Open Access Article
S.
Kazim
a,
D.
Mastrippolito
b,
P.
Moras
c,
M.
Jugovac
c,
T.
Klimczuk
d,
M.
Ali
be,
L.
Ottaviano
bf and
R.
Gunnella
*ag
aSchool of Science and Technology Physics Section University of Camerino, Via Madonna delle Carceri 9, 62032 Camerino, MC, Italy. E-mail: roberto.gunnella@unicam.it
bDipartimento di Scienze Fisiche e Chimiche (DSFC), Università degli Studi dell'Aquila, Via Vetoio 10, 67100 L'Aquila, Italy
cIstituto di Struttura della Materia-CNR (ISM-CNR), S.S. 14, Km 163,5, 34149 Trieste, Italy
dFaculty of Applied Physics and Mathematics, and Advanced Materials Centre, Gdansk University of Technology, ul. Narutowicza 11/12, 80-233 Gdansk, Poland
eDepartment of Physics, Division of Science and Technology, University of Education Lahore, Jauharabad Campus, Pakistan
fCNR-SPIN UoS L' Aquila, Via Vetoio 10, 67100 L'Aquila, Italy
gINFN-Sez. Perugia, Via Pascoli Perugia, Italy
First published on 22nd December 2022
We investigate the experimentally challenging CrCl3 surface by photon energy dependent photoemission (PE). The core and valence electrons after cleavage of a single crystal, either in a ultra-high vacuum (UHV) or in air, are studied by keeping the samples at 150 °C, aiming at confirming the atomic composition with respect to the expected bulk atomic structure. A common spectroscopic denominator revealed by data is the presence of a stable, but only partially ordered Cl–O–Cr surface. The electronic core levels (Cl 2p, Cr 2p and 3p), the latter ones of cumbersome component determination, allowed us to quantify the electron charge transfer to the Cr atom as a net result of this modification and the increased exchange interaction between metal and ligand atoms. In particular, the analysis of multiplet components by the CMT4XPS code evidenced the charge transfer to be favored, and similarly the reduced crystal field due to the established polarization field. Though it is often claimed that a significant amount of Cl and Cr atomic vacancies has to be included, such a possibility can be excluded on the basis of the sign and the importance of the shift in the binding energy of core level electrons. The present methodological approach can be of great impact to quantify the structure of ordered sub-oxide phases occurring in mono or bi-layer Cr trihalides.
structure (i.e., BiI3 like) with transition to monoclinic (C2/m),9 with metal ions in a honeycomb coordinated geometry with Cl6 edge-sharing octahedra. As a result, trilayers of Cl–Cr–Cl are stacked along the c-axis (c = 0.69 nm) while the thickness (Cl–Cl distance) is 0.27 nm as sketched in Fig. 1 for the in-plane and vertical sections of the surface structure. In the same sketch, the possible hollow adsorption position of oxygen is shown. The characteristic properties of CrCl3 with respect to other halides might be related to the presence of a native termination layer14,15 behaving differently from the normal state, resulting in a material with electronic charge transfer (CT) rather than a pure Mott–Hubbard (MH) system16 with strong implications for the resulting magnetization. The magnetic properties of CrCl3 have been recently reported in ref. 17.
In fact, Cr-trihalides belong to the Mott–Hubbard (MH) insulators family, whose p-states do not contribute to the valence electrons while the d-states are responsible for the transport and magnetic properties. Nevertheless, upon varying the radii of the atomic components, the presence of hybridization might induce 2D materials to increase charge transfer to obtain half-metallicity (HM) i.e., the presence of a metallic spin channel and insulating one in a manner different from the Mott–Hubbard mechanism.18 Several transition metal compounds are predicted to exhibit such a half-metallic character. There are Density Functional Theory (DFT) studies that predicted the transition from the insulator to HM in trihalides after introducing point defects, chemisorbed atoms and carrier dopants at specific locations affecting in various ways the magnetic properties.6,19,20 Another important defect type is the atomic vacancy site also proposed as a way to reach half-metallicity.19 In fact, the above modifications might induce the ferromagnetism (FM) of 2D materials even though their bulk counterparts are antiferromagnetic (AFM).21 After doping by means of holes/electrons in a two-dimensional Cr–O–Cl hexagonal system, the enhancement of FM interaction by superexchange coupling between Cr atoms mediated by the anion/halogen atom might occur. Such enhancement is assisted by structural distortion, and consequent filling of the dz2 state from the initial t↑↑↑2g configuration as expected for Cr+3 atoms.6 In a previous work, we determined the valence electron structure of the same system after exfoliation in air, by means of valence band PE and scanning tunnelling spectroscopy (STS) with the aim to single out the formation of a Cr–Cl–O hybridization state, correctly identified by total energy calculations.15 The above study established the link to a possible future technological implementation of the material, but a necessary validation under vacuum conditions is one of the aims of the present paper. Experimental attempts to investigate beyond the application-oriented properties must rely on X-ray absorption, emission22 and photoemission spectroscopy (PES).23 In particular, the latter is an ineludible way to characterize the surface and modifications occurring during the preparation. Its surface sensitivity achieved by the short-range character of the electrons when passing through the matter at a few tens of eV kinetic energy,24 is able to better depict the properties of the most superficial layer of the crystal under study. To this aim, the tuning of the photon energy guaranteed by the synchrotron radiation facilities is an enormous advantage.
