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Reply to ”Comment on the ’Decrease of the surface resistance in superconducting niobium resonator cavities by the microwave field’”

G. Ciovati gciovati@jlab.org Thomas Jefferson National Accelerator Facility, Newport News, Virginia 23606, USA    P. Dhakal Thomas Jefferson National Accelerator Facility, Newport News, Virginia 23606, USA    A. Gurevich Department of Physics, and Center for Accelerator Science, Old Dominion University, Norfolk, Virginia 23529, USA
(August 16, 2025)
Abstract

In a recent comment Romanenko and Grassellino rom_com made unsubstantiated statements about our work [Appl. Phys. Lett. 104, 092601 (2014)] and ascribed to us wrong points which we had not made. Here we show that the claims of Romanenko and Grassellino are based on misinterpretation of Ref. apl_Qrise, , and inadequate data analysis in their earlier work rom .

preprint: AIP/123-QED

The goal of Ref. apl_Qrise, was to reveal mechanisms of the microwave enhancement of the quality factor Q(H)Q(H) observed on Ti-alloyed Nb cavities. This was done using the standard Arrhenius method to deconvolute a thermally-activated and residual contributions to the surface resistance apl_Qrise ,

Rs(Ts)=AeU/kTs+Ri.R_{s}(T_{s})=Ae^{-U/kT_{s}}+R_{i}. (1)

The Arrhenius method was used in Ref. gigi, to separate the temperature-independent residual resistance RiR_{i} from the conventional BCS contribution RBCS(T)AeU/kTsR_{BCS}(T)\simeq Ae^{-U/kT_{s}} measured in Nb cavities at low H=4H=4 mT. This procedure was based on the Mattis-Bardeen expression mb for RBCS(T)R_{BCS}(T), which enables one to unambiguously separate the quasiparticle contribution RBCSR_{BCS} from additional temperature-independent contributions to RiR_{i} at TTcT\ll T_{c} which are not described by the simplest version of the BCS model. In Refs. rom, ; apl_Qrise, the Arrhenius method was adopted to analyze Rs(T,H)R_{s}(T,H) at strong rf fields in the region of nonlinear electromagnetic response. In this case no simple theoretical expression for the quasiparticle contribution is available so the physical meaning of the phenomenological parameters in Eq. (1) becomes far from obvious. This is because the thermally-activated contribution A(H)exp[U(H)/kTs(H)]A(H)\exp[-U(H)/kT_{s}(H)] becomes highly nonlinear in HH and gets intertwined with complex nonequilibrium kinetics of quasiparticles kopnin , and with such extrinsic mechanisms as trapped vortices, proximity coupled normal oxide regions, etc. One of the manifestations of nonequilibrium effects is rf heating which makes the local temperature of quasiparticles TsT_{s} higher than the bath temperature T0T_{0}, the electron temperature can be higher than the lattice temperature at kT<<UkT<<U ( Ref. kopnin, ).

In our work we stated two facts: 1. Alloying Nb cavities with Ti or N significantly extends the field region where Q(H)Q(H) exhibits a remarkable increase with HH, 2. Heating effects were disregarded in the analysis of Ref. rom, . Contrary to the assertion of Romanenko and Grassellino, we did not make any comments on the validity of Ref. rom, , nor did we suggest that the mechanism of the significant increase of Q(H)Q(H) observed on Ti and N alloyed cavities Dhakal ; Anna is the same as the low-field increase of Q(H)Q(H) observed on non-alloyed Nb cavities Padamsee2009 . And we certainly did not suggest that the microwave suppression of RsR_{s} is due to heating. What we did say was that it is important to separate intrinsic mechanisms of rf nonlinearity from heating effects to reveal the physics of the microwave suppression of Rs(H)R_{s}(H). In any case, the Arrhenius method in which heating was taken into accountapl_Qrise cannot be less accurate than the same method in which heating was disregardedrom , and the claim of Romanenko and Grassellino that taking heating into account can somehow produce some unspecified ”systematic errors” was not substantiated.

The reason why our measurements of Q(H)Q(H) were performed in the extended temperature region 1.6 K <T<5<T<5 K with 20-30 TT-datapoints per each rf field value, and a self-consistent account of rf heating is that the Arrhenius fit becomes far more reliable than what was done in Ref. rom, where heating was disregarded and data were taken only in a very narrow temperature range 1.6 K <T<2<T<2 K per each rf field value rom . The actual number of TT-datapoints per each rf field value was not specified: the inset in Fig. 1b of Ref. rom, shows RBCS(H,T)R_{BCS}(H,T) for only four T-datapoints at 1.7, 1.8, 1.9 and 2 K, which would be insufficient for a stable fit. In any case, the accuracy of UU extracted from the Arrhenius fit of lnRs(T)\ln R_{s}(T) in such narrow temperature region, 1.6<T<21.6<T<2 K is poor, but the accuracy of evaluation of AA and RiR_{i} in Eq. (1) from the extrapolation of the semi-logarithmic plot of lnRs\ln R_{s} versus 1/T1/T is much worse.

