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Exact solutions for static spherically symmetric spacetime with a perfect fluid in Rastall theory
In general relativity, exact Liouvillian solutions for a static and spherically symmetric spacetime with a perfect fluid and the equation of state $p(r)=wρ(r)$ are known only for $w=0,-\frac{1}{6}, -\frac{1}{5}, -\frac{1}{3}$, and $-1$. We extend this setup to Rastall theory, presenting the relation
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