Results 111 to 120 of about 10,538 (228)
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page i-xlii, August 2024.
wiley +2 more sources
Core-collapse supernovae and nucleosynthesis [PDF]
I discuss some of the physics that governs the collapse and explosion of a massive star, including issues such as lepton number losses in the infall stage and neutrino heating and convection following the core bounce. I review recent work on the neutrino
Haxton, W. C., Haxton, W C
core
From the s-Process to the i-Process: A New Perspective on the Chemical Enrichment of Extrinsic Stars
Separating stars enriched in the s- and r-processes of nucleosynthesis is usually achieved by analyzing the element ratios of s-process elements (like Ba or La) to r-process elements (like Eu).
Sophie Van Eck +11 more
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Contents
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 2-29, August 2025.
wiley +1 more source
Exploring Nucleosynthesis Models through Inertial Confinement Fusion
openUnderstanding the origin and evolution of the elements remains one of the key challenges in astro- physics. While traditional nucleosynthesis studies rely on accelerator-based experiments conducted in underground laboratories, these setups are ...
PAVAN, LIDIA GIUDITTA
core
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
New Results on Nucleosynthesis in Massive Stars; Nuclear Data Needs for Nucleosynthesis
We review the current status of the nuclear reaction rates needed to study nucleosynthesis in massive stars. Results for the calculated nucleosynthesis of all stable species from Hydrogen to Bismuth in a completely evolved 25 M{sub {circle_dot}} star of ...
Rauscher, T +3 more
core
Neutrino-driven winds and nucleosynthesis [PDF]
Baryonic outflows from proto-neutron stars formed in core-collapse supernova explosions are one of the possible scenarios for the production of heavy elements via the r-process.
O'Connor, E. +6 more
core
From (p)reheating to nucleosynthesis
This paper gives a brief qualitative description of the possible evolution of the early universe between the end of an inflationary epoch and the end of big-bang nucleosynthesis.
Jedamzik, K.
core
Constraints on Tsallis Cosmology from Big Bang Nucleosynthesis and the Relic Abundance of Cold Dark Matter Particles. [PDF]
Jizba P, Lambiase G.
europepmc +1 more source

