
2
enhanced by interfacial effects [16–21]. It has been observed by means of several experimental techniques, including
angle-resolved photoemission spectroscopy, that FeSe ML is strongly electron doped [12,17,20,22–24]. The origin of
this large carrier density inside FeSe ML has been postulated to be due to the charge transfer from the substrate into
the film [18,25]. However, a direct and unambiguous evidence of such a large charge transfer has not been reported
experimentally.
Here by probing the dynamic charge response of the FeSe/STO interface, by means of high-resolution spectroscopy of
slow electrons, we show that the experimentally measured frequency and momentum resolved dynamic charge response
cannot be explained by assuming a simple film/substrate model only. Our detailed analysis unambiguously identifies a
charge free depletion region in the STO substrate at the interface with FeSe ML. The existence of such a thick depletion
layer is accompanied with a considerably large charge transfer from the STO into FeSe ML. The presence of the
depletion region along with the large interfacial charge transfer leads to a substantial band bending and renormalization
of the electronic bands at the interface. In addition to the fact that our findings contribute to the understanding
of HTSC in FeSe ML, they would provide guidelines for designing new high-temperature superconductors through
interface engineering. Moreover, the presence of a depletion layer at the interface is rather general and is expected to
be observed in many combinations of VdW MLs put in contact with dielectric oxides or semiconducting substrates.
II. RESULTS AND DISCUSSIONS
The frequency and momentum resolved dynamic charge response of the epitaxial FeSe MLs grown on Nb-doped
STO(001) (hereafter Nb-STO) was probed by means of high-resolution electron energy-loss spectroscopy (HREELS)
(see Sec. IV A of Materials and Methods for details), using slow electrons. Generally, in the electron scattering
experiments from surfaces the scattering near the specular geometry is governed by the dipolar scattering mechanism
[26]. In this region, known as dipolar lobe, the incoming electron interacts with the total charge density of the sample
via dipolar interactions. This means that the scattering intensity includes information from both electrons as well as
the ions in the sample. The dipolar interaction is of Coulomb nature and hence is long range. Therefore, the scattered
electrons carry information from the charge density fluctuations located not only near the surface region but also
far below the surface, depending on their kinetic energy. The lower the kinetic energy the more surface sensitivity
[27–29]. Since in our experiments we are mainly interested in the properties of FeSe ML and the interfacial region,
we use electrons with kinetic energies as low as 4 to 8 eV.
Figure 1ashows the HREEL spectra recorded on the surface of FeSe ML grown on Nb-STO(001). The spectra were
recorded at a temperature of T= 15 K, below the superconducting transition temperature of the sample and at two
different incident beam energies, namely Ei= 4.07 eV and Ei= 7.23 eV. The spectral function S(qk, ω) measured
by HREELS directly reflects the dynamical response of the collective charge excitations in the system and is directly
proportional to the imaginary part of the dynamic charge susceptibility Imχ(q, ω) [30,31]. Since the electrons are
scattered by the total charge distribution of the sample, the scattering intensity must include information regarding
collective ionic excitations i.e, phonons as well as collective electronic excitations i.e., plasmons. Moreover, any type
of excitation representing a hybrid mode should also be excited within this mechanism. In the measured spectra
presented in Fig. 1aone observes several interesting features. Besides the elastic peak at the energy-loss of ~ω= 0
(zero-loss peak, ZLP) there are small peaks at ~ω= 11.8, 20.5, 24.8 and 36.7 meV. These are the phonon peaks of
FeSe ML, which match perfectly to those probed on FeSe(001) single crystals [32–34] and also those reported for the
FeSe films on Nb-STO(001) of different thicknesses [35]. The most prominent features are the so-called Fuchs-Kliewer
(FK) phonons of the STO substrate, which appear at the energies of ~ω= 59.3 and 94.5 meV.
In principle, electrons can also excite multiple quanta (higher order harmonics) of FK phonons. Hence one should
observe these excitations at the multiple frequencies of the principle excitations. The most interesting observation is
that unlike the bare STO surfaces [36], in the case of FeSe/STO the higher order harmonics of the FK modes are
strongly suppressed. Note that within the dipolar-scattering mechanism for a semi-infinite substrate the intensities of
dipolar losses normalized to the elastic peak intensity scale in a 1/√Eimanner, where Eiis the energy of the incident
electron beam. This means that the lower the incident energy the larger the amplitude of FK modes. The intensities
of the higher order harmonics of FK modes obey a Poisson distribution [26,37]. Hence, in the spectra recorded using
such low incident energies one shall clearly observe both the FK modes and their higher order harmonics, if they are
present in the system. We will see that the strong suppression of the higher order harmonics of FK modes is due to
the presence of the free charge carriers in FeSe ML and in the deeper layers of the Nb-STO substrate.
In order to shed light on the origin of the observed phenomenon the measured HREEL spectra were simulated. The
simulation is based on the dipolar scattering theory (see Sec. IV B of Materials and Methods for details). Our analysis
indicates that considering ML FeSe on a semi-infinite doped STO(001) cannot explain the experimental spectra. The
best model explaining the experimental spectra is considering a system composed of one ML of FeSe on 17 unit cells
of charge free insulating STO(001) on top of a semi-infinite Nb-STO(001). In this model the Fe plane in FeSe ML is