Abstract
Correlated electron systems are highly susceptible to various forms of electronic order. By tuning the transition temperature towards absolute zero, striking deviations from conventional metallic (Fermi-liquid) behaviour can be realized. Evidence for electronic nematicity, a correlated electronic state with broken rotational symmetry, has been reported in a host of metallic systems1,2,3,4,5 that exhibit this so-called quantum critical behaviour. In all cases, however, the nematicity is found to be intertwined with other forms of order, such as antiferromagnetism5,6,7 or charge-density-wave order8, that might themselves be responsible for the observed behaviour. The iron chalcogenide FeSe1−xSx is unique in this respect because its nematic order appears to exist in isolation9,10,11, although until now, the impact of nematicity on the electronic ground state has been obscured by superconductivity. Here we use high magnetic fields to destroy the superconducting state in FeSe1−xSx and follow the evolution of the electrical resistivity across the nematic quantum critical point. Classic signatures of quantum criticality are revealed: an enhancement in the coefficient of the T2 resistivity (due to electron–electron scattering) on approaching the critical point and, at the critical point itself, a strictly T-linear resistivity that extends over a decade in temperature T. In addition to revealing the phenomenon of nematic quantum criticality, the observation of T-linear resistivity at a nematic critical point also raises the question of whether strong nematic fluctuations play a part in the transport properties of other ‘strange metals’, in which T-linear resistivity is observed over an extended regime in their respective phase diagrams.
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Main
The crystal structure of pristine FeSe is shown in Fig. 1a. At the structural phase-transition temperature Ts ≈ 90 K, FeSe undergoes a tetragonal-to-orthorhombic transition that is accompanied by a lowering of the symmetry of the electronic state, manifest as a deformation of the Fermi surface from fourfold to twofold symmetry11. At T = Ts, the nematic susceptibility (extracted from elasto-resistance measurements) is found to be strongly peaked and follows a Curie–Weiss law9. Crucially, there is no evidence for magnetic order or enhanced spin fluctuations around Ts (ref. 10). With S substitution, Ts is suppressed and ultimately, driven to zero temperature at a ‘critical’ S concentration xc ≈ 0.16 (Fig. 1b), at which the Fermi surface distortion vanishes12,13, the nematic susceptibility is maximized and the effective Curie–Weiss temperature is zero9.
The nematic phase (orange region in Fig. 1b) is identified by a kink in the derivative of the in-plane resistivity ρab(T, x), the raw data for which are displayed in Fig. 1c (for the derivatives themselves, see Extended Data Fig. 8). In contrast to what is found, say, in the Fe-pnictides14, the superconducting phase (blue area in Fig. 1b) shows little variation with x; its transition temperature Tc ≈ 8–10 K for 0 ≤ x ≤ 0.25, the range of x studied here. Between Ts and Tc, ρab(T) of FeSe1−xSx exhibits an anomalous quasi-linear T-dependence over a wide range of x (ref. 9). This is reminiscent of the ‘strange metal’ behaviour found in the systems highlighted above and raises the question: does the limiting low-T behaviour of ρab(T) in FeSe1−xSx also exhibit the hallmarks of quantum criticality? To address this question, it is necessary to suppress the superconductivity in FeSe1−xSx, for example, using high magnetic fields, and to follow the evolution of ρab(T, x) down to low temperatures.
In anisotropic or quasi-two-dimensional superconductors, the magnetic field H is typically applied perpendicular to the conducting planes, where the upper critical field Hc2 is smallest15,16,17. In this orientation, however, there is invariably a sizeable transverse orbital magnetoresistance that in some cases follows a non-analytical form, thus making it difficult to extract the intrinsic (zero-field) normal state resistivity. The anisotropy in Hc2 in FeSe1−xSx, however, is only a factor of two, making it possible to access the normal state using static (direct current) magnetic fields while at the same time minimizing the magnetoresistance by studying the evolution of ρab(T, x) in the longitudinal configuration. To illustrate this point, we show in Fig. 2a a comparison of the normal-state magnetoresistance (for x = 0.16) with B//c and B//ab up to 15 T. While the transverse magnetoresistance is already around 20%, the longitudinal magnetoresistance is negligible (and remains so, in fact, up to 35 T), implying that the resistivity measured at maximal field is the same as the resistivity that would have been measured in zero field in the absence of superconductivity. For all x > xc, the longitudinal magnetoresistance is negligible, as exemplified in Extended Data Fig. 2a for x = 0.2. In samples with lower S concentration, the longitudinal magnetoresistance is finite, though even here, the magnetoresistance merely shifts the resistivity vertically, without adversely affecting its overall temperature dependence. A representative set of longitudinal magnetoresistance curves is displayed in Fig. 2b for x = 0.13 (see Extended Data Fig. 3 and discussion in Methods for more details). The only exception to this behaviour is pure FeSe, where the longitudinal magnetoresistance is largest (about 25%) in the normal state above Tc but becomes negligible at temperatures below 4 K (Extended Data Fig. 2b).
