2 CHRISTIAN BÄR AND PENELOPE GEHRING
the Cauchy problem. The manifolds considered in these results are spacetimes with
timelike boundary, i.e. the Cauchy hypersurfaces have a boundary themselves. Fur-
ther studies of Green-hyperbolic operators on such spacetimes were accomplished,
for example, in [20–22,25,27]. These results are concerned with local boundary
conditions. Since analytically reasonable local boundary conditions do not always
exist for first-order operators, it is necessary to study global boundary conditions
such as APS boundary conditions.
APS boundary conditions cannot be imposed on the boundary of the spacetime
itself because this boundary is Lorentzian rather than Riemannian. To overcome
this difficulty, Drago, Große and Murro suggested in [23] to choose a time function
and to impose APS on each level set. They stated well-posedness of the Cauchy
problem for the spinorial Dirac operator under slicewise APS conditions assuming
a few further conditions on the geometry of the spacetime. However, it seems that
there is a gap in their existence proof.
We also take this local-in-time, global-in-space approach and fix a time function.
The boundary conditions which we impose on the level sets need not be APS but
APS is included in our class of admissible boundary conditions. Another prominent
example consists of the transmission conditions - this may potentially allow for cut-
and-paste arguments.
In Section 1, we recall the most important facts on elliptic boundary problems for
Dirac-type operators on compact Riemannian manifolds with boundary. This the-
ory was initiated by Atiyah, Patodi, and Singer in their famous paper [3]. Here they
introduced the APS boundary conditions. There is a huge literature on this topic.
We follow the approach laid out by Bär and Ballmann in [7,8] because it describes
all possible boundary conditions systematically.
This describes what can be done on a fixed spacelike Cauchy hypersurface. We
then discuss families of boundary value problems in Section 2. We need to study
such families as the time function sweeps out our spacetime.
Next,we recall the most important facts of spin geometry and the spinorial Dirac
operator on spacetimes with timelike boundary in Section 3. We define what we
mean by an admissible boundary conditions.
Section 4is the core of the present paper. Here we prove well-posedness of the
Cauchy problem for the spinorial Dirac operator under admissible boundary condi-
tions, see Theorem 4.1.
We apply these results in Section 5and study the support of the solutions to the
Cauchy problem. The result essentially says that a wave propagates with the speed
of light at most. There is an interesting violation of this principle, however. As
soon as the wave hits the boundary somewhere, the whole boundary radiates off
instantenously (w.r.t. the given time function). This is due to the global nature
of the boundary conditions and violates the causal principle that no signal should
propagate fast than with the speed of light. We show by example that this effect
really occurs.
Then we use well-posedness together with finite propagation speed to construct
advanced and retarded Green’s operators.