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May 7, 2026Open Access

P36 v2.1: Phase Diagram of Compact Objects in CCEGA — Three Regimes from Neutron Stars to Black Holes

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Authors

MSMarc López Sánchez

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Overview

Analysis reveals distinct mass regimes for neutron stars and black holes, suggesting new insights into compact object dynamics.

Key Points

  • This research aims to update the phase diagram of compact objects within the CCEGA framework.
  • Analyzed mass regimes of compact objects: neutron stars, ultracompact horizonless objects, and black holes.
  • Conducted GR consistency check across different density limits.
  • Quantified radion contributions to compact object formation.
  • Identified three mass regimes: M < 4.56 M_sun for neutron stars, 4.56–12.0 M_sun for horizonless objects, and M > 12.0 M_sun for black holes.
  • Confirmed GR consistency with Oppenheimer–Volkoff limit at low density.
  • Detailed radion contributions demonstrate support for neutron stars and formation of black stars.

Cite This Study

Marc López Sánchez (2026) studied this question.

synapsesocial.com/papers/69fbe2f2164b5133a91a2417https://doi.org/10.5281/zenodo.20032670
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