# Controlling the dynamic range of a Josephson parametric amplifier

- Christopher Eichler
^{1}Email author and - Andreas Wallraff
^{1}

**1**:2

**DOI: **10.1140/epjqt2

© Eichler and Wallraff; licensee Springer on behalf of EPJ. 2014

**Received: **30 May 2013

**Accepted: **25 September 2013

**Published: **29 January 2014

## Abstract

One of the central challenges in the development of parametric amplifiers is the control of the dynamic range relative to its gain and bandwidth, which typically limits quantum limited amplification to signals which contain only a few photons per inverse bandwidth. Here, we discuss the control of the dynamic range of Josephson parametric amplifiers by using Josephson junction arrays. We discuss gain, bandwidth, noise, and dynamic range properties of both a transmission line and a lumped element based parametric amplifier. Based on these investigations we derive useful design criteria, which may find broad application in the development of practical parametric amplifiers.

## 1 Introduction

Due to the rapidly evolving field of quantum optics and information processing with superconducting circuits the interest in low-noise amplifiers has dramatically increased in the past five years and has lead to a body of dedicated research on Josephson junction based amplifiers [1–15]. The most successful quantum limited detectors which have so far been realized in the microwave frequency range are based on the principle of parametric amplification [16–19]. Josephson parametric amplifiers (JPAs) have not only been used to generate squeezed radiation [6, 13, 20–22], but moreover enabled the realization of quantum feedback and post-selection based experiments [23–26], the efficient displacement measurement of nanomechanical oscillators [27] and the exploration of higher order photon field correlations [28, 29].

While JPAs have been demonstrated to operate close to the quantum limit, their performance is to date mostly limited by their relatively small dynamic range, *i.e.* the saturation of the gain for large input signals. Here, we discuss the control of the dynamic range by making use of Josephson junctions arrays in the parametric amplifier circuit, which we have already employed in recent experiments [29, 30]. After reviewing the principles of parametric amplification we discuss bandwidth and noise constraints in dependence on the circuit design, based on which we derive simple strategies for optimized circuit design.

## 2 Principles of parametric amplification

### 2.1 Parametric processes at microwave frequencies

In quantum optics the word *parametric* is used for processes in which a nonlinear refractive medium is employed for mixing different frequency components of light. Such processes are parametric in the sense that a coherent pump field, applied to a nonlinear medium, modulates its refractive index, which appears as a *parameter* in a semi-classical treatement. This time-varying parameter is affecting modes with frequencies detuned from the frequency of the pump field and can stimulate their population with photons. The energy for creating these photons is provided by the pump field.

The refractive index in optics is equivalent to the impedance of electrical circuits. In order to realize parametric processes at microwave frequencies we therefore modulate an effective impedance. This is achieved by varying the parameters of either a capacitive or an inductive element in time. Although there have been early proposals for fast time-varying capacitances [31], it now is considered to be more convenient to make use of dissipationless Josephson junctions for this purpose. In a regime in which the current *I* flowing through a Josephson junction is much smaller than its critical current ${I}_{C}\equiv 2e{E}_{J}/\u0127$ its associated inductance is approximately $L\approx {L}_{J}(1+\frac{1}{6}{(I(t)/{I}_{C})}^{2})$. Applying an *AC* current through the junction using appropriate microwave drive fields therefore leads to the desired time-varying impedance. Because of the proportionality of the inductance *L* to the square of the current ${I}^{2}(t)$, such a drive results in a four-wave mixing process [32].

The effective impedance can alternatively be modulated by varying the magnetic flux threading a superconducting quantum interference device (SQUID) loop [5] such that the effective inductance is approximately modulated proportionally to the AC current $I(t)$ flowing in the loop, $L\approx {L}_{J}(1+I(t)/{I}_{0})$. The quantity ${I}_{0}$ in this expression depends on the DC flux bias point of the SQUID loop. Since the relation between current and inductance is in this case linear, the magnetic flux drive results in a three-wave mixing process [33].

In order to enhance parametric amplification in a well-controlled frequency band while suppressing it for frequencies out of this band, the modulated Josephson inductance is frequently integrated into a microwave frequency resonator. This is the simplest way to control the band in which parametric amplification occurs. A number of variations of this basic idea are now explored. The circuit design has recently been modified to achieve a spatial separation of signal and idler modes [9, 21, 34–36] and to build traveling wave amplifiers, in which a field is amplified while propagating in forward direction coaxially with a pump field [37, 38]. Various drive mechanisms ranging from single and double pumps [8] to magnetic flux drives [5, 39, 40] have been explored. Being aware of this variety of possible approaches, we focus here on a single mode (degenerate) parametric amplifier driven with one pump tone close to its resonance frequency.

### 2.2 Circuit QED implementation of a parametric amplifier

where *A* labels the annihilation operator of the intra-resonator field. Expressions for the resonance frequency ${\tilde{\omega}}_{0}/2\pi $ and the effective Kerr nonlinearity *K* are derived in Section 4 based on the full circuit model. In the following section we analytically study the dynamics of this system using the input-output formalism. Before presenting the mathematical derivations, we qualitatively describe different dynamical regimes of this nonlinear oscillator and explain the mechanism which leads to amplification.

