Catalina
Nicolau
,
Sergi
Burguera
,
María de las Nieves
Piña
and
Antonio
Bauzá
*
Ctra. de Valldemossa, km. 7.5, Universitat de les Illes Balears, 07122, Palma de Mallorca, Islas Baleares, Spain. E-mail: antonio.bauzaatuib.es
First published on 10th April 2025
Adsorption of amino acids (AAs) onto Ag and Au surfaces has attracted much interest in the past years, owing to their ability to control and tune the structure of Ag and Au nanoparticles (NPs) during the synthetic procedure and to enhance their stability under various conditions. Despite this, the molecular recognition events that are responsible for such stabilization as well as the role of the AA residue moieties is still not completely understood. To tackle this point, we computationally evaluated the weak interactions involved in the AA⋯Ag/AuNP recognition process from a theoretical perspective. In more detail, we analysed the strength and physical nature of the interactions established between twenty essential AAs and Ag/AuNPs at the PBE0-D3/def2-TZVP level of theory. The structural and energetic studies were complemented by the use of the quantum theory of atoms in molecules (QTAIM), non-covalent interaction plot (NCIplot) and energy decomposition analysis (EDA) techniques, providing new insights into the nature and spatial extension of the interactions studied herein. We believe that the results reported in this exploratory study will be useful for researchers working in the fields of bioinorganic chemistry, biotechnology and supramolecular chemistry by shedding light on the weak binding phenomena that are crucial for achieving AA⋯Ag/AuNP recognition.
A crucial aspect of their functionality in biological systems is their interaction with biomolecules, particularly peptides, proteins, and amino acids (AAs),7 for instance, for controlling the structure of Ag/AuNPs during synthesis and improve their stability under various conditions.8 In this context, studies have demonstrated that the binding affinity of a given peptide for a particular region of the metal surface is related to the peptide's ability to control nanoparticle synthesis and enhance stability.9,10
Peptides, proteins, and AAs exhibit a diverse range of interactions with metallic nanoparticles, influenced by factors such as nanoparticle size, shape, surface charge, and functionalization, as well as the intrinsic properties of the biomolecules themselves.11 These interactions can lead to the formation of stable protein coronas,12 affect protein conformational stability,13 and influence cellular uptake and biological responses.14 In fact, the ability of AAs to bind to metal surfaces through functional groups such as thiols, amines, and carboxyls plays a pivotal role in modulating nanoparticle behavior and stability.15 In this regard, previous experimental and computational studies have delved into the atomic-level details of binding between peptides and Ag surfaces.16,17 However, the nature of the interactions governing the AA⋯NP molecular recognition mechanism is not completely understood, and its study is essential for designing novel NPs for specific biomedical applications (e.g. to increase therapeutic efficacy or to improve targeting specificity in drug delivery systems).
This study aims to explore the noncovalent interactions (NCIs) between AAs and Ag/AuNPs from a theoretical perspective. To achieve this, we have used twenty natural AAs and a model of Ag/AuNPs (see Fig. 1 and the Methods section). In more detail, we have computationally simulated the supramolecular complexes formed when the AAs are adsorbed onto the metallic surface, leading to the characterization of the NCIs responsible for this process. The supramolecular assemblies found were further studied using quantum mechanical techniques including the molecular electrostatic potential (MEP), the quantum theory of atoms in molecules (QTAIM), the non-covalent interaction plot (NCIplot) and the energy decomposition analysis (EDA) methodologies.
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Fig. 1 Schematic representation of the AAs used in this study (brown = non-polar, green = aromatic, red and blue = polar charged, orange = polar neutral). |
The MEP surfaces were computed at the PBE0-D3/def2-TZVP level of theory using the Gaussian 16 software25 and analyzed using the GaussView 5.0 program.26 The calculations for the wavefunction analysis27 were also carried out at the PBE0-D3/def2-TZVP level of theory and analyzed using the AIMAll software.28
In addition, the energy decomposition analysis (EDA)29,30 scheme was used to understand the role of electrostatics, exchange-repulsion, orbital, dispersion and electron correlation contributions in the formation of the noncovalent complexes studied herein at the PBE0-D3/def2-TZVP level of theory using TURBOMOLE 7.7 software and the COSMO-RS approximation.
