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Also at ]Electrical Engineering Department, Faculty of Physical and Mathematical Sciences, University of Chile, Santiago, Chile

Collective enhancement in dissipative quantum batteries

Javier Carrasco [ [email protected] Department of Physics, Faculty of Physical and Mathematical Sciences, University of Chile, Santiago, Chile    Jerónimo R. Maze Institute of Physics, Pontificia Universidad Católica de Chile, Santiago, Chile Research Center for Nanotechnology and Advanced Materials, Pontificia Universidad Católica de Chile, Santiago, Chile    Carla Hermann-Avigliano Department of Physics, Faculty of Physical and Mathematical Sciences, University of Chile, Santiago, Chile ANID - Millennium Science Initiative Program - Millennium Institute for Research in Optics (MIRO), Chile    Felipe Barra Department of Physics, Faculty of Physical and Mathematical Sciences, University of Chile, Santiago, Chile
(December 27, 2024)
Abstract

We study a quantum battery made out of NN non-mutually interacting qubits coupled to a dissipative single electromagnetic field mode in a resonator. We quantify the charging energy, ergotropy, transfer rate, and power of the system, showing that collective enhancements are still present despite of losses, and can even increase with dissipation. Moreover, we observe that a performance deterioration due to dissipation can be reduced by scaling up the battery size. This is useful for experimental realizations when controlling the quality of the resonator and the number of qubits are limiting factors.

I Introduction

The possibility of using quantum resources for technological purposes is currently an active research field, in which quantum batteries (QBs) have emerged as promising tools for the thermodynamic control at the quantum scale Campaioli et al. (2018); Henao and Serra (2018); Andolina et al. (2019a, b); Santos et al. (2019, 2020); Bhattacharjee and Dutta (2021). A quantum battery is a quantum mechanical system that behaves as an efficient energy storage device. Its realization is motivated by the fact that genuine quantum effects such as entanglement or squeezing can typically boost the performances of classical protocols, e.g., by speeding up the underlying dynamics Deffner and Campbell (2017); Giovannetti et al. (2003). Enhancements provided by quantum correlations in the charging (or discharging) process of a QB has been previously discussed in Alicki and Fannes (2013); Hovhannisyan et al. (2013); Binder et al. (2015); Campaioli et al. (2017); Julià-Farré et al. (2020); Rossini et al. (2020); Rosa et al. (2020). Possible realizable models have been explored, including spin-chains and qubits interacting with electromagnetic fields Le et al. (2018); Ferraro et al. (2018); Andolina et al. (2018); Zhang et al. (2019); Crescente et al. (2020); Delmonte et al. (2021); Yao and Shao (2021); Barra et al. (2022). More recently, an experimental realization using organic microcavities has been reported Quach et al. (2022).

Up to now, research efforts have been mostly focused on understanding QBs as closed systems, isolated from the environment. The dissipation of real QBs has only recently been considered Farina et al. (2019); Barra (2019); Pirmoradian and Mølmer (2019); Liu et al. (2019); Carrega et al. (2020); Gherardini et al. (2020); Bai and An (2020); Quach and Munro (2020); Ghosh et al. (2021); Santos (2021). Hence, an important question to answer is how dissipation harms the performance of a QB. Understanding collective enhancements in the presence of dissipation is crucial to experimentally realize QBs.

In this Letter we address the aforementioned question by analyzing the case of NN non-mutually interacting two-level systems (qubits) charged via a single electromagnetic field mode in a resonator. This system is described by the Tavis-Cummings model Tavis and Cummings (1968, 1969), which is known to provide an effective description of experimentally feasible many-body systems in circuit and cavity QED Fink et al. (2009); Leek et al. (2009); Lolli et al. (2015); Yang et al. (2018). This configuration is compared to NN copies of a resonator with one qubit. The former is a collective QB while the latter is a parallel QB. Our findings show that the performance of parallel and collective QBs (for instance, the power) decreases under dissipation as expected. Nevertheless, the ratio between the power of the collective over the parallel QB increases with dissipation meaning that the deterioration in performance is smaller for the collective QB. More remarkably, we find that the loss in performance due to dissipation can be reduced by scaling up the QB, which means equally increasing the injected energy and number of qubits. In many systems this is easier to do than decreasing dissipation. We also analyze collective enhancements and performances in charging energy, ergotropy, and transfer rate. For the first two, we obtain similar results as for the charging power. For the transfer rate, instead, we find that its collective enhancement decreases and its performance increases as the dissipation rate increases.

