Changes between Version 5 and Version 6 of u/erica/JeansInstability


Ignore:
Timestamp:
06/21/13 11:21:03 (11 years ago)
Author:
Erica Kaminski
Comment:

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  • u/erica/JeansInstability

    v5 v6  
    1717When
    1818
     19[[latex($\omega^2 > 0$)]]
     20
     21or
     22
     23[[latex($4 \pi G \rho_0 < C_s^2 k^2 $)]] 
     24
     25[[latex($\omega$)]] is real, and the density perturbation has the form:
     26
     27[[latex($\rho_1 = e^{i(\vec{k} \cdot \vec{x})} e^{-i(^+_- \omega t)} $)]]
     28
     29which is oscillatory. Thus the density perturbation propagates through the medium as a sound wave, i.e. pressure gradients are strong enough to support the medium against self-gravitational collapse. On the other hand, when
     30
    1931[[latex($\omega^2 < 0$)]]
    2032
     
    3345[[latex($\rho_1 = \cos(kx)e^{^+ _-\omega t}$)]]
    3446
    35 Thus, the perturbation takes on a form that is oscillatory in x and exponential in time. What we'd like to do now is determine, for which frequencies is the perturbation ''unstable'' (exponentially growing), and for what frequencies is the perturbation ''stable'' (exponentially decaying). In order to determine this we can rewrite [[latex($\omega$)]] into a more intuitive form.
     47Thus, the perturbation takes on a form that is oscillatory in x and exponential in time. To get the critical length scale (aka Jeans length) for the oscillations, we write the oscillatory condition
     48
     49[[latex($C_s^2 k^2 > 4 \pi G \rho_0$)]]
     50
     51Substituting [[latex($2 \pi / \lambda $)]] for k and solving for [[latex($\lambda$)]] we have
     52
     53[[latex($ \lambda < \frac{2 \pi C_s}{(4 \pi G \rho_0)^{1/2}} $)]]
     54
     55That is, for wavelengths smaller than [[latex($2 \pi C_s / (4 \pi G \rho_0)$)]], the perturbation is stable to collapse. You can think of this wavelength as length scales over which the average [[latex($\rho = \rho_0$)]]. The critical length is known as the Jeans length and is given by:
     56
     57[[latex($\lambda_J = Cs(\frac{\pi}{G \rho_0})^{1/2}$)]]
     58
     59
     60
     61
     62What we'd like to do now is determine, for which frequencies is the perturbation ''unstable'' (exponentially growing), and for what frequencies is the perturbation ''stable'' (exponentially decaying). In order to determine this we can rewrite [[latex($\omega$)]] into a more intuitive form.
    3663
    3764