  We obtain the accretion, evaporation and superradiance phase diagram of
astrophysical and primordial black holes in the mass range $10^{-33}-10^{11} \,
M_\odot $. This black hole mass range corresponds to production of $10^{-21} -
10^{21}$ eV particles for superradiance (bosons) and evaporation (bosons and
fermions). Only accretion and superradiance processes are relevant for heavy
black holes, on the other hand for light black holes of primordial origin, all
three processes can be relevant. We find that superradiance instability can
happen even for black hole spin values as low as $10^{-9}-10^{-2}$. Since light
black holes are very unstable to these perturbations and sensitive probes of
bosonic particles, a single moderately spinning BH can probe 2-9 orders of
magnitude of mass parameter space depending on the nature of the perturbations
that are scalar (axion), vector (dark photon and/or photon with effective mass)
and spin-2. If spinning black holes are observed, namely superradiance is not
observed, due to self-interactions, we find limits on the axion decay constant
and energy density.
