Decay of the r-process nuclides 137,138,139Sb, and the A=130 solar r-process abundance peak

Details Decay of the r-process nuclides 137,138,139Sb, and the A=130 solar r-process abundance peak Decay of the r-process nuclides 137,138,139Sb, and the A=130 solar r-process abundance peak

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011phrvc..84f1307a&link_type=abstract

Physical Review C, vol. 84, Issue 6, id. 061307

Physics

1

Beta Decay, Double Beta Decay, Electron And Muon Capture, Lifetimes, R-Process, 90<=A<=149

Scientific paper

Half-life (T1/2) and β-delayed neutron branching (Pn) values of 492(25) ms and 49(8)%, 350(15) ms and 72(8)%, and 93(13) ms and 90(10)% for the r-process nuclei 137,138,139Sb, respectively, have been measured at the CERN On-Line Isotope Mass Separator (ISOLDE) facility by counting β-delayed neutrons. More precise T1/2 and Pn values of 300(15) ms and 27(4)%, and 273(7) ms and 50(8)% for 136,137Sn, respectively, have also been measured. The sources were prepared by using the selective ionization of Sb or Sn with the Resonance Ionization Laser Ion Source and the high-resolution mass separator. The new data for Sb isotopes are compared with calculated T1/2 and Pn values for both spherical and nonspherical shapes. The data have been incorporated into parametrized nucleosynthesis calculations of the r process in high-entropy winds of core-collapse supernovae in order to study the properties of the A = 130 solar-system r-process abundance peak.

Affiliated with

Also associated with

No associations

Rating

Decay of the r-process nuclides 137,138,139Sb, and the A=130 solar r-process abundance peak does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Decay of the r-process nuclides 137,138,139Sb, and the A=130 solar r-process abundance peak, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Decay of the r-process nuclides 137,138,139Sb, and the A=130 solar r-process abundance peak will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1438765