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Sound wave seems to be modified in the medium where the selfgravity is important.
Beside the continuity equation (2.35)

(2.45) 
and the equation of motion (2.37)

(2.46) 
the linearized Poisson equation

(2.47) 
should be included.
(2.46) gives

(2.48) 
where we used equation (2.47) to eliminate .
This yields

(2.49) 
where we used
(2.45).
This is the equation which characterizes the growth of density perturbation owing to the selfgravity.
Here we consider the perturbation are expressed by the linear combination of plane waves as

(2.50) 
where and represent the wavenumber and the angular frequency of the wave.
Picking up a plane wave and putting into equation (2.49), we obtain the dispersion relation
for the gravitational instability as

(2.51) 
Reducing the density to zero, the equation gives us the same dispersion relation as that of the sound wave as
.
For short waves (
), since the wave is ordinary oscillatory wave.
Increasing the wavelength (decreasing the wavenumber), becomes negative for
.
For negative , can be written
using a positive real .
In this case, since
, the wave which has
increases
its amplitude exponentially.
This means that even if there are density inhomogeneities only with small amplitudes,
they grow in a time scale of and form density inhomogeneities with large amplitudes.
Figure 2.2:
Dispersion Relation

The critical wavenumber

(2.52) 
corresponds to the wavelength

(2.53) 
which is called the Jeans wavelength.
Ignoring a numerical factor of the order of unity, it is shown that the Jeans wavelength is approximately equal to
the freefall time scale (eq.[2.26]) times the sound speed.
The short wave with
does not suffer from the selfgravity.
For such a scale, the analysis we did in the preceding section is valid.
Typical values in molecular clouds,
such as
,
, give us the Jeans wavelength as
.
The mass contained in a sphere with a radius is often called Jeans mass,
which gives a typical mass scale above which the gas collapses.
Typical value of the Jeans mass is as follows

(2.54) 
Using again the above typical values in the molecular clouds,
,
,
the Jeans mass of this gas is equal to
.
Next: Gravitational Instability of Thin
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Kohji Tomisaka
20070708