Results 111 to 120 of about 24,208 (239)

The β-decay rates of 59Fe isotopes in shell burning environments and their influences on the production of 60Fe in massive star

open access: yesEPJ Web of Conferences, 2016
The experimental B(GT) strengths of the 59Fe excited states were employed to determine the transition strengths which greatly contribute 59Fe stellar β–decay at typical carbon shell burning temperature.
Li K.   +4 more
doaj   +1 more source

Stellar Nucleosynthesis Nuclear Data Mining

open access: yes, 2012
Stellar nucleosynthesis is an important nuclear physics phenomenon that is responsible for presently observed chemical elements and isotope abundances. It is also one of the corner stone hypotheses that provides basis for our understanding of Nature. Its theoretical predictions are often verified through the astrophysical observation and comparison of ...
openaire   +4 more sources

87th Annual Meeting of the Meteoritical Society 2025: Abstracts

open access: yes
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley   +1 more source

On the Sensitivity of Massive Star Nucleosynthesis and Evolution to Solar Abundances and to Uncertainties in Helium Burning Reaction Rates

open access: yes, 2007
We explore the dependence of pre-supernova evolution and supernova nucleosynthesis yields on the uncertainties in helium burning reaction rates. Using the revised solar abundances of Lodders (2003) for the initial stellar composition, instead of those of
Alexander Heger   +3 more
core   +1 more source

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

open access: bronze, 2014
Anders Jerkstrand   +6 more
openalex   +1 more source

Corrigendum: “Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesis” [Phys. Lett. B 790 (2019) 458–465]

open access: diamond, 2023
C. Lederer-Woods   +99 more
openalex   +1 more source

TheZr92(n,γ) reaction and its implications for stellar nucleosynthesis [PDF]

open access: bronze, 2010
G. Tagliente   +99 more
openalex   +1 more source

Underground nuclear astrophysics studies with CASPAR

open access: yesEPJ Web of Conferences, 2016
The drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to stellar burning processes and elemental production through stellar nucleosynthesis, over the energy range of astrophysical interest.
Robertson Daniel   +4 more
doaj   +1 more source

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