cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ²Ð¸ÑÐ° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´Ð°Ð½Ð½ÑÑ Ð²Ð¸Ð´ÐµÐ¾ÑÐ¸ÐºÑÐ°ÑÐ¸Ð¸ Ð½Ð°ÑÑÑÐµÐ½Ð¸Ð¹ Ð¿ÑÐ°Ð²Ð¸Ð» Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð ÑÐ´ÐµÐ½ÐºÐ¾, Ð¢Ð°ÑÑ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: 2018
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ
ÐÑÐ°Ð²Ð¸Ð»Ð° Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ
ÑÐµÑÐ²Ð¸Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´Ð°Ð½Ð½ÑÑ
Ð²Ð¸Ð´ÐµÐ¾ÑÐ¸ÐºÑÐ°ÑÐ¸Ñ Ð½Ð°ÑÑÑÐµÐ½Ð¸Ð¹
ÑÐ±Ð¾Ñ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ¸

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ²Ð¸ÑÐ° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´Ð°Ð½Ð½ÑÑ Ð²Ð¸Ð´ÐµÐ¾ÑÐ¸ÐºÑÐ°ÑÐ¸Ð¸ Ð½Ð°ÑÑÑÐµÐ½Ð¸Ð¹ ÐÐÐ. ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½ ÐºÑÐ°ÑÐºÐ¸Ð¹ Ð¾Ð±Ð·Ð¾Ñ Ð¾ÑÐ³Ð°Ð½Ð° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´Ð°Ð½Ð½ÑÑ Ð²Ð¸Ð´ÐµÐ¾ÑÐ¸ÐºÑÐ°ÑÐ¸Ð¸ Ð½Ð°ÑÑÑÐµÐ½Ð¸Ð¹, Ð° ÑÐ°Ðº Ð¶Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ. Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¿Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð². Ð ÐµÐ·ÑÐ»ÑÑÐ°Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÑÑÑ Ð´Ð»Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾ÑÐ³Ð°Ð½Ð°Ñ Ð¦ÐÐ¤ÐÐ (Ð¦ÐµÐ½ÑÑ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÐºÑÐ°ÑÐ¸Ð¸ Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ°Ð²Ð¾Ð½Ð°ÑÑÑÐµÐ½Ð¸Ð¹ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ) Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸.
title: ÐÐ¸Ð·Ð°Ð¹Ð½-Ð¿ÑÐ¾ÐµÐºÑ Ð¼Ð°ÐºÐµÑÐ° Ð¿ÐµÑÐ¸Ð¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¤ÐµÐ´Ð¾ÑÐ¸Ð½Ð°, ÐÑÐ´Ð¼Ð¸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: 2016
Subjects: Ð´Ð¸Ð·Ð°Ð¹Ð½
Ð¶ÑÑÐ½Ð°Ð»
Ð²ÐµÑÑÑÐºÐ°

description: Ð¡Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð´Ð¸Ð·Ð°Ð¹Ð½-Ð¿ÑÐ¾ÐµÐºÑ Ð¼Ð°ÐºÐµÑÐ° Ð¿ÐµÑÐ¸Ð¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ. Ð¡Ð¾Ð·Ð´Ð°Ð½Ð° Ð¿ÐµÑÐ°ÑÐ½Ð°Ñ Ð²ÐµÑÑÐ¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ Losko magazine (www.losko.ru). Ð ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð´Ð¸Ð·Ð°Ð¹Ð½-ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ.
House & Garden: The Winter Care of Dahlias by Martha Prentice Strong, September 1914
Creators: name: Strong, Martha Prentice
Publisher: name: Garden Club of East Hampton
Year: 1914
Subjects: Gardening
Gardens
Social organizations
Organizations
East Hampton (N.Y.)

description: This article was written by Mrs. Martha Prentice Strong on the winter season care of the flower Dahlias. This was published in House & Gardens in September 1914.
Anomalous asymmetry of the Fermi surface in the YBa2Cu4O8 high temperature superconductor revealed by Angle Resolved Photoemission Spectroscopy
Creators: name: Kondo, Takeshi
name: Khasanov, R.
name: Sassa, Y.
name: Bendounan, A.
name: Pailhes, S.
name: Chang, J.
name: Mesot, J.
name: Keller, H.
name: Zhigadlo, N. D.
name: Shi, M.
name: Kazakov, S. M.
name: Karpinski, J.
name: Kaminski, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We use microprobe Angle-Resolved Photoemission Spectroscopy to study the Fermi surface and band dispersion of the CuO2 planes in the high temperature superconductor, YBa2Cu4O8. We find a strong in-plane asymmetry of the electronic structure between directions along a and b axes. The saddle point of the antibonding band lies at a significantly higher energy in the a direction (pi,0) than the b direction (0,pi), whereas the bonding band displays the opposite behavior. We demonstrate that the abnormal band shape is due to a strong asymmetry of the bilayer band splitting, likely caused by a non-trivial hybridization between the planes and chains. This asymmetry has an important implication for interpreting key properties of the Y-Ba-Cu-O (YBCO) family, especially the superconducting gap, transport and results of inelastic neutron scattering.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾ÑÐ¾Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¸ÐºÐ¾Ð² Ð´Ð»Ñ Ð±Ð»Ð¸Ð¶Ð½ÐµÐ³Ð¾ Ð¸ ÑÑÐµÐ´Ð½ÐµÐ³Ð¾ ÐÐ-Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ð¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð³ÐµÑÐµÑÐ¾ÑÑÑÑÐºÑÑÑÑ GaSb/GaAlAsSb
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Ð¸Ð²Ð¾Ð²Ð°ÑÐ¾Ð²Ð°, ÐÐ½ÑÐ¾Ð½Ð¸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: Ð¤Ð¾ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ
ÐÐ½ÑÑÐ°ÐºÑÐ°ÑÐ½ÑÐµ Ð»ÑÑÐ¸

