The S251112cm Gravitational-Wave Event as a Potential Observational Anchor for the Substrate of the Swygert Theory of Everything AO

The S251112cm Gravitational-Wave Event as a Potential Observational Anchor for the Substrate of the Swygert Theory of Everything AO

DOI: to be assigned

John Swygert

April 3, 2026

Abstract

The LIGO-Virgo-KAGRA candidate event S251112cm, reported in November 2025, presents a binary merger involving at least one likely sub-solar-mass compact object in a mass regime not naturally explained by standard stellar-evolution channels. Recent analyses (arXiv:2602.21295 and 2603.25795) argue that a primordial-black-hole interpretation is viable within current observational bounds. This paper proposes that, if that interpretation is confirmed, S251112cm may serve as a meaningful observational anchor consistent with the substrate framework of the Swygert Theory of Everything AO. The event would thereby illustrate how the ordered equilibrium conditions of the earliest universe could leave behind persistent, macroscopic relics that remain relationally connected across cosmic time, offering a concrete point of contact between gravitational-wave astronomy and the foundational substrate described by the theory.

I. The Substrate of TSTOEAO

The Swygert Theory of Everything AO begins with the recognition that the universe rests upon a foundational substrate: a condition of pure ordered equilibrium, without energy, mass, or dimension in the ordinary sense, yet encoded with law that governs the emergence of all subsequent structure. This substrate is not itself a physical medium or cause in the conventional sense; it is the generative ground from which the first large-scale physical expressions arise. In the earliest moments after the Big Bang, that encoded order manifested as a hot, dense, near-homogeneous plasma in which tiny primordial density fluctuations existed within a globally ordered equilibrium. From this phase, macroscopic structures emerge not as random accidents but as persistent, relationally connected relics that preserve the original order across time and scale. Any stable, non-stellar object traceable to those first instants therefore stands as a potential observational contact point with the substrate itself.

II. The S251112cm Event

On 12 November 2025, the LIGO-Virgo-KAGRA network recorded gravitational-wave candidate S251112cm. The signal is consistent with a binary merger whose component masses fall well below the Chandrasekhar limit and below the minimum mass expected for astrophysical black holes or neutron stars. Detailed follow-up studies (Magaraggia & Cappelluti 2026; Haque et al. 2026) demonstrate that no conventional stellar-evolution channel accounts for the observed parameters. The analyses instead argue that a primordial-black-hole interpretation is viable within current observational bounds. The predicted merger rate and abundance constraints align with existing limits, leaving open the possibility that this event represents the first candidate detection of such objects.

III. Relation to the Substrate

Within the framework of TSTOEAO, primordial black holes of sub-solar mass can be interpreted as relic imprints of the equilibrium conditions that prevailed in the first fractions of a second after the Big Bang. They are not the end products of later stellar evolution; they would be frozen macroscopic expressions of the primordial density perturbations that arose directly from the substrate-encoded order. Their survival to the present epoch would demonstrate the persistence of relational structure across cosmic time — a central expectation of the theory. Moreover, the same population offers a natural candidate for a significant fraction (or potentially all) of dark matter, thereby keeping the visible and invisible sectors inside one coherent relational order rather than treating them as disconnected puzzles. If confirmed, S251112cm would therefore supply a concrete observational anchor for the substrate: not proof, but a meaningful empirical contact point between the earliest equilibrium phase and modern gravitational-wave astronomy.

IV. Implications for the Theory

Should future observations strengthen the primordial-black-hole interpretation of S251112cm, the event would illustrate how the substrate’s encoded order can produce stable, detectable structures that persist from the earliest moments of cosmic history to the present. This would not constitute final validation of the theory, but it would provide a clear and testable point of contact between TSTOEAO and ongoing gravitational-wave data. Future detections of similar sub-solar-mass events, or tighter constraints on the primordial black-hole mass spectrum, would further refine and test this picture while maintaining the theory’s emphasis on ordered relation across all scales.

Conclusion

The LIGO candidate S251112cm, interpreted as a possible primordial-black-hole merger, stands as a potentially important observational development consistent with the substrate framework of the Swygert Theory of Everything AO. It offers a meaningful empirical contact point between gravitational-wave astronomy and the foundational ordered equilibrium that the theory takes as its starting point. In doing so, it reminds us that structure is not imposed upon chaos after the fact; it is the natural and enduring expression of the primordial substrate itself. The event therefore marks not only a milestone in observational cosmology but a valuable opportunity to examine how the earliest encoded order continues to manifest in the modern universe.

References

Magaraggia, A., & Cappelluti, N. (2026). Implications for PBH Dark Matter from a single Sub-Solar-Mass GW Detection in LVK O1–O4. arXiv:2602.21295.

Haque, M. R., et al. (2026). Primordial Black Hole interpretation of the sub-solar merger event S251112cm. arXiv:2603.25795.

Swygert, J. (2025–2026). Foundational papers on the substrate and early-universe equilibrium, Ivory Tower Journal and TSTOEAO archive.