cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿Ð»Ð°Ð½Ð° Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð² Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ Ð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ÐµÑÐµÐ»Ð¸Ð½Ð°, 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: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÐ°
Ð°Ð±Ð¸ÑÑÑÐ¸ÐµÐ½ÑÑ
Ð¿ÐµÑÐµÐ´Ð¾Ð²ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³Ð¾Ð²ÑÐ¹ ÑÐµÐ½ÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐ½ÑÑÐ¸ÑÑÑ Ð¿ÐµÑÐµÐ´Ð¾Ð²ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾. Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ: ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿Ð»Ð°Ð½Ð° Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð² Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ ÐÐÐÐ¢ Ð¡ÐÐ±ÐÐ£. Ð ÑÐ²ÑÐ·Ð¸ Ñ Ð²ÑÑÐ¾ÐºÐ¸Ð¼ ÑÐµÐ¼Ð¿Ð¾Ð¼ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÐµÑÐµÐ´Ð¾Ð²ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÑÑÑÐ°Ð½Ðµ Ð¸ Ð¼Ð¸ÑÐµ Ð² ÐÐ¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¼ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐµ Ð½Ð° Ð±Ð°Ð·Ðµ Ð¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð³Ð¾ ÑÐµÐ½ÑÑÐ° Â«Ð¦ÐµÐ½ÑÑ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³Ð°Â» ÑÐ¾Ð·Ð´Ð°Ð½Ð° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð³Ð¾ Â«ÑÐ¿ÐµÑÐ½Ð°Ð·Ð°Â» - Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð¾ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð². Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð½Ð° Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸Ðµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð² Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ Ð·Ð½Ð°Ð½Ð¸Ñ Ð¾Ð± Ð¸Ð½ÑÑÐ¸ÑÑÑÐµ Ð² ÑÐµÐ»Ð¾Ð¼. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°ÑÑÐ°Ñ; Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð¼ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
Superintegrability on N-dimensional curved spaces: Central potentials, centrifugal terms and monopoles
Creators: name: Ballesteros, Angel
name: Enciso, Alberto
name: Herranz, Francisco J.
name: Ragnisco, Orlando
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mathematical Physics (math-ph)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: The N-dimensional Hamiltonian H formed by a curved kinetic term (depending on a function f), a central potential (depending on a function U), a Dirac monopole term, and N centrifugal terms is shown to be quasi-maximally superintegrable for any choice of the functions f and U. This result is proven by making use of the underlying sl(2,R)-coalgebra symmetry of H in order to obtain a set of (2N-3) functionally independent integrals of the motion, that are explicitly given. Such constants of the motion are "universal" since all of them are independent of both f and U. This Hamiltonian describes the motion of a particle on any ND spherically symmetric curved space (whose metric is specified by a function f) under the action of an arbitrary central potental U, and includes simultaneously a monopole-type contribution together with N centrifugal terms that break the spherical symmetry. Moreover, we show that two appropriate choices for U provide the "intrinsic" oscillator and the KC potentials on these curved manifolds. As a byproduct, the MIC-Kepler, the Taub-NUT and the so called multifold Kepler systems are shown to belong to this class of superintegrable Hamiltonians, and new generalizations thereof are obtained. The Kepler and oscillator potentials on N-dimensional generalizations of the four Darboux surfaces are discussed as well.
description: 22 pages
title: Abriss des vierten Traktats des dritten Teils des Liber de triplici motu
Creators: name: Trzeciok, Stefan Paul
Publisher: name: Max-Planck-Gesellschaft zur Förderung der Wissenschaften
Year: 2016

description: Kapitel 3.4.1
Kapitel 3.4.2
Kapitel 3.4.3
Kapitel 3.4.4
Kapitel 3.4.5
Fußnoten
MPEC 2023-K38 : 2023 JT4
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 JT4

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ðµ
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¡Ð¾ÐºÐ¾Ð»Ð¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ð¹ ÑÑÐµÑ
ÑÐµÐ±ÐµÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ
Ð¼ÐµÑÐ¾Ð´Ñ ÐºÐ°Ð»ÑÐºÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹
ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ ÐÐÐ ÑÐµÑÑÑÐ¾ÑÐµÑÐºÐ¸Ð¹ ÑÐ»ÐµÐ±Ð¾Ð·Ð°Ð²Ð¾Ð´
Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ
Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ°
ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸.
ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð·Ð°Ð´Ð°ÑÐ° Ð¸Ð·ÑÑÐ¸ÑÑ
ÑÑÑÐ½Ð¾ÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ°, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÑÑ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸
Ð·Ð°ÑÑÐ°Ñ,Ð¿ÑÐµÐ´Ð»Ð¾Ð¶Ð¸ÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° Ð½Ð° Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð¼ Ð¾Ð±ÑÐµÐºÑÐµ.
Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð¾Ð±ÑÐµÐ½Ð°ÑÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ,
ÑÐ°ÐºÐ¸Ðµ ÐºÐ°Ðº Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¸Ð½ÑÐµÐ·. ÐÐ»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ
Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐ»Ð¸ÑÑ Ð¼ÐµÑÐ¾Ð´Ñ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ, ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÐ½ÑÐ¹ Ð¼ÐµÑÐ¾Ð´.
Ð ÑÐ¾Ð´Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ»Ð¾ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾ ÑÑÐ¾ Ð² Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ðµ ÐÐÐ ÑÐµÑÑÑÐ¾ÑÐµÑÐºÐ¸Ð¹
Ð·Ð°Ð²Ð¾Ð´ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸ Ð¾ÑÑÑÑÑÑÐ²ÑÐµÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ°, ÑÑÐ¾
Ð¿ÑÐ¸Ð²ÐµÐ»Ð¾ Ðº Ð½Ð¸Ð·ÐºÐ¾Ð¹ ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
ÐÑÐ½Ð¾Ð²Ð½ÑÐ¼Ð¸ Ð¿ÑÑÑÐ¼Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° Ð²
Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ðµ ÐÐÐ ÑÐµÑÑÑÐ¾ÑÐµÑÐºÐ¸Ð¹ Ð·Ð°Ð²Ð¾Ð´ Ð±ÑÐ»Ð¾ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¾ Ð²ÐµÑÑÐ¸
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÑÑ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÑ,ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°ÑÑ ÑÐ°Ð±Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ 1Ð¡
Ð´Ð¾ Ð²ÐµÑÑÐ¸Ð¸ 8.2. Ð ÑÐ°Ðº Ð¶Ðµ Ð²ÐµÑÑÐ¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð·Ð° Ð¿ÐµÑÐ²Ð¸ÑÐ½Ð¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸ÐµÐ¹.
The impacts of recreation on mountain goats in Banff and Yoho national parks
Creators: name: Wrazej, Madeleine Claire
Publisher: name: University of British Columbia
Year: 2024

