Published October 29, 2026 | Version v1

PUH Theorem 402 — The Shell's Answer to a Static Tide: As T259's Bubble It Gives Λ = −0.74 at X = 14, Where a Black Hole Gives Zero, and Each of Three Readings of Its Shape Gives Λ < 0

  • 1. Independent Researcher

Description

Photonic Universe Hypothesis (PUH) — Theorem 402.

A black hole's static tidal deformability is exactly zero.

T311 placed the Shell of a Planck core 7.7 per cent outside the horizon and found that a surface there has a static tidal response suppressed only as α/|ln ε|, but left the coefficient α, and with it the sign, underived; T400 called this PUH's sharpest test.

This paper derives it under stated conditions. Outside the Shell the field is T401's, Einstein's equation under that paper's stated postulates. 

At the Shell two statements of the archive are used. Its place: the Shell sits where the tension reaches its threshold, which under T299's identification is a surface of constant clock rate, −g_tt = 1/X.

T299's identification is posited, T342 found that T175's multiplier cannot be the metric (at rest, T377), and T400 lists the Shell's place as open, so this is a stated premise.

Its shape: T259's soap bubble, 'a constant-mean-curvature surface', held by tension against pressure, 'not where gravity balances pressure' (T357), the two combined in T386's Young–Laplace balance; a rigid Shell and a weighted bubble, whose own weight enters its balance, are carried alongside.

No junction condition, no stress of the Shell in Einstein's equations, no interior and no field equation at the Shell is used.

 

Result 402.1: place and shape give one condition on the field outside, and the dimensionless tidal deformability in closed form, Λ(X) = −(16/15)/[3 ln X − q(X)], with q(X) = (X − 1)(8X² − X − 1)/[X(X² + 2X − 1)] for the bubble.

At T300's floor, X = 14, the bubble gives Λ = −0.735 (k₂ = −0.0238), a rigid Shell −0.540 and a weighted bubble −0.235.

Λ is negative in each reading and at every X, by proof, where a black hole answers zero and a neutron star a positive value.

Result 402.2: far from the horizon every reading answers like an earthed conducting sphere, k₂ → −1/2.

Near it the bubble's Λ → −(16/15)/(3 ln X − 8) and the rigid Shell's → −(16/15)/(3 ln X − 7), so T311's α = −16/45 for Λ, and the rigid Shell's law is a perfect mirror's (Cardoso et al. 2017); the weighted bubble's answer falls as ε, with no logarithm.

At a Planck offset the bubble gives −0.00194, 379 times less than at X = 14. Result 402.3: for the bubble and the rigid Shell, holding place and shape against a static tide gives the logarithmic answer that only reflection at zero frequency gives (Chakraborty et al. 2024).

T307's Shell absorbs waves, and these answers need that absorption to fade for a slow tide.

A Shell that gave way to a slow tide as a horizon does would answer as a black hole does near the horizon, but not at T300's floor (+0.21 at X = 14 in one model).

Result 402.4: GW250114's limits (Λ < 28.2 and 45.7 at 90 per cent; Andrés-Carcasona and Caneva Santoro 2025) were set for positive values only, so the Shell's answer is untested; the Einstein Telescope's projected reach, |Λ| ≈ 0.067 (Cardoso et al. 2017), lies 11 times below the bubble at X = 14.

 

What it means:

IF the Shell sits on T299's surface of constant clock rate and holds its shape against a slow tide, a Planck core answers a tide with a negative tidal deformability, well above ε in size for the bubble and the rigid Shell.

A negative value would mark a holding surface, a Shell or another such object, and neither a black hole nor neutron-star matter; reading it needs analyses that admit negative values.

Not claimed: which reading of its shape the Shell follows; that it holds against a slow tide; a value for the fraction s it holds; the answer to a changing tide; spinning cores.

OPEN: what holds the Shell's shape against a tide; whether its absorption fades for a slow tide; the Shell's place; a spinning core; X itself. Kill-conditions are stated. Scripts and outputs are supplied.

Notes (English)

T402 takes up T311's open coefficient — 'Deriving α for an absorbing Shell is the natural successor and would convert a comparative statement into a prediction' — and T400's Point 400.6 and kill-condition (v), 'armed once the tidal coefficient of an absorbing Shell is derived'. The field outside the Shell is T401's (Einstein's equation under that paper's stated postulates); at the Shell only two archive statements are used — its place (T298/T299's surface of constant clock rate, a stated premise after T342, T377 and T400) and its shape (T259's constant-mean-curvature bubble, T357's balance of tension against pressure; a rigid Shell and a weighted bubble carried alongside). No junction condition, Shell stress in Einstein's equations, interior or field equation at the Shell. [IsSupplementTo] T311 (ITS COEFFICIENT DERIVED UNDER STATED CONDITIONS: α = −16/45 FOR Λ IN THE BUBBLE AND RIGID READINGS; SIGN NEGATIVE IN EVERY READING; Λ = −0.735 AT X = 14 FOR THE BUBBLE; ITS PREMISE THAT ANY SURFACE HAS A NONZERO VALUE HOLDS ONLY FOR A SURFACE THAT HOLDS AGAINST A SLOW TIDE; 'SEVENTY TIMES' BECOMES 379, 'TWENTY-SEVEN' 43) and T400 (POINT 400.6'S SIZE AND SIGN GIVEN UNDER STATED CONDITIONS; KILL-CONDITION (v) ARMED FOR EACH READING AT A GIVEN X). "References" for the rest. SUPPLEMENTARY FILES (PUH_T402_supplementary_files.zip): puh_t402_shell_tides.py (with its _output.txt and puh_t402_data.npz), puh_t402_fig.py (with its _output.txt), PUH_T402_fig1_shell_tides.png (Figure 1). Tested: from a clean folder the scripts reproduce their outputs, data and figure exactly. ***

