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conirmed by x-ray diffraction (XRD) and energy-dispersive x-ray spectrometry analyses.
Ojea-Jimenez et al . 13 demonstrated the use of Au@citrate NPs of 8.9 ± 1.6 nm size for
sequestration of Hg 2+ ions from Milli-Q and real waters. They have proposed that the sur-
face of gold NPs catalyze the reduction of Hg 2+ by citrate groups that are present on their
surfaces. The formation of an Au 3 Hg alloy was identiied. Gold may be recovered from the
alloy. Mercaptosuccinic acid (MSA)-protected Ag NPs of different sizes were studied for
Hg 2+ sorption.
Sumesh et al . 14 have synthesized Ag@MSA NPs of sizes 9 ± 2 nm and 20 ± 5 nm for
which Ag/MSA mole ratios was maintained as 1:6 and 1:3, respectively (Figure 26.2a).
These NPs were supported on alumina, and they were used for Hg 2+ removal in column
setups. A solution of 2 ppm Hg 2+ was passed in separate columns containing 1:3 and 1:6
Ag@MSA materials at identical low rates. Mercury was detected in the eluent after pass-
ing 2.0 and 5.5 L Hg 2+ solutions in the case of 1:3 and 1:6 Ag@MSA, respectively (Figure
26.2b). Concentration of Hg 2+ went below 85 ppb (in the case of 1:6 Ag@MSA) with an input
concentration of 2 ppm. A high removal ability of 800 mg Hg/g Ag@MSA was achieved in
the case of 1:6 Ag@MSA. From this, it is clear that small NPs (1:6 Ag@MSA) adsorb larger
quantities of mercury owing to the presence of a larger number of functional groups per
unit mass compared with NPs of a bigger size.
Gold and silver QCs were shown to have an ability to detect Hg 2+ ions down to 2 ppb
level. This concentration is the maximum contamination limit in drinking water set by
the US EPA. Xie et al . 15 used red-emitting Au 25 clusters encapsulated in a protein matrix
(bovine serum albumin [BSA]) for highly selective detection of Hg 2+ . Here, detection has
been on the basis of quenching of the PL of encapsulated clusters due to a high degree of
Hg 2+ -Au + (d 10 -d 10 ) interactions. The detection limit was 0.5 nM (0.1 ppb). Luminescence
had partially been regained after reducing Hg 2+ to Hg 0 by an NaBH 4 solution. Speciic d 10 -
d 10 interactions were noticed in the Ag + -Cu + cases also. For this, they had prepared core-
shell Au@Ag clusters by reducing Ag + ions on as-prepared Au 25 BSA clusters. Introduction
of Cu 2+ ion quenches the luminescence of the Au@AgBSA clusters due to Ag + -Cu + metallo-
philic interactions. Here, formation of Cu + was by the reduction of Cu 2+ by BSA molecules.
(a)
(b)
-1:6 Ag@MSA
-1:3 Ag@MSA
1500
1200
900
600
300
0
01
2
34567
50 nm
Volume passed (L)
FIGURE 26.2
(a) TEM image of parent 1:6 Ag@MSA NPs. (b) Plot of the concentration of Hg 2+ detected in the eluent as a func-
tion of the volume of Hg 2+ solution passed through individual columns packed with 3.0 g each of 1:3 and 1:6
Ag@MSA NPs supported on alumina. Loading of 1:6 and 1:3 Ag@MSA NPs on alumina was 0.5 and 0.3 wt%,
respectively. (Adapted from Sumesh, E. et al., J. Hazard. Mater ., 189, 450, 2011. Copyright with permission from
Elsevier.)
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