The horizon of a static black hole in anti-de Sitter space can be spherical
, planar, or hyperbolic. The microscopic dynamics of the first two classes
of black holes have been extensively discussed recently within the context
of the AdS/CFT correspondence. We argue that hyperbolic black holes introdu
ce new and fruitful features in this respect, allowing for more detailed co
mparisons between the weak and strong coupling regimes. In particular, by f
ocussing on the stress tensor and entropy of some particular states, we ide
ntify unexpected increases in the entropy of Super-Yang-Mills theory at str
ong coupling that are not accompanied by increases in the energy. We descri
be a highly degenerate state at zero temperature and zero energy density. W
e also find that the entanglement entropy across a Rindler horizon in exact
AdS(5) is larger than might have been expected from the dual SYM theory. B
esides, we show that hyperbolic black holes can be described as thermal Rin
dler states of the dual conformal field theory in at space.