| Literature DB >> 31817077 |
Alexey Lezov1, Alexander Gubarev1, Maria Mikhailova1, Alexandra Lezova1, Nina Mikusheva1, Vladimir Kalganov1, Marina Dudkina2, Andrey Ten'kovtsev2, Tatyana Nekrasova2, Larisa Andreeva2, Natalia Saprykina2, Ruslan Smyslov2,3, Yulia Gorshkova4, Dmitriy Romanov5, Stephanie Höppener6,7, Igor Perevyazko1, Nikolay Tsvetkov1.
Abstract
The interaction of silver nitrate with star-shaped poly(2-ethyl-2-oxazoline) and poly(2-isopropyl-2-oxazoline) containing central thiacalix[4]arene cores, which proceeds under visible light in aqueous solutions at ambient temperature, was studied. It was found that this process led to the formation of stable colloidal solutions of silver nanoparticles. The kinetics of the formation of the nanoparticles was investigated by the observation of a time-dependent increase in the intensity of the plasmon resonance peak that is related to the nanoparticles and appears in the range of 400 to 700 nm. According to the data of electron and X-ray spectroscopy, scanning and transmission electron microscopy, X-ray diffraction analysis, and dynamic light scattering, the radius of the obtained silver nanoparticles is equal to 30 nm. In addition, the flow birefringence experiments showed that solutions of nanoparticles have high optical shear coefficients.Entities:
Keywords: colloidal solution; silver nanoparticles; star-shaped polymer; temperature-responsive polymers
Year: 2019 PMID: 31817077 PMCID: PMC6960741 DOI: 10.3390/polym11122006
Source DB: PubMed Journal: Polymers (Basel) ISSN: 2073-4360 Impact factor: 4.329
Scheme 1Chemical structure of star-PETOX and star-PIPOX macromolecules.
Figure 1(a) Time dependence of optical density normalized to its value measured after 24 h I24 of irradiation obtained for the solution of star-PIPOX (nAg/nS = 11) divided into 2 parts: the first part was kept in the dark (control solution), another one was exposed to the light at λmax = 412 nm. (b) Normalized absorption spectra of star-PETOX and star-PIPOX complexes with Ag nanoparticles at nAg/nS = 0.1.
Figure 2(a) Normalized distributions of equivalent disc radii (Rcirc) in polymer/Ag0 samples obtained by SEM. The inset (b) shows the SEM image of a single particle present in the star-PETOX/Ag0 complex and profile of its width. High resolution TEM images of star-PETOX/Ag0 (c) and star-PIPOX/Ag0 (d) which display the crystalline structure of the obtained nanoparticles.
Hydrodynamic radii Rh obtained by dynamic light scattering (DLS), and Rsf obtained by analytical ultracentrifugation (AUC) of water solutions of star-PETOX and star-PIPOX and their complexes with Ag nanoparticles at 15 °C.
| Sample | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| star-PETOX | 0 | - | 5.3 | 25 | 7.7 * | |||||
| 0.1 | - | 7.9 | 58 | ~1–2 | 10 | 50 | 8.1 | 1.3 | ||
| 1.1 | - | 6.3 | 42 | |||||||
| 11 | - | 3.6 | 19.7/110 | |||||||
| star-PIPOX | 0 | 2.3 | 11 | - | 4.6 * | |||||
| 0.1 | 8.8 | 59 | ~1–2 | 45 | 1.2 | |||||
| 1.1 | 6.6 | 54 | ||||||||
| 11 | 5.4 | 16.3/68 |
* Molar masses of individual star-PETOX and star-PIPOX macromolecules, obtained in tetrahydrofuran solution, where aggregation is absent [15]. The detailed information on velocity sedimentation data is presented in Table S1 (Supplementary Materials).
Figure 3Normalized scattered light intensity versus hydrodynamic radius Rh plots obtained for complexes of silver nanoparticles with star-PETOX (a) and star-PIPOX (b).
Apparent average hydrodynamic radii of complexes (RhCUM) obtained from DLS autocorrelation function at scattering angle θ = 90°, and the corresponding polydispersity indices (PDI).
| Sample | PDICUM | ||
|---|---|---|---|
| Star-PETOX/Ag0 | 0.1 | 49 | 0.65 |
| 1.1 | 45 | 1.30 | |
| 11 | 54 | 1.52 | |
| Star-PIPOX/Ag0 | 0.1 | 49 | 0.70 |
| 1.1 | 35 | 1.20 | |
| 11 | 39 | 2.06 |
Figure 4The sedimentation coefficient distributions of the largest size silver particles stabilized with star-PETOX [nAg/nS = 0.1] (a) and star-PIPOX [nAg/nS = 0.1] (b) obtained at 3000 rpm rotor speed. The distributions were resolved by using c(s) and ls-g*(s) models implemented in Sedfit within a wide concentration range. (c) The distributions of sedimentation coefficients obtained for NP1(1), NP2(2) particles at 3000 rpm stabilized with star-PETOX and star-PETOX (3) distribution itself acquired with the “differential sedimentation” approach. (d) The data obtained for star-PIPOX/NP and star-PIPOX itself with the same approach. The X-axis at (c) and (d) is presented in logarithmic (lg) scale.
Figure 5(a)—SANS curves (dots) for 6 wt % solution of star-PETOX in D2O (blue), 6 wt % solution of star-PETOX/Ag0 in D2O (red), and 6 wt % solution of star-PIPOX/Ag0 in D2O (green) approximated using the Beaucage model (lines) (Equation (S4)); (b)—Kratky (star-PETOX (blue); star-PETOX/Ag0 (red); star-PIPOX/Ag0 (green)), and (c)—Guinier representations of the experimental data (star-PETOX (blue); star-PETOX/Ag0 (red); star-PIPOX/Ag0 (green)), vertical dashed line corresponds to the border of low Q regime (QRg < 1.3), where Rg values were obtained.
Radii of gyration (Rgi) and power indices in the generalized Porod law (ni) obtained by the Beaucage model Equations (S3) and (S4); characteristic dimensions of scattering inhomogeneities in the star-PETOX macromolecules, star-PETOX/Ag0 complexes, and star-PIPOX/Ag0 complexes in D2O (reduced chi squared, χ2).
| System |
|
|
| ||||
|---|---|---|---|---|---|---|---|
| star-PETOX | 7.99 ± 0.13 | 2.84 ± 0.03 | 10.4 | 3.76 ± 0.12 | 1.96 ± 0.08 | 5.34 | 0.8 |
| star-PETOX/Ag⁰ | 9.86 ± 0.17 | 2.72 ± 0.10 | 13.0 | 3.53 ± 0.16 | 1.96 ± 0.14 | 5.02 | 0.5 |
| star-PIPOX/Ag⁰ | 9.54 ± 0.33 | 2.74 ± 0.10 | 12.5 | 4.09 ± 0.29 | 1.99 ± 0.03 | 5.79 | 0.4 |
Figure 6Dependence of birefringence Δn on shear stress Δτ in water solution for star-PIPOX/Ag0 (nAg/nS = 11) (red dots, red approximation line); the solution after centrifugation (9000 rpm for 30 min) (black squares, black approximation line).