cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Lessons from Germany’s hard coal mining phase-out: policies and transition from 1950 to 2018
Creators: name: Oei, Pao-Yu
name: Brauers, Hanna
name: Herpich, Philipp
Publisher: name: Technische Universität Berlin
Year: 2019
Subjects: subject: 330 Wirtschaft
subject: coal phase-out
subject: Germany
subject: just transition
subject: structural policy
subject: transformation

description: German hard coal production ended in 2018, following the termination of subsidies. This paper looks at 60 years of continuous decline of an industry that employed more than 600,000 people, through a case study comparing Germany’s two largest hard coal mining areas (Ruhr area and Saarland). Although predominantly economic drivers underlay the transitions, both provide valuable lessons for upcoming coal phase-outs induced by stricter climate policies, including beyond Germany. The analysis identifies the main qualitative and quantitative characteristics of the two regions. It then discusses policy instruments implemented to guide the transition, including measures for the conservation of coal production, regional economic reorientation, and the easing of the transition’s social impacts. The success of these policies is evaluated using economic, social, and geographical indicators that were developed within three interdisciplinary research projects running from 2016 to 2019. A key lesson from the examined case studies is the importance of combining not only policies addressing unemployment and the attraction of new energy corporations and investments, but also measures improving infrastructure, education, research facilities and soft location factors. Protecting a declining industry for decades caused increased transition costs compared to an earlier phase-out. Economic reorientation and changing regional identities have proven most difficult in the past. However, the German example illustrates that the complexity of the challenges of a transition can be mastered if city, regional, and national governments and institutions cooperate in a polycentric approach.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸ÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡Ð¾ÐºÐ¾Ð»Ð¸ÑÑÐ½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ²Ð°Ð½Ð¾Ð², ÐÐ°ÐºÑÐ¸Ð¼
name: Ð¡Ð¾ÐºÐ¾Ð»Ð¸ÑÑÐ½Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2016
Subjects: Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐ¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸ÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ½Ð¾ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÐµÐ»Ð¸ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼ Ð¸ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ð¹ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ ÑÐ¸ÑÐ¼. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¾-Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸ÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼ Ð¸ Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑÑ Ð¿ÑÐ¸ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸Ð¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð¡ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¾-Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÑÑÑÑÐ¾Ð² Ð¼ÐµÐ¶Ð´Ñ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ°Ð¼Ð¸ ÐÐ§Ð-Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð². ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð²ÑÐ·Ð¾Ð², ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ñ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ¸ÑÐ¼, ÑÐ¸ÑÐ¾ÐºÐ¾Ð³Ð¾ ÐºÑÑÐ³Ð° ÑÐ¸ÑÐ°ÑÐµÐ»ÐµÐ¹, Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸ÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°Ð¼Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼.
P.Oxy. LXXXIV 5424. Apollonius Rhodius, Argonautica 3.1322–6 (Addendum to XXXIV 2699)
Creators: name: Oxyrhynchus Papyri
Publisher: name: University of Oxford
Year: 2022
Subjects: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
P.Oxy. LXXXIV 5425. Apollonius Rhodius, Argonautica 4.232–42, 269–80
Creators: name: Oxyrhynchus Papyri
Publisher: name: University of Oxford
Year: 2022
Subjects: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
P.Oxy. LXXXIV 5426. Apollonius Rhodius, Argonautica 4.504–19 (Addendum to XXXIV 2691)
Creators: name: Oxyrhynchus Papyri
Publisher: name: University of Oxford
Year: 2022
Subjects: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
P.Oxy. LXXXIV 5427. Apollonius Rhodius, Argonautica 4.877–85, 917–23
Creators: name: Oxyrhynchus Papyri
Publisher: name: University of Oxford
Year: 2022
Subjects: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
Applying automotive industry materials and manufacturing processes in the aerospace industry in order to reduce cost
Creators: name: Aliage Maraver, Luis
name: Egurrola, Dr. José Javier
name: Castillo Acero, Miguel Á.
Publisher: name: Zenodo
Year: 2020
Subjects: advanced rear end
CRFP
Clean Sky 2 Joint Undertaking
European Union (EU)
Horizon 2020
HLFC
Thermostamping
Compression moulding

description: This presentation describes the technological transfer between automotive and aeronautical sectors. This project has received funding from the Clean Sky 2 Joint Undertaking (JU) under grant agreement No 945583. The JU receives support from the European Union’s Horizon 2020 research and innovation programme and the Clean Sky 2 JU members other than the Union. The results, opinions, conclusions, etc. presented in this work are those of the author(s) only and do not necessarily represent the position of the JU; the JU is not responsible for any use made of the information contained herein.
Measurements of Secondary Cosmic Microwave Background Anisotropies with the South Pole Telescope
Creators: name: Lueker, M.
name: Reichardt, C. L.
name: Schaffer, K. K.
name: Zahn, O.
name: Ade, P. A. R.
name: Aird, K. A.
name: Benson, B. A.
name: Bleem, L. E.
name: Carlstrom, J. E.
name: Chang, C. L.
name: Cho, H. M.
name: Crawford, T. M.
name: Crites, A. T.
name: de Haan, T.
name: Dobbs, M. A.
name: George, E. M.
name: Hall, N. R.
name: Halverson, N. W.
name: Holder, G. P.
name: Holzapfel, W. L.
name: Hrubes, J. D.
name: Joy, M.
name: Keisler, R.
name: Knox, L.
name: Lee, A. T.
name: Leitch, E. M.
name: McMahon, J. J.
name: Mehl, J.
name: Meyer, S. S.
name: Mohr, J. J.
name: Montroy, T. E.
name: Padin, S.
name: Plagge, T.
name: Pryke, C.
name: Ruhl, J. E.
name: Shaw, L.
name: Shirokoff, E.
name: Spieler, H. G.
name: Staniszewski, Z.
name: Stark, A. A.
name: Vanderlinde, K.
name: Vieira, J. D.
