300 7. THE REDUCED DISTANCE
SOLUTION TO EXERCISE 7.21. Consider a maximal Einstein solution
to the backward Ricci flow h (r), TE [O, T), where Re= - 2 (i-T)h is nega-
tive. In this case h (r) = TTT h (0) (which is easy to see from Rch(T) being
independent of r). The £-geodesic equation (7.32) for/ (r) is
(7.38) V'xX +(I_ --
1
-) X = 0.
2T T-T
Let f3 (p) ~ / (J (p)) , where 1 is defined by
J' u-l (r)) ~exp (/
7
( 2 ~ - T ~ r) dr)
=fi(T-r),
i.e., l' (p) = VTfP) (T - 1 (p)). Then /3 (p) ~ ~ = ~; (J (p)) l' (p). Let
T ~ 1 (p). Equation (7.38) and the definition of 1 imply
\i' /3(p)/3 (p) = \i' f'(p)!r;(T) (t (p) ~~ (7))
= J" (p) d1 (r) _ l' (p) l' (p) (I_ __ 1_) d1 (r)
dr 2r T-r dr
= !!__ (1' (p) - exp (Jf(p) (
1
_ - ~) dr)). di (r)
~ ~ T~r ~
=0.
That is, f3 (p) is a constant speed geodesic with respect to h (0). We make
the rationalizing substitution x : VTfP), so that
=! l'(p)dp = 2 / dx =-l lo (VT+x)
p VTfP) (T - 1 (p)) T - x^2 VT g VT - x ·
That is,
1 (p) = x2 = T (-e~_TP-_1)2
evTp + 1
or
1-1 (r) = _1 log (VT+ VT).
VT VT-./T
Using I ( T) = f3 u-^1 ( T)) and the fact that f3 is constant speed with re~pect
to h (0), we compute
l
dr/
2
= T-r j/J(J-l(r))j2 d(J-1)
2
dr h(T) T h(O) dr Tr (T-r)'
canst
since h (r) = TY,^7 h (0) and
d u-1) - (^1 1)