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ¾ÑÐ¾Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¸ÐºÐ¾Ð² Ð´Ð»Ñ ÑÑÐµÐ´Ð½ÐµÐ¹ Ð¸ Ð±Ð»Ð¸Ð¶Ð½ÐµÐ¹ ÐÐ Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÐµÐºÑÑÐ° 1,1â 1,85 Ð¼ÐºÐ¼. Ð¢Ð°ÐºÐ¸Ðµ ÑÐ¾ÑÐ¾Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¸ÐºÐ¸ Ð¸Ð·Ð³Ð¾ÑÐ°Ð²Ð»Ð¸Ð²Ð°Ð»Ð¸ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð³ÐµÑÐµÑÐ¾ÑÑÑÑÐºÑÑÑ GaSb/GaAlAsSb Ñ Ð½Ð¸Ð·ÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸ÐµÐ¹ Ð½Ð¾ÑÐ¸ÑÐµÐ»ÐµÐ¹ Ð² Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. Ð£Ð½Ð¸ÐºÐ°Ð»ÑÐ½ÑÐ¹ Ð¼ÐµÑÐ¾Ð´ Ð²ÑÑÐ°ÑÐ¸Ð²Ð°Ð½Ð¸Ñ GaSb Ð¸Ð· ÑÐ²Ð¸Ð½ÑÐ¾Ð²ÑÑ ÑÐ°ÑÑÐ²Ð¾ÑÐ¾Ð²-ÑÐ°ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð» Ð´Ð¾ÑÑÐ¸ÑÑ Ð½Ð¸Ð·ÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ð¸ Ð½Ð¾ÑÐ¸ÑÐµÐ»ÐµÐ¹ Ð² Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ n = 2ï´1015 ÑÐ¼ï­3. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐµ ÑÐ¾ÑÐ¾Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¸ÐºÐ¸ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÑÑ Ð²ÑÑÐ¾ÐºÐ¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐ²ÑÑÐ²Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ SÎ»= 0,95Ð/ÐÑ Ð² Ð¼Ð°ÐºÑÐ¸Ð¼ÑÐ¼Ðµ, Ð¾ÑÐ½Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð¼Ð°Ð»Ð¾Ð¹ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ°ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ¼Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÐºÐ° j = (4ï­9)ï´10â3 Ð/ÑÐ¼2 Ð¿ÑÐ¸ Urev = 1,0 ï­ 2,0 Ð Ð¸ Ð²ÑÑÐ¾ÐºÐ¸Ð¼ Ð±ÑÑÑÑÐ¾Ð´ÐµÐ¹ÑÑÐ²Ð¸ÐµÐ¼ (Ð²ÑÐµÐ¼Ñ Ð¾ÑÐºÐ»Ð¸ÐºÐ° 5 ï­ 10 Ð½Ñ).
Physarum bitectum G. Lister 1911
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Physarales
Physaraceae
Physarum
Physarum bitectum

description: ● Physarum bitectum G. Lister (expected transfer to the genus Angioridium (García-Martín et al 2023)),
dubultā rāpulīte
- leg. J.Kluša, 07 Oct 2021, Jūrmala, on mosses, plants and litter in a black alder swamp forest, det. J.Kluša, 2021; (NMKK), very rare.
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
Authors without Borders
Publisher: name: Online Ethics Center
Year: 2023
Subjects: International Perspectives
Collaboration
International Collaboration
Interdisciplinary Research
Communicating Science and Engineering
Publication Ethics
Authorship
Social Responsibility

description: This resource, Authors Without Borders: Guidelines for Discussion Authorship with Collaborators, intends to (i) enhance awareness of ethical issues associated with authorship that researchers might face in collaborative projects, (ii) assist in the identification of frequent sources of misunderstanding associated with authorship that can result in conflicts, and (iii) contribute to the development of guidelines for discussion that can serve as a basis for proactive, ethical and culturally sensitive conversations about co-authorship.
Silicate Evolution in Brown Dwarf Disks
Creators: name: Riaz, B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a compositional analysis of the 10 micron silicate spectra for brown dwarf disks in the Taurus and Upper Scorpius (UppSco) star-forming regions, using archival Spitzer/IRS observations. A variety in the silicate features is observed, ranging from a narrow profile with a peak at 9.8 micron, to nearly flat, low-contrast features. For most objects, we find nearly equal fractions for the large-grain and crystalline mass fractions, indicating both processes to be active in these disks. The median crystalline mass fraction for the Taurus brown dwarfs is found to be 20%, a factor of ~2 higher than the median reported for the higher mass stars in Taurus. The large-grain mass fractions are found to increase with an increasing strength in the X-ray emission, while the opposite trend is observed for the crystalline mass fractions. A small 5% of the Taurus brown dwarfs are still found to be dominated by pristine ISM-like dust, with an amorphous sub-micron grain mass fraction of ~87%. For 15% of the objects, we find a negligible large-grain mass fraction, but a >60% small amorphous silicate fraction. These may be the cases where substantial grain growth and dust sedimentation has occurred in the disks, resulting in a high fraction of amorphous sub-micron grains in the disk surface. Among the UppSco brown dwarfs, only usd161939 has a S/N high enough to properly model its silicate spectrum. We find a 74% small amorphous grain and a ~26% crystalline mass fraction for this object.
description: Accepted in ApJ
Study of Barnard's Star B as an Analog for Titan-like Exoplanets
Creators: name: Felton, Ryan
name: Domagal-Goldman, Shawn
name: Arney, Giada
name: Gao, Peter
name: Lora, Juan
name: Villaneuva, Geronimo
name: Hebrard, Eric
Publisher: name: Zenodo
Year: 2021

