r-process nucleosynthesis in hot accretion disk flows from black hole-neutron star mergers

R. Surman, G. C. McLaughlin, M. Ruffert, H. -Th. Janka, W. R. Hix

Research output: Contribution to journalArticlepeer-review

Abstract

We consider hot accretion disk outflows from black hole-neutron star mergers in the context of the nucleosynthesis they produce. We begin with a three-dimensional numerical model of a black hole-neutron star merger and calculate the neutrino and antineutrino fluxes emitted from the resulting accretion disk. We then follow the element synthesis in material outflowing the disk along parameterized trajectories. We find that at least a weak r-process is produced, and in some cases a main r-process as well. The neutron-rich conditions required for this production of r-process nuclei stem directly from the interactions of the neutrinos emitted by the disk with the free neutrons and protons in the outflow.

Original languageEnglish
Pages (from-to)L117-L120
Number of pages4
JournalAstrophysical Journal Letters
Volume679
Issue number2
DOIs
Publication statusPublished - Jun 2008

Keywords

  • neutrinos
  • nuclear reactions, nucleosynthesis, abundances
  • stars : neutron

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