Phase-resolved Higgs response in superconducting cuprates

In high-energy physics, the Higgs field couples to gauge bosons and fermions and gives mass to their elementary excitations. Experimentally, such couplings can be inferred from the decay product of the Higgs boson, i.e., the scalar (amplitude) excitation of the Higgs field. In superconductors, Cooper pairs bear a close analogy to the Higgs field. Interaction between the Cooper pairs and other degrees of freedom provides dissipation channels for the amplitude mode, which may reveal important information about the microscopic pairing mechanism. To this end, we investigate the Higgs (amplitude) mode of several cuprate thin films using phase-resolved terahertz third harmonic generation (THG). In addition to the heavily damped Higgs mode itself, we observe a universal jump in the phase of the driven Higgs oscillation as well as a non-vanishing THG above Tc. These findings indicate coupling of the Higgs mode to other collective modes and potentially a nonzero pairing amplitude above Tc. Interaction between Cooper pairs and other collective excitations may reveal important information about the pairing mechanism. Here, the authors observe a universal jump in the phase of the driven Higgs oscillations in cuprate thin films, indicating the presence of a coupled collective mode, as well as a nonvanishing Higgs-like response at high temperatures, suggesting a potential nonzero pairing amplitude above Tc.

F or field theories with U(1) continuous symmetry and respecting Lorentz invariance or particle-hole symmetry, spontaneous symmetry breaking gives rise to an order parameter with two orthogonal collective modes: the Goldstone mode along the azimuthal direction, and the Higgs mode along the radial direction 1 . In superconductors, discussions about the Higgs mode and the Higgs mechanism precede those in highenergy physics 2,3 . However, their significance to superconductivity has been more slowly appreciated. Experimental detection of the Higgs mode has also been hampered by its lack of electric and magnetic dipole moments in most superconductors. Recently, it was proposed that the Higgs mode may reveal the superconducting gap symmetry and multiplicity [4][5][6] , unveil coupled collective modes 7 , or explain aspects of light-induced superconductivity 8 . Novel methods for exciting and detecting the superconducting Higgs mode were also demonstrated using ultrafast terahertz techniques in the meantime 9,10 . Specifically, free oscillations of the Higgs mode, with its characteristic frequency of 2Δ, can be launched by an ultrashort terahertz pulse quenching the free energy of the order parameter 9 . Alternatively, it could also be periodically driven at 2ω through nonlinear coupling between the electromagnetic vector potential A(ω) and the superconducting condensate [10][11][12] . The resulting free (driven) Higgs oscillation manifests itself in terahertz transmissivity as an oscillation at 2Δ (2ω). In the latter scenario, the 2ω oscillation of the condensate interacts with the driving field A(ω), leading to sum frequency generation or third harmonic generation (THG), which is resonantly enhanced when 2ω = 2Δ(T) 10,13 .
While both free and driven Higgs oscillations have been demonstrated in s-wave superconductors, the Higgs mode of dwave superconductors is more complex. The continuous variation of Δ between 0 and Δ max along different directions of the Brillouin zone leads to strong dephasing of the mode. This is compounded by the existence of quasiparticle excitations at arbitrarily low energies, which provide rapid decay channels and significantly damp the mode 14 . Terahertz pump optical probe experiments on Bi 2 Sr 2 CaCu 2 O 8+x single crystals have provided the first experimental evidence for an isotropic Higgs response of d-wave superconductors in the form of an |A| 2 response in the condensate's optical reflectivity to a monocycle terahertz pulse 15 . On the other hand, periodically driving the Higgs oscillation would provide useful phase information that may indicate resonance and coupling to other modes. Such an experiment requires a multicycle, carrier-envelope phase-stable terahertz source with a narrow bandwidth and high electric field strength, which is provided by the TELBE superradiant undulator source at HZDR 16 . Using this facility, we investigate the THG response of optimally-doped La 1.84 Sr 0.16 CuO 4 (T c = 45 K), DyBa 2 Cu 3 O 7−x (T c = 90 K), YBa 2 Cu 3 O 7−x (T c = 88 K), and overdoped Bi 2 Sr 2 -CaCu 2 O 8+x (T c = 65 K) thin films (Supplementary Note 1). Our experiment is performed with 0.7 THz driving frequency, with an electric field up to~50 kV cm −1 (Supplementary Note 2). In all of these samples, we observe an increase in THG intensity (I TH ) below T c that is consistent with a heavily damped Higgs oscillation. In addition, in LSCO(OP45), DyBCO(OP90) and YBCO (OP88), a universal jump in the relative phase between the THG response and the linear drive (Φ TH ) at T < T c is observed, signifying the coupling of the Higgs mode to another collective mode. We also observe a nonzero I TH persisting above T c in all of the samples, which may indicate preformed Cooper pairs above T c .

