1. IntroductionSince the establishment of transformation optics,[1–6] the methodology for engineering wave functional devices via coordinate transformation has spread to various wave systems due to their common character, i.e., the form invariance of wave equations in arbitrary curvilinear coordinates and curved spacetimes. Transformation acoustics (TA) is one of these developments, which offers a standard procedure to design the material parameters so that sound waves propagate along prospective trajectories or hold proleptic properties in these materials.[7,8] The most representative device of TA is the acoustic cloak that guides sound waves traveling around the cloaked objects without scattering and thus make itself and the hidden objects invisible from acoustic detections.[9–13] From the standard approach of TA, acoustic cloaks in fluid are made up of anisotropic materials with tensor mass densities. Though real fluids do not possess these properties, a variety of cloaks have been produced by using artificial acoustic metamaterials.[14–18]
On the other hand, it has been realized long ago that moving media act as curved spacetimes and can be used to simulate cosmic phenomena for both electromagnetic waves[19–22] and sound waves.[23–30] In the pioneering works of Unruh,[24,25] he discovered the dynamic analogy between the massless particles in the spacetime of Schwarzschild black hole and the sound waves dominated by the radially flowing fluid. This analogy is also valid for superfluid[31–34] in which the effects associated with acoustic black hole have been observed experimentally.[35–37] In recent years, García-Meca et al. combined the ideas of moving media and TA, and proposed the method of analogue transformation acoustics (ATA).[38–41] They made use of background flow, instead of anisotropic effective media, to mimic the metric of spacetime, and to fabricate the desired acoustic devices, such as spacetime cloak and time-dependent spatial compressor. Through forcing the effective metric to have a certain form, the parameters of background flow, i.e., the flow velocity, the speed of sound and the mass density, can be determined. However, García-Meca et al. never discussed the feasibility of these requisite parameters of background flow, although they are not unrestricted but submitted to the laws of fluid theoretically.
In this paper, we try to reconcile the ATA-determined parameters with the basic laws of fluid dynamics and show several constraints of the background flow. First, the governing equation of sound waves in ATA is accurate only when the background flow is irrotational, or at least the vorticity of the flow Ω should be much smaller than the frequency of sound ω, in order that the analogy between the flow fields and curved spacetime is applicable.[30] Second, there should exist external force fields (momentum sources) and external mass sources in general to guarantee momentum and mass conservations of the background flow. Third, since the spatial distribution of pressure and mass density are fixed after ATA procedures, their relation restricts the state equation of the background fluid. As an example, we put forward a scheme for constructing spherical cloaks with background flow which complies with the realistic fluid dynamics. In addition, we investigate the propagation of sound in this cloaking system with both geometric acoustics approach and solving the wave equation analytically. Our results show that the major difference of our scheme from the standard TA cloak is the phase retardation (or lead) effect of the sound waves traveling around the cloak. For eliminating the singularities of the parameters at the cloak surface, we introduce the unideal cloaks and evaluate their cloaking abilities.
2. Basic theoryTo begin with, we briefly review the framework of ATA. The motion of ideal fluid (with no viscosity and thermal conductivity) obeys Euler equation and the continuity equation which correspond to the momentum and mass conservations respectively. If the fluid is barotropic, i.e., its density ρ only depends on pressure P, and the flow velocity v is irrotational, the compressible fluid submits to the following equations[42]
where
ψ is the velocity potential (
υ = ∇
ψ),
H(
ρ) =
∫ d
P/
ρ =
∫ d
ρ c2/
ρ is the enthalpy per unit mass,
is the speed of sound,
F(
t) is an arbitrary integral constant with respect to time, and we have supposed the existence of the external potential of momentum source
U(
r) and the external mass source
M(
r,t). Indeed, there are two origins of
U(
r), one is the external bulk force
f = −∇
U0, the other corresponds to the mass source, thus
U =
U0 +
∫ Mυ· d
r (suppose
Mυ is integrable). As we will see afterward, the two external sources are necessary.
Considering sound waves traveling on a background flow with the parameters {u, ψ, ρ,P} obeying Eq. (1), the sound waves perform as the perturbations of the flow. Taking the substitutions into Eq. (1), we can obtain the governing equations of sound wave in linear approximation[24–26]
The sound pressure satisfies
Equation (
2) is identical with the D’Alembert equation in a curved spacetime
with the effective metric
where
ρ1 =
ρ/
ρ0,
c1 =
c/
c0,
ρ0 and
c0 are constants with dimension of density and velocity respectively,
γi j denotes the spatial metric given in an arbitrary coordinate system of flat space, and d
x0 = d
t. This form of metric can be regarded as the generalized Schwarzschild metric written in the Painlevé–Gullstrand type coordinate system (PG system).
