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New J. Phys. 10 (2008) 095018
doi:10.1088/1367-2630/10/9/095018

Dissipation in circuit quantum electrodynamics: lasing and cooling of a low-frequency oscillator

Julian Hauss1,2, Arkady Fedorov1,3, Stephan André1, Valentina Brosco1, Carsten Hutter1,4, Robin Kothari1,5, Sunil Yeshwanth1,6, Alexander Shnirman7,8,9 and Gerd Schön1,8

1 Institut für Theoretische Festkörperphysik, Universität Karlsruhe, D-76128 Karlsruhe, Germany
2 Lichttechnisches Institut, Universität Karlsruhe, D-76128 Karlsruhe, Germany
3 Kavli Institute of Nanoscience, Delft University of Technology, 2600 GA Delft, The Netherlands
4 Department of Physics, Stockholm University, AlbaNova University Center, SE-106 91 Stockholm, Sweden
5 Department of Physics, Indian Institute of Technology Bombay, Mumbai 400076, India
6 Department of Physics, Indian Institute of Technology, Kanpur 208016, India
7 Institut für Theorie der Kondensierten Materie, Universität Karlsruhe, D-76128 Karlsruhe, Germany
8 DFG-Center for Functional Nanostructures (CFN), Universität Karlsruhe, D-76128 Karlsruhe, Germany

9 Author to whom any correspondence should be addressed.

E-mail: shnirman@tkm.uni-karlsruhe.de

Received 5 June 2008
Published 30 September 2008

Abstract. Superconducting qubits coupled to electric or nanomechanical resonators display effects previously studied in quantum electrodynamics (QED) as well as extensions thereof. Here, we consider a driven qubit coupled to a low-frequency oscillator and study the influence of dissipation. When the qubit is driven to perform Rabi oscillations, with Rabi frequency in resonance with the oscillator, the latter can be driven far from equilibrium. Blue detuned driving leads to a population inversion in the qubit and lasing behavior of the oscillator (`single-atom laser'). For red detuning, the qubit cools the oscillator. This behavior persists at the symmetry point where the qubit–oscillator coupling is quadratic and decoherence effects are minimized. Here, the system realizes a `single-atom-two-photon laser'.

Contents

1. Introduction

Recent experiments on quantum state engineering with superconducting circuits realized concepts originally introduced in the field of quantum optics, as well as extensions thereof, e.g. to the regime of strong coupling [1]–[8]. Josephson qubits play the role of two-level atoms, whereas electric or nanomechanical oscillators play the role of the quantized radiation field. These `circuit quantum electrodynamics (QED)' experiments prompted substantial theoretical activities [9]–[19]. In most QED or circuit QED experiments, the atom or qubit transition frequency is near resonance with the oscillator. In contrast, in the experiments of [1], with setup shown in figure 1(a), the qubit is coupled to a slow LC tank circuit with frequency (ωT/2π~MHz) much lower than the qubit's level splitting ( \Delta E/2\pi \hbar \sim 10\,{\rm GHz} ). The idea of this experiment is to drive the qubit to perform Rabi oscillations with Rabi frequency in resonance with the oscillator, ΩR≈ωT. In this situation, the driven qubit should excite the oscillator, and indeed in the experiments a substantial enhancement of the amplitude of the oscillator was observed [1].

Figure 1

Figure 1. (a) In the setup of [1], an externally driven three-junction flux qubit is coupled inductively to an LC oscillator. (b) A charge qubit is coupled capacitively to a mechanical resonator.

Initial attempts to explain the effect did not resolve several issues [20, 21]. In the experiments, in order to minimize decoherence effects, the Josephson flux qubit was biased near the flux degeneracy point. At this symmetry point also the coupling to the oscillator is tuned to zero, and the enhancement should vanish. Uncontrolled small deviations from the symmetry point might lead to the observed effect [1, 20], but this explanation was not supported by experiments. Here, we explore an alternative, namely that a quadratic coupling to the oscillator near the resonance condition ΩR≈2ωT is responsible for the observed enhancement. In the following, we will consider both linear as well as quadratic coupling, which dominate away from the symmetry point and at this point, respectively.

