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New nonlocal effective action

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

2 Pith papers citing it
abstract

We suggest a new method for the calculation of the nonlocal part of the effective action. It is based on resummation of perturbation series for the heat kernel and its functional trace at large values of the proper time parameter. We derive a new, essentially nonperturbative, nonlocal contribution to the effective action in spacetimes with dimensions $d>2$.

citation-role summary

background 1

citation-polarity summary

fields

gr-qc 1 hep-ph 1

years

2026 1 2025 1

verdicts

UNVERDICTED 2

roles

background 1

polarities

background 1

representative citing papers

Unveiling horizons in quantum critical collapse

gr-qc · 2025-09-03 · unverdicted · novelty 6.0 · 2 refs

Semiclassical one-loop analysis of solvable near-critical collapse solutions shows quantum corrections selecting a Boulware-like state and producing a growing mode that yields a finite mass gap and a transition to Type I behavior, enforcing weak cosmic censorship.

Axion Inflation from Heavy-Fermion One-Loop Effects

hep-ph · 2026-04-15 · unverdicted · novelty 6.0

One-loop integration of a heavy fermion with inflaton-dependent mass in axion inflation generates localized gauge-field production and a detectable chiral gravitational-wave signal in the deci-hertz range.

citing papers explorer

Showing 2 of 2 citing papers.

  • Unveiling horizons in quantum critical collapse gr-qc · 2025-09-03 · unverdicted · none · ref 231 · 2 links · internal anchor

    Semiclassical one-loop analysis of solvable near-critical collapse solutions shows quantum corrections selecting a Boulware-like state and producing a growing mode that yields a finite mass gap and a transition to Type I behavior, enforcing weak cosmic censorship.

  • Axion Inflation from Heavy-Fermion One-Loop Effects hep-ph · 2026-04-15 · unverdicted · none · ref 155

    One-loop integration of a heavy fermion with inflaton-dependent mass in axion inflation generates localized gauge-field production and a detectable chiral gravitational-wave signal in the deci-hertz range.