If we assume for the moment that the JPA has no internal losses, all the incident power is reflected from the resonator and the classical response (*i.e.* reflection coefficient) is completely specified by the phase *φ* of the reflected field. In contrast to a linear system, where *φ* only depends on the frequency $\omega /2\pi $, it also depends on the power of the probe field in the case of a nonlinear oscillator. In Figure 1(b), the theoretically expected value of *φ* is plotted as a function of the probe amplitude for two characteristic drive frequencies. While the phase is constant for low drive powers (quasi-linear response), the phase changes significantly for increased drive power. Depending on the probe frequency we either find a bistable regime where two stable solutions exist [41, 42] or a regime where the phase has a unique solution (red and blue data sets in Figure 1(b)). In both cases the phase significantly depends on the input power. The bistable response can for example be used to realize a bifurcation amplifier [43, 44] and for nonlinear dispersive readout [45], which has been intensely studied in the context of circuit QED.

Since we are particularly interested in *linear* amplification the following discussion is focused on the regime, in which the response has a unique solution (blue data set). The mechanism of amplification can be understood qualitatively in the following way. If we imagine that the device is constantly driven at a frequency and power at which the reflected phase *φ* depends sensitively on power (see gray circle in Figure 1(b)), the system will strongly react to small perturbations. Such perturbations, which could be caused by an additional small signal field for example, are therefore translated into a large change of the output field.

We illustrate this process leading to amplification by plotting the resonator response for input fields ${\alpha}_{\mathrm{in}}$ with slightly varying amplitude and phase. In Figure 1(c) we indicate the input fields by a blue circle around the mean value (arrow). The small differences in amplitude of the input field translate into large changes in *φ* of the output field ${\alpha}_{\mathrm{out}}$ (red ellipse). If we interpret the arrow in Figure 1(c) as a constant pump field and its difference to the points on the blue circle as an additional signal, the signal is either amplified or deamplified depending on its phase relative to the pump.

The mechanism of amplification can thus be understood intuitively by considering the nonlinear response to a monochromatic drive field. In order to characterize the exact behavior of input fields with finite bandwidth we analyze the response in more detail below.

## 3 Input-output relations for the parametric amplifier

### 3.1 Classical nonlinear response

*κ*to a transmission line, through which the pump and signal fields propagate. Based on this model and the Hamiltonian in Eq. (1) we obtain the following equation of motion for the intra-resonator field

*κ*we account for potential radiation loss mechanisms by introducing the coupling to modes ${b}_{\mathrm{in}}(t)$ with loss rate

*γ*, compare Figure 2(a). A boundary condition equivalent to

*α*, ${\alpha}_{\mathrm{in}}$, ${\alpha}_{\mathrm{out}}$ represent the classical parts of the field which are associated with the pump, while

*a*, ${a}_{\mathrm{in}}$, ${a}_{\mathrm{out}}$ account for the quantum signal fields. Since all

*α*’s are complex numbers the modes

*a*satisfy the same bosonic commutation relations as modes

*A*do. By multiplying the field modes defined in Eq. (4) with the additional exponential factor ${e}^{-i{\omega}_{p}t}$, one works in a frame rotating at the pump frequency ${\omega}_{p}$. The strategy is to first solve the classical response for the pump field

*α*exactly and then linearize the equation of motion for the weak quantum field

*a*in the presence of the pump. Finally, we derive a scattering relation between input modes ${a}_{\mathrm{in}}$ and reflected modes ${a}_{\mathrm{out}}$.

*δ* is the detuning between pump and resonator frequency in units of the total resonator linewidth, ${\tilde{\alpha}}_{\mathrm{in}}$ is the dimensionless drive amplitude, and *ξ* is the product of drive power and nonlinearity, also expressed in dimensionless units. Finally, *n* is the mean number of pump photons in the resonator relative to the incident pump power. As an important consequence, we notice from Eq. (8) that only the product of drive power and nonlinearity determines the dynamics but not each quantity itself. Therefore, a small nonlinearity can at least in principle be compensated by increasing the drive power. Properties such as the gain-bandwidth product are therefore independent of the strength of the nonlinearity as long as the pump power is much larger than the power of amplified fluctuations. Furthermore, the solutions of Eq. (7) for negative *ξ* values are identical to those for positive *ξ* up to a sign change in *δ*. Since *ξ* is negative for the Josephson parametric amplifier, we focus on this particular case.

