cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ¾Ð¼Ð°ÑÐ½Ð¾Ð¹ Ð¿Ð°ÑÑÑ, ÑÐµÐ°Ð»Ð¸Ð·ÑÐµÐ¼Ð¾Ð¹ Ð² ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ ÑÐµÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð³Ð¾ÑÐ½ÑÐº, ÐÐ»ÐµÐ½Ð°
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Ð¾Ð¼Ð°ÑÐ½Ð°Ñ Ð¿Ð°ÑÑÐ°
ÑÐ¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ Ñ Ð°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°
Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð°
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð¼Ð°ÑÐ½Ð°Ñ Ð¿Ð°ÑÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ ÐÐÐ Â«ÐÐ¼Ð¿ÐµÑÐ¸Ñ - ÐÐ¸Ð½Â». Ð¦ÐµÐ»ÑÑ 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¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð¾Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ¾Ð¼Ð°ÑÐ½Ð¾Ð¹ Ð¿Ð°ÑÑÑ. ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð´Ð²Ðµ Ð³Ð»Ð°Ð²Ñ. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ¾Ð¼Ð°ÑÐ½Ð¾Ð¹, Ð²Ð¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐ¼Ð¿ÐµÑÐ¸Ñ - ÐÐ¸Ð½Â». ÐÐ°Ð½Ð½Ð°Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð° ÐºÐ°Ðº ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¾Ð²Ð°ÑÐ¾Ð² ÑÐ¾Ð¼Ð°ÑÐ½Ð¾Ð¹ Ð¿Ð°ÑÑÑ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Â«ÐÐ¼Ð¿ÐµÑÐ¸Ñ - ÐÐ¸Ð½Â».
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¸ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»Â»)
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐµÐ³ÐºÐ¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹
ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸
ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹
Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð½ÐµÑÐ½ÐµÐ¹ Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¹ ÑÑÐµÐ´Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»Â». Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»Â» Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑ Ð¿Ð¾ ÐµÑ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð²ÑÑÑÑÐºÐ¸ Ð¸ Ð·Ð°ÑÑÐ°Ñ Ð¾Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹. ÐÑÐ±ÑÐ°Ð½ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÐ¹ Ð²Ð°ÑÐ¸Ð°Ð½Ñ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð´Ð»Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑ, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð»Ð¾ÑÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½ÑÑ ÐºÐ»Ð¸ÐµÐ½ÑÐ¾Ð², Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸.
A Comparison of Mental Health Outcomes in the United States and Italy at Different Levels of Cumulative COVID-19 Prevalence
Creators: name: Mancini, Anthony
name: Prati, Gabriele
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Social and Behavioral Sciences

description: This registration includes data, syntax, codebook, and item-level description of all measures used in the study.
title: ÐÑÐ¿ÑÑÐ°Ð½Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹ Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ Ð°Ð³ÑÐµÐ³Ð°ÑÐ¾Ð². ÐÑÐ¿ÑÑÐ°Ð½Ð¸Ñ ÑÐ¸Ð½Ñ ÑÐ¾Ð½Ð¸Ð·Ð°ÑÐ¾ÑÐ¾Ð²
title: Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ðº Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð²Ð°Ð»ÑÑÑÐº, Ð.
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 1999
Subjects: ÐÐ²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ð¸

description: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ âÐÑÐ¿ÑÑÐ°Ð½Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹ Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ Ð°Ð³ÑÐµÐ³Ð°ÑÐ¾Ð²â Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 551400 âÐÐ°Ð·ÐµÐ¼Ð½ÑÐµ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñâ. Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ðº Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ ÑÐ¸Ð½ÑÑÐ¾Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ñ ÑÑÐ¸Ð»Ð¸Ñ Ð²ÐºÐ»ÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½ÑÑÐ¾Ð½Ð¸Ð·Ð°ÑÐ¾ÑÐ¾Ð² Ð² ÐºÐ¾ÑÐ¾Ð±ÐºÐ°Ñ Ð¿ÐµÑÐµÐ´Ð°Ñ. ÐÐ»Ð°Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹ ÑÐ¸Ð½ÑÑÐ¾Ð½Ð¸Ð·Ð°ÑÐ¾ÑÐ¾Ð². ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ 150100 âÐÐ²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ðµ- Ð¸ ÑÑÐ°ÐºÑÐ¾ÑÐ¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµâ Ð¸ 150300 âÐÐ½Ð¾Ð³Ð¾ÑÐµÐ»ÐµÐ²ÑÐµ Ð³ÑÑÐµÐ½Ð¸ÑÐ½ÑÐµ Ð¸ ÐºÐ¾Ð»ÐµÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñâ Ð²ÑÐµÑ ÑÑÐ¾Ð²Ð½ÐµÐ¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸.
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 ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð·Ð°ÑÑÐ´Ð½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° STM 32
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐµÐ´Ð¸ÑÐ¸Ð½, 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: Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ðµ Ð·Ð°ÑÑÐ´Ð½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Qi
Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑ
Ð¿ÐµÑÐ°ÑÐ½Ð°Ñ Ð¿Ð»Ð°ÑÐ°