description: Radial velocity measurements of Barnard's Star have shown the potential for there to be a planet – Barnard's Star b – with a minimum mass of 3.2 Me, orbiting with a semimajor axis near the snow-line of the system. The size and orbital properties of Barnard b are somewhat Titan-like in nature: Barnard b is a potentially rocky planet with a thick atmosphere above it, orbiting at a distance at which methane could condense. Further, Barnard's Star is 1.8 parsecs from the Sun, which is close enough to allow direct-imaging of this world with a large space-based telescope such as LUVOIR-A. We present simulations of the observational features of Titan, as an exoplanet, using the known properties of Barnard b and the performance of LUVOIR's coronagraph (ECLIPS). These simulations were done using the Planetary Spectrum Generator (PSG) to produce synthetic reflectance spectrum of a Titan-like Barnard's Star b. First, we discuss our efforts to validate PSG against Titan observations for transit and reflection spectroscopy. We discuss validation issues encountered and how they were mitigated and present simulations for Barnard's Star b, pointing out the observable features of that planet.
How to Measure the Transmission Phase via a Quantum Dot in a Two-Terminal Interferometer
Creators: name: Puller, Vadim
name: Meir, Yigal
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Measurement of the transmission phase through a quantum dot (QD) embedded in an arm of a two-terminal Aharonov-Bohm (AB) interferometer is inhibited by phase symmetry, i.e. the property that the linear response conductance of a two-terminal device is an even function of magnetic field. It is demonstrated that in a setup consisting of an interferometer with a QD in each of its arms, with one of the QDs capacitively coupled to a nearby quantum point contact (QPC), phase symmetry is broken when a finite voltage bias is applied to the QPC. The transmission phase via the uncoupled QD can then be deduced from the amplitude of the odd component of the AB oscillations.
title: ÐÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ ÑÑÐ°ÑÑÑ Ð±ÐµÐ¶ÐµÐ½ÑÐµÐ² Ð¸ Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½ÑÑ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÑÐµÐ²: Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð°ÑÐ¿ÐµÐºÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÑÑÐ´Ð»Ñ , Ð£ÑÑÐ°Ð½
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¶ÐµÐ½ÐµÑ
Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½ÑÐ¹ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÐµÑ
Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ñ
Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ ÑÑÐ°ÑÑÑ
Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ ÑÑÐ°ÑÑÑ Ð±ÐµÐ¶ÐµÐ½ÑÐµÐ² Ð¸ Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½ÑÑ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÑÐµÐ² Ñ ÑÐ¾ÑÐºÐ¸ Ð·ÑÐµÐ½Ð¸Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ°Ð²Ð°. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾Ð±ÑÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¿Ð¾Ð½ÑÑÐ¸Ð¹ Ð±ÐµÐ¶ÐµÐ½ÐµÑ Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½ÑÐ¹ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÐµÑ, ÐºÐ°Ðº Ð² Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¼ Ð¿ÑÐ°Ð²Ðµ, ÑÐ°Ðº Ð¸ Ð² Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¼ Ð¿ÑÐ°Ð²Ðµ. Ð¥Ð°ÑÐ°ÐºÑÐµÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ñ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð°ÐºÑÑ, ÑÐµÐ³ÑÐ»Ð¸ÑÑÑÑÐ¸Ðµ Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ ÑÑÐ°ÑÑÑ Ð±ÐµÐ¶ÐµÐ½ÑÐµÐ² Ð¸ Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½ÑÑ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÑÐµÐ² Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ Ð¼Ð¸ÑÐµ. Ð¢Ð°Ðº Ð¶Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ ÑÐ´ÐµÐ»ÑÐ»Ð¸ÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð±ÐµÐ¶ÐµÐ½ÑÐµÐ² Ð¸ Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½ÑÑ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÑÐµÐ², ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ Ð¸Ñ ÑÑÑÐ´Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾Ð¼, ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÐ¼ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸ÐµÐ¼, Ð¿ÑÐ¸Ð·Ð½Ð°Ð½Ð¸ÐµÐ¼ Ð·Ð° Ð½Ð¸Ð¼Ð¸ ÑÑÐ°ÑÑÑÐ° Ð±ÐµÐ¶ÐµÐ½ÑÐ° Ð¸Ð»Ð¸ Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÑÐ° Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ Ð¼Ð¸ÑÐµ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ ÑÐµÑÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼.
description: ÐÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð², ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð±ÐµÐ¶ÐµÐ½ÑÐ°Ð¼Ð¸ Ð¸ Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÑÐ°Ð¼Ð¸ Ð²ÐºÐ»ÑÑÐ°ÐµÑ ÑÐ¸ÑÐ¾ÐºÐ¸Ð¹ ÐºÑÑÐ³ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÑ Ð°ÐºÑÐ¾Ð² Ð¸ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð². ÐÑÐ°Ð²Ð° Ð±ÐµÐ¶ÐµÐ½ÑÐµÐ² Ð¸ Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½ÑÑ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÑÐµÐ² Ð·Ð°ÐºÑÐµÐ¿Ð»ÐµÐ½Ñ Ð² Ð·Ð°ÐºÐ¾Ð½Ð°Ñ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Â«Ð Ð±ÐµÐ¶ÐµÐ½ÑÐ°ÑÂ» Ð¸ Â«Ð Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½ÑÑ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÑÐ°ÑÂ» ÐÐ° Ð¿ÑÐ°ÐºÑÐ¸ÐºÐµ Ð²ÑÑÐ²Ð»ÑÑÑÑÑ Ð¼Ð½Ð¾Ð³Ð¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, ÐºÐ°ÑÐ°ÑÑÐ¸ÐµÑÑ ÑÑÐ°ÑÑÑÐ° Ð±ÐµÐ¶ÐµÐ½ÑÐ° Ð¸ Ð²ÑÐ½ÑÐ¶Ð´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½ÑÐ°, Ð¿Ð¾ÑÐºÐ¾Ð»ÑÐºÑ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÐµÑÐµÐ½Ð¸Ð¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð´Ð°Ð»ÐµÐºÐ¾ Ð½Ðµ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÐµÐ½.
title: ÐÐ½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¾Ð±Ð·Ð¾Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐµÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐ°ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¸ Ð¼Ð°Ð»ÑÑ Ð²Ð¾Ð·Ð¼ÑÑÐµÐ½Ð¸ÑÑ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¸Ñ ÐµÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð²
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ°ÑÐ½Ð¾Ð²Ð° , 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: 2017
Subjects: Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°
ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
Ð¼Ð°Ð»Ð¾Ðµ Ð²Ð¾Ð·Ð¼ÑÑÐµÐ½Ð¸Ðµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐ¸ÑÑÐµÐ¼Ñ
ÑÐ¾Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ðµ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸

description: Ð ÑÐ°Ð±Ð¾ÑÐµ, Ð½Ð¾ÑÑÑÐµÐ¹ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑ, ÑÐ´ÐµÐ»Ð°Ð½Ð° Ð¿Ð¾Ð¿ÑÑÐºÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð¸ÑÑ Ð¿ÑÐ¾Ð·ÑÐ°ÑÐ½Ð¾Ðµ Ð¸, Ð¿Ð¾ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸, ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð², Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÑ Ð´Ð»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¿ÑÐ¸ Ð½Ð°Ð»Ð¸ÑÐ¸Ð¸ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¸Ñ Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐ½Ð½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð²Ð¾Ð·Ð¼ÑÑÐµÐ½Ð¸Ñ.
title: Ð¡ÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ð¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»Ð¸Ð½Ð³ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÐ¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÐµÐ¼
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡ÑÐ»Ð¾ÐµÐ²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
name: ÐÑÑÐ°Ð½Ð¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2014
Subjects: ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ð¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»Ð¸Ð½Ð³
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

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title: Ð¡Ð»Ð°Ð±Ð¾ÑÐ¾ÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð½ÑÐ¾Ð² Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«ÐÐ¾Ð¶Ð°ÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÂ»
titleType: Subtitle
Creators: name: ÐÐ°Ð±Ð¸ÐºÐ¾Ð², ÐÐ³Ð¾ÑÑ
name: ÐÑÐ±Ð¸Ð½Ð°, ÐÐ»ÑÐ³Ð°
name: Ð¢Ð°Ð½ÐºÐ»ÐµÐ²ÑÐºÐ¸Ð¹, ÐÐµÐ¾Ð½Ð¸Ð´
name: Ð¢Ð¾Ð¼Ð°ÑÐ¾Ð²Ð°, 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¢ÐµÑ Ð½Ð¸ÐºÐ° Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸
Ð¡Ð¸Ð³Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ

description: Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¤ÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Â«Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾Â» Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 20.04.01 Ð¢ÐµÑÐ½Ð¾ÑÑÐµÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ, Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð¡Ð»Ð°Ð±Ð¾ÑÐ¾ÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸Â». Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¸ÐºÐ¾Ð² ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°Ð²ÑÐºÐ¾Ð² Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸, Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐµÐºÑÐ¾Ð². ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ.
Developing a New Taxonomy for Comets Based on Updated Molecular Abundances
Creators: name: Lippi, Manuela
name: Villanueva, Geronimo L.
name: Mumma, Michael J.
name: Faggi, Sara
Publisher: name: Zenodo
Year: 2021

description: We present updated molecular abundances in 20 comets observed since 1985, using different ground-based high resolution infrared spectrometers.With this technique it is possible to sample emission lines produced by solar-pumped fluorescence of primary molecules released directly from the nucleus, and to investigate cosmogonic indicators such as rotational temperatures, production rates and mixing ratios, that are expected to remain unaltered since the comet's formation. Our results show that some of the previous published results contain inaccuracies introduced by the continuous evolution of the algorithms used for interpreting fluorescence in comets; moreover, for some species, we measure molecular abundances not reported in the past due to the lack of specific molecular models. Our revision impacts mostly comets that were observed before 2011, which constitute the majority of targets in our database. The correct statistics and interpretation of the updated molecular abundances, may yield important clues regarding the conditions present in the proto-planetary disk, when/where a specific comet formed, and can help us in building a chemical taxonomy for these bodies.
title: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ Ð¼ÐµÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÐ»ÐµÐ½Ð¸Ñ Kenotec Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ MSAccess Ð¸ ÑÐ·ÑÐºÐ° SQL
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
title: Programming and controlling of the Kenotec Sputtering system based on MS Access and SQL language
Creators: name: ÐÑÐ½ Ð¦Ð¸Ð¶ÑÐ½
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°ÑÐ¾Ð´Ð½Ð¾Ðµ ÑÐ°ÑÐ¿ÑÐ»ÐµÐ½Ð¸Ðµ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐµ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð½Ð°Ð¿ÑÐ»ÐµÐ½Ð¸Ñ Kenotec, ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½Ð¾Ðµ Ð² ÑÑÐµÐ´Ðµ MSAccess Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ·ÑÐºÐ° VBA. Ð¢Ð°ÐºÐ¶Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÑÐºÑÑÑÑ ÑÐ¿Ð¸Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÐºÐ»Ð°Ð¿Ð°Ð½Ð° Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Kenotec. ÐÐ»Ð¸ÑÐ½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¾ÑÐ¶Ð¸Ð³Ð° Ð½Ð° ÑÑÑÐµÐºÑ GMR ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð²ÐµÑÑÐµÑÑÑ Ð² Ð¿ÑÐ¾ÐµÐºÑÐµ. ÐÐ¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ Ð¿ÑÐµÐ´ÑÐ´ÑÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÑ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð´Ð°ÑÑÐ¸ÐºÐ° GMR ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð»Ð¸ÑÐ¾Ð³ÑÐ°ÑÐ¸Ð¸.
description: In this thesis, the control and programming of the Kenotec sputtering system is implemented in the MS Access environment with the VBA language. Then the spin valve structure is manufactured with the Kenotec system and characterized in the clean room. The effects of the annealing process on the GMR effect are also tested in the project. With the results of the previous work, the pattern of the GMR sensor is designed and realized by the lithography process.
A bubble-powered micro-rotor: conception, manufacturing, assembly, and characterization
Creators: name: Kao, Jonathan
name: Wang, Xiaolin
name: Warren, John
name: Xu, Jie
name: Attinger, Daniel
Publisher: name: arXiv
Year: 2009
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: A steady fluid flow, called microstreaming, can be generated in the vicinity of a micro-bubble excited by ultrasound. In this article, we use this phenomenon to assemble and power a microfabricated rotor at rotation speeds as high as 625 rpm. The extractible power is estimated to be on the order of a few femtowatts. A first series of experiments with uncontrolled rotor shapes is presented, demonstrating the possibility of this novel actuation scheme. A second series of experiments with 65 micron rotors micromanufactured in SU-8 resin are presented. Variables controlling the rotation speed and rotor stability are investigated, such as the bubble diameter, the acoustic excitation frequency and amplitude, and the rotor geometry. Finally, an outlook is provided on developing this micro-rotor into a MEMS-based motor capable of delivering tunable, infinitesimal rotary power at the microscale.
Security of Scottish electricity supply: gauging the perceptions of industry stakeholders
Creators: name: Nedd, Marcel
name: Bell, Keith
Publisher: name: University of Strathclyde
Year: 2022
Subjects: Security of electricity supply
Blackout
Electricity grid

