No dark matter particles, no Λ, no singularities. Just geometry. Who wants to do the math?tl;dr: 5D manifold with skew/non-orthogonal embedding instead of compact Kaluza-Klein. Everything falls out: Dark Matter as gravitational shadow from offset brane, Dark Energy as entropic pressure gradient from standing wave, quantum stuff as phase brushes.Quick hierarchy:- D1–D3: normal space- D4: time/entropy arrow- D5: phase/orientation (charge = p5, antiparticles = inverse phase)- D6: embedding plane for 90°-ish intersections between 5D sheets- D1–D6 = many-worlds block- D7+ = hypertemporal line through universesStart with 5D Einstein-Hilbert:S = ∫ d5x √(-g(5)) R(5)Decompose metric with non-orthogonal terms (key difference from standard KK):g_AB = [g_μν + κ2φ2 A_μ A_ν κφ2 A_μ] [κφ2 A_ν φ2 ]Allow ∂_μ φ ≠ 0 and g_μ5 ≠ 0 induced stress-energy T_μν^induced from bulk curvature R_5μ5νΛ_eff ~ (∂_5 φ)2 acceleration from pressure imbalance (compressed low-entropy behind pushes, high-entropy ahead resists less)Who can:1. Reduce the action, get effective 4D equations with correction terms2. Fit induced T_μν to SPARC rotation curves (no DM particles)3. Solve for a(t) with Λ_eff and check vs supernova/BAO data4. Constrain skew angle from torsion-balance short-distance tests or α variationPost your LaTeX, plots, or why it dies.Pic unrelated, its just cool looking and I needed an image. TIA
1) There's a fucking built in TeX editor. Put some effort into formatting your math instead of fucking spamming unformatted LLM output. That's the least you can do.2) This is literally nothing. This falls into the category of "not