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð·Ð°ÑÑÐ´Ð½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð²ÑÐ±ÑÐ°Ð½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¸Ð°Ð»ÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° Ð¸ Ð¿ÐµÑÐ°ÑÐ½Ð°Ñ Ð¿Ð»Ð°ÑÐ° Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°. Ð¢Ð°ÐºÐ¶Ðµ Ð²Ð¾ Ð²ÑÐµÐ¼Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ Ð¼Ð¾Ð½ÑÐ°Ð¶ Ð¸ ÑÐ±Ð¾ÑÐºÐ° Ð¿Ð»Ð°ÑÑ.
Tuning Fermilab Heavy Quarks in 2+1 Flavor Lattice QCD with Application to Hyperfine Splittings
Creators: name: Bernard, C.
name: DeTar, C.
name: Di Pierro, M.
name: El-Khadra, A. X.
name: Evans, R. T.
name: Freeland, E. D.
name: Gámiz, E.
name: Gottlieb, Steven
name: Heller, U. M.
name: Hetrick, J. E.
name: Kronfeld, A. S.
name: Laiho, J.
name: Levkova, L.
name: Mackenzie, P. B.
name: Simone, J. N.
name: Sugar, R.
name: Toussaint, D.
name: Van de Water, R. S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We report the non-perturbative tuning of parameters--- kappa_c, kappa_b, and kappa_crit ---that determine the heavy-quark mass in the Fermilab action. This requires the computation of the masses of Ds^(*) and Bs^(*) mesons comprised of a Fermilab heavy quark and a staggered light quark. Additionally, we report the hyperfine splittings for Ds and Bs mesons as a cross-check of our simulation and analysis methods. We find a splitting of 145 +/- 15 MeV for the Ds system and 40 +/- 9 MeV for the Bs system. These are in good agreement with the Particle Data Group average values of 143.9 +/- 0.4 MeV and 46.1 +/- 1.5 MeV, respectively. The calculations are carried out with the MILC 2+1 flavor gauge configurations at three lattice spacings $a$ approximately 0.15, 0.12, and 0.09 fm.
description: 34 pages, 8 figures, 26 tables; some sections rearranged for clarity; conclusions unchanged; version accepted by Phys. Rev.D
Experimental EPR-Steering of Bell-local States
Creators: name: Saunders, D. J.
name: Jones, S. J.
name: Wiseman, H. M.
name: Pryde, G. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Entanglement is the defining feature of quantum mechanics, and understanding the phenomenon is essential at the foundational level and for future progress in quantum technology. The concept of steering was introduced in 1935 by Schrödinger as a generalization of the Einstein-Podolsky-Rosen (EPR) paradox. Surprisingly, it has only recently been formalized as a quantum information task with arbitrary bipartite states and measurements, for which the existence of entanglement is necessary but not sufficient. Previous experiments in this area have been restricted to the approach of Reid [PRA 40, 913], which followed the original EPR argument in considering only two different measurement settings per side. Here we implement more than two settings so as to be able to demonstrate experimentally, for the first time, that EPR-steering occurs for mixed entangled states that are Bell-local (that is, which cannot possibly demonstrate Bell-nonlocality). Unlike the case of Bell inequalities, increasing the number of measurement settings beyond two--we use up to six--dramatically increases the robustness of the EPR-steering phenomenon to noise.
description: 5pages, 5figures, letter
title: Ð¢ÐµÑ Ð½Ð¾ÑÑÐµÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ. ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¤Ð°ÑÑÑÐ¾Ð², 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: ÐÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°
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description: ÐÐ»Ð°Ð²Ð½Ð°Ñ Ð·Ð°Ð´Ð°ÑÐ° Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ â Ð¿Ð¾Ð¼Ð¾ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð² Ð¾ÑÐ²Ð¾ÐµÐ½Ð¸Ð¸ Ð½Ð¾Ð²ÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð² Ð±ÑÐ´ÑÑÐµÐ¼ Ð±ÑÐ´ÑÑ Ð¸Ð·ÑÑÐµÐ½Ñ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Â«Ð¢ÐµÑÐ½Ð¾ÑÑÐµÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÂ». ÐÐ¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð° Â«ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÂ» ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²ÑÐµÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¸ Ð¸Ð½ÑÐµÑÐµÑÐ° Ðº Ð¿Ð¾Ð»ÑÑÐ°ÐµÐ¼Ð¾Ð¹ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¸. ÐÐ¾ÑÐ»Ðµ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÐºÑÑÑÐ°, ÑÑÑÐ´ÐµÐ½Ñ Ð±ÑÐ´ÐµÑ Ð·Ð½Ð°ÑÑ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÑ Ð±ÑÐ´ÑÑÐµÐ¹ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¸ Ð¸ Ð±ÑÐ´ÐµÑ Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½Ð¾ Ð½Ð°ÑÑÑÐ¾ÐµÐ½ Ðº Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¾Ð¿ÑÑÐ° Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐµÑÐµ.
Near-equilibrium measurements of nonequilibrium free energy
Creators: name: Sivak, David A.
name: Crooks, Gavin E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: A central endeavor of thermodynamics is the measurement of free energy changes. Regrettably, although we can measure the free energy of a system in thermodynamic equilibrium, typically all we can say about the free energy of a non-equilibrium ensemble is that it is larger than that of the same system at equilibrium. Herein, we derive a formally exact expression for the probability distribution of a driven system, which involves path ensemble averages of the work over trajectories of the time-reversed system. From this we find a simple near-equilibrium approximation for the free energy in terms of an excess mean time-reversed work, which can be experimentally measured on real systems. With analysis and computer simulation, we demonstrate the accuracy of our approximations for several simple models.
description: 5 pages, 3 figures
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐÂ«ÐÐ¶Ð¸-ÐÐ¸-ÑÐ-Ð¢ÑÐ°Ð½Ð·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®Ð´Ð¸Ð½Ð°, ÐÑÐµÐ½Ð¸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: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
Ð°Ð½Ð°Ð»Ð¸Ð· Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð·Ð°Ð¿Ð°ÑÐ°Ð¼Ð¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ¶Ð¸-ÐÐ¸-ÑÐ-Ð¢ÑÐ°Ð½Ð·Ð¸ÑÂ».
Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹Ì ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹Ì ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑ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 ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ¶Ð¸-ÐÐ¸-ÑÐ-Ð¢ÑÐ°Ð½Ð·Ð¸ÑÂ»).
ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ ÑÐ°ÑÐºÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑÑ, Ð´Ð°Ð½Ð° ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° Ð²Ð½ÐµÑÐ½ÑÑ Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÑÑ ÑÑÐµÐ´Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð·Ð° 2014- 2017 Ð³Ð¾Ð´Ñ.
ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð² ÑÐµÐ»ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð±ÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð·Ð°Ð¿Ð°ÑÐ°Ð¼Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð´Ð¾Ð»Ð³Ð¾ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÐºÑÐµÐ´Ð¸ÑÐ°.
ÐÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÐ¼ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¾Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹: ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð¸Ðµ ÑÐµÐ±ÐµÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÐ¾Ð²Ð°ÑÐ°, Ð²Ð¾Ð·Ð²ÑÐ°ÑÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸.
Ion thermal effects in oscillating multi-ion plasma sheath theory
Creators: name: Vranjes, J.
name: Pandey, B. P.
name: Tanaka, M. Y.
name: Poedts, S.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The effects of ion temperature are discussed in a two-ion electron plasma and for a model applicable to the oscillating sheath theory that has recently been much in the focus of researchers. The differences between the fluid and kinetic models have been pointed out, as well as the differences between the approximative kinetic description (which involves the expansion of the plasma dispersion function), and the exact kinetic description. It is shown that the approximative kinetic description, first, can not describe the additional acoustic mode which naturally exists in the plasma with an additional ion population with a finite temperature, and, second, it yields an inaccurate Landau damping of the bulk ion acoustic mode. The reasons for these two failures are described. In addition to this, a fluid model is presented that is capable of capturing both of these features that are missing in the approximative kinetic description, i.e., two (fast and slow) ion acoustic modes, and the corresponding Landau damping of both modes.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¡Ð¨Ð Ð¿ÐµÑÐµÐ´Ð°ÑÑÐ¸ÐºÐ° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð´Ð¸Ð¾Ð´Ð° Ñ Ð½Ð°ÐºÐ¾Ð¿Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð·Ð°ÑÑÐ´Ð°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ³ÑÑÐµÑÐ½Ð¸ÐºÐ¾Ð²Ð°, Ð®Ð»Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ¸Ð¾Ð´Ñ Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²ÑÐµ
ÐÐµÐ½ÐµÑÐ°ÑÐ¾ÑÑ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½ÑÐµ

