Open Access Article
Dietrich Haasea,
Jörn Manz
*a,
Beate Paulusa,
Jonathan Scherlitzki
a and
Jean Christophe Tremblay
*b
aInstitut für Chemie und Biochemie, Freie Universität Berlin, 14195 Berlin, Germany. E-mail: jmanz@chemie.fu-berlin.de
bCNRS-Université de Lorraine, LPCT, 57070 Metz, France. E-mail: jean-christophe.tremblay@univ-lorraine.f
First published on 10th February 2026
Electronic chirality flips in achiral molecules is a hot topic in attosecond and femtosecond chemistry and physics. Our quantum dynamics simulations show that this effect can be induced by a simple Franck–Condon excitation of the A′ + A″ superposition of the electronic A′ ground state plus the first excited A″ state in the oriented bent triatomic heteronuclear molecule NSF.
The key to these phenomena in achiral molecules4–6 is the fact that fs laser pulses can prepare electronic superposition states which break electronic symmetry without breaking nuclear symmetry.7,8 This effect may last for a few fs, when the nuclei are practically frozen. In extreme cases, the laser pulses can even break all electronic symmetries. Consequently, the electronic density of the corresponding superposition states is chiral even though the constituting electronic eigenstates and the nuclear frame are achiral. However, breaking all electronic symmetries is quite a challenge if the underlying nuclear frame has many symmetry elements. For example, the nuclear frames and the electronic eigenstates of heteronuclear diatomic molecules such as NaK4 or RbCs5 have C∞v symmetry with an infinite number of symmetry elements. Amazingly, these can be broken by a well-designed set of two circularly polarized laser pulses.4,5
By comparison with the pioneering references,4,5 this work presents quantum dynamics simulations of a much simpler realization of laser-induced electronic chirality flips in an achiral molecule. For this purpose, we consider a bent triatomic heteronuclear molecule, specifically oriented thiazyl fluoride (NSF), a key substance in sulfur–nitrogen–fluorine chemistry.9 Its nuclear frame and consequently the electronic eigenstates have Cs symmetry, i.e., they possess only one symmetry element, the symmetry plane σ, in addition to the omnipresent identity E. It is easy to predict that breaking the single symmetry element σ of the electronic densities of eigenstates in NSF should be much easier than breaking the corresponding infinite number of symmetry elements of NaK or RbCs. Specifically, we shall show that a simple Franck–Condon (FC) excitation from the electronic ground state A′ to the first excited eigenstate A″ can prepare an electronic superposition state ψ which does not possess any mirror plane, or in other words: preparation of ψ breaks Cs symmetry. Hence, ψ must be chiral, and since it is not an eigenstate, it is time-dependent and induces electronic chirality flips.
![]() | ||
| Fig. 1 Geometries of NSF in the electronic ground state A′ and in the first excited state A″, oriented in the xy-plane. Fluorine in green, sulfur in yellow, nitrogen in blue. | ||
Quantum chemical calculations—performed using the Molpro14 implementation of the (1,2)-SA-CASSCF/SS-CASSCF method15–17 with an aug-cc-pVTZ basis set18 on all atoms—yield the electronic eigenfunctions of the ground and excited states, respectively labeled ψA′(x; Q) and ψA″(x; Q). They depend on the N electronic coordinates x = {r1, ς1, r2, ς2, …, rN, ςN}, where ri is the position of the electron and ςi is its spin, and (parametrically) on all nuclear coordinates, Q. Varying the nuclear configuration yields the potential energy surfaces (PESs) VA′(Q) and VA″(Q) associated with NSF in the electronic ground and first excited states. The corresponding irreducible representations are A′ and A″, cf. the character table of Cs symmetry in Table 1; here the notation σ is also used for reflection at NSF's mirror plane. As only singlet states of NSF are considered, the effect of spin–orbit coupling is assumed to be negligible for electronic excitations.
| Cs | E | σ |
|---|---|---|
| A′ | 1 | 1 |
| A″ | 1 | −1 |
Accordingly, reflection σ at NSF's mirror plane yields
| σψA′(x; Q) = ψA′(x; Q), | (1) |
| σψA″(x; Q) = −ψA″(x; Q). | (2) |
| VA′(Qm,A′) = 0. |
The nuclear wavefunction χA′,0(Q) of the vibrational ground state embedded in the ground electronic PES VA′(Q) represents the lowest vibronic state of the system. In the present work, it is computed by imaginary time propagation of a full-dimensional nuclear wave packet on the ground electronic PES using the Heidelberg implementation of the Multi-Configuration Time-Dependent Hartree (MCTDH) method, as described in ref. 19.
