cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐÐµÐ»Ð¾Ð³Ð¾ Ð·Ð°Ð»Ð° Ð¤ÐÐÐÐ£ÐÐ Â«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¸ÐºÐ¾Ð³Ð¾Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ°Ð²ÑÐµÐ½ÐºÐ¾, ÐÑÐ±Ð¾Ð²Ñ
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ÐµÐ³Ð¼ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐµÐ½Ð¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·

description: ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ ÑÑÐ½Ð¾Ðº, Ð½Ð° ÐºÐ¾ÑÐ¾ÑÐ¾Ð¼ Ð½Ð°ÑÐ¾Ð´Ð¸ÑÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐµÐ³Ð¼ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÐµÐ¹, Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¾ÑÐ½Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ ÑÐµÐ³Ð¼ÐµÐ½ÑÐ°, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÑÑÐ»ÑÐ³. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð°, Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾ Ð¾ÑÐºÑÑÑÐ¸Ñ ÑÐ¸Ð»Ð¸Ð°Ð»Ð° ÐºÐ¾Ð½ÑÐµÑÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÐ¸ Ð¿Ð¾ ÑÑÐµÐ¼ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ°Ð¼. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½ÑÑ, Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð·Ð°ÑÑÐ°Ñ Ð¿ÑÐ¾ÐµÐºÑÐ°. ÐÑÐ±ÑÐ°Ð½ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ.
title: Ð¡Ð¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð² Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¹
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¤Ð¸Ð»Ð¸Ð¿Ð¾Ð²ÑÐºÐ¸Ð¹, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸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Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¤ÐÐÐ¡ ÐÐ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 27.03.04 Â«Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÂ» (ÑÑÐ¾Ð²ÐµÐ½Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ°). Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð±Ð°Ð·Ð¾Ð²ÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð³Ð¾ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ° ÑÐµÐ¾ÑÐ¸Ð¸ - Ð¼ÐµÑÐ¾Ð´Ð° Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð° ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¹. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ ÑÐ¾ÑÐ¼Ñ Ð²ÐµÐºÑÐ¾ÑÐ½Ð¾-Ð¼Ð°ÑÑÐ¸ÑÐ½Ð¾Ð¹ Ð·Ð°Ð¿Ð¸ÑÐ¸ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼, Ð²ÐºÐ»ÑÑÐ°Ñ ÑÐ¾ÑÐ¼Ñ ÐÐ¾ÑÐ¸ Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð² Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¹, Ñ Ð¿ÐµÑÐµÑÐ¾Ð´Ð¾Ð¼ Ð¾Ñ Ð¾Ð´Ð½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ðº Ð´ÑÑÐ³Ð¾Ð¹. ÐÐ·Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ ÑÐ¸Ð½ÑÐµÐ·Ð° Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ Ð¸ Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ. Ð ÑÐ´ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¸Ð½ÑÐµÐ·Ð° Ð¿ÑÐ¾Ð¸Ð»Ð»ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ð¼Ð¸. ÐÐ°ÑÑÐ¾ÑÑÐµÐµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÐÑÑÑÐµÐ¹ Ð¨ÐºÐ¾Ð»Ñ ÐÐ¸Ð±ÐµÑÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¸ Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ (Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Â«Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÂ») Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ²Ð¾ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ° Â«Ð¡Ð¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÂ».
Investigating the Far-IR/Radio Correlation of Star Forming Galaxies to z=3
Creators: name: Seymour, N.
name: Huynh, M.
name: Dwelly, T.
name: Symeonidis, M.
name: Hopkins, A.
name: McHardy, I. M.
name: Page, M.
name: Rieke, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In order to examine the far-IR/radio correlation at high redshift we have studied the Spitzer 70um/far-infrared (far-IR) properties of sub-mJy radio sources from the 13^H XMM-Newton/Chandra Deep Field by redshift and galaxy type: active galactic nucleus (AGN) or star forming galaxy (SFG). We directly detect 70um counterparts (at >3sigma significance) for 22.5% (92/408) of the radio sources, while for the rest we perform stacking analysis by redshift and galaxy type. For the sources detected at 70um we find that the median and scatter of the observed flux density ratio, q70, are similar to previous results in the literature, but with a slight decrease in q70 towards higher redshifts. Of the radio sources detected at 70um 8/92 were already classified as AGN, but two of which maybe SFGs. For the stacked sources we obtain a detection for the SFGs at every redshift bin which implies they have mean flux densities a factor ~5 below the original 70um detection limit. For the stacked AGN we obtain a detection only in our highest redshift bin (1
description: 10 pages, 4 figures, accepted for publication in MNRAS
title: ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ ÑÐµÐ¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑ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ÐµÑÐ¼Ð¸Ð½Ð¾Ð²Ð°, ÐÐ¸ÐºÑÐ¾Ñ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Ð¸ÑÐµÐ²ÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
ÑÐµÐ¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÑ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð¾ÑÐ½Ð°ÑÐµÐ½Ð½Ð¾ÑÑÑ
ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÑÐ¾Ð²ÐµÐ½Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐµÐ¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ. ÐÐ·ÑÑÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº ÐµÐ³Ð¾ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð²ÑÐµÑÑÐ¾ÑÐ¾Ð½Ð½Ð¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾, ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ Ð¾ÑÐ½Ð°ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³Ð°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð» Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ°.
Additional file 1 of Ultrasensitive and colorimetric small extracellular vesicles (sEVs) analysis via dual-cycle signal tool
Creators: name: Ning, Linhong
name: Zhou, Yuan
name: Xie, Yang
name: Duan, Zhixiong
name: Yu, Feng
name: Cheng, Heng
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Developmental Biology
subject: Cancer
subject: Virology
subject: Computational Biology

