostro inviato Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Un team di scienziati dell’Università Complutense di Madrid in Spagna, del  Cégep de Sherbrooke in Canada, e un gruppo di volontari hanno dato il via a un progetto chiamato Cities at Night per monitorare il fenomeno dell’inquinamento luminoso, sfruttando le tantissime immagini scattate negli anni dagli astronauti della Stazione Spaziale Internazionale. I primi risultati presentati all'Assemblea Generale della IAU a Honolulu, Hawaii
Un buco nero piccino picciò’
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Nel cuore di una galassia nana a 340 milioni di anni luce, gli astronomi dell'Università del Michigan hanno identificato il più piccolo buco nero supermassiccio mai trovato. Con una massa di 50 mila masse solari, l'oggetto è più di due volte più piccolo di ogni altro oggetto noto del suo genere e 100 mila volte meno massivo dei buchi neri più grossi che risiedono nei nuclei delle altre galassie. I risultati su Astrophysical Journal Letters
A product involving the $β$-family in stable homotopy theory
Creators: name: Liu, Xiugui
name: Li, Wending
Publisher: name: arXiv
Year: 2009
Subjects: subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics
subject: 55Q45, 55T15

description: In the stable homotopy groups $π_{q(p^n+p^m+1)-3}(S)$ of the sphere spectrum $S$ localized at the prime $p$ greater than three, J. Lin constructed an essential family $ξ_{m,n}$ for $n \geq m + 2 >5$. In this paper, the authors show that the composite $ξ_{m,n}β_{s}\in π_{q(p^n+p^m+sp+s)-5}(S)$ for $2 \leq s < p$ is non-trivial, where $q=2(p-1)$ and $β_s \in π_{q(sp+s-1)-2}(S)$ is the known $β$-family. We show our result by explicit combinatorial analysis of the (modified) May spectral sequence.
description: 10 pages
Additional file 1 of Mechanical hyperinflation maneuver and intracranial compliance of critical neurological patients: protocol for a randomized controlled equivalence trial
Creators: name: de Almeida Souza, Daniela
name: Branco, Marina Wolff
name: Carraro Junior, Hipólito
name: Zocolotti, Ana Márcia Delattre
name: Takeda, Sibele Yoko Mattozo
name: Valderramas, Silvia
Publisher: name: figshare
Year: 2023
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. SPIRIT Checklist for Trials.
Canonical high power blazars
Creators: name: Ghisellini, G.
name: Tavecchio, F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The jets of powerful blazars propagate within regions relatively dense of radiation produced externally to the jet. This radiation is a key ingredient to understand the origin of the high energy emission of blazars, from the X-ray to the gamma-ray energy band. These external radiation fields control the amount of the inverse Compton radiation with respect to the synchrotron flux. Therefore the predicted spectral energy distribution (SED) will depend on where the jet dissipates part of its energy to produce the observed radiation. We investigate in detail how the SED changes as a function of the location of the jet dissipation region, by assuming rather "standard" (i.e. "canonical") prescriptions for the accretion disk and its X-ray corona, the profile of the jet magnetic field and the external radiation. The magnetic energy density of a "canonical" jet almost never dominates the radiative cooling of the emitting electrons, and consequently the inverse Compton flux almost always dominates the bolometric output. This is more so for large black hole masses. Dissipation taking place beyond the broad line region is particularly interesting, since it accounts in a simple way for the largest inverse Compton to synchrotron flux ratios accompanied by an extremely hard X-ray spectrum. Furthermore it makes the high power blazars at high redshift useful tools to study the optical to UV cosmic backgrounds.
description: Revised version accepted for publication in MNRAS
Via col voto!
Creators: Sabrina Masiero
Publisher: name: Media Inaf
Year: 2015

