Skip to content
DraconiticResearch
Search Sources API
201,683 studies31 sourcesUpdated 52 min ago
PreprintCC BY 4.0arXiv

The trans-Planckian problem and gravitational interactions

Abstract

The strong gravitational interaction of counter-propagating quantum field modes is of foundational importance to the trans-Planckian problem of black hole horizons. This article, in memory of Renaud Parentani, is primarily an exposition of Renaud's attempt, using perturbation theory, a large N approximation, and spherical reduction, to capture a mechanism by which those interactions might quench the trans-Planckian near-horizon quantum field correlations. Before giving a detailed account of Renaud's calculation, the trans-Planckian problem is briefly introduced, and the paper concludes with a discussion of related issues and questions.

Versions

Related

  1. Classical and Stochastic Trans-Planckian Censorship
    Omer Guleryuz
    arXivPreprintarXiv licenceFull textGravitation & general relativityHigh-energy & particle physicsarXiv
  2. Say Hello, Wave Goodbye: Gravitational Waves from Hyperbolic PBH-SMBH Interactions
    Laura Burn, Nelson Christensen, Richard Easther
    HALPreprintLicence not statedGeneral astronomyGravitation & general relativityHAL
  3. Gravitational wave interactions with matter: beyond quadrupolar perturbations
    Ulrich K. Beckering Vinckers, Nigel T. Bishop
    arXivPreprintarXiv licenceFull textGravitation & general relativityarXiv
  4. Gravitational quantum friction and the information-loss problem
    Francesco Del Porro, Francesco Di Filippo
    arXivPreprintarXiv licenceFull textGravitation & general relativityHigh-energy & particle physicsarXiv
  5. Gravitational Interactions in Nuclear Clocks
    Konstantin Beyer, Niklas E. Önne, Shimon Kolkowitz +4
    arXivPreprintarXiv licenceFull textAtomic, molecular & optical physicsGravitation & general relativityarXiv
BibTeX
@misc{jacobson2026transplanckian,
  title = {{The trans-Planckian problem and gravitational interactions}},
  author = {Ted Jacobson},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.03071},
  eprint = {2609.03071},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.03071},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - The trans-Planckian problem and gravitational interactions
AU  - Ted Jacobson
PY  - 2026
DA  - 2026/09/02
PB  - arXiv
DO  - 10.48550/arxiv.2609.03071
UR  - https://arxiv.org/abs/2609.03071
AB  - The strong gravitational interaction of counter-propagating quantum field modes is of foundational importance to the trans-Planckian problem of black hole horizons. This article, in memory of Renaud Parentani, is primarily an exposition of Renaud's attempt, using perturbation theory, a large N approximation, and spherical reduction, to capture a mechanism by which those interactions might quench the trans-Planckian near-horizon quantum field correlations. Before giving a detailed account of Renaud's calculation, the trans-Planckian problem is briefly introduced, and the paper concludes with a discussion of related issues and questions.
ER  -