Open Access Article
Saraf Mohaimen Chowdhury
a and
Salena Akther
*bc
aDepartment of Electrical and Electronic Engineering, Port City International University, Chattogram 4202, Bangladesh
bDepartment of Natural Science, Port City International University, Chattogram 4202, Bangladesh. E-mail: salenaakther@portcity.edu.bd
cDepartment of Mathematics, Chittagong University of Engineering and Technology, Chattogram 4349, Bangladesh
First published on 2nd April 2026
Spin-texture and wavefunction modification is still a central problem in the attempt to control spin orientation and distribution, realize effective spin transport, minimize energy dissipation, and improve functionality in spin-based information processing. Here, we studied a specific combination of atomically thin, nonmagnetic, group-13-based post-transition metal chalcogenide (PTMC) quantum dots (M10X12; M = Ga, In, Tl; X = S, Se, Te) with a single transition metal (Zr, Mo, Mn) introduced at the central site using density functional theory. It is observed that the spatial distributions of frontier orbitals are not only spin-selective but also site-selective in real-space due to the induced TM–X3 hybridization, which could allow independent tuning of both spin and spatial characteristics simultaneously. The normalized density overlap can differ by up to 10−3, whereas the normalized signed-amplitude overlap of the corresponding wavefunctions can reach values less than or equal to 10−4. The local and effective magnetic moments of the M9TMX12 structure can range from 1 → 7µB and 1.62 → 20.93µB, respectively, while the spatial extent of identical-spin orbitals can differ by up to ∼197 a.u. Moreover, the energy gap of the pristine combination ranges between 0.89 and 5.02 eV, and it widens upon TM substitution for E↑g (2.6–5.41 eV) while narrowing for E↓g (1.62–5.36 eV), which demonstrates that one spin channel can consistently remain energetically more accessible. A clear directional imbalance in the nonlinear optoelectronic response is observed, with the induced polarization switching between in-phase and out-of-phase (phase inversion) based on the field direction. The hyperpolarizability components reach maximum values of up to ∼106 (β‖) and ∼109 (γ‖, γ⊥), while the relative distribution between parallel and perpendicular directions remains consistent. Such multifunctional responses resulting from a single-site TM perturbation facilitate fundamental insight into how localized electronic changes simultaneously modulate spin selectivity, orbital anisotropy, and nonlinear polarization as interdependent quantum variables in low-dimensional nanoflakes, which holds promise for the design of multivariable quantum information processing architectures and next-generation nano-spintronic materials.
Previous studies on wavefunction modification in 2D or dot-based systems include experimental efforts to understand the electronic structure, charge localization, and optical properties induced with different point defects,26–28 as well as the manipulation of orbital degrees of freedom through inter-dot coupling, dot deformation, or external fields, using microscopy and DFT calculations.29–31 However, these studies do not answer how the spatial distributions or defect-induced relocalizations of orbitals contribute, which could have built a more constructive understanding of charge localization mechanisms. Present works32–34 however address primarily problems and challenges such as electronic wave functions to control optical and electronic properties, orbital quenching from strong crystal field effects, wavefunction overlap in multi-dot arrays, which leads to a loss of well-defined orbitals, and lack of independent control on spin and orbital states. Recently, it has been shown that, unlike conventional TMDs, PTMC-based thin flakes have heavy elements with large atomic masses, which enhance orbital contributions to magnetism and make them a suitable platform to study orbital-dominated and anisotropic magnetic responses.35 Because their d-orbitals are fully occupied and chemically inert, PTM-based low-dimensional systems tend to form s–p orbital interactions when bonded with chalcogens. Due to such characteristics, their ability to respond to point-defect perturbations would likely be more pronounced and the modulation of electronic wavefunctions would be more effective under atomic confinement. Substitutional doping, being one of the earliest and widely used perturbative approaches in semiconductor technology, has long been used to alter the physicochemical properties of materials by introducing localized perturbations in the potential landscape.36 In particular, the partially filled d-orbitals of TM atoms can favor manipulation of carrier concentration, Fermi level positioning, defect-induced states, band alignment, and band offsets within the host lattice. In this context, p–d orbital hybridization, by means of substitution of group-13 cations, is expected to form localized, symmetry-broken electronic states in real-space in confined 2D metal chalcogenide nanodots. This can minimize orbital quenching and allow greater spatial and spin-orbital control under weak crystal field constraints.
Magnetoelectronic properties are not the only physicochemical characteristics modified by doping, as both linear and nonlinear optical responses are also effectively reconfigured in the nanodots.37,38 A previous study reveals how metal substitution in 2D α-In2Se3 semiconductors creates Janus structures like InGaSe3 and GaInSe339 which results in enhancement of nonlinear optical properties, particularly second-harmonic generation (SHG), making them a promising candidate for advanced photonic devices. Furthermore, recent spectroscopic measurements found that quantification of third-harmonic generation (THG) is of great importance for layered III–VI compounds as nanoflakes of GaSe and GaTe showed strong third-harmonic peaks at wavelengths of ≈520 nm under an excitation wavelength of 1560 nm.40 Such strong nonlinear optical responses, in both static and dynamic limits, are important for developing applications in electro-optic modulations, optical nano-sensors, and optical communications due to their higher-order susceptibility.41–43 Hence, to build a complete description of such interrelated aspects, a constructive theoretical study is essential to account for how a small defect would govern electronic disposition, spatial distribution of spins, and nonlinear polarization in a confined molecular region.
