Nucleosynthesis Predictions and High-Precision Deuterium Measurements
Two new high-precision measurements of the deuterium abundance from absorbers along the line of sight to the quasar PKS1937–1009 were presented. The absorbers have lower neutral hydrogen column densities (N(HI) ≈ 18 cm − 2 ) than for previous ...
Signe Riemer-Sørensen +1 more
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Dynamical ejecta of neutron star mergers with nucleonic weak processes\n I: Nucleosynthesis [PDF]
I Kullmann +5 more
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r -process nucleosynthesis from matter ejected in binary neutron star mergers [PDF]
When binary systems of neutron stars merge, a very small fraction of their rest mass is ejected, either dynamically or secularly. This material is neutron-rich and its nucleosynthesis provides the astrophysical site for the production of heavy elements ...
L. Bovard +5 more
semanticscholar +1 more source
Impact of newly measured 26Al(n, p)26Mg and 26Al(n, α)23Na reaction rates on the nucleosynthesis of 26Al in stars [PDF]
U. Battino +8 more
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Structure effects of 20N in elemental abundance estimations during explosive nucleosynthesis [PDF]
Most nuclei far from the valley of stability, and typically near the drip lines, exhibit exotic features that have challenged our current understanding of nuclear structure.
Barman Jinti, Chatterjee Rajdeep
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Three-body optical potentials in
M. J. Dinmore +2 more
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The Physics of Core-Collapse Supernovae: Explosion Mechanism and Explosive Nucleosynthesis
Recent developments in multi-dimensional simulations of core-collapse supernovae have considerably improved our understanding of this complex phenomenon.
Luca Boccioli, Lorenzo Roberti
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86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page i-xlii, August 2024.
wiley +2 more sources
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
Evolution and nucleosynthesis in low mass Asymptotic Giant Branch stars [PDF]
S. Cristallo
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