ABSTRACT
Masses of neutron-deficient 58Ni projectile fragments have been measured at the HIRFL-CSR facility in Lanzhou, China employing the isochronous mass spectrometry technique. Masses of a series of short-lived Tz = −3/2 nuclides including the 45Cr nucleus have been measured with a relative uncertainty of about 10−6–10−7. The new 45Cr mass turned out to be essential for modeling the astrophysical rp-process. In particular, we find that the formation of the predicted Ca–Sc cycle in X-ray bursts can be excluded.
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