II Dissipative Quantum Batteries

We start by defining a general model for a QB. It consists of two subsystems: an energy “holder” that stores energy for long times, and an energy “charger” that acts as transducer of energy to deliver external input energy into the holder. The charger can also be used as a discharging path for the holder, unless the battery is designed to be directly discharged from the holder via external classical fields. We define the former discharging mode as “normal”, and the latter as “transducing”. Furthermore, we identify that the battery can be charged up either from initial conditions or through external classical driving. In this work we focus on the former charging case, where the charger is prepared in an energetic state and then left to interact with the holder allowing for energy transfer. Therefore, the QB system is effectively described by the Hamiltonian

λ=c+h+λch,\displaystyle\mathcal{H}_{\lambda}=\mathcal{H}_{c}+\mathcal{H}_{h}+\lambda\mathcal{H}_{c-h}, (1)

where c,h\mathcal{H}_{c,h} are the free Hamiltonians of the charger and holder, respectively, interacting via the Hamiltonian ch\mathcal{H}_{c-h}. The parameter λ\lambda can be 0 or 1 and defines in which stage the QB is: λ=1\lambda=1 for the charging and normal discharging stages, and λ=0\lambda=0 for the storage and transducing discharging stages. For this QB protocol to work, the switching time between stages must be much smaller than the characteristic time of the dynamical evolution of the battery in each separate stage. If this condition is fulfilled, the Hamiltonian λ\mathcal{H}_{\lambda} is correctly considered time-independent in each separate stage. The previously defined QB model is pictured in Fig. 1.

We focus on a model in which the charger is a single electromagnetic field mode in a resonator coupled to an array of NN non-mutually interacting identical qubits that act as the holder Ferraro et al. (2018). Under the rotating wave approximation, the Hamiltonian is that of the Tavis-Cummings model Tavis and Cummings (1968, 1969); Carmichael (2002); Klimov and Chumakov (2009); Putz (2017); Kirton et al. (2019): c=ωcaa,h=ωhi=1Nσi+σi,ch=gi=1N(aσi++aσi)\mathcal{H}_{c}=\hbar\omega_{c}a^{\dagger}a,\mathcal{H}_{h}=\hbar\omega_{h}\sum_{i=1}^{N}\sigma_{i}^{+}\sigma_{i}^{-},\mathcal{H}_{c-h}=\hbar g\sum_{i=1}^{N}(a\sigma_{i}^{+}+a^{\dagger}\sigma_{i}^{-}), where aa (a)(a^{\dagger}) is a bosonic annihilation (creation) operator, σi±\sigma_{i}^{\pm} are raising (++) or lowering (-) atomic operators for the ii-th qubit, ωc,h\omega_{c,h} are the characteristic frequencies of the resonator and the qubits, respectively, gg is the coupling strength, and \hbar is the reduced Planck’s constant. We use g=103ωcg=10^{-3}\omega_{c} to be consistent with the rotating wave approximation. In this physical system, transitioning between battery stages means to change between negligible (λ=0\lambda=0) and non-negligible (λ=1\lambda=1) holder-charger interaction, which can be achieved by external fields that modify ωc,h\omega_{c,h} to transition between far-from-resonant (|ωcωh|g,\absolutevalue{\omega_{c}-\omega_{h}}\ll g, hence λ=0\lambda=0) and resonant (ωc=ωh,\omega_{c}=\omega_{h}, hence λ=1\lambda=1) dynamics. Hence, ωc=ωh\omega_{c}=\omega_{h} during charging and normal discharging stages Ferraro et al. (2018).

