cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ¸ÑÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ñ Ð¸ ÑÐ¿Ð°ÐºÐ¾Ð²ÐºÐ¸ Ð´Ð»Ñ Ð¼ÑÐ»Ð° ÑÑÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾Ñ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»Ð¸Ð½Ð¾Ð²Ð°, ÐÐ¾Ð»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Ð¾Ð²Ð°ÑÐ½ÑÐ¹ Ð·Ð½Ð°Ðº
Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ
Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ
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description: Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ¿Ð°ÐºÐ¾Ð²ÐºÐ° Ð´Ð»Ñ Ð¼ÑÐ»Ð° ÑÑÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ¸ÑÐ¼Ñ Â«JANNASOAPÂ» Ñ Ð½Ð¾Ð²ÑÐ¼ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐµÑÐµÐ½Ð¸ÐµÐ¼, ÐºÐ¾ÑÐ¾ÑÑÑ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶Ð¸Ð²Ð°ÐµÑ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´Ð°ÑÑÐ°Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ. ÐÐ»Ñ ÑÑÐ¾Ð³Ð¾ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸ Ð¿Ð¾Ð´Ð¾Ð±Ð½Ð¾Ð³Ð¾ ÑÐ¾Ð²Ð°ÑÐ°, Ð²ÑÐ±ÑÐ°Ð½Ñ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, Ð¸Ð·ÑÑÐµÐ½Ñ Ð¸Ð¼ÐµÑÑÐ¸Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÐ¿Ð°ÐºÐ¾Ð²ÐºÐ¸. ÐÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÐºÑÐ¾Ñ ÑÐ¿Ð°ÐºÐ¾Ð²ÐºÐ¸, ÑÐ¾Ð²Ð°ÑÐ½Ð¾Ð³Ð¾ Ð·Ð½Ð°ÐºÐ°, Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´Ð°ÑÑÐµÐ¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸: Ð²Ð¸Ð·Ð¸ÑÐºÐ°, Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð²ÐºÐ»Ð°Ð´ÑÑâ Ð±ÑÐ»Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ: AdobePhotoshop CC, AdobeIllustrator CC Ð¸ AdobeIndesign CC. ÐÐ»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÐºÐµÑÐ° ÑÐ¿Ð°ÐºÐ¾Ð²Ð¾Ðº Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐ»Ð°ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Ð´Ð»Ñ 3DÐ¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ: 3dsMax.
title: Ð¦Ð¸ÑÐºÑÐ»ÑÑÐ¸Ð¾Ð½Ð½ÑÐ¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð°ÑÐ¾ÑÐ½ÑÐ¹ Ð°Ð³ÑÐµÐ³Ð°Ñ Ð¦Ð­ÐÐ 40 000-27 Ð´Ð»Ñ ÐÐÐ­Ð¡ 2
title: Circulating electric pump unit CENA 40 000-27 for LAES-2
Creators: name: ÐÐ¾ÑÐ±Ð°ÑÐ¾Ð², ÐÐ°Ð½Ð¸Ð¸Ð»
name: ÐÐ°Ð»Ð°ÐµÐ², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: Ð¨ÑÐ¼Ð¸Ð»Ð¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
name: "ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ, Ð³Ð¸Ð´ÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ Ð¸ Ð³Ð¸Ð´ÑÐ¾Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ°. Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2020; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: ÐÐ°ÑÐ¾ÑÑ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½ÑÐµ

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð´Ð²Ð° Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ° Ð¿ÑÐ¾ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð²ÐµÑÑÐ¸ÐºÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾Ð³Ð¾ Ð½Ð°ÑÐ¾ÑÐ° Ð±ÑÑÑÑÐ¾ÑÐ¾Ð´Ð½Ð¾ÑÑÑÑ ns = 308 Ð¸ ns = 387. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÑÑÑÑÐ° ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿ÑÐ¾ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸, Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ¶Ð´Ð°ÑÑÐ¸Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð·Ð°Ð´Ð°Ð½Ð½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð².
description: Two variants of the flow part of a vertical centrifugal pump with a speed of ns = 308 and ns = 387 are considered. The results of hydraulic calculation of the flow part elements are presented, confirming the provision of the specified parameters.
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¿Ð¾Ð¸ÑÐºÐ° ÐºÑÐ°ÑÑÐ°Ð¹ÑÐµÐ³Ð¾ Ð¿ÑÑÐ¸ Ð² Ð³ÑÐ°ÑÐµ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ½Ð¾Ð², ÐÑÑÐµÐ¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð´ÐµÐ¹ÐºÑÑÑÑ
Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾ÑÐ¾ÑÐ½ÑÐ¹ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼
ÑÐµÐ¾ÑÐ¸Ñ Ð³ÑÐ°ÑÐ¾Ð²
Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾ÑÑÑ
ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·

description: Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° Ð¿Ð¾Ð¸ÑÐºÐ° ÐºÑÐ°ÑÑÐ°Ð¹ÑÐµÐ³Ð¾ Ð¿ÑÑÐ¸ Ð² Ð³ÑÐ°ÑÐµ - Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° ÐÐµÐ¹ÐºÑÑÑÑ. Ð Ð°ÑÐºÑÑÐ²Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð², Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð±Ð°Ð·Ð¾Ð²ÑÐµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸Ð· ÑÐµÐ¾ÑÐ¸Ð¸ Ð³ÑÐ°ÑÐ¾Ð², Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÐµÑÑÑ Ð²Ð°Ð¶Ð½Ð¾ÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° Ð¿Ð¾Ð¸ÑÐºÐ° ÐºÑÐ°ÑÑÐ°Ð¹ÑÐµÐ³Ð¾ Ð¿ÑÑÐ¸ Ð² Ð³ÑÐ°ÑÐµ, Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸ Ð´Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑÑÑ ÐµÐ³Ð¾ ÐºÐ¾ÑÑÐµÐºÑÐ½Ð¾ÑÑÑ, Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¹, Ð´ÐµÐ»Ð°ÐµÑÑÑ Ð²ÑÐ²Ð¾Ð´ Ð¾ ÑÐ»ÑÑÐ°ÑÑ ÑÐ¼ÐµÑÑÐ½Ð¾Ð³Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð³Ð¾ Ð¸Ð»Ð¸ Ð¸Ð½Ð¾Ð³Ð¾ Ð²Ð¸Ð´Ð° Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð°. ÐÐ°Ðº ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ, Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð½Ð° Ð¼Ð½Ð¾Ð³Ð¾ÑÐ´ÐµÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÐµÐµ Ð¾Ð´Ð½Ð¾Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¾Ð³Ð°.
