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A hierarchy of coupled mode and envelope models for bi-directional microresonators with Kerr nonlinearity

Dmitry V. Skryabin\authormark Department of Physics, University of Bath, Bath BA2 7AY, UK
Russian Quantum Centre, Skolkovo 121205, Russia
\authormark*d.v.skryabin@bath.ac.uk
Abstract

We consider interaction of counter-propagating waves in a bi-directionally pumped ring microresonator with Kerr nonlinearity. We introduce a hierarchy of the mode expansions and envelope functions evolving on different time scales set by the cavity linewidth and nonlinearity, dispersion, and repetition rate, and provide a detailed derivation of the corresponding hierarchy of the coupled mode and of the Lugiato-Lefever-like equations. An effect of the washout of the repetition rate frequencies from the equations governing dynamics of the counter-propagating waves is elaborated in details.

journal: osac

1 Introduction

Microresonator frequency combs have been attracting a significant recent attention with their numerous practical applications and as an experimental setting to study fundamental physics of dissipative optical solitons, see [1, 2, 3] for recent reviews. So called Lugiato-Lefever (LL) model has become a paradigm in this research area [3, 4, 5, 6]. Its soliton solutions have some pre- and post- Lugiato-Lefever history in and outside the optics context, see, e.g., [7, 8, 9, 10, 11, 12, 13, 14]. However, the area has exploded after a breakthrough experimental demonstration of Ref. [5]. In terms of the first principle approach to the Kerr microresonator model development, the decade old work [6] has remained a main reference. However, together with experimental progress in the area of Kerr microresonators, the underpinning theory deserves a refreshed outlook. One of the recent challenges has emerged after a series of experiments with birectionally pumped microresonators, where combs and solitons have been observed in counter-propagating waves [15, 16, 17, 18, 19]. Bi-directionally pumped and, related dual-ring, microresonators have also been recently studied for symmetry breaking [30, 31, 32, 33, 34] and gyroscope [20, 21, 22, 23, 24, 25] related effects, including idealised PT-symmetric cases [26, 27, 28].

A variety of models has been reported in the context of experiments dealing with a single mode operation in each direction [30, 31, 32, 33, 34, 29]. We note, here that studies into single mode bidirectional lasers, laser gyroscopes and symmetry breaking in them have history going back to 1980’s, see, e.g., [35, 36, 37]. To interpret recent soliton experiments, [15, 18] have used models without nonlinear cross-coupling, while [16] has accounted for it. As we will see below, neglecting by the nonlinear cross-coupling was probably a better approach to analyse the experimental measurements under the circumstances, when modelling in neither of [15, 16, 18] included the effect of opposing group velocities, i.e., opposite signs of the resonator repetition rates for counter-propagating waves.

Due to complexity of the problem and diversity of equations both met in literature and the ones that are encountered during first principle analysis of the problem, it appears beneficial to have a detailed reference derivation that can be followed and tailored by a reader. Such mathematically transparent and physically motivated derivation that can be readily mapped onto a variety of experimental setups is present below. Focus of our work is to identify a hierarchy of the mode expansions and envelope functions evolving on different time scales set by the cavity linewidth, nonlinearity and 2nd order dispersion (slow time scales), and by the repetition rate (fast time scale), which can be used to derive a hierarchy of the coupled mode and envelope equations. We pay particular attention to comprehensive explanations of our derivation steps and interpretation of the results.

2 Hierarchies of mode expansions and envelope functions

This Section introduces physical system and discusses a hierarchy of mode amplitudes and envelope functions accounting for different time-scales. It also outlines plan of work for the rest of the paper.

Maxwell equations written for the electric field components α{\cal E}_{\alpha} using Einstein’s notations read as

c2αα1α1c2α1α1α+t2ε(tt,r,θ,z)α(t,r,θ,z)𝑑t=t2𝒩α.c^{2}\partial_{\alpha}\partial_{\alpha_{1}}{\cal E}_{\alpha_{1}}-c^{2}\partial_{\alpha_{1}}\partial_{\alpha_{1}}{\cal E}_{\alpha}+\partial_{t}^{2}\int_{-\infty}^{\infty}\varepsilon(t-t^{\prime},r,\theta,z){\cal E}_{\alpha}(t^{\prime},r,\theta,z)dt^{\prime}=-\partial_{t}^{2}{\cal N}_{\alpha}. (1)

Here ε^\widehat{\varepsilon} is the dielectric response function varying in space and time. It is assumed to be scalar for the sake of brevity. θ[0,2π)\theta\in[0,2\pi) is the azimuthal coordinate varying along the ring circumference. zz axis is perpendicular to the ring, while r=x2+y2r=\sqrt{x^{2}+y^{2}} measures distance from the ring centre. 𝒩α{\cal N}_{\alpha} is the nonlinear part of the material polarization and cc is the vacuum speed of light. We assume 3rd order nonlinearity, so that

𝒩α=χαα1α2α3(3)α1α2α3,{\cal N}_{\alpha}=\chi^{(3)}_{\alpha\alpha_{1}\alpha_{2}\alpha_{3}}{\cal E}_{\alpha_{1}}{\cal E}_{\alpha_{2}}{\cal E}_{\alpha_{3}}, (2)

where α1,2,3\alpha_{1,2,3} and α\alpha represent either of the three Cartesian projections, x,yx,y or zz, of a physical quantity they are used with. An implicit summation is assumed over any repeated α\alpha^{\prime}s. χαα1α2α3(3)\chi^{(3)}_{\alpha\alpha_{1}\alpha_{2}\alpha_{3}} is a 4th rank tensor of the third order nonlinear susceptibility, which is taken to be nondispersive (Kleinman condition, i.e., interchangeability of all four indices).

Electric field vector α{\cal E}_{\alpha} inside a ring resonator is expressed as a superposition of its linear modes Fαj(r,z)eijθ±iωjtF_{\alpha j}(r,z)e^{ij\theta\pm i\omega_{j}t}, which are solutions of Eq. (1) with 𝒩α=0{\cal N}_{\alpha}=0:

α=j=jminjmaxbjFαjeijθCj(t)+c.c.,CjBj+(t)eiωjt+Bj(t)eiωjt.{\cal E}_{\alpha}=\sum_{j=j_{min}}^{j_{max}}b_{j}F_{\alpha j}e^{ij\theta}C_{j}(t)+c.c.,~{}C_{j}\equiv B^{+}_{j}(t)e^{-i\omega_{j}t}+B^{-}_{j}(t)e^{i\omega_{j}t}. (3)

Here j>0j>0 is an azimuthal mode number, or angular momentum, and ωj>0\omega_{j}>0 is the corresponding mode frequency. Bj±B^{\pm}_{j} are the amplitudes of the clockwise (CW) and counter-clockwise (CCW) modes. For typical microresonators geometries, either bulk crystalline or chip integrated, the transverse mode profiles FαjF_{\alpha j} can be divided into quasi-TE quasi-radial modes (|Fxj,yj||Fzj||F_{xj,yj}|\gg|F_{zj}|) and quasi-TM (|Fzj||Frj,θj||F_{zj}|\gg|F_{rj,\theta j}|). For many practical purposes, which is in our case calculation of the overlap integrals in the nonlinear terms, it often suffices to neglect the smaller components of FαjF_{\alpha j}. We also assume that the dominant components of FαjF_{\alpha j} and ωj\omega_{j} are real, so that Fαj=FαjF_{\alpha j}=F_{\alpha j}^{*}, ωj=ωj\omega_{j}=\omega_{j}^{*}. Thus for TE modes FxjcosθFrF_{xj}\approx\cos\theta F_{r}, FyjsinθFrF_{yj}\approx\sin\theta F_{r}, Fzj0F_{zj}\approx 0 and for TM modes Fxj,yj0F_{xj,yj}\approx 0.

