cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Long-Term Evolution of Slowly Rotating Collapsar in Special Relativistic Magnetohydrodynamics
Creators: name: Harikae, Seiji
name: Takiwaki, Tomoya
name: Kotake, Kei
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present our numerical results of two-dimensional magnetohydrodynamic (MHD) simulations of the collapse of rotating massive stars in light of the collapsar model of gamma-ray bursts (GRBs). Pushed by recent evolution calculations of GRB progenitors, we focus on lower angular momentum of the central core than the ones taken mostly in previous studies. By performing special relativistic simulations including both realistic equation of state and neutrino coolings, we follow a unprecedentedly long-term evolution of the slowly rotating collapsars up to $\sim$ 10 s, accompanied by the formation of jets and accretion disks. Our results show that for the GRB progenitors to function as collapsars, there is a critical initial angular momentum, below which matter is quickly swallowed to the central objects, no accretion disks and no MHD outflows are formed. When larger than the criteria, we find the launch of the MHD jets in the following two ways. For models with stronger initial magnetic fields, the magnetic pressure amplified inside the accretion disk can drive the MHD outflows, which makes the strong magnetic explosions like a 'magnetic tower' (type II). For the models with weaker initial magnetic fields, the magnetic tower stalls first and the subsequent MHD outflows are produced by some eventual inflows of the accreting material from the equator to the polar regions (type I). Regardless of type I or II, the jets can attain only mildly relativistic speeds with the explosion energy less than $10^{49} \erg$, which could possibly be related to the X-ray flashes. Due to high opacity for neutrinos inside the disk, we find that the luminosities of $ν_e$ and $\barν_e$ become almost comparable, which is advantageous for making the energy deposition rate larger.
description: 53 pages with 19 figures
title: ÐÐ¾Ð½ÑÑÐ½ÐºÑÑÑÐ° ÑÑÐ½ÐºÐ° ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
Creators: name: ÐÐ»ÐµÐºÑÐµÐµÐ²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
name: ÐÐ°Ð¿ÑÑÑÐ¸Ð½Ð°, ÐÑÐ¸Ð½Ð°
name: ÐÑÐ¿ÐµÐ½ÑÐ¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸

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title: Ð­ÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ñ Ð¸ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº
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 Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â»
titleType: Subtitle
Creators: name: Ð ÑÐ±Ð°Ð»ÐºÐ¾, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: Ð¢ÑÑÐ±Ð¸Ð½Ð½ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸

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Video Source Characterization Using Encoding and Encapsulation Characteristics
Creators: name: Altinisik, Enes
name: Sencar, Husrev Taha
name: Tabaa, Diram
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cryptography and Security (cs.CR)
subject: Multimedia (cs.MM)
subject: FOS: Computer and information sciences

description: We introduce a new method for camera-model identification. Our approach combines two independent aspects of video file generation corresponding to video coding and media data encapsulation. To this end, a joint representation of the overall file metadata is developed and used in conjunction with a two-level hierarchical classification method. At the first level, our method groups videos into metaclasses considering several abstractions that represent high-level structural properties of file metadata. This is followed by a more nuanced classification of classes that comprise each metaclass. The method is evaluated on more than 20K videos obtained by combining four public video datasets. Tests show that a balanced accuracy of 91% is achieved in correctly identifying the class of a video among 119 video classes. This corresponds to an improvement of 6.5% over the conventional approach based on video file encapsulation characteristics. Furthermore, we investigate a setting relevant to forensic file recovery operations where file metadata cannot be located or are missing but video data is partially available. By estimating a partial list of encoding parameters from coded video data, we demonstrate that an identification accuracy of 57% can be achieved in camera-model identification in the absence of any other file metadata.
The Chandra ACIS Survey of M33: X-ray, Optical and Radio Properties of the Supernova Remnants
Creators: name: Long, Knox S.
name: Blair, William P.
name: Winkler, P. Frank
name: Becker, Robert H.
name: Gaetz, Terrance J.
name: Ghavamian, Parviz
name: Helfand, David J.
name: Hughes, John P.
name: Kirshner, Robert P.
name: Kuntz, Kip D.
name: McNeil, Emily K.
name: Pannuti, Thomas G.
name: Plucinsky, Paul P.
name: Saul, Destry
name: Tuellmann, Ralph
name: Williams, Benjamin
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: M33 contains a large number of emission nebulae identified as supernova remnants (SNRs) based on the high [S II]:Ha ratios characteristic of shocked gas. Using Chandra data from the ChASeM33 survey with a 0.35-2 keV sensitivity of about 2 x 10**34 ergs/s, we have detected 82 of 137 SNR candidates, yielding confirmation of (or at least strongly support for) their SNR identifications. This provides the largest sample of remnants detected at optical and X-ray wavelengths in any galaxy, including the Milky Way. A spectral analysis of the seven X-ray brightest SNRs reveals that two, G98-31 and G98-35, have spectra that appear to indicate enrichment by ejecta from core-collapse supernova explosions. In general, the X-ray detected SNRs have soft X-ray spectra compared to the vast majority of sources detected along the line of sight to M33. It is unlikely that there are any other undiscovered thermally dominated X-ray SNRs with luminosities in excess of about 4 x 10**35 ergs/s in the portions of M33 covered by the ChASeM33 survey. We have used a combination of new and archival optical and radio observations to attempt to better understand why some objects are detected as X-ray sources and others are not. We have also developed a morphological classification scheme for the optically-identified SNRs, and discuss the efficacy of this scheme as a predictor of X-ray detectability. Finally, we have compared the SNRs found in M33 to those that have been observed in the Galaxy and the Magellanic Clouds. There are no close analogs of Cas A, Kepler's SNR, Tycho's SNR or the Crab Nebula in the regions of M33 surveyed, but we have found an X-ray source with a power law spectrum coincident with a small-diameter radio source that may be the first pulsar-wind nebula recognized in M33.
description: 142 pages, including 8 talbes and 50 figures, to be published in ApJ Supplements
Севастопольский музейный комплекс «35-я береговая батарея» как составная часть актуальной программы патриотического воспитания молодежи в РФ
Creators: name: Володин Валерий Иванович
Publisher: name: Zenodo
Year: 2025
Subjects: 35-я береговая батарея
Великая Отечественная война
патриотическое воспитание молодежи
35th Coastal Battery
Great Patriotic War
patriotic education of youth

