Introduction

Kagome metals have attracted much attention due to the special lattice structure and associated physical properties1,2,3,4. The ongoing interest is further energized by Kagome superconductors AV3Sb5 (A = K, Rb and Cs), in which many exotic phenomena have been observed5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38,39,40,41,42,43,44,45,46,47,48,49,50, ranging from superconductivity5,6,7,8,9, charge density wave (CDW)5,6,10,11,12,13,14,15,16,17,18,19, nematic order20,21, pair density wave22, topological states5,23,24 and the time-reversal symmetry breaking state17,25,26,27. While the origins of these phenomena remain unclear, it is interesting that most of them are closely related to the CDW state5,6,10,11,12,13,14,15,16,17,18,19. In this regard, it is important to understand the driving mechanism of the CDW. Two scenarios have been primarily suggested15,29,30,31,32,33,34,35,36. The first is associated with the electronic instability, presumably driven by Fermi surface nesting15,29,30,31,32, and the second is related to the structural instability via electron-phonon coupling15,32,33,34,35,36. In order to examine the origin, doping evolution of the CDW has been experimentally investigated by chemical element substitutions38,39,40,41,42,43,44,45. Nevertheless, both the carrier concentration and the crystal lattice have been changed in this process. Surface doping has also been performed by Cs surface deposition46. Comparing to the bulk element substitutions, the surface doping primarily induces carriers (electrons) to the surface layers of the samples46. Its application on a pristine CsV3Sb5 compound has led to a monotonic suppression of the CDW order46. Despite the continuous efforts, it remains challenging to differentiate the roles played by electron and lattice degrees of freedom38,39,40,41,42,43,44,45,46.

In this paper, we investigate the evolution of CDW order in CsV3Sb5 via a combination of both bulk and surface doping. Angle-resolved photoemission spectroscopy (ARPES) measurements, which are sensitive to both doping methods51, have been carried out to track the evolution of the CDW order in this material. First, Ti substitution of V is applied to the bulk crystal of CsV3Sb5, which induces hole doping and modifies the V Kagome net simultaneously. Continuous Cs surface deposition is then carried out on the CsV3-xTixSb5 samples, which gradually induces electrons to compensate the holes doped by the Ti substitution. It is interesting that the CDW order is reversible as a function of carrier concentration in the lightly Ti doped regime. This is evidenced by the CDW gap, which disappears with Ti doping, but reappears with Cs surface deposition. However, excessive Ti bulk doping permanently destroys the CDW order, which becomes irreversible by tuning the carrier concentration. These results reveal a two-dimensional phase diagram of the CDW order in doped CsV3Sb5, and provide key insights to the associated driving mechanism.

Results

Evolution of CDW as a function of bulk and surface doping

Figure 1 shows the electronic structure of CsV3-xTixSb5 as a function of Ti bulk doping (see Supplementary Note 1 and Supplementary Fig. 1 for the sample characterization), measured at a low temperature (10 K). The photoemission measurements are carried out along Γ-K-M direction, where the CDW gap is most clearly revealed in the pristine CsV3Sb5 compound32,47,48. In order to visualize the evolution of the gap, low energy spectra around the van Hove singularity (vHs, marked by the red dotted boxes in Fig. 1a–d) are symmetrized with respect to the Fermi level (EF) (Fig. 1e–h). It is clear that the CDW gap decreases with Ti doping and disappears at doping levels x ≥ 0.13 (Fig. 1g, h). This is quantified by the corresponding energy distribution curves (EDCs) (Fig. 1i–p), where both Fermi–Dirac divided and symmetrized EDCs reveal the same doping evolution. Momentum dependence of the CDW gap is also examined on a Ti doped sample (x = 0.03), which is largely consistent with that of the pristine CsV3Sb5 compound, but with an overall smaller magnitude of the gap (Fig. 1q–s).

Fig. 1: Electronic structure of CsV3-xTixSb5 as a function of the Ti substitution level, measured at 10 K.
figure 1

ad Photoelectron intensity plot of the band structure along the Γ-K-M direction on CsV3-xTixSb5 samples with x = 0 (a), 0.08 (b), 0.13 (c) and 0.39 (d). eh symmetrized low energy spectrum near the vHs region in (ad). ip EDCs in the red dotted boxes in (ad). The EDCs are divided by the Fermi–Dirac function (i, k, m, o) and symmetrized with respect to EF (j, l, n, p), respectively. EDCs at the Fermi momenta are highlighted in blue. The EDC peaks are marked by triangles and circles. q Schematic Fermi Surface of CsV3-xTixSb5 (x = 0.03). r, s EDCs at representative momentum points. The momentum locations of the points are shown in (q).

