cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Conical Intersections, Charge Transfer and Photoisomerization Pathway Selection in a Minimal Model of a Degenerate Monomethine Dye
Creators: name: Olsen, Seth
name: McKenzie, Ross H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We propose a minimal model Hamiltonian for the electronic structure of a monomethine dye, in order to describe the photoisomerization of such dyes. The model describes interactions between three diabatic electronic states, each of which can be associated with a valence bond structure. Monomethine dyes are characterized by a charge-transfer resonance; the indeterminacy of the single-double bonding structure dictated by the resonance is reflected in a duality of photoisomerization pathways corresponding to the different methine bonds. The possible multiplicity of decay channels complicates mechanistic models of the effect of the environment on fluorescent quantum yields, as well as coherent control strategies. We examine the extent and topology of intersection seams between the electronic states of the dye, and how they relate to charge localization and selection between different decay pathways. We find that intersections between the S1 and S0 surfaces only occur for large twist angles. In contrast, S2/S1 intersections can occur near the Franck-Condon region. When the molecule has left-right symmetry, all intersections are associated with con- or dis-rotations and never with single bond twists. For asymmetric molecules (i.e. where the bridge couples more strongly to one end) then the S2 and S1 surfaces bias torsion about different bonds. Charge localization and torsion pathway biasing are correlated. We relate our observations to several recent experimental and theoretical results, which have been obtained for dyes with similar structure.
description: This manuscript is a significant rewrite of an earlier manuscript (arXiv:0906.3914). The current version expands significantly on the previous model. It includes several new figures and the text has been completely rewritten. A shortened version of this manuscript has been accepted for publication in The Journal of Chemical Physics
Octopus australis Gunther, Dallas, Carruthers & Francis, 1885, n. sp.
Creators: name: Gunther, Albert C. L. G.
name: Dallas, William S.
name: Carruthers, William
name: Francis, William
Publisher: name: TAYLOR AND FRANCIS
Year: 1885
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Cephalopoda
Octopoda
Octopodidae
Octopus
Octopus australis

description: Octopus australis, n. sp.
The Body is rounded, and wider behind than in front; depressed, and with a well-marked ventral median groove. The mantle-opening extends nearly halfway round the body. The siphon is of medium size, at first the lateral margins are parallel and then taper rapidly to a blunt point; it ex ­ tends less than halfway to the umbrella-margin.
The Head is narrower than the body, and the eyes some ­ what prominent, dorsally rather than laterally.
The Arms are unequal, the lateral being slightly the longest, and about three times as long as the body; they are slender and tapering. The umbrella is longer than the length of the body, larger ventrally than dorsally, and largest of all laterally. The suckers arc prominent and closely set; they are altogether larger on the lateral arms, and extend in a double row to the centre; the radial grooves are deep and extend quite to the margin. The hectocoty Lus is absent.
The Surface of the back of the body, head, and dorsal aspects of the umbrella and arms is covered with thick-set hemisphe ­ rical pimples, -which are also found on the inner side of the membrane between the two dorsal arms, and on the inner surface of the arms between the suckers; they are smaller and more sparse on the ventral surface of the body. A large rough cirrus and a few larger pimples are found over each eye. A raised ridge passes backwards from the base of the siphon along the ventro-lateral margin of the body, meeting its fellow of the opposite side at the posterior extremity*.
The Colour is deep purplish on the back, mottled on the sides, and cream below.
Hab. Port Jackson, Australia, 6-15 fathoms. Two speci ­ mens, 1 ♀, 1 juv.
description: Published as part of Gunther, Albert C. L. G., Dallas, William S., Carruthers, William & Francis, William, 1885, The Annals and Magazine of Natural History, Including Zoology, Botany, and Geology, pp. 1-96 in Reptiles and Batrachians from Brazil, LONGMANS, GREEN, AND CO.; SIMPKIN, MARSHALL, AND CO.; KENT AND CO.,; WHITT AKER AND CO.: BAILLIERE, PARIS: MACLACHLAN AND STEWART, EDINBURGH: HODGES, FOSTER, AND CO., DUBLIN: AND ASHER, BERLIN :TAYLOR AND FRANCIS on page 224, DOI: 10.5281/zenodo.14926803
REPOPSI Shiny App: Training Materials
Creators: name: Blagojev, Tijana
name: Medić, Duško
Publisher: name: Zenodo
Year: 2023
Subjects: REPOPSI
Shiny
R

description: Slides from an online training session held for the REPOPSI project team on April 28, 2023. The training was dedicated to the development and maintenance of the Shiny app built for searching REPOPSI, the open repository of psychological instruments in Serbian. The slides can also be accessed at https://treningshinyapprepopsi.netlify.app/#/ This upload contains a HTML and a PDF file to view the slides. The R Markdown (.Rmd) file, together with the slike.rar folder, can be used to reproduce the slides in R. The slides are in Serbian. Tijana Blagojev and Duško Medić organized the training and prepared the slides. More information about the Shiny app, together with the open-access code to reproduce it, is available at: https://doi.org/10.5281/zenodo.7934950
description: This project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 101017536 and is supported by the EOSC Future (https://eoscfuture.eu/) through the RDA (https://www.rd-alliance.org/) Open Call mechanism (https://eoscfuture-grants.eu/provider/research-data-alliance), based on evaluations of external, independent experts.
title: ÐÐ»Ð¸ÑÐ½Ð¸Ðµ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð½Ð° Ð´Ð¸Ð·Ð°Ð¹Ð½ Ð´ÐµÑÑÐºÐ¾Ð¹ Ð¸Ð³ÑÑÑÐºÐ¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÑÐµÑÐºÐ¾, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¥ÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð´Ð¸Ð·Ð°Ð¹Ð½
Ð¸Ð³ÑÑÑÐºÐ¸
Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÐºÑÐ¾ÑÑ

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ ÑÑÐµÐ¿ÐµÐ½Ð¸ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð½Ð° Ð´Ð¸Ð·Ð°Ð¹Ð½ Ð´ÐµÑÑÐºÐ¾Ð¹ Ð¸Ð³ÑÑÑÐºÐ¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð´Ð¸Ð·Ð°Ð¹Ð½-ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ Ð´Ð»Ñ Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð° Ð¸Ð³ÑÑÑÐºÐ¸.
BMSSM Implications for Cosmology
Creators: name: Bernal, Nicolas
name: Blum, Kfir
name: Losada, Marta
name: Nir, Yosef
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The addition of non-renormalizable terms involving the Higgs fields to the MSSM (BMSSM) ameliorates the little hierarchy problem of the MSSM. We analyze in detail the two main cosmological issues affected by the BMSSM: dark matter and baryogenesis. The regions for which the relic abundance of the LSP is consistent with WMAP and collider constraints are identified, showing that the bulk region and other previously excluded regions are now permitted. Requiring vacuum stability limits the allowed regions. Based on a two-loop finite temperature effective potential analysis, we show that the electroweak phase transition can be sufficiently first order in regions that for the MSSM are incompatible with the LEP Higgs mass bound, including parameter values of \tanβ\lsim 5, m_{\tilde{t}_{1}} > m_t, m_Q << TeV.
description: 28 pages, 4 figures. References added
title: Ð Ð°ÑÑÐµÑ Ð²Ð¾Ð´Ð½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°Ð±Ð¾ÑÑ ÐºÐ°ÑÐºÐ°Ð´Ð° ÐÐ°ÑÐ°Ð¼Ð°Ð³ÑÐºÐ¸Ñ ÐÐ­Ð¡
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Ð²Ð°ÑÐ¾Ð², ÐÐ¸ÐºÐ¸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: 2017
Subjects: ÐÐ¸Ð´ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð´ÐµÑÐ¸Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ
ÐÐ¸Ð´ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸
Ð²Ð¾Ð´Ð½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐ¶Ð¸Ð¼Ñ
Ð±Ð°ÑÑÐµÐ¹Ð½ ÑÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
Ð¿ÑÐ¸ÑÐ¾ÑÐ½Ð¾ÑÑÑ
ÐºÐ°ÑÐºÐ°Ð´Ñ

description: ÐÐ±ÑÐµÐºÑ ÑÐ°ÑÑÐµÑÐ° - ÐºÐ°ÑÐºÐ°Ð´ ÐÐ°ÑÐ°Ð¼Ð°Ð³ÑÐºÐ¸Ñ ÐÐ­Ð¡, ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ Ð² Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐµ Ð¡ÐµÐ²ÐµÑÐ½Ð°Ñ ÐÑÐµÑÐ¸Ñ - ÐÐ»Ð°Ð½Ð¸Ñ. Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð±Ð°Ð»Ð°Ð½Ñ ÑÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸, Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐºÐ°Ð´Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð³ÑÐ°ÑÐ¸ÐºÐ¾Ð² Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸, Ð°Ð½Ð°Ð»Ð¸Ð· ÐµÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¸ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐºÐ¸ ÐÑÐ´Ð¾Ð½. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°Ð±Ð¾ÑÑ Ð´ÐµÑÐ¸Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð½ÐµÐ»Ñ â 2. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð²Ð¾Ð´Ð½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐ°Ð±Ð¾ÑÑ ÐºÐ°ÑÐºÐ°Ð´Ð°.
Octopus hongkongensis Steenstrup, AIS.
Creators: name: Gunther, Albert C. L. G.
name: Dallas, William S.
name: Carruthers, William
name: Francis, William
Publisher: name: TAYLOR AND FRANCIS
Year: 1885
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Cephalopoda
Octopoda
Octopodidae
Octopus
Octopus hongkongensis