We assume that the molecule is prepared in the superposition state
| ψ(x; Qm,A′) = cA′eiδA′ψA′(x; Qm,A′) + cA″eiδA″ψA″(x; Qm,A′) | (3) |
Neglecting diabatic transitions, the corresponding electronic populations are
![]() | (4) |
The vertical excitation energy is
| ΔE = VA″(Qm,A′) − VA′(Qm,A′) ≡ ℏω | (5) |
| ψ(x,t; Qm,A′) = cA′eiδA′ψA′(x; Qm,A′) + cA″eiδA″ψA″(x; Qm,A″)e−iωt, | (6) |
| |ψ(t)〉 = cA′eiδA′|ψA′〉 + cA″eiδA″|ψA″〉e−iωt. | (7) |
The corresponding one-electron density of the electrons at position r is obtained as the expectation value of the density operator,
, over the wave packet. It evolves in time as
![]() | (8) |
![]() | (9) |
![]() | (10) |
![]() | (11) |
These densities are computed by analytical integration of the N-electron wave packet over all electrons and spin degrees of freedom using ORBKIT.20,21
The expression for the time evolution of the electronic density is an approximation that depends on electronic coherence in the ground and excited states. This coherence can be measured by the overlap
| SA′,A″(t) = 〈χA′(Q,t)|χA″(Q,t)〉 | (12) |
Evaluations of SA′A″(t) require calculations of χA′(Q,t) and χA″(Q,t). Using the FC excitation picture, the initial nuclear wavefunction in the excited state is
| χA″(Q,0) = χA′,0(Q) | (13) |
Subsequently, χA″(Q,t) evolves on the PES VA″(Q) starting from this initial condition. The nuclear quantum dynamics of χA″(Q,t) is evaluated using the MCTDH method.19,24 For this purpose, the potential energy surface VA″(Q) is adjusted using the PotFit algorithm implemented in the Heidelberg package.19 More details on the dynamical simulations can be found in the SI, section S3.
We assume that the nuclear wavefunction in the ground state remains robust,
| χA′(Q,t) = χA′,0(Q), | (14) |
| SA′A″(t) ≈ 〈χA′,0(Q)|χA″(Q,t)〉 = 〈χA″(Q,0)|χA″(Q,t)〉, | (15) |
In the following, we consider the scenario where the FC transition transfers half of the population of the ground state to the excited state,
![]() | (16) |
For the present investigation, the most important property of the superposition state ψ(x,t; Qm,A′) is that it is not an eigenstate of reflection at the nuclear mirror plane,
| σψ(x,t; Qm,A′) ≠ ±ψ(x,t; Qm,A′), | (17) |
This result is also obtained directly from the character table (Table 1), cf. ref. 8 the two constituents of ψ(x,t; Qm,A′) have irreducible representations A′ and A″. The only symmetry element common to A′ and A″ is the identity E. Hence, the symmetry of the superposition state ψ(x,t; Qm,A′) is C1 instead of Cs. Consequently, ψ(x,t; Qm,A′) is chiral, although the nuclei still transform according to the Cs point group. The derivation in ref. 8 shows that if ψ(x,t; Qm,A′) is chiral, then its one-electron density ρ(r,t) is also chiral, except at the rare times when its time-dependent part vanishes, i.e. when
| cos(δA′ − δA″ + ωt) = 0 | (18) |
To document the chirality of the electronic density ρ(r,t) of the superposition state ψ(x,t; Qm,A′), we focus on its time-dependent part, divided by the scaling factor 2cA′cA″ (equal to 1 in the present scenario). Thus, we analyze the universal term
| cos(δA′ − δA″ + ωt)ρA′A″(r) | (19) |
The electronic density is periodic, with period
![]() | ||
| Fig. 2 Attosecond charge migration in the A′ + A″ superposition state of NSF. The time-evolution of the wave packet is documented by the universal transition density component, eqn (19), of the one-electron density, eqn (8). (a) in-plane view, with S pointing away from the reader; (b) top view, as in Fig. 1. The respective upper/lower panels show selected snapshots during the first/second half period of charge migration. The vertical dashed line marks the time at which chirality flips occur. In panels (a), the horizontal solid line emphasizes the mirror symmetry of the transition density over the two half-periods. Positive/negative isocontours at ±0.0025/a03 in orange/blue. | ||
Apparently, the electron density is always chiral except at the special time over the first half period
The series of snapshots in Fig. 2a and b also shows that the amplitude of the time-dependent term cos(δA′ − δA″ + ωt)ρA′A″ varies periodically, but the shape of ρA′A″ remains invariant. Note that the results are obtained for a 1
:
1 superposition state in a two-level systems, but they would be valid for different excitation scenarios, e.g., less efficient population transfer or non-zero phases.
