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April 13, 2026Open Access

SIP-PHY-01d Quasars as α-Regulated Engines

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Authors

JSJohn Richard SmithSHSHAI / HATI2

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Overview

This framework reveals quasar dynamics through a novel non-equilibrium model, suggesting implications for black hole behavior.

Key Points

  • This research aims to develop a non-equilibrium framework for understanding black hole dynamics, specifically focusing on quasars.
  • Developed a framework based on dynamic imbalance using Bogoliubov coefficients in curved spacetime.
  • Extended the Clausius relation to encompass irreversible horizon thermodynamics.
  • Derived the Bekenstein-Hawking Area Law from first principles and analyzed quasar properties with quantifiable metrics.
  • Quasar light curves exhibit 1/f flicker noise, with a scaling exponent related to the Eddington ratio.
  • Decreased variance of α is observed with increasing black hole mass, indicating a homeostatic behavior.
  • Effective temperature of Hawking radiation is reduced by a factor during high-accretion events.

Cite This Study

Smith et al. (2026) studied this question.

synapsesocial.com/papers/69dc88d83afacbeac03eaa3bhttps://doi.org/10.5281/zenodo.19507795
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