Gas Dynamic to Acoustic wave equation

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SUMMARY

The discussion focuses on deriving the one-dimensional wave equation in the acoustical limit from the gas dynamic equations. The key equation to derive is ##\frac{1}{c_0^2} \frac{\partial^2 p}{\partial t^2} = \frac{\partial^2 p}{\partial x^2}##, where ##c_0 = \sqrt{\frac{\gamma p_0}{\rho_0}}##. The solution involves expanding the material derivative and combining equations while neglecting quadratic terms due to the assumption that ##u << c##. The final steps include substituting variables for pressure, density, and velocity.

PREREQUISITES
  • Understanding of gas dynamics and the compressible Euler equations
  • Familiarity with wave equations and acoustical limits
  • Knowledge of the relationship between pressure, density, and sound speed in fluids
  • Basic calculus, particularly partial derivatives
NEXT STEPS
  • Study the derivation of the compressible Euler equations in one dimension
  • Learn about the relationship between pressure, density, and sound speed, specifically ##c^2=\gamma p/\rho##
  • Explore isotropic flow concepts and their implications in gas dynamics
  • Practice deriving wave equations from fundamental principles in fluid dynamics
USEFUL FOR

Students and professionals in fluid dynamics, physicists studying wave phenomena, and engineers working with acoustics or gas dynamics will benefit from this discussion.

Trevorman
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Homework Statement


Derive from the formulas
##\frac{D^\pm}{Dt}(u \pm F) = 0##

where
##\frac{D^\pm}{Dt} = \frac{\partial}{dt} + ( u \pm c) \frac{\partial}{\partial x}##
the one-dimensional wave equation in the acoustical limit.

\begin{cases}
u << c\\
c \approx c0 = const\\
F = \frac{2c}{\gamma-1}
\end{cases}

Homework Equations


The answer should be
## \frac{1}{c_0^2} \frac{\partial^2 p}{\partial t^2} = \frac{\partial^2 p}{\partial x^2}##
where
##c_0 = \sqrt{\frac{\gamma p_0}{\rho_0}}##

The Attempt at a Solution


Expanding
##\frac{D}{Dt} = \frac{\partial}{\partial t}+\frac{\partial u}{\partial x} \pm \frac{\partial c}{\partial x}##

Now combining equations
##\left( \frac{\partial}{\partial t}+\frac{\partial u}{\partial x} \pm\frac{\partial c}{\partial x} \right) \cdot (u \pm F) = 0 \Rightarrow##
##\Rightarrow\dot{u} \pm\dot{F} + uu^\prime + Fu^\prime + uc^\prime +Fc^\prime = 0 ##

Since ##c = c_0 = const## and ##u<<c \Rightarrow uc^\prime \approx 0 ##, the quadratic terms are neglected. ##\dot{F} = 0## ,and substituting F
##\frac{\partial u}{\partial t} + u \frac{\partial u}{\partial x} + \frac{2c}{\gamma-1} \frac{\partial c }{\partial x} = 0##

This should be done by substituting

##c=c_0 + c^\prime##
##u=u^\prime##
##p = p_0 + p^\prime##
##\rho = \rho_0 + \rho^\prime##
and by neglecting small terms as ##u^\prime c^\prime##

I do not know how to proceed with this example.

Thank you!
 
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This is nothing but the characteristic form of the 1-D gas equations. No perturbations are necessary.
1) Write out the compressible Euler equations in 1D
2) Note that c^2=\gamma p/rho
3) The flow you're looking for is isotropic so p=A\rho^{\gamma}
4) Play.
 

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