The cold and hot CNO cycles
M Wiescher, J Görres, E Uberseder… - Annual Review of …, 2010 - annualreviews.org
New experimental methods and techniques, combined with the development of new
theoretical tools, have opened new avenues to explore nuclear reactions of significance for …
theoretical tools, have opened new avenues to explore nuclear reactions of significance for …
Nuclear astrophysics: the unfinished quest for the origin of the elements
Half a century has passed since the foundation of nuclear astrophysics. Since then, this
discipline has reached its maturity. Today, nuclear astrophysics constitutes a …
discipline has reached its maturity. Today, nuclear astrophysics constitutes a …
Charged-particle thermonuclear reaction rates: II. Tables and graphs of reaction rates and probability density functions
Numerical values of charged-particle thermonuclear reaction rates for nuclei in the A= 14 to
40 region are tabulated. The results are obtained using a method, based on Monte Carlo …
40 region are tabulated. The results are obtained using a method, based on Monte Carlo …
Charged-particle thermonuclear reaction rates: III. Nuclear physics input
The nuclear physics input used to compute the Monte Carlo reaction rates and probability
density functions that are tabulated in the second paper of this series (Paper II) is presented …
density functions that are tabulated in the second paper of this series (Paper II) is presented …
Improved Direct Measurement of the 64.5 keV Resonance Strength in the Reaction at LUNA
The O 17 (p, α) N 14 reaction plays a key role in various astrophysical scenarios, from
asymptotic giant branch stars to classical novae. It affects the synthesis of rare isotopes such …
asymptotic giant branch stars to classical novae. It affects the synthesis of rare isotopes such …
New high accuracy measurement of the (,) reaction rate at astrophysical temperatures
The O 17 (p, α) N 14 reaction is of fundamental relevance in several astrophysical scenarios,
such as novae, asymptotic giant branch nucleosynthesis, and γ-ray astronomy. We report on …
such as novae, asymptotic giant branch nucleosynthesis, and γ-ray astronomy. We report on …
The RGB and AGB Star Nucleosynthesis in Light of the Recent 17O (p, α) 14N and 18O (p, α) 15N Reaction-rate Determinations
S Palmerini, ML Sergi, M La Cognata… - The Astrophysical …, 2013 - iopscience.iop.org
In recent years, the Trojan Horse Method (THM) has been used to investigate the low-
energy cross sections of proton-induced reactions on A= 17 and A= 18 oxygen isotopes …
energy cross sections of proton-induced reactions on A= 17 and A= 18 oxygen isotopes …
Improvement of the high-accuracy reaction-rate measurement via the Trojan Horse method for application to nucleosynthesis
The O 17 (p, α) N 14 and O 17 (p, γ) F 18 reactions are of paramount importance for the
nucleosynthesis in a number of stellar sites, including red giants (RGs), asymptotic giant …
nucleosynthesis in a number of stellar sites, including red giants (RGs), asymptotic giant …
Resonance strengths in the 17,18O(p, α)14,15N reactions and background suppression underground: Commissioning of a new setup for charged-particle detection …
LUNA Collaboration, CG Bruno, DA Scott… - The European Physical …, 2015 - Springer
We report on measurements of resonance strengths and energies for the E_p=151 and 193
keV resonances in the 18 O (p, α) 15 N and 17 O (p, α) 14 N reactions, respectively …
keV resonances in the 18 O (p, α) 15 N and 17 O (p, α) 14 N reactions, respectively …
New reaction rate for () and its influence on the oxygen isotopic ratios in massive AGB stars
The O 16 (p, γ) F 17 reaction rate is revisited with special emphasis on the stellar
temperature range of T= 60-100 MK, important for hot bottom burning in asymptotic giant …
temperature range of T= 60-100 MK, important for hot bottom burning in asymptotic giant …