1 Introduction
The first theoretical work on hydroacoustic waves was done by Longuet-Higgins (Reference Longuet-Higgins1950), who argued that the water can be treated as incompressible only when the time taken for the disturbance to propagate to the bottom is small compared to the period of waves. Considering the compressibility of water, Longuet-Higgins (Reference Longuet-Higgins1950) found that hydroacoustic waves, which affect the whole water column, can be generated by the nonlinear interaction of two progressive gravity waves with the same wavelength travelling in opposite directions. Longuet-Higgins (Reference Longuet-Higgins1950) also mentioned that the resonant triad interactions of acoustic–gravity waves exist at the special water depths
$h\approx (n+0.5)\unicode[STIX]{x03C0}c/\unicode[STIX]{x1D714}_{3}$
, where
$n=0,1,2,\ldots \,$
,
$h$
is the water depth,
$c$
is the speed of sound in the water, which is of the order of
$1500~\text{m}~\text{s}^{-1}$
and
$\unicode[STIX]{x1D714}_{3}$
is the frequency of the resulting hydroacoustic wave. However, Longuet-Higgins (Reference Longuet-Higgins1950) did not obtain solutions of resonant acoustic–gravity waves. Later, Kibblewhite & Wu (Reference Kibblewhite and Wu1991) argued that the hydroacoustic wave can be generated by two opposite gravity waves with slightly different wavenumbers. The interaction between two primary gravity waves and the resulting hydroacoustic wave can be described as
where
$\boldsymbol{k}_{1}$
,
$\boldsymbol{k}_{2}$
and
$\unicode[STIX]{x1D714}_{1}$
,
$\unicode[STIX]{x1D714}_{2}$
are the wavenumbers and wave frequencies of two primary gravity waves,
$\boldsymbol{k}_{3}$
is the horizontal component of the wavenumber of the hydroacoustic wave. For the Longuet-Higgins case,
$|\boldsymbol{k}_{3}|$
is equal to
$0$
. When
$|\boldsymbol{k}_{3}|\geqslant \unicode[STIX]{x1D714}_{3}/c$
, the hydroacoustic response degenerates into an inhomogeneous wave decaying with increasing water depth. In this paper, we consider the non-resonance and resonance cases of Longuet-Higgins with
$|\boldsymbol{k}_{3}|=0$
and one more general resonance case with
$0<|\boldsymbol{k}_{3}|<\unicode[STIX]{x1D714}_{3}/c$
. The interactions of two gravity waves travelling in opposite directions were investigated by many researchers, such as Kibblewhite & Ewans (Reference Kibblewhite and Ewans1985), Webb (Reference Webb1992, Reference Webb1998), Bowen et al. (Reference Bowen, Richard, Mancini, Fessatidis and Crooker2003), Naugolnikh & Rybak (Reference Naugolnikh and Rybak2003), Farrell & Munk (Reference Farrell and Munk2010), Ardhuin & Herbers (Reference Ardhuin and Herbers2013), Ardhuin et al. (Reference Ardhuin, Lavanant, Obrebski, Marie, Royer, D’Eu, Howe, Lukas and Aucan2013). But none of them focussed on the exact resonance of waves.
Recently, considering the resonance of two opposite gravity waves and the resulting hydroacoustic wave, Kadri & Stiassnie (Reference Kadri and Stiassnie2013) found that the condition for the exactly resonating triads is
where
$g$
is the gravitational acceleration,
$\unicode[STIX]{x1D706}_{3}$
is a parameter associated with the vertical wavenumber of the hydroacoustic wave. They found that when the resonance condition is satisfied, the amplitude equations of the resonant acoustic–gravity triads are the same as those of resonant gravity triads (Phillips Reference Phillips1960; Benney Reference Benney1962; Longuet-Higgins Reference Longuet-Higgins1962; Bretherton Reference Bretherton1964). This conclusion was confirmed by Kadri & Akylas (Reference Kadri and Akylas2016), who obtained resonant acoustic–gravity waves with periodically changing wave spectrum and found that the interaction time scale is longer than that of a standard resonant triad. Note that, without considering the compressibility of the water, three-wave resonance does not occur for gravity waves (Dyachenko & Zakharov Reference Dyachenko and Zakharov1994). Kadri (Reference Kadri2015) followed Longuet-Higgins (Reference Longuet-Higgins1950) to generalize the resonance condition of the acoustic–gravity waves and found that the resonances given by Longuet-Higgins (Reference Longuet-Higgins1950) are just particular cases. Kadri (Reference Kadri2015) also got the solution of the Longuet-Higgins resonance case, which is similar to that obtained by Kadri & Stiassnie (Reference Kadri and Stiassnie2013). However, to the best of our knowledge, the steady-state resonant acoustic–gravity waves with time-independent wave spectrum have never been obtained before in water of uniform depth.
On the other hand, the studies of two progressive gravity waves in opposite directions focused on the pressure field of the water, especially on the bottom. Even without considering the compressibility of the water, the interaction can produce a second-order pressure term that does not attenuate with depth. In particular, Renzi & Dias (Reference Renzi and Dias2014) mentioned that the compressibility is not the main driving mechanism. This conclusion was confirmed by Pellet et al. (Reference Pellet, Christodoulides, Donne, Bean and Dias2017) who obtained a second-order pressure field generated by two opposite travelling gravity waves, which is independent of water depth and periodic in time with twice the frequency of the primary gravity waves. Besides, considering the compressibility of the water, Longuet-Higgins (Reference Longuet-Higgins1950) and Kadri & Stiassnie (Reference Kadri and Stiassnie2013) obtained the solution of acoustic–gravity waves in the case of non-resonance. Kadri & Stiassnie (Reference Kadri and Stiassnie2013) and Kadri & Akylas (Reference Kadri and Akylas2016) got the solution of exact resonance acoustic–gravity waves with periodic wave spectrum. So, the pressure on the bottom of the water, which is dependent of water depth and time, can be obtained directly. In addition, the hydroacoustic waves produced by a moving bottom were studied by Yamamoto (Reference Yamamoto1982), Stiassnie (Reference Stiassnie2010), Oliveira & Kadri (Reference Oliveira and Kadri2016) and Kadri (Reference Kadri2017). Eyov et al. (Reference Eyov, Klar, Kadri and Stiassnie2013) and Kadri & Stiassnie (Reference Kadri and Stiassnie2012) studied effects of different hydroacoustic modes on two types of bottoms (an elastic bottom and a bottom with a step) in a compressible ocean. Note that these studies related to the motion of the bottom did not consider the exact resonance.
In this paper, we first consider the non-resonance conditions of acoustic–gravity waves, the solutions of which have been obtained previously, for example by Longuet-Higgins (Reference Longuet-Higgins1950) and Kadri & Stiassnie (Reference Kadri and Stiassnie2013). But, more importantly, we focus on the steady-state resonant triad interactions of acoustic–gravity waves with time-independent wave spectrum, which have never been obtained before. We use the resonance condition
where
$\unicode[STIX]{x1D6FE}=g/2c^{2}$
, which is similar to (1.2) given by Kadri & Stiassnie (Reference Kadri and Stiassnie2013), who found that all amplitudes of the wave components vary periodically, i.e. with periodic wave spectrum, when the resonance condition is exactly satisfied. Are there any steady-state resonant acoustic–gravity waves whose spectrum is independent of time? In this steady-state system, there is no exchange of wave energy between different wave components, i.e. all amplitudes of wave components are independent of time. For the normal gravity waves, the answer is yes. Liao (Reference Liao2011b
) found steady-state resonant gravity waves in deep water by means of the homotopy analysis method (HAM) (Liao Reference Liao1992, Reference Liao2003, Reference Liao2010, Reference Liao2011a
; Van Gorder & Vajravelu Reference Van Gorder and Vajravelu2008; Vajravelu & Van Gorder Reference Vajravelu and Van Gorder2012; Zhong & Liao Reference Zhong and Liao2017, Reference Zhong and Liao2018a
,Reference Zhong and Liao
b
). Then it was found that the steady-state resonant gravity waves exist extensively in both infinite and finite water depth by Xu et al. (Reference Xu, Lin, Liao and Stiassnie2012) and Liu & Liao (Reference Liu and Liao2014), which were even confirmed experimentally by Liu et al. (Reference Liu, Xu, Li, Peng, Alsaedi and Liao2015). In addition, Liao, Xu & Stiassnie (Reference Liao, Xu and Stiassnie2016) successfully applied the HAM to obtain the steady-state nearly resonant gravity waves in deep water, and Liu, Xu & Liao (Reference Liu, Xu and Liao2018) found finite amplitude steady-state waves with multiple near-resonant interactions. The purpose of this paper is to confirm the existence of the steady-state resonant acoustic–gravity waves.
It has been commonly accepted that the generation of hydroacoustic waves in the ocean is due to the nonlinear interaction of two gravity waves that travel in opposite directions. If we ignore the compressibility of water, two gravity waves travelling in opposite directions with the same amplitude and wavelength create a standing wave with an infinite number of ‘singularities’ (i.e. zero denominators) when one uses classical methods, like perturbation methods. As mentioned by Dias & Bridges (Reference Dias and Bridges2006), most studies of standing waves are based on semi-analytical methods and numerical methods because of the inherent analytical difficulties. So, the first obstacle of acoustic–gravity waves in deep water is how to handle the small denominators which are similar to the ‘singularities’ in the problem of standing waves, which is a big challenge in the framework of perturbation methods, as mentioned by Madsen & Fuhrman (Reference Madsen and Fuhrman2012). Besides, when the exact resonance condition is satisfied, one more ‘singularity’ corresponding to the hydroacoustic wave component must be considered.