[26] If
u/(
c2 −
u2) is integrable, we can obtain the Schwarzschild-type coordinate system (Sch. system), through the coordinate transformation
where
τ is the
x0 coordinate of Sch. system. Then the metric turns into the standard form
In Sch. system, time dimension and space dimensions are decoupled, nevertheless, the spatial projection of geodesics in this system holds the same form as in PG system, since the spatial coordinates do not change. As pointed out in Ref. [
41], a major distinction between ATA and ordinary TA is that one generally deals with the wave equation of sound pressure in TA, while the kernel equation of ATA used to draw the analogy with curved spacetime is the equation of velocity potential. As a result, TA is restricted to design isobaric systems, whereas ATA is demanded to be globally barotropic.
[41]According to the procedure of ATA, if we let the effective metric either in PG system or in Sch. system equal to the requisite form gained by TA, the expressions of u, ρ, c, can be determined. However, these quantities should also compose a real solution of fluid dynamics. By plugging this quantities back into Eq. (1), the required external sources are fixed. Besides, it is notable that the governing Eq. (4) of ATA and Eq. (7) (if used) are valid only if u and u/(c2 − u2) are irrotatinal. All these matters restrict the selective freedom of the background flow.
Now we show how to construct a spherical cloak with background flow. For spherically symmetric systems, all parameters are merely functions of radius and the flow velocity u is radial. Consequently, u and u/(c2 − u2) would always be integrable. It is convenient to discuss the problem in spherical coordinates {r,θ,ϕ}, thus we have (γi j) = diag(1, r2, r2 sin2 θ) and (ui) = (u,0,0). In the light of TA, the effective metric for a spherical cloak reads[6]
Here
f(
r) is an arbitrary radial transformation satisfying the invisibility condition
f(
a) = 0, where
a is the inner radius of the cloak. We demand
f(
r) obeys the limit lim
r→∞ (
f(
r) −
r) = 0, so that the background flow goes to a homogenous and hydrostatic state with
ρ →
ρ0,
u → 0,
c →
c0,
P →
P0, when
r → ∞. Letting Eq. (
7) equal to the effective metric of spherical cloak, we obtain
The signs ± of
u indicate that the flow could be either emanative or convergent. In terms of the barotropic postulate, the pressure can be derived by
We can further obtain the required state equation of the fluid, namely the constitutive relation between
P and
ρ, in terms of Eq. (
9a) and Eq. (
10). Substituting Eqs. (
9a)–(
9c) into Eq. (
1), we get the required external potential and mass source
Obviously, the desired background flow would not generally satisfy the momentum and mass conservations unless the above external source terms are provided. In principle, the external potential could be made up with external electric fields acting on charged fluid. The mass sources could be realized via the mass exchange of chemical reactions or via phase transition of multiphase fluid,
[43] or even via discretely distributed jets and outlets.
A class of functions satisfying the conditions f(a) = 0 and f(r) → r as r → ∞ is
We calculate the profiles of
u,
ρ,
c,
P,
M with respect to
r for
n = 2,3,4, and obtain the required state equation
P(
ρ). The results are shown in Fig.
1. The figures illustrate the case of outgoing flow from the center (
u holds the sign of “+″ in Eq. (
9c)). In this case, the external potential is attractive and the mass source is negative. If
u is convergent to the center, the mass source should be positive while other variables do not change.
