*Corresponding author: Dai Hai Nguyen, Institute of Applied Materials Science, Vietnam Academy of Science and Technology, 01 Mac Dinh Chi, District 1, Ho Chi Minh City, Ho Chi Minh 7000
Trang 1*Corresponding author: Dai Hai Nguyen, Institute of Applied
Materials Science, Vietnam Academy of Science and Technology,
01 Mac Dinh Chi, District 1, Ho Chi Minh City, Ho Chi Minh 70000,
Vietnam, e-mail: nguyendaihai0511@gmail.com
Phuong Phong Nguyen Thi: University of Science, National
University of Ho Chi Minh City, 227 Nguyen Van Cu, District 5, Ho Chi
Minh City, Ho Chi Minh 70000, Vietnam
Phuong Phong Nguyen Thi and Dai Hai Nguyen*
Gelatin as an ecofriendly natural polymer for
preparing colloidal silver@gold nanobranches
DOI 10.1515/gps-2016-0036
Received March 7, 2016; accepted July 6, 2016; previously published
online August 17, 2016
Abstract: We report star-shaped silver@gold (Ag@Au)
nanoparticles (NPs) in gelatin suspensions for the purpose
of enhancing the stability of Ag@Au NPs In this case, Ag
NPs were designed as nucleating agents, whereas gelatin
was used as a protecting agent for Au development
Espe-cially, variable gelatin concentrations were also prepared
to explore its ability to increase the stability of Ag@Au
NPs The obtained samples were then characterized by
UV-visible spectroscopy, transmission electron spectroscopy
(TEM), X-ray diffraction, and Fourier transform infrared
spectroscopy The maximum absorption wavelength of all
samples (566–580 nm) indicated that branched Ag@Au@
gelatin NPs were successfully synthesized In addition, our
TEM results revealed that the size of branched Ag@Au@
gelatin NPs was found to be between 20 and 45 nm as
influ-enced by the component ratio and the pH value These
results can provide valuable insights into the improvement
of Ag@Au NP stability in the presence of gelatin
Keywords: gelatin; gold; silver; stabilizer; star-shaped.
1 Introduction
Nanotechnology has been recognized as a revolutionary
approach to materials science over the last decade [1–6]
Furthermore, nanoparticles (NPs), one of the most active
research areas of nanotechnology, have optimal clearance
characteristics, including nanosize, distribution, and
morphology, and many uses in the field of practical
appli-cations, such as catalysis, thermoelectrics,
microelectron-ics, sensing, and biodiagnostics Metal NPs, in particular,
possess specific physical and chemical properties due to
their small-size effect, surface effect, and quantum-size effect Among different kinds of metal materials, gold (Au) and silver (Ag) have advantages of creating various nanostructures in forms such as rods, cubes, flat trian-gles, polybranched, and star-shaped NPs Interestingly, nonspherical rather than spherical NPs show strong cata-lytic activity and surface-enhanced Raman spectroscopy (SERS) behavior caused by the anisotropic distribution of electromagnetic field (EMF) near the tips of the branched NPs [7, 8] Moreover, the unique morphology of star-shaped Au NPs not only improves the EMF without the necessity for the aggregation of particles but also exhib-its plasmon resonances in either the visible or the near-infrared region Therefore, star-shaped Au NPs have been extensively used in many fields in recent years [9]
Various methods, including physical, chemical, and biochemical techniques, have been studied for the prepa-ration of branched Au and Ag NPs [1–3] However, the NPs produced by these methods are often unstable and tend to aggregate together; accordingly, stabilizers play a critical role in controlling the formation of NPs and their disper-sion stability Several agents, such as thiols, surfactants, polymers, and polyelectrolytes, have been used as protec-tive agents for preventing NPs from aggregation Particu-larly, polymers are commonly used as particle stabilizers, owing to their effective ability to avoid agglomeration and precipitation of particles, resulting in NPs with homoge-neous distributions [10–12] For instance, Cheng et al reported a simple method to synthesize spiky star-shaped Au/Ag nanostructured materials using chitosan (Cts) as stabilizing reagents [9] Neupane et al also developed gelatin-stabilized Au NPs (Au NPs-gelatin) with variation