title: ÐÐ²Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð¾Ð¿ÑÐ¸ÐºÐ°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Â«Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â»
titleType: Subtitle
Creators: name: ÐÐµÑÑÑÐ½ÑÐºÐ¸Ð½, ÐÑÐµÐ²Ð¾Ð»Ð¾Ð´
name: ÐÑÑÐ°ÑÐºÐ¾, Ð.
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2011
Subjects: ÐÐ²Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð¾Ð¿ÑÐ¸ÐºÐ°
ÐÐ²Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ°

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð»ÐµÐ½Ð¸Ñ, Ð² ÐºÐ¾ÑÐ¾ÑÑÑ Ð²Ð°Ð¶Ð½Ð° ÐºÐ²Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ½Ð¾ÑÑÑ ÑÐ²ÐµÑÐ°. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð´Ð°Ð½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÐºÐ²Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÐ²ÐµÑÐ° Ñ Ð²ÐµÑÐµÑÑÐ²Ð¾Ð¼ Ð½Ð° ÑÑÐ¾Ð²Ð½Ðµ, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾Ð¼ Ð´Ð»Ñ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÐºÐ²Ð°Ð½Â­ÑÐ¾Ð²Ð°Ñ ÑÐµÐ¾ÑÐ¸Ñ Ð»Ð°Ð·ÐµÑÐ° Ð¸ Ð¾Ð¿ÑÐ¸ÐºÐ° ÑÐ¾ÑÐ¾Ð½Ð¾Ð². Ð Ð¿Ð¾ÑÐ»ÐµÐ´Ð½ÐµÐ¹ ÑÐ°ÑÑÐ¸ Ð¾Ð±ÑÑÐ¶Ð´Ð°ÑÑÑÑ Ð½ÐµÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ²ÐµÑÐ°: ÑÐ¶Ð°ÑÑÐ¹ ÑÐ²ÐµÑ Ð¸ Ð¿ÐµÑÐµÐ¿ÑÑÐ°Ð½Ð½ÑÐµ ÑÐ¾ÑÑÐ¾ÑÂ­Ð½Ð¸Ñ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½ÐµÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¹ ÑÐ²ÐµÑÐ° Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð¸ Ð² ÐºÐ²Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÐºÑÐ¸Ð¿ÑÐ¾Ð³ÑÐ°ÑÐ¸Ð¸. ÐÐ°Ð½Ð¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ¾ÑÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 553100 Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â». ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Â­Ð²Ð°Ð½Ð¾ Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸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°.
Phase Shift in the Whitham Zone for the Gurevich-Pitaevskii Special Solution of the Korteweg-de Vries Equation
Creators: name: Garifullin, R.
name: Suleimanov, B.
name: Tarkhanov, N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: We get the leading term of the Gurevich-Pitaevskii special solution to the KdV equation in the oscillation zone without using averaging methods.
description: 13 pages, 3 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ 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Ð¾Ð±Ð¾ÑÐºÐ¾, ÐÐ°ÑÐº
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¸Ð·Ð½ÐµÑ Ð¿Ð»Ð°Ð½
ÑÐ°Ð»Ð¾Ð½ ÐºÑÐ°ÑÐ¾ÑÑ
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
ÑÐ¸ÑÐºÐ¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð»Ð¾Ð½ ÐºÑÐ°ÑÐ¾ÑÑ Â«ÐÑÑ-ÐÐ¾ÑÐºÂ».
ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¿Ð»Ð°Ð½ Ð¿Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ°Ð»Ð¾Ð½Ð° ÐºÑÐ°ÑÐ¾ÑÑ.
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 ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð±Ð¸Ð·Ð½ÐµÑ Ð¿Ð»Ð°Ð½Ð° Ð¿Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ°Ð»Ð¾Ð½Ð° ÐºÑÐ°ÑÐ¾ÑÑ Â«ÐÑÑ-ÐÐ¾ÑÐº.
Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÑÑÑÑ Ð¿ÑÐ¾ÑÐµÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹, Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°ÑÑÐµÑÐ°, Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð½ÑÑ ÑÐ°ÑÑÐµÑÐ¾Ð², Ð¸Ñ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸, Ð±Ð°Ð·Ð¾Ð²ÑÐµ Ð¸ ÑÐ³Ð»ÑÐ±Ð»ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð·Ð½Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð¸ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° ÑÐ¸ÑÐºÐ¾Ð².
Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½Ð¾ÑÐ½ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹, ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¿Ð»Ð°Ð½, Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ°Ð»Ð¾Ð½Ð° ÐºÑÐ°ÑÐ¾ÑÑ.
