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Abstract
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In this study, we explore the black bounce solution in Rastall gravity and its
potential source field, which can be described as a black hole or wormhole solution depending
on certain parameters. We focus on the Bardeen-Type black bounce and Simpson-Visser
solution and aim to identify an appropriate source field for these solutions. Our findings suggest
that in Rastall gravity, a source for the black bounce solution with non-linear electromagnetic
can be found. However, in the presence of a non-linear electromagnetic source, it is impossible
to identify an appropriate source for the black bounce solution without a scalar field. We
also investigate the energy conditions outside the event horizon for two types of black bounce
solutions: Simpson-Visser and Bardeen. We find that these solutions do not satisfy the null
energy condition, but we also reveal that Rastall gravity has more flexibility for maintaining
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