pith. sign in

Koemans Collado, P

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it

citation-role summary

background 1 baseline 1

citation-polarity summary

fields

hep-th 2 gr-qc 1

years

2026 2 2025 1

verdicts

UNVERDICTED 3

representative citing papers

Wave-optics gravitational wave lensing in modified gravity

gr-qc · 2026-05-20 · unverdicted · novelty 8.0

In a curvature-coupled propagation framework for modified gravity, gravitational-wave lensing in wave optics shows persistent infrared interactions that prevent the amplification factor from approaching unity at zero frequency, requiring an interacting Green function and partial-wave treatment.

Eikonal, nonlocality and regular black holes

hep-th · 2026-04-20 · unverdicted · novelty 5.0

Nonlocal form factors in D-dimensional gravity yield effective geometries whose nonlinear completion gives regular, asymptotically flat Schwarzschild deformations with de Sitter cores.

citing papers explorer

Showing 3 of 3 citing papers.

  • Wave-optics gravitational wave lensing in modified gravity gr-qc · 2026-05-20 · unverdicted · none · ref 98

    In a curvature-coupled propagation framework for modified gravity, gravitational-wave lensing in wave optics shows persistent infrared interactions that prevent the amplification factor from approaching unity at zero frequency, requiring an interacting Green function and partial-wave treatment.

  • Analytic structure of the high-energy gravitational amplitude: multi-H diagrams and classical 5PM logarithms hep-th · 2025-11-14 · unverdicted · none · ref 93

    Computes the leading double logarithm at 5PM in the high-energy gravitational amplitude via multi-H diagrams and dispersion relations, extracting the single-log imaginary part of the eikonal phase.

  • Eikonal, nonlocality and regular black holes hep-th · 2026-04-20 · unverdicted · none · ref 8

    Nonlocal form factors in D-dimensional gravity yield effective geometries whose nonlinear completion gives regular, asymptotically flat Schwarzschild deformations with de Sitter cores.