cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A search for correlated low-energy electron antineutrinos in KamLAND with gamma-ray bursts
Creators: name: Abe, S.
name: Asami, S.
name: Gando, A.
name: Gando, Y.
name: Gima, T.
name: Goto, A.
name: Hachiya, T.
name: Hata, K.
name: Hosokawa, K.
name: Ichimura, K.
name: Ieki, S.
name: Ikeda, H.
name: Inoue, K.
name: Ishidoshiro, K.
name: Kamei, Y.
name: Kawada, N.
name: Kishimoto, Y.
name: Kinoshita, T.
name: Koga, M.
name: Maemura, N.
name: Mitsui, T.
name: Miyake, H.
name: Nakamura, K.
name: Nakamura, K.
name: Nakamura, R.
name: Ozaki, H.
name: Sakai, T.
name: Sambonsugi, H.
name: Shimizu, I.
name: Shirai, J.
name: Shiraishi, K.
name: Suzuki, A.
name: Suzuki, Y.
name: Takeuchi, A.
name: Tamae, K.
name: Eizuka, M.
name: Kurasawa, M.
name: Nakahata, T.
name: Futagi, S.
name: Watanabe, H.
name: Yoshida, Y.
name: Obara, S.
name: Ichikawa, A. K.
name: Yoshida, S.
name: Umehara, S.
name: Fushimi, K.
name: Berger, B. E.
name: Fujikawa, B. K.
name: Learned, J. G.
name: Maricic, J.
name: Axani, S. N.
name: Smolsky, J.
name: Laber-Smith, C.
name: Winslow, L. A.
name: Fu, Z.
name: Ouellet, J.
name: Efremenko, Y.
name: Karwowski, H. J.
name: Markoff, D. M.
name: Tornow, W.
name: Li, A.
name: Detwiler, J. A.
name: Enomoto, S.
name: Decowski, M. P.
name: Grant, C.
name: Song, H.
name: O'Donnell, T.
name: Dell'Oro, S.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present the results of a time-coincident event search for low-energy electron antineutrinos in the KamLAND detector with gamma-ray bursts from the Gamma-ray Coordinates Network and Fermi Gamma-ray Burst Monitor. Using a variable coincidence time window of $\pm$500s plus the duration of each gamma-ray burst, no statistically significant excess above background is observed. We place the world's most stringent 90% confidence level upper limit on the electron antineutrino fluence below 17.5 MeV. Assuming a Fermi-Dirac neutrino energy spectrum from the gamma-ray burst source, we use the available redshift data to constrain the electron antineutrino luminosity and effective temperature.
description: 9 pages, 3 figures
Additional file 5 of Tumor infiltrating neutrophil might play a major role in predicting the clinical outcome of breast cancer patients treated with neoadjuvant chemotherapy
Creators: name: Geng, Sheng-Kai
name: Fu, Shao-Mei
name: Ma, Shi-Hong
name: Fu, Yi-Peng
name: Zhang, Hong-Wei
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Plant Biology

description: Additional file 5: Supplement Table 1. Clinicopathological Characteristics: Univariate and Multivariate Survival Analyses.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¸ÑÑÐµÐ¼Ñ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð´Ð»Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ ÑÐºÐ»Ð°Ð´Ð° Ñ ÐÐÐ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð¶Ð½ÐµÐ²Ð°, ÐÑ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ÐºÐ»Ð°Ð´Ñ
Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð²
Ð¿ÑÐ¾ÐµÐºÑÑ
ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾

description: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ ÑÐºÐ»Ð°Ð´Ð° Ð´Ð»Ñ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð»ÐµÐ³ÐºÐ¾-Ð²Ð¾ÑÐ¿Ð»Ð°Ð¼ÐµÐ½ÑÑÑÐ¸ÑÑÑ Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐµÐ¹. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¸ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÑÑÑÑ Ðº ÑÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Â«Ð ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°Â» Ð¸ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Â«Ð ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¿ÑÐµÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð²Â» ÐºÐ¾ÑÐ¾ÑÑÐµ Ð±ÑÐ´ÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. ÐÐ°Ð½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²ÑÑÑ ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð¸Ñ ÑÐµÐºÑÑÐµÑÑÐ¸ ÐºÐ°Ð´ÑÐ¾Ð², Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÑÑÐ´Ð¾Ð²ÑÑ Ð¾Ð±ÑÐ·Ð°Ð½Ð½Ð¾ÑÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ°Ð¼Ð¸.
Dirac neutrinos from a second Higgs doublet
Creators: name: Davidson, Shainen M.
name: Logan, Heather E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose a minimal extension of the Standard Model in which neutrinos are Dirac particles and their tiny masses are explained without requiring tiny Yukawa couplings. A second Higgs doublet with a tiny vacuum expectation value provides neutrino masses while simultaneously improving the naturalness of the model by allowing a heavier Standard Model-like Higgs boson consistent with electroweak precision data. The model predicts a mu to e gamma rate potentially detectable in the current round of experiments, as well as distinctive signatures in the production and decay of the charged Higgs H+ of the second doublet which can be tested at future colliders. Neutrinoless double beta decay is absent.