A rare case of urachal adenocarcinoma arising in urachal cyst: clinical and radiological features
Creators: name: Di Caprera, Elena
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Abdomen
subject: CT
subject: MR
subject: PET-CT
subject: Ultrasound
subject: Diagnostic procedure
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 45 years
description: Clinical History: A 45-year-old female patient was referred to our hospital with a few month history of abdominal mass which was rounded with hard consistence.The Patient reported that this mass was not painful and that it had become evident during an interrupted pre... Final Diagnosis: Urachal Adenocarcinoma
Characterization of Brazilian monofloral and polyfloral honey by UHPLC-MS and classic physical-chemical analyses
Creators: name: Archilia, Mariana Degaki
name: Neto, Amandio Augusto Lagareiro
name: Marcucci, Maria Cristina
name: Alonso, Roberta Caroline Bruschi
name: de Camargo, Thaiana Cristina
name: Camargo, Ricardo Costa
name: Sawaya, Alexandra Christine Helena Frankland
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Fifty samples of honey, reported by the suppliers as being: orange (Citrus sinensis), eucalyptus (Eucalyptus spp.), coffee (Coffea Arabica), cipo uva (Cissus rhombifolia), quince (Cydonia oblonga), monjoleiro (Acacia polyphylla), mangrove and honeydew were collected from different states of Brazil, between 2014 and 2016, with the aim of studying their physical-chemical properties and chemical composition, searching for markers to determine their floral origin, authenticity, and quality. There is little information on some of these types of honey, such as quince honey, whose chemical characteristics were defined in the present study. Thus, the total phenolic and flavonoid contents, proteins, color, moisture, and electrical conductivity were evaluated. All the samples presented satisfactory results for color and percentage of sugars in relation to the Brazilian legislation, as well as protein concentration; most were within the limit of conductivity established by the Council of the European Union. Only six samples indicated a probability of overheating, having high HMF values. Phenolic compounds were extracted, analyzed by ultra-high-performance liquid chromatography with mass spectrometry and the data extracted and treated by chemometrics. Honey samples classified as quince by the producers were predominantly monofloral and had a distinct chemical marker; abscisic acid. Some of the samples declared as orange and coffee were clearly grouped, however, some samples declared as eucalyptus, coffee, and orange honey were probably not monofloral. Eucalyptus honey had high total phenolics and flavonoids, thus probably has a higher antioxidant function when compared to the other floral origins analyzed herein.
Leptogenesis, Z' bosons, and the reheating temperature of the Universe
Creators: name: Racker, J.
name: Roulet, E.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the impact for leptogenesis of new U(1) gauge bosons coupled to the heavy Majorana neutrinos. They can significantly enhance the efficiency of thermal scenarios in the weak washout regime as long as the Z' masses are not much larger than the reheating temperature ($M_{Z'}<10 T_{rh}$), with the highest efficiencies obtained for Z' bosons considerably heavier than the heavy neutrinos ($M_{Z'} > 100 M_1$). We show how the allowed region of the parameter space is modified in the presence of a Z' and we also obtain the minimum reheating temperature that is required for these models to be successful.
description: 14 pages, 6 figures; One figure added, discussion on the reheating temperature extended
title: ÐÑÐ½Ð¾Ð²Ñ Ð¿Ð»Ð°Ð·Ð¼Ð¾Ñ Ð¸Ð¼Ð¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð§ÐµÑÐ½Ð¾Ð²ÐµÑ, ÐÐ¾ÑÐ¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: ÐÐ»Ð°Ð·Ð¼Ð¾Ñ Ð¸Ð¼Ð¸Ñ

description: ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÑÐ¸Ð¼ÑÐ»ÑÑÐ¸Ð¸ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐµÐ²ÑÐ°ÑÐµÐ½Ð¸Ð¹ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð¾Ð¼ ÑÐµÐ°Ð³ÐµÐ½ÑÐ¾Ð² Ð² Ð¿Ð»Ð°Ð·Ð¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð²Ð¾Ð·Ð±ÑÐ¶Ð´ÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð·Ð¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°ÑÐ½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð³Ð»Ð°Ð²Ð½ÑÐ¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼ Ð²Ð½ÑÑÑÐµÐ½Ð½ÑÑ ÑÐ½ÐµÑÐ³Ð¸Ñ Ð°ÑÐ¾Ð¼Ð¾Ð² Ð¸ Ð¼Ð¾Ð»ÐµÐºÑÐ» Ñ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ Ð¸Ñ Ð¾Ð±Ð¾Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ñ ÑÑÐ¾Ð»ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ð¹. ÐÐ»Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¸Ð·ÑÑÐµÐ½Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² Ð¿Ð»Ð°Ð·Ð¼Ð¾ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¾Ð±ÑÑÐ¶Ð´ÐµÐ½Ð¸Ðµ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐµÐ¹ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð² Ð²Ð¾Ð·Ð±ÑÐ¶Ð´ÐµÐ½Ð½ÑÐµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Â«ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð½Ð°Ð½Ð¾Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¸ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ½Ð¸ÐºÐ¸Â» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 152100 Â«ÐÐ°Ð½Ð¾Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÂ». ÐÐ½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 150100 Â«ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²Â», 223200 Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â», Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸, Ð² ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿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°.
