cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Observation of muon intensity variations by season with the MINOS far detector
Creators: name: The MINOS Collaboration
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The temperature of the upper atmosphere affects the height of primary cosmic ray interactions and the production of high-energy cosmic ray muons which can be detected deep underground. The MINOS far detector at Soudan MN, USA, has collected over 67 million cosmic ray induced muons. The underground muon rate measured over a period of five years exhibits a 4% peak-to-peak seasonal variation which is highly correlated with the temperature in the upper atmosphere. The coefficient, $α_T$, relating changes in the muon rate to changes in atmospheric temperature was found to be: $α_T = 0.874 \pm 0.009$ (stat.) $\pm 0.010$ (syst.). Pions and kaons in the primary hadronic interactions of cosmic rays in the atmosphere contribute differently to $α_T$ due to the different masses and lifetimes. This allows the measured value of $α_T$ to be interpreted as a measurement of the K/$π$ ratio for $E_{p}\gtrsim$\unit[7]{TeV} of $0.13 \pm 0.08$, consistent with the expectation from collider experiments.
description: 8 pages, 9 figures, accepted for publication in Phys. Rev. D
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¹ ÑÐµÐ¿ÑÑÐ°ÑÐ¸Ð¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼Ð¸ PR (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐºÐ½Ð¸Ð¶Ð½Ð¾Ð³Ð¾ Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð´ÐµÑÑÐºÐ¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Â«ÐÐ¾Ð»ÑÐ½Ð´ÑÐ¸ÑÂ»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¸Ð¿Ð¾Ð²Ð°, 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: 2016
Subjects: ÑÐ²ÑÐ·Ð¸ Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑÑ
Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð¾
Ð¿Ð°Ð±Ð»Ð¸ÑÐ¸ÑÐ¸
public relations
publishing house
publicity

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð½Ð° ÑÐµÐ¼Ñ Â«Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¹ ÑÐµÐ¿ÑÑÐ°ÑÐ¸Ð¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼Ð¸ PR (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐºÐ½Ð¸Ð¶Ð½Ð¾Ð³Ð¾ Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð´ÐµÑÑÐºÐ¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Â«ÐÐ¾Ð»ÑÐ½Ð´ÑÐ¸ÑÂ»)Â» Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ¸ ÑÐ°Ð±Ð¾ÑÑ PR-ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ° Ð½Ð°Ð´ ÑÐµÐ¿ÑÑÐ°ÑÐ¸ÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐµÐ¹ÑÑ ÐºÐ½Ð¸Ð³Ð¾Ð¿ÐµÑÐ°ÑÐ°Ð½Ð¸ÐµÐ¼. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÑÐ½ÐºÐ° ÐºÐ½Ð¸Ð³Ð¾Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ, Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¾ÑÑÐ°ÑÐ»Ð¸. Ð Ð·Ð°ÐºÐ»ÑÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð´Ð°Ð½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ PR-Ð¾ÑÐ´ÐµÐ»Ð° Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Â«ÐÐ¾Ð»ÑÐ½Ð´ÑÐ¸ÑÂ».
description: The research paper titled "Formation of goodwill profit organization means PR (on the example of book publishers of children's literature" Polyandriya ")" conducted a study the specifics of PR-specialist at a reputable company engaged in the printing press. The main ways of doing this activity in the conditions of the Russian publishing market, problems and development trends of the industry. The final part of the final qualification paper are proposals to improve the functioning of PR-department "Polyandriya" publishing.
title: Ð£ÑÐµÑ Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ°
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¾Ð»Ð¾Ð²ÑÐ¾Ð²Ð°, ÐÐºÐ°ÑÐµÑ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: 2016
Subjects: ÑÑÐµÑ Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹
ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ð¹ Ð±Ð°Ð½Ðº

description: Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð°Ñ Ð±Ð°Ð·Ð° Ð¿Ð¾ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð°Ð¼ ÑÑÐµÑÐ° Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ°. ÐÑÐ¾ÑÐ°Ñ Ð³Ð»Ð°Ð²Ð° ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÑÑ ÑÐ°Ð±Ð¾ÑÑ, ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð· Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐ°ÑÑÐµÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð±Ð°Ð½ÐºÐ°, ÑÑÐµÑ Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð»Ð¸Ñ Ð² ÐÐÐ ÐÐÐ¡ÐÐÐÐÐÐÐ. Ð¢ÑÐµÑÑÑ Ð³Ð»Ð°Ð²Ð° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¸ Ð¼Ð½ÐµÐ½Ð¸Ðµ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ Ð² ÐÐÐ ÐÐÐ¡ÐÐÐÐÐÐÐ.