In this paper, the acoustic–gravity wave problem is solved by means of the homotopy analysis method (HAM), an analytic technique for nonlinear problems. Using the HAM, the infinite number of small denominators in the acoustic–gravity waves problem can be avoided conveniently once and for all by means of choosing a proper auxiliary linear operator, as described later in this paper. Besides, different from perturbation methods, the HAM has nothing to do with any small/large physical parameters. More importantly, it provides us a simple way to guarantee the convergence of the solution.
The structure of the paper is presented below. The mathematical formulae are described in § 2. The solutions of non-resonant acoustic–gravity waves are given in § 3.1. The steady-state resonant triad interactions of acoustic–gravity waves are studied in detail in § 3.2. Conclusions and discussions are presented in § 4.
2 Mathematical formulae
2.1 Governing equations
Let us consider the nonlinear interactions of two progressive gravity waves and one hydroacoustic wave in water of uniform depth. A Cartesian coordinate system is adopted with the
$x$
-axis and the
$y$
-axis located on the mean water plane and the
$z$
-axis pointing vertically upwards. Longuet-Higgins (Reference Longuet-Higgins1950) derived the water wave equations together with their boundary conditions in a heavy compressible fluid, in the absence of viscosity and surface tension. The governing equation for the velocity potential has linear, quadratic and cubic terms. Kadri & Stiassnie (Reference Kadri and Stiassnie2013) used the same governing equation as Longuet-Higgins, without the cubic term. Here we use the same equation as Longuet-Higgins without the nonlinear terms. The justification is given in the paper by Longuet-Higgins (Reference Longuet-Higgins1950) itself. Indeed, Longuet-Higgins solved for the velocity potential by using a method of successive approximations. At second order, the velocity potential given by his equation (159) has five types of terms. Longuet-Higgins writes below his equation (169) that the first two terms in equation (159) are negligible compared with the fourth, and then writes a simplified expression for the second-order velocity potential (see his equation (172)). We checked that this is equivalent to neglecting the quadratic terms in the governing equation. Therefore, in our paper, we use the governing equation
subject to the boundary conditions:
where
is a linear operator with
$\boldsymbol{i}$
,
$\boldsymbol{j}$
,
$\boldsymbol{k}$
denoting the unit vector in the
$x$
,
$y$
,
$z$
direction,
$\unicode[STIX]{x1D711}$
is the velocity potential,
$\unicode[STIX]{x1D702}$
is the wave elevation,
$t$
denotes the time,
$h$
is the water depth,
$c$
is the speed of sound in water,
$g$
is the acceleration due to gravity, respectively. Note that the governing equation (2.1) was also used by Kadri & Stiassnie (Reference Kadri and Stiassnie2013). The pressure field of the water can be obtained by Bernoulli’s equation
$$\begin{eqnarray}\displaystyle p & = & \displaystyle p_{a}-\unicode[STIX]{x1D70C}gz-\unicode[STIX]{x1D70C}\left(\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D711}}{\unicode[STIX]{x2202}t}+\frac{1}{2}\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D711}^{2}}{\unicode[STIX]{x2202}x}+\frac{1}{2}\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D711}^{2}}{\unicode[STIX]{x2202}y}+\frac{1}{2}\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D711}^{2}}{\unicode[STIX]{x2202}z}\right)\nonumber\\ \displaystyle & = & \displaystyle p_{a}-\unicode[STIX]{x1D70C}gz+p_{d},\quad -h\leqslant z\leqslant \unicode[STIX]{x1D702}(x,y,t),~(x,y)\in \mathbb{R}^{2},\end{eqnarray}$$
where
$p_{a}-\unicode[STIX]{x1D70C}gz$
is the hydrostatic pressure and
$p_{d}$
is the dynamic pressure,
$\unicode[STIX]{x1D70C}=1025~\text{kg}~\text{m}^{-3}$
.
The linear solutions of the governing equations (2.1)–(2.4) given by Dalrymple & Rogers (Reference Dalrymple and Rogers2006) read
where
$\unicode[STIX]{x1D6FE}=g/2c^{2}$
,
$k^{2}=\unicode[STIX]{x1D706}^{2}+\unicode[STIX]{x1D714}^{2}/c^{2}-\unicode[STIX]{x1D6FE}^{2}$
and the dispersion relation is given by
where
$\tilde{A}$
denotes the wave amplitude,
$\boldsymbol{k}$
is the wavenumber,
$k=|\boldsymbol{k}|$
,
$\unicode[STIX]{x1D714}$
is the wave frequency and
$\boldsymbol{r}=x\boldsymbol{i}+y\boldsymbol{j}$
.
Let
$\unicode[STIX]{x1D70E}_{i}$
denote the actual wave frequency of two primary gravity waves. Due to the weakly nonlinearity on the free surface of the water, the actual wave frequency
$\unicode[STIX]{x1D70E}_{i}$
is slightly different from the linear frequency
$\unicode[STIX]{x1D714}_{i}$
. Write
where the value of
$\unicode[STIX]{x1D716}_{i}$
is slightly different from 1. Then, we define the variables
For steady-state wave systems, all wave amplitudes
$a_{i}$
, wavenumbers
$\boldsymbol{k}_{i}$
and actual wave frequencies
$\unicode[STIX]{x1D70E}_{i}$
, where
$i=1,2$
, are time independent. Using the new variables
$\unicode[STIX]{x1D709}_{i}$
, the original initial/boundary-value problem governed by (2.1)–(2.4) can be transformed into a boundary-value one. In the new coordinate system (
$\unicode[STIX]{x1D709}_{1}$
,
$\unicode[STIX]{x1D709}_{2}$
,
$z$
), the governing equation (2.1) becomes
$$\begin{eqnarray}\displaystyle & & \displaystyle \mathop{\sum }_{i=1}^{2}\mathop{\sum }_{j=1}^{2}\unicode[STIX]{x1D70E}_{i}\unicode[STIX]{x1D70E}_{j}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D711}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{i}\unicode[STIX]{x1D709}_{j}}-c^{2}\mathop{\sum }_{i=1}^{2}\mathop{\sum }_{j=1}^{2}\boldsymbol{k}_{i}\boldsymbol{\cdot }\boldsymbol{k}_{j}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D711}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{i}\unicode[STIX]{x1D709}_{j}}\nonumber\\ \displaystyle & & \displaystyle \qquad -\,c^{2}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D711}}{\unicode[STIX]{x2202}z^{2}}+g\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D711}}{\unicode[STIX]{x2202}z}=0,\quad -h\leqslant z\leqslant \unicode[STIX]{x1D702}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2}),\end{eqnarray}$$
subject to the two boundary conditions on the unknown free surface
$z=\unicode[STIX]{x1D702}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2})$
,
$$\begin{eqnarray}\displaystyle {\mathcal{N}}_{1}[\unicode[STIX]{x1D711},\unicode[STIX]{x1D70E}_{1},\unicode[STIX]{x1D70E}_{2}] & = & \displaystyle \mathop{\sum }_{i=1}^{2}\mathop{\sum }_{j=1}^{2}\unicode[STIX]{x1D70E}_{i}\unicode[STIX]{x1D70E}_{j}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D711}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{i}\unicode[STIX]{x1D709}_{j}}+g\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D711}}{\unicode[STIX]{x2202}z}-2\mathop{\sum }_{i=1}^{2}\unicode[STIX]{x1D70E}_{i}\frac{\unicode[STIX]{x2202}f}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{i}}\nonumber\\ \displaystyle & & \displaystyle +\,\mathop{\sum }_{i=1}^{2}\mathop{\sum }_{j=1}^{2}\boldsymbol{k}_{i}\boldsymbol{\cdot }\boldsymbol{k}_{j}\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D711}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{i}}\frac{\unicode[STIX]{x2202}f}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{j}}+\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D711}}{\unicode[STIX]{x2202}z}\frac{\unicode[STIX]{x2202}f}{\unicode[STIX]{x2202}z}=0,\quad \text{on}~z=\unicode[STIX]{x1D702}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2}),\end{eqnarray}$$
and one impermeable condition at the bottom,
where
and
${\mathcal{N}}_{1}$
and
${\mathcal{N}}_{2}$
are two nonlinear operators defined above.
For a steady-state wave system, there is no exchange of wave energy between different wave components, i.e. all physical quantities related to the wave systems are constant. Thus, the steady-state wave elevation
$\unicode[STIX]{x1D702}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2})$
can be expressed by
where
$a_{m_{1},m_{2}}$
is a constant to be determined later. Similarly, according to the governing equations (2.11) and the bottom boundary condition (2.14), the velocity potential
$\unicode[STIX]{x1D711}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2},z)$
should be in the form
with the definition
$$\begin{eqnarray}\displaystyle \unicode[STIX]{x1D6F9}_{m_{1},m_{2}}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2},z) & = & \displaystyle \frac{\unicode[STIX]{x1D706}_{m_{1},m_{2}}\cosh [\unicode[STIX]{x1D706}_{m_{1},m_{2}}(h+z)]-\unicode[STIX]{x1D6FE}\sinh [\unicode[STIX]{x1D706}_{m_{1},m_{2}}(h+z)]}{\unicode[STIX]{x1D706}_{m_{1},m_{2}}\cosh (\unicode[STIX]{x1D706}_{m_{1},m_{2}}h)-\unicode[STIX]{x1D6FE}\sinh (\unicode[STIX]{x1D706}_{m_{1},m_{2}}h)}\nonumber\\ \displaystyle & & \displaystyle \times \,\text{e}^{\unicode[STIX]{x1D6FE}z}\sin (m_{1}\unicode[STIX]{x1D709}_{1}+m_{2}\unicode[STIX]{x1D709}_{2}),\end{eqnarray}$$
where
$b_{m_{1},m_{2}}$
is a constant to be determined later. It should be emphasized that (2.17) automatically satisfies the bottom boundary condition (2.14). It also satisfies the governing equation (2.11), provided that
$k_{m_{1},m_{2}}^{2}=\unicode[STIX]{x1D706}_{m_{1},m_{2}}^{2}+\unicode[STIX]{x1D70E}_{m_{1},m_{2}}^{2}/c^{2}-\unicode[STIX]{x1D6FE}^{2}$
, where
$k_{m_{1},m_{2}}=|m_{1}\boldsymbol{k}_{1}+m_{2}\boldsymbol{k}_{2}|$
,
$\unicode[STIX]{x1D70E}_{m_{1},m_{2}}=m_{1}\unicode[STIX]{x1D70E}_{1}+m_{2}\unicode[STIX]{x1D70E}_{2}$
. Because the nonlinearities in the paper of all examples are weak, we choose
$\unicode[STIX]{x1D706}_{m_{1},m_{2}}^{2}\approx k_{m_{1},m_{2}}^{2}-\unicode[STIX]{x1D714}_{m_{1},m_{2}}^{2}/c^{2}+\unicode[STIX]{x1D6FE}^{2}$
