STARLIB: A NEXT-GENERATION REACTION-RATE LIBRARY FOR NUCLEAR ASTROPHYSICS
By A. Sallaska, C. Iliadis, A. E. Champange, S. Goriely, S. Starrfield, Francis Timmes. 2011
165 citations recorded by the source corpus.
STARLIB is a next-generation, all-purpose nuclear reaction-rate library. For the first time, this library provides the rate probability density at all temperature grid points for convenient implementation in models of stellar phenomena. The recommended rate and its associated uncertainties are also included. Currently, uncertainties are absent from all other rate libraries, and, although estimates have been attempted in previous evaluations and compilations, these are generally not based on rigorous statistical definitions. A common standard for deriving uncertainties is clearly warranted. STARLIB represents a first step in addressing this deficiency by providing a tabular, up-to-date database that supplies not only the rate and its uncertainty but also its distribution. Because a majority of rates are lognormally distributed, this allows the construction of rate probability densities from the columns of STARLIB. This structure is based on a recently suggested Monte Carlo method to calculate reaction rates, where uncertainties are rigorously defined. In STARLIB, experimental rates are supplemented with: (1) theoretical TALYS rates for reactions for which no experimental input is available, and (2) laboratory and theoretical weak rates. STARLIB includes all types of reactions of astrophysical interest to Z = 83, such as (p, γ), (p, α), (α, n), and corresponding reverse rates. Strong rates account for thermal target excitations. Here, we summarize our Monte Carlo formalism, introduce the library, compare methods of correcting rates for stellar environments, and discuss how to implement our library in Monte Carlo nucleosynthesis studies. We also present a method for accessing STARLIB on the Internet and outline updated Monte Carlo-based rates.
Subfields: Aerospace Engineering, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/47c90f12cb2c481ba62815e6a51f8a00ff5e40a7
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In Aerospace Engineering
In Nuclear and High Energy Physics
Citations in the corpus
- Modules for Experiments in Stellar Astrophysics (MESA): Time-dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure (2022, background): “Examples include Astropy (Astropy Collaboration et al. 2018, 2022), Athena++ (Stone et al. 2020; Jiang 2021), Castro (Almgren et al. 2020), Dedalus (Burns et al. 2020), emcee (Foreman-Mackey et al. 2013), Flash-X (Dubey et al. 2022), GYRE (Townsend 4 & Teitler 2013; Townsend et al. 2018), MAESTROeX ”