Equation (7) is a cubic equation in *n* and can therefore be solved analytically. We do not present the lengthy solutions here explicitly, but assume in the following that we have an explicit analytical expression for *n* in terms of *δ* and *ξ*. In Figure 2(b) we plot *n* for various parameters *ξ* as a function of *δ*. At the critical value ${\xi}_{\mathrm{crit}}=-1/\sqrt{27}$ the derivative $\partial n/\partial \delta $ diverges and thus the response of the parametric amplifier becomes extremely sensitive to small changes. For even stronger effective drive powers $\xi /{\xi}_{\mathrm{crit}}>1$ the cubic Eq. (7) has three real solutions. The solutions for the high and low photon numbers are stable, while the intermediate one is unstable. The system bifurcates in this regime as mentioned earlier. The critical detuning below which the system becomes bistable is ${\delta}_{\mathrm{crit}}=-\sqrt{3}/2$. The critical point $({\xi}_{\mathrm{crit}},{\delta}_{\mathrm{crit}})$ is the one at which both $\partial \delta /\partial n$ and ${\partial}^{2}\delta /{\partial}^{2}n$ vanish. In scale invariant units the maximal value of *n* is 4, which is reached at the detuning $\delta =4\xi $.

In Figure 2(c) we plot the absolute value of the reflection coefficient at $\xi ={\xi}_{\mathrm{crit}}$ for various loss rates *γ*. For vanishing losses $\gamma =0$ all the incident drive power is reflected from the device and $|\mathrm{\Gamma}|=1$. Note that also in this case the resonance is clearly visible in the phase of the reflected signal (not shown here). When the loss rate *γ* becomes similar to the external coupling rate *κ* part of the radiation is dissipated into the loss modes. In the case of critical coupling $\gamma =\kappa $ all the coherent power is transmitted into the loss modes at resonance. This is equivalent to the case of a symmetrically coupled $\lambda /2$ resonator, for which the transmission coefficient is one at resonance [48].

### 3.2 Linearized response for weak (quantum) signal fields

*a*in the presence of the pump field. In order to preserve the validity of this approximation even for larger input signals, the amplitude

*α*of the pump field needs to be increased. Experimentally, this can be achieved by reducing the strength of the nonlinearity

*K*as discussed in Section 3.3 in more detail. Substituting Eq. (4) into Eq. (2) and keeping only terms which are linear in

*a*one finds

*ϕ*is the phase of the intra-resonator pump field, defined by $\alpha =|\alpha |{e}^{i\varphi}$. The fact that Eq. (12) couples modes ${a}_{\mathrm{\Delta}}$ and ${a}_{-\mathrm{\Delta}}^{\u2020}$ can be interpreted as a wave mixing process. In order to express ${a}_{\mathrm{\Delta}}$ in terms of the input fields ${c}_{\mathrm{in},\mathrm{\Delta}}$, Eq. (12) is rewritten as a matrix equation

and Eq. (15b) is identical to a two-mode squeezing transformation [19, 49] with gain ${G}_{\mathrm{\Delta}}$. The two-mode squeezing transformation describes a linear amplifier in its minimal form (compare Ref. [50]), of which we discuss characteristic properties in the following section.

### 3.3 Gain, bandwidth, noise and dynamic range

For simplicity we consider the case of no losses $\gamma =0$, for which the parametric amplifier response is described by Eq. (15b). An incoming signal at detuning Δ is thus amplified by the power gain ${G}_{\mathrm{\Delta}}={|{g}_{S,\mathrm{\Delta}}|}^{2}$ and mixed with the frequency components at the opposite detuning from the pump. Characteristic properties of the parametric amplifier, such as the maximal gain and the bandwidth, are thus encoded in the quantity ${g}_{S,\mathrm{\Delta}}$ as a function of pump-resonator detuning *δ*, effective drive strength *ξ* and detuning between signal and pump Δ.

*δ*and

*ξ*. We find that the maximal gain increases with increasing drive strength

*ξ*while the optimal value for

*δ*at which this gain is reached, shifts approximately linearly with increasing

*ξ*. The optimal values for

*δ*are indicated as a dashed white line in Figure 3(a). Mathematically, the gain diverges when

*ξ*approaches the critical value ${\xi}_{\mathrm{crit}}$. In practice, the gain is limited to finite values due to the breakdown of the stiff pump approximation (see discussion below).

By changing the pump parameters *ξ* and *δ* we can adjust the gain ${G}_{0}$ to a desirable value, which is typically about 20 dB. Note that the gain can take values smaller than one, in the presence of finite internal losses $\gamma >0$. Once the pump parameters are fixed we characterize the bandwidth of the amplifier by analyzing the gain as a function of the signal detuning Δ. In Figure 3(b) we plot the gain as a function of Δ for the indicated values of $\xi /{\xi}_{\mathrm{crit}}$ and the corresponding optimal pump detunings *δ* (compare dashed white line in (a)). The gain curves are well approximated by Lorentzian lines as indicated by the dashed black lines in Figure 3(b). When the gain is increased, the band of amplification becomes narrower. This is quantitatively expressed by the gain-bandwidth relation $\sqrt{{G}_{0}}B\approx 1$, where *B* is the detuning Δ for which the gain reaches half of its maximal value. This gain-bandwidth relation follows from the Lorentzian approximation of the gain curves shown as black dashed lines in Figure 3(b)) and holds for gain values above a few dB. Remember that Δ is defined in units of the resonator linewidth $\kappa +\gamma $, which means that the amplifier bandwidth equals approximately the resonator linewidth divided by the square root of the gain.