, where
$\unicode[STIX]{x1D714}_{m_{1},m_{2}}=m_{1}\unicode[STIX]{x1D714}_{1}+m_{2}\unicode[STIX]{x1D714}_{2}$
. The corresponding parameter
$\unicode[STIX]{x1D706}$
in (2.7) is
$\unicode[STIX]{x1D706}_{m_{1},m_{2}}$
. Thus, the unknown coefficients
$a_{m_{1},m_{2}}$
and
$b_{m_{1},m_{2}}$
are determined by the two fully nonlinear boundary conditions (2.12) and (2.13). Once the velocity potential is obtained, we can directly obtain the pressure field of the water from (2.6). Here, we focus on the dynamic pressure
$p_{d}$
in the whole water field. From (2.17), the dynamic pressure
$p_{d}$
is in the form as
Based on (1.1a–c
), we consider the case
$k_{1}=|\boldsymbol{k}_{1}|$
slightly different from
$k_{2}=|\boldsymbol{k}_{2}|$
. When
$m_{1}\neq m_{2}$
, the value of
$(\unicode[STIX]{x1D714}_{m_{1},m_{2}}^{2}/c^{2}-\unicode[STIX]{x1D6FE}^{2})$
is very small (the frequency
$\unicode[STIX]{x1D714}_{i}$
of the primary waves considered in this paper is around
$1~\text{s}^{-1}$
) compared to
$k_{m_{1},m_{2}}$
, so that
$\unicode[STIX]{x1D706}_{m_{1},m_{2}}\approx k_{m_{1},m_{2}}$
, which represents gravity waves in water of uniform depth. When
$m_{1}=m_{2}$
,
$k_{m_{1},m_{2}}$
is very small.
$\unicode[STIX]{x1D706}_{m_{1},m_{2}}$
is an imaginary number, which represents the hydroacoustic wave. Further, when
$m_{1}=m_{2}>1$
, the corresponding hydroacoustic wave is generated by two high-order gravity waves. In this paper, we focus on the resulting hydroacoustic wave, when
$m_{1}=m_{2}=1$
.
2.2 Solution procedure
In 2011, Liao (Reference Liao2011b ) successfully applied the HAM to obtain the solutions of steady-state resonant gravity waves governed by the fully nonlinear wave equations. Thereafter, Xu et al. (Reference Xu, Lin, Liao and Stiassnie2012), Liu & Liao (Reference Liu and Liao2014), Liao et al. (Reference Liao, Xu and Stiassnie2016) and Liu et al. (Reference Liu, Xu and Liao2018) made further contributions in the study of steady-state resonant gravity waves. Detailed mathematical derivations can be found in these articles. So, for the sake of simplicity, we just give some important formulae here.
Let
$q\in [0,1]$
denote an embedding parameter. In the framework of HAM, we first construct a family of solutions
$\unicode[STIX]{x1D6F7}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2},z;q)$
,
$\unicode[STIX]{x1D701}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2};q)$
,
$\unicode[STIX]{x1D6EC}_{1}(q)$
and
$\unicode[STIX]{x1D6EC}_{2}(q)$
in
$q\in [0,1]$
by means of the so-called zeroth-order deformation equations,
$$\begin{eqnarray}\displaystyle & & \displaystyle \mathop{\sum }_{i=1}^{2}\mathop{\sum }_{j=1}^{2}\unicode[STIX]{x1D70E}_{i}\unicode[STIX]{x1D70E}_{j}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D6F7}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{i}\unicode[STIX]{x1D709}_{j}}-c^{2}\mathop{\sum }_{i=1}^{2}\mathop{\sum }_{j=1}^{2}\boldsymbol{k}_{i}\boldsymbol{\cdot }\boldsymbol{k}_{j}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D6F7}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{i}\unicode[STIX]{x1D709}_{j}}\nonumber\\ \displaystyle & & \displaystyle \qquad -\,c^{2}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D6F7}}{\unicode[STIX]{x2202}z^{2}}+g\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D6F7}}{\unicode[STIX]{x2202}z}=0,\quad -h\leqslant z\leqslant \unicode[STIX]{x1D701}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2};q),\end{eqnarray}$$
subject to the two boundary conditions on the unknown wave elevation
$z=\unicode[STIX]{x1D702}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2};q)$
and the impermeable condition at the bottom
where
${\mathcal{N}}_{1}$
and
${\mathcal{N}}_{2}$
are the two nonlinear operators defined by (2.12) and (2.13),
${\mathcal{L}}^{\ast }$
is an auxiliary linear operator and
$\unicode[STIX]{x1D711}_{0}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2},z)$
is an initial guess of
$\unicode[STIX]{x1D711}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2},z)$
,
$c_{0}\neq 0$
is the so-called ‘convergence-control parameter’ without physical meaning, respectively. Here,
$\unicode[STIX]{x1D6F7}$
,
$\unicode[STIX]{x1D701}$
,
$\unicode[STIX]{x1D6EC}_{1}$
,
$\unicode[STIX]{x1D6EC}_{2}$
correspond to the unknown
$\unicode[STIX]{x1D711}$
,
$\unicode[STIX]{x1D702}$
,
$\unicode[STIX]{x1D70E}_{1}$
,
$\unicode[STIX]{x1D70E}_{2}$
, respectively. It should be emphasized that we have great freedom to choose the auxiliary linear operator. Obviously, when
$q=0$
,
When
$q=1$
, equations (2.20)–(2.23) are equivalent to the original equations (2.11)–(2.14), respectively, therefore we have
Thus, as
$q$
increases from 0 to 1,
$\unicode[STIX]{x1D6F7}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2},z;q)$
deforms continuously from the initial guess
$\unicode[STIX]{x1D711}_{0}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2},z)$
to the unknown potential function
$\unicode[STIX]{x1D711}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2},z)$
, so does
$\unicode[STIX]{x1D701}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2};q)$
from
$0$
to the unknown wave profile
$\unicode[STIX]{x1D702}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2})$
,
$\unicode[STIX]{x1D6EC}_{1}(q),\unicode[STIX]{x1D6EC}_{2}(q)$
from the initial guesses
$\unicode[STIX]{x1D70E}_{1,0},\unicode[STIX]{x1D70E}_{2,0}$
to the unknown frequencies
$\unicode[STIX]{x1D70E}_{1},\unicode[STIX]{x1D70E}_{2}$
, respectively.
Assuming that the convergence-control parameter
$c_{0}$
is properly chosen so that the Maclaurin series of
$\unicode[STIX]{x1D6F7}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2},z;q)$
,
$\unicode[STIX]{x1D701}(\unicode[STIX]{x1D709}_{1},\unicode[STIX]{x1D709}_{2};q)$
,
$\unicode[STIX]{x1D6EC}_{1}(q)$
and
$\unicode[STIX]{x1D6EC}_{2}(q)$
with respect to the embedding parameter
$q$
, i.e.
exist and converge at
$q=1$
, we have the so-called homotopy-series solution
respectively.
Substituting the Maclaurin series (2.26) into the zeroth-order deformation equations (2.20)–(2.23) and then equating the like powers of
$q$
, we obtain the so-called high-order deformation equations
$$\begin{eqnarray}\displaystyle & & \displaystyle \mathop{\sum }_{i=1}^{2}\mathop{\sum }_{j=1}^{2}\unicode[STIX]{x1D70E}_{i}\unicode[STIX]{x1D70E}_{j}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D711}_{m}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{i}\unicode[STIX]{x1D709}_{j}}-c^{2}\mathop{\sum }_{i=1}^{2}\mathop{\sum }_{j=1}^{2}\boldsymbol{k}_{i}\boldsymbol{\cdot }\boldsymbol{k}_{j}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D711}_{m}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D709}_{i}\unicode[STIX]{x1D709}_{j}}\nonumber\\ \displaystyle & & \displaystyle \qquad -\,c^{2}\frac{\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D711}_{m}}{\unicode[STIX]{x2202}z^{2}}+g\frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D711}_{m}}{\unicode[STIX]{x2202}z}=0,\quad -h\leqslant z\leqslant 0,\end{eqnarray}$$
subject to the linear boundary condition
and the bottom condition
together with
where
$\unicode[STIX]{x1D712}_{1}=0$
and
$\unicode[STIX]{x1D712}_{m}=1$
for
$m>1$
.
$\bar{S}_{m}$
and
$S_{m}$
are dependent upon the chosen auxiliary linear operator and thus will be given later. The definitions of
$\unicode[STIX]{x1D6E5}_{m-1}^{\unicode[STIX]{x1D711}}$
and
$\unicode[STIX]{x1D6E5}_{m-1}^{\unicode[STIX]{x1D702}}$
are given in the Appendix. Note that all of the
$\unicode[STIX]{x1D6E5}_{m-1}^{\unicode[STIX]{x1D711}}$
,
$\unicode[STIX]{x1D6E5}_{m-1}^{\unicode[STIX]{x1D702}}$
,
$\bar{S}_{m}$
and
$S_{m}$
on the right-hand side of (2.29) and (2.31) are determined by the known previous approximations
$\unicode[STIX]{x1D702}_{j}$
and
$\unicode[STIX]{x1D711}_{j}~(j=0,1,2,\ldots ,m-1)$
, and thus can be regarded as known terms.
2.3 Small denominators of the acoustic–gravity waves
Let
${\mathcal{L}}$
denote a differential operator corresponding to the linear parts of (2.12), i.e.
which has the property
where
Therefore, its inverse operator
${\mathcal{L}}^{-1}$
is given by
Considering the gravity wave components (
$m_{1}\neq m_{2}$
),
$\tilde{\unicode[STIX]{x1D706}}_{m_{1},m_{2}}\approx g|m_{1}\boldsymbol{k}_{1}+m_{2}\boldsymbol{k}_{2}|-(m_{1}\unicode[STIX]{x1D714}_{1}+m_{2}\unicode[STIX]{x1D714}_{2})^{2}$
. And based on (1.1), we have
$k_{1}\approx k_{2}=k$
and
$\unicode[STIX]{x1D714}_{1}\approx \unicode[STIX]{x1D714}_{2}=\sqrt{gk}$
. For gravity wave components, when
$\tilde{\unicode[STIX]{x1D706}}_{m_{1},m_{2}}\approx 0$
, we have
The above equation has an infinite number of integer solutions, as shown in table 1, corresponding to an infinite number of small denominators. Thus, it is very difficult to obtain the steady-state acoustic–gravity waves by traditional methods such as perturbation methods. Considering the hydroacoustic wave components (
$m_{1}=m_{2}$
), when the resonance condition (1.3) is satisfied, one more zero denominator
$\tilde{\unicode[STIX]{x1D706}}_{1,1}=0$
must be considered.
2.4 Choice of auxiliary linear operator
There exists an infinite number of small denominators even in the case of non-resonance. In the framework of perturbation techniques, it is rather difficult to handle such an infinite number of small denominators. However, different from perturbation methods, HAM provides us great freedom to choose the auxiliary linear operator, so that we can choose an auxiliary linear operator that is different from (2.32). Such kind of freedom of the HAM allows us to choose an appropriate auxiliary linear operator to avoid an infinite number of small denominators conveniently, as mentioned below.
The values of
$(m_{1},m_{2})$
corresponding to
$\tilde{\unicode[STIX]{x1D706}}_{m_{1},m_{2}}\approx 0$
.

