New findings demonstrate reduced uncertainty in baryon density in cosmology, highlighting the need for better reaction rates.
We report on a high-precision measurement of the D($γ$, n)p photodisintegration reaction at the newly commissioned Shanghai Laser Electron Gamma Source (SLEGS), employing a quasi-monochromatic $γ$-ray beam from Laser Compton Scattering. The cross sections were determined over E_γ=2.327-7.089 MeV, achieving up to a factor of 2.2 improvement in precision near the neutron separation threshold. Combined with previous data in a global Markov chain Monte Carlo (MCMC) analysis using dibaryon effective field theory, we obtained the unprecedentedly precise p(n, $γ$)D cross sections and thermonuclear rate, with a precision up to 3.8 times higher than previous evaluations. Implemented in a standard Big-Bang Nucleosynthesis (BBN) framework, this new rate decreases uncertainty of the key cosmological parameter of baryon density Ωb h² by up to ≈16% relative to the LUNA result. A residual ≈1.2$σ$ tension between Ωb h² constrained from primordial D/H observations and CMB measurements persists, highlighting the need for improved $dd$ reaction rates and offering potential hints of new physics beyond the standard model of cosmology.
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Chen et al. (2025) studied this question.
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