Varnika Prakasha,
Rekha Bharb,
Shweta Sharmaa and
S. K. Mehta*b
aInstitute of Forensic Science and Criminology, Panjab University, Chandigarh, 160014, India
bDepartment of Chemistry, Centre of Advanced Studies, Panjab University, Chandigarh, 160014, India. E-mail: skmehta@pu.ac.in
First published on 18th July 2019
In the present work, an attempt has been made to elucidate the structural features of synthesized graphite materials, i.e., expanded graphite (EG) and an expanded graphite/silver nanoparticles (EG/AgNPs) nanocomposite. In order to obtain knowledge about the functional groups present, the interlayer spacing between the carbon layers, topographical features, and the characterization of the materials were carried out using Fourier-transformer infrared spectroscopy, X-ray diffraction, Raman spectroscopy, field emission scanning electron microscopy-energy dispersive X-ray spectroscopy and atomic force microscope. Furthermore, the quenching efficiency of the synthesized graphite materials was also compared using Rhodamine B (Rhd B) as a fluorescent probe. The non-linear behaviour of the Stern–Volmer plots suggested that the complex quenching mechanism (a combination of static and dynamic quenching) was responsible for the decrease in photoluminescence intensity. At a lower concentration of the quencher, the static quenching mechanism was dominant whereas at a higher concentration dynamic processes seemed to be more likely. The binding strength of the complexation between the fluorophore and the quencher at lower concentrations was studied in detail for both of the synthesized materials. The analysis showed that the EG/AgNPs exhibited better quenching efficiency and possessed a strong binding strength in comparison to EG. The thermodynamic parameters of this association suggested that the interaction process was spontaneous and exothermic in nature. Thus, this work offers helpful insights into the fluorescence quenching mechanisms of the Rhd B/EG and its composite system.
In various studies, FL is the most commonly used method to investigate the structural features of graphene-based materials. Evaluation of emitted radiation can reveal not only information about the structural features14 but also the molecular interactions with the fluorophores15 and the thermodynamics of the system.16 Generally, these studies are used for sensing and detection of ionic species,17,18 biomolecules,19 and hazardous chemicals.20 A quantitative analysis of the quenching efficiencies of various graphene materials has been carried out, which explained how chemically exfoliated rGO was better than graphite and GO.21 Liu et al.22 investigated the electron transfer efficiency of GO and graphene using different dyes, namely, eosin, Rhodamine B (Rhd B) and Methylene blue. It was observed that the rate of electron transfer was much higher and efficient for graphene because of its stronger electrostatic interactions with dyes. Lu et al.23 also compared GO and rGO for a better adsorption capability and sensing of fluorescent labeled DNA.
The electron transfer or Förster resonance energy transfer (FRET) processes are known to be responsible for the quenching capability of graphene materials.24 The graphene material acts as an energy acceptor that quenches the FL of an energy donor. Lin et al.25 stated that strong London dispersion forces were responsible for polarization and closeness in the graphene layers and organic dye molecules. The quenching mechanism involved electron transfer from the dye (donor) to the graphene (acceptor) involving intimate π–π interactions. The thermodynamics of the quenching system can provide significant information, as it categorizes the quenching mechanism to be either static or dynamic and also describes the nature of the reaction. Static quenching, which results because of a ground state complex formation between the fluorophore and the quencher, gives information about the binding strength and tertiary or quaternary structural changes in the macromolecule.26 The static interactions are stronger when compared to the random weak collisional dynamic ones. The experiments, and their results, described in this paper are an attempt to unravel the structural details, and the binding strength of the synthesized material with the fluorophore. The thermodynamics involved during the quenching of Rhd B as a fluorophore by the synthesized EG and its composite were also studied.
The Fourier-transform infrared (FTIR) spectra of the synthesized materials were recorded using potassium bromide pellets on a RZX FTIR spectrophotometer from (PerkinElmer) in the mid-infra-red region (4000–400 cm−1). A D8 Advance X-ray diffractometer (Bruker) equipped with a Cu-Kα radiation source (λ = 1.54 Å) under an accelerating voltage of 40 kV and 25 mA for a 2θ range of 5–50° was used for recording X-ray diffraction patterns (XRD) patterns. The field emission-scanning electron microscopy (FESEM) images were recorded using a SU8010 emission scanning electron microscope (Hitachi). The energy-dispersive X-ray spectral analysis (EDX) used for the elemental mapping of EG and EG/AgNPs was performed in a confined region of 100 nm using a Bruker EDX analyzer. The quantitative elemental the analysis of elements such as carbon (C), nitrogen (N) and oxygen (O) in both the prepared materials were performed.
