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Jeans Length




The formula for Jeans Length is:

:\lambda_J=\sqrt{ rac{15k_{B}T}{4\pi G \mu ho}}
where k_B is Boltzmann's Constant , T is the temperature of the cloud, r is the radius of the cloud, \mu is the mass per particle in the cloud, G is the Gravitational Constant and ho is the cloud's mass density (i.e. the cloud's mass divided by the cloud's volume). {Link without Title}

Perhaps the easiest way to conceptualize Jeans' Length is in terms of a close approximation, in which we discard the factors 15 and 4\pi and in which we rephrase ho as rac{M}{r^3}. The formula for Jeans' Length then becomes:

:\lambda_J\approx\sqrt{ rac{k_B Tr^3}{GM \mu}}

It is then immediately obvious that \lambda_J=r when k_{B}T= rac{GM \mu}{r} i.e. the cloud's radius is the Jeans' Length when thermal energy per particle equals gravitational work per particle. At this critical length the cloud neither expands nor contracts. It is only when thermal energy is not equal to gravitational work that the cloud either expands and cools or contracts and warms, a process that continues until equilibrium is reached.


JEANS' LENGTH AS OSCILLATION WAVELENGTH

The Jeans' Length is the oscillation wavelength below which stable oscillations rather than gravitational collapse will occur.

:\lambda_J= rac{2\pi}{k_J}=c_s\left( rac{\pi}{G ho} ight)^{1/2}

Where G is the Gravitational Constant , c_s is the Sound Speed , and ho is the enclosed mass density.

It is also the distance a Sound Wave would travel in the Collapse Time .


SEE ALSO