Abstract
We study low-frequency linearly polarized laser-dressing in materials with valley (graphene and hexagonal-Boron-Nitride) and topological (Dirac- and Weyl-semimetals) properties. In Dirac-like linearly dispersing bands, the laser substantially moves the Dirac nodes away from their original position, and the movement direction can be fully controlled by rotating the laser polarization. We prove that this effect originates from band nonlinearities away from the Dirac nodes. We further demonstrate that this physical mechanism is widely applicable and can move the positions of the valley minima in hexagonal materials to tune valley selectivity, split and move Weyl cones in higher-order Weyl semimetals, and merge Dirac nodes in three-dimensional Dirac semimetals. The model results are validated with ab initio calculations. Our results directly affect efforts for exploring light-dressed electronic structure, suggesting that one can benefit from band nonlinearity for tailoring material properties, and highlight the importance of the full band structure in nonlinear optical phenomena in solids.
Keywords: Nonlinear optics, topological materials, valleytronics, Floquet physics, ARPES
Light-induced band structure and optoelectronic device engineering has gained considerable attention in recent years due to its potential to revolutionize electronics.1−21 Within this paradigm, a system is irradiated by a coherent laser pulse that dresses the electronic states, potentially changing their properties. The process allows modifying band dispersions, turning insulators into conductors and vice versa, altering the crystal symmetry, and tuning the system’s topology.2,3,9,15,20−32
One of the most-studied materials for light-induced band engineering is graphene, which in the absence of driving is a two-dimensional (2D) Dirac semimetal with the band touching at the K and K′ points in the Brillouin zone (BZ). The degeneracies can be lifted when driving the system with circularly polarized light, generating diverse topological phases.15,18,22,23,26 The effect is attributed to the breaking of time-reversal symmetry (TRS). The gap opening in light-driven graphene has not yet been observed in angle-resolved photoemission spectroscopy (ARPES) due to various possible experimental limitations,32−35 but hybridization gaps have been seen in other systems.2,36 On the other hand, topologically trivial gap opening in graphene also occurs without breaking TRS if inversion symmetry is lifted37,34 or strain is introduced (moving the Dirac nodes until oppositely charged nodes annihilate to open a gap).38,39 It was also shown in optical lattices that by shaking the lattice, one can move the Dirac nodes along high-symmetry axes until they merge,40,41 with analogous phenomena occurring in the very intense high frequency driven regimes.42
Here we show that with strong-field and low frequency laser driving, a linearly polarized monochromatic field can move the Dirac nodes in the BZ by a substantial amount, and the movement’s direction is fully controlled by the laser polarization. Effectively, this opens a large pseudogap at the original position of the Dirac nodes. We analytically show that the physical mechanism for the effect relies on band nonlinearities and therefore does not appear in the simplest linearized low-energy model of Dirac bands. We validate these results with time-dependent density functional theory (TDDFT) calculations of ARPES spectra. Lastly, we show that this physical mechanism is general and allows versatile control of the band engineering in a wide range of materials. As examples, we demonstrate control over the position of the valley minima and valleytronics in hexagonal-Boron-Nitride (hBN, allowing valleytronics control in transition-metal-dichalcogenides),43−46 splitting and moving charge-II Weyl cones,47 and merging Dirac nodes in three-dimensional (3D) Dirac semimetals.48,49
We begin by analyzing a graphene system with a two-band tight-binding (TB) model with fifth-order nearest-neighbor (NN) terms.50 In the basis of creation/annihilation operators on the A/B sublattice sites of the honeycomb lattice, the field-free Hamiltonian is
| 1 |
where
is the identity matrix, ti are hopping amplitudes to
the ith NN site, and fi(k) are structure factors (see Supporting Information (SI) section I). The second
term in eq 1 conveniently
sets the
top of the valence band to zero energy, while the first term represents
the various hopping processes. Note that
inherently does not
include
, setting the gap to
zero and resulting
in Dirac cones with local linear dispersion in the K/K′ points.
