A A A Volume : 44 Part : 2 Morphology influence on the acoustics of permeo-elastic mediaClaude Boutin 1ENTPE Université de Lyon UMR CNRS 5513, Vaulx-en-Velin, FranceRodolfo Venegas 2University Austral of Chile, Institute of Acoustics Valdivia, ChileABSTRACT Permeo-elastic media consist of a rigid porous skeleton to which are attached flexible elastic films. Under acoustic waves the films interact with the gas that saturates the pores and introduces an elastic energy in addition to the viscous dissipation and kinetic energy. The corresponding non- conventional acoustic flow regimes are studied by the two-scale asymptotic homogenization method. The morphology influence on the acoustic features is investigated by considering permeo-elastic media with (i) fully connected pores, (ii) strictly unconnected pores (closed by films) (iii) partially connected pores (iv) mixed morphologies. The analysis shows that in specific frequency ranges, the film-fluid system behaves like an equivalent viscoelastic fluid and that local film-fluid resonances can be observed. These results enables to design materials with either unconventional conductivity or unconventional compressibility, or both, in distinct or common frequency ranges, by playing on the morphological and / or mechanical parameters of the films.1. INTRODUCTIONThis paper studies the acoustic properties of permeo-elastic materials. These fluid-saturated porous materials consist of a rigid skeleton to which thin, highly flexible films are attached. Foams can be an example of such media, the thin membranes (with our without holes) acting as films and the rigid structure being formed by the thick struts. Under acoustic waves unconventional flow regimes appears because the film’s elastic energy of deformation energy combines with the viscous dissipation of the fluid and the inertia of both film and fluid. In particular, over specific frequency ranges, the film-fluid system behaves like an equivalent viscoelastic fluid and local film-fluid resonances can be observed, [1, 2]. For these reasons, the acoustic behavior di ff ers from that of standard porous materials, [3], for which the fluid flow is independent of the solid matrix deformation. The porous network of materials with flexible internal membranes can be fully connected, partially connected or unconnected, see Figure 1. We show that these morphological aspects play an essential1 claude.boutin@entpe.fr2 rodolfo.venegas@uach.cla slaty. inter.noise 21-24 AUGUST SCOTTISH EVENT CAMPUS O ¥, ? GLASGOW role on the acoustic properties by acting either on the conductivity, or on the compressibility or on both. By assuming acoustics wavelengths much larger than the characteristic pore size, the two-scale asymptotic homogenization method, [4, 5], is used to identify how and under what circumstances the elastic and kinematic energy of the films modifies the e ff ective parameters of conductivity and / or compressibility. This approach provides a guide line for developing new acoustic meta-materials which brings together film e ff ects similar to those observed e.g. [6, 7] and resonator e ff ects as e.g. [8,9]. The paper is organized as follows. The basic assumptions and general framework are first presented, then we successively examine the cases of permeo-elastic materials with :– Fully connected pores, i.e. no pores are closed by the films,– Unconnected pores, i.e. all pores are closed by films,– Partially connected pores, i.e. some pores are closed by the films.– Mixed morphologies.For conciseness the theoretical developments are not detailed. The reader may refer to [1], [2], [10]. for further details.Figure 1: Exemples of possible morphologies of permeo-elastic media2. GENERAL FRAMEWORKConsider periodic permeo-elastic media of period Ω and characteristic size ℓ that comprises (i) a fluid network Ω f , (ii) a rigid impervious frame Ω s with surface Γ s = ∂ Ω s , and (iii) highly flexible thin flat films Γ p whose edges ∂ Γ p are clamped on Ω s .The in-plane dimension of the film is h = O ( ℓ ), much larger than the film thickness t , i.e. t ≪ h . The films behave as Kirchho ff plates with apparent Young’s modulus E p = E / (1 − ν 2 ). The bending sti ff ness is E p I , where I = t 3 / 12 is the inertia moment, and ρ p t is the surface density of the films. The saturating gaz is