Lastly, the NCIplot31 isosurfaces correspond to both favorable and unfavorable interactions, as differentiated by the sign of the second-density Hessian eigenvalue and defined by the isosurface color. The color scheme is a red–yellow–green–blue scale, with red indicating repulsive (ρcut+) and blue indicating attractive (ρcut−) NCI interaction densities. Yellow and green surfaces correspond to weak repulsive and weak attractive interactions, respectively. The surfaces were visualized using the Visual Molecular Dynamics (VMD) software.32
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Fig. 2 Optimized geometries at the PBE0-D3/def2-TZVP level of theory of complexes 4, 7, 14, 30 and 32. The AA⋯Ag26/Au26 distance is also given in Å. |
Complex | AA | ΔE | d | |
---|---|---|---|---|
AA⋯Ag complexes | ||||
1 | GLY | −3.8 | 2.787 | 0.75 |
2 | ALA | −4.4 | 3.142 | 0.84 |
3 | VAL | −8.0 | 2.528 | 0.68 |
4 | LEU | −9.5 | 2.793 | 0.75 |
5 | ILE | −9.9 | 2.701 | 0.72 |
6 | PHE | −18.2 | 3.039 | 0.71 |
7 | TYR | −18.7 | 3.098 | 0.77 |
8 | TRP | −18.6 | 2.995 | 0.70 |
9 | ASP | −14.6 | 2.721 | 0.68 |
10 | GLU | −9.5 | 2.593 | 0.64 |
11 | LYS | −6.5 | 2.829 | 0.76 |
12 | ARG | −13.0 | 3.610 | 0.84 |
13 | HIS | −13.5 | 3.048 | 0.73 |
14 | MET | −13.7 | 2.853 | 0.65 |
15 | CYS | −10.0 | 3.115 | 0.70 |
16 | SER | −10.6 | 3.278 | 0.81 |
17 | THR | −5.8 | 3.022 | 0.75 |
18 | ASN | −7.2 | 2.855 | 0.71 |
19 | GLN | −10.6 | 2.884 | 0.72 |
20 | PRO | −7.4 | 2.882 | 0.78 |
AA⋯Au complexes | ||||
21 | GLY | −5.7 | 2.673 | 0.73 |
22 | ALA | −6.3 | 3.118 | 0.85 |
23 | VAL | −11.5 | 2.484 | 0.68 |
24 | LEU | −13.1 | 2.771 | 0.76 |
25 | ILE | −13.5 | 2.645 | 0.72 |
26 | PHE | −24.8 | 2.959 | 0.70 |
27 | TYR | −25.6 | 3.135 | 0.79 |
28 | TRP | −27.6 | 3.006 | 0.71 |
29 | ASP | −18.5 | 2.564 | 0.70 |
30 | GLU | −14.1 | 2.556 | 0.65 |
31 | LYS | −10.4 | 2.802 | 0.77 |
32 | ARG | −17.9 | 3.557 | 0.84 |
33 | HIS | −18.6 | 3.025 | 0.74 |
34 | MET | −21.3 | 2.675 | 0.62 |
35 | CYS | −13.5 | 2.994 | 0.69 |
36 | SER | −11.3 | 3.299 | 0.84 |
37 | THR | −6.5 | 3.312 | 0.84 |
38 | ASN | −10.2 | 3.011 | 0.76 |
39 | GLN | −14.6 | 3.001 | 0.76 |
40 | PRO | −10.5 | 2.881 | 0.79 |
Firstly, from complexes 1 and 21 (GLY) to complexes 5 and 25 (ILE), we observed a progressive reinforcement of the interaction energy value, in line with the increase in the extension of the AA residue. These aliphatic AAs based their interaction with the metallic surface on CH–Rg (Rg = Ag and Au) contacts, similarly to the results obtained in our previous study involving aryl substituted aromatic VOCs.33 These NCIs can also be understood as hydrogen bonds (HBs), since the electrostatic potential surface of the metallic layers exhibits both positive (holes) and negative (lumps) regions, thus being able to act as both an electron donor and an acceptor moiety (see Fig. 3).