of gelatin concentrations by reducing in situ tetrachloro-auric acid with sodium citrate [13] Besides, Ahmad et al synthesized Ag NPs in Cts, gelatin, and Cts/gelatin sus-pensions, in which case Cts and gelatin were made up
as natural stabilizers and solid supports [14] According
to the TEM images, Ag NPs with the combination of both Cts and gelatin showed a good distribution compared to
Ag NPs with Cts or gelatin alone This accounts for the potentially different properties of polymers that are incor-porated into metal particles, which allow them to serve many biological applications (biosensors, diagnostics, and photothermal therapy)
Trang 2In this study, we focused on the synthesis of
star-shaped Ag@Au@gelatin NPs via the seeded growth
method In such system, gelatin was used as a stabilizer
for Ag@Au NPs due to the presence of nonpolar amino
acid content ( > 80%) of gelatin [15, 16] Initially, Ag seeds
were prepared by the reduction of silver nitrate (AgNO3)
using trisodium citrate (TSC) and sodium borohydride
(NaBH4) Next, these preformed Ag seeds were used for
the further preparation of Ag@Au particles with different
gelatin concentrations These samples were mainly
deter-mined by UV-visible spectroscopy (UV-Vis) and
trans-mission electron spectroscopy (TEM) for the purpose of
checking the plasmon adsorption maximum and its
corre-lation with different shapes The study is expected to offer
valuable information for stabilizing Ag@Au particles by
gelatin
2 Materials and methods
2.1 Materials
AgNO3 (99.8%), tetrachloroauric(III) acid trihydrate (HAuCl4·3H2O;
99.5%), and NaBH4 (Reagent Plus 98%) were purchased from Merck
(Darmstadt, Germany) TSC and L(+)-ascorbic acid (AA) were
pur-chased from Prolabo (Paris, France) Gelatin type A was obtained
from Sigma-Aldrich (St Louis, MO, USA) All reagents and solvents
were used without any further purification.
2.2 Methods
Preparation of Ag colloids: Ag seeds were synthesized using NaBH4
and sodium citrate as reducing agents according to a previous report
[17] Briefly, the aqueous solution of AgNO3 (1.5 ml, 1 mm) was mixed
with the TSC solution (10 ml, 0.25 mm) Then, ice-cooled NaBH4
solu-tion (20 ml, 10 mm) was immediately introduced into the mixture,
leading to the formation of Ag NPs with greenish yellow color The Ag
seed solution was dialyzed by a dialysis membrane (MWCO: 3500 Da;
Spectrum Laboratories, Inc., Rancho Dominguez, CA, USA) against
distilled water under static conditions for several hours Importantly,
this sample should be protected against light to avoid
photodegrada-tion Lastly, the Ag seeds were then characterized by UV-Vis and TEM.
Preparation of Ag@Au@gelatin NPs: Ag@Au NPs were fabricated
using the preformed Ag seeds (Figure 1) [18] In brief, the HAuCl4 solution (10 ml, 0.5 mm) containing 0.1% K2CO3, 200 μl of the Ag seeds, and different amounts of gelatin (0.04 mm) was placed in a
50 ml glass containing a magnetic stirring bar The AA solution (1.5
ml, 100 mm) was then added dropwise into the mixture, and deion-ized water was added to reach a final volume of 17 ml The color
of the samples turned from transparent to pink, blue violet, and finally dark blue, which corresponds to the formation of Ag@Au@ gelatin NPs The mixture was stirred for another 5 h at room tem-perature to achieve complete reduction After that, samples were dialyzed for about 3 days against distilled water and stored at room temperature Lastly, Ag@Au@gelatin was then characterized by TEM, X-ray diffraction (XRD), and Fourier transform infrared (FTIR) spectroscopy.
Characterization: To investigate the presence of Ag@Au NPs, the
samples were examined by FTIR spectroscopy (a Magna-IR™ 550 spectrometer, Nicolet, USA) using KBr pellet UV-Vis spectra were obtained using a Cary 50 UV-Vis spectrometer from Varian (Palo Alto,
CA, USA), and the spectra were recorded over a wavelength range of 300–800 nm The shape, particle size, and size distribution of NPs were imaged by TEM (300 kV; JEOL, Tokyo, Japan) The samples were prepared in distilled water at concentration of 1 mg/ml and equili-brated at 37°C A drop of the solution was placed on a carbon-copper grid (300 mesh; Ted Pella, Inc., Redding, CA, USA) and air-dried for
10 min [19, 20] XRD was performed using a Rigaku DMAX 2000 dif-fractometer (Rigaku Americas Corp., Woodlands, TX, USA) equipped with Cu/Kα radiation at scanning rate of 4°/min in the 2θ range of 30°–70° (λ = 0.15405 nm, 40 kV, 40 mA).
