  Moduli fields with Planck-suppressed couplings to light species are common in
string compactifications. Decays of these moduli can reheat the universe at a
late time and produce dark matter non-thermally. For generic moduli fields
motivated by string theory with masses similar to that of the gravitino and
TeV-scale superpartners in the minimal supersymmetric Standard Model (MSSM),
the non-thermal production of the lightest superpartner (LSP) tends to create
an unacceptably large relic density or too strong of an indirect detection
signal. We call this the moduli-induced LSP problem of the MSSM. In this paper
we investigate extensions of the MSSM containing new LSP candidates that can
alleviate this tension. We examine the viability of this scenario in models
with light Abelian and non-Abelian hidden sectors, and symmetric or asymmetric
dark matter. In these extensions it is possible, though somewhat challenging,
to avoid a moduli-induced LSP problem. In all but the asymmetric scenario, the
LSP can account for only a small fraction of the observed dark matter density.