Si apre, durante la XXIX Assemblea Generale IAU che si tiene in questi giorni a Honolulu, la fase effettiva di votazione del nome da assegnare ai 20 sistemi planetari a conclusione della campagna promossa dall’Unione Astronomica Internazionale. Tutti possono partecipare alla votazione delle migliori proposte candidate da tutto il Mondo. Qui vi descriviamo le due selezionate da INAF e SAIt.
Il Sole scagionato
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Un nuovo metodo di conteggio delle macchie solari mostra un'attività stabile negli ultimi 400 anni, in contrasto con l'aumento progressivo, frutto, pare, di un errore di calibrazione. Questo risultato mette in forte crisi l'ipotesi che vi sia una correlazione tra l'attività solare e i cambiamenti climatici osservati sul nostro pianeta. Il nuovo studio è stato presentato alla XXIX Assemblea Generale dell'IAU
Radio observations of ZwCl 2341.1+0000: a double radio relic cluster
Creators: name: van Weeren, R. J.
name: Rottgering, H. J. A.
name: Bagchi, J.
name: Raychaudhury, S.
name: Intema, H. T.
name: Miniati, F.
name: Ensslin, T. A.
name: Markevitch, M.
name: Erben, T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Context: Hierarchal models of large scale structure (LSS) formation predict that galaxy clusters grow via gravitational infall and mergers of (smaller) mass concentrations, such as clusters and galaxy groups. Diffuse radio emission, in the form of radio halos and relics, is found in clusters undergoing a merger, indicating that shocks or turbulence associated with the merger are capable of accelerating electrons to highly relativistic energies. Here we report on radio observations of ZwCl 2341.1+0000, a complex merging structure of galaxies located at z=0.27, using Giant Metrewave Radio Telescope (GMRT) observations. Aims: The main aim of the observations is to study the nature of the diffuse radio emission in the galaxy cluster ZwCl 2341.1+0000. Methods: We have carried out GMRT 610, 241, and 157 MHz continuum observations of ZwCl 2341.1+0000. The radio observations are combined with X-ray and optical data of the cluster. Results: The GMRT observations show the presence of a double peripheral radio relic in the cluster ZwCl 2341.1+0000. The spectral index is -0.49 \pm 0.18 for the northern relic and -0.76 \pm 0.17 for the southern relic respectively. We have derived values of 0.48-0.93 microGauss for the equipartition magnetic field strength. The relics are probably associated with an outwards traveling merger shock waves.
description: 14 pages, 10 figures, accepted for publication in A&A on July 30, 2009
ATLAS: arriva la sentinella anti asteroidi
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Si chiama Asteroid Terrestrial-impact Last Alert System telescope e promette di difenderci da tutti quegli asteroidi che potrebbero rappresentare una minaccia per la Terra. Appena completato sulla cima del vulcano Haleakala alle Hawaii, è un progetto finanziato dalla NASA
Possible Reversible Cerebral Vasoconstriction Syndrome Associated with Eucalyptus: Case Report
Creators: name: Zeenat Qureshi Stroke Institutes
Publisher: name: Zenodo
Year: 2023

description: Background

Reversible cerebral vasoconstrictive syndrome (RCVS) has characteristic clinical features, brain imaging and Angiographic features. The majority of RCVS cases are associated with the use of antidepressants, polysubstance abuse, and nasal decongestants. We here present a case that highlights the use of eucalyptus herbs as a possible precipitant factor for RCVS formation.

Case Presentation

A 42-year-old woman presented to the emergency department with a tingling sensation on the right-hand side of her body and a two-week progressive throbbing severe holocranial headache radiating to the neck, with associated nausea, photophobia, and phonophobia. She denied any seizures and recent trauma or fevers. She was not taking scheduled medications, but she had used inhaling vapors obtained from boiling eucalyptus leaves to alleviate sinus congestion. Initial imaging revealed subarachnoid hemorrhage at bilateral posterior parietal convexity leading to her admission into the intensive care unit. Further work up disclosed the presence of findings consistent with RCVS.
Rosetta spritz
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Un getto record di materiale cometario, lungo oltre 186 km, è stato prodotto da 67P/Churyumov–Gerasimenko il 29 luglio scorso e catturato prontamente dai sensori della sonda ESA Rosetta. Alessandra Rotundi (responsabile dello strumento GIADA): «Un autentico dust party!»
Two-dimensional GaAs/AlGaAs superlattice structures for solar cell applications: ultimate efficiency estimation
Creators: name: Klos, Jaroslaw
name: Krawczyk, Maciej
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We calculate the band structure of a two-dimensional GaAs/AlGaAs superlattice and estimate the ultimate efficiency of solar cells using this type of structure for solar energy conversion. The superlattice under consideration consists of gallium arsenide rods forming a square lattice and embedded in aluminium gallium arsenide. The ultimate efficiency is determined versus structural parameters including the filling fraction, the superlattice constant, the rod geometry and the concentration of Al in the matrix material. The calculated efficiency of the superlattice proves to exceed the efficiency of each component material in the monolithic state in a wide range of parameter values.
description: 11 pages, 7 figures
Additional file 4 of Sex differences in impact of cumulative systolic blood pressure from childhood to adulthood on albuminuria in midlife: a 30-year prospective cohort study
Creators: name: Wang, Dan
name: Kou, Pu-qing
name: Liao, Yue-yuan
name: Wang, Ke-ke
name: Yan, Yu
name: Chen, Chen
name: Chu, Chao
name: Wang, Yang
name: Niu, Ze-Jiaxin
name: Ma, Qiong
name: Sun, Yue
name: Mu, Jian-jun
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Mental Health

