Diferencia entre revisiones de «Inestabilidad de Jeans»

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Srbanana (discusión · contribs.)
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:<math>R_J = \frac{c_s}{\sqrt{G \rho}} </math>
 
<nowiki>It was later pointed out by other astrophysicists that in fact, the original analysis used by Jeans was flawed, for the following reason. In his formal analysis, Jeans assumed that the collapsing region of the cloud was surrounded by an infinite, static medium. In fact, because all scales greater than the Jeans length are also unstable to collapse, any initially static medium surrounding a collapsing region will in fact also be collapsing. As a result, the growth rate of the gravitational instability ''relative to the density of the collapsing background'' is slower than that predicted by Jeans' original analysis. This flaw has come to be known as the "Jeans swindle". Later analysis by Hunter corrects for this effect.</nowiki> este texto se ha realizado por pol sala 2b el crak de la astrofisica
 
==Condición necesaria para su ocurrencia==