characterized by its dynamic viscosity η , equilibrium density ρ 0 , and adiabatic compressibility β = γ/ P e ; the mean density of the fluid-film system is ϱ = ρ 0 + ρ p t Γ / Ω f . We focus on the propagation of harmonic ( e j ω t ) acoustic waves of long wavelengths for which the ratio between ℓ and the reduced wavelength L = λ/ 2 π is a small parameter ε = ℓ/ L ≪ 1. Furthermore, for the sake of clarity, one assumes that (i) the thermal exchanges can be disregarded (however, their inclusion is easy), (ii) the material is assumed macroscopically isotropic. The local physics is described by the following set of equations– The fluid in the pore network Ω f is governed by the usual set of linearized equations3S SB SG complemented by the continuity of the fluid and film velocities ( v = j ω u ) on Γ pdiv( σ ) j ωρ 0 v in Ω f , (1) div( v ) − j ω p β in Ω f , (2) v 0 on Γ s , (3) v j ω u N on Γ p . (4)In these equations, v and p stand for the oscillatory velocity and pressure, respectively, σ = 2 η D ( v ) − p I , where I is the unitary tensor and D ( v ) = ( ∇ v + ( ∇ v ) T ) / 2 is the strain rate tensor.– The films undergo out-of-plane 2D bending while their edges ∂ Γ p are clamped on to the solid boundary. The out-of-plane film deflection u is governed by the classical Kirchho ff plates di ff erential set :f div( T ) − ρ p t ω 2 u − [ σ · N ] · N on Γ p , (5)T − f div( M ) , (6) M E p I (1 − ν ) e e ( e ∇ u ) + ν e △ u e I , (7)u 0 and e ∇ u = 0 on ∂ Γ p . (8)The tilded operators act in the plane Γ p of the films, e.g. e ∇ is the in-plane gradient vector and the in-plane tensor e e is the symmetric part of the gradient tensor, i.e., 2 e e ( − ) = e ∇ ( − ) + ( e ∇ ( − )) T . T and M denotes the transverse force vector and the bending moment tensor ; e I is the in plane unit tensor. The fluid loading on the films is accounted for by the right-most term in Equation 5 where [ · ] indicates the ’jump’ of the normal component of the fluid stress vector across Γ p .2.1. Physical analysis and Homogenisation procedure Assuming long-wavelengths induces that, as in conventional porous materials, the pressure and fluid volume variation evolves at the macroscopic scale and balance each other, while the fluid velocity and its rate of deviatoric strain fluctuate locally. Furthermore, the viscous and inertial terms balance the pressure gradient. Thus, in terms of dimensional analysis,|∇ p | = O (p / L ) ; | div( v ) | = O (v / L ) = O ( ω p β ) ,| div(2 η D ( v )) | = O ( η v /ℓ 2 ) ; O ( η v /ℓ 2 ) = O ( ρ 0 ω v) = O (p / L ) .In addition, with regards to the fluid’s stress jump across Γ p , one has O ([ η v /ℓ ]) = O ( η v /ℓ ) but O ([ p ] /ℓ ) = O (p / L ). The continuity of film and fluid velocities leads to O ( v ) = O ( ω u ) so that the film velocity varies at the local scale, as well as the transverse force and bending moment tensor, hence, [1]! = O ρ p t ω 2 u = O η v = O ℓL p ! . (9)O E p I uℓ 4ℓThe long-wavelength framework ( ε → 0) enable the use of the classical homogenization method [4,5] of periodic media for deriving the macroscopic description. To properly accounts for the above dimensional analysis, the two-scale asymptotic method of homogenization is applied to the following rescaled equations, the others one remains unchanged (for more details see [1,2]).ε f div( T ) j ωρ p tv − [(2 ηε D ( v ) − ε − 1 p I ) · N ] · N , (10)T − ε f div( M ) , (11)M ε 2 E p Ij ω (1 − ν ) e e ( e ∇ v ) + ν e △ v e I , (12)ε 2 div(2 η D ( v )) −∇ p j ωρ 0 v . (13) 2.2. Macroscopic description The homogenization approach shows that the more general macroscopic model of permeo-elastic isotropic media presents the same formal structure as for conventional porous media. The physical variables are, P , the uniform pressure at the dominant order in the pores, and, ⟨ v ⟩ , the averaged gaz velocity in the pores. The e ff ective parameters are the conductivity K ( ω, P p , P f ) and the e ff ective compressibility C ( ω, P p ), where P f = { η, ρ 0 , Ω f } , denotes the physical properties of the saturating gaz and pore space geometry while P p = { E p I , ρ e t , Γ p } denotes the mechanical and geometrical properties of the elastic films. Hence, we haveZ⟨ v ⟩ = 1Ω f v d Ω − K ( ω, P p , P f ) · ∇ x P (14)Ω f∇ x · ⟨ v ⟩ − j ω P C ( ω, P p ) (15)and the complexe and frequency dependent acoustic