Using the freedom of the HAM mentioned above, we choose such an auxiliary linear operator
where
which has the property
where
So its inverse operator
${\mathcal{L}}^{\ast -1}$
reads
When considering the gravity wave components (
$m_{1}\neq m_{2}$
) and
$\tilde{\unicode[STIX]{x1D706}}_{m_{1},m_{2}}^{\ast }\approx 0$
, we have
which does not have an infinite number of integer solutions. When
$m_{1}=1,m_{2}=0$
and
$m_{1}=0,m_{2}=1$
, the auxiliary linear operators
${\mathcal{L}}^{\ast }$
and
${\mathcal{L}}$
in (2.32) are the same,
$\tilde{\unicode[STIX]{x1D706}}_{1,0}^{\ast }=\tilde{\unicode[STIX]{x1D706}}_{0,1}^{\ast }=0$
. For the rest, we choose
$\unicode[STIX]{x1D707}=\unicode[STIX]{x03C0}/3$
as an irrational number. When
$m_{1}=m_{2}$
,
$\unicode[STIX]{x1D707}|m_{1}-m_{2}|=0$
,
$-(m_{1}+m_{2})^{2}\not =0$
. When
$m_{1}\not =m_{2}$
,
$\unicode[STIX]{x1D707}|m_{1}-m_{2}|$
is a non-zero irrational number but
$-(m_{1}+m_{2})^{2}$
is a rational number, therefore it holds that
$\unicode[STIX]{x1D707}|m_{1}-m_{2}|-(m_{1}+m_{2})^{2}\not =0$
, because the sum of a rational number and a non-zero irrational number is always a non-zero irrational number. In this way, equation (2.42) has only two integer solutions:
$m_{1}=1,m_{2}=0$
and
$m_{1}=0,m_{2}=1$
. Thus, we have
$\tilde{\unicode[STIX]{x1D706}}_{m_{1},m_{2}}^{\ast }=0$
for only two cases even for resonance conditions:
Until now, with the proper auxiliary linear operator, an infinite number of small denominators are avoided once and for all automatically. It should be emphasized that we choose two different values of
$\unicode[STIX]{x1D707}$
(
$\unicode[STIX]{x03C0}/3$
and
$\sqrt{2}$
) but obtain the same result. So, without loss of generality, we choose
$\unicode[STIX]{x1D707}=\unicode[STIX]{x03C0}/3$
in the calculations of this paper.
Based on the auxiliary linear operator (2.37),
$\bar{S}_{m}$
and
$S_{m}$
in high-order deformation equations are defined by
where
$\unicode[STIX]{x1D6FD}_{i,j}^{n,m}$
and
$\unicode[STIX]{x1D6FE}_{i,j}^{n,m}$
are defined by (A 19) and (A 20).
2.5 Choice of the initial guess
In case of non-resonance, using the freedom of the HAM in the choice of the initial guess solution
$\unicode[STIX]{x1D711}_{0}$
, we let the initial guess
$\unicode[STIX]{x1D711}_{0}$
contain two non-trivial components
where
$\unicode[STIX]{x1D714}_{1}=\unicode[STIX]{x1D714}_{2}=\unicode[STIX]{x1D714}$
,
$A$
and
$B$
are constants, which will be chosen for different cases. The real frequencies
$\unicode[STIX]{x1D70E}_{1,0}$
and
$\unicode[STIX]{x1D70E}_{2,0}$
are unknown.
In the case of resonating triads,
$\tilde{\unicode[STIX]{x1D706}}_{1,1}=0$
corresponding to the resonant hydroacoustic wave component must be considered. Assuming that the resonant hydroacoustic wave occupies a significant energy (compared to the non-resonance case) in the wave system, our strategy is to add the resonant hydroacoustic wave component to the initial guess so that the initial guess is closer to the exact solution, which will make for rapid convergence. With the great freedom in the choice of the initial guess, we let the initial guess
$\unicode[STIX]{x1D711}_{0}$
contain two non-trivial components and one resonant component
where
$A$
and
$B$
are constants, which will be chosen for different cases.
$C$
is related to
$A$
and
$B$
. It is found that, when
$C=\min \{A,B\}$
, convergence can be obtained in all cases in which the steady-state resonant acoustic–gravity waves exist in the present paper.
3 Results analysis
3.1 Non-resonant waves
For acoustic–gravity waves far from resonance, we take the same case as that considered by Kadri & Stiassnie (Reference Kadri and Stiassnie2013):
where
$A^{(i)}$
represents the wave amplitude. For the same case, we get a convergent solution by choosing
$A=B=1/10~\text{m}$
in the initial guess
There is a slight difference between (3.2) and (3.3), because Kadri & Stiassnie (Reference Kadri and Stiassnie2013) considered the second-order equations of the boundary condition on the free surface but we consider the fully nonlinear boundary condition. This illustrates the validity of our HAM approach.
3.2 Resonant waves
The resonant triad interactions of acoustic–gravity waves exist at special water depths
$h\approx (n+0.5)\unicode[STIX]{x03C0}c/\unicode[STIX]{x1D714}_{3}$
, as mentioned by Longuet-Higgins (Reference Longuet-Higgins1950). From
$h\approx (n+0.5)\unicode[STIX]{x03C0}c/\unicode[STIX]{x1D714}_{3}$
, we have
Substituting
$c=1500~\text{m}~\text{s}^{-1}$
and
$h=4000~\text{m}$
into the above algebraic equation, we have
When
$n=0,1,2,3,\ldots$
,
$\unicode[STIX]{x1D714}_{3}\approx 0.589049~\text{s}^{-1},1.76715~\text{s}^{-1},2.94529~\text{s}^{-1},4.12334~\text{s}^{-1},\ldots$
, respectively. Actually, we can get the convergent solution of the steady-state acoustic–gravity waves for the cases of mode
$n=1$
and mode
$n=2$
, but not for the cases of mode
$n=0$
and mode
$n=3$
. This illustrates that steady-state resonant acoustic–gravity waves do not exist in all cases, as Xu et al. (Reference Xu, Lin, Liao and Stiassnie2012) mentioned for general steady-state resonant gravity waves. We obtain the cases of exact resonating triads in a way similar to that of Kadri & Stiassnie (Reference Kadri and Stiassnie2013).
3.2.1 Resonant waves for the case with
$|\boldsymbol{k}_{3}|=0$
(mode
$n=1$
)
For the resonant waves, we consider first the case of Longuet-Higgins with
$|\boldsymbol{k}_{3}|=0$
and present detailed results for mode
$n=1$
near the non-resonance case we considered in § 3.1, say,
$\unicode[STIX]{x1D714}_{3}=1.76784~\text{s}^{-1}$
. So, we investigate here the following resonant acoustic–gravity wave system:
The solution of (3.8) in the case of
$h=4000~\text{m}$
,
$k_{1}=k_{2}=0.0796449~\text{m}^{-1}$
,
$A=1/20~\text{m}$
,
$B=1/50~\text{m}$
,
$C=1/50~\text{m}$
.