Raman spectroscopic analysis was carried out using an ISA LabRam-300 Raman spectrometer (Horiba Scientific). The excitation of the helium-neon laser was 538.2 nm with power of 10 mW and about a 1–2 μm laser spot size.
The atomic force microscopy (AFM) studies were conducted using a di-Innova atomic force microscope (Veeco Instruments) in tapping mode equipped with a silicon substrate and cantilever, a resonance frequency of 300 kHz and a spring constant of 60 N m−1. The FL spectra were recorded using an F-7000 FL spectrophotometer (Hitachi).
Fig. 1 FTIR spectra of EG and EG/Ag showing the presence of polar functionalities on the surface of the synthesized materials. |
The XRD pattern obtained for EG showed a peak at a 2θ of 26.3 which was a characteristic graphitic peak corresponding to the (002) plane. This peak was also seen in EG/AgNPs with a very slight shift at a 2θ of 26.7. The shift can be ascribed to the change in diffraction angle because of the presence of the AgNPs. The smaller peak seen for EG at 54.1° was ascribed to (004) graphitic plane. However, the additional sharp peaks at 38.1°, 44.5°, 64.5°, and 77.6° were observed for the EG/AgNPs, which were assigned to silver crystalline planes (111), (200), (220), (311) of face centred cubic (fcc) unit cell, respectively (Fig. 2).
The corresponding interlayer distance in EG and the EG/AgNPs composite was estimated to be 3.39 Å and 3.29 Å, respectively, using Bragg's equation. The positive interaction between the AgNPs and EG were responsible for the closer proximity of the two EG layers, thus, a smaller interlayer distance was observed for the EG/AgNPs. The calculated average crystallite size of the AgNPs using the Debye–Scherrer's eqn (1) was 31.7 nm.
(1) |
The results of the Raman analysis show that the graphitic carbon nature of the EG was denoted by the G peak seen at about 1570 cm−1 and a peak at about 1350 cm−1 suggests that there are covalently attached oxygen functionalities such as epoxide on the EG surface28 (Fig. 3). Another broadened two-dimensional (2D) peak at about 2700 cm−1 was seen in EG which tended to shift in the case of EG NPs. The broadening of the 2D peak was an indication of a multiple layer graphene structure. In both cases, the broadened 2D peak was suggestive of multi-layer graphene, with a shift and an additional peak at about 653 cm−1 which was because of the incorporation of AgNPs on the EG surface.29
Fig. 3 Raman spectra of EG and EG/AgNPs showing the D, G, and 2D peaks. The peak marked in red for the EG/AgNPs samples indicates the presence of AgNPs. |
The FESEM images (Fig. 4) show exfoliated sheets for EG which were morphologically different from that of pristine graphite flakes (Fig. S2, ESI†). The microscopic images of graphite show closely stacked multi-layered carbon sheets, whereas, EG shows exfoliated carbon sheets. The tendency of intercalated acid molecules to escape increased because of the pressure generated during the heating (microwave) process. This resulted in an expansion of the adjoining carbon layers. The intercalated acid molecules after the microwave treatment were evolved in the form of gases such as nitrogen dioxide and sulfur dioxide. However, the EG/AgNP images show that the AgNPs were adsorbed on the EG surface. The shape of the AgNPs was cuboidal and the size varied from 15 nm to 30 nm. The AgNPs were prone to agglomeration because of the active surface plasmon resonance,30 however, in the present case minimum aggregation was observed. The exfoliated carbon layers acted as a substrate for the efficient adsorption of AgNPs resulting in their fine dispersion. In addition, PVP also assisted in stabilizing and governing the shape and size of the particles.
The EG/AgNPs images show that the AgNPs were adsorbed on the EG surface. The shape of the AgNPs was cuboidal and the size varied from 15 nm to 30 nm. The exfoliated carbon layers acted as a substrate for an efficient adsorption of AgNPs, resulting in their fine dispersion. In addition, PVP also assisted in stabilizing and governing the shape and size of the particles.
Furthermore, the EDX analysis, confirmed that the major elemental composition was: C, O, S, and N for the EG together with additional Ag for the EG/AgNPs. The corresponding elemental percentage of C, O, S, N in EG was 94.3%, 1.89%, 0.46%, 3.55%, respectively, whereas in the EG/AgNPs it was 88%, 2.96%, 0.55% and 2.24%, respectively, with 5.80% of Ag.
