Introduction

Magnetoresistance (MR), defined as the variation in resistance under an applied magnetic field, serves as a crucial probe into Fermi surface properties and holds promise for applications in magnetic sensors and hard disk drives1,2. In the realm of extreme quantum limits, where the magnetic field quantizes orbital motion, the dominance of the lowest Landau level (LL) typically leads to the expectation of pronounced quasi-linear MR at high fields3,4. The exotic MR behavior in Dirac and Weyl materials has led to a flurry of extensive research, including significant negative linear MR in Dirac semimetals Cd3As25 and Na3Bi4, and titanic MR in Type II Weyl semimetal WTe26. These Dirac and Weyl fermions in those topological materials also manifest various exotic quantum phenomena, including chiral anomaly and nontrivial quantum oscillations7,8. In addition, several non-magnetic materials with zero-gap properties show large unsaturated positive MR, the possible mechanism is based on the classical theory of long transport mean free path caused by mobility distribution or the quantum effect with linear dispersive band structure9,10. Consequently, MR will exhibit unconventional behaviors across diverse novel materials11,12, thereby fostering the development of potential electronic devices.

The “heavy” element bismuth and its compounds are predestined for topological properties induced by spin-orbit coupling (SOC)13. The AMnBi2 (A = Sr, Ca, Eu, or Yb) systems14,15 exhibit fascinating properties that derive from their building unit, a two-dimensional Bi square net containing relativistic fermions. In parallel, the Ln3MX5 system (Ln = rare earth; M = transition metals; X = As, Sb, Bi) is predicted to be a topological candidate owing to its linear Bi chains. The quasi-one-dimensional chains in Sm3ZrBi5 give rise to dispersive linear and flat bands, while Bi-Bi interaction results in topological band crossing16,17. Experimental verification of nontrivial topological bands in the Ln3MX5 family has been successfully demonstrated via de Haas van Alphen (dHvA) oscillation analysis in La3MgBi518,19. These compounds are intriguing due to their narrow-gap topological bands influenced by SOC, potentially exhibiting novel electronic transport properties when subjected to a magnetic field. Notably, research on the MR of the low-dimensional Ln3MX5 system remains limited.

In this work, we report details of single-crystal growth of hypervalent bismuthide La3ScBi5 with one-dimensional Bi chains from the Ln3MX5 family. Density functional theory calculations indicate that SOC significantly affects La3ScBi5, as the band structure near the Fermi energy is predominantly comprised of Bi p orbitals. The electrical transport and magnetic properties were comprehensively investigated, leading to a study of the electron band structure in both the bulk and surface regions. The bulk crystal shows that the magnetoresistance exhibits a crossover between a conventional quadratic law and an unusual linear dependence, along with highly anisotropic electronic transport properties. Analysis of the Hall effect reveals that the Fermi surface of La3ScBi5 consists of multiple pockets arising from a multiband electronic structure. Even La3ScBi5, which has quasi-one-dimensional features and pronounced anisotropy, has a distinctly three-dimensional electronic structure, as evidenced by its angle-dependent dHvA oscillations. Notably, the presence of a prominent paramagnetic singularity suggests the potential nontrivial nature of its surface states. Our study employs La3ScBi5 as a model system to investigate hypervalent bismuthides, focusing on the quasi-linear MR and paramagnetic singularities observed in electron-rich motifs.

Results

Quasi-one-dimensional patterns of crystal structure

La3ScBi5 crystallizes in a rod-like, hexagonal structure, characteristic of other members in the Ln3MX5 family, with a space group of P63/mcm (No. 193). Analysis of the single-crystal X-ray diffraction (XRD) data reveals that La3ScBi5 exhibits lattice parameters of a = 9.746(3) Å and c = 6.561(3) Å, matching closely with the previous single-crystalline study20. The single-crystal XRD data collection and refinement parameters are gathered in Tables SI-III (Supporting Information). The (h00) reflections in Fig. 1b demonstrate the excellent crystal quality.

Fig. 1: Crystal structure of La3ScBi5.
figure 1

a Schematic diagram of crystal structure with a view along the c-axis projection. b Single-face X-ray diffraction pattern for a flux-grown single crystal. The inset presents an optical photograph of a typical single crystal. c Quasi-one-dimensional patterns in La3ScBi5: The separate one-dimensional (1D) ScBi6 face-sharing octahedral chains, 1D Bi chains, and La zig-zag chains. d Electronic band structure of La3ScBi5 with spin-orbit coupling (SOC), which emphasizes the contribution of band projection of Bi chain p orbitals. e Partial density of states calculations with SOC, highlighting the contribution of Bi p states at the Fermi level.

