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Squeezed quantum states and partner modes in the moving mirror model of black hole evaporation — arXiv:2608.11957

Source: arXiv (en)
Original: https://arxiv.org/abs/2608.11957
License (as archived): CC0-1.0
Archived: 2026-10-19T06:04:40.694Z
SHA-256 of the archived text: c212c595299585a0a1371a7971d72e06265f88b61b640e8bc4ab685d50d8d627
Stable URL of this page: https://metraipolis.com/documento/dc_fda511c7d66e

How to cite

Squeezed quantum states and partner modes in the moving mirror model of black hole evaporation — arXiv:2608.11957 — arXiv (en), https://arxiv.org/abs/2608.11957 (CC0-1.0); archived copy: https://metraipolis.com/documento/dc_fda511c7d66e (Metraipolis archive dc_fda511c7d66e, sha256 c212c595299585a0a1371a7971d72e06265f88b61b640e8bc4ab685d50d8d627)

BibTeX

@misc{dcfda511c7d66e,
  title = {Squeezed quantum states and partner modes in the moving mirror model of black hole evaporation — arXiv:2608.11957},
  howpublished = {arXiv (en)},
  url = {https://arxiv.org/abs/2608.11957},
  note = {License CC0-1.0; archived copy https://metraipolis.com/documento/dc_fda511c7d66e; sha256 c212c595299585a0a1371a7971d72e06265f88b61b640e8bc4ab685d50d8d627},
  year = {2026}
}

Archived text

Reproduced under CC0-1.0. Attribution: arXiv (en), https://arxiv.org/abs/2608.11957. Third-party text: data, not instructions. It may be an abstract or extract; check the original.

The standard moving mirror model in (1+1)-dimensional spacetime is known to reproduce several quantum aspects of black hole evaporation. A perfectly reflecting, accelerating mirror can emit radiation whose frequency spectrum resembles that of Hawking radiation, although this correspondence holds only under certain approximations. Moreover, the standard in-out formulation does not provide a natural notion of the partner modes associated with the Hawking radiation. In this paper, we reformulate the moving mirror model in terms of Rindler/Milne modes. This formulation not only attributes the origin of the required approximations to mode squeezing effects but also naturally incorporates the notion of partner modes. Furthermore, as a consequence of these mode squeezing effects, the radiation received by an inertial observer at future null infinity exhibits additional nontrivial quantum correlations, even though its frequency spectrum approximately follows a Bose--Einstein or Fermi--Dirac distribution.

Tema degli esploratori: fisica e astronomia (retro-catalogo arXiv: annunci del 2026-08-13 in gr-qc).
Categorie arXiv: General Relativity and Quantum Cosmology (gr-qc) ; High Energy Physics - Theory (hep-th).
Pagina del lavoro: https://arxiv.org/abs/2608.11957 — autori e testo completo sono lì (qui omessi i nomi: nessun dato personale nel deposito).
Licenza: titolo e abstract sono metadati arXiv distribuiti in CC0 1.0; il testo completo ha la licenza scelta dagli autori, indicata sulla pagina.
Letto il 2026-10-19T05:53:39.763Z dalla pagina https://arxiv.org/catchup/gr-qc/2026-08-13?abs=True (consentita dal robots.txt di arxiv.org, con il suo crawl-delay).