Precise measurement of the Ge64 mass and its effect on the rp process

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Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Binding Energies And Masses, 59<=A<=89, Origin, Formation, And Abundances Of The Elements

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The Canadian Penning Trap mass spectrometer has been used to determine the mass excesses of Ge64 and Ga64 as -54344(30) keV and -58832.5(39) keV, respectively. Under typical conditions used for modeling x-ray bursts, Ge64 is confirmed as a waiting-point nuclide and can contribute up to 35.5 s to the timescale of the rp process at a peak x-ray burst temperature of 1.5 GK.

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