High-energy emission from jet-clump interactions in microquasars
Creators: name: Araudo, Anabella T.
name: Bosch-Ramon, Valenti
name: Romero, Gustavo E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: High-mass microquasars are binary systems consisting of a massive star and an accreting compact object from which relativistic jets are launched. There is considerable observational evidence that winds of massive stars are clumpy. Individual clumps may interact with the jets in high-mass microquasars to produce outbursts of high-energy emission. Gamma-ray flares have been detected in some high-mass X-ray binaries, such as Cygnus X-1, and probably in LS 5039 and LS I+61 303. We predict the high-energy emission produced by the interaction between a jet and a clump of the stellar wind in a high-mass microquasar. Assuming a hydrodynamic scenario for the jet-clump interaction, we calculate the spectral energy distributions produced by the dominant non-thermal processes: relativistic bremsstrahlung, synchrotron and inverse Compton radiation, for leptons, and for hadrons, proton-proton collisions. Significant levels of emission in X-rays (synchrotron), high-energy gamma rays (inverse Compton), and very high-energy gamma rays (from the decay of neutral pions) are predicted, with luminosities in the different domains in the range ~ 10^{32}-10^{35} erg/s. The spectral energy distributions vary strongly depending on the specific conditions. Jet-clump interactions may be detectable at high and very high energies, and provide an explanation for the fast TeV variability found in some high-mass X-ray binary systems. Our model can help to infer information about the properties of jets and clumpy winds by means of high-sensitivity gamma-ray astronomy.
description: Accepted for publication in A&A (10 pages, 8 figures)
More time to fly: with a warming climate the Western honey bee (Apis mellifera, Linnaeus) now has more temperature-eligible flight hours than 40 years ago
Creators: name: Rogers, Richard
name: Hassler, Edgar
name: Carey, Quinn
name: Cazier, Joseph
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: There have been official NOAA and EPA reports of measurable changes in temperature across the United States over the last several decades with average temperatures increasing in most areas and decreasing in a few others. In order to fly, honey bees need optimal temperatures ranging from 13 °C (55 °F) to 38 °C (100 °F), sunlight, low wind, and no rain. This study looks at changes in temperature-eligible flight times of honey bees across the US and Canada. Four decades of weather data from 60 locations in the US and Canada for the period 1980 through 2019 were analyzed. We discovered that honey bee flight hours are increasing almost everywhere, but most dramatically in the northern regions of Canada and Alaska, and also in a few locations in the US south of the border with Canada. Warming temperatures (ignoring all other factors), may lead to more flight time for honey bees; may affect plant bloom times and species distributions; and may change the exposure of honey bee colonies to pests, parasites, and pathogens. Therefore, beekeepers must be prepared to modify management practices to accommodate possible plant–pollinator mismatches and timings for seasonal and pest management. This study highlights that a warming climate will increase temperature-eligible flight hours for honey bees. Further research is needed to consider how other climate change factors, in combination with temperature, will affect actual honey bee flight opportunities and behavior, as well as, overall colony management.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð·ÐµÐ¼ÐµÐ»ÑÐ½ÑÐ¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸ Ð¸ ÐºÐ°Ð´Ð°ÑÑÑ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð´ÐµÐ½ÐºÐ¾, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ°ÑÐ¼Ð°Ð½Ð¾Ð², ÐÐ¸ÑÐ°Ð»Ð¸Ð¹
name: Ð¢ÐµÑÐ»ÐµÐµÐ², ÐÐ¸ÑÐ°Ð»Ð¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2017
Subjects: Ð·ÐµÐ¼ÐµÐ»ÑÐ½ÑÐµ ÑÐµÑÑÑÑÑ
ÐºÐ°Ð´Ð°ÑÑÑ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ðµ Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð·ÐµÐ¼ÐµÐ»ÑÐ½ÑÑ ÑÐµÑÑÑÑÐ¾Ð², ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð±Ð°Ð·Ñ Ð¿Ð¾ Ð·ÐµÐ¼Ð»ÐµÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÐµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ Ð²Ð¾Ð´Ð¾ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÐ¼ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾Ð¼. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¸Ð· ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð·ÐµÐ¼ÐµÐ»ÑÐ½ÑÐ¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ 08.03.01 ââÐ¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾" Ð¸ 20.03.02 "ÐÑÐ¸ÑÐ¾Ð´Ð¾Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð¸ Ð²Ð¾Ð´Ð¾Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµâ; Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¸ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ°ÑÐµÑÐ¸Ð°Ð», Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐ¹ Ð² ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸, Ð±ÑÐ´ÐµÑ Ð¸Ð½ÑÐµÑÐµÑÐµÐ½ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°Ð¼ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð²Ð¾Ð´Ð¾ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°.
Additional file 2 of Transcriptomics and metabolomics reveal changes in the regulatory mechanisms of osteosarcoma under different culture methods in vitro
Creators: name: Yang, Sen
name: Tian, Zhi
name: Feng, Yi
name: Zhang, Kun
name: Pan, Yongchun
name: Li, Yuan
name: Wang, Zhichao
name: Wei, Wenhao
name: Qiao, Xiaochen
name: Zhou, Ruhao
name: Yan, Lei
name: Li, Qian
name: Guo, Hua
name: Yuan, Jie
name: Li, Pengcui
name: Lv, Zhi
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Additional file 2: Fig S2. Total ion Chromatogram of OS samples based on ionic strength. The signal intensity of the sample quality spectrum can be controlled as a whole by taking the time point as the abscissa and the sum of the intensity of all ions in the mass spectrum as the ordinate. A POS, B NEG.