This work presents a framework to investigate how modification of only a single site in nonmagnetic PTMC (M10X12; M = Ga, In, Tl and X = S, Se, Te) nanoflakes can lead to the independent control of spatial localization and higher-order hyperpolarizabilities, whose sizes are comparable to the sub-de Broglie length scale. Besides wavefunction relocalization and orbital orthogonality, we found large anisotropic g-factor shifts, high spin-polarization, and spin-selective trap-like localized states, which appear to be major contributors for having enormous directional linear and nonlinear optoelectronic responses, as observed from the partial density of states (PDOS). The isosurface plots of the highest occupied and lowest unoccupied molecular orbitals (HOMO/LUMO), along with calculation of the electronic spatial extent (ESE), reveal that perturbed wavefunctions can simultaneously exhibit both localization and delocalization characteristics relative to the substituted site, mainly controlled by the unpaired d-electron count (4d2, 4d5, 3d5). In addition, some QDs exhibit phase-inversion characteristics with a consistent ratio between first- and second-hyperpolarizability relative to the induced polarizations. Overall, these findings show how effectively a nonmagnetic host system can control the intrinsic spin-dependent spatial characteristics over its confined region for possible applications in spintronics, magneto-optical modulation, reconfigurable quantum logic gates, quantum sensing, and magnetic and spin memory technologies.
Before going into the detailed discussion, an overview of the figures is presented briefly. Fig. 1 and 2 show the atomic structure of the quantum dots discussed in this work. Fig. 3(a)–(c) describes the projections of the total contributions from each orbital's density of states in the quantum dots. Fig. 4 represents the HOMO and LUMO distributions of the pristine configurations, while Fig. 5(a)–(i) depicts the spin-dependent HOMO–LUMO distributions in the centrally perturbed configurations. Fig. 6 shows how the spin densities are spread across different spatial regions. Finally, Fig. 7 compares the directional uniformity preserved in the systems, even after an increase in their respective anisotropic components. The following subsections describe these figures in detail, using a topic-based order that best supports the flow of the discussion rather than a strict numerical order.
: average bond length; dTM–X: dopant–neighbor bond length
| System | Pristine QDs | Substituted QDs | |||||||
|---|---|---|---|---|---|---|---|---|---|
| Dmax (Å) | Rg (Å) | (Å) |
dmin–dmax (Å) | Dmax (Å) | Rg (Å) | (Å) |
dmin–dmax (Å) | dTM–X (Å) | |
| Ga-based QDs | |||||||||
| Ga10S12/Ga9ZrS12 | 12.733 | 5.021 | 2.345 | 2.130–2.625 | 13.110 | 5.034 | 2.366 | 2.130–2.764 | 2.558, 2.523, 2.558 |
| Ga10Se12/Ga9MoSe12 | 13.217 | 5.270 | 2.470 | 2.259–2.753 | 13.260 | 5.267 | 2.466 | 2.264–2.786 | 2.527, 2.517, 2.527 |
| Ga10Te12/Ga9MoTe12 | 14.075 | 5.656 | 2.659 | 2.455–2.954 | 13.713 | 5.605 | 2.624 | 2.538–2.750 | 2.750, 2.750, 2.750 |
| In-based QDs | |||||||||
| In10S12/In9ZrS12 | 13.631 | 5.369 | 2.495 | 2.293–2.740 | 13.662 | 5.397 | 2.504 | 2.294–2.750 | 2.432, 2.432, 2.432 |
| In10Se12/In9MoSe12 | 14.128 | 5.627 | 2.628 | 2.421–2.890 | 13.740 | 5.526 | 2.585 | 2.483–2.733 | 2.663, 2.637, 2.636 |
| In10Te12/In9MoTe12 | 14.990 | 6.017 | 2.822 | 2.609–3.113 | 14.451 | 5.895 | 2.768 | 2.691–2.874 | 2.788, 2.788, 2.788 |
| Tl-based QDs | |||||||||
| Tl10S12/Tl9MnS12 | 14.292 | 5.646 | 2.625 | 2.406–2.891 | 14.298 | 5.517 | 2.587 | 2.391–2.920 | 2.391, 2.449, 2.391 |
| Tl10Se12/Tl9MnSe12 | 14.748 | 5.888 | 2.748 | 2.530–3.022 | 14.585 | 5.756 | 2.709 | 2.495–3.029 | 2.525, 2.495, 2.525 |
| Tl10Te12/Tl9MnTe12 | 15.586 | 6.269 | 2.937 | 2.715–3.236 | 15.950 | 6.174 | 2.912 | 2.670–3.269 | 2.671, 2.693, 2.670 |
In pristine [Ga/In/Tl]–[S/Se/Te] nanoflakes, the 4p, 5p, and 6p orbitals of the metal atoms primarily interact with chalcogen's 3p, 4p, and 5p orbitals, while the filled d-shells remain as spectators. The binding energies (Eb) have been derived to measure and quantify these interaction strengths with eqn (S1) (see the SI). As presented in Table 2(b), for all the MX systems, it is found that Eb increases when larger chalcogens are placed, due to their more diffuse orbitals and effect on charge redistribution. The highest (3.64 eV) Eb is observed for Ga10S12, while the lowest (2.53 eV) is derived for Tl10Te12 in pristine dots. It is also observed that after substitution of a single metal atom with a TM (Zr, Mo, Mn) from the central site, the interaction energy increases, as the TM's partially filled d-orbitals can hybridize more frequently with the orbitals of the host elements. The emergent d–p covalent framework strengthens the interatomic bonding which maintains the same chalcogen-dependent energy hierarchy. The smallest increment (0.2 eV) occurs in Mn-substituted Tl9Te12, whereas Mo-substituted Ga9Te12 exhibits the largest (0.27 eV). Conceptually, the binding energies shift scales with the electronegativity difference between the TM dopant and the chalcogen:
