A Simultaneous Solution to the ^6Li and ^7Li Big Bang Nucleosynthesis Problems from a Long-Lived Negatively-Charged Leptonic Particle
| dc.creator | Kusakabe, Motohiko | |
| dc.creator | Kajino, Toshitaka | |
| dc.creator | Boyd, Richard N. | |
| dc.creator | Yoshida, Takashi | |
| dc.creator | Mathews, Grant J. | |
| dc.date | 2007-11-24 | |
| dc.date.accessioned | 2026-07-07T12:13:55Z | |
| dc.date.available | 2026-07-07T12:13:55Z | |
| dc.description | The $^6$Li abundance observed in metal poor halo stars exhibits a plateau similar to that for $^7$Li suggesting a primordial origin. However, the observed abundance of $^6$Li is a factor of $10^3$ larger and that of $^7$Li is a factor of 3 lower than the abundances predicted in the standard big bang when the baryon-to-photon ratio is fixed by WMAP. Here we show that both of these abundance anomalies can be explained by the existence of a long-lived massive, negatively-charged leptonic particle during nucleosynthesis. Such particles would capture onto the synthesized nuclei thereby reducing the reaction Coulomb barriers and opening new transfer reaction possibilities, and catalyzing a second round of big bang nucleosynthesis. This novel solution to both of the Li problems can be achieved with or without the additional effects of stellar destruction. | |
| dc.description | 6 pages, 2 figures, to be published in Physical Review D | |
| dc.identifier | https://arxiv.org/abs/0711.3854 | |
| dc.identifier | http://arxiv.org/abs/0711.3854 | |
| dc.identifier | Phys.Rev.D76:121302,2007 | |
| dc.identifier | doi:10.1103/PhysRevD.76.121302 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/211014 | |
| dc.subject | Astrophysics | |
| dc.title | A Simultaneous Solution to the ^6Li and ^7Li Big Bang Nucleosynthesis Problems from a Long-Lived Negatively-Charged Leptonic Particle | |
| dc.type | text |