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Introduction to Acoustics

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952 Part G Structural <strong>Acoustics</strong> and Noise<br />

Part G 22.7<br />

Example of a Quadratic Nonlinear Coupling<br />

Here, the case of a quadratic nonlinear coupling between<br />

two oscilla<strong>to</strong>rs is investigated using the multiple-scales<br />

method [22.57]. The equations are:<br />

⎧<br />

⎨<br />

¨x1 + ω<br />

⎩<br />

2 1x1 = ε � �<br />

− β12x1x2 − 2µ1 ˙x1 ,<br />

¨x2 + ω2 2x2 = ε � − β21x2 1 − 2µ2 ˙x2 + P cos Ωt � ,<br />

(22.416)<br />

where x1 and x2 are the displacements, ω1 and ω2<br />

are the eigenfrequencies of the oscilla<strong>to</strong>rs in the linear<br />

range. The perturbation terms are grouped on the<br />

right-hand side of (22.416). The nondimensional parameter<br />

ε ≪ 1 indicates that these terms are small. The<br />

quadratic nonlinear coupling is due <strong>to</strong> the presence of<br />

the terms β12x1x2 and β21x 2 1<br />

. It is assumed that the sys-<br />

tem has a so-called internal resonance in the sense that<br />

ω2 = 2ω1 + εσ1, whereσ1 is the internal detuning parameter.<br />

The forcing frequency Ω is close <strong>to</strong> ω2 so that<br />

we can write Ω = ω2 + εσ2 where σ2 is the external detuning<br />

parameter, and µ1 and µ2 are viscous damping<br />

parameters.<br />

Resolution with the Method of Multiple Scales<br />

Solving the above equations involves calculating the amplitudes<br />

a1 and a2 of both oscilla<strong>to</strong>rs as a function of the<br />

external detuning parameter σ2. Another goal is <strong>to</strong> determine<br />

the values of the threshold in terms of amplitude<br />

and frequency, at which the nonlinear set of oscilla<strong>to</strong>rs<br />

exhibit bifurcations and unstable behavior. The present<br />

example contains most of the concepts and methods<br />

used in the theory of multiple scales applied <strong>to</strong> nonlinear<br />

oscilla<strong>to</strong>rs. The main steps of the calculations are the<br />

following:<br />

1. Definition of time scales and general form of the<br />

solution<br />

2. Solvability conditions. Elimination of secular terms<br />

3. Au<strong>to</strong>nomous system and fixed points<br />

4. Stability of the system<br />

5. Amplitudes and phases of the solution<br />

Definition of Time Scales and General Form of the<br />

Solution. The time scales are defined as<br />

Tj = ε j t with j ≥ 0 (22.417)<br />

and the solutions are expanded in<strong>to</strong><br />

⎧<br />

⎨<br />

x1(t) = x10(T0, T1) + εx11(T0, T1) + O(ε<br />

⎩<br />

2 )<br />

x2(t) = x20(T0, T1) + εx21(T0, T1) + O(ε2 )<br />

,<br />

(22.418)<br />

where the expansion is limited here <strong>to</strong> the first order in ε.<br />

The differentiation opera<strong>to</strong>rs can be written<br />

⎧<br />

∂<br />

⎪⎨ ∂t<br />

⎪⎩<br />

∂2 ∂t2 = ∂<br />

+ ε<br />

∂T0<br />

∂<br />

,<br />

∂T1<br />

∂2<br />

=<br />

∂T 2 0<br />

+ 2ε ∂<br />

∂T0<br />

∂<br />

.<br />

∂T1<br />

(22.419)<br />

In what follows, we write D j = ∂/∂Tj. Inserting<br />

(22.419) in<strong>to</strong>(22.416) and matching the coefficients of<br />

terms with the same power in ε yields:<br />

• for the zero-order term ε 0 = 1<br />

D 2 0 x10 + ω 2 1 x10 = 0 ; D 2 0 x20 + ω 2 2 x20 = 0 ;<br />

(22.420)<br />

• for the first-order term ε:<br />

⎧<br />

D2 0x11 + ω2 1x11 ⎪⎨ =−2D0D1x10 − β12x10x20 − 2µ1 D0x10 ,<br />

D2 0x21 + ω2 2x21 =−2D0D1x20 − β21x<br />

⎪⎩<br />

2 10<br />

−2µ2 D0x20 + P cos Ωt .<br />

The solutions of (22.420) can be written<br />

(22.421)<br />

x10(t) = A1(T1)e iω1t ∗<br />

+ A1 (T1)e −iω1t<br />

;<br />

x20(t) = A2(T1)e iω2t ∗<br />

+ A2 (T1)e −iω2t<br />

, (22.422)<br />

where the ( ∗ ) indicates the complex conjugate.<br />

Solvability Conditions. In order <strong>to</strong> calculate the complex<br />

terms A1(T1)andA2(T1), the expressions (22.422)<br />

are inserted in<strong>to</strong> (22.421). Then, conditions are determinedsothatnosecularterms,suchast<br />

cos ωt, exist<br />

in the solution. This leads <strong>to</strong> the so-called solvability<br />

conditions:<br />

⎧ � �<br />

∂A1<br />

−2iω1 + µ1 A1 − β12 A<br />

⎪⎨ ∂T1<br />

⎪⎩<br />

∗ 1 A2 e iσ1T1 = 0 ,<br />

� �<br />

∂A2<br />

−2iω2 + µ2 A2 − β21 A<br />

∂T1<br />

2 1 e−iσ1T1<br />

+ P<br />

2 eiσ2T1 = 0 .<br />

(22.423)

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