In this paper we discuss to what extent one can infer details of the interior structure of a black hole based on its horizon. Recalling that black hole thermal properties are connected to the non-classical nature of gravity, we circumvent the restrictions of the no-hair theorem by postulating that the black hole interior is singularity free due to violations of the usual energy conditions. Further these conditions allow one to establish a one-to-one, holographic projection between Planckian areal “bits” on the horizon and “voxels”, representing the gravitational degrees of freedom in the black hole interior. We illustrate the repercussions of this idea by discussing an example of the black hole interior consisting of a de Sitter core postulated to arise from the local graviton quantum vacuum energy. It is shown that the black hole entropy can emerge as the statistical entropy of a gas of voxels.

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nohair theorem voxels black hole thermal properties statistical entropy interior structure gravitational degrees of freedom usual energy onetoone holographic projection planckian areal bits de sitter core nonclassical nature of gravity horizon local graviton quantum vacuum

Piero Nicolini,Douglas Singleton,.Connecting horizon pixels and interior voxels of a black hole. 738 (C),.

Piero Nicolini,Douglas Singleton,"Connecting horizon pixels and interior voxels of a black hole" 738

Piero Nicolini,Douglas Singleton,"Connecting horizon pixels and interior voxels of a black hole"