description: Although parks and protected areas provide essential refuges for wildlife from spreading anthropogenic disturbance, intensifying recreational pressure can have negative impacts on protected landscapes. Mountain goats (Oreamnos americanus) are sensitive to human disturbance relative to other ungulates, but the effects of recreation on mountain goats are still not well understood. Mountain goats inhabit mountainous regions of western North America, including Banff and Yoho National Parks. With visitation to these parks increasing, there is a need to quantify the potential impacts of recreation on local goat herds. My research investigated the impacts of recreation on mountain goat behaviour and stress. I used camera traps to test three main hypotheses framed by the concepts of landscape of fear, habituation and human shield. Each hypothesis predicted how recreation might differently influence goat activity patterns and habitat use, proposing negative, neutral, or positive effects respectively. Additionally, I used hair cortisol concentrations (HCC) in shed hair to assess if goats exposed to high levels of recreation pressure were more stressed than those exposed to minimal human disturbance. The results of my study found a mix of support for the landscape of fear and habituation hypotheses with regards to diel activity and habitat use. Recreation had minimal influence on goat diel activity patterns. Conversely, high weekly numbers of recreationists had an overall negative effect on goat space use with goats tending to select sites closer to escape terrain when in high human use areas. Furthermore, my results supported the prediction that goats in high human use areas are more stressed, as they had higher mean HCC levels than those exposed to minimal human disturbance. Overall, my results suggest that high levels of recreation may have subtle negative impacts on the mountain goats in these flagship national parks, highlighting the need for careful monitoring of these populations over the long term. I also demonstrated a novel use of shed mountain goat hair as a non-invasive method to measure stress in mountain goats. Furthermore, I showed how using camera traps and stress hormone sampling can provide a more comprehensive understanding of human impacts on wildlife behaviour and health.
Image, Identity and Illusion: the Ridley Monuments in St. Nicholas Cathedral, Newcastle upon Tyne
Creators: name: Pears, Richard
Publisher: name: Archaeology Data Service
Year: 2022

description: Archaeologia Aeliana, 49.5, 241-259
description: From medieval to modern times St Nicholas's Church (Cathedral since 1882) was the venue for religious and civic ceremonies, and until the nineteenth century it was a burial place for parishioners, particularly the wealthiest inhabitants. There are a significant number of eighteenth and nineteenth-century memorials and three of these, to members of the Ridley family, are discussed in this article to investigate the local, national and international identities of Newcastle's wealthiest inhabitants in the eighteenth and nineteenth centuries.
The reaction ppbar -> Lambda_c-Lambda_cbar close to threshold
Creators: name: Haidenbauer, J.
name: Krein, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Predictions for the charm-production reaction antiproton-proton -> antiLambda_c-Lambda_c for energies near the threshold are presented. The calculations are performed in a meson-exchange framework in close analogy to our earlier study on antiproton-proton -> antiLambda-Lambda by connecting the two processes via SU(4) symmetry. The obtained antiLambda_c-Lambda_c production cross sections are in the order of 1 to 7 \mub, i.e. a factor of around 10 smaller than the corresponding cross sections for antiLambda-Lambda. However, they are 100 to 1000 times larger than predictions of other model calculations in the literature.
description: 12 pages, 4 figures
title: Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¸Ð·Ð¼Ð° Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ Ð¸ ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸
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¸Ð»ÑÐµÐ²Ð°, ÐÐ°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: Ð½Ð°ÑÑÐ½ÑÐ¹ ÑÑÑÐ¸Ð·Ð¼
ÑÐµÑ Ð½Ð¾Ð¿Ð°ÑÐº
ÑÑÑÐ¸ÑÑÑÐºÐ¸Ð¹ ÑÑÐ½Ð¾Ðº
ÑÑÑÐ¸ÑÑÑÐºÐ¸Ðµ ÑÐ¸ÑÐ¼Ñ
Ð½Ð°ÑÑÐ½ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»