title: Ð¤Ð¸ÐºÑÐ°ÑÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾ Ð²Ð½ÐµÑÐ½ÐµÐ¼ Ð¾Ð±Ð»Ð¸ÐºÐµ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ° Ð¸ ÐºÑÐ¸Ð¼Ð¸Ð½Ð°Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ ÑÑÐ´ÐµÐ±Ð½Ð¾-Ð¿Ð¾ÑÑÑÐµÑÐ½Ð¾Ð¹ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÑÐ½, Ð Ð¾Ð·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: ÑÐ¾ÑÐ¾ÑÐ¸ÐºÑÐ°ÑÐ¸Ñ
Ð²Ð¸Ð´ÐµÐ¾ÑÐ¸ÐºÑÐ°ÑÐ¸Ñ
Ð²Ð½ÐµÑÐ½Ð¸Ð¹ Ð¾Ð±Ð»Ð¸Ðº ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°
ÑÐ»Ð¾Ð²ÐµÑÐ½ÑÐ¹ Ð¿Ð¾ÑÑÑÐµÑ
ÑÑÐ´ÐµÐ±Ð½Ð¾-Ð¿Ð¾ÑÑÑÐµÑÐ½Ð°Ñ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð°

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑ ÑÐµÐ¼Ñ ÑÐ¸ÐºÑÐ°ÑÐ¸Ð¸ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ Ð¾Ð±Ð»Ð¸ÐºÐ° ÑÐµÐ»Ð¾Ð²ÐµÐºÐ° Ð¸ ÐºÑÐ¸Ð¼Ð¸Ð½Ð°Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ ÑÑÐ´ÐµÐ±Ð½Ð¾-Ð¿Ð¾ÑÑÑÐµÑÐ½Ð¾Ð¹ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ. ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð²Ð½ÐµÑÐ½Ð¸Ð¹ Ð¾Ð±Ð»Ð¸Ðº ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°. ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â Ð²Ð¸Ð´Ñ ÑÐ¸ÐºÑÐ°ÑÐ¸Ð¸ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ Ð¾Ð±Ð»Ð¸ÐºÐ° ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°, Ð° Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸ â ÑÐ»Ð¾Ð²ÐµÑÐ½ÑÐ¹ Ð¿Ð¾ÑÑÑÐµÑ. ÐÑ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼ ÑÐ°ÐºÐ¸Ðµ Ð²Ð¸Ð´Ñ ÑÐ¸ÐºÑÐ°ÑÐ¸Ð¸ Ð²Ð½ÐµÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°Ðº ÑÐ¾ÑÐ¾-, Ð²Ð¸Ð´ÐµÐ¾Ð·Ð°Ð¿Ð¸ÑÑ, ÑÑÐ±ÑÐµÐºÑÐ¸Ð²Ð½ÑÐ¹ Ð¿Ð¾ÑÑÑÐµÑ, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¿Ð¾ Ð¿ÑÐ°Ð²Ð¸Ð»Ð°Ð¼ ÑÐ»Ð¾Ð²ÐµÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÑÐµÑÐ°, Ð±Ð¾Ð»ÐµÐµ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ ÑÐ°ÑÐºÑÑÐ²Ð°Ñ Ð¿Ð¾ÑÐ»ÐµÐ´Ð½Ð¸Ð¹ Ð¸Ð· Ð½Ð°Ð·Ð²Ð°Ð½ÑÑ Ð²Ð¸Ð´ ÑÐ¸ÐºÑÐ°ÑÐ¸Ð¸ Ð²Ð½ÐµÑÐ½Ð¾ÑÑÐ¸. ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ°Ðº Ð¶Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, Ð³Ð°Ð±Ð¸ÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸ Ð¸ Ð¸ÑÐµÑ Ð¿ÑÑÐ¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² ÑÐ¸ÐºÑÐ°ÑÐ¸Ð¸ Ð¸ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð²Ð½ÐµÑÐ½Ð¾ÑÑÐ¸.
Additional file 6 of Prognostic risk factors of serous ovarian carcinoma based on mesenchymal stem cell phenotype and guidance for therapeutic efficacy
Creators: name: Yang, Xiaohui
name: Zheng, Minying
name: Ning, Yidi
name: Sun, Jie
name: Yu, Yongjun
name: Zhang, Shiwu
Publisher: name: figshare
Year: 2023
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Additional file 6. Protocol for reverse transcription and real-time polymerase chain reaction. Details for reverse transcription and real-time polymerase chain reaction.
High order discretization methods for spatial-dependent SIR models
Creators: name: Takács, Bálint
name: Hadjimichael, ##!Error: Attribute  Unknown!##
Publisher: name: Weierstrass Institute
Year: 2021
Subjects: subject: epidemic models
subject: SIR model
subject: integro-differential equations
subject: strong stability preservation
subject: 5M12
subject: 65L07
subject: 65L06
subject: 91D25

description: In this paper, an SIR model with spatial dependence is studied and results regarding its stability and numerical approximation are presented. We consider a generalization of the original Kermack and McKendrick model in which the size of the populations differs in space. The use of local spatial dependence yields a system of integro-differential equations. The uniqueness and qualitative properties of the continuous model are analyzed. Furthermore, different choices of spatial and temporal discretizations are employed, and step-size restrictions for population conservation, positivity, and monotonicity preservation of the discrete model are investigated. We provide sufficient conditions under which high order numerical schemes preserve the discrete properties of the model. Computational experiments verify the convergence and accuracy of the numerical methods.
Topological phase transitions driven by gauge fields in an exactly solvable model
Creators: name: Lahtinen, Ville
name: Pachos, Jiannis K.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We demonstrate the existence of a new topologically ordered phase in Kitaev's honeycomb lattice model. This new phase appears due to the presence of a vortex lattice and it supports chiral Abelian anyons. We characterize the phase by its low-energy behavior that is described by a distinct number of Dirac fermions. We identify two physically distinct types of topological phase transitions and obtain analytically the critical behavior of the extended phase space. The Fermi surface evolution associated with the transitions is shown to be due to the Dirac fermions coupling to chiral gauge fields. Finally, we describe how the new phase can be understood in terms of interactions between the anyonic vortices.
description: 5 pages, 5 figures, published version
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸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Ð°Ð±Ð°ÐµÐ²Ð°, ÐÐ°Ð»ÐµÑ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: 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¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°
ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÑ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸
Ð¼Ð°ÑÐ¶Ð° Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¡ÐÐÐ Â«Ð ÐµÑÐ¾-ÐÐ°ÑÐ°Ð½ÑÐ¸ÑÂ».
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°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¡ÐÐÐ Â«Ð ÐµÑÐ¾-ÐÐ°ÑÐ°Ð½ÑÐ¸ÑÂ» Ð´Ð»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ.
ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¡ÐÐÐ Â«Ð ÐµÑÐ¾-ÐÐ°ÑÐ½ÑÐ¸ÑÂ». Ð¡ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÐ¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ 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Ð»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¡ÐÐÐ Â«Ð ÐµÑÐ¾-ÐÐ°ÑÐ°Ð½ÑÐ¸ÑÂ».
ÐÑÐ»Ð° Ð¾ÑÐµÐ½ÐµÐ½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¡ÐÐÐ Â«Ð ÐµÑÐ¾-ÐÐ°ÑÐ°Ð½ÑÐ¸ÑÂ».
Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Additional file 1 of BUTTERFLY: addressing the pooled amplification paradox with unique molecular identifiers in single-cell RNA-seq
Creators: name: Gustafsson, Johan
name: Robinson, Jonathan
name: Nielsen, Jens
name: Pachter, Lior
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Supplementary information.
Probing the Warm Dark Matter with High-z Quasar Luminosity Function
Creators: name: Song, Hyunmi
name: Lee, Jounghun
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In a warm dark matter (WDM) cosmology, the first objects to form at z>=20 are one dimensional filaments with mean length on the order of the WDM free-streaming scale. Gao and Theuns recently claimed by using high-resolution hydrodynamic simulations that the eventual collapse of these WDM filaments along their longest axes may seed the supermassive black holes that power high-z quasars. In this picture, it is supposed that the high-z quasar luminosity function should reflect how abundant the WDM filaments are in the early universe. We derive analytically the mass function of early-universe filaments with the help of the Zel'dovich approximation. Then, we determine the rate of its decrease in the mass section corresponding to the free streaming scale of a WDM particle of mass m_v. Adjusting the value of m_v, we fit the slope of the analytic model to that of the high-z quasar luminosity function measured from the Sloan Digital Sky Survey DR3. A new WDM constraint from this feasibility study is found to be consistent with the lightest super-symmetric partner.
description: ApJL in press, revised version, figure 1 replotted correctly, discussion improved, 4 pages, 2 figures
title: ÐÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ ÐºÐ¾ÑÐ°Ð±Ð»ÐµÐ¹ Ð¸ ÑÑÐ´Ð¾Ð². ÐÑÐ¸ÑÐµÑÐ¸Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐ¾Ð²ÑÐºÐ¸Ð¹, ÐÐ³Ð¾ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¡ÑÐ´Ð° Ð¼Ð¾ÑÑÐºÐ¸Ðµ
ÐÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°
Ð¾Ð¿Ð°ÑÐ½ÑÐµ Ð³ÑÑÐ·Ñ
ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÐµ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸ Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾ÑÐ°Ð±Ð»ÐµÐ¹ Ð¸ ÑÑÐ´Ð¾Ð², Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÐ¼ÑÐµ Ð´Ð»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐ¾ÐµÐºÑÐ½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð² ÐºÐ¾ÑÐ°Ð±Ð»ÐµÑÑÑÐ¾ÐµÐ½Ð¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ Ð¿Ð»Ð°Ð½Ð¾Ð² Ð½Ð° ÐºÐ¾ÑÐ°Ð±Ð»ÑÑ (ÑÑÐ´Ð°Ñ) Ð¸ Ð² Ð¼Ð¾ÑÑÐºÐ¸Ñ Ð¿Ð¾ÑÑÐ°Ñ. ÐÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÐºÐ°Ðº ÑÐ²Ð¾Ð¹ÑÑÐ²Ð¾ ÐºÐ¾ÑÐ°Ð±Ð»Ñ Ð¸Ð»Ð¸ ÑÑÐ´Ð½Ð°, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÐµÐµ ÑÑÐµÐ¿ÐµÐ½Ñ Ð·Ð°ÑÐ¸ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐºÐ¸Ð¿Ð°Ð¶Ð°, Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð¸ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ Ñ ÑÑÐµÑÐ¾Ð¼ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ Ð°Ð²Ð°ÑÐ¸Ð¹ Ð¸ Ð²Ð»Ð¸ÑÑÑÐµÐµ Ð½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾ÑÐ°Ð±Ð»Ñ (ÑÑÐ´Ð½Ð°). ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÐºÐ° ÐºÐ°Ðº ÐºÑÐ¸ÑÐµÑÐ¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð±Ð°Ð·Ðµ Ð Ð¤. ÐÐ±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº Ð¾ÑÐµÐ½ÐºÐµ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾ÑÐ°Ð±Ð»ÐµÐ¹ Ð¸ ÑÑÐ´Ð¾Ð², ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½ÑÑ ÐºÑÐ¸ÑÐµÑÐ¸ÐµÐ² Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸, ÑÑÐ¸ÑÑÐ²Ð°ÑÑÐ¸Ñ Ð²ÑÑ ÑÐ¾Ð²Ð¾ÐºÑÐ¿Ð½Ð¾ÑÑÑ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² ÑÐ¸ÑÐºÐ°, Ð¿ÑÐ¸ÑÑÑÐ¸Ñ Ð´Ð°Ð½Ð½ÑÐ¼ Ð¾Ð±ÑÐµÐºÑÐ°Ð¼.