The eigenvalues of
,
denoted as ϵ±(k), are obtained
analytically. The hopping amplitudes are
fitted through least-squares such that ϵ±(k) match bands obtained from density functional theory (DFT)
calculations performed using octopus code51−53 within the
local density approximation (see SI sections
II and III). Notably, the TB model provides very good bands around
the K/K′ valleys (the main region of interest) but fails around
the Γ-point.
is
coupled to an external laser by Peierls
substitution, yielding
where
is light’s vector potential within
the dipole approximation. Here, E0 is
the field amplitude, ω is the driving frequency, c is the speed of light, and ê is a polarization
vector. From this time-periodic Hamiltonian we obtain the Floquet
Hamiltonian in the basis of harmonic functions of ω with the
sub-blocks:
| 2 |
where |n – m| is the photon channel order,
and the integrals in eq 2 are solved numerically.
is then
exactly diagonalized, and the eigen-energies
are corrected by their photon-channel index. The resulting Floquet
quasi-energy valence and conduction bands, ϵ±F(k), are taken as the bands that converge to the field-free bands for E0 → 0.
Our main interest is the
position of the Dirac nodes in the driven
system. Since in graphene the Dirac nodes host a nonzero Berry phase,54−56 they cannot be removed by a linearly polarized laser field (that
does not break inversion or TRS57) unless
oppositely charged nodes merge.58 However,
we can still track the nodes’ movements with respect to laser
driving. In order to simplify the analysis, we initially ask whether
a Floquet quasi-energy gap can open in the original positions of the
Dirac nodes at K/K′, defined as EgF = ϵ+(K) –
ϵ–F(K). If a gap opens, the linearly dispersing
nodes have moved (note that we will later analyze directly the movement
of the nodes). We analyze the Floquet propagator,
, and use
atomic units unless stated otherwise.
describes time propagation
over one laser
cycle, and taking the logarithm of its eigenvalues is formally equivalent
to diagonalizing the Floquet Hamiltonian.27 The propagator can be represented by a time-independent effective
Hamiltonian,26,59
, where
comprises a Magnus series expansion:
![]() |
3 |
In this representation
acts as a direct time-averaged
Hamiltonian,
and higher orders capture effects due to the Hamiltonian not commuting
with itself at different times. This notation is especially appealing
for analyzing gap openings in graphene, because
does not include
terms;
hence,
purely comprises
,
, and
terms, and
purely comprises gap-opening
terms. The next orders
follow such that
only even-order terms in the Magnus expansion allow potential gap
openings at K/K′.
The main question of interest is under
which conditions do the
even-order terms vanish. Let us first prove that for the perfectly
linear low-energy Dirac Hamiltonian, fields that do not break TRS
cannot open a gap at K. For this, we take the first-order expansion
of
around K, 
, where Δk is the momenta
away from K and vf is the Fermi velocity.
Coupling
to an external laser field provides a time-periodic
Hamiltonian that is inserted in the Magnus expansion. Due to the linearity
of the Dirac Hamiltonian, we obtain
(because ∫02π/ωA(t) = 0). Thus, for the Dirac Hamiltonian, only higher order
terms can alter the band structure. For
, we find
| 4 |
There are three main terms inside the integral in eq 4: the first two in the top row vanish at K (Δk = 0). The third term is k-independent, and the only one that survives at K. This term clearly vanishes for linear driving since then one of the laser polarization components is zero. We now show that it also vanishes for any TRS field. First, we separate the double integral in the third term in eq 4:
![]() |
5 |
Next, without loss of generality
we represent A(t) with a pure harmonic
sine series, A(t) = ∑am sin (mωt), such that the electric field is given by a pure cosine series, E(t) =
, inherently
respecting TRS (E(t) = E(−t)).
Plugging these into eq 5, we note that one polarization component of A(t) is always integrated over in the t′
integral, giving a time-even function, while the other component remains
time-odd. The second temporal integral over t then
vanishes since it integrates a time-odd function. Thus,
in the Dirac Hamiltonian for any TRS drive.
In the SI (section VI), we generalize this
proof to all even orders of the Magnus expansion. Overall, a Floquet
pseudogap cannot open in the low-energy Dirac Hamiltonian driven by
a TRS field. This is a well-established result that has been shown
with other methodologies. It is, however, potentially misleading because
it seemingly pinpoints the physical reason a gap does not open at
K to the presence of TRS. Contrarily, we argue that the physical origin
of the effect is the linearity of the Hamiltonian (and similarly,
Weyl13 or other linearly dispersing systems7). Indeed, if one repeats the analysis for a field-free
parabolic Hamiltonian of the form
, the proof no longer holds regardless
of
TRS. One can verify that in that case, a Floquet gap does open, even
though the Hamiltonian is spherically symmetric and in a low-energy
continuum form.