description: Supplementary Material 4
Il lento spegnersi dell’Universo
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

L'Universo si sta spegnendo lentamente. E' quanto emerge da uno studio che ha permesso di determinare il bilancio energetico dell'Universo locale grazie all'analisi dei dati di oltre 200 mila galassie. I risultati, che saranno riportati su Monthly Notices, suggeriscono che l'energia prodotta oggi in una certa zona dello spazio risulta circa la metà di quella prodotta due miliardi di anni fa e questa diminuzione avviene a tutte le lunghezze d'onda
Geodromicus beibienkoi Tichomirova 1973
Creators: name: Cheng, Zhi-Fei
name: Shavrin, Alexey V.
name: Peng, Zhong
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Geodromicus
Geodromicus beibienkoi

description: Geodromicus beibienkoi Tichomirova, 1973
(Figs. 2, 8–12, 113)
 Geodromicus beibienkoi Tichomirova, 1973: 156; Shavrin 2018: 156, Zerche 2003: 284, Kim et al. 2008: 642
 Material examined (9 ♂♂, 1 ♀): CHINA: NEIMENGGU AUTONOMOUS REGION: 4 ♂♂, 1 ♀: Aershan National Forest Park [ȐAEƜOiẎÁḨĿẘ]. 18.07.2004. Li & Huang leg. (SNUC);  HEBEI PROVINCE:  3 ♂♂: Yu County [Üƃ], Jinhekou [ḔñD]. 1,300 m a.s.l. 23.08.2005. Li-Zhen Li leg. (SNUC); SHANXI: 2 ♂♂: Ningwu County [ŤȄƃ], Luyashan [ḌṞƜ]. 17– 18.07.2001. Li & Zhao leg. (SNUC).
 Additional material examined (2 ♀♀): RUSSIA: MARITIME PROVINCE: 2 ♀♀: Tigroviy. 25– 27.07.1990. S. Becvar leg. (CZ).
 Remarks. Habitus as in Fig. 2. Male abdominal tergite VIII as in Fig. 8, and male abdominal sternite VIII as in Fig. 9. Aedeagus as in Figs. 10–12. The species is distributed from Cisbaikalia to the southern Russian Far East, Northwest China, and Korea (Shavrin 2018). It was recorded from Heilongjiang by Zerche (2003), and from Heilongjiang and Jilin by Shavrin (2018). The distribution of G. beibienkoi in China is shown in Fig. 113. It is here recorded from Neimenggu Autonomous Region, Hebei and Shanxi for the first time.
description: Published as part of Cheng, Zhi-Fei, Shavrin, Alexey V. & Peng, Zhong, 2020, New species and records of Geodromicus Redtenbacher, 1857 from China (Coleoptera: Staphylinidae: Omaliinae: Anthophagini), pp. 132-170 in Zootaxa 4789 (1) on pages 136-137, DOI: 10.11646/zootaxa.4789.1.4, http://zenodo.org/record/3884789
title: ÐÐ¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð² ÑÐµÑÑÐ¾ÑÐ°Ð½Ð½Ð¾Ð¼ Ð±Ð¸Ð·Ð½ÐµÑÐµ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¾Ð²Ð³Ð¸Ñ, 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: 2017
Subjects: Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ
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ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð°ÑÐ¿ÐµÐºÑÐ¾Ð² Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÐ¾Ðµ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐ»Ð¾ÑÑ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° ÐÐÐ Â«ÐÐ°Ð½Ð´Ð°Ð½Ð°Â». ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐ½Ð¾ÑÑÐ¸ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð°, ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð°ÑÐ¿ÐµÐºÑÐ¾Ð² Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¸ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐ°Ð½Ð´Ð°Ð½Ð°Â». ÐÐ½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑ Ð¿Ð¾Ð²ÑÑÐ¸Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° ÐÐÐ Â«ÐÐ°Ð½Ð´Ð°Ð½Ð°Â». Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¾ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð¸ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð². Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° ÐÐÐ Â«ÐÐ°Ð½Ð´Ð°Ð½Ð°Â». ÐÐ´ÐµÑ Ð¿ÑÐ¾ÐµÐºÑÐ° - ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Â«ÐÐ°Ð½Ð´Ð°Ð½Ð°Â» Ð½Ð° ÑÑÐ½ÐºÐµ Ð³Ð¾ÑÐ¾Ð´Ð°, Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð¸ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð³ÐµÐ¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÐ¼ÑÑ ÑÑÐ»ÑÐ³ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ. ÐÐ¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»ÐµÐ¹.
Additional file 5 of Sex differences in impact of cumulative systolic blood pressure from childhood to adulthood on albuminuria in midlife: a 30-year prospective cohort study
Creators: name: Wang, Dan
name: Kou, Pu-qing
name: Liao, Yue-yuan
name: Wang, Ke-ke
name: Yan, Yu
name: Chen, Chen
name: Chu, Chao
name: Wang, Yang
name: Niu, Ze-Jiaxin
name: Ma, Qiong
name: Sun, Yue
name: Mu, Jian-jun
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Mental Health

