The Mass of <sup>128</sup>Sb and its Role as an Astromer
ORAL
Abstract
Recently it was shown that nuclear isomers play a significant role in nucleosynthetic pathways, in particular the rapid neutron-capture process. These astrophysically metastable isomers, otherwise known as ``astromers", influence the population of unstable nuclei and hence can impact the heating and light output. We have recently performed the first direct mass measurements of one such astromer 128Sb and of the ground state 128Sb using the Canadian Penning Trap mass spectrometer at Argonne National Laboratory. We find an excitation energy of this astromer that differs significantly from the previous upper limit, changing its thermalization temperature. Our measurement provides the first step in understanding the role of 128Sb in the rapid neutron-capture process, and we will discuss some of the implications.
*This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344, and supported from the Natural Sciences and Engineering Research Council of Canada: Grant SAPPJ-2018-00028, as well as by the U.S. Department of Energy, Office of Nuclear Physics, under Contract No. DE-AC02-06CH11357. L. V. was supported by the National Science Foundation Graduate Research Fellowship under Grant No. DGE-1746045. M.B. acknowledges support from the NSF under Grant No. PHY-2011890. This research used resources of ANL's ATLAS facility, which is a DOE Office of Science User Facility.
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Presenters
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Daniel E Hoff
- Lawrence Livermore National Laboratory
- University of Massachusetts Lowell