description: 7 pages, 3 figures; v2: intro expanded, refs added, submitted to PRD
Light bending from eikonal in worldline quantum field theory
Creators: name: Bastianelli, Fiorenzo
name: Comberiati, Francesco
name: de la Cruz, Leonardo
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Using the worldline quantum field theory (WQFT) formalism for classical scattering, we study the deflection of light by a heavy massive spinless/spinning object. WQFT requires the use of the worldline dressed propagator of a photon in a gravitational background, which we construct from first principles. The action required to set up the worldline path integral is constructed using auxiliary variables, which describe dynamically the spin degrees of freedom of the photon and take care of path ordering. We test the fully regulated path integral by recovering the photon--photon-graviton vertex. With the dressed propagator at hand, we follow the WQFT procedure by setting up the partition function and deriving the Feynman rules which can be used to evaluate it perturbatively. These rules depend on the auxiliary variables. The latter ultimately do not contribute in the geometric-optics regime, which realizes the equivalence between the scattering of a photon and a massive scalar with that of a massless and a massive scalar. Then, the calculation of the eikonal phase and the deflection angle simplifies considerably. Using the eikonal phase defined in terms of the partition function, we calculate explicitly the deflection angle at NLO in the spinless case, and at LO in the spinning case up to quadratic order in spin.
description: 33 pages; v2: references added, minor changes, version to be published
title: ÐÐ°Ð·ÐµÑÑ. ÐÐ·Ð¼ÐµÑÐµÐ½Ð¸Ñ. ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ. 2013. Ð¢. 2
title: ÑÐ±Ð¾ÑÐ½Ð¸Ðº Ð´Ð¾ÐºÐ»Ð°Ð´Ð¾Ð² 23-Ð¹ ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸
titleType: Subtitle
Creators: name: "ÐÐ°Ð·ÐµÑÑ. ÐÐ·Ð¼ÐµÑÐµÐ½Ð¸Ñ. ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (23; 2013; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: ÐÐµÐ½ÐµÑÐ°ÑÐ¾ÑÑ ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÐµ
ÐÐ°Ð·ÐµÑÐ½Ð¾Ðµ Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ðµ

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸Ðº Ð²ÐºÐ»ÑÑÐµÐ½Ñ Ð´Ð¾ÐºÐ»Ð°Ð´Ñ, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð½Ð° 23-Ð¹ ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Â«ÐÐ°Ð·ÐµÑÑ. ÐÐ·Ð¼ÐµÑÐµÐ½Ð¸Ñ. ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ. 2013Â». Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½ Ð½Ð° Ð½Ð°ÑÑÐ½ÑÑ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð², Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑÐ¾Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹.
A frequency doubled 1534 nm laser system for potassium laser cooling
Creators: name: Stern, Guillaume
name: Allard, Baptiste
name: Robert-de-Saint-Vincent, Martin
name: Brantut, Jean-Philippe
name: Battelier, Baptiste
name: Bourdel, Thomas
name: Bouyer, Philippe
Publisher: name: arXiv
Year: 2010
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We demonstrate a compact laser source suitable for the trapping and cooling of potassium. By frequency doubling a fiber laser diode at 1534 nm in a waveguide, we produce 767 nm laser light. A current modulation of the diode allows to generate the two required frequencies for cooling in a simple and robust apparatus. We successfully used this laser source to trap ^39 K.
Cosmology with the shear-peak statistics
Creators: name: Dietrich, J. P.
name: Hartlap, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Weak-lensing searches for galaxy clusters are plagued by low completeness and purity, severely limiting their usefulness for constraining cosmological parameters with the cluster mass function. A significant fraction of `false positives' are due to projection of large-scale structure and as such carry information about the matter distribution. We demonstrate that by constructing a "peak function", in analogy to the cluster mass function, cosmological parameters can be constrained. To this end we carried out a large number of cosmological N-body simulations in the Ω_m-σ_8 plane to study the variation of this peak function. We demonstrate that the peak statistics is able to provide constraints competitive with those obtained from cosmic-shear tomography from the same data set. By taking the full cross-covariance between the peak statistics and cosmic shear into account, we show that the combination of both methods leads to tighter constraints than either method alone can provide.
description: 11 pages, 6 figures, accepted for publication in MNRAS. Minor changes to description of N-body and ray-tracing simulations
Additional file 1 of Continuity in general practice and hospitalization patterns: an observational study
Creators: name: Wensing, Michel
name: Szecsenyi, Joachim
name: Laux, Gunter
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Additional file 1 Table S1. List of ICD 10-GM Codes Used to Identify Hospitalizations for Ambulatory Care–Sensitive Conditions.
title: ÐÐµÑÐ¾Ð´Ñ Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð° Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð² Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Â«Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÂ»
titleType: Subtitle
Creators: name: ÐÑÐ±Ð¾Ð¼ÑÐ´ÑÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐ°ÐºÐ°ÑÐ¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: Ð¢Ð°ÑÐ°ÑÐ¾Ð², Ð¡ÑÐ°Ð½Ð¸ÑÐ»Ð°Ð²
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2011
Subjects: ÐÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¸ Ð¿ÑÐ¸Ð±Ð¾ÑÑ

description: ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð¿Ð¾ Ð²ÑÐ±Ð¾ÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð² Ð´Ð»Ñ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ Ð¸ ÑÐ³Ð»Ð¾Ð²ÑÑ ÑÐ°Ð·Ð¼ÐµÑÐ¾Ð², Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð·ÑÐ±ÑÐ°ÑÑÑ ÐºÐ¾Ð»ÐµÑ, Ð¿Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ð¹ Ð´Ð»Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐ°Ð·Ð¼ÐµÑÐ¾Ð², ÑÐ¾ÑÐ¼Ñ Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð½Ð¾Ð³Ð¾ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐµÐ¹ Ð´ÐµÑÐ°Ð»Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÐµÐ´ÑÑÐ² Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ. ÐÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÑÐµÐ´ÑÑÐ² Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Â» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÂ», Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«ÐÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Â» Ð¸ Â«ÐÐ°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ».