Figure 1c showcases quasi-one-dimensional patterns within La3ScBi5, composed of the separate one-dimensional (1D) ScBi6 face-sharing octahedral chains, 1D Bi chains, and La zig-zag chains aligned along the c axis, rather than forming a perfect 1D system. A notable feature is the Bi-Bi bond length within the chain, measuring approximately 3.28 Å, significantly longer than expected for a localized and covalent Bi-Bi single bond. This elongated yet symmetric bonding can be comprehended by “hypervalent” bonding, wherein a − 2 charge on Bi is stabilized by the delocalization of electrons within the chain21. The presence of extended hypervalent bonds necessitates an electron count of one electron per bond, resulting in half-filled bonds crucial for stabilizing symmetry-protected band crossings22,23,24. Moreover, hypervalent bonds exhibit greater orbital overlap compared to metallic bonds, resulting in steep and widely dispersed bands16,23. The double layers of the La atoms are stacked by 63 spiral axes parallel to the c direction, giving rise to La-based zig-zag chains with the nearest La-La distance of 4.01 Å.

To gain a deeper understanding of the electronic structure of La3ScBi5, the projection of Bi p orbitals onto the density functional theory band structure was analyzed according to the 4d Wyckoff position, as shown in Fig. 1d. It is observed that the band near the Fermi level exhibits a significant contribution from 1D Bi chains. It is worth noting that the band projection between Γ and A reveals a steep slope, indicating a high Fermi velocity and suggesting excellent potential for thermal conductivity. This is primarily attributed to the 1D hypervalent Bi chains characteristics along the c-axis, where electron hopping is significantly greater than other directions, leading to more pronounced band dispersion. The partial density of states (DOS) incorporating SOC in Fig. 1e shows a small, broad peak near the Fermi level, predominantly arising from the total Bi p orbitals, with notable hybridization from the La d and Sc d states. Taken together, the hypervalent Bi chains are essential in determining a range of physical properties, and additional experiments are required to delve into the thermal properties of La3ScBi5.

Quasi-linear magnetoresistance and nonlinear hall resistivity

Temperature-dependent resistivity of materials reflects the scattering of charge carriers by impurities and phonons at low and high temperatures, respectively. In La3ScBi5, the electrical resistivity, ρ||(T) (I // c) and ρ(T) (I // b), were investigated under a zero field as a function of temperature, as depicted in Fig. 2a. La3ScBi5 exhibits a metallic character with a residual resistivity ratio (ρ||, 300 K/ρ||, 2 K) of approximately 19. This RRR value, while not exceptionally larger, suggests the presence of significant disorder scattering. Despite the similar overall temperature dependencies of resistivity along both crystallographic axes, it was observed that ρ is an order of magnitude higher than ρ||, yielding an anisotropy ratio (ρ/ρ||) of around 20 at 2 K. The high-temperature behavior of ρ||(T) can be effectively described by the Bloch-Grüneisen (BG) formula25:

$${\rho \left(T\right)}_{{BG}}=\,{\rho }_{0}+\alpha {\left(\frac{T}{{T}_{D}}\right)}^{n}{\int }_{0}^{\frac{{T}_{D}}{T}}\frac{{x}^{n}{dx}}{\left({e}^{x}-1\right)\left(1-{e}^{-x}\right)}\,$$
(1)
Fig. 2: Charge transport of La3ScBi5 of ρ||(T) (I // c).
figure 2

a Temperature dependence of ρ||(I // c) and ρ(T) (I // b) under zero field on sample S1. The solid line is the fit of data to the BG formula. Inset: Temperature dependence of the radio of ρ/ρ||. b Temperature dependence of ρ||(T) with H // a (I // c) up to 16 T below 50 K. The red arrows denote the temperature T*. Inset: ρ||(T) below 50 K and fitting curve (solid line). c Field dependence of magnetoresistance at various temperatures. d Kohler plot: MR versus B/ρ||(T, B = 0). The solid line is the fit to MR = 4.11(B/ρ0)1.29.

Here, ρ0 represents the residual resistivity, TD corresponds to the Debye temperature. By utilizing the optimal parameters of n = 3, with values of ρ0 = 1.67 μΩ cm, TD = 187.37 K, and \(\alpha\) = 34.17 μΩ cm/K, the BG formula provides a good fit for ρ|| in the temperature range of 2 to 300 K. The obtained TD value closely aligns with that derived from the specific heat of La3ScBi5 (Figure S4, Supporting Information). The low-temperature (< 30 K) ρ|| follows a power law behavior ρ(T) = ρ0’ + ATn’ with ρ0’ = 1.65 μΩ cm and n’ = 2.88, as shown in the inset of Fig. 2b. Both values of n are nearly exactly 3, exhibiting a T3 dependence, indicating that the primary interaction in our system is likely inter-band electron-phonon scattering26,27. Similar analyses and interpretations have been applied to isomorphic compounds such as Sm3ZrBi516, as well as to ZrSiS28 and TiS229.