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Fig. 3 MEP surfaces of Ag26 (a) and Au26 (b) layers. The energy values at concrete parts of the surface are given in kcal mol−1 (0.002 a.u.). |
Secondly, for complexes 6–8 and 26–28 (PHE, TYR and TRP), the interaction energy values obtained were similar in the case of Ag26 (−18.2, −18.7 and −18.6 kcal mol−1, respectively), while more noticeable energetic differences were found among the Au26-involving complexes (−24.8, −25.6 and −27.6 kcal mol−1, respectively). In both sets, we observed a strengthening of the interaction from PHE to TYR owing to the alcohol group that establishes an additional regium bond (RgB)34–39 with the metallic layer (see also Fig. 4a and b). However, we found that in the case of Ag26, complex 8 involving TRP achieved a very similar value to complex 7 involving TYR, while in the case of Au26 we obtained an increase of 2 kcal mol−1 in stability, which is likely due to the higher stability exhibited by Au Rg–π bonds involving extended aromatic systems.40
For complexes involving charged AAs, that is, 9–12 and 29–32 (ASP, GLU, LYS and ARG), we also observed the same behaviour comparing the Ag26 with the Au26 series. Concretely, complexes involving ASP (9 and 29) and ARG (12 and 32) achieved higher interaction energy values than those involving GLU (10 and 30) and LYS (11 and 31). This is likely due to a larger contact area in the case of ARG-involving complexes owing to the presence of the guanidinium group, while between ASP and GLU, the latter showed the interaction of both carboxylate groups with the metal layer, thus partly overestimating the interaction energy value obtained.
Lastly, among the polar and neutral AAs (complexes 13–20 and 33–40), several interesting points are worth discussing. For instance, between the two S-containing AAs (MET and CYS), a larger interaction energy value was obtained for complexes 14 (−13.7 kcal mol−1) and 34 (−21.3 kcal mol−1) involving the former, owing to its slightly higher basicity (in line with the shorter MET⋯NP distances). On the other hand, among the O-containing AAs (SER, THR, ASN and GLN), SER complexes (16 and 36) and GLN complexes (19 and 39) obtained the largest interaction energy values (−10.6 and −11.3 kcal mol−1 and −10.6 and −14.6 kcal mol−1), owing to the formation of moderately strong O⋯Ag/Au RgBs. Furthermore, ASN complexes (18 and 38) obtained lower interaction energy values (−7.2 and −10.2 kcal mol−1) compared to those involving GLN, likely due to the shorter aliphatic chain present in the former. Moreover, HIS complexes (13 and 33) and PRO complexes (20 and 40) also exhibited moderately strong Rg–π and CH–Rg interactions, being HIS complexes more stable than their PRO analogues by around 6–8 kcal mol−1.
Since most of the molecular recognition events occur due to a charge complementarity between the electron donor and acceptor molecules, we have computed the electrostatic potential surfaces of the two metallic layers used herein, Ag26 and Au26. As noted in Fig. 3, we found positive electrostatic potential regions (located over the Ag and Au atoms), which accounted for the presence of holes, and also negative potential regions (located in between the metal atoms), confirming the presence of lumps. These positive and negative potential regions allowed the metal layers to favorably interact with both electron-rich and electron-poor AA residues from an electrostatic point of view. Also, the MEP value over the holes is similar for both metal clusters (+3.5 kcal mol−1 in Ag26 and +3.3 kcal mol−1 in Au26), while the lumps present in the Ag26 cluster exhibited a more negative potential (−4.8 kcal mol−1) compared to the Au26 cluster (−1.9 kcal mol−1). In general, although the positive and negative electrostatic potential values obtained for both metal surfaces are useful to understand the role of electrostatics, the slight differences observed in the MEP values are not sufficient to completely rationalize the interaction energy values obtained; therefore, an energy decomposition study was also performed to further understand these energetic results (see below).