The analysis of our own data shows that, had we restricted our measurements to 1.6 K <T<2<T<2 K like in Ref. rom, , the accuracy and the scattering of the fit parameters AA and RiR_{i} with nine T-datapoints per each rf field value would have been so bad that no reliable conclusions about the physical mechanisms of Rs(H)R_{s}(H) could have been made, even though Eq. (1) still provides a good fit to the Rs(T)R_{s}(T) data, as illustrated in Figs. 1 and 2. This is because there are not enough datapoints to constrain the fit parameters for the acceptable chi-square statistical minimization for which it is important to have enough data points above Tλ=2.17T_{\lambda}=2.17 K, where the exponential temperature dependence of Rs(T)R_{s}(T) dominates and rf heating must be taken into account. Otherwise, the fit parameters AA and RiR_{i} become poorly constrained, leading to erroneous dependencies of AA, UU and RiR_{i} on HH. This issue, combined with the increased systematic uncertainty in measuring quality factor value of 1011\sim 10^{11} at 1.6\sim 1.6 K, shows that the physical conclusions inferred from the RsR_{s}-decomposition of Ref. rom, can hardly be trusted. This problem with the procedure of Ref. rom, may explain the negative residual resistance resulting from a fit of one of the data set shown in Fig. 6 of Ref. rom_bake, , the unrealistically large ratio Δ/kTc=2.4\Delta/kT_{c}=2.4 for Nb at 20 mT and non-systematic oscillations of U(H)U(H) and Ri(H)R_{i}(H) shown in Fig. 1a of Ref. rom, .

Refer to caption
Figure 1: Subset of mean Rs(T0)R_{s}(T_{0}) data below TλT_{\lambda} after 1400 C HT at μ0H=6.2±0.4\mu_{0}H=6.2\pm 0.4 mT (circles) and μ0H=27±1\mu_{0}H=27\pm 1 mT (squares) apl_Qrise . Solid lines were obtained from a fit with Eq. (1) using Ts=T0T_{s}=T_{0}.
Refer to caption
Figure 2: Dependencies of AA, UU and RiR_{i} on the rf field amplitude after 1400 C HT (circles) and after \simμ\mum BCP (triangles) obtained by fitting only the data below TλT_{\lambda} with Eq. (1), like in Refs. rom_com, ; rom, . This fit results in large scattering and unphysical values of the parameters (Ri<0R_{i}<0, U<1U<1 meV).

Heating even below the lambda point could result in significant effects. Indeed, a small local temperature increase δTT0\delta T\ll T_{0} at the inner cavity surface increases RBCSR_{BCS} to:

RBCS(T)=RBCS(T0)exp(UδT/kT02)R_{BCS}(T)=R_{BCS}(T_{0})\exp(U\delta T/kT_{0}^{2}) (2)

Overheating at the inner cavity surface by 50 mK increases RBCSR_{BCS} by 24%\sim 24\% at 2.0 K and UU\simeq1.5 meV for Nb, and by 55%\sim 55\% for δTs=0.1\delta T_{s}=0.1 K. Temperature maps of the outer cavity surfaces have routinely revealed local temperature increases, 50100\simeq 50-100 mK at the rf fields 90100\sim 90-100 mT Padamsee2009 ; gc , which indicates higher δT>ΔT\delta T>\Delta T in hotspots at the inner surface gc . It is generally difficult to accurately extract TsT_{s} from the thermometry data since the temperature of the outer surface cannot be measured directly because only a fraction of the heat is transferred to the thermometers. Moreover, hotspots can result in significant admixture of the BCS component to the averaged residual resistance R¯i\bar{R}_{i} and its significant temperature and field dependencies at strong fields gc . This effect masks the intrinsic field and temperature dependencies of RsR_{s}, so the separation of heating effects is essential.

Romanenko and Grassellino apparently misunderstood our interpretation of the microwave suppression of RsR_{s} which was based on the analysis of the experimental data and the well-known results of the BCS theory. The mechanism suggested in Ref. apl_Qrise, not only explains the observed extended increase of Q(H)Q(H) but also predicts a logarithmic field dependence of A(H)A(H) in excellent agreement with the data. The opinion of Romanenko and Grassellino stems from the model of Ref. rom, which assumes that the BCS contribution can be unambiguously separated from the residual resistance at any rf field because RiR_{i} dominates at TTcT\ll T_{c}. The latter is based on the incorrect postulate that the residual resistance is physically unrelated to the quasiparticle BCS contribution in the simplest version of the BCS model in which the density of states N(E)N(E) vanishes at all energies below the gap |E|<Δ|E|<\Delta, and RBCSR_{BCS} at high fields can be evaluated a-priori using the Mattis-Bardeen formula which is only valid in the limit of H0H\to 0.

The quasiparticle BCS surface resistance can be intertwined with the residual resistance, particularly at high fields. One mechanism related to the vortex hotspotsgc was already mentioned above. Another mechanism of coupling berween RiR_{i} and RBCSR_{BCS} is due to the current pairbreaking induced by the rf field which makes U(H)U(H) smaller than Δ\Delta, and a finite N(E)N(E) at E<ΔE<\Delta due to the sub-gap states at H=0H=0 which have been revealed by numerous tunneling experiments on all superconducting materials (see, e.g., Ref. ag, and references therein). Because small but finite N(E)N(E) at E<ΔE<\Delta gives rise to a weakly temperature dependent contribution attributed to the residual resistance, the latter is a natural part of the quasiparticle (BCS) contribution taking into account the realistic N(E)N(E) observed on superconducting materials (other extrinsic contributions to RiR_{i} were discussed in Ref. ag, ). As the rf field amplitude increases, the rf currents further broaden N(E)N(E) resulting in the microwave suppression of Rs(H)R_{s}(H). The importance of the sub-gap states and the interplay of the ”natural” and the rf broadening of N(E)N(E) and their effect on the observed increase of Q(H)Q(H) with HH was discussed at the end of our Letter apl_Qrise .

In conclusion, none of the claims of Romanenko and Grassellino is relevant or backed by scientific arguments. At the same time, the physical conclusions based on the deconvolution of RBCSR_{BCS} and RiR_{i} using the procedure of Ref. rom, are questionable because of the incorrect model assumptions, and poor stability and accuracy of the Arrhenius fit for the insufficient number of the temperature datapoints, as discussed above.

References

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