Origin of the elements
A Arcones, FK Thielemann - The Astronomy and Astrophysics Review, 2023 - Springer
What is the origin of the oxygen we breathe, the hydrogen and oxygen (in form of water
H2O) in rivers and oceans, the carbon in all organic compounds, the silicon in electronic …
H2O) in rivers and oceans, the carbon in all organic compounds, the silicon in electronic …
Neutrinos and nucleosynthesis of elements
T Fischer, G Guo, K Langanke… - Progress in Particle and …, 2024 - Elsevier
Neutrinos are known to play important roles in many astrophysical scenarios from the early
period of the big bang to current stellar evolution being a unique messenger of the fusion …
period of the big bang to current stellar evolution being a unique messenger of the fusion …
Nuclei in core-collapse supernovae engine
S Furusawa, H Nagakura - Progress in Particle and Nuclear Physics, 2023 - Elsevier
Herein, we review the nuclear equations of state (EOSs) and the constituent nuclei of core-
collapse supernovae (CCSNe) and their roles in CCSN simulations. Various nuclei such as …
collapse supernovae (CCSNe) and their roles in CCSN simulations. Various nuclei such as …
Spin-isospin excitations in the direction of decay for and at finite temperature
We investigate the Gamow-Teller (GT) and spin-dipole (SD) transitions in the direction of β+
decay for neutron-rich N= 50 nucleus Zn 80 and N= 82 nucleus Ru 126, which are important …
decay for neutron-rich N= 50 nucleus Zn 80 and N= 82 nucleus Ru 126, which are important …
Multipole responses in fissioning nuclei and their uncertainties
T Li, N Schunck, M Grosskopf - Physical Review C, 2024 - APS
Electromagnetic multipole responses are key inputs to model the structure, decay, and
reactions of atomic nuclei. With the introduction of the finite amplitude method (FAM), large …
reactions of atomic nuclei. With the introduction of the finite amplitude method (FAM), large …
Comparison of electron capture rates in the N= 50 region using 1D simulations of core-collapse supernovae
Z Johnston, S Wasik, R Titus, MKL Warren… - The Astrophysical …, 2022 - iopscience.iop.org
Recent studies have highlighted the sensitivity of core-collapse supernovae (CCSNe)
models to electron-capture (EC) rates on neutron-rich nuclei near the N= 50 closed-shell …
models to electron-capture (EC) rates on neutron-rich nuclei near the N= 50 closed-shell …
Original e− Capture Cross Sections for Hot Stellar Interior Energies
P Giannaka, T Kosmas, H Ejiri - Particles, 2022 - mdpi.com
The nuclear electron capture reaction possesses a prominent position among other weak
interaction processes occurring in explosive nucleosynthesis, especially at the late stages of …
interaction processes occurring in explosive nucleosynthesis, especially at the late stages of …
The axially-deformed relativistic quasiparticle random phase approximation based on point-coupling interactions
Collective nuclear excitations, like giant resonances, are sensitive to nuclear deformation, as
evidenced by alterations in their excitation energies and transition strength distributions. A …
evidenced by alterations in their excitation energies and transition strength distributions. A …
Self-consistent microscopic calculations for electron captures on nuclei in core-collapse supernovae
Calculations for electron capture rates on nuclei with atomic numbers between $ Z= 20$ and
$ Z= 52$ are performed in a self-consistent finite-temperature covariant energy density …
$ Z= 52$ are performed in a self-consistent finite-temperature covariant energy density …
Strong Coupling of Hydrodynamics and Reactions in Nuclear Statistical Equilibrium for Modeling Convection in Massive Stars
We build on the simplified spectral deferred corrections (SDC) coupling of hydrodynamics
and reactions to handle the case of nuclear statistical equilibrium (NSE) and …
and reactions to handle the case of nuclear statistical equilibrium (NSE) and …