Bounds on neutrino-scalar nonstandard interactions from big bang nucleosynthesis
arXiv:2009.08104 · doi:10.1103/PhysRevD.103.043534
Abstract
Coherent forward scattering processes by neutrino-scalar nonstandard interactions (SNSI) induce an effective neutrino mass. In the Early Universe, a large neutrino effective mass restricts the production of neutrinos. The SNSI effect is modulated by two effective couplings, these account for the coupling between neutrinos and electrons/positrons, , and the neutrino self-interaction, . These parameters are directly related to the effective number of relativistic species and non-zero values imply a smaller than expected . We employ big bang nucleosynthesis to constraint the SNSI effect. We find that MeV and MeV at 68\% CL. For a scalar mass in the range , our neutrino-scalar coupling constraint is more restrictive than any previous result.
arXiv commentFigure added. Improved discussion and computation of the neutrino decoupling due to SNSI. Accepted for publication in PRD
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