UV-Irradiation-Induced Templated/In-Situ Formation of Ultrafine Silver/Polymer Hybrid Nanoparticles as Antibacterial

Langmuir ◽  
2013 ◽  
Vol 29 (51) ◽  
pp. 16018-16024 ◽  
Author(s):  
Mengjun Chen ◽  
Yining Zhao ◽  
Wantai Yang ◽  
Meizhen Yin
Keyword(s):  
Uv Irradiation ◽  
Hybrid Nanoparticles ◽  
Polymer Hybrid ◽  
In Situ Formation

Core-Shell Magnesium Hydroxide/Polymermer Nanoparticles Prepared by In Situ Emulsion Copolymerization

2011 ◽  
Vol 233-235 ◽  
pp. 2125-2128
Author(s):  
Li Li Xu ◽  
Sheng Peng Liu ◽  
Xuan Li
Keyword(s):  
Magnesium Hydroxide ◽  
Chemical Structure ◽  
Hybrid Nanoparticles ◽  
Core Shell ◽  
Polymer Shell ◽  
Emulsion Copolymerization ◽  
The Core ◽  
Polymer Hybrid ◽  
Transmission Electron

In this paper, vinylated magnesium hydroxide (MH) nanosheets were prepared with 3-(trimethoxysilyl) propyl methacrylate (γ-MPS) and pristine MH nanosheets, then the MH/polymer hybrid nanoparticles were prepared by in-situ emulsion copolymerization of vinylated MH nanosheets and styrene (St) monomer and styrene/butyl acrylate (St/BA) comonomer. The morphology, thermal stability and chemical structure of the final products were investigated in detail with transmission electron microscopy (TEM), thermogravimetric analysis (TGA) and Fourier-transform infrared spectra (FTIR). The TEM results showed that the core-shell structure of MH/Polymer nanoparticles with MH-cores and Polymer-shell was formed.

In Situ Formation of Ag Nanoparticles in Spherical Polyacrylic Acid Brushes by UV Irradiation

2007 ◽  
Vol 111 (21) ◽  
pp. 7676-7681 ◽  
Author(s):  
Yan Lu ◽  
Yu Mei ◽  
Marc Schrinner ◽  
Matthias Ballauff ◽  
Michael W. Möller ◽  
...  
Keyword(s):  
Uv Irradiation ◽  
Polyacrylic Acid ◽  
Ag Nanoparticles ◽  
In Situ Formation

Solid Lipid–Polymer Hybrid Nanoparticles by In Situ Conjugation for Oral Delivery of Astaxanthin

2018 ◽  
Vol 66 (36) ◽  
pp. 9473-9480 ◽  
Author(s):  
Taoran Wang ◽  
Qiaobin Hu ◽  
Ji-Young Lee ◽  
Yangchao Luo
Keyword(s):  
Oral Delivery ◽  
Hybrid Nanoparticles ◽  
Solid Lipid ◽  
Polymer Hybrid

scholarly journals Formation of compact systems of super-Earths via dynamical instabilities and giant impacts

2019 ◽  
Vol 491 (4) ◽  
pp. 5595-5620 ◽  
Author(s):  
Sanson T S Poon ◽  
Richard P Nelson ◽  
Seth A Jacobson ◽  
Alessandro Morbidelli
Keyword(s):  
Initial Conditions ◽  
Post Processing ◽  
Significant Modification ◽  
Kepler Mission ◽  
Giant Impacts ◽  
Low Mass ◽  
In Situ Formation ◽  
Dynamical Instabilities ◽  
Gaseous Envelopes

ABSTRACT The NASA’s Kepler mission discovered ∼700 planets in multiplanet systems containing three or more transiting bodies, many of which are super-Earths and mini-Neptunes in compact configurations. Using N-body simulations, we examine the in situ, final stage assembly of multiplanet systems via the collisional accretion of protoplanets. Our initial conditions are constructed using a subset of the Kepler five-planet systems as templates. Two different prescriptions for treating planetary collisions are adopted. The simulations address numerous questions: Do the results depend on the accretion prescription?; do the resulting systems resemble the Kepler systems, and do they reproduce the observed distribution of planetary multiplicities when synthetically observed?; do collisions lead to significant modification of protoplanet compositions, or to stripping of gaseous envelopes?; do the eccentricity distributions agree with those inferred for the Kepler planets? We find that the accretion prescription is unimportant in determining the outcomes. The final planetary systems look broadly similar to the Kepler templates adopted, but the observed distributions of planetary multiplicities or eccentricities are not reproduced, because scattering does not excite the systems sufficiently. In addition, we find that ∼1 per cent of our final systems contain a co-orbital planet pair in horseshoe or tadpole orbits. Post-processing the collision outcomes suggests that they would not significantly change the ice fractions of initially ice-rich protoplanets, but significant stripping of gaseous envelopes appears likely. Hence, it may be difficult to reconcile the observation that many low-mass Kepler planets have H/He envelopes with an in situ formation scenario that involves giant impacts after dispersal of the gas disc.

Lipid-polymer hybrid nanoparticles: Synthesis strategies and biomedical applications

2019 ◽  
Vol 160 ◽  
pp. 130-142 ◽  
Author(s):  
Vivek Dave ◽  
Kajal Tak ◽  
Amit Sohgaura ◽  
Ashish Gupta ◽  
Veera Sadhu ◽  
...  
Keyword(s):  
Biomedical Applications ◽  
Hybrid Nanoparticles ◽  
Polymer Hybrid ◽  
Nanoparticles Synthesis

scholarly journals Method for determining the thermal conductivity of in situ formation rock using drilling cuttings

AIP Advances ◽  
2021 ◽  
Vol 11 (6) ◽  
pp. 065015
Author(s):  
Fu Yi ◽  
Xupeng Qi ◽  
Xuexin Zheng ◽  
Huize Yu ◽  
Wenming Bai ◽  
...  
Keyword(s):  
Thermal Conductivity ◽  
In Situ Formation
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