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Bounds for the discrete correlation of infinite sequences on k symbols and generalized Rudin-Shapiro sequences
Creators: name: Grant, E.
name: Shallit, J.
name: Stoll, T.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Combinatorics (math.CO)
subject: Formal Languages and Automata Theory (cs.FL)
subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 68R15; 11K38; 11A63; 05D99; 11K31

description: Motivated by the known autocorrelation properties of the Rudin-Shapiro sequence, we study the discrete correlation among infinite sequences over a finite alphabet, where we just take into account whether two symbols are identical. We show by combinatorial means that sequences cannot be "too" different, and by an explicit construction generalizing the Rudin-Shapiro sequence, we show that we can achieve the maximum possible difference.
description: Improved Introduction and new Section 6 (Lovasz local lemma)
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, Ð¾ÑÐ½Ð°ÑÑÐºÐ¸ Ð¸ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð³Ð¾ÑÑÑÐµÐ¹ Ð¾Ð±ÑÐµÐ¼Ð½Ð¾Ð¹ ÑÑÐ°Ð¼Ð¿Ð¾Ð²ÐºÐ¸ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ Â«Ð¨ÐµÑÑÐµÑÐ½Ñ ÐºÐ¾Ð½Ð¸ÑÐµÑÐºÐ°ÑÂ»
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ¼Ð°Ð½Ð¾Ð², ÐÐµÐ½Ð¸Ð°Ð¼Ð¸Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¨ÑÐ°Ð¼Ð¿Ð¾Ð²ÐºÐ° Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð³Ð¾ÑÑÑÐ°Ñ
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Additional file 1 of Clinical outcome and pathologic correlation of stereotactic body radiation therapy as a bridge to transplantation for advanced hepatocellular carcinoma: a case series
Creators: name: Wang, Ying-Fu
name: Dai, Yang-Hong
name: Chun-Shu Lin
name: Hao-Chih Chang
name: Po-Chien Shen
name: Jen-Fu Yang
name: Chih-Weim Hsiang
name: Cheng-Hsiang Lo
name: Huang, Wen-Yen
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Cell Biology
Pharmacology
Cancer
Science Policy

description: Additional file 1: Table S1: Prognostic factors influencing RFS and OS after LT using the Cox proportional hazards model.
title: ÐÑÐ½Ð¾Ð²Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸. Ð§. 2, ÐÐ»Ð³ÐµÐ±ÑÐ°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°
titleType: Subtitle
Creators: name: ÐÐ·Ð¾ÑÐ¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
name: ÐÐ°Ð´Ð°Ð½Ð¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: Ð¡ÑÑÑÐ³Ð¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: Ð§Ð°Ð¹ÐºÐ¸Ð½Ð°, Ð¢Ð°Ð¼Ð°ÑÐ°
Publisher: name: [Ð¡ÐÐ±ÐÐ¢Ð£]
Year: 1993
Subjects: ÐÐ»Ð³ÐµÐ±ÑÐ°

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¾ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¾Ð¿ÑÑÐ° Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸ Ð½Ð° Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐµ Ð¡ÐÐ±ÐÐ¢Ð£. ÐÐ½Ð¾ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¼ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÐ¾ÑÐµÐ½Ð¸Ñ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÐºÑÑÑÐ° ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°ÑÐ½Ð¾Ð¹ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÐ½Ð¾Ð² Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð²ÑÑÑÐµÐ¹ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸ Ð¸ Ð¿ÑÐµÐ´Ð¼ÐµÑÐ¾Ð² ÐµÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾-Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð°. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· ÑÑÐµÑ ÑÐ°ÑÑÐµÐ¹. Ð§Ð°ÑÑÑ Ð¿ÐµÑÐ²Ð°Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÐ¸ÑÐ»Ð¾Ð²ÑÑ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ², Ð¿Ð»Ð°Ð½Ð¸Ð¼ÐµÑÑÐ¸Ð¸ Ð¸ Ð²ÐµÐºÑÐ¾ÑÐ½Ð¾Ð¹ Ð°Ð»Ð³ÐµÐ±ÑÑ. ÐÐ½Ð° ÑÐ²Ð»ÑÐµÑÑÑ Ð±Ð°Ð·Ð¾Ð²Ð¾Ð¹ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð² Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸,ÑÐ¸Ð·Ð¸ÐºÐ¸ Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð³ÑÐ°ÑÐ¸ÐºÐ¸. Ð§Ð°ÑÑÑ Ð²ÑÐ¾ÑÐ°Ñ Ð¸ ÑÑÐµÑÑÑ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ñ Ð°Ð»Ð³ÐµÐ±ÑÐµ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ¾Ð¶Ð´ÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¸ Ð¸ÑÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð²ÑÑÐ°Ð¶ÐµÐ½Ð¸Ð¹, Ð¸ÑÑÐ»ÐµÐ´ÑÑÑÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°ÑÐ½ÑÑ ÑÑÐ½ÐºÑÐ¸Ð¹, Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¸Ð·ÑÑÐ°ÑÑÑÑ Ð°Ð»Ð³ÐµÐ±ÑÐ°Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð½ÐµÑÐ°Ð²ÐµÐ½ÑÑÐ²Ð°. ÐÐ¾ÑÐ»ÐµÐ´Ð½ÑÑ Ð³Ð»Ð°Ð²Ð° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐµÐ¾ÑÐ¸Ð¸ Ð»Ð¾Ð³Ð°ÑÐ¸ÑÐ¼Ð¾Ð², ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°Ð¼ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¸ Ð»Ð¾Ð³Ð°ÑÐ¸ÑÐ¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐ½ÐºÑÐ¸Ð¹. ÐÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ Ð±Ð¾Ð»ÑÑÐ¾Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¿ÑÐ¸Ð¼ÐµÑÐ¾Ð² Ñ ÑÐµÑÐµÐ½Ð¸ÑÐ¼Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ. Ð¡ ÑÐµÐ»ÑÑ Ð³ÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÐºÑÑÑÐ° Ð² ÐºÐ¾Ð½ÑÐµ ÐºÐ°Ð¶Ð´Ð¾Ð¹ Ð³Ð»Ð°Ð²Ñ Ð´Ð°ÐµÑÑÑ ÐºÑÐ°ÑÐºÐ°Ñ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¾Ð¿ÑÐ°Ð²ÐºÐ°. ÐÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»Ð¸ Ð¼Ð¾Ð³ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ ÑÑÐ¾Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð½Ð° Ð·Ð°Ð½ÑÑÐ¸ÑÑ Ñ ÑÐµÐ»ÑÑ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐµÑÐµÑÐ° Ðº Ð¿ÑÐµÐ´Ð¼ÐµÑÑ, Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð½Ð°ÑÑÐ½Ð¾Ð¼Ñ ÑÑÐ¸Ð»Ñ ÑÐµÑÐ¸. ÐÐ²ÑÐ¾ÑÑ Ð±Ð»Ð°Ð³Ð¾Ð´Ð°ÑÑÑ ÐÑÑÑÐ·Ð¾Ð²Ñ Ð. Ð. Ð·Ð° ÑÐµÐ½Ð½ÑÐµ Ð·Ð°Ð¼ÐµÑÐ°Ð½Ð¸Ñ Ð¸ ÑÐµÐ´Ð°ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÑÐºÐ¾Ð³Ð¾ ÑÐµÐºÑÑÐ°. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ð¾ Ðº Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ ÐºÐ°ÑÐµÐ´ÑÐ¾Ð¹ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸ Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¡Ð¾Ð²ÐµÑÐ¾Ð¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°.
Direct observation of number squeezing in an optical lattice
Creators: name: Itah, A.
name: Veksler, H.
name: Lahav, O.
name: Blumkin, A.
name: Moreno, C.
name: Gordon, C.
name: Steinhauer, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We present an in-situ study of an optical lattice with tunneling and single lattice site resolution. This system provides an important step for realizing a quantum computer. The real-space images show the fluctuations of the atom number in each site. The sub-Poissonian distribution results from the approach to the Mott insulator state, combined with the dynamics of density-dependent losses, which result from the high densities of optical lattice experiments. These losses are clear from the shape of the lattice profile. Furthermore, we find that the lattice is not in the ground state despite the momentum distribution which shows the reciprocal lattice. These effects may well be relevant for other optical lattice experiments, past and future. The lattice beams are derived from a microlens array, resulting in lattice beams which are perfectly stable relative to one another.
Additional file 1 of Past, present, and future of smart learning: a topic-based bibliometric analysis
Creators: name: Xieling Chen
name: Zou, Di
name: Haoran Xie
name: Wang, Fu Lee
Publisher: name: figshare
Year: 2021
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences
subject: Computer Software
subject: Information Systems

description: Additional file 1. Additional tables.
title: ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸Ñ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ÐµÐ²Ð°Ðº, ÐÐ°Ð´ÐµÐ¶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: ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸
Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÑÑÑÑÑ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«Ð¡Ð¸ÑÐ¸Ð¼Ð°ÐºÑÂ».
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ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
Creators: name: Rhee, Jinsu
name: Elahi, Pascal
name: Yi, Sukyoung K.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Cosmological simulations are useful tools for studying the evolution of galaxies, and it is critical to accurately identify galaxies and their halos from raw simulation data. The friends-of-friend (FoF) algorithm has been widely adopted for this purpose because of its simplicity and expandability to higher dimensions. However, it is cost-inefficient when applied to high-resolution simulations because standard FoF implementation leads to too many distance calculations in dense regions. We confirm this through our exercise of applying the 6-dimensional (6D) FoF galaxy finder code, VELOCIraptor (Elahi et al. 2019), on the NewHorizon simulation (Dubois et al. 2021). The high particle resolution of NewHorizon ($M_{\rm star} \sim 10^4 M_{\odot}$) allows a large central number density ($10^{6}\,{\rm kpc}^{-3}$) for typical galaxies, resulting in a few days to weeks of galaxy searches for just one snapshot. Even worse, we observed a significant decrease in the FoF performance in the high-dimensional 6D searches: "the curse of dimensionality" problem. To overcome these issues, we have developed several implementations that can be readily applied to any tree-based FoF code. They include limiting visits to tree nodes, re-ordering the list of particles for searching neighbor particles, and altering the tree structure. Compared to the run with the original code, the new run with these implementations results in the identical galaxy detection with the ideal performance, $O(N \log{N})$, $N$ being the number of particles in a galaxy -- with a speed gain of a factor of 2700 in 3D or 12 in 6D FoF search.
