cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Enhancing Flood Forecasting with Dual State-Parameter Estimation and Ensemble-based SAR Data Assimilation
Creators: name: Nguyen, Thanh Huy
name: Ricci, Sophie
name: Piacentini, Andrea
name: Suquet, Raquel Rodriguez
name: Blanchet, Gwendoline
name: Luque, Santiago Pena
name: Kettig, Peter
Publisher: name: arXiv
Year: 2022
Subjects: subject: Image and Video Processing (eess.IV)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Ensemble data assimilation in flood forecasting depends strongly on the density, frequency and statistics of errors associated with the observation network. This work focuses on the assimilation of 2D flood extent data, expressed in terms of wet surface ratio, in addition to the in-situ water level data. The objective is to improve the representation of the flood plain dynamics with a TELEMAC-2D model and an Ensemble Kalman Filter (EnKF). The EnKF control vector is composed of friction coefficients and corrective parameters to the input forcing. It is augmented with the water level state averaged over selected subdomains of the floodplain. This work focuses on the 2019 flood event that occurred over the Garonne Marmandaise catchment. The merits of assimilating SAR-derived flood plain data complementary to in-situ water level observations are shown in the control parameter and observation spaces with 1D and 2D assessment metrics. It was also shown that the assimilation of Wet surface Ratio in the flood plain complementary to in-situ data in the river bed brings significative improvement when a corrective term on flood plain hydraulic state is included in the control vector. Yet, it has barely no impact in the river bed that is sufficiently well described by in-situ data. We highlighted that the correction of the hydraulic state in the flood plain significantly improved the flood dynamics, especially during the recession. This proof-of-concept study paves the way towards near-real-time flood forecast, making the most of remote sensing-derived flood observations.
description: 9 pages, 7 figures. Submitted to the 28th TELEMAC User Conference, 18-19 October 2022, Paris-Saclay, France. arXiv admin note: text overlap with arXiv:2205.08471
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ°Ð±Ð¾ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð±Ð°ÑÐ½Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÐºÑÐ°Ð½Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ´Ð¸Ð»Ð¾Ð², 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: 2017
Subjects: Ð¿ÑÐ¾Ð²ÐµÑÐ¾ÑÐ½ÑÐ¹ ÑÐ°ÑÑÐµÑ
Ð±Ð°ÑÐ½Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÐºÑÐ°Ð½Ð°
ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
Ð²ÐµÑÑÐ¾Ð²ÑÐµ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸
Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ðµ
Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ
Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ
Ð¼ÐµÑÐ¾Ð´ ÐºÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð²

description: Ð¦ÐµÐ»Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° - Ð¿ÑÐ¾Ð²ÐµÑÑÐ¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð¿Ð¾Ð²ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð±Ð°ÑÐµÐ½Ð½ÑÑ ÐºÑÐ°Ð½Ð¾Ð², Ð´Ð»Ñ Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÑÐ¾ÑÑ Ð¿Ð¾Ð´ÑÐµÐ¼Ð° ÐºÑÐ°Ð½Ð° Ð¸ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²ÐµÑÐ° Ð³ÑÑÐ·Ð°, Ð²ÑÐ±ÑÐ°ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð¼Ð¾Ð´ÑÐ»Ñ Ð±Ð°ÑÐ½Ð¸ Ð¸ Ð¿Ð¾Ð´Ð¾Ð±ÑÐ°ÑÑ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¾ÑÑÐ°Ð²Ð¸ÑÑ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½Ð¸ÑÑ ÑÑÐµÐ±ÑÐµÐ¼ÑÐµ Ð¿ÑÐ¾Ð²ÐµÑÐ¾ÑÐ½ÑÐµ ÑÐ°ÑÑÐµÑÑ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°Ð±Ð¾ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð±Ð°ÑÐ½Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÐºÑÐ°Ð½Ð°, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð±Ð°ÑÐ½Ð¸, ÑÐ°ÑÑÐµÑÑ Ð±Ð°ÑÐ½Ð¸, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ¸Ðµ ÐµÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ, ÑÐ°ÑÑÐµÑÑ Ð² Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐµ Ð¸ ÑÑÐ°ÑÐ¸ÐºÐµ.
Advanced Bent Crystal Collimation Studies at the Tevatron (T-980)
Creators: name: V. Zvoda
name: G. Annala
name: R. Carrigan
name: A. Drozhdin
name: T. Johnson
name: S. Kwan
name: N. Mokhov
name: A. Prosser
name: R. Reilly
name: R. Rivera L. Uplegger
name: V. Shiltsev
name: D. Still
name: J. Zagel
name: V. Guidi
name: E. Bagli
name: A. Mazzolari
name: Yu. Ivanov
name: Yu. Chesnokov
name: I. Yazynin
Publisher: name: INFN Open Access Repository
Year: 2012

description: The T-980 bent crystal collimation experiment at the Tevatron has recently
acquired substantial enhancements. First, two new crystals - a 16-strip one
manufactured and characterized by the INFN Ferrara group and a quasi-mosaic
crystal manufactured and characterized by the PNPI group. Second, a two plane
telescope with 3 high-resolution pixel detectors per plane along with
corresponding mechanics, electronics, control and software has been
manufactured, tested and installed in the E0 crystal region. The purpose of the
pixel telescope is to measure and image channeled (CH), volume-reflected (VR)
and multiple volume-reflected (MVR) beam profiles produced by bent crystals.
Third, an ORIGIN-based system has been developed for thorough analysis of
experimental and simulation data. Results of analysis are presented for
different types of crystals used from 2005 to present for channeling and volume
reflection including pioneering tests of two-plane crystal collimation at the
collider, all in comparison with detailed simulations.