The second unresolved problem is the magnitude of the effect. The experiments [1] showed an increase by a factor of 4–5 in the amplitude, i.e. 16–25 in the number of oscillator quanta. The theory of [20], valid in the perturbative regime, predicts a much weaker effect. We obtain a strong effect as follows [18]: for blue detuning of the qubit driving, a population inversion is created in the qubit at the Rabi frequency, and at the resonance ΩR≈ωT the system becomes a `single-atom laser', or for ΩR≈2ωT a `single-atom-two-photon laser' [22, 23]. In both cases, the lasing instability is reached for realistic system parameters. In this state, the oscillator no longer responds linearly to external perturbations (its effective friction constant becomes negative), and the number of quanta in the oscillator increases strongly until saturation is reached due to nonlinear effects. The analysis of the driven circuit QED system shows that its properties depend strongly on relaxation and decoherence effects in the qubit.

A related situation, called `dressed-state lasing', had been studied before in quantum optics [24]–[26]. The present scenario differs from that one in so far as the resonator modes are coupled to the low-frequency Rabi oscillations rather than to the high-frequency Mollow transitions. The Rabi frequency can be readily tuned to resonance with the oscillator, which should facilitate reaching the lasing threshold and a proper lasing state. The unusual resonance condition has also been explored in [27] in connection with coupling of atoms.

For red detuning of the qubit driving, the qubit should cool the oscillator [18]. A similar strategy for cooling of a nanomechanical resonator via a Cooper pair box qubit has been recently suggested in [28].

Also in situations where the qubit, e.g. a Josephson charge qubit, is coupled to a nano-mechanical oscillator (figure 1(b)) it either cools or amplifies the oscillator. On one hand, this provides an important tool on the way to ground state cooling, on the other hand, it provides a realization of what is called a SASER [29].

Lasing and cooling of the oscillator have also been observed in a slightly different setup, when the Rabi-driven qubit is replaced by a superconducting single-electron transistor (SSET) biased near the Josephson quasiparticle cycle [30]–[32]. Coupled to a nanomechanical or an electric oscillator, the SSET can be used to either cool the oscillator [33]–[38] or to produce laser-like behavior. The latter has been demonstrated recently in the experiments of Astafiev et al [39].

The present paper is organized as follows. In the following section, the system of driven qubit coupled to a low-frequency oscillator is introduced and analyzed theoretically using the appropriate rotating wave approximations (RWAs) and the Schrieffer–Wolf transformation. We thus arrive at an effective Hamiltonian of the system, which allows us to proceed using techniques from quantum optics. We then consider dissipation in the rotating frame and show that it plays a crucial role for the lasing state. In particular, we formulate the master equation, which forms the basis for a numerical analysis. Finally, we derive the Langevin equations describing the dynamics of the oscillator in the presence of the driven qubit. In the next section, we present the results of the numerical analysis of the Langevin equations as well as of the full master equation and interpret them in terms of lasing with or without bistability and cooling. The paper concludes with a discussion covering several extensions.

2. Theory

2.1. The Hamiltonian

The systems to be considered are shown in figure 1. A qubit is coupled to an oscillator and driven to perform Rabi oscillations. To be specific, we first analyze a flux qubit coupled to an electric oscillator (figure 1(a)) with Hamiltonian

Equation (1)

The first two terms describe the qubit, with Pauli matrices σx, z operating in the flux basis of the qubit. The energy bias between the flux states epsilonxdc) is controlled by an external dc magnetic flux Φxdc , and Δ is the tunneling amplitude between the basis states. The resulting level spacing \Delta E \equiv \sqrt{\epsilon^2+\Delta^2} typically lies in the range of several GHz. The third term accounts for the driving of the qubit by an applied ac magnetic flux with amplitude ΩR0 and frequency ωd. The last two terms describe the oscillator with frequency \omega_{\rm T}=1/\sqrt{L_{\rm T}C_{\rm T}} as well as the qubit–oscillator interaction. In the experiments of [1], ωT lies in the range of several 10 MHz, whereas the coupling constant gMIpIT, 0 is of the order of 10 MHz. Here M is the mutual inductance, Ip the magnitude of the persistent current in the qubit, and I_{{\rm T},0}=\sqrt{\hbar\omega_{\rm T}/2L_{\rm T}} the amplitude of the vacuum fluctuation of the current in the LC oscillator.

After transformation to the eigenbasis of the qubit, which is the natural basis for the description of the dissipation, the Hamiltonian reads

Equation (2)

with tan ζ = epsilon/Δ and \Delta E \equiv \sqrt{\epsilon^2+\Delta^2} .

