Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-07-19
Phys.Rev.D72:123505,2005
Astronomy and Astrophysics
Astrophysics
6 pages, 7 figures
Scientific paper
10.1103/PhysRevD.72.123505
We present a new astrophysical site of the big bang nucleosynthesis (BBN) that are very peculiar compared with the standard BBN. Some models of the baryogenesis suggest that very high baryon density regions were formed in the early universe. On the other hand, recent observations suggest that heavy elements already exist in high red-shifts and the origin of these elements become a big puzzle. Motivated by these, we investigate BBN in very high baryon density regions. BBN proceeds in proton-rich environment, which is known to be like the p-process. However, by taking very heavy nuclei into account, we find that BBN proceeds through both the p-process and the r-process simultaneously. P-nuclei such as 92Mo, 94Mo, 96Ru, 98Ru whose origin is not well known are also synthesized.
Fujimoto Shouji
Hashimoto Makoto
Matsuura Shuji
Nishimura Satoru
Sato Kachishige
No associations
LandOfFree
Heavy Element Production in Inhomogeneous Big Bang Nucleosynthesis 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 Heavy Element Production in Inhomogeneous Big Bang Nucleosynthesis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Heavy Element Production in Inhomogeneous Big Bang Nucleosynthesis will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-287055