The process: Nuclear physics, stellar models, and observations
F Käppeler, R Gallino, S Bisterzo, W Aoki - Reviews of Modern Physics, 2011 - APS
Nucleosynthesis in the s process takes place in the He-burning layers of low-mass
asymptotic giant branch (AGB) stars and during the He-and C-burning phases of massive …
asymptotic giant branch (AGB) stars and during the He-and C-burning phases of massive …
LUNA: Status and prospects
The essential ingredients of nuclear astrophysics are the thermonuclear reactions which
shape the life and death of stars and which are responsible for the synthesis of the chemical …
shape the life and death of stars and which are responsible for the synthesis of the chemical …
NACRE II: an update of the NACRE compilation of charged-particle-induced thermonuclear reaction rates for nuclei with mass number A< 16
Y Xu, K Takahashi, S Goriely, M Arnould, M Ohta… - Nuclear Physics A, 2013 - Elsevier
An update of the NACRE compilation [3] is presented. This new compilation, referred to as
NACRE II, reports thermonuclear reaction rates for 34 charged-particle induced, two-body …
NACRE II, reports thermonuclear reaction rates for 34 charged-particle induced, two-body …
Direct Measurement of the Cross Section into the -Process Gamow Peak
One of the main neutron sources for the astrophysical s process is the reaction C 13 (α, n) O
16, taking place in thermally pulsing asymptotic giant branch stars at temperatures around …
16, taking place in thermally pulsing asymptotic giant branch stars at temperatures around …
The s-process in asymptotic giant branch stars of low metallicity and the composition of carbon-enhanced metal-poor stars
We present models for the slow neutron-capture process (s-process) in asymptotic giant
branch stars of metallicity [Fe/H]=− 2.3 and masses 0.9–6 M☉. We encountered different …
branch stars of metallicity [Fe/H]=− 2.3 and masses 0.9–6 M☉. We encountered different …
CONVECTIVE–REACTIVE PROTON–12C COMBUSTION IN SAKURAI'S OBJECT (V4334 SAGITTARII) AND IMPLICATIONS FOR THE EVOLUTION AND YIELDS …
F Herwig, M Pignatari, PR Woodward… - The Astrophysical …, 2011 - iopscience.iop.org
Depending on mass and metallicity as well as evolutionary phase, stars occasionally
experience convective–reactive nucleosynthesis episodes. We specifically investigate the …
experience convective–reactive nucleosynthesis episodes. We specifically investigate the …
Evolution and nucleosynthesis of asymptotic giant branch stellar models of low metallicity
CK Fishlock, AI Karakas, M Lugaro… - The Astrophysical …, 2014 - iopscience.iop.org
We present stellar evolutionary tracks and nucleosynthetic predictions for a grid of stellar
models of low-and intermediate-mass asymptotic giant branch (AGB) stars at Z= 0.001 …
models of low-and intermediate-mass asymptotic giant branch (AGB) stars at Z= 0.001 …
Deep Underground Laboratory Measurement of in the Gamow Windows of the and Processes
B Gao, TY Jiao, YT Li, H Chen, WP Lin, Z An, LH Ru… - Physical Review Letters, 2022 - APS
The C 13 (α, n) O 16 reaction is the main neutron source for the slow-neutron-capture
process in asymptotic giant branch stars and for the intermediate process. Direct …
process in asymptotic giant branch stars and for the intermediate process. Direct …
CIELO collaboration summary results: international evaluations of neutron reactions on uranium, plutonium, iron, oxygen and hydrogen
The CIELO collaboration has studied neutron cross sections on nuclides that significantly
impact criticality in nuclear technologies-235,238 U, 239 Pu, 56 Fe, 16 O and 1 H-with the …
impact criticality in nuclear technologies-235,238 U, 239 Pu, 56 Fe, 16 O and 1 H-with the …
Horizons: nuclear astrophysics in the 2020s and beyond
Nuclear astrophysics is a field at the intersection of nuclear physics and astrophysics, which
seeks to understand the nuclear engines of astronomical objects and the origin of the …
seeks to understand the nuclear engines of astronomical objects and the origin of the …