description: Efforts to reduce greenhouse gas (GHG) emissions together with the increase in electricity generated from renewable energy are dramatically changing the electricity supply landscape. This document reports and reviews the opinions of industry experts and stakeholders regarding security of electricity supply in Scotland, collected in May 2021 via an online survey and subsequent discussions in a roundtable event in July 2021.
title: ÐÑÐ°Ð²Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð±Ð¸Ð·Ð½ÐµÑÐ°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð·Ð»Ð¾Ð², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2014
Subjects: Ð¿ÑÐµÐ´Ð¿ÑÐ¸Ð½Ð¸Ð¼Ð°ÑÐµÐ»ÑÑÑÐ²Ð¾
Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð²ÑÑÑÐµÐ³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº Ð¾Ð±ÑÐ·Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ Ð¼Ð¸Ð½Ð¸Ð¼ÑÐ¼Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 080100 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» Ð¿Ð¾ ÑÐ¸ÐºÐ»Ñ Ð.1 Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ° Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð½Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 080200 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ» Ð¿Ð¾ ÑÐ¸ÐºÐ»Ñ Ð.1. ÐÐ¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð° Â«ÐÑÐ°Ð²Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð±Ð¸Ð·Ð½ÐµÑÐ°Â» Ð¿ÑÐµÐ´ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÑÐµÐ±Ð½ÑÐ¼ Ð¿Ð»Ð°Ð½Ð¾Ð¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 080100 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 080200 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð», ÑÐ²Ð»ÑÑÑÐ¸Ð¹ÑÑ Ð±Ð°Ð·Ð¾Ð²ÑÐ¼ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐµÐ¼ ÐºÑÑÑÐ°. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ Ð²ÑÐµÑ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÑÐ°Ð²Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð±Ð¸Ð·Ð½ÐµÑÐ°Â».
Programa de Prevención y Promoción de la Salud para mitigar el ausentismo y presentismo laboral
Creators: name: Medina Parada, Laudyd Marcela
name: Contreras Henao, Emilio del Carmen
name: Rolon Ibarra, Gian Carlos
name: Pérez Fernández, Blanca Johanna
Publisher: name: Zenodo
Year: 2023
Subjects: Programa de Prevención y Promoción de la Salud
Seguridad
Condiciones de Salud
mitigar
Ausentismo y Presentismo Laboral por Causa Médica

description: OBJETIVO GENERAL

El presente programa tiene por objetivo disminuir el ausentismo y presentismo laboral de los trabajadores de un centro de trabajo ubicado en la ciudad de Cúcuta, fomentando hábitos y estilos de vida saludables, con el fin de promocionar la salud, previniendo eventos generales, laborales, patologías y condiciones incapacitantes de salud.
Holographic formula for the determinant of the scattering operator in thermal AdS
Creators: name: Díaz, Danilo E.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Differential Geometry (math.DG)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: A 'holographic formula' expressing the functional determinant of the scattering operator in an asymptotically locally anti-de Sitter(ALAdS) space has been proposed in terms of a relative functional determinant of the scalar Laplacian in the bulk. It stems from considerations in AdS/CFT correspondence of a quantum correction to the partition function in the bulk and the corresponding subleading correction at large N on the boundary. In this paper we probe this prediction for a class of quotients of hyperbolic space by a discrete subgroup of isometries. We restrict to the simplest situation of an abelian group where the quotient geometry describes thermal AdS and also the non-spinning BTZ instanton. The bulk computation is explicitly done using the method of images and the answer can be encoded in a (Patterson-)Selberg zeta-function.
description: 11 pages, published JPA version
Bare and effective fluid description in brane world cosmology
Creators: name: Cruz, Norman
name: Lepe, Samuel
name: Pena, Francisco
name: Saavedra, Joel
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 - Theory (hep-th)
subject: FOS: Physical sciences