description: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¡Ð¨Ð Ð¿ÐµÑÐµÐ´Ð°ÑÑÐ¸ÐºÐ° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð´Ð¸Ð¾Ð´Ð° Ñ Ð½Ð°ÐºÐ¾Ð¿Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð·Ð°ÑÑÐ´Ð°. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¡Ð¨Ð ÑÐ¸Ð³Ð½Ð°Ð»Ð°, Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½Ð¾Ð¹ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¡Ð¨Ð Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ° Ð¸ ÑÑÐµÐ¼Ñ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ° Ñ Ð¿ÑÑÐ¼ÑÐ¼ Ð¸ Ð¾Ð±ÑÐ°ÑÐ½ÑÐ¼ Ð²ÐºÐ»ÑÑÐµÐ½Ð¸ÐµÐ¼ Ð´Ð¸Ð¾Ð´Ð°. ÐÐ°ÑÐµÐ¼ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°Ð»Ð¸ÑÑ ÑÑÐµÐ¼Ñ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ Ð¿ÐµÑÐµÐ´Ð°ÑÑÐ¸ÐºÐ¾Ð². ÐÐ°Ð»ÐµÐµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÑÐµÑ ÑÑÐµÐ¼ ÑÐµÐ°Ð»ÑÐ½Ð¾ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¿ÐµÑÐµÐ´Ð°ÑÑÐ¸ÐºÐ¾Ð². ÐÐ°ÑÐµÐ¼ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð»Ð°ÑÑ ÑÑÐµÐ¼Ð° Ð¡Ð¨Ð Ð¿ÐµÑÐµÐ´Ð°ÑÑÐ¸ÐºÐ° Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð° Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð½ÑÐ¼ ÐÐÐ Ð½Ð° ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ñ, Ð²ÑÑÑÐ¾ÐµÐ½Ð½ÑÑ Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ ÑÑÐµÐ´Ñ AWR. ÐÐ°Ð»ÐµÐµ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐ»ÑÑ Ð¸Ð¼Ð¿Ð¾ÑÑ ÑÐµÐ°Ð»ÑÐ½Ð¾ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð². ÐÐ¾ÑÐ»Ðµ Ð¸Ð¼Ð¿Ð¾ÑÑÐ° Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐ»Ð°ÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÐµÐ¼Ñ Ð¸ Ð¿Ð¾Ð´ÑÑÑÐ¾Ð¹ÐºÐ° Ð½Ð¾Ð¼Ð¸Ð½Ð°Ð»Ð¾Ð² ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ°ÐºÐ¸Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼, ÑÑÐ¾Ð±Ñ ÑÐ»ÑÑÑÐ¸ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÑÐµÐ¼Ñ. ÐÐ¼Ð¿Ð»Ð¸ÑÑÐ´Ð° Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ° ÑÐ¾ÑÑÐ°Ð²Ð¸Ð»Ð° Ð¾ÐºÐ¾Ð»Ð¾ 8.4Â Ð, ÑÐ¸ÑÐ¸Ð½Ð° Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ° Ð¾ÐºÐ°Ð·Ð°Ð»Ð°ÑÑ ÑÐ°Ð²Ð½Ð¾Ð¹ 4Â Ð½Ñ, ÑÐ°ÑÑÐ¾ÑÐ° Ð¿Ð¾Ð²ÑÐ¾ÑÐµÐ½Ð¸Ñ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ¾Ð² ÑÐ¾ÑÑÐ°Ð²Ð¸Ð»Ð° Ð¿ÑÐ¸Ð±Ð»Ð¸Ð·Ð¸ÑÐµÐ»ÑÐ½Ð¾ 0.5 ÐÐÑ.
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð²Ð¾Ð·Ð¾Ð±Ð½Ð¾Ð²Ð»ÑÐµÐ¼Ð¾Ð¹ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¨ÐºÐ»ÑÑÑÐº, ÐÐ°ÑÐ¸Ñ
name: ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: Ð­Ð½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°
ÐÐ¾Ð·Ð¾Ð±Ð½Ð¾Ð²Ð»ÑÐµÐ¼ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ ÑÐ½ÐµÑÐ³Ð¸Ð¸

