4. ASYMPTOTICS OF THE HEAT KERNEL FOR A STATIC METRIC 255
Now we compute the expansion for </>1 up to first order. From (23.26)
we have
</>1 (x, y) = a-^1 /^2 (x, y) fo
1
( a^112 b.x<Po) (expy (pr (x). V), y) dp,
where V E TyM is the unit vector tangent to the unique minimal geodesic
from y to x. Let {xi} be geodesic normal coordinates centered at y and let
xi also denote the i-th coordinate of x. We have xi (expy (pr (x) V)) = pxi.
By (23.124) and since a^112 = 1+0 (r^2 ), we have
( a^112 b.x
Hence, using a-^112 (x, y) = 1+0 (r (x)^2 ), we have
From this we immediately obtain
LEMMA 23.33.
(23.125)
REMARK 23.34. We have
1 12 1 2 1 2
(23.126) </>2 (y, y) =
30
b.R + 72 R - 180 IRcl + 180 IRml ,
where 1Rcl^2 ~ gikgj.e.RijRke and 1Rml^2 ~ gipgjqgkris~jk£Rpqrs and the RHS
is evaluated at y (see Gilkey [72]).
time-dependent metric 3. Aspects of the asymptotics of the heat kernel for a
manifold.
Motivated by §9.6 in Perelman [152], we consider an aspect of the heat
kernel asymptotics on a fixed Riemannian manifold related to entropy.
Differentiating the logarithm of (23.9), i.e., differentiating the equation
(23.127) 2( ) ( N )
n d x,y k
logHN=--log(41T't)-
4
+log L<f>kt ,
2 t k=O
in both time and space, we have
.§.__lo H - _!!_ d2 (x, y) I:f=1 k<f>ktk-1
at g N - 2t + 4t^2 + °'\:"'N A-tk
L..k=O '+'k
= _!!_ d2 (x, y) </>1 0 (t)
2t + 4t^2 + <Po +