
Abstract Nuclear fusion reactions generate the energies by which stars stabilize during their long lives in hydrostatic equilibrium. In late-stage stellar evolution and during core collapse of massive stars nuclear reactions mediated by the weak force are essential. Finally, a large network of nuclear reactions is operational during explosive nucleosynthesis in the aftermath of a supernova explosion.
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 1 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