When operating the JPA, we also have to understand its behavior in terms of added noise. In the ideal case with zero loss rate ($\gamma =0$), the input-output relation of the parametric amplifier in Eq. (15b) has the minimal form of a scattering mode amplifier [19]. The amplification process reaches the vacuum limit as long as the input modes are cooled into the vacuum. In practice, however, the device may have finite loss *γ* which increases the effectively added noise by a factor of $(\kappa +\gamma )/\kappa $. This is due to the additional amplified noise, which originates from the modes ${b}_{\mathrm{in},\mathrm{\Delta}}$ and contributes to the output field ${a}_{\mathrm{out},\mathrm{\Delta}}$ (compare Eq. (15a)). Another potential source of noise is related to the stability of the resonance frequency of the parametric amplifier. Magnetic flux noise in the SQUID loop may lead to a fluctuating resonance frequency and thus a fluctuating effective gain.

*i.e.*the value ${n}_{1\phantom{\rule{0.2em}{0ex}}\mathrm{dB}}$ of input photons ${n}_{\mathrm{th}}$ at which the JPA gain ${G}_{0}$ decreases by 1 dB compared to the stiff pump approximated gain value. As shown in Figure 4(b), the 1 dB compression point increases proportionally to $\kappa /|K|$ in the limit of ${n}_{1\mathrm{dB}}\gg 1$. The presence of constant vacuum fluctuations leads to a gain compression by more than 1 dB even for ${n}_{\mathrm{th}}=0$ when $\kappa /|K|$ becomes smaller. We can qualitatively explain this behavior by comparing the pump power ${P}_{p}=\u0127{\omega}_{p}{|{\alpha}_{\mathrm{in}}|}^{2}$ with the power of amplified signal and vacuum fields

## 4 Effective system parameters from distributed circuit model

In the previous section we have analyzed the model of a nonlinear resonator with resonance frequency ${\tilde{\omega}}_{0}$, Kerr nonlinearity *K* and decay rate *κ*. Here, we explicitly derive this effective Hamiltonian from the full circuit model of a $\lambda /4$ - transmission line resonator, which is terminated by a SQUID loop at the short-circuited end and coupled capacitively to a transmission line, see Figure 1(a). These calculations allow us to determine ${\tilde{\omega}}_{0}$, *K*, *κ* from the distributed circuit parameters and give insight into potential limitations of the effective model. We also compare the obtained parameter relations with those of a lumped element parametric amplifier.

### 4.1 Resonator mode structure in the linear regime

with the reduced flux quantum ${\phi}_{0}=\u0127/2e$. Since we work in a limit in which the plasma frequency of the SQUID is much larger than the resonance frequencies of interest, we neglect the self-capacitance of the SQUID. Note that Ref. [52] provides a detailed study of the effect of the self-capacitance in various parameter regimes. We furthermore describe the SQUID as a single junction with tunable effective Josephson energy ${E}_{J}$.

### 4.2 Kerr nonlinear terms and effective Hamiltonian

*i.e.*the current flowing through the Josephson junction is small compared to its critical current. We can therefore expand the SQUID cosine potential and take into account only the first non-quadratic correction

As expected the linear part of the Lagrangian is diagonal in the normal mode basis. It describes a set of uncoupled *LC* oscillators for which the effective resonance frequencies coincide with the product of phase velocity and wave vector ${\omega}_{j}={k}_{j}v=1/\sqrt{{L}_{j}{C}_{j}}$.

*i.e.*removing all terms with an unequal number of creation and annihilation operators), and neglecting the small photon number independent frequency shifts due to the nonlinear terms (

*i.e.*Lamb shifts) we arrive at

The quantity $K={K}_{00}$ is the Kerr nonlinearity of the fundamental mode, which is used for the parametric amplification process. The terms proportional to ${K}_{ij}$ with unequal $i\ne j$ are cross Kerr interaction terms which couple different modes to each other. Such an interaction can for example be used for counting the number of photons in one mode by probing another one with a coherent field [54–61], similarly to a dispersive qubit measurement. Note that the values resulting from Eq. (37) are divided by the square of the number of SQUIDs, if an array is used instead of a single SQUID, as discussed in the following section.

### 4.3 Decay rate and resonance frequency correction for low *Q* resonators

*κ*, typical devices are designed to have a low external quality factor, which is achieved by increasing the coupling capacitance ${C}_{\kappa}$ between transmission line and resonator (Figure 1). The coupling of an oscillator to the environment shifts its resonance frequency ${\omega}_{j}\to {\tilde{\omega}}_{j}$ [48], which can be significant if the coupling rate is large. When designing parametric amplifier devices, it is therefore necessary to take these shifts into account. Based on the effective inductance and capacitances calculated in Eq. (32) we find

for resonance frequency and decay rate of the *j* th mode of the parametric amplifier device. The external quality factor is given by ${Q}_{j}\equiv {\tilde{\omega}}_{j}/{\kappa}_{j}$.