In the present work, the surface represents our best approximation of 2D crystals with quality comparable to the bulk material.25 On the other side, optical techniques or electron microscopy techniques are less sensitive as they average over several layers of the sample or include unwanted topographic defects like in STS. Photon energy-dependent PE by using synchrotron radiation is described in Section II. In Section III the analysis of photoemission spectra of electrons from core levels will be described, together with the estimation of the electronic charge transfer between the neighbour atoms. Similarly, the spectra from the valence band and their dependence on the photon energy reinforcing the results are reported as well. Finally, conclusions follow in Section IV.
To expand our knowledge about the system, we performed X-ray photoemission spectroscopy (XPS) measurements using a tunable and monochromatized photon energy source (0.1 × 0.3 mm) available at the “VUV-Photoemission” beamline of the Elettra synchrotron in Trieste. The photon energy was varied between 40 and 700 eV, with horizontal polarization and with an incidence angle of 45°. The spectra were acquired using a Gammadata Scienta R4000WAL analyzer in a normal emission geometry, with a total energy resolution (light source and electron analyser) of about 0.1 eV, while maintaining the sample temperature at 150 °C in order to prevent charging effects. The binding energy (BE) scale was calibrated by using adventitious carbon as a reference at 284.8 eV. We used Fityk 1.3.1 data analysis software for processing Cl 2p core level data after subtracting the Shirley background while the Voigt line shape was used for multicomponent analysis of the spectra. The Cr core levels could not be treated similarly because of the multiplets taking place of the atomic doublet. With regard to the Cr 2p and 3p analyses a conventional treatment of spectrum components28 by means of Voigt functions, would lead to unrealistic lineshape parameters (spin–orbit splitting and branching ratios). For the above reason, we took advantage of a multiplet component analysis based on calculations from the CTM4XPS program.29–31 The procedure for the determination of the transfer of electronic charge has been described in detail in the ESI† and the parameters used for the calculations are listed in the following together with transfer parameters for reference materials CrCl316 and Cr2O3.32
:
1.
Weak C 1s and O 1s signals were also visible in the in situ cleaved sample. The corrected atomic sensitivity ratio was derived thoroughly in the ESI.† The modification of CrCl3 was studied by improving the surface sensitivity of the PE experiment by changing the photon energy.
To investigate the surface character, we compared the spectra recorded at normal emission at 700 eV photon energy, corresponding approximately to 1 nm probing depth, with those having higher surface sensitivities obtained by lowering the photon energy. The amount of oxygen in in situ cleaved samples corresponded to 1% and 2% of the Cl 2p peak at, respectively, 700 and 650 eV. If corrected for the 1
:
2 factor of the atomic sensitivity of O with respect to Cl at about 700 eV photon energy,33 we can estimate for in situ cleaved samples an amount of 1 to 4% in oxygen while going from 700 to 650 eV and correspondingly increasing the sensitivity towards the surface. This amount is about a factor 5–10 times less than that observed in ex situ prepared samples and it is of different character as will be evident below.