Next, Cs surface doping is gradually carried out on the CsV3-xTixSb5 (x = 0.13) sample at a fixed low temperature (10 K). As illustrated in Fig. 1 (also shown in Fig. 2a, e, f), the CDW gap is completely suppressed by Ti doping in this sample. Upon Cs surface doping, a slight downward shift of the V bands is observed (Fig. 2a–d, for example, see the band top near K point, marked by the black triangles). Most strikingly, a spectral weight suppression starts to appear near EF, indicating the possible reappearance of an energy gap. This behavior is quantitatively revealed by the EDCs around the vHs region, where an energy gap gradually forms at EF as a function of the Cs surface doping (Fig. 2e–l). In order to examine whether the gap opening is associated with the reappearance of the CDW order or created by extrinsic effects (e.g., a possible localization effect induced by disorders), the Cs surface doping is repeated on the CsV3-xTixSb5 (x = 0.13) sample, but at a much higher temperature (100 K). Different from the behavior at low temperature, now the system remains gapless after the Cs surface doping (Fig. 2m–r). Nevertheless, the energy gap starts to appear on the band near the vHs (with V d-orbitals) when the temperature is cooled down to ~40 K (Fig. 2o, p). This gap becomes more evident at a lower temperature of 10 K (Fig. 2o, p). On the contrary, the band around the Γ point (with the Sb P-orbital) remains gapless at all temperatures (Fig. 2q, r). The above temperature and momentum (orbital) dependent behaviors of the gap are highly consistent with those of the CDW gap, demonstrating the reappearance of the CDW order in this system.

Fig. 2: Evolution of the electronic structure with Cs surface doping on the CsV3-xTixSb5 (x = 0.13) sample.
figure 2

ad Photoelectron intensity plot of the band structure along the Γ-K-M direction as a function of Cs surface doping at 10 K. el EDCs in the red dotted boxes in (ad). The EDCs are divided by the Fermi–Dirac function (e, g, i, k) and symmetrized with respect to EF (f, h, j, l), respectively. EDCs at the Fermi momenta are highlighted in blue. m, n Photoelectron intensity plot of the band structure along the Γ-K-M direction before (m) and after (n) Cs surface deposition at 100 K. The red arrows mark the Fermi momenta. o, p Temperature dependence of the EDC at the Fermi momentum near the vHs. To reveal the gap opening, the EDC is divided by the Fermi–Dirac function (o) and symmetrized with respect to EF (p), respectively. q, r Same as (o, p), but measured at the Fermi momentum near Γ. The black triangles in (c, d, n) mark the band top between Γ and K.

In order to further understand the evolution of the CDW order, the surface Cs doping is carried out on another CsV3-xTixSb5 sample, but with a higher bulk doping level (x = 0.39) at 10 K. Apparently, the CDW order is completely suppressed in this sample before the Cs surface doping, evidenced by the absence of the CDW gap (Fig. 3a, e, i, j). Upon the Cs doping, an overall downward shift of the V bands is observed as before (Fig. 3a–d). We note that excessive Cs doping has been applied on this sample (Fig. 3c, d) to ensure that the holes induced by the higher level of Ti substitution are sufficiently compensated and a similar total carrier concentration is achieved as before. This is evidenced by similar positions of the energy features on the band structure of the two samples after Cs deposition (e.g., compare the band top between Γ and K in Figs. 2c, d, n and 3c, d, marked by the black triangles). However, distinct from the earlier case, no evidence of gap opening is observed on the CsV3-xTixSb5 (x = 0.39) sample with Cs surface doping. This gapless state remains robust, regardless of the electron doping level induced by the Cs surface deposition (Fig. 3e–p).

Fig. 3: Evolution of the electronic structure with Cs surface doping on the CsV3-xTixSb5 (x = 0.39) sample.
figure 3

ad Photoelectron intensity plot of the band structure along the Γ-K-M direction as a function of Cs surface doping at 10 K. The black triangles in (c, d) mark the band top between Γ and K. eh Symmetrized low energy spectrum near the vHs region in (ad). ip EDCs in the red dotted boxes in (ad). The EDCs are divided by the Fermi–Dirac function (i, k, m, o) and symmetrized with respect to EF (j, l, n, p), respectively. EDCs at the Fermi momenta are highlighted in blue.