For an isolated QB, the dynamics would simply be determined by the Hamiltonian λ\mathcal{H}_{\lambda}. However, to account for dissipation and decoherence on the QB due to its coupling with the environment, a master equation is needed where a dissipator super-operator 𝔇[]\mathfrak{D}[\cdot] is added to the Liouville-von Neumann equation giving Breuer et al. (2002); Rivas and Huelga (2011); Carmichael (2002)

dρdt=i[λ,ρ]+𝔇[ρ],\displaystyle\derivative{\rho}{t}=-\frac{\mathrm{i}}{\hbar}\commutator{\mathcal{H}_{\lambda}}{\rho}+\mathfrak{D}[\rho], (2)

where ρ\rho is the density operator or state of the QB. Moreover, we argue that a QB has practical sense only if the dissipation rate of the holder, κh\kappa_{h}, is much lower than that of the charger, κc\kappa_{c}. Hence, if the frequency holder-charger effective coupling factor is geffκhg_{\mathrm{eff}}\gg\kappa_{h} but comparable to κc\kappa_{c}, it is sufficient to consider only the charger dissipator 𝔇c\mathfrak{D}_{c} during charging and discharging stages. Thus we set 𝔇𝔇c\mathfrak{D}\approx\mathfrak{D}_{c} in the master equation. During the storage stage, holder dissipators might be added. However, storage times τs2π/κh\tau_{s}\ll 2\pi/\kappa_{h} where holder dissipation is negligible are still relevant as a battery if τs2π/κc\tau_{s}\gg 2\pi/\kappa_{c}, meaning that we could achieve energy storage beyond what would be possible with just the charger.

For our Tavis-Cummings QB in study, geff=gNg_{\mathrm{eff}}=g\sqrt{N} Haroche and Raimond (2006); Putz (2017) and the charger dissipator is 𝔇c[]=κ(nth+1)(2aaaaaa)+κnth(2aaaaaa)\mathfrak{D}_{c}[\cdot]=\kappa(n_{\mathrm{th}}+1)(2a\cdot a^{\dagger}-a^{\dagger}a\cdot-\cdot a^{\dagger}a)+\kappa n_{\mathrm{th}}(2a^{\dagger}\cdot a-aa^{\dagger}\cdot-\cdot aa^{\dagger}), which is given by an environment of thermal photons with mean number nth=1/(eωc/kBT1)n_{\mathrm{th}}=1/(\mathrm{e}^{\hbar\omega_{c}/k_{\mathrm{B}}T}-1) at temperature TT, 2κ2\kappa is the charger dissipation rate κc\kappa_{c}, and kBk_{\mathrm{B}} is Boltzmann’s constant. We use nth=0n_{\mathrm{th}}=0 to solely study the dissipation from the charger avoiding the re-population effects of a nonzero temperature.

Refer to caption
FIG. 1: A generic QB consisting of a charger “cc” and a holder “hh” in its three operation stages: charging, storage, and discharging. The holder, initially empty, obtains energy from the charger interacting a time τc\tau_{c} with the Hamiltonian ch\mathcal{H}_{c-h}. The energy transferred to the holder is stored for a time τs\tau_{s} until we desire to use the energy. To discharge the holder in a time τd\tau_{d} we can proceed in transducing mode (bottom) with external classical fields over the holder through a unitary operation 𝒰t\mathcal{U}_{t}, or in normal mode (top) through the charger where the dissipation channels might be used to finally extract the energy. We focus on time scales for which the charger dissipation (𝔇\mathfrak{D}) is relevant, but holder dissipation is negligible.

III Collective Enhancement

Refer to caption
FIG. 2: Collective (#) and parallel (\parallel) versions of a QB of size NN. The collective QB has one charger “cc” with EcE_{c} initial energy and one holder “hh” consisting in NN units cells “h1h_{1}”. The parallel QB has NN copies of “cc” with Ec/NE_{c}/N initial energy, each interacting with a different unit cell “h1h_{1}” as holder. Hence, the \parallel QB is just NN copies of the NN-times down-scaled # QB.

If the holder of a QB consists in NN copies of a subsystem, i.e. NN holder unit cells, we can compare its performance versus NN copies of the QB with only one holder unit cell. These represent two versions of a QB that have the same maximum storable energy. The former is the collective version (#\#) as it has NN holder unit cells interacting with the same charger, while the latter is the parallel version (\parallel) as it has NN independent copies of one charger with one holder unit cell (see Fig. 2). When compared, the collective version shows an increase in the transfer rate due to correlations Alicki and Fannes (2013); Hovhannisyan et al. (2013); Binder et al. (2015); Campaioli et al. (2017). This motivates the definition of the transfer rate collective enhancement (similar to the quantum advantage Campaioli et al. (2018)) Γ1/τ¯=(1/τ¯#)/(1/τ¯)Ω¯#/Ω¯\Gamma_{1/\bar{\tau}}=(1/\bar{\tau}^{\#})/(1/\bar{\tau}^{\parallel})\equiv\bar{\Omega}^{\#}/\bar{\Omega}^{\parallel} where τ¯#\bar{\tau}^{\#} and τ¯\bar{\tau}^{\parallel} are the interaction times needed to charge or discharge the QB up to its first dynamical maximum in the collective and parallel versions, respectively. Γ1/τ¯\Gamma_{1/\bar{\tau}} quantifies how much larger is the transfer rate Ω¯2π/τ¯\bar{\Omega}\equiv 2\pi/\bar{\tau} for the collective version compared to the parallel one. If Γ1/τ¯>1\Gamma_{1/\bar{\tau}}>1, the collective QB has a larger transfer rate than the parallel QB, meaning that Ω¯\bar{\Omega} is enhanced in the collective version of the QB. We extend the previous concept to all interesting figures of merit ff of a QB that quantify its performance (larger ff, better battery), including charging and discharging energy, transfer rate, power, and maximum extractable energy through unitary operations (ergotropy Allahverdyan et al. (2004)), by defining the collective enhancements Γf¯=f¯#/f¯\Gamma_{\bar{f}}=\bar{f}^{\#}/\bar{f}^{\parallel}. More generally, if Γf¯>1\Gamma_{\bar{f}}>1, ff is enhanced in the collective version. For isolated QBs, Γ1/τ¯>1\Gamma_{1/\bar{\tau}}>1 and ΓE¯h<1\Gamma_{\bar{E}_{h}}<1, where EhE_{h} is the holder energy, and the bar represents the event of first maximum transferred energy into the holder during the charging stage (see Fig. 3). However, in the thermodynamic limit (NN\rightarrow\infty) these inequalities might change Julià-Farré et al. (2020). In general, the figures of merit depend on the duration τ\tau of the charging (τc\tau_{c}), storage (τs\tau_{s}) or discharging (τd\tau_{d}) stages depicted in Fig. 1, and f¯=f(τ¯)\bar{f}=f(\bar{\tau}). In this work we show that the former inequality also holds for non-isolated QBs, while the latter changes.

IV Results

Refer to caption
FIG. 3: Mean energy EhE_{h} and ergotropy h\mathcal{E}_{h} charged on the holder (array of NN qubits) when charging from an initial Fock light state. The mean energy EcE_{c} of the charger (resonator) and heat QQ from the QB are also shown. The dynamics seen correspond to Rabi-like oscillations, transferring energy from the charger to the holder. The holder oscillations for different NN and κ\kappa are given in Appendix C. The segmented lines define τ¯\bar{\tau} and E¯h\bar{E}_{h}.
Refer to caption
FIG. 4: Collective (a) enhancements Γf¯\Gamma_{\bar{f}} and (b) performances for the first maximum charge when charging from Fock initial conditions for energy, transfer rate, power, and ergotropy. The results for coherent and thermal initial conditions are given in Appendix C.
Refer to caption
FIG. 5: Distribution of the total energy over the QB. Collective (#) and parallel (\parallel) are compared for the three cases of initial conditions simulated.