![]() | ||
| Fig. 3 Normalized Cl 2p PE core level spectra of UHV cleaved (a) and air cleaved (b) CrCl3. Photon energy was varied from 700 to 270 eV to increase surface sensitivity. | ||
| Parameters used for Cl 2p fitting for CrCl3 | |||||
|---|---|---|---|---|---|
| Exp. | hν (eV) | Gw (eV) | FWHM (eV) | SO (eV) | BR |
| Vacuum | 700 | 0.47 | 0.85 | 1.57 | 0.35 |
| 650 | 0.46 | 0.83 | 1.57 | 0.45 | |
| 350 | 0.45 | 0.86 | 1.6 | 0.55 | |
| 270 | 0.57 | 1.0 | 1.57 | 0.45 | |
| Air | 700 | 0.53 | 1.0 | 1.57 | 0.43 |
| 650 | 0.54 | 1.0 | 1.55 | 0.46 | |
| 350 | 0.53 | 1.1 | 1.57 | 0.45 | |
| 270 | 0.53 | 1.1 | 1.57 | 0.47 | |
The spin–orbit splitting energy value of Cl 2p doublets is between 1.55 eV and 1.6 eV, and the branching ratio varies around the expected 1
:
2 value by less than 20%. This deviation in the branching ratio may be related to the angular resolution of the analyzer and to photoelectron diffraction effects.34 Gaussian broadening equal to 2
ln(2) × Gw and full width half maximum (FWHM) were varied by less than 10% during photon energy tuning. The parameters used for the fitting are explicitly listed in Table 1 for each photon energy, including the branching ratios (BRs) and the spin orbit (SO) splitting of the Cl 2p doublet.
The main component is found at 199.6 eV binding energy. With surface sensitivity, a second peak is seen at a higher binding energy (≈0.9 eV). This fact excludes the case of Cl vacancy sites on the surface of Cr trichloride, already observed at lower binding energies after prolonged annealings at T ≥ 200 °C.15 This would rather create the conditions of increased charge available from the Cr first neighbours for each Cl atom, leading to a lower binding energy component of the Cl 2p core level, that we cannot detect within the sensitivity of the technique. After annealing at 300 °C (see the ESI†) clear signatures of vacancy formation are eventually observed. Similarly, the presence of lower energy shift components is evident in the air-cleaved samples of Fig. 3(b). The higher binding energy component of Cl 2p in Fig. 3(a) covers from 0% to 30% of the main peak when changing to more surface sensitive energies (top curves) and at the first sight is of unclear origin. This must be assigned to the formation of a Cr–O–Cl surface phase as the component is not seen in the experiment of Mastrippolito et al.15 done in bulk sensitivity/air cleaved experiments. We stress that the present feature is not due to a simple Cr oxidization and cannot be relegated to the case of adventitious oxidation of the surface. As no interaction occurs between Cl and O, the origin of that shift is related to the energy stability induced by the charge transfer to Cr(III) atoms and of the consequent transition from a Cr low spin state S = 3/2 to a high spin S = 2 configuration that might be even 2 eV more stable35,36 than the low spin state. A consequence would be the distortion of the local geometry and relaxation of the Cr–Cl bond leading to a high energy shift of the core level. In particular, the Cl–Cr–Cl bond will assume two different configurations with bond angles different from 90° but split into two of 98° and 83° respectively. In addition a slight extension of the bond length due to oxygen intercalation and consequent interlayer distance expansion also occurred.15
In Fig. 5(a) the spectrum taken at 700 eV, for the samples cleaved in UHV, has been reproduced with components calculated using CTM4XPS with parameters reported in Table 2. The contribution of Cr 2p with two different charge states, namely CrCl3 and the state called CT (charge transfer), in a ratio of 9
:
1 is the best combination which fits the experiment at 700 eV in Fig. 5(a). The individual curves obtained by CTM4XPS were also plotted in Fig. 5(b) for the experiment at 650 eV. In this case, a 4
:
6 ratio is obtained with a predominance of the CT component and slight broadening implying a certain degree of disorder. The main information obtained from the comparison of the calculated Cr 2p spectra is the increase of a CT phase, which we can claim to be related to the presence of a structure as reported in Fig. 1. In the case of full occupation of oxygen in “hollow” positions, following the model of Mastrippolito et al.,15 the O–CrCl3 surface would have a composition given by Cl
:
Cr
:
O equal to 24
:
8
:
3, i.e., the oxygen would be about 9.5% of the atomic composition. Actually, a maximum content of 5% of atomic oxygen was measured from the PE intensity of the O 1s core level in Fig. 2. We can conclude that the coverage of this heterogeneous phase corresponds to about 50% of the surface. Such a value must be intended as a lower limit because of the depth profile sensitivity of the XPS, which is slightly larger than the thickness of the layer structure of about 2.75 Å, as reported in Fig. 1. We calculated in Fig. 6, the 90% confidence interval of the intensity ratio (CrCl3-CT)/CrCl3 of the Cr 2p core level at various electron mean free paths (MFPs) depending on the photon energy. The two values reported in red squares in Fig. 6 correspond to the experimental ratio intensities of surface to the bulk component of 1.5 and 0.12 respectively, as found for photon energies of 650 eV (estimated MFP about 4 Å) and 700 eV (estimated MFP of 8 Å). The intensity ratio of the two Cr 2p components can be calculated using following eqn (1)38 as a function of the mean free path λ and oxide phase coverage percent β (to be determined):
