1998/10/15 by T. Rauscher, Rauscher, T.
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Geophysics and Gravity Measurements #Magnetic confinement fusion research #Nuclear Theory (nucl-th) #Solar and Space Plasma Dynamics #astro-ph #nucl-th
paper · pdf · doi:10.48550/arxiv.nucl-th/9810050
7 pages, nicV.sty included, invited talk at "Nuclei in the Cosmos V" 1998, to appear in the conference proceedings, ed. N. Prantzos (Editions Frontieres)
arxiv created 1998/10/15 · openalex publication_date 1998/10/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Recent improvements and remaining problems in the prediction of thermonuclear rates are reviewed. The main emphasis is on statistical model calculations, but the challenge to include direct reactions close to the driplines is also briefly addressed. Further theoretical as well as experimental investigations are motivated.