name: Williamson, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We report cosmic microwave background (CMB) power spectrum measurements from the first 100 sq. deg. field observed by the South Pole Telescope (SPT) at 150 and 220 GHz. On angular scales where the primary CMB anisotropy is dominant, ell ~< 3000, the SPT power spectrum is consistent with the standard LambdaCDM cosmology. On smaller scales, we see strong evidence for a point source contribution, consistent with a population of dusty, star-forming galaxies. After we mask bright point sources, anisotropy power on angular scales of 3000 < ell < 9500 is detected with a signal-to-noise > 50 at both frequencies. We combine the 150 and 220 GHz data to remove the majority of the point source power, and use the point source subtracted spectrum to detect Sunyaev-Zel'dovich (SZ) power at 2.6 sigma. At ell=3000, the SZ power in the subtracted bandpowers is 4.2 +/- 1.5 uK^2, which is significantly lower than the power predicted by a fiducial model using WMAP5 cosmological parameters. This discrepancy may suggest that contemporary galaxy cluster models overestimate the thermal pressure of intracluster gas. Alternatively, this result can be interpreted as evidence for lower values of sigma8. When combined with an estimate of the kinetic SZ contribution, the measured SZ amplitude shifts sigma8 from the primary CMB anisotropy derived constraint of 0.794 +/- 0.028 down to 0.773 +/- 0.025. The uncertainty in the constraint on sigma8 from this analysis is dominated by uncertainties in the theoretical modeling required to predict the amplitude of the SZ power spectrum for a given set of cosmological parameters.
description: 28 pages, 11 figures, submitted to ApJ
Anomaly of non-Abelian discrete symmetries
Creators: name: Kobayashi, Tatsuo
name: Uchida, Hikaru
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study anomalies of non-Abelian discrete symmetries; which part of non-Abelian group is anomaly free and which part can be anomalous. It is found that the anomaly-free elements of the group $G$ generate a normal subgroup $G_0$ of $G$ and the residue class group $G/G_0$, which becomes the anomalous part of $G$, is isomorphic to a single cyclic group. The derived subgroup $D(G)$ of $G$ is useful to study the anomaly structure. This structure also constrains the structure of the anomaly-free subgroup; the derived subgroup $D(G)$ should be included in the anomaly-free subgroup. We study the detail structure of the anomaly-free subgroup from the structure of the derived subgroup in various discrete groups. For example, when $G=S_n \simeq A_n \rtimes Z_2$ and $G=Δ(6n^2) \simeq Δ(3n^2) \rtimes Z_2$, in particular, $A_n$ and $Δ(3n^2)$ are at least included in the anomaly-free subgroup, respectively. This result holds in any arbitrary representations.
description: 25 pages, 1 figure
Dynamics of lane formation in driven binary complex plasmas
Creators: name: Sütterlin, K. R.
name: Wysocki, A.
name: Ivlev, A. V.
name: Räth, C.
name: Thomas, H. M.
name: Rubin-Zuzic, M.
name: Goedheer, W. J.
name: Fortov, V. E.
name: Lipaev, A. M.
name: Molotkov, V. I.
name: Petrov, O. F.
name: Morfill, G. E.
name: Löwen, H.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The dynamical onset of lane formation is studied in experiments with binary complex plasmas under microgravity conditions. Small microparticles are driven and penetrate into a cloud of big particles, revealing a strong tendency towards lane formation. The observed time-resolved lane formation process is in good agreement with computer simulations of a binary Yukawa model with Langevin dynamics. The laning is quantified in terms of the anisotropic scaling index, leading to a universal order parameter for driven systems.
description: 4 pages, 3 figures, movies available at http://www.mpe.mpg.de/pke/lane-formation/
Inhomogeneous structure formation may alleviate need for accelerating universe
Creators: name: Hansson, Johan
name: Lindkvist, Jesper
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: When taking the real, inhomogeneous and anisotropic matter distribution in the semi-local universe into account, there may be no need to postulate an accelerating expansion of the universe despite recent type Ia supernova data. Local curvatures must be integrated (over all space) to obtain the global curvature of the universe, which seems to be very close to zero from cosmic microwave background data. As gravitational structure formation creates bound regions of positive curvature, the regions in between become negatively curved in order to comply with a vanishing global curvature. The actual dynamics of the universe is altered due to the self-induced inhomogeneities, again more prominently so as structure formation progresses. Furthermore, this negative curvature will increase as a function of time as structure formation proceeds, which mimics the effect of "dark energy" with negative pressure. Hence, the "acceleration" may be merely a mirage. We make a qualitative and semi-quantitative analysis, using newtonian gravity corrected for special relativistic effects, which works surprisingly well, to corroborate and illustrate/visualize these statements. This article may be seen as a plea to start taking seriously the observed inhomogeneous distribution and the nonlinearities of nonperturbative general relativity, and their impact on the dynamics and behavior of the cosmos.
A graphene inspired electromagnetic superlens
Creators: name: Lannebère, Sylvain
name: Silveirinha, Mário G.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Optics (physics.optics)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In this paper we propose a new paradigm to create superlenses inspired by n-p-n junctions of graphene. We show that by adjoining a n-type region and a p-type region with a crystal dislocation, it is possible to mimic the interaction of complementary Hamiltonians and achieve subwavelength imaging. We introduce an effective model of the system, and show that it predicts perfect lensing for both propagating and evanescent waves due to the excitation of a resonant mode at the interface between each region. This phenomenon is the consequence of a nontrivial boundary condition at the n-p interfaces due to a dislocation of the graphene "atoms". We discuss practical realizations of such superlenses in electronic and photonic platforms. Using full wave simulations, we study in detail the performance of a photonic realization of the lens based on a honeycomb array of dielectric cylinders embedded in a metal.
description: 6 figures
Lepton-Flavor-Violating tau decays at BaBar
Creators: name: Marchiori, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present the most recent searches for lepton-flavor-violating tau decays in BaBar. We find no evidence of tau decaying to three charged leptons or to a charged lepton and a neutral meson (KS, rho, phi, K*0, anti-K*0), and set upper limits on the corresponding branching fractions between 1.8 and 19 times 10-8 at 90% confidence level.