wave celerity issj ω K ( ω, P p , P f )C ( ω ) =C ( ω, P p ) (16)However, despite the formal similarity, the acoustic behaviour of permeo-elastic media can deviate significantly from that of conventional porous media because the conductivity and the e ff ective compressibility reflect the e ff ects of elastic films. Moreover, as shown in the next section, these parameters are strongly influenced by the morphology.3. INFLUENCE OF THE MORPHOLOGY3.1. Permeo-elastic media with connected pores Let us first consider permeo-elastic medium with connected pores as investigated in [1, 2]. This morphology does not prevent that some films close a pore section but the connection is ensured by another path. This situation could correspond to a foam with open membranes or having with some dispersed closed membranes. In that case the e ff ective description reads :Z⟨ v ⟩ = 1Ω f v d Ω − K O ( ω, P p , P f ) · ∇ x P (17)Ω f∇ x · ⟨ v ⟩ − j ω P γP e (18)Note that the compressibility is not modified by the presence of the films (and takes the classical adiabatic value because thermal exchanges are disregarded for simplicity). Conversely the conductivity K O ( ω, P p , P f ) accounts for the presence of the films. Di ff erent flow regimes can be observed :– Quasi-rigid films . That case corresponds to sti ff films or to low frequency so that the film motion tends to vanish. As a result, the conductivity is assessed asK O ≈ K r ( ω ) + j ωχ r ( ω )K . (19)where K r ( ω ) is the dynamic Darcean pemeability that would be obtain for perfectly rigid films. The elastic corrector K j ωχ r ( ω ) describes the fact that the films are (weakly) deformed in response to the stress induced by the fluid. In this corrector, the dimensionless complex function χ r ( ω ) accounts for the slight deformation of the films while K is related to the elasticity of the films and defined by K Γ p = E p IΩ f . If furthermore the e ff ect of inertia can be neglected, then one shows that the fluid flow is characterized by the intrinsic permeability K r = K r (0) /η corresponding to perfectly rigid films and a e ff ective saturating fluid that behaves as a Maxwell fluid, defined by the viscosity of the fluid η connected in series with the e ff ective elasticity of the sti ff films K K r /χ r (0), [1]. – Highly deformable films . That case corresponds to films of weak sti ff ness or to high frequencies so that that whatever the amplitude of the film motion, the elastic energy of deformation is weak. Thus, the conductivity is assessed as :1 K O ≈ 1 K s ( ω ) + K χ s ( ω )K s K s(20)j ωwhere K s ( ω ) is the dynamic Darcean pemeability that would be obtain for infinitely flexible films (i.e. almost as in absence of film except for the ki nem atic restriction, Equation 4, that the films impose on the flow). The elastic corrector K χ s ( ω )K s K s describes the fact that the film is forced to move by the fluid. In addition, if the e ff ect of inertia can be neglected, the fluid flow is characterized by the intrinsic permeability K s = K s (0) /η corresponding infinitely flexible films and a e ff ective saturating fluid that behaves as a Kelvin fluid, defined by the viscosity of the fluid η connected in parrallel with the e ff ective elasticity of the sti ff films K K s /χ s (0), [1]. To sum up, ignoring for the moment the inertial e ff ects, the e ff ect of viscosity, dominates at both low and high, frequency while the elastic e ff ect are maximized at intermediate frequencies. – Anti-resonant and resonant regimes . Such regimes occurs when (i) the energy dissipated by viscosity is negligible compared to the elastic energy of the films and the kinetic energy of the film and fluid and (ii) when these to latter energy balance each other. The anti-resonance is reached at a frequency ω a such that the internal motions of the fluid and film compensate each other so that the mean velocity vanishes meanwhile the kinetic energy is not zero, while resonance is reached at a frequency ω g such that the fluid-film system moves globally. It can be shown that both ω a and ω g are of the order of K /ϱ. Furthermore we have the following estimates, where ρ ∗ a and ρ ∗ g are dimensionless parameters that account for the structure of the fluid-film flow in these two regimes:j ωω 2 a ) ; j ω K O ( ω ) − 1 ( ω → ω g ) ≈ ϱρ ∗ g (1 − ω 2 g ω 2 ) (21)