![]() | (1) |
![]() | ||
| Fig. 6 Intensity ratio of surface vs bulk Cr 2p components taken at 650 and 700 eV, respectively, as a function of the electron mean free path. The upper and lower curves represent the 90% confidence interval for such an intensity ratio. Comparison with the two experimental determinations (red squares on the basis of the estimated mean free path during the respective photon energy Cr 2p photoemission38). | ||
As can be observed from the confidence interval, the comparison is well verified for the surface-sensitive case in Fig. 6, with an estimated β = 70% CT phase on the first layer; while the calculation overestimates the Cr–O–Cl component in the bulk sensitive experiment. The latter is the probable occurrence of interlayer forward focusing of photoelectrons also known as the lens effect induced by collinear scattering39 amplifying the bulk signal. The latter considerations are a further evidence of the high quality of van der Waals crystals because collinear effects would be strongly damped in disordered systems.40
Such an effect, enhanced using a high-resolution solid angle acceptance analyser, slightly affects the comparison of the PE intensity with the atomic composition because of the anisotropy of the detected intensity. More reliable is the result obtained with surface sensitive photons. As a direct result of this comparison, the 70% contribution of the oxide phase of Fig. 1 would correspond to the amount of 6% of atomic oxygen. This estimated figure is consistent with the other estimate obtained from the O 1s to Cl 2p peaks ratio taken at 650 eV normalized by respective sensitivity factors of O 1s and Cl 2p (1
:
2). Such an evidence further confirm that the present surface is a stable and chemically ordered termination phase of CrCl3, in principle a candidate to harness the functionality of the 2D properties of the CrCl3 layers. Within this hypothesis, the origin of a Cr 2p lower binding energy shifts after the formation of the O–CrCl3 phase might be due to the O−2 ions in “hollow” positions polarizing the entire O–Cr–Cl structure (Fig. 1) in a way similar to the onset of an electrostatic cage on Cr atoms, provided a charge transfer mechanism from Cl 3p levels to Cr 3d ones. The additional covalent bonding induced by the oxygen in position “hollow” would be at the origin of the optimal parameter Δ = 5.5 eV, charge transfer energy lower than the 6.5 eV expected in CrCl3.16
Another parameter of the model that had to be reduced was the crystal field of 10 Dq value to 0.5 eV from the nominal value of 2.0 eV, which suggested the transition from the Mott–Hubbard insulator to a polarized metal band configuration.41
We note that in the case of hypothetical Cr vacancies,19 the effect on Cr 2p core electron levels would be mediated by Cl atoms, which would induce a higher oxidation state on the nearby Cr atoms, leading to a higher binding energy that is not observed.
Here, we used two 10 Dq values, i.e., 4 eV and 2 eV for spectra related to bulk and surface, respectively, to take into consideration the reasons above. Noteworthily, in all presented cases, we always consider equal to zero the valence spin–orbit parameter.30,31 We have taken the Lorentzian and Gaussian broadening σ ≈ 0.35 eV for surface sensitive spectra and 0.3 eV for the bulk ones. The parameters used to fit the Cr 3p core electron level spectra are reported in Table 3.
| Charge transfer energy for Cr 3p core level | |||||||
|---|---|---|---|---|---|---|---|
| Compounds | dn | Delta | U dd | U pd | 10 Dq | T e | T 2g |
| CrCl3 | d3 | 5.4 | 3.3 | 3.2 | 4.0–2.0 | 1.6 | 0.8 |
| CT | d3 | 5.5 | 5.5 | 6.0 | 0.5 | 1.6 | 0.8 |
Fig. 7 shows the Cr 3p spectra where the black curves correspond to the experimental spectra at different photon energies and the red curves are associated with a mix of normal and CT phases. It is quite evident that the CT phase, we supposed due to the O–Cr–Cl contribution, increases from 20% to 70% as one moves to the more superficial layers of the sample by reducing the photon energy.
![]() | ||
| Fig. 8 Valence band spectra of UHV cleaved CrCl3 with the variation of photon energies from 700 to 70 eV. The red and green dotted lines represent the Cl 3p and Cr 3d states. | ||
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d2cp04586a |
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