description: 4 pages, 2 figures. To appear in the SUSY09 conference proceedings
Medieval Treasures from Hildesheim
Creators: name: Kruppa, Nathalie
Publisher: name: Concilium medii aevi
Year: 2020

description: Rezension zu: Medieval Treasures from Hildesheim, hg. von Peter Barnet, Michael Brandt und Gerhard Lutz, The Metropolitan Museum of Art, New York, New Haven, Conn., und London, Yale University Press, 2013, S. 148, Abb. 115, ISBN: 978-0-300-19699-3
description: Concilium medii aevi, Bd. 17 (2014): Concilium medii aevi
„Dietrich Engelhus, eine geschichtliche Quellenforschung“. Über die ungedruckte Habilitationsschrift Karl Lamprechts in der Universitäts- und Landesbibliothek Bonn
Creators: name: Kümper, Hiram
Publisher: name: Concilium medii aevi
Year: 2020

description: Concilium medii aevi, Bd. 17 (2014): Concilium medii aevi
Julia Barrow, The Clergy in the Medieval World. Secular Clerics, Their Families and Careers in North-Western Europe, c. 800–c. 1200
Creators: name: Berger, Daniel
Publisher: name: Concilium medii aevi
Year: 2020

description: Rezension zu: Julia Barrow, The Clergy in the Medieval World. Secular Clerics, Their Families and Careers in North-Western Europe, c. 800–c. 1200, Cambridge, University Press, 2015, XXI–447 S., 3 Karten, £ 65,00. ISBN 978-1-107-08638-8.
description: Concilium medii aevi, Bd. 19 (2016): Concilium medii aevi
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ "ÐÐ°ÑÐ°Ð±Ð°Ð½"
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°ÑÐ¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð±Ð°ÑÐ°Ð±Ð°Ð½
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ
ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ: ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ½Ð°ÑÑÐºÐ¸ Ð´Ð»Ñ ÑÐ¾Ð»Ð¾Ð´Ð½Ð¾Ð¹ Ð¾Ð±ÑÐµÐ¼Ð½Ð¾Ð¹ ÑÑÐ°Ð¼Ð¿Ð¾Ð²ÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ "ÐÐ°ÑÐ°Ð±Ð°Ð½". Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ°ÑÐ°Ð±Ð°Ð½Â» Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð³Ð¾ÑÑÑÐµÐ¹ Ð¾Ð±ÑÐµÐ¼Ð½Ð¾Ð¹ ÑÑÐ°Ð¼Ð¿Ð¾Ð²ÐºÐ¸. Ð¡Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð²ÑÐµ Ð¿ÐµÑÐµÑÐ¾Ð´Ñ ÑÑÐ°Ð¼Ð¿Ð¾Ð²ÐºÐ¸ Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµ DeForm. Ð¡Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÑÐ°Ð¼Ð¿Ð¾Ð²Ð°Ñ Ð¾ÑÐ½Ð°ÑÑÐºÐ°. ÐÑÐ±ÑÐ°Ð½Ð¾ Ð¿Ð¾ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÑ Ð¿Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÑÑÐµÑÑÐ°Ð¼Ð¸ Ð¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ½ÑÐ¼Ð¸ ÑÐ¸ÑÑÐ°ÑÐ¸ÑÐ¼Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÑÑÐ»ÑÐ³ Ð³Ð¾ÑÑÐµÐ¿ÑÐ¸Ð¸Ð¼ÑÑÐ²Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ½ÑÐ·ÑÐºÐ¾Ð²Ð°, ÐÐ¸ÑÐ¾ÑÐ»Ð°Ð²Ð°
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ÐµÑÑ
Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°Ð·ÑÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð²
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description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð¸ Ð²Ð½ÐµÐ´ÑÐ¸ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°Ð·ÑÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð² Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐµÑÑ ÑÑÐ»ÑÐ³ ÐÐÐ Â«Ð¤Ð°Ð²Ð¾ÑÐ¸ÑÂ». ÐÐ½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð² Ð² ÐÐÐ Â«Ð¤Ð°Ð²Ð¾ÑÐ¸ÑÂ» Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð» Ð²ÑÑÐ²Ð¸ÑÑ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ ÑÑÑÐµÑÑÐ¾Ð²ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹ Ð² ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð²Ðµ. Ð­ÑÐ¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ (Ð² Ð²Ð¸Ð´Ñ ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð¸Ñ ÑÑÐ°ÑÐ° ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¸ Ð²ÐµÐ´ÑÑ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÑ Ð±Ð¾ÑÑÐ±Ñ Ð·Ð° Ð´Ð¾Ð»Ð¶Ð½Ð¾ÑÑÑ, ÑÑÐ¾ Ð¿ÑÐ¾Ð²Ð¾ÑÐ¸ÑÑÐµÑ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÑ Ð¼ÐµÐ¶Ð´Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ°Ð¼Ð¸). Ð­ÑÐ¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ (ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð·Ð°ÑÐ°Ð±Ð¾ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿Ð¾ÑÐµÑÐ¸ Ð¸Ð·-Ð·Ð° Ð¾ÑÐ¸Ð±Ð¾Ðº ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐºÐ°Ð·ÑÐ²Ð°ÑÑÐ¸ÐµÑÑ Ð½Ð° ÑÑÑÐµÑÑÐ¾ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ ÐÐÐ Â«Ð¤Ð°Ð²Ð¾ÑÐ¸ÑÂ»). Ð¡Ð¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ (Ð¿ÑÐ¸Ð´Ð¸ÑÑÐ¸Ð²Ð¾ÑÑÑ Ð¸ Ð½ÐµÐ´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²Ð¾ ÑÐ°Ð±Ð¾ÑÐ¾Ð¹ ÐºÐ¾Ð»Ð»ÐµÐ³ Ð²Ð²Ð¸Ð´Ñ Ð²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ½Ð¾ÑÑÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°). ÐÑÑÐ°ÑÐ»ÐµÐ²ÑÐµ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ (Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ Ð¾Ñ ÑÐ¸ÐºÐ»Ð¸ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ¾ÑÐ° Ð½Ð° ÑÑÐ»ÑÐ³Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ). Ð¡ ÑÐµÐ»ÑÑ Ð¿ÑÐ¾ÑÐ¸Ð»Ð°ÐºÑÐ¸ÐºÐ¸ ÑÑÑÐµÑÑÐ¾Ð² Ð¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð² Ð½Ð° ÑÑÐ¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¾ ÑÐ»ÐµÐ´ÑÑÑÐµÐµ: Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ ÑÑÐµÐ½Ð¸Ð½Ð³Ð¸ (Ð¸Ð³ÑÑ) Ð½Ð° ÑÐ¿Ð»Ð¾ÑÐµÐ½Ð¸Ðµ ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð²Ð°; Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑ ÑÐ°Ð±Ð¾ÑÑ Ñ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð³ÐµÐ½Ð½ÑÐ¼Ð¸ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ°Ð¼Ð¸; Ð²Ð½ÐµÐ´ÑÐ¸ÑÑ Ð½Ð¾ÑÐ¼Ñ ÑÑÐ¸ÐºÐ¸ Ð² ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð²Ðµ; Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑ ÑÐ°ÑÑÑÐ°Ð½Ð¾Ð²ÐºÑ ÐºÐ°Ð´ÑÐ¾Ð² Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¸ÑÐ¾ÑÐ¸Ð¿Ð° ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ°; Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ ÑÐ¼Ð¾Ñ Ð´Ð»Ñ ÑÐ³Ð»Ð°Ð¶Ð¸Ð²Ð°Ð½Ð¸Ñ Ð½ÐµÐ·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½ÑÑ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð². ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑ ÑÐ»ÑÑÑÐ¸ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð² ÑÐµÐ»Ð¾Ð¼.