description: Additional file 1. Table S1. Details of the sequences used in this research, Supporting information. Table S2. Comparison of the established approach with former ones.
Clouds, solar irradiance and mean surface temperature over the last century
Creators: name: Erlykin, A. D.
name: Sloan, T.
name: Wolfendale, A. W.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Geophysics (physics.geo-ph)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The inter-relation of clouds, solar irradiance and surface temperature is complex and subject to different interpretations. Here, we continue our recent work, which related mainly to the period from 1960 to the present, back to 1900 with further, but less detailed, analysis of the last 1000 years. The last 20 years is examined especially. Attention is given to the mean surface temperature, solar irradiance correlation, which appears to be present (with decadal smoothing) with a 22-year period; it is stronger than the 11-year cycle correlation with one year resolution. UV in the solar radiation is a likely cause. Cloud data are taken from synoptic observations back to 1952 and, again, there appears to be a correlation - with opposite phase for high and low clouds - at the 20-30y level. Particular attention is devoted to answering the question, 'what fraction of the observed increase in mean Global temperature (~0.7^oC) can be attributed to solar, as distinct from man-made, effects?' We conclude that a best estimate is 'essentially' all from 1900 to 1956 and <14% from 1956 to the present.
description: 10 pages, 6 figures, accepted by Journal of Atmospheric and Solar-Terrestrial Physics
title: ÐÐ½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¾ÑÑÐ° ÑÑÑÐ°Ð½ ÐÐ ÐÐÐ¡
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð½Ð¾Ð², ÐÐ¸ÐºÐ¸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: 2017
Subjects: ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ
Ð¸Ð½Ð´ÐµÐºÑ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð¾Ð¹ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸
Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐµÐ¹
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ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ¾ÑÑ

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - ÑÑÑÐ°Ð½Ñ ÐÐ ÐÐÐ¡. Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¾ÑÑÐ° ÑÑÑÐ°Ð½ ÐÐ ÐÐÐ¡. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ°Ð½ ÐÐ ÐÐÐ¡, Ð¸Ð·ÑÑÐµÐ½Ñ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð¿Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÑÑÐ°Ð½ Ð¸ Ð¾Ð±ÑÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ Ð² ÑÐµÐ»Ð¾Ð¼, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸Ð½Ð´ÐµÐºÑÐ° Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð¾Ð¹ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¹ ÑÑÑÐ°Ð½ Ð² ÑÐµÐ¹ÑÐ¸Ð½Ð³Ðµ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð¾Ð¹ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸, Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐµÐ¹ÑÑ Ð² ÐµÐ¶ÐµÐ³Ð¾Ð´Ð½Ð¾Ð¼ Ð¾ÑÑÐµÑÐµ ÐÑÐµÐ¼Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¤Ð¾ÑÑÐ¼Ð°. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ ÑÐ»ÑÑÑÐ¸ÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸, ÑÑÐ¾ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¹ Ð½Ð° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð°ÑÐµÐ½Ðµ.
Filling the disk hollow following binary black hole merger: The transient accretion afterglow
Creators: name: Shapiro, Stuart L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Tidal torques from a binary black hole (BHBH) empty out the central regions in any circumbinary gaseous accretion disk. The balance between tidal torques and viscosity maintain the inner edge of the disk at a radius r ~ 1.5a -- 2a, where a is the binary semimajor axis. Eventually, the inspiraling binary decouples from disk and merges, leaving behind a central hollow ("donut hole") in the disk orbiting the remnant black hole. We present a simple, time-dependent, Newtonian calculation that follows the secular (viscous) evolution of the disk as it fills up the hollow down to the black hole innermost stable circular orbit and then relaxes to stationary equilibrium. We use our model to calculate the electromagnetic radiation ("afterglow") spectrum emitted during this transient accretion epoch. Observing the temporal increase in the total electromagnetic flux and the hardening of the spectrum as the donut hole fills may help confirm a BHBH merger detected by a gravitational wave interferometer. We show how the very existence of the initial hollow can lead to super-Eddington accretion during this secular phase if the rate is not very far below Eddington prior to decoupling. Our model, though highly idealized, may be useful in establishing some of the key parameters, thermal emission features and scalings that characterize this transient. It can serve as a guide in the design and calibration of future radiation-magnetohydrodynamic simulations in general relativity.
description: 9 pages, 5 figures; submitted to PRD
Berry-like phases in structured atoms and molecules
Creators: name: Meyer, Edmund R.
name: Leanhardt, Aaron
name: Cornell, Eric
name: Bohn, John L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: FOS: Physical sciences

