The Leo Monichan BH–WH Hypothesis

The Leo Monichan BH–WH Hypothesis is a speculative theoretical-physics research manuscript proposing a two-stage black-hole process: an assumed quantum-gravitational bounce from an initial black hole (BH₁) to a white-hole-like post-bounce state (WH₁), followed by an interaction between WH₁ and a second black hole (BH₂) that may produce a new black hole (BH₃) and exported energy. The manuscript develops a phenomenological energy-accounting relation, called the Leo Monichan BH Formula: Mᴸ = Mᴮ + Mᵂ − Eᵣ/c² The paper examines conditions under which the final black hole could have greater, equal, or lower mass than the second black hole, and discusses the corresponding effective Schwarzschild-radius relation. It also identifies the theoretical requirements needed to determine whether such a black-hole formation process can occur, including quantum-gravity dynamics, trapped-surface formation, numerical-relativity calculations, energy and angular-momentum flux, and possible observational consequences. This work is presented as a hypothesis and phenomenological research framework, not as an experimentally established physical law or a confirmed prediction of quantum gravity. This accurately reflects your manuscript's stated scope and avoids claiming that the hypothesis has been experimentally proven. �

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-09-25
DOI
https://doi.org/10.5281/zenodo.22948931
Primary Topic
Quantum Electrodynamics and Casimir Effect
Type
preprint
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The Leo Monichan BH–WH Hypothesis

Leo Monichan
Zenodo (CERN European Organization for Nuclear Research)
Quantum Electrodynamics and Casimir Effect
preprint

The Leo Monichan BH–WH Hypothesis

Leo Monichan
preprint en

Abstract

The Leo Monichan BH–WH Hypothesis is a speculative theoretical-physics research manuscript proposing a two-stage black-hole process: an assumed quantum-gravitational bounce from an initial black hole (BH₁) to a white-hole-like post-bounce state (WH₁), followed by an interaction between WH₁ and a second black hole (BH₂) that may produce a new black hole (BH₃) and exported energy. The manuscript develops a phenomenological energy-accounting relation, called the Leo Monichan BH Formula: Mᴸ = Mᴮ + Mᵂ − Eᵣ/c² The paper examines conditions under which the final black hole could have greater, equal, or lower mass than the second black hole, and discusses the corresponding effective Schwarzschild-radius relation. It also identifies the theoretical requirements needed to determine whether such a black-hole formation process can occur, including quantum-gravity dynamics, trapped-surface formation, numerical-relativity calculations, energy and angular-momentum flux, and possible observational consequences. This work is presented as a hypothesis and phenomenological research framework, not as an experimentally established physical law or a confirmed prediction of quantum gravity. This accurately reflects your manuscript's stated scope and avoids claiming that the hypothesis has been experimentally proven. �

Zenodo (CERN European Organization for Nuclear Research)
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Quantum Electrodynamics and Casimir Effect
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