3 Results and discussion
The Ag metal has the same lattice parameters and the face-centered crystal structure Moreover, the diversity of
Ag properties depends on the variation in molar element ratio so that the use of Ag particles as seeds for the syn-thesis of star-shaped Au NPs is quite interesting In this case, NaBH4 was prepared as a reducing agent and TSC was used as a supporting, reducing agent as well as a stabilizer in the production of Ag seeds; the COO groups
of TSC were advanced in stabilizing NPs and protecting them from clumping [21, 22] As a result, Ag seeds weere
Figure 1: Schematic illustration of the preparation of star-shaped Ag@Au@gelatin NPs.
Trang 3successfully synthesized by AgNO3, NaBH4, and TSC
[23] In this experiment, the results provided no
conclu-sive evidence for determining the stability of Ag seeds
because they were quickly used for the formation of
star-shaped Ag@Au NPs However, the information about Ag
seeds was first indicated by the distinctive color in the
colloidal solution with a plasmon absorption band near
394 nm, which means that Ag ions were reduced to Ag0 in
the aqueous phase [23, 24] The Ag seeds were then
deter-mined by TEM (Figure 2A), and the seeds were spherical
in shape with a narrow size distribution ranging in
diam-eter from 6 to 10 nm
Our results were quite consistent with those of
previ-ous publications for the synthesis of Ag NPs via the
chemi-cal reduction method [23, 25] The mild reducing agent AA
was carried out for reducing Au3+ ions because it not only
favored the growth of Ag@Au core-shell but also limited
the new generation of nuclei in the solution, the leading
cause of a desirable size distribution In addition,
ascor-bic ions had a pronounced impact on the formation of
branched nanocrystals and the durability of NP
disper-sion plays a critical role in their application Importantly,
in this research, the effect of gelatin in the growth of
star-shaped Ag@Au NPs was discovered by adding different
concentrations of gelatin solution to the reaction media
(Table 1) [26]
The results of UV-Vis showed that the maximum
absorption wavelength (566–580 nm) of all samples
has no significant difference The absorption peak of
sample a was sharp and symmetrical with the
increas-ing absorption intensity compared to the
remain-ing samples, so more NPs with evenly distributed
particle sizes could be formed As the amount of gelatin
increases in the solution, NPs tend to clump together
to provide highly specific aggregations, which caused
heterogeneous reactions, resulting in the lower absorp-tion intensity of NPs
In the present study, the stability of the samples was investigated at room temperature for 1 month The results indicated that there were no significant changes over the absorption wavelengths from 580 to 600 nm, whereas the intensive absorption band noticeably decreased by 62% corresponding to sample a After 1 month, the intensive absorption of sample b was reduced to at least 9.3% with
no precipitation; thus, that was the most appropriate amount of gelatin for the protection of star-shaped Ag@
Au NPs Besides, the continuous increase in the number
of gelatin decreased the intensive absorption of NPs, and
it may be because gelatin could no longer function in col-loidal protection at a relatively high concentration The results were completely consistent with the precipitated layer observed at the bottom region of the sample after 1 month
The TEM images of sample b (Figure 3C′) and sample f were examined after 1 month The results of both samples were significantly different Sample f induced structural change, whereas sample b just underwent a little change
in structure Gelatin was, in particular, clumping at high concentration and was not performing its stabilization function; therefore, Ag@Au@gelatin NPs tended to aggre-gate together and then formed larger clusters Meanwhile,
in sample b, gelatin showed excellent ability to protect Ag@Au NPs NPs were star in shape and possessed strong stability The results indicated that 3 ml of 0.04 mm gelatin was the appropriate amount for improving the stability
of Ag@Au NPs Consequently, stable Ag@Au@gelatin NPs with the size of 20–45 nm have a great potential for passive targeting to cancer cells
Powder XRD was further used to analyze the forma-tion of Ag@Au NPs All the Au has similar XRD patterns
1 0.8 0.6 0.4 0.2
0
300 400 500 600 700
Wavelength (nm)
Figure 2: TEM image (A), UV-Vis absorption spectrum (B), and digital photograph (C) of Ag seeds.