Searching for electromagnetic counterparts of gravitational wave
  transients
Creators: name: M. Branchesi
name: Collaboration, On Behalf Of The LIGO Scientific
name: Collaboration, The Virgo
name: A. Klotz
name: M. Laas-Bourez
Publisher: name: INFN Open Access Repository
Year: 2011

description: A pioneering electromagnetic (EM) observation follow-up program of candidate
gravitational wave (GW) triggers has been performed, Dec 17 2009 to Jan 8 2010
and Sep 4 to Oct 20 2010, during the recent LIGO/Virgo run. The follow-up
program involved ground-based and space EM facilities observing the sky at
optical, X-ray and radio wavelengths. The joint GW/EM observation study
requires the development of specific image analysis procedures able to
discriminate the possible EM counterpart of GW trigger from background events.
The paper shows an overview of the EM follow-up program and the developing
image analysis procedures as they are applied to data collected with TAROT and
Zadko.
The Formation of Condensation on Cherenkov Telescope Mirrors
Creators: name: P. M. Chadwick
name: S. A. Cleaver
name: M. Dyrda
name: A. Förster
name: J. Michalowski
name: J. Niemiec
name: C. Schultz
name: M. Stodulski
name: For The CTA Consortium.
Publisher: name: INFN Open Access Repository
Year: 2013

description: The mirrors of imaging atmospheric Cherenkov telescopes are different from
those of conventional astronomical telescopes in several ways, not least in
that they are exposed to the elements. One of the issues which may arise is
condensation forming on the mirrors during observing under certain atmospheric
conditions, which has important consequences for the operation of the
telescopes. This contribution discusses why telescope mirrors suffer
condensation and describes the atmospheric conditions and mirror designs which
are likely to be problematic.
title: ÐÐ³ÑÐ°Ð´Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ñ Ð·Ð°ÑÐ¸ÑÐ¾Ð¹ Ð¾ÑÐºÐ¾ÑÐ¾Ð² Ð¾Ñ ÑÐ°Ð·Ð¼ÑÐ²Ð° Ð² Ð¿Ð¾ÑÑÑ ÐÑÑÐ¾ÑÐº
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ»Ð°ÑÐ¾Ð², ÐÐ°Ð²ÐµÐ»
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Ð¾ÑÑÐ¾Ð²ÑÐµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¾Ð³ÑÐ°Ð´Ð¸ÑÐµÐ»ÑÐ½ÑÐµ
ÐÑÐºÐ¾ÑÑ Ð½Ð°ÑÑÐ¿ÐµÐ¹ Ð¸ Ð±ÐµÑÐµÐ³Ð¾Ð²

description: Ð¦ÐµÐ»ÑÑ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿Ð¾ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð¾Ð³ÑÐ°Ð´Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸ÐµÐ¼ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ¿Ð¾ÑÐ¾Ð±Ð° ÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÐºÐ¾ÑÐ¾Ð² Ð¸ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð·Ð°ÑÐ¸ÑÑ Ð¾Ñ ÑÐ°Ð·Ð¼ÑÐ²Ð°. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¾Ð³ÑÐ°Ð´Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹. Ð¢Ð°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°Ð·Ð±Ð¾Ñ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÑ Ð½Ð°ÑÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ ÑÐµÐ¼Ðµ Â«Ð¾Ð³ÑÐ°Ð´Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸ÑÂ», Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¸Ð½ÑÑÑÐµ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°ÑÑÐµÑÐ¾Ð²: - ÑÐ°Ð·Ð¼ÑÐ²Ð° Ð´Ð½Ð° Ñ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¾Ð³ÑÐ°Ð´Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¸ Ð²Ð¾Ð»Ð½Ð¾Ð²Ð¾Ð¼ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¸; - Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¼Ð°ÑÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ° ÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¼Ð¾ÑÐ¸ÑÑÐ¾Ð³Ð¾ Ð¾ÑÐºÐ¾ÑÐ° Ð¾Ð³ÑÐ°Ð´Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹; - ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð²Ð¾Ð»Ð½ Ð½Ð° Ð¾Ð³ÑÐ°Ð¶Ð´ÐµÐ½Ð½Ð¾Ð¹ Ð°ÐºÐ²Ð°ÑÐ¾ÑÐ¸Ð¸.
Effects of shell structure in reactions leading to the same compound
  nucleus or different isotopes
Creators: name: A. K. Nasirov
name: G. Fazio
name: G. Giardina
name: A. Lamberto
name: R. Ruggeri
name: A. Taccone
name: A. I. Muminov
name: F. Hanappe
name: R. Palamara
name: L. Stuttg'e
Publisher: name: INFN Open Access Repository
Year: 2001

description: The role of the entrance channel in fusion-fission reactions was studied by
the theoretical analysis of the experimental evaporation residue excitation
functions for reactions leading to the same compound nucleus. The evaporation
residues cross sections for xn-channels were calculated in the frame of the
combined dinuclear system concept and advanced statistical model. The revealed
differences between experimental data on the evaporation residues in the
^{40}Ar+^{176}Hf, ^{86}Kr + ^{130}Xe and ^{124}Sn + ^{92}Zr reactions leading
to the ^{216}Th^* compound nucleus are explained by the different spin
distributions of compound nuclei which are formed. It is shown that the
intrinsic fusion barrier B^*_{fus} and size of potential well are different for
every entrance channel.
