255 citations · 1.1k across the 23 of their papers we have counts for
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Lifetime measurements of excited states in O
B. Frentz, A. Aprahamian, A. M. Clark +14
The CNO cycle is the main energy source in stars more massive than our sun, it defines the energy production and the cycle time that lead to the lifetime of massive stars, and it i…
The 12C(a,g)16O reaction and its implications for stellar helium burning
R. J. deBoer, J. Gorres, M. Wiescher +10
The creation of carbon and oxygen in our universe is one of the forefront questions in nuclear astrophysics. The determination of the abundance of these elements is key to both our…
Experimental study of the astrophysical gamma-process reaction 124Xe(alpha,gamma)128Ba
Z. Halász, E. Somorjai, Gy. Gyürky +8
The synthesis of heavy, proton rich isotopes in the astrophysical gamma-process proceeds through photodisintegration reactions. For the improved understanding of the process, the r…
Probing astrophysically important states in Mg nucleus to study neutron sources for the -Process
R. Talwar, T. Adachi, G. P. A. Berg +20
The Ne(,n)Mg reaction is the dominant neutron source for the slow neutron capture process (-process) in massive stars and contributes, together with the …
Experimental cross sections of 165Ho(α,n)168Tm and 166Er(α,n)169Yb for optical potential studies relevant for the astrophysical γ-process
Jan Glorius, Kerstin Sonnabend, Joachim Goerres +10
Background: Optical potentials are crucial ingredients for the prediction of nuclear reaction rates needed in simulations of the astrophysical γ-process. Associated uncertainties a…
Measurement of the Ni(,)Zn reaction and its astrophysical impact
S. J. Quinn, A. Spyrou, E. Bravo +23
Cross section measurements of the Ni(,)Zn reaction were performed in the energy range MeV at the Nuclear Science Laboratory of the University of N…