[Submitted on 1 Mar 2016] (cross-list from astro-ph.HE)
The unreasonable weakness of r-process cosmic rays in the neutron-star-merger nucleosynthesis scenario
Koutarou Kyutoku · Kunihito Ioka
We reach the robust conclusion that, by combining the observed cosmic rays of r-process elements with the fact that the velocity of the neutron-star-merger ejecta is much higher than that of the supernova ejecta, either (1) the reverse shock in the neutron-star-merger ejecta is a very inefficient accelerator that converts less than 0.003% of the ejecta kinetic energy to the cosmic-ray energy or (2) the neutron star merger is not the origin of the Galactic r-process elements. We also find that the acceleration efficiency should be less than 0.1% for the reverse shock of the supernova ejecta with the observed cosmic rays lighter than the iron.
- Comments:
- 5 pages, 1 figure
- Subjects:
- High Energy Astrophysical Phenomena (astro-ph.HE); Nuclear Theory (nucl-th)
- arXiv:
- 1603.00467 [pdf]