Collapse models represent one of the possible solutions to the measurement problem. These models modify the Schrödinger dynamics with non-linear and stochastic terms, which guarantee the localization in space of the wave function avoiding macroscopic superpositions, like that described in the Schrödinger's cat paradox. The Ghirardi-Rimini-Weber (GRW) and the Continuous Spontaneous Localization (CSL) models are the most studied among the collapse models. Here, we briefly summarize the main features of these models and the advances in their experimental investigation.3 It possible to define the model also through a stochastic differential equation describing the interaction with a Poissonian noise, see Smirne et al. (2014); Toroš et al. (2016). 4 In their original formulation Ghirardi et al. (1986), Ghirardi, Rimini and Weber considered the possibility that different particles can have different collapse rate λi. However, this is not required and in literature only one λ, representing the collapse rate for a nucleon, is considered. For composite objects, the corresponding total collapse rate can be calculated through the amplification mechanism discussed below.