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In most of the existing SMA constitutive models, it is assumed that transformation starts when a thermodynamic driving force reaches a specified amount regardless of loading history. In this work, a phenomenological approach is used to develop an enhanced one-dimensional constitutive model in which loading history is directly considered as one of the main parameters affecting the transformation start conditions. To generalize the model to three-dimensional cases, a microplane formulation based on volumetric-deviatoric is employed. A free energy potential is defined at the microplane level, integrated over all orientations at a material point to provide the macroscopic free energy. Experiments are carried out on Nitinol superelastic tubes to validate the newly proposed constitutive model. In these experiments, interruptions are applied during transformations to show the effects of loading history on transformation start conditions. Numerical results are compared with the experimental data to demonstrate the accuracy of the enhanced model.
A multilayer film of TiClx, model Ziegler−Natta catalyst for stereospecific polymerization, was produced by electron beam-induced deposition of TiCl4 on an Au substrate at 100 K. The deposition of solid-phase TiClx took place by dissociation of TiCl4 adsorbed at the substrate surface by electronsboth primary and secondary. The deposition kinetics, surface composition, and structure were studied with X-ray photoelectron spectroscopy and temperature-programmed desorption. Its polymerization stereochemistry was studied by analyzing the polypropylene products with infrared spectroscopy and atomic force microscopy. The deposited film was stable at temperatures lower than 450 K and had a high concentration of chemisorbed TiCl4 species. The film surface was composed of mostly a nonbasal plane (defective) structure. When activated by reactions with Al(C2H5)3, the TiClx film selectively produced isotactic polypropylene. The absence of atactic polypropylene was due to the lack of TiClx sites with the basal plane structure, caused by the deposition method involving high-energy electrons and low substrate temperature.
ADVERTISEMENT RETURN TO ISSUEPREVArticleNEXTDivalent lanthanide chemistry. Preparation and crystal structures of sodium tris[bis(trimethylsilyl)amido]europate(II) and sodium tris[bis(trimethylsilyl)amido]ytterbate(II), NaM[N(SiMe3)2]3T. Don Tilley, Richard A. Andersen, and Allan ZalkinCite this: Inorg. Chem. 1984, 23, 15, 2271–2276Publication Date (Print):July 1, 1984Publication History Published online1 May 2002Published inissue 1 July 1984https://pubs.acs.org/doi/10.1021/ic00183a013https://doi.org/10.1021/ic00183a013research-articleACS PublicationsRequest reuse permissionsArticle Views738Altmetric-Citations140LEARN ABOUT THESE METRICSArticle Views are the COUNTER-compliant sum of full text article downloads since November 2008 (both PDF and HTML) across all institutions and individuals. These metrics are regularly updated to reflect usage leading up to the last few days.Citations are the number of other articles citing this article, calculated by Crossref and updated daily. Find more information about Crossref citation counts.The Altmetric Attention Score is a quantitative measure of the attention that a research article has received online. Clicking on the donut icon will load a page at altmetric.com with additional details about the score and the social media presence for the given article. Find more information on the Altmetric Attention Score and how the score is calculated. Share Add toView InAdd Full Text with ReferenceAdd Description ExportRISCitationCitation and abstractCitation and referencesMore Options Share onFacebookTwitterWechatLinked InRedditEmail Other access optionsGet e-AlertscloseSupporting Info (1)»Supporting Information Supporting Information Get e-Alerts
The majority of Type II-plateau supernovae (SNe IIP) have light curves that are not compatible with the explosions of stars in a vacuum; instead, the light curves require the progenitors to be embedded in circumstellar matter (CSM). We report on the successful fitting of the well-observed SN IIP 2021yja as a core-collapse explosion of a massive star with an initial mass of ~15 Msun and a pre-explosion radius of 631 Rsun. To explain the early-time behaviour of the broad-band light curves, the presence of 0.55 Msun CSM within ~2x10^14 cm is needed. Like many other SNe IIP, SN 2021yja exhibits an early-time flux excess including ultraviolet wavelengths. This, together with the short rise time (<2 days) in the gri bands, indicates the presence of a compact component in the CSM, essentially adjacent to the progenitor. We discuss the origin of the pre-existing CSM, which is most likely a common property of highly convective red supergiant envelopes. We argue that the difficulty in fitting the entire light curve with one spherical distribution indicates that the CSM around the SN 2021yja progenitor was asymmetric.