Cosmic-Ray Lithium Production at the Nova Eruption Followed by a Type Ia Supernova
High Energy Astrophysical Phenomena
2018-01-31 v2
Abstract
Recent measurements of cosmic-ray light nuclei by AMS-02 have shown that there is an unexpected component of cosmic-ray (CR) lithium whose spectral index is harder than that expected from the secondary production scenario. We propose the nearby Type Ia supernova following a nova eruption as the origin of lithium nuclei in the CRs. By fitting the data of CR protons, helium, and lithium fluxes provided by AMS-02 with our theoretical model we show that this scenario is consistent with the observations. The observational tests that can check our hypothesis are briefly discussed.
Keywords
Cite
@article{arxiv.1707.00212,
title = {Cosmic-Ray Lithium Production at the Nova Eruption Followed by a Type Ia Supernova},
author = {Norita Kawanaka and Shohei Yanagita},
journal= {arXiv preprint arXiv:1707.00212},
year = {2018}
}
Comments
6 pages, 2 figures, accepted for publication in PRL