The Role of Mass Asymmetry and Shell Structure in the Evaporation
  Residues Production
Creators: name: G. Fazio
name: G. Giardina
name: A. Lamberto
name: A. I. Muminov
name: A. K. Nasirov
name: U. T. Yakhshiev
name: Yu. Ts. Oganessian
name: A. G. Popeko
name: R. N. Sagaidak
name: A. V. Yeremin
name: S. Hofmann
name: F. Hanappe
name: L. Stuttge
Publisher: name: INFN Open Access Repository
Year: 2002

description: The effects of the entrance channel and shell structure of reacting nuclei on
the experimental evaporation residues have been studied by analysing the
40Ar+176Hf, 86Kr+130,136Xe, 124Sn+92Zr and 48Ca+174Yb reactions leading to the
216Th* and 222Th* compound nuclei. The measured excitation function of
evaporation residues for the 124Sn+92Zr reaction was larger than that for the
86Kr+130Xe reaction. The experimental values of evaporation residues in the
86Kr+136Xe reaction were about 500 times larger than that in the 86Kr+130Xe
reaction. These results are explained by the initial angular momentum
dependence of the fusion excitation functions calculated in framework of the
dinuclear system concept and by the differences in survival probabilities
calculated in framework of advanced statistical model. The dependencies of the
fission barrier and the \Gamma_n / \Gamma_f ratio on the angular momentum of
the excited compound nucleus are taken into account.
title: Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¿Ð»Ð¾ÑÐµÑ Ð½Ð¸ÐºÐ¸. Ð§Ð¸ÑÐ»ÐµÐ½Ð½ÑÐ¹ Ð¼ÐµÑÐ¾Ð´ ÑÐ°ÑÑÐµÑÐ° ÑÐµÐ¿Ð»Ð¾Ð¾Ð±Ð¼ÐµÐ½Ð° Ð² Ð¿Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð¼ ÑÐ»Ð¾Ðµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÑÐ¸ÐºÐ¾Ð², ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 1999
Subjects: ÐÐ¾Ð³ÑÐ°Ð½Ð¸ÑÐ½ÑÐ¹ ÑÐ»Ð¾Ð¹ ÑÑÑÐ±ÑÐ»ÐµÐ½ÑÐ½ÑÐ¹

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð°Ð²ÑÐ¾ÑÑÐºÐ¾Ð¼Ñ ÐºÑÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ "Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¿Ð»Ð¾ÑÐµÑÐ½Ð¸ÐºÐ¸" Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 552700 "Ð­Ð½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ" Ð¸ 550900 "Ð¢ÐµÐ¿Ð»Ð¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°". Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ°ÐºÑÐ¾ÑÑ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ, Ð²Ð»Ð¸ÑÑÑÐ¸Ðµ Ð½Ð° Ð»Ð¾ÐºÐ°Ð»ÑÐ½ÑÐ¹ ÑÐµÐ¿Ð»Ð¾Ð¾Ð±Ð¼ÐµÐ½ Ð² Ð¿Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð¼ ÑÐ»Ð¾Ðµ, Ð²ÐºÐ»ÑÑÐ°ÑÑÐµÐ¼ Ð² ÑÐµÐ±Ñ Ð»Ð°Ð¼Ð¸Ð½Ð°ÑÐ½ÑÐ¹, Ð¿ÐµÑÐµÑÐ¾Ð´Ð½ÑÐ¹ Ð¸ ÑÑÑÐ±ÑÐ»ÐµÐ½ÑÐ½ÑÐ¹ ÑÑÐ°ÑÑÐºÐ¸ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÐ¿Ð¸ÑÐ°Ð½Ð° Ð°Ð»Ð³ÐµÐ±ÑÐ°Ð¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÑÑÐ±ÑÐ»ÐµÐ½ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð»Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ½ÑÑ Ð¾Ð±Ð»Ð°ÑÑÐµÐ¹ Ð¿Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ²Ð¾Ñ, ÑÑÐµÐ¼Ð° Ðº Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÐµ Ð±Ð»Ð¾ÐºÐ¸ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ. ÐÐ»Ð°Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ ÑÐ°ÑÑÐµÑÐ½Ð¾Ð¼Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð¾Ð´Ð½Ð¾Ð³Ð¾ (Ð´Ð²ÑÑ) ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð½Ð° ÑÐµÐ¿Ð»Ð¾Ð¾Ð±Ð¼ÐµÐ½ Ð² Ð¿Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð¼ ÑÐ»Ð¾Ðµ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐµÑÑÐ¾Ð²ÑÑ Ð·Ð°Ð´Ð°Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÑÐµÑÑÐµÐ³Ð¾ Ð¸ Ð¿ÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ¾Ð² ÑÐ½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ "Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¿Ð»Ð¾ÑÐµÑÐ½Ð¸ÐºÐ¸" Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Ð¸ Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÑ ÑÐ°Ð±Ð¾Ñ.
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 ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Additional file 2 of EchinoDB: an update to the web-based application for genomic and transcriptomic data on echinoderms
Creators: name: Mittal, Varnika
name: Reid, Robert W.
name: Machado, Denis Jacob
name: Mashanov, Vladimir
name: Janies, Daniel A.
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: File S1. EchinoDB user manual contains screenshots of the outputs to assist new users with the features and functionality of the application.