Figure 2c–f displays resistivity curves measured in both zero field and in a 35 T field (B//ab) for four representative x values. (The data for all eight crystals are shown in Extended Data Fig. 4). For samples with x < xc (Fig. 2c and d), ρab(T) at 35 T (thick black curve) decreases linearly with temperature down to approximately 10 K, at which point it passes through an inflection point. For xc = 0.16 (Fig. 2e), ρab(T) is strictly T-linear from 13.5 K down to at least 1.5 K, below which superconducting fluctuations are still discernible (as shown in Extended Data Fig. 10, Hc2 exhibits a slight peak at x ≈ xc). For x > xc, ρab(T) ≈ T2 over an extended temperature range (Fig. 2f).
To determine the precise form of ρab(T), we examine its temperature derivative dρab/dT. This is plotted in Fig. 3a for FeSe (at 35 T). (Again, other derivatives are shown in Extended Data Fig. 5). Below a temperature marked T2 = 4.5 ± 0.5 K, dρab/dT is T-linear with a zero intercept, implying that ρab(T) is strictly quadratic below T2, as confirmed by plotting ρab(T) as a function of T2 (inset of Fig. 3a). Note that the magnitude of the T2 component of ρab(T) far exceeds the residual resistivity. Above a second temperature scale T1 = 10.5 ± 1.5 K, dρab/dT is constant, implying that ρab(T) is strictly T-linear. As mentioned above, the longitudinal magnetoresistance for x = 0 is negligible below 4 K. Thus, the crossover from T-linear to T2-resistivity with decreasing T is a robust feature of the data—only the inflection point in ρab(T) becomes less pronounced with decreasing field strength.
A quadratic T-dependence of the limiting low-T resistivity is a hallmark of a (correlated) Fermi liquid with dominant electron–electron scattering. The coefficient of the T2 term in FeSe is A = 260 ± 55 nΩ cm K−2. This coefficient contains important information about the enhancement of the quasiparticle effective mass m*, as encapsulated in the empirical Kadowaki–Woods ratio that links the coefficient of the T2-resistivity to the square of the electronic specific heat coefficient18. As described in Methods, the magnitude of A in FeSe is found to be in good agreement with the known Fermi surface parameters for the two cylindrical pockets revealed by quantum oscillation experiments.
A T2 resistivity was found for all x ≠ xc at low T. The resulting variation of A with x, plotted (as solid black triangles) in Fig. 3b, follows closely that of the superconducting energy gap Δ (open triangles in Fig. 3b) on the hole band19. The marked asymmetry in both A and Δ across xc implies that the coupling of quasiparticles to nematic fluctuations is different on either side of xc and that this in turn may influence the pairing strength. This is not the whole story, however. The evolution of the low-T form of the resistivity in FeSe1−xSx with increasing x, from Fermi liquid to non-Fermi liquid and back to Fermi-liquid-like, together with the variation in T2 with doping and its depression at x = xc (see Fig. 4b), are classic signatures of quantum criticality in metals. Typically, the reduction in T2 is accompanied by a divergence in A. Although the raw data do not show a divergence in A, the analysis outlined below suggests that this third key characteristic of critical behaviour is also realized in FeSe1−xSx.
While the proportionality of A with (m*)2 is well established, the magnitude of A also depends on the carrier concentration n (ref. 18). In FeSe1−xSx, it has been shown that both the electron and hole pockets expand with increasing S content12,20. Were m* to remain constant across the series, A would fall as both x and the effective carrier density increases. By contrast, A is found to grow with increasing x, at least up to xc = 0.16 (see Fig. 3b). To compensate for the increase in carrier density, m* must increase markedly over the same range of x. To be more quantitative, we first take into account the influence of n on A. Using experimental data for the Fermi surface areas in FeSe1−xSx (ref. 20), we extract a new parameter A* that more faithfully tracks the evolution of m*2 across the phase diagram (see Extended Data Fig. 9 and accompanying explanation in Methods for more details). The result is shown in Fig. 4a. The variation in A* at low x exhibits a clear enhancement on approaching xc from either side, indicating a tendency for m* to diverge at xc. This enhancement in A* is matched by a corresponding decrease in T2 (and T1), which both approach zero at x ≈ xc (Fig. 4b). All these observations are consistent with those found in other quantum critical metals and suggest a strong coupling of itinerant fermions to quantum fluctuations of the relevant order parameter.