Figure 2b illustrates the temperature dependence of ρ||(T) under various fields with the H // a axis. In the absence of an external magnetic field, the resistivity decreases monotonically with a reduction in temperature. However, upon ramping the magnetic field to 16 T, a distinctive turn-on behavior is observed, leading to a resistivity minimum at T* before eventually plateauing. This magnetic-field-driven resistivity upturn followed by a resistivity plateau is interpreted as a potential transport hallmark of conducting surface states, attributed to the LL quantization of relativistic electrons30,31. Such a turn-on behavior has been documented in topological materials such as PtTe232 and WTe233. Another viable mechanism posits that the reentrant metallic state is a consequence of the scaling behavior in magnetoresistance, driven by the power-law dependence of the magnetic field and temperature34. The corresponding field-dependent MR ratio, [ρ||(B) - ρ||(0 T)]/ρ||(0 T), at various temperatures is depicted in Fig. 2c. Notably, the MR value peaks at 28% at 2 K and 9 T, displaying no saturation tendency. Particularly intriguing is the nearly linear dependence of MR on the magnetic field, most evident beyond the low-field regime. A similar quasi-linear positive MR phenomenon has been observed in HoAgGe, attributed to uncompensated charge carriers35. It’s noteworthy to mention that this linear MR might also be a signature of charge density wave materials, including TbTe3, HoTe336, and LaAuSb237. The existence of inhomogeneity and open Fermi surfaces or electron-phonon coupling along with a nested imperfect Fermi surface may be plausible mechanisms36,38,39.

To further research the underlying electronic structure influencing the MR behavior, we have conducted an analysis based on Kohler’s rule in Fig. 2d, which dictates that the MR in a conventional metal obeys a scaling behavior of Δρ/ρ(0) = F[B/ρ(0)]. The MR data at low temperatures exhibit a remarkable collapse onto a singular curve, which can be effectively approximated by the formula: MR = 4.11(B/ρ0)1.29, indicating that La3ScBi5 does not conform to an electron-hole compensated system6,40. The MR depicted in Figure S5a (Supporting Information) was calculated using the WannierTools package, employing the Boltzmann transport equation and Wannier function techniques. The calculated ρ||τ demonstrates a nonsaturating dependence of (Bτ)1.25, which is quite consistent with the experimental results of MR \(\propto\) B1.29. The agreement between theoretical calculation and experiment suggests that the MR may be explained by the semiclassical theory, with no significant role from the Berry curvature aspect of topological Dirac points. The adherence to Kohler’s rule serves as a pivotal indication; it underscores that the observed upturns and low-temperature plateaus are not indicative of a metal-insulator transition but rather stem from factors such as small residual resistivity, high mobilities, and a low charge-carrier density6,33,34.

Our investigation also systematically explored the transport properties along the c-crystallographic directions, unveiling anisotropic characteristics in the seemingly unsaturated MR. The ρ(T) curves obtained under various magnetic fields are compiled in Fig. 3a, where the turn-on behavior is also observed at 3 T and above. The saturation value and the range of upturn amplify with the applied magnetic field strength, indicative of the positive MR effect. Figure 3b, c illustrate the magnetic field dependence of MR at diverse temperatures and the field derivative of MR, dMR/dB, respectively. The quasi-linear behavior extends to notably low crossover fields B, beyond which MR transitions to a weak-field semiclassical quadratic dependence, which is consistent with the behavior of the theoretically calculated MR (Figure S5b, Supporting Information). Here, the B denotes the point where the fitting lines intersect. With increasing temperature, the field range exhibiting quasi-linear MR diminishes, and MR decreases, consistent with observations in 112-type materials such as CaMnBi241, YbMnBi242 and LaAgBi243, suggesting the possible existence of a nontrivial state. In the quantum limit where all carriers occupy solely the lowest LL, the observed B corresponds to the quantum limit of \({B}^{* }=\left(1/2e{{\hslash }}{\upsilon }_{F}^{2}\right){\left({k}_{B}T+{E}_{F}\right)}^{2}\) 44,45. As depicted in Fig. 3d, the experimental data for B align well with the above equation, further indicating the possibility of nontrivial states in La3ScBi5. Moreover, with increasing temperature, the linear term coefficient A1 is suppressed due to the temperature smearing of the LL splitting43. Future investigations, requiring more systematic Angle-Resolved Photoemission Spectroscopy (ARPES) studies, are necessary to probe the existence of Dirac cones in the electronic structure. Such the peculiar behavior of MR is predominantly governed by the multi-band features near the Fermi surface. Through the projection of individual atomic orbitals (Figure S2, Supporting Information) and DOS analysis, it is evident that the Bi p orbitals exhibit substantial contributions, as do hybrids between other orbitals, which together have a comprehensive effect on MR.