description: An effective fluid description, for a brane world model in five dimensions, is discussed for both signs of the brane tension. We found several cosmological scenarios where the effective equation differs widely from the bare equation of state. For universes with negative brane tension, with a bare fluid satisfying the strong energy condition, the effective fluid can cross the barrier $ω_{eff} =-1$.
description: 6 pages
title: ÐÐ¸ÐºÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½Ð°Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ° Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 100 ÐºÐÑ Ñ Ð²ÑÐ½Ð¾ÑÐ½Ð¾Ð¹ ÐºÐ°Ð¼ÐµÑÐ¾Ð¹ ÑÐ³Ð¾ÑÐ°Ð½Ð¸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Ð³Ð¾ÑÐ¾Ð²Ð°, ÐÐ½Ð½Ð°
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: Ð¼Ð¸ÐºÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½Ð°Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°
Ð³Ð°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½Ð°Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°
ÐºÐ°Ð¼ÐµÑÐ° ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ
ÑÐ°ÑÑÐµÑ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÑ ÐµÐ¼Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð³Ð°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 100ÐºÐÑ Ñ Ð²ÑÐ½Ð¾ÑÐ½Ð¾Ð¹ ÐºÐ°Ð¼ÐµÑÐ¾Ð¹ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð° ÐÐ¢Ð-100 Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð¾Ð¹ ÐÐÐ Â«ÐÐ¢Ð¦ Â«ÐÐ¸ÐºÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â». ÐÐ°Ð½Ð¾ Ð¾Ð±ÑÐµÐµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸-Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð° Ð¸ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÑÐµÐ¼Ñ Ð¸ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐµÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ·Ð»Ð¾Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸. ÐÐ·ÑÑÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ÑÑÑÑÑÐ²ÑÑÑÐ¸Ñ Ð² ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐµ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð².
Numerical model of a mechanical metamaterial with adaptable stiffness
Creators: name: Haid, Daniel
name: Duncan, Olly
name: Hart, John
name: Foster, Leon
Publisher: name: Loughborough University
Year: 2024

description: Engineering of Sport 15 - Proceedings from the 15th International Conference on the Engineering of Sport (ISEA 2024)

Ice hockey has one of the highest concussion rates in sport. A challenge in developing helmets is the range of common head impacts. Current ice hockey helmets are relatively stiff to protect during falls on the ice, as assessed in certification standards. However, more than 90% of concussions are caused by collisions between players. Consequently, liners do not compress through most of their range during impacts with more compliant bodies, increasing accelerations and injury risks. A helmet liner that can adapt its compressive properties, dependent on the nature of impact, could improve helmets during collisions whilst maintaining a high stiffness during rigid surface impacts. A previously presented rate-dependent mechanical metamaterial with adaptable buckling behaviour could achieve such a switch in stiffness. The concept must be rigorously assessed before potential application in safety equipment. Numerical analysis could support testing and development of the concept and reduce the need for more time and cost intensive methods.
Supplementary Movie from Tomopac2: an unfolded-slab plate reconstruction validated via mantle circulation models in a closed-loop experiment*
Creators: name: Chen, Yi-Wei
name: Wu, Jonny
name: Bunge, Hans-Peter
name: Stotz, Ingo
name: Robl, Gabriel
name: Schuberth, Bernhard S. A.
Publisher: name: The Royal Society
Year: 2025
Subjects: classificationCode: 3705
subject: Geology
subject: FOS: Earth and related environmental sciences
classificationCode: 370511
subject: Structural geology and tectonics
classificationCode: 3706
subject: Geophysics

description: Tomopac2 reconstruction (same as Fig. 5)
Close-in satellite detections in the trans-Neptunian region: the special case of Varuna.
Creators: name: Fernandez, Estela
name: Ortiz, Jose Luis
name: Morales, Nicolás
name: Santos-Sanz, Pablo
name: Lellouch, Emmanuel
name: Duffard, René
Publisher: name: Zenodo
Year: 2021

description: Photometric techniques can be used to reveal the existence satellites around solar system bodies, but such methods have not been applied to Trans-neptunian objects (TNOs). Specifically, using rotational light-curves it is possible to reveal satellites much closer-in than using the direct imaging technique, and thus helping to remove biases in our current knowledge of the population of binaries in the trans-neptunian region, for which all the known satellites have been detected through high resolution imaging. In this work, we present short-term photometric measurements of the large TNO Varuna in 10 epochs. We have detected changes in the overall shape of the rotational light-curve over shorter time scales that could be due to a close-in satellite whose rotation induces an additional periodicity of 11.9819 h, detected applying the Lomb periodogram technique. Assuming that the satellite is tidally locked we estimate that the satellite orbits Varuna with a period of 11.9819 h, which would imply a distance to the primary of 1300 km, assuming a density of 1100 kg/m^3. This is well outside the Roche limit and too close for direct detection with HST.
The Star Formation and Nuclear Accretion Histories of Normal Galaxies in the AGES Survey
Creators: name: Watson, Casey R.
name: Kochanek, Christopher S.
name: Forman, William R.
name: Hickox, Ryan C.
name: Jones, Christine J.
name: Brown, Michael J. I.
name: Brand, Kate
name: Dey, Arjun
name: Jannuzi, Buell T.
name: Kenter, Almus T.
name: Murray, Steve S.
name: Vikhlinin, Alexey
name: Eisenstein, Daniel J.
name: Fazio, Giovani G.
name: Green, Paul J.
name: McNamara, Brian R.
name: Rieke, Marcia
name: Shields, Joseph C.
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: We combine IR, optical and X-ray data from the overlapping, 9.3 square degree NOAO Deep Wide-Field Survey (NDWFS), AGN and Galaxy Evolution Survey (AGES), and XBootes Survey to measure the X-ray evolution of 6146 normal galaxies as a function of absolute optical luminosity, redshift, and spectral type over the largely unexplored redshift range 0.1 < z < 0.5. Because only the closest or brightest of the galaxies are individually detected in X-rays, we use a stacking analysis to determine the mean properties of the sample. Our results suggest that X-ray emission from spectroscopically late-type galaxies is dominated by star formation, while that from early-type galaxies is dominated by a combination of hot gas and AGN emission. We find that the mean star formation and supermassive black hole accretion rate densities evolve like (1+z)^3, in agreement with the trends found for samples of bright, individually detectable starburst galaxies and AGN. Our work also corroborates the results of many previous stacking analyses of faint source populations, with improved statistics.
description: 19 pages, 15 figures, 3 tables, accepted for publication in ApJ
Ground and space based observatories: the feasibility of measuring D/H in exoplanet atmospheres
Creators: name: Kofman, Vincent
name: Villanueva, Geronimo
Publisher: name: Zenodo
Year: 2021