In order to cut notational complexity and drop the α\alpha index, we consider TM family, so that from now on FzjFjF_{zj}\to F_{j}, and

𝒩z=𝒩=χ(3)z3.{\cal N}_{z}={\cal N}=\chi^{(3)}{\cal E}_{z}^{3}. (4)

Results of our derivations would be the same for TE modes, FrjFjF_{rj}\to F_{j}, and therefore, what we are loosing is only formal consideration of the nonlinear coupling between the TE and TM families.

We assume that inhomogeneities of the resonator surfaces result in scattering in general and in backscattering, in particular, and hence lead to the linear coupling between the modes. We account for these effects assuming

ε(t,θ,r,z)=εid(t,r,z)(1+εin(θ)).\varepsilon(t,\theta,r,z)=\varepsilon_{id}(t,r,z)\big{(}1+\varepsilon_{in}(\theta)\big{)}. (5)

Here εid\varepsilon_{id} is the dispersive dielectric function of the ideal (no backscattering) geometry, that does not depend on θ\theta, while relatively small εin(θ)\varepsilon_{in}(\theta) accounts for inhomogeneities along the ring. Mode profiles Fj(r,z)F_{j}(r,z) are calculated for εin=0\varepsilon_{in}=0.

{\cal E} is measured in V/m, hence normalising linear modes as maxr,z|Fj|=1\max_{r,z}|F_{j}|=1 makes units of bjBj±b_{j}B^{\pm}_{j} to be V/m. Real field amplitude of a CCW mode is 2bj|Bj+|2b_{j}|B^{+}_{j}|, so that its intensity is Ij+=2cϵvacnjbj2|Bj+|2I^{+}_{j}=2c\epsilon_{vac}n_{j}b_{j}^{2}|B^{+}_{j}|^{2} and power is Ij+/SjI^{+}_{j}/S_{j}. SjS_{j} is the effective transverse mode area, Sj=(|Fj|2𝑑x𝑑z)2/|Fj|4𝑑x𝑑zS_{j}=\big{(}\iint|F_{j}^{\prime}|^{2}dxdz\big{)}^{2}/\iint|F_{j}^{\prime}|^{4}dxdz and Fj=Fj(r,z)|y=0F_{j}^{\prime}=F_{j}(r,z)|_{y=0}. njn_{j} is the linear refractive index, nj2=εid(τ,r=r0,z=0)eiωjτdτn_{j}^{2}=\int_{-\infty}^{\infty}\varepsilon_{id}(\tau,r=r_{0},z=0)e^{i\omega_{j}\tau}d\tau, where r0r_{0} is the distance between the zz axis and a point of maximum of |Fj||F_{j}|. We define scaling factors bjb_{j} as

bj2=12ϵvacSjnjc,b_{j}^{2}=\frac{1}{2\epsilon_{vac}S_{j}n_{j}c}, (6)

so that the |Bj±|2|B^{\pm}_{j}|^{2} are measured in Watts. ϵvac\epsilon_{vac} is the vacuum susceptibility.

We assume that the resonator is pumped into its jpj_{p} mode and introduce the mode index offset μ=jjp\mu=j-j_{p}. The real field expression, Eq. (3), is then

z(t,θ,r,z)bjpFjp,\displaystyle{\cal E}_{z}(t,\theta,r,z)\simeq b_{j_{p}}F_{j_{p}}{\cal E},
(t,θ)=μ(Bμ+eijμθiωμt+Bμeijμθ+iωμt)+c.c.,\displaystyle{\cal E}(t,\theta)=\sum_{\mu}\Big{(}B^{+}_{\mu}e^{ij_{\mu}\theta-i\omega_{\mu}t}+B^{-}_{\mu}e^{ij_{\mu}\theta+i\omega_{\mu}t}\Big{)}+c.c., (7)

where jμ=jp+μ=jj_{\mu}=j_{p}+\mu=j and μ=|jpjmin|,,0,,|jmaxjp|\mu=-|j_{p}-j_{min}|,\dots,0,\dots,|j_{max}-j_{p}|. Here (t,θ){\cal E}(t,\theta) is the real electric field measured in W1/2W^{1/2}, which dependence on the transverse coordinates has been factored out. Introducing pump laser frequency Ω\Omega, we define mode detunings

δμ=ωμΩ,\delta_{\mu}=\omega_{\mu}-\Omega, (8)

where δ0\delta_{0} is the detuning for mode jpj_{p}, and

ωμ=ω0+D1μ+12!D2μ2+13!D3μ3+,\omega_{\mu}=\omega_{0}+D_{1}\mu+\tfrac{1}{2!}D_{2}\mu^{2}+\tfrac{1}{3!}D_{3}\mu^{3}+\dots, (9)

where a desired number of the dispersion orders can be included to approximate ωμ\omega_{\mu} over a required spectral range.

D1D_{1} is the resonator repetition rate (or free spectral range (FSR)) and D2D_{2} is its group velocity dispersion. D2>0D_{2}>0 implies anomalous and D2<0D_{2}<0 normal dispersion. For example, the work [15] deals with a bi-directionally pumped silica ring with radius 1.51.5mm and it has D1=2π×22D_{1}=2\pi\times 22GHz, D2=2π×16D_{2}=2\pi\times 16kHz. The linewidth of this resonator is κ=2π×1.5\kappa=2\pi\times 1.5MHz, and hence the corresponding finesse =D1/κ13000{\cal F}=D_{1}/\kappa\simeq 13000. The mode area estimate is Sjp30μS_{j_{p}}\simeq 30\mum2, which gives bj24×1012b_{j}^{2}\simeq 4\times 10^{12}V2W-1m-2. Pump laser wavelength was 1550\simeq 1550nm (ω02π×193\omega_{0}\simeq 2\pi\times 193THz) and the comb spectra observed there were relatively narrow and span over 20\sim 20nm bandwidth, corresponding to about 300300 modes, and the momentum of a mode nearest to the pump is estimated as jp=8700j_{p}=8700.

In order to introduce a new set of mode amplitudes important in what follows, we transform Eq. (7) further:

\displaystyle{\cal E} =eijpθiΩtμBμ+eiδμt+iμθ+eijpθ+iΩtμBμeiδμt+iμθ+c.c.\displaystyle=e^{ij_{p}\theta-i\Omega t}\sum_{\mu}B^{+}_{\mu}e^{-i\delta_{\mu}t+i\mu\theta}+e^{ij_{p}\theta+i\Omega t}\sum_{\mu}B^{-}_{\mu}e^{i\delta_{\mu}t+i\mu\theta}+c.c. (10a)
=eijpθiΩtμQμ+eiμθ+eijpθ+iΩtμQμeiμθ+c.c.\displaystyle=e^{ij_{p}\theta-i\Omega t}\sum_{\mu}Q^{+}_{\mu}e^{i\mu\theta}+e^{ij_{p}\theta+i\Omega t}\sum_{\mu}Q^{-*}_{\mu}e^{i\mu\theta}+c.c. (10b)
=eijpθiΩtQ++eijpθ+iΩtQ+c.c..\displaystyle=e^{ij_{p}\theta-i\Omega t}Q_{+}+e^{ij_{p}\theta+i\Omega t}Q_{-}^{*}+c.c.~{}. (10c)

Newly introduced mode amplitudes Qμ±Q_{\mu}^{\pm} are defined as

Qμ+=Bμ+eiδμt,Qμ=Bμeiδμt,Q_{\mu}^{+}=B_{\mu}^{+}e^{-i\delta_{\mu}t},~{}Q_{\mu}^{-}=B_{\mu}^{-*}e^{-i\delta_{\mu}t}, (11)

and as we can see they absorb frequency scales associated with both D1D_{1} and D2D_{2}. The corresponding CW and CCW envelope functions are

Q±(t,θ)=μQμ±e±iμθ.Q_{\pm}(t,\theta)=\sum_{\mu}Q_{\mu}^{\pm}e^{\pm i\mu\theta}. (12)

Inclusion of the backscattering effects to the envelope equations, see Section 5, requires introducing of the envelope functions with reflections of their spatial coordinate,

Q±(r)(t,θ)=μQμ±eiμθ,\displaystyle Q_{\pm}^{(r)}(t,\theta)=\sum_{\mu}Q_{\mu}^{\pm}e^{\mp i\mu\theta}, (13a)
Q±(r)(t,θ)=Q±(t,2πθ).\displaystyle Q^{(r)}_{\pm}(t,\theta)=Q_{\pm}(t,2\pi-\theta). (13b)

The above definition of the space reflected functions follows a text-book list of properties of Fourier transforms, where an equivalent transformation is typically introduced in time domain and could be called as either time reflection or time inversion transformation. Differential equations involving functions with reflections of their arguments also attracted some attention from a more general mathematics prospective, see, e.g., [38], while our system reveals their role in nonlinear photonics.

