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physics.ins-det2024
The Felsenkeller shallow-underground laboratory for nuclear astrophysics
Daniel Bemmerer, Axel Boeltzig, Marcel Grieger +12
In the Felsenkeller shallow-underground site, protected from cosmic muons by a 45 m thick rock overburden, a research laboratory including a 5 MV Pelletron ion accelerator and a nu…
nucl-ex2024
First direct measurement of the 64.5 keV resonance strength in O(p,)F reaction
R. M. Gesuè, G. F. Ciani, D. Piatti +50
The CNO cycle is one of the most important nuclear energy sources in stars. At temperatures of hydrostatic H-burning (20 MK T 80 MK) the O(p,)F reaction r…