We now study the robustness of the collective enhancements when dissipation is taken into account in the Tavis-Cummings QB. The following initial conditions of the resonator are studied: Fock, coherent, and thermal states. All three with mean number of photons Tr{aaTrh{ρ(0)}}=N\Tr\{a^{\dagger}a\Tr_{h}\{\rho(0)\}\}=N. In all cases, the qubits are initially in their ground state. We analyze the holder (charger) energy Eh(c)E_{h(c)}, transfer rate Ωh(c)2π/τ\Omega_{h(c)}\equiv 2\pi/\tau, power Ph(c)Eh(c)/τP_{h(c)}\equiv E_{h(c)}/\tau, and ergotropy h(c)\mathcal{E}_{h(c)} for the charging stage. Fig. 3 depicts EhE_{h}, EcE_{c}, the holder ergotropy, which is computed from the reduced state of the holder at the given time, and the heat from the QB, Q(t)0tTr{(t)𝔇[ρ(t)]}dtQ(t)\equiv-\int_{0}^{t}\Tr\{\mathcal{H}(t^{\prime})\mathfrak{D}[\rho(t^{\prime})]\}\differential t^{\prime}, over time. The total energy is given by Eh(t)+Ec(t)+Q(t)=NωcE_{h}(t)+E_{c}(t)+Q(t)=N\hbar\omega_{c}. Frequencies are shown in terms of the Rabi frequency of the Fock case when N=1N=1 and κ=0\kappa=0, given by ΩR2g\Omega_{R}\equiv 2g. Fig. 4 shows the collective enhancements Γf¯\Gamma_{\bar{f}} and performances f¯\bar{f} for the Fock case for different values of κ\kappa and NN. The other two cases produce very similar results and hence are included in Appendix C. Nonetheless, the key differences between them are visualized in Fig. 5 for the respective collective and parallel QBs.

Naturally, larger dissipation rates produce faster loss of energy available to charge up the holder resulting in a decrease of E¯h#\bar{E}_{h}^{\#} as well as ¯h#\bar{\mathcal{E}}_{h}^{\#} (see Fig. 4). On the other hand, larger κ\kappa also means that the first maximum transferred energy into the holder, although smaller, is reached sooner, and therefore the transfer rate performance increases (see Fig. 4). Hence, as the decrease of E¯h#\bar{E}_{h}^{\#} shows to be higher than the increase of Ω¯h#\bar{\Omega}_{h}^{\#}, the charging power P¯h#\bar{P}_{h}^{\#} ends up decreasing. These results are plotted for different NN in Fig. 4.b, which shows that the curves move upwards when NN increases, meaning that a reduction in performance due to dissipation may be restored by scaling up the QB. For κ=0\kappa=0 this behavior was obtained in Ferraro et al. (2018), and our results for κ>0\kappa>0 can here be considered as an extrapolation of those results. Although, caution must be taken with the statement about restoring the performance, because the separation between curves of consecutive values of NN seems to get smaller in each increment for a fixed κ\kappa, and even more as κ\kappa is also increased. However, for values of κ\kappa around 4g4g or smaller, we argue that we do not need to fabricate a resonator with the highest possible quality factor as long as we compensate by scaling up the QB. This can be of practical advantage for realizing a QB with systems where adding more qubits and photonic energy is feasible, as in the case of NV centers, which come as natural defects in diamond crystals Schirhagl et al. (2014).

The increase of performances with NN is explained (for κ=0\kappa=0 Klimov and Chumakov (2009)) by the collective behavior of the qubits producing a larger effective Rabi frequency, allowing for a faster population of the excited eigenenergies. This upgrade of the performances is better quantified as collective enhancement in Fig. 4.a, where it is clear that the collective QB version is better than the parallel one (Γf¯>1\Gamma_{\bar{f}}>1), except for the energies at κ0\kappa\approx 0 where ΓE¯h1\Gamma_{\bar{E}_{h}}\leq 1. This exception is important because it shows that a simple extrapolation of the collective enhancement in energy obtained at κ=0\kappa=0 would give the wrong result as if the parallel battery were to perform better. Moreover, we observe that collective enhancements in energy and power increase for larger dissipation rates, which means that despite of the decrease of the respective performances in both QB versions, the collective ones decrease less, i.e. they are more robust under dissipation. Instead, the collective enhancement in charging transfer rate decreases with larger κ\kappa, meaning that the parallel QB is more robust in this regard.