description: Quantum mechanical phases arising from a periodically varying Hamiltonian are considered. These phases are derived from the eigenvalues of a stationary, ``dressed'' Hamiltonian that is able to treat internal atomic or molecular structure in addition to the time variation. In the limit of an adiabatic time variation, the usual Berry phase is recovered. For more rapid variation, non-adiabatic corrections to the Berry phase are recovered in perturbation theory, and their explicit dependence on internal structure emerges. Simple demonstrations of this formalism are given, to particles containing interacting spins, and to molecules in electric fields.
description: 29 pages, 2 figures, submitted to PRA
SDSS J080434.20+510349.2: Eclipsing WZ Sge-Type Dwarf Nova with Multiple Rebrightenings
Creators: name: Kato, Taichi
name: Pavlenko, Elena P.
name: Maehara, Hiroyuki
name: Nakajima, Kazuhiro
name: Andreev, Maksim
name: Shugarov, Sergei Yu.
name: de Ponthiere, Pierre
name: Brady, Steve
name: Klingenberg, Geir
name: Shears, Jeremy
name: Imada, Akira
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We observed the 2006 superoutburst of SDSS J080434.20+510349.2 during its plateau phase, rebrightening phase, and post-superoutburst final decline. We found that this object is a grazing eclipsing system with a period of 0.0590048(2) d. Well-defined eclipses were only observed during the late stage of the superoutburst plateau and the depth decreased during the subsequent stages. We determined the superhump period during the superoutburst plateau to be 0.059539(11) d, giving a fractional superhump excess of 0.90(2)%. During the rebrightening and post-superoutburst phases, persisting superhumps with periods longer than those of superhumps during the plateau phase: 0.059632(6) during the rebrightening phase and 0.05969(4) d during the final fading. This phenomenon is very well in line with the previously known long-period "late superhumps" in GW Lib, V455 And and WZ Sge. The amplitudes of orbital humps between different states of rebrightenings suggest that these humps do not arise from the classical hot spot, but are more likely a result of projection effect in a high-inclination system. There was no clear evidence for the enhanced hot spot during the rebrightening phase. We also studied previously reported "mini-outbursts" in the quiescent state and found evidence that superhumps were transiently excited during these mini-outbursts. The presence of grazing eclipses and distinct multiple rebrightenings in SDSS J080434.20+510349.2 would provide a unique opportunity to understanding the mechanism of rebrightenings in WZ Sge-type dwarf novae.
description: 14 pages, 12 figures, PASJ accepted
The Most Metal-Poor Quadruple System of Subdwarfs G89-14
Creators: name: Rastegaev, D. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The system of subdwarfs G89-14 is one of the most metal-poor multiple stars with an atmospheric metal abundance $\mathrm{[m/H]}=-1.9$. Speckle interferometry at the 6-m BTA telescope has revealed that G89-14 consists of four components. Measurements of the magnitude difference between the components and published data have allowed their masses to be estimated: $M_{A}\approx0.67 M_{\odot}$, $M_{B}\approx0.24 M_{\odot}$, $M_{C}\approx0.33 M_{\odot}$, and $M_{D}\approx0.22 M_{\odot}$. The ratio of the orbital periods of the subsystems has been obtained, 0.52 yr : 3 000 yr : 650 000 yr (1:5769:1250000), indicative of a high degree of hierarchy of G89-14 and its internal dynamical stability. The calculated Galactic orbital elements and the low metallicity of the quadruple system suggest that it belongs to the Galactic halo.
description: 5 pages, 3 figures
title: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð´Ñ Ð¾Ð´Ñ Ðº Ð¾ÑÐµÐ½ÐºÐµ ÑÑÐ¾Ð²Ð½Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð²ÑÐ¸Ð»Ð¾Ð²Ð°, ÐÐ°Ð»ÐµÐ½Ñ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: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÑ
Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð±ÐµÐ·Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÑ
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð»Ð¸ÑÐ½ÑÐ¼ Ð±ÑÐ´Ð¶ÐµÑÐ¾Ð¼
Ð»Ð¸ÑÐ½ÑÐ¹ Ð±ÑÐ´Ð¶ÐµÑ

description: Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ.
Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¹ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ Ð±Ð°Ð·Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ.
ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾Ð±ÑÑÑÐ½ÑÑÑ Ð½Ð¸Ð·ÐºÐ¸Ð¹ ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð Ð¤.
Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÐ¾Ð²Ð½Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð².
Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑ Ð´Ð°ÑÑ ÑÐ¾Ð»ÑÐ¾Ðº Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð¸ Ð¸ Ð¿Ð¾Ð¼Ð¾Ð¶ÐµÑ Ð¸Ð¼ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑ ÑÐ²Ð¾Ð¸Ð¼Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ°Ð¼Ð¸.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑ Ð°ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° ÑÑÐ°Ð½Ð³Ð¾Ð²Ð¾Ð³Ð¾ Ð½Ð°ÑÐ¾Ñ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Ð½Ð´ÑÐ¾Ð½Ð¾Ð², 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: 2018
Subjects: ÐÐµÑ Ð°ÑÑÐ¾Ð½Ð¸ÐºÐ°
ÐÑÐ¸Ð²Ð¾Ð´Ñ
ÐÐ°ÑÐ¾ÑÑ Ð³Ð»ÑÐ±Ð¸Ð½Ð½ÑÐµ
Ð­Ð»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ

description: ÐÑ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° Â«ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ°ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° ÑÑÐ°Ð½Ð³Ð¾Ð²Ð¾Ð³Ð¾ Ð½Ð°ÑÐ¾ÑÐ°Â» Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¾Ð² Ñ ÑÐ°Ð·Ð½ÑÐ¼Ð¸ Ð·Ð°ÐºÐ¾Ð½Ð°Ð¼Ð¸ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð¾Ð±ÑÐ°Ð·ÑÐ¾Ð² Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ñ ÑÐµÐ»ÑÑ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¾Ð¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð¸Ñ Ð¼Ð°ÑÐ¸Ð½ Ð¸ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¸Ñ ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸.
Homology of free quantum groups
Creators: name: Collins, B.
name: Härtel, J.
name: Thom, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Operator Algebras (math.OA)
subject: Quantum Algebra (math.QA)
subject: FOS: Mathematics
subject: 16W35, 58B32, 16E40, 46L54

description: We compute the Hochschild homology of the free orthogonal quantum group $A_o(n)$. We show that it satisfies Poincaré duality and should be considered to be a 3-dimensional object. We then use recent results of R. Vergnioux to derive results about the $\ell^2$-homology of $A_o(n)$ and estimates on the free entropy dimension of its set of generators. In particular, we show that the $\ell^2$ Betti-numbers of $A_o(n)$ all vanish and that the free entropy dimension is less than 1.
description: 8 pages
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°ÑÑÐµÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð·Ð°ÑÐºÐ¾ÑÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð²ÑÑÐ¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÐµÐ½ÐºÐ¾, ÐÐ¸Ð°Ð¼Ð°Ñ
Publisher: name: [ÐÐÐ]
Year: 1977
Subjects: Ð¯ÐºÐ¾ÑÐ½ÑÐµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¸Ð·Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ñ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÑÐµÑÐ¾Ð² ÑÐ¸ÑÑÐµÐ¼ Ð·Ð°ÑÐºÐ¾ÑÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð²ÑÑÐ¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð², ÑÑÑÐ°Ð½Ð°Ð²Ð»Ð¸Ð²Ð°ÐµÐ¼ÑÑ Ð½Ð° Ð³Ð»ÑÐ±Ð¸Ð½Ð°Ñ Ð´Ð¾ 200-300 Ð¼. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¸Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐµÑÐ¾Ð² Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð­ÐÐ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð² ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð²ÑÐ·Ð¾Ð², Ð¸Ð¼ÐµÑÑÐ¸Ñ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ°Ð¼Ð¸-Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Ð¼Ð¸ Ð¿ÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ¸ÑÑÐµÐ¼ Ð·Ð°ÑÐºÐ¾ÑÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð²ÑÑÐ¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð², ÑÑÑÐ°Ð½Ð°Ð²Ð»Ð¸Ð²Ð°ÐµÐ¼ÑÑ Ð¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ¸ÑÑÐµÐ¼ÑÑ Ð² Ð±ÐµÑÐµÐ³Ð¾Ð²Ð¾Ð¹ Ð¸ ÑÐµÐ»ÑÑÐ¾Ð²Ð¾Ð¹ Ð·Ð¾Ð½Ð°Ñ Ð¼Ð¾ÑÐµÐ¹ Ð¸ Ð¾ÐºÐµÐ°Ð½Ð¾Ð².
Psychosocial challenges in adolescents and young adults affected by cancer : a systematic review of qualitative research
Creators: name: Lee, Olivia Nicole
Publisher: name: University of British Columbia
Year: 2024