Trang 4(Figure 4A, i) The XRD peaks at about 38.3°, 44.2°, 65.1°, and 78° 2θ values corresponded to the 111, 200, 220, and 311 planes of the face-centered cubic crystal of Au, respectively For Ag@Au NPs, the XRD peaks appeared
at 37.97°, 44.05°, 64.21°, and 77.21° related to Ag NPs Additionally, the existence of Ag@Au@gelatin NPs was confirmed as the final product (Figure 4A, ii) The (200), (220), and (311) Bragg reflection planes were weak and widened compared to the intense reflection at (111)
1.2
A
1
0.8
0.6
0.4
0.2
0
400 450 500 550
Wavelength (nm)
1.2
1
a b c d e f
a b c d e f 0.6
0.8
0.4
0.2
0
600 650 700
40 30 20 10 0
400
15 20 25
30 35 40
60 45 30 15 0 15
10 20 25
Diameter (nm)
60 45 30 15 0
20 25 30 35 40 45 50
30 35 40
450 500 550 Wavelength (nm)
600 650 700
Figure 3: UV-Vis absorption spectrum of samples a to f (A) and after 1 month (A′) and TEM image (scale bar, 50 nm) and size distribution of
sample b (B and C) and sample f (D and E) and after 1 month b (B′ and C′) and f (D′), respectively.
Table 1: Synthesis specifications of star-shaped Ag@Au NPs.
Sample VHAuCl4 (ml) VAA (ml) VAg seeds (μl) Vgelatin (ml)
Trang 5These results indicated that Ag@Au@gelatin NPs were
mainly oriented to the (111) plane and Ag@Au@gelatin
NPs obtained from XRD were smaller in size compared to
this NPs measured by TEM
The vibration frequencies of gelatin and Ag@Au@
gelatin NPs were obtained by FTIR spectroscopy for
comparing the secondary structure of the blank gelatin
(Figure 4B, i) and the Ag@Au@gelatin NPs (Figure 4B,
ii) The spectra of gelatin showed vibration bands at
3285 cm-1 (N-H stretch coupled with hydrogen bonding),
3085 cm-1 (alkenyl C-H stretch), 2956 cm-1 (CH2
asymmetri-cal stretching), 1631 cm-1 (C = O stretch/HB coupled with
COO-), 1533 cm-1 (N-H bend coupled with CN stretch), 1444
cm-1 (CH2 bend), 1240 cm-1 (NH bend), and 1078 cm-1 (C-O
stretch) These results implied that gelatin was
success-fully attached to the surface of Ag@Au NPs
4 Conclusion
Star-shaped Ag@Au@gelatin NPs were successfully
fabricated and found to be stable for a long time with a
suitable amount of gelatin The average diameter of
star-shaped Ag@Au@gelatin NPs was between 20 and 45
nm, with the maximum surface plasmon resonance peak
at 566–580 nm In addition, star-shaped NPs tended to
clump together at high gelatin concentrations The results
suggest that star-shaped Ag@Au@gelatin NPs could serve
as a foundation for developing a novel star-shaped
parti-cles with high stability
Acknowledgments: This research was funded by the
Viet-nam National Foundation for Science and Technology
Development (NAFOSTED) grant no 104.02-2014.83
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Bionotes
Phuong Phong Nguyen Thi
Phuong Phong Nguyen Thi received her PhD in 2003 at the Institute
of Applied Materials Science, Vietnam Academy of Science and
Technology She is head of the Nanochemistry Laboratory at the Ho
Chi Minh City University of Natural Sciences She became an
associ-ate professor in 2011 She is also an invited lecturer at the Lac Hong
University and Ho Chi Minh City University of Natural Sciences.
Dai Hai Nguyen
Dai Hai Nguyen obtained his PhD in 2013 at Ajou University, Repub-lic of Korea Currently, he works as a researcher at the Institute of Applied Materials Science, Vietnam Academy of Science and Tech-nology He is also an invited lecturer at the TraVinh University and
Ho Chi Minh City University of Natural Sciences.