Results
THG response of d-wave superconductors. To illustrate the THG response of d-wave superconductors, first we show terahertz transmission through LSCO(OP45). As Fig. 1a-d shows, while the residual fundamental harmonic (FH) dominates the terahertz transmission above T c , a large amplitude of third harmonic (TH) becomes visible below T c . Moreover, FH transmission (I FH ) monotonically decreases with decreasing temperature as shown in Fig. 1e. In comparison, TH intensity (I TH ) exhibits a maximum below T c . In the context of superconductors, the nonlinear Meissner effect 17,18 , charge density fluctuations (CDF) 19 , and   Higgs oscillations have been previously reported or discussed to give rise to THG. Unlike what is observed in this study, the nonlinear Meissner effect manifests as a narrow peak around T c in the 3 rd order nonlinear current. It is often discussed in terms of nonlinear Josephson current and might be probing the phase response of weakly connected superconducting islands 1 . On the other hand, studies on s-wave and d-wave superconductors have suggested an anisotropic response from CDF, while THG from the fully symmetric (A 1g ) Higgs oscillation is expected to be isotropic 15,[19][20][21] . To distinguish between CDF and the A 1g Higgs response, we performed THG polarization dependence measurements. An isotropic response is found to dominate (Fig. 2a, c). In addition, we performed terahertz pump optical probe (TPOP) measurements similar to Reference 15. An |A(ω)| 2 response to the A(ω) driving field is also seen in the condensate's optical reflectivity (Fig. 2b). These results may not uniquely identify, but are consistent with a driven Higgs response to the multicycle terahertz pulse and its role in THG below T c . The THG polarization dependence indicates that there might be a finite contribution from other sources such as CDF or additional nonlinear mechanisms not yet discussed or experimentally evidenced. Therefore, a full understanding of the different sources of THG in addition to the driven Higgs oscillations requires further experimental and theoretical efforts. For instance, it will be interesting to investigate the systematic doping dependence of the anisotropic response in THG and TPOP experiments to quantify the relative contributions between different symmetry components 15 . Finally, to ensure that the Higgs oscillation stays in the perturbative excitation regime, we performed fluence dependence measurements. An excellent agreement with the expected I TH ∝ I FH 3 dependence is observed (Fig. 1f) (Supplementary Note 6).
Temperature dependence of THG. To look for potential resonance of the Higgs oscillation at 2ω = 2Δ(T), we performed detailed temperature dependence measurements as shown in Fig. 3a-c. In LSCO(OP45) we observe a peak in I TH near 0.6T c , as well as a smaller peak around 0.9T c . DyBCO(OP90) exhibits a similar peak in I TH near 0.6T c . In comparison, YBCO(OP88) exhibits a sharp peak in I TH near 0.9T c and a hump around T c . In BSCCO(OD65), a continuously increasing I TH with decreasing temperature is observed (Supplementary Note 7). A careful examination of the transmitted I FH reveals that the main peak in I TH originates from the competition between a growing nonlinear response of the Higgs oscillation and an increasing screening of the driving field as temperature decreases (Supplementary Note 3). Therefore, the main peak is not a resonance feature. In fact, for optimally-doped cuprates, we expect Δ(T = 0) ≳ 20 meV and a steep onset of Δ at T c . Therefore, the 2ω = 2Δ(T) resonance, if present, is expected to be satisfied immediately below T c for ω = 0.7 THz (~3 meV). Moreover, as the Higgs mode of d-wave systems is heavily damped, a resonance peak in I TH is expected to be significantly broadened. This motivates us to investigate the phase of the driven Higgs oscillation, which is expected to exhibit a prominent change across resonance even in the presence of strong damping (Supplementary Note 8).
Phase evolution of THG below T c . In Fig. 3d-f, we extracted the relative phase (Φ TH ) of the TH with respect to the FH signal (Supplementary Note 4). Despite dissimilar features in I TH, all three samples exhibit a similar response in Φ TH. In particular, an abrupt jump of nearly π happens at a temperature T π < T c . In YBCO(OP88), T π is in the range where 2ω = 2Δ(T) is expected to be satisfied. However, such a sharp phase jump is again inconsistent with the resonance of a heavily damped collective mode. In LSCO(OP45) and DyBCO(OP90), T π is significantly lower than T c . In light of these, we do not attribute the universal phase jump to the 2ω = 2Δ(T) Higgs resonance. A more striking evidence for such an interpretation comes from the direction of the phase jump. Since the low-temperature regime corresponds to driving below resonance (2ω < 2Δ(T)) and the high-temperature regime to driving above resonance (2ω > 2Δ(T)), a resonance-like phase jump should evolve positively with temperature whereas the observed Φ TH jumps negatively with temperature.