Substituting this initial guess into the so-called first-order deformation equation (2.29) (
$m=1$
) in the framework of HAM, we have
$$\begin{eqnarray}\displaystyle {\mathcal{L}}^{\ast }[\unicode[STIX]{x1D711}_{1}] & = & \displaystyle c_{0}\unicode[STIX]{x1D6E5}_{0}^{\unicode[STIX]{x1D711}}-\bar{S}_{1}\nonumber\\ \displaystyle & = & \displaystyle \overline{b}_{1,0}\sin (\unicode[STIX]{x1D709}_{1})+\overline{b}_{0,1}\sin (\unicode[STIX]{x1D709}_{2})+\overline{b}_{2,0}\sin (2\unicode[STIX]{x1D709}_{1})+\overline{b}_{0,2}\sin (2\unicode[STIX]{x1D709}_{2})\nonumber\\ \displaystyle & & \displaystyle +\,\overline{b}_{1,1}\sin (\unicode[STIX]{x1D709}_{1}+\unicode[STIX]{x1D709}_{2})+\overline{b}_{1,-1}\sin (\unicode[STIX]{x1D709}_{1}-\unicode[STIX]{x1D709}_{2})+\overline{b}_{2,1}\sin (2\unicode[STIX]{x1D709}_{1}+\unicode[STIX]{x1D709}_{2})+\overline{b}_{1,2}\sin (\unicode[STIX]{x1D709}_{1}+2\unicode[STIX]{x1D709}_{2})\nonumber\\ \displaystyle & & \displaystyle +\,\overline{b}_{3,1}\sin (3\unicode[STIX]{x1D709}_{1}+\unicode[STIX]{x1D709}_{2})+\overline{b}_{2,2}\sin (2\unicode[STIX]{x1D709}_{1}+2\unicode[STIX]{x1D709}_{2})+\overline{b}_{1,3}\sin (\unicode[STIX]{x1D709}_{1}+3\unicode[STIX]{x1D709}_{2})\nonumber\\ \displaystyle & & \displaystyle +\,\overline{b}_{3,2}\sin (3\unicode[STIX]{x1D709}_{1}+2\unicode[STIX]{x1D709}_{2})+\overline{b}_{2,3}\sin (2\unicode[STIX]{x1D709}_{1}+3\unicode[STIX]{x1D709}_{2})+\overline{b}_{3,3}\sin (3\unicode[STIX]{x1D709}_{1}+3\unicode[STIX]{x1D709}_{2}),\end{eqnarray}$$
where
$\overline{b}_{m_{1},m_{2}}$
depends upon
$\unicode[STIX]{x1D70E}_{1,0}$
,
$\unicode[STIX]{x1D70E}_{2,0}$
, which is unknown in the initial guess (2.47). Owing to the property of the inverse linear operator (2.41), the coefficients of the terms
$\sin (\unicode[STIX]{x1D709}_{1})$
and
$\sin (\unicode[STIX]{x1D709}_{2})$
on the right-hand side of the first-order deformation equation (2.29) (
$m=1$
) must be zero so as to avoid secular terms. This provides two coupled nonlinear algebraic equations for
$\unicode[STIX]{x1D70E}_{1,0}$
,
$\unicode[STIX]{x1D70E}_{2,0}$
$$\begin{eqnarray}\displaystyle \unicode[STIX]{x1D702}_{1} & = & \displaystyle c_{0}\unicode[STIX]{x1D6E5}_{0}^{\unicode[STIX]{x1D702}}\nonumber\\ \displaystyle & = & \displaystyle \overline{a}_{1,0}\cos (\unicode[STIX]{x1D709}_{1})+\overline{a}_{0,1}\cos (\unicode[STIX]{x1D709}_{2})+\overline{a}_{1,1}\cos (\unicode[STIX]{x1D709}_{1}+\unicode[STIX]{x1D709}_{2})\nonumber\\ \displaystyle & & \displaystyle +\,\overline{a}_{2,1}\cos (2\unicode[STIX]{x1D709}_{1}+\unicode[STIX]{x1D709}_{2})+\overline{a}_{1,2}\cos (\unicode[STIX]{x1D709}_{1}+2\unicode[STIX]{x1D709}_{2}),\end{eqnarray}$$
where
$\overline{a}_{m_{1},m_{2}}$
are known constants.
Now, all terms on the right-hand side of the first-order deformation equation (2.29) (
$m=1$
) are known, so it is straightforward to obtain
$\unicode[STIX]{x1D711}_{1}$
:
Since the components
$A(\unicode[STIX]{x1D714}/g)\unicode[STIX]{x1D6F9}_{1,0}$
and
$B(\unicode[STIX]{x1D714}/g)\unicode[STIX]{x1D6F9}_{0,1}$
of the two primary waves are given, we have
$A^{\ast }=B^{\ast }=0$
so that
$$\begin{eqnarray}\displaystyle \unicode[STIX]{x1D711}_{1} & = & \displaystyle {\mathcal{L}}^{\ast -1}[c_{0}\unicode[STIX]{x1D6E5}_{0}^{\unicode[STIX]{x1D711}}-\bar{S}_{1}]\nonumber\\ \displaystyle & = & \displaystyle \overline{d}_{1,0}\unicode[STIX]{x1D6F9}_{1,0}+\overline{d}_{0,1}\unicode[STIX]{x1D6F9}_{0,1}+\overline{d}_{2,0}\unicode[STIX]{x1D6F9}_{2,0}+\overline{d}_{0,2}\unicode[STIX]{x1D6F9}_{0,2}+\overline{d}_{1,1}\unicode[STIX]{x1D6F9}_{1,1}+\overline{d}_{1,-1}\unicode[STIX]{x1D6F9}_{1,-1}+\overline{d}_{2,1}\unicode[STIX]{x1D6F9}_{2,1}\nonumber\\ \displaystyle & & \displaystyle +\,\overline{d}_{1,2}\unicode[STIX]{x1D6F9}_{1,2}+\overline{d}_{3,1}\unicode[STIX]{x1D6F9}_{3,1}+\overline{d}_{2,2}\unicode[STIX]{x1D6F9}_{2,2}+\overline{d}_{1,3}\unicode[STIX]{x1D6F9}_{1,3}+\overline{d}_{3,2}\unicode[STIX]{x1D6F9}_{3,2}+\overline{d}_{2,3}\unicode[STIX]{x1D6F9}_{2,3}+\overline{d}_{3,3}\unicode[STIX]{x1D6F9}_{3,3},\end{eqnarray}$$
where
$\overline{d}_{m_{1},m_{2}}=\overline{b}_{m_{1},m_{2}}/\tilde{\unicode[STIX]{x1D706}}_{m_{1},m_{2}}^{\ast }$
. We substitute
$\unicode[STIX]{x1D711}_{1}$
into the second-order deformation equation (2.29) (
$m=2$
). Note that coefficients of
$\sin (m_{1}\unicode[STIX]{x1D709}_{1}+m_{2}\unicode[STIX]{x1D709}_{2})$
contain
$\unicode[STIX]{x1D70E}_{1,1}$
and
$\unicode[STIX]{x1D70E}_{2,1}$
that are unknown right now. Then, enforcing the coefficients of
$\sin (\unicode[STIX]{x1D709}_{1})$
and
$\sin (\unicode[STIX]{x1D709}_{2})$
on its right-hand side to be zero so as to avoid secular terms, we can further determine
$\unicode[STIX]{x1D70E}_{1,1}$
and
$\unicode[STIX]{x1D70E}_{2,1}$
in a similar way. Then, we can similarly obtain
$\unicode[STIX]{x1D702}_{2}$
,
$\unicode[STIX]{x1D711}_{2}$
, and so on.
In addition, the ‘convergence-control parameter’
$c_{0}$
can provide a convenient way to guarantee the convergence of the solution series in the framework of HAM. The optimal value of
$c_{0}$
is determined through the minimum residuals of (2.12) and (2.13) to guarantee the convergence of the HAM approximations. Define the averaged residual square as
for the
$m$
th-order approximation of
$\unicode[STIX]{x1D719}$
and
$\unicode[STIX]{x1D702}$
. The residual errors of
$\unicode[STIX]{x1D700}_{m}^{\unicode[STIX]{x1D719}}$
and
$\unicode[STIX]{x1D700}_{m}^{\unicode[STIX]{x1D702}}$
both decrease sharply when the value of
$c_{0}$
is close to
$-1.35$
, as shown in figure 1. Then, we choose
$c_{0}=-1.35$
. The corresponding residual error squares of the two boundary conditions decease rather quickly to the level
$10^{-16}$
at 20th order, as shown in table 3 and figure 2. Then, we can obtain the convergent wave frequencies and amplitudes, which are given in table 4. The
$a_{1,1}^{\ast }$
represents the amplitude corresponding to the resonant hydroacoustic wave component. If we neglect the
$g(\unicode[STIX]{x2202}\unicode[STIX]{x1D711}/\unicode[STIX]{x2202}z)$
term in (2.1), we can also get the convergent series solutions of the steady-state resonant acoustic–gravity waves, as shown in table 5. It is found that the gravity contribution in (2.1) is very small. The existence of
$g(\unicode[STIX]{x2202}\unicode[STIX]{x1D711}/\unicode[STIX]{x2202}z)$
has negligible effect on the calculation results of this paper. Actually, one can omit the gravity contribution in (2.1) for practical purposes. This conclusion was also confirmed by Abdolali & Kirby (Reference Abdolali and Kirby2017), who showed the negligible role of
$g(\unicode[STIX]{x2202}\unicode[STIX]{x1D711}/\unicode[STIX]{x2202}z)$
on hydroacoustic waves and surface gravity waves with short wavelength. Furthermore, we investigate different cases in a similar way, as shown in table 6.
Averaged residual squares versus
$c_{0}$
in the case of
$h=4000~\text{m}$
,
$k_{1}=k_{2}=0.0796449~\text{m}^{-1}$
,
$A=1/20~\text{m}$
,
$B=1/50~\text{m}$
,
$C=1/50~\text{m}$
. Solid line: first-order approximation; dashed line: third-order approximation; dash-dot-dotted line: fifth-order approximation; dotted line: seventh-order approximation. Panel (a) represents averaged residual square of
$\log _{10}\unicode[STIX]{x1D700}_{m}^{\unicode[STIX]{x1D719}}$
versus
$c_{0}$
and (b) represents averaged residual square of
$\log _{10}\unicode[STIX]{x1D700}_{m}^{\unicode[STIX]{x1D702}}$
versus
$c_{0}$
.