description: The D/H ratio is a powerful window into the evolution of atmospheres. Atmospheric escape results loss of the lighter isotope, which, in the Solar System, has allowed us to conclude that Mars and Venus lost significant amount of water. Measuring the D/H ratio in exoplanet atmospheres is possible by looking at the absorption/emission features of water or methane in the mid-infrared. Even at natural isotopic abundances, the deuterated isotopes have regions where the absorption surpasses the main isotopes. The ro-vibrational opacities of the relevant couples (i.e. H2O/HDO and CH4/CH3D) have to be very well constrained however. Combining both experimental and ab-initio line lists offers the most complete and accurate way to calculate molecular absorptions. We combine these datasets, and the feasibility of detecting D/H in exoplanets is assessed using both ground and space based observatories, and considering a number of different atmospheres and planetary sizes.
title: ÐÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¢ÐÐ-1)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐºÐ¾Ð²Ð°, Ð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: 2017
Subjects: ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¿ÐµÑÑÐ¾Ð½Ð°Ð» ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹
Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼

description: Ð ÑÐ¾Ð´Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð·Ð½Ð°ÐºÐ¾Ð¼Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ñ ÐºÐ°Ðº ÑÐ»ÐµÐ¼ÐµÐ½Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼, Ð¸Ð·ÑÑÐµÐ½Ñ ÑÑÐ°Ð¿Ñ, Ð²Ð¸Ð´Ñ, ÑÐ¸Ð¿Ñ, Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð¼ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÐºÑÐ¾ÑÑ, Ð½Ð° Ð½ÐµÑ Ð²Ð»Ð¸ÑÑÑÐ¸Ðµ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾Ð±ÑÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÑÐ´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿Ð¾ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐµ ÑÐ¸ÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÑ ÑÐµÐºÑÑÐµÑÑÐ¸ Ð¸ Ð¿Ð¾ÑÑÐ¾ÑÐ½ÑÑÐ²Ð° ÐºÐ°Ð´ÑÐ¾Ð² Ð·Ð° Ð³Ð¾Ð´, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°ÑÐ¸ÐºÐµ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸.
Temperature and abundance profiles of hot gas in galaxy groups - II. Implications for feedback and ICM enrichment
Creators: name: Rasmussen, Jesper
name: Ponman, Trevor J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the history of galactic feedback and chemical enrichment within a sample of 15 X-ray bright groups of galaxies, on the basis of the inferred Fe and Si distributions in the hot gas and the associated metal masses produced by core-collapse and type Ia supernovae (SN). Most of these cool-core groups show a central Fe and Si excess, which can be explained by prolonged enrichment by SN Ia and stellar winds in the central early-type galaxy alone, but with tentative evidence for additional processes contributing to core enrichment in hotter groups. Inferred metal mass-to-light ratios inside r_500 show a positive correlation with total group mass but are generally significantly lower than in clusters, due to a combination of lower global ICM abundances and gas-to-light ratios in groups. This metal deficiency is present for products from both SN Ia and SN II, and suggests that metals were either synthesized, released from galaxies, or retained within the ICM less efficiently in lower-mass systems. We explore possible causes, including variations in galaxy formation and metal release efficiency, cooling-out of metals, and gas and metal loss via AGN- or starburst-driven galactic winds from groups or their precursor filaments. Loss of enriched material from filaments coupled with post-collapse AGN feedback emerge as viable explanations, but we also find evidence for metals to have been released less efficiently from galaxies in cooler groups and for the ICM in these to appear chemically less evolved, possibly reflecting more extended star formation histories in less massive systems. Some implications for the hierarchical growth of clusters from groups are briefly discussed.
description: 26 pages, 20 figures, MNRAS accepted
Proceedings 8th International Workshop on Parallel and Distributed Methods in verifiCation
Creators: name: Brim, Lubos
name: van de Pol, Jaco
Publisher: name: arXiv
Year: 2009
Subjects: subject: Logic in Computer Science (cs.LO)
subject: Computational Engineering, Finance, and Science (cs.CE)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: The 8th International Workshop on Parallel and Distributed Methods in verifiCation (PDMC 2009) took place on November 4, 2009 at the Eindhoven University of Technology, in conjunction with Formal Methods 2009 and other related events for the first time under the heading of Formal Methods Week. This volume contains the final workshop proceedings.
Exoplanetary transits in the Galactic bulge
Creators: name: Ferreira dos Santos, Thiago
name: Kalbusch Saito, Roberto
Publisher: name: Zenodo
Year: 2021

