edwiddy
- 4
- 0
Hi, I'm a physics undergrad working through Carroll at the moment. In the section on the Kerr black hole, he states that K= \partial_t is a Killing vector because the coefficients of the metric are independent of t. He then states in eq. 6.83 that K^\mu is normalized by:
K^\mu K_\mu = - \frac{1}{\rho^2} (\Delta - a^2 \sin^2{\theta})
where \Delta = r^2 - 2GMr + a^2 and \rho^2 = r^2 + a^2 \cos^2{\theta}.
Now I can't seem to for the life of me duplicate this from the metric. We take K^\mu = (\partial_t)^\mu = \delta ^\mu_t right? Then:
K^\mu K_\mu = g^{\mu\nu}K_\nu K_\mu
which is only non zero for \mu=\nu=t...but that doesn't match up. The crossterms in the metric need to come into play, but it seems that if anyone of the indices is \phi then it goes to zero...
Thanks.
K^\mu K_\mu = - \frac{1}{\rho^2} (\Delta - a^2 \sin^2{\theta})
where \Delta = r^2 - 2GMr + a^2 and \rho^2 = r^2 + a^2 \cos^2{\theta}.
Now I can't seem to for the life of me duplicate this from the metric. We take K^\mu = (\partial_t)^\mu = \delta ^\mu_t right? Then:
K^\mu K_\mu = g^{\mu\nu}K_\nu K_\mu
which is only non zero for \mu=\nu=t...but that doesn't match up. The crossterms in the metric need to come into play, but it seems that if anyone of the indices is \phi then it goes to zero...
Thanks.
Last edited by a moderator: