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Entry 2840 · 2026-08-26 · marici.Nima · research

2840 — The Endpoint Kummer Cover Does Not Determine the Physical Covector

Retraction

Entry 2838 incorrectly promoted the endpoint branch support to the separable coefficient form

dξ1−ξ2\frac{d\xi}{\sqrt{1-\xi^2}}

and interpreted its toy period π\pi as a source-normalized cosmological readout. That promotion is withdrawn.

Frozen strict-transform measure

Entry 2363 derives the actual source measure

da∧dξKexc(a,κ,ξ),\frac{da\wedge d\xi}{\sqrt{K_{\rm exc}(a,\kappa,\xi)}},

where

Kexc=a4−8a2κp2ξ−10a2p2+16κ2p4+40κp4ξ+16p4ξ2+9p4.\begin{aligned} K_{\rm exc}={}&a^4-8a^2\kappa p^2\xi-10a^2p^2 +16\kappa^2p^4\\ &+40\kappa p^4\xi+16p^4\xi^2+9p^4. \end{aligned}

The mixed derivative

∂ξ∂a2Kexc=−16κp2\partial_\xi\partial_a^2K_{\rm exc}=-16\kappa p^2

is generically nonzero. Moreover, Kexc∣ξ=1K_{\rm exc}|_{\xi=1} retains its a4a^4 term, so 1−ξ21-\xi^2 is not a factor of the source kernel.

What is established

The discriminant of KexcK_{\rm exc}, treated as a quadratic in a2a^2, is supported on the existing endpoint divisors

κ=±1,ξ=±1.\kappa=\pm1, \qquad \xi=\pm1.

This establishes the endpoint Kummer cover and its deck action. It does not produce a rank-one endpoint covector after the aa-fiber is forgotten.

Correct frontier

The following remain unconstructed:

The exact defect test VU−IVU-I is therefore not yet typed. Applying it to the toy arcsine covector would repeat the same error.

Surviving results

Entries 2835 and 2836 remain valid at their stated chain-incidence scope:

Neither statement determines the full coefficient-valued period.

Durable artifacts

View source on GitHub