description: Background: Psychosocial challenges in adolescents and young adults (AYAs) affected by cancer encompass wide-ranging concerns, including emotional distress, impaired cognition, reduced self-concept, existential concerns, sexual and reproductive health issues, interruptions to education and/or employment, and strained relationships, which can have negative implications on quality of life. The prevalence of psychosocial challenges has been estimated to impact over 60% of AYAs affected by cancer. Yet, no synthesis of qualitative evidence describing psychosocial challenges from the perspectives of AYAs themselves has been conducted leaving important knowledge gaps. Further, healthcare providers (HCPs) have described lacking AYA- specific knowledge and skills to deliver age-tailored cancer care, possibly hindering their capacity to support this population. Objective: The primary objective of this systematic review was to appraise and synthesize qualitative evidence regarding the psychosocial challenges in AYAs affected by cancer. A secondary objective was to discuss implications for HCPs caring for this population. Methods: MEDLINE, CINAHL, and PsycINFO were searched for qualitative studies published between 2006 and July 13, 2023. Included studies reported on psychosocial challenges experienced by AYAs, diagnosed with any cancer, between the ages of 15 and 39. A meta- aggregative approach was utilized to synthesize data and report the findings. Findings: Forty-seven articles were included and 13 distinct psychosocial challenges were generated that were organized into 4 overarching themes: (1) physical, (2) psychological, (3) interpersonal, and (4) daily living challenges. Clinical implications for HCPs were discussed in 25 articles and synthesized into 4 thematic findings: (1) providing information; (2) shared decision-making; (3) connecting to resources; and (4) assessing and affirming. Conclusion: This systematic review of qualitative research extends extant literature, affording an integrated and nuanced understanding of the psychosocial challenges in AYAs affected by a cancer experience. The findings provide insights that HCPs may utilize to better address the psychosocial challenges of this unique population through age-tailored and effective care.
Direct measurement of the magnetic field effects on carrier mobilities and recombination in tri-(8-hydroxyquinoline)-aluminum based light-emitting diodes
Creators: name: Li, Feng
name: Xin, Linyuan
name: Liu, Shiyong
name: Hu, Bin
Publisher: name: arXiv
Year: 2010
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The magnetic field effects on the carrier mobilities and recombination in tri-(8-hydroxyquinoline)-aluminum (Alq3) based light-emitting diodes have been measured by the method of transient electroluminescence. It is confirmed that the magnetic field has no effect on the electron and hole mobilities in Alq3 layers and can decrease the electron-hole recombination coefficient. The results imply that the dominant mechanism for the magnetic field effects in Alq3 based light-emitting diodes is the interconversion between singlet e-h pairs and triplet e-h pairs modulated by the magnetic field when the driving voltage is larger than the onset voltage of the electroluminescence.
description: 14 pages, 4 figures,The revised version submitted to applied physics letters
Investigating the Potential of Blended Learning to Develop Critical Thinking Skills among Student Teachers in Saudi Arabia
Creators: name: Alharbi, Mona Muzil
Publisher: name: University of Leicester
Year: 2022
Subjects: Uncategorized

description: Developing critical thinking (CT) skills among student teachers while they at teacher preparation programmes is crucial in order to be better equipped for their future career and help in promoting their future students’ CT abilities. However, lack of CT skills remains a major problem at teacher preparation programmes in Saudi Arabia. This study made an attempt to address this issue by proposing a Blended Learning Model to promote critical thinking (CT) skills within the context of the academic subject area. The Model consisted of a variety of activities that distributed before, during and after sessions and designed based on Laurillard’s Conversational Framework.The aim of this study is to examine the effectiveness of the Blended Learning Model in developing CT skills. It also examines how student teachers perceived and engaged with this model by gathering their perceptions. For this purpose, this study employed a mixed-methods approach using case study research design. At first, pre-tests were applied to measure student teachers’ current ability in CT before the application of the Blended Learning Model. Thereafter, data from the focus group interviews was collected continuously during the course. The post-tests and perception questionnaires were then conducted at the end of the course. The study was conducted over 14 weeks with 33 student teachers at a Saudi university during the educational year 2017-18.The findings suggest that the Blended Learning Model is effective for developing CT skills. The findings also indicated positive perceptions toward the proposed Model and highlight its potentials in terms of learning and skills development. However, challenges associated with technology use, collaboration and workload were encountered by some learners which affected their perceptions. It is therefore recommended to take those challenges into consideration when using this model or designing a blended course using Laurillard’s Conversational Framework.
title: Ð ÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð²ÐµÐ½ÑÑÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð° Ð½Ð° ÑÑÐ½Ð¾Ðº ÑÐ°ÑÑÐ½ÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ¾Ð²
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ»ÐµÐ², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð²ÐµÐ½ÑÑÑÐ½ÑÐµ ÑÐ¾Ð½Ð´Ñ
ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ
ÑÐ°ÑÑÐ½ÑÐµ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÑ
ÐºÐ¾Ð½ÑÐµÐ½Ñ
Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÐºÐ»Ð°Ð¼Ð°
Ð±Ð»Ð¾Ð³Ð¸
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venture funds
advertising providing
private investors
content
internet advertisement
blogs
webinar

description: ÐÐ»Ð°Ð²Ð° 1. Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð²ÐµÐ½ÑÑÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð° Ð½Ð° ÑÑÐ½Ð¾Ðº ÑÐ°ÑÑÐ½ÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ¾Ð². ÐÐ»Ð°Ð²Ð° 2. ÐÐ½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²ÑÐ±Ð¾ÑÐ° Ð²ÐµÑÐ±Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° Ð´Ð»Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð²ÐµÐ½ÑÑÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð° Ð½Ð° ÑÑÐ½Ð¾Ðº ÑÐ°ÑÑÐ½ÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ¾Ð². ÐÐ»Ð°Ð²Ð° 3. Ð¡Ð¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐµÐ½ÑÐ° ÐºÐ°Ðº ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð²ÐµÐ½ÑÑÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð° Ð½Ð° ÑÑÐ½Ð¾Ðº ÑÐ°ÑÑÐ½ÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ¾Ð².
description: Chapter 1. Theoretical justification of creation of advertising providing of promotion of venture fund to the market of private investors. Chapter 2. Analytical justification of the choice of verbal tool for the promotion of venture fund to the market of private investors. Chapter 3. Maintenance of effective content as advertising providing of promotion of venture fund to the market of private investors.
title: The Impact of DOPO and TPP Flame Retardants on Flame Spread over the Surface of Cast PMMA Slabs
Creators: name: Trubachev, S.
name: Korobeinichev, O.
name: Gonchikzhapov, M.
name: Paletsky, A.
name: Shmakov, A.
name: Tereshchenko, A.
name: Karpov, A.
name: Hu, Y.
name: Wang, X.
name: Hu, W.
name: International Seminar On Fire And Explosion Hazards (9; 2019; Saint Petersburg, Russia)
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: 2019