description: Supplementary Material 5
È ORA per Steven Tingay
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2015

Un australiano alla guida di ORA, l’Osservatorio di Radioastronomia nato dalla fusione di due istituti dell’Istituto Nazionale di Astrofisica, l’Osservatorio Astronomico di Cagliari, dove opera il piùgrande radiotelescopio d'Europa con superficie attiva, il Sardinia Radio Telescope e l’Istituto di Radioastronomia di Bologna, con il radiotelescopio di Medicina e la Croce del Nord e il radiotelescopio di Noto
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð² ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸Ð½ÑÐµÑÑÐµÑÐ¾Ð²
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¾Ð½ÐµÐ², 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: 2018
Subjects: Ð¥ÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
ÐÐ¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹
Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð°Ñ ÑÐµÐ°Ð»ÑÐ½Ð¾ÑÑÑ
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð² ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸Ð½ÑÐµÑÑÐµÑÐ¾Ð². ÐÑÐ¾ÑÐµÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð·Ð°ÐºÐ»ÑÑÐ°Ð»ÑÑ Ð² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð´Ð¸Ð·Ð°Ð¹Ð½-Ð¿ÑÐ¾ÐµÐºÑÐ° Ð°Ð¿Ð°ÑÑÐ°Ð¼ÐµÐ½ÑÐ¾Ð², Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð»Ñ Ð´ÐµÐ¼Ð¾Ð½ÑÑÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÐºÐ»Ð¸ÐµÐ½ÑÑ. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð²Ð¾Ð¿ÑÐ¾ÑÐ° Ð¿Ð¾ÐºÐ°Ð·Ð°Ð»Ð¾, ÑÑÐ¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° ÑÐµÐ³Ð¾Ð´Ð½ÑÑÐ½Ð¸Ð¹ Ð´ÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ Ð¸ Ð³Ð¾ÑÐ¾Ð²Ð¾ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ²Ð¾Ð¸Ñ Ð½ÐµÐ¿Ð¾ÑÑÐµÐ´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð´Ð°Ñ.
Scoperto il decimo “Tatooine”
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Sfruttando i dati raccolti dal telescopio spaziale Kepler, un gruppo di astronomi della San Diego State University ha scoperto Kepler-453 b: il decimo pianeta circumbinario, ovvero che orbita attorno a due stelle come Tatooine, il pianeta immaginario di Guerre Stellari. La scoperta dimostra che questo tipo di sistemi è meno raro di quanto pensassimo
Perseidi, la settimana dei desideri
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Non solo San Lorenzo: lo show delle meteore, iniziato a metà luglio, ci allieterà fino all’ultima settimana di agosto. Ma il picco è in questi giorni, e in particolare nella notte fra il 12 e il 13. Meteo permettendo, grazie alla luna nuova si preannuncia uno spettacolo imperdibile
Là dove nascono le meteoriti
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Aspettando la notte di San Lorenzo, uno studio appena pubblicato dai ricercatori del Planetary Science Institute di Tucson getta nuova luce sull’origine delle meteoriti ordinarie. Le condriti H non arriverebbero tutte dalla fascia principale degli asteroidi, ma anche da regioni esterne
Indian housing and welfare : a study of the housing conditions and welfare needs of the Mission Reserve Indians
Creators: name: Toren, Cyril Kirby
Publisher: name: University of British Columbia
Year: 2012