description: ÐÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¸Ð·Ð¼Ð° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ð¹ Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐµÑÑÐ° Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸.
ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¸ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¸Ð·Ð¼Ð°.
ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¸Ð·Ð¼Ð° Ð² Ð Ð¤.
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· Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¸ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¾Ð¿ÑÑÐ° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¸Ð·Ð¼Ð° Ð¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐµÐ³Ð¾ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸.
ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¸ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¾Ð¿ÑÑÐ° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¸Ð·Ð¼Ð° ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¼ÐµÑÑ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¸Ð·Ð¼Ð° Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¾ÑÑÐ°ÑÐ»ÑÑ.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð²Ð¸ÑÑÑÐ½ÑÑ Ð»ÐµÐºÐ°ÑÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð½ÑÑ Ð¿ÑÐµÐ¿Ð°ÑÐ°ÑÐ° Ð½ÑÐºÐ»ÐµÐ¾Ð·Ð¸Ð½Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ¸ÑÐ¸Ð½Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ¸ÑÑÑÐ¾Ð»Ð¾Ð³Ð¸Ñ
Ð²Ð¸ÑÑÑ Ð³ÑÐ¸Ð¿Ð¿Ð°
Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð²Ð¸ÑÑÑÐ½ÑÐµ Ð¿ÑÐµÐ¿Ð°ÑÐ°ÑÑ
Ð½ÑÐºÐ»ÐµÐ¾Ð·Ð¸Ð½
Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð²Ð¸ÑÑÑÐ½Ð°Ñ ÑÐµÑÐ°Ð¿Ð¸Ñ
Ð½ÑÐºÐ»Ð¾Ð¿ÑÐ¾ÑÐµÐ¸Ð½

description: ÐÐ±ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ ÑÑÑÐ¾ÐµÐ½Ð¸Ð¸ Ð²Ð¸ÑÐ¸Ð¾Ð½Ð¾Ð² Ð³ÑÐ¸Ð¿Ð¿Ð° Ð¸ Ð¸Ñ Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½Ð¾Ð¼ ÑÐ¸ÐºÐ»Ðµ. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾Ð¿ÑÐ±Ð»Ð¸ÐºÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð²Ð¸ÑÑÑÐ½Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑÑ Ð½ÑÐºÐ»ÐµÐ¾Ð·Ð¸Ð½Ð°. ÐÐ·ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ ÑÑÐ¸Ð¾ÑÑÐ¾Ð¿Ð½Ð¾Ð¹ ÑÐµÑÐ°Ð¿Ð¸Ð¸ Ð²Ð¸ÑÑÑÐ° Ð³ÑÐ¸Ð¿Ð¿Ð° Ð¸ Ð½ÑÐºÐ»ÐµÐ¾Ð¿ÑÐ¾ÑÐµÐ¸Ð½ (NP) ÐºÐ°Ðº Ð¼Ð¸ÑÐµÐ½Ñ. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð²Ð¸ÑÑÑÐ½Ð°Ñ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð½ÑÐºÐ»ÐµÐ¾Ð·Ð¸Ð½Ð° Ð¸ Ð´Ð²ÑÑ ÐµÐ³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð½ÑÑ in vitro Ð½Ð° ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑÐ°Ñ MDCK Ð¸ in vivo Ð½Ð° Ð±ÐµÐ»ÑÑ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ Ð¼ÑÑÐ°Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¾ÐºÑÐ¸ÑÐ½Ð¾ÑÑÐ¸, ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð²Ð¸ÑÑÑÐ½Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð½ÑÑ Ð½ÑÐºÐ»ÐµÐ¾Ð·Ð¸Ð½Ð°. ÐÑÐµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ²ÐµÐ´ÐµÐ½Ñ Ð² ÑÐ°Ð±Ð»Ð¸ÑÑ Ð¸ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ Ð²ÑÐµ Ð¸Ð·ÑÑÐµÐ½Ð½ÑÐµ Ð¿ÑÐµÐ¿Ð°ÑÐ°ÑÑ Ð½Ðµ ÑÐ²Ð»ÑÑÑÑÑ ÑÐ¾ÐºÑÐ¸ÑÐ½ÑÐ¼Ð¸ Ð´Ð»Ñ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑ Ð¸ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ Ð¼ÑÑÐµÐ¹. ÐÐµÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿ÑÐµÐ¿Ð°ÑÐ°ÑÑ Ð¿ÑÐ¾ÑÐ²Ð¸Ð»Ð¸ Ð²ÑÑÐ¾ÐºÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¸ Ð¿ÑÐ¾ÑÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ. Ð¡Ð¿ÐµÐºÑÑ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÐ¸Ñ Ð¿ÑÐµÐ¿Ð°ÑÐ°ÑÐ¾Ð² Ð²ÐºÐ»ÑÑÐ°Ð» ÐºÐ°Ðº Ð²Ð¸ÑÑÑÑ Ð³ÑÐ¸Ð¿Ð¿Ð° Ð, ÑÐ°Ðº Ð¸ Ð³ÑÐ¸Ð¿Ð¿Ð° B. Ð Ð¾Ð¿ÑÑÐ°Ñ in vivo ÑÑÐ¸ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ ÑÐ½Ð¸Ð¶Ð°Ð»Ð¸ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð³Ð¸Ð±ÐµÐ»Ð¸ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ Ð½Ð° 37,5% Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ Ð³ÑÑÐ¿Ð¿Ð¾Ð¹ Ð¿Ð»Ð°ÑÐµÐ±Ð¾, Ð½Ð¾ÑÐ¼Ð°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð»Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÑ Ð²ÐµÑÐ° Ð¸ Ð´Ð¾ÑÑÐ¾Ð²ÐµÑÐ½Ð¾ ÑÐ½Ð¸Ð¶Ð°Ð»Ð¸ ÑÐ°Ð·Ð¼ÐµÑÑ Ð¾ÑÐ°Ð³Ð¾Ð² Ð¿Ð¾ÑÑÐ³ÑÐ¸Ð¿Ð¿Ð¾Ð·Ð½Ð¾Ð¹ Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð½Ð¸Ð¸. Ð¢Ð°ÐºÐ¸Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼, Ð½ÑÐºÐ»ÐµÐ¾Ð·Ð¸Ð½ Ð¸ ÐµÐ³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð½ÑÐµ ÑÐ²Ð»ÑÑÑÑÑ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½ÑÐ¼Ð¸ Ð¿ÑÐµÐ¿Ð°ÑÐ°ÑÐ°Ð¼Ð¸ Ð´Ð»Ñ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹.
THE DEGREE OF STUDY OF THE CONCEPT "CHILD" IN DIFFERENT LANGUAGES
Creators: name: Yakubova, Gulnoza
Publisher: name: Zenodo
Year: 2024