3. Geometric acousticsIn this section, we study the propagation of sound waves with geometric acoustics approximation in the shortwave limit. Under the eikonal hypothesis, the velocity potential takes the form , and the phase Φ satisfies the eikonal equation H = h(xμ)gμν kμ kν = 0, where kμ = ∂μ Φ, h(xμ) can be an arbitrary non-degenerate function, and
Sound rays obey the following canonical equations
It can be verified that the formulas of sound rays are identical with the geodesics in the P-G system with the effective metric. If
gμν is time-independent, d
k0/d
s = −
∂H/
∂t ≡ 0, thus the frequency
ω = −
k0 is conserved along a ray. Letting
h(
xμ) =
c0cρ1,
, we obtain
ω =
u ·
k +
ck, which is exactly the dispersion relation of sound waves in moving media,
[42] and is always applicable in the limit of geometric acoustics no matter if the background flow is irrotational or not. Therefore, although the analogy between background flow and the curved spacetime is rigorous only for potential flow, nevertheless, this restriction can be drawn off in the limit of geometric acoustics. In fact, as proved in Ref. [
30], the analogy is still valid as long as the frequency of the sound is sufficiently larger than the vorticity of the flow
Ω = ∇ ×
u:
ω ≫ |
Ω|, but there is no requirement of the magnitude of the spatial inhomogeneity comparing with wavelength. Substituting the Hamiltonian into the first set of the canonical equations, we obtain
Cancellation of d
s leads to
The result is identical with the group velocity of the sound wave,
υg = ∇
kω =
u +
ck/
k. Actually, for arbitrary eikonal equations
H(−
ω,
ki,
xμ) = 0,
Therefore, the group velocity is always along the solution of the canonical equations.
For spherically symmetric metric, kϕ is conserved along a ray, since dkϕ/ds = 0. If we let kϕ = 0, then ϕ ≡ ϕ0, and dkθ/ds = 0. As a result, the angular momentum of phonon perpendicular to the orbit kθ ≡ L is also conserved. We can further remove all the wave vector terms in the canonical equations, and obtain
with d
σ = 2
c2d
s. Inserting Eq. (
16c) into Eq. (
16b), we get the compact form of the geodesic equation
Substitution of the parameters of the spherical cloak yields
By integration, we obtain the general analytic solution of the sound rays
where
Lc0/
ω denotes the impact parameter of the phonon incident from infinity. Actually, equation (
19) is exactly transformed from the straight lines
r sin(
θ −
θ0) = const. according to TA. Moreover, based on Eq. (
17), the sound rays only depend on
u and
c but are independent of the density distribution
ρ, therefore, we have a freedom to select
ρ in the limit of geometric acoustics.
Figure 2 displays a set of rays (blue curves) incident with the same direction but different impact parameters. Despite the same trajectories as in TA cloak, the wave fronts Φ = const., shown by the red curves in Fig. 2, significantly differ from those in TA cloak. In our case, the wave fronts before bypassing the cloak are asymmetric to those after bypassing the cloak, however, this symmetry exists in TA cloak.[3,9–11] This effect presents the phase retardation of the waves when bypassing the cloak, and it is essentially induced by the background flow u. In the next section, we will further investigate this effect.
4. Analytic solutionAccording to Eq. (6), by applying the rules
the wave equation (
2) in Sch. system takes the form
Substituting Eqs. (
9a)–(
9c) into Eq. (
20), we have
Considering monofrequent wave
, since
the velocity potential can be expressed as
with
Then equation (
21) becomes
where
and
is the abbreviation of
. By separation of variables,
, the radial equation of
R(
f) is spherical Bessel equation, and the angular equation is spherical harmonious equation. Therefore, the solutions can be expressed by
where
and
are the velocity potentials of incident wave and scattering wave respectively,
denote the
l-order spherical Bessel, Neumann, and first Hankel functions respectively, and Y
lm(
θ,
ϕ) denotes the (
l,
m)-order spherical harmonics. We demand that the incident wave tends to plane wave at infinity:
with
al =
A(2
l + 1)i
l. The incident wave thus can be written as
where
P
l(cos
θ) is the
l-order Legendre polynomial, and the signs ∓ in the last line correspond to emanative and convergent flows respectively (the signs ∓ have the same meaning in all of the following equations). At the inner interface
r =
a, we suppose there is a hard boundary of the sound wave:
In Sch. system, the boundary condition turns into
Then the scattering wave is derived as
with
, and
If
f(
a) = 0, the scattering wave
. Consequently, we accomplish ideal acoustic invisibility cloaking by means of background flow. The sound pressure can be obtained from the following equation
For the ideal case, equation (
30) reduces to
Figure 3 shows the field distributions of both velocity potential and sound pressure for the case of idea cloaking with emanative background flow. As shown in the figures, the fields are asymmetric with respect to the z = 0 plane in contrast to the case of TA cloak. For the incident half place (z < 0), the phases of the fields are compressed heavily, while the phases are stretched in the outgoing half place (z > 0). According to the expression of the wave fronts
the phase retardation and lead originates exactly from the additional phase
Besides, if
u is convergent to the center, the effect turns into the opposite, namely the phases are stretched in the incident half place while are compressed in the outgoing half, and the field distributions shown in Fig.