New cosmological constraints on primordial black holes
Creators: name: Carr, B. J.
name: Kohri, Kazunori
name: Sendouda, Yuuiti
name: Yokoyama, Jun'ichi
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We update the constraints on the fraction of the Universe going into primordial black holes in the mass range 10^9--10^17 g associated with the effects of their evaporations on big bang nucleosynthesis and the extragalactic photon background. We include for the first time all the effects of quark and gluon emission by black holes on these constraints and account for the latest observational developments. We then discuss the other constraints in this mass range and show that these are weaker than the nucleosynthesis and photon background limits, apart from a small range 10^13--10^14 g, where the damping of cosmic microwave background anisotropies dominates. Finally we review the gravitational and astrophysical effects of nonevaporating primordial black holes, updating constraints over the broader mass range 1--10^50 g.
description: 41 pages, 10 figures, REVTeX 4.1
Analysing the form of the confined uniaxial compression curve of various soils
Creators: name: Tang, Anh-Minh
name: Cui, Yu-Jun
name: Eslami, Javad
name: Défossez, Pauline
Publisher: name: arXiv
Year: 2008
Subjects: subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: The soil compaction by vehicles is a major factor responsible for physical degradation of cultivated soils. Uniaxial confined compression tests are usually performed to characterise the compaction properties of soil. Two main forms of compression curve have been observed: (i) the bi-linear curve having an elastic rebound curve at low stresses and a linear virgin compression curve at higher stresses; (ii) the S-shaped curve having deviation of the virgin compression curve at high stresses. In the present work, uniaxial confined compression tests were performed on four soils having various textures and different plasticity. Tests were performed on undisturbed and remould samples, at various initial dry bulk densities and water contents. The S-shaped compression curves were observed more frequently when the clay content and/or the initial water content were high. In addition, the S-shaped curves were observed more frequently on remould soils than on undisturbed soils. The difference between the compression of air-filled pores and that of meso-pores storing water subjected to high capillary forces could explain the observed S-shaped curves.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÑÑÐµÑÐµ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð° Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«ÐÑÐ°Ð½ ÑÐ¸ÑÐµÐ¹Ð» Ð Ð¾ÑÑ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° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð©ÐµÑÐ±Ð¸Ð½Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð²ÑÐ¹ ÑÐ¸ÑÐµÐ¹Ð»
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¸ÑÐµÐ¹Ð»Ð° Â«ÐÑÐ°Ð½ ÑÐ¸ÑÐµÐ¹Ð» Ð Ð¾ÑÑÐ¸ÑÂ». Ð¦ÐµÐ»Ñ: Ð¿ÑÐ¾Ð²ÐµÑÑÐ¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð° Ð¸ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ Ð² ÑÐ¸ÑÑÐ¾Ð²ÑÑ ÑÐ¿Ð¾ÑÑ Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«ÐÑÐ°Ð½ ÑÐ¸ÑÐµÐ¹Ð» Ð Ð¾ÑÑÐ¸ÑÂ» Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÑ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ Ð´Ð»Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ½ÐºÐ° Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ Â«ÐÑÐ°Ð½ ÑÐ¸ÑÐµÐ¹Ð» Ð Ð¾ÑÑÐ¸ÑÂ». ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÑ ÑÐ¸Ð» ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, ÑÐ´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð²ÑÑÑÑÐºÐ¸ Ð¸ Ð·Ð°ÑÑÐ°Ñ Ð¿ÑÐ¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ð¸ Ð½Ð¾Ð²Ð¾Ð¹ CRM-ÑÐ¸ÑÑÐµÐ¼Ñ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐµÐµ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÑÐ½Ð½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð»Ð¾, ÑÑÐ¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð²ÑÐµ ÑÐ¸ÑÐµÐ¹Ð»Ñ ÑÑÑÐµÐ¼ÑÑÑÑ Ðº ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ CRM-ÑÐ¸ÑÑÐµÐ¼ Ð´Ð»Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Â¬Ð½Ð¸Ñ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, Ð´ÐµÐ»Ð°Ñ ÐµÑ Ð±Ð¾Ð»ÐµÐµ Ð³Ð¸Ð±ÐºÐ¾Ð¹ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð² ÑÐ»Ð¾Ð¶Ð¸Ð²ÑÐµÐ¹ÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸. ÐÐ¸ÑÐ¾Ð²Ð¾Ð¹ Ð¾Ð¿ÑÑ Ð¿Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð²Ð½Ð¸Ð¼Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ CRMâÑÐ¸ÑÑÐµÐ¼ Ð²Ð¾ Ð¼Ð½Ð¾Ð³Ð¸Ðµ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÐ¾Ð²ÐµÐ¹ÑÐ¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, ÑÐ°Ð±Ð¾ÑÐ°ÑÂ¬ÑÐ¸Ðµ Ð½Ð° Ð¿ÑÐ¾Ð´ÑÐºÐ¾Ð²Ð¾Ð¼ ÑÑÐ½ÐºÐµ, Ð¼Ð¾Ð³ÑÑ Ð´Ð¾ÑÑÐ¸ÑÑ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ Ð¸ Ð²ÑÑÐµÑÂ¬Ð½Ð¸ÑÑ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð²ÑÐµ ÑÐ¸ÑÐµÐ¹Ð»Ñ, Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÑÑ ÐºÐ»Ð¸ÐµÐ½ÑÐ°Ð¼ Ð±Ð¾Ð»ÐµÐµ ÑÐ´Ð¾Ð±Ð½ÑÐµ Ð¸ Ð±ÑÑÑÑÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÑ Ð¸ ÑÑÐ»ÑÐ³Ð¸.
How do galaxies populate Dark Matter halos?
