  The surprising discovery by MAGIC of an intense, rapidly varying emission in
the energy range 70 - 400 GeV from the flat spectrum radio quasar PKS 1222+216
represents a challenge for all interpretative scenarios. Indeed, in order to
avoid absorption of \gamma rays in the dense ultraviolet radiation field of the
broad line region (BLR), one is forced to invoke some unconventional
astrophysical picture, like for instance the existence of a very compact (r\sim
10^{14} cm) emitting blob at a large distance (R \sim10^{18} cm) from the jet
base. We offer the investigation of a scenario based on the standard blazar
model for PKS 1222+216 where \gamma rays are produced close to the central
engine, but we add the new assumption that inside the source photons can
oscillate into axion-like particles (ALPs), which are a generic prediction of
several extensions of the Standard Model of elementary particle interactions.
As a result, a considerable fraction of very-high-energy photons can escape
absorption from the BLR through the mechanism of photon-ALP oscillations much
in the same way as they largely avoid absorption from extragalactic background
light when propagating over cosmic distances in the presence of large-scale
magnetic fields in the nG range. In addition we show that the above MAGIC
observations and the simultaneous Fermi/LAT observations in the energy range
0.3 - 3 GeV can both be explained by a standard spectral energy distribution
for experimentally allowed values of the model parameters. In particular, we
need a very light ALP just like in the case of photon-ALP oscillations in
cosmic space. Moreover, we find it quite tantalizing that the most favorable
value of the photon-ALP coupling happens to be the same in both situations.
Although our ALPs cannot contribute to the cold dark matter, they are a viable
candidate for the quintessential dark energy. [abridged]