description: 24 pages, 16 figures, and 2 tables. Accepted for publication in ApJ
Additional file 2 of Developing a family-reported measure of experiences with home-based pediatric palliative and hospice care: a multi-method, multi-stakeholder approach
Creators: name: Boyden, Jackelyn Y.
name: Feudtner, Chris
name: Deatrick, Janet A.
name: Widger, Kimberley
name: LaRagione, Gwenn
name: Blyth Lord
name: Ersek, Mary
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2:. Demographic and Clinical Characteristics of Parent Participants and Their Children (Phase 4).
title: ÐÐ¿Ð¿Ð°ÑÐ°ÑÐ½ÑÐµ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ Ð²ÑÑÑÐ°Ð¸Ð²Ð°ÐµÐ¼ÑÑ ÑÐ¸ÑÑÐµÐ¼. ÐÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð°Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ½Ð°Ñ Ð±Ð°Ð·Ð°. ÐÐ¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÑ 1986BE92
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: ÐÐ¾Ð»Ð¾Ð´ÐµÐ·Ð½Ð¸ÐºÐ¾Ð², ÐÐ²Ð°Ð½
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2015
Subjects: ÐÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÐºÑÑÑÐ° Â«ÐÐ¿Ð¿Ð°ÑÐ°ÑÐ½ÑÐµ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ Ð²ÑÑÑÐ°Ð¸Ð²Ð°ÐµÐ¼ÑÑ ÑÐ¸ÑÑÐµÐ¼Â» Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Â«ÐÑÑÑÐ°Ð¸Ð²Ð°ÐµÐ¼ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÂ» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Â«ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ°Â».
Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÐºÑÐ°ÑÐºÐ¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÑ Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° Â«ÐÐ¸Ð»Ð°Ð½Ð´Ñ 1986ÐÐ92Â», ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¿Ð¾ Ð½Ð°ÑÑÑÐ¾Ð¹ÐºÐµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ ÑÑÐµÐ±Ð½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐµÐ´Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ IAR Embedded Workbench for ARM. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² 6-Ð³Ð¾ ÐºÑÑÑÐ° ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¡ÐÐ±ÐÐ£, Ð° ÑÐ°ÐºÐ¶Ðµ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ¾Ð², ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ¾Ð² Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ Ð¡Ð¾Ð²ÐµÑÐ° Ð¿Ð¾ Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð£ÑÐµÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾.
Coulomb interaction at the metal-insulator critical point in graphene
Creators: name: Juricic, Vladimir
name: Herbut, Igor F.
name: Semenoff, Gordon W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We compute the renormalization group flow of the long-ranged electron-electron interaction at the Gross-Neveu quantum critical point between the semimetal and the excitonic insulator in graphene, perturbatively in the small parameter $ε=d-1$, with $d$ as the spatial dimension. The $O(ε)$ correction to the usual beta-function makes the long-range interaction only more irrelevant at the critical than at the Gaussian fixed point. A weak long-range tail of the Coulomb interaction is found to be marginally irrelevant also in arbitrary dimension when the number of Dirac fermions is large. Its ultimate irrelevancy notwithstanding, it is shown that the metal-insulator transition may still be induced by increasing only the long-range tail of the Coulomb interaction.
description: 4 pages, 4 figures; published version
Light element abundances in carbon-enhanced metal-poor stars
Creators: name: Stancliffe, Richard J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We model the evolution of the abundances of light elements in carbon-enhanced metal-poor (CEMP) stars, under the assumption that such stars are formed by mass transfer in a binary system. We have modelled the accretion of material ejected by an asymptotic giant branch star on to the surface of a companion star. We then examine three different scenarios: one in which the material is mixed only by convective processes, one in which thermohaline mixing is present and a third in which both thermohaline mixing and gravitational settling are taken in to account. The results of these runs are compared to light element abundance measurements in CEMP stars (primarily CEMP-s stars, which are rich in $s$-processes elements and likely to have formed by mass transfer from an AGB star), focusing on the elements Li, F, Na and Mg. None of the elements is able to provide a conclusive picture of the extent of mixing of accreted material. We confirm that lithium can only be preserved if little mixing takes place. The bulk of the sodium observations suggest that accreted material is effectively mixed but there are also several highly Na and Mg-rich objects that can only be explained if the accreted material is unmixed. We suggest that the available sodium data may hint that extra mixing is taking place on the giant branch, though we caution that the data is sparse.
description: Accepted for publication in MNRAS. 9 figures, 1 table
Additional file 1 of Empowerment and health care access barriers among currently married women in Myanmar
Creators: name: Htun, Nang Mie Mie
name: Zar Lwin Hnin
name: Khaing, Win
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: Additional file 1. Women’s empowerment indicator factor component after factor analysis.
Superconductivity of electron-hole pairs in a bilayer graphene system in a quantizing magnetic field
Creators: name: Fil, D. V.
name: Kravchenko, L. Yu.