Creators: name: Guo, Qi
name: White, Simon
name: Li, Cheng
name: Boylan-Kolchin, Michael
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: For any assumed stellar Initial Mass Function, the Sloan Digital Sky Survey (SDSS) gives a precise determination of the stellar mass function of galaxies for 10^8 M_sun < M_* < 10^12 M_sun. Within the concordance LCDM cosmology, the Millennium simulations give a precise halo mass function for all halos within which galaxies can form. Under the plausible hypothesis that the stellar mass of a galaxy is an increasing function of the maximum mass ever attained by its halo, these combine to give halo mass as a function of stellar mass. The result agrees quite well with observational estimates of mean halo mass as a function of stellar mass from stacking analyses of the gravitational lensing signal and the satellite dynamics of SDSS galaxies. For M_* ~ 5.5 x 10^10 M_sun, the stellar mass usually assumed for the Milky Way, the implied halo mass is ~ 2 x 10^12 M_sun, consistent with most recent direct estimates and inferences from the MW/M31 Timing Argument. The fraction of the baryons associated with each halo which are present as stars in its central galaxy reaches a maximum of 20% at masses somewhat below that of the Milky Way, and falls rapidly at both higher and lower masses. These conversion efficiencies are lower than in almost all recent high-resolution simulations of galaxy formation, showing that these are not yet viable models for the formation of typical members of the galaxy population. When inserted in the Millennium-II Simulation, our derived relation between stellar mass and halo mass predicts a stellar mass autocorrelation function in excellent agreement with that measured directly in the SDSS. The implied Tully-Fisher relation also appears consistent with observation, suggesting that galaxy luminosity functions and Tully-Fisher relations can be reproduced simultaneously in a LCDM cosmology.
description: 11 pages, 7 figures; revisions to both text and figures; matches version submitted to MNRAS
title: ÐÐ¸ÑÐ¾Ð²Ð¾Ð¹ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ ÑÑÐ½Ð¾Ðº. Ð¢ÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸, Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð° Ð Ð¾ÑÑÐ¸Ð¸ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼Ð¸ Ð²Ð°Ð»ÑÑÐ½Ð¾-ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¼Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÐ¼Ð¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ¤ Ð¸ ÐÐÐÐ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¢ÑÐ±Ð°Ð½Ð¾Ð²Ð° , ÐÐ»Ñ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: 2016
Subjects: Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð¹ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ ÑÑÐ½Ð¾Ðº
ÐºÑÐµÐ´Ð¸ÑÐ½ÑÐ¹ ÑÑÐ½Ð¾Ðº
ÐºÑÐµÐ´Ð¸Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ°, Ð²Ð°Ð»ÑÑÐ½Ð¾Ð³Ð¾ Ð¸ ÐºÑÐµÐ´Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ¾Ð². ÐÐ·ÑÑÐµÐ½Ð° Ð¸ÑÑÐ¾ÑÐ¸Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð° ÐÐÐ¤ Ð¸ ÐÐÐÐ Ñ Ð Ð¾ÑÑÐ¸ÐµÐ¹. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¹ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð Ð¾ÑÑÐ¸Ð¸ Ñ ÐÐÐ¤ Ð¸ ÐÐÐÐ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð²ÑÐ±Ð¾ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð° Ð Ð¾ÑÑÐ¸Ð¸ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼Ð¸ Ð²Ð°Ð»ÑÑÐ½Ð¾-ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¼Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÐ¼Ð¸.
Generalized Lee-Wick Formulation from Higher Derivative Field Theories
Creators: name: Cho, Inyong
name: Kwon, O-Kab
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study a higher derivative (HD) field theory with an arbitrary order of derivative for a real scalar field. The degree of freedom for the HD field can be converted to multiple fields with canonical kinetic terms up to the overall sign. The Lagrangian describing the dynamics of the multiple fields is known as the Lee-Wick (LW) form. The first step to obtain the LW form for a given HD Lagrangian is to find an auxiliary field (AF) Lagrangian which is equivalent to the original HD Lagrangian up to the quantum level. Till now, the AF Lagrangian has been studied only for N=2 and 3 cases, where $N$ is the number of poles of the two-point function of the HD scalar field. We construct the AF Lagrangian for arbitrary $N$. By the linear combinations of AF fields, we also obtain the corresponding LW form. We find the explicit mapping matrices among the HD fields, the AF fields, and the LW fields. As an exercise of our construction, we calculate the relations among parameters and mapping matrices for $N=2,3$, and 4 cases.
description: 23 pages, version to appear in PRD, we improved the transformation from HD to LW in Subsection 3.1, added comments on gauge field related with AF Lagrangians in Conclusion, and added references
title: ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°ÐºÑÐ¸ÐºÐ¾-ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð² ÑÐ¸ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð²Ð¸Ð´Ð°Ñ ÑÐ¿Ð¾ÑÑÐ° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ
title: Features of tactical and technical training in situational sports on the basis of coordination motor tasks
Creators: name: Ð¡Ð°Ð²Ð¸Ð½ÑÐºÐ¸Ð¹, ÐÐµÑÑ
name: Ð Ð¾Ð¼Ð°Ð½Ð¾Ð², ÐÐ°ÑÐ¸Ð»Ð¸Ð¹
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐ°ÐºÑÐ¸ÐºÐ°
ÑÐµÑ Ð½Ð¸ÐºÐ°
ÑÐ¸ÑÑÐ°ÑÐ¸Ñ
ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°ÑÐ¸Ñ
Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ
tactics
technique
situation
coordination
information

description: Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð¸ ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ²Ð¸Ð´ÐµÑÐµÐ»ÑÑÑÐ²ÑÑÑ, ÑÑÐ¾ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÑÐºÑÑÑÑ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð³Ð¾ÑÐ¾Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð° Ðº ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ Ð´Ð°ÐµÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð´Ð¸ÑÑÐµÑÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°ÑÑ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÐºÑÐ¸ÐºÐ¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸. ÐÑÐ¸ ÑÑÐ¾Ð¼ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°ÑÐ¿ÐµÐºÑ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ñ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð° ÑÐ¼ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÑÐ½ÑÐµ Ð·Ð°Ð´Ð°ÑÐ¸. ÐÐ°Ð½Ð½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÐ°ÐºÑÐ¸ÐºÐ¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸, ÑÑÐ¾ ÑÐºÐ°Ð·ÑÐ²Ð°ÐµÑÑÑ Ð½Ð° ÑÐ»ÑÑÑÐµÐ½Ð¸Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸.