In order to take control of D1D_{1} in our future calculations, we define yet another set of slow amplitudes

Aμ+=Bμ+eiδμt,Aμ=Bμeiδμt,\displaystyle A_{\mu}^{+}=B_{\mu}^{+}e^{-i{\delta}^{\prime}_{\mu}t},~{}A_{\mu}^{-}=B_{\mu}^{-*}e^{-i{\delta}^{\prime}_{\mu}t}, (14a)
δμ=δ0+12D2μ2.\displaystyle{\delta}^{\prime}_{\mu}=\delta_{0}+\tfrac{1}{2}D_{2}\mu^{2}. (14b)

Here D1D_{1} is moved away from the exponential factors defining our third and final set of amplitudes Aμ±A_{\mu}^{\pm}. Instead, exponents with D1D_{1} appear explicitly in the total field equation that uses Aμ±A_{\mu}^{\pm},

=(eijpθiΩtμAμ+eiμ(θD1t)+eijpθ+iΩtμAμeiμ(θ+D1t))+c.c..{\cal E}=\Big{(}e^{ij_{p}\theta-i\Omega t}\sum_{\mu}A^{+}_{\mu}e^{i\mu\big{(}\theta-D_{1}t\big{)}}+e^{ij_{p}\theta+i\Omega t}\sum_{\mu}A^{-*}_{\mu}e^{i\mu\big{(}\theta+D_{1}t\big{)}}\Big{)}+c.c.~{}. (15)

We also use Aμ±A_{\mu}^{\pm} to define the corresponding envelope functions and their reflections

A±=μAμ±e±iμθ,A±(r)=μAμ±eiμθ,\displaystyle A_{\pm}=\sum_{\mu}A_{\mu}^{\pm}e^{\pm i\mu\theta},~{}A_{\pm}^{(r)}=\sum_{\mu}A_{\mu}^{\pm}e^{\mp i\mu\theta}, (16a)
A±(r)(t,θ)=A±(t,2πθ).\displaystyle A^{(r)}_{\pm}(t,\theta)=A_{\pm}(t,2\pi-\theta). (16b)

Though the envelopes A±A_{\pm} can not be used themselves to define the electric field {\cal E} (only their mode amplitudes can), cf. Eq. (15) and (16), they play a pivotal role in the transition from the coupled mode to the partial differential equations, see Section 5.

To summarize this section: Bμ±B_{\mu}^{\pm} amplitudes absorb only the slowest time scales associated with the nonlinear effects and resonator losses. Aμ±A_{\mu}^{\pm} absorb time scales associated with the second and higher order dispersions, in addition to the ones already inside Bμ±B_{\mu}^{\pm}. Qμ±Q_{\mu}^{\pm} amplitudes evolve with the highest in our hierarchy frequency determined by the resonator repetition rate. To see how these different time scales and mode amplitudes are used to express the total field, {\cal E}, one should compare Eqs. (10a), (10b) and (15).

The rest of this work is structured as follows: In section 3, we first derive a system of equations for Bμ±B^{\pm}_{\mu} and perform its exact reduction to the equations for Qμ±Q^{\pm}_{\mu}. In Section 4, we come back to the equations for Bμ±B^{\pm}_{\mu}, make the D1D_{1} role explicit, eliminate the associated fast oscillations and derive a simpler system for Aμ±A^{\pm}_{\mu}. Corresponding mean-field equations for the envelope functions Q±Q_{\pm} and A±A_{\pm} and their counter parts with the reflected spatial coordinates are derived in Section 5.

3 Coupled mode equations

3.1 Separating equations for CW and CCW amplitudes

Substituting t=tτt^{\prime}=t-\tau in Eqs. (1), (3) we then assume that material response is fast so that Cj(tτ)Cj(t)τtCj+C_{j}(t-\tau)\simeq C_{j}(t)-\tau\partial_{t}C_{j}+\dots. Neglecting all the 2nd and higher order time derivatives of Bμ±B^{\pm}_{\mu} we find that Eq. (1) transforms to

t2𝒩bjpFjpμeijμθ×(nμ2ωμ2εin(θ)Bμ+eiωμt2iωμsμeiωμttBμ+\displaystyle-\partial_{t}^{2}{\cal N}\simeq b_{j_{p}}F_{j_{p}}\sum_{\mu}e^{ij_{\mu}\theta}\times\Big{(}-n_{\mu}^{2}\omega_{\mu}^{2}\varepsilon_{in}(\theta)B^{+}_{\mu}e^{-i\omega_{\mu}t}-2i\omega_{\mu}s_{\mu}e^{-i\omega_{\mu}t}\partial_{t}B^{+}_{\mu}
nμ2ωμ2εin(θ)Bμeiωμt+2iωμsμeiωμttBμ)\displaystyle-n_{\mu}^{2}\omega_{\mu}^{2}\varepsilon_{in}(\theta)B^{-}_{\mu}e^{i\omega_{\mu}t}+2i\omega_{\mu}s_{\mu}e^{i\omega_{\mu}t}\partial_{t}B^{-}_{\mu}\Big{)}
+bjpFjpμeijμθ×(nμ2ωμ2εin(θ)Bμ+eiωμt+2iωμsμeiωμttBμ+\displaystyle+b_{j_{p}}F_{j_{p}}\sum_{\mu}e^{-ij_{\mu}\theta}\times\Big{(}-n_{\mu}^{2}\omega_{\mu}^{2}\varepsilon_{in}(\theta)B^{+*}_{\mu}e^{i\omega_{\mu}t}+2i\omega_{\mu}s_{\mu}e^{i\omega_{\mu}t}\partial_{t}B^{+*}_{\mu}
nμ2ωμ2εin(θ)Bμeiωμt2iωμsμeiωμttBμ),\displaystyle-n_{\mu}^{2}\omega_{\mu}^{2}\varepsilon_{in}(\theta)B^{-*}_{\mu}e^{-i\omega_{\mu}t}-2i\omega_{\mu}s_{\mu}e^{-i\omega_{\mu}t}\partial_{t}B^{-*}_{\mu}\Big{)}, (17)

where sμ=nμ2+12ωμωnμ2nμ2s_{\mu}=n_{\mu}^{2}+\frac{1}{2}\omega_{\mu}\partial_{\omega}n_{\mu}^{2}\simeq n_{\mu}^{2}. We then expand nonlinear polarization 𝒩{\cal N} in Fourier series

𝒩(r,z,θ,t)=μ𝒩jμ(r,z,t)eijμθ+c.c..{\cal N}(r,z,\theta,t)=\sum_{\mu}{\cal N}_{j_{\mu}}(r,z,t)e^{ij_{\mu}\theta}+c.c.. (18)

In order to carry out separation of the CW and CCW equation we also need to define CW and CCW components of nonlinear polarization, Pjμ±eiωjμtP^{\pm}_{j_{\mu}}e^{\mp i\omega_{j_{\mu}}t}, such that

𝒩jμPjμ+eiωjμt+Pjμeiωjμt.{\cal N}_{j_{\mu}}\equiv P^{+}_{j_{\mu}}e^{-i\omega_{j_{\mu}}t}+P^{-}_{j_{\mu}}e^{i\omega_{j_{\mu}}t}. (19)

Explicit expressions for Pjμ±P^{\pm}_{j_{\mu}} are given by Eqs. (29) below.

