Introduction to R Process Abundances
Discover more insights into R Process Abundances
Keywords frequently search together with R Process Abundances
Narrow sentence examples with built-in keyword filters
It is unclear if neutron star mergers can explain the observed r-process abundances of metal-poor stars.
Calculations including a predicted Fe i line blueward of the Pb ii line, and assuming the lead abundance scales with r-process abundances, match all four profiles extremely well.
The impact of nuclear mass uncertainties on the r-process abundances has been systematically studied with the classical r-process model by varying the mass of every individual nucleus in the range of ±0.
We find ubiquitous flavor oscillations that result in a significantly more neutron-rich outflow, providing lanthanide and 3rd-peak r-process abundances similar to solar abundances.