Quantum Key Distribution by Utilizing Four-Level Particles
Creators: name: Yan, Tao
name: Yan, Fengli
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a quantum key distribution protocol based on four-level particles entanglement. Furthermore, a controlled quantum key distribution protocol is proposed by utilizing three four-level particles. We show that the two protocols are secure.
description: 5 pages, no figure
DAFNE operation with the FINUDA experiment
Creators: name: C. Milardi
name: D. Alesini
name: G. Benedetti
name: M. E. Biagini
name: C. Biscari
name: R. Boni
name: M. Boscolo
name: A. Clozza
name: D. Delle Monache
name: G. Di Pirro
name: A. Drago
name: A. Gallo
name: A. Ghigo
name: S. Guiducci
name: M. Incurvati
name: C. Ligi
name: F. Marcellini
name: G. Mazzitelli
name: L. Pellegrino
name: M. A. Preger
name: P. Raimondi
name: R. Ricci
name: U. Rotundo
name: C. Sanelli
name: M. Serio
name: F. Sgamma
name: B. Spataro
name: A. Stecchi
name: A. Stella
name: C. Vaccarezza
name: M. Vescovi
name: M. Zobov
Publisher: name: INFN Open Access Repository
Year: 2004

description: DAFNE operation restarted in September 2003, after a six month shut-down for
the installation of FINUDA, a magnetic detector dedicated to the study of
hypernuclear physics. FINUDA is the third experiment running on DAFNE and
operates while keeping on place the other detector KLOE. During the shut-down
both Interaction Regions have been equipped with remotely controlled
quadrupoles in order to operate at different solenoid fields. Among many other
hardware upgrades one of the most significant is the reshaping of the wiggler
pole profile to improve the field quality and the machine dynamic aperture.
Commissioning of the collider in the new configuration has been completed in
short time. The peak luminosity delivered to FINUDA has reached 6 10^31
s-1cm-2, with a daily integrated value close to 4 pb-1.
Advances in ultrafast plasmonics
Creators: name: Koya, Alemayehu Nana
name: Romanelli, Marco
name: Kuttruff, Joel
name: Henriksson, Nils
name: Stefancu, Andrei
name: Grinblat, Gustavo
name: De Andres, Aitor
name: Schnur, Fritz
name: Vanzan, Mirko
name: Marsili, Margherita
name: Rahaman, Mahfujur
name: Rodríguez, Alba Viejo
name: Tapani, Tilaike
name: Lin, Haifeng
name: Dana, Bereket Dalga
name: Lin, Jingquan
name: Barbillon, Grégory
name: Zaccaria, Remo Proietti
name: Brida, Daniele
name: Jariwala, Deep
name: Veisz, László
name: Cortes, Emiliano
name: Corni, Stefano
name: Garoli, Denis
name: Maccaferri, Nicolò
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Applied Physics (physics.app-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In the past twenty years, we have reached a broad understanding of many light-driven phenomena in nanoscale systems. The temporal dynamics of the excited states are instead quite challenging to explore, and, at the same time, crucial to study for understanding the origin of fundamental physical and chemical processes. In this review we examine the current state and prospects of ultrafast phenomena driven by plasmons both from a fundamental and applied point of view. This research area is referred to as ultrafast plasmonics and represents an outstanding playground to tailor and control fast optical and electronic processes at the nanoscale, such as ultrafast optical switching, single photon emission and strong coupling interactions to tailor photochemical reactions. Here, we provide an overview of the field, and describe the methodologies to monitor and control nanoscale phenomena with plasmons at ultrafast timescales in terms of both modeling and experimental characterization. Various directions are showcased, among others recent advances in ultrafast plasmon-driven chemistry and multi-functional plasmonics, in which charge, spin, and lattice degrees of freedom are exploited to provide active control of the optical and electronic properties of nanoscale materials. As the focus shifts to the development of practical devices, such as all-optical transistors, we also emphasize new materials and applications in ultrafast plasmonics and highlight recent development in the relativistic realm. The latter is a promising research field with potential applications in fusion research or particle and light sources providing properties such as attosecond duration.
Phase-stabilized, 1.5-W frequency comb at 2.8 to 4.8 micron
Creators: name: Adler, Florian
name: Cossel, Kevin C.
name: Thorpe, Michael J.
name: Hartl, Ingmar
name: Fermann, Martin E.
name: Ye, Jun
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We present a high-power optical parametric oscillator-based frequency comb in the mid-infrared wavelength region using periodically poled lithium niobate. The system is synchronously pumped by a 10-W femtosecond Yb:fiber laser centered at 1.07 um and is singly resonant for the signal. The idler (signal) wavelength can be continuously tuned from 2.8 to 4.8 um (1.76 to 1.37 um) with a simultaneous bandwidth as high as 0.3 um and a maximum average idler output power of 1.50 W. We also demonstrate the performance of the stabilized comb by recording the heterodyne beat with a narrow-linewidth diode laser. This OPO is an ideal source for frequency comb spectroscopy in the mid-IR.
description: 4 figures
Progress and Validation of Geant4 Based Radioactive Decay Simulation
  Using the Examples of Simbol-X and IXO
Creators: name: S. Hauf
name: M. Kuster
name: M. G. Pia
name: Z. Bell
name: U. Briel
name: R. Chipaux
name: D. H. H. Hoffmann
name: E. Kendziorra
name: P. Laurent
name: L. Strüder
name: C. Tenzer
name: G. Weidenspointer
name: A. Zoglauer
Publisher: name: INFN Open Access Repository
Year: 2009

description: The anticipated high sensitivity and the science goals of the next generation
X-ray space missions, like the International X-ray Observatory or Simbol-X,
rely on a low instrumental background, which in turn requires optimized
shielding concepts. We present Geant4 based simulation results on the IXO Wide
Field Imager cosmic ray proton induced background in comparison with previous
results obtained for the Simbol-X LED and HED focal plane detectors. Our
results show that an improvement in mean differential background flux compared
to actually operating X-ray observatories may be feasible with detectors based
on DEPFET technology. In addition we present preliminary results concerning the
validation of Geant4 based radioactive decay simulation in space applications
as a part of the Nano5 project.
Measuring redshift-space distortions with future SKA surveys
Creators: name: Raccanelli, Alvise
name: Bull, Philip
name: Camera, Stefano
name: Bacon, David
name: Blake, Chris
name: Dore, Olivier
name: Ferreira, Pedro
name: Maartens, Roy
name: Santos, Mario
name: Viel, Matteo
name: Gong-Bo Zhao
Publisher: name: INFN Open Access Repository
Year: 2015

description: The peculiar motion of galaxies can be a particularly sensitive probe of
gravitational collapse. As such, it can be used to measure the dynamics of dark
matter and dark energy as well the nature of the gravitational laws at play on
cosmological scales. Peculiar motions manifest themselves as an overall
anisotropy in the measured clustering signal as a function of the angle to the
line-of-sight, known as redshift-space distortion (RSD). Limiting factors in
this measurement include our ability to model non-linear galaxy motions on
small scales and the complexities of galaxy bias. The anisotropy in the
measured clustering pattern in redshift-space is also driven by the unknown
distance factors at the redshift in question, the Alcock-Paczynski distortion.
This weakens growth rate measurements, but permits an extra geometric probe of
the Hubble expansion rate. In this chapter we will briefly describe the
scientific background to the RSD technique, and forecast the potential of the
SKA phase 1 and the SKA2 to measure the growth rate using both galaxy
catalogues and intensity mapping, assessing their competitiveness with current
and future optical galaxy surveys.
Lattice Theta Constants vs Riemann Theta Constants and NSR Superstring Measures
Creators: name: Dunin-Barkowski, P.
name: Morozov, A.
name: Sleptsov, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Algebraic Geometry (math.AG)
subject: Number Theory (math.NT)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We discuss relations between two different representations of hypothetical holomorphic NSR measures, based on two different ways of constructing the semi-modular forms of weight 8. One of these ways is to build forms from the ordinary Riemann theta constants and another -- from the lattice theta constants. We discuss unexpectedly elegant relations between lattice theta constants, corresponding to 16-dimensional self-dual lattices, and Riemann theta constants and present explicit formulae expressing the former ones through the latter. Starting from genus 5 the modular-form approach to construction of NSR measures runs into serious problems and there is a risk that it fails completely already at genus 6.
description: 16 pages
Scalar conservation laws with nonconstant coefficients with application to particle size segregation in granular flow
Creators: name: May, Lindsay B. H.
name: Shearer, Michael
name: Daniels, Karen E.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Analysis of PDEs (math.AP)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: Granular materials will segregate by particle size when subjected to shear, as occurs, for example, in avalanches. The evolution of a bidisperse mixture of particles can be modeled by a nonlinear first order partial differential equation, provided the shear (or velocity) is a known function of position. While avalanche-driven shear is approximately uniform in depth, boundary-driven shear typically creates a shear band with a nonlinear velocity profile. In this paper, we measure a velocity profile from experimental data and solve initial value problems that mimic the segregation observed in the experiment, thereby verifying the value of the continuum model. To simplify the analysis, we consider only one-dimensional configurations, in which a layer of small particles is placed above a layer of large particles within an annular shear cell and is sheared for arbitrarily long times. We fit the measured velocity profile to both an exponential function of depth and a piecewise linear function which separates the shear band from the rest of the material. Each solution of the initial value problem is non-standard, involving curved characteristics in the exponential case, and a material interface with a jump in characteristic speed in the piecewise linear case.
Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
Creators: name: Beltz-Mohrmann, Gillian D.
name: Szewciw, Adam O.
name: Berlind, Andreas A.
name: Sinha, Manodeep
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: This paper represents an effort to provide robust constraints on the galaxy-halo connection and simultaneously test the Planck LCDM cosmology using a fully numerical model of small-scale galaxy clustering. We explore two extensions to the standard Halo Occupation Distribution model: assembly bias, whereby halo occupation depends on both halo mass and the larger environment, and velocity bias, whereby galaxy velocities do not perfectly trace the velocity of the dark matter within the halo. Moreover, we incorporate halo mass corrections to account for the impact of baryonic physics on the halo population. We identify an optimal set of clustering measurements to constrain this "decorated" HOD model for both low- and high-luminosity galaxies in SDSS DR7. We find that, for low-luminosity galaxies, a model with both assembly bias and velocity bias provides the best fit to the clustering measurements, with no tension remaining in the fit. In this model we find evidence for both central and satellite galaxy assembly bias at the 99% and 95% confidence levels, respectively. In addition, we find evidence for satellite galaxy velocity bias at the 99.9% confidence level. For high luminosity galaxies, we find no evidence for either assembly bias or velocity bias, but our model exhibits significant tension with SDSS measurements. We find that all of these conclusions still stand when we include the effects of baryonic physics on the halo mass function, suggesting that the tension we find for high luminosity galaxies may be due to a problem with our assumed cosmological model.
description: 27 pages, 13 figures
Black hole-black string phase transitions from hydrodynamics
Creators: name: Maeda, Kei-ichi
name: Miyamoto, Umpei
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We discuss the phase transitions between three states of a plasma fluid (plasma ball, uniform plasma tube, and non-uniform plasma tube), which are dual to the corresponding finite energy black objects (black hole, uniform black string, and non-uniform black string) localized in an asymptotically locally AdS space. Adopting the equation of state for the fluid obtained by the Scherk-Schwarz compactification of a conformal field theory, we obtain axisymmetric static equilibrium states of the plasma fluid and draw the phase diagrams with their thermodynamical quantities. By use of the fluid/gravity correspondence, we predict the phase diagrams of the AdS black holes and strings on the gravity side. The thermodynamic phase diagrams of the AdS black holes and strings show many similarities to those of the black hole-black string system in a Kaluza-Klein vacuum. For instance, the critical dimension for the smooth transition from the uniform to non-uniform strings is the same as that in the Kaluza-Klein vacuum in the canonical ensemble. The analysis in this paper may provide a holographic understanding of the relation between the Rayleigh-Plateau and Gregory-Laflamme instabilities via the fluid/gravity correspondence.