We now multiply the left and right hand-sides of Eq. (17) by bjpFjpexpijμθb_{j_{p}}F_{j_{p}}\exp^{-ij_{\mu^{\prime}}\theta}, integrate in r,zr,z and θ\theta, and approximate ωμω0=ωjp\omega_{\mu}\simeq\omega_{0}=\omega_{j_{p}}, nμn0n_{\mu}\simeq n_{0} inside all the pre-factors, but not in the powers of the exponents. The resulting model, see Eqs. (22), makes use of the two scattering matrices having dimensions of angular frequencies. One characterises scattering induced coupling between the co-propagating modes

Γ^μμ=12ω002πei(μμ)θεin(θ)dθ2π,\widehat{\Gamma}_{\mu\mu^{\prime}}=\tfrac{1}{2}\omega_{0}\int_{0}^{2\pi}e^{i(\mu-\mu^{\prime})\theta}\varepsilon_{in}(\theta)\frac{d\theta}{2\pi}, (20)

and the other one describes backscattering induced mode coupling,

^μμ=12ω002πei(2jp+μ+μ)θεin(θ)dθ2π.\widehat{\cal R}_{\mu\mu^{\prime}}=\tfrac{1}{2}\omega_{0}\int_{0}^{2\pi}e^{-i(2j_{p}+\mu+\mu^{\prime})\theta}\varepsilon_{in}(\theta)\frac{d\theta}{2\pi}. (21)

The projected equation itself is

μΓ^μμBμ+eiωμtieiωμttBμ+μΓ^μμBμeiωμt+ieiωμttBμ\displaystyle-\sum_{\mu}\widehat{\Gamma}_{\mu\mu^{\prime}}B^{+}_{\mu}e^{-i\omega_{\mu}t}-ie^{-i\omega_{\mu^{\prime}}t}\partial_{t}B^{+}_{\mu^{\prime}}-\sum_{\mu}\widehat{\Gamma}_{\mu\mu^{\prime}}B^{-}_{\mu}e^{i\omega_{\mu}t}+ie^{i\omega_{\mu^{\prime}}t}\partial_{t}B^{-}_{\mu^{\prime}}
μ^μμBμ+eiωμtμ^μμBμeiωμt\displaystyle-\sum_{\mu}\widehat{\cal R}_{\mu\mu^{\prime}}B^{+*}_{\mu}e^{i\omega_{\mu}t}-\sum_{\mu}\widehat{\cal R}_{\mu\mu^{\prime}}B^{-*}_{\mu}e^{-i\omega_{\mu}t}
=πω0n02Vpbjp2t2𝒩jμbjpFjpr𝑑r𝑑z\displaystyle=-\frac{\pi\omega_{0}}{n_{0}^{2}V_{p}b_{j_{p}}^{2}}\partial_{t}^{2}\iint{\cal N}_{j_{\mu^{\prime}}}b_{j_{p}}F_{j_{p}}rdrdz
πω0n02Vpbjp2(Pjμ+eiωμt+Pjμeiωμt)bjpFjpr𝑑r𝑑z.\displaystyle\simeq\frac{\pi\omega_{0}}{n_{0}^{2}V_{p}b_{j_{p}}^{2}}\iint\Big{(}P^{+}_{j_{\mu}^{\prime}}e^{-i\omega_{\mu^{\prime}}t}+P^{-}_{j_{\mu}^{\prime}}e^{i\omega_{\mu^{\prime}}t}\Big{)}b_{j_{p}}F_{j_{p}}rdrdz. (22)

where Vp=2πFjp2r𝑑r𝑑zV_{p}=2\pi\iint~{}F_{j_{p}}^{2}rdrdz is the mode volume for j=jpj=j_{p}.

Eq. (22) can now be split, as per rotating wave approximation, into the parts proportional to e±iωjμte^{\pm i\omega_{j_{\mu}}t} exponents, so that we have two equations defined on the slow, D2D_{2} related, time scales:

itBμ+=μ(Γ^μμBμ++^μμBμ)ei(ωμωμ)t+πω0n02Vpbjp2Pjμ+bjpFjpr𝑑r𝑑z,\displaystyle-i\partial_{t}B^{+}_{\mu}=\sum_{\mu^{\prime}}\Big{(}\widehat{\Gamma}_{\mu^{\prime}\mu}B^{+}_{\mu^{\prime}}+\widehat{\cal R}_{\mu^{\prime}\mu}B^{-*}_{\mu^{\prime}}\Big{)}e^{i(\omega_{\mu}-\omega_{\mu^{\prime}})t}+\frac{\pi\omega_{0}}{n_{0}^{2}V_{p}b_{j_{p}}^{2}}\iint P^{+}_{j_{\mu}}b_{j_{p}}F_{j_{p}}rdrdz, (23a)
itBμ=μ(Γ^μμBμ+^μμBμ+)ei(ωμωμ)t+πω0n02Vpbjp2PjμbjpFjpr𝑑r𝑑z,\displaystyle i\partial_{t}B^{-}_{\mu}=\sum_{\mu^{\prime}}\Big{(}\widehat{\Gamma}_{\mu^{\prime}\mu}B^{-}_{\mu^{\prime}}+\widehat{\cal R}_{\mu^{\prime}\mu}B^{+*}_{\mu^{\prime}}\Big{)}e^{-i(\omega_{\mu}-\omega_{\mu^{\prime}})t}+\frac{\pi\omega_{0}}{n_{0}^{2}V_{p}b_{j_{p}}^{2}}\iint P^{-}_{j_{\mu}}b_{j_{p}}F_{j_{p}}rdrdz, (23b)

where we have also swapped μ\mu and μ\mu^{\prime}.

In order to be used to describe laboratory experiments with microresonators, Eqs. (23) have to be amended with the single mode pump term and losses accounting for the finite linewidth. We take, for the laser frequency at the exact cavity resonance Ω=ωμ=0=ωj=jp\Omega=\omega_{\mu=0}=\omega_{j=j_{p}} and for the low pump levels, i.e., linear regime, the intracavity powers of CW and CCW waves to be |±|2=|Bμ±|2|{\cal H}_{\pm}|^{2}=|B^{\pm}_{\mu}|^{2}. This is achieved via a phenomenological substitution

itBμ±itBμ±+i12κ(Bμ±δ^μ,0±e±i(ωμΩ)t).i\partial_{t}B^{\pm}_{\mu}\to i\partial_{t}B^{\pm}_{\mu}+i\tfrac{1}{2}\kappa\left(B^{\pm}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{\pm}e^{\pm i(\omega_{\mu}-\Omega)t}\right). (24)

Here, Kronecker delta is defined as δ^μ,μ1=1\widehat{\delta}_{\mu,\mu_{1}}=1 for μ=μ1\mu=\mu_{1} and is 0 otherwise.

If pump is absent, then the field power would decay with the rate κ\kappa (full width of the resonance). An expression linking ±{\cal H}_{\pm} with the laser powers 𝒲±{\cal W}_{\pm} is

|±|2=ηπ𝒲±,|{\cal H}_{\pm}|^{2}=\frac{\eta}{\pi}{\cal F}{\cal W}_{\pm}, (25)

where 𝒲±{\cal W}_{\pm} are the laser powers pumping, respectively, CW and CCW waves. η<1\eta<1 is the coupling efficiency via, e.g., a prism or a waveguide, into a resonator mode. η=κc/κ\eta=\kappa_{c}/\kappa, where κc\kappa_{c} is the coupling pump rate (equals coupling loss rate). /π{\cal F}/\pi is the cavity induced power enhancement. Detailed theoretical and experimental studies of the power enhancement effect and coupling in and out considerations for ring cavities can be found in, e.g., [39, 40].

