The influence of neutrinos on r-process nucleosynthesis in the ejecta of black hole–neutron star mergers
Author(s)
Roberts, Luke F.
Lippuner, Jonas
Duez, Matthew D.
Faber, Joshua A.
Foucart, Francois
Lombardi, James C., Jr. (Jamie)
Ning, Sandra
Ott, Christian D.
Ponce, Marcelo
Date Issued
October 12, 2016
Abstract
During the merger of a black hole and a neutron star, baryonic mass can become unbound from the system. Because the ejected material is extremely neutron-rich, the r-process rapidly synthesizes heavy nuclides as the material expands and cools. In this work, we map general relativistic models of black hole–neutron star mergers into a Newtonian smoothed particle hydrodynamics (SPH) code and follow the evolution of the thermodynamics and morphology of the ejecta until the outflows become homologous. We investigate how the subsequent evolution depends on our mapping procedure and find that the results are robust. Using thermodynamic histories from the SPH particles, we then calculate the expected nucleosynthesis in these outflows while varying the level of neutrino irradiation coming from the post-merger accretion disc. We find that the ejected material robustly produces r-process nucleosynthesis even for unrealistically high neutrino luminosities, due to the rapid velocities of the outflow. None the less, we find that neutrinos can have an impact on the detailed pattern of the r-process nucleosynthesis. Electron neutrinos are captured by neutrons to produce protons while neutron capture is occurring. The produced protons rapidly form low-mass seed nuclei for the r-process. These low-mass seeds are eventually incorporated into the first r-process peak at A ∼ 78. We consider the mechanism of this process in detail and discuss if it can impact galactic chemical evolution of the first peak r-process nuclei.
Journal
Monthly Notices of the Royal Astronomical Society
Department
Physics
Citation
Roberts, L.F., Lippuner, J. Duez, M.D. et al. (2017). The influence of neutrinos on r-process nucleosynthesis in the ejecta of black hole-neutron star mergers. Monthly Notices of the Royal Astronomical Society 464(4): 3907-3919. Doi:10.1093/mnras/stw2622
Publisher
Oxford University Press
Version of Article
Published article
DOI
10.1093/mnras/stw2622
ISSN
0035-8711
1365-2966
Rights
This article is published and view-able. Copyright is retained by publisher. Contact the author or publisher for further use of this material.
File(s)![Thumbnail Image]()
Name
Lombardi_2017_RoyalAstronomical_Neutrinos.pdf
Description
Main Document
Size
3.22 MB
Format
Adobe PDF
Checksum (etag)
eb156233dfd2f7a34091adbca43e951d