description: Octopus hongkongensis, Steenstrup, AIS.
The Body is rounded, with a median ventral furrow, and depressed (? from pressure). The 'mantle-opening is slightly less than half the circumference, and terminates midway be ­ tween the siphon and the eye, and a little behind the latter. The siphon is comparatively short and conical, and extends one third the distance to the umbrella-margin.
The Head is comparatively broad, almost as broad as the body, and the eyes appear to have been prominent.
* I have considerable doubt whether this be really one of the specific characters; but as it occurs in both specimens, I have thought it well to mention it.
The Anns are unequal, the ventral considerably shorter than the dorsal and dorso-lateral, on an average six times as long as the body, stout and tapering very rapidly towards the ends. The umbrella reaches up one fifth of the length of the dorsal arms, and is a little wider between the lateral and a little narrower between the ventral arms. The suckers are not closely packed and not enlarged on the dorsal arms, notwithstanding the sex of the specimen. The hectocotylized arm is very short, but the modified extremity is long and narrow, with parallel sides tapering only at the extremity to a blunt point; a narrow fillet runs between the two marginal ridges.
The Surface of the body is sprinkled dorsally with minute hemispherical warts, which become smaller and gradually disappear on the sides and lower surface; they are also found on the dorsal surface of the head and of the umbrella. Above each pupil stands a small cirrus, immediately behind which is a larger one.
The Colour is a dull red on the dorsal surface, lighter and brighter below, sprinkled with dull reddish-brown dots.
Hab. The Hyalonema- ground south of Japan, 345 fathoms (Station 232). One specimen, ♂.
description: Published as part of Gunther, Albert C. L. G., Dallas, William S., Carruthers, William & Francis, William, 1885, The Annals and Magazine of Natural History, Including Zoology, Botany, and Geology, pp. 1-96 in Reptiles and Batrachians from Brazil, LONGMANS, GREEN, AND CO.; SIMPKIN, MARSHALL, AND CO.; KENT AND CO.,; WHITT AKER AND CO.: BAILLIERE, PARIS: MACLACHLAN AND STEWART, EDINBURGH: HODGES, FOSTER, AND CO., DUBLIN: AND ASHER, BERLIN :TAYLOR AND FRANCIS on pages 224-225, DOI: 10.5281/zenodo.14926803
title: Ð¤Ð¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð¿ÑÑÐ¸ ÐµÐµ ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð½Ð¸ÐºÐ°ÑÐ¾Ð²Ð°, Ð®Ð»Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ
Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
financial stability
solvency
enterprise

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÑÑÐ½Ð¾ÑÑÑ, Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ¸Ð¿Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÐÐÐ "ÐÐ¾Ð»Ð¾Ð³Ð´Ð°Ð¡ÑÑÐ¾Ð¹ÐÐ°ÐºÐ°Ð·ÑÐ¸Ðº" Ð¿Ð¾ Ð°Ð±ÑÐ¾Ð»ÑÑÐ½ÑÐ¼ Ð¸ Ð¾ÑÐ½Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¼ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÐ¼. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð½Ð° Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÑÑ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÐµÐµ ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ.
description: This paper considers the essence, main types of financial stability. The analysis of financial stability, OOO "Vologdasetremont" in absolute and relative terms. The forecast of financial stability in future and proposed areas to strengthen it.
Additional file 1 of A drug delivery system constructed by a fusion peptide capturing exosomes targets to titanium implants accurately resulting the enhancement of osseointegration peri-implant
Creators: name: Li, Xuewen
name: Liu, Zihao
name: Xu, Shendan
name: Ma, Xinying
name: Zhao, Zhezhe
name: Hu, Han
name: Deng, Jiayin
name: Peng, Cheng
name: Wang, Yonglan
name: Ma, Shiqing
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Figure S1. Pseudo-3D views and the secondary structure prediction of PEP1–3. Figure S2. SEM imaged the surface topography of titanium surface. Figure S3. A) CLSM imaged the distribution of PEP1–3. B) CLSM colocalized DiRlabeled exosomes and FITC-labeled PEP of EXO-PEP1–3. C) the fluorescence intensity was quantitated. Figure S4. Representative ex vivo images of A) PEPs and B) EXO-PEPs in different organs and femurs. Figure S5. Flow cytometry for rhodamine-labeled PEP-exosome complexes to determine the quantity of PEP diafiltrated and un-diafiltrated. Figure S6. A) CCK-8 assay determined most optimum concentration of EXOpep. B) CCK-8 assay determined to the cytotoxicity of different bioactive molecules. C) CCK-8 assay determined to the proliferation of BMSCs cultured on the titanium discs incubated with different treatment after 1, 2, 3, 4, 5, 6 and 7 day culture periods (P < 0.05). D) AO/EB assay determined to the proliferation of BMSCs. E) CLSM determined to the morphology of BMSCs. red: phalloidin; blue, DAPI. Figure S7. A) Characterization and B) quantity analysis of exosome uptake by hBMSCs analyzed by representative confocal microscopic images. Figure S8. A 3D-printed titanium implant (2 mm in thickness，5 mm in lengthen, 4 mm in width) was used to replace the femur bone defection (2 mm in width，5 mm in lengthen, 4 mm in depth) on the rat. Figure S9. Measurement of serum Crea and BUN in rats injected PBS, EXO, EXOPEP and EXO-PEP (UF). Figure S10. The 3D reconstructed models and the section images of bone defect replaced by the implant in coronal, axial and sagittal view. Purple refers bone tissue, green refers titanium implant, yellow refers the contour of bone. Figure S11. Western blot analysis the expression of osteogenesis signal pathway.
Analytic properties of the scattering amplitude and resonances parameters in a meson exchange model
Creators: name: Döring, M.
name: Hanhart, C.
name: Huang, F.
name: Krewald, S.
name: Meißner, U. -G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The analytic properties of scattering amplitudes provide important information. Besides the cuts, the poles and zeros on the different Riemann sheets determine the global behavior of the amplitude on the physical axis. Pole positions and residues allow for a parameterization of resonances in a well-defined way, free of assumptions for the background and energy dependence of the resonance part. This is a necessary condition to relate resonance contributions in different reactions. In the present study, we determine the pole structure of pion-nucleon scattering in an analytic model based on meson exchange. For this, the sheet structure of the amplitude is determined. To show the precision of the resonance extraction and discuss phenomena such as resonance interference, we discuss the S11 amplitude in greater detail.
description: 22 pages, 22 figures
Joule Heating and Anomalous Resistivity in the Solar Corona
Creators: name: Spangler, Steven R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent radioastronomical observations of Faraday rotation in the solar corona can be interpreted as evidence for coronal currents, with values as large as $2.5 \times 10^9$ Amperes (Spangler 2007). These estimates of currents are used to develop a model for Joule heating in the corona. It is assumed that the currents are concentrated in thin current sheets, as suggested by theories of two dimensional magnetohydrodynamic turbulence. The Spitzer result for the resistivity is adopted as a lower limit to the true resistivity. The calculated volumetric heating rate is compared with an independent theoretical estimate by Cranmer et al (2007). This latter estimate accounts for the dynamic and thermodynamic properties of the corona at a heliocentric distance of several solar radii. Our calculated Joule heating rate is less than the Cranmer et al estimate by at least a factor of $3 \times 10^5$. The currents inferred from the observations of Spangler (2007) are not relevant to coronal heating unless the true resistivity is enormously increased relative to the Spitzer value. However, the same model for turbulent current sheets used to calculate the heating rate also gives an electron drift speed which can be comparable to the electron thermal speed, and larger than the ion acoustic speed. It is therefore possible that the coronal current sheets are unstable to current-driven instabilities which produce high levels of waves, enhance the resistivity and thus the heating rate.
description: Submitted to Nonlinear Processes in Geophysics as a contribution from the 7th International Workshop on Nonlinear Waves and Turbulence in Space Plasmas", Beaulieu, France, April 21-25, 2008
title: ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÐ°ÑÑÐ°ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¾Ð¹
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: ÐÐ»ÐµÐ½ÐµÐ², 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: 2016
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ
ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ

description: Ð¦ÐµÐ»ÑÑ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð²Ð°ÐºÑÑÐ¼Ð½ÑÐ¼ Ð´ÐµÐ°ÑÑÐ°ÑÐ¾ÑÐ¾Ð¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð²Ð°ÐºÑÑÐ¼Ð½ÑÐ¼ Ð´ÐµÐ°ÑÑÐ°ÑÐ¾ÑÐ¾Ð¼ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ ÑÐ¾ÐºÑÐ°ÑÐ¸ÑÑ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ¾-ÑÐµÑÑÑÑÑ Ð½Ð° ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð´ÐµÐ°ÑÑÐ°ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸, Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð´ÐµÐ°ÑÑÐ°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¾Ð²Ð°ÑÑ Ð·Ð°ÑÐ¸ÑÑ Ð¾Ñ Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹. ÐÐµÐ°ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ° Ð¾Ð±Ð»Ð°Ð´Ð°ÐµÑ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²Ð¾Ð¼ Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ñ ÑÐ²ÑÐ·ÐµÐ¹, ÑÑÐ¾ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÐµÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð½ÑÑ ÑÐ»Ð¾Ð¶Ð½Ð¾ÑÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ. Ð¡Ð»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÐµÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ñ ÑÐµÐ»ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½ÑÑ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÐ¾Ð² ÑÐµÐ³ÑÐ»ÑÑÐ¾ÑÐ¾Ð².
Octopus tonganus Gunther, Dallas, Carruthers & Francis, 1885, n. sp.
Creators: name: Gunther, Albert C. L. G.
name: Dallas, William S.
name: Carruthers, William
name: Francis, William
Publisher: name: TAYLOR AND FRANCIS
Year: 1885
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Cephalopoda
Octopoda
Octopodidae
Octopus
Octopus tonganus

description: Octopus tonganus, n. sp.
The Body is rounded, depressed, and broader than long, with a marked but shallow median groove on the ventral surface. The mantle-opening extends about one third round the circumference of the body, terminating nearer to the funnel than to the eye. The siphon is short and conical, and extends rather more than halfway to the umbrella-margin.
The Head is small and the eyes prominent.
The Arms are unequal, the order being 3, 2,4, 1; on an average they are nearly ten times as long as the body, and taper gradually to very fine points. The umbrella is very small and slightly narrower dorsally than laterally. The suckers are for the most part small and closely packed, the first four are arranged in a single row; in the male there are four large ones on each lateral arm opposite the margin of the umbrella, beyond which they gradually diminish. The hectocotylus is very minute.
The Surface is in general smooth; the back bears a few small papillae, but owing to the compression of the, specimens it is impossible to make out their exact number. There are three minute cirri over each eye.
The Colour is on the whole grey, paler below; this is due to dark specks sprinkled more or less closely over a creamcoloured ground. One specimen has a purplish patch at either side of the mantle-opening.
Hab. The Reefs, Tongatabu. Three mutilated specimens, 1♂ 2♀.
description: Published as part of Gunther, Albert C. L. G., Dallas, William S., Carruthers, William & Francis, William, 1885, The Annals and Magazine of Natural History, Including Zoology, Botany, and Geology, pp. 1-96 in Reptiles and Batrachians from Brazil, LONGMANS, GREEN, AND CO.; SIMPKIN, MARSHALL, AND CO.; KENT AND CO.,; WHITT AKER AND CO.: BAILLIERE, PARIS: MACLACHLAN AND STEWART, EDINBURGH: HODGES, FOSTER, AND CO., DUBLIN: AND ASHER, BERLIN :TAYLOR AND FRANCIS on pages 225-226, DOI: 10.5281/zenodo.14926803
Higgs Mechanism for Gravitons
Creators: name: Oda, Ichiro
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Just like the vector gauge bosons in the gauge theories, it is now known that gravitons acquire mass in the process of spontaneous symmetry breaking of diffeomorphisms through the condensation of scalar fields. The point is that we should find the gravitational Higgs mechanism such that it results in massive gravity in a flat Minkowski space-time without non-unitary propagating modes. This is usually achieved by including higher-derivative terms in scalars and tuning the cosmological constant to be a negative value in a proper way. Recently, a similar but different gravitational Higgs mechanism has been advocated by Chamseddine and Mukhanov where one can relax the negative cosmological constant to zero or positive one. In this work, we investigate why the non-unitary ghost mode decouples from physical Hilbert space in a general space-time dimension. Moreover, we generalize the model to possess an arbitrary potential and clarify under what conditions the general model exhibits the gravitational Higgs mechanism. By searching for solutions to the conditions, we arrive at two classes of potentials exhibiting gravitational Higgs mechanism. One class includes the model by Chamseddine and Mukhanov in a specific case while the other is completely a new model.
description: 11 pages
Additional file 1 of A comparison of the expression patterns and diagnostic capability of the ncRNAs NEAT1 and miR-34a in non-obstructive azoospermia and severe oligospermia
Creators: name: Salman, Aya
name: Radwan, Abdullah F.
name: Shaker, Olfat G.
name: A., Adel
name: Sayed, Ghadir A.
Publisher: name: figshare
Year: 2025
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Mental Health

description: Supplementary Material 1
Data from "From commensalism to parasitism within a genus-level clade of barnacles"
Creators: name: Watanabe, Hiromi Kayama
name: Uyeno, Daisuke
name: Yamamori, Luna
name: Jimi, Naoto
name: Chen, Chong
Publisher: name: figshare
Year: 2023
Subjects: Evolutionary biology not elsewhere classified

description: Sequence alignments and raw output files of phylogenetic reconstructions in "From commensalism to parasitism within a genus-level clade of barnacles" by Watanabe et al. in Biology Letters.
title: Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°Ðº Ð¾Ð´Ð¸Ð½ Ð¸Ð· ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð°
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Ð±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: 2017
Subjects: ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÑ Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ Ð¡Ð¡Ð¡Ð
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸
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Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ

description: Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð² Ð Ð¤ Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÑÑÐ´Ð° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸. ÐÐ°Ð´Ð°ÑÐ¸: Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¸ ÑÑÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð² Ð Ð¤; Ð²ÑÑÐ²Ð¸ÑÑ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ ÑÑÐµÑÑ Ð² Ð Ð¤; Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹ Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ°Ð½Ñ; Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ ÑÐ¾Ð²Ð¾ÐºÑÐ¿Ð½ÑÐ¹ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð» ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹; ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ ÑÑÐµÑÑ ÑÑÑÐ°Ð½Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð±Ð¾ÑÑ, Ð½Ð°ÑÑÐ½Ð°Ñ Ð½Ð¾Ð²Ð¸Ð·Ð½Ð° Ð±ÑÐ´ÐµÑ Ð·Ð°ÐºÐ»ÑÑÐ°ÑÑÑÑ Ð² Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·ÐµÐ¹ Ð¼ÐµÐ¶Ð´Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸ÑÐ¼Ð¸. ÐÐ¼ÐµÐ½Ð½Ð¾ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¸ Ð¼Ð¾Ð³ÑÑ ÑÑÐ°ÑÑ Ð³Ð»Ð°Ð²Ð½ÑÐ¼ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð¼ Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ°Ð½Ñ. ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÑ Ð Ð¾ÑÑÐ¸Ð¸, Ðº ÑÐ¾Ð¶Ð°Ð»ÐµÐ½Ð¸Ñ, Ð¾ÑÑÑÐ°ÐµÑ Ð¾Ñ ÑÐ°Ð·Ð²Ð¸ÑÑÑ ÑÑÑÐ°Ð½ Ð¼Ð¸ÑÐ°, Ð¸ Ð¸Ð¼ÐµÐ½Ð½Ð¾ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ°Ñ Ð¼Ð¾Ð¶ÐµÑ Ð¾ÐºÐ°Ð·Ð°ÑÑÑÑ Ð·Ð½Ð°ÑÐ¸Ð¼ÑÐ¼ ÑÐ¾Ð»ÐºÐ¾Ð¼ Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ð¸ ÑÑÐ¾Ð¹ Ð½Ð¸ÑÐ¸. ÐÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÑÐ¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ ÑÑÐµÑÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹ Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¸Ñ ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Â«ÐÐ²ÐµÐ·Ð´Ð°-ÑÐ½ÐµÑÐ³ÐµÑÐºÐ¸ÐºÐ¸Â» Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÑÐµÐ¼ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÑÐµÐ¹ Ð¿Ð¾ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÑ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ°Ð½Ñ.
Additional file 1 of Socioeconomic position and the effect of energy labelling on consumer behaviour: a systematic review and meta-analysis
Creators: name: Robinson, Eric
name: Polden, Megan
name: Langfield, Tess
name: Clarke, Katie
name: Calvert, Lara
name: Colombet, Zoé
name: O’Flaherty, Martin
name: Marty, Lucile
name: Tapper, Katy
name: Jones, Andrew
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1. Online supplementary materials.
Self-Organization in a Driven Dissipative Plasma System
Creators: name: Shaikh, Dastgeer
name: Dasgupta, B.
name: Hu, Q.
name: Zank, G. P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Space Physics (physics.space-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We perform a fully self-consistent 3-D numerical simulation for a compressible, dissipative magneto-plasma driven by large-scale perturbations, that contain a fairly broader spectrum of characteristic modes, ranging from largest scales to intermediate scales and down to the smallest scales, where the energy of the system are dissipated by collisional (Ohmic) and viscous dissipations. Additionally, our simulation includes nonlinear interactions amongst a wide range of fluctuations that are initialized with random spectral amplitudes, leading to the cascade of spectral energy in the inertial range spectrum, and takes into account large scale as well as small scale perturbation that may have been induced by the background plasma fluctuations, also the non adiabatic exchange of energy leading to the migration of energy from the energy containing modes or randomly injected energy driven by perturbations and further dissipated by the smaller scales. Besides demonstrating the comparative decays of total energy and dissipation rate of energy, our results show the existence of a perpendicular component of current, thus clearly confirming that the self-organized state is non-force free.
description: Paper is accepted in Journal of Plasma Physics - In Press
Carteriuspongla caliciformis Gunther, Dallas, Carruthers & Francis, 1885, n. sp.
Creators: name: Gunther, Albert C. L. G.
name: Dallas, William S.
name: Carruthers, William
name: Francis, William
Publisher: name: TAYLOR AND FRANCIS
Year: 1885
Subjects: Biodiversity
Taxonomy
Animalia
Carteriuspongla
Carteriuspongla caliciformis