^μμ2π×4\widehat{\cal R}_{\mu\mu}\sim 2\pi\times 4 kHz in Ref. [15]. In this regime, it is safe to assume that κ\kappa dominates over Γ^\widehat{\Gamma} and ^\widehat{\cal R} terms. Using this we disregard Γ^μμ\widehat{\Gamma}_{\mu^{\prime}\mu} in what follows, and retain only the dominant diagonal terms in ^μμ\widehat{\cal R}_{\mu^{\prime}\mu}, i.e., ^μμμ0\widehat{\cal R}_{\mu^{\prime}\mu\neq\mu^{\prime}}\approx 0. Dispersion of the diagonal terms is also disregarded, ^μμ^00=R\widehat{\cal R}_{\mu\mu}\simeq\widehat{\cal R}_{00}=R. Accounting for all of the above and complex conjugating second of Eqs. (23) we conclude this subsection with

itBμ+=i12κ(Bμ+δ^μ,0+eiδμt)RBμπω0n02Vpbjp2Pjμ+bjpFjpr𝑑r𝑑z,\displaystyle i\partial_{t}B^{+}_{\mu}=-i\tfrac{1}{2}\kappa\left(B^{+}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{+}e^{i\delta_{\mu}t}\right)-RB^{-*}_{\mu}-\frac{\pi\omega_{0}}{n_{0}^{2}V_{p}b_{j_{p}}^{2}}\iint P_{j_{\mu}}^{+}b_{j_{p}}F_{j_{p}}rdrdz, (26a)
itBμ=i12κ(Bμδ^μ,0eiδμt)RBμ+πω0n02Vpbjp2PjμbjpFjpr𝑑r𝑑z.\displaystyle i\partial_{t}B^{-*}_{\mu}=-i\tfrac{1}{2}\kappa\left(B^{-*}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{-}e^{i\delta_{\mu}t}\right)-R^{*}B^{+}_{\mu}-\frac{\pi\omega_{0}}{n_{0}^{2}V_{p}b_{j_{p}}^{2}}\iint P_{j_{\mu}}^{-*}b_{j_{p}}F_{j_{p}}rdrdz. (26b)

3.2 Opening up nonlinearity

Using Eqs. (4), (7) we have

𝒩=bjp3Fjp3χ(3)3,{\cal N}=b_{j_{p}}^{3}F_{j_{p}}^{3}\chi^{(3)}{\cal E}^{3}, (27)

and

3=3{eijpθiΩt(|Q+|2+2|Q|2)Q++eijpθiΩt(|Q|2+2|Q+|2)Q+}+c.c..{\cal E}^{3}=3\Big{\{}e^{ij_{p}\theta-i\Omega t}\left(|Q_{+}|^{2}+2|Q_{-}|^{2}\right)Q_{+}+e^{-ij_{p}\theta-i\Omega t}\left(|Q_{-}|^{2}+2|Q_{+}|^{2}\right)Q_{-}+\dots\Big{\}}+c.c.~{}. (28)

Comparing Eqs. (27), (28) and Eqs. (18), (19), one can define explicit expressions for Pjμ±P^{\pm}_{j_{\mu}}. Assuming spectrally narrow combs, and therefore omitting all terms with exponential factors oscillating in space with multiples of jpj_{p} and in time with multiples of Ω\Omega, we find

Pjμ+=3bjp3Fjp3χ(3)ei(ωjμΩ)t02π(|Q+|2+2|Q|2)Q+eiμθdθ2π,\displaystyle P_{j_{\mu}}^{+}=3b_{j_{p}}^{3}F_{j_{p}}^{3}\chi^{(3)}e^{i(\omega_{j_{\mu}}-\Omega)t}\int_{0}^{2\pi}\left(|Q_{+}|^{2}+2|Q_{-}|^{2}\right)Q_{+}e^{-i\mu\theta}\frac{d\theta}{2\pi}, (29a)
Pjμ=3bjp3Fjp3χ(3)ei(ωjμΩ)t02π(|Q|2+2|Q+|2)Qeiμθdθ2π.\displaystyle P_{j_{\mu}}^{-}=3b_{j_{p}}^{3}F_{j_{p}}^{3}\chi^{(3)}e^{-i(\omega_{j_{\mu}}-\Omega)t}\int_{0}^{2\pi}\left(|Q_{-}|^{2}+2|Q_{+}|^{2}\right)Q_{-}^{*}e^{-i\mu\theta}\frac{d\theta}{2\pi}. (29b)

Thereby, Eqs. (26) become

itBμ+=i12κ(Bμ+δ^μ,0+eiδμt)RBμγeiδμt02π(|Q+|2+2|Q|2)Q+eiμθdθ2π,\displaystyle i\partial_{t}B^{+}_{\mu}=-i\tfrac{1}{2}\kappa\left(B^{+}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{+}e^{i\delta_{\mu}t}\right)-RB^{-*}_{\mu}-\gamma e^{i\delta_{\mu}t}\int_{0}^{2\pi}\left(|Q_{+}|^{2}+2|Q_{-}|^{2}\right)Q_{+}e^{-i\mu\theta}\frac{d\theta}{2\pi}, (30a)
itBμ=i12κ(Bμδ^μ,0eiδμt)RBμ+γeiδμt02π(|Q|2+2|Q+|2)Qeiμθdθ2π,\displaystyle i\partial_{t}B^{-*}_{\mu}=-i\tfrac{1}{2}\kappa\left(B^{-*}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{-}e^{i\delta_{\mu}t}\right)-R^{*}B^{+}_{\mu}-\gamma e^{i\delta_{\mu}t}\int_{0}^{2\pi}\left(|Q_{-}|^{2}+2|Q_{+}|^{2}\right)Q_{-}e^{i\mu\theta}\frac{d\theta}{2\pi}, (30b)

where nonlinear coefficient is

γ=32ω0bjp2n022πVpχ(3)Fjp4r𝑑r𝑑z.\gamma=\frac{3}{2}\frac{\omega_{0}b_{j_{p}}^{2}}{n_{0}^{2}}\frac{2\pi}{V_{p}}\iint\chi^{(3)}F_{j_{p}}^{4}rdrdz. (31)

Total refractive index, nn, for a single mode operation is n={n02+3χ(3)bjp2|Bjp+|2}1/2n0+32n0χ(3)bjp2|Bjp+|2=n0+n2Ijp+n=\{n_{0}^{2}+3\chi^{(3)}b_{j_{p}}^{2}|B^{+}_{j_{p}}|^{2}\}^{1/2}\simeq n_{0}+\tfrac{3}{2n_{0}}\chi^{(3)}b_{j_{p}}^{2}|B^{+}_{j_{p}}|^{2}=n_{0}+n_{2}I^{+}_{j_{p}}, see definition of intensity before Eq. (6). Hence, Kerr coefficient is n2=34χ(3)(n02ϵvacc)1n_{2}=\tfrac{3}{4}\chi^{(3)}(n_{0}^{2}\epsilon_{vac}c)^{-1}. Using Eqs. (6), (31), an expression for γ\gamma in terms of more often used n2n_{2} is

γ=ω0Sjpn02πVpn2Fjp4r𝑑r𝑑z.\gamma=\frac{\omega_{0}}{S_{j_{p}}n_{0}}\frac{2\pi}{V_{p}}\iint n_{2}F_{j_{p}}^{4}rdrdz. (32)

Assuming that the jpj_{p} mode is well confined within the resonator material, the mode shape can be approximated by a Gaussian function (allowing for different widths along zz and xx), and rdrr0dxrdr\approx r_{0}dx (see text before Eq. (6)), gives 2πFjp4r𝑑r𝑑z/Vp122\pi\iint F_{j_{p}}^{4}rdrdz/V_{p}\approx\tfrac{1}{2} and

γω0n22Sjpn0.\gamma\approx\frac{\omega_{0}n_{2}}{2S_{j_{p}}n_{0}}. (33)

Eq. (32) and Eq. (33) have been compared using mode profiles calculated with Comsol and it was found that the latter provides a very practical approximation. For ω0=2π×193\omega_{0}=2\pi\times 193THz, n0=1.47n_{0}=1.47 and n23.2×1020n_{2}\simeq 3.2\times 10^{-20}m2/W2 (silica glass), and mode area Sjp30μS_{j_{p}}\approx 30\mum2 we have γ2π×70\gamma\simeq 2\pi\times 70kHz/W. SjpS_{j_{p}} is an order of magnitude smaller and n2n_{2} is an order of magnitude larger in integrated Si3N4 microresonators, and their combined effect boosts γ\gamma up by two orders of magnitude.

