|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
• |
Textbook
(Combes et al.) goes through the old
|
|
|
approach
of flattened spheroids with a particular
|
|
|
mass
density as a function of radius.
This is
|
|
|
perhaps
useful review for qualifying exam as an
|
|
|
exercise
in gravitational physics.
|
|
|
• |
Key
is to use the rotation curve.
|
|
|
• |
Solutions
are appropriately simple for flat curves:
|
|
|
– |
M(total) = V2rot R/G (spherical dark matter)
|
|
|
|
|
|
– |
M(total) = (2/π) V2rot R/G (disk dark
matter)
|
|
|
|
|
• |
Where
the disk is cut off at r=R, and V = constant (flat curve)
|
|
|
inside
r < R.
|
|
|
|
• |
Mass
increases linearly with r, for V = constant
|
|
|
|
• |
Mass/Light
ratio increases faster
|
|