Paper 2, Section II, D

General Relativity | Part II, 2015

(a) The Schwarzschild metric is

ds2=(1rs/r)dt2+(1rs/r)1dr2+r2(dθ2+sin2θdϕ2)d s^{2}=-\left(1-r_{s} / r\right) d t^{2}+\left(1-r_{s} / r\right)^{-1} d r^{2}+r^{2}\left(d \theta^{2}+\sin ^{2} \theta d \phi^{2}\right)

(in units for which the speed of light c=1c=1 ). Show that a timelike geodesic in the equatorial plane obeys

12r˙2+V(r)=12E2\frac{1}{2} \dot{r}^{2}+V(r)=\frac{1}{2} E^{2}

where

2V(r)=(1rsr)(1+h2r2)2 V(r)=\left(1-\frac{r_{s}}{r}\right)\left(1+\frac{h^{2}}{r^{2}}\right)

and EE and hh are constants.

(b) For a circular orbit of radius rr, show that

h2=r2rs2r3rs.h^{2}=\frac{r^{2} r_{s}}{2 r-3 r_{s}} .

Given that the orbit is stable, show that r>3rsr>3 r_{s}.

(c) Alice lives on a small planet that is in a stable circular orbit of radius rr around a (non-rotating) black hole of radius rsr_{s}. Bob lives on a spacecraft in deep space far from the black hole and at rest relative to it. Bob is ageing kk times faster than Alice. Find an expression for k2k^{2} in terms of rr and rsr_{s} and show that k<2k<\sqrt{2}.

Typos? Please submit corrections to this page on GitHub.