description: 22 pages, 6 figures, 2 tables; v3: Appendix B added
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÐºÑÑ Ð½Ð¸ Ð½Ð° 50 Ð¼ÐµÑÑ Ð² ÐÐ°ÑÐ¸Ð»ÐµÐ¾ÑÑÑÐ¾Ð²ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐµÐ½ÐºÐ¾Ð²Ð°, ÐÐ½Ð¶ÐµÐ»Ð¸ÐºÐ°
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ÐµÑÑÐ¾ÑÐ°Ð½
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
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description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð°, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
Nanotechnology as a Field of Science: Its Delineation in terms of Journals and Patents
Creators: name: Leydesdorff, Loet
name: Zhou, Ping
Publisher: name: arXiv
Year: 2009
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: The Journal Citation Reports of the Science Citation Index 2004 were used to delineate a core set of nanotechnology journals and a nanotechnology-relevant set. In comparison with 2003, the core set has grown and the relevant set has decreased. This suggests a higher degree of codification in the field of nanotechnology: the field has become more focused in terms of citation practices. Using the citing patterns among journals at the aggregate level, a core group of ten nanotechnology journals in the vector space can be delineated on the criterion of betweenness centrality. National contributions to this core group of journals are evaluated for the years 2003, 2004, and 2005. Additionally, the specific class of nanotechnology patents in the database of the U.S. Patent and Trade Office (USPTO) is analyzed to determine if non-patent literature references can be used as a source for the delineation of the knowledge base in terms of scientific journals. The references are primarily to general science journals and letters, and therefore not specific enough for the purpose of delineating a journal set.
Glitches Compensation in EXAFS Data Collection
Creators: name: F. Comin
name: L. Incoccia
name: S. Mobilio
Publisher: name: INFN Open Access Repository
Year: 1982

description: In all the Synchrotron X-ray beam lines, one of the major experimental problems in due to the 'glitches' that distort monochromatized radiation. In principle, if the X-ray absorption measuring apparatus were linear, such distortions should be compensed. In practice this is not always so because of many frequent experimental inaccuracies. We analyzed the most important of these, and suggest the correct procedure to avoid them.
Heavy Baryons in Compact Stars
Creators: name: Sedrakian, Armen
name: Li, Jia-Jie
name: Weber, Fridolin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We review the physics of hyperons and $Δ$-resonances in dense matter in compact stars. The covariant density functional approach to the equation of state and composition of dense nuclear matter in the mean-field Hartree and Hartree-Fock approximation is presented, with regimes covering cold $β$-equilibrated matter, hot and dense matter with and without neutrinos relevant for the description of supernovas and binary neutron star mergers, as well as dilute expanding nuclear matter in collision experiments. We discuss the static properties of compact stars with hyperons and $Δ$-resonances in light of constraints placed in recent years by the multimessenger astrophysics of compact stars on the compact stars' masses, radii, and tidal deformabilities. The effects of kaon condensation and strong magnetic fields on the composition of hypernuclear stars are also discussed. The properties of rapidly rotating compact hypernuclear stars are discussed and confronted with the observations of 2.5-2.8 solar mass compact objects in gravitational wave events. We further discuss the cooling of hypernuclear stars, the neutrino emission reactions, hyperonic pairing, and the mass hierarchy in the cooling curves that arises due to the onset of hyperons. The effects of hyperons and $Δ$-resonances on the equation of state of hot nuclear matter in the dense regime, relevant for the transient astrophysical event and in the dilute regime relevant to the collider physics is discussed. The review closes with a discussion of universal relations among the integral parameters of hot and cold hypernuclear stars and their implications for the analysis of binary neutron star merger events.