description: Аннотация. В статье изучена история создания и практика военно-патриотической работы Музейного историко-мемориального комплекса «35-я береговая батарея». Описаны различные практики и мероприятия, внедренные как в сотрудничестве с федеральными властями, командованием Вооруженных Сил России, так и с региональной властью, музеями Севастополя, общественностью. Сделан вывод, что необходимо дальнейшее укрепление взаимодействия с органами образования и руководством Вооруженных Сил в деле патриотического воспитания молодежи, в том числе на базе МИМК «35-я береговая батарея».

Abstract. The article examines the history of the creation and practice of military-patriotic work of the Museum Historical and Memorial Complex «35th Coastal Battery». Various practices and events implemented in cooperation with the federal authorities, the command of the Armed Forces of Russia, as well as with the regional authorities, museums of Sevastopol, and the public are described. It is concluded that it is necessary to further strengthen cooperation with educational authorities and the leadership of the Armed Forces in the matter of patriotic education of youth, including on the basis of the Museum Historical and Memorial Complex «35th Coastal Battery».
Equilibrium Sequences of Rotating Neutron Stars for New Microscopic
  Equations of State
Creators: name: B. Datta
name: A. V. Thampan
name: I. Bombaci
Publisher: name: INFN Open Access Repository
Year: 1998

description: For four newly suggested microscopic equations of state of neutron star
matter, we construct equilibrium sequences of rapidly rotating neutron stars in
general relativity. The sequences are the normal and supramassive evolutionary
sequences of constant rest mass. We find that for these equations of state the
maximum (gravitational) mass rotating models occur (in central density and
rotation rate $\Omega$) before the maximum--$\Omega$ models. We calculate
equilibrium sequences for a constant value of $\Omega$ corresponding to the
most rapidly rotating pulsar PSR 1937+21. Also calculated is the radius of the
marginally stable orbit and its dependence on $\Omega$.
The ROSAT Deep Cluster Survey: Constraints on Cosmology
Creators: name: S. Borgani
name: P. Rosati
name: R. Della Ceca
name: P. Tozzi
name: C. Norman
Publisher: name: INFN Open Access Repository
Year: 1999

description: We use the ROSAT Deep Cluster Survey (RDCS) to trace the evolution of the
cluster abundance out to $z\simeq 0.8$ and constrain cosmological models. We
resort to a phenomenological prescription to convert masses into $X$-ray fluxes
and apply a maximum-likelihood approach to the RDCS redshift- and
luminosity-distribution. We find that, even changing the shape and the
evolution on the $L_{bol}$-$T_X$ relation within the observational
uncertainties, a critical density Universe is always excluded at more than
$3\sigma$ level. By assuming a non-evolving $X$-ray luminosity-temperature
relation with shape $L_{bol}\propto T_X^3$, it is
$\Omega_m=0.35^{+0.35}_{-0.25}$ and $\sigma_8=0.76^{+0.38}_{-0.14}$ for flat
models, with uncertainties corresponding to $3\sigma$ confidence levels.
Additional file 4 of Amphibian richness along modified riparian areas of central Mexico: conservation priorities
Creators: name: Oropeza-Sánchez, Marco Tulio
name: Suazo-Ortuño, Ireri
name: Benítez-Malvido, Julieta
name: Monroy-Hernández, Erandi
name: Munguía-Steyer, Roberto
Publisher: name: figshare
Year: 2022
Subjects: subject: Ecology
subject: FOS: Biological sciences

