Q_β Measurement of the N=Z rp-Process Waiting-Point Nucleus ^68Se and its Astrophysical Implications

Details Q_β Measurement of the N=Z rp-Process Waiting-Point Nucleus ^68Se and its Astrophysical Implications Q_β Measurement of the N=Z rp-Process Waiting-Point Nucleus ^68Se and its Astrophysical Implications

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..dnp.cd006w&link_type=abstract

American Physical Society, Division of Nuclear Physics Fall Meeting, October 30 - November 1, 2003, Tucson, Arizona, MEETING ID:

Physics

Nuclear Physics

Scientific paper

Precise mass measurements of nuclides along the N=Z line are important input parameters for rp-process calculations. Of particular interest is the mass of the ^68_34Se_34 rp-process waiting point nucleus. This mass was determined via the β-endpoint measurement of ^68Se. The ^68Se was produced via the ^12C(^58Ni,2n)^68Se reaction. In addition to the experiment a study of the influence of different masses on the rp-process has been performed. Both, the result and the astrophysical consequences will be presented.

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