作者: M A Rodríguez-Meza , A X González-Morales , R F Gabbasov , Jorge L Cervantes-Cota
DOI: 10.1088/1742-6596/91/1/012012
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摘要: We present ?CDM N-body cosmological simulations in the framework of a static general scalar-tensor theory gravity. Due to influence non-minimally coupled scalar field, gravitational potential is modified by Yukawa type term, yielding new structure formation dynamics. some preliminary results and, particular, we compute density and velocity profiles most massive group.