| Literature DB >> 28773393 |
Anna Dzimitrowicz1, Piotr Jamroz2, Marcin Nyk3, Pawel Pohl4.
Abstract
A direct current atmospheric pressure glow microdischarge (dc-μAPGD) generated between an Ar nozzle microjet and a flowing liquid was applied to produce Au-Ag core-shell nanoparticles (Au@AgCSNPs) in a continuous flow system. Firstly, operating dc-μAPGD with the flowing solution of the Au(III) ions as the cathode, the Au nanoparticles (AuNPs) core was produced. Next, to produce the core-shell nanostructures, the collected AuNPs solution was immediately mixed with an AgNO₃ solution and passed through the system with the reversed polarity to fabricate the Ag nanoshell on the AuNPs core. The formation of Au@AgCSNPs was confirmed using ultraviolet-visible (UV-Vis) absorbance spectrophotometry, transmission electron microscopy (TEM), and energy-dispersive X-ray spectroscopy (EDS). Three localized surface plasmon resonance absorption bands with wavelengths centered at 372, 546, and 675 nm were observed in the UV-Vis spectrum of Au@AgCSNPs, confirming the reduction of both the Au(III) and Ag(I) ions. The right configuration of metals in Au@AgCSNPs was evidenced by TEM. The Au core diameter was 10.2 ± 2.0 nm, while the thickness of the Ag nanoshell was 5.8 ± 1.8 nm. The elemental composition of the bimetallic nanoparticles was also confirmed by EDS. It is possible to obtain 90 mL of a solution containing Au@AgCSNPs per hour using the applied microdischarge system.Entities:
Keywords: atmospheric pressure plasmas; core-shell nanoparticles; gold; nanoparticles characterization; nanoparticles properties; silver
Year: 2016 PMID: 28773393 PMCID: PMC5502932 DOI: 10.3390/ma9040268
Source DB: PubMed Journal: Materials (Basel) ISSN: 1996-1944 Impact factor: 3.623
Figure 1The UV-Vis spectrum of the Au@AgCSNPs. The broad visible absorption spectrum of Au@AgCSNPs (black line) was deconvoluted into three prominent peaks centered at the following wavelength: 372 nm (the absorption plasmon band of the Ag shell—blue line), 546 nm (the absorption plasmon band of the Au core—green line) and 675 nm (the longitudinal plasmon band of the Au core—red line).
Figure 2Analysis of the size of the Au@AgCSNPs. (a,b) Representative TEM micrographs of the Au@AgCSNPs; (c) A histogram displaying the size distribution of the shell thickness of the Au@AgCSNPs; (d) A histogram showing the size distribution of the core diameter of the Au@AgCSNPs.
Figure 3Elemental analysis of the obtained Au@AgCSNPs. (a) Representative TEM micrographs of the spherical Au@AgCSNPs; (b) EDS analysis of the dark inner core of the Au@AgCSNPs. Numerous large peaks corresponding to Au and Ag are present.
Figure 4A schematic representation of the dc-µAPGD systems used to obtain the Au@AgCSNPs. (A) An overall set up of the dc-µAPGD system; (B) A close up of the reactor used to generate the microdischarge between a flowing liquid cathode and an Ar nozzle microjet anode for the AuNPs production; (C) A close up of the reactor with the reverse polarity, i.e., using a flowing liquid anode and an Ar nozzle microjet cathode, for the production Au@AgCSNPs.