rp Process and Masses of N≈Z≈34 Nuclides

Details rp Process and Masses of N≈Z≈34 Nuclides rp Process and Masses of N≈Z≈34 Nuclides

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009phrvl.102m2501s&link_type=abstract

Physical Review Letters, vol. 102, Issue 13, id. 132501

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17

Binding Energies And Masses, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, 59<=A<=89

Scientific paper

High-precision Penning-trap mass measurements of the N≈Z≈34 nuclides Se68, Se70, Br70m, and Br71 were performed, reaching experimental uncertainties of 0.5-15 keV. The new and improved mass data together with theoretical Coulomb displacement energies were used as input for rp process network calculations. An increase in the effective lifetime of the waiting point nucleus Se68 was found, and more precise information was obtained on the luminosity during a type I x-ray burst along with the final elemental abundances after the burst.

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