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: The state with a spontaneous interlayer phase coherence in a graphene based bilayer quantum Hall system is studied. This state can be considered as a gas of superfluid electron-hole pairs with the components of the pair belonging to different layers. Superfluid flux of such pairs is equivalent to two electrical supercurrents in the layers. It is shown that the state with the interlayer phase coherence emerges in the graphene system if a certain imbalance of the Landau level filling factors of the layers is created. We obtain the temperature of transition into the superfluid state, the maximum interlayer distance at which the phase coherence is possible, and the critical values of the supercurrent. The advantages of use of graphene systems instead of GaAs heterostructures for the realization of the bilayer electron-hole superconductivity is discussed.
description: 16 pages, 8 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÑÐ¸Ð·Ð¼Ð° Ð² ÐÐ¾Ð²Ð³Ð¾ÑÐ¾Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð¿Ð°ÑÐ¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð­ÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ
ÐÐ¾Ð²Ð³Ð¾ÑÐ¾Ð´ÑÐºÐ°Ñ Ð¾Ð±Ð»Ð°ÑÑÑ
ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÑÑÐ¸Ð·Ð¼
ÑÑÑÐ¸ÑÑÑÐºÐ¸Ð¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ
Ð¿ÑÐ¸ÑÐ¾Ð´Ð½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ
ÑÑÑÐ¸ÑÑÑÐºÐ°Ñ Ð¸Ð½ÑÑÐ°ÑÑÑÑÐºÑÑÑÐ°
ecologis
Novgorod region
ecological tourism
tourist base
natural complex
tourist infrastructure

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÑÐ¸Ð·Ð¼Ð° Ð² ÐÐ¾Ð²Ð³Ð¾ÑÐ¾Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ Ð±Ð°Ð·Ñ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÑÑÐ¸Ð·Ð¼Ð° Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð¿Ð¾ ÑÐµÐ¼Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð±ÑÐ» ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÑÑÐ¸ÑÑÑÐºÐ¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð´Ð»Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÑÐ¸ÑÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð±ÑÐ»Ð¾ Ð²ÑÐ´Ð²Ð¸Ð½ÑÑÐ¾ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¾ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹, ÐºÐ°ÑÐ°ÑÑÐ¸ÑÑÑ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ ÑÑÑÐ¸ÑÑÐ¾Ð² Ðº ÐÐ¾Ð²Ð³Ð¾ÑÐ¾Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. ÐÑÐ»Ð¸ Ð¿Ð¾ÑÑÐ¸ÑÐ°Ð½Ñ ÑÑÐ¾Ðº Ð¾ÐºÑÐ¿Ð°ÐµÐ¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¸ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð´Ð¾ÑÐ¾Ð´Ñ Ð¾Ð±Ð»Ð°ÑÑÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¾Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐºÐ»Ð°Ð¼Ñ Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÑÑÐ¾Ð².
description: Bachelor's thesis is devoted to the development of proposals on evolvement of ecological tourism in Novgorod state. The legal regulatory framework of the Russian Federation in the sphere of tourism law was analyzed and statistical analysis of the main indicators relating to the work was made. As a result there was developed a project of creation a tourist base for ecological tourists and there was created some proposals about attracting interest of the tourists to Novgorod region. There were counted terms of payback of this project and potential income of the region and besides that there were counted presumable results from implementation of advertising and from tour creation.
Photometric Variability of the T2.5 Brown Dwarf SIMP J013656.5+093347; Evidence for Evolving Weather Patterns
Creators: name: Artigau, Étienne
name: Bouchard, Sandie
name: Doyon, René
name: Lafrenière, David
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report the discovery of a photometric variability in the bright T2.5 brown dwarf SIMP J013656.5+093347. Continuous J-band photometry has been obtained for several hours on four different nights. The light curves show a periodic modulation with a period of ~2.4 hours, a peak-to-peak amplitude of ~50 mmag and significant night-to-night evolution. We suggest that the light curve modulation is due to the brown dwarf's rotation and that the longer term variations come from surface features evolution and/or differential rotation. We obtained complementary observations over a single night in the J and Ks bands; the object displays correlated photometric variability in both bands, albeit with smaller Ks-band amplitude. The ratio of the Ks and J variability amplitudes puts strong constraints on the physical mechanisms at play. Based on theoretical models of brown dwarf atmospheres, our results suggest that the atmosphere of SIMP0136 is comprised of both grain-free and colder (by ~100 K) grain-bearing cloudy regions. This discovery, and its interpretation, provide a natural explanation of the so-called J-band brightening.
description: Accepted for publication in ApJ. Modification in the replacement : One author missing in the astro-ph metadata
title: Автоматизация технологических процессов зерноперерабатывающих предприятий
Creators: name: ELS IPR BOOKS
Publisher: name: Донской государственный технический университет
Year: 2023

description: Изложены основы современных средств автоматизации технологических процессов в пищевой промышленности. Приведены практические примеры реализации технологических процессов с использованием современных средств автоматизации. Предназначено для обучающихся очной и заочной формы обучения по направлениям подготовки 12.03.02 Технологические машины и оборудование, 19.03.02 Продукты питания из растительного сырья, а также для специалистов, занимающихся вопросами промышленной автоматизации технологических процессов зерноперерабатывающих предприятий.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹
Creators: name: Ð¡ÐµÐ»ÑÑÐ¸Ð½Ð°, Ð.
