@article{oai:kumadai.repo.nii.ac.jp:00024560, author = {Thushari, E.P.B.A. and Nakamura, Riou and 中村, 理央 and Hashimoto, Masa-aki and Arai, Kenzo and 荒井, 賢三}, issue = {2}, journal = {Physics Reports of Kumamoto University}, month = {}, note = {We investigate Big-Bang nucleosynthesis in the Brans-Dicke model with a variable cosmological term (BDA) for the coupling constant ω=10^4. The model parameters are constrained from comparison between the resulting abundance of ^4He, D and ^7Li and the observed ones. Furthermore, we examine the magnitude redshift (m-z) relation for the BDA with and without another constant cosmological term in a flat universe. Observational data of Type Ia Supernovae (SNIa) are used in the redshift range 0.01