### 4.4 Lumped element JPA

As already mentioned in the introduction, a JPA can also be realized as a lumped element resonator by shunting a SQUID with a large capacitance ${C}_{J}$ [10, 11]. In this case the resonator is described by the transmon Hamiltonian [62], which in the deep transmon limit ${E}_{J}\gg {E}_{C}\equiv {e}^{2}/2{C}_{J}$ takes the form of Eq. (1) with anharmonicity $K\approx {E}_{C}/\u0127$ and resonance frequency ${\tilde{\omega}}_{0}\approx 1/\sqrt{{L}_{J}{C}_{J}}$. Also for this type of resonators the coupling rate *κ* to the transmission line can be designed independently of ${E}_{J}$ and ${E}_{C}$ by designing an appropriate capacitive network. Similarly as for the transmission line JPA, the description in terms of the effective Hamiltonian Eq. (1) is based on the assumption that for relevant resonator fields the phase drop across the Josephson junctions is small (compare Eq. (30)). In the following section we study the validity of this approximation when the resonator is driven close to the bifurcation point where we expect parametric amplification to occur and analyze its implications for realizing a parametric amplifier with large bandwidth and dynamic range.

## 5 Bandwidth and dynamic range constraints

### 5.1 Validity of the quartic approximation

In Section 3.3 we have shown that the dynamic range of the JPA scales with $\kappa /|K|$. Also the bandwidth becomes larger with increasing *κ*, which indicates that a large *κ* is desirable for JPAs. However, there are limitations on the maximal possible value for *κ* as discussed in the following.

For deriving the Hamiltonian in Eq. (1), or more generally Eq. (36), we have expanded the SQUID cosine potential to quartic order in the dimensionless flux variable ${\mathrm{\Phi}}_{n}/{\phi}_{0}$, where ${\mathrm{\Phi}}_{n}\equiv \mathrm{\Phi}(x=d)$ is the phase drop across the SQUID. To guarantee that this approximation holds when we operate the device in the parametric amplification regime, we have to make sure that ${\mathrm{\Phi}}_{n}/{\phi}_{0}$ is small even when it is driven close to the bifurcation point. This is equivalent to keeping the current flowing through the SQUID small compared to the critical current.

*α*in mode

*j*leads to a maximal amplitude of ${\mathrm{\Phi}}_{n}={\varphi}_{\mathrm{zpf},j}2\alpha cos({k}_{j}d)$ across the tunnel junctions, based on which we define the critical amplitude as

*α*is much smaller than this maximal amplitude $\alpha <{\alpha}_{\mathrm{max},j}$. In Section 3.1 we have found that the photon number in a resonator mode at the bifurcation point is ${N}_{\mathrm{crit}}=(\kappa +\gamma )/\sqrt{3}K$. The ratio between ${N}_{\mathrm{crit}}$ and the maximal coherent photon number ${N}_{\mathrm{max},j}\equiv {|{\alpha}_{\mathrm{max},j}|}^{2}$ is therefore given by

*κ*needs to be sufficiently small as well. One may also want to increase the dynamic range by reducing the Kerr nonlinearity $|K|$. While this can in principle be achieved by choosing a small ratio ${L}_{J}/ld$ between Josephson and geometric inductance, care has to be taken when using this approach because additional geometric inductance leads to a larger ratio ${N}_{\mathrm{crit}}/{N}_{\mathrm{max}}$ as illustrated in Figure 7.

*K*, can in principle be made smaller without affecting ${N}_{\mathrm{crit}}/{N}_{\mathrm{max}}$. However, in practice a small Josephson inductance has to be compensated by a large lumped element capacitor to retain the desired resonance frequency, which is challenging to realize without introducing additional parasitic geometric inductances. It therefore seems difficult to build a parametric amplifier with large bandwidth and high dynamic range at the same time using a single SQUID only. In the following we show how one can keep ${N}_{\mathrm{crit}}/{N}_{\mathrm{max}}$ constant while decreasing the nonlinearity and thus increasing the dynamic range of the amplifier, by replacing the single SQUID with a serial array of

*M*SQUIDs of

*M*-times larger Josephson energy per SQUID (Figure 8).

### 5.2 Josephson junction arrays

For simplicity we assume that all SQUIDs in the array have the same effective Josephson energy $M{E}_{J}$. Since the spatial extent of the junction is still small compared to typical resonance wavelengths, we can treat the array as a lumped element. To derive the nonlinearity of the oscillator for this situation we investigate how the different terms in the Lagrangian scale with *M*.

which leads to a quadratic decrease in the effective Kerr nonlinearity $K\to K/{M}^{2}$ and thus a quadratic increase in ${N}_{\mathrm{crit}}\propto {M}^{2}$. Furthermore, the maximal photon number also scales as ${N}_{\mathrm{max}}\propto {M}^{2}$ since the critical current of each junction is larger by a factor of *M*. In other words, the ratio ${N}_{\mathrm{crit}}/{N}_{\mathrm{max}}$ only depends on the total Josephson inductance whereas the bifurcation power increases quadratically in *M*. We thus conclude that the dynamic range of a JPA can be increased without affecting the amplifier bandwidth, by using an array of SQUIDs instead of a single SQUID. This conclusion is valid for both the transmission line JPA and the lumped element JPA.

In practice, the Josephson energies in the array are not all equal due to inhomogeneous coupling to the external magnetic flux and scatter in the critical current of Josephson junctions due to unavoidable variations in fabrication. A quantitative analysis of the influence of such variations of Josephson energies on the parametric amplifier characteristics could be an interesting task for future studies. This would help to quantify limitations in the accessible tuning range of the parametric amplifier and a realistic understanding of the breakdown of the low order expansion of the cosine potential. For such an approach the methods used in Ref. [63] could turn out to be useful.

## 6 Conclusion

In summary, we have presented a detailed analysis of Josephson junction based parametric amplifiers, including a discussion of bandwidth, noise and dynamic range. By establishing relations between basic JPA properties and designable circuit parameters we have been able to derive two simple design strategies to achieve optimized JPA performance. On the one hand the contribution of the Josephson inductance to the total effective inductance of the resonant circuit has to be chosen sufficiently large. On the other hand the use of SQUID arrays instead of single SQUIDs provides the possibility to enhance the strength of the pump field close at the bifuraction point and with it the dynamic range of the JPA.

## Declarations

### Acknowledgements

The authors would like to acknowledge helpful discussions with Alexandre Blais, Vitaly Shumeiko and Sebastian Schmidt. This work was supported by the European Research Council (ERC) through a Starting Grant and by ETHZ.

