Non-universal BBN bounds on electromagnetically decaying particles
arXiv:1503.04852 · doi:10.1103/PhysRevD.91.103007
Abstract
In Poulin and Serpico [Phys. Rev. Lett. 114, 091101 (2015)] we have recently argued that when the energy of a photon injected in the primordial plasma falls below the pair-production threshold, the universality of the non-thermal photon spectrum from the standard theory of electromagnetic cascades onto a photon background breaks down. We showed that this could reopen or widen the parameter space for an exotic solution to the 'lithium problem'. Here we discuss another application, namely the impact that this has on non-thermal big bang nucleosynthesis constraints from 4He, 3He and 2H, using the parametric example of monochromatic photon injection of different energies. Typically, we find tighter bounds than those existing in the literature, up to more than one order of magnitude. As a consequence of the non-universality of the spectrum, the energy-dependence of the photodissociation cross-sections is important. We also compare the constraints obtained with current level and future reach of cosmic microwave background spectral distortion bounds.
8 pages, 7 figures. v2: minor typographical corrections, extended comments and references
References in corpus (7)
- Primordial Nucleosynthesis: from precision cosmology to fundamental physics
- Big Bang Nucleosynthesis Constraints on Hadronically and Electromagnetically Decaying Relic Neutral Particles
- Big Bang Nucleosynthesis as a Probe of New Physics
- Deuterium Abundance in the Most Metal-Poor Damped Lyman alpha System: Converging on Omega_baryons
- A robust deuterium abundance; Re-measurement of the z=3.256 absorption system towards the quasar PKS1937-1009
- A loophole to the universal photon spectrum in electromagnetic cascades: application to the "cosmological lithium problem"
- Effects of Long-lived 10 MeV Scale Sterile Neutrino on Primordial Elemental Abundances and Effective Neutrino Number