A crucial question then emerges: what is the relevant order parameter? The dashed line in Fig. 4a shows the expected enhancement in A near a nematic quantum critical point21. Although this appears consistent to within experimental uncertainty, as discussed below, there is no known theory for a T-linear resistivity down to T = 0 at a nematic quantum critical point in a clean system. Whereas FeSe exhibits only nematic order below Ts, a spin-density-wave state is stabilized under relatively modest pressures22, and the spin-lattice relaxation rate (at ambient pressure) shows evidence for enhanced spin fluctuations below Ts (ref. 23), though not at Ts itself. Moreover, critical behaviour can be seen in the muon spin depolarization rate for Ts > T > T* (about 10 K)24, the same range over which ρab(T) is quasi-T-linear, suggesting a possible link between T-linear resistivity and antiferromagnetic, rather than nematic, fluctuations.
Although there exists a region in the temperature–pressure phase diagram of pure FeSe, in which nematic and spin-density-wave states overlap or coexist, with increasing x, these two phases become decoupled25. The range of nematic order shrinks, eventually vanishing at xc while the dome of spin-density-wave orders shifts to higher pressures25. Thus, at x = xc, the spin-density-wave phase is located far from the ambient pressure axis at which our experiments are conducted. Moreover, nuclear magnetic resonance (NMR) experiments have shown that spin fluctuations, although present in FeSe1−xSx at low x values, are strongly suppressed by S substitution23. These combined results imply that the critical behaviour we observe at x = xc cannot be associated with proximity to a magnetic phase.
The T2 resistivity appearing below the quantum critical fan suggests a predominance of umklapp-type processes involving large-Q momentum transfer. Such processes ought to be negligible in low-carrier-density metals near a Q = 0 Pomeranchuk instability where the effective interaction is long-range26, particularly metals with convex and simply connected Fermi surfaces21. Thus, naively, one would not expect signatures of nematic quantum criticality in ρ(T). Such arguments, however, neglect the role of impurity scattering, which is an important source of momentum relaxation, particularly in multi-band systems like FeSe that contain bands of different mass27. Whenever impurity scattering is more efficient than umklapp processes at relaxing momentum, both quantum critical scaling of the T2 resistivity and a non-Fermi-liquid form of the resistivity at the quantum critical point28,29 can emerge. It is unlikely, however, that such conditions are satisfied in pristine FeSe where the T2 resistivity is by far the dominant contribution to ρ(T), yet its low-T resistivity is identical to that of more disordered FeSe1−xSx.
These arguments suggest therefore that we may need to look beyond the long-wavelength critical fluctuations associated with the Pomeranchuk instability. Recently it has been argued that FeSe possesses Q = (π, 0) antiferroquadrupolar order, which could also lead to a breaking of C4 symmetry30. According to Yu and Si30, coupling of this antiferroquadrupolar order to the itinerant fermions will suppress any tendency towards antiferromagnetism and thus offers an explanation of why the structural transition at Ts is not accompanied by static antiferromagnetism. More importantly, this coupling could provide a channel for momentum relaxation and clearly motivates a need to calculate the electrical resistivity within this model. Antiferroquadrupolar order may also exist in the pnictides, though nematicity is not necessarily the dominant order parameter there. Nevertheless, the evolution of the normal state in-plane resistivity reported here and summarized in the phase diagram of Fig. 4d raises the prospect that nematic fluctuations may have a much stronger influence on the transport properties of other so-called ‘strange metals’ than previously thought, though disentangling the effects of nematicity from other competing or co-existing order parameters will remain a challenge.
Finally, we discuss the character of the T-linear resistivity above T1. Combining the Fermi surface parameters for FeSe1−xSx with our values for dρab/dT, we extract an estimate for the transport scattering rate ħ/τ = αkBT within the quantum critical fan (see Methods for more details) where ħ is the reduced Planck constant and kB is the Boltzmann constant. Intriguingly, α ≈ 1 for all x (Fig. 4c). Recently, this inequality was found to be a generic property of a host of strongly correlated electron systems exhibiting a T-linear resistivity31. Comparison with the metamagnetic metal Sr3Ru2O7 is quite informative in this respect as both FeSe1−xSx and Sr3Ru2O7 show T-linear resistivity at the critical magnitude despite the fact that thermodynamically, not all sections of the Fermi surface show enhanced masses on approach to the quantum critical point20,31. As discussed in ref. 31, this strongly suggests that the quantum criticality in both FeSe1−xSx and Sr3Ru2O7 is associated with the onset of efficient scattering, with strength proportional to T, which affects all of the quasiparticles.
