  Primordial black holes (PBHs) are black holes which may form in the early
Universe through the gravitational collapse of primordial cosmological density
fluctuations. Due to Hawking radiation these PBHs are supposed to evaporate by
emitting particles. Recent developments in the experimental searching for
evaporating PBHs in the local Universe are reviewed. The multimessenger
techniques of searching for signals from evaporating PBHs are discussed.
