cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð²ÐµÐ¹Ð²Ð»ÐµÑ-Ð½ÐµÐ¹ÑÐ¾ÑÐµÑÐµÐ¹ Ð´Ð»Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ ÑÐ³ÑÐ¾Ð· Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð¼ÐµÐ¶Ð¼Ð°ÑÐ¸Ð½Ð½ÑÑ ÑÐµÑÑÑ VANET
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ´ÑÐ¼Ð°Ðº, ÐÐ½Ð´Ñ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°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÐµÑÐµÐ¹ VANET
Ð²ÐµÐ¹Ð²Ð»ÐµÑ-Ð½ÐµÐ¹ÑÐ¾ÑÐµÑÑ
Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÑÑ ÑÐµÑÐµÐ¹
ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ
QOS

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° ÑÑÑÐ½Ð¾ÑÑÑ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ ÑÐ³ÑÐ¾Ð· Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° Ð´Ð¾ÑÑÑÐ¿Ð½Ð¾ÑÑÑ ÑÐµÑÐ¸, Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð²ÐµÐ¹Ð²Ð»ÐµÑ-Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²ÐµÐ¹Ð²Ð»ÐµÑ ÑÑÐ½ÐºÑÐ¸Ð¹. ÐÐ·ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð°ÑÐ°Ðº Ð½Ð° VANET. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ð¹ ÑÐµÑÐ¸ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð²ÐµÐ¹Ð²Ð»ÐµÑ-Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð².
Low $Q^2$ proton structure function, using gluon and pseudoscalar meson clouds in the constituent quark framework
Creators: name: Mirjalili, A.
name: Yazdanpanah, M. M.
name: Taghavi-Shahri, F.
name: Ghorbani, K.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The idea of the meson cloud approach in the chiral quark model has been extended to include gluon cloud in order to achieve the parton densities in the nucleon, based on the constitute quark framework. The splitting function of the quark to the quark-meson and quark-gluon at low $Q^2$ value are used to obtain parton densities in the constituent quark. The phenomenological constituent model is employed to extract the parton distributions in the proton at low $Q^2$ value. Since we have access to the parton densities at low $Q^2$, we are able to obtain $F_{2}(x,Q^2)$ structure function at low $Q^2$ value. The result is in good agreement with available experimental data and some theoretical models. To confirm the validity of our calculations, the fraction of total momentum of proton which is carried by gluon at high $Q^2$ and also the Gottfried sum rule are computed. The results are in good agreement with what are expected.
description: 13 pages, 3 figures
Equations for General Perturbation Method for Satellite Constellation Reconfiguration Using Low-Thrust Maneuvers
Creators: name: McGrath, Ciara
name: Macdonald, Malcolm
Publisher: name: Zenodo
Year: 2019

description: Equations from the paper General Perturbation Method for Satellite Constellation Reconfiguration Using Low-Thrust Maneuvers published in the AIAA Journal of Guidance, Control, and Dynamics. The equations are provided in forms suitable for use in Wolfram Mathematica (.nb), Matlab (.m) and Python (.py).
Common origin of the shoulder structure and of the oscillations of
  moments in multiplicity distributions in e(+)e(-) annihilations
Creators: name: Giovannini, Alberto
name: Lupia, Sergio
name: Ugoccioni, Roberto
Publisher: name: INFN Open Access Repository
Year: 1996

description: We show, via a simple parametrization of the multiplicity distribution of
charged particles in e(+)e(-) annihilation at the Z0 peak in terms of the
weighted superposition of two negative binomial distributions, that both the
shoulder structure in the intermediate multiplicity range and the oscillation
in sign of the ratio of factorial cumulants over factorial moments of
increasing order are related to hard gluon radiation.
On the Effect of Magnetic Spots on Stellar Winds and Angular Momentum Loss
Creators: name: Cohen, O.
name: Drake, J. J.
name: Kashyap, V. L.
name: Gombosi, T. I.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We simulate the effect of latitudinal variations in the location of star spots, as well as their magnetic field strength, on stellar angular momentum loss to the stellar wind. We use the Michigan solar corona global MagnetoHydroDynamic model, which incorporates realistic relation between the magnetic field topology and the wind distribution. We find that the spots location significantly affects the stellar wind structure, and as a result, the total mass loss rate and angular momentum loss rate. In particular, we find that the angular momentum loss rate is controlled by the mass flux when spots are located at low latitudes but is controlled by an increased plasma density between the stellar surface and the Alfven surface when spots are located at high latitudes. Our results suggest that there might be a feedback mechanism between the magnetic field distribution, wind distribution, angular momentum loss through the wind, and the motions at the convection zone that generate the magnetic field. This feedback might explain the role of coronal magnetic fields in stellar dynamos.
Multiparticle production in high-mass diffraction dissociation and the
  interplay of photons and pomerons
Creators: name: F. W. Bopp
name: R. Engel
name: J. Ranft
name: A. Rostovtsev
Publisher: name: INFN Open Access Repository
Year: 1997

description: Multiple interaction models satisfying $s$-channel unitarity predict that, in
contrast to inelastic processes, factorization is violated in diffractive
processes. The size of this effect can be characterized in terms of the
rapidity gap survival probability. The possibility of its measurement at HERA
is pointed out. Furthermore a method to measure photon diffraction dissociation
at LEP2 and planned linear colliders is discussed and cross section predictions
are given.
title: ÐÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð² ÐÐÐ "ÐÐ°Ð»ÑÐ¸Ð¹ÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÐµÐºÑ"
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐ¿Ð¾ÑÑÑÐºÐ¾ , 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: 2017
Subjects: ÑÑÑÑÐºÑÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ
ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹ ÑÑÐ½Ð¾Ðº Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸
ÑÑÑÑÐºÑÑÑÐ° ÑÐµÐ¿Ð¸ Ð¿Ð¾ÑÑÐ°Ð²Ð¾Ðº