Using Eqs. (11) to express amplitudes Bμ±B_{\mu}^{\pm} via Qμ±Q_{\mu}^{\pm} we find that all the time dependent exponents cancel out and the resulting coupled mode equations for Qμ±Q_{\mu}^{\pm} amplitudes are

itQμ+=δμQμ+i12κ(Qμ+δ^μ,0+)RQμγ02π(|Q+|2+2|Q|2)Q+eiμθdθ2π,\displaystyle i\partial_{t}Q^{+}_{\mu}=\delta_{\mu}Q^{+}_{\mu}-i\tfrac{1}{2}\kappa\left(Q^{+}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{+}\right)-RQ^{-}_{\mu}-\gamma\int_{0}^{2\pi}\left(|Q_{+}|^{2}+2|Q_{-}|^{2}\right)Q_{+}e^{-i\mu\theta}\frac{d\theta}{2\pi}, (34a)
itQμ=δμQμi12κ(Qμδ^μ,0)RQμ+γ02π(|Q|2+2|Q+|2)Qeiμθdθ2π,\displaystyle i\partial_{t}Q^{-}_{\mu}=\delta_{\mu}Q^{-}_{\mu}-i\tfrac{1}{2}\kappa\left(Q^{-}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{-}\right)-R^{*}Q^{+}_{\mu}-\gamma\int_{0}^{2\pi}\left(|Q_{-}|^{2}+2|Q_{+}|^{2}\right)Q_{-}e^{i\mu\theta}\frac{d\theta}{2\pi}, (34b)

where Q±Q_{\pm} envelopes are given by Eqs. (12).

4 Washout of the repetition rate timescales from the coupled mode equations

Systems of Eqs. (30), (11), (12) on one side, and Eqs. (34), (12) on the other, are mathematically and physically equivalent. However, there are important observations to be made here. If one could assume that |Q+|2+2|Q|2|Q_{+}|^{2}+2|Q_{-}|^{2} under the integrals in the right hand sides of Eqs. (30) and Eqs. (34) is a slow function of time, then these integrals would be approximately equal to Qμ±eiδμtQ_{\mu}^{\pm}e^{-i\delta_{\mu}t}, see Eqs. (11). Balancing these with the eiδμte^{i\delta_{\mu}t} exponents before the integrals in Eqs. (30), one would end up with equations involving time scales determined only by the linewidths, pump detuning and nonlinear resonance shifts, which are all order of MHz. MHz frequencies would be far simpler to resolve numerically, compare to GHz-THz frequencies associated with D1D_{1}, that are directly implicated inside δμ\delta_{\mu} in the linear parts of Eqs. (34).

In this Section, we demonstrate that there are both slow and fast time scales inside the nonlinear terms in Eqs. (30), and that the latter can be eliminated resulting in a simpler and better balanced system of equations for the Aμ±A_{\mu}^{\pm} amplitudes, see Eqs. (14), (39).

We proceed by taking Eqs. (30a), express Q±Q_{\pm} via Bμ±B_{\mu}^{\pm}, see Eqs. (11), (12), calculate integrals in the nonlinear terms, see Eq. (35a), and perform the two step transformation, see Eqs. (35b), (35c),

itBμ++i12κ(Bμ+δ^μ,0±eiδμt)+RBμ=\displaystyle i\partial_{t}B^{+}_{\mu}+i\tfrac{1}{2}\kappa\left(B^{+}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{\pm}e^{i\delta_{\mu}t}\right)+RB^{-*}_{\mu}=
γeiδμtμ1μ2μ3(δ^μ1+μ2μ3,μBμ1+Bμ2+Bμ3+ei(δμ1δμ2+δμ3)t\displaystyle-\gamma e^{i\delta_{\mu}t}\sum_{\mu_{1}\mu_{2}\mu_{3}}\Big{(}\widehat{\delta}_{\mu_{1}+\mu_{2}-\mu_{3},\mu}B_{\mu_{1}}^{+}B_{\mu_{2}}^{+}B_{\mu_{3}}^{+*}e^{i(-\delta_{\mu_{1}}-\delta_{\mu_{2}}+\delta_{\mu_{3}})t}
+2δ^μ1μ2+μ3,μBμ1+Bμ2Bμ3ei(δμ1δμ2+δμ3)t)=\displaystyle+2\widehat{\delta}_{\mu_{1}-\mu_{2}+\mu_{3},\mu}B_{\mu_{1}}^{+}B_{\mu_{2}}^{-}B_{\mu_{3}}^{-*}e^{i(-\delta_{\mu_{1}}-\delta_{\mu_{2}}+\delta_{\mu_{3}})t}\Big{)}= (35a)
γμ1μ2μ3δ^μ1+μ2μ3,μ(Bμ1+Bμ2+Bμ3+ei(δμ1δμ2+δμ3+δμ)t\displaystyle-\gamma\sum_{\mu_{1}\mu_{2}\mu_{3}}\widehat{\delta}_{\mu_{1}+\mu_{2}-\mu_{3},\mu}\Big{(}B_{\mu_{1}}^{+}B_{\mu_{2}}^{+}B_{\mu_{3}}^{+*}e^{i(-\delta_{\mu_{1}}-\delta_{\mu_{2}}+\delta_{\mu_{3}}+\delta_{\mu})t}
+2Bμ1+Bμ3Bμ2ei(δμ1δμ3+δμ2+δμ)t)=\displaystyle+2B_{\mu_{1}}^{+}B_{\mu_{3}}^{-}B_{\mu_{2}}^{-*}e^{i(-\delta_{\mu_{1}}-\delta_{\mu_{3}}+\delta_{\mu_{2}}+\delta_{\mu})t}\Big{)}= (35b)
γμ1μ2μ3δ^μ1+μ2μ3,μ(Bμ1+Bμ2+Bμ3+eiD22(μ2μ12μ22+μ32)t\displaystyle-\gamma\sum_{\mu_{1}\mu_{2}\mu_{3}}\widehat{\delta}_{\mu_{1}+\mu_{2}-\mu_{3},\mu}\Big{(}B_{\mu_{1}}^{+}B_{\mu_{2}}^{+}B_{\mu_{3}}^{+*}e^{\tfrac{iD_{2}}{2}(\mu^{2}-\mu_{1}^{2}-\mu_{2}^{2}+\mu_{3}^{2})t}
+2Bμ1+Bμ2Bμ3ei2D1(μ2μ3)teiD22(μ2μ12μ32+μ22)t).\displaystyle+2B_{\mu_{1}}^{+}B_{\mu_{2}}^{-*}B_{\mu_{3}}^{-}e^{i2D_{1}(\mu_{2}-\mu_{3})t}e^{\tfrac{iD_{2}}{2}(\mu^{2}-\mu_{1}^{2}-\mu_{3}^{2}+\mu_{2}^{2})t}\Big{)}. (35c)