description: Additional file 4: Appendix S4. Effect of each explaining variable on detection and occupancy probability of every amphibian species and the community on logit scale.
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ ÑÐ¾Ð½ÐºÐ¾Ð¹ Ð¿Ð»ÐµÐ½ÐºÐ¸ Ð¿Ð¾Ð»Ð¸Ð¿ÑÐ¾Ð¿Ð¸Ð»ÐµÐ½Ð° Ð¿ÑÐ¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ñ
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¢ÑÐ¼ÑÑÐ¾Ð²Ð°, 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: 2017
Subjects: ÐÐ»ÐµÐ½ÐºÐ¸ ÑÐ¾Ð½ÐºÐ¸Ðµ
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description: ÐÑÐ»Ð° Ð¸Ð·ÑÑÐµÐ½Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¿ÑÐ¾Ð½Ð¾ÑÑÑ ÑÐ¾Ð½ÐºÐ¾Ð¹ Ð¿Ð»ÐµÐ½ÐºÐ¸ Ð¿Ð¾Ð»Ð¸Ð¿ÑÐ¾Ð¿Ð¸Ð»ÐµÐ½Ð° ÑÐ¾Ð»ÑÐ¸Ð½Ð¾Ð¹ 2 Ð¼ÐºÐ¼ Ð¿ÑÐ¸ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½Ð¾Ð¼ Ð¸ ÐºÐ²Ð°Ð·Ð¸Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½Ð¾Ð¼ ÑÐµÐ¶Ð¸Ð¼Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ñ. ÐÐ°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ðµ Ð½Ð° Ð¾Ð±ÑÐ°Ð·ÑÐµ Ð²Ð¾Ð·ÑÐ°ÑÑÐ°ÐµÑ ÑÐºÐ¿Ð¾Ð½ÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½Ð¾ Ð¸ Ð´Ð¾ÑÑÐ¸Ð³Ð°ÐµÑ Ð´Ð¾ 2000 Ð, ÑÑÐ¾Ð½Ñ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ° Ð¿ÑÐ¸ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½Ð¾Ð¼ ÑÐµÐ¶Ð¸Ð¼Ðµ Ð¼ÐµÐ½ÑÐµÑÑÑ Ð¾Ñ 26 Ð½Ñ Ð´Ð¾ 1116 Ð½Ñ, Ð¿ÑÐ¸ ÐºÐ²Ð°Ð·Ð¸Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½Ð¾Ð¼ ÑÐµÐ¶Ð¸Ð¼Ðµ Ð¾Ñ 1,85 Ñ Ð´Ð¾ 71 Ñ. ÐÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð¿ÑÐ¾Ð±Ð¸Ð²Ð½Ð¾Ðµ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ðµ Ð¿Ð»ÐµÐ½ÐºÐ¸ ÐÐ Ð¿ÑÐ¸ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½Ð¾Ð¼ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ð¸ Ð¸ Ð² ÐºÐ²Ð°Ð·Ð¸ÑÑÐ°ÑÐ¸Ð¾Ð½Ð°ÑÐ½Ð¾Ð¼ ÑÐµÐ¶Ð¸Ð¼Ð°Ñ Ð¾Ð´Ð¸Ð½Ð°ÐºÐ¾Ð²Ñ.
Superfluid to Mott-insulator transition of cold atoms in optical lattices
Creators: name: Dupuis, N.
name: Sengupta, K.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We review the superfluid to Mott-insulator transition of cold atoms in optical lattices. The experimental signatures of the transition are discussed and the RPA theory of the Bose-Hubbard model briefly described. We point out that the critical behavior at the transition, as well as the prediction by the RPA theory of a gapped mode (besides the Bogoliubov sound mode) in the superfluid phase, are difficult to understand from the Bogoliubov theory. On the other hand, these findings appear to be intimately connected to the non-trivial infrared behavior of the superfluid phase as recently studied within the non-perturbative renormalization group.
description: 6 pages, Proceedings of the 5th International Workshop on Electronic Crystals (ECRYS 2008)
Glimpses of a strange star
Creators: name: Jishnu Dey
name: Subharthi Ray
name: Li, Xiang-Dong
name: Dey, Mira
name: Bombaci, Ignazio
Publisher: name: INFN Open Access Repository
Year: 2000

description: There are about 2000 gamma ray burst (GRB) events known to us with data
pouring in at the rate of one per day. While the afterglows of GRBs in radio,
optical and X-ray bands are successfully explained by the fireball model, a
significant difficulty with the proposed mechanisms for GRBs is that a small
amount ($\le 10^{-6} M_{\odot}$) of baryons in the ejecta can be involved.
There are very few models that fulfill this criteria together with other
observational features, among which are the differentially rotating collapsed
object model and the "supernova" model. These models generally invoke rapidly
rotating neutron stars, and may be subject to uncertainties in the formation
mechanisms and the equations of state of neutron stars. According to Spruit,
the problem of making a GRB from an X-ray binary is reduced to finding a
plausible way to make the star rotate differentially. We suggest that a model
of strange star (SS) can naturally explain many of these bursts with not only
their low baryon content, but the differential rotation which leads to an
enhanced magnetic field that surfaces up and is responsible for GRBs.
title: Ð¡Ð°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²ÐºÐ° ÑÑÐ´ÐµÐ¹ Ð¿Ð¾ Ð¼Ð¸Ð½Ð¸-ÑÑÑÐ±Ð¾Ð»Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹
title: Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¾Ð»Ð¾ÑÐ¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ°ÐºÐ°ÐµÐ², ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
name: ÐÐ¾Ð¿Ð¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ²Ð°, ÐÐ°Ð»ÐµÑÐ¸Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: Ð¼Ð¸Ð½Ð¸-ÑÑÑÐ±Ð¾Ð»
Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° ÑÑÐ´ÐµÐ¹
Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ

description: Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²ÐºÐ¸ ÑÑÐ´ÐµÐ¹ Ð¿Ð¾ Ð¼Ð¸Ð½Ð¸-ÑÑÑÐ±Ð¾Ð»Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²ÐºÐ¸ ÑÑÐ´ÐµÐ¹ Ð¿Ð¾ Ð¼Ð¸Ð½Ð¸-ÑÑÑÐ±Ð¾Ð»Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÐºÑÑÑÑ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð° Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÑÐ´ÐµÐ¹ Ðº Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ Ð¸Ð³Ñ. ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¼ÐµÑÐ¾Ð´Ð°Ð¼ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð½Ð°Ð´ ÑÑÐ¾Ð²Ð½ÐµÐ¼ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð³Ð¾ÑÐ¾Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÐ´ÐµÐ¹ Ð¿Ð¾ Ð¼Ð¸Ð½Ð¸-ÑÑÑÐ±Ð¾Ð»Ñ.
ÐÐ¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð° Ð´Ð»Ñ ÑÑÐ´ÐµÐ¹ Ð¿Ð¾ Ð¼Ð¸Ð½Ð¸-ÑÑÑÐ±Ð¾Ð»Ñ, ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð¸ ÑÑÐµÐ½ÐµÑÐ¾Ð² Ð¿Ð¾ Ð¼Ð¸Ð½Ð¸-ÑÑÑÐ±Ð¾Ð»Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸Ð½ÑÑÐ¸ÑÑÑÐ¾Ð² ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ.
Application of EFT at Thermal Energies
Creators: name: Sadeghi, H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We have been evaluated some observables of n-d systems by using pionless Effective Field Theory(\EFTNoPion) and insertion of the three-body force up to next-to-next to leading order(N$^2$LO). The evaluated data has been compared with experimental and the three-nucleon calculation of the total cross section with modern realistic two- and three-nucleon forces AV18/UrbIX potential models calculations.
description: 3 pages, 1 figure and 1 table. Talk given at 20th European Conference on Few-Body Problems in Physics (EFB 20), Pisa, Italy, 10-14 Sep 2007
NLO quark self-energy and dispersion relation using the hard thermal loop resummation
Creators: name: Sumit
name: Haque, Najmul
name: Patra, Binoy Krishna
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Using the hard-thermal-loop (HTL) resummation in real-time formalism, we study the next-to-leading order (NLO) quark self-energy and corresponding NLO dispersion laws. In NLO, we have replaced all the propagators and vertices with the HTL-effective ones in the usual quark self-energy diagram. Additionally, a four-point vertex diagram also contributes to the quark NLO self-energy. We calculate the usual quark self-energy diagram and the four-point vertex diagram separately. Using those, we express the NLO quark self-energy in terms of the three- and four-point HTL-effective vertex functions. Using the Feynman parametrization, we express the integrals containing the three- and four-point HTL effective vertex functions in terms of the solid angles. After completing the solid angle integrals, we numerically calculate the momentum integrals in the NLO quark self-energy and plot them as a function of the ratio of momentum and energy. Using the NLO quark self-energy, we plot the NLO correction to dispersion laws.
description: 35 pages, 19 figures
Shadows of Relic Neutrino Masses and Spectra on Highest Energy GZK
  Cosmic Rays
Creators: name: D. Fargion
name: M. Grossi
name: P. G. De Sanctis Lucentini
name: C. Di Troia
name: R. V. Konoplich
Publisher: name: Dark Matter in Astro and Particle Physics,Dark
  2000,Heidelberg,10-14 July,Ed.H.V.Klapdor-Kleingrothaus,Springer
  2001,p.455-468
Year: 2001

description: The Ultra High Energy (UHE) neutrino scattering onto relic cosmic neutrinos
in galactic and local halos offers an unique way to overcome GZK cut-off. The
UHE nu secondary of UHE photo-pion decays may escape the GZK cut-off and travel
on cosmic distances hitting local light relic neutrinos clustered in dark
halos. The Z resonant production and the competitive W^+W^-, ZZ pair production
define a characteristic imprint on hadronic consequent UHECR spectra. This
imprint keeps memory both of the primary UHE nu spectra as well as of the
possible relic neutrino masses values, energy spectra and relic densities. Such
an hadronic showering imprint should reflect into spectra morphology of cosmic
rays near and above GZK 10^{19}-10^{21}eV cut-off energies. A possible neutrino
degenerate masses at eVs or a more complex and significant neutrino mass split
below or near Super-Kamiokande \triangle m_{\nu_{SK}}= 0.1 eV masses might be
reflected after each corresponding Z peak showering, into new twin unexpected
UHECR flux modulation behind GZK energies: E_{p} sim 3(frac{triangle
m_{\nu_{SK}}}/m_{\nu}10^{21}),eV.
  Other shadowsof lightest, nearly massless, neutrinos m_{nu_{2K} simeq 0.001eV
simeq kT_{\nu}, their lowest relic temperatures, energies and densities might
be also reflected at even higher energies edges near Grand Unification: E_{p}
\sim 2.2(m_{\nu_{2K}/E_{\nu}})10^{23}, eV .
title: ÐÑÐ°ÐºÑÐ¸ÐºÑÐ¼ Ð¿Ð¾ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ñ ÑÐµÐºÑÑÐ¾Ð² Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸ (Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº). Ð§. 2
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð³Ð¾Ð´Ð¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
name: Ð¡Ð¼Ð¸ÑÐ½Ð¾Ð²Ð°, ÐÐ°ÑÐ¸ÑÐ°
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: Ð°ÑÑÐµÐ½ÑÐ¸ÑÐ½ÑÐµ ÑÐµÐºÑÑÑ
Ð¼Ð°ÑÐ¸Ð½Ð½ÑÐ¹ Ð¿ÐµÑÐµÐ²Ð¾Ð´
ÑÐµÐ´Ð°ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²
Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº

description: ÐÐ°Ð½Ð½Ð¾Ðµ ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Â«ÐÑÐ°ÐºÑÐ¸ÐºÑÐ¼ Ð¿Ð¾ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ñ ÑÐµÐºÑÑÐ¾Ð² Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸Â», Ð§. II, ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐ¼ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ Ð¿Ð¾ ÐºÑÑÑÑ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð¸ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐ°ÐµÑÑÑ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ° 2-3 ÐºÑÑÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ âÐÑÐ°ÐºÑÐ¸ÐºÑÐ¼ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÐµÐºÑÑÐ¾Ð²â ÐºÐ°ÑÐµÐ´ÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸. Ð ÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð½Ð° Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸ÑÑ: Ð² Ð°ÑÐ´Ð¸ÑÐ¾ÑÐ½Ð¾Ð¹ Ð¸ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð² ÑÐµÐ¶Ð¸Ð¼Ðµ On-line Ð´Ð»Ñ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð°Ð´ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð¾Ð¼ Ð½ÐµÐ°Ð´Ð°Ð¿ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐµÐºÑÑÐ¾Ð² Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ° Ð½Ð° ÑÑÑÑÐºÐ¸Ð¹. Ð¢ÐµÐºÑÑÑ Ð²ÑÐ¾ÑÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ñ Ð´Ð»Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¼ÐµÐ½Ð¸Ð¹, Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð°ÑÑÐµÐ½ÑÐ¸ÑÐ½ÑÑ ÑÐµÐºÑÑÐ¾Ð² Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² ÑÐ¾Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð°, ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐºÑÑÐ° (ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿Ð»Ð°Ð½Ð°, ÑÐµÑÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ) Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ° Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° ÑÐµÐºÑÑÐ°. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¾Ð±ÑÑÐ°ÐµÑ ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¸ ÑÐµÐ´Ð°ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð¾Ð² ÑÐµÐºÑÑÐ¾Ð² Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¸ ÑÑÑÑÐºÐ¸Ñ ÑÐ·ÑÐºÐ¾Ð² Ð¸Ð· Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¸ Ð»ÐµÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÐµÐ´Ð¸Ð½Ð¸Ñ
Ð² Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ»Ð¾Ð²Ð°ÑÑÑ (Google,Yandex etc).
Additional file 5 of Amphibian richness along modified riparian areas of central Mexico: conservation priorities
Creators: name: Oropeza-Sánchez, Marco Tulio
name: Suazo-Ortuño, Ireri
name: Benítez-Malvido, Julieta
name: Monroy-Hernández, Erandi
name: Munguía-Steyer, Roberto
Publisher: name: figshare
Year: 2022
Subjects: subject: Ecology
subject: FOS: Biological sciences

description: Additional file 5: Appendix S5. Coefficients of each variable in the models to explain occupancy of amphibians in riparian zones of Northwest Michoacán, Mexico.
Monumenta Germaniae Historica, Diplomata regum et imperatorum Germaniae. Die Urkunden der Deutschen Könige und Kaiser Bd. 14,1: Friderici II. diplomata inde ab anno MCXCVIII usque ad annum MCCXII. Die Urkunden Friedrichs II. 1198-1212
Creators: name: Petersen, Stefan
Publisher: name: Concilium medii aevi
Year: 2021

description: Rezension zu: Monumenta Germaniae Historica, Diplomata regum et imperatorum Germaniae. Die Urkunden der Deutschen Könige und Kaiser Bd. 14,1: Friderici II. diplomata inde ab anno MCXCVIII usque ad annum MCCXII. Die Urkunden Friedrichs II. 1198-1212, bearb. v. Walter KOCH unter Mitwirkung von Klaus Höflinger und Joachim Spiegel und unter Verwendung von Vorarbeiten von Charlotte Schroth-Köhler (†), Hannover 2002. 522 S. – ISBN 3-7752-2001-1
description: Concilium medii aevi, Bd. 6 (2003): Concilium medii aevi
Mesoscopic Properties of Molecular Folding and Aggregation Processes
Creators: name: Bachmann, Michael
name: Janke, Wolfhard
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Protein folding, peptide aggregation and crystallization, as well as adsorption of molecules on soft or solid substrates have an essential feature in common: In all these processes, structure formation is guided by a collective, cooperative behavior of the molecular subunits lining up to build chainlike macromolecules. Proteins experience conformational transitions related to thermodynamic phase transitions. For chains of finite length, an important difference of crossovers between conformational (pseudo)phases is, however, that these transitions are typically rather smooth processes, i.e., thermodynamic activity is not necessarily signalized by strong entropic or energetic fluctuations. Nonetheless, in order to understand generic properties of molecular structure-formation processes, the analysis of mesoscopic models from a statistical physics point of view enables first insights into the nature of conformational transitions in small systems. Here, we review recent results obtained by means of sophisticated generalized-ensemble computer simulations of minimalistic coarse-grained models.
description: 28 pages, 10 figures, 2 tables
Chemical Enrichment and Energetics of the ICM with Redshift
Creators: name: A. Pipino
name: F. Matteucci
name: S. Borgani
name: A. Biviano
Publisher: name: INFN Open Access Repository
Year: 2001

