 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
|
Text examines
isothermal and adiabatic
|
|
|
perturbations. There are problems.
|
|
|
|
|
We know
baryons are not dominant.
|
|
|
|
|
Big issue is
that temperature fluctuations observed
|
|
are not big
enough:
|
|
|
|
|
Should be >
0.001 for this analysis, required to be
|
|
|
even in
general, but are much smaller.
|
|
|
|
|
Its a bit
more complex than this, but the general
|
|
|
arguments
hold.
|
|