Fig. 3: Charge transport of La3ScBi5 of ρ(T) (I // b).
figure 3

a Temperature dependence of ρ(T) with H // c (I // b) under various fields on sample S1. Inset: Enlarged view of ρ(T) below 50 K. The red arrows denote the temperature T*. b Field dependence of MR at various temperatures. c The field derivative of MR at various temperatures. In the high-field regime, fitting results using MR = A1B + O(B2) are represented by lines, while in the low-field region, MR = A2B is employed. d Temperature dependence of the critical field B* (Purple squares). The solid line depicts the fitting results of B*, utilizing \({B}^{* }=\left(1/2e{\rm{\hslash }}{\upsilon }_{F}^{2}\right){\left({k}_{B}T+{E}_{F}\right)}^{2}\). The red circle corresponds to the linear coefficient A1 in the high-field MR.

To determine the mobility of the charge carriers, Fig. 4a illustrates the field dependence of the Hall resistivity ρyx at various temperatures, revealing a nonmonotonic behavior in La3ScBi5 below 30 K, indicative of its multiband nature. At high temperatures (T ≥ 30 K), ρyx remains positive and exhibits a linear relationship with the applied magnetic field, suggesting predominant transport by single-hole-type carriers. Figure 4b presents the field dependence of Hall resistance considering a relaxation time of 0.17 ps. Remarkably, our calculation shows the same trend as the experimental measurements, which exhibit nonlinear behavior that demonstrates the multicarrier behavior. We apply Kohler’s rule for Hall resistivity to La3ScBi5, demonstrating that the Hall resistivity scales with both magnetic field and temperature, akin to the longitudinal resistivity scaling under the relaxation time approximation. This theoretical framework was initially proposed by Zhang et al. 46, and is further elaborated in Note 1 (Supporting Information). This observed scaling behavior shows reasonable agreement with theoretical calculations. Compared with the case of ρ||, Kohler’s rule is basically obeyed over a large temperature range for ρyx (Fig. 4c). Hence, a multi-band model can be used to analyze the obtained results47,48:

$${\sigma }_{{xy}}\left(B\right)=\frac{{\rho }_{{yx}}}{{{\rho }_{{||}}}^{2}+{{\rho }_{{xy}}}^{2}}={eB}\mathop{\sum }\limits_{i}^{N}\frac{{n}_{i}{\mu }_{i}^{2}}{1+{\mu }_{i}^{2}{B}^{2}},$$
(2)
$${\sigma }_{{xx}}\left(B\right)=\frac{{\rho }_{{\rm{||}}}}{{{\rho }_{{\rm{||}}}}^{2}+{{\rho }_{{yx}}}^{2}}=e\mathop{\sum }\limits_{i}^{N}\frac{{n}_{i}{\mu }_{i}}{1+{\mu }_{i}^{2}{B}^{2}}.$$
(3)
Fig. 4: Hall effect of La3ScBi5.
figure 4

a Field dependence of Hall resistivity ρyx(B) at various temperatures. Inset: The temperature dependence of R0(T). A diagram of the Hall bar is shown, where I+ and I- are a pair of current leads, and V+ and V- are a pair of voltage leads, with H // a, I // c, and V // b. b The calculated field dependence of Hall resistivity at T = 2 K. Inset: The experimental field dependence of Hall resistivity at T = 2 K. c ρyxα ρ0 versus H/α ρ0. ρ0 is derived from ρ|| (T, H = 0) data. Inset: The temperature dependence of α. d Conductivity and Hall conductivity of La3ScBi5 at T = 2 K, the black line represents the fitted line using the multi-band model.

A typical fitting for T = 2 K is presented in Fig. 4d, yielding carrier densities of ne1 = 1.6 × 1021 cm−3, ne2 = 6.3 × 1019 cm−3, nh1 = 1.9 × 1019 cm−3, and nh2 = 5.1 × 1018 cm−3, along with mobility values of me1 = 139 cm2 V−1 s−1, me2 = 1184 cm2 V−1 s−1, mh1 = 893 cm2 V−1 s−1, and mh2 = 4276 cm2 V−1 s−1. It is noteworthy that an excessive number of fitting parameters may lead to significant errors, potentially failing to accurately reflect the physical essence of the multi-band system47. For the multi-band system of La3ScBi5, fitting the multi-band model with smaller N values is particularly challenging, possibly due to the lack of suitable initial values. Similar limitations are observed in other multiband systems, such as the pyrite-type bismuthide PtBi249 and the 3D Weyl semimetal TaAs50.