description: Linguoculturology is an interdisciplinary field that merges linguistics and cultural studies. It examines how language and culture influence each other, focusing on the ways in which linguistic practices reflect cultural norms, values, and identities.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð³ÑÐ°ÑÐµÐ½Ð° Ð¿ÑÐ¸ Ð¿Ð¾ÑÑÑÐ¾ÑÑÐ¾Ð²Ð¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐµ
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¢Ð¾Ð½ÐºÐ¾Ð², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð³ÑÐ°ÑÐµÐ½
Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ°
ÑÐ´ÐµÐ»ÑÐ½Ð¾Ðµ ÑÐ¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ðµ
Ð±Ð¾Ð¼Ð±Ð°ÑÐ´Ð¸ÑÐ¾Ð²ÐºÐ° Ð¸Ð¾Ð½Ð°Ð¼Ð¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð³ÑÐ°ÑÐµÐ½, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐ¹ Ð¡VDÐ¼ÐµÑÐ¾Ð´Ð¾Ð¼. Ð¦ÐµÐ»ÑÑ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð¹ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ ÑÐ´ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ñ Ð³ÑÐ°ÑÐµÐ½Ð°, Ð¿Ð¾ÑÐ»Ðµ ÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð² ÑÐ¼ÐµÑÐ¸ Ð³Ð°Ð·Ð¾Ð² Ð°ÑÐ³Ð¾Ð½Ð° Ð¸ Ð²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð°, Ð¸ Ð¿Ð¾ÑÐ»Ðµ Ð±Ð¾Ð¼Ð±Ð°ÑÐ´Ð¸ÑÐ¾Ð²ÐºÐ¸ Ð¸Ð¾Ð½Ð°Ð¼Ð¸ Ð°ÑÐ³Ð¾Ð½Ð°. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÐ¹ Ð¾Ð±Ð·Ð¾Ñ, Ð² ÐºÐ¾ÑÐ¾ÑÐ¾Ð¼ Ð¿Ð¸ÑÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð³ÑÐ°ÑÐµÐ½Ð° Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ ÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¢Ð°ÐºÐ¶Ðµ, Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ². ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ ÑÐ´ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ñ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ Ð¿Ð¾Ð´ Ð´ÐµÐ¹ÑÑÐ²Ð¸ÐµÐ¼ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÑÐ»Ð¾Ð²Ð¸Ñ ÑÐ¸Ð½ÑÐµÐ·Ð° Ð½Ð° ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸ÑÑÐ¾Ð´Ð½ÑÑ Ð¾Ð±ÑÐ°Ð·ÑÐ¾Ð².
On the effective action of confining strings
Creators: name: Aharony, Ofer
name: Karzbrun, Eyal
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We study the low-energy effective action on confining strings (in the fundamental representation) in SU(N) gauge theories in D space-time dimensions. We write this action in terms of the physical transverse fluctuations of the string. We show that for any D, the four-derivative terms in the effective action must exactly match the ones in the Nambu-Goto action, generalizing a result of Luscher and Weisz for D=3. We then analyze the six-derivative terms, and we show that some of these terms are constrained. For D=3 this uniquely determines the effective action for closed strings to this order, while for D>3 one term is not uniquely determined by our considerations. This implies that for D=3 the energy levels of a closed string of length L agree with the Nambu-Goto result at least up to order 1/L^5. For any D we find that the partition function of a long string on a torus is unaffected by the free coefficient, so it is always equal to the Nambu-Goto partition function up to six-derivative order. For a closed string of length L, this means that for D>3 its energy can, in principle, deviate from the Nambu-Goto result at order 1/L^5, but such deviations must always cancel in the computation of the partition function. Next, we compute the effective action up to six-derivative order for the special case of confining strings in weakly-curved holographic backgrounds, at one-loop order (leading order in the curvature). Our computation is general, and applies in particular to backgrounds like the Witten background, the Maldacena-Nunez background, and the Klebanov-Strassler background. We show that this effective action obeys all of the constraints we derive, and in fact it precisely agrees with the Nambu-Goto action (the single allowed deviation does not appear).
description: 71 pages, 7 figures. v2: added reference, minor corrections. v3: removed one term from the effective action since it is trivial. The conclusions on the corrections to energy levels are unchanged, but the claim that the holographic computation shows a deviation from Nambu-Goto was modified. v4: added references
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð²
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÑÐºÐ¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð°Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÑ
ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÑ
Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ

description: Ð Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐºÑÑÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐ¸ÑÑÐ°Ð½ ÐÑÐ½ÑÑÑÐºÑÑÑÐ¸Ð½Ð³ Ð ÑÑÂ», Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ð¹ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ°, ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð², Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÐµÐ¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð²ÑÐ±ÑÐ°Ð½ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ Ð²Ð¸Ð·ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð½Ð¾ÑÐ°ÑÐ¸Ð¸ IDEF0 Ð² Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ¿ÐµÐ½Ð¸ Ð¿ÑÐ¸Ð¼ÐµÐ½Ð¸Ð¼ÑÐ¹ Ð´Ð»Ñ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð´Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ° (AS-TO-BE). Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ°, Ð² ÑÐ°Ð¼ÐºÐ°Ñ ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¾, ÑÑÐ¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½ÑÐ¼ Ð¸ Ð²ÑÐ³Ð¾Ð´Ð½ÑÐ¼ Ð´Ð»Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Diderma umbilicatum Pers.
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Physarales
Didymiaceae
Diderma
Diderma umbilicatum