Methods
Growth and characterization of samples
Single crystals of FeSe1−xSx were grown by the chemical vapour transport technique. A mixture of Fe, Se and S powders together with KCl and AlCl3 powders was sealed in an evacuated SiO2 tube and heated to 390–450 °C on one end, while the other end was kept at 140–200 °C. The actual sulphur composition x was determined by energy dispersive X-ray spectroscopy and found to be about 80% of the nominal x. All x values quoted are the nominal values.
Measurements
The crystals were cut into rectangular-shaped samples and six electrical contacts applied to each sample in a Hall bar geometry. The contacts were made manually by indium-soldering 25-μm-diameter Au wires onto the samples with a sharp hot tip. To ensure a uniform current flow, a layer of Dupont 4929 Ag paint was added on the two edges around the indium point contacts employed for the current flow. The resistances of both sides of the samples were always measured simultaneously and showed consistent behaviour, confirming the homogeneous flow of current through each sample. The data were acquired using a standard four-probe technique, applying a constant current of 1 mA for temperatures above 4.2 K, or 500 μA below, with lock-in amplifiers and transformers used to measure the response of the samples.
All magnetotransport measurements were carried out at the High Field Magnet Laboratory (HFML) in Nijmegen. All samples were preliminarily characterized in a superconducting magnet with a maximum magnetic field of 16 T. The high-field data were acquired in a resistive Bitter magnet with a maximum field of 35 T using a combination of He-4 and He-3 cryostats. All high-field measurements were performed employing the same transport probe, equipped with a rotating sample holder, a Cernox CX-SD temperature sensor, an RS Pro foil strain gauge heater and an Arepoc s.r.o. LHP-NUs Hall probe. The orientation of the samples with respect to the applied magnetic field was determined by first using the Hall probe signal to orient the rotating platform, and then the magnetoresistance of the sample itself to locate the longitudinal field orientation more precisely. See Extended Data Fig. 1 and Methods section ‘Thermometer calibration in field’ for details about the temperature determination in the high-field environment.
Thermometer calibration in field
The Cernox resistance thermometer used for the high-field experiments was calibrated in zero magnetic field in the range 0.3–300 K. To obtain a reliable temperature reading while varying the temperature in a constant magnetic field of 35 T, the magnetoresistance of the Cernox had to be taken into account. Field sweeps at constant temperature were used to record the Cernox output at zero field (T(0 T)) and at 35 T (T(35 T)) at numerous temperatures. To stabilize temperature in the range 0.3 K < T < 1.4 K, the He-3 vapour pressure was varied without applying any heat into the sample space. For 1.4 K < T < 4.2 K, He-4 vapour pressure was similarly used. The 4.2 K temperature point was recorded by putting the sample in good thermal contact with a liquid He-4 bath at ambient pressure. For temperatures above 4.2 K, a constant heater power was applied through a strain gauge, controlled by a Lakeshore temperature controller. Once the temperature had been stabilized at zero field (typically within a precision of a few millikelvin for 10 min), the field was then ramped. In this way, the plot in Extended Data Fig. 1 was obtained. The data points are divided into four intervals (identified by different colours) in which the temperature dependence of the magnetoresistance has a slightly different form. Third-order polynomial fits, with different fitting parameters, were then calculated for the first three ranges, while a linear fit was calculated for the highest temperature range. The fits are represented by the solid lines in Extended Data Fig. 1. The inset displays a blow-up at the lowest temperatures. After acquiring the 35 T temperature ramps shown in the main paper, the temperature was then corrected by means of the fitting functions plotted in Extended Data Fig. 1.
Longitudinal magnetoresistance of FeSe1−xSx
To probe the normal state of FeSe1−xSx in a high magnetic field, it is crucial to ensure as far as possible that the effect of the field is only to suppress superconductivity, without introducing any extrinsic contribution to the normal state resistivity. In our case, this was achieved by measuring the longitudinal magnetoresistance (that is, with B//I//ab) of all samples. For all x, the magnetoresistance was either vanishingly small or merely introduced a (small) offset with a negligible temperature dependence.
Extended Data Fig. 2a shows a set of field sweep curves for x = 0.2. As can be seen, the variation in ρab(H) is essentially constant (within the field-accessed normal state) over the entire temperature range studied, implying that the values of the resistivity measured at 35 T and at 0 T have the same temperature dependence. For 0.05 ≤ x ≤ 0.13, the magnetoresistance is finite and positive over the entire field range, but only results in a constant shift in ρab(T). This is illustrated in Extended Data Fig. 3, where we plot the slope of the magnetoresistance sweeps for x = 0.13 between 34 T and 35 T (extracted from linear fits) at different temperatures. We find a broad temperature region (1.5 K ≤ T ≤ 30 K) in which the slope is constant to within our experimental uncertainty. Thus, the only effect of the field is to shift ρab to higher values, without any influence on its variation with temperature. Below 1.5 K, the maximum field is no longer strong enough to fully suppress superconductivity, resulting in a sharp increase in the slope. A similar behaviour is found for Δρab = ρab(35 T) – ρextrap(0 T), where ρextrap(0 T) is the extrapolation at 0 T of the linear fits calculated between 34 T and 35 T. Only for pure FeSe does the magnetoresistance vary with temperature, but even this vanishes at lower T, as shown in Extended Data Fig. 2b.
A coefficients and the temperature scales T 1 and T 2 for FeSe1−xSx
The A coefficients and the temperature scales T1 and T2 for each x value were determined primarily from the temperature derivative dρab/dT of the 35 T resistivity curves. To calculate these derivatives, the raw ρab(T) curves of Extended Data Fig. 4 were first binned and smoothed. As shown in Extended Data Fig. 5, for every x ≠ xc, dρab/dT exhibits three distinct regimes. At the lowest temperatures, dρab/dT has a linear slope with a zero intercept. This corresponds to a quadratic temperature dependence for ρab(T). The temperature at which dρab/dT first deviates from linearity is then defined as T2 and the slope itself is equal to 2A. The uncertainty in A comes from both the scatter in the derivative data and the geometric uncertainty in the sample dimensions. Once T2 is obtained, a second determination of A can be obtained from a plot of ρab versus T2—see Extended Data Fig. 6 (raw data) and Extended Data Fig. 7 (smoothed data)—and the linear fit drawn between the lowest measured temperature point and (T2)2.
At higher temperatures, the derivative attains a constant value, implying that the resistivity has become T-linear. The onset temperature of this T-linear resistivity is labelled T1. The constant value of dρab/dT can then be compared with the one obtained when fitting the curves in Extended Data Fig. 4 with straight lines down to T = T1 to obtain two estimates of the T-linear slope. For T2 < T <T1, ρab(T) exhibits a gradual crossover from the T2 resistivity at low T to the T-linear resistivity at higher temperatures. This crossover is rather smooth for x > xc but for x < xc, it presents a peak, presumably due to the finite magnetoresistance in the latter case.
For xc = 0.16, we estimate T1 to be lower than 1.5 K (the lowest temperature that we could access with our current magnetic field range). Looking at the behaviour of samples with x < xc, we estimate the maximum value of T2 to be at least half of T1, but with an error bar extending between 0 K and 0.75 K (see Fig. 4b). For an estimate of the lower bound of A for xc = 0.16, see Extended Data Fig. 11 and the ‘Estimation of the A coefficient and the extent of the T-linear regime for x = 0.16’ section in Methods.
Calculation of A for FeSe from existing Fermi surface parameters
The A coefficient of the T2 resistivity contains important information about the enhancement of the quasiparticle effective mass m*, as encapsulated in the empirical Kadowaki–Woods ratio that links the coefficient of the T2-resistivity to the square of the electronic specific heat coefficient and is expressed for a multiband quasi-two-dimensional metal as18:
where c is the c-axis lattice parameter, N is the number of formula units per unit cell, kFi is the Fermi wave vector for the individual Fermi pockets and \(\mathop{a}\limits^{ \sim }\) is the effective minimum mean-free-path \({\ell }\) (the Mott–Ioffe–Regel limit), that can be set, depending on the appropriate definition, to be equal to a, the a-axis lattice parameter (\({\ell }\) = a) or 1/kF (kF\({\ell }\) = 1).