Probing AdS4/CFT3 proposals beyond chiral rings
Creators: name: Kim, Seok
name: Park, Jaemo
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We calculate the superconformal Witten index for the Chern-Simons-matter theory which was proposed to describe multiple M2-branes on $C^2 X C^2/Z_k$. We consider a variant of this model, which exhibits explicit N=3 supersymmetry and has the advantage of not having an exotic branch of the moduli space. At $k=1$, we compare the index with that from the proposed gravity dual and find a disagreement.
description: references added; introduction modified
Additional file 1 of Prenatal social support in low-risk pregnancy shapes placental epigenome
Creators: name: Tesfaye, Markos
name: Wu, Jing
name: Biedrzycki, Richard J.
name: Grantz, Katherine L.
name: Joseph, Paule
name: Tekola-Ayele, Fasil
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Fig S1. Manhattan plot and QQ plot of CpGs in placenta associated with maternal social support for all pregnancies. Fig S2. Manhattan plot and QQ plot of CpGs in placenta associated with maternal social support for pregnancies with male fetus. Fig S3. Manhattan plot and QQ plot of CpGs in placenta associated with maternal social support for pregnancies with female fetus. Fig S4. Distribution of post hoc power analyzed for DNA methylation effect sizes. Fig S5. Tissue expression of VGF. Fig S6. Tissue expression of ILVBL. Table S1. Characteristics of study participants who provided placenta samples and those who did not. Table S2. Sensitivity analysis for CpGs in placenta associated with maternal social support. Table S3. CpGs in placenta associated with maternal social support in pregnancies with male fetus. Table S4. CpGs in placenta associated with maternal social support in pregnancies with female fetus. Table S5. Sensitivity analysis for CpGs in placenta associated with maternal social support in pregnancies with male fetus. Table S6. Sensitivity analysis for CpGs in placenta associated with maternal social support in pregnancies with female fetus.
Effect of Background Evolution on the Curvaton Non-Gaussianity
Creators: name: Enqvist, Kari
name: Takahashi, Tomo
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate how the background evolution affects the curvature perturbations generated by the curvaton, assuming a curvaton potential that may deviate slightly from the quadratic one, and parameterizing the background fluid density as ρ\propto a^{-α}, where a is the scale factor, and αdepends on the background fluid. It turns out that the more there is deviation from the quadratic case, the more pronounced is the dependence of the curvature perturbation on α. We also show that the background can have a significant effect on the nonlinearity parameters f_NL and g_NL. As an example, if at the onset of the curvaton oscillation there is a dimension 6 contribution to the potential at 5 % level and the energy fraction of the curvaton to the total one at the time of its decay is at 1 %, we find variations Δf_NL \sim \mathcal{O}(10) and Δg_NL \sim \mathcal{O}(10^4) between matter and radiation dominated backgrounds. Moreover, we demonstrate that there is a relation between f_NL and g_NL that can be used to probe the form of the curvaton potential and the equation of state of the background fluid.
description: 14 pages, 8 figures
Energy gaps in quantum first-order mean-field-like transitions: The problems that quantum annealing cannot solve
Creators: name: Jorg, T.
name: Krzakala, F.
name: Kurchan, J.
name: Maggs, A. C.
name: Pujos, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Computational Complexity (cs.CC)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We study first-order quantum phase transitions in models where the mean-field traitment is exact, and the exponentially fast closure of the energy gap with the system size at the transition. We consider exactly solvable ferromagnetic models, and show that they reduce to the Grover problem in a particular limit. We compute the coefficient in the exponential closure of the gap using an instantonic approach, and discuss the (dire) consequences for quantum annealing.
description: 6 pages, 3 figures
Breeding for hygienic behavior in honey bees (Apis mellifera): a strong paternal effect
Creators: name: Seltzer, Rya
name: Kamer, Yosef
name: Kahanov, Paz
name: Splitt, Aleksandra
name: Bieńkowska, Małgorzata
name: Hefetz, Abraham
name: Soroker, Victoria
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: Marine Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: The haplodiploid sex determination of honey bees and the multiple mating of queens pose challenges in determining the genetic contribution of drones (male honey bees). This is especially important for breeding programs as, for example, when attempting to reinforce traits governing social immunity against pests and diseases. Here, we focused on breeding aiming at enhancing hygienic behavior, a trait that is known to reduce parasite load in honey bee colonies. To evaluate the contribution of drones versus queens to this trait, we conducted a two-step bidirectional selection program. First, we selected colonies with consistent phenotypes for low- or high-hygienic behavior (generation P). From those, we generated two types of daughter colonies (F1). One type originated from queens that had been artificially inseminated with selected drones that originated from queens of either low- or high-hygienic phenotype. The other type of colonies was set from naturally mated queens. We then compared the hygienic performance of the progeny colonies. In the next step, we used the F1 colonies (from either artificially inseminated or naturally mated queens) to produce naturally mated queens, which subsequently generated F2 colonies. These were then examined for the level of hygienic behavior. The results demonstrate the significant contribution of both parents to the phenotype of offspring. In particular, drones had a consistent and significant influence on the hygienic performance of the progeny throughout generations. These findings emphasize the great potential to propagate the hygienic trait in local populations by selecting lines for drones that carry the high-hygienic trait.