description: The survey arose out of the interest of the Indian Affairs Branch in present and future housing needs of the Squamish Band. The information gathered was to be used for the purpose of planning an adequate housing scheme and for the development of a modern community. The plan of the study was to present some historical background of the Squamish people, to show through the survey of the reserve, the need for better housing, and the rehabilitation possibilities of the people through the development of a modern community project on the Capilano Reserve. Implicit in the study of housing needs were the welfare needs of the people. Two surveys were made, and two schedules were involved in the gathering of the material. The method used was that of visiting the homes and families on the reserve, and having the questionnaires completed. There was thus a day to day visit to the reserves, and a continuous contact with the people over a considerable period of time. Although almost all homes on the reserve were visited, the information used in the tables was based on a random selection of twenty-seven homes. The study revealed in its broad outline that the second-class status of the Indian people has resulted in second-class living conditions. Housing conditions are sub-marginal and overcrowding is general in almost every instance. The welfare program lacks coordination and is inadequate to the needs of the families. Breakdown of family life is general. It appeared obvious that only a comprehensive program meeting the social and psychological needs of the people could adequately solve the many inter-related problems of the Squamish people. In addition it seemed clear that no program could really succeed unless the people themselves were intimately involved in its development.
Optical Sum Rule anomalies in the High-Tc Cuprates
Creators: name: Marsiglio, F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We provide a brief summary of the observed sum rule anomalies in the high-T$_c$ cuprate materials. A recent issue has been the impact of a non-infinite frequency cutoff in the experiment. In the normal state, the observed anomalously high temperature dependence can be explained as a `cutoff effect'. The anomalous rise in the optical spectral weight below the superconducting transition, however, remains as a solid experimental observation, even with the use of a cutoff frequency.
description: 4 pages, 2 figures, very brief review of optical sum rule anomaly
title: ÐÐ¾Ð´Ð¸ÑÐ¸Ð°ÑÐ¸Ñ ÑÑÑÑÐºÑÑÑÑ Ð°Ð»Ð¼Ð°Ð·Ð¾Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÑ ÑÐ³Ð»ÐµÑÐ¾Ð´Ð½ÑÑ Ð¿Ð»ÐµÐ½Ð¾Ðº Ð¸Ð¾Ð½Ð½ÑÐ¼ Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸ÐµÐ¼
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ÐµÐµÐ²Ð°, ÐÐ»Ð¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¼Ð½Ð¾Ð³Ð¾Ð²Ð¾Ð»Ð½Ð¾Ð²Ð°Ñ ÑÐ°Ð¼Ð°Ð½Ð¾Ð²ÑÐºÐ°Ñ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ñ
Ð¸Ð¾Ð½Ð½Ð¾Ðµ Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ðµ
Ð°Ð»Ð¼Ð°Ð·Ð¾Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÐµ Ð¿Ð»ÐµÐ½ÐºÐ¸
Ð¼Ð°Ð³Ð½ÐµÑÑÐ¾Ð½Ð½Ð¾Ðµ ÑÐ°ÑÐ¿ÑÐ»ÐµÐ½Ð¸Ðµ
Ð¿Ð»Ð°Ð·Ð¼Ð¾Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾ÑÐ°Ð¶Ð´ÐµÐ½Ð¸Ðµ