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÂ» (ÑÐ°Ð·Ð´ÐµÐ» 2) Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ 080500 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ», Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸Â». Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÐÐÐ­, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼Ð¾Ð´ÑÐ»ÑÐ½Ð°Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ¸ÑÑÐµÐ¼ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÐÐÐ­. ÐÐ»Ð°Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ ÑÐ¸ÑÑÐµÐ¼Ð°Ð¼ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾Ð·Ð¾Ð±Ð½Ð¾Ð²Ð»ÑÐµÐ¼ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ Ð·Ð° ÑÑÐ±ÐµÐ¶Ð¾Ð¼. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 080502 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸Â» Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ° Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð¾ÑÐ½Ð¾-Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ.
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°.
Lo zoccolo duro di Andromeda
Creators: Daniela Cipolloni
Publisher: name: Media Inaf
Year: 2011

Per la prima volta un gruppo internazionale di astronomi ha osservato un disco spesso, molto antico, nella vicina Andromeda. Quasi impossibili osservazioni simili nella Via Lattea. Aiuterà a ricostruire le prime fasi della formazione delle galassie a spirale.
A systematic review on the use of chicken embryos in scientific research - Protocol
Creators: name: Eusemann, Beryl
name: Wilzopolski, Jenny
name: Paternella Suzanne Verhave
name: Butzke, Daniel
name: Sommerer, Adrian
name: Bannach-Brown, Alexandra
name: Schadock, Ines
name: Heinl, Celine
name: Bert, Bettina
name: Hermann, Clara
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Animal Sciences
subject: Other Animal Sciences
subject: Life Sciences
subject: Laboratory and Basic Science Research Life Sciences
subject: Poultry or Avian Science
subject: systematic review
subject: 3R
subject: pain
subject: chick embryo
subject: chicken embryo
subject: animal welfare

description: This systematic review will give an overview about the use of chicken embryos in scientific research in the year 2021 and whether the experiments may have led to pain and distress in the chicken embryos. The protocol defines the research questions as well as methods of the systematic review.
Evolutionary advantage of small populations on complex fitness landscapes
Creators: name: Jain, Kavita
name: Krug, Joachim
name: Park, Su-Chan
Publisher: name: arXiv
Year: 2010
Subjects: subject: Populations and Evolution (q-bio.PE)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: Background: Recent experimental and theoretical studies have shown that small asexual populations evolving on complex fitness landscapes may achieve a higher fitness than large ones due to the increased heterogeneity of adaptive trajectories. Here we introduce a class of haploid three-locus fitness landscapes that allows to investigate this scenario in a precise and quantitative way. Results: Our main result derived analytically shows how the probability of choosing the path of largest initial fitness increase grows with the population size. This makes large populations more likely to get trapped at local fitness peaks and implies an advantage of small populations at intermediate time scales. The range of population sizes where this effect is operative coincides with the onset of clonal interference. Additional studies using ensembles of random fitness landscapes show that the results achieved for a particular choice of three-locus landscape parameters are robust and also persist as the number of loci increases. Conclusions: Our study indicates that an advantage for small populations is likely whenever the fitness landscape contains local maxima. The advantage appears at intermediate time scales, which are long enough for trapping at local fitness maxima to have occurred but too short for peak escape by the creation of multiple mutants.
description: Version to appear in Evolution
The information paradox: A pedagogical introduction
Creators: name: Mathur, Samir D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The black hole information paradox is a very poorly understood problem. It is often believed that Hawking's argument is not precisely formulated, and a more careful accounting of naturally occurring quantum corrections will allow the radiation process to become unitary. We show that such is not the case, by proving that small corrections to the leading order Hawking computation cannot remove the entanglement between the radiation and the hole. We formulate Hawking's argument as a `theorem': assuming `traditional' physics at the horizon and usual assumptions of locality we will be forced into mixed states or remnants. We also argue that one cannot explain away the problem by invoking AdS/CFT duality. We conclude with recent results on the quantum physics of black holes which show the the interior of black holes have a `fuzzball' structure. This nontrivial structure of microstates resolves the information paradox, and gives a qualitative picture of how classical intuition can break down in black hole physics.
description: 38 pages, 7 figures, Latex (Expanded form of lectures given at CERN for the RTN Winter School, Feb 09), typo corrected
Nephus bipunctatus
Creators: name: Poorani, J.
name: Lalitha, N.
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Coccinellidae
Nephus
Nephus bipunctatus

