Geometric Horizon Inflation: A Precise Prediction for Next-Generation Gravitational Wave Detectors

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Authors: Raghu Kulkarni
Cited by: 0

Abstract

Recent spectroscopic analyses of the gravitational wave event GW250114 (SNR ≈80) report a final remnant area of ≈400,000 km2, representing a ≈7.1% excess over standard General Relativistic predictions. While Neutron Stars exhibit a full lattice sintering boost of 8.3% due to material support (K = 12 →13), we propose that the event horizon represents a Frustrated Phase Transition. Lacking nucleon degeneracy pressure, the vacuum lattice cannot sustain a fully sintered shell (K = 13) and collapses into a Holographic Projection of the transition. We derive a geometric constraint factor η = 1/√3, which suppresses the full 8.3% boost to a projected value of 7.13%. This model accurately predicts the observed anomaly while maintaining consistency with the “Vacuum Fluid” hypothesis required for gravitational echo delays.

Fields of Study & Subjects

Black Holes and Theoretical Physics Pulsars and Gravitational Waves Research Noncommutative and Quantum Gravity Theories

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
27 January 2026
Document type
Preprint