description: The results of the study of training and competitive activities indicate that the assessment of the structure of the athleteâs integral readiness for competitions makes it possible to differentiate the process of improving tactical and technical training. At the same time, the pedagogical aspect of training activity consists in the methodically consistent formation of the athleteâs ability to coordinate motor tasks. This approach allows you to significantly increase the level of tactical and technical readiness, which affects the improvement of the effectiveness of competitive activity.
Additional file 10 of Prognostic risk factors of serous ovarian carcinoma based on mesenchymal stem cell phenotype and guidance for therapeutic efficacy
Creators: name: Yang, Xiaohui
name: Zheng, Minying
name: Ning, Yidi
name: Sun, Jie
name: Yu, Yongjun
name: Zhang, Shiwu
Publisher: name: figshare
Year: 2023
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Additional file 10. KEGG pathway analysis between low and high MSC score group. KEGG pathway analysis of DEGs between groups with low and high MSC scores.
Mapping the available evidence on the impact of ingested live microbes on health: a scoping review protocol
Creators: name: Mukherjee, Arghya
name: Iyer, Ajay
name: Gómez-Sala, Beatriz
name: O'CONNOR, EIBHLIS
name: G Kenny, John
name: D Cotter, Paul
Publisher: name: University of Limerick
Year: 2023
Subjects: subject: Biological sciences
subject: FOS: Biological sciences

description: Introduction It has been hypothesised that the regular consumption of safe, live microbes confers health-promoting attributes, including the prevention of disease. To address this hypothesis, we propose a scoping review approach that will systematically assess the large corpus of relevant literature that is now available on this research topic. This article outlines a protocol for a scoping review of published studies on interventions with live microbes in non-patient populations across eight health categories. The scoping review aims to catalogue types of interventions, measured outcomes, dosages, effectiveness, as well as current research gaps. Methods and analysis The scoping review will follow the six-staged protocol as proposed by Arksey and O’Malley and will include the following stages: defining the research questions (stage 1); defining the eligibility criteria and finalising search strategy (stage 2); selection of studies based on the eligibility criteria (stage 3); development of a data extraction framework and charting of data (stage 4); aggregation of results and summarisation of findings (stage 5); and the optional consultation with stakeholders (stage 6), which will not be performed. Ethics and dissemination Since the scoping review synthesises information from existing literature, no separate ethical approval is required. The findings of the scoping review will be communicated for publication to an open-access, peer-reviewed scientific journal, presented at relevant conferences, and disseminated at future workshops with all relevant data and documents being available online through the Open Science Framework (https://osf.io/kvhe7).
title: ÐÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÐºÑÑ Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¸Ð½Ð¾ÑÐ·ÑÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÐÐ¸ÑÐ°Ðµ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¨Ð°Ð½Ñ Ð°Ðµ)
title: Historical facts and modern tendencies in foreign language educational system of China (on the example of Shanghai)
Creators: name: ÐÐ¾ÑÑÐ¼ÐºÐ¸Ð½Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐµ ÑÐ·ÑÐºÐ¸
Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ

description: Education is usually seen as an achieved factor, but its attainment is unavoidably affected by peopleâs social origins or ascribed factors which leads to the specific traditions in educational systems of different countries.
The dilution peak, metallicity evolution, and dating of galaxy interactions and mergers
Creators: name: Montuori, M.
name: Di Matteo, P.
name: Lehnert, M. D.
name: Combes, F.
name: Semelin, B.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Strong inflows of gas from the outer disk to the inner kiloparsecs are induced during the interaction of disk galaxies. This inflow of relatively low-metallicity gas dilutes the metallicity of the circumnuclear gas. We have investigated several aspects of the process as the timing and duration of the dilution and its correlation with the induced star formation. We analysed major (1:1) gas-rich interactions and mergers, spanning a range of initial orbital characteristics. Star formation and metal enrichment from SNe are included in our model. Our results show that the strongest trend is between the star formation rate and the dilution of the metals in the nuclear region; i.e., the more intense the central burst of star formation, the more the gas is diluted. This trend comes from strong inflows of relatively metal-poor gas from the outer regions of both disks, which fuels the intense star formation and lowers the overall metallicity for a time. The strong inflows happen on timescales of about 10^8 years or less, and the most intense star formation and lowest gas phase metallicities are seen generally after the first pericentre passage. As the star formation proceeds and the merger advances, the dilution reduces and enrichment becomes dominant - ultimately increasing the metallicity of the circumnuclear gas to a level higher than the initial metallicities of the merging galaxies. The "fly-bys" - pairs that interact but do not merge - also cause some dilution. We even see some dilution early in the merger or in the "fly-bys" and thus do not observe a strong trend between the nuclear metallicities and separation in our simulations until the merger is well advanced. We also analyse the O and Fe enrichment of the ISM, and show that the evolution of the alpha/Fe ratios, as well as the dilution of the central gas metallicity, can be used as a clock for "dating" the interaction.
description: 13 pages, 11 figures, A&A in press. Final version after language editing
The UN Global Compacts and the Common European Asylum System: Coherence or Friction?
