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Trojan Horse Investigation for AGB Stellar Nucleosynthesis [PDF]

open access: goldUniverse, 2022
Asymptotic Giant Branch (AGB) stars are among the most important astrophysical sites influencing the nucleosynthesis and the chemical abundances in the Universe. From a pure nuclear point of view, several processes take part during this peculiar stage of
Maria Letizia Sergi   +17 more
doaj   +3 more sources

Electron Capture Cross Sections for Stellar Nucleosynthesis [PDF]

open access: goldAdvances in High Energy Physics, 2015
In the first stage of this work, we perform detailed calculations for the cross sections of the electron capture on nuclei under laboratory conditions.
P. G. Giannaka, T. S. Kosmas
doaj   +6 more sources

Neutron-Driven Nucleosynthesis in Stellar Plasma

open access: yesFrontiers in Physics, 2022
A large uncertainty for the slow neutron capture nucleosynthesis (s-process) models is caused by the amount of neutrons available to the process itself.
R. Spartà   +24 more
doaj   +2 more sources

Underground laboratory JUNA shedding light on stellar nucleosynthesis [PDF]

open access: bronzeNuclear Science and Techniques, 2023
Extremely low background experiments to measure key nuclear reaction cross sections of astrophysical interest are conducted at the world's deepest underground laboratory, the Jingping Underground laboratory for Nuclear Astrophysics (JUNA). High precision
Toshitaka Kajino
openalex   +3 more sources

The nebular spectra of SN 2012aw and constraints on stellar nucleosynthesis from oxygen emission lines [PDF]

open access: bronze, 2014
We present nebular-phase optical and near-infrared spectroscopy of the Type IIP supernova SN 2012aw combined with non-local thermodynamic equilibrium radiative transfer calculations applied to ejecta from stellar evolution/explosion models.
Anders Jerkstrand   +6 more
openalex   +3 more sources

Presolar Grain Isotopic Ratios as Constraints to Nuclear and Stellar Parameters of Asymptotic Giant Branch Star Nucleosynthesis [PDF]

open access: bronzeAstrophysical Journal, 2021
Recent models for evolved low-mass stars (with M ≲ 3 M ⊙), undergoing the asymptotic giant branch (AGB) phase assume that magnetic flux-tube buoyancy drives the formation of 13C reservoirs in He-rich layers.
S. Palmerini   +10 more
openalex   +3 more sources

Residual Abundances in GALAH DR3: Implications for Nucleosynthesis and Identification of Unique Stellar Populations [PDF]

open access: goldAstrophysical Journal, 2022
We investigate the [X/Mg] abundances of 16 elements for 82,910 Galactic disk stars from GALAH+ DR3. We fit the median trends of low-Ia and high-Ia populations with a two-process model, which describes stellar abundances in terms of a prompt core-collapse
Emily J. Griffith   +5 more
openalex   +3 more sources

The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars [PDF]

open access: bronzePublications Astronomical Society of Australia, 2014
The chemical evolution of the Universe is governed by the chemical yields from stars, which in turn are determined primarily by the initial stellar mass.
Amanda I. Karakas, John C. Lattanzio
openalex   +3 more sources

Stellar signatures of inhomogeneous big bang nucleosynthesis [PDF]

open access: hybrid, 2020
We evaluate abundance anomalies generated in patches of the Universe where the baryon-to-photon ratio was locally enhanced by possibly many orders of magnitude in the range η=10-10–10-1.
Alexandre Arbey   +2 more
openalex   +3 more sources

Deep Mixing of 3 He: Reconciling Big Bang and Stellar Nucleosynthesis [PDF]

open access: greenScience, 2006
Low-mass stars, ∼1 to 2 solar masses, near the Main Sequence are efficient at producing the helium isotope 3He, which they mix into the convective envelope on the giant branch and should distribute into the Galaxy by way of envelope loss. This process is
P. P. Eggleton   +2 more
openalex   +3 more sources

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