18-10.
We need some assumptions:
- flat universe
- Wm ~ 0.3
- mass of galaxy Mg ~ 1012Msun
- present horizon radius d ~ 2/H0
Let M(t) = 4/3pd3(t) rm(t) be the mass contained within the horizon radius d. Using (18.47), the constancy of rma3 and the present value rm(t0) = Wmrcrit = 3WmH02/8p we find
| dM
dt
|
= 4prm(t) d2(t) so at present | dM
dt
|
~ 6Wm ~ 1.8. |
|
The required time Dt is therefore
Dt = | Mg
dM/dt
|
~ |
1012 Msun×(1.5 km/Msun)
1.8 ×(3×105 km/s)
| ~ 106 s ~ 1 month. |
|
18-20
The Friedmann equation (18.77) becomes (with â(t) = a(t)/a0)
| æ è
| dâ
dt
|
ö ø |
2
|
= Wv â2 + |
Wm
ä
|
|
|
This can be solved by separation of variables (the substitution y = â3/2 helps),
â(t) = | æ è |
Wm
Wv
| ö ø
| 1/3
|
sinh2/3(3/2 Wv½
H0t). |
|
The present moment occurs when â(t0) = 1, namely
t0 = | æ è
| 2
3H0 Wv½
| ö ø
| sinh-1 | é ë
| æ è
| wv Wm
| ö ø
| 1/2
|
ù û | . |
|
18-24
a) Look for the maximum of Ueff of (18.78): this occurs when -(Wm/â2) + 2Wvâ = 0 or rm = 2 rv = L/4p.
b) From the Friedman equation (18.77) we have Ueff(â) = 1/2 Wc or
-8p/3 (rm +rvac ) a2 = -1 hence a = L-½
so the volume is V = 2p2 a3 = 2p2 L-3/2.
c) The plot of Ueff in Fig 18.9 shows that a small change in rm will either cause the universe to expand to infinite volume, or to collapse to a singularity.
18-27
a) From (18.63) and (18.77) we have
The first law of thermo (18.20) gives
p(a) = - |
d(ra3)
d(a3)
|
= |
1
4pa2
|
|
d[aUeff(a)]
da
|
|
|
That's your parametric representation.
b) The potential should be like (18.78) down to a universe radius when kBT ~ 10 Mev; for smaller a it should rise beyond the value it has a amax in order to cause a bounce.
c) From the above equations,
So r+ 3p must be negative in the 'smaller a" region of b).
18-30
a) We need r(c) and z(c) such that the geometry to be embedded can be written
dS2 = dc2 + sinh2cdf2 = dr2 + r2 df2 + dz2
Evidently r(c) = sinh(c), but then
|
æ è
|
d\z
dc
|
ö ø
|
2
|
= 1 - cosh2c < 0 |
|
does not work.
b) Exchange sinh and cosh in the above, and the equation does have a solution namely
r(u) = cosh u z(u) = |
ó õ
|
u
0
|
(1 - sinh2u¢)1/2 du¢ |
|
which defines an embedded surface but only up to u = sinh-1(1) = 0.88.