description: Carteriuspongla caliciformis, n. sp.
Specimen dry, thin, shallow, cup-like, with wide undulating brim, short thick stem, and small, erect, proliferous crest in the bottom. Consistence firm. Colour now light grey. Surface arenaceous, uniformly granulated. Pores on the outer and vents on the inner side of the cup among the granulations. Wall almost entirely composed of short-jointed keratose fibre of a sponge-yellow colour, in which there is very little sand, and that chiefly towards the surface, while there is a great deal outside the fibre in the adjoining sarcode. Size of specimen 6 in. across the brim, 1 in. deep in the centre, | in. through the wall in the centre, diminishing towards the circumference.
Hab. Marine.
Loc. Port Phillip Heads, South Australia. Depth?
Obs. The pores being in the dermal incrustation outside, while the vents are immediately opposite, in the dermal incrustation of the cup inside, causes the wall, when the incrustations on both sides are washed off, to present a sievelike. structure.
description: Published as part of Gunther, Albert C. L. G., Dallas, William S., Carruthers, William & Francis, William, 1885, The Annals and Magazine of Natural History, Including Zoology, Botany, and Geology, pp. 1-96 in Reptiles and Batrachians from Brazil, LONGMANS, GREEN, AND CO.; SIMPKIN, MARSHALL, AND CO.; KENT AND CO.,; WHITT AKER AND CO.: BAILLIERE, PARIS: MACLACHLAN AND STEWART, EDINBURGH: HODGES, FOSTER, AND CO., DUBLIN: AND ASHER, BERLIN :TAYLOR AND FRANCIS on pages 221-222, DOI: 10.5281/zenodo.14926803
Reimagining the Child Development Theory-Practice Gap in the Australian Early Childhood Education Sector
Creators: name: ELLIS, EMMA LOUISE
Publisher: name: Monash University
Year: 2023
Subjects: Teacher education and professional development of educators
Early childhood education
Educational psychology

description: In light of claims that early childhood educators lack sufficient knowledge of child development, this thesis explores the alleged child development theory-practice gap in the Australian early childhood education sector. Studies investigate the teaching, discussion, and use of theories of child development for university lecturers, early career preschool teachers, and teacher mentors. Contrary to the image of the gap being portrayed as problematic, findings suggest it is not necessarily conceived as a problem by those interviewed and striving to close the gap may be impossible. Rather than a ‘chronic problem’, this thesis reimagines the gap as an unavoidable development opportunity.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "Baby Hit")
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ°Ð»ÑÑÐ¸Ðº, Ð­Ð´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: 2017
Subjects: ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸
ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ°Ñ Ð¾ÑÐµÐ½ÐºÐ°
ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑ

description: ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÐ¸Ðµ ÑÐµÐºÑÑÐµÐµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð² Ð¿ÐµÑÐ¸Ð¾Ð´Ðµ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ½ÐºÐ° Ð´ÐµÑÑÐºÐ¸Ñ Ð¸ Ð¿Ð¾Ð´ÑÐ¾ÑÑÐºÐ¾Ð²ÑÑ ÑÐ¾Ð²Ð°ÑÐ¾Ð², Ð² ÑÐ¾Ð´Ðµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð±ÑÐ» Ð²ÑÑÐ²Ð»ÐµÐ½ Ð¿ÑÐ¸Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½ÑÐ¹ Ð´Ð»Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÐ³Ð¼ÐµÐ½Ñ - Ð´ÐµÑÑÐºÐ°Ñ Ð¸ Ð¿Ð¾Ð´ÑÐ¾ÑÑÐºÐ¾Ð²Ð°Ñ Ð¾Ð´ÐµÐ¶Ð´Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾ - ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· 4 Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð², Ñ ÑÐµÐ»ÑÑ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð´Ð»Ñ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ³Ð¾ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð²ÑÑÐ¾Ð´Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð½Ð° ÑÑÐ½Ð¾Ðº Ð¸ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ.
Impact of granulation effects on the use of Balmer lines as temperature indicators
Creators: name: Ludwig, H. -G.
name: Behara, N. T.
name: Steffen, M.
name: Bonifacio, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Balmer lines serve as important indicators of stellar effective temperatures in late-type stellar spectra. One of their modelling uncertainties is the influence of convective flows on their shape. We aim to characterize the influence of convection on the wings of Balmer lines. We perform a differential comparison of synthetic Balmer line profiles obtained from 3D hydrodynamical model atmospheres and 1D hydrostatic standard ones. The model parameters are appropriate for F,G,K dwarf and subgiant stars of metallicity ranging from solar to 1/1000 solar. The shape of the Balmer lines predicted by 3D models can never be exactly reproduced by a 1D model, irrespective of its effective temperature. We introduce the concept of a 3D temperature correction, as the effective temperature difference between a 3D model and a 1D model which provides the closest match to the 3D profile. The temperature correction is different for the different members of the Balmer series and depends on the adopted mixing-length parameter in the 1D model. Among the investigated models, the 3D correction ranges from -300K to +300K. Horizontal temperature fluctuations tend to reduce the 3D correction. Accurate effective temperatures cannot be derived from the wings of Balmer lines, unless the effects of convection are properly accounted for. The 3D models offer a physically well justified way of doing so. The use of 1D models treating convection with the mixing-length theory do not appear to be suitable for this purpose. In particular, there are indications that it is not possible to determine a single value of the mixing-length parameter which will optimally reproduce the Balmer lines for any choice of atmospheric parameters.
description: 6 pages, 3 figures, accepted for publication in A&A
title: ÐÐ±Ð·Ð¾Ñ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°ÐµÐºÑÐ¾ÑÐ¸Ð¸ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ ÐÐÐ Ð² ÑÑÐµÐ´Ðµ Ñ Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸ÑÐ¼Ð¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÑÐ±ÐµÐ², ÐÐ½ÑÐ¾Ð½
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ÐÐ
Ð¼ÑÐ»ÑÑÐºÐ¾Ð¿ÑÐµÑ
Ð¾Ð±Ð»ÐµÑ Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ð¹
RRT*
ROS

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Ð¾Ð±Ð»ÐµÑÐ° Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ð¹ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½ÑÐ¼ Ð»ÐµÑÐ°ÑÐµÐ»ÑÐ½ÑÐ¼ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ¾Ð¼.
Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ â ÑÑÐ°Ð²Ð½Ð¸ÑÑ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¾Ð±Ð»ÐµÑÐ° Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ð¹ ÐÐÐ Ð² ÑÐµÐ°Ð»ÑÐ½Ð¾Ð¼ Ð²ÑÐµÐ¼ÐµÐ½Ð¸.
Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¾ÑÑ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¸ Ð²ÑÐ±Ð¾Ñ Ð»ÑÑÑÐ¸Ñ Ð¿Ð¾ ÐºÑÐ¸ÑÐµÑÐ¸ÑÐ¼ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸, ÑÐºÐ¾ÑÐ¾ÑÑÐ¸, ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° ÑÑÐµÐ¿ÐµÐ½ÐµÐ¹ ÑÐ²Ð¾Ð±Ð¾Ð´Ñ Ð¸ ÑÐ»Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼ RRT* Ð±ÑÐ» Ð¼Ð¾Ð´Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½. ÐÑÐ±ÑÐ°Ð½Ð½ÑÐµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Ð±ÑÐ»Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ñ Ð² ÑÑÐµÐ´Ðµ ROS.
Additional file 1 of Comparative analysis of large language models on rare disease identification
Creators: name: Ao, Guangyu
name: Chen, Min
name: Li, Jing
name: Nie, Huibing
name: Zhang, Lei
name: Chen, Zejun
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Information Systems not elsewhere classified
subject: Cancer

description: Additional file 1.
Dysidea chaliniformis Gunther, Dallas, Carruthers & Francis, 1885, n. sp.
Creators: name: Gunther, Albert C. L. G.
name: Dallas, William S.
name: Carruthers, William
name: Francis, William
Publisher: name: TAYLOR AND FRANCIS
Year: 1885
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Demospongiae
Dictyoceratida
Dysideidae
Dysidea
Dysidea chaliniformis