description: 12. Nephus bipunctatus -group
(FIG. 14)
 Brief description: LENGtH 1.90–2.20 MM, WIDtH 1.30–1.50 MM. FORM (FIG. 14A) ElONGAtE OVAl, DORSUM MODERAtElY cONVEX AND DENSElY PUbEScENt. HEAD AND PRONOtUM DARk bROWN tO PIcEOUS. ElYtRA DARk bROWN tO PIcEOUS WItH tWO cIRcUlAR, ORANGE-REDDISH SPOtS IN tHE POStERIOR HAlF. ANtENNA cOMPOSED OF 10 ANtENNOMERES. AbDOMINAl POStcOXAl lINE (FIG. 14b) INcOMPlEtE. MAlE GENItAlIA (FIGS 14c–E) AND FEMAlE SPERMAtHEcA (FIG. 14F) AS IllUStRAtED.
 Notes: THIS SPEcIES bElONGS tO tHE Nephus bipunctatus- GROUP AS DEFINED bY FüRScH (1965) AND IS WIDElY DIStRIbUtED IN INDIA. THERE IS cONSIDERAblE VARIAtION IN tHIS SPEcIES AND It IS NOt POSSIblE tO IDENtIFY It cONclUSIVElY At PRESENt AS INDIAN SPEcIES OF Nephus ARE bADlY IN NEED OF REVISION. THE MAlE GENItAlIA OF tHIS SPEcIES ARE NEARlY IDENtIcAl tO tHE IllUStRAtIONS GIVEN bY REN et al. (2009) FOR Nephus quadrimaculatus (HERbSt), WHIcH IS MOSt lIkElY tO bE A MISIDENtIFIcAtION. It FEEDS ON A VARIEtY OF MEAlYbUGS INclUDING M. hirsutus IN SOUtH INDIA (lAbEl DAtA) AND tHE SPEcIMENS StUDIED FROM WESt BENGAl WERE cOllEctED ON MUlbERRY MEAlYbUG.
description: Published as part of Poorani, J. & Lalitha, N., 2018, Illustrated accounts of coccinellid predators of Maconellicoccus hirsutus (Green) (Hemiptera: Sternorrhyncha: Pseudococcidae) on mulberry in India, with description of a new species of Scymnus Kugelann (Coleoptera: Coccinellidae) from West Bengal, pp. 93-120 in Zootaxa 4382 (1) on page 107, DOI: 10.11646/zootaxa.4382.1.3, http://zenodo.org/record/1181566
Per un pugno di raggi X
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2011

Lastre mediche più sicure grazie al sistema SSRX, progettato da un team di scienziati guidato da ricercatori dell’INAF-IASF di Bologna. È il frutto di tecnologie impiegate nei rivelatori a bordo dei satelliti per astrofisica delle alte energie.
Growth and photosynthetic responses of two subtropical seagrasses, Thalassia testudinum and Halodule wrightii to in situ manipulations of irradiance
Creators: name: Czerny, Andrew Barthel
Publisher: name: The University of Texas at Austin
Year: 1994
Subjects: subject: Halodule wrightii
subject: Thalassia testudinum
subject: Turtle grass
subject: Seagrasses
subject: Growth
subject: Effect of light on
subject: Manipulations of irradiance
subject: Underwater light reduction
subject: Effect of light reduction on
subject: In situ ambient
subject: Photosynthetic responses
subject: Turtle grass--Growth
subject: Turtle grass--Effect of light on
subject: Seagrasses--Growth
subject: Seagrasses--Effect of light on