## Authors’ Affiliations

## References

- Yurke B, Buks E:
*J Lightwave Technol*. 2006, 24: 5054.View ArticleADSGoogle Scholar - Castellanos-Beltran MA, Lehnert KW:
*Appl Phys Lett*. 2007., 91: Article ID 083509 Article ID 083509Google Scholar - Tholén E, Ergül A, Doherty E, Weber F, Grégis F, Haviland D:
*Appl Phys Lett*. 2007., 90: Article ID 253509 Article ID 253509Google Scholar - Kinion D, Clarke J:
*Appl Phys Lett*. 2008., 92: Article ID 172503 Article ID 172503Google Scholar - Yamamoto T, Inomata K, Watanabe M, Matsuba K, Miyazaki T, Oliver WD, Nakamura Y, Tsai JS:
*Appl Phys Lett*. 2008., 93: Article ID 042510 Article ID 042510Google Scholar - Castellanos-Beltran MA, Irwin KD, Hilton GC, Vale LR, Lehnert KW:
*Nat Phys*. 2008, 4: 929. 10.1038/nphys1090View ArticleGoogle Scholar - Palacios-Laloy A, Nguyen F, Mallet F, Bertet P, Vion D, Esteve D:
*J Low Temp Phys*. 2008, 151: 1034. 10.1007/s10909-008-9774-xView ArticleADSGoogle Scholar - Kamal A, Marblestone A, Devoret M:
*Phys Rev B*. 2009., 79: Article ID 184301 Article ID 184301Google Scholar - Bergeal N, Schackert F, Metcalfe M, Vijay R, Manucharyan VE, Frunzio L, Prober DE, Schoelkopf RJ, Girvin SM, Devoret MH:
*Nature*. 2010, 465: 64. 10.1038/nature09035View ArticleADSGoogle Scholar - Hatridge M, Vijay R, Slichter DH, Clarke J, Siddiqi I:
*Phys Rev B*. 2011., 83: Article ID 134501 Article ID 134501Google Scholar - Vijay R, Slichter DH, Siddiqi I:
*Phys Rev Lett*. 2011., 106: Article ID 110502 Article ID 110502Google Scholar - Gao J, Vale LR, Mates JAB, Schmidt DR, Hilton GC, Irwin KD, Mallet F, Castellanos-Beltran MA, Lehnert KW, Zmuidzinas J, Leduc HG:
*Appl Phys Lett*. 2011., 98: Article ID 232508 Article ID 232508Google Scholar - Eichler C, Bozyigit D, Lang C, Baur M, Steffen L, Fink JM, Filipp S, Wallraff A:
*Phys Rev Lett*. 2011., 107: Article ID 113601 Article ID 113601Google Scholar - Abdo B, Kamal A, Devoret M:
*Phys Rev B*. 2013., 87: Article ID 014508 Article ID 014508Google Scholar - Kamal A, Clarke J, Devoret MH:
*Phys Rev B*. 2012., 86: Article ID 144510 Article ID 144510Google Scholar - Louisell WH, Yariv A, Siegman AE:
*Phys Rev*. 1961, 124: 1646. 10.1103/PhysRev.124.1646MATHView ArticleADSGoogle Scholar - Gordon JP, Louisell WH, Walker LR:
*Phys Rev*. 1963, 129: 481. 10.1103/PhysRev.129.481MATHMathSciNetView ArticleADSGoogle Scholar - Mollow BR, Glauber RJ:
*Phys Rev*. 1967, 160: 1076. 10.1103/PhysRev.160.1076View ArticleADSGoogle Scholar - Clerk AA, Devoret MH, Girvin SM, Marquardt F, Schoelkopf RJ:
*Rev Mod Phys*. 2010, 82: 1155. 10.1103/RevModPhys.82.1155MATHMathSciNetView ArticleADSGoogle Scholar - Mallet F, Castellanos-Beltran MA, Ku HS, Glancy S, Knill E, Irwin KD, Hilton GC, Vale LR, Lehnert KW:
*Phys Rev Lett*. 2011., 106: Article ID 220502 Article ID 220502Google Scholar - Flurin E, Roch N, Mallet F, Devoret MH, Huard B:
*Phys Rev Lett*. 2012., 109: Article ID 183901 Article ID 183901Google Scholar - Menzel EP, Di Candia R, Deppe F, Eder P, Zhong L, Ihmig M, Haeberlein M, Baust A, Hoffmann E, Ballester D, Inomata K, Yamamoto T, Nakamura Y, Solano E, Marx A, Gross R:
*Phys Rev Lett*. 2012., 109: Article ID 250502 Article ID 250502Google Scholar - Vijay R, Macklin C, Slichter DH, Weber SJ, Murch KW, Naik R, Korotkov AN, Siddiqi I:
*Nature*. 2012, 490: 77. 10.1038/nature11505View ArticleADSGoogle Scholar - Johnson JE, Macklin C, Slichter DH, Vijay R, Weingarten EB, Clarke J, Siddiqi I:
*Phys Rev Lett*. 2012., 109: Article ID 050506 Article ID 050506Google Scholar - Ristè D, van Leeuwen JG, Ku H-S, Lehnert KW, DiCarlo L:
*Phys Rev Lett*. 2012., 109: Article ID 050507 Article ID 050507Google Scholar - Campagne-Ibarcq P, Flurin E, Roch N, Darson D, Morfin P, Mirrahimi M, Devoret MH, Mallet F, Huard B:
*Phys Rev X*. 2013., 3: Article ID 021008 Article ID 021008Google Scholar - Teufel JD, Donner T, Li D, Harlow JW, Allman MS, Cicak K, Sirois AJ, Whittaker JD, Lehnert KW, Simmonds RW:
*Nature*. 2011, 475: 359. 10.1038/nature10261View ArticleADSGoogle Scholar - Eichler C, Bozyigit D, Wallraff A:
*Phys Rev A*. 2012., 86: Article ID 032106 Article ID 032106Google Scholar - Eichler C, Lang C, Fink JM, Govenius J, Filipp S, Wallraff A:
*Phys Rev Lett*. 2012., 109: Article ID 240501 Article ID 240501Google Scholar - Steffen L, Salathe Y, Oppliger M, Kurpiers P, Baur M, Lang C, Eichler C, Puebla-Hellmann G, Fedorov A, Wallraff A:
*Nature*. 2013, 500: 319. 10.1038/nature12422View ArticleADSGoogle Scholar - Louisell WH:
