A weighted Riemann-Liouville fractional derivative is introduced; near the classical limit, the fractional Einstein equations with the BTZ metric reproduce a charged BTZ solution with an anisotropic cosmological constant.
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Fractional Einstein field equations in $2+1$ dimensional spacetime
A weighted Riemann-Liouville fractional derivative is introduced; near the classical limit, the fractional Einstein equations with the BTZ metric reproduce a charged BTZ solution with an anisotropic cosmological constant.