Measurements of Key Reactions for the Production and Destruction of Elements in Stars

Physics

1. S-Process 100%
2. Asymptotic Giant Branch Stars 73%
3. Massive Star 60%
4. Absorption Cross Sections 52%
5. Isotopic Abundance 39%
6. Stellar Model 39%
7. Nuclear Reaction 34%
8. Supernovae 34%
9. Ion Beam 34%
10. Nuclear Fusion 34%
11. Stellar Temperature 26%
12. Stellar Nucleosynthesis 21%
13. Metallicity 21%
14. High-Mass Stars 17%
15. Shedding 17%
16. Heavy Ion 17%
17. Thermal Neutron 17%
18. Neutron Emission 17%
19. Proton Energy 17%
20. Center of Mass 17%
21. High Resolution 17%
22. Deceleration 17%
23. Electron Paramagnetic Resonance 17%
24. Beamline 17%
25. Accelerator Mass Spectrometry 17%
26. Stable Isotope 17%
27. Solar Abundances 8%
28. Chemical Evolution 8%
29. Liquid Lithium 8%
30. Novae 8%
31. White Dwarf 8%
32. Core-Collapse Supernovae 8%
33. Solar Mass 8%
34. Ejecta 8%
35. Nuclear Astrophysics 8%
36. Physics 8%