5.1 Recall that the partition function for the canonical
ensemble at temperature
is given by
where
is a "density
of states" measure, which does not depend on
Then one
computes the average energy
the entropy
and the fluctuation
Now fix a closed manifold with a probability measure
,
and suppose that our system is described by a metric
which depends on the temperature
according
to equation
where
and the partition
function is given by
(We do not
discuss here what assumptions on
guarantee that the
corresponding "density of states" measure can be found) Then we
compute
Alternatively, we could
prescribe the evolution equations by replacing the -derivatives
by minus
-derivatives in (3.3 ), and get the same formulas
for
with
replaced by
Clearly, is nonnegative; it vanishes only on a gradient
shrinking soliton.
is nonnegative as well, whenever the flow
exists for all sufficiently small
(by proposition 1.2).
Furthermore, if (a)
tends to a
-function as
or (b)
is a limit of a sequence of functions
such
that each
tends to a
-function as
and
then
is also nonnegative. In case (a) all
the quantities
tend to zero as
while
in case (b), which may be interesting if
goes
singular at
the entropy
may tend to a positive
limit.
If the flow is defined for all sufficiently large
(that is, we have an ancient solution to the Ricci flow, in
Hamilton's terminology), we may be interested in the behavior of
the entropy
as
A natural question is whether
we have a gradient shrinking soliton whenever
stays bounded.
5.2 Remark. Heuristically, this statistical analogy is related to the description of the renormalization group flow, mentioned in the introduction: in the latter one obtains various quantities by averaging over higher energy states, whereas in the former those states are suppressed by the exponential factor.
5.3* An entropy formula for the Ricci flow in dimension two was found by Chow [C]; there seems to be no relation between his formula and ours.
The interplay of statistical physics and (pseudo)-riemannian geometry occurs in the subject of Black Hole Thermodynamics, developed by Hawking et al. Unfortunately, this subject is beyond my understanding at the moment.