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Bekenstein bound from the Pauli principle: a brief introduction
2021
Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020)
unpublished
Preserved Fulltext
Here we briefly resume the idea, originally introduced in Phys. Rev. D 102, 106002 (2020), that the Bekenstein bound on entropy is a consequence of the fermionic nature of fundamental degrees of freedom, which arrange themselves to form matter and spacetime. The main point is discussed by means of a toy-model of black hole evaporation, which describes the dynamics of such degrees of freedom, called ons. An intrinsic notion of interior/exterior of the black hole during the evaporation process is
doi:10.22323/1.390.0681
fatcat:ddrqkpig7rgbtfglmxqo7wqnwe