AFM was used to measure the graphite sheet size and thickness. The EG and EG/AgNPs were mixed ultrasonically and dispersed in propanol. A portion (20 μl) of this solution was drop casted over a previously cleaned silicon wafer and dried at room temperature. The thickness of the carbon sheet at the blue mark was about 16 nm which drastically decreased to 3 nm near the edges (red mark, Fig. 5). This can be corroborated by the fact that the intercalated acid molecules at the edges were loosely bound when compared to the molecules in the centre, and thus could easily escape. As a result of this, the layer at the edges expanded to a greater extent. The AFM results obtained were in good agreement with the results of the FESEM and XRD analysis. Also, the height profile analysis showed that nanosheets of 12 nm mean thickness were present in the EG sample.
Fig. 6 (a) FL plots of Rhd B in presence of EG, and (b) EG/AgNPs, (c and d) corresponding Stern–Volmer plots (lower concentration range) at different temperatures. |
An absence of shift in λmax confirmed that the quenchers do not cause any structural change in the Rhd B fluorophore. Positive interactions of EG and EG/AgNPs with the conjugated π electron cloud of the dye lead to photophysical intermolecular deactivation of the process. Functionalities such as carbonyl, ethanolic, ethylenic and enolic groups present on the surface of EG and EG/AgNPs can easily interrupt the conjugation of the π electron cloud of the dye by electrostatic interactions. The functional groups present on the surface of EG and EG/AgNPs act as energy acceptors, thus, providing an alternative non-radiative electron transfer pathway.18 Comparing the two, the EG/AgNPs seem to be a more potent quencher than EG alone (Fig. 7).
Fig. 7 Schematic representation of the likely mechanism of the photodeactivation process of Rhd B on the introduction of the functionalized EG sheets. |
In order to obtain further information, Stern–Volmer (SV) plots were drawn (Fig. S2, ESI†). A plot between (F0/F) − 1 versus concentration (eqn (2)) showed an upward curvature which indicated a dual quenching mechanism, i.e., static as well as dynamic.
(2) |
Fig. S2 (ESI)† can be segregated into two linear segments before and after the inflection point (yellow mark), one being at a lower concentration range (0.0048–0.046 mg ml−1) and another at a higher concentration range (0.048–0.066 mg ml−1). The decrease in FL intensity was gradual at a lower concentration range in comparison to a prominently sharp change at a higher concentration range. At a lower concentration, the probability of complex formation between Rhd B and the quencher molecule (EG and EG/AgNPs) was very high. However, at a higher concentration, this probability decreased because of extensive inter-particle collisions. Thus, the lower concentration range can be designated as a static quenching mechanism, whereas at a higher concentration, it was a dual quenching mechanism, i.e., a static, as well as dynamic process, is followed.31,32 To determine the binding strength, a linear fit was applied to the static region of the SV plots (Fig. 6c and d).
The value of KSV which was analogous to the binding strength is listed in Table 1. The interactive forces between Rhd B and the quencher are stronger for the EG/AgNPs when compared to EG as was suggested by the higher KSV values. The presence of Ag NPs may provide more active sites to interact with Rhd B, thus making the EG/AgNPs a stronger binder. Furthermore, with an increase in temperature, KSV values decreased in both cases. Lowering of the binding strength with an increase in temperature can be allocated to the fact that the higher temperature may weaken the interaction forces by providing heat energy to the system.
Temp (K) | KSV (L g−1) | |
---|---|---|
EG | EG/AgNPs | |
298.15 | 28.60 | 46.18 |
303.15 | 21.18 | 18.71 |
308.15 | 14.31 | 10.21 |
(3) |
ΔG = ΔH − TΔS | (4) |
The parameters obtained from the Van't Hoff equation are shown in Table 2.
T (K) | ΔG (kJ g−1) | ΔH (kJ g−1) | TΔS (J) | |||
---|---|---|---|---|---|---|
EG | EG/AgNPs | EG | EG/AgNPs | EG | EG/AgNPs | |
298.15 | −8.355 | −9.365 | −52.848 | −115.414 | −44.491 | −106.605 |
303.15 | −7.608 | −7.587 | −45.232 | −107.827 | ||
308.15 | −6.862 | −5.808 | −45.982 | −109.605 |
A negative value of ΔG indicated that the interaction process between Rhd B and the quenchers was spontaneous. At a higher temperature, the process became less probable as shown by the lower value of ΔG. Also, a negative value of enthalpy changes suggested that heat energy was evolved during the interaction or that the process was exothermic in nature. The results were in agreement with the non-radiative emission of the energy during the quenching. The positive interactions between the two species lead to the closer proximity of the two, and as a result, the randomness of the system decreased. This fact was also supported by the negative value of ΔS. Comparing the two systems, the interaction of EG/AgNPs with Rhd B was more spontaneous which was also in good agreement with the SV constant and other findings. All the parameters reinforced the likely interaction between Rhd B and EG and its conjugate with AgNPs (Fig. 8).
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c9ra03325d |
This journal is © The Royal Society of Chemistry 2019 |