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ Ð±Ð°Ð·Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¿Ð¾ÑÐºÐ¸ Ð¿Ð¾ÑÑÐ°Ð²Ð¾Ðº Ñ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸ÐµÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð²ÑÐ±Ð¾ÑÐ°, Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð² Ð¸ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸ÐµÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð². ÐÑÐ±ÑÐ°Ð½ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐ¸Ð¹ Ð¼ÐµÑÐ¾Ð´ Ð¸ÐµÑÐ°ÑÑÐ¸Ð¸ Ð¢. Ð¡Ð°Ð°ÑÐ¸. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð°Ñ Ð¾ÑÐµÐ½ÐºÐ° Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½ Ð¿Ð¾Ð»Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð¿ÑÐ¸Ð¾ÑÐ¸ÑÐµÑÐ¾Ð² Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐµÑÐ¾Ð².
Renormalons and Higher-Twist Contributions to Structure Functions
Creators: name: M. Maul
name: E. Stein
name: L. Mankiewicz
name: M. Meyer-Hermann
name: A. Schafer
Publisher: name: INFN Open Access Repository
Year: 1997

description: We review the possibility to use the renormalons emerging in the perturbation
series of the twist-2 part of the nonsinglet structure functions FL, F2, F3,
and g1 to make approximate predictions for the magnitude of the appertaining
twist-4 corrections.
Determination of the CKM unitarity triangle parameters by end 1999
Creators: name: F. Caravaglios
name: F. Parodi
name: P. Roudeau
name: A. Stocchi
Publisher: name: INFN Open Access Repository
Year: 2000

description: Within the Standard Model, a review of the current determination of the CKM
unitarity triangle parameters is presented, using experimental constraints from
the measurements of |epsilon_K|, V_ub/V_cb, Delta m_d and from the limit on
Delta m_s, available by end 1999.
Particle candidates for dark matter: a case for (dominant or
  subdominant) relic neutralinos
Creators: name: A. Bottino
name: F. Donato
name: N. Fornengo
name: S. Scopel
Publisher: name: INFN Open Access Repository
Year: 2001

description: After a short introduction on particle candidates for dark matter within
possible extensions of the standard model, we concentrate on Weakly Interacting
Massive Particles, and on one of their most interesting physical realizations:
the neutralino. We analyze how detectability of relic neutralinos by direct and
indirect means is related to their local and cosmological densities; we use
simple general arguments to discusss different scenarios where relic
neutralinos make up the dominant bulk of dark matter or only a small fraction
of it. Our general arguments are further corroborated by specific numerical
results. We show to which extent the present experiments of direct searches for
WIMPs, when interpreted in terms of relic neutralinos, probe interesting
regions of the supersymmetric parameter space. Our analysis is performed in a
number of different supersymmetric schemes.
Geoneutrino Analysis in KamLAND: Input and Desiderata
Creators: name: G. L. Fogli
name: E. Lisi
name: A. Palazzo
name: A. M. Rotunno
Publisher: name: INFN Open Access Repository
Year: 2004

description: The Kamioka Liquid scintillator Anti-Neutrino Detector (KamLAND) is
collecting antineutrino events generated by nuclear reactors and by Thorium and
Uranium decay in the Earth interior. We comment on a systematic approach to the
evaluation of the geo-neutrino contribution and of its uncertainties in
KamLAND, taking into account geophysical and geochemical indications,
estimates, and data. The results can help to improve both the neutrino
oscillation analysis and the knowledge of the Earth interior. Input and
desiderata for future geoneutrino analyses are identified.
Comment on "Groverian Entanglement Measure and Evolution of Entanglement in Search Algorithm for n(= 3, 5)-Qubit Systems with Real Coefficients" (Volume 6, Number 4, August 2007), by Arti Chamoli and C. M. Bhandari
Creators: name: Parashar, Preeti
name: Rana, Swapan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We point out that the main results-the analytic expressions for the Groverian Measure of Entanglement, in the above mentioned paper are erroneous. The technical mistake of the paper is discussed. It is shown by an explicit example that the formula for calculating the Groverian measure yields G(|ψ>) = 0 for some entangled states.
description: 4 pages, published online in Quantum Info. Process. on 24 July 2009
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÐÐÐÐ£Ð¤ ÐÐÐÐÐÐÐÐÐÐ¬ Ð² Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐ¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸ÑÑ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð·Ð´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Ð¾Ð¿Ð¾Ð², ÐÐ¸ÑÐ¸Ð»Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÐÐ´Ð°Ð½Ð¸Ðµ
Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐ¸Ðµ ÐÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸
ÑÐ°Ð¿ÑÐ¸Ñ-3d
Autodesk Revit

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð·Ð°Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð·Ð´Ð°Ð½Ð¸Ðµ Ñ Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐ¸Ð¼Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸ÑÐ¼Ð¸ ÐÐÐÐ£Ð¤ ÐÐÐÐÐÐÐÐÐÐ¬ ÐÐ°ÑÑÐ¶Ð½Ð°Ñ ÑÑÐµÐ½Ð°. ÐÑÐ» ÑÐ¾Ð·Ð´Ð°Ð½ ÑÑÐºÐ¸Ð¹ Ð¸ Ð²ÑÑÐ°Ð·Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ½ÑÐ¹ Ð¾Ð±Ð»Ð¸Ðº Ð·Ð´Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð·Ð´Ð°Ð½Ð¸Ñ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÐµÐ¼Ð° Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²ÐºÐ¸ Ð·ÐµÐ¼ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ°, Ð¿ÑÐ¸Ð½ÑÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÑÑÐµÑÐ° Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð·Ð´Ð°Ð½Ð¸Ñ, ÑÐ¾Ð·Ð´Ð°Ð½ Ð¿ÑÐ¾ÐµÐºÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ ÐºÐ°Ð»ÐµÐ½Ð´Ð°ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð° Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð³ÐµÐ½ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð°, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¿Ð¾Ð¶Ð°ÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸Ð½ÑÑÐ¾Ð¹ Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐµÐ¹ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸.
Neutrino mass and mixing parameters: A short review
Creators: name: G. L. Fogli
name: E. Lisi
name: A. Marrone
name: A. Palazzo
name: A. M. Rotunno
Publisher: name: INFN Open Access Repository
Year: 2005