*** NOTE ON CHECKING: Read before computing: T311, T400 and T401 in full; T298, T299, T300, T342, T344, T357, T359, T386, T312, T313, T315, T318, T307, T308, T355 and T387; after the first check, T259, T377, T383, T384, T351 and T367; and the continuity notes on what PUH must meet (results that general relativity predicts and experiment confirms are targets; nothing at the Shell from Einstein's equations). The supersession check was run on every cited paper in its database; it surfaced T342 and T377 on T299's identification, T344 on T342's wording and T351 on T315's clock. Every quotation from the archive was matched by an automated pass to the corpus text (24 of 24) or, for T400, to its own text; every decimal in the paper was matched to the script outputs. External references by web search, no wiki-type sources; two pages refused the fetch and were not retried — arxiv.org/abs/2604.08679 (rate-limited) and the Semantic Scholar page for Martel and Poisson (client error), whose journal reference was confirmed from the publisher's DOI link. CORRECTED BEFORE CHECKING: the first script's near-horizon constants (the rigid law's denominator written 3 ln(1/eps) - 5, from H_Q -> 1/(2 eps) - 3 and K_Q -> 3 ln(1/eps) - 6) were wrong; 90-digit evaluation gives -5/2, -8 and 3 ln X - 7, and a closed form replaced a float evaluation that had lost 0.4 per cent at X = 1e10. INDEPENDENT CHECK, TWO ROUNDS AND A FINAL READING: a separate agent, without the scripts or the builder, recomputed every number from its own code (the static Zerilli equation to 1e-35, the closed forms to 120 digits, the full-metric quantities exactly by dual numbers) and read the paper cold against the corpus and the external sources. Round 1 reproduced every computed value except two illustrative second-order spreads (since removed) and found the physics overclaimed in five places, all corrected: the static answer needs the Shell to hold against a slow tide (Chakraborty, Maggio, Silvestrini and Pani 2024: a nonzero static Love number needs zero-frequency reflectivity R_0 = 1), which the first draft had hidden behind the claim that absorption does not enter; the standing of T299's identification after T342 and T377 was understated; 'round' had been read as intrinsically round, which a tension-held surface is not, so the paper now carries T259's bubble (constant mean curvature, T357's tension against pressure, T386's Young-Laplace balance) first, with a rigid Shell and a weighted bubble alongside, all three in closed form and with sign proofs; 'fingerprint' claimed more than a sign can show (other exotic objects also have negative Love numbers); and a LISA projection was quoted without its context. Round 2 reproduced all 36 entries of Table 1 and every new number, confirmed the three derivations, closed forms and derivatives g', found the bubble a faithful reading of T259, T357 and T386, and showed that holding is reflection at zero frequency only for the bubble and the rigid Shell (the weighted bubble holds yet answers near the horizon as a non-reflecting surface, falling as eps), and that a Shell that gives way is not negligible at T300's floor (+0.209 at X = 14 in a model now in Section 4); both corrected. The final reading confirmed every round-2 correction and every new number; its points of wording were taken. Not checked independently: the scripts' byte-for-byte reproducibility (the reader did not run them, by design); T388-T399, not in the corpus the reader had.

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Additional details

Software

Repository URL
https://github.com/BrianMartell/Photonic-universe-hypothesis
Programming language
Python , TeX
Development Status
Active

References

  • T. Hinderer, 'Tidal Love numbers of neutron stars', Astrophys. J. 677, 1216 (2008); Erratum, Astrophys. J. 697, 964 (2009). T. Binnington and E. Poisson, 'Relativistic theory of tidal Love numbers', Phys. Rev. D 80, 084018 (2009). T. Damour and A. Nagar, 'Relativistic tidal properties of neutron stars', Phys. Rev. D 80, 084035 (2009). E. Poisson and I. Vlasov, 'Geometry and dynamics of a tidally deformed black hole', Phys. Rev. D 81, 024029 (2010). S. Postnikov, M. Prakash and J. M. Lattimer, 'Tidal Love numbers of neutron and self-bound quark stars', Phys. Rev. D 82, 024016 (2010). K. Uchikata, S. Yoshida and P. Pani, 'Tidal deformability and I-Love-Q relations for gravastars with polytropic thin shells', Phys. Rev. D 94, 064015 (2016). F. J. Zerilli, 'Effective potential for even-parity Regge–Wheeler gravitational perturbation equations', Phys. Rev. Lett. 24, 737 (1970). K. Martel and E. Poisson, 'Gravitational perturbations of the Schwarzschild spacetime: A practical covariant and gauge-invariant formalism', Phys. Rev. D 71, 104003 (2005), arXiv:gr-qc/0502028. V. Cardoso, E. Franzin, A. Maselli, P. Pani and G. Raposo, 'Testing strong-field gravity with tidal Love numbers', Phys. Rev. D 95, 084014 (2017), arXiv:1701.01116. S. Chakraborty, E. Maggio, M. Silvestrini and P. Pani, 'Dynamical tidal Love numbers of Kerr-like compact objects', Phys. Rev. D 110, 084042 (2024), arXiv:2310.06023. LIGO Scientific, Virgo and KAGRA Collaborations, 'GW250114: Testing Hawking's Area Law and the Kerr Nature of Black Holes', Phys. Rev. Lett. 135, 111403 (2025). M. Andrés-Carcasona and G. Caneva Santoro, 'No Love for black holes: tightest constraints on tidal Love numbers of black holes from GW250114', arXiv:2512.01918 (2025).