description: In this paper we show preliminary results concerning the chemical and
energetic enrichment of the ICM by means of supernova-driven wind models in
elliptical galaxies. These models are obtained by taking into account new
prescriptions about supernova remnant evolution in the interstellar medium. We
find that models, which can reproduce the Fe abundance and the [$\alpha$/Fe]
ratios observed in the ICM, predict that the SN energy input can provide about
0.3 keV per ICM particle. We have obtained this result by assuming that each SN
explosion inject on the average into the ISM no more than 20% of its initial
blast wave energy. The predicted energy per particle is not enough to break the
cluster self-similarity but is more than predicted in previous models.
title: ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ñ ÐºÐ¸ÑÐ°Ð¹ÑÐµÐ²
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ»ÐµÐºÐ±ÐµÑÐ¾Ð², Ð Ð¾Ð¼Ð°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: 2017
Subjects: ÑÑÐ½Ð¾Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸Ñ
Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐ°Ñ Ð°Ð½ÑÑÐ¾Ð¿Ð¾Ð»Ð¾Ð³Ð¸Ñ
Ð¼ÐµÐ¶ÐºÑÐ»ÑÑÑÑÐ½Ð°Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ñ
Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ¸ Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð´Ð°Ð½Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÑÐ½Ð¾Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸ ÐºÐ°Ðº Ð½Ð°ÑÐºÐ¸, ÐµÐµ Ð¸ÑÑÐ¾ÑÐ¸Ñ, Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾Ð½Ð° Ð¿ÐµÑÐµÐ´ ÑÐ¾Ð±Ð¾Ð¹ ÑÑÐ°Ð²Ð¸Ñ. ÐÐ°Ð½Ð° ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÑÐ½Ð¾Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð¸ÑÐµÐ»ÐµÐ¹ Ð°Ð·Ð¸Ð°ÑÑÐºÐ¾Ð¹ Ð¸ ÐµÐ²ÑÐ¾Ð¿ÐµÐ¹ÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð³Ð¾ Ð²ÐµÑÐ±Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð½ÐµÐ²ÐµÑÐ±Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð´Ð°Ð½Ð° Ð¾Ð±ÑÐ°Ñ Ð¾ÑÐµÐ½ÐºÐ° Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÐ¼ ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð³Ð¾ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÑÐ°ÐºÑÐµÑÐ°.
X-ray temperature and morphology of z>0.8 clusters of galaxies
Creators: name: B. Holden
name: S. A. Stanford
name: P. Rosati
name: P. Tozzi
name: G. Squires
name: S. Borgani
name: P. Eisenhardt
Publisher: name: INFN Open Access Repository
Year: 2001

description: We discuss our current progress in studying a sample of z>0.8 clusters of
galaxies from the ROSAT Distant Cluster Survey. To date, we have Chandra
observations for four of the ten clusters. We find that the morphology of two
of these four are quite regular, with deviations from circular of less than 5%,
while two are strikingly elliptical. When the temperatures and luminosities of
our sample are grouped with six other high-redshift measurements, there is no
measured evolution in the luminosity-temperature relation. We identify a number
of X-ray emitting point sources that are potential cluster members. These could
be sources of intracluster medium heating, adding the entropy necessary to
explain the cluster luminosity-temperature relation.
Stadt – Gemeinde – Genossenschaft. Festschrift für Gerhard Dilcher zum 70. Geburtstag
Creators: name: Petersen, Stefan
Publisher: name: Concilium medii aevi
Year: 2021

description: Rezension zu: Stadt – Gemeinde – Genossenschaft. Festschrift für Gerhard Dilcher zum 70. Geburtstag, hg. v. Albrecht Cordes, Joachim Rückert, Reiner Schulze, Berlin 2003. 500 S. – ISBN 3-503-06163-0
description: Concilium medii aevi, Bd. 6 (2003): Concilium medii aevi
Equilibrium Molecular Dynamics Study of Lattice Thermal Conductivity/Conductance of Au-SAM-Au Junctions
Creators: name: Luo, Tengfei
name: Lloyd, John R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: In this paper, equilibrium molecular dynamics simulations were performed on Au-SAM (self-assembly monolayer)-Au junctions. The SAM consisted of alkanedithiol molecules. The out-of-plane (z-direction) thermal conductance and in-plane (x- and y-direction) thermal conductivities were calculated. Simulation finite size effect, gold substrate thickness effect, temperature effect, normal pressure effect, molecule chain length effect and molecule coverage effect on thermal conductivity/conductance were studied. Vibration power spectra of gold atoms in the substrate and sulfur atoms in the SAM were calculated and vibration coupling of these two parts was analyzed. The calculated thermal conductance values of Au-SAM-Au junctions are in the range of experimental data on metal-nonmetal junctions. The temperature dependence of thermal conductance has similar trend to experimental observations. It is concluded that the Au-SAM interface resistance dominates thermal energy transport across the junction, while the substrate is the dominant media in which in-plane thermal energy transport happens.
description: 23 pages, 11 figures, 6 tables, Submitted to Journal of Heat Transfer
title: Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡ÑÑÐ½Ð¸ÐºÐ¾Ð², ÐÐ¸ÐºÑÐ¾Ñ
name: ÐÐµÑÐ°Ð»ÐºÐ¸Ð½Ð°, Ð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: 2022
Subjects: Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ
Ð´Ð°ÑÑÐ¸ÐºÐ¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½
Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð²
Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ¾ÑÐ¼ÑÐ»Ñ Ð¸ ÑÐ°ÑÑÐµÑÑ Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¸Ð·ÑÑÐ°ÑÑÑÑ Ð² ÐºÑÑÑÐµ Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹Â», Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐµ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ð¼Ð¸ Ð² Ð¡ÐÐ±ÐÐ£ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÐ¼Ð¸ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ°Ð¼Ð¸. Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð¿ÑÐ¸ ÑÐ°Ð±Ð¾ÑÐµ Ñ ÑÐ°ÑÑÐµÑÐ½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸ÑÐ¼Ð¸, ÐºÑÑÑÐ¾Ð²ÑÐ¼Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸, Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¼Ð¸ ÑÐ°Ð±Ð¾ÑÐ°Ð¼Ð¸, Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ðº ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐ¼ ÑÐ°Ð±Ð¾ÑÐ°Ð¼, Ð·Ð°ÑÐµÑÐ°Ð¼ Ð¸ ÑÐºÐ·Ð°Ð¼ÐµÐ½Ð°Ð¼. Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð´Ð»Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ 12.03.01 Â«ÐÑÐ¸Ð±Ð¾ÑÐ¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ» Ð¸ 27.03.01 Â«Ð¡ÑÐ°Ð½Ð´Ð°ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¸ Ð¼ÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÂ».
Peter Wolf, Michael Henker, Evamaria Brockhoff, Barbara Steinherr, Stephan Lippold (Hrsg.), Der Winterkönig Friedrich V. Der letzte Kurfürst aus der Oberen Pfalz
Creators: name: Plath, Christian
Publisher: name: Concilium medii aevi
Year: 2021