The four-wave mixing momentum matching conditions are reflected in the Kronecker delta’s in front of the nonlinear terms in the second line of the above and directly follow from taking the integrals in θ\theta. Swapping of μ2\mu_{2} and μ3\mu_{3} inside the nonlinear cross-coupling is a critical step that a reader should pay attention to, see Eq. (35b). This operation equals the Kronecker delta’s, but it re-orders the amplitudes and respective frequency detunings in the second nonlinear term. After inserting explicit expressions for δμ\delta_{\mu}, see Eqs. (8), (9), and using the momentum matching condition,

μ1+μ2=μ3+μ,\mu_{1}+\mu_{2}=\mu_{3}+\mu, (36)

we find that D1D_{1} frequencies cancel out inside the nonlinear self-action terms, but remain in the cross-action ones providing μ2μ3\mu_{2}\neq\mu_{3}, see Eq. (35c). Thus if D1D_{1} oscillations are much faster than dynamics associated with the other time scales left in the equations, i.e., κ\kappa, RR and nonlinear frequency shifts, then the fast oscillating components can be disregarded [19, 41]. This leaves us only with μ2=μ3\mu_{2}=\mu_{3} components in the cross-action terms, so that

itBμ++i12κ(Bμ+δ^μ,0±eiδμt)+RBμ=\displaystyle i\partial_{t}B^{+}_{\mu}+i\tfrac{1}{2}\kappa\left(B^{+}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{\pm}e^{i\delta_{\mu}t}\right)+RB^{-*}_{\mu}=
γμ1μ2μ3δ^μ1+μ2μ3,μBμ1+Bμ2+Bμ3+eiD22(μ2μ12μ22+μ32)t2γBμ+μ2|Bμ2|2.\displaystyle-\gamma\sum_{\mu_{1}\mu_{2}\mu_{3}}\widehat{\delta}_{\mu_{1}+\mu_{2}-\mu_{3},\mu}B_{\mu_{1}}^{+}B_{\mu_{2}}^{+}B_{\mu_{3}}^{+*}e^{\tfrac{iD_{2}}{2}(\mu^{2}-\mu_{1}^{2}-\mu_{2}^{2}+\mu_{3}^{2})t}-2\gamma B_{\mu}^{+}\sum_{\mu_{2}}|B_{\mu_{2}}^{-}|^{2}. (37)

Nonlinear terms in Eqs. (37) are now grouped into the phase insensitive pure cross-Kerr term, that contains nonlinear shift of the CW resonance frequencies due to CCW wave, and into the term that mixes both phase sensitive and phase insensitive four-wave mixing CW-CW nonlinearities. The phase sensitive effects come only from the CW-CW interaction, because all the phase sensitive CW-CCW dynamics develops with the 2D12D_{1} frequencies and is washed out by the high repetition rates. This can be called the washout effect of high repetition rates on nonlinear frequency mixing of the counter-propagating waves in a ring resonator.

Using Aμ±A_{\mu}^{\pm} amplitudes and detunings δμ\delta^{\prime}_{\mu}, which are both D1D_{1} free, see Eqs. (14), allows to hide eiD2μ2t/2e^{iD_{2}\mu^{2}t/2} exponents in Eqs. (37). Adding the CCW equation, we have

itAμ+δμAμ++i12κ(Aμ+δ^μ,0±)+RAμ=\displaystyle i\partial_{t}A^{+}_{\mu}-\delta^{\prime}_{\mu}A^{+}_{\mu}+i\tfrac{1}{2}\kappa\left(A^{+}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{\pm}\right)+RA^{-}_{\mu}=
γμ1μ2μ3δ^μ1+μ2μ3,μAμ1+Aμ2+Aμ3+2γAμ+μ2|Aμ2|2,\displaystyle-\gamma\sum_{\mu_{1}\mu_{2}\mu_{3}}\widehat{\delta}_{\mu_{1}+\mu_{2}-\mu_{3},\mu}A_{\mu_{1}}^{+}A_{\mu_{2}}^{+}A_{\mu_{3}}^{+*}-2\gamma A_{\mu}^{+}\sum_{\mu_{2}}|A_{\mu_{2}}^{-}|^{2}, (38a)
itAμδμAμ+i12κ(Aμδ^μ,0±)+RAμ+=\displaystyle i\partial_{t}A^{-}_{\mu}-\delta^{\prime}_{\mu}A^{-}_{\mu}+i\tfrac{1}{2}\kappa\left(A^{-}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{\pm}\right)+R^{*}A^{+}_{\mu}=
γμ1μ2μ3δ^μ1+μ2μ3,μAμ1Aμ2Aμ32γAμμ2|Aμ2+|2.\displaystyle-\gamma\sum_{\mu_{1}\mu_{2}\mu_{3}}\widehat{\delta}_{\mu_{1}+\mu_{2}-\mu_{3},\mu}A_{\mu_{1}}^{-}A_{\mu_{2}}^{-}A_{\mu_{3}}^{-*}-2\gamma A_{\mu}^{-}\sum_{\mu_{2}}|A_{\mu_{2}}^{+}|^{2}. (38b)

The difference of the above nonlinear terms with the ones in the equations for Qμ±Q^{\pm}_{\mu}, see Eq. (34), that include un-averaged D1D_{1} oscillations, becomes more obvious, if the sums in Eqs. (38) are replaced with the integrals, see also Eq. (16a),

itAμ+δμAμ++i12κ(Aμ+δ^μ,0±)+RAμ=\displaystyle i\partial_{t}A^{+}_{\mu}-\delta^{\prime}_{\mu}A^{+}_{\mu}+i\tfrac{1}{2}\kappa\left(A^{+}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{\pm}\right)+RA^{-}_{\mu}=
γ02π|A+|2A+eiμθdθ2π2γAμ+02π|A|2dθ2π,\displaystyle-\gamma\int_{0}^{2\pi}|A_{+}|^{2}A_{+}e^{-i\mu\theta}\frac{d\theta}{2\pi}-2\gamma A_{\mu}^{+}\int_{0}^{2\pi}|A_{-}|^{2}\frac{d\theta}{2\pi}, (39a)
itAμδμAμ+i12κ(Aμδ^μ,0±)+RAμ+=\displaystyle i\partial_{t}A^{-}_{\mu}-\delta^{\prime}_{\mu}A^{-}_{\mu}+i\tfrac{1}{2}\kappa\left(A^{-}_{\mu}-\widehat{\delta}_{\mu,0}{\cal H}_{\pm}\right)+R^{*}A^{+}_{\mu}=
γ02π|A|2Aeiμθdθ2π2γAμ02π|A+|2dθ2π.\displaystyle-\gamma\int_{0}^{2\pi}|A_{-}|^{2}A_{-}e^{i\mu\theta}\frac{d\theta}{2\pi}-2\gamma A_{\mu}^{-}\int_{0}^{2\pi}|A_{+}|^{2}\frac{d\theta}{2\pi}. (39b)

The last terms in Eqs. (39) follow from the Parseval’s theorem. Thus Eqs. (37) include only effects of the second and higher order dispersions in both linear and nonlinear terms, that in microresonators are associated with the kHz to MHz time scales. Hence solving Eqs. (37) is expected to provide significant computational advantages over all other versions of the coupled mode equations.