description: We present a brief review of the current status of neutrino mass and mixing
parameters, based on a comprehensive phenomenological analysis of neutrino
oscillation and non-oscillation searches, within the standard three-neutrino
mixing framework.
Topological Field Theory and Nonlinear $σ$-Models on Symmetric
  Spaces
Creators: name: L. Martina
name: O. K. Pashaev
name: G. Soliani
Publisher: name: INFN Open Access Repository
Year: 1995

description: We show that the classical non-abelian pure Chern-Simons action is related to
nonrelativistic models in (2+1)-dimensions, via reductions of the gauge
connection in Hermitian symmetric spaces. In such models the matter fields are
coupled to gauge Chern-Simons fields, which are associated with the isotropy
subgroup of the considered symmetric space. Moreover, they can be related to
certain (integrable and non-integrable) evolution systems, as the Ishimori and
the Heisenberg model. The main classical and quantum properties of these
systems are discussed in connection with the topological field theory and the
condensed matter physics.
Direct determination of the collective pinning radius in high temperature superconductors
Creators: name: Dolz, Moira I.
name: Kolton, Alejandro B.
name: Pastoriza, Hernan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We study finite-size effects at the onset of the irreversible magnetic behaviour of micron-sized Bi$_2$Sr$_2$CaCu$_2$O$_{8+δ}$ single crystals by using silicon micro-oscillators. We find an irreversibility line appearing well below the thermodynamic Bragg-glass melting line at a magnetic field which increases both with increasing the sample radius and with decreasing the temperature. We show that this size-dependent irreversibility line can be identified with the crossover between the Larkin and the random manifold regimes of the vortex lattice transverse roughness. Our method allows to determine the three-dimensional weak collective pinning Larkin radius in a {\it direct way}.
description: 4 pages, 3 figs
$R_{AA}$ of $J/ψ$ near mid-rapidity in heavy ion collisions at $\sqrt{s_{NN}}=200$ GeV
Creators: name: Song, Taesoo
name: Park, Woosung
name: Lee, Su Houng
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We build up a model to reproduce the experimentally measured $R_{AA}$ of $J/ψ$ near midrapidty in Au+Au collision at $\sqrt{s_{NN}}=200$ GeV. The model takes into account the $J/ψ$ suppression from the quark-gluon plasma and hadron gas as well as the nuclear absorption of primordial charmonia and the regeneration effects at the hadronization stage, and hence is a generalization of the two component model introduced by Grandchamp and Rapp. The improvements in this work are twofold; the addition of the initial local temperature profile and a consistent use of QCD NLO formula for both the dissociation cross section in the hadron gas and the thermal decay widths in the quark-gluon plasma for the charmonium states. The initial local temperature profile is determined from the assumption that the local entropy density is proportional to a formula involving the number densities of the number of participants and of the binary collisions that reproduces the multiplicities of charged particles at chemical freeze-out. The initial local temperature profile brings about a kink in the $R_{AA}$ curve due to the initial melting of $J/ψ$. The initially formed fireball, composed of weakly interacting quarks and gluons with thermal masses that are extracted from lattice QCD, follows an isentropic expansion with cylindrical symmetry. The fit reproduces well the Au+Au as well as the Cu+Cu data. The same method is applied to predict the $R_{AA}$ expected from the Pb+Pb collision at LHC energy.
description: 18 pages, 13 figures
title: ÐÐ¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¾ÑÐµÐ½Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÑÐ°ÑÐ¸Ð½, ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
name: ÐÐ·ÐµÑÐ¾Ð², ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
name: ÐÑÐ¿ÐµÐ½ÑÐ¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: Ð¾ÑÐµÐ½Ð¾ÑÐ½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ

description: ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¾ÑÐµÐ½Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ
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Ð¸ Ð´ÐµÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹, ÐºÐ°ÑÐ°ÑÑÐ¸ÑÑÑ Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ, Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð²ÑÐµÑ ÑÐ¸Ð¿Ð¾Ð² Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¸Ñ Ð¿ÑÐ°Ð² Ð¸ ÐºÐ¾Ð½ÑÑÐ»ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð½Ð° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸
Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¾ÑÐµÐ½ÐºÐ¸.
ÐÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¸ ÑÐµÐ´Ð°ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸
ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¸ Ð¿ÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð½Ð¾Ð²ÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ Ð¾ÑÐµÐ½Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð½Ð¾Ð²ÑÐµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¼Ð¾Ð³ÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÑÑÑÑ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÑÑÐ¸Ð¼Ð¸ Ð¾ÑÐµÐ½ÑÐ¸ÐºÐ°Ð¼Ð¸
Ð¸ Ð¾ÑÐµÐ½ÑÐ¸ÐºÐ°Ð¼Ð¸-ÐºÐ¾Ð½ÑÑÐ»ÑÑÐ°Ð½ÑÐ°Ð¼Ð¸ Ð¿ÑÐ¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð² ÑÐµÐºÑÑÐ°Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð½Ð° Ð¾ÑÐµÐ½ÐºÑ
Ð¸ Ð² Ð¾ÑÑÐµÑÐ°Ñ Ð¾Ð± Ð¾ÑÐµÐ½ÐºÐµ ÑÑÐ¾ÑÐ½ÐµÐ½Ð¸Ð¹ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð², ÑÐµÐ³Ð»Ð°Ð¼ÐµÐ½ÑÐ¸ÑÑÑÑÐ¸Ñ ÑÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ.
title: Ð ÐµÐ¶Ð¸Ð¼Ñ ÑÐ°Ð±Ð¾ÑÑ ÐÐ­Ð¡ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÑÐ°Ð½Ð¾Ð², ÐÐ»ÐµÐ³
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐ°Ð±Ð¾ÑÑ
ÑÑÑÐ¾ÑÐ½ÑÐµ Ð²ÐµÐ´Ð¾Ð¼Ð¾ÑÑÐ¸

