The rp-process near A=80

Details The rp-process near A=80 The rp-process near A=80

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..dnp2wb008r&link_type=abstract

American Physical Society, 2002 Fall Meeting of the Division of Nuclear , abstract #2WB.008

Astronomy and Astrophysics

Astrophysics

Scientific paper

The astrophysical rp-process is thought to be responsible for the
production of proton rich nuclides up to A ˜100. The role of the N
˜Z nuclei near A=80 in the nucleosynthetic process will be
discussed. Emphasis will be placed on the ^80Zr beta decay half-life and
isomers in ^80Y.

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