Variation of the fine structure constant in the light of recent helium abundance measurement

Abstract

We point out that the recent result of primordial helium-4 (${}^4$He) abundance measurement by EMPRESS, which has reported a smaller ${}^4$He abundance than other measurements, can be well fitted by assuming a time-variation of the fine structure constant $\alpha$ which is slightly smaller than the present value during big bang nucleosynthesis (BBN). We find that the EMPRESS result in combination with deuterium abundance measurement indicates $-2.6\%<\Delta \alpha /\alpha <-1.4\%$ (68\% C.L.) where $\Delta \alpha$ is the difference between the values of $\alpha$ at the BBN and present epochs, while $-1.2\%<\Delta \alpha /\alpha <0.4\%$ (68\% C.L.) is obtained from other previous ${}^4$He abundance data. We also investigate its effects in the framework where the effective number of neutrino species and the lepton asymmetry, which are other typical interpretations of the EMPRESS result, are allowed to vary. Once a smaller $\alpha$ is adopted, the EMPRESS result can be explained without assuming any non-standard values for the effective number of neutrino species and lepton asymmetry.

arXiv comment16 pages, 5 figures

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