Because of the large difference of the energy scales between the qubit and the oscillator, \Delta E \gg \hbar \omega_{\rm T} , it is tempting, in the spirit of the usual RWA, to drop the transverse coupling term –gcos ζ σx(a + a) of equation (2). However, near the symmetry point (where sin ζ = 0) the longitudinal coupling is weak. Therefore, we retain the transverse coupling, but transform it by employing a Schrieffer–Wolff transformation, US = exp(iS), with generator S = (gE)cos ζ (a + a) σy, into a second-order longitudinal coupling. On the other hand, since \hbar \omega_{\rm d}\sim \Delta E , we can drop within RWA the longitudinal driving term -\hbar\Omega_{{\rm R}0}\cos(\omega_{\rm d}t)\sin\zeta\,{\sigma}_{z} . The Hamiltonian then reads

Equation (3)

A further unitary transformation with UR = exp(–iωdσzt/2) brings the Hamiltonian to the rotating frame, \skew4\tilde H \equiv {U}_{\rm R}^{\phantom{\dagger}}H{U}_{\rm R}^{\dagger}+ {\rm i}\hbar {\dot U}_{\rm R}^{\phantom{\dagger}}{U}_{\rm R}^{\dagger} , with

Equation (4)

Here \delta\omega \equiv \omega_{\rm d}-\Delta E/\hbar is the detuning. After diagonalization of the qubit terms, we obtain

Equation (5)

with \Omega_{\rm R}=\sqrt{\Omega_{\rm R0}^{2}\cos^2\zeta+\delta\omega^{2}} and tan β = δω/(ΩR0 cos ζ).

Finally, we employ a second RWA. While the first one dropped counter-rotating terms with frequencies of order \Delta E/\hbar , the second one drops terms oscillating with Rabi frequency ΩR or the oscillator frequency ωT. This (second RWA) approximation will be justified below. In the interaction representation with respect to the non-interacting Hamiltonian, \skew4\tilde H_0=(\hbar\Omega_{\rm R}/2){\sigma}_z+\hbar\omega_{\rm T} {a}^{\dagger}{a} , we finally arrive at

Equation (6)

We kept both single-photon and two-photon interactions, with g1 = –gsin ζcos β and g2 = (g2E)cos2ζcos β, although within RWA only one of them survives, i.e. the single-photon term for ΩRT, or the two-photon term for ΩR~2ωT. The last term of (6) with g3 = –(g2E)cos2ζsin β is the ac-Stark effect, causing a qubit-state-dependent frequency shift of the oscillator [40]. In what follows, we will assume that the qubit is kept near the symmetry point, i.e. epsilon ll Δ and cos ζ≈1.

2.2. Transition rates in the rotation frame

The transformation to `dressed states' in the rotating frame modifies the relaxation, excitation and decoherence rates as compared to the standard results [41, 42]. To illustrate these effects and justify the treatment of the dissipation in later sections, we first consider a driven qubit (ignoring the coupling to the resonator) coupled to a bath observable \skew4\hat X ,

Equation (7)

In the absence of driving, ΩR0 = 0, and for regular (i.e. smooth as a function of the frequency) power spectra of the fluctuating bath observables, we can proceed using golden rule-type arguments [41, 42]. The transverse noise, coupling to σx and σy, is responsible for relaxation and excitation processes with rates

Equation (8)

whereas longitudinal noise, coupling to σz, produces a pure dephasing with rate

Equation (9)

Here bbx + iby, and we introduced the ordered correlation function \langle\skew4\hat{X} ^{2}\rangle_{\omega}\equiv\int {\rm d}t {\rm e}^{{\rm i}\omega t}\langle\skew4\hat{X} (t)\skew4\hat{X} (0)\rangle , as well as the power spectrum, i.e. the symmetrized correlation function, S_{X}(\omega)\equiv (\langle\skew4\hat{X} ^{2}\rangle_{\omega}+\langle\skew4\hat{X} ^{2}\rangle_{-\omega})/2 . The rates (8) and (9) also define the relaxation rate 1/T1 = Γ1 = Γ + Γ and the total dephasing rate 1/T2 = Γvarphi = Γ1/2 + Γvarphi*, which appear in the Bloch equations for the qubit.

To account for the driving with frequency ωd, it is convenient to transform to the rotating frame via a unitary transformation UR = exp(–iωdσzt/2). Within RWA, the transformed Hamiltonian reduces to

Equation (10)

with detuning \delta\omega\equiv\omega_{\rm d}-\Delta E/\hbar . The RWA cannot be used in the second line of (10), since the fluctuations \skew4\hat X contain potentially all frequencies, including those of order ±ωd, which can compensate fast oscillations.

Diagonalizing the first term of (10) one obtains

Equation (11)

with \Omega_{\rm{R}}=\sqrt{\Omega_{\rm{R}0}^{2}+\delta\omega^{2}} and tan β = δω/ΩR0.