Vetoing atmospheric neutrinos in a high energy neutrino telescope
Creators: name: Schönert, Stefan
name: Gaisser, Thomas K.
name: Resconi, Elisa
name: Schulz, Olaf
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss the possibility to suppress downward atmospheric neutrinos in a high energy neutrino telescope. This can be achieved by vetoing the muon which is produced by the same parent meson decaying in the atmosphere. In principle, atmospheric neutrinos with energies $E_ν> 10$ TeV and zenith angle up to 60 degree can be vetoed with an efficiency of > 99%. Practical realization will depend on the depth of the neutrino telescope, on the muon veto efficiency and on the ability to identify downward moving neutrinos with a good energy estimation.
description: 10 pages, 3 figures, accepted for publication in Physical Review D
Additional file 1 of Transcriptomics and metabolomics reveal changes in the regulatory mechanisms of osteosarcoma under different culture methods in vitro
Creators: name: Yang, Sen
name: Tian, Zhi
name: Feng, Yi
name: Zhang, Kun
name: Pan, Yongchun
name: Li, Yuan
name: Wang, Zhichao
name: Wei, Wenhao
name: Qiao, Xiaochen
name: Zhou, Ruhao
name: Yan, Lei
name: Li, Qian
name: Guo, Hua
name: Yuan, Jie
name: Li, Pengcui
name: Lv, Zhi
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Additional file 1: Fig S1. Appearance of each 3D cultured OS tissue. A 3D cells, B 3D cell-printed tissue, C isolated tissue.
ПОТЕНЦИАЛ ЗАМЕЩЕНИЯ УГОЛЬНЫХ МОЩНОСТЕЙ СОЛНЕЧНОЙ ЭНЕРГЕТИКОЙ
Creators: name: РЕВА А.Р.
Publisher: name: Инновации и инвестиции
Year: 2020
Subjects: ВЫБРОСЫ СО2
ЭКОНОМИЧЕСКИЙ РОСТ
ТЕСТ ДИКИ-ФУЛЛЕРА
КРИВАЯ КУЗНЕЦА
ИНДИЯ
CO2 EMISSIONS
ECONOMIC GROWTH
DICKEY-FULLER TEST
KUZNETS CURVE
INDIA

description: Экономическое развитие, а в частности, долгосрочный экономический рост страны в значительной степени зависит от долгосрочного обеспечения энергией и нагрузки на окружающую среду. Ожидается, что в ближайшие годы Индии удастся поддержать адекватные поставки энергии. Фактор загруженности угольных электростанций ниже ожидаемых значений по всей стране, отказ от угля стал основополагающим фактором новой политики. Данный подход предоставляет Индии прекрасную возможность возглавить глобальный переход к экономике чистой энергии. В связи с глобальным потеплением и зависимостью от ископаемого топлива тяготящим экономику Индии возникает вопрос чем его заменить? Возобновляемые источники энергии, в частности, солнечная энергия и модернизация электросетей должны сыграть важную роль в замене выбывающих угольных мощностей и, таким образом, снизить темп со строительством новых заводов по производству природного газа. Понятие экологической кривой Кузнеца (ЭКК), которая связывает экономическое развитие с загрязнением, хорошо известно, существуют разногласия относительно ее формы, распространенности и переменных. Исходная литература по ЭКК ограничивается квадратичной формой, тогда как новая литература устанавливает, что кубическая форма является более подходящей. В статье рассматривается вопрос о том, влияет ли на экономический рост на загрязнение окружающей среды, если да то как избежать противоречия в контексте Индии, с использованием годовых данных, охватывающих период с 1980 по 2017 годы. Тесты ADF показывают, что обе серии после логарифмического преобразования нестационарны на уровне и стационарны при первой разности. Данный результат подтверждает гипотезу и эмпирически доказывает, что выбросы на начальном этапе являются ограничивающим фактором экономического роста.
A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey
Creators: name: Dilday, Benjamin
name: Bassett, Bruce
name: Becker, Andrew
name: Bender, Ralf
name: Castander, Francisco
name: Cinabro, David
name: Frieman, Joshua A.
name: Galbany, Lluís
name: Garnavich, Peter
name: Goobar, Ariel
name: Hopp, Ulrich
name: Ihara, Yutaka
name: Jha, Saurabh W.
name: Kessler, Richard
name: Lampeitl, Hubert
name: Marriner, John
name: Miquel, Ramon
name: Mollá, Mercedes
name: Nichol, Robert C.
name: Nordin, Jakob
name: Riess, Adam G.
name: Sako, Masao
name: Schneider, Donald P.
name: Smith, Mathew
name: Sollerman, Jesper
name: Wheeler, J. Craig
name: Östman, Linda
name: Bizyaev, Dmitry
name: Brewington, Howard
name: Malanushenko, Elena
name: Malanushenko, Viktor
name: Oravetz, Dan
name: Pan, Kaike
name: Simmons, Audrey
name: Snedden, Stephanie
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: ABRIDGED We present measurements of the Type Ia supernova (SN) rate in galaxy clusters based on data from the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. The cluster SN Ia rate is determined from 9 SN events in a set of 71 C4 clusters at z <0.17 and 27 SN events in 492 maxBCG clusters at 0.1 < z < 0.3$. We find values for the cluster SN Ia rate of $({0.37}^{+0.17+0.01}_{-0.12-0.01}) \mathrm{SNu}r h^{2}$ and $({0.55}^{+0.13+0.02}_{-0.11-0.01}) \mathrm{SNu}r h^{2}$ ($\mathrm{SNu}x = 10^{-12} L_{x\sun}^{-1} \mathrm{yr}^{-1}$) in C4 and maxBCG clusters, respectively, where the quoted errors are statistical and systematic, respectively. The SN rate for early-type galaxies is found to be $({0.31}^{+0.18+0.01}_{-0.12-0.01}) \mathrm{SNu}r h^{2}$ and $({0.49}^{+0.15+0.02}_{-0.11-0.01})$ $\mathrm{SNu}r h^{2}$ in C4 and maxBCG clusters, respectively. The SN rate for the brightest cluster galaxies (BCG) is found to be $({2.04}^{+1.99+0.07}_{-1.11-0.04}) \mathrm{SNu}r h^{2}$ and $({0.36}^{+0.84+0.01}_{-0.30-0.01}) \mathrm{SNu}r h^{2}$ in C4 and maxBCG clusters. The ratio of the SN Ia rate in cluster early-type galaxies to that of the SN Ia rate in field early-type galaxies is ${1.94}^{+1.31+0.043}_{-0.91-0.015}$ and ${3.02}^{+1.31+0.062}_{-1.03-0.048}$, for C4 and maxBCG clusters. The SN rate in galaxy clusters as a function of redshift...shows only weak dependence on redshift. Combining our current measurements with previous measurements, we fit the cluster SN Ia rate data to a linear function of redshift, and find $r_{L} = $ $[(0.49^{+0.15}_{-0.14}) +$ $(0.91^{+0.85}_{-0.81}) \times z]$ $\mathrm{SNu}B$ $h^{2}$. A comparison of the radial distribution of SNe in cluster to field early-type galaxies shows possible evidence for an enhancement of the SN rate in the cores of cluster early-type galaxies... we estimate the fraction of cluster SNe that are hostless to be $(9.4^+8._3-5.1)%$.