description: v3 and v2: 79 pages, 26 figures, final version (minor changes and additions, typos corrected). v1: 76 pages, 26 figures. arXiv admin note: text overlap with arXiv:2105.14050
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð²ÑÑ Ð¾Ð´Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð½Ð° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ ÑÑÐ½Ð¾Ðº (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Â«ÐÐ»ÑÑ-Ð¡ÐÂ»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð³ÑÐ½, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸
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description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð° Ð´Ð»Ñ Ð²ÑÑÐ¾Ð´Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«ÐÐ»ÑÑ-Ð¡ÐÂ» Ð½Ð° Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÐ¹ ÑÑÐ½Ð¾Ðº, Ð° ÑÐ°ÐºÐ¶Ðµ ÐµÐ³Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ, ÑÐ¾ ÐµÑÑÑ ÑÐ°ÑÑÐµÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° Ð¾ÑÑÐ°Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð²Ð¸Ð´ÐµÐ¾Ð½Ð°Ð±Ð»ÑÐ´ÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÐ½ÐºÐ° Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÐÐ°Ð·Ð°ÑÑÑÐ°Ð½Ð°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐ¹ ÑÐ¿Ð¾ÑÐ¾Ð± Ð²ÑÑÐ¾Ð´Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«ÐÐ»ÑÑ-Ð¡ÐÂ» Ð½Ð° ÑÑÐ½Ð¾Ðº ÐÐ°Ð·Ð°ÑÑÑÐ°Ð½Ð° Ð¸ ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ Ð´Ð»Ñ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ³Ð¾ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¸ÑÐ¼Ñ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸: ÑÐ¸ÑÑÐ°Ñ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð½Ð°Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ (NPV), Ð²Ð½ÑÑÑÐµÐ½Ð½ÑÑ Ð½Ð¾ÑÐ¼Ð° Ð´Ð¾ÑÐ¾Ð´Ð½Ð¾ÑÑÐ¸ (IRR), Ð¸Ð½Ð´ÐµÐºÑ Ð¿ÑÐ¸Ð±ÑÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ (PI), ÐºÐ¾ÑÐ¾ÑÑÐµ Ð´Ð¾ÐºÐ°Ð·Ð°Ð»Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ¸Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½ ÑÑÐ¾Ðº Ð¾ÐºÑÐ¿Ð°ÐµÐ¼Ð¾ÑÑÐ¸ Ð¸ Ð½Ð°Ð¹Ð´ÐµÐ½Ð° ÑÐ¾ÑÐºÐ° Ð±ÐµÐ·ÑÐ±ÑÑÐ¾ÑÐ½Ð¾ÑÑÐ¸, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿Ð¾Ð¼Ð¾Ð³ÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«ÐÐ»ÑÑ-Ð¡ÐÂ» ÑÐµÑÐºÐ¾ ÑÐ¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÐ²Ð¾Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð² ÑÐ¾Ð´Ðµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð²ÑÑÐ¾Ð´Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«ÐÐ»ÑÑ-Ð¡ÐÂ» Ð½Ð° ÑÑÐ½Ð¾Ðº ÐÐ°Ð·Ð°ÑÑÑÐ°Ð½Ð°, Ð´Ð¾ÐºÐ°Ð·Ð°Ð½Ð° Ð²Ð°Ð¶Ð½Ð¾ÑÑÑ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¸ Ð²ÑÑÐ¾Ð´Ðµ Ð½Ð° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ ÑÑÐ½Ð¾Ðº.
Imaginary Powers of the Dunkl Harmonic Oscillator
Creators: name: Nowak, Adam
name: Stempak, Krzysztof
Publisher: name: arXiv
Year: 2009
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics

description: In this paper we continue the study of spectral properties of the Dunkl harmonic oscillator in the context of a finite reflection group on $\mathbb{R}^d$ isomorphic to $\mathbb{Z}^d_2$. We prove that imaginary powers of this operator are bounded on $L^p$, $1
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð´Ð¸Ð·Ð°Ð¹Ð½Ð° ÐºÐ½Ð¸Ð³Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐµÐ·Ð¾Ð²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð´Ð¸Ð·Ð°Ð¹Ð½ ÐºÐ½Ð¸Ð³Ð¸
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description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ ÐºÐ½Ð¸Ð³Ð¸ Ñ Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¸ÑÐ¼Ð¸, Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¸ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¹ Ð³ÑÐ°ÑÐ¸ÐºÐ¸. ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð´Ð¸Ð·Ð°Ð¹Ð½Ð° ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð²Ð¼ÐµÑÐµÐ½Ð¸Ðµ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¹ Ð³ÑÐ°ÑÐ¸ÐºÐ¸ Ð¸ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¸Ð¸. ÐÐ½Ð¸Ð³Ð° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ 18 ÑÑÑÐ°Ð½Ð¸Ñ, Ð¸Ð· ÐºÐ¾ÑÐ¾ÑÑÑ 16 ÑÐ¾Ð´ÐµÑÐ¶Ð°Ñ ÑÐ²ÐµÑÐ½ÑÐµ Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¸Ð¸.
Coherent generation and control of tunable narrowband THz radiation from laser-induced air-plasma filament
Creators: name: Zhou, Xiaoyue
name: Lin, Yuchen
name: Chan, Yi
name: Deng, Fu
name: Zhang, Jingdi
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We report on the proof-of-principle experiment of generating carrier-envelope phase (CEP)-controllable and frequency-tunable narrowband terahertz (THz) radiation from air-plasma filament prescribed by the beat of temporally stretched two-color laser pulse sequence. The pulse sequence was prepared by propagating the fundamental ultrafast laser pulse through a grating stretcher and Michelson interferometer with variable inter-arm delay. By partially frequency-doubling and focusing the pulse sequence, an air-plasma filament riding a beat note was created to radiate THz wave with primary pulse characteristics (center frequency and CEP) under coherent control. To reproduce experimental results and elucidate complex nonlinear light-matter interaction, numerical simulation has been performed. This work demonstrates the feasibility of generating coherently controlled narrowband THz wave with high tunability in laser-induced air plasma.
description: 14 pages, 4 figures
Classification of Topological Insulators and Superconductors
Creators: name: Schnyder, Andreas P.
name: Ryu, Shinsei
name: Furusaki, Akira
name: Ludwig, Andreas W. W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: An exhaustive classification scheme of topological insulators and superconductors is presented. The key property of topological insulators (superconductors) is the appearance of gapless degrees of freedom at the interface/boundary between a topologically trivial and a topologically non-trivial state. Our approach consists in reducing the problem of classifying topological insulators (superconductors) in d spatial dimensions to the problem of Anderson localization at a (d-1) dimensional boundary of the system. We find that in each spatial dimension there are precisely five distinct classes of topological insulators (superconductors). The different topological sectors within a given topological insulator (superconductor) can be labeled by an integer winding number or a Z_2 quantity. One of the five topological insulators is the 'quantum spin Hall' (or: Z_2 topological) insulator in d=2, and its generalization in d=3 dimensions. For each dimension d, the five topological insulators correspond to a certain subset of five of the ten generic symmetry classes of Hamiltonians introduced more than a decade ago by Altland and Zirnbauer in the context of disordered systems (which generalizes the three well known "Wigner-Dyson'' symmetry classes).
description: 12 pages, 5 figures; Proceedings of the L.D. Landau Memorial Conference, 2008
Additional file 3 of EchinoDB: an update to the web-based application for genomic and transcriptomic data on echinoderms
Creators: name: Mittal, Varnika
name: Reid, Robert W.
name: Machado, Denis Jacob
name: Mashanov, Vladimir
name: Janies, Daniel A.