description: ÐÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð¼ÐµÑÐ¾Ð´Ð° ÑÐ°Ð¼Ð°Ð½Ð¾Ð²ÑÐºÐ¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐ¾Ð½ÐºÐ¸Ñ Ð°Ð»Ð¼Ð°Ð·Ð¾Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÑ ÑÐ³Ð»ÐµÑÐ¾Ð´Ð½ÑÑ Ð¿Ð»ÐµÐ½Ð¾Ðº Ð¿ÑÐ¸ Ð¸Ñ Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ð¸ ÑÑÐºÐ¾ÑÐµÐ½Ð½ÑÐ¼Ð¸ Ð¸Ð¾Ð½Ð°Ð¼Ð¸ ÑÐ¾ÑÑÐ¾ÑÐ°. ÐÐ¾Ð»ÑÑÐµÐ½ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ Ð±Ð¾Ð»ÑÑÐ¾Ð¹ Ð¾Ð±ÑÐµÐ¼ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð² ÑÐ¸ÑÐ¾ÐºÐ¾Ð¼ Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ðµ Ð´Ð¾Ð· Ð¸Ð¾Ð½Ð¾Ð² Ð¸ Ð´Ð»Ð¸Ð½ Ð²Ð¾Ð»Ð½ ÑÐ°Ð¼Ð°Ð½Ð¾Ð²ÑÐºÐ¾Ð³Ð¾ Ð²Ð¾Ð·Ð±ÑÐ¶Ð´ÐµÐ½Ð¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐµÐ¹ Ð¼Ð¾Ð¶Ð½Ð¾ ÑÐºÐ°Ð·Ð°ÑÑ, ÑÑÐ¾ Ð² Ð°Ð»Ð¼Ð°Ð·Ð¾Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÑ Ð¿Ð»ÐµÐ½ÐºÐ°Ñ, Ð²ÑÑÐ°ÑÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ PECVD Ð¸ÑÑÐ¾Ð´Ð½Ð¾ Ð¿ÑÐ¸ÑÑÑÑÑÐ²ÑÐµÑ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð°ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÐºÐ¾Ð»ÐµÑ. Ð¡ ÑÐ¾ÑÑÐ¾Ð¼ Ð´Ð¾Ð· Ð¸Ð¾Ð½Ð¾Ð² ÐºÐ¾Ð»ÑÑÐ° ÑÐ°Ð·ÑÑÑÐ°ÑÑÑÑ Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÑÑÑ ÑÐ°Ð·ÑÐ¿Ð¾ÑÑÐ´Ð¾ÑÐµÐ½Ð½ÑÑ ÑÐµÑÐºÑ ÑÐ³Ð»ÐµÑÐ¾Ð´Ð½ÑÑ ÑÐµÐ¿Ð¾ÑÐµÐº. ÐÐ¸Ð½ÐµÑÐ¸ÐºÐ° Ð¿ÐµÑÐµÑÑÑÐ¾Ð¹ÐºÐ¸ ÑÑÑÑÐºÑÑÑÑ Ð¿Ð»ÐµÐ½ÐºÐ¸ Ð¿ÑÐ¸ ÐµÐµ Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ð¸ ÑÐ¾Ð²Ð¿Ð°Ð´Ð°ÐµÑ Ñ ÑÐ°Ð½ÐµÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð½ÑÐ¼ ÑÐ¾Ð´Ð¾Ð¼ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ð¹, ÐºÐ¸Ð½ÐµÑÐ¸ÐºÐ¾Ð¹ ÑÐ²ÐµÐ»Ð»Ð¸Ð½Ð³Ð° Ð¿Ð»ÐµÐ½Ð¾Ðº Ð¸ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð°Ð±ÑÐ¾Ð»ÑÑÐ½ÑÑ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ð¹ ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ sp3 Ð¸ sp2 ÑÐ²ÑÐ·ÐµÐ¹.
title: ÐÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¡Ð¨Ð Ð¸ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÑÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸ (Ð¢Ð°Ð¹Ð²Ð°Ð½Ñ)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ°ÑÐ°ÑÐ°Ð½Ð¾Ð²Ð°, Ð¡ÑÑÑÐ³Ð¼Ð°
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¸Ð¿Ð»Ð¾Ð¼Ð°ÑÐ¸Ñ
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ÐÐ¸ÑÐ°Ð¹ÑÐºÐ°Ñ ÑÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ°
ÐÐµÑÐ²Ð°Ñ Ð¼Ð¸ÑÐ¾Ð²Ð°Ñ Ð²Ð¾Ð¹Ð½Ð°
Ð¯Ð¿Ð¾Ð½Ð¸Ñ
Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ
ÐÑÐ¾ÑÐ°Ñ Ð¼Ð¸ÑÐ¾Ð²Ð°Ñ Ð²Ð¾Ð¹Ð½Ð°
diplomacy
USA
Republic of China
the First world war
Japan
international relations
the Second world war