The averaged residual squares of
$\unicode[STIX]{x1D700}_{m}^{\unicode[STIX]{x1D719}}$
and
$\unicode[STIX]{x1D700}_{m}^{\unicode[STIX]{x1D702}}$
in the case of
$h=4000~\text{m}$
,
$k_{1}=k_{2}=0.0796449~\text{m}^{-1}$
,
$A=1/20~\text{m}$
,
$B=1/50~\text{m}$
,
$C=1/50~\text{m}$
by means of
$c_{0}=-1.35$
.

Averaged residual squares of
$\unicode[STIX]{x1D700}_{m}^{\unicode[STIX]{x1D719}}$
and
$\unicode[STIX]{x1D700}_{m}^{\unicode[STIX]{x1D702}}$
versus the approximation order
$m$
by means of
$c_{0}=-1.35$
in the case of
$h=4000~\text{m}$
,
$k_{1}=k_{2}=0.0796449~\text{m}^{-1}$
,
$A=1/20~\text{m}$
,
$B=1/50~\text{m}$
,
$C=1/50~\text{m}$
.

Time variation of dynamic pressure (
$p_{d}$
) induced by the resulting hydroacoustic wave in the case
$k_{1}=k_{2}=0.0796449~\text{m}^{-1}$
,
$A=1/20~\text{m}$
,
$B=1/50~\text{m}$
,
$C=1/50~\text{m}$
.

Analytical approximations of the dimensional angular frequencies and wave amplitude components (m) in the case of
$k_{1}=k_{2}=0.0796449~\text{m}^{-1}$
,
$A=1/20~\text{m}$
,
$B=1/50~\text{m}$
,
$C=1/50~\text{m}$
.

The dimensionless angular frequencies and the wave amplitude components (m) in the case with
$|\boldsymbol{k}_{3}|=0$
(mode
$n=1$
),
$A=1/20~\text{m}$
and
$B=1/50~\text{m}$
with or without the
$g(\unicode[STIX]{x2202}\unicode[STIX]{x1D711}/\unicode[STIX]{x2202}z)$
term in (2.1).

The dimensionless angular frequencies and the wave amplitude components (m) versus
$A$
(m) and
$B$
(m) in the case of
$k_{1}=k_{2}=0.0796449~\text{m}^{-1}$
.

The energy distribution of the wave system versus
$A$
(m) and
$B$
(m) in the case of
$k_{1}=k_{2}=0.0796449~\text{m}^{-1}$
.