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: File S2. EchinoidDB user manual contains instructions to help users with the resources and operations available in the application.
Some factors which influence the use of dwarf and semi-dwarf apple trees for commercial orchards in the Okanagan Valley of British Columbia
Creators: name: Van Roechoudt, Louis Laurent Leon
Publisher: name: University of British Columbia
Year: 2011

description: An investigation was carried out in order to evaluate some of the factors which influence the use of dwarf and semi-dwarf apple trees in commercial orchards in the Okanagan Valley of British Columbia. Three determining factors were found to be of prime importance: the planting density of the trees in the orchard, the tree form as determined by the pruning and training system carried out and the nature of the rootstock used. In the Doornberg Orchards at Okanagan Centre where the experiments were conducted, semi-dwarf trees on Malling VII rootstock trained as hedgerows and planted at a high density per acre gave the optimum earliest and total yields and returns. The experiments were carried out from planting time up to the end of the sixth growing season. The variety of apple used in the experiment was Golden Delicious.
title: ÐÑÐ¾ÐµÐºÑ ÑÐ¾Ð»Ð½ÐµÑÐ½Ð¾-Ð´Ð¸Ð·ÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð² ÑÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐµ Ð¡Ð°Ñ Ð° (Ð¯ÐºÑÑÐ¸Ñ)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¼Ð¸ÑÐ½Ð¾Ð²Ð°, ÐÐ°ÑÐ³Ð°ÑÐ¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ¾ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð°Ð½ÐµÐ»Ð¸
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐ°Ð¿Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¡Ð­Ð¡ Ð² ÑÐ¾ÑÑÐ°Ð²Ðµ ÑÐ¾Ð»Ð½ÐµÑÐ½Ð¾-Ð´Ð¸Ð·ÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð´Ð»Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«ÐÐ°Ð»ÑÐ²Ð¸ÑÐ° Ð ÑÐ±Ð·Ð°Ð²Ð¾Ð´Â» Ð² ÑÐµÐ»Ðµ ÐÐ°Ð»ÑÐ²Ð¸ÑÐ° Ð² ÐÐ¾Ð±ÑÐ¹ÑÐºÐ¾Ð¼ ÑÐ»ÑÑÐµ. ÐÐ°Ð½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¾Ð»Ð½ÐµÑÐ½Ð¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÐ¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°. ÐÐ±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ Ð¡Ð­Ð¡, ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²ÐºÐ°, ÑÐ°ÑÑÐµÑ Ð²ÑÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ¾Ð»Ð½ÐµÑÐ½Ð¾-Ð´Ð¸Ð·ÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸. ÐÐ°Ð½Ð¾ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ°.
Fermions, Skyrmions and the 3-Sphere
Creators: name: Goatham, Stephen W.
name: Krusch, Steffen
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: This paper investigates a background charge one Skyrme field chirally coupled to light fermions on the 3-sphere. The Dirac equation for the system commutes with a generalised angular momentum or grand spin. It can be solved explicitly for a Skyrme configuration given by the hedgehog form. The energy spectrum and degeneracies are derived for all values of the grand spin. Solutions for non-zero grand spin are each characterised by a set of four polynomials. The paper also discusses the energy of the Dirac sea using zeta function regularization.
description: 19 pages, 2 figures
Additional file 4 of EchinoDB: an update to the web-based application for genomic and transcriptomic data on echinoderms
Creators: name: Mittal, Varnika
name: Reid, Robert W.
name: Machado, Denis Jacob
name: Mashanov, Vladimir
name: Janies, Daniel A.
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4: File S3. OphiuroidDB user manual to describe operations and capabilities of the application.
Bounding Real Tensor Optimizations via the Numerical Range
Creators: name: Johnston, Nathaniel
name: Pipes, Logan
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optimization and Control (math.OC)
subject: Quantum Physics (quant-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We show how the numerical range of a matrix can be used to bound the optimal value of certain optimization problems over real tensor product vectors. Our bound is stronger than the trivial bounds based on eigenvalues, and can be computed significantly faster than bounds provided by semidefinite programming relaxations. We discuss numerous applications to other hard linear algebra problems, such as showing that a real subspace of matrices contains no rank-one matrix, and showing that a linear map acting on matrices is positive.
description: 22 pages
Perturbative and numerical approach to plasma strong lensing
Creators: name: Crisnejo, Gabriel
name: Gallo, Emanuel
name: Boero, Ezequiel
name: Moreschi, Osvaldo M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: {Using two different approaches, we study imaging in the strong lens regime taking into account the effects of plasmatic environments on light propagation. First, we extend the use of a perturbative approach that allows us to quickly and analytically calculate the position and shape of the images of a circular source lensed by a galaxy. Such approach will be compared with that obtained from the numerical solution of the lens equations. Secondly, we introduce a 3-dimensional spheroidal model to describe the spacetime associated with the dark matter halo around the lens galaxy and an associated optical metric to incorporate the presence of the plasma medium. The (chromatic) deformation on caustic and critical curves and associated multiplicity of images is also analyzed for particular configurations.