Discussion
To obtain an intuitive understanding of the phase response, we look at a driven coupled harmonic oscillators model. Whereas isolated oscillators exhibit a maximum in their amplitude and a positive phase jump ≲ π across resonance 13 (Supplementary Note 8), the coupled oscillators system develops an antiresonance in addition to resonances. This manifests as a minimum in the amplitude of the driven oscillator, simultaneous with a phase jump in the negative direction (Fig. 4a). To more closely model our experiment, we fix the driving frequency but allow the energetics of the oscillators to depend on temperature (Fig. 4b) (Supplementary Note 8). By choosing their resonance frequencies (n s is the experimentally measured superfluid density in LSCO(OP45)), the model recaptures the essential features of LSCO(OP45) (Fig. 3a,  d). In YBCO(OP88) a smaller dip in I TH (T) is seen while in DyBCO(OP90) a kink in I TH (T) is observed at the T π . This could be due to the sharpness of the phase jump in these two samples, causing the dip in I TH (T) to be very narrow in temperature and buried between the measured temperature points. In the framework of the coupled oscillators model, this suggests that the coupled mode is less damped in the bilayer systems compared to the single-layer LSCO(OP45). A classical Fresnel analysis of the thin film effects excludes the possibility of the phase jump coming from linear shifts in Φ FH (T) and Φ TH (T) (Supplementary Note 5).
While our classical toy model does not aim to explain the microscopic origin of the observed THG response, it allows us to learn about the dynamics and energetics of the coupled mode. It suggests that the coupled mode is underdamped and has an energy scale comparable to the Higgs mode. Moreover, the energy of this mode and/or its coupling to the Higgs mode depends on temperature. Within these constraints, potential candidates for the coupled collective mode include paramagnons, collective charge fluctuations of the incipient charge density wave (CDW) order, or phonons. In particular, coupling between the Higgs mode and CDW excitations has been observed in NbSe 2 and 2H-TaS 2 superconductors 22,23 . In cuprates, charge order exhibits a similar energy scale as the superconducting gap 24 . Evidence for the incipient charge order in a wide range of the phase diagram has also been reported 25 . On the other hand, paramagnons are strongly renormalized in the superconducting state into a sharp underdamped resonance mode in a similar energy window as the superconducting gap 26 . They are prominent candidates for mediating Cooper pairing in high-T c superconductors. Last but not least, strong electron-phonon coupling may also contribute a phononic character to the superconducting order parameter 27 , leading to new amplitude mode(s) in the Higgs response 7 . Other exotic but potential candidates include the Bardasis-Schrieffer mode 28,29 and the anisotropic A 2g /B 1g Higgs mode 4,6 (Supplementary Note 9), which are also collective modes of the superconducting order parameter. Future doping and magnetic field dependence studies may shed light on the identity of the coupled mode.
While the identity of the coupled mode demands further scrutiny, our experiment also reveals a non-vanishing THG response above T c in all samples. In Fig. 4c, we plot the temperature dependence of (I TH /I FH 3 ) 1/4 , which is theoretically predicted to be ∝ Δ away from resonance 13 . Indeed, (I TH /I FH 3 ) 1/4 exhibits an order parameter-like temperature dependence below T c . Surprisingly, it remains nonzero up to T > 1.5T c , similar to the temperature regime where superconducting fluctuations are observed in Nernst effect measurements 30 . This is more clearly illustrated by the transmitted TH waveform from LSCO(OP45) at T = 50 K > T c (Fig. 4d). Our observation may indicate preformed Cooper pairs in cuprates without global phase coherence, or the intense terahertz field might enforce phase coherence above T c 12 . The pseudogap, and its various ordered phases including the CDW order, may also play a role in THG above T c 31,32 .
While the coupled oscillators model offers an intuitive explanation for the unexpected phase jump in THG in several families of cuprates, it is a classical toy model and calls for a full quantum mechanical treatment of the subject to provide deeper insight. In parallel, future magnetic field and doping dependence investigations may further help unveil the nature of the coupled mode and the non-vanishing THG response above T c . Sweeping the driving frequency may also help distinguish the different scenarios of dwave gap closing or filling as temperature approaches T c . While these initiatives are underway, our technique may also serve as a probe for non-equilibrium superconductivity 33,34 . With so many interesting prospects, we see a bright future for phase-resolved spectroscopy of collective modes in superconductors and beyond [35][36][37][38] . . d-f Temperature dependence of the relative phase between the TH response and the FH drive, extracted from waveforms such as those in Fig. 1c, d. Inset shows representative TH waveforms across the π phase jump temperature (T π ). The dotted line (black) denotes T c and the solid line (red) denotes T π . The error bars represent the two sigma uncertainty from fitting the phase of TH and FH waveforms (Supplementary Note 4).

