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PreprintarXiv licencearXiv

Interferometric trilemma for ultraviolet-softened gravity

Abstract

Ultraviolet-softened extensions of general relativity can weaken gravity at short distances, whereas a positive Källén--Lehmann spectral density forbids gravity from falling below Newtonian strength. Which property of the mediator must such a weakening sacrifice? For Lorentz-invariant Gaussian mediators coupled linearly to the conserved stress tensor, we formulate three independent interferometric conditions that jointly imply this bound: visibility is never amplified, decoherence is fixed by the energy radiated by the difference source, and no interferometer responds to a later one. At tree level, the three ghost prescriptions of quadratic gravity each violate exactly one: negative-norm ghosts amplify coherence, negative-energy ghosts decohere without positive energy transfer from the difference source, and a time-symmetric fakeon response produces advanced fringe shifts. Any universal short-distance weakening of gravity therefore certifies that its mediator violates one of these conditions, and the observables proposed to certify quantum gravity become consistency tests of its ultraviolet completion.

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BibTeX
@misc{matsui2026interferometric,
  title = {{Interferometric trilemma for ultraviolet-softened gravity}},
  author = {Hiroki Matsui},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.25994},
  eprint = {2610.25994},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.25994},
}
RIS
TY  - UNPB
TI  - Interferometric trilemma for ultraviolet-softened gravity
AU  - Hiroki Matsui
PY  - 2026
DA  - 2026/10/19
PB  - arXiv
DO  - 10.48550/arxiv.2610.25994
UR  - https://arxiv.org/abs/2610.25994
AB  - Ultraviolet-softened extensions of general relativity can weaken gravity at short distances, whereas a positive Källén--Lehmann spectral density forbids gravity from falling below Newtonian strength. Which property of the mediator must such a weakening sacrifice? For Lorentz-invariant Gaussian mediators coupled linearly to the conserved stress tensor, we formulate three independent interferometric conditions that jointly imply this bound: visibility is never amplified, decoherence is fixed by the energy radiated by the difference source, and no interferometer responds to a later one. At tree level, the three ghost prescriptions of quadratic gravity each violate exactly one: negative-norm ghosts amplify coherence, negative-energy ghosts decohere without positive energy transfer from the difference source, and a time-symmetric fakeon response produces advanced fringe shifts. Any universal short-distance weakening of gravity therefore certifies that its mediator violates one of these conditions, and the observables proposed to certify quantum gravity become consistency tests of its ultraviolet completion.
ER  -