Quantum oscillations and fermi surface properties

The quantitative analyses of dHvA oscillations reveal the nature of electrons and serve as a powerful tool in studying topological physics. Figure 5a shows the beautiful dHvA oscillations that persist to about 10 K for sample S1 for field orientation H // a up to 9 T. The oscillatory components ΔM, obtained by subtracting a smooth background, are plotted against 1/B in Fig. 5b. From the fast Fourier transform (FFT) analyses of the oscillatory components ΔM, three principal frequencies (Fα = 33.8 T, Fα = 56.1 T, and Fβ = 90.5 T) are derived (Fig. 5c). The Fα component exhibits a significantly greater oscillation amplitude compared to Fα and Fβ components, making the Fα frequency the focal point of research interest. Similar multifrequency oscillations have also been observed in the isostructural compound La3MgBi518,19, which is suggestive of a 3D-like electronic structure. Note that similar dHvA measurements were observed on a crystal from the same batch as the sample S1(Figure S7, Supporting Information). The oscillation frequency is directly linked to the cross-sectional area of the Fermi pockets normal to the magnetic field AF through the Onsager relation F = (Φ0/2π2)AF. Specifically, the AF associated with the main peak is estimated to be 3.23 × 10−3 Å−2 for the α bands, yielding the Fermi vector kα = 3.20 × 10−2 Å−1. The corresponding parameters for three different pockets are listed in Table SIV (Supporting Information). It is noteworthy that distinct and varying quantum oscillations were observed in the H // b orientation (Figure S6, Supporting Information), indicating pronounced in-plane anisotropy within the ab-plane of La3ScBi5.

Fig. 5: Analyses of the de Haas-van Alphen (dHvA) oscillations for H // a in La3ScBi5.
figure 5

a Isothermal magnetization at different temperatures with the magnetic field parallel to the a-axis on sample S1. b The oscillatory components of magnetization ΔM. c The corresponding FFT spectrum of the oscillatory component of the dHvA oscillations at various temperatures. d The fits of the FFT amplitudes of Fα, Fα, and Fβ to the temperature damping factor RT by the LK formula. e Multiband LK fit of the oscillation components of the dHvA oscillations at 2 K. The black lines show the fits of the oscillation pattern to the generalized three-band LK formula for three different frequency oscillations. f The LL index fan diagram for α band derived from oscillatory magnetization at 2 K.

The oscillatory magnetization of a Dirac system is generally described by the Lifshitz-Kosevich (LK) formula51, accounting for the Berry phase52:

$$\Delta M\propto \,-{B}^{\lambda }{R}_{T}{R}_{D}{R}_{S}\sin \left[2{\rm{\pi }}\left(\frac{F}{B}-{\rm{\gamma }}-{\rm{\delta }}\right)\right]$$
(4)

where \({R}_{\text{T}}=({KT}\mu /B)/\sinh ({KT}\mu /B)\), \(K=2{\pi }^{2}{k}_{B}{m}_{\text{e}}/(\hslash /e)\) ≈ 14.69 T/K, \({R}_{\text{D}}=\exp (-K{T}_{\text{D}}\mu /B)\). μ represents the ratio of effective cyclotron mass to free electron mass, while RS denotes the spin reduction factor arising from Zeeman splitting. The oscillation of ΔM is delineated by the sine term with the phase factor \(1/2-{\varphi }_{B}/2{\rm{\pi }}-\delta\). The phase shift δ adopts values of 0 and ±1/8 for the 2D and 3D Fermi surfaces, respectively. Utilizing the LK formula, the effective mass m* can be derived by fitting the temperature-dependent oscillation amplitude to the thermal damping factor RT, as depicted in Fig. 5d. Here, B denotes the inverse average of the field window employed for Fourier analysis53, given by Bave = [(1/Bmax + 1/Bmin)/2] = 6.43 T with Bmax = 9 T and Bmin = 5 T, leading to calculated m*/m0 of 0.206, 0.227 and 0.234 for α, α’ and β pockets, respectively. The small values of m* imply the presence of relativistic charge carriers. Given that the Fermi surface of La3ScBi5 is of a strong 3D character, we have adopted the oscillation pattern at 2 K using the multiband LK formula with fixed frequency and fixed effective mass (Fig. 5e), yielding the Dingle temperature TD = 4.56 K for the Fα band, which corresponds to the quantum relaxation time \({\tau }_{q}\) = \({{\hslash }}\) / (2\(\pi\)kBTD) = 2.67 × 10−13 s, and quantum mobility \({\mu }_{q}=e\,{\tau }_{q}/{m}_{\alpha }^{* }\) = 2726 cm2/ V−1 s−1. From the LK fit of oscillations with Fα = 33.8 T, a phase factor of −γ − δ = 1.97 is obtained, yielding the Berry phase \({\varphi }_{B}\) is determined to be 0.69π (\(\delta\) = −1/8) or 1.19π (\(\delta\) = 1/8). Based on the calculated Fermi surface presented below, with \({\varphi }_{B}=\,\)0.69π (\(\delta\) = −1/8), the oscillation of the probe Fα corresponds to the minimum cross-section. The Dingle temperature, relation time, quantum mobility, and Berry phase obtained by LK fitting for Fα and Fβ are summarized in Table SIV (Supporting Information). Certainly, the fitting performed below 5 T is based on a limited number of data points, which may introduce greater uncertainty for Berry phases with multiple LK fits.