Methods
Sample growth and characterization.

Data availability
The data that support the findings of this study are available from the first author and the corresponding authors upon reasonable request. The raw pre-sorted and pre-binned data that allow statistical analysis is available at https://doi.org/10.14278/rodare.277 together with the software tools that were used for data treatment. Further requests on data treatment should be sent to HZDR via S.Ko.

Code availability
The numerical code used to calculate the results for this work is available from H.C. and L.S. upon reasonable request. The dotted lines depict the amplitude response of a critically damped harmonic oscillator and an underdamped harmonic oscillator as the driving frequency ω is varied. When these two oscillators are coupled, the coupled system retains two resonances but also develops an anti-resonance. Across the anti-resonance (vertical dotted line), the amplitude (solid red line) of the driven oscillator goes through a minimum while its phase (solid blue line) jumps negatively with the driving frequency. b Assuming the driving frequency is fixed as in our experiment, but that the resonance frequency of the two oscillators varies with temperature as Δ(T) and δΔ(T) (δ < 1), the response of the coupled oscillators system is shown as a function of T. The anti-resonance in a is recaptured: the amplitude of the Higgs oscillation (thin red line) goes through a minimum while its phase (thick blue line) jumps negatively with T. The dotted line illustrates the effect of screening, which is to reduce the driving force and hence the amplitude at lower T. c Temperature dependence of (I TH /I FH 3 ) 1/4 , which remains finite above T c . (I TH /I FH 3 ) 1/4 is theoretically predicted to be ∝ Δ away from resonance. d FH and TH components extracted from the transmitted waveform from LSCO(OP45) at 50 K > T c . NATURE COMMUNICATIONS | https://doi.org/10.1038/s41467-020-15613-1 ARTICLE NATURE COMMUNICATIONS | (2020) 11:1793 | https://doi.org/10.1038/s41467-020-15613-1 | www.nature.com/naturecommunications