| ΔEb ∝ (χTM − χX)2 |
| (a) | |||
|---|---|---|---|
| Host | Eb (eV) | Eg (eV) | μ0 (a.u.) |
| Ga10S12 | 3.64 | 0.89 | 0.0022 |
| Ga10Se12 | 3.32 | 1.30 | 0.0026 |
| Ga10Te12 | 2.83 | 3.50 | 0.0203 |
| In10S12 | 3.47 | 3.90 | 0.0029 |
| In10Se12 | 3.17 | 4.80 | 0.0013 |
| In10Te12 | 2.72 | 4.60 | 0.0015 |
| Tl10S12 | 3.15 | 5.02 | 0.0242 |
| Tl10Se12 | 2.92 | 2.85 | 0.0169 |
| Tl10Te12 | 2.53 | 4.40 | 0.0261 |
| (b) | ||||||
|---|---|---|---|---|---|---|
| Host | Dp | Eform (eV) | Eb (eV) | E↑g (eV) | E↓g (eV) | μ0 (a.u.) |
| Ga9S12 | Zr | −4.78 | 3.86 | 5.30 | 4.90 | 1.8587 |
| Ga9Se12 | Mo | −4.90 | 3.55 | 4.36 | 2.10 | 4.2452 |
| Ga9Te12 | Mo | −4.54 | 3.10 | 5.33 | 1.62 | 5.9322 |
| In9S12 | Zr | −5.17 | 3.70 | 5.41 | 5.36 | 0.0033 |
| In9Se12 | Mo | −4.74 | 3.40 | 5.23 | 1.70 | 6.8281 |
| In9Te12 | Mo | −4.88 | 2.94 | 5.50 | 1.65 | 0.0079 |
| Tl9S12 | Mn | −4.84 | 3.40 | 4.85 | 1.94 | 3.0787 |
| Tl9Se12 | Mn | −4.20 | 3.10 | 4.66 | 1.88 | 1.9514 |
| Tl9Te12 | Mn | −4.62 | 2.73 | 2.60 | 4.05 | 5.3514 |
| (c) | ||||||||
|---|---|---|---|---|---|---|---|---|
| Host | Dp | M | μnet (µB) | Δgxx | Δgyy | Δgzz | geff | μeff (µB) |
| Ga9S12 | Zr | 4 | 3.00 | −1.076 | −0.998 | −0.146 | 1.26 | 2.44 |
| Ga9Se12 | Mo | 6 | 5.00 | −0.434 | −0.275 | −0.010 | 1.76 | 5.22 |
| Ga9Te12 | Mo | 8 | 7.00 | 0.494 | 1.141 | 5.862 | 4.50 | 17.86 |
| In9S12 | Zr | 2 | 1.00 | −0.204 | −0.204 | −0.003 | 1.87 | 1.62 |
| In9Se12 | Mo | 8 | 7.00 | 0.048 | 0.424 | 0.650 | 2.38 | 9.43 |
| In9Te12 | Mo | 8 | 7.00 | 0.884 | 0.892 | 8.042 | 5.28 | 20.93 |
| Tl9S12 | Mn | 7 | 6.00 | 0.032 | 0.149 | 0.231 | 2.14 | 7.41 |
| Tl9Se12 | Mn | 7 | 6.00 | 0.947 | 1.632 | 2.481 | 3.70 | 12.78 |
| Tl9Te12 | Mn | 5 | 4.00 | −1.232 | −1.207 | −0.073 | 1.17 | 2.85 |
After introducing the TM atoms at the central site, the formation energy is computed as
| Eform = E(M9TMX12) + EM − E(M10X12) − ETM, | (1) |
As observed from the PDOS analysis in Fig. 3, the low-lying s–p states are shifted and hybridized with the TM d states, and these overlaps are visible around the HOMO and LUMO regions. The orbital overlap increases compared to the pristine's orbital hybridization, and the increased p-orbital contribution mainly originates from the high-energy p orbitals introduced by the Ga/In/Tl atoms. The energy levels are more densely spaced around the energy gap region, particularly for β-channels, which causes the energy gap to be lower in that channel for most of the configurations. The pristine nanodots adopt closed-shell singlet ground states in SCF calculations, with all electrons paired in occupied orbitals. The derived HOMO–LUMO gap ranges from 0.89 to 5.02 eV, according to Table 2. For Ga-based nanodots, the highest energy gap is shown by Ga10Te12 (3.5 eV) and the gap keeps reducing when the chalcogen changes from Te to S. For the In-based QDs, the gap increases when S → Se (by 0.9 eV) but slightly decreases when Se → Te (by 0.2 eV), while for the Tl-based QDs it sharply decreases by 2.17 eV (for S → Se) and then again decreases by 1.55 eV (for Se → Te). Such non-monotonic behavior observed in In- and Tl-based QDs is primarily due to their larger orbital energy (5p1, 6p1) compared to the smaller orbital energy of Ga-based MXs (4p1). The larger orbital tends to be more diffusive, and these diffuse orbitals extend further into space, which can increase the orbital interaction range. The replacement with TM atoms causes the energy gaps to split into spin-up (E↑g) and spin-down (E↓g) orbital channels, and almost for all the systems the E↓g channel is more energetically accessible, as presented in Table 2(b). Also a considerable widening of 4.41 (E↑g) and 4.01 (E↓g) eV is observed for Ga9S12 QDs upon Zr substitution. However, this shift notably reduces at E↑g (by 1.51 eV) and E↓g (by 1.46 eV) when the host metal is replaced by indium, which indicates host-dependent orbital hybridization for the chosen dopants. The dipole moment analysis from Table 1(a) supports such host-dependent orbital hybridization by quantifying the charge redistribution upon incorporation of the dopant. Table 2 shows that inclusion of Zr heavily alters the charge distributions (by nearly three orders of magnitude) in the Ga–S framework in contrast to the In–S framework (only ∼0.67 times). Moreover, a reasonable energy gap increment of 3.06 (E↑g), 0.8 (E↓g), and 1.83 (E↑g), −1.88 (E↓g) eV is observed for Ga9Se12 and Ga9Te12, respectively, upon introducing a 4d5 perturbation. In contrast, the corresponding increments for In9Se12 and In9Te12 are relatively modest, at approximately 0.43 (E↑g), −3.1 (E↓g) eV, and 0.9 (E↑g), −2.95 (E↓g) eV. A decrease in the E↑g-channel is found for both Tl9S12 and Tl9Te12 by 0.17 and 1.8 eV, while the E↓g-channel drops by 3.08 and 0.35 eV. For Tl9Se12, E↑g increases by 1.81 eV, whereas E↓g decreases by 0.97 eV. Such variations show how local TM defect sites can differently affect the spin-resolved electronic structures across various host compositions.