*Coupled Mode and Parametric Electronics*. John Wiley, New York; 1960.Google Scholar - Slusher RE, Hollberg LW, Yurke B, Mertz JC, Valley JF:
*Phys Rev Lett*. 1985, 55: 2409. 10.1103/PhysRevLett.55.2409View ArticleADSGoogle Scholar - Burnham DC, Weinberg DL:
*Phys Rev Lett*. 1970, 25: 84. 10.1103/PhysRevLett.25.84View ArticleADSGoogle Scholar - Bergeal N, Vijay R, Manucharyan VE, Siddiqi I, Schoelkopf RJ, Girvin SM, Devoret MH:
*Nat Phys*. 2010, 6: 296. 10.1038/nphys1516View ArticleGoogle Scholar - Bergeal N, Schackert F, Frunzio L, Devoret MH:
*Phys Rev Lett*. 2012., 108: Article ID 123902 Article ID 123902Google Scholar - Roch N, Flurin E, Nguyen F, Morfin P, Campagne-Ibarcq P, Devoret MH, Huard B:
*Phys Rev Lett*. 2012., 108: Article ID 147701 Article ID 147701Google Scholar - Ho Eom B, Day PK, LeDuc HG, Zmuidzinas J:
*Nat Phys*. 2012, 8: 623. 10.1038/nphys2356View ArticleGoogle Scholar - Yaakobi O, Friedland L, Macklin C, Siddiqi I:
*Phys Rev B*. 2013., 87: Article ID 144301 Article ID 144301Google Scholar - Wilson CM, Johansson G, Pourkabirian A, Simoen M, Johansson JR, Duty T, Nori F, Delsing P:
*Nature*. 2011, 479: 376. 10.1038/nature10561View ArticleADSGoogle Scholar - Wustmann W, Shumeiko V:
*Phys Rev B*. 2013., 87: Article ID 184501 Article ID 184501Google Scholar - Dykman M, Krivoglaz M:
*Phys A, Stat Mech Appl*. 1980, 104: 480. 10.1016/0378-4371(80)90010-2MathSciNetView ArticleGoogle Scholar - Marthaler M, Dykman MI:
*Phys Rev A*. 2006., 73: Article ID 042108 Article ID 042108Google Scholar - Siddiqi I, Vijay R, Pierre F, Wilson CM, Metcalfe M, Rigetti C, Frunzio L, Devoret MH:
*Phys Rev Lett*. 2004., 93: Article ID 207002 Article ID 207002Google Scholar - Vijay R, Devoret MH, Siddiqi I:
*Rev Sci Instrum*. 2009., 80: Article ID 111101 Article ID 111101Google Scholar - Mallet F, Ong FR, Palacios-Laloy A, Nguyen F, Bertet P, Vion D, Esteve D:
*Nat Phys*. 2009, 5: 791. 10.1038/nphys1400View ArticleGoogle Scholar - Gardiner CW, Collett MJ:
*Phys Rev A*. 1985, 31: 3761. 10.1103/PhysRevA.31.3761MathSciNetView ArticleADSGoogle Scholar - Walls DF, Milburn GJ:
*Quantum Optics*. Springer, Berlin; 1994.MATHView ArticleGoogle Scholar - Göppl M, Fragner A, Baur M, Bianchetti R, Filipp S, Fink JM, Leek PJ, Puebla G, Steffen L, Wallraff A:
*J Appl Phys*. 2008., 104: Article ID 113904 Article ID 113904Google Scholar - Braunstein SL, van Loock P:
*Rev Mod Phys*. 2005, 77: 513. 10.1103/RevModPhys.77.513MATHMathSciNetView ArticleADSGoogle Scholar - Caves CM:
*Phys Rev D*. 1982, 26: 1817. 10.1103/PhysRevD.26.1817View ArticleADSGoogle Scholar - Wallquist M, Shumeiko VS, Wendin G:
*Phys Rev B*. 2006., 74: Article ID 224506 Article ID 224506Google Scholar - Bourassa J, Beaudoin F, Gambetta JM, Blais A:
*Phys Rev A*. 2012., 86: Article ID 013814 Article ID 013814Google Scholar - Girvin SM: Lectures delivered at Ecole d’Eté Les Houches. To be published by Oxford University Press, 2011. Girvin SM: Lectures delivered at Ecole d’Eté Les Houches. To be published by Oxford University Press, 2011.Google Scholar
- Imoto N, Haus HA, Yamamoto Y:
*Phys Rev A*. 1985, 32: 2287. 10.1103/PhysRevA.32.2287View ArticleADSGoogle Scholar - Sanders BC, Milburn GJ:
*Phys Rev A*. 1989, 39: 694. 10.1103/PhysRevA.39.694View ArticleADSGoogle Scholar - Santamore DH, Goan H-S, Milburn GJ, Roukes ML:
*Phys Rev A*. 2004., 70: Article ID 052105 Article ID 052105Google Scholar - Buks E, Yurke B:
*Phys Rev A*. 2006., 73: Article ID 023815 Article ID 023815Google Scholar - Helmer F, Mariantoni M, Solano E, Marquardt F:
*Phys Rev A*. 2009., 79: Article ID 052115 Article ID 052115Google Scholar - Johnson BR, Reed MD, Houck AA, Schuster DI, Bishop LS, Ginossar E, Gambetta JM, DiCarlo L, Frunzio L, Girvin SM, Schoelkopf RJ:
*Nat Phys*. 2010, 6: 663. 10.1038/nphys1710View ArticleGoogle Scholar - Suchoi O, Abdo B, Segev E, Shtempluck O, Blencowe MP, Buks E:
*Phys Rev B*. 2010., 81: Article ID 174525 Article ID 174525Google Scholar - Kirchmair G, Vlastakis B, Leghtas Z, Nigg SE, Paik H, Ginossar E, Mirrahimi M, Frunzio L, Girvin SM, Schoelkopf RJ:
*Nature*. 2013, 495: 205. 10.1038/nature11902View ArticleADSGoogle Scholar - Koch J, Yu TM, Gambetta J, Houck AA, Schuster DI, Majer J, Blais A, Devoret MH, Girvin SM, Schoelkopf RJ:
*Phys Rev A*. 2007., 76: Article ID 042319 Article ID 042319Google Scholar - Ferguson DG, Houck AA, Koch J:
*Phys Rev X*. 2013., 3: Article ID 011003 Article ID 011003Google Scholar

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