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Surface configuration in R+μ4/R gravity

    https://doi.org/10.1142/S0217732315501710Cited by:1 (Source: Crossref)

    We investigate the conditions on the additional constant μ in the so-called R+μ4/R theory of gravity, due to existence of different kinds of space-like surfaces in both weak field and strong field limits, and their possible correspondence to black hole event horizons. Adopting a Schwarzschild limit, we probe the behavior of μ in different contexts of radial and radial–rotational congruence of null geodesics. We show that these cases serve as correspondents to black hole horizons in some peculiar cases of study.

    PACS: 04.20.Dw, 04.20.Fy, 04.20.Jb