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸ÑÐ¼ Ð¡Ð¨Ð Ð¸ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÑÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐµ Ð² XX Ð²ÐµÐºÐµ. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¡Ð¨Ð Ð¸ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÑÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐµ: ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹, ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, ÑÑÑÐµÑÑÐ²Ð¾Ð²Ð°Ð²ÑÐ¸Ðµ Ð¼ÐµÐ¶Ð´Ñ Ð¡Ð¨Ð Ð¸ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÑÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸ Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ 1937-1949, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¿ÑÑÐ¸ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð°. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¡Ð¨Ð Ð¸ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÑÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸, ÑÐ¾ Ð²ÑÐµÐ¼ÐµÐ½ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÐÐ¾Ð¼Ð¸Ð½ÑÐ´Ð°Ð½Ð° Ð¸ ÐÐÐ, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¼Ð¾Ð¼ÐµÐ½ÑÑ, Ð² ÐºÐ¾ÑÐ¾ÑÑÑ Ð¿ÑÐ¾ÑÐ²Ð»ÑÐ»Ð¾ÑÑ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¡Ð¨Ð Ð½Ð° Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÑ ÐÐ¾Ð¼Ð¸Ð½ÑÐ´Ð°Ð½Ð°. ÐÐ·ÑÑÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð´Ð²ÑÑ ÑÑÑÐ°Ð½.
description: This work is dedicated to the US relationship and the Republic of China in the XX century. The paper discusses the relationship between the United States and the Republic of China: the development of relations, the state at the present stage.The problems that existed between the United States and the Republic of China in the period 1937-1949, as well as possible ways of cooperation. Analyzed the relations between the US and the Republic of China, from the time of the confrontation of the KMT and the CPC, studied the moments in which US influence was manifested in the policies of the Kuomintang. Studied modern relations between the two countries.
CP asymmetry in the decays B --> (X_s, X_d) mu+ mu- with four generations
Creators: name: Alok, Ashutosh Kumar
name: Dighe, Amol
name: Ray, Shamayita
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We estimate the CP asymmetry A_{CP}(q^2) in the decays B --> X_s mu+ mu- and B --> X_d mu+ mu- in the standard model (SM) with an additional fourth generation. We use a parametrization that allows us to explore the complete parameter space of the 4X4 quark mixing matrix, and constrain these parameters from the current data on B decays. We find that the enhancement in A_{CP}(q^2) depends strongly on the mass of the t', the up-type quark in the fourth generation. For m_t' around 400 GeV, the CP asymmetry in the high-q^2 region (q^2 > 14.4 GeV^2) can be enhanced by more than an order of magnitude for B --> X_s mu+ mu- and up to a factor of 6 for B --> X_d mu+ mu-. There is no enhancement in the low-q^2 region (1< q^2 <6 GeV^2). With increasing m_t', the A_{CP}(q^2) in the high-q^2 (low-q^2) region first decreases (increases) and then saturates at a value a few times the SM prediction. In the high-q^2 region of B --> X_s mu+ mu-, this saturation value may be up to 25 times the SM expectation.
description: 22 pages, 4 figures; corrected typos, added references