description: Rezension zu: Peter Wolf, Michael Henker, Evamaria Brockhoff, Barbara Steinherr, Stephan Lippold (Hrsg.), Der Winterkönig Friedrich V. Der letzte Kurfürst aus der Oberen Pfalz. Amberg – Heidelberg – Prag – Den Haag, Katalog zur bayerischen Landesausstellung im Stadtmuseum Amberg 2003 (Veröffentlichungen zur Bayerischen Geschichte und Kultur 46/03), Augsburg 2003, Katalog + 1 CD-Rom
description: Concilium medii aevi, Bd. 6 (2003): Concilium medii aevi
Cross-Lingual Dialogue Dataset Creation via Outline-Based Generation
Creators: name: Majewska, Olga
name: Razumovskaia, Evgeniia
name: Ponti, Edoardo Maria
name: Vulić, Ivan
name: Korhonen, Anna
Publisher: name: arXiv
Year: 2022
Subjects: subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: Multilingual task-oriented dialogue (ToD) facilitates access to services and information for many (communities of) speakers. Nevertheless, the potential of this technology is not fully realised, as current datasets for multilingual ToD - both for modular and end-to-end modelling - suffer from severe limitations. 1) When created from scratch, they are usually small in scale and fail to cover many possible dialogue flows. 2) Translation-based ToD datasets might lack naturalness and cultural specificity in the target language. In this work, to tackle these limitations we propose a novel outline-based annotation process for multilingual ToD datasets, where domain-specific abstract schemata of dialogue are mapped into natural language outlines. These in turn guide the target language annotators in writing a dialogue by providing instructions about each turn's intents and slots. Through this process we annotate a new large-scale dataset for training and evaluation of multilingual and cross-lingual ToD systems. Our Cross-lingual Outline-based Dialogue dataset (termed COD) enables natural language understanding, dialogue state tracking, and end-to-end dialogue modelling and evaluation in 4 diverse languages: Arabic, Indonesian, Russian, and Kiswahili. Qualitative and quantitative analyses of COD versus an equivalent translation-based dataset demonstrate improvements in data quality, unlocked by the outline-based approach. Finally, we benchmark a series of state-of-the-art systems for cross-lingual ToD, setting reference scores for future work and demonstrating that COD prevents over-inflated performance, typically met with prior translation-based ToD datasets.
Explorations of pseudo-Dirac dark matter having keV splittings and interacting via transition electric and magnetic dipole moments
Creators: name: Chatterjee, Shiuli
name: Laha, Ranjan
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study a minimal model of pseudo-Dirac dark matter, interacting through transition electric and magnetic dipole moments. Motivated by the fact that xenon experiments can detect electrons down to $\sim$\,keV recoil energies, we consider $\mathcal{O}$(keV) splittings between the mass eigenstates. We study the production of this dark matter candidate via the freeze-in mechanism. We discuss the direct detection signatures of the model arising from the down-scattering of the heavier state, that are produced in Solar upscattering, finding observable signatures at the current and near-future xenon based direct detection experiments. We also study complementary constraints on the model from fixed target experiments, lepton colliders, supernovae cooling and cosmology. We show that the latest XENONnT results rule out parts of the parameter space for this well motivated and minimal dark matter candidate. Next generation xenon experiments can either discover or further constrain how strongly inelastic dark matter can interact via the dipole moment operators.
description: 50 pages, 14 figures. Updated to include XENONnT results. Matches published version
Radio Polarization Observations of G319.9-0.7: A Bow-shock Nebula with an Azimuthal Magnetic Field Powered by Pulsar J1509-5850
Creators: name: Ng, C. -Y.
name: Gaensler, B. M.
name: Chatterjee, S.
name: Johnston, S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report radio polarization observations of G319.9-0.7 (MSC 319.9-0.7) at 3 and 6 cm obtained with the Australia Telescope Compact Array. The source shows a highly elongated morphology with the energetic pulsar J1509-5850 located at the tip. We found a flat radio spectrum of index α=-0.26 +/- 0.04 and a high degree of linear polarization. These results confirm G319.9-0.7 as a bow-shock pulsar wind nebula. The polarization maps suggest a helical magnetic field trailing the pulsar, with the symmetry axis parallel to the system's inferred direction of motion. This is the first time such a field geometry has been seen in a bow-shock nebula, and it may be the result of an alignment between the pulsar spin axis and its space velocity. Compared to other bow-shock examples, G319.9-0.7 exhibits very different properties in the field structure and surface brightness distribution, illustrating the large diversity of the population.
description: 11 pages, 6 figures, accepted for publication in ApJ
Von Eleganz und Barbarei. Lateinische Grammatik und Stilistik in Renaissance und Barock
Creators: name: Rädle, Fidel
Publisher: name: Concilium medii aevi
Year: 2021