description: ● Diderma umbilicatum Pers.,
pērļainā olīte
- leg. L.Birziņa, 12 Dec 2020, Ādaži, on mosses and deciduous log in a deciduous forest, det. E.Johannesen, 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
Improvement of Text Dependent Speaker Identification System Using Neuro-Genetic Hybrid Algorithm in Office Environmental Conditions
Creators: name: Islam, Md. Rabiul
name: Rahman, Md. Fayzur
Publisher: name: arXiv
Year: 2009
Subjects: subject: Sound (cs.SD)
subject: FOS: Computer and information sciences

description: In this paper, an improved strategy for automated text dependent speaker identification system has been proposed in noisy environment. The identification process incorporates the Neuro- Genetic hybrid algorithm with cepstral based features. To remove the background noise from the source utterance, wiener filter has been used. Different speech pre-processing techniques such as start-end point detection algorithm, pre-emphasis filtering, frame blocking and windowing have been used to process the speech utterances. RCC, MFCC, MFCC, MFCC, LPC and LPCC have been used to extract the features. After feature extraction of the speech, Neuro-Genetic hybrid algorithm has been used in the learning and identification purposes. Features are extracted by using different techniques to optimize the performance of the identification. According to the VALID speech database, the highest speaker identification rate of 100.000 percent for studio environment and 82.33 percent for office environmental conditions have been achieved in the close set text dependent speaker identification system.
description: International Journal of Computer Science Issues (IJCSI), Volume 1, pp42-48, August 2009
The excavation of a waggonway at Newbottle, Tyne and Wear
Creators: name: C Platell, Andrew
name: M T Walsh, Rebekah
Publisher: name: Archaeology Data Service
Year: 2022

description: Archaeologia Aeliana, 49.5, 261-277
description: A length of waggonway was excavated and recorded at Newbottle, Tyne and Wear. The waggonway fabric had been recycled following decommissioning, but the remains indicate that it had originally consisted of one line of wooden sleepers directly overlying the natural ground surface, with rails above. Clay and stone ballast filled the gaps between the sleepers. The waggonway had a gauge of 1.22m (4ft 0in). A drainage ditch was present on each side; there was a second later ditch on the east side. The remains are thought to be a previously unrecorded part of the original line of the Newbottle waggonway, serving pits to the south. It is thought to date to the mid-18th century. Cartographic evidence shows it was decommissioned and dismantled by 1817 at the latest. The Newbottle waggonway was extensively remodelled in 1812, but no indications of any alterations were identified in the excavated section, suggesting that closure predated this remodelling.
Galaxy formation with cold gas accretion and evolving stellar initial mass function
Creators: name: Kang, Xi
name: Lin, WeiPeng
name: Skibba, Ramin A.
name: Chen, Dongni
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The evolution of the galaxy stellar mass function is especially useful to test the current model of galaxy formation. Observational data have revealed a few inconsistencies with predictions from the $Λ{\rm CDM}$ model. For example, most massive galaxies have already been observed at very high redshifts, and they have experienced only mild evolution since then. In conflict with this, semi-analytical models of galaxy formation predict an insufficient number of massive galaxies at high redshift and a rapid evolution between redshift 1 and 0 . In addition, there is a strong correlation between star formation rate and stellar mass for star-forming galaxies, which can be roughly reproduced with the model, but with a normalization that is too low at high redshift. Furthermore, the stellar mass density obtained from the integral of the cosmic star formation history is higher than the measured one by a factor of 2. In this paper, we study these issues using a semi-analytical model that includes: 1) cold gas accretion in massive halos at high redshift; 2) tidal stripping of stellar mass from satellite galaxies; and 3) an evolving stellar initial mass function (bottom-light) with a higher gas recycle fraction. Our results show that the combined effects from 1) and 2) can predict sufficiently massive galaxies at high redshifts and reproduce their mild evolution at low redshift, While the combined effects of 1) and 3) can reproduce the correlation between star formation rate and stellar mass for star-forming galaxies across wide range of redshifts. A bottom-light/top-heavy stellar IMF could partly resolve the conflict between the stellar mass density and cosmic star formation history.
description: 9 pages, 7 figures. Accepted for publication in ApJ
A Pluzhnikov's Theorem, Brownian motions and Martingales in Lie Group with skew-symmetric connections
Creators: name: Stelmastchuk, S. N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Differential Geometry (math.DG)
subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 53C43, 58E20, 58J65, 60H30, 60G48