description: The search and detection of exoplanets orbiting red dwarf stars are one of the main objectives of the VVV & VVV-X surveys, whence has been observed in near-IR bands the region of the bulge and Galactic disk during the last decade. At first, we selected dwarf stars based on PSF photometry data and distinguished red dwarfs from giant stars, spurious to our current analysis, using astrometric data from the VIRAC and Gaia DR2 projects. This particular type of star becomes of great interest in exoplanetary studies due to its relative low dimensions and temperatures, which maximizes researches on potentially habitable rocky exoplanets orbiting such stars. Subsequently, we searched for periodic light variations by implementing the box-fitting and the Lomb-Scargle methods in order to detect such exoplanets transits. Through parameters such as depth, transit width and orbital period, as well as knowing the spectral subtype of the central star, besides determining its distance, it is possible to estimate the dimensions of the exoplanet, or even exoplanetary systems, as to radius, surface temperature and mass, important factors in the characterization of an exoplanet as to its habitability.
title: Ð¡Ð¸ÑÑÐµÐ¼Ð° ÑÐ°ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð²ÑÑÐµÐ³Ð¾ Ð´Ð¾ÐºÐ° Ð½Ð° Ð°ÐºÐ²Ð°ÑÐ¾ÑÐ¸Ð¸ ÐÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð° Ð¼Ð¾ÑÑ
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¨Ð°Ð¿Ð¾Ð²Ð°Ð»Ð¾Ð², ÐÐ½ÑÐ¾Ð½
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Ð¾ÐºÐ¸ Ð¿Ð»Ð°Ð²ÑÑÐ¸Ðµ
ÐÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾ Ð¼Ð¾ÑÐµ
Ð·Ð°ÑÐºÐ¾ÑÐµÐ½Ð½ÑÐµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ
anchored structures
Bering sea

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¿Ð»Ð°Ð²ÑÑÐ¸Ð¹ Ð´Ð¾Ðº Ñ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ ÑÐ°ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ, ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ Ð² Ð·Ð°ÑÐ¸ÑÐµÐ½Ð½Ð¾Ð¹ Ð¼Ð¾Ð»Ð¾Ð¼ Ð°ÐºÐ²Ð°ÑÐ¾ÑÐ¸Ð¸ ÐÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð° Ð¼Ð¾ÑÑ. ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð²ÑÑÐµÐ³Ð¾ Ð´Ð¾ÐºÐ° Ð¿ÑÐ¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¸ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ°Ñ ÑÐ°ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ. Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ°ÑÑÐµÑÐ° ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ°ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð²ÑÑÐµÐ³Ð¾ Ð´Ð¾ÐºÐ° Ð½Ð° Ð·Ð°ÑÐ¸ÑÐµÐ½Ð½Ð¾Ð¹ Ð¼Ð¾Ð»Ð¾Ð¼ Ð°ÐºÐ²Ð°ÑÐ¾ÑÐ¸Ð¸ ÐÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð° Ð¼Ð¾ÑÑ. Ð Ð°Ð±Ð¾ÑÐ° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, ÑÐµÑÑÑÐµÑ Ð³Ð»Ð°Ð² Ð¸ Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ñ.
description: The object of study - the floating dock with a mount system, located in the protected waters of Bering Sea. Subject of research - behaviors of floating dock under different treatments and options for mount system. The master's thesis presents the methodology and results of the calculation of mount system of a floating dock on the protected waters of the Bering Sea. The work consists of an introduction, four chapters and a conclusion.
FPGAs as General-Purpose Accelerators for Non-Experts via HLS: The Graph Analysis Example
Creators: name: Silva, Pedro Filipe
name: Bispo, João
name: Paulino, Nuno
Publisher: name: Zenodo
Year: 2021

description: Artefacts/code linked to FPGAs as General-Purpose Accelerators for Non-Experts via HLS: The Graph Analysis Example. Code/implementations for DC1, PR, and SSSP: impl.tar Dataset (spm_graph_c.tar.xz) README: SPARSE MATRIX GRAPH COLLECTION
 NAMES AND SOURCES:
 SO soc-Orkut Ryan A. Rossi and Nesreen K. Ahmed. The network data repository with interactive graph analytics and visualization, 2015. URL: https://networkrepository.com
 SO^T soc-Orkut (transposed) -
 LJ soc-LiveJournal1 Jure Leskovec and Andrej Krevl. SNAP Datasets: Stanford large network dataset collection,June 2014. URL:http://snap.stanford.edu/data
 CO com-Orkut Same as LJ.
 USA USA-road-d.USA DIMACS. 9th DIMACS Implementation Challenge - Shortest Paths, 2006. URL:http://www.diag.uniroma1.it/challenge9/
 RMAT RMAT22 Ruohuang Zheng and Sreepathi Pai. Efficient Execution of Graph Algorithms on CPU with SIMD Extensions. In 2021 IEEE/ACM Int. Symp. Code Gener. Optim., February 2021. IEEE. DOI: 10.1109/CGO51591.2021.9370326
 R4 r4-2e23 Same as RMAT.
 FILEPATHS AND DOMAINS:
 SO large/soc-orkut*213M* social
 SO^T large/soc-orkut*trans* -
 LJ large/soc-LiveJournal1 social
 SO large/com-Orkut* social
 USA small/US-road-d* road
 RMAT small/rmat* random
 R4 small/r4* random
 FORMAT:
 Matrices in CSR have the csr.mtx extension.
 Matrices in CSC have the csc.mtx extension. Offset file: off.{csr, csc}.mtx
 First line is $NUM_VERTICES $NUM_VERTICES.
 Standard CSR/CSC offset (row/column index) contents follow, separated by \n. Column/row file: {col.csr, row.csc}.mtx
 First line is $NUM_EDGES.
 Contents are $COL_INDEX $VALUE or $ROW_INDEX $VALUE, separated by \n.
 NOTES:
 Filenames include number of edges in M.
 d/ud: originally a directed/undirected graph.
 sym/usym: symmetric/asymmetric matrix.
 Some datasets sanitised (e.g. diagonals zeroed out).