Creators: name: Guild, Elspeth
name: Allinson, Kathryn
name: Busuttil, Nicolette
Publisher: name: Zenodo
Year: 2022
Subjects: PROTECT Consortium
Global Compacts
non-regression
non-discrimination
rule of law
human rights
Common European Asylum System (CEAS)

description: This paper examines the “protective potential” of the Global Compacts on Refugees and Migrants visà-vis existing commitments to fundamental rights within the European Union (EU). The relationship between the two normative frameworks is scrutinised to establish the extent to which the two might be mutually supportive or contradictory, since this determines the Compacts’ capacity to inform the interpretation of EU fundamental rights within the Common European Asylum System (CEAS). This paper explores this protective potential through three of the Compacts’ key guiding principles: respect for human rights and the rule of law, the principle of non-regression, and the principle of non-discrimination. The Compacts’ commitments to the first two are presented as sites of coherence where the Compacts concretely express pre-existing protections within EU law and provide a blueprint for implementation in the migration sphere. Yet, the Compacts’ principle of non-discrimination reveals an area of friction with EU primary law. It is argued that the implementation of this principle can address the inherently discriminatory system underpinning EU law. Within the EU, rather than undermining international and national human rights obligations, the Compacts present an opportunity to refine the implementation of existing EU fundamental rights obligations applicable to migrants and refugees.
Edge-State Velocity and Coherence in a Quantum Hall Fabry-Perot Interferometer
Creators: name: McClure, D. T.
name: Zhang, Yiming
name: Rosenow, B.
name: Levenson-Falk, E. M.
name: Marcus, C. M.
name: Pfeiffer, L. N.
name: West, K. W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We investigate nonlinear transport in electronic Fabry-Perot interferometers in the integer quantum Hall regime. For interferometers sufficiently large that Coulomb blockade effects are absent, a checkerboard-like pattern of conductance oscillations as a function of dc bias and perpendicular magnetic field is observed. Edge-state velocities extracted from the checkerboard data are compared to model calculations and found to be consistent with a crossover from skipping orbits at low fields to E x B drift at high fields. Suppression of visibility as a function of bias and magnetic field is accounted for by including energy- and field-dependent dephasing of edge electrons.
description: related papers at http://marcuslab.harvard.edu
title: ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÑÑÑÐ¸Ð·Ð¼Ðµ Ð¸ Ð¸Ð½Ð´ÑÑÑÑÐ¸Ð¸ Ð³Ð¾ÑÑÐµÐ¿ÑÐ¸Ð¸Ð¼ÑÑÐ²Ð°
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°ÑÐ°ÑÑÐµÐ½ÐºÐ¾, ÐÑÑ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: 2018
Subjects: ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð½Ð°Ð½Ð¸Ð¹
ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸
Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÑÑÐ½Ð¾ÑÑÐ¸
Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸Ñ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸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Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÑ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÑ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐµÑÐ²Ð¸ÑÐ° Ð¸ ÑÑÑÐ¸Ð·Ð¼Ð°, Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð°Ñ Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð´ÑÐºÑÐ° Ð´Ð»Ñ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
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ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
ÐÐ½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸, ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð·Ð°ÑÑÐ°Ñ Ð½Ð° ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸, ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð³ÐµÐ¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, ÐºÑÑÐ³Ð° ÐºÐ»Ð¸ÐµÐ½ÑÐ¾Ð², ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð·Ð°Ð³ÑÑÐ¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÐµÐ´Ð½ÐµÐ³Ð¾ ÑÐµÐºÐ° Ð½Ð° Ð¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°.
Adolescent sleep research in low- and middle-income countries: a scoping review protocol
Creators: name: Raniti, Monika
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Mental Disorders
subject: Maternal and Child Health
subject: Psychiatry and Psychology
subject: Public Health
subject: Medicine and Health Sciences
subject: Epidemiology
subject: Cognitive Behavioral Therapy
subject: Mental and Social Health
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology
subject: adolescent
subject: adolescents
subject: global health
subject: interventions
subject: LMIC
subject: paediatric
subject: pediatric
subject: population health
subject: programs
subject: sleep

description: This paper describes the protocol of a scoping review of sleep research in adolescents aged 10 to 24 years in low- and middle-income countries (LMICs) with the aim of synthesising the evidence base over the past decade. The objective of this scoping review is to understand the extent and type of peer-reviewed evidence in relation to: 1) the prevalence of sleep problems and disorders; 2) subjective sleep assessment measures; and 3) sleep interventions (including programs, treatments, and policies) for adolescents in LMICs. At the time of publication of this protocol on Open Science Framework, full-text article screening has been completed but data extraction is yet to commence.
Additional file 3 of BUTTERFLY: addressing the pooled amplification paradox with unique molecular identifiers in single-cell RNA-seq
Creators: name: Gustafsson, Johan
name: Robinson, Jonathan
name: Nielsen, Jens
name: Pachter, Lior
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3. Review history.