As presented in the isosurface plots of HOMO and LUMO for the pristine (Fig. 4) and substituted (Fig. 5) cases, for the pristine metal-chalcogenide dots, the occupied states are localized at the edge sites as a contribution of the more effective local bonding environment, in contrast to the unoccupied states, which tend to be more dispersed and pronounced around the center region. This particular arrangement results from the extended nature of conduction states that are less tightly bound at these atomic sites. As a consequence, substitution with an unpaired d-orbital atom at this site increases the overall binding energy for the d-orbital-induced hybridization, as depicted in Table 2. According to PDOS analysis, it is also observed that due to such site-specific defect, few spin-dependent localized states appeared within and near the HOMO–LUMO region that has very short amplitudes. These states hybridize with the TM's d-orbitals and form localized wavefunctions that are visible as spatially distinct regions in their corresponding isosurfaces. As a result, these localized regions exhibit not only spin-selectivity but also site-selectivity in physical space. Such spatial-duality is predominantly noticeable for [Ga/In]9ZrS12, [Ga/In]9MoSe12, α-Ga9MoTe12, Tl9MnS12, α-Tl9MnSe12, and Tl9MnTe12 nanoflakes (Fig. 5(a)–(d), (e) and (g)–(i)). Such presence of asymmetric hybridization also arises from the large local dipolar differences induced by TM substitution, as reported in Table 2. We find that the charge redistributions in the aforementioned nanodots are significantly increased relative to their pristine counterparts, with reported values of 1633, 1380, 5254, and 1888 (a.u.) times for selected systems. These outcomes suggest that the coexistence of such varying spin gaps and spatially non-uniform orbitals may allow the nanodots to host multiple energetically distinct electronic states.
To understand whether these molecular dots can represent multiple independent electronic states simultaneously, one way is to verify this theoretically by measuring the spatial correlation between same-spin probability densities. The normalized density–density overlap measures whether spin-dependent electron densities share the same spatial region or are localized at different sites. We can compute this pair-density overlap as
![]() | (2) |
in order to remove the dependence on the absolute spatial localization of individual orbitals and to obtain a bounded, dimensionless measure of relative spatial correlation. As presented in Table 3, the normalized density correlation (
HL) tends to approach zero for most of the QDs. The measured
HL confirms our intuition that two electron-density distributions that are separated by a finite energy gap are apparently orthogonal (essentially ≤10−3) in terms of their real-space envelopes for most of the dots. However, this correlation measurement of identical spin-densities with |ψ|2 can only capture the positive phase and disregards signed-amplitudes or nodal structures.
