Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-12-02
Astronomy and Astrophysics
Astrophysics
5 pages, 2 figures, proceedings of Nuclei in the Cosmos 2000, to be published in Nucl. Phys. A; minor correction
Scientific paper
10.1016/S0375-9474(01)00724-2
We present the results of fully dynamical r-process network calculations for the ejecta of neutron star mergers (NSMs). The late stages of the inspiral and the final violent coalescence of a neutron star binary have been calculated in detail using a 3D hydrodynamics code (Newtonian gravity plus backreaction forces emerging from the emission of gravitational waves) and a realistic nuclear equation of state. The found trajectories for the ejecta serve as input for dynamical r-process calculations where all relevant nuclear reactions (including beta-decays depositing nuclear energy in the expanding material) are followed. We find that all the ejected material undergoes r-process. For an initial Ye close to 0.1 the abundance distributions reproduce very accurately the solar r-process pattern for nuclei with A above 130. For lighter nuclei strongly underabundant (as compared to solar) distributions are encountered. We show that this behaviour is consistent with the latest observations of very old, metal-poor stars, despite simplistic arguments that have recently been raised against the possibility of NSM as possible sources of Galactic r-process material.
Freiburghaus Ch.
Rosswog Stefan
Thielemann Friederich-Karl
No associations
LandOfFree
Nucleosynthesis Calculations for the Ejecta of Neutron Star Coalescences 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 Nucleosynthesis Calculations for the Ejecta of Neutron Star Coalescences, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nucleosynthesis Calculations for the Ejecta of Neutron Star Coalescences will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-463935