Given that dM/dB is directly proportional to the density of states at the Fermi level54,55, we can associate the minimum of ΔM with N − 1/4, where N represents the LL index. However, due to the Landau indices of Fβ being far from the quantum limit, there is notable uncertainty in determining the intercept. As depicted in Fig. 5f, the LL indices N for α bands are plotted against 1/B. The solid lines depict linear fits based on the Lifshitz-Onsager quantization criterion N = F/B + \({\varphi }_{B}\)/2π\(-\delta\). The slope of the linear fits yields a value of 34.31 T, consistent with the FFT derived result, thereby affirming the reliability of the linear fit within the LL fan diagram. The intercept extracted from linear extrapolation is 0.430 ± 0.018, corresponding to a Berry phase of 0.72π (\(\delta\) = −1/8), aligning with the findings obtained from LK fitting. While a finite Berry phase is generally considered indicative of topologically nontrivial bands, it may not reflect the intrinsic properties of a 3D-Dirac Fermi surface, but could simply be a consequence of time-reversal symmetry56. However, the phase shift can be affected by spin splitting and g-factor, making it challenging to determine the topological properties of the band from magnetic transport measurements alone. The similar deviation in the intercept was observed in the study of PtBi257, which was attributed to the Fermi level not intersecting the degeneracy point.

In a manner analogous to the in-plane cyclotron motions observed for H // a, electrons engaged in interlayer cyclotron motions under fields along the c-axis exhibit quantum oscillation behavior. Figure S8a and S8b (Supporting Information) depict dHvA oscillations of H // c overlaid on a diamagnetic background in sample S1 and their respective oscillatory components. In contrast to the dHvA oscillations for H // a, those for H // c consist of more frequencies. FFT analyses (Figure S8c, Supporting Information) reveal a predominantly low frequency (106.8 T) and three high frequencies (181.8, 215.2, and 249.1 T), and this phenomenon is also reproduced for samples S2 and S3 (Figure S9, Supporting Information). The electron cyclotron masses for H // c range slightly higher, approximately between 0.366 and 0.529 m0 across all probed oscillation frequencies. This anisotropic effective mass is consistent with the quasi-1D structure of La3ScBi5. The lower single-frequency component, extracted by isolating the higher-frequency component, can be analyzed using the widely adopted LL fan diagram method, as demonstrated in Figure S8d (Supporting Information). The intercept derived from the linear fit in the fan diagram yields 0.234 ± 0.092 for Fγ, with uncertainties suggesting δ values of 1/8 or −1/8, resulting in an uncertain phase of 0.71π or 0.21π. Additionally, the fitted oscillation frequency for Fγ is 108.09 T, closely aligning with FFT results. Noted that significant fitting errors limit the precision of determining \({\varphi }_{B}\) for γ band. Furthermore, accurately determining the LL index field for each frequency remains challenging in the case of multifrequency oscillations for Fη54,58. Nonetheless, we did not detect Shubnikov-de Hass (SdH) oscillations either in the MR or in the Hall resistivity up to 9 T, which warrants further measurements at higher magnetic fields and lower temperatures. It is conceivable that SdH oscillations come from the oscillating scattering rate and can thus be complicated by the detailed scattering processes while the dHvA effect is caused directly by the free energy oscillations of a system59,60.