title: Ð­ÐºÑÐ¿ÐµÑÑÐ½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°, Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÐ°Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¸Ð½ÑÐµÑÑÐµÑÐ¾Ð¼ÐµÑÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐ°ÐµÐ², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¸Ð½ÑÐµÑÑÐµÑÐ¾Ð¼ÐµÑÑÑ
ÑÐºÑÐ¿ÐµÑÑÐ½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°
Ð»ÐµÐ³ÐºÐ¾Ð³Ð°Ð·Ð¾Ð²Ð°Ñ Ð¼ÐµÑÐ°ÑÐµÐ»ÑÐ½Ð°Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°
Ð²ÑÑÐ¾ÐºÐ¾ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾Ðµ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ðµ

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÐµ Ñ ÑÐµÐ»ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², Ð¿Ð¾Ð´Ð²ÐµÑÐ³Ð½ÑÑÑÑ ÑÐ´Ð°ÑÐ½Ð¾Ð¼Ñ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ñ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹ Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° ÑÐµÑÐ¸Ñ Ð¾Ð¿ÑÑÐ¾Ð² Ñ Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸ÐµÐ²ÑÐ¼ ÑÐ¿Ð»Ð°Ð²Ð¾Ð¼ Ð16. ÐÐ»Ñ ÑÐµÐ³Ð¸ÑÑÑÐ°ÑÐ¸Ð¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐ´Ð°ÑÐ½ÑÑ Ð²Ð¾Ð»Ð½ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»ÑÑ Ð´Ð²ÑÑÐºÐ°Ð½Ð°Ð»ÑÐ½ÑÐ¹ Ð»Ð°Ð·ÐµÑÐ½ÑÐ¹ Ð¸Ð½ÑÐµÑÑÐµÑÐ¾Ð¼ÐµÑÑ. Ð¤Ð¸Ð»ÑÑÑÐ°ÑÐ¸Ñ Ð¸ ÑÐ°ÑÑÐ¸ÑÑÐ¾Ð²ÐºÐ° Ð¸Ð½ÑÐµÑÑÐµÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐ»Ð°ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾. ÐÐ»Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð±ÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐºÑÐ¿ÐµÑÑÐ½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°, ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ ÑÐºÐ¾ÑÐ¾ÑÑÐ¸ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð¹ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°, Ð¿Ð¾Ð´Ð²ÐµÑÐ³Ð½ÑÑÐ¾Ð³Ð¾ Ð½Ð°Ð³ÑÑÐ·ÐºÐ°Ð¼, Ð¸ Ð´ÑÑÐ³Ð¸Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº.
Generalised constraints on the curvature perturbation from primordial black holes
Creators: name: Josan, Amandeep S.
name: Green, Anne M.
name: Malik, Karim A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Primordial black holes (PBHs) can form in the early Universe via the collapse of large density perturbations. There are tight constraints on the abundance of PBHs formed due to their gravitational effects and the consequences of their evaporation. These abundance constraints can be used to constrain the primordial power spectrum, and hence models of inflation, on scales far smaller than those probed by cosmological observations. We compile, and where relevant update, the constraints on the abundance of PBHs before calculating the constraints on the curvature perturbation, taking into account the growth of density perturbations prior to horizon entry. We consider two simple parameterizations of the curvature perturbation spectrum on the scale of interest: constant and power-law. The constraints from PBHs on the amplitude of the power spectrum are typically in the range 10^{-2}-10^{-1} with some scale dependence.