Clumps in the Outer Disk by Disk Instability: Why They are Initially Gas Giants and the Legacy of Disruption
Creators: name: Boley, Aaron C.
name: Hayfield, Tristen
name: Mayer, Lucio
name: Durisen, Richard H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We explore the initial conditions for fragments in the extended regions ($r\gtrsim 50$ AU) of gravitationally unstable disks. We combine analytic estimates for the fragmentation of spiral arms with 3D SPH simulations to show that initial fragment masses are in the gas giant regime. These initial fragments will have substantial angular momentum, and should form disks with radii of a few AU. We show that clumps will survive for multiple orbits before they undergo a second, rapid collapse due to H$_2$ dissociation and that it is possible to destroy bound clumps by transporting them into the inner disk. The consequences of disrupted clumps for planet formation, dust processing, and disk evolution are discussed. We argue that it is possible to produce Earth-mass cores in the outer disk during the earliest phases of disk evolution.
description: Accepted for publication in Icarus. The arguments have been greatly expanded (from v1) to address comments by the referees
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ»ÑÐ¶Ð±Ñ Ñ Ð¾ÑÐ³Ð°Ð½Ð°Ð¼Ð¸ Ð¾Ñ ÑÐ°Ð½Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾Ð¿Ð¾ÑÑÐ´ÐºÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ°Ð»Ð¸Ð½Ð¸Ð½ÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°)
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: ÐÐ°Ð²ÑÐ½, Ð®Ð»Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð£Ð¤ÐÐ¡
Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ñ
Ð¿Ð¾Ð»Ð¸ÑÐ¸Ñ
FMS
migration
police

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿Ð¾ÑÐ¾ÐºÐ¸ Ð±ÐµÐ¶ÐµÐ½ÑÐµÐ² Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð£Ð¤ÐÐ¡ ÐÐ°Ð»Ð¸Ð½Ð¸Ð½ÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° Ð³Ð¾ÑÐ¾Ð´Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³. ÐÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÑÑÐ´ ÑÐ»Ð¾Ð¶Ð¸Ð²ÑÐ¸ÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ»ÑÐ¶Ð±Ñ Ñ Ð¾ÑÐ³Ð°Ð½Ð°Ð¼Ð¸ Ð¾ÑÑÐ°Ð½Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ´ÐºÐ°, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾: 1. ÐÑÐ¸Ð½ÑÑÐ¸Ðµ ÐÐ¸Ð³ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð´ÐµÐºÑÐ°; 2. ÐÑÐ½ÐµÑÐµÐ½Ð¸Ðµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ð¹, ÑÐ¾ÑÑÐ¾ÑÑÐ¸Ñ Ð² Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¼ Ð¿Ð¾Ð»Ðµ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÐÐÐ Ð¸ Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ»ÑÐ¶Ð±Ñ Ðº Â«ÐºÐ¾Ð½ÑÐ¸Ð´ÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹Â»; 3. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð´ÑÑÐ¶Ð¸Ð½ Ð¿Ð¾ÑÑÐµÐ´ÑÑÐ²Ð¾Ð¼ Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð Ð¾ÑÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð¾; 4. ÐÑÐ¸Ð½ÑÑÐ¸Ðµ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ Ð¼ÐµÐ¶Ð²ÐµÐ´Ð¾Ð¼ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ³Ð»Ð°Ð¼ÐµÐ½ÑÐ° Â«Ð Ð¿Ð¾ÑÑÐ´ÐºÐµ Ð¾Ð±Ð¼ÐµÐ½Ð° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐµÐ¹ Ð¼ÐµÐ¶Ð´Ñ ÐÐÐ Ð¸ Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ»ÑÐ¶Ð±Ð¾Ð¹Â».
description: The work considers the migration flows of refugees, for example, the FMS of the Kalinin district of St. Petersburg. Identified a number of existing problems. Developed recommendations for improving the system of interaction of the migration service, bodies of protection of a public order. Namely: 1. The adoption of the Migration code; 2. The classification of information, including information in the field of cooperation of the interior Ministry and the migration service to "confidential"; 3. The project national teams through youth project Rossotrudnichestvo; 4. The interagency adoption of internal regulations On the procedure for the exchange of information between the police Department and the migration service".
Pseudographs and Lax-Oleinik semi-group: a geometric and dynamical interpretation
Creators: name: Arnaud, Marie-Claude
Publisher: name: arXiv
Year: 2010
Subjects: subject: Symplectic Geometry (math.SG)
subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics

description: Let H be a Tonelli Hamiltonian defined on the cotangent bundle of a compact and connected manifold and let u be a semi-concave function defined on M. If E (u) is the set of all the super-differentials of u and (ϕt) the Hamiltonian flow of H, we prove that for t > 0 small enough, ϕ-t (E (u)) is an exact Lagrangian Lipschitz graph. This provides a geometric interpretation/explanation of a regularization tool that was introduced by P.~Bernard to prove the existence of C 1,1 subsolutions.
Anisotropic spin fluctuations and multiple superconducting gaps in hole-doped Ba_0.7K_0.3Fe_2As_2: NMR in a single crystal
Creators: name: Matano, K.
name: Sun, G. L.
name: Sun, D. L.
name: Lin, C. T.
name: Ichioka, M.
name: Zheng, Guo-qing
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report the first ^{75}As-NMR study on a single crystal of the hole-doped iron-pnictide superconductor Ba_{0.7}K_{0.3}Fe_2As_{2} (T_c = 31.5 K). We find that the Fe antiferromagnetic spin fluctuations are anisotropic and are weaker compared to underdoped copper-oxides or cobalt-oxide superconductors. The spin lattice relaxation rate 1/T_1 decreases below T_c with no coherence peak and shows a step-wise variation at low temperatures, which is indicative of multiple superconducting gaps, as in the electron-doped Pr(La)FeAsO$_{1-x}$F$_{x}$. Furthermore, no evidence was obtained for a microscopic coexistence of a long-range magnetic and superconductivity.
On Galilean and Lorentz invariance in pilot-wave dynamics
Creators: name: Valentini, Antony
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: It is argued that the natural kinematics of the pilot-wave theory is Aristotelian. Despite appearances, Galilean invariance is not a fundamental symmetry of the low-energy theory. Instead, it is a fictitious symmetry that has been artificially imposed. It is concluded that the search for a Lorentz-invariant extension is physically misguided.
description: 13 pages. Published in 1997, recently latexed