  The information paradox can be realized in anti-de Sitter spacetime joined to
a Minkowski region. In this setting, we show that the large discrepancy between
the von Neumann entropy as calculated by Hawking and the requirements of
unitarity is fixed by including new saddles in the gravitational path integral.
These saddles arise in the replica method as complexified wormholes connecting
different copies of the black hole. As the replica number $n \to 1$, the
presence of these wormholes leads to the island rule for the computation of the
fine-grained gravitational entropy. We discuss these replica wormholes
explicitly in two-dimensional Jackiw-Teitelboim gravity coupled to matter.