description: The effect of flame retardants DOPO and TPP on combustion of PMMA and on its thermal
decomposition has been investigated. It was suggested that the presence of an oxidizer in the pyrolysis
zone affects the flame propagation rate in the case of PMMA-TPP and has no effect in the case of
PMMA-DOPO. With the addition of TPP and DOPO a reduction of the total heat flux from the flame to
the surface was detected. Before the flame front, diffusion of the oxidant takes place in the longitudinal
direction to the flame zone. local increase of the heat flux near the flame front in the case of PMMA-TPP
was found, as opposed to in PMMA without additives. From the data of the species concentrations in the
flame zone of a PMMA-TPP slab, the presence of oxygen at the flame front (up to 10%) was detected.
PMMA-TPP decomposes more rapidly than PMMA and PMMA-DOPO in the oxidizing medium. Farther
from the flame front, where there is no oxygen, addition of TPP does not affect the decomposition rate of
PMMA in an inert medium. The DOPO additive, in turn, affects the kinetics of thermal decomposition
and reduces the heat flux from the flame. An oxidant does not affect PMMA-DOPO decomposition.
Thus, it was concluded that the presence of oxygen near the pyrolysis surface affects the flame
propagation velocity in the case of PMMA-TPP and has no effect in the case of PMMA-DOPO.
Very high energy gamma-ray observations of the galaxy clusters Abell 496 and Abell 85 with H.E.S.S
Creators: name: Collaboration, H. E. S. S.
name: :
name: Aharonian, F.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Aims: The nearby galaxy clusters Abell 496 and Abell 85 are studied in the very high energy (VHE, E > 100 GeV) band to investigate VHE cosmic rays (CRs) in this class of objects which are the largest gravitationally bound systems in the Universe. Methods: H.E.S.S., an array of four Imaging Atmospheric Cherenkov Telescopes (IACT), is used to observe the targets in the range of VHE gamma rays. Results: No significant gamma-ray signal is found at the respective position of the two clusters with several different source size assumptions for each target. In particular, emission regions corresponding to the high density core, to the extension of the entire X-ray emission in these clusters, and to the very extended region where the accretion shock is expected, are investigated. Upper limits are derived for the gamma-ray flux at energies E>570 GeV for Abell 496 and E>460 GeV for Abell 85. Conclusions: From the non-detection in VHE gamma rays, upper limits on the total energy of hadronic CRs in the clusters are calculated. If the cosmic-ray energy density follows the large scale gas density profile, the limit on the fraction of energy in these non-thermal particles with respect to the total thermal energy of the intra-cluster medium (ICM) is 51% for Abell 496 and only 8% for Abell 85 due to its larger mass and higher gas density. These upper limits are compared with theoretical estimates. They predict about ~10% of the thermal energy of the ICM in non-thermal particles. The observations presented here can constrain these predictions especially for the case of the Abell 85 cluster.
description: 11 pages, 4 figures, accepted for publication in A&A
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ±ÑÑÐ° ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð³ÑÐµÐ±Ð½ÑÐºÐ¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ±ÑÑÐ°
ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ
Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐ¾Ð²Ð°ÑÐ½ÑÐµ Ð³ÑÑÐ¿Ð¿Ñ

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ â Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ±ÑÑÐ¾Ð¼ ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð½Ð° ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ±ÑÑÐ° ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾ â ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«Ð¡ÐÐÐ Ð¢ÐÐ¥Â». 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Ð°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ ÑÐ±ÑÑÐ° ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð½Ð° ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ Â«Ð¡ÐÐÐ Ð¢ÐÐ¥Â».
On the Relation between Hybrid and Pure Spinor String Theory
Creators: name: Gerigk, Sebastian
name: Kirsch, Ingo
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we revisit Berkovits' pure spinor formalism in lower dimensions. We are particularly interested in relating a six-dimensional pure spinor action previously constructed in the literature to other superstring formalisms. In order to gain some insight into six-dimensional pure spinors, we first derive their action by gauge-fixing the classical six-dimensional Green-Schwarz action. We then consider a hybrid pure spinor construction in which the spacetime symmetries of six of the ten dimensions are described in pure spinor variables, while the remaining four dimensions are parameterized in terms of RNS variables. We relate this pure spinor formalism to the Berkovits-Vafa-Witten hybrid formalism of string theory on R^6 x T^4.
description: 15 pages, 1 figure
Size of Orbital Ordering Domain Controlled by the Itinerancy of the 3d Electrons in a Manganite Thin Film
Creators: name: Wakabayashi, Y.
name: Sagayama, H.
name: Arima, T.
name: Nakamura, M.
name: Ogimoto, Y.
name: Kubo, Y.
name: Miyano, K.
name: Sawa, H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: An electronic effect on a macroscopic domain structure is found in a strongly correlated half-doped manganite film Nd$_{0.5}$Sr$_{0.5}$MnO3 grown on a (011) surface of SrTiO3. The sample has a high-temperature (HT) phase free from distortion above 180K and two low-temperature (LT) phases with a large shear-mode strain and a concomitant twin structure. One LT phase has a large itinerancy (A-type), and the other has a small itinerancy (CE-type), while the lattice distortions they cause are almost equal. Our x ray diffraction measurement shows that the domain size of the LT phase made by the HT-CE transition is much smaller than that by the HT-A transition, indicating that the difference in domain size is caused by the electronic states of the LT phases.
description: 9 pages, 4 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ¾Ð½ÑÐµÐ½Ñ-Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð´Ð»Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ ÐºÐ»Ð¸Ð½Ð¸ÐºÐ¸ Ð¿Ð»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ñ Ð¸ÑÑÑÐ³Ð¸Ð¸ ÐÐÐ Â«ÐÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÂ»
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð§ÐµÑÐ¸ÐºÑÐ¸ÐµÐ², Ð¡ÑÐ°Ð½Ð¸ÑÐ»Ð°Ð²
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: ÐºÐ¾Ð½ÑÐµÐ½Ñ-Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
Ð¿Ð»Ð°ÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ñ Ð¸ÑÑÑÐ³Ð¸Ñ
ÑÐµÐºÐ»Ð°Ð¼Ð°