Complexa | ρ × 100 | ∇2ρ × 100 | V × 100 | G × 100 | H × 100 | −G/V |
---|---|---|---|---|---|---|
a Only the bcps exhibiting the largest density values were considered. | ||||||
4 | 0.61 | 2.32 | −0.53 | 0.56 | 0.03 | 1.06 |
7 | 1.06 | 3.81 | −0.72 | 0.84 | 0.12 | 1.17 |
10 | 2.85 | 11.25 | −3.20 | 3.01 | −0.19 | 0.94 |
12 | 0.80 | 3.04 | −0.72 | 0.74 | 0.02 | 1.03 |
14 | 3.26 | 8.17 | −2.77 | 2.40 | 0.13 | 0.87 |
24 | 1.15 | 2.94 | −0.63 | 0.68 | 0.05 | 1.08 |
27 | 1.17 | 4.26 | −0.83 | 0.95 | 0.08 | 1.14 |
30 | 3.68 | 13.19 | −3.60 | 3.45 | −0.15 | 0.96 |
32 | 1.16 | 3.48 | −0.74 | 0.81 | 0.07 | 1.09 |
34 | 5.31 | 11.57 | −4.69 | 3.79 | −0.90 | 0.81 |
As shown in Fig. 4, for complexes 4 and 24 involving LEU, the interaction between the AA and the metallic layer is characterized by the presence of several bond critical points (bcps) and bond paths connecting the alkyl group of LEU to the Ag/Au layer, thus confirming the presence of CH–Rg (Rg = Ag and Au) contacts. For complexes 7 and 27 involving TYR, the bcps and bond paths mainly connect the C atoms from the aromatic ring with the Ag/Au atoms from the metallic layer, thus characterizing these complexes as Rg–π bonds. In addition, the O atom from the alcohol group also shows a bcp and a bond path that connects it to a metal atom, thus also contributing to the overall stabilization of these complexes through the formation of a O⋯Rg RgB.
For complexes 10, 12, 30 and 32 involving GLU and ARG residues, several bcps and bond paths denote the presence of (i) CH–Rg interactions, (ii) RgBs, with the electron donor moiety being the AA in the case of complexes 10 and 12, and (iii) Rg–π interactions in the case of complexes 30 and 32. The CH–Rg contacts are characterized by the presence of bcps and bond paths connecting the CH bonds and the metal atoms, while RgBs and Rg–π interactions are denoted by O⋯Rg and N⋯Rg bcps and bond paths that involve either the carboxylate group or the guanidinium group of the AA and the metal layer.
Lastly, for complexes 14 and 34 involving MET, very similar bcp and bond path distribution were observed, including the presence of CH–Rg bcps and bond paths as well as a S⋯Rg bcp and a bond path that characterizes the presence of a RgB.
On the other hand, regarding the NCIplot analyses, in all the complexes a greenish isosurface was found, located between the AA and the metallic layer, which denotes the presence of weak but attractive NCIs. Additionally, in the case of the O⋯Rg and S⋯Rg interactions present in complexes 10, 14, 30 and 34, a more bluish isosurface colour was observed, thus indicating the presence of a stronger interaction that likely dictates the molecular recognition event between both counterparts.
Table 2 presents the values of the Laplacian at the bcps that characterize the AA⋯NP interaction (∇2ρ × 100), resulting in positive values in all cases, as it is common in closed shell calculations. Furthermore, the values of the potential (V × 100) and kinetic (G × 100) energy densities lie within the same range in all the cases, leading to −G/V ratios around 1, which confirm the noncovalent nature of the AA⋯NP interactions.
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Fig. 5 Graphical representation of the Ele, Orb, Cor and Disp terms for complexes 4 and 24 (LEU), 7 and 27 (TYR), 10 and 30 (GLU), 12 and 32 (ARG) and 14 and 34 (MET). |
As noted, in the case of the Ag26 layer, the dispersion term was the most noticeable contributor in the case of complexes involving ARG (12), TYR (7) and LEU (4), followed by correlation and orbital terms, which exhibited very similar values, and lastly electrostatics being the least favorable contributor to the stability of these supramolecular assemblies. This behavior was also observed for their Au26 analogues (complexes 32, 27 and 24). Additionally, in the case of complexes involving GLU (10) and MET (14), the orbital contribution was the most favorable one, followed by electrostatics and correlation, which exhibited very similar values in the case of complex 10 involving GLU.
In the case of complex 14, the dispersion term exhibited a close value to electrostatics and correlation, while for complex 10 it was the least favorable energy term. On the other hand, complex 30 involving GLU exhibited the same tendency as its Ag26 analogue (10), while in the case of complex 34 involving MET, electrostatics and dispersion terms inverted their behavior compared to complex 14, with the latter being the least favorable energy contributor.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d5cp01106j |
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