description: The growth and photosynthetic responses of two species of subtropical seagrasses, Thalassia testudinum and Halodule wrightii, were examined in relation to reductions in underwater light. Shade screens reduced irradiance to roughly 30% and 20% of in situ ambient (ISA). Short shoots of T. testudinum had a greater ability to tolerate a ten month period of light reduction as demonstrated by the longer survival of plants exposed to 30% ISA. Evidence for photoadaptation was observed in plants from shaded treatments compared to unshaded controls (plants receiving 100% ISA). Leaf elongation rates were lower in T. testudinum plants exposed to 20% ISA for one month (October 1992 to November 1992) compared to plants receiving 100% ISA, but there were no differences between treatments for the months of January, February, March, and May. However, by July both levels of shaded T. testudinum had significantly lower growth rates compared to plants receiving 100% ISA. Water temperatures above 25°C and the depletion of stored reserves by spring growth most likely contributed to the disappearance of all short shoots of T. testudinum shaded at 20% ISA and both shaded plots of H. wrightii by August 1993. Photosynthesis versus irradiance (P vs. I) parameters revealed significant differences in the rates of light saturated photosynthesis (P [subscript max]), respiration, saturation irradiance (I [subscript k]), and relative quantum efficiency (α) between the two species. In particular, the significantly lower respiration rates of Thalassia testudinum (89.8 ± 8.4 μmol O₂ gdw⁻¹ h⁻¹ at 30°C) compared to Halodule wrightii (186.0 ± 20.0 μmol O₂ gdw⁻¹ h⁻¹ at 30°C ) may contribute to its survival in light-limited environments. Respiration rates and P [subscript max] for both species significantly increased with seasonal increases in temperature. No significant differences were noted in shaded versus unshaded H. wrightii at 20°C or 30°C; however, in T. testudinum, after four months of shading at 20% ISA, P [subscript max] was significantly lower and α significantly higher relative to unshaded controls. The lower growth rates and increased light harvesting capability of T. testudinum in response to reduced irradiance reflects the K-selected strategy of this species compared to H. wrightii
The environments of starburst and post-starburst galaxies at z=0.4-0.8
Creators: name: Poggianti, Bianca M.
name: Aragon-Salamanca, Alfonso
name: Zaritsky, Dennis
name: De Lucia, Gabriella
name: Milvang-Jensen, Bo
name: Desai, Vandana
name: Jablonka, Pascale
name: Halliday, Claire
name: Rudnick, Gregory
name: Varela, Jesus
name: Bamford, Steven
name: Best, Philip
name: Clowe, Douglas
name: Noll, Stefan
name: Saglia, Roberto
name: Pello, Roser
name: Simard, Luc
name: von der Linden, Anja
name: White, Simon
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Post-starburst (E+A or k+a) spectra, characterized by their exceptionally strong Balmer lines in absorption and the lack of emission lines, belong to galaxies in which the star formation activity ended abruptly sometime during the past Gyr. We perform a spectral analysis of galaxies in clusters, groups, poor groups and the field at z=0.4-0.8 based on the ESO Distant Cluster Survey. The incidence of k+a's at these redshifts depends strongly on environment. K+a's reside preferentially in clusters and, unexpectedly, in a subset of the sigma = 200-400 km/s groups, those that have a low fraction of [OII] emitters. In these environments, 20-30% of the recently star-forming galaxies have had their star formation activity recently truncated. In contrast, there are proportionally fewer k+a's in the field, the poor groups and groups with a high [OII] fraction. The incidence of k+a galaxies correlates with the cluster velocity dispersion: more massive clusters have higher proportions of k+a's. Spectra of dusty starburst candidates, with strong Balmer absorption and emission lines, present a very different environmental dependence from k+a's. They are numerous in all environments at z=0.4-0.8, but they are especially numerous in all types of groups, favoring the hypothesis of triggering by a merger. Our observations are consistent with previous suggestions that cluster k+a galaxies are observed in a transition phase as massive S0 and Sa galaxies, evolving from star-forming later types to passively evolving early-type galaxies. The correlation between k+a fraction and cluster sigma supports the hypothesis that k+a galaxies in clusters originate from processes related to the intracluster medium, while several possibilities are discussed for the origin of the k+a frequency in low-[OII] groups.(abr.)
description: accepted for publication in ApJ
Additional file 1 of ER membrane receptor FgGET2 plays critical roles in hyphal growth, asexual development, stress responses, and pathogenicity of Fusarium graminearum
Creators: name: Liu, Caihong
name: Lei, Lu
name: Zhu, Jing
name: Zhang, Mi
name: Zhang, Ziyi
name: Peng, Shijing
name: Tang, Jie
name: Chen, Lirun
name: Chen, Qing
name: Kong, Li
name: Jiang, Yunfeng
name: Chen, Guoyue
name: Jiang, Qiantao
name: Zhang, Yazhou
name: Xu, Qiang
name: Zheng, Youliang
name: Kogel, Karl-Heinz
name: Wei, Yuming
name: Qi, Pengfei
Publisher: name: figshare
Year: 2025
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 1: Table S1. Primers used in this study.
Illeis confusa Timberlake 1943
Creators: name: Poorani, J.
name: Lalitha, N.
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Coccinellidae
Illeis
Illeis confusa

description: 18. Illeis confusa Timberlake, 1943
(FIG. 20)
 Brief description: LENGtH 4.15–5.34 MM, WIDtH 3.00–3.96 MM. VERY SIMIlAR tO I. cincta IN GENERAl APPEARANcE (FIGS 20A, b), PRONOtUM cREAMY WHItE WItH tWO blAck SPOtS, ElYtRAl cOlORAtION VARIAblE FROM PAlE PINkISH tO cREAMY YEllOW tO bRIGHt YEllOW, lAtERAl MARGINS OF PRONOtUM AND ElYtRA tRANSPARENt. MAlE GENItAlIA (FIGS 20c–F) DIAGNOStIc.
 Notes: THIS SPEcIES IS WIDElY DIStRIbUtED IN tHE NORtHERN, EAStERN AND NORtHEAStERN REGIONS OF INDIA. It FEEDS ON POWDERY MIlDEWS INFEStING MUlbERRY, Dalbergia sissoo, cHIllI, ROSE, AND OtHER PlANtS (lAbEl DAtA).
description: Published as part of Poorani, J. & Lalitha, N., 2018, Illustrated accounts of coccinellid predators of Maconellicoccus hirsutus (Green) (Hemiptera: Sternorrhyncha: Pseudococcidae) on mulberry in India, with description of a new species of Scymnus Kugelann (Coleoptera: Coccinellidae) from West Bengal, pp. 93-120 in Zootaxa 4382 (1) on page 119, DOI: 10.11646/zootaxa.4382.1.3, http://zenodo.org/record/1181566
Come un vero sbarco su Marte
Creators: Elena Lazzaretto
Publisher: name: Media Inaf
Year: 2011

