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

4 Pith papers citing it

years

2026 3 2025 1

verdicts

UNVERDICTED 4

representative citing papers

Opening the Window of Ultra-Light PBHs by Exorcising the Poltergeist

hep-ph · 2026-05-20 · unverdicted · novelty 6.0

Incorporating the general-relativity mass tail df_PBH/d ln M ∝ M^3.78 smooths PBH evaporation, suppresses the scalar-induced GW signal by orders of magnitude, and reopens the ultra-light PBH window for the hot Big Bang.

Holographic pressure and volume for black holes

hep-th · 2026-02-04 · unverdicted · novelty 5.0

Introduces a holographic pressure and volume for static spherically symmetric black holes via quasi-local thermodynamics, showing large black holes become extensive in the large-system limit while small ones do not.

Semi-classical spacetime thermodynamics

hep-th · 2025-09-05 · unverdicted · novelty 5.0

Derives semi-classical gravity from thermodynamics of stretched light cones in 2D dilaton gravity with explicit conformal anomaly backreaction and shows equations of motion follow from dynamical Wald entropy in Brans-Dicke theories.

citing papers explorer

Showing 4 of 4 citing papers.

  • Gravitational Waves from Black Hole Reheating: The Scalar-Induced Component hep-ph · 2026-05-20 · unverdicted · none · ref 247

    Accounting for the minimal mass spread of primordial black holes from gravitational collapse suppresses the Poltergeist GW background to the level of generic scalar-induced signals and reopens ultra-light PBH parameter space.

  • Opening the Window of Ultra-Light PBHs by Exorcising the Poltergeist hep-ph · 2026-05-20 · unverdicted · none · ref 60

    Incorporating the general-relativity mass tail df_PBH/d ln M ∝ M^3.78 smooths PBH evaporation, suppresses the scalar-induced GW signal by orders of magnitude, and reopens the ultra-light PBH window for the hot Big Bang.

  • Holographic pressure and volume for black holes hep-th · 2026-02-04 · unverdicted · none · ref 4

    Introduces a holographic pressure and volume for static spherically symmetric black holes via quasi-local thermodynamics, showing large black holes become extensive in the large-system limit while small ones do not.

  • Semi-classical spacetime thermodynamics hep-th · 2025-09-05 · unverdicted · none · ref 3

    Derives semi-classical gravity from thermodynamics of stretched light cones in 2D dilaton gravity with explicit conformal anomaly backreaction and shows equations of motion follow from dynamical Wald entropy in Brans-Dicke theories.