description: Rezension zu: Von Eleganz und Barbarei. Lateinische Grammatik und Stilistik in Renaissance und Barock, hg. von Wolfram Ax (Wolfenbütteler Forschungen Band 95), Harrassowitz Verlag, Wiesbaden 2001
description: Concilium medii aevi, Bd. 6 (2003): Concilium medii aevi
Isolating noise and amplifying signal with quantum Cheshire cat
Creators: name: Ghoshal, Ahana
name: Sau, Soham
name: Das, Debmalya
name: Sen, Ujjwal
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The so-called quantum Cheshire cat is a phenomenon in which an object, identified with a "cat", is dissociated from a property of the object, identified with the "grin" of the cat. We propose a thought experiment, similar to this phenomenon, with an interferometric setup, where a property (a component of polarization) of an object (photon) can be separated from the object itself and can simultaneously be amplified when it is already decoupled from its object. We further show that this setup can be used to dissociate two complementary properties, e.g., two orthogonal components of polarization of a photon and identified with the grin and the snarl of a cat, from each other and one of them can be amplified while being detached from the other. Moreover, we extend the work to a noisy scenario, effected by a spin-orbit-coupling -like additional interaction term in the Hamiltonian for the measurement process, with the object in this scenario being identified with a so-called confused Cheshire cat. We devise a gedanken experiment in which such a "confusion" can be successfully dissociated from the system, and we find that the dissociation helps in the amplification of signals.
description: 10 pages, 3 figures. Published as "Isolating noise and amplifying the signal using weak quantum measurement and postselection"
title: Ð¢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¸Ð»Ð¸Ð½Ð´ÑÂ» Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¶ÑÑÐµÐ³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ½Ð¸ÑÐ¸Ð¼Ð¾Ð², ÐÐ»ÐµÐ³
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ
ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ
Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾

description: Ð Ð¿ÐµÑÐ²Ð¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð¹ Ð´ÐµÑÐ°Ð»Ð¸ âÐ¦Ð¸Ð»Ð¸Ð½Ð´Ñâ, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð²ÑÐ±Ð¾ÑÐ° Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÐµÐµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸, Ð²ÑÐ±Ð¾Ñ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¾ÑÐ½Ð°ÑÑÐºÐ¸, ÑÐ°ÑÑÐµÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð½Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¿Ð¾ÑÑÐ´Ð¾Ðº ÑÐ°ÑÑÐµÑÐ° ÑÐµÐ¶ÑÑÐ¸Ñ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð´Ð»Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð½Ð° Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸ÑÑ: ÑÐ°ÑÐ¾Ð½Ð½ÑÐ¹ Ð´Ð¸ÑÐºÐ¾Ð²ÑÐ¹ ÑÐµÐ·ÐµÑ, ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼ÐµÑÑÐ¸ÐºÐ¾Ð² Ð¸ ÑÐµÑÐ²ÑÑÐ½Ð°Ñ ÑÑÐµÐ·Ð° Ð´Ð»Ñ Ð½Ð°ÑÐµÐ·Ð°Ð½Ð¸Ñ ÑÐ¸Ð»Ð¸Ð½Ð´ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·ÑÐ±ÑÐ°ÑÑÑ ÐºÐ¾Ð»ÐµÑ. Ð ÑÑÐµÑÑÐµÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÑÐ¾Ð´Ð° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸. ÐÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ñ Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð¸ Ð¾ÑÑÐµÐºÐ°ÑÐµÐ»Ñ. Ð¢Ð°ÐºÐ¶Ðµ Ð±ÑÐ» Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð° ÑÐ¸ÐºÐ»Ð¾Ð³ÑÐ°Ð¼Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ ÑÑÐ°Ð½ÐºÐ°.
Additional file 1 of Effects of rapid fluid infusion on hemoglobin concentration: a systematic review and meta-analysis
Creators: name: Quispe-Cornejo, Armin A.
name: Alves da Cunha, Ana L.
name: Njimi, Hassane
name: Mongkolpun, Wasineenart
name: Valle-Martins, Ana L.
name: Arébalo-López, Mónica
name: Creteur, Jacques
name: Vincent, Jean-Louis
Publisher: name: figshare
Year: 2022
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Computational Biology

description: Additional file 1. Online supplementary data.
Die Chroniken Bertholds von Reichenau und Bernolds von Konstanz 1054-1100
Creators: name: Flachenecker, Helmut
Publisher: name: Concilium medii aevi
Year: 2021

description: Rezension zu: Die Chroniken Bertholds von Reichenau und Bernolds von Konstanz 1054-1100, hrsg. von IAN S. ROBINSON (Monumenta Germaniae Historica. Scriptores rerum Germanicarum Nova Series 14). Hannover, Hahnsche Buchhandlung, 2003, 645 S. incl. Namen- und Wortregister
description: Concilium medii aevi, Bd. 6 (2003): Concilium medii aevi