description: 10 pages, 2 figures, version to appear in Phys. Rev. D with minor change to calculation of constraints for spectral index not equal to one
title: Ð Ð¸ÑÐºÐ¸ Ð½Ð¸Ð·ÐºÐ¾Ð³Ð¾ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±Ð°Ð·Ñ "Ð½ÑÐ»ÐµÐ²Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»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° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¾Ð±Ð¸Ð½Ð°, ÐÐ°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: Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ
Ð·ÐµÐ¼ÐµÐ»ÑÐ½ÑÐµ ÑÑÐ°ÑÑÐºÐ¸
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description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð²Ð¾Ð¿ÑÐ¾Ñ, Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐ¹ Ð´Ð»Ñ Ð³Ð¾ÑÐ¾Ð´Ð¾Ð² Ñ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð·Ð°ÑÑÑÐ¾Ð¹ÐºÐ¾Ð¹ â Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ Ð²ÑÑÐ²Ð»ÑÐµÐ¼ÑÑ Ð½Ð° ÑÑÐ°Ð¿Ðµ Ð½ÑÐ»ÐµÐ²Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° ÐÐ¡Ð ÑÐ¸ÑÐºÐ¾Ð², ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸ÑÐ¼Ð¸ (Ð¾Ð±ÑÐµÐ¼ÐµÐ½ÐµÐ½Ð¸ÑÐ¼Ð¸) Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ Ðº Ð·Ð°ÑÑÑÐ¾Ð¹ÐºÐµ Ð·ÐµÐ¼ÐµÐ»ÑÐ½ÑÑ ÑÑÐ°ÑÑÐºÐ¾Ð². ÐÐ»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð²Ð¾Ð¿ÑÐ¾ÑÐ° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð² Ð²Ð¸Ð´Ðµ Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð¹ ÐºÐ°ÑÑÑ Ð¿Ð¾ Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÐºÐ¾Ð² Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¿Ð¾ÑÐµÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ° Ð¿ÑÐ¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ð¸ Ð² Ð³ÑÑÐ½ÑÐµ Ð¾ÑÐ²Ð°Ð¸Ð²Ð°ÐµÐ¼Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ° ÑÐ°Ð½ÐµÐµ Ð½ÐµÐ¸Ð·Ð²ÐµÑÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°-Ð¾Ð±ÑÐµÐ¼ÐµÐ½ÐµÐ½Ð¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð°ÑÑÐµÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°ÑÐ¾Ð´Ð¾Ðº). ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ (Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð¹ ÐºÐ°ÑÑÑ) Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð² Ð²Ð¸Ð´Ðµ Ð¿ÑÐ¸Ð¼ÐµÑÐ° ÑÐ°ÑÑÐµÑÐ¾Ð² Ð´ÐµÐ½ÐµÐ¶Ð½ÑÑ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð² Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÐºÐ°Ð»ÐµÐ½Ð´Ð°ÑÐ½ÑÑ Ð³ÑÐ°ÑÐ¸ÐºÐ¾Ð² Ð´Ð»Ñ ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð³Ð¾ ÐÐ¡Ð.
title: Effect of Oxygen Environment on Soot Characteristics in Ethylene Laminar Diffusion Flames
Creators: name: Zeng, D.
name: Xiong, G.
name: Wang, Y.
name: International Seminar On Fire And Explosion Hazards (9; 2019; Saint Petersburg, Russia)
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: 2019

description: Radiative characteristics and soot distribution of laminar diffusion flame of ethylene is studied
experimentally over a wide range of oxygen index (OI) (from 13.3% to 20.9%) and fuel flow rates. The
flame is established on a circular burner surrounded by the coflows of various oxygen concentrations. The
effect of OI on flame at smoke-point is investigated. When the OI decreases, the smoke-point flame flow
rate reduces but the flame length first increases then decreases. The radiant profile along the flame height
shows the radiant power shifts to a larger height with increased OI, and the flame radiant fraction reduces.
Furthermore, it is found that the radiant fraction of laminar diffusion flame linearly correlates with those
of buoyant turbulent flames at the same adiabatic flame temperature. The soot volume fraction of flames
of different flow rates under several oxygen concentrations is measured using the laser-induced
incandescence (LII) technique. The soot volume fraction distribution shows that the lower OI condition
has a smaller soot formation rate. Moreover, as OI reduces, the position for maximum soot volume
fraction shifts towards the centerline region at a larger flame height. Compared to the laminar diffusion
flames with fuel diluted with nitrogen, the flame with oxidizer diluted has a lower activation energy of
127 kJ/mol of the soot formation reaction.
Patrizia Carmassi (Bearb.), Katalog der mittelalterlichen und frühneuzeitlichen Handschriften in Halberstadt
Creators: name: Popp, Christian
Publisher: name: Concilium medii aevi
Year: 2020

description: Rezension zu: Patrizia Carmassi (Bearb.), Katalog der mittelalterlichen und frühneuzeitlichen Handschriften in Halberstadt. Verzeichnis der Bestände der Kulturstiftung Sachsen-Anhalt, Domschatz zu Halberstadt, und des Historischen Archivs der Stadt Halberstadt, Harrassowitz Verlag, Wiesbaden 2018, ISBN 978-3-447-10981-9, 333 Seiten
description: Concilium medii aevi, Bd. 22 (2019): Concilium medii aevi
Predictors of intraparenchymal hemorrhage progression and markers of injury severity on magnetic resonance imaging following acute cervical spinal cord injury
Creators: name: Malomo, Toluyemi Adefolarin
Publisher: name: University of British Columbia
Year: 2025

description: Background: Prior to the release of the 2024 management guidelines for spinal cord injury (SCI), previous guidelines suggested augmenting the systemic mean arterial pressure (MAP) to a target of 85-90mmHg for the first 7 days after injury. Although this may improve blood flow to the injured cord and reduce ischemia, it could cause an inadvertent increase in intraparenchymal hemorrhage (IPH). This study aims to assess the impact of MAP augmentation and venous thromboembolism (VTE) prophylaxis on IPH progression after acute human SCI. Methods: In SCI patients, Norepinephrine alone or in conjunction with Vasopressin was used to keep MAP between 85-90 mmHg. Magnetic Resonance Imaging (MRI) was done on admission (within 24 hours post-SCI) and on days 2, 4, 7, and 14 post-injury. Hemorrhage was quantified on T2-weighted MRI scans. Hemorrhage progression (Delta IPH or ΔIPH) was determined by calculating the difference between the hemorrhage volume on the baseline MRI and at other time points. The cumulative MAP exposure is the Time-Weighted Average MAP (TWA-MAP), which was calculated by dividing the area under the curve of the MAP measurements by the total hours of exposure. Regression (simple and multivariate) and linear mixed effect model analysis were used to explore the relationship between Delta IPH and TWA-MAP and the factors influencing hemorrhage progression after SCI. Results: Data from 13 patients were analyzed. While IPH progressively increased on days 2 and 4, it decreased from day 7. TWA-MAP was significantly associated with Delta IPH p=<0.0001 during the first two days following SCI. The baseline IPH was the most significant predictor of hemorrhage progression from the time of injury to days 2 and 4 post-trauma. From days 2 to 4 post-trauma, TWA-MAP was the most important predictor of hemorrhage progression. The time to initiation of VTE and Norepinephrine dose did not affect hemorrhage progression. Conclusions: There is a positive correlation between MAP exposure and hemorrhage progression after SCI, more evident with severe IPH at baseline. Hence, harmful bleeding within the spinal cord may be a contributing factor to the difficulty of establishing the effectiveness of maintaining MAP above 85 mmHg for neurological recovery.