description: Let $G$ be a Lie Group with a left invariant connection such that its connection function is skew-symmetric. Our main goal is to show a version of Pluzhnikov's Theorem for this kind of connection. To this end, we use the stochastic logarithm. More exactly, the stochastic logarithm gives characterizations for Brownian motions and Martingales in $G$, and these characterzations are used to prove Pluzhnikov's Theorem.
description: 14 pages
Big Bang Nucleosynthesis and Particle Dark Matter
Creators: name: Jedamzik, Karsten
name: Pospelov, Maxim
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We review how our current understanding of the light element synthesis during the Big Bang Nucleosynthesis era may help shed light on the identity of particle dark matter.
description: a mini-review for the NJP special issue on dark matter
Covariant density functional theory: The role of the pion
Creators: name: Lalazissis, G. A.
name: Karatzikos, S.
name: Serra, M.
name: Otsuka, T.
name: Ring, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We investigate the role of the pion in Covariant Density Functional Theory. Starting from conventional Relativistic Mean Field (RMF) theory with a non-linear coupling of the $σ$-meson and without exchange terms we add pions with a pseudo-vector coupling to the nucleons in relativistic Hartree-Fock approximation. In order to take into account the change of the pion field in the nuclear medium the effective coupling constant of the pion is treated as a free parameter. It is found that the inclusion of the pion to this sort of density functionals does not destroy the overall description of the bulk properties by RMF. On the other hand, the non-central contribution of the pion (tensor coupling) does have effects on single particle energies and on binding energies of certain nuclei.
description: 12 pages, 5 figures
Towards a Complete Census of AGNs in Nearby Galaxies: The Incidence of Growing Black Holes
Creators: name: Goulding, Andy D.
name: Alexander, David M.
name: Lehmer, Bret D.
name: Mullaney, James R.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We investigate the local supermassive black hole (SMBH) density function and relative mass accretion rates of all active galactic nuclei (AGNs) identified in a volume-limited sample of infrared (IR) bright galaxies (L_IR > 3 x 10^9 L_sun) to D<15 Mpc (Goulding & Alexander 2009). A database of accurate SMBH mass (M_BH) estimates is compiled from literature sources using physically motivated AGN modeling techniques (reverberation mapping, maser mapping and gas kinematics) and well-established indirect M_BH estimation methods (the M-sigma and M_BH-L_(K,bul) relations). For the three sources without previously published M_BH estimates, we use 2MASS K-band imaging and GALFIT to constrain the bulge luminosities, and hence SMBH masses. In general, we find the AGNs in the sample host SMBHs which are spread over a wide mass range (M_BH ~ (0.1-30) x 10^7 M_sun), but with the majority in the poorly studied M_BH ~ 10^6-10^7 M_sun region. Using sensitive hard X-ray (2-10 keV) and mid-IR constraints we calculate the bolometric luminosities of the AGNs (L_(Bol,AGN)) and use them to estimate relative mass accretion rates. We use these data to calculate the volume-average SMBH growth rate of galaxies in the local Universe and find that the AGNs hosting SMBHs in the mass range M_BH ~ 10^6-10^7 M_sun are dominated by optically unidentified AGNs. These relatively small SMBHs are acquiring a significant proportion of their mass in the present-day, and are amongst the most rapidly growing in the local Universe (SMBH mass doubling times of ~6 Gyrs). Additionally, we find tentative evidence for an increasing volume-weighted AGN fraction with decreasing SMBH mass in the M_BH ~ 10^6-10^8 M_sun range. Overall, we conclude that significant mass accretion onto small SMBHs may be missed in even the most sensitive optical surveys due to absent or weak optical AGN signatures.
description: 17 pages, 5 figures. Accepted for publication in MNRAS
title: Ð¡Ð»ÐµÐ½Ð³ Ð°Ð½Ð³Ð»Ð¾ÑÐ·ÑÑÐ½ÑÑ Ð²Ð¸Ð´ÐµÐ¾Ð¸Ð³Ñ Ð² ÑÐ°Ð·Ð³Ð¾Ð²Ð¾ÑÐ½Ð¾Ð¹ ÑÐµÑÐ¸ (Ð½Ð° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ðµ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¸ ÑÑÑÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ¾Ð²)
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ÑÐ¾Ð³Ð»ÑÐ´Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ»ÐµÐ½Ð³
Ð·Ð°Ð¸Ð¼ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ
Ð²Ð¸Ð´ÐµÐ¾Ð¸Ð³ÑÑ
Ð°Ð½Ð³Ð»Ð¸ÑÐ¸Ð·Ð¼Ñ
ÑÐ°Ð·Ð³Ð¾Ð²Ð¾ÑÐ½Ð°Ñ ÑÐµÑÑ
ÑÐ¾ÑÐ¸Ð¾Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÐºÐ°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¿ÑÑÐ¸ Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ñ Ð·Ð°Ð¸Ð¼ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐ½Ð³Ð¾Ð²ÑÑ ÑÐ»Ð¾Ð² Ð¸Ð· ÑÑÐµÑÑ Ð²Ð¸Ð´ÐµÐ¾Ð¸Ð³Ñ Ð² ÑÐ°Ð·Ð³Ð¾Ð²Ð¾ÑÐ½ÑÑ ÑÐµÑÑ. ÐÐ°Ð½Ñ Ð¾Ð±ÑÐ¸Ðµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¸ Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ñ Ð¸ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð·Ð°Ð¸Ð¼ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð±ÑÐ°Ð½Ð½ÑÑ Ð¿ÑÑÐµÐ¼ ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð¿ÑÐ¾ÑÐ° ÑÐ»Ð¾Ð², Ð²ÑÐ¾Ð´ÑÑÐ¸Ñ Ð² Ð´Ð°Ð½Ð½ÑÐ¹ ÑÐ»ÐµÐ½Ð³. Ð¡Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÑÑÐ¸Ñ ÑÐ»Ð¾Ð² Ñ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸ÐµÐ¼ ÑÐ¿Ð¾ÑÐ¾Ð±Ð° Ð¸Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¾Ð»ÐºÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸, ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð² Ð½Ð°Ð·Ð²Ð°Ð½Ð¸ÑÑ Ð²Ð½ÑÑÑÐ¸Ð¸Ð³ÑÐ¾Ð²ÑÑ Ð¿ÑÐµÐ´Ð¼ÐµÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸Ñ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð°.
Excavations of the waggonway, early iron railway, and workers housing at Redburn Row, Chilton Moor, Sunderland
Creators: name: C Platell, Andrew
name: J Randerson, M
Publisher: name: Archaeology Data Service
Year: 2022

