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A new mass table calculated by the relativistic mean field approach with thestate-dependent BCS method for the pairing correlation is applied for the firsttime to study r-process nucleosynthesis. The solar r-process abundance is wellreproduced within a waiting-point approximation approach. Using an exponentialfitting procedure to find the required astrophysical conditions, the influenceof mass uncertainty is investigated. R-process calculations using the FRDM,ETFSI-Q and HFB-13 mass tables have been used for that purpose. It is foundthat the nuclear physical uncertainty can significantly influence the deducedastrophysical conditions for the r-process site. In addition, the influence ofthe shell closure and shape transition have been examined in detail in ther-process simulations.

Application of the RMF mass model to the r-process and the influence of mass uncertainties