Empirical analysis of the solar contribution to global mean air surface temperature change
Creators: name: Scafetta, Nicola
Publisher: name: arXiv
Year: 2009
Subjects: subject: Geophysics (physics.geo-ph)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: The solar contribution to global mean air surface temperature change is analyzed by using an empirical bi-scale climate model characterized by both fast and slow characteristic time responses to solar forcing: $τ_1 =0.4 \pm 0.1$ yr, and $τ_2= 8 \pm 2$ yr or $τ_2=12 \pm 3$ yr. Since 1980 the solar contribution to climate change is uncertain because of the severe uncertainty of the total solar irradiance satellite composites. The sun may have caused from a slight cooling, if PMOD TSI composite is used, to a significant warming (up to 65% of the total observed warming) if ACRIM, or other TSI composites are used. The model is calibrated only on the empirical 11-year solar cycle signature on the instrumental global surface temperature since 1980. The model reconstructs the major temperature patterns covering 400 years of solar induced temperature changes, as shown in recent paleoclimate global temperature records.
description: 9 pages, 6 figures
title: ÐÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼Ð¸ÐºÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 05.04.12 "Ð¢ÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÑÑÐ±Ð¾ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸"
titleType: Subtitle
Creators: name: ÐÐµÑÐµÐ´Ð¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
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: 2021
Subjects: Ð¢ÑÑÐ±Ð¸Ð½Ð½ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð¸ÐºÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº. ÐÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÐ¸Ð¿Ð¾Ð² ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð¹ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ ÑÑÐµÐ¼,Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÑÑÑÐºÑÑÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð², ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¼Ð¸ÐºÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð½ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð¸ÐºÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº.
Competition between Ta-Ta and Te-Te bonding leading to the commensurate charge density wave in TaTe4
Creators: name: Guster, Bogdan
name: Pruneda, Miguel
name: Ordejón, Pablo
name: Canadell, Enric
Publisher: name: arXiv
Year: 2021
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The origin of the charge density wave in TaTe$_4$ is discussed on the basis of a first-principles DFT analysis of the Fermi surface, electron-hole response function, phonon band structure of the average structure and structural optimization of the modulated phase. Analysis of the band structure and Fermi surface of the average structure clearly proves that despite the presence of TaTe$_4$ chains in the crystal structure, TaTe$_4$ is in fact a 3D material as far as the electronic structure near the Fermi level is concerned. A Fermi surface nesting mechanism is dismissed as the origin of the 2$a\times2a\times3c$ structural modulation. The optimized 2$a$\xone2$a$\xone3$c$ structure, which is found to be the more stable modulation in agreement with the experimental observations, can be obtained directly from a soft-phonon mode computed for the undistorted structure. Our results suggest that the driving force for the distortion is the maximization of Ta-Ta metal-metal bonding subject to inducing the minimum bonding decrease in the Te sublattice.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÑÐµÐ´Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð¸ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑÑ ÐÐÐ Â«ÐÐÐÐÐÐ-Ð­ÐÐÐ ÐÐÐ¢ÐÐÐÂ»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÐºÐ¾Ð²Ð°, ÐÐ½Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ°Ñ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑ
ÐºÑÐµÐ´Ð¸ÑÐ¾ÑÑÐºÐ°Ñ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑ
Ð¾Ð±Ð¾ÑÐ°ÑÐ¸Ð²Ð°ÐµÐ¼Ð¾ÑÑÑ
accounts receivable
accounts payable
turnover

description: ÐÐ°Ð½Ð½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÑÐµÐ´Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð¸ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÐÐÐÐÐ-Ð­ÐÐÐ ÐÐÐ¢ÐÐÐÂ». Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ ÐµÐ³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¾ÑÐ°Ñ Ð³Ð»Ð°Ð²Ð° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð°ÑÐ¿ÐµÐºÑÐ°Ð¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÑÐµÐ´Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð¸ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑÑ. Ð Ð½ÐµÐ¹ ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑÑÑ ÑÑÑÐ½Ð¾ÑÑÑ Ð´Ð°Ð½Ð½ÑÑ ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¹, Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ, Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ ÑÑÐµÑÐ°. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ³Ð»ÑÐ±Ð»ÐµÐ½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð¸ ÐºÑÐµÐ´Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÑÐ¾ÑÐ¼Ð¸ÑÑÑÑÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð¼Ð¸ Ð¸ ÑÐ°ÑÑÑÐ¸ÑÑÐ²Ð°ÐµÑÑÑ ÑÑÑÐµÐºÑ Ð¾Ñ Ð¸Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ.
description: This research focuses on the formation of proposals on improvement of payables and receivables management system in the JSC Â«ZVEZDA-ENERGETIKAÂ». In the first chapter analyzed the organizational structure of the enterprise and its financial and economic activity. The second chapter is devoted to the theoretical aspects of accounts receivable management. It reveals the essence of these categories, a classification, methods of analysis and accounting.The third chapter is carried out in-depth analysis of the receivables and payables of the investigated companies formed measures to improve the management system and their calculated effect of their implementation.