To provide a quantitative measure of the magnitude of this effect, we choose to investigate the expectation value of the out-of-plane coordinate, z, as a function of time. It documents the asymmetry with respect to the molecular plane and the degree of chirality. The results are shown in Fig. 3. In the optimal scenario studied here, the magnitude of the induced chirality is found to be small. Yet, it is likely to be sufficiently large to be observed experimentally via the variation of the electric dipole perpendicular to the molecular plane.
![]() | ||
| Fig. 3 Evolution of the chirality, measured as the expectation value of the out-of-plane coordinate as a function of time, 〈z〉(t) = ∫∫∫zρ(r,t)dxdydz. | ||
The rather complex shape of the transition density is well approximated by the simple expression
![]() | (20) |
![]() | ||
| Fig. 4 Validity of the dominant-determinant approximation. Left: transition density matrix driving the attosecond chirality flip in eqn (19) obtained from the full many-electron wave packet. Positive/negative isocontours at ±0.01/a03 in orange/blue. Right: transition density matrix (top) obtained from the dominant-determinant approximation, eqn (20). Positive/negative isocontours at ±0.01/a03 in purple/green. The transition amounts approximately to a transition from HOMO to LUMO, which is depicted below. Positive/negative isocontours at ±0.1/a03 in purple/green. | ||
As explained in Section II, eqn (8) for the electronic density ρ(r,t) is an approximation that relies on electronic coherence in the A′ + A″ superposition state. A criterion for the validity of this approximation is that the magnitude of the autocorrelation function, |SA′A″(t)|, should remain close to 1. To investigate this, we calculate |SA′A″(t)| as outlined in Section II. The result is shown in Fig. 5. Apparently, |SA′A″(t)| decays rapidly. Nevertheless, during the first ∼ 1.3 fs, the values of |SA′A″(t)| remain sufficiently close to 1 to ensure approximate electronic coherence. This means that the present FC-excited superposition state ψ(r,t; Qm,A′) accounts for at least two electronic chirality flips, as illustrated in Fig. 2a/b.
![]() | ||
| Fig. 5 Early-time evolution of the electronic coherences for a wave packet prepared in the A′ + A″ electronic superposition state by FC excitation of NSF. | ||
Section S3 presents a detailed analysis of the rapid decay of |SA′A″(t)|. In brief, after vertical A′ → A″ FC excitation of (part of) the vibrational ground state χA′,0(Q), the nuclear wavepacket χA″(Q,t) on the excited uncoupled, adiabatic PES VA″(Q) rapidly departs from its initial state χA′(Q,0), which is centered at Qm,A′, and moves toward Qm,A″, the minimum of the excited-state PES. This causes rapid decay of the overlap 〈χA″(Q,0)|〈χA″(Q,t)〉. Consequently, the rapid loss of electronic coherence—which limits the number of chirality flips of NSF in the superposition state ψ(x,t; Qm,A′)—is primarily a consequence of the geometric shift from the potential minimum Qm,A′ to Qm,A″.
One might suggest that this simple approach could also be applied to any planar molecules with more than three atoms. While this may be true for special cases, there is a counterexample: X-ray excitation of formic acid HCOOH to a superposition state of the electronic ground state plus a very highly excited state induces pyramidalization.27 Consequently, the molecule which is achiral in the planar ground state is chiral in the pyramidal excited state. One can then no longer talk about electronic chirality in an achiral molecule. In contrast, triatomic heteronuclear molecules such as NSF cannot pyramidalize; they remain achiral as long as they are bent in both the electronic ground and excited states.
The present example NSF suffers from rapid electronic decoherence in the chiral A′ + A″ superposition state. Consequently, this allows only few chirality flips. The analysis in Section III shows that this disadvantage is mainly due to the shift of the minimum Qm,A′ of the potential energy surface VA′(Q) in the ground state A′ to the different minimum Qm,A″ of VA″(Q) in the excited state A″. As an outlook, this suggests searching for bent triatomic heteronuclear molecules with near or, in the ideal case, perfectly coincident minima Qm,A′ and Qm,A″ of the PES in the electronic ground A′ and excited A″ states. Such molecules should exhibit a much larger number of chirality flips in the A′ + A″ superposition states, compared to NSF. Nevertheless, NSF will serve as a reference for the—most probably—simplest approach to electronic chirality flips in achiral molecules.
| This journal is © the Owner Societies 2026 |