| System | Channel | Overlap pair | DHL | HL |
|---|---|---|---|---|
| Ga9ZrS12 | α | Hα–Lα | 3.3888 × 10−4 | 0.0746 |
| β | Hβ–Lβ | 3.1734 × 10−5 | 0.0103 | |
| Ga9MoSe12 | α | Hα–Lα | 5.1302 × 10−5 | 0.0104 |
| β | Hβ–Lβ | 3.2719 × 10−5 | 0.0123 | |
| Ga9MoTe12 | α | Hα–Lα | 1.5198 × 10−4 | 0.0594 |
| β | Hβ–Lβ | 8.9530 × 10−4 | 0.7851 | |
| In9ZrS12 | α | Hα–Lα | 1.0305 × 10−4 | 0.0350 |
| β | Hβ–Lβ | 1.5528 × 10−5 | 0.0043 | |
| In9MoSe12 | α | Hα–Lα | 2.4522 × 10−4 | 0.0536 |
| β | Hβ–Lβ | 1.4173 × 10−3 | 0.9492 | |
| In9MoTe12 | α | Hα–Lα | 2.2926 × 10−4 | 0.1213 |
| β | Hβ–Lβ | 7.4158 × 10−4 | 0.7850 | |
| Tl9MnS12 | α | Hα–Lα | 1.0665 × 10−4 | 0.0489 |
| β | Hβ–Lβ | 3.1691 × 10−5 | 0.0109 | |
| Tl9MnSe12 | α | Hα–Lα | 1.6890 × 10−4 | 0.0928 |
| β | Hβ–Lβ | 1.7834 × 10−3 | 0.8797 | |
| Tl9MnTe12 | α | Hα–Lα | 1.8716 × 10−5 | 0.0081 |
| β | Hβ–Lβ | 6.1843 × 10−5 | 0.0477 |
This leads us to measure another quantity which can characterize the real-space interrelation of spatial phases and nodal structures between two same-spin orbitals, and is rotation-invariant. Because two orbitals may occupy the same spatial region (as per the overlapping envelopes) but have opposite signs or nodes locally, it may be possible to address them selectively or separately (as they correspond to energetically distinct levels). In order to verify this, the spatial overlap between same-spin orbital wavefunctions is evaluated from the reconstructed three-dimensional wavefunction grids ψ(x,y,z), that are derived from the signed real-space orbital amplitudes ψ(r). The overlap integral S quantifies the spatial correlation between HOMO and LUMO orbitals within a spin channel (which is basically 〈ψH|ψL〉), where the normalized overlap Snorm accounts for orbital scaling. Within each spin channel, the overlap integral
![]() | (3) |
| System | Channel | Overlap pair | S | |Snorm| | 〈r2〉H | 〈r2〉L |
|---|---|---|---|---|---|---|
| Ga9ZrS12 | α | Hα–Lα | 1.2474 × 10−6 | 0.0000 | 26.5133 | 73.4516 |
| β | Hβ–Lβ | 1.7430 × 10−6 | 0.0000 | 182.1451 | 165.0047 | |
| Ga9MoSe12 | α | Hα–Lα | −3.8323 × 10−5 | 0.0000 | 188.4636 | 30.0014 |
| β | Hβ–Lβ | −1.9331 × 10−6 | 0.0000 | 188.3397 | 184.7601 | |
| Ga9MoTe12 | α | Hα–Lα | −1.2736 × 10−6 | 0.0000 | 80.1892 | 99.1496 |
| β | Hβ–Lβ | −9.4803 × 10−6 | 0.0000 | 189.8775 | 202.7604 | |
| In9ZrS12 | α | Hα–Lα | 2.6031 × 10−5 | 0.0000 | 215.4526 | 57.3589 |
| β | Hβ–Lβ | −8.6911 × 10−6 | 0.0000 | 215.4633 | 18.0892 | |
| In9MoSe12 | α | Hα–Lα | −1.3074 × 10−4 | 0.0001 | 33.8344 | 94.8511 |
| β | Hβ–Lβ | 2.2814 × 10−4 | 0.0002 | 203.5608 | 214.1154 | |
| In9MoTe12 | α | Hα–Lα | −7.8615 × 10−5 | 0.0001 | 99.3915 | 114.9374 |
| β | Hβ–Lβ | −6.7803 × 10−4 | 0.0007 | 214.9433 | 228.5232 | |
| Tl9MnS12 | α | Hα–Lα | 6.4360 × 10−6 | 0.0000 | 192.6453 | 99.3229 |
| β | Hβ–Lβ | 1.1188 × 10−6 | 0.0000 | 193.1523 | 191.1198 | |
| Tl9MnSe12 | α | Hα–Lα | 1.7724 × 10−4 | 0.0002 | 206.9119 | 111.9279 |
| β | Hβ–Lβ | −1.4000 × 10−5 | 0.0000 | 200.9388 | 198.8377 | |
| Tl9MnTe12 | α | Hα–Lα | 3.4190 × 10−5 | 0.0000 | 228.2090 | 182.6864 |
| β | Hβ–Lβ | 6.4570 × 10−7 | 0.0000 | 228.2522 | 146.3248 |
Such existence of spin-selective orbital reconfiguration can further be understood if we observe how the atomic spins are spatially populated, as depicted with the spin-density plot (Fig. 6). It is observed that due to the presence of nested TM–X3 hybridization in the host configuration, the distribution of spin-up (α) and spin-down (β) electronic states varies significantly. This implies that the physical occupation of different spin-dependent orbitals in real-space would be vastly different, and as we can see from the isosurface plots it is entirely selective of the host structure. Such variations of spin-distribution provide a core intuition that if we introduce site-specific defects with a particular dopant (that has unpaired d-electrons) in the nonmagnetic host to form localized hybridization, it creates a major imbalance of spins; hence it is possible to achieve mapping of electronic orbitals in a way that they would distribute asymmetrically and disparately in real-space. This intuition is consistent with our findings, as not only spin-density plots but also the PDOS analysis suggests (discussed earlier) that the number of different orbital and atomic electronic states are distributed at distinct energy levels due to the presence of Zr–S3, Mo–(Se/Te)3, and Mn–(S/Se/Te)3 hybridization. As a consequence, the α-spin and β-spin orbitals occupy different spatial regions while still hybridizing energetically, and exhibit site-selective localization, for which the reconfigurations are real, rational, and spin-dependent. The spin-selective orbital reconfiguration observed in these nanodots originates from a combined effect of the dopant electronic structure and local hybridization geometry. First, the d-orbital occupancy of the TMs (3d5, 4d2, 4d5) determines how many spin-polarized states are available to participate in bonding, which governs whether the resulting orbital reconfiguration is strong, weak, or absent. This electronic configuration gives rise to an exchange splitting between spin-up and spin-down components, and the magnitude of such splitting then energetically separates the E↑g and E↓g channels and enforces spin selectivity at the level of the frontier orbitals. Moreover, the relative overlap between the p- and d-orbital energy of TM and chalcogens controls which orbitals hybridize and within which energy window, which in turn causes different TM–X3 motifs to exhibit distinct reconfiguration patterns. It is further evident that the local TM–X3 coordination symmetry lifts the degeneracy among spatial orbitals, and as a result, the hybridized states are shaped into distinct spatial orientations and nodal structures. Together, these factors give rise to a logical, site-selective, and spin-dependent orbital reconfiguration, which is consistently supported by spin-density distributions, PDOS features, and real-space isosurface plots.