Zoomorphe Stadtpläne? Der Löwe von Königslutter, das Pferd von Heiligenstadt und verwandte Anlagen des hohen Mittelalters. Neue Thesen zur Siedlungsentwicklung
Creators: name: Küntzel, Thomas
Publisher: name: Concilium medii aevi
Year: 2020

description: Concilium medii aevi, Bd. 22 (2019): Concilium medii aevi
title: Ð¡Ð¸ÑÑÐµÐ¼Ð° PR-ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ½ÑÐµÐºÐ¾Â»)
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°ÑÑÑÑÐ½Ð¾Ð²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´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: PR-ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ
ÑÐ¸ÑÑÐµÐ¼Ð°
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¸Ñ
PR-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ Ð¾Ð¿ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¸Ð¸. ÐÐ²ÑÐ¾ÑÐ¾Ð¼ ÑÐ°ÑÐºÑÑÑÐ° ÑÑÑÐ½Ð¾ÑÑÑ PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¼ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÑÐ½ÐºÐµ Ð¸ Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ PR-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÐ¼ÑÐµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐ¼Ð¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸ÑÐ¼Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· PR-ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐ½ÑÐµÐºÐ¾Â», Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° PR-ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐ½ÑÐµÐºÐ¾Â».
title: Ð¤ÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ ÑÐ¾Ð»Ñ ÑÐ¸Ð³Ð¼Ð° 1 ÑÐµÑÐµÐ¿ÑÐ¾ÑÐ° Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð±Ð¾Ð»ÐµÐ·Ð½Ð¸ Ð¥Ð°Ð½ÑÐ¸Ð½Ð³ÑÐ¾Ð½Ð°
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 03.01.03 Â«ÐÐ¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð°Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÂ»
titleType: Subtitle
Creators: name: ÐÑÐ°ÑÐºÐ¾Ð²ÑÐºÐ°Ñ, Ð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: 2021
Subjects: ÐÐµÐ¹ÑÐ¾Ð½Ñ
ÐÐ°Ð»ÑÑÐ¸Ð¹
Ð½ÐµÐ¹ÑÐ¾Ð´ÐµÐ³ÐµÐ½ÐµÑÐ°ÑÐ¸Ð²Ð½ÑÐµ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸Ñ
Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸Ñ
Ð±Ð¾Ð»ÐµÐ·Ð½Ñ Ð¥Ð°Ð½ÑÐ¸Ð½Ð³ÑÐ¾Ð½Ð°
Ð½ÐµÑÐ²Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÑÑÐ½ÐµÐ½Ð° ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ ÑÐ¾Ð»Ñ ÑÐ¸Ð³Ð¼Ð° 1 ÑÐµÑÐµÐ¿ÑÐ¾ÑÐ° Ð½Ð° Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð±Ð¾Ð»ÐµÐ·Ð½Ð¸ Ð¥Ð°Ð½ÑÐ¸Ð½Ð³ÑÐ¾Ð½Ð°. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¾ÑÐ¸Ð³Ð¸Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð»Ð°, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ðµ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÑÐ¼Ð¾Ð³Ð¾ ÑÐµÐ¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÐµÑÐ²Ð¸ÑÐ½ÑÑ Ð´ÐµÑÐ¼Ð°Ð»ÑÐ½ÑÑ ÑÐ¸Ð±ÑÐ¾Ð±Ð»Ð°ÑÑÐ¾Ð² Ð² ÑÑÐµÐ´Ð½Ð¸Ðµ ÑÐ¸Ð¿Ð¸ÐºÐ¾Ð²ÑÐµ Ð½ÐµÐ¹ÑÐ¾Ð½Ñ ÑÑÑÐ¸Ð°ÑÑÐ¼Ð°. ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð» Ð¿Ð¾Ð»ÐµÐ·ÐµÐ½ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ Ð²Ð¾Ð·ÑÐ°ÑÑ-Ð°ÑÑÐ¾ÑÐ¸Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð¾-ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¹ Ð² ÑÑÐµÐ´Ð½Ð¸Ñ ÑÐ¸Ð¿Ð¸ÐºÐ¾Ð²ÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð°Ñ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ Ð¿Ð°ÑÐ¾Ð³ÐµÐ½ÐµÐ·Ð° Ð±Ð¾Ð»ÐµÐ·Ð½Ð¸ Ð¥Ð°Ð½ÑÐ¸Ð½Ð³ÑÐ¾Ð½Ð°.
The SEDIGISM survey: a search for molecular outflows
Creators: name: Yang, A. Y.
name: Urquhart, J. S.
name: Wyrowski, F.
name: Thompson, M. A.
name: König, C.
name: Colombo, D.
name: Menten, K. M.
name: Duarte-Cabral, A.
name: Schuller, F.
name: Csengeri, T.
name: Eden, D.
name: Barnes, P.
name: Traficante, A.
name: Bronfman, L.
name: Sanchez-Monge, A.
name: Ginsburg, A.
name: Cesaroni, R.
name: Lee, M. -Y.
name: Beuther, H.
name: Medina, S. -N. X.
name: Mazumdar, P.
name: Henning, T.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Context. The formation processes of massive stars are still unclear but a picture is emerging involving accretion disks and molecular outflows in what appears to be a scaled-up version of low-mass star formation. A census of outflow activity towards massive star-forming clumps in various evolutionary stages has the potential to shed light on massive star formation (MSF). Aims. We conducted an outflow survey towards ATLASGAL clumps using SEDIGISM data and aimed to obtain a large sample of clumps exhibiting outflows in different evolutionary stages. Methods. We identify the high-velocity wings of the 13CO lines toward ATLASGAL clumps by (1) extracting the simultaneously observed 13CO and C18O spectra from SEDIGISM, and (2) subtracting Gaussian fits to the scaled C18O from the 13CO, line after considering opacity broadening. Results. We have detected high-velocity gas towards 1192 clumps out of a total sample of 2052, giving an overall detection rate of 58%. Outflow activity has been detected in the earliest quiescent clumps (i.e., 70$μ$m weak), to the most evolved HII region stages i.e., 8$μ$m bright with MSF tracers. The detection rate increases as a function of evolution (quiescent=51%, protostellar=47%, YSO=57%, UCHII regions=76%). Conclusion. Our sample is the largest outflow sample identified so far. The high-detection rate from this large sample is consistent with previous results and supports that outflows are a ubiquitous feature of MSF. The lower detection rate in early evolutionary stages may be due to that outflows in the early stages are weak and difficult to detect. We obtain a statistically significant sample of outflow clumps for every evolutionary stage, especially for outflow clumps in the 70$μ$m dark stage. This suggests that the absence of 70$μ$m emission is not a robust indicator of starless/pre-stellar cores.
