By week:
|
Week 8 - Black Holes
Problem Set
Problem 1 - Photon Orbit 
We are going to find a radius at which a light will orbit a black hole.
-
Start with the Schwarschild metric. We want a circular orbit so
we will set dr=0, d (theta)=0 and theta=π/2. What is ds2 for
a photon (a photon travels along a null geodesic)?
Solve for (dφ/dt)2.
-
dφ/dt is simply Ω for the photon orbit. Kepler's third law works
in the Schwarschild spacetime for circular orbits. Solve for M.
Answer for Problem 1
-
ds=0 for a photon, so we get
/ | \ |
dφ
d t
|
\2 | / |
= |
1 - 2M/r
r2
|
-
Ω2 = M/r3. This gives M = r - 2 M or r=3 M
Problem 2 - Kepler's Law 
The equation for a geodesic (an orbit) is given by
d uμ
d τ
|
+
|
&Gammaμαβ uα uβ=0
|
where uμ is the four-velocity. When an index in an expression
is repeated you are supposed to sum over the index. The indices run
through t, r, theta and φ.
-
Let's suppose that the particle at one moment is just going around
the center of the black hole so the velocities in the r and theta directions
vanish and we'll take theta=π/2 (the equatorial plane).
In this situtation ut and uφ are the only
components of the four velocity that don't vanish and
Γrtt and
Γrφφ are the only Christoffel
symbols that don't vanish. Write out the geodesic equations.
-
We would like for the velocity to be constant around the circular orbit
so we would like
the first term in the geodesic equation to vanish. Solve for
Ω = uφ/ut in terms of the non-vanishing
Christoffel symbols.
-
The two non-vanishing Christoffel symbols are
&Gammartt =
|
(r - 2 M) M
r3
|
and
&Gammarφφ =
(2 M - r) sin2 theta. What is Ω in terms of M and r?
-
Substitute your value of Ω into the Schwarzschild metric and
calculate ds2 along the circular orbit. Over what range
of radii can a material object (a toaster, UBC undergrad etc.) travel
in a circular orbit around a Schwarzschild black hole.
Answer for Problem 2
- The geodesic equation gives
d ut
d τ
|
=
|
d utheta
d τ
|
=
|
d uφ
d τ
|
= 0
|
and
d ur
d τ
|
+
|
&Gammartt ut ut+
&Gammarφφ uφ uφ=
0
|
-
Because the first term vanishes, the second term must vanish as well
this gives
-
Ω2 = M/r3. Kepler would be pleased.
-
ds2 = ( 1 - 3 M/r ) dt2
If r>3M then ds2 is positive which is what you need for a
toaster to orbit the black hole.
Last modified: Tuesday, 06 April 2004 07:28:08
|