To further support the real-space orbital and spin-density analyses, we performed Mulliken population analysis for all pristine and centrally perturbed nanodots (Tables S4–S12) along with their representative charged state (Tables S13–S21). It is observed that the resulting charge and spin populations are consistent with the site-selective and spin-dependent electronic reconfigurations identified from the orbital isosurfaces and overlap analyses. Because Mulliken populations project the spin-resolved density matrix on to atom-centered basis functions, the observed atom-resolved spin moments represent the total integrated consequence of the spin-selective orbital reconfigurations, which are visually observed in real-space. In the subsequent analysis, we discuss that, apart from the orthogonality of spin-dependent energy states, the same-spin orbitals also encompass distinct spatial radius, which would provide a more constructive understanding of their spatially independent nature. Collectively, these results imply that most of the nanodots demonstrate quasi-independent like electronic states within their same-spin channel, which could inform future experimental efforts.
![]() | (4) |
In the case of different energy orders with the same spins, the quadrupole moment analysis can give a more constructive outlook (see Table S2 in the SI), as it quantifies the degree of spatial asymmetry and directional electron density distortion across the molecular framework, and indicates a more spatial polarization and anisotropy in the substituted configurations. As per Table 4, for the same energy order with different spins, we can see that due to the Zr–S3 interaction within the host of Ga9S12 QDs, ESE shifts about +155.6 and +91.5 a.u. for the spin-up and spin-down orbitals, respectively. However for the same hybridization, In9S12 shows an identical distribution of E↑g electrons and a reduction of 39 a.u. for E↓g. Moreover, configurations like α-Ga9MoS12, α/β-In9ZrS12, α-Tl9MnS12, and α-Tl9MnSe12 have a comparatively large spatial difference of 158.4, 158.1, 197.37, 93.3, and 95 (a.u.), respectively, which tells us that alongside their orthogonal behavior the expansion in real-space deviates such that each of the orbitals can possibly be realized as a quasi-independent state (in real-space).
For the rest of the dots, the ESE shifts positively and Table S3 (in the SI) verifies whether the spatial distribution of both spins within the same energy window is identical. We find that the occupied orbitals of Ga9MoSe12, In9ZrS12, Tl9MnS12, and Tl9MnTe12 are non-orthogonal in nature and normalized as
![]() | (5) |
Such coexistence of a small but finite density overlap with a vanishing signed wavefunction overlap, as well as distinct spatial extent, shows that these states remain functionally decoupled due to site- and node-selective separation, rather than only phase cancellation within the same region. Moreover, though PDOS depicts the presence of energetic hybridization between dopant and host orbitals, the overlap results show that these states remain spatially distinct and occupy different sites and spatial radii. This spatial separation limits real-space coexistence despite energy-space mixing, which in turn allows the spin-dependent orbitals to behave as distinguishable spatial channels. Such real-space localization suggests that selective excitation or manipulation of site- and spin-specific states could be feasible, which holds promise for memory or logic functionalities at such nanoscale limits. Taken together, the observed anisotropic spatial distribution of orbitals allows us to control each of the parameters independently and suggests that such spin-dependent, site-specific confinement provokes differential localization of orbital polarization, which in turn leads to selective spatial distribution of frontier orbitals and spin channels.
The magnetic responses of the nanodots when interacting with an external magnetic field are presented in Table 2(c). As presented, the significant shifts in directional g-tensors which increase the effective g-factor are the direct consequences of the high spin–orbit coupling (SOC) effect in the nanoflakes resulting from the combined orbital's contribution from transition metals and heavy metals to magnetism being much higher and dominating over the spin's contributions. In response to the interaction with a magnetic field, the QDs exhibit an effective magnetic moment which can be quantified as
. geff is derived from the g-shifts of each principal axis and calculated as their averaged value, where μeff increases along with the increase in geff. The computed g-tensors include contributions from orbital-Zeeman and perturbative spin–orbit terms (gOZ/SOC), and the observed anisotropic g-factor shifts primarily arise from orbital-Zeeman contributions, where SOC provides a quantitative correction. Deviations from the free-electron g-factor indicate enhanced orbital participation and anisotropic magnetic response induced by the dopants. The mean g-factor of the free electron is a key descriptor to understand the spin behavior, where ge ∼ 2.002 and any deviation from this value indicates modifications of SOC and exchange interaction in the molecular electronic configurations due to central defects. The deviation of g-factor along the principal axis is derived with the GIAO formalism, and the details are presented in the methodology section of the SI. As we can see, when the effective g-factor increases, μeff exhibits higher response, which reflects its ability to enhance orbital-induced magnetism due to the strong presence of SOC. The field-induced magnetic moments due to such effect show very strong magnetic moments, as the derived μeff ranges between 1.62µB and 20.93µB. This kind of large magnetic response suggests multifunctional magnetic behaviors of these nanoflakes, which show the simultaneous presence of spin-selective orbital distribution in real-space and field-controllable magnetic moments.