For completeness, we repeat the analysis for
the TB Hamiltonian
at K, keeping only up to second-order NN terms and employing a linearly
polarized drive along ky (respecting TRS).
takes the form:
| 6 |
where the
function under the double integral
is composed of nested trigonometric functions (see SI section VI) and cannot be analytically integrated. Still, eq 6 can be evaluated numerically,
and we have found that generally
. The SI (section
VI) presents exemplary results for the size of
vs the laser amplitude and wavelength,
showing power-law-like scalings. We also note some analytical intuition
arises from this analysis, e.g., that the gap at K should scale parabolically
with t1 and be independent of t2 (as well as t5) because they only couple to
terms
that commute. However, the size of
the gap and its scaling with the laser parameters is not expected
to correspond well with the size of
because in practical conditions, higher
order terms in the magnus expansion cannot be neglected.60,61 Moreover, in the fifth-NN TB Hamiltonian, the t1 hopping term interferes with higher-order terms, leading
to more complex dynamics (see SI section
VI). Nonetheless, even if not quantitative, this analysis establishes
the gap opening at K and its physical origin—if
, higher order terms will also
be nonzero,
and there is no general symmetry constraint that causes their summation
to vanish. In the SI (section VI), we provide
thorough exact numerical investigations of the size of the pseudogap;
it indeed scales parabolically with t1 and does not scale with t2, corroborating
the analytical analysis. We generally found that the gap at K can
be very substantial (up to 0.5 eV). Practically, we recall that this
pseudogap means that the Dirac nodes moved elsewhere, where a larger
gap suggests the positions have moved further away from K/K′.
Before moving further, it is worth highlighting some noteworthy points: (i) If E0/ω ∼ 1, the Magnus series can converge very slowly, or even diverge, but it is still valid for determining if a gap opens at K. (ii) The gap at K (and Dirac nodes movement) arises from band nonlinearity in the field-free Hamiltonian away from K, and it vanishes in the limit where the low-energy Dirac Hamiltonian becomes valid. However, simply evaluating the Hamiltonian in the vicinity of K does not guarantee that the low-energy expansion around it is valid; rather, E0/ω must be sufficiently small. This condition breaks if E0 is large, or ω is small, as obtained in the strong-field limit, and it is already broken in often-employed conditions for observing Floquet sidebands (powers of ∼1011 W/cm2 and wavelengths ∼1600 nm open a pseudogap of ∼50 meV and move the Dirac node ∼0.3% of the BZ along kx). (iii) The Dirac node motion strongly depends on the laser orientation, since that greatly changes the Magnus expansion. For instance, for a laser polarized along kx, we obtain g(t,t′) = 0, and only even terms beyond the fourth-order in the Magnus expansion are nonzero.
Having established this result, we numerically investigated its dependence on the laser parameters. When graphene is driven along high symmetry axes (along Γ–M or Γ–K), we find that the Dirac nodes only move along the kx axis (similarly to shaken optical lattices40). Figure 1(a,b) presents the distance of the out-of-equilibrium Dirac nodes from K (ΔK) vs laser power and wavelength, which can be quite substantial, and up to ∼10% of the BZ in reasonable experimental conditions. In more extreme cases, oppositely charged Dirac nodes can even merge. We determined that this process requires laser powers of ∼1013 W/cm2 (at 1600 nm driving wavelength along the x-axis), although this value is qualitative because it depends on the details of the TB model around Γ, where it fails. This critical power is slightly higher than graphene’s damage threshold, implying that linearly polarized driving cannot open a proper gap.
Figure 1.
Dirac node motion in graphene driven by linearly polarized light. (a) Floquet–Dirac node distance from the original K-point along the kx-axis vs driving wavelength for a power of 1011 W/cm2, and driving along x- and y-axes. (b) Same as (a), but vs driving power for a wavelength of 1600 nm. The highlighted point signifies a Dirac node merger event (blue) and merger events with Floquet replicas (purple). (c) Angle of the Dirac node (with respect to the kx-axis) vs the driving polarization angle (with respect to the x-axis), for power of 1011 W/cm2 and wavelength of 1600 nm. (d) Same as (c), but presenting the radial distance of the Dirac node from its equilibrium position at K. Inset in (d) shows the trajectory (red) of the Dirac nodes around K/K′ in the BZ as the laser polarization rotates (size enhanced for clarity). Inset in (c) shows the graphene lattice.
