Squeezed Gravitons and One-Loop Self-Energy under Light-Cone Smearing

@misc{matsui2026squeezed,
  title = {{Squeezed Gravitons and One-Loop Self-Energy under Light-Cone Smearing}},
  author = {Hiroki Matsui},
  howpublished = {arXiv},
  year = {2026},
  month = aug,
  doi = {10.48550/arxiv.2605.05916},
  eprint = {2605.05916},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2605.05916},
}

TY  - UNPB
TI  - Squeezed Gravitons and One-Loop Self-Energy under Light-Cone Smearing
AU  - Hiroki Matsui
PY  - 2026
DA  - 2026/08/24
PB  - arXiv
DO  - 10.48550/arxiv.2605.05916
UR  - https://arxiv.org/abs/2605.05916
AB  - We investigate light-cone smearing induced by quantum fluctuations of gravitons and its implications for the ultraviolet structure of quantum field theory. By treating the first-order correction to Synge's world function as an operator, we show that the retarded Green's function is smeared by the variance of graviton fluctuations. The smearing width depends on the quantum state of gravitons: vacuum fluctuations generate a Gaussian smearing of the light cone, coherent states shift the light-cone position, and squeezed states modify the smearing width itself. We then apply the smeared Feynman propagator to one-loop self-energies in interacting scalar field theories. Within a phenomenological finite-resolution prescription that keeps the effective width nonzero, the ultraviolet-sensitive short-distance terms in the ϕ^3 bubble and ϕ^4 tadpole diagram expressions are finite. For the illustrative choice that the coarse-graining scale is the Planck length, primordial gravitons induce a relative correction of order 10^−10 to the one-loop self-energy. Our results suggest that the quantum state of gravitons can leave a finite imprint on the causal and short-distance structure of quantum field theory.
ER  -