The PDOS for all the considered quantum dots is shown in Fig. 3a–c, which depict the specific orbital contributions involved in host-TM hybridization. For the pristine gallium- and indium-based MX dots, it is observed that metal s, p and chalcogen p orbitals dominate primarily because the d-orbitals remain stable (appear at very low energies) and do not participate in bonding, staying inactive near or around the energy gap region. Compared to the thallium-based QDs, electrons from the d-orbitals actively participate in the PDOS spectra of the pristine system. This behavior arises from relativistic effects, particularly scalar relativistic contraction of the 6s orbital and expansion of the 5d shell, which raise the energy of the 5d states and enhance their spatial extension. As a result, Tl's 5d orbitals can hybridize appreciably with neighboring p orbitals (from chalcogen atoms and the host configuration), and show a detectable d-character near the HOMO–LUMO region of the electronic spectrum. A tiny contribution comes up from Zr's 4d2 orbitals in the Ga9S12 and In9S12 nanodots upon single Zr substitution (Fig. 3a), showing a marginal overlap with the host orbitals. It is worth noting that this limited interaction still contributes to the spin-polarization observed in the quartet (M = 4) and doublet (M = 2) magnetic states (spin-density isosurface of Fig. 6a and d), particularly for the In9S12 system, where the spin density is closely confined at the substituted site. In contrast to the Tl9S12 QDs, Mn substitution results in more noticeable orbital overlap due to its higher number of unpaired d-electrons (3d5), and in both spin channels this interaction is visible along the HOMO–LUMO (Fig. 3c) region. Despite the lower availability of electronic states, the interactions are effective enough to produce high septet polarization, and the resultant magnetic moments show a broad spatial distribution from the center to an in-plane edge site adjacent to the substituted site (Fig. 6g).
Following Mo-induced perturbation in Ga9Se12, Ga9Te12, In9Se12, and In9Te12 nanoflakes, the orbital interactions lead to much higher spin-polarized states. The presence of 4d5 orbitals, which hybridize in the midgap region of Ga9Se12 (Fig. 3a), results in asymmetric spin localization around the dopant and at an edge site (Fig. 6b), similar to what is observed for Ga9S12 and Tl9S12 nanoflakes. This sort of spatial separation of spin densities at a peripheral site on the same plane as the dopant is evident in Tl9Se12 (Fig. 6h) and Tl9Te12 (Fig. 6i) QDs, where d-orbital-induced hybridization via Mn substitution is noticeably stronger and denser (Fig. 3c).
But a more widespread delocalization of magnetic moment, which extends from the central to peripheral edge sites across the plane, is observed for Ga9Te12 (Fig. 6c), In9Se12 (Fig. 6e), and In9Te12 (Fig. 6f) nanoflakes. The nested Mo–(Se, Te)3 interactions shift the low-lying valence states upward in energy through 4d5 orbital overlap (Fig. 3a and b), and consequently, the magnetic configuration corresponds to the octet state, which is the highest among the group (Table 2). It is understandable from our PDOS analysis that when the number of overlapping states from hybridized orbitals increases near or above the energy gap, exchange interactions become more strong, which in turn leads to the emergence of site-specific spin textures and higher spin polarization in the system. To provide a more detailed outlook on atomic contributions, the element-projected PDOS is presented in the SI (Fig. S1).
| Host | Dp | αiso (a.u.) | αaniso (a.u.) | β‖ (a.u.) | β⊥ (a.u.) | γ‖ (a.u.) | γ⊥ (a.u.) |
|---|---|---|---|---|---|---|---|
| Ga10S12 | — | 6.1 × 102 | 6.0 × 102 | −3.8 × 101 | −1.3 × 101 | 3.7 × 105 | 1.2 × 105 |
| Ga9S12 | Zr | 6.1 × 102 | 5.6 × 102 | 1.8 × 103 | 6.1 × 102 | 6.1 × 105 | 2.0 × 105 |
| Ga10Se12 | — | 7.4 × 102 | 7.7 × 102 | 5.6 | 1.9 | 4.3 × 105 | 1.5 × 105 |
| Ga9Se12 | Mo | 7.5 × 102 | 5.0 × 102 | 4.5 × 103 | 1.5 × 103 | 8.2 × 105 | 2.7 × 105 |
| Ga10Te12 | — | 1.0 × 103 | 1.1 × 103 | 2.8 | 9.4 × 10−1 | 6.2 × 105 | 2.1 × 105 |
| Ga9Te12 | Mo | 1.1 × 103 | 1.3 × 103 | 2.2 × 105 | 7.2 × 104 | 3.7 × 108 | 1.2 × 108 |
| In10S12 | — | 7.3 × 102 | 7.1 × 102 | 3.5 × 101 | 1.2 × 101 | 9.1 × 105 | 3.1 × 105 |
| In9S12 | Zr | 7.5 × 102 | 6.9 × 102 | 2.0 × 101 | 6.5 | 9.3 × 105 | 3.1 × 105 |
| In10Se12 | — | 8.8 × 102 | 8.8 × 102 | −1.5 × 101 | −5.0 | 2.7 × 105 | 8.0 × 105 |
| In9Se12 | Mo | 9.2 × 102 | 9.7 × 102 | 1.4 × 105 | 4.7 × 104 | 9.9 × 107 | 3.3 × 107 |
| In10Te12 | — | 1.1 × 103 | 1.2 × 103 | −7.6 × 101 | −2.5 × 101 | 1.1 × 106 | 3.5 × 105 |
| In9Te12 | Mo | 1.2 × 103 | 1.3 × 103 | 2.2 × 105 | 7.3 × 104 | 1.6 × 108 | 5.2 × 107 |
| Tl10S12 | — | 8.4 × 102 | 9.0 × 102 | 2.7 × 101 | 9.2 | 8.0 × 105 | 2.7 × 105 |
| Tl9S12 | Mn | 8.2 × 102 | 8.7 × 102 | 3.0 × 103 | 1.0 × 103 | 9.9 × 105 | 3.3 × 105 |
| Tl10Se12 | — | 1.0 × 103 | 1.1 × 103 | 2.2 × 101 | 7.2 | 8.2 × 105 | 2.7 × 105 |
| Tl9Se12 | Mn | 1.7 × 102 | 2.2 × 103 | −5.6 × 104 | −1.9 × 104 | −1.2 × 108 | −3.9 × 107 |
| Tl10Te12 | — | 1.3 × 103 | 1.5 × 103 | 1.2 × 102 | 4.0 × 101 | 1.1 × 106 | 3.8 × 105 |
| Tl9Te12 | Mn | 1.3 × 103 | 1.4 × 103 | 2.3 × 103 | 7.6 × 102 | 2.3 × 105 | 7.6 × 104 |
This large increment due to Mn–Se3 can be rationalized upon inspection of the corresponding isosurface plots of the HOMO (Fig. 5(c), (e), (f), (g) and (i)). They show a highly asymmetric localization of wavefunctions and diffuse orbitals, where the spin-up orbitals are primarily confined to one edge site, while the spin-down orbitals are distributed along a different peripheral site in the opposite direction (yet along the same axis). Such directional separation from the overlap of 6p1–3d5–4p4 intensifies charge polarization along one axis, which in turn amplifies the anisotropic response of this quantum dot.