From here golden rule arguments yield the relaxation and excitation rates in the rotating frame [43]

Equation (12)

as well as the `pure' dephasing rate [43]

Equation (13)

We note the effect of the frequency mixing, and due to the diagonalization the effects of longitudinal and transverse noise on relaxation and decoherence get mixed. In addition, we note that the rates also depend on the fluctuations' power spectrum at the Rabi frequency, \langle\skew4\hat{X} ^{2}\rangle_{\pm\Omega_{\rm R}} .

For a sufficiently regular power spectrum of the fluctuations at frequencies \omega \approx \pm \Delta E/\hbar , we can ignore the effect of detuning and the small shifts by ±ΩR as compared to the high frequency \omega_{\rm d}\approx \Delta E/\hbar . We further assume that \Omega_{\rm R}\ll k T /\hbar . In this case, we find the simple relations

Equation (14)

where the rates in the lab frame are given by equation (8) and the new rate, \Gamma_\nu \equiv \frac{1}{2\hbar^2} \,b_{z}^{2} \,S_{X}(\Omega_{\rm R}) , depends on the power spectrum at the Rabi frequency.

To proceed, we concentrate on the regime relevant for our system. At low temperatures, k_{\rm B}T \ll \Delta E \approx \hbar\omega_{\rm d} , we can neglect Γ as it is exponentially small. We also assume that the system is tuned near the symmetry point of the qubit, where bz≈0. More precisely, we assume that Γν can be neglected as compared to Γ. Even if very strong 1/f noise causes substantial pure dephasing at and near the symmetry point, the rate Γν depends on the noise power spectrum at the frequency ΩR which is usually higher than the characteristic frequencies of the 1/f noise. Thus we can safely neglect Γν and we are left with

Equation (15)

where

Equation (16)

The ratio of up- and down-transitions depends on the detuning and can be expressed by an effective temperature. Right on resonance, where β = 0, we have \tilde\Gamma_{\uparrow}=\tilde\Gamma_{\downarrow} , corresponding to infinite temperature or a classical drive. For `blue' detuning, β > 0, we find \tilde\Gamma_{\uparrow}  >  \tilde\Gamma_{\downarrow} , i.e. negative temperature. This leads to a population inversion of the qubit, which is the basis for the lasing behavior which will be described below.

In a more careful analysis, not making use of the `white noise' approximation, we obtain for β = 0

Equation (17)

For example, for Ohmic noise and low bath temperature this reduces to \tilde\Gamma_\downarrow/\tilde\Gamma_\uparrow \approx 1+2\Omega_{\rm R}/\omega_{\rm d} , which corresponds to an effective temperature of order 2\hbar\omega_{\rm d}/k_{\rm B}\approx 2\Delta E/k_{\rm B} , which by assumption is high but finite. The infinite temperature threshold is crossed toward negative temperatures at weak blue detuning when the condition

Equation (18)

is satisfied. We note that all qualitative features are well reproduced by the approximation (15).

To illustrate how the population inversion is created for blue detuning we show in figure 2 the level structure, i.e. the formation of dressed states, of a near-resonantly driven qubit. For the purpose of this explanation the driving field is quantized. This level structure was described first by Mollow [25]. The picture also illustrates how for blue detuning a pure relaxation process, Γ = Γ0, in the laboratory frame predominantly leads to an excitation process, \tilde\Gamma_\uparrow , in the rotating frame.

Figure 2

Figure 2. Relaxation rates in the basis of the dressed states. The left staircase denotes the eigenstates of the undriven qubit, |↑rangle, |↓rangle and of the (quantized) driving field, |mrangle, before the driving is switched on, i.e. for ΩR0 = 0. The Hamiltonian in this basis is obtained from (3) by replacing \protect\hbar \Omega_{{\rm R}0}\cos\omega_{\rm d} t with λ(d + d), where λ is the coupling constant between the qubit and the driving field and d and d are the annihilation and the creation operators of the driving field. The right staircase stands for the dressed states of a driven qubit near resonance. They are obtained by, e.g. diagonalization (blue dashed lines) of the 2×2 Hamiltonian which couples the states |m, ↑rangle and |m + 1, ↓rangle. This gives \vert g\rangle=\cos(\frac{\pi}{4}-\frac{\beta}{2})\vert m,\uparrow\rangle +\sin(\frac{\pi}{4}-\frac{\beta}{2})\vert m+1,\downarrow\rangle and \vert e\rangle=-\sin(\frac{\pi}{4}-\frac{\beta}{2})\vert m,\uparrow\rangle +\cos(\frac{\pi}{4}-\frac{\beta}{2})\vert m+1,\downarrow\rangle . The bare Rabi frequency is given by \Omega_{{\rm R}0} \approx \lambda\sqrt{\bar m} , where \bar m is the average number of photons in the coherent (classical) driving field. The red arrows stand for relaxation rates. All rates are directed down in energy, since only the relaxation Γ is considered. However, in the dressed states basis, the dominant rate is from the state |grangle to the state |erangle, i.e. an inversion takes place.