3 are identical to the situation of a wave incident from the right side. This effect also can be viewed in the light of the sound velocities. According to Eq. (
31), the wave vector reads
Hence, the phase velocity of the sound can be obtained by
vp =
ω/
k with
Note that
c is the phase velocity of sound wave in static fluid, but
vp ≠
c in moving media. Also, the group velocity is
Figure 4 exhibits the distributions of phase velocity and group velocity corresponding to the sound fields given in Fig. 3. As we can see, the phase velocity and the group velocity slow down as the sound wave approaches the inner boundary r = a from the left side, whereas the velocities have extremely large values at the right side of inner boundary. For the case of convergent back ground flow, the distributions in Fig. 4 should still correspond to the wave incident from the right side. It is precisely the asymmetric distribution of phase velocity that causes the phase retardation and lead in corresponding regions.
It is noteworthy that an alternative scheme of acoustic cloak based on velocity potential wave equation has been proposed in Ref. [41]. In spite of the remarkable differences between their results and the ordinary TA cloaks treated with sound pressure equation, their proposal is more similar to a standard TA device than ours, since their primary method is still to construct effective anisotropic media with the conventional procedure used in TA,[1,3] but our key idea totally originates from the analogy between the moving media and curved spacetime.
5. Unideal cloakingTo realize ideal cloaking, all parameters of the background flow should tend to infinity at the inner boundary r = a as shown in Fig. 1, however, it is impossible in practice. In this section, we would discuss the unideal case with simply cutting off the infinite parameters. We still use the radial transformation f(r) to construct the background flow, but let its zero point be a′ = (1 − δ)a in order to escape the singularity at the inner boundary, when δ → 0 the cloak approaches to an ideal one. In terms of Eq. (28), the scattering wave tends to
with
Therefore, we can evaluate the cloaking ability of the background flow by means of the differential scattering cross section (DSCS)
and the total scattering cross section (TSCS)
We have checked the angular distributions of DSCS, and TSCS changing with wave length for δ = 0.1, δ = 0.05, δ = 0.02, and δ = 0.01 in comparison with the uncloaking results, as shown in Fig. 5. The results reveal that the unideal constructions still have good property of cloaking for nearly full band of wave length as δ ≤ 0.05. However, for the case of δ = 0.1, only when λ > 2a, its invisibility effect is acceptable. In addition, the angular distributions of DSCS show that the wave scatters quite uniformly in all directions when the background flow exists, whereas there are usually large components of back scattering in the uncloaking cases.
Finally, we shall discuss the required state equation of the background fluid. Though the constitutive relation between P and ρ is determined by the coordinate transformation, we can use Virial expansion to approach our constitutive relation. The Virial expansion is a physical state equation that can be derived directly from statistical thermodynamics, which takes the form
where
kB,
T denote Boltzmann constant and temperature respectively, and
Bl is the
l-th order Virial coefficient. In Fig.
6, we fit the
P–
ρ relation for the unideal cloak of
δ = 0.1, corresponding to Eq. (
12) with
n = 4, by 5-order Virial expansion. The fitting coefficients are
B1 = 1994.73,
B2 = −2430.51,
B3 = 1447.21,
B4 = −422.527,
B5 = 48.7926, and the pressure at infinity is
P0 = 624.479 (all coefficients are nondimensionalized in terms of the unit quantities
ρ0,
c0). Note that the expansion is not unique, since we can choose different orders to fit.
6. ConclusionTo summarize, we design an acoustic cloaking scheme by using background flow based on the method of ATA, and give all of the required physical parameters of the flow complying with the dynamic laws of fluid. We reveal that it is not enough to merely give the background velocity as previous works just did,[38–40] but some restrictions should be satisfied, and some other necessities, such as the external mass and momentum sources, should be supplied. We also provide a comprehensive investigation about the propagation of sound waves in our cloaking system. According to our results, the major distinctive effect in our system is the phase retardation and lead when sounds bypass the cloak. Furthermore, we analyze the cloaking ability of unideal constructions and use Virial equation of state to fit the required constitutive relation of the background fluid. Our research not only offers a novel path to achieve acoustic cloaking but also complements the framework of ATA.