description: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°Ð±Ð¾ÑÑ Ð³Ð¸Ð´ÑÐ¾Ð°Ð³ÑÐµÐ³Ð°ÑÐ¾Ð², ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÑ Ð¸ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÐ»Ð¾Ð¶Ð¸Ð²ÑÐ¸ÐµÑÑ Ð½Ð° ÑÐµÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ ÐÐ­Ð¡ ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐ¶Ð¸Ð¼Ð½ÑÐµ ÑÑÐ»Ð¾Ð²Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° Ð½Ð° ÑÐ¾ÑÐ°Ð»ÑÐ½Ð¾Ð¼ Ð°Ð½Ð°Ð»Ð¸Ð·Ðµ ÐµÐ¶ÐµÑÐ°ÑÐ½ÑÑ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¹ ÑÐµÐ¶Ð¸Ð¼Ð½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð¸ ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ ÑÐ¾ÐºÑÐ°ÑÐ°ÐµÑ ÑÑÑÐ´Ð¾ÐµÐ¼ÐºÐ¾ÑÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°Ð±Ð¾ÑÑ Ð³Ð¸Ð´ÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿Ð¾Ð²ÑÑÐ°ÐµÑ Ð´Ð¾ÑÑÐ¾Ð²ÐµÑÐ½Ð¾ÑÑÑ Ð¿Ð¾Ð»ÑÑÐ°ÐµÐ¼ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð². Ð­ÑÐ¾ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ñ Ð²ÑÑÐ¾ÐºÐ¾Ð¹ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÑÑ Ð¿Ð¾Ð´Ð¾Ð±ÑÐ°ÑÑ Ð½Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ ÐÐ­Ð¡, Ð¿ÑÐ¸ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¼ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐ¹ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÑÑÐµÐºÑ Ð¾Ñ Ð¿ÑÐ¾ÑÐ¾Ð´ÑÑÐµÐ³Ð¾ ÑÐµÑÐµÐ· ÑÑÑÐ±Ð¸Ð½Ñ Ð²Ð¾Ð´Ð¾ÑÐ¾ÐºÐ° Ð¸, Ð² ÐºÐ¾Ð½ÐµÑÐ½Ð¾Ð¼ ÑÑÑÑÐµ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ðµ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð¹ Ð²ÑÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³Ð¸Ð¸.
Attraction to a radiation-like era in early superstring cosmologies
Creators: name: Bourliot, Francois
name: Kounnas, Costas
name: Partouche, Herve
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Starting from an initial classical four dimensional flat background of the heterotic or type II superstrings, we are able to determine at the string one-loop level the quantum corrections to the effective potential due to the spontaneous breaking of supersymmetry by "geometrical fluxes". Furthermore, considering a gas of strings at finite temperature, the full "effective thermal potential" is determined, giving rise to an effective non-trivial pressure. The backreaction of the quantum and thermal corrections to the space-time metric as well as to the moduli fields induces a cosmological evolution that depends on the early time initial conditions and the number of spontaneously broken supersymmetries. We show that for a whole set of initial conditions, the cosmological solutions converge at late times to two qualitatively different trajectories: They are either attracted to (i) a thermal evolution similar to a radiation dominated cosmology, implemented by a coherent motion of some moduli fields, or to (ii) a "Big Crunch" non-thermal cosmological evolution dominated by the non-thermal part of the effective potential or the moduli kinetic energy. During the attraction to the radiation-like era, periods of accelerated cosmology can occur. However, they do not give rise to enough inflation (e-fold < 0.2) for the models we consider, where N>1 supersymmetry is spontaneously broken to N=0.
description: 38 pages, 4 figures, added references, added comments in the abstract
Untangling the Web of E-Research: Towards a Sociology of Online Knowledge
Creators: name: Meyer, Eric T.
name: Schroeder, Ralph
Publisher: name: arXiv
Year: 2009
Subjects: subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: e-Research is a rapidly growing research area, both in terms of publications and in terms of funding. In this article we argue that it is necessary to reconceptualize the ways in which we seek to measure and understand e-Research by developing a sociology of knowledge based on our understanding of how science has been transformed historically and shifted into online forms. Next, we report data which allows the examination of e-Research through a variety of traces in order to begin to understand how the knowledge in the realm of e-Research has been and is being constructed. These data indicate that e-Research has had a variable impact in different fields of research. We argue that only an overall account of the scale and scope of e-Research within and between different fields makes it possible to identify the organizational coherence and diffuseness of e-Research in terms of its socio-technical networks, and thus to identify the contributions of e-Research to various research fronts in the online production of knowledge.
Electron motion in a pre-accelerator cavity
Creators: name: Vermeulen, Fred Eric
Publisher: name: University of British Columbia
Year: 2011

description: Relativistic electron motion in a time varying, uniform, uni-directional electric field is examined. The information obtained is applied to study the dynamics of an electron beam which is injected uniformly at low energy into a high field intensity, long transit angle pre-accelerator cavity. Numerical calculations are made for a particular cavity, and the results are presented in graphical form. The equations of motion of an electron in a travelling wave are derived and used to obtain numerical data on a particular main accelerator. This data is presented in graphical form and is designed to be used in conjunction with the pre-accelerator results to supply information on the joint operation of the pre-accelerator and the main accelerator.
title: ÐÐ·ÑÑÐµÐ½Ð¸Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ°Ð· Ð¿ÑÐ¸ Ð¼ÐµÑ Ð°Ð½Ð¾Ð»ÐµÐ³Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ "TiN-TiC-TiBâ-(TiOâ)"
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¢ÑÐ¾ÑÐºÐ¸Ð¹, ÐÐ¸ÑÐ°Ð¸Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¢ÐµÑÐ¼Ð¸ÑÐµÑÐºÐ°Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð²
Ð¢Ð¸ÑÐ°Ð½, ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ
ÐÐ¾ÐºÑÑÑÐ¸Ñ
ÐÐµÑÐ°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¸ Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ
Ð¡Ð¿ÐµÐºÐ°Ð½Ð¸Ðµ (ÑÐµÑ Ð½.)