description: 46 pages. ApJ in press. v2 fixes some references.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐµÑÐ¾ÑÐ°ÑÐ¼Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð·Ð¸Ð½, ÐÑÑÑÐ¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ñ
Ð¾Ð¿Ð»Ð°ÑÐ° ÑÑÑÐ´Ð°
Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ

description: Ð¦ÐµÐ»Ð¸ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸Ð»Ð¸ ÐµÐ³Ð¾ ÑÑÑÑÐºÑÑÑÑ: ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, ÑÑÐµÑ Ð³Ð»Ð°Ð², Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ñ. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÐºÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸, Ð²Ð¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐ´Ð¾Ð²ÑÑ ÑÐµÑÑÑÑÐ¾Ð² ÐÐÐ Â«ÐÐµÑÐ¾ÑÐ°ÑÐ¼Â». Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð´Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐÐÐ Â«ÐÐµÑÐ¾ÑÐ°ÑÐ¼Â».
More time to fly: with a warming climate the Western honey bee (Apis mellifera, Linnaeus) now has more temperature-eligible flight hours than 40 years ago
Creators: name: Rogers, Richard
name: Hassler, Edgar
name: Carey, Quinn
name: Cazier, Joseph
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: There have been official NOAA and EPA reports of measurable changes in temperature across the United States over the last several decades with average temperatures increasing in most areas and decreasing in a few others. In order to fly, honey bees need optimal temperatures ranging from 13 °C (55 °F) to 38 °C (100 °F), sunlight, low wind, and no rain. This study looks at changes in temperature-eligible flight times of honey bees across the US and Canada. Four decades of weather data from 60 locations in the US and Canada for the period 1980 through 2019 were analyzed. We discovered that honey bee flight hours are increasing almost everywhere, but most dramatically in the northern regions of Canada and Alaska, and also in a few locations in the US south of the border with Canada. Warming temperatures (ignoring all other factors), may lead to more flight time for honey bees; may affect plant bloom times and species distributions; and may change the exposure of honey bee colonies to pests, parasites, and pathogens. Therefore, beekeepers must be prepared to modify management practices to accommodate possible plant–pollinator mismatches and timings for seasonal and pest management. This study highlights that a warming climate will increase temperature-eligible flight hours for honey bees. Further research is needed to consider how other climate change factors, in combination with temperature, will affect actual honey bee flight opportunities and behavior, as well as, overall colony management.
A subset of wild bee species boosts the pollination of pigeon pea (Cajanus cajan: Fabaceae), an important crop plant of Cameroon
Creators: name: Mazi, Sanda
name: Paxton, Robert J.
name: Osterman, Julia
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Cell Biology
subject: Neuroscience
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Plant Biology

description: Bee species are thought to vary in their pollination efficiency, but they are rarely compared, particularly in the tropics. Here we determined the role in the pollination of 13 native bee species (Apis mellifera and 12 other wild bee species) when visiting pigeon pea (Cajanus cajan) flowers across two growing seasons in Cameroon. Using observations of floral visits coupled with a field experiment to quantify single-visit pollination efficiency, we found that Chalicodoma rufipes was the most efficient pollinator and most abundant flower visitor of pigeon pea. Most other flower visitors, including Apis mellifera, detracted from pigeon pea seed set. Our study highlights the importance of quantifying pollination to reveal functionally important bee species.
Solving the angular momentum problem in the cold feedback mechanism of cooling flows
Creators: name: Pizzolato, Fabio
name: Soker, Noam
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We show that cold clumps in the intra--cluster medium (ICM) efficiently lose their angular momentum as they fall in, such that they can rapidly feed the central AGN and maintain a heating feedback process. Such cold clumps are predicted by the cold feedback model, a model for maintaining the ICM in cooling flows hot by a feedback process. The clumps very effectively lose their angular momentum in two channels: the drag force exerted by the ICM and the random collisions between clumps when they are close to the central black hole. We conclude that the angular momentum cannot prevent the accretion of the cold clumps, and the cold feedback mechanism is a viable model for a feedback mechanism in cooling flows. Cold feedback does not suffer from the severe problems of models that are based on the Bondi accretion.
