Cosmic Ray Production of Beryllium and Boron at High Redshift
| Autor: | Elisabeth Vangioni, E. Rollinde, Keith A. Olive, David Maurin, Susumu Inoue |
|---|---|
| Rok vydání: | 2008 |
| Předmět: |
Physics
Structure formation Star formation Astrophysics::High Energy Astrophysical Phenomena Metallicity Astrophysics (astro-ph) FOS: Physical sciences Astronomy and Astrophysics Cosmic ray Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Galaxy Redshift Galactic halo Space and Planetary Science Intergalactic travel Astrophysics::Galaxy Astrophysics |
| Zdroj: | The Astrophysical Journal. 673:676-685 |
| ISSN: | 1538-4357 0004-637X |
| Popis: | Recently, new observations of Li6 in Pop II stars of the galactic halo have shown a surprisingly high abundance of this isotope, about a thousand times higher than its predicted primordial value. In previous papers, a cosmological model for the cosmic ray-induced production of this isotope in the IGM has been developed to explain the observed abundance at low metallicity. In this paper, given this constraint on the Li6, we calculate the non-thermal evolution with redshift of D, Be, and B in the IGM. In addition to cosmological cosmic ray interactions in the IGM, we include additional processes driven by SN explosions: neutrino spallation and a low energy component in the structures ejected by outflows to the IGM. We take into account CNO CRs impinging on the intergalactic gas. Although subdominant in the galactic disk, this process is shown to produce the bulk of Be and B in the IGM, due to the differential metal enrichment between structures (where CRs originate) and the IGM. We also consider the resulting extragalactic gamma-ray background which we find to be well below existing data. The computation is performed in the framework of hierarchical structure formation considering several star formation histories including Pop III stars. We find that D production is negligible and that a potentially detectable Be and B plateau is produced by these processes at the time of the formation of the Galaxy (z ~ 3). 9 pages, 7 figures |
| Databáze: | OpenAIRE |
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