Production of Mo and Ru Isotopes in Neutrino-driven Winds: Implications for Solar Abundances and Presolar Grains

Bliss, J.; Arcones, A.; Qian, Y. -Z.

doi:10.3847/1538-4357/aade8d

Title: Production of Mo and Ru Isotopes in Neutrino-driven Winds: Implications for Solar Abundances and Presolar Grains

Journal Article · 16 October 2018 · The Astrophysical Journal (Online)

DOI: https://doi.org/10.3847/1538-4357/aade8d · OSTI ID:1610092

Bliss, J. ^[1]; Arcones, A. ^[2];

^[3]

Technische Univ. Darmstadt (Germany). Inst. fur Kernphysik; DOE/OSTI
Technische Univ. Darmstadt (Germany). Inst. fur Kernphysik; GSI-Darmstadt (Germany)
Univ. of Minnesota, Minneapolis, MN (United States); Tsung-Dao Lee Inst., Shanghai (China)

The origin of the so-called p-isotopes $${}^{\mathrm{92,94}}\mathrm{Mo}$$ and $${}^{\mathrm{96,98}}\mathrm{Ru}$$ in the solar system remains a mystery, as several astrophysical scenarios fail to account for them. In addition, data on presolar silicon carbide grains of type X (SiC X) exhibit peculiar Mo patterns, especially for $${}^{\mathrm{95,97}}\mathrm{Mo}$$. We examine the production of Mo and Ru isotopes in neutrino-driven winds associated with core-collapse supernovae (CCSNe) over a wide range of conditions. We find that proton-rich winds can make dominant contributions to the solar abundance of $${}^{98}\mathrm{Ru}$$ and significant contributions to those of 96Ru, 92Mo, and 94Mo. In contrast, neutron-rich winds make negligible contributions to the solar abundances of 92,94Mo and cannot produce 96,98Ru, whereas the early ejecta of CCSNe can make dominant contributions to the solar abundance of 92Mo. Furthermore, we show that some neutron-rich winds can account for the peculiar Mo patterns in SiC X grains. Our results can be generalized if conditions similar to those studied here are also obtained for other types of ejecta in either CCSNe or neutron star mergers.

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Research Organization:: Univ. of Minnesota, Minneapolis, MN (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: FG02-87ER40328

OSTI ID:: 1610092

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 866; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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