È stata effettuata la prima delle tre uscite previste nell’ambito della simulazione Mars500 dell'ESA. Anche se la passeggiata è stata virtuale, l'emozione è autentica per il nostro Diego Urbina, protagonista dell'impresa insieme al compagno di viaggio Alexandr Smoleevskiy.
Finite size effects on transport coefficients for models of atomic wires coupled to phonons
Creators: name: Bartsch, Christian
name: Gemmer, Jochen
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We consider models of quasi-1-d, planar atomic wires consisting of several, laterally coupled rows of atoms, with mutually non-interacting electrons. This electronic wire system is coupled to phonons, corresponding, e.g., to some substrate. We aim at computing diffusion coefficients in dependence on the wire widths and the lateral coupling. To this end we firstly construct a numerically manageable linear collision term for the dynamics of the electronic occupation numbers by following a certain projection operator approach. By means of this collision term we set up a linear Boltzmann equation. A formula for extracting diffusion coefficients from such Boltzmann equations is given. We find in the regime of a few atomic rows and intermediate lateral coupling a significant and non-trivial dependence of the diffusion coefficient on both, the width and the lateral coupling. These results, in principle, suggest the possible applicability of such atomic wires as electronic devices, such as, e.g., switches.
description: 9 pages, 5 figures, accepted for publication in Eur. Phys. J. B
title: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ðº ÐºÐ¾Ð»Ð»Ð¾ÐºÐ²Ð¸ÑÐ¼Ñ Ð¿Ð¾ ÐÑÑÑÐµÐ¹ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐµ. Ð Ð°Ð·Ð´ÐµÐ»Ñ Â«ÐÑÐ½Ð¾Ð²Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð¹ Ð°Ð»Ð³ÐµÐ±ÑÑ. ÐÐ½ÑÐµÐ³ÑÐ°Ð»ÑÐ½Ð¾Ðµ Ð¸ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ðµ ÑÑÐ½ÐºÑÐ¸Ð¸ Ð¾Ð´Ð½Ð¾Ð¹ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹Â» (Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ ÐºÑÑÑÐ° ÐÐÐÐ¸Ð¢).
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐ»ÑÐ½Ð¸ÑÐ°, ÐÐ½ÑÐ¾Ð½
name: ÐÐ¶Ð¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2022
Subjects: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°
ÐÐ½ÑÐµÐ³ÑÐ°Ð»Ñ
ÐºÐ¾Ð»Ð»Ð¾ÐºÐ²Ð¸ÑÐ¼
ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐµ ÑÐ¸ÑÐ»Ð°
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ ÐºÑÑÑÐ° ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸: 15.03.01 Â«ÐÐ°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ», 15.03.05 Â«ÐÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Â», 23.03.01 Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð²Â», 23.03.02 Â«ÐÐ°Ð·ÐµÐ¼Ð½ÑÐµ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑÂ».
What can one learn from reproducing machine learning experiments?
Creators: name: Machicao, Jeaneth
name: Ben Abbes, Ali
name: Specht, Alison
name: Correa, Pedro Pizzigatti
Publisher: name: Zenodo
Year: 2022

description: This talk was part of the November Narratives Twin-Talks - Reproducibility of ML Experiments and National Research Graph on 17 Nov 2022. It provides some insights from the paper ‘Mitigation Strategies to Improve Reproducibility of Poverty Estimations from Remote Sensing Images Using Deep Learning’ Machicao, J., Ben Abbes, A., Meneguzzi, L., Corrêa, P.L.P., Specht, A., David, R., Subsol, G., Vellenich, D., Devillers, R., Stall, S., Mouquet, N., Chaumont, M., Berti‐Equille, L., Mouillot, D., 2022. Mitigation Strategies to Improve Reproducibility of Poverty Estimations From Remote Sensing Images Using Deep Learning. Earth and Space Science 9. https://doi.org/10.1029/2022EA002379 You can watch the talk on: https://www.youtube.com/watch?v=gAmL40vtcTg This research is product of the PARSEC group funded by the Belmont Forum as part of its Collaborative Research Action (CRA) on Science-Driven e-Infrastructures Innovation (SEI) with support from FAPESP, JST, ANR and NSF, and the synthesis centre CESAB of the French Foundation for Research on Biodiversity.
Equivalent birational embeddings II: divisors
Creators: name: Mella, Massimiliano
name: Polastri, Elena
Publisher: name: arXiv
Year: 2009
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14E25

description: Two divisors in $¶^n$ are said to be Cremona equivalent if there is a Cremona modification sending one to the other. We produce infinitely many non equivalent divisorial embeddings of any variety of dimension at most 14. Then we study the special case of plane curves and rational hypersurfaces. For the latter we characterise surfaces Cremona equivalent to a plane.
description: v2 Exposition improved, thanks to referee, unconditional characterization of surfaces Cremona equivalent to a plane
Il buco nero attorciglia la luce
Creators: Luca Nobili
Publisher: name: Media Inaf
Year: 2011

I buchi neri ruotanti fanno fare le "piroette" alla luce che li attraversa. A provare questa proprietà delle onde elettromagnetiche, chiamata vorticità, è uno studio internazionale guidato da Fabrizio Tamburini, dell'Università di Padova. Importanti le ricadute per la ricerca astrofisica e le telecomunicazioni.
Cluster characters II: A multiplication formula
Creators: name: Palu, Yann
Publisher: name: arXiv
Year: 2009
Subjects: subject: Representation Theory (math.RT)
subject: FOS: Mathematics

description: Let $\mathcal{C}$ be a Hom-finite triangulated 2-Calabi-Yau category with a cluster tilting object. Under some constructibility assumptions on $\mathcal{C}$ which are satisfied for instance by cluster categories, by generalized cluster categories and by stable categories of modules over a preprojective algebra, we prove a multiplication formula for the cluster character associated with any cluster tilting object. This formula generalizes those obtained by Caldero-Keller for representation finite path algebras and by Xiao-Xu for finite-dimensional path algebras. It is analogous to a formula obtained by Geiss-Leclerc-Schröer in the context of preprojective algebras.
description: v3: Updated references. Section on Fu--Keller's cluster character. v4: Some expository changes as suggested by the referee. To appear in Proceedings LMS
Un cacciatore di Terre al TNG
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2011