According to electronic structure calculations based on density functional theory, the Fermi surface of FeSe comprises five cylindrical pockets: three hole pockets in the centre of the zone and two electron pockets at the zone corners. However, two independent quantum oscillation studies carried out in high magnetic fields up to 35 T by Terashima et al.13 and Watson et al.11 found only four fundamental frequencies that one might attribute to the extremal areas of the different cylinders. A comparison of the findings of the two studies is shown in Extended Data Table 1. As one can see, good agreement was found between the two studies. Similar frequencies were also reported (albeit with smaller masses) in an earlier pulsed-field experiment32.
The absolute value of the low-temperature electronic specific heat coefficient γel places a strong thermodynamic constraint on the possible assignment of these oscillation frequencies to individual pockets. For quasi-two-dimensional FeSe, γel can be estimated simply by multiplying the sum of the (averaged) masses of all the individual pockets by 0.7 mJ mol−1 K−2 (refs 11,13). Moreover, in order to ensure charge neutrality in (stoichiometric) FeSe, we should ensure, within experimental uncertainty, that the (averaged) areas of the individual electron and hole pockets are equivalent. With this in mind, the best pairing of the four oscillation frequencies turns out to be α/δ and β/γ as the minimum/maximum of each pocket respectively. We note that this assignment is qualitatively consistent with the observation that the magnitude of α and β increases with increasing polar angle13, while that of δ and γ correspondingly decreases. This assignment also has the advantage of making the individual pockets more warped, in agreement with the relatively low electrical anisotropy or low (factor of two) anisotropy in Hc2.
With this assignment, one then obtains (averaged) effective masses m* for the two pockets of 3.35me and 5.55me from which γel = 6.2 mJ mol−1 K−2, that is, in good agreement with the as-measured value of 5.7–6.8 mJ mol−1 K−2 (refs 33,34,35). Making the pairings α/γ and β/δ, as done by Terashima et al.13, also gives γel = 6.2 mJ mol−1 K−2, but does not satisfy charge neutrality. Under the assumption that there were three rather than two pockets in FeSe, Watson et al.11 estimated γel to be 9.4 mJ mol−1 K−2, 50% higher than the measured value. In summary, the combination of quantum oscillation studies and specific heat measurements suggests that there are only two pockets in FeSe containing equal numbers of electrons and holes. We cannot completely rule out, however, the possibility of a second very small electron pocket with a light mass that has been inferred from multiband analysis of Hall and magnetotransport data36,37. In the following, we consider a purely two-band picture.
The existence of singular cylindrical pockets of equal (averaged) cross-section simplifies our working considerably. First, our expression for A now becomes:
From the quantum oscillation frequencies reported in refs 3,4, we find kF = 1.07(1) nm−1. Taking m* = 3.35me and 5.55me for the two pockets and noting that N = 2 and c = 5.52 Å, we obtain A = 90 nΩ cm K−2 and 230 nΩ cm K−2 assuming \({\ell }\) = a and kF\({\ell }\) = 1, respectively. The latter is in reasonable agreement with the measured value (A = 260 nΩ cm K−2) and suggests that the origin of the T2 resistivity of FeSe within the nematic phase is (enhanced) electron–electron scattering.
Calculation of A* for FeSe1−xSx
Quantum oscillations have been measured for several members of the FeSe1−xSx family (0.0 ≤ x ≤ 0.19) by Coldea et al.20. The same frequencies found in pristine FeSe can be tracked as a function of x and show a gradual increase in magnitude with the possible appearance of an additional frequency or frequencies at higher x. (The new frequency ε reported in ref. 20 at F ≈ 400 T is assumed here to be the second harmonic of β (F ≈ 200 T), rather than arising from a third pocket which, as described above, would be inconsistent with the measured electronic specific heat coefficient). As indicated by equation (1), the A coefficient in the electrical resistivity is dependent on both (m*)2 and (kF)3. To isolate the change in A that arises from (m*)2 alone, in the following we use the data of ref. 20 to track the evolution of kF and then obtain a renormalized A coefficient given by the following expression:
where kF(0) = 1.07 nm−1 is the effective Fermi wave vector for both pockets in FeSe. (Note that this expression is only strictly valid in the regime of charge neutrality where the kF values for both the electron and hole pockets remain equivalent.)
Extended Data Fig. 9 shows the evolution of the two sums (α + δ and β + γ) as a function of x, obtained from figure 3c of ref. 20. As one can see, the charge compensation condition is found to be satisfied well for all x < 0.17. For x = 0.19, the discrepancy may indicate the appearance of a third pocket, a point we shall return to later. In the following, however, we assume that charge neutrality is preserved across the phase diagram and obtain effective kF values for the electron and hole pocket for each x using the dashed lines shown in Extended Data Fig. 9, and finally A* using equation (3) above. The resulting plot for A*(x) is shown in Fig. 4a.