description: Archaeologia Aeliana, 49.5, 279-302
description: This article presents the results of archaeological works conducted in advance of a development at Redburn Row, Chilton Moor, Sunderland. Two waggonway tracks were recorded, an embanked track to the west and an unembanked one to the east. The embanked track was the earlier, dating from the 18th century, and had remained in use until the late 19th century. The lower track was a later addition, dating from the 1820s, and had been built with iron rails. It was only used for a short time before being abandoned without modification; it therefore presents a clear example of early iron rail technology. Two phases of a domestic coal depot were located to the east of the embankment, the latter phase was cut into the side of the embankment and partly truncated the lower track. A 19th century housing terrace was also excavated elsewhere on the site. All features were covered by coal waste overlain by clay, deposited as a 20th-century ground remediation measure.
Endochronic theory, non-linear kinematic hardening rule and generalized plasticity: a new interpretation based on generalized normality assumption
Creators: name: Erlicher, Silvano
name: Point, Nelly
Publisher: name: arXiv
Year: 2008
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: A simple way to define the flow rules of plasticity models is the assumption of generalized normality associated with a suitable pseudo-potential function. This approach, however, is not usually employed to formulate endochronic theory and non-linear kinematic (NLK) hardening rules as well as generalized plasticity models. In this paper, generalized normality is used to give a new formulation of these classes of models. As a result, a suited pseudo-potential is introduced for endochronic models and a non-standard description of NLK hardening and generalized plasticity models is also provided. This new formulation allows for an effective investigation of the relationships between these three classes of plasticity models.
title: ÐÑÑÐ¾ÑÐ¸Ñ ÐºÐ½Ð¸Ð¶Ð½Ð¾Ð³Ð¾ Ð´ÐµÐ»Ð°. Ð§. 4
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð Ð¾ÑÑÐ¾Ð²ÑÐµÐ², ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: ÐÐ½Ð¸Ð³Ð°
ÐºÐ½Ð¸Ð¶Ð½Ð¾Ðµ Ð´ÐµÐ»Ð¾
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Ð¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ 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° Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ âÐÑÑÐ¾ÑÐ¸Ñ ÐºÐ½Ð¸Ð¶Ð½Ð¾Ð³Ð¾ Ð´ÐµÐ»Ð°â. Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» ÑÑÐµÑ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² ÐºÑÑÑÐ° (ÑÐµÐ¼Ñ 7-8), Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð½ÑÑ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ ÐºÐ½Ð¸Ð³Ð¸ XIX â Ð½Ð°ÑÐ°Ð»Ð° XX Ð². Ð¢ÐµÐ¼Ð° 7 Ð¾ÑÐ²Ð°ÑÑÐ²Ð°ÐµÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð», ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐ¹ Ñ Ð¸ÑÑÐ¾ÑÐ¸ÐµÐ¹ ÐºÐ½Ð¸Ð¶Ð½Ð¾Ð³Ð¾ Ð´ÐµÐ»Ð° Ð·Ð° ÑÑÐ±ÐµÐ¶Ð¾Ð¼, ÑÐµÐ¼Ð° 8 Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ¾ÑÐ¸Ð¸ ÐºÐ½Ð¸Ð¶Ð½Ð¾Ð³Ð¾ Ð´ÐµÐ»Ð° Ð² Ð Ð¾ÑÑÐ¸Ð¸. ÐÐ¾ ÐºÐ°Ð¶Ð´Ð¾Ð¹ ÑÐµÐ¼Ðµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½ ÑÐ¿Ð¸ÑÐ¾Ðº ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÐ¼Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ âÐÐ·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ðµ Ð´ÐµÐ»Ð¾â, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ Ð´Ð»Ñ ÑÐ¸ÑÐ¾ÐºÐ¾Ð³Ð¾ ÐºÑÑÐ³Ð° ÑÐ¸ÑÐ°ÑÐµÐ»ÐµÐ¹, Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸ÑÑÑ Ð¸ÑÑÐ¾ÑÐ¸ÐµÐ¹ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð¹ Ð¸ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ½Ð¸Ð¶Ð½Ð¾Ð¹ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¸.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Psychological consequences of financial scarcity
Creators: name: Tomm, Brandon M.
Publisher: name: University of British Columbia
Year: 2024

