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Scientific paper
Jul 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..576..358b&link_type=abstract
The CAARI 2000: Sixteenth international conference on the application of accelerators in research and industry. AIP Conference
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1
Radiative Capture, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments
Scientific paper
The trajectory of the high-temperature rp-process passes through nuclei close to the proton drip line. Some of these can decay by β-delayed proton emission, which may shift the final mass distribution produced by this form of stellar burning from that of its progenitors. This will also apply to other processes that can synthesize very proton-rich nuclides, including the γ-process and the repetitive rp-process, or (rp)2-process. The very proton-rich nuclides above mass 74 u that cannot be synthesized by either the r- or s-processes can serve as excellent tests of the theoretical models of the rp-, (rp)2-, and γ-processes, especially in the mass region 70 to 100 u, where these processes may operate concurrently. .
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