Calculation of α
It has been shown for a number of correlated metals near quantum criticality that the strength of the T-linear scattering rate ħ/τ ≈ αkBT where α is a number close to unity31. In order to test this relation in FeSe1−xSx, we use the simple Drude expression for the electrical conductivity for a quasi-two-dimensional metal to obtain the following formula for α (again assuming perfect compensation and kFe = kFh = kF):
where dρ/dT is the slope of the T-linear resistivity and all the other labels refer to the same parameters as above. The kF values were obtained from Extended Data Fig. 9 using the same procedure as for A* while the m* values were determined from A*(x) using the scaling relation.
where A*(0) = 260 nΩ cm K−2 (for FeSe) and m*(0) = (5.55 + 3.35)me/2 = 4.45me is the pocket-averaged effective mass for FeSe.
Determination of the upper critical field
The upper critical field Hc2(x) (for B//ab) is defined in Extended Data Fig. 10a as the field strength at which ρab first deviates by 1.5σ (σ is the standard deviation) from its high-field slope. For consistency, these values were determined at the same temperature, T = 1.35 K, the lowest temperature that we could access the normal state resistivity for all x ≠ 0.16 with the maximal magnetic field available to us. For x = 0.16, we extrapolated the value of the upper critical field at 1.35 K by fitting the points at higher temperatures to the formula \({H}_{{\rm{c}}2}\left(T\right)={H}_{{\rm{c}}2}^{0}\left(1-{\left(\frac{T}{{T}_{{\rm{c}}}}\right)}^{2}\right)\). The values obtained are plotted in Extended Data Fig. 10b as a function of x. The jump in Hc2 above x = 0 is probably due to the increased disorder that modifies the effective coherence length. The peak in Hc2 at the critical doping xc is presumed to be due to the renormalization of vF (through m*) at the quantum critical point.
Estimation of the A coefficient and the extent of the T-linear regime for x = 0.16
As reported in Fig. 2e, the resistivity for the sample closest to the quantum critical point (x = 0.16) appears to vary linearly with temperature down to 1.5 K—the lowest temperature at which we could access the normal state. This confirms an earlier study for x = 0.16 down to 4.2 K, in which ρab(T) was determined by extrapolating the positive magnetoresistance (with B//c) above Hc2 (ref. 17). To determine a lower limit for the T2-coefficient for x = 0.16, the temperature derivative of the resistivity curve acquired in 35 T was replotted in Extended Data Fig. 11. Even though it is not possible to distinguish any deviation from a T-linear behaviour down to the lowest measured temperature, an estimation of the A coefficient was extracted from the slope of a straight line passing through the origin and through the mean value of the derivative at the lowest measured temperature, thus assuming that ρab would cross over to a T2 behaviour below the accessible temperature range of our experiments. Extended Data Fig. 11 also defines the upper bound of the strictly T-linear regime, as indicated by the arrow.
Data availability
The data that support the findings of this study are available from the authors on reasonable request. See the ‘Author Contributions’ section for specific datasets.
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Acknowledgements
We acknowledge discussions with Q. Si, A. Chubukov and J. Schmalian. We also acknowledge the support of the HFML-RU/NWO, a member of the European Magnetic Field Laboratory (EMFL). This work is part of the research programme ‘Strange Metals’ (grant number 16METL01) of the former Foundation for Fundamental Research on Matter (FOM), which is financially supported by the Netherlands Organisation for Scientific Research (NWO). A portion of this work was also supported by the Engineering and Physical Sciences Research Council (grant number EP/L015544/1), by Grants-in-Aid for Scientific Research (KAKENHI) (grant numbers 15H02106, 15H03688, 15KK0160, 18H01177 and 18H05227) and Innovative Areas ‘Topological Material Science’ (grant number 15H05852) from the Japan Society for the Promotion of Science (JSPS).
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N.E.H. initiated the project (in collaboration with Y.M. and T.S.). S.K. synthesized the FeSe1−xSx single crystals. S.L., J.B., J.A. and J.L. performed the magnetotransport measurements. S.L. and N.E.H. analysed the data. N.E.H. and S.L. wrote the manuscript with input from all co-authors.
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Extended data figures and tables
Extended Data Fig. 1 Calibration of the Cernox temperature sensor in a magnetic field of 35 T between 0.3 K and 30 K.