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸, Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð¼ÐµÑÐ°Ð½Ð¾ÑÐ¸Ð½ÑÐµÐ·Ð°, Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð Ð¤Ð Ð¸ Ð Ð¤Ð­Ð¡ Ð²Ð½Ð¾Ð²Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐ°Ð½Ð° Ñ Ð°Ð·Ð¾ÑÐ¾Ð¼, ÑÐ³Ð»ÐµÑÐ¾Ð´Ð¾Ð¼, Ð±Ð¾ÑÐ¾Ð¼ Ð¸ ÐºÐ¸ÑÐ»Ð¾ÑÐ¾Ð´Ð¾Ð¼. ÐÐµÑÐ¾Ð´Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ â Ð¼ÐµÑÐ°Ð½Ð¾ÑÐ¸Ð½ÑÐµÐ· Ð¸ ÑÐ¿ÐµÐºÐ°Ð½Ð¸Ðµ. ÐÑÑÐ¾Ð´Ð½ÑÐµ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ ÑÐ¼ÐµÑÐ¸ ÑÐ¾ÑÑÐ¾ÑÐ»Ð¸ Ð¸Ð· Ð±Ð¸Ð½Ð°ÑÐ½ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¸ÑÐ°Ð½Ð°, ÑÐ°ÐºÐ¸Ñ ÐºÐ°Ðº Ð½Ð¸ÑÑÐ¸Ð´, Ð¾ÐºÑÐ¸Ð´, Ð´Ð¸Ð±Ð¾ÑÐ¸Ð´ Ð¸ ÐºÐ°ÑÐ±Ð¸Ð» ÑÐ¸ÑÐ°Ð½Ð°. Ð­ÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½Ñ Ð¿ÑÐ¾ÑÐ¾Ð´Ð¸Ð» Ð² ÑÑÐ¸ ÑÑÐ°Ð´Ð¸Ð¸: Ð² Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÑÐ°Ð´Ð¸Ð¸ Ð±ÑÐ» ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½ Ð¼ÐµÑÐ°Ð½Ð¾ÑÐ¸Ð½ÑÐµÐ· ÑÐ¼ÐµÑÐ¸ TiN-TiC-TiB2, Ð½Ð° Ð²ÑÐ¾ÑÐ¾Ð¹ â Ð´Ð¾Ð±Ð°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð² Ð²ÑÑÐµ ÑÐºÐ°Ð·Ð°Ð½Ð½ÑÑ ÑÐ¼ÐµÑÑ Ð¾ÐºÑÐ¸Ð´Ð° ÑÐ¸ÑÐ°Ð½Ð°, Ð½Ð° ÑÑÐµÑÑÐµÐ¹ ÑÐ¿ÐµÐºÐ°Ð½Ð¸Ðµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð¹ ÑÐ¼ÐµÑÐ¸. ÐÐ¾Ð»ÑÑÐµÐ½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð»Ð¸ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð Ð¤Ð Ð¸ Ð Ð¤Ð­Ð¡. ÐÐ½Ð°Ð»Ð¸Ð· Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ´Ð¸Ð» Ð½Ð°Ð»Ð¸ÑÐ¸Ðµ Ð½Ð¾Ð²ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹, ÑÐ°ÐºÐ¸Ñ ÐºÐ°Ðº TixNyOz, TixNyBz TixNyOz Ð¸ Ñ. Ð´.
title: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°: Ð¼ÐµÑÐ¾Ð´ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ðº Ð¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð´ÐµÐ½ÐºÐ¾, ÐÐ°Ð»Ð¸Ð½Ð°
name: ÐÐµÑÐºÐ¾Ð², ÐÐ°Ð´Ð¸Ð¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2022
Subjects: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°
Ð½ÐµÐ¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½ÑÐµ Ð·Ð°Ð´Ð°ÑÐ¸
Ð¼ÐµÑÐ¾Ð´Ñ Ð¤ÑÑÑÐµ
ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÐµ ÑÑÐ½ÐºÑÐ¸Ð¸
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: ÐÐµÑÐ¾Ð´ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ðº Ð¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÑÑÑ Ðº Ð½ÐµÐ¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½ÑÐ¼ Ð·Ð°Ð´Ð°ÑÐ°Ð¼ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸Ð·Ð¸ÐºÐ¸ Ñ ÑÐ°Ð·Ð´ÐµÐ»ÑÑÑÐ¸Ð¼Ð¸ÑÑ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½ÑÐ¼Ð¸. Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð°, Ð² ÐºÐ¾ÑÐ¾ÑÐ¾Ð¼ ÑÐµÑÐµÐ½Ð¸Ðµ Ð½Ð°ÑÐ¾Ð´Ð¸Ð¼ Ð² Ð²Ð¸Ð´Ðµ ÑÑÐ¼Ð¼Ñ Ð´Ð²ÑÑ ÑÑÐ½ÐºÑÐ¸Ð¹, Ð¿ÑÐ¸ÑÐµÐ¼ Ð´Ð»Ñ Ð¾Ð´Ð½Ð¾Ð¹ Ð¸Ð· ÑÑÐ¸Ñ ÑÑÐ½ÐºÑÐ¸Ð¹ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÐµÑÑÑ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ°Ñ Ð¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½Ð°Ñ Ð·Ð°Ð´Ð°ÑÐ°, a Ð´ÑÑÐ³Ð°Ñ ÑÑÐ½ÐºÑÐ¸Ñ Ð±ÑÐ´ÐµÑ ÑÐ°ÑÑÐ½ÑÐ¼ ÑÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð½ÐµÐ¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¤Ð¸Ð·Ð¸ÐºÐ¾-Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 01.06.01Â«ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ°Â», 01.03.02Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°Â», 01.04.02Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°Â», 01.03.03Â«ÐÐµÑÐ°Ð½Ð¸ÐºÐ° Ð¸ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÂ», 01.04.03Â«ÐÐµÑÐ°Ð½Ð¸ÐºÐ° Ð¸ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÂ», 03.03.01Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ°Â», 03.04.01Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ°Â», 15.03.03Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ°Â», 15.04.03Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ°Â». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ°ÐºÐ¶Ðµ Ð±ÑÐ´ÐµÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ Ð²ÑÐµÐ¼ Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ð¼ÑÑ, Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸Ð¼ÑÑ Ð¿Ð¾Ð¸ÑÐºÐ¾Ð¼ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð·Ð°Ð´Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸Ð·Ð¸ÐºÐ¸.
title: ÐÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÑÑÑÐºÑÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÐºÐ¾Ð³ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Problems of structuring the riskogenic information space of the enterprise
Creators: name: ÐÐ°ÑÐ°Ð»Ð¾Ð², Ð Ð¾Ð¼Ð°Ð½
name: Ð¡Ð»ÐµÐ¿ÑÐ¾Ð²Ð°, Ð®Ð»Ð¸Ñ
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ñ (Ð ÐÐ¡ÐâÐ­â2022)", Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ (8; 2022; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÑÐ¸ÑÐºÐ¾Ð³ÐµÐ½Ð½Ð¾Ðµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð¾
ÑÐµÐ½Ð¾Ð¼ÐµÐ½ ÑÐ¸ÑÐºÐ°
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ¸ÑÐº
ÑÐ¸ÑÑÐ°ÑÐ¸Ñ ÑÐ¸ÑÐºÐ°
ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÐ¸ÑÐºÐ°
ÑÐ°ÐºÑÐ¾Ñ ÑÐ¸ÑÐºÐ°
riskogenic information space
risk phenomenon
economic risk
risk situation
risk level
risk factor