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ñ", 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 (Ð ÐÐ¡ÐâÐ­â2018) (2018; 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: 2018

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÑÐµÑÐ° Ð¸ Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÐºÐ¾Ð² Ð² ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ðµ. ÐÐºÑÐµÐ½ÑÐ¸ÑÑÐµÑÑÑ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð°Ñ Ðº ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð² ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ðµ. Ð¡Ð´ÐµÐ»Ð°Ð½
ÑÑÐ´ Ð½Ð°ÑÑÐ½ÑÑ Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð¸Ð¹ Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð°Ð²ÑÐ¾ÑÑÐºÐ°Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ
ÑÐ¸ÑÐºÐ¾Ð² ÑÐ¿ÐµÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð´Ð»Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð½Ð° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÑ.
title: Amtliches Mitteilungsblatt der BTU Cottbus–Senftenberg, 2025,08 (31.03.2025)
Creators: name: (:Unav)
Publisher: name: BTU  Cottbus - Senftenberg
Year: 2025
Subjects: subject: 000 Informatik, Informationswissenschaft, allgemeine Werke

description: Vierte Änderungssatzung der Grundordnung für die Brandenburgische Technische Universität Cottbus–Senftenberg (GO BTU) vom 23. Januar 2025

Neuverkündung: Grundordnung für die Brandenburgische Technische Universität Cottbus–Senftenberg (GO BTU) vom 08. Januar 2016 (AMbl. 01/2016 vom 08. Januar 2016), zuletzt geändert durch die Vierte Änderungssatzung der Grundordnung für die Brandenburgische Technische Universität Cottbus–Senftenberg (GO BTU) vom 23. Januar 2025 (AMbl. 08/2025 vom 31.03.2025, Seite 3)
description: Amtliches Mitteilungsblatt der BTU Cottbus–Senftenberg; 2025, H. 08
Dynamical masses for two M1 + mid-M dwarf binaries monitored during the SPHERE-SHINE survey
Creators: name: Biller, Beth A.
name: Grandjean, Antoine
name: Messina, Sergio
name: Desidera, Silvano
name: Delorme, Philippe
name: Lagrange, Anne-Marie
name: Hambsch, Franz-Josef
name: Mesa, Dino
name: Janson, Markus
name: Gratton, Raffaele
name: D'Orazi, Valentina
name: Langlois, Maud
name: Maire, Anne-Lise
name: Schlieder, Joshua
name: Henning, Thomas
name: Zurlo, Alice
name: Hagelberg, Janis
name: Brown, S.
name: Romero, C.
name: Bonnefoy, Mickaël
name: Chauvin, Gael
name: Feldt, Markus
name: Meyer, Michael
name: Vigan, Arthur
name: Pavlov, A.
name: Soenke, C.
name: LeMignant, D.
name: Roux, A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present orbital fits and dynamical masses for HIP 113201AB and HIP 36985AB, two M1 + mid-M dwarf binary systems monitored as part of the SPHERE SHINE survey. To robustly determine ages via gyrochronology, we undertook a photometric monitoring campaign for HIP 113201 and for GJ 282AB, the two wide K star companions to HIP 36985, using the 40 cm Remote Observatory Atacama Desert (ROAD) telescope. We adopt ages of 1.2$\pm$0.1 Gyr for HIP 113201AB and 750$\pm$100 Myr for HIP 36985AB. To derive dynamical masses for all components of these systems, we used parallel-tempering Markov Chain Monte Carlo sampling to fit a combination of radial velocity, direct imaging, and Gaia and Hipparcos astrometry. Fitting the direct imaging and radial velocity data for HIP 113201 yields a primary mass of 0.54$\pm$0.03 M$_{\odot}$, fully consistent with its M1 spectral type, and a secondary mass of 0.145$\pm$ M$_{\odot}$. The secondary masses derived with and without including Hipparcos/Gaia data are more massive than the 0.1 M$_{\odot}$ estimated mass from the photometry of the companion. An undetected brown dwarf companion to HIP 113201B could be a natural explanation for this apparent discrepancy. At an age $>$1 Gyr, a 30 M$_{Jup}$ companion to HIP 113201B would make a negligible ($
description: accepted to A&A
title: ÐÑÐ·ÑÐºÐ°Ð»ÑÐ½Ð°Ñ ÐºÑÐ»ÑÑÑÑÐ° ÐÑÐµÐ²Ð½ÐµÐ³Ð¾ ÐÐ¸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Ð¾ÑÐ¾Ð²Ð¸Ð»Ð¾Ð², ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
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: Ð¼ÑÐ·ÑÐºÐ°Ð»ÑÐ½Ð°Ñ ÐºÑÐ»ÑÑÑÑÐ°
ÐÑÐµÐ²Ð½Ð¸Ð¹ ÐÐ¸ÑÐ°Ð¹
ÑÐ¿Ð¾Ñ Ð° Ð§Ð¶Ð¾Ñ
Ð¼ÑÐ·ÑÐºÐ°Ð»ÑÐ½ÑÐµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼ÑÐ·ÑÐºÐ°Ð»ÑÐ½Ð¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ Ð² ÑÐ¿Ð¾ÑÑ Ð§Ð¶Ð¾Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÑÐ¸Ð»Ð¾ÑÐ¾ÑÑÐºÐ¸Ñ ÑÐºÐ¾Ð» Ð½Ð° Ð¼ÑÐ·ÑÐºÐ°Ð»ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑÑ ÐÑÐµÐ²Ð½ÐµÐ³Ð¾ ÐÐ¸ÑÐ°Ñ, ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¼ÑÐ·ÑÐºÐ°Ð»ÑÐ½ÑÐµ Ð¶Ð°Ð½ÑÑ ÑÐ¾Ð³Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð¸, Ð²ÑÐ´ÐµÐ»ÐµÐ½Ð° ÑÐ¾Ð»Ñ Ð¼ÑÐ·ÑÐºÐ¸ Ð² Ð´ÑÐµÐ²Ð½ÐµÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¼ Ð¾Ð±ÑÐµÑÑÐ²Ðµ Ð¸ Ð¸Ð·ÑÑÐµÐ½Ñ Ð¼ÑÐ·ÑÐºÐ°Ð»ÑÐ½ÑÐµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ñ ÑÐ¾Ð»Ñ Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ð¸ ÐºÑÐ»ÑÑÑÑÑ ÐÐ¸ÑÐ°Ñ.
