  Multiple Populations represent the standard for Globular Clusters (GC): a
fraction (10-50%) of their stars have the same elemental abundances of halo
stars of similar metallicity (first generation, or 1G), but the other stars
(second generation, 2G) are characterised by patterns of light elements
abundances which resemble those typical of gas processed by proton-capture
reactions at high temperature. Consequently, we should naively expect that
Lithium is destroyed in the 2G stars, but instead it is generally observed, at
abundances only slightly depleted with respect to the 1G stars. After
discussing the models for the formation of multiple populations, I examine the
role of dilution with pristine gas and the possible role of the Asymptotic
Giant Branch (AGB) scenario in accounting for the Lithium patterns in GC stars.
Super-AGB and AGB yields of Lithium, produced by the Cameron Fowler mechanism
in the `Hot Bottom Burning' convective envelopes, may help to explain the
peculiar high Lithium in a few extreme 2G stars. On the other hand, modeling
the abundances in mild 2G stars depends explicitly on whether the initial Li in
the gas forming the 1G stars and the diluting gas of the 2G ones is that
predicted by the Big Bang nucleosynthesis or the ~3 times smaller value
observed at the surface of halo dwarfs.