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»ÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð¾Ð±ÑÑÐ»Ð¾Ð²Ð»ÐµÐ½Ð½ÑÑ Ð¿Ð¾ÑÐ²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð² Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½ÐµÐ¸Ð·Ð²ÐµÑÑÐ½ÑÑ ÑÐ²Ð»ÐµÐ½Ð¸Ð¹, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð³ÐµÐ½ÐµÑÐ¸ÑÑÑÑ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÐµ Ð¼ÐµÑÐ°ÑÑÐ¸Ðµ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð½Ð° Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾Ð±ÑÐµÐºÑÑ. Ð¡ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐµÐ¾ÑÐ¸Ð¸ Ð. Ð£. ÐÑÐ¸Ð´Ð¶Ð¼ÐµÐ½Ð° Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÐµÑÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð´Ð»Ñ Ð¿ÑÐµÐ¾Ð´Ð¾Ð»ÐµÐ½Ð¸Ñ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼. ÐÐ¾Ð´ÑÐ¾Ð±Ð½Ð¾ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐ»ÑÑÐ°Ð¸ Ð¿ÑÐ¾ÑÐ²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ½Ð¾Ð¼ÐµÐ½Ð° ÑÐ¸ÑÐºÐ°, ÐµÐ³Ð¾ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¸ Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° ÑÑÐµÐ¿ÐµÐ½Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÐ¼Ð¸.
description: In this study, the conditions for achieving the goals of enterprises activities are considered, due to the appearance in practice of unknown phenomena that generate some interfering effects on the studied economic objects. With the help of P. W. Bridgman's operational theory, the necessity of introducing additional characteristics to overcome emerging problems is substantiated. The cases of manifestation of the phenomenon of risk, its operational characteristics and their impact on the degree of the aim achievement of enterprise management are considered.
Open discussion at the IGS symposium on ‘The edges of glaciology’, 7 July 2023
Creators: name: Fowler, Andrew
Publisher: name: University of Limerick
Year: 2025
Subjects: classificationCode: 49
subject: Mathematical sciences

description: There follows the open discussion which took place at the IGS symposium on ‘The Edges of Glaciology’, in July 2023. The discussion was curated by Doug Benn. The time of speaking in minutes and seconds into the Panopto recording is given in bold figures. The recording itself is provided as electronic supplementary material. It has been transcribed and edited by Andrew Fowler, with much (and much-needed) assistance from the participants. Footnotes (mostly references) are editorial intrusions.
title: ÐÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¿Ð¾ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐ²ÐµÑÐ´ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½ÑÑ Ð¾ÑÑ Ð¾Ð´Ð¾Ð² Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÑÑ Ð² Ð³Ð¾ÑÐ¾Ð´Ðµ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³
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»Ð¾ÑÐ½Ð¸ÐºÐ¾Ð²Ð°, ÐÑÐ±Ð¾Ð²Ñ
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ÑÑÐ¾Ð²ÑÐµ Ð¾ÑÑ Ð¾Ð´Ñ
ÐÐ¸Ð»ÑÐµ ÐºÐ²Ð°ÑÑÐ°Ð»Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ²ÐµÑÐ´ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½ÑÑ Ð¾ÑÑÐ¾Ð´Ð¾Ð², ÑÐ´ÐµÐ»Ð°Ð½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹. ÐÑÐ±ÑÐ°Ð½ Ð¼ÐµÑÐ¾Ð´ ÑÐµÑÐ¸ÐºÐ»Ð¸Ð½Ð³Ð° Ð´Ð»Ñ Ð³Ð¾ÑÐ¾Ð´Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³. ÐÐ¿Ð¸ÑÐ°Ð½Ñ Ð¸ Ð¿Ð¾Ð´Ð¾Ð±ÑÐ°Ð½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½ÑÐµ ÑÐµÑÐ¸. ÐÐ¾Ð´Ð¾Ð±ÑÐ°Ð½Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð»Ñ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ²ÐµÑÐ´ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½ÑÑ Ð¾ÑÑÐ¾Ð´Ð¾Ð² Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸ÐµÐ¼ ÑÑÑÑÑ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐµÐ½ÑÐ°Ð±Ð¸Ð»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð° ÑÐ°Ðº Ð¶Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð² ÑÑÐµÑÐµ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ²ÐµÑÐ´ÑÑ Ð±ÑÑÐ¾Ð²ÑÑ Ð¾ÑÑÐ¾Ð´Ð¾Ð² Ð²Ð¾ Ð²ÑÐ¾ÑÐ¸ÑÐ½Ð¾Ðµ ÑÑÑÑÐµ.
Comparison of Alpha-Element Enhanced Simple Stellar Population Models with Milky Way Globular Clusters
Creators: name: Lee, Hyun-chul
name: Worthey, Guy
name: Dotter, Aaron
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present simple stellar population (SSP) models with scaled-solar and alpha-element enhanced abundances. The SSP models are based on the Dartmouth Stellar Evolution Database, our library of synthetic stellar spectra, and a detailed systematic variation of horizontal-branch (HB) morphology with age and metallicity. In order to test the relative importance of a variety of SSP model ingredients, we compare our SSP models with integrated spectra of 41 Milky Way Globular Clusters (MWGCs) from Schiavon et al. (2005). Using the Mg b and Ca4227 indices, we confirm that Mg and Ca are enhanced by about +0.4 and +0.2 dex, respectively, in agreement with results from high resolution spectra of individual stars in MWGCs. Balmer lines, particularly Hgamma and Hdelta, of MWGCs are reproduced by our alpha-enhanced SSP models not only because of the combination of isochrone and spectral effects but also because of our reasonable HB treatment. Moreover, it is shown that the Mg abundance significantly influences Balmer and iron line indices. Finally, the investigation of power-law initial mass function (IMF) variations suggests that an IMF much shallower than Salpeter is unrealistic because the Balmer lines are too strong on the metal-poor side to be compatible with observations.
description: 38 pages, 18 figures, AJ accepted. Models are available from http://astro.wsu.edu/hclee/sp_LWD09.html and http://astro.wsu.edu/hclee/sp.html
title: Ð ÐµÑÑÑÑÑ ÐºÐ¾ÑÐ¿ÑÑÐ½Ð¾Ð¹ Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÐºÐ¸ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾-Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð¼Ñ ÑÐ·ÑÐºÑ
title: Resources of corpus linguistics in teaching professionally-oriented foreign language
Creators: name: Ð¢Ð°ÑÐ½Ð°ÐµÐ²Ð°, ÐÐ°ÑÐ¸ÑÐ°
name: ÐÐµÐ±Ð¾Ð¶Ð¸Ð½Ð°, ÐÑÐµÐ½Ð¸Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
ÐÐ°Ð·Ñ Ð´Ð°Ð½Ð½ÑÑ
ÐºÐ¾ÑÐ¿ÑÑÐ½Ð°Ñ Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÐºÐ°
ÑÐ·ÑÐºÐ¾Ð²Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»
Ð°ÑÑÐµÐ½ÑÐ¸ÑÐ½Ð¾ÑÑÑ
Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ

description: Ð¡ÑÐ°ÑÑÑ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð»Ð¸Ð½Ð³Ð²Ð¾Ð´Ð¸Ð´Ð°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° ÐºÐ¾ÑÐ¿ÑÑÐ½Ð¾Ð¹ Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÐºÐ¸. ÐÐ½Ð°Ð»Ð¸Ð· ÑÑÐ´Ð° Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÐºÐ¾ÑÐ¿ÑÑÐ¾Ð² Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð» ÑÐ´ÐµÐ»Ð°ÑÑ Ð²ÑÐ²Ð¾Ð´ Ð¾ ÑÐ¾Ð¼, ÑÑÐ¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÑÑÑÑÐ° Ð¸Ð¼ÐµÐµÑ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð»Ð¸Ð½Ð³Ð²Ð¾Ð´Ð¸Ð´Ð°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð».
description: The article focuses on identifying the linguodidactic potential of corpus linguistics. The analysis of a number of linguistic corpora led to the conclusion that the use of this electronic resource has a significant linguodidactic potential.
Additional file 1 of Association between serum S100A11 levels and glucose metabolism in diabetic process
Creators: name: Wu, Yao
name: Wu, Shaobo
name: Li, Fang
name: Zeng, Ting
name: Luo, Xiaohe
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Computational Biology

description: Additional file 1: Table S1. Multivariate regression for effect of serum S100A11 level on metabolic markers in male group. Crude model: we did not adjust other covariates. Adjusted model I: We adjusted age, BMI, WHR. Adjusted model II: We adjusted AGE, BMI, WHR, HbA1c/0.5hPPI/0.5hPPG/FPG/FPI, glucose tolerance. Table S2. Multivariate regression for effect of serum S100A11 level on metabolic markers in female group. Crude mode I: we did not adjust other covariates. Adjusted model I: We adjusted age, BMI, WHR. Adjusted model II: We adjusted AGE, BMI, WHR, HbA1c/0.5hPPI/0.5hPPG/FPG/FPI, glucose tolerance. Table S3. Threshold effect analysis of S100A11 on metabolic markers by using two-piecewise linear regression, stratified by glucose tolerance. Effect: HbA1c, 0.5hPPI, 0.5hPPG, HOMA-β, ISI (the liver); cause: S100A11. Adjusted: sex, age, BMI, WHR, 0.5hPPG/0.5hPPI/HbA1c/FPG/FPI. Table S4. Threshold effect analysis of S100A11 on metabolic markers by using two-piecewise linear regression, stratified by sex. Effect: FPG, 0.5hPPI; cause: S100A11. Adjusted: glucose tolerance, age, BMI, WHR, 0.5hPPG/0.5hPPI/HbA1c/FPG/FPI. Figure S1. Multivariate adjusted smoothing spline plots of metabolic markers by serum S100A11. Red dotted lines represent the spline plots of S100A11 and blue dotted lines represent the 95% confidence intervals of the spline plots. Adjusted for sex/glucose tolerance, age, BMI, WHR, 0.5hPPG/0.5hPPI/HbA1c/FPG/FPI.
title: ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¾ÑÑÑÐ¾ÑÐ½ÑÑ Ð²ÐµÑÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ°Ð½ÑÐ¸Ð¹
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°Ð½ÑÐ½Ñ, ÐÐ½Ð´ÑÐ¾Ð½Ð¸Ðº
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐµÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÑÑÑÑ
ÐÐµÑÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸
ÐÐµÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ°

description: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð²ÐµÑÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ°Ð½ÑÐ¸Ð¹ Ð¼Ð¾ÑÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²ÐµÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÑÐ°ÑÐ»Ð¸, Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½ ÑÑÐ°Ð¿ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÑÑÐ¾ÑÐ½Ð¾Ð¹ Ð²ÐµÑÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐ°Ð½ÑÐ¸Ð¸ (Ð¾Ñ ÑÐ°ÑÑÐµÑÐ° ÑÐ½ÐµÑÐ³Ð¾ÑÐµÑÑÑÑÐ° Ð´Ð¾ Ð²ÑÐ±Ð¾ÑÐ° ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°), Ð¸Ð·ÑÑÐµÐ½ Ð¿ÑÐ¾ÑÐµÑÑ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° ÑÑÐµÐ¼Ð° Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ°Ñ ÐµÐ³Ð¾ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ.
Towards an Algebraic Classification of Calabi-Yau Manifolds I: Study of
  K3 Spaces
Creators: name: F. Anselmo
name: J. Ellis
name: D. V. Nanopoulos
name: G. Volkov
Publisher: name: Phys.Part.Nucl.32:318-375,2001; Fiz.Elem.Chast.Atom.Yadra
  32:605-698,2001
Year: 2000