 “Sono particolarmente soddisfatto di questo accordo – afferma il Presidente dell’Istituto Nazionale di Astrofisica, Tommaso Maccacaro – che permette alla comunità italiana di inserirsi attivamente, con il TNG, in un importante filone di ricerca”. Lo spettrometro, operativo dal 2012, sarà sinergico anche a Kepler.
Additional file 1 of A cash transfer plus gender transformative economic empowerment intervention seeking to improve the wellbeing of caregivers of children and adolescents living with HIV in South Africa: a feasibility study protocol for a pilot cluster randomized trial
Creators: name: Govindasamy, Darshini
name: Shai, Nwabisa
name: Mwandacha, Nelly
name: Carries, Stanley
name: Sithole, Nokwanda
name: Closson, Kalysha
name: Bhana, Arvin
name: Sigwadhi, Lovemore
name: Washington, Laura
name: Gibbs, Andrew
name: Kaida, Angela
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Appendix A—SPIRIT Checklist. Checklist of recommended items to address in a clinical trial protocol.
34 occhi per un nuovo sistema solare
Creators: Francesco Rea
Publisher: name: Media Inaf
Year: 2011

I successi di Kepler fanno guardare con grande aspettativa a PLATO, la missione dell'ESA destinata alla ricerca di pianeti extrasolari, se sarà selezionata nel programma Cosmic Vision. All'INAF, si deve il disegno dei 34 telescopi a bordo del satellite. Ne parliamo con Giusi Micela, del team di Plato.
Pattern avoidance and RSK-like algorithms for alternating permutations and Young tableaux
Creators: name: Lewis, Joel Brewster
Publisher: name: arXiv
Year: 2009
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05A05 (Primary), 05A10, 05A15, 05A19 (Secondary)

description: We define a class L_{n, k} of permutations that generalizes alternating (up-down) permutations and give bijective proofs of certain pattern-avoidance results for this class. As a special case of our results, we give two bijections between the set A_{2n}(1234) of alternating permutations of length 2n with no four-term increasing subsequence and standard Young tableaux of shape (3^n), and between the set A_{2n + 1}(1234) and standard Young tableaux of shape (3^{n - 1}, 2, 1). This represents the first enumeration of alternating permutations avoiding a pattern of length four. We also extend previous work on doubly-alternating permutations (alternating permutations whose inverses are alternating) to our more general context. The set L_{n, k} may be viewed as the set of reading words of the standard Young tableaux of a certain skew shape. In the last section of the paper, we expand our study to consider pattern avoidance in the reading words of standard Young tableaux of any skew shape. We show bijectively that the number of standard Young tableaux of shape lambda/mu whose reading words avoid 213 is a natural mu-analogue of the Catalan numbers (and in particular does not depend on lambda, up to a simple technical condition), and that there are similar results for the patterns 132, 231 and 312.
description: 35 pages, 12 figures. v3: this version extends the published version. In the published version, the order of Sections 4.1 and 4.2 is reversed, and the proofs in the present Section 4.1 are omitted. Otherwise, the two versions are essentially the same
Un miliardesimo di grammo
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2011

È l’incredibile sensibilità delle microbilance a cristalli di quarzo create nei laboratori dell’INAF di Napoli. Progettate per pesare le polveri delle comete o delle tempeste marziane, non c‘è sulla Terra particella che sfugga al loro controllo. Dallo smog alle eruzioni, innumerevoli sono le applicazioni.
Duemila stelle in Nord America
Creators: Daniela Cipolloni
Publisher: name: Media Inaf
Year: 2011

Gli occhi infrarossi del telescopio spaziale Spitzer della NASA hanno guardato dentro la Nebulosa Nord America, così chiamata per il suo profilo. Hanno trovato una famiglia di circa duemila stelle appena nate o che stanno per nascere. Prima di queste immagini, ne erano note solo 200.
Marte, arriviamo!
Creators: Elena Lazzaretto
Publisher: name: Media Inaf
Year: 2011

Dopo oltre 8 mesi di "volo", il 14 febbraio l'italo-colombiano Diego Urbina e il russo Alexandr Smoleevskiy approdano sulla superficie del Pianeta Rosso nella simulazione Mars500. La missione dell'ESA è la prima riproduzione fedele di un vero viaggio di andata, permanenza e ritorno su Marte.
Additional file 2 of A cash transfer plus gender transformative economic empowerment intervention seeking to improve the wellbeing of caregivers of children and adolescents living with HIV in South Africa: a feasibility study protocol for a pilot cluster randomized trial
Creators: name: Govindasamy, Darshini
name: Shai, Nwabisa
name: Mwandacha, Nelly
name: Carries, Stanley
name: Sithole, Nokwanda
name: Closson, Kalysha
name: Bhana, Arvin
name: Sigwadhi, Lovemore
name: Washington, Laura
name: Gibbs, Andrew
name: Kaida, Angela
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Appendix C—SRD Grant Eligibility Criteria. Eligibility criteria for South Africa’s COVID- 19 SRD grant.
Luci intermittenti sulle aurore di Giove
Creators: Daniela Cipolloni
Publisher: name: Media Inaf
Year: 2011

Nuove osservazioni con il telescopio spaziale Hubble rivelano che dalle aurore del gigante gassoso sprizzano intensi "flares"di luce ultravioletta: durano diverse decine di secondi e si ripetono con regolarità ogni 2-3 minuti. Di che si tratta? Lo studio su Geophysical Research Letters.