2
[13]. An ideal candidate for such an observation would be a single layer of FeSe grown on SrTiO3(001), an ideal two-
dimensional high temperature superconductor (HTSC) [14–20]. In the case of ultrathin films the inversion symmetry
in the direction perpendicular to the surface is broken. A large SOC together with the broken inversion symmetry
can provide the necessary fundamental basis required for the observation of topological states in the system [21,22].
Hence a direct probing of SOC in this class of materials is essential in connection with the possibility of the formation
of topological states. Unfortunately, the strength of SOC in such two-dimensional superconductors is hitherto fully
unknown.
Irrespective of the importance of SOC for the topological superconductivity, the presence of this interaction is of
prime importance to understand the underlying physics of HTSC in general [21,23]. In most theoretical approaches
describing the microscopic mechanism of superconductivity and Cooper pairing of electrons SOC is assumed to be very
small and, therefore, has been neglected. There are only a few theoretical models which include SOC in bulk HTSCs,
showing that the presence of this interaction is essential in the determination of the symmetry of the order parameter as
well as the electronic states involved in superconductivity [21,23]. Generally the impact of SOC becomes increasingly
important when reducing the systems’ dimensionality. This is due to the emergence of new symmetry aspects in
low-dimensional solids. Surprisingly, so far no direct signature of SOC and its impact in ultrathin (two-dimensional)
HTSCs have been reported experimentally. A direct measure of SOC would, therefore, be extremely valuable in the
context of microscopic physical mechanism behind high temperature superconductivity in low-dimensional HTSCs.
Here by performing high resolution spectroscopy of spin-polarized slow electrons on epitaxial FeSe monolayers
grown on Nb-doped strontium titanate SrTiO3(001), a prototypical two-dimensional superconductor, we demonstrate
that the frequency and momentum dependent scattering cross-section depends strongly on the spin of the incoming
electron. A careful analysis of the spectra reveals that the observed effect is due to the presence of a considerably
large SOC in this system. Such a large SOC together with other symmetry aspects provides the required ingredients
for the formation of topologically nontrivial states and would shed light on the mysterious origin of superconductivity
in this system.
II. RESULTS
The epitaxial FeSe monolayer was grown by molecular beam epitaxy on Nb-doped SrTiO3(001) (hereafter STO).
The dynamic charge response of the system was probed by means of spin-polarized high-resolution electron energy-
loss spectroscopy (SPHREELS) (see Sec. V A of Materials and Methods for details on the substrate preparation, film
growth and SPHREELS experiments). The scattering geometry is sketched in Fig. 1a. The scattering plane was
chosen to be parallel to the [100]-direction of STO(001), as indicated in Fig. 1band c. This would allow probing
the dynamic response of the system along the high symmetry ¯
Γ–¯
X direction of the surface Brillouin zone (SBZ). In
order to be sensitive to the spin-dependent effects associated with the broken inversion symmetry in the direction
perpendicular to the surface, we used a longitudinally spin-polarized electron beam with the spin orientation being
parallel and antiparallel to the scattering’s plane normal vector n(see Supplementary Note 1 for an explanation).
These incoming spin states are denoted by |+iand |−i, respectively. Figure 1dshows the spin-resolved spectra
recorded in the superconducting state of the sample and using an incident electron beam energy Ei= 4.07 eV. The
spectra were recorded at the ¯
Γ–point of SBZ. Beside the so-called zero loss peak at the energy-loss ~ω= 0, one
observes several features as a result of the excitation of several collective modes. The peaks with lower intensity at
~ω= 11.8, 20.5, 24.8 and 36.7 meV represent the various phonon modes of the FeSe film itself [24–26]. More obviously
the so-called Fuchs-Kliewer (FK) phonon modes of the underlying STO substrate can also be recognized at the loss
energies ~ω= 59.3 and 94.5 meV [27,28].
Generally the spectral function S(q, ω) measured by SPHREELS directly reflects the dynamic response of the
collective charge excitations in the system. This quantity is proportional to the imaginary part of the dynamic
charge susceptibility Imχ(q, ω) [29–31]. The electrons are scattered by the total charge distribution of the sample
and, hence, the scattering intensity carries information regarding collective excitations of the lattice i.e, phonons,
collective electronic excitations i.e., plasmons and any type of excitation representing a hybrid mode of these two [31].
The most interesting observation here is that S(q, ω) depends strongly on the spin. The spin asymmetry defined as
A=I|+i−I|−i/I|+i+I|−iis shown in the lower part of Fig. 1d. Here I|+iand I|−i denote the intensity of the
scattered electrons when the incoming electron’s spin is parallel and antiparallel to n, respectively.
In order to shed light on the origin of the observed spin asymmetry, its dependency on the physical variables e.g.,
temperature, incident energy, and wavevector transfer qwas measured and the results are summarized in Fig. 2.
Data presented in Fig. 2aclearly demonstrate that the spin asymmetry does not depend on temperature. In both
superconducting and normal states one observes a value as large as 11%. This fact indicates that the spin asymmetry
is not related to the superconducting (or magnetic) phase transition and is due to the intrinsic SOC of the system.
Next we check the dependence of the spin asymmetry on the incident beam energy Ei. Generally for very low incident