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We show that a self-consistent and coupled treatment of the weak decoupling, big bang nucleosynthesis, and photon decoupling epochs can be used to provide new insights and constraints on neutrino sector physics from high-precision measurements of light element abundances and cosmic microwave background observables.
1917
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C. J. Smith, G. M. Fuller, C. T. Kishimoto, and K. N. Abazajian, Light element signatures of sterile neutrinos and cosmological lepton numbers
2006
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