Hyperons in Neutron Stars

In this work I briefly review some of the effects of hyperons on the properties of neutron and proto-neutron stars. In particular, I revise the problem of the strong softening of the EoS, and the consequent reduction of the maximum mass, induced by the presence of hyperons, a puzzle which has become more intringuing and difficult to solve because of the recent measurements of the unusually high masses of the millisecond pulsars PSR J1903+0327 ,(1.667 +/- 0.021 M-circle dot), PSR J1614-2230 (1.97 +/- 0.04 M-circle dot), and PSR J0348+0432 (2.01 +/- 0.04 M-circle dot). Some of the solutions proposed to tackle this problem are discussed. Finally, I re-examine also the role of hyperons on the cooling properties of newly born neutron stars and on the so-called r-mode instability.