Define
The wave amplitudes and energy distributions of the two primary waves and resonant hydroacoustic wave component are given in table 7. It is found that the two primary gravity waves and the resonant hydroacoustic wave as a whole occupy most wave energy in all considered cases. A similar conclusion was found for steady-state exactly/nearly resonant gravity waves by Liao (Reference Liao2011b ), Xu et al. (Reference Xu, Lin, Liao and Stiassnie2012), Liu & Liao (Reference Liu and Liao2014), Liu et al. (Reference Liu, Xu, Li, Peng, Alsaedi and Liao2015) and Liao et al. (Reference Liao, Xu and Stiassnie2016).
Next, we discuss the pressure distribution of the steady-state resonant acoustic–gravity waves. We consider here the dynamic pressure
$p_{d}$
of the resulting hydroacoustic wave in the whole fluid. Figure 3 shows the time variation of dynamic pressure (
$p_{d}$
) induced by the hydroacoustic wave in the case
$k_{1}=k_{2}=0.0796449~\text{m}^{-1}$
,
$A=1/20~\text{m}$
,
$B=1/50~\text{m}$
. It is found that, when the resonance condition is exactly satisfied, acoustic–gravity waves can also generate a periodic pressure on the ocean floor, whose frequency is the superposition of the actual wave frequencies of the two primary waves. If the amplitudes of the two primary waves are the same (the cases corresponding to
$A=B$
in the initial guess
$\unicode[STIX]{x1D711}_{0}$
), the actual wave frequencies of the two primary waves are the same. So, the frequency of the pressure at the sea bottom is exactly twice the wave frequency of the primary gravity waves. The pressure generated by the acoustic–gravity waves is dependent of the water depth, as shown in figure 3. The magnitude of pressure is related to the amplitude of the hydroacoustic wave, which is determined by the value of
$A$
and
$B$
in the initial guess of the velocity potential
$\unicode[STIX]{x1D711}_{0}$
. In the present case, the maximum dynamic pressure on the bottom is approximately 70 kPa, which is much larger than the pressure (
${\approx}3.5~\text{Pa}$
) obtained in the above-mentioned case of non-resonance with the same amplitude
$A=1/20~\text{m}$
and
$B=1/50~\text{m}$
of the velocity potential
$\unicode[STIX]{x1D711}_{0}$
. This value is of the same order of magnitude as the maximum dynamic pressure of the first acoustic–gravity wave mode generated by bottom motion in the study of Oliveira & Kadri (Reference Oliveira and Kadri2016). So, the resonant acoustic–gravity waves might indeed trigger microseisms in the Earth.
The second-order pressure induced by two opposite primary waves in the case of
$\unicode[STIX]{x1D714}_{1}=0.884266~\text{s}^{-1}$
,
$a_{1,0}=0.0500210~\text{m}$
,
$a_{0,1}=0.0200522~\text{m}$
.

Without considering the compressibility of the water, Pellet et al. (Reference Pellet, Christodoulides, Donne, Bean and Dias2017) obtained a second-order pressure field generated by two exactly opposite travelling gravity waves (
$\boldsymbol{k}_{1}+\boldsymbol{k}_{2}=\mathbf{0}$
), which is independent of water depth and periodic in time with twice the frequency of the primary gravity waves. It reads
We choose the same amplitudes of the two primary waves as these in the resonance case (3.6).
$a_{1,0}=0.0500210~\text{m},a_{0,1}=0.0200522~\text{m}$
. Then we can get the second-order pressure field, as shown in figure 4. The second-order pressure is proportional to the amplitudes of the two primary waves. It is found that when the acoustic–gravity waves resonance occurs, the maximum dynamic pressure on the bottom is approximately 70 kPa (with compressibility), which is much larger than the second-order pressure (
${\approx}6~\text{Pa}$
) (without compressibility) obtained with the same amplitudes of the two primary waves. The reason is that no resonance occurs in the whole system, when we ignore the compressibility of water.
3.2.2 Resonant waves for the case with
$|\boldsymbol{k}_{3}|=0$
(mode
$n=2$
)
Here, we investigate the following resonant acoustic–gravity wave system (mode
$n=2$
):
Time variation of dynamic pressure (
$p_{d}$
) induced by the resulting hydroacoustic wave in the case
$k_{1}=k_{2}=0.221124~\text{m}^{-1}$
,
$A=1/50~\text{m}$
,
$B=1/100~\text{m}$
.

The dimensionless angular frequencies and the wave amplitude components (m) versus
$B$
(m) in the case of
$k_{1}=k_{2}=0.221124~\text{m}^{-1}$
,
$A=1/50~\text{m}$
.

The energy distribution of the wave system versus
$B$
(m) in the case of
$k_{1}=k_{2}=0.221124~\text{m}^{-1}$
,
$A=1/50~\text{m}$
.

3.2.3 Resonant waves for the case with
$0<|\boldsymbol{k}_{3}|<\unicode[STIX]{x1D714}_{3}/c$
The resonance case (mode
$n=1$
) given by Kadri & Stiassnie (Reference Kadri and Stiassnie2013) is
The dimensionless angular frequencies and the wave amplitude components (m) versus
$B$
(m) in the case of
$k_{1}=0.102249~\text{m}^{-1}$
,
$k_{2}=0.101625~\text{m}^{-1}$
,
$A=1/20~\text{m}$
.

The energy distribution of the wave system versus
$B$
(m) in the case of
$k_{1}=0.102249~\text{m}^{-1}$
,
$k_{2}=0.101625~\text{m}^{-1}$
,
$A=1/20~\text{m}$
.

