scholarly journals Nuclear Theory for Nucleosynthesis: Contribution to the 2014 DNP White Paper on Nuclear Physics in Astrophysics

2014 ◽  
Author(s):  
J. E. Escher
Keyword(s):  
Nuclear Physics ◽  
White Paper ◽  
Nuclear Theory

scholarly journals White paper on nuclear astrophysics and low-energy nuclear physics, Part 2: Low-energy nuclear physics

2017 ◽  
Vol 94 ◽  
pp. 68-124 ◽  
Author(s):  
Joe Carlson ◽  
Michael P. Carpenter ◽  
Richard Casten ◽  
Charlotte Elster ◽  
Paul Fallon ◽  
...  
Keyword(s):  
Nuclear Physics ◽  
Nuclear Astrophysics ◽  
White Paper ◽  
Low Energy ◽  
Low Energy Nuclear Physics

scholarly journals White paper on nuclear astrophysics and low energy nuclear physics Part 1: Nuclear astrophysics

2017 ◽  
Vol 94 ◽  
pp. 1-67 ◽  
Author(s):  
Almudena Arcones ◽  
Dan W. Bardayan ◽  
Timothy C. Beers ◽  
Lee A. Bernstein ◽  
Jeffrey C. Blackmon ◽  
...  
Keyword(s):  
Nuclear Physics ◽  
Nuclear Astrophysics ◽  
White Paper ◽  
Low Energy ◽  
Low Energy Nuclear Physics

scholarly journals Quantum Computing for Theoretical Nuclear Physics, A White Paper prepared for the U.S. Department of Energy, Office of Science, Office of Nuclear Physics

2018 ◽  
Author(s):  
Joseph Carlson ◽  
David J. Dean ◽  
Morten Hjorth-Jensen ◽  
David Kaplan ◽  
John Preskill ◽  
...  
Keyword(s):  
Quantum Computing ◽  
Nuclear Physics ◽  
White Paper ◽  
Department Of Energy ◽  
The U.S

Nuclear Processes Related to the Ap Stars and the Heaviest Chemical Elements

1976 ◽  
Vol 32 ◽  
pp. 169-182
Author(s):  
B. Kuchowicz
Keyword(s):  
Nuclear Physics ◽  
Nuclear Reactions ◽  
Chemical Elements ◽  
Fission Products ◽  
Abundance Pattern ◽  
Isotopic Shifts ◽  
Processed Material ◽  
R Process ◽  
Ap Stars ◽  
Nuclear Processes

SummaryIsotopic shifts in the lines of the heavy elements in Ap stars, and the characteristic abundance pattern of these elements point to the fact that we are observing mainly the products of rapid neutron capture. The peculiar A stars may be treated as the show windows for the products of a recent r-process in their neighbourhood. This process can be located either in Supernovae exploding in a binary system in which the present Ap stars were secondaries, or in Supernovae exploding in young clusters. Secondary processes, e.g. spontaneous fission or nuclear reactions with highly abundant fission products, may occur further with the r-processed material in the surface of the Ap stars. The role of these stars to the theory of nucleosynthesis and to nuclear physics is emphasized.

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