Nuclear physics of stars

454 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Origin of the Chemical Elements (2010, background): “An introduction to astrophysical S-factors and reaction rates can be found in many textbooks on nuclear astrophysics, e.g. Arnett 1996, Rolfs and Rodney 1988, Iliadis 2007, Boyd 2008.”
A simple approach to the supernova progenitor–explosion connection (2016, unknown): “, Travaglio et al. 2004; Ting et al. 2012; Hansen et al. 2012, 2014), which is thought to be related to the existence of corecollapse supernova sub-populations. More indirect constraints on the fate of massive stars come from, for example, the comparison of the observed star formation and supernova ”
Precision big bang nucleosynthesis with improved Helium-4 predictions (2018, methodology): “We summarize here a few results, to be used in this review, and refer to (Angulo et al., 1999; Clayton, 1983; Iliadis, 2007; Longland et al., 2010) for a detailed treatment.”
STARLIB: A NEXT-GENERATION REACTION-RATE LIBRARY FOR NUCLEAR ASTROPHYSICS (2011, methodology): “The reaction rate is directly proportional to the lognormally distributed strength (see Longland et al. 2010b; Iliadis 2007) and will thus also follow a lognormal distribution.”