“…Among the reactions of interest, AsFiN considers the 14 O(α,p) 17 F and the 18 Ne(α,p) 21 Na that could be the onset of a possible route that breaks out from the HCNO cycles, and the 34 Ar(α,p) 37 K, since 34 Ar is a waiting point in X-ray bursts nucleosynthesis. As long as SPES will not be available, the AsFiN collaboration plans to perform these measurements at LNS using the in Flight Radioactive Ion Beams (FRIBs) facility at LNS [161] and at other RIBs facilities such as CRIB-RIKEN and MARS-TAMU; then the research activity will be shifted on RIBs at SPES, owing to the foreseen intensities and beam quality. In particular, there is an accepted letter of intent about measurements involving 26 Al m (isomeric state at 228 keV, T 1/2 = 6.35 s) beam, for studying the 26 Al m (n,α) 23 Na and the 26 Al m (n,p) 26 Mg reactions by means of the THM, using a deuteron to transfer a neutron.…”