Two-dimensional phase diagram of the CDW order

The above bulk and surface doping dependent measurements (Fig. 4a–c) reveal a two-dimensional phase diagram of the CDW in doped CsV3Sb5 (Fig. 4d). First, the CDW order is monotonically suppressed as a function of the Ti bulk doping, and the CDW gap disappears at the doping level of x = 0.13. Then, continuous surface doping at the fixed Ti doping level (x = 0.13) leads to the reappearance of the CDW gap. However, the Cs surface doping shows little effect on the sample with a higher Ti doping level of x = 0.39. The sample remains gapless, regardless of the surface doping level.

Fig. 4: Two-dimensional phase diagram of the CDW in doped CsV3Sb5 and total energy profiles of CsV3-xTixSb5.
figure 4

ac Schematics of the doping processes. d two-dimensional phase diagram of the CDW gap in CsV3Sb5 as a function of Ti substitution and Cs surface deposition. eg Calculated total energy of pristine CsV3Sb5 (e), CsV3-xTixSb5 (x = 0.125) (f), and CsV3-xTixSb5 (x = 0.375) (g). ΔE represents the relative total energy with respect to that of the Kagome structure. It is shown in the 2 × 2 × 2 supercell (72 atoms) for all cases.

Discussion

Finally, we discuss the implications of such an experimental phase diagram. First, the Ti bulk doping changes both the carrier concentration and the lattice of the material. On one hand, the substitution of V atoms by Ti atoms effectively induces holes into the Kagome layer. On the other hand, the new Ti atoms would inevitably modify the original V Kagome net and affect the lattice vibration. The totality of these effects results in the suppression of the CDW order. Second, the Cs surface doping primarily induces electrons to the sample. In pristine CsV3Sb5, a suppression of CDW with Cs surface doping has been reported46, where the surface induced electrons may shift the carrier concentration away from the optimal doping. On the other hand, the electrons induced by Cs surface deposition would compensate the holes doped by Ti substitution in the CsV3-xTixSb5 compound. The reappearance of the CDW order in the lightly Ti doped regime (x = 0.13) demonstrates that the carrier concentration is important for the CDW. It also provides a tuning knob to manipulate the CDW order. However, the suppression of CDW order becomes irreversible by surface doping in the heavily bulk doped regime (x = 0.39), which indicates that the carrier concentration is not the only controlling parameter of the CDW. In order to better understand the role of lattice, we have calculated the total energy profiles of CsV3-xTixSb515,52,53 at the Ti doping levels of x = 0 (pristine CsV3Sb5, Fig. 4e), x = 0.125 (Fig. 4f) and x = 0.375 (Fig. 4g) (see Supplementary Note 2 for the details of the calculation), which are very close to the doping levels of the samples measured in the experiments. It is clear that the Kagome structure is unstable in the pristine compound, in which the Inverse Star of David (ISD) structure has the lowest total energy15 (see Supplementary Fig. 2 for the schematics of Kagome, Star of David and Inverse Star of David structures). This lattice instability persists to the Ti doping level of x = 0.125 (Fig. 4f), but disappears at x = 0.375 (Fig. 4g). These results, when combined with the experimental observations, point to a unified understanding of the two-dimensional phase diagram. The coexistence of lattice instability and appropriate amount of carrier concentration is needed to establish the CDW order in the CsV3Sb5 system. In this regard, the lattice instability naturally provides a tendency towards the CDW transition, and the carrier concentration serves as a tuning knob to change the magnitude (and possibly correlation length) of the CDW order. When the lattice instability persists (for example, in a finite Ti doping range around x = 0.13), the CDW order is reversible by tuning the carrier concentration. In addition, the change of carrier concentration may also affect the electronic correlation in the material system (for example, via screening effect). In this sense, our observations can also reconcile the earlier reports that multiple unconventional properties in the CDW state are associated with electronic correlation20,22,25,26,27, but the electronic instability itself is insufficient to drive the CDW phase transition34,35,49,54.

In summary, by utilizing high-resolution ARPES measurements, we have revealed a two-dimensional phase diagram of the CDW in CsV3Sb5 as a function of both Ti bulk substitution and Cs surface deposition. The distinct evolutions in this phase diagram reveal the roles played by both electrons and lattice. These observations provide key insights to understand the driving mechanism of the CDW order in Kagome metals.

Methods

Sample growth

Single crystals of CsV3−xTixSb5 were grown by self-flux growth method. The details of the crystal growth and characterizations are described in the Supplementary Note 1.

ARPES measurements

The samples were cleaved in situ with a base pressure of better than 5 × 10−11 Torr. ARPES measurements were carried out at our lab-based ARPES system using 21.2 eV photons with a total energy resolution of ~3 meV. The Fermi level was obtained by measuring the polycrystalline Au in electrical contact with the samples.