The anisotropic characteristics of the Fermi surface of La3ScBi5 are further elucidated through an investigation of ΔM versus 1/B and corresponding dHvA oscillation frequencies at 2 K across various magnetic field orientations. Figure 6a illustrates angle-dependent quantum oscillation as the magnetic field rotates from the [100] to [001] direction. Figure 6b reveals the oscillatory component after subtracting the background, demonstrating a distinct evolution of the angle θ, defined as the angle between the field direction and [100] direction. The oscillation amplitude diminishes progressively with increasing the tilt angle. Additionally, there is one more frequency Fγ detected at θ ≥ 75° in the FFT spectra (Fig. 6c). These angular dependencies of dHvA oscillation frequencies clearly indicate the complex 3D nature of the Fermi surface morphology in La3ScBi5 despite its quasi-1D structure. In Fig. 6d, we summarize the angle dependence of each frequency. The oscillation frequencies Fα exhibits a weak angular dependence at lower angles and can be fitted with the formula F = F3D + F2D /cos θ, where F2D and F3D represent the contributions from 2D and 3D components. The relative weight between 2D and 3D components derived from the fit, F2D/F3D ≈ 0.6, suggests dimensionality between 2D and 3D. Moreover, Figure S10 presents the Fermi surfaces incorporating SOC, and the complexity of these Fermi surfaces leads to an angular dependence in dHvA oscillation frequencies. Utilizing the SKEAF package61, we calculated the angular dependence of the dHvA oscillations, as depicted in Fig. 6e, which shows general agreement with the experimental results. These calculations enable us to identify the origins of the dHvA frequencies observed in experiments. The Fermi surface is intricate, revealing in particular one electron pocket and one hole pocket, which may correspond to the \(\alpha\) and \(\eta\) branches in the angular dependence of dHvA oscillation frequencies, respectively (Figure S10, Supporting Information). In conjunction with the projections of each atom, it is evident that the Bi p orbitals play a crucial role in this electron pocket.

Fig. 6: Fermi surface morphology of La3ScBi5.
figure 6

a Isothermal magnetization of La3ScBi5 at various angles for T = 2 K on sample S1. b Oscillatory components of magnetization at 2 K under different magnetic field orientations. c The corresponding FFT spectrum of the oscillatory component of the dHvA oscillations for various angles. d Angular dependence of dHvA oscillation frequencies, with error bars defined as half the width at the half-height of FFT peaks. Black lines represent fits to F = F3D + F2D/cos θ for Fα. e Angular dependence of calculated dHvA oscillation frequencies below 600 T. Fα contributed from e pocket is indicated by red circles while Fη contributed from h pocket is denoted with purple stars.

Paramagnetic Singularity in Magnetization

The magnetization of La3ScBi5 exhibits pronounced anisotropy with respect to the field orientations, as depicted in Fig. 7a. Along the a-axis (χa) and c-axis (χc), the temperature-dependent magnetic susceptibility shows distinct behaviors. χa manifests paramagnetic, nearly independent of temperature, with a broad shoulder around 75 K and a notable upturn below 15 K. These features persist as the applied field increases, ruling out magnetic impurity effects. Additionally, Fig. 7b reveals the absence of anomalies near 75 K in dχ/dt, providing further evidence of the intrinsic nature of this magnetic response in La3ScBi5. Similar T-independent susceptibility behaviors have been observed in bismuthides like Bi2Se362 and PtBi263,64. This behavior can be attributed to potential contributions from Pauli paramagnetism, van Vleck paramagnetism, Landau diamagnetism, and core diamagnetism59,62,63.

Fig. 7: Magnetism of La3ScBi5.
figure 7

a Temperature dependence of the magnetic susceptibilities measured at H = 1 kOe on sample S1. b χ(T) curves under various magnetic fields for H // a. c Low field region of the magnetic moment vs. B curves at various temperatures for H // c. The measurements are performed sequentially from low to high temperature, spanning from 2 K to 300 K. d Magnetic susceptibility χ(=dM/dB) is calculated by differentiating the magnetic moment, plotted as a function of the magnetic field (additional details are provided in Figure S13, Supporting Information).

In contrast, the interplane χc is diamagnetic and undergoes a rapid increase at low temperatures. Specifically, the low-field region of M(B) curves in Fig. 7c shows a significant paramagnetic contribution near the zero field, as also observed in Figure S9 for the same sample batch. The χ(B) curves sharply rise above the diamagnetic ‘floor’ within a narrow field range and approach χ(0) in a straight line (Fig. 7d). The cusp observed in the low-field region are robust and prominent, with singular field dependence persisting up to the maximum measured temperature of 300 K. Additionally, there is a noticeable directional dependence, leading us to speculate that these features may be an inherent property of La3ScBi5 crystals, rather than being attributed to magnetic impurities in the diamagnetic matrix. With increasing temperature, the cusp exhibits a tendency to be inhibited, which may may be due to aging effect (Figure S12, Supporting Information) or insufficient measurement accuracy, but also need further systematic research. Such cusp-like paramagnetic susceptibility be traced most naturally to the helical spin texture of topological electrons on the surface, a signature observed across the family of three-dimensional topological materials65,66. The proposed mechanism suggests that the electron spins at the Dirac point lack a specific orientation. As long as the Dirac cone is not fragmented, these electron spins can align freely along the external magnetic field. In the low-field region, such freely oriented spins are expected to generate paramagnetic singularities in the M(B) curve65. More experiments, such as ARPES and scanning tunneling microscopy measurements, are highly desirable to probe the nontrivial surface and bulk states in La3ScBi5.

