Resonant destruction as a possible solution to the cosmological lithium problem

We explore a nuclear physics resolution to the discrepancy between the predicted standard big-bang nucleosynthesis (BBN) abundance of ⁷Li and its observational determination in metal-poor stars. The theoretical ⁷Li abundance is 3--4 times greater than the observational values, assuming the baryon-to-photon ratio, ηwmap, determined by WMAP. The ⁷Li problem could be resolved within the standard BBN picture if additional destruction of $A=7$ isotopes occurs due to new nuclear reaction channels or upward corrections to existing channels. This could be achieved via missed resonant nuclear reactions, which is the possibility we consider here. We find some potential candidate resonances which can solve the lithium problem and specify their required resonant energies and widths. For example, a 1^- or 2^- excited state of ¹⁰C sitting at approximately 15.0 MeV above its ground state with an effective width of order 10 keV could resolve the ⁷Li problem; the existence of this excited state needs experimental verification. Other examples using known states include ⁷Be+t→¹⁰B(18.80 MeV), and ⁷Be+d→⁹B(16.71 MeV). For all of these states, a large channel radius (a>10 fm) is needed to give sufficiently large widths. Experimental determination of these reaction strengths is needed to rule out or confirm these nuclear physics solutions to the lithium problem.