| Literature DB >> 32558982 |
Ming Luo1,2, Mingjun Xuan2,3, Shuaidong Huo2, Jilin Fan2,3, Gurudas Chakraborty2,3, Yixi Wang1, Hui Zhao1,4, Andreas Herrmann2,3, Lifei Zheng2,3.
Abstract
Organization of gold nanoobjects by oligonucleotides has resulted in many three-dimensional colloidal assemblies with diverse size, shape, and complexity; nonetheless, autonomous and temporal control during formation remains challenging. In contrast, living systems temporally and spatially self-regulate formation of functional structures by internally orchestrating assembly and disassembly kinetics of dissipative biomacromolecular networks. We present a novel approach for fabricating four-dimensional gold nanostructures by adding an additional dimension: time. The dissipative character of our system is achieved using exonuclease III digestion of deoxyribonucleic acid (DNA) fuel as an energy-dissipating pathway. Temporal control over amorphous clusters composed of spherical gold nanoparticles (AuNPs) and well-defined core-satellite structures from gold nanorods (AuNRs) and AuNPs is demonstrated. Furthermore, the high specificity of DNA hybridization allowed us to demonstrate selective activation of the evolution of multiple architectures of higher complexity in a single mixture containing small and larger spherical AuNPs and AuNRs.Entities:
Keywords: DNA; dissipative assembly; gold; nanoparticles; nanorods
Year: 2020 PMID: 32558982 PMCID: PMC7540408 DOI: 10.1002/anie.202007616
Source DB: PubMed Journal: Angew Chem Int Ed Engl ISSN: 1433-7851 Impact factor: 15.336
Figure 1Representation of the dissipative clustering of spherical AuNPs using a DNA strand as the fuel and Exo III as the energy‐dissipating element. DNA hybridization and the associated fuel strand digestion act as antagonistic processes to induce the assembly and disassembly of AuNPs, respectively.
Figure 2a) Gel electrophoretic analysis of fuel strand digestion by Exo III under non‐dissipative conditions. DNA 1 and 2 represent the sequences that will be attached to gold while DNA 3 represents the fuel strand (★: another portion of the fuel DNA 3 was added to the digested solution). b) UV/Vis absorption spectra measured every 5 min after the addition of fuel DNA (0.04 nmol) in the presence of 8 U μL−1 enzyme. c) DLS measurements under the described conditions. d) TEM images acquired before and after the addition of fuel DNA (0.04 nmol) at 10 and 25 min in the presence of 8 U μL−1 enzyme; scale bar=100 nm.
Figure 3a) Recovery time for different cycles in the presence of 2, 4, 6, and 8 U μL−1 enzyme. b) Linear relationship between recovery time and the amount of fuel DNA (0.04, 0.08, 0.12, and 0.16 nmol) in the presence of 6 U μL−1 enzyme. c) Change of wavelength at the absorption maximum after sequential addition of the fuel DNA in the presence of 8 U μL−1 enzyme. d) Absorbance at 522 nm after sequential addition of the fuel DNA in the presence of 8 U μL−1 enzyme.
Figure 4a) Representation of the structural evolution of the dissipative assembly of core–satellite architectures between 15‐AuNPs and AuNRs. b) Time‐dependent average number of 15‐AuNPs assembled on AuNRs in the presence of 2 U μL−1 Exo‐III. Average numbers for each time point were calculated for 68–82 aggregates from 16–21 TEM images. c) TEM studies on the structural evolution of core–satellite architectures; scale bars=100 nm.
Figure 5a) Representation of the consecutive structural evolution of dissipatively assembled core–satellite architectures involving 15‐AuNPs, 55‐AuNPs, and AuNRs. b) Time‐dependent average number of 15‐AuNPs assembled on AuNRs and spherical 55‐AuNPs in the presence of 3 U μL−1 Exo‐III. Average numbers for each time point were calculated for 35–43 aggregates from 12–16 TEM images. c) TEM studies showing the consecutive structural evolution of dissipative core–satellites activated by the sequential addition of two fuel DNA sequences; scale bars=100 nm.