description: We present an inductive algebraic approach to the systematic construction and
classification of generalized Calabi-Yau (CY) manifolds in different numbers of
complex dimensions, based on Batyrev's formulation of CY manifolds as toric
varieties in weighted complex projective spaces associated with reflexive
polyhedra. We show how the allowed weight vectors in lower dimensions may be
extended to higher dimensions, emphasizing the roles of projection and
intersection in their dual description, and the natural appearance of
Cartan-Lie algebra structures. The 50 allowed extended four-dimensional vectors
may be combined in pairs (triples) to form 22 (4) chains containing 90 (91) K3
spaces, of which 94 are distinct, and one further K3 space is found using
duality. In the case of CY_3 spaces, pairs (triples) of the 10~270 allowed
extended vectors yield 4242 (259) chains with K3 (elliptic) fibers containing
730 additional K3 polyhedra. A more complete study of CY_3 spaces is left for
later work.
title: ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¸ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
title: Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ, Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð¸ Ð·Ð°ÑÐ¸ÑÐµ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð²
titleType: Subtitle
Creators: name: Ð¥Ð¾Ð´ÑÑÐµÐ², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 2002
Subjects: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐµ ÑÐ°Ð±Ð¾ÑÑ
Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ

description: Ð Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐºÐ°Ð·Ð°Ð½Ð¸ÑÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ, ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¸ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°. ÐÐ»Ð°Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð²ÑÐ±Ð¾ÑÐ° ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ ÑÐµÐ¼Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°, ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð½Ð° ÐµÐ³Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¸ ÑÐ±Ð¾ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°, Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾ÑÑÐ¸ ÐµÐ³Ð¾ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ; ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÐÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ, Ð¸Ð»Ð»ÑÑÑÑÐ¸ÑÑÑÑÐ¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ðµ ÑÐ°Ð·Ð´ÐµÐ»Ñ. ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ñ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ° ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 061000 "ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¸ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ".
CARS: the CFHTLS-Archive-Research Survey; I. Five-band multi-colour data from 37 sq. deg. CFHTLS-Wide observations
Creators: name: Erben, T.
name: Hildebrandt, H.
name: Lerchster, M.
name: Hudelot, P.
name: Benjamin, J.
name: van Waerbeke, L.
name: Schrabback, T.
name: Brimioulle, F.
name: Cordes, O.
name: Dietrich, J. P.
name: Holhjem, K.
name: Schirmer, M.
name: Schneider, P.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the CFHTLS-Archive-Research Survey (CARS). It is a virtual multi-colour survey based on public archive images from the CFHT-Legacy-Survey. Our main scientific interests in CARS are optical searches for galaxy clusters from low to high redshift and their subsequent study with photometric and weak-gravitational lensing techniques. As a first step of the project we present multi-colour catalogues from 37 sq. degrees of the CFHTLS-Wide component. Our aims are to create astrometrically and photometrically well calibrated co-added images. Second goal are five-band (u*, g', r', i', z') multi-band catalogues with an emphasis on reliable estimates for object colours. These are subsequently used for photometric redshift estimates. The article explains in detail data processing, multi-colour catalogue creation and photometric redshift estimation. Furthermore we apply a novel technique, based on studies of the angular galaxy cross-correlation function, to quantify the reliability of photo-z's. The accuracy of our high-confidence photo-z sample (10-15 galaxies per sq. arcmin) is estimated to $σ_{Δ_z/(1+z)}\approx 0.04-0.05$ up to i'<24 with typically only 1-3% outliers. Interested users can obtain access to our data by request to the authors.
description: 31 pages, 18 figures, 6 tables; accepted for publication by A&A main journal
title: Ð Ð°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐµÑÑÑÑÐ¾Ð² Ð¿ÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ°Ð¼Ð¸ ÑÐ°Ð´Ð¸Ð¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð²
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°ÑÑÐ¾Ð²ÐµÐ½ÐºÐ¾, ÐÐ°Ð»ÐµÐ½ÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
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description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐµÑÑÑÑÐ¾Ð² Ð¿ÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ°Ð¼Ð¸ ÑÐ°Ð´Ð¸Ð¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð², Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð½Ð¾Ð²ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ ÐºÐ²Ð°Ð·Ð¸Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐµÑÑÑÑÐ¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¸Ð½ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ¾Ð² Ð´Ð»Ñ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð².
Little heterotic strings
Creators: name: Faraggi, Alon E.
name: Manno, Elisa
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss toroidal orbifolds of the E8XE8 heterotic string, in which the free fermionic Higgs-matter splitting is implemented by a shift in the internal lattice coupled with the fermion numbers of the gauge degrees of freedom. We consider models in which some choices of the orbifold result in the projection of the graviton. In the models that we consider the projection also results in flipping the spin-statistics assignments in the massive string spectrum, whereas the massless spectrum retains the conventional spin-statistics assignments. We argue that the partition functions are mathematically consistent for one- and multi-loop amplitudes, owning to the existence of supersymmetry in the spectrum. A duality between different models at nonzero temperature is briefly discussed.
description: 19 pages
Hadronic string and chiral symmetry breaking
Creators: name: A. A. Andrianov
name: D. Espriu
Publisher: name: INFN Open Access Repository
Year: 2002

description: We assume that QCD can be effectively described with string-like variables.
The hadronic string is built over the chirally non-invariant QCD vacuum by
means of the boundary interaction with background chiral fields associated with
pions. By making this interaction compatible with the conformal symmetry of the
string and with the unitarity constraint on chiral fields we reconstruct the
equations of motion for the latter ones and furthermore recover the Lagrangian
of non-linear sigma model of pion interactions. The estimated chiral structural
constants of Gasser and Leutwyler fit well the phenomenological values.