The coloured symbols in the graph are the data points taken at different constant temperatures as explained in the text. The points were then divided into four temperature intervals to calculate phenomenological fits, plotted here as lines. The inset shows a detail of the lowest temperature range.
Extended Data Fig. 2 Low-temperature magnetoresistance of FeSe1−xSx.
a, Field sweeps obtained for a sample with x = 0.2 at several fixed temperatures. The magnetoresistance itself has a negligible temperature dependence over the entire temperature range studied. b, Comparison of a selection of field sweeps for x = 0. Note that the extent of the y scale is different for the 1 K curve because ρab is much smaller than at higher temperatures.
Extended Data Fig. 3 Field derivative of the magnetoresistance between 34 T and 35 T at different temperatures for x = 0.13.
The blue symbols represent the slope of linear fits to the magnetoresistance (dρab/dB) curves, while the pink symbols are the difference between the 35 T resistivity and its extrapolated value at zero field. Down to about 1.5 K, the magnitude of the magnetoresistance (MR) is essentially constant. Below 1.5 K, the effect of superconducting (SC) fluctuations on the magnetoresistance can be clearly seen. Vertical error bars represent a compound error of the difference in slope maxima and mimina associated with the scatter in the data and uncertainty in the geometrical factors.
Extended Data Fig. 4 Temperature dependence of the in-plane resistivity ρab of FeSe1−xSx.
The plots show ρab(T) curves in zero field and in a 35 T magnetic field B//ab, for all x.
Extended Data Fig. 5 Definition of the temperature scales T1 and T2.
For each x value, the temperature derivative of the resistivity curve was obtained after binning and smoothing the 35 T data of Extended Data Fig. 4. The extent of the T-linear behaviour of dρab/dT defines T2, whereas the onset temperature of the constant regime is T1.
Extended Data Fig. 6 Determination of the A coefficients from the resistivity curves.
Raw data plotted against T2.
Extended Data Fig. 7 Determination of the A coefficients from the resistivity curves.
Binned and smoothed data plotted against T2.
Extended Data Fig. 8 Determination of Ts.
The structural phase-transition temperature Ts is determined from the temperature derivatives of the resistivity curves in a broad temperature range of up to about 150 K. The kink in the resistivity curves that can be seen in Fig. 1c corresponds to a dip in the derivatives.
Extended Data Fig. 9 The x-dependence of the quantum oscillation frequencies F in FeSe1−xSx.
The black circles and terracotta diamonds represent respectively the evolution, as a function of S substitution x, of the sums α+δ and β+γ of the quantum oscillation frequencies reported in ref. 21. The two dashed lines are linear fits that were used in the determination of kF (at each x) for the renormalization of the A coefficient (to A*) and in the estimate of α, the prefactor in the strength of the T-linear scattering rate. See Methods for more details.
Extended Data Fig. 10 Determination of Hc2.
a, Definition of Hc2 at T = 1.35 K for x = 0.25. b, Plotted values of Hc2(T = 1.35 K) as a function of varying x. The black dashed lines are exponential fits. Hc2(T = 1.35 K, x = 0) is much smaller than at higher S concentrations, presumably owing to the lower level of disorder in FeSe. Vertical error bars originate from uncertainties in the determination of Hc2 (as defined in Methods) due to scatter in the raw field sweeps. The larger error bar for x = 0.16 is due to the additional uncertainty caused by having to extrapolate the Hc2 curve below 4.2 K.
Extended Data Fig. 11 T-linear resistivity at x ≈ xc.
Estimation of lower limit of A for x = 0.16 from the temperature derivative of the 35 T resistivity curve. The slope of the blue dashed line is 2A = 0.66 μΩ cm K−2. The arrow indicates the temperature at which ρab(T) ceases to be strictly linear. As shown in Fig. 4b, T2 (the temperature below which the T2 resistivity first appears) is approximately half that of T1 (the temperature down to which the resistivity remains T-linear) for all x < 0.16. Thus, it is not unreasonable to assume that the maximum value of T2 for xc = 0.16, if indeed the resistivity does cross over to T2, is a factor of two smaller than the base temperature of our experiment, making our estimate for the minimum value of A twice the absolute minimum plotted in Fig. 3b.
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Licciardello, S., Buhot, J., Lu, J. et al. Electrical resistivity across a nematic quantum critical point. Nature 567, 213–217 (2019). https://doi.org/10.1038/s41586-019-0923-y
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DOI: https://doi.org/10.1038/s41586-019-0923-y
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