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Peer-reviewedCC BY 4.0Journal of High Energy Physics

A QFT information protocol for charged black holes

  1. 1Università degli studi di Napoli Federico II
  2. 2Complesso Universitario di Monte S. Angelo

Abstract

A generalization for the quantum information retrieval protocol recently illustrated by Verlinde and van der Heijden for evaporating black holes is provided to inclusions of type III von Neumann factors. The physical interest of such scenario arises in Quantum Field Theory, where local algebras are type III von Neumann algebras. The formula obtained can be easily interpreted in terms of the statistical dimension of superselection sectors in the case of black holes undergoing charge evaporation, thanks to the index-statistics theorem, leading to a thermodynamic interpretation. A constraint on the values of the index leads to a final remark about the quantization of the charge emitted by the black hole during the evaporation process.

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BibTeX
@article{palumbo2026information,
  title = {{A QFT information protocol for charged black holes}},
  author = {Paolo Palumbo},
  journal = {Journal of High Energy Physics},
  year = {2026},
  month = oct,
  doi = {10.1007/jhep10(2026)259},
  url = {https://link.springer.com/article/10.1007/JHEP10(2026)259},
  note = {CC BY 4.0},
}
RIS
TY  - JOUR
TI  - A QFT information protocol for charged black holes
AU  - Paolo Palumbo
PY  - 2026
DA  - 2026/10/26
JO  - Journal of High Energy Physics
DO  - 10.1007/jhep10(2026)259
UR  - https://link.springer.com/article/10.1007/JHEP10(2026)259
AB  - A generalization for the quantum information retrieval protocol recently illustrated by Verlinde and van der Heijden for evaporating black holes is provided to inclusions of type III von Neumann factors. The physical interest of such scenario arises in Quantum Field Theory, where local algebras are type III von Neumann algebras. The formula obtained can be easily interpreted in terms of the statistical dimension of superselection sectors in the case of black holes undergoing charge evaporation, thanks to the index-statistics theorem, leading to a thermodynamic interpretation. A constraint on the values of the index leads to a final remark about the quantization of the charge emitted by the black hole during the evaporation process.
SN  - 1029-8479
ER  -