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Realistic compact stars in conformal teleparallel gravity
Progress of Theoretical and Experimental Physics
We explore an interior solution of a physically symmetric vierbein with two unknown functions in conformal teleparallel gravity. The field equations can be described in a closed system for a particular form of the metric potentials and an appropriate anisotropic function. As a result, we find a new set of configurations consistent with observed pulsars. In particular, the boundary conditions for the interior spacetime are used for the Schwarzschild spacetime to constrain the conformal fielddoi:10.1093/ptep/ptac121 fatcat:jmi6yngqzffgzelixvsdt7lmmy