description: 13 pages, 10 figures, accepted by Astronomy & Astrophysics (A&A)
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Ð´Ð»Ñ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐµÑ Ð¼ÐµÑÐ½ÑÑ ÑÑÐµÐ½ Ð² ÑÐµÐ°Ð»ÑÐ½Ð¾Ð¼ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° ÑÑÐ°ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð¿ÑÑÐ¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐµÐ»Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÑÐ°ÑÑÐ¸ÑÐ¾Ð²ÐºÐ° Ð¿ÑÑÐ¸
ÑÑÐ°ÑÑÐ¸ÑÐ¾Ð²ÐºÐ° Ð»ÑÑÐµÐ¹
ÐºÐ¾ÑÑÐµÐºÑÐ½ÑÐ¹ ÑÐµÐ½Ð´ÐµÑÐ¸Ð½Ð³
Ð¼ÐµÑÐ¾Ð´ ÐÐ¾Ð½ÑÐµ-ÐÐ°ÑÐ»Ð¾
Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½ÑÐµ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð´ÑÐºÑÐ° Ð´Ð»Ñ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¾ÑÐ¾ÑÐµÐ°Ð»Ð¸ÑÑÐ¸ÑÐ½ÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ð² ÑÐµÐ°Ð»ÑÐ½Ð¾Ð¼ Ð²ÑÐµÐ¼ÐµÐ½Ð¸. ÐÐ³Ð¾ ÑÐ°Ð±Ð¾ÑÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° Ð½Ð° Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ðµ ÑÑÐ°ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð¿ÑÑÐ¸, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÐµÑ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ ÑÐµÐ°Ð»Ð¸ÑÑÐ¸ÑÐ½Ð¾ÑÑÑ Ð¿Ð¾Ð»ÑÑÐ°ÐµÐ¼Ð¾Ð³Ð¾ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ. Ð¡Ð¸ÑÑÐµÐ¼Ð° ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸ ÐºÐ¾ÑÑÐµÐºÑÐ½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð´Ð°ÐµÑ Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾Ðµ Ð¾ÑÐ²ÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð¸Ñ. ÐÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ ÑÐ°ÑÐ¿Ð°ÑÐ°Ð»Ð»ÐµÐ»Ð¸Ð²Ð°ÑÑÑÑ Ð½Ð° Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐµ. Ð­ÑÐ¾ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¼Ð°ÑÑÑÐ°Ð±Ð½ÑÐµ, Ð²ÑÑÐ¾ÐºÐ¾ Ð´ÐµÑÐ°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÑÐµÑÐ¼ÐµÑÐ½ÑÐµ ÑÑÐµÐ½Ñ ÑÐ¾ ÑÐºÐ¾ÑÐ¾ÑÑÑÑ Ð´Ð¾ 30 ÐºÐ°Ð´ÑÐ¾Ð² Ð² ÑÐµÐºÑÐ½Ð´Ñ, Ñ ÑÐµÐ¼ Ð½Ðµ ÑÑÐ°Ð²Ð½ÑÑÑÑ "ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ" Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ ÑÑÐ°ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð»ÑÑÐµÐ¹, Ð½Ð° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¼Ð¾Ð¶ÐµÑ ÑÑÐ¾Ð´Ð¸ÑÑ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¾ ÑÐ°ÑÐ¾Ð².
The relationship between BMI and health-related quality of life (HRQoL) for overweight and obese individuals: evidence from weight loss trials
Creators: name: Buckell, John
name: Mei, Xue
name: Becker, Frauke
name: Clarke, Philip
name: Aveyard, Paul
name: Jebb, Susan
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Health Economics
subject: Other Public Health
subject: Diseases
subject: Public Health
subject: Medicine and Health Sciences
subject: Endocrine System Diseases
subject: Economics
subject: Nutritional and Metabolic Diseases
subject: Social and Behavioral Sciences

description: Using data from randomized controlled trials to assess the relationship between weight change and health-related quality of life.
Organización del ADN
Creators: name: Hernández Anastasio, Marlen
Publisher: name: Zenodo
Year: 2022
Subjects: ADN; organización del ADN; histonas; cromosomas; cromatina.

description: Resumen El núcleo de las células eucariotas es un organelo voluminoso que esta delimitado por una envoltura nuclear. Dentro del núcleo se encuentra el ADN genómico o genoma de la célula, el cual se encuentra repartido en los cromosomas lineales. La matriz semifluida del núcleo (nucleoplasma) rodeado por la envoltura nuclear, contiene la cromatina, el cual es el material genético más todas las moléculas que se encuentran relacionadas con su organización, fundamentalmente histonas. El ADN no se encuentra libre en el nucleoplasma sino asociado a proteínas como las histonas y a otras proteínas implicadas en su procesamiento (proteínas de andamiaje), formando en conjunto la cromatina. Las histonas son proteínas asociadas al ADN que determinan su organización. El ADN se organiza estructuralmente en cromosomas. A nivel funcional se organiza en genes, que son piezas de ADN que generan características físicas específicas. Para poder entender mejor como es la actividad de una macromolécula compleja, como lo es el ADN, es necesario conocer como se integra dicha molécula y las estructuras en las que se puede organizar [1-4].
description: {"references": ["[1]. Benjamin Lewin. (2008). Genes Ix (9th ed.). McGraw+Hill Interamericana Editores.", "[2]. Karp Gerald. (2010). Biolog\u00eda celular y molecular (6th ed.). McGRAW-HILL INTERAMERICANA EDITORES, S.A. de C.V.", "[3]. Olby, R. (1974). The Path to the Double Helix. MacIvl..illan, London.", "[4[. Ridgway P, Maison C, Almouzni G . Chromatin. Atlas Genet Cytogenet Oncol Haematol. April 2002."]}
Der heilige Konrad, Bischof von Konstanz (934–975), in der welfischen Memorialüberlieferung des 12. Jahrhunderts
Creators: name: Fleischer, Leonhard
Publisher: name: Concilium medii aevi
Year: 2020

description: Concilium medii aevi, Bd. 23 (2020): Concilium medii aevi