description: Financial scarcity affects attention and decision making, but it is not known how these effects translate to behaviours which can make the condition of scarcity even worse. It is also not well understood which cognitive mechanisms are affected by scarcity. In 10 experiments, I used a variety of scarcity-induction methods and scarcity measurements to examine how scarcity can affect a variety of psychological processes. I found that scarcity induced an attentional bias such that people under an objective financial constraint were not able to adaptively up-regulate attention to useful information, resulting in a reduction in the use of a useful discount that would have alleviated the financial constraint in the first place (Chapter 2). Follow-up studies suggested that the attentional burden of scarcity can be partially alleviated by moving crucial information closer to the centre of focus (Chapter 3). Next, I used a numerical perception paradigm to investigate how both scarcity-scenario priming and cognitive load affect perception of hypothetical future income and future expenses (Chapter 4). This paradigm was extensively fruitful in showing how objective scarcity, subjective scarcity, and relative subjective scarcity can have independent effects on numerical perception. In general, people under objective scarcity estimate lower totals of future income and expenses while people under subjective scarcity estimated higher totals of future income and expenses. This is a novel finding with important theoretical implications for the scarcity literature: Scarcity is not a unitary construct and future research must account for the variety of ways scarcity can be experienced. Finally, I investigated how scarcity affects attention and decision making with regard to a job advertisement (Chapter 5). I found no evidence that scarcity affects how people attended to the job advertisement. These results support the need to differentiate the different varieties of scarcity in future research.
title: Ð¤Ð¸Ð·Ð¸ÐºÐ° Ð¿Ð»Ð°Ð·Ð¼Ñ. ÐÑÐ°ÐºÑÐ¸ÐºÑÐ¼
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² "Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°"
titleType: Subtitle
Creators: name: ÐÑÐ»Ð°Ð½Ð¸Ð½, ÐÐ¸ÐºÑÐ¾Ñ
name: Ð Ð¾Ð¶Ð°Ð½ÑÐºÐ¸Ð¹, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: Ð¡ÐµÐ½Ð¸ÑÐµÐ½ÐºÐ¾Ð², ÐÐ»ÑÑ
name: Ð¡Ð¼Ð¸ÑÐ½Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: Ð§ÐµÑÐ½Ð¾Ð¸Ð·ÑÐ¼ÑÐºÐ°Ñ, Ð¢Ð°ÑÑÑÐ½Ð°
name: Ð¨Ð°ÑÐ°Ð»Ð¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
name: Ð¯ÑÑÐºÐ¾Ð²Ð°, 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Ð»Ð°Ð·Ð¼Ð° (ÑÐ¸Ð·.)

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ 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° Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ âÐ¤Ð¸Ð·Ð¸ÐºÐ° Ð¿Ð»Ð°Ð·Ð¼Ñâ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 011200 âÐ¤Ð¸Ð·Ð¸ÐºÐ°â, Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ âÐ¤Ð¸Ð·Ð¸ÐºÐ° Ð¿Ð»Ð°Ð·Ð¼Ñâ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 223200 âÐ¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°â, Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ âÐÐ°ÐºÑÑÐ¼Ð½Ð°Ñ Ð¸ Ð¿Ð»Ð°Ð·Ð¼ÐµÐ½Ð½Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°â Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 210100 âÐ­Ð»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ° Ð¸ Ð½Ð°Ð½Ð¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°â, Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½ â Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¿Ð»Ð°Ð·Ð¼Ñâ Ð¸ âÐ¤Ð¸Ð·Ð¸ÐºÐ° Ð½Ð¸Ð·ÐºÐ¾ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°Ð·Ð¼Ñâ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 011200 âÐ¤Ð¸Ð·Ð¸ÐºÐ°â. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð·Ð°Ð´Ð°ÑÐ¸, Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ Ð½Ð° Ð·Ð°ÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹, Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¸Ð·Ð¸ÐºÐ¸ Ð¿Ð»Ð°Ð·Ð¼Ñ Ð¸ Ð¾ÑÐ²Ð°ÑÑÐ²Ð°ÑÑÐ¸Ðµ Ð¿Ð¾ ÑÐµÐ¼Ð°ÑÐ¸ÐºÐµ Ð²ÑÐµ ÑÐ°Ð·Ð´ÐµÐ»Ñ Ð¿ÐµÑÐµÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½. ÐÐ°Ð´Ð°ÑÐ¸ Ð² ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ ÑÐ³ÑÑÐ¿Ð¿Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿Ð¾ ÐºÑÑÑÐ°Ð¼ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½, Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¾Ð½Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐÐ½ÑÑÐ¸ÑÑÑÐ° ÑÐ¸Ð·Ð¸ÐºÐ¸, Ð½Ð°Ð½Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
The relativistic equation of motion in turbulent jets
Creators: name: Zaninetti, Lorenzo
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The turbulent jets are usually described by classical velocities. The relativistic case can be treated starting from the conservation of the relativistic momentum. The two key assumptions which allow to obtain a simple expression for the relativistic trajectory and relativistic velocity are null pressure and constant density.
description: 2 figures 7 pages
An Apple Tree on Hadrian's Wall at Denton
Creators: name: J Breeze, David
Publisher: name: Archaeology Data Service
Year: 2022

description: Archaeologia Aeliana, 49.5, 303-306
description: The possibility that an apple tree in the former vicarage garden at Stamfordham is a descendant of the twigs taken from the apple tree at Denton in 1845 by the Rev. J. F. Bigge is considered.
Bayesian inference of jet bulk-flow speeds in FRII radio sources
Creators: name: Mullin, L. M.
name: Hardcastle, M. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Radio jet and core data for a complete sample of 98 FRII sources with z < 1 are analysed with a Markov-Chain Monte Carlo (MCMC) model fitting method to obtain constraints on bulk-flow speeds in the beam. The Bayesian parameter-inference method is described and demonstrated to be capable of providing meaningful constraints on the Lorentz factor at both kiloparsec and parsec scales. For both jets and cores we show that models in which some intrinsic dispersion is present in the features' intrinsic prominence, bulk-flow speeds or both provide the best fit to the data. The constraints on the Lorentz factor on parsec scales are found to be consistent with the expected values given VLBI observations and other evidence, with mean gamma ~ 10-14. On kiloparsec scales, the Lorentz factor is found to be ~ 1.18 - 1.49, in agreement with the results of previous analyses of radio jet data. These values are clearly not consistent with the gamma ~ 10 speeds required by beamed inverse-Compton models of X-ray emission from quasar jets; our results therefore support models that require velocity structure in powerful jets.
description: 17 pages, 5 tables, 5 figures