jeans mass gravitational collapse well understood from time of newtonian theory sir james jeans...
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Jeans Mass
Gravitational collapse well understood from time of Newtonian theory
Sir James Jeans first developed from this to a theory for gravitational collapse of a static, non-viscous fluid
Despite using Newtonian gravity, it’s a good approx.
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Overdense regions
• Imagine a smooth distribution of matter containing a slightly denser-than-average region
• WHAT HAPPENS?
• Answer depends on relative strength of two forces– gravity
– fluid pressure
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Overdense regions
• Recall hydrostatic equilibrium in stars
• If density of the region is not too high then pressure will support it and it will oscillate like a sound wave
(sound waves represent traveling pressure perturbations in a gas/fluid)
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JEANS MASS
• If the density of the clump is very high then the pressure force cannot overcome gravity and the dense region collapses in on itself
There is a minimum mass required for the dense region to collapse in on itself (recall Chandresekhar limit) -this minimum mass is called the JEANS MASS
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THE JEANS MASS AND THE ONSET OF COLLAPSE
• Summary:– Imagine an overdense
clump of mass M.– If clump is very small,
sound waves will smooth it out.
– If clump is very big, it will gravitationally collapse.
– The threshold mass separating these behaviors is called the Jeans Mass, MJ
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JEANS MASS
ρ3
3
G
speed) sound(=JM
MJ obtained by equating gravitational energy of the perturbation (which controls its collapse) with the thermal energy (generates pressure to oppose collapse)
ρ is the density of the clump
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THE JEANS MASS AND THE ONSET OF COLLAPSE
ρ3
3
G
speed) sound(=JM
MJ depends mainly on ratio of time a sound wave takes to cross a perturbation, compared to the time for gravitational collapse of the perturbation
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THE JEANS MASS AND THE ONSET OF COLLAPSE
ρ3
3
G
speed) sound(=JM
If sound can cross the region before collapse can get underway then pressure waves can restore hydrostatic equilibrium
If collapse begins before sounds gets across the region then gravity wins
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JEANS MASS
ρ3
3
G
speed) sound(=JM
So, gravitational collapse favors larger clumps containing more mass and/or low temperatures so sound travels slowly
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Jeans Mass
• Explains how we got from the almost perfect homogeneity just after the big bang to the “lumpy” and “bumpy” situation we have nowadays?
• Basic answer – gravitational collapse of regions with mass > Jeans mass
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JEANS MASS - more detailThe Virial Theorem states that, for a stable, self-gravitating, spherical distribution of equal mass objects (stars, galaxies, etc), the total kinetic energy of the objects is equal to minus 1/2 times the total gravitational potential energy.
so
the Jeans Condition
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JEANS MASS - more detail
the Jeans Condition
there is a min mass below which thermal pressure prevents grav collapse
Now EG=-GMm/r =-GM2/r
N is # atoms, mean molecular weight, mp is mass of proton
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JEANS MASS - more detail
combining these gives
high density favors collapse, high temperatures favor large Jeans Mass
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JEANS MASS - more detail
In early Universe (at a time called the decoupling time) when T~ 3000 K, n ~ 6 x 103 -> MJ ~ 105 M
In the interstellar medium T~1000, n~ 103 -> MJ~ 500 M
So in the early universe the smallest thing which could collapse was massive ! 105 M
Today, smallish molecular clouds can collapse - form individual stars.
Jeans mass versus time/conditions for the early universe is an important constraint on how galaxies formed!