Recently, the electron screening effect in metallic environments has been experimentally investigated by many groups in low-energy nuclear reactions. The similar effect is expected in radioactive decays where the decay constant should be dependent on the valence electron density of the host material. Since metals represents a very good model for dense astrophysical plasmas, comparison of both effects can deliver new information about mechanism of the enhanced electron screening and consequences for nuclear processes taking place in stellar interior. Here, we present a new experimental investigation of screening effect in the d + d nuclear reactions under UHV conditions. Based on those experimental results a host material dependence of the alpha decay probability has been predicted.
10th Symposium on Nuclei in the Cosmos