Slightly different results are observed for y-polarized driving, where the Dirac nodes move in the opposite direction (Figure 1(a,b)). Interestingly, here, the Dirac node at K(K′) interacts with the hybridized Floquet sidebands (replicas of K′(K)) until they gradually merge and open a gap for a certain critical pump wavelength and power. At that point, another gapless sideband enters the region. Such dynamics continue for longer wavelengths (or higher intensities), where more sidebands enter the region around K/K′. The effect is similar to phenomena observed in other driving conditions with Dirac point spawning,26,37 but seems distinct to very long wavelength driving at which it also becomes difficult to distinguish between Floquet replicas and the original Dirac points (see SI section VI). Thus, measuring the position of the Dirac nodes with respect to the driving parameters could potentially probe additional information about the system such as band hybridization.
Figure 1(c,d) plots the position of the Dirac nodes in the driven system vs the laser polarization axis (both angle, θK—the angle of the shifted Dirac point around its original position, and distance, RK—the distances of the shifted Dirac point from its original position; see illustrated trajectories in the inset of Figure 1(d)). As the laser polarization rotates, the Dirac nodes smoothly rotate (with a trigonal pattern) around their equilibrium positions in correspondence. This verifies that a single monochromatic linearly polarized laser can arbitrarily place the Dirac nodes in the BZ.
We next show that these results are not specific to graphene, or even to linearly dispersing systems; band nonlinearity inherently exists in all periodic systems regardless of their low-energy local structure. First, we perform similar calculations in monolayer hBN (see SI section V and ref (62) for details). Figure 2(a,b) shows that the position of the valley minima (defined as the minimal optical gap points in the BZ) moves around with the laser drive and rotates around their equilibrium position by few percent. This provides a potential path to optically tune valley selectivity (also in transition-metal-dichalcogenides) without circular driving, because the local orbital character around the minima point differs from that at K/K′, and the valley minima can be arbitrarily shifted away (whereas with circular driving, it is fixed due to rotational symmetry). This is especially clear if one considers that valley optical selection rules can be explicitly derived only at K/K′ points, while the Bloch states have mixed character in their vicinity.45,46 Second, we perform similar calculations in the 3D Dirac semimetal, Na3Bi48,49 (see SI section V). Crucially, in Na3Bi even the low-energy Hamiltonian contains large nonlinearities at the Dirac nodes because they arise from a crossing of two parabolic bands. Figure 2(c) shows that linearly polarized laser driving can move the Dirac nodes just as in graphene. The two nodes merge at laser powers of ∼1011 W/cm2 (at 1600 nm), which is within experimental feasibility. Physically, this merging is possible in Na3Bi because the nodes are initially relatively close to each other. However, this predicted critical power might slightly differ in the realistic system due to the validity of the low energy Hamiltonian around Γ. Third, we calculate the Floquet quasi-energy bands for linearly polarized driven SrSi2, which is a Charge-II Weyl semimetal with parabolically dispersing Weyl cones.47 Due to the parabolic dispersion, the system is inherently nonlinear (see SI section V). We find that the laser splits the Charge-II Weyl cone into two Charge-I linearly dispersing cones. Figure 2(d) shows that as the driving power increases, the new charge-I cones move further apart. We have found that their motion can be fully controlled within the xy-plane, in which the field-free bands are parabolic (following the laser polarization). Along the kz-axis on the other hand, the electronic bands are linearly dispersing and no driving parameters can move the Weyl cones. This highlights that the physical mechanism relies on band nonlinearity.
Figure 2.

Results in other material systems. (a) Angle of the valley minima point in hBN with the same notations and conditions as those in Figure 1. (b) Same as (a), but presenting the distance of the Dirac node from its equilibrium position at K. (c) Floquet–Dirac node motion in Na3Bi—Dirac node distance from the original position vs laser power, for a wavelength of 1600 nm and x-axis polarization. The highlighted point signifies a Dirac node merger event. (d) Charge-II Weyl cone splitting, and Charge-I Weyl cone motion, in SrSi2—Floquet–Weyl cone distance from its original position vs driving power for similar laser conditions as (c). Inset in (b) shows the trajectory (blue) of the valley minima around K/K′ in the BZ as the laser polarization rotates (size enhanced for clarity). Insets in (a), (c), and (d) show the hBN, Na3Bi, and SrSi2, lattice structures, respectively.
