TY  - JOUR
A1  - Nicolini, Piero
A1  - Singleton, Douglas
T1  - Connecting horizon pixels and interior voxels of a black hole
T2  - Physics Letters B
N2  - 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.
Y1  - 2014
UR  - http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/54707
UR  - https://nbn-resolving.org/urn:nbn:de:hebis:30:3-547075
SN  - 1873-2445
SN  - 0370-2693
N1  - This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/3.0/).
VL  - 738.2014
SP  - 213
EP  - 217
PB  - Elsevier
CY  - Amsterdam
ER  -