5 Envelope models

Connection of the coupled mode equations to the wave dynamics becomes more intuitive, if one now derives the envelope, Lugiato-Lefever like, equations. First, we take the Qμ±Q_{\mu}^{\pm} model, see Eqs. (34), and multiply Eq. (34a) with eiμθe^{i\mu\theta} and (34b) with eiμθe^{-i\mu\theta}. We then sum up each of the equations in μ\mu and use Eqs. (12), (13) connecting the envelopes Q±Q_{\pm} and the reflected envelopes Q±(r)Q_{\pm}^{(r)} to their mode amplitudes. This procedure is free from approximations and it leads to a system of partial differential equations for Q±Q_{\pm} and Q±(r)Q_{\pm}^{(r)},

itQ+=δ0Q++(iD1θ12!D2θ2+i13!D3θ3+)Q+RQ(r)\displaystyle i\partial_{t}Q_{+}=\delta_{0}Q_{+}+\left(-iD_{1}\partial_{\theta}-\tfrac{1}{2!}D_{2}\partial_{\theta}^{2}+i\tfrac{1}{3!}D_{3}\partial_{\theta}^{3}+\dots\right)Q_{+}-RQ_{-}^{(r)}
i12κ(Q++)γ(|Q+|2+2|Q|2)Q+,\displaystyle-i\tfrac{1}{2}\kappa(Q_{+}-{\cal H}_{+})-\gamma(|Q_{+}|^{2}+2|Q_{-}|^{2})Q_{+}, (40a)
itQ=δ0Q+(+iD1θ12!D2θ2i13!D3θ3+)QRQ+(r)\displaystyle i\partial_{t}Q_{-}=\delta_{0}Q_{-}+\left(+iD_{1}\partial_{\theta}-\tfrac{1}{2!}D_{2}\partial_{\theta}^{2}-i\tfrac{1}{3!}D_{3}\partial_{\theta}^{3}+\dots\right)Q_{-}-R^{*}Q_{+}^{(r)}
i12κ(Q)γ(|Q|2+2|Q+|2)Q.\displaystyle-i\tfrac{1}{2}\kappa(Q_{-}-{\cal H}_{-})-\gamma(|Q_{-}|^{2}+2|Q_{+}|^{2})Q_{-}. (40b)

To form a closed system, the above pair of equations should be supplemented with two more equations for the Q±(r)Q_{\pm}^{(r)}, see Eqs. (13) defining θ\theta reflection.

Starting from the equations for Aμ±A_{\mu}^{\pm}, see Eqs. (39), we follow a modified procedure. Namely, we multiply both CW and CCW equations by the same exponent eiμθe^{i\mu\theta}, use the envelope definitions in Eqs. (16), observe that 02π|A|2Aeiμθ𝑑θ=2π0|A(r)|2A(r)eiμθ𝑑θ\int_{0}^{2\pi}|A_{-}|^{2}A_{-}e^{i\mu\theta}d\theta=\int^{0}_{-2\pi}|A_{-}^{(r)}|^{2}A_{-}^{(r)}e^{-i\mu\theta}d\theta and, due to periodicity, =02π|A(r)|2A(r)eiμθ𝑑θ=\int_{0}^{2\pi}|A_{-}^{(r)}|^{2}A_{-}^{(r)}e^{-i\mu\theta}d\theta, sum up in μ\mu, and derive the following envelope equations

itA+=δ0A++(12!D2θ2+i13!D3θ3+)A+RA(r)γ|A+|2A+\displaystyle i\partial_{t}A_{+}=\delta_{0}A_{+}+\left(-\tfrac{1}{2!}D_{2}\partial_{\theta}^{2}+i\tfrac{1}{3!}D_{3}\partial_{\theta}^{3}+\dots\right)A_{+}-RA_{-}^{(r)}-\gamma|A_{+}|^{2}A_{+}
i12κ(A++)2γA+02π|A(r)(θ)|2dθ2π,\displaystyle-i\tfrac{1}{2}\kappa(A_{+}-{\cal H}_{+})-2\gamma A_{+}\int_{0}^{2\pi}|A_{-}^{(r)}(\theta^{\prime})|^{2}\frac{d\theta^{\prime}}{2\pi}, (41a)
itA(r)=δ0A(r)+(12!D2θ2+i13!D3θ3+)A(r)RA+γ|A(r)|2A(r)\displaystyle i\partial_{t}A_{-}^{(r)}=\delta_{0}A_{-}^{(r)}+\left(-\tfrac{1}{2!}D_{2}\partial_{\theta}^{2}+i\tfrac{1}{3!}D_{3}\partial_{\theta}^{3}+\dots\right)A_{-}^{(r)}-R^{*}A_{+}-\gamma|A_{-}^{(r)}|^{2}A_{-}^{(r)}
i12κ(A(r))2γA(r)02π|A+(θ)|2dθ2π.\displaystyle-i\tfrac{1}{2}\kappa(A_{-}^{(r)}-{\cal H}_{-})-2\gamma A_{-}^{(r)}\int_{0}^{2\pi}|A_{+}(\theta^{\prime})|^{2}\frac{d\theta^{\prime}}{2\pi}. (41b)

The above equations do not only exclude the D1D_{1} dynamics, but also form a closed system of two equations for the CW A+A_{+} envelope and for the reflected CCW A(r)A_{-}^{(r)} envelope, see Eqs. (16). They can also be supplemented with equations for A+(r)A_{+}^{(r)}, AA_{-}, but this time those are left as an independent pair. Again numerical modelling of Eqs. (41) is expected to have great advantages relative to working with Eqs. (40). Similar to ours procedure to remove the D1D_{1} linked time scales has been developed for the Kerr Fabry-Perot cavities supporting a single family of standing waves and hence yielding a one-component Lugiato-Lefever model [41]. The respective ring geometry model in [19] mixes all four envelope functions, i.e., A±A_{\pm}, A±(r)A_{\pm}^{(r)}, and is limited by the second order dispersion.

Eqs. (40) (not Eqs. (41)) could in fact, be written without a rigorous derivation, by simply relying on common knowledge, let aside reflected envelopes in the backscattering terms. These equations include traditional cross-phase modulation, and also repetition rates terms and other odd order dispersion terms with the opposite signs. Contrary, Eqs. (41) have no repetition rate terms, i.e., D1D_{1}-terms, and the remaining odd dispersions, i.e., D3D_{3}, D5D_{5}, etc., come with the same signs. Simultaneously, phase sensitive nonlinear wave mixing effects induced by CW-CCW interaction have been washed out. The only nonlinear cross-interaction left comes from the integrated power, which merely shifts the detuning parameters. Thus, in the absence of backscattering a nonlinear bi-directional resonator operates as a uni-directional one, but with the detuning parameter altered by the total power of the counter-propagating wave.

6 Summary

We have derived coupled mode equations describing nonlinear wave mixing processes in Kerr microresonator with counter-propagating waves. Features of the first two coupled mode formulations given by Eqs. (30) and Eqs. (34) are that they fully account for the repetition rate effects and that nonlinear terms are taken in the real space, and can be evaluated via Fourier transforms, see also [42]. We then proceeded to present simplified multi-mode equations that neglect the repetition rate dynamics driving the phase sensitive terms responsible for nonlinear interaction between the counter-propagating fields (washout effect, section 4), and again deal with the nonlinearity in the real space, see Eqs. (39).

Finally, we demonstrated that coupled mode equations (34) and Eqs. (39) are equivalent to two different, Lugiato-Lefever-like, envelope models. The one that involves the repetition rate dynamics, see Eqs. (40), links two usual envelopes for the CW and CCW fields, with two of their space reflections. While the one with the repetition rate averaged out, see Eqs. (41), makes a closed system already for two envelopes, A±A_{\pm}, one of which is reflected. We note, that Q±Q_{\pm} can be used directly to reconstruct total electric field, see Eq. (10c), while A±A_{\pm} can not, but their respective mode amplitudes can, see Eqs. (15), (16a).

We have taken care to reveal all mathematical transformations, that allow a reader to verify our derivation steps and apply modifications if required. Opportunities for future theoretical and numerical studies offered by the models presented here are numerous, as well as their potential to guide and interpret experimental work.

Funding

EU Horizon 2020 Framework Programme (812818, MICROCOMB); UK EPSRC (EP/R008159); Russian Science Foundation (17-12-01413).

Acknowledgement

Discussions with authors of [19] and with greatly missed M.L. Gorodetsky are gratefully acknowledged.

Disclosures

The author declares no conflicts of interest.

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