Lastly, to further establish the model results, we performed ab initio TDDFT calculations of ARPES in light-driven graphene. The methodology follows ref (63), but with artificially doping the conduction band to make the ARPES signals from it more visible. All details of these calculations are delegated to the SI section IV (see also refs (51−53), (64−67)). Figure 3 presents the resulting spectra along kx- and ky-axes overlaid with the quasi-energy bands obtained from the model, which agree remarkably well; a large gap of ∼0.18 eV opens at the original K point (seen when plotting along ky), and the Dirac nodes shifts by ∼1.15% of the BZ along kx. Note that the use of the Dirac Hamiltonian in this case completely fails in describing the spectra because it fixes the Dirac nodes to K/K′. We further emphasize that even though intense pumping is required to observe these phenomena in ARPES, intensities of up to 4 × 1010 W/cm2 are already achievable,68 and work is underway to allow even more intense pumping.69 Moreover, by utilizing longer wavelength pumps (e.g., in the THz regime70), weaker peak powers can be used to observe similar phenomena (see SI section VI). Regardless, even weaker signals of Dirac point motion could be extracted from experimental spectra by subtracting the field-free backgrounds or utilizing only their asymmetric part. Furthermore, as the motion is polarization-dependent, spectra obtained at different polarizations will help distill the signal. Therefore, these predictions should be experimentally accessible with the current technology.
Figure 3.
Ab initio TDDFT calculations of ARPES from light-driven graphene for linearly polarized driving along kx at 3200 nm and 1011 W/cm2. The spectrum is plotted along ky (a) and kx (b), in the region of K, and is saturated for clarity. The overlaid dashed lines denote the Floquet quasi-energy bands obtained from the model in the same driving conditions. Arrows indicate shifting of the Dirac node and opening a gap at K.
To conclude, we investigated several material systems irradiated by intense low-frequency linearly polarized lasers. For Dirac linearly dispersing systems, we showed that the laser moves the Dirac nodes away from their initial position. This motion is substantial and can be fully controlled by changing the laser parameters (intensity, wavelength, polarization). The effect was analytically shown to originate from band nonlinearities, highlighting the importance of the employed model. Consequently, our results emphasize the obvious yet sometimes overlooked feature that low-energy Hamiltonians fail when driven by sufficiently intense or long-wavelength lasers. We further validated the generality of the physical mechanism with extensive additional calculations, showing that linearly polarized driving can: (i) control the positions of valley minima in valley-selective materials (tuning valleytronics), (ii) merge Dirac nodes in 3D Dirac semimetals, and (iii) split high-order Weyl cones and control the positions of the resulting linearly dispersing cones. We confirmed the model results with ab initio TDDFT calculations and outlined an ARPES setup able to test our predictions.
The present findings should help guide future experiments and theory of Floquet band engineering; and in particular, to benefit from electronic band structure nonlinearities to tailor material properties. Our results also emphasize the importance of the full BZ and band structure away from the minimal gap points in strong-field physics processes in solids, such as high harmonic generation,71−73 photogalvanic effects,74−76 magneto-optical effects,77,78 and more. This is especially relevant in quantum materials and systems with topological or linearly dispersing bands,70,79−83 motivating development of ab initio methodologies. We expect that the movement of the high-symmetry points in the BZ will imprint additional characteristics not only directly in ARPES, but also for linear and nonlinear optical responses such as transient absorption spectra and high harmonic generation, which should motivate future work.
Acknowledgments
This work was supported by the Cluster of Excellence Advanced Imaging of Matter (AIM) – EXC 2056 – project ID 390715994, SFB-925 “Light induced dynamics and control of correlated quantum systems”, project 170620586 of the Deutsche Forschungsgemeinschaft (DFG), Grupos Consolidados (IT1453-22), and the Max Planck–New York City Center for Non-Equilibrium Quantum Phenomena. The Flatiron Institute is a division of the Simons Foundation. O.N. gratefully acknowledges the generous support of a Schmidt Science Fellowship.
Supporting Information Available
The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/acs.nanolett.3c02139.
Technical details of the tight-binding model. Technical details about the DFT calculations and fitting procedures of the tight binding hopping amplitudes. Technical details of the TDDFT calculations and ARPES calculations. Technical details of the Floquet calculations in material systems other than graphene. Extended proof that all higher-order even Magnus expansion terms vanish in the Dirac Hamiltonian driven by time-reversal symmetric light. Extended numerical investigation of the pseudogap opening in graphene and its scaling with laser parameters and tight-binding parameters. Additional results of tr-ARPES in graphene for other laser parameters. (PDF)
Open access funded by Max Planck Society.
The authors declare no competing financial interest.
Supplementary Material
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