Regarding the ergotropy, its collective enhancement is not shown as the numerator and denominator become (non-simultaneously) exactly zero very often. Except for values of κ0\kappa\sim 0, we get Γ¯>1\Gamma_{\bar{\mathcal{E}}}>1, meaning that for transducing QBs more energy is available in the collective version. This is shown in Fig. 5, specially clear for the Fock case. Fig. 5 shows the energy distributed in its different available forms, and from here it is concluded that the coherent case is the best. This happens because the coherent case is much more robust than the Fock one against dissipation. Only for κ0\kappa\approx 0 and N1N\approx 1 the Fock case is better as seen in Appendix C. For κ=0\kappa=0 and large enough NN, the coherent case is better because when the initial condition is a coherent state, the amount of energy locked in the charger-holder correlations is minimized as studied in Andolina et al. (2019b).

In the discharging stage, the initial condition of the holder is the one reached after the charging process, and the charger is empty. The subsequent dynamics is again a Rabi-like oscillation, as shown in Fig. 3. Therefore, similar results of performances and collective enhancements are expected for the normal discharging stage.

V Conclusions

In this Letter we have defined different types of open QBs and analyzed them in the context of the Tavis-Cummings model, studying their collective behavior under dissipation, considering three types of initial conditions. For this study, we have defined the collective enhancements as figures of merit for the performance of a collective QB over its parallel version. In particular, we have also focused on the case of a QB made of a photonic resonator and an array of qubits to obtain quantitative estimations.

We observed that dissipation, while diminishing the performance in charging energy and power, the corresponding collective enhancements are instead boosted up, because the collective QB version is more robust against dissipation. Regarding the charging transfer rate, the opposite occurs as the parallel version is more robust in this quantity. In addition, we showed that, a higher collective performance can be achieved by scaling up the QB, i.e. increasing the number of qubits and photonic energy in the same amount, although due to the decrease in energy performance, this effect is only meaningful for κ4g\kappa\lesssim 4g. Furthermore, this up-scaling increases all collective enhancements. Also, we showed that initially preparing the resonator light mode in a coherent state produces better results in ergotropy performance than a Fock or thermal state.

Our work shows that collective QBs are better than parallel ones in a different way than simple extrapolation from results of isolated QBs (κ=0\kappa=0) as we commented for the energy collective enhancement. It also shows that the dissipation rate κc\kappa_{c} and the scale NN of the QB can be seen as degrees of freedom to design a QB with a desired performance, while understanding that collective QBs are more robust under changes in dissipation. This is particularly useful if increasing NN is much easier than decreasing κc\kappa_{c} in the specific system to experimentally realize, or if the precision error in obtaining a specific κc\kappa_{c} is important.

Finally, the collective enhancements and performances introduced here, along the clarification of different types of QBs, will serve for future studies in the field, considering different batteries and their experimental realizations.

All simulations were performed with QuTiP Johansson et al. (2013) in Python.

VI Acknowledgments

J.R.M. acknowledges support from Conicyt Fondecyt Regular grant No. 1180673, Conicyt PIA/Anillo ACT192023, AFOSR grant No. FA9550-18-1-0513, and ONR grant No. N62909-18-1-2180. C.H-A. acknowledges support from Fondecyt Grant Nº 11190078, and Conicyt-PAI grant 77180003, and ANID - Millennium Science Initiative Program - ICN17_012. J.C. and F.B. acknowledge support from Fondecyt grant No. 1191441, and the ANID Millennium Nucleus “Physics of active matter”.