Discussion

We have conducted comprehensive investigations into the physical properties of the quasi-one-dimensional single crystal La3ScBi5, belonging to the Ln3MX5 family (Ln = rare-earth; M = transition metals; X = As, Sb, Bi). Density functional theory calculations reveal a complex and non-trivial electronic structure with SOC. Transport measurements reveal quasi-linear anisotropic magnetoresistance, with the MR isotherm following the Kohler scaling law with an index of m = 1.29, deviating from ideal electron-hole compensation. Nonlinear Hall resistivity further confirms the multi-band nature of electrical conductivity in La3ScBi5, with moderate charge compensation. The theoretical calculations agree with the experimental results of the behavior, demonstrating that both complex magnetoresistance and Hall resistivity behaviors may be accounted for by the semiclassical Boltzmann transportation theory.

Our magnetism studies demonstrate anisotropic magnetic susceptibility and detect dHvA oscillations for magnetic fields aligned parallel to both the a and c axes. Angle-dependent dHvA oscillations are essential to gain deeper insights into its fermiology and potential topological nature of the system. Notably, a robust and prominent paramagnetic singularity may underscore the non-trivial nature of the surface states, marking the groundbreaking observation within the Ln3MX5 family. This research offers valuable insights into the behavior of similar quasi-one-dimensional systems containing heavy elements. The rod-like La3ScBi5, suitable for mechanical exfoliation, presents an ideal platform for device applications and topological physics.

Methods

Crystal growth

Large single crystals of La3ScBi5 were grown using the self-flux method with excess Sc and Bi as flux. La (lump), Sc (piece), and Bi (pill) were initially mixed in a molar ratio of 1: 2: 5, loaded into an alumina crucible, and sealed into an evacuated quartz tube. The temperature was gradually raised to 1000 °C and maintained for 20 h, followed by slow cooling to 700 °C at a rate of 1 °C/h to facilitate single crystal growth. Subsequently, the excess flux was separated from the resulting rod-shaped La3ScBi5 crystals using a centrifuge. It’s worth noting that prolonged exposure to air or contact with alcohol would cause decomposition.

Bulk characterization

Single crystal x-ray diffraction (SCXRD) for La3ScBi5 was conducted on a Bruker D8 Venture diffractometer at room temperature using Mo Kα radiation (λ = 0.71073 Å). The collected data were refined by the least-square method of F2 using SHELXL-2018/367. The diffraction peaks for a single-crystalline surface were obtained via a Bruker D2 phaser XRD detector using Cu Kα1 radiation (λ = 1.54184 Å). Element analysis was performed using energy dispersive x-ray (EDX) in a Hitachi S-4800 scanning electron microscopy (SEM) with an accelerated voltage of 15 kV. Characteristic details can be shown in Figure S1a–f.

Transport and magnetism measurements

Electronic resistivity measurements up to 16 T were conducted on polished crystals to remove Bi flux droplets on the surface using a Physical Properties Measurement System (PPMS, Quantum Design). Magnetic susceptibility and isothermal magnetizations of La3ScBi5 were performed in a 9 T PPMS in vibrating sample magnetometer (VSM) mode. Heat capacity was measured by the thermal relaxation method in the PPMS, with thermal contact achieved using Apezion N-grease. Three different single crystal samples named S1, S2, and S3 were used for measurements, with mass bits of 32 mg, 80 mg, and 190 mg respectively.

Electronic structure and transport calculations

Theoretical calculations were performed using density functional theory (DFT) as implemented in the Vienna ab initio Simulation Package (VASP)68,69 with the generalized gradient approximation (GGA) of Perdew-Burke-Ernzerhof (PBE) exchange-correlation potential70. A plane wave basis with a kinetic energy cutoff of 500 eV was employed. Brillouin zone sampling was conducted using a 4×4×6 k-point mesh, with Gaussian smearing of 0.05 eV applied around the Fermi surface. Structural optimization was carried out with both cell parameters and internal atomic positions allowed to relax until the forces on all atoms were less than 10−7 eV Å−1. Spin-orbit coupling effects were included in the electronic property calculations. MR was computed using the WannierTools package71, employing the Boltzmann transport equation72,73 and Wannier function techniques74. These calculations utilized a 100 × 100 × 100 k-point mesh, with the assumption of identical relaxation times (τ) for charge carriers. The angular dependence of dHvA oscillation frequencies was calculated using the SKEAF package61.