More interestingly, the first-hyperpolarizability tensor components (β‖, β⊥) exhibit phase (direction of the induced polarization) inversion between the applied electric field and the induced polarization. As shown in Table 4, this phase inversion becomes switchable to in-phase polarization through Zr and Mo substitution in pristine Ga10S12, In10Se12, and In10Te12, while Mn substitution in Tl10Se12 induces out-of-phase polarization relative to its pristine counterpart. The in-phase polarization increased by roughly ∼102 to ∼104 times of magnitude, while the out-of-phase response reached up to ∼103 times of magnitude in their corresponding β‖ components. Alongside this, the Ga9MoTe12 nanodot exhibits the highest increase, increasing approximately six orders of magnitude, and the largest variation between the parallel and perpendicular components is observed for In9ZrS12 (RB reaches about 3.06).
In addition, a similar phase reversion in second-hyperpolarizability tensor components (γ‖, γ⊥) is also observed for the Tl9MnSe12 nanodot, where the intensity reaches approximately 109 and 108 along the field direction and perpendicular to it, respectively. As reported in Table 5, the third-order nonlinear response is the strongest among all considered QDs, which suggests that such confined geometry, zigzag edge-bonding, and local perturbations give rise to long-range, non-saturating, and significant static nonlinearity in these sub-de Broglie length regimes. The highest anisotropy ratio (RΓ) is observed for the Ga10S12 nanoflake (∼3.1), which indicates that its wavefunction delocalization (Fig. 4(a) and (b)) is much more pronounced along the direction of the interacting field. The directional uniformity preserved in the systems, in accordance with such amplified intensities, can be more easily understood from Fig. 7.
The predicted spin- and site-selective orbital reconfigurations could be experimentally validated in several ways.49–52 Spin-polarized scanning tunneling microscopy (SP-STM) can directly visualize the real-space spin densities and reveal the spatial separation between E↑g and E↓g orbitals. Another method could be X-ray magnetic circular dichroism (XMCD), which can probe the spin-dependent contributions of the transition metal dopants and confirm magnetic anisotropy. Moreover, spin-resolved photoemission spectroscopy (spin-PES) can measure the energy-level separation between spin-up and spin-down orbitals, which may directly validate the predicted exchange splitting. In addition to this, STM or scanning tunneling spectroscopy (STS) can map the local density of states to confirm site-specific localization of frontier orbitals. X-ray absorption spectroscopy (XAS) or electron energy-loss spectroscopy (EELS) can also probe the symmetry and spatial distribution of unoccupied orbitals. The effective g-factor enhancement due to the SOC effect can be confirmed via electron spin resonance (ESR) experiments under applied magnetic fields. Furthermore, linear polarizability and first/second-hyperpolarizabilities can be measured using techniques like electric-field-induced second-harmonic generation (EFISHG), optical absorption spectroscopy, or hyper-Rayleigh scattering (HRS) measurements, which provide information on charge distribution and anisotropy in orbital delocalization. Taken together, these findings highlight that engineered point-defect perturbations lead to systematic tuning of the magnitude, directionality, and phase of static linear and nonlinear optical responses through controlled spin–orbital reconfiguration, where spin-selective orbital localization, edge-confined geometry, and TM-dopant identity collectively govern these properties across sub-de Broglie length scale quantum dots.
The edge atoms of the QDs were modeled in their under-coordinated form (without applying explicit passivation) to isolate the intrinsic effects of internal substitutional defects, while TM dopants were placed at a central interior site to ensure a controlled coordination environment. Future work could explore the effects of alternative defect configurations or host stoichiometry, which may include different TM incorporation sites, vacancies, and edge substitutions with appropriate chemical passivation, to establish broader structure–property trends in QDs. Such studies would extend insights into how defect configurations influence the electronic and optical behavior of quantum dots.
Information on supporting data from this study remains privately accessible to the authors, who can provide it to qualified requesters upon request.
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