Even in the cases of
$h=2000~\text{m}$
and
$h=3000~\text{m}$
, we also obtain the steady-state resonant acoustic–gravity waves. It means that steady-state resonant acoustic–gravity waves commonly exist in water of uniform depth. This agrees with Kadri & Stiassnie (Reference Kadri and Stiassnie2013), who pointed out that the water depth
$h$
should be greater than
$h_{cr}\equiv \unicode[STIX]{x03C0}c/2\unicode[STIX]{x1D714}_{3}$
for the existence of a hydroacoustic wave.
4 Concluding remarks and discussion
The steady-state acoustic–gravity waves are studied under non-resonance and exact resonance conditions. In the framework of traditional methods, like the perturbation methods, there exist an infinite number of small denominators. However, in the framework of HAM, these infinite number of small denominators can be avoided conveniently by means of choosing a piecewise auxiliary linear operator. Besides, the so-called convergence-control parameter provides a simple way to guarantee the convergence of solution series. Considering the works of Liao (Reference Liao2011b ), Xu et al. (Reference Xu, Lin, Liao and Stiassnie2012), Liu & Liao (Reference Liu and Liao2014), Liu et al. (Reference Liu, Xu, Li, Peng, Alsaedi and Liao2015), Liao et al. (Reference Liao, Xu and Stiassnie2016) and Liu et al. (Reference Liu, Xu and Liao2018), the steady-state waves with time-independent wave spectrum commonly exist not only for gravity waves in various depths of water but also for acoustic–gravity waves in deep water of uniform depth.
In the considered case without resonance, the solutions given by our HAM approach agree well with those obtained by Kadri & Stiassnie (Reference Kadri and Stiassnie2013). This illustrates the validity of our HAM approach. In the considered cases with resonance, steady-state resonant acoustic–gravity waves have been obtained for the first time, to the best of our knowledge. Like the steady-state resonant gravity waves (Xu et al. Reference Xu, Lin, Liao and Stiassnie2012; Liu & Liao Reference Liu and Liao2014; Liu et al. Reference Liu, Xu, Li, Peng, Alsaedi and Liao2015; Liao et al. Reference Liao, Xu and Stiassnie2016), the two primary gravity waves and the resonant acoustic–gravity occupy most of wave energy. This illustrates the common existence of the steady-state resonant waves.
When dealing with the pressure field caused by the hydroacoustic waves, most of researchers considered the non-resonant acoustic–gravity waves and the hydroacoustic waves generated by the vertical oscillations of ocean floor. For the resonance state, no specific analysis of the pressure field was given. In this paper, we obtained the steady-state acoustic–gravity waves under the exact resonance criterion. So, it is easy for us to get the pressure field caused by the steady-state resonant hydroacoustic wave component. It is found that the resonant acoustic–gravity waves can indeed generate a pressure on the ocean floor, the frequency of which is the superposition of the actual wave frequencies of the two primary waves. The maximum dynamic pressure on the bottom is much larger than the pressure in the case of non-resonance and the second-order pressure without considering the compressibility of the water, which might trigger microseisms in the Earth.
In addition, we also successfully obtained the steady-state resonant acoustic–gravity waves in some cases with different water depths, such as
$h=3000~\text{m}$
and
$h=2000~\text{m}$
. This indicates that the steady-state resonant acoustic–gravity waves commonly exist in deep water of uniform depth. The steady-state resonant acoustic–gravity waves obtained in this paper are helpful to enrich our understanding about resonant acoustic–gravity waves.
Acknowledgements
We are grateful to the National Natural Science Foundation of China (approval no. 11432009) for financial support. This work is also partly supported by the Lloyd’s Register Foundation (LRF). Lloyd’s Register Foundation works on achieving advances in engineering-related education, public engagement and the application of research to protect life and property. F.D. was partially funded through the US-Ireland Research & Development Partnership Programme as part of the collaborative project ‘Understanding Extreme Nearshore Wave Events through Studies of Coastal Boulder Transport’ (grant nos 14/US/E3111 and NSF 1529756).
Appendix A. Definitions of
$\unicode[STIX]{x1D6E5}_{m}^{\unicode[STIX]{x1D711}}$
and
$\unicode[STIX]{x1D6E5}_{m}^{\unicode[STIX]{x1D702}}$
in (2.29) and (2.31)
The definitions of
$\unicode[STIX]{x1D6E5}_{m}^{\unicode[STIX]{x1D711}}$
and
$\unicode[STIX]{x1D6E5}_{m}^{\unicode[STIX]{x1D702}}$
in (2.29) and (2.31) are given by
where
$$\begin{eqnarray}\displaystyle \unicode[STIX]{x1D6EC}_{m} & = & \displaystyle \mathop{\sum }_{n=0}^{m}(k_{1}^{2}\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\unicode[STIX]{x1D6E4}_{m-n,1}+k_{2}^{2}\bar{\unicode[STIX]{x1D711}}_{n}^{0,1}\unicode[STIX]{x1D6E4}_{m-n,2}+\bar{\unicode[STIX]{x1D711}}_{z,n}^{0,0}\unicode[STIX]{x1D6E4}_{m-n,3})\nonumber\\ \displaystyle & & \displaystyle +\,\boldsymbol{k}_{1}\boldsymbol{\cdot }\boldsymbol{k}_{2}\mathop{\sum }_{n=0}^{m}(\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\unicode[STIX]{x1D6E4}_{m-n,2}+\bar{\unicode[STIX]{x1D711}}_{n}^{0,1}\unicode[STIX]{x1D6E4}_{m-n,1}),\end{eqnarray}$$
with the definitions
$$\begin{eqnarray}\displaystyle \unicode[STIX]{x1D6E4}_{m,0} & = & \displaystyle \frac{k_{1}^{2}}{2}\mathop{\sum }_{n=0}^{m}\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\bar{\unicode[STIX]{x1D711}}_{m-n}^{1,0}+\boldsymbol{k}_{1}\boldsymbol{\cdot }\boldsymbol{k}_{2}\mathop{\sum }_{n=0}^{m}\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\bar{\unicode[STIX]{x1D711}}_{m-n}^{0,1}+\frac{k_{2}^{2}}{2}\mathop{\sum }_{n=0}^{m}\bar{\unicode[STIX]{x1D711}}_{n}^{0,1}\bar{\unicode[STIX]{x1D711}}_{m-n}^{0,1}\nonumber\\ \displaystyle & & \displaystyle +\,\frac{1}{2}\mathop{\sum }_{n=0}^{m}\bar{\unicode[STIX]{x1D711}}_{z,n}^{0,0}\bar{\unicode[STIX]{x1D711}}_{z,m-n}^{0,0},\end{eqnarray}$$
$$\begin{eqnarray}\displaystyle \unicode[STIX]{x1D6E4}_{m,1} & = & \displaystyle \mathop{\sum }_{n=0}^{m}(k_{1}^{2}\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\bar{\unicode[STIX]{x1D711}}_{m-n}^{2,0}+k_{2}^{2}\bar{\unicode[STIX]{x1D711}}_{n}^{0,1}\bar{\unicode[STIX]{x1D711}}_{m-n}^{1,1}+\bar{\unicode[STIX]{x1D711}}_{z,n}^{0,0}\bar{\unicode[STIX]{x1D711}}_{z,m-n}^{1,0})\nonumber\\ \displaystyle & & \displaystyle +\,\boldsymbol{k}_{1}\boldsymbol{\cdot }\boldsymbol{k}_{2}\mathop{\sum }_{n=0}^{m}(\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\bar{\unicode[STIX]{x1D711}}_{m-n}^{1,1}+\bar{\unicode[STIX]{x1D711}}_{n}^{2,0}\bar{\unicode[STIX]{x1D711}}_{m-n}^{0,1}),\end{eqnarray}$$
$$\begin{eqnarray}\displaystyle \unicode[STIX]{x1D6E4}_{m,2} & = & \displaystyle \mathop{\sum }_{n=0}^{m}(k_{1}^{2}\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\bar{\unicode[STIX]{x1D711}}_{m-n}^{1,1}+k_{2}^{2}\bar{\unicode[STIX]{x1D711}}_{n}^{0,1}\bar{\unicode[STIX]{x1D711}}_{m-n}^{0,2}+\bar{\unicode[STIX]{x1D711}}_{z,n}^{0,0}\bar{\unicode[STIX]{x1D711}}_{z,m-n}^{0,1})\nonumber\\ \displaystyle & & \displaystyle +\,\boldsymbol{k}_{1}\boldsymbol{\cdot }\boldsymbol{k}_{2}\mathop{\sum }_{n=0}^{m}(\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\bar{\unicode[STIX]{x1D711}}_{m-n}^{0,2}+\bar{\unicode[STIX]{x1D711}}_{n}^{0,1}\bar{\unicode[STIX]{x1D711}}_{m-n}^{1,1}),\end{eqnarray}$$
$$\begin{eqnarray}\displaystyle \unicode[STIX]{x1D6E4}_{m,3} & = & \displaystyle \mathop{\sum }_{n=0}^{m}(k_{1}^{2}\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\bar{\unicode[STIX]{x1D711}}_{z,m-n}^{1,0}+k_{2}^{2}\bar{\unicode[STIX]{x1D711}}_{n}^{0,1}\bar{\unicode[STIX]{x1D711}}_{z,m-n}^{0,1}+\bar{\unicode[STIX]{x1D711}}_{z,n}^{0,0}\bar{\unicode[STIX]{x1D711}}_{zz,m-n}^{0,0})\nonumber\\ \displaystyle & & \displaystyle +\,\boldsymbol{k}_{1}\boldsymbol{\cdot }\boldsymbol{k}_{2}\mathop{\sum }_{n=0}^{m}(\bar{\unicode[STIX]{x1D711}}_{n}^{1,0}\bar{\unicode[STIX]{x1D711}}_{z,m-n}^{0,1}+\bar{\unicode[STIX]{x1D711}}_{n}^{0,1}\bar{\unicode[STIX]{x1D711}}_{z,m-n}^{1,0}).\end{eqnarray}$$
The expressions for
$\bar{\unicode[STIX]{x1D711}}_{n}^{i,j}$
,
$\bar{\unicode[STIX]{x1D711}}_{z,n}^{i,j}$
and
$\bar{\unicode[STIX]{x1D711}}_{zz,n}^{i,j}$
are
with the definitions
$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D707}_{m,n}=\left\{\begin{array}{@{}ll@{}}\unicode[STIX]{x1D702}_{n}, & m=1,n\geqslant 1,\\ \displaystyle \mathop{\sum }_{i=m-1}^{n-1}\unicode[STIX]{x1D707}_{m-1,i}\unicode[STIX]{x1D702}_{n-i}, & m\geqslant 2,n\geqslant m,\end{array}\right. & \displaystyle\end{eqnarray}$$
$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D6FD}_{i,j}^{n,m}=\left\{\begin{array}{@{}ll@{}}\unicode[STIX]{x1D713}_{i,j}^{n,0}, & m=0,\\ \displaystyle \mathop{\sum }_{s=1}^{m}\unicode[STIX]{x1D713}_{i,j}^{n,s}\unicode[STIX]{x1D707}_{s,m}, & m\geqslant 1,\end{array}\right. & \displaystyle\end{eqnarray}$$
$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D6FE}_{i,j}^{n,m}=\left\{\begin{array}{@{}ll@{}}\unicode[STIX]{x1D713}_{i,j}^{n,1}, & m=0,\\ \displaystyle \mathop{\sum }_{s=1}^{m}(s+1)\unicode[STIX]{x1D713}_{i,j}^{n,s+1}\unicode[STIX]{x1D707}_{s,m}, & m\geqslant 1,\end{array}\right. & \displaystyle\end{eqnarray}$$
$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D6FF}_{i,j}^{n,m}=\left\{\begin{array}{@{}ll@{}}2\unicode[STIX]{x1D713}_{i,j}^{n,2}, & m=0,\\ \displaystyle \mathop{\sum }_{s=1}^{m}(s+1)(s+2)\unicode[STIX]{x1D713}_{i,j}^{n,s+2}\unicode[STIX]{x1D707}_{s,m}, & m\geqslant 1.\end{array}\right. & \displaystyle\end{eqnarray}$$
A detailed derivation can be found in the appendix in Liao (Reference Liao2011b ).