Appendix A Ergotropy of the Jaynes-Cummings Model

If the state ρ\rho and (non-degenerate) Hamiltonian \mathcal{H} of a system are written orderly as

ρ\displaystyle\rho =krk|rkrk|,rkrk+1,\displaystyle=\sum_{k}r_{k}\outerproduct{r_{k}}{r_{k}},\ r_{k}\geq r_{k+1}, (3)
\displaystyle\mathcal{H} =kϵk|ϵkϵk|,ϵk<ϵk+1,\displaystyle=\sum_{k}\epsilon_{k}\outerproduct{\epsilon_{k}}{\epsilon_{k}},\ \epsilon_{k}<\epsilon_{k+1}, (4)

where rk,ϵkr_{k},\epsilon_{k} are the eigenvalues and |rk,|ϵk\ket{r_{k}},\ket{\epsilon_{k}} the eigenkets of the state and Hamiltonian, respectively; then the ergotropy of ρ\rho can be calculated by Allahverdyan et al. (2004)

[ρ]=jkrjϵk(|rj|ϵk|2δjk),\displaystyle\mathcal{E}[\rho]=\sum_{jk}r_{j}\epsilon_{k}(\absolutevalue{\innerproduct{r_{j}}{\epsilon_{k}}}^{2}-\delta_{jk}), (5)

where δjk\delta_{jk} is the Kronecker delta. Thus, for the case of the Jaynes-Cummings model (N=1N=1) with a Fock state as the charger initial condition, focusing on the qubit sub-system (tracing over the resonator), it is easy to obtain the state of the qubit

ρ=sin2(gt)|ee|+cos2(gt)|gg|,\displaystyle\rho=\sin^{2}(gt)\outerproduct{e}{e}+\cos^{2}(gt)\outerproduct{g}{g}, (6)

which is diagonal in the energy basis with eigenvalues λ1(t)=sin2(gt)\lambda_{1}(t)=\sin^{2}(gt) and λ2(t)=cos2(gt)\lambda_{2}(t)=\cos^{2}(gt) corresponding to the eigenkets |e\ket{e} and |g\ket{g}, respectively.

It can be seen that if

λ1(t)λ2(t)\displaystyle\lambda_{1}(t)\geq\lambda_{2}(t) cos(2gt)0\displaystyle\Longleftrightarrow\cos(2gt)\leq 0 (7)
gt[π4,3π4]±kπ,k.\displaystyle\Longleftrightarrow gt\in\left[\frac{\pi}{4},\frac{3\pi}{4}\right]\pm k\pi,k\in\mathbb{N}. (8)

Therefore, outside of these intervals, the ordering of the eigenvalues is inverted.

Now, in units of ωc\hbar\omega_{c}, H=σz/2H=\sigma_{z}/2 with eigenvalues ϵ1=1/2\epsilon_{1}=-1/2, ϵ2=1/2\epsilon_{2}=1/2 and eigenkets |ϵ1=|g\ket{\epsilon_{1}}=\ket{g}, |ϵ2=|e\ket{\epsilon_{2}}=\ket{e}.

Finally, by simply applying the formula 3, the ergotropy is obtained as

(t)={12cos2(gt),gt[π4,3π4]±kπ 0gt[π4,3π4]±kπ,\displaystyle\mathcal{E}(t)=\begin{cases}1-2\cos^{2}(gt),\ &gt\in\left[\frac{\pi}{4},\frac{3\pi}{4}\right]\pm k\pi\\ \mbox{\quad\quad}0\ &gt\not\in\left[\frac{\pi}{4},\frac{3\pi}{4}\right]\pm k\pi\end{cases}, (9)

which corresponds to h/(ωc)\mathcal{E}_{h}/(\hbar\omega_{c}), and clearly has the first maximum at t=2π/4gπ/ΩRt=2\pi/4g\equiv\pi/\Omega_{R} (used as timescale for all plots) with a value ¯h=ωc\bar{\mathcal{E}}_{h}=\hbar\omega_{c}, after recovering the original units in energy.

For the Tavis-Cummings model (N1N\geq 1), the equivalent numerical procedure is done to calculate the ergotropy.

Appendix B Typical Experimental Values

For our Tavis-Cummings QB in study, geff=gNg_{\mathrm{eff}}=g\sqrt{N} Haroche and Raimond (2006); Putz (2017) and typical experimental values are κh0.5×102geff\kappa_{h}\approx 0.5\times 10^{-2}g_{\mathrm{eff}}, with geff0.5×103ωcg_{\mathrm{eff}}\approx 0.5\times 10^{-3}\omega_{c}, achieved with NV centers as qubits Doherty et al. (2013); Putz (2017); Eisenach et al. (2021). In the case of using Rydberg atoms as qubits, the typical values are κh102g\kappa_{h}\approx 10^{-2}g, with g×106ωcg\approx\times 10^{-6}\omega_{c} Haroche and Raimond (2006); Guerlin et al. (2007); Uria et al. (2020). Regarding κc\kappa_{c}, its value depends on the quality factor of the fabricated resonator, which can reach values such that the charger dissipation can be neglected. However, we study the case in which this is not a precondition.

Appendix C Additional Simulations Data

Simulation results complementary to Fig. 4 of the main text are shown in Figs. 6 to 7, where the cases of coherent and thermal states as the charger initial condition are included, as well as the heat from the QB. The coherent and thermal cases have been simulated up to N=4N=4 and N=6N=6, respectively, due to the rapid increment in numerical complexity.

Simulation results complementary to Fig. 3 of the main text are shown in Figs. 8 to 11, showing the Rabi-like oscillations up to near the first energy maximum, for N=1,,4N=1,...,4 and κ[0,2ΩR]\kappa\in[0,2\Omega_{R}], for the three cases of charger initial conditions studied. These results correspond to the collective QB version.

The performances of the figures of merit are presented in Fig. 6. These results are very similar if we compare them with each other by fixing the figure of merit and changing the charger initial condition. The collective enhancements are presented in Fig. 7. These results are also very similar if we compare them with each other by fixing the figure of merit and changing the charger initial condition, excepting the ergotropy, as the appearance of zeros in the denominator appear in the Fock and Thermal cases, resulting in non-plotted data. Hence, the ergotropy is better analyzed with Fig. 9, which clearly shows that the coherent case is the more robust against dissipation, and explains the ergotropy shown in Fig. 5 of the main text.

Further data and analyses can be found in Carrasco (2021), where the holder populations are plotted and a deeper study on the feasibility of using NV centers as qubits for Tavis-Cummings QBs is also done.

References

Refer to caption
FIG. 6: Performances of the collective QB for Fock, coherent and thermal states as the charger initial condition. Comparing between these cases of initial condition, there is no significant meaningful difference, justifying the use of only the Fock case in the main manuscript.
Refer to caption
FIG. 7: Collective enhancements of the relevant figures of merit for Fock, coherent and thermal states as the charger initial condition. Comparing between these cases of initial condition, there is no significant meaningful difference, excepting the ergotropy, justifying the use of only the Fock case in the main manuscript, where the ergotropy is analyzed separately.
Refer to caption
FIG. 8: Holder energy over time up to near the first maximum for Fock, coherent and thermal states as the charger initial condition. Results of the collective QB version. It it observed that the Fock case reaches a higher first maximum of holder energy EhE_{h} than the coherent and thermal cases. Nonetheless, these maximums are obtained in a shorter time in the thermal case. Also, as the dissipation rate growths, the three cases tend to the same curve.
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FIG. 9: Holder ergotropy over time up to near the first holder energy maximum for Fock, coherent and thermal states as the charger initial condition. Results of the collective QB version. The Fock case shows the highest ergotropy for κ0\kappa\approx 0, but it rapidly goes to zero as κ\kappa increases. Instead, the coherent case changes less, which means that its ergotropy performance is more robust under dissipation.
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FIG. 10: Resonator energy over time up to near the first holder energy maximum for Fock, coherent and thermal states as the charger initial condition. Results of the collective QB version. These plots can be seen as the complement of Fig. 8, since it shows how the resonator energy ErE_{r} is reduced while it is been transferred to the holder as EhE_{h}. Although, Er+EhE_{r}+E_{h} is not a constant because some energy is lost in form of heat QQ, shown in Fig. 11.
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FIG. 11: Heat from the QB over time up to near the first holder energy maximum for Fock, coherent and thermal states as the charger initial condition. Results of the collective QB version. These plots are very similar between the three cases of initial condition, with small differences only appreciable for κ0\kappa\approx 0.