Measurement of CP violation observables and parameters for the decays $B^{\pm}\to D K^{*\pm}$
Creators: name: The BaBar Collaboration
name: Aubert, B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We study the decay $B^-\to DK^{*-}$ using a sample of 379$\times 10^6$ $Υ(4S)\to B\bar{B}$ events collected with the BABAR detector at the PEP-II $B$-factory. We perform a "GLW" analysis where the $D$ meson decays into either a CP-even ($CP+$) eigenstate ($K^+K^-$, $π^+π^-$), CP-odd ($CP-$) eigenstate ($K^0_Sπ^0$, $K^0_Sϕ$, $K^0_Sω$) or a non-CP state ($K^-π^+$). We also analyze $D$ meson decays into $K^+π^-$ from a Cabibbo-favored $\bar{D}^0$ decay or doubly suppressed $D^0$ decay ("ADS" analysis). We measure observables that are sensitive to the CKM angle $γ$: the partial-rate charge asymmetries ${\cal A}_{CP\pm}$, the ratios ${\cal R}_{CP\pm}$ of the B-decay branching fractions in $CP\pm$ and non-CP decay, the ratio ${\cal R}_{ADS}$ of the charge-averaged branching fractions, and the charge asymmetry ${\cal A}_{ADS}$ of the ADS decays: ${\cal A}_{CP+}= 0.09\pm0.13 \pm 0.06$, ${\cal A}_{CP-}=-0.23\pm 0.21\pm 0.07$, ${\cal R}_{CP+} =2.17 \pm 0.35 \pm 0.09$,${\cal R}_{CP-} =1.03\pm 0.27\pm 0.13$, ${\cal R}_{ADS}=0.066\pm0.031\pm0.010$, and ${\cal A}_{ADS}=-0.34\pm0.43\pm 0.16$, where the first uncertainty is statistical and the second is systematic. Combining all the measurements and using a frequentist approach yields the magnitude of the ratio between the Cabibbo-suppressed and favored amplitudes, $r_B$ = 0.31 with a one (two) sigma confidence level interval of [0.24, 0.38] ([0.17, 0.43]). The value $r_B=0$ is excluded at the 3.3 sigma level. A similar analysis excludes values of $γ$ in the intervals $[0, 7]^{\circ}, [55, 111]^{\circ}$, and $[175, 180]^{\circ}$ ([85, 99]$^{\circ}$) at the one (two) sigma confidence level.
description: 15 pages, 13 figures (.eps), to be submitted to PRD
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¢ÑÑÑÐ¸Ð¸ Ð¸ ÐÐÐ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¤ÑÐ°Ñ ÐÐºÐºÐ¾Ñ
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ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ
Ð¢ÑÑÑÐ¸Ñ
ÐÐÐ
Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸ÑÐ¼ Ð¼ÐµÐ¶Ð´Ñ Ð¢ÑÑÑÐ¸ÐµÐ¹ Ð¸ ÐÐÐ . Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ: Ð¸ÑÑÐ¾ÑÐ¸Ñ Ð½Ð°ÑÐ°Ð»Ð° Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÐ¶Ð´Ñ Ð´Ð²ÑÐ¼Ñ ÑÑÑÐ°Ð½Ð°Ð¼Ð¸, Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ, ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ðµ, ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð¾. Ð Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¢ÑÑÑÐ¸Ð¸ Ð¸ ÐÐÐ  Ð·Ð°ÑÑÐ¾Ð½ÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð²Ð¾ÐºÑÑÐ³ Ð¡Ð¸Ð½ÑÑÐ·ÑÐ½ â Ð£Ð¹Ð³ÑÑÑÐºÐ¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ°, ÐµÐ³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð½Ð° ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð¾. ÐÐ°Ð¼ÐµÑÐµÐ½Ñ Ð¿ÑÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð±ÑÐ´ÑÑÐ¸Ðµ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¢ÑÑÐµÑÐºÐ¾ â ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹.
Magnetic Quantum Wire as a Spin Filter: An Exact Study
Creators: name: Dey, Moumita
name: Maiti, Santanu K.
name: Karmakar, S. N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We propose that a magnetic quantum wire composed of magnetic and non-magnetic atomic sites can be used as a spin filter for a wide range of applied bias voltage. We adopt a simple tight-binding Hamiltonian to describe the model where the quantum wire is attached to two semi-infinite one-dimensional non-magnetic electrodes. Based on single particle Green's function formalism all the calculations are performed numerically which describe two-terminal conductance and current through the wire. Our exact results may be helpful in fabricating mesoscopic or nano-scale spin filter.
description: 6 pages, 5 figures