Cosmological solutions to the Lithium problem: Big-bang nucleosynthesis with photon cooling, \(X\)-particle decay and a primordial magnetic field

Abstract

The \(^7\)Li abundance calculated in BBN with the baryon-to-photon ratio fixed from fits to the CMB power spectrum is inconsistent with the observed lithium abundances on the surface of metal-poor halo stars. Previous cosmological solutions proposed to resolve this \(^7\)Li problem include photon cooling (possibly via the Bose-Einstein condensation of a scalar particle) or the decay of a long-lived \(X-\)particle (possibly the next-to-lightest supersymmetric particle). In this paper we reanalyze these solutions, both separately and in concert. We also introduce the possibility of a primordial magnetic field (PMF) into these models. We constrain the \(X-\)particles and the PMF parameters by the observed light element abundances using a likelihood analysis to show that the inclusion of all three possibilities leads to an optimum solution to the lithium problem. We deduce allowed ranges for the \(X-\)particle parameters and energy density in the PMF that can solve \(^7\)Li problem.