description: Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÑÐ°Ð¿Ð¾Ð² Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÐµÐ½Ñ-Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð° Ð´Ð»Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ ÐºÐ»Ð¸Ð½Ð¸ÐºÐ¸ Ð¿Ð»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÑÐ³Ð¸Ð¸ ÐÐÐ Â«ÐÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÂ».
title: Ð¡Ð¾Ð·Ð´Ð°Ð½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ PR-Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð²: Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ¦ "ÐÐ°ÑÐ¼Ð¾Ð½Ð¸Ñ")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐ°Ð¹Ð»ÐµÑÐºÐ°Ñ, 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: PR-Ð¿ÑÐ¾ÐµÐºÑÑ
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ
Ð´ÐµÑÐ¸-ÑÐ¸ÑÐ¾ÑÑ
Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ¾ÑÐ¸Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð°ÐºÑÑÐ°Ð»Ð¸Ð·Ð¸ÑÑÐµÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð° ÑÐ¾ÑÐ¸Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð´ÐµÑÐµÐ¹-ÑÐ¸ÑÐ¾Ñ Ð¸ Ð´ÐµÑÐµÐ¹, Ð¾ÑÑÐ°Ð²ÑÐ¸ÑÑÑ Ð±ÐµÐ· Ð¿Ð¾Ð¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¾Ð´Ð¸ÑÐµÐ»ÐµÐ¹ Ð¸ Ð²Ð¾ÑÐ¿Ð¸ÑÑÐ²Ð°ÑÑÐ¸ÑÑÑ Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ. ÐÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÑÑÑ ÑÐ¿Ð¾ÑÐ¾Ð± ÑÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐµÑÐµÐ· ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ PR-Ð¿ÑÐ¾ÐµÐºÑÐ°. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¿ÑÐ¸Ð¼ÐµÑÐ° Ð´Ð°ÐµÑÑÑ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ PR-Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ 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ÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾. ÐÐ¾Ð´Ð²Ð¾Ð´ÑÑÑÑ Ð¿ÑÐ¾Ð¼ÐµÐ¶ÑÑÐ¾ÑÐ½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ PR-Ð¿ÑÐ¾ÐµÐºÑÐ°.
title: ÐÐ¾ÑÐµÐ½Ð¸Ðµ Ð¸ Ð²Ð·ÑÑÐ²
Creators: name: Ð¥ÑÐ°Ð¼Ð¾Ð², ÐÐµÐ½Ð½Ð°Ð´Ð¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2010
Subjects: ÐÐ¾ÑÐµÐ½Ð¸Ðµ
ÐÐ·ÑÑÐ²

