64 research outputs found

    Development of a “Universal” Phantom for Standardization of Chemical Exchange Saturation Transfer (CEST) MRI

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    https://openworks.mdanderson.org/sumexp22/1039/thumbnail.jp

    From carbon nanotubes and silicate layers to graphene platelets for polymer nanocomposites

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    In spite of extensive studies conducted on carbon nanotubes and silicate layers for their polymer-based nanocomposites, the rise of graphene now provides a more promising candidate due to its exceptionally high mechanical performance and electrical and thermal conductivities. The present study developed a facile approach to fabricate epoxy–graphene nanocomposites by thermally expanding a commercial product followed by ultrasonication and solution-compounding with epoxy, and investigated their morphologies, mechanical properties, electrical conductivity and thermal mechanical behaviour. Graphene platelets (GnPs) of 3.5

    Structure-Based Peptide Inhibitor Design of Amyloid-β Aggregation

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    Many human neurodegenerative diseases are associated with amyloid fibril formation. Inhibition of amyloid formation is of importance for therapeutics of the related diseases. However, the development of selective potent amyloid inhibitors remains challenging. Here based on the structures of amyloid β (Aβ) fibrils and their amyloid-forming segments, we designed a series of peptide inhibitors using RosettaDesign. We further utilized a chemical scaffold to constrain the designed peptides into β-strand conformation, which significantly improves the potency of the inhibitors against Aβ aggregation and toxicity. Furthermore, we show that by targeting different Aβ segments, the designed peptide inhibitors can selectively recognize different species of Aβ. Our study developed an approach that combines the structure-based rational design with chemical modification for the development of amyloid inhibitors, which could be applied to the development of therapeutics for different amyloid-related diseases

    Sandage-Loeb test for the new agegraphic and Ricci dark energy models

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    The Sandage-Loeb (SL) test is a unique method to explore dark energy at the ``redshift desert'' (2≲z≲52\lesssim z\lesssim 5), an era not covered by any other dark energy probes, by directly measuring the temporal variation of the redshift of quasar (QSO) Lyman-α\alpha absorption lines. In this paper, we study the prospects for constraining the new agegraphic dark energy (NADE) model and the Ricci dark energy (RDE) model with the SL test. We show that, assuming only a ten-year survey, the SL test can constrain these two models with high significance.Comment: 14 pages, 5 figures; version for publication in Phys.Lett.

    Theoretical Limits on Agegraphic Quintessence from Weak Gravity Conjecture

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    In this paper, we investigate the possible theoretical constraint on the parameter nn of the agegraphic quintessence model by considering the requirement of the weak gravity conjecture that the variation of the quintessence scalar field ϕ\phi should be less than the Planck mass MpM_{\rm{p}}. We obtain the theoretical upper bound n≲2.5n\lesssim 2.5 that is inconsistent with the current observational constraint result 2.637<n<2.9832.637<n<2.983 (95.4% CL). The possible implications of the tension between observational and theoretical constraint results are discussed.Comment: 14 pages, 3 figure

    A more general interacting model of holographic dark energy

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    So far, there have been no theories or observational data that deny the presence of interaction between dark energy and dark matter. We extend naturally the holographic dark energy (HDE) model, proposed by Granda and Oliveros, in which the dark energy density includes not only the square of the Hubble scale, but also the time derivative of the Hubble scale to the case with interaction and the analytic forms for the cosmic parameters are obtained under the specific boundary conditions. The various behaviors concerning the cosmic expansion depend on the introduced numerical parameters which are also constrained. The more general interacting model inherits the features of the previous ones of HDE, keeping the consistency of the theory.Comment: 7 pages, 8 figures, references adde

    Photochemical origin of SiC2_2 in the circumstellar envelope of carbon-rich AGB stars revealed by ALMA

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    Whether SiC2_2 is a parent species, that is formed in the photosphere or as a by-product of high-temperature dust formation, or a daughter species, formed in a chemistry driven by the photodestruction of parent species in the outer envelope, has been debated for a long time. Here, we analyze the ALMA observations of four SiC2_2 transitions in the CSEs of three C-rich AGB stars (AI Vol, II Lup, and RAFGL 4211), and found that SiC2_2 exhibits an annular, shell-like distribution in these targets, suggesting that SiC2_2 can be a daughter species in the CSEs of carbon-rich AGB stars. The results can provide important references for future chemical models.Comment: Accepted in Frontiers in Astronomy and Space Science
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