description: 4. Dysidea chaliniformis, n. sp.
Caulescent, branched, stipitatc; consisting of a compressed bunch of solid cylindrical stalks rising from a common stem; branches numerous, small and simple below, some not more than⅛ in. in thickness, ending in a sharp point, which is sometimes bifurcated; increasing in size upwards, dividing and interuniting; the whole most irregularly. Consistence light, fragile, compressible. Colour reddish brown. Surface even, but minutely wrinkled from the sinking of the dermal pore-membrane upon the subjacent arenated fibre. Pores plentifully scattered throughout the dermal membrane. Vents also numerous, scattered over the flattened portions of the branches or in a line along them. Structure fibrous, fibre arenated throughout; texture fine. Size of specimen about 12 in. long by 5 x 1 in. horizontally. Great diversity in the size of the branches, of which the largest and longest are ¼ in. in diameter, while the smallest do not exceed yof an inch.
Hab. Marine.
Loc. Port Phillip Heads, South Australia. Depth 19fath.
Obs. The caulescent character of this species, together with the solid, cylindrical, simple, and subdivided condition of the branches and the arrangement of their vents, would, at first sight, lead to the supposition that it was a specimen of Chalina polijehotoma, Esper,= Chalina oenlata, Bk., such is the tendency, as before stated, of the sponge-sarcode throughout the class to produce the same kind of forms whatever the composition may be; so that here, although the form is like that of a caulescent Chalina, the characteristic toughness and resiliency of the latter, which arises from the presence of a large amount of keratine, is absent in Dysidea, chaliniformis, where the opposite state renders it so brittle that, when wet, it is almost impossible to handle the specimen without a piece coming off, and in drying it breaks down under the slightest force.
There is another chaliniform specimen in the collection, but here the increased development of keratine, of which the lateral fibre is exclusively composed, not only lessens the amount of brittleness, but necessitates its being relegated to another genus, in which it will be found hereafter.
description: Published as part of Gunther, Albert C. L. G., Dallas, William S., Carruthers, William & Francis, William, 1885, The Annals and Magazine of Natural History, Including Zoology, Botany, and Geology, pp. 1-96 in Reptiles and Batrachians from Brazil, LONGMANS, GREEN, AND CO.; SIMPKIN, MARSHALL, AND CO.; KENT AND CO.,; WHITT AKER AND CO.: BAILLIERE, PARIS: MACLACHLAN AND STEWART, EDINBURGH: HODGES, FOSTER, AND CO., DUBLIN: AND ASHER, BERLIN :TAYLOR AND FRANCIS on pages 217-218, DOI: 10.5281/zenodo.14926803
Tsallis' deformation parameter q quantifies the classical-quantum transition
Creators: name: Kowalski, A. M.
name: Martin, M. T.
name: Plastino, A.
name: Zunino, L.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We investigate the classical limit of a type of semiclassical evolution, the pertinent system representing the interaction between matter and a given field. On using as a quantifier of the ensuing dynamics Tsallis q-entropy, we encounter that it not only appropriately describes the quantum-classical transition, but that the associated deformation-parameter q itself characterizes the different regimes involved in the process, detecting the most salient fine details of the changeover.
description: 19 pages, 7 figures
title: Ð­Ð»ÐµÐºÑÑÐ¾Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð°Ñ ÑÐ¾Ð²Ð¼ÐµÑÑÐ¸Ð¼Ð¾ÑÑÑ ÑÐ°Ð´Ð¸Ð¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 16.04.01 "Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°"
titleType: Subtitle
Creators: name: ÐÐ²ÐµÑÐ¸ÑÑÐ½, ÐÐ°Ð°Ð½
name: ÐÐ°ÐºÐ°ÑÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐ°Ð²ÑÑÐ»Ð¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: Ð Ð°Ð´Ð¸Ð¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÐ¾Ð½ÑÑÐ¾Ð»Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸ÑÂ». ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 19.03.04 Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸ÑÂ». ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·ÐµÐ½ Ð´Ð»Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð², ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÐ¸ÑÑÑ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ, Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°ÑÑÐ½ÑÐ¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑÐ¼ 05.18.15 Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ ÑÐ¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¿Ð¸ÑÐµÐ²ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ Ð¸ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸ÑÂ», 05.18.07 Â«ÐÐ¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿Ð¸ÑÐµÐ²ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² Ð¸ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ²Â».
Towards the Properties of Long Gamma-Ray Burst Progenitors with Swift Data
Creators: name: Cui, Xiao-Hong
name: Liang, En-Wei
name: Lv, Hou-Jun
name: Zhang, Bin-Bin
name: Xu, Ren-Xin
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We investigate the properties of both the prompt and X-ray afterglows of gamma-ray bursts (GRBs) in the burst frame with a sample of 33 Swift GRBs. Assuming that the steep decay segment in the canonical X-ray afterglow lightcurves is due to the curvature effect, we fit the lightcurves with a broken power-law to derive the zero time of the last emission epoch of the prompt emission (t1) and the beginning as well as the end time of the shallow decay segment (t2 and t3).We show that both the isotropic peak gamma-ray luminosity and gamma-ray energy are correlated with the isotropic X-ray energy of the shallow decay phase and the isotropic X-ray luminosity at t2. We infer the properties of the progenitor stars based on a model proposed by Kumar et al. who suggested that both the prompt gamma-rays and the X-ray afterglows are due to the accretions of different layers of materials of the GRB progenitor star by a central black hole (BH). We find that most of the derived masses of the core layers are 0.1-5 solar mass with a radius of 10^8-10^10 cm. The rotation parameter is correlated with the burst duration, being consistent with the expectation of collapsar models. The estimated radii and the masses of the fall-back materials for the envelope layers are 10^10-10^12 cm and 10^-3~1 solar mass, respectively. The average accretion rates in the shallow decay phase are correlated with those in the prompt gamma-ray phase, but they are much lower. The derived radii of the envelope are smaller than the photospheric radii of Wolf-Rayet (WR) stars. It is interesting that the assembled mass density profile for the bursts in our sample is also well consistent with the simulation for a pre-supernova star with 25 solar mass.
description: 12 pages in MNRAS two-column style, 8 figures, 3 tables, accepted for publication in MNRAS