description: Submitted to MNRAS; corrected an error in a numerical procedure, conclusions unchanged; any comment welcome
Spanning Forests on Random Planar Lattices
Creators: name: Caracciolo, Sergio
name: Sportiello, Andrea
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Lattice (hep-lat)
subject: Mathematical Physics (math-ph)
subject: Combinatorics (math.CO)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: The generating function for spanning forests on a lattice is related to the q-state Potts model in a certain q -> 0 limit, and extends the analogous notion for spanning trees, or dense self-avoiding branched polymers. Recent works have found a combinatorial perturbative equivalence also with the (quadratic action) O(n) model in the limit n -> -1, the expansion parameter t counting the number of components in the forest. We give a random-matrix formulation of this model on the ensemble of degree-k random planar lattices. For k = 3, a correspondence is found with the Kostov solution of the loop-gas problem, which arise as a reformulation of the (logarithmic action) O(n) model, at n = -2. Then, we show how to perform an expansion around the t = 0 theory. In the thermodynamic limit, at any order in t we have a finite sum of finite-dimensional Cauchy integrals. The leading contribution comes from a peculiar class of terms, for which a resummation can be performed exactly.
description: 43 pages, Dedicated to Edouard Brezin and Giorgio Parisi, on the occasion of their special birthday
VariCS Data Collection Instruments
Creators: name: Cleland, Joanne
name: Stuart-Smith, Jane
name: Taylor, Lauren
name: Kuschmann, Anja
name: Smith, Amy
name: Mridhula Murali
Publisher: name: OSF
Year: 2024

description: Participant information sheets and consent forms for the main project as well as the ultrasound project; Demographic information questionnaire for the project
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸ÑÐ° Ð·Ð°Ð¼ÐµÑÐ¾Ðº Ñ ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð½Ð° ÑÑÐ¾ÑÐ¾Ð½Ðµ ÐºÐ»Ð¸ÐµÐ½ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð»Ð°Ð³Ð°ÐµÐ², ÐÑÑÐµÐ¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸Ñ
Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¸Ð½ÑÐµÑÑÐµÐ¹Ñ
Ð¸ÑÑ Ð¾Ð´Ð½ÑÐ¹ ÐºÐ¾Ð´
Ð°ÑÑ Ð¸ÑÐµÐºÑÑÑÐ° ÑÐµÑÐµÐ½Ð¸Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð° Ð¾ÑÐºÑÑÑÐ¾Ð³Ð¾ Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸ÑÐ° Ð·Ð°Ð¼ÐµÑÐ¾Ðº Ñ ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð½Ð° ÐºÐ»Ð¸ÐµÐ½ÑÑÐºÐ¾Ð¹ ÑÑÐ¾ÑÐ¾Ð½Ðµ. ÐÐ´Ðµ Ð² Ð²Ð¸Ð´Ðµ ÐºÐ»ÑÑÐ° ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ Ð¿Ð°ÑÐ¾Ð»Ñ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»Ñ. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÐµÑÐ²Ð¸ÑÐ° Ð·Ð°Ð¼ÐµÑÐ¾Ðº Ñ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ¾Ð¼, Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸ÐµÐ¹ Ð² ÑÐµÑÐ¸ Ð¸Ð½ÑÐµÑÐ½ÐµÑ Ð¸ Ð¾ÑÐºÑÑÑÑÐ¼ Ð¸ÑÑÐ¾Ð´Ð½ÑÐ¼ ÐºÐ¾Ð´Ð¾Ð¼.
Dynamical mass segregation on a very short timescale
Creators: name: Allison, R. J.
name: Goodwin, S. P.
name: Parker, R. J.
name: de Grijs, R.
name: Zwart, S. F. Portegies
name: Kouwenhoven, M. B. N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We discuss the observations and theory of star cluster formation to argue that clusters form dynamically cool (subvirial) and with substructure. We then perform an ensemble of simulations of cool, clumpy (fractal) clusters and show that they often dynamically mass segregate on timescales far shorter than expected from simple models. The mass segregation comes about through the production of a short-lived, but very dense core. This shows that in clusters like the Orion Nebula Cluster the stars >4 Msun can dynamically mass segregate within the current age of the cluster. Therefore, the observed mass segregation in apparently dynamically young clusters need not be primordial, but could be the result of rapid and violent early dynamical evolution.
description: ApJ Letter, accepted
title: Ð ÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¦ÐµÐ½ÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¢Ð­Ð¦
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ÑÐ¾Ð², ÐÐ¸ÑÐ°Ð¸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¢ÐµÐ¿Ð»Ð¾Ð²ÑÐµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸
ÐÐ°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð¦ÐµÐ½ÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¢Ð­Ð¦, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ°Ñ Ð·Ð°Ð¼ÐµÐ½Ð¸ÑÑ ÑÑÐ°ÑÐ¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ²ÐµÐ»Ð¸ÑÐ¸ÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÑÑ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑ ÑÑÐ°Ð½ÑÐ¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐ¾ÐºÐ¾Ð² ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ Ð² Ð³Ð»Ð°Ð²Ð½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐµÐ¼Ðµ Ð¸ ÑÑÐµÐ¼Ðµ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´ ÑÑÐ°Ð½ÑÐ¸Ð¸. ÐÑÐ±ÑÐ°Ð½Ð¾ Ð³Ð»Ð°Ð²Ð½Ð¾Ðµ ÑÐ¸Ð»Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸, ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐ±ÑÐ°Ð½Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð² ÑÑÐµÐ¼Ðµ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð²Ð¾Ð¿ÑÐ¾Ñ Ð¿ÑÑÐºÐ° ÐÐ¢Ð£. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¾ÑÑÐ°Ð½Ñ ÑÑÑÐ´Ð° Ð¸ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐµÐ±ÐµÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð½Ð° Ð¢Ð­Ð¦.