description: Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¼ Ð²Ð¸Ð´Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð², Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð½ÑÑ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð¼ÐµÑÐ½Ð¾ÑÑÑÐ¼ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð³Ð¾ÑÐµÐ½Ð¸Ñ Ð¸ Ð²Ð·ÑÑÐ²Ð° Ð¸ Ð¾ÑÐµÐ½ÐºÐµ Ð¸Ñ Ð¿Ð¾ÑÐ°Ð¶Ð°ÑÑÐµÐ³Ð¾ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ. ÐÐ·Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ° ÑÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÐ°Ð¶Ð°ÑÑÐ¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð¸ Ð¾ÑÐ°Ð³Ð¾Ð² Ð¿Ð¾ÑÐ°Ð¶ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ Ð°Ð²Ð°ÑÐ¸ÑÑ Ð¸ ÐºÐ°ÑÐ°ÑÑÑÐ¾ÑÐ°Ñ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð¿Ð¾Ð¶Ð°ÑÐ°Ð¼Ð¸ Ð¸ Ð²Ð·ÑÑÐ²Ð°Ð¼Ð¸. ÐÐ¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð° Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð²ÑÐ·Ð¾Ð², Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð¢ÐµÐ¾ÑÐ¸Ñ Ð³Ð¾ÑÐµÐ½Ð¸Ñ Ð¸ Ð²Ð·ÑÑÐ²Ð°Â» Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«ÐÐ°ÑÐ¸ÑÐ° Ð² ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸ÑÑÂ», Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾Ð¹ Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð², ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸ÑÑ Ð² ÑÐµÑÐ½Ð¾Ð³ÐµÐ½Ð½Ð¾Ð¹ ÑÑÐµÑÐµ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð²ÑÐ±Ð¾ÑÐ° Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð´Ð»Ñ ÑÐ¸Ð¿Ð¾Ð²ÑÑ Ð¾Ð±ÑÐµÐ¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ð¾Ð²
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»ÐµÐºÑÐµÐµÐ²Ð°, ÐÐ²Ð³ÐµÐ½Ð¸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ÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ð¸ ÑÐ½ÐµÑÐ³Ð¸Ð¸
Ð­Ð»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ Ð°ÑÐ¸Ð½Ñ ÑÐ¾Ð½Ð½ÑÐµ
ÐÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ð¸ ÑÐ°ÑÑÐ¾ÑÑ
ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð¿Ð»Ð°Ð²Ð½Ð¾Ð³Ð¾ Ð¿ÑÑÐºÐ°

description: Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð°ÑÐ¸Ð½ÑÑÐ¾Ð½Ð½ÑÐ¼ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¾Ð¼, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð²ÑÐ±Ð¾ÑÐ° Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð´Ð»Ñ ÑÐ¸Ð¿Ð¾Ð²ÑÑ Ð¾Ð±ÑÐµÐ¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð², ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²ÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ñ ÑÐ´ÐµÐ»Ð°ÑÑ Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½ÑÐ¹ Ð²ÑÐ±Ð¾Ñ. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð¿Ð¾Ð»ÑÑÐµÐ½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ð¹ Ð²ÑÐ±ÑÐ°ÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ñ Ð½Ð°Ð¸Ð¼ÐµÐ½ÑÑÐ¸Ð¼Ð¸ Ð·Ð°ÑÑÐ°ÑÐ°Ð¼Ð¸. Ð ÑÐ»ÑÑÐ°Ðµ Ð½ÐµÐ¾Ð´Ð½Ð¾Ð·Ð½Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ Ð²ÑÐ±Ð¾ÑÐµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÑÑÑ Ð¿ÑÐ¾Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´ Ñ ÑÐµÐ»ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÐµÑÑ ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ°.
Badhamia melanospora Speg.
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Physarales
Physaraceae
Badhamia
Badhamia melanospora

description: B● Badhamia melanospora Speg.,
krumpainā dzelksnīte
- leg. L.Birziņa, 11 Nov 2021, Ādaži, 1 m high on a thin trunk of dead Acer negundo in the deciduous forest by the river, det. L.Birziņa & J.Kluša, 2022; (NMKK), very rare.
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«Ð ÑÑÐ°Ð³Â»
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¿ÑÑÑÐ¸Ð½, ÐÐ¼Ð¸ÑÑÐ¸Ð¹
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°Ð³Ð¾ÑÐ¾Ð²ÐºÐ°
ÑÐ°Ð·Ð¼ÐµÑÐ½Ð°Ñ Ð½Ð°Ð»Ð°Ð´ÐºÐ°
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
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Study 1: Replication of Poliseno et al., 2010 (Nature)
Creators: name: Errington, Timothy
name: Pandya, Kumar
name: Kerwin, John
name: Cowley, Dale
name: Khan, Israr
name: Iorns, Elizabeth
name: Tsui, Rachel
name: Denis, Alexandria
name: Perfito, Nicole
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Other Life Sciences
subject: Life Sciences
subject: Biochemistry, Biophysics, and Structural Biology
subject: Metascience
subject: Noncoding RNA
subject: Pseudogene
subject: PTEN
subject: Replication
subject: Reproducibility
subject: Reproducibility Project: Cancer Biology

description: This registration contains all of the methods, data, analysis scripts, figures, and manuscript files associated with the published results of this replication effort, which can be found here: https://doi.org/10.7554/eLife.51019
The Dark Matter Annihilation Signal from Dwarf Galaxies and Subhalos
Creators: name: Kuhlen, Michael
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Dark Matter annihilation holds great potential for directly probing the clumpiness of the Galactic halo that is one of the key predictions of the Cold Dark Matter paradigm of hierarchical structure formation. Here we review the gamma-ray signal arising from dark matter annihilation in the centers of Galactic subhalos. We consider both known Galactic dwarf satellite galaxies and dark clumps without a stellar component as potential sources. Utilizing the Via Lactea II numerical simulation, we estimate fluxes for 18 Galactic dwarf spheroidals with published central densities. The most promising source is Segue 1, followed by Ursa Major II, Ursa Minor, Draco, and Carina. We show that if any of the known Galactic satellites can be detected, then at least ten times more subhalos should be visible, with a significant fraction of them being dark clumps.
description: 13 pages, 5 figures, invited review/tutorial paper (including some new results), submitted to Advances in Astronomy for the special edition "Dwarf Galaxy Cosmology", v2: added several references