where Ωis a domain of M, and νis the normal outward unit vector about ∂Ω
with respect to g. For general Riemannian manifolds, solutions of overdetermined
elliptic problems of the form (1.2) are obtained in [10,11,16,26,27,37].
It is clear that any symmetry result on the solutions of (1.2) tightly depends on
the symmetry of the ambient manifold. In a given arbitrary manifold, geodesic
balls are not domains where (1.2) can be solved. As shown in [10], for small vol-
umes it is possible to construct solutions of (1.2) with f(u) = λ u in perturbations
of geodesic balls centered at specific points of the manifold, but such domains in
general are not geodesic balls. In fact, one can expect to obtain a Serrin-type result
only for manifolds that are symmetric in a suitable sense. More precisely (see also
the introduction of [11]), the key ingredient for the moving plane method is the
use of the reflexion principle in any point and any direction. For this we need that
for any p∈Mand any two vectors v, w ∈TpMthere exists an isometry of Mleav-
ing pfixed and transporting vinto w(i.e. Mis isotropic) and that such isometry
is induced by the reflection with respect to a hypersurface. Such last hypersur-
face must be totally geodesic, being the set of fixed points of an isometry. But an
isotropic manifold admitting totally geodesic hypersurfaces must have constant
sectional curvature (see for example [7], p. 295) and the only isotropic Riemannian
manifolds of constant sectional curvature are the Euclidean space Rd, the round
sphere Sd, the hyperbolic space Hdand the real projective space RPd(see [42]).
Now, domains in RPdarise naturally to domains in its universal covering Sd, so
we are left to consider our problem in Rd,Sdand Hd.
Being the problem in Rdcompletely understood by Serrin, the framework of
the other two space form manifolds has been treated in 1998 in the paper by S.
Kumaresan and J. Prajapat [24]. In the case of Hdthey obtained a complete coun-
terpart of the Serrin’s theorem: namely, by using the moving plane method, they
show that if Ωis a bounded domain of Hdand (1.2) admits a solution, then Ωmust
be a geodesic ball. The case of Sdis different. In fact, even if the reflexion principle
is valid in any point, one needs to have a totally geodesic hypersurface that does
not intersect the domain in order to start the moving plane. This is not a problem
in Rdor Hd, but it is in Sd. Since the totally geodesic hypersurfaces are the equa-
tors, one can start the moving plane method if and only if the domain is contained
on a hemisphere. And this is exactly the case considered in [24]: if Ωis contained
in a hemisphere and (1.2) admits a solution, then Ωmust be a geodesic ball.
Other natural domains of Sdwhere (1.2) has solutions are symmetric neigh-
borhoods of any equator. Such symmetric annuli are not contractible and their
existence comes from the geometry of Sdin the same way as they exist in a cylin-
der or in a torus. Moreover, perturbations of such domains in Sdwhere (1.2) still
admits a solution have been built in [15] in the same way as this has been done for
the same kind of domains in cylinders or in tori [36].
Taking these facts in account, the following question arises naturally: is it true
that if Ω⊂Sdis contractible and (1.2) can be solved, then Ωmust be a geodesic
ball? In [12], J.M. Espinar and L. Mazet give an affirmative answer to this question
if d= 2 but under some extra assumptions on the nonlinear term f(u). The proof
of such result shows again an analogy between overdetermined elliptic problems
and constant mean curvature surfaces, because it is highly inspired by the proof of
3