2.3. The Liouville equation in the rotating frame

Within the approximation leading to the rates (14) the Liouville equation governing the dynamics of the density matrix in the rotating frame and in the interaction representation with respect to \skew4\tilde H_0 can be presented in a simple Lindblad form,

Equation (19)

where \tilde{\rho} is the density matrix in the rotating frame in the interaction representation. The qubit dissipation is described by

Equation (20)

It has the same form as in the lab frame, except that the rates are those appropriate for the rotating frame. Within the approximations leading to the rates (15), the master equation (19) can be obtained from the master equation in the lab frame by performing the transformations outlined above for the Hamiltonian. The resonator damping, with strength parametrized by κ, can be written as [44]

Equation (21)

Here N_{\rm th}=1/[\exp(\hbar\omega_{\rm T}/k T)-1] is the thermal photon number in the resonator.

Since we consider qubits with high degree of coherence, we are motivated to study the regime Γ0, κ, g1, g2, g3 ll ωT, ΩR, where the second RWA performed above with respect to frequencies ωT, ΩR is justified (from now on we set \hbar=1 ).

2.4. The single-qubit laser

In the following we will consider two resonance situations, when the Rabi frequency is in resonance with the oscillator, ΩR≈ωT, or when ΩR≈2ωT. In these cases either the one- or the two-photon interactions dominate. We will study the effects of detuning of the Rabi frequency ΩR relative to that of the oscillator. We will also investigate the effects of blue or red detuning of the qubit driving frequency, \delta\omega\equiv\omega_{\rm d}-\Delta E .

2.4.1. One-photon interaction Near the resonance condition, ΩR≈ωT, the Hamiltonian (6) in RWA reduces to

Equation (22)

From here we can proceed in the frame of the standard semiclassical approach [44, 45] of laser physics with the following main steps: in the absence of fluctuations, the system is described by Maxwell–Bloch equations for the classical variables α = langlearangle, α* = langlearangle, s± = langleσ±rangle and sz = langleσzrangle, which can be derived from the Hamiltonian (22) if all correlation functions are assumed to factorize. Next the qubit variables can be adiabatically eliminated as long as \kappa,\, g_1\ll\tilde\Gamma_1,\tilde\Gamma_ {\varphi} , which leads to a closed equation of motion for α. If we account for fluctuations, e.g. due to thermal noise in the resonator, α becomes a stochastic variable obeying a Langevin equation [44],

Equation (23)

Here C≡2g12, and s_z^{\rm st}=-D_0/(1+\vert\alpha^2\vert/\tilde n_0) is the stationary value of the population difference between the qubit levels, with D_0=(\tilde\Gamma_\downarrow-\tilde\Gamma_\uparrow)/\tilde \Gamma_1 being the normalized difference between the rates with \tilde\Gamma_1=\tilde\Gamma_{\uparrow}+\tilde\Gamma_{\downarrow} . Furthermore, \tilde\Gamma_\varphi=\tilde\Gamma_1/2+\tilde\Gamma_{\varphi}^{\ast} is the total dephasing rate. The detuning of the Rabi frequency enters in combination with a frequency renormalization, δΩ≡ΩR–ωT + g3|α|2. We further introduced the photon saturation numbers n_0=\tilde\Gamma_{\varphi}\tilde\Gamma_1/4g_1^2 and \tilde n_0 \equiv n_0(1+\delta\Omega^2/\tilde\Gamma_\varphi^2) .

As one can see from equation (23) the driving increases the photon number n = |α|2. Once it reaches \tilde n_0 the qubit's negative contribution to the oscillator's effective friction coefficient starts to diminish and, finally, causes the saturation of n. The saturation number is easiest to understand in the framework of the Jaynes–Cummings spectrum, i.e. the spectrum of a coupled system consisting of a two-level system and an oscillator at resonance with each other. The coupling lifts the degeneracy between the states |↑,nrangle and |↓,n + 1rangle and creates an energy splitting of order g_1 \sqrt{n} . Once the occupation number n reaches the saturation number n0 the energy splitting g_1 \sqrt{n} becomes larger than the rate Γ1 which, in the case of population inversion, serves also as the pumping rate. At this stage, the pumping becomes ineffective and the growth of n slows down and for still larger photon numbers stops.

The Langevin force ξ = ξosc + ξqb arises due to the thermal noise of the oscillator's dissipative environment, ξosc, as well as the noise of the driven qubit, ξqb. By the fluctuation dissipation theorem, the former satisfies langleξosc(tosc*(t ' )rangle = κNthδ(tt ' ) and langleξosc(tosc(t ' )rangle = 0. The noise originating from the qubit can be estimated as \langle \xi_{\rm qb}(t)\xi_{\rm qb}^{\ast}(t')\rangle = (g_1^2/\tilde\Gamma_\varphi)\delta(t-t') and langleξqb(tqb(t ' )rangle = 0. Provided the oscillator's thermal noise is strong, i.e. if \kappa N_{\rm th}\gg g_1^2/\tilde\Gamma_\varphi , the qubit's noise can be neglected compared to the former.

2.4.2. Two-photon interaction The two-photon effect dominates near the resonance ΩR≈2ωT. In RWA, the Hamiltonian reduces to

Equation (24)

The corresponding Langevin equation for the resonator variable reads

Equation (25)

i.e. it is of the same form as equation (23) except that C≡4g22|α|2 and s_z^{\rm st}=-D_0/(1+(\vert \alpha^2\vert/\tilde n_0)^2) . The photon saturation number is now given by n_0=(\tilde\Gamma_{\varphi} \tilde\Gamma_1/4g_2^2)^{1/2} and \tilde n_0 \equiv n_0(1+\delta\Omega^2/\tilde\Gamma_\varphi^2)^ {1/2} . The detuning of the Rabi frequency for two-photon interaction is given by δΩ≡ΩR–2ωT + g3|α|2. Again ξ(t) is mostly due to the thermal noise, while noise arising from the qubit can be neglected if \kappa N_{\rm th}\gg g_2^2 \bar n/\tilde\Gamma_\varphi .

3. Results

3.1. Results obtained from the Langevin equation

If one neglects the frequency shifts of the oscillator, i.e. for g3 = 0, the Fokker–Planck equations corresponding to the Langevin equations (23) and (25) have exact analytic solutions [45]. Also for g3≠0 the equations (23) and (25) written as \dot\alpha=- f(n) \alpha/2 +\xi(t) can be transformed into equations for the average number of photons \langle\vert\alpha\vert^2\rangle=\bar n in the form \dot{\bar n}=-\langle n {\rm Re}[f(n)]\rangle +\kappa N_{\rm th} . In the steady state, for \bar n\gg 1 they can be approximated by \bar n {\rm Re}[f(\bar n)]=\kappa N_{\rm th} . The results of this analysis are shown in figure 3. To demonstrate both the one-photon and the two-photon effects, we assumed that the qubit is biased sightly off the symmetry point, epsilon = 0.01Δ. The two-photon resonance (the outer one) persists for epsilon = 0, whereas the one-photon resonance (the inner one) vanishes there. We observe that the solution shows bistability bifurcations [46] (see below). As a result, we see in figure 3 sharp drops of \bar n for both resonances as only the lowest stable value is plotted.

Figure 3

Figure 3. Average number of photons in the resonator as a function of the driving detuning δω and amplitude ΩR0. Peaks at δω > 0 correspond to lasing, while dips at δω < 0 correspond to cooling. The inner curve corresponds to the one-photon resonance which exists only away from the symmetry point. Here, we assumed epsilon = 0.01Δ. The outer curve describes the two-photon resonance, which persists at epsilon = 0. In domains of bistability the lowest value of \bar n is plotted (leading to the sharp drops in both curves). We chose the following parameters for the qubit: Δ/2π = 1 GHz, epsilon = 0.01Δ, Γ0/2π = 125 kHz, the resonator: ωT/2π = 6 MHz, κ/2π = 0.34 kHz, and the coupling: g/2π = 3.3 MHz. The bath temperature is T = 10 mK.

In the lasing regime, we can estimate the asymptotic solutions analytically. In the one-photon case, assuming \bar n \gg \tilde n_0 , we obtain from equation (23)

Equation (26)

This result holds independent of whether the second contribution due to the qubit is larger or smaller than the thermal number Nth as long as \bar n \gg \tilde n_0 . In the two-photon case, assuming \bar n \gg \tilde n_0 , we obtain from equation (25)

Equation (27)

3.2. Solution of the master equation

We also solved the full master equation (19) numerically, which provides access not only to the average number of photons in the oscillator, \bar n , but also to the whole distribution function P(n). Assuming a low thermal number, Nth = 5 and a relatively high relaxation constant of the oscillator κ/2π = 1.7 kHz, we reach convergence with a limited number of photon basis states (n≤100). In figure 4, the solutions of the Langevin equations (23) and (25) and those of the master equation (19) are compared. By construction, the solution of the master equation (19) provides the uniquely defined stationary distribution function for the occupation number P(n). Thus, the average occupation number defined as \bar n =\sum_n n P(n) is also uniquely defined and is plotted in figure 4. In contrast, the Langevin equations (23) or (25) yield in a certain interval of parameters two stable solutions for \bar n=|\alpha|^2 , as shown in figure 4. We observe that in regimes of single stability the solutions of the master equation and of the Langevin equations agree very well. In the bistability regime, the master equation produces approximately the average between the two stable solutions of the Langevin equation. This indicates that in the bistability regime, the system switches between the two stable states. Further indications of this `telegraph' behavior are obtained from the analysis of the Fano factor.

Figure 4

Figure 4. Average number of photons \bar n versus the detuning. The blue dashed and the green dotted curves are obtained from the Langevin equations (23) and (25). They show the bistability with the blue dashed curve denoting stable solutions, whereas the green dotted curve denotes the unstable solution. The red solid curve is obtained from a numerical solution of the master equation (19). The driving amplitude is taken as ΩR0/2π = 5 MHz. The parameters of the qubit: Δ/2π = 1 GHz, epsilon = 0.01Δ, Γ0/2π = 125 kHz, the resonator: ωT/2π = 6 MHz, κ/2π = 1.7 kHz, Nth = 5, and the coupling: g/2π = 3.3 MHz.

In figure 5, the Fano factor F = (langlen2ranglelanglenrangle2)/langlenrangle of the photon number distribution is presented. We observe two phenomena. First, in the regime of lasing without bistability, the Fano factor is reduced as compared to that of the thermal state. Indeed, the Fano factor in the ideal lasing state should approach 1, down from the thermal value Nth + 1. In contrast, in the bistable regime the Fano factor increases. We interpret this result as another indication of the switching between the two stable solutions. In the cooling regime, the Fano factor, as expected, follows the effective temperature of the oscillator, i.e. is reduced.

Figure 5

Figure 5. The Fano factor (dashed blue), and the average photon number \bar n (solid red). The parameters are as in figure 4.

In figure 6, the distribution function, P(n), for the number of photons in the oscillator is plotted both for the cooling and lasing regimes. For comparison, also the thermal (Bose–Einstein) distribution is plotted. We observe that in the lasing regime, the distribution function combines the Poisson-like part and the thermal-like one. This is yet another indication of the bistability. On the other hand, in the cooling regime the distribution function is thermal-like with the reduced effective temperature.

Figure 6

Figure 6.  The distribution function, P(n), obtained by numerically solving the master equation (19). Blue solid curve: cooling regime of the one-photon resonance with ΩR0 = 2π×5 MHz and δω = –2π×3.2 MHz. Red dashed curve: lasing regime of the two-photon resonance with ΩR0 = 2π×5 MHz and δω = 2π×11.7 MHz. We observe a peak in the P(n) distribution between n = 20 and 30 as a result of the lasing behavior. Black dotted curve: thermal distribution with Nth = 5. The parameters are as in figure 4.

The lasing and cooling effects described here rely crucially on the transition rates, as described by the Liouville equations. In order to demonstrate this dependence, we plot in figure 7 the average photon number versus the qubit's relaxation rate at the one-photon resonance. We note a non-monotonic dependence. This behavior is explained by the dependence of the saturation number n0 on Γ0 indicated in figure 7. While n0 grows quadratically with Γ0 the average occupation number \bar{n} grows only linearly, cf equations (26) and (27). This regime holds as long as \bar{n} >  n_0 . Indeed, in this regime the pumping rate is limited by Γ0, leading to a roughly linear growth of the photon number with increasing Γ0, consistent with equations (26) and (27). Once the saturation threshold is reached, \bar n \sim n_0 , the effective coupling \sim \! g_1 \sqrt{\bar n} becomes comparable to Γ0 and the photon number becomes insensitive to small variations of Γ0. Since the saturation number n0 continues to grow, the regime \bar n  <  n_0 is reached. In this case, a further increase of Γ0 predominantly increases the dephasing rate \tilde\Gamma_{\varphi} . As can be seen from equation (23) this reduces the effect of the qubit on the oscillator and the photon number decreases towards Nth. In figure 7, we plot both the results of a numerical solution of the master equation and of the Langevin equation. We find a good agreement between the two.

Figure 7

Figure 7. Average number of photons in the resonator as a function of the qubit's relaxation rate, Γ0 at the one-photon resonance, ΩR = ωT for g3 = 0 and Nth = 5. The dark blue line shows the numerical solution of the master equation, the light blue solid line represents the solution of the Langevin equation, equation (23). The green and red dashed curves represent, respectively, the saturation number n0 and the thermal photon number Nth. The parameters are as in figure 4 (except for Γ0).

4. Discussion

We summarize our main conclusions. Our results for the number of photons \bar n are plotted in figure 3 as a function of the detuning δω of the driving frequency and driving amplitude ΩR0. It exhibits sharp structures along two curves corresponding to the one- and two-photon resonance conditions, \Omega_{\rm R}=\omega_{\rm T}-g_3\bar n and \Omega_{\rm R}=2\omega_{\rm T}-g_3\bar n . Blue detuning, δω > 0, induces a strong population inversion of the qubit levels, which in resonance leads to one-qubit lasing. In experiments the effect can be measured as a strong increase of the number of photons in the resonator above the thermal values. Red detuning produces a one-qubit cooler with resulting photon numbers substantially below the thermal value.

The bistability of the solution of the Langevin description is illustrated in figure 4. In the range of bistability, we expect a telegraph-like noise corresponding to the random switches between the two solutions.

Potentially useful applications of the considered scheme are the lasing behavior and the creation of a highly non-thermal population of the oscillator as well as the cooling. Within the accuracy of our approach, we estimate that a population of order \bar n=1 can be reached for optimal detuning.

So far we have described an LC-oscillator coupled to a flux qubit. But our analysis equally applies for a nanomechanical resonator coupled capacitively to a Josephson charge qubit [6] (see figure 1(b)). In this case, σz stands for the charge of the qubit and both the coupling to the oscillator as well as the driving are capacitive, i.e. involve σz. To produce the capacitive coupling between the qubit and the oscillator, the latter could be metal-coated and charged by the voltage source Vx. The dc component of the gate voltage Vg puts the system near the charge degeneracy point, where the dephasing due to the 1/f charge noise is minimal. Rabi driving is induced by an ac component of Vg. Realistic experimental parameters are expected to be very similar to the ones used in the examples discussed above, except that a much higher quality factor of the resonator (~105) and a much higher number of quanta in the oscillator can be reached. This number will easily exceed the thermal one, thus a proper lasing state with Poisson statistics, appropriately named SASER [29], is produced. One should then observe the usual line narrowing [44] with line width given by \kappa \! N_{\rm th}/(4\bar n) \sim \kappa^2 N_{\rm th}/\tilde\Gamma_1 . Experimental observation of this line-width narrowing would constitute a confirmation of the lasing/sasing.

In experiments with the same setup as shown in figure 1(a)—but in a different parameter regime when the relaxation rate of the qubit is close to the oscillator's frequency—the mechanisms of Sisyphus cooling and amplification have recently been demonstrated [7]. In these experiments, the LC tank circuit is driven near-resonantly by a low-frequency ac current, and its response, which is influenced by the high-frequency driven qubit, is detected. For red-detuned high-frequency driving of the qubit the low-frequency LC-circuit carries out work in its forward and backward oscillation cycle, always increasing the energy of the qubit (similar to Sisyphus always pushing up a rock). This produces additional damping and a reduction of the effective quality factor, which can be associated with cooling of the oscillator. For blue-detuned qubit driving, the same mechanism leads to Sisyphus amplification (`lucky Sisyphus' rolling the rock down) and a precursor of lasing of the resonator. It is accompanied by an enhancement of the effective quality factor. These effects were confirmed in the second series of experiments where the power spectrum of the oscillator, i.e. the number of photons and the line-width, were measured directly. A quantitative analysis [7] in the frame of the theory outlined in this paper confirms this picture and allows parameter regimes to be identified where these effects are optimized.

Acknowledgments

We thank E Il'ichev, O Astafiev, A Blais, M Devoret, D Esteve, M D LaHaye, M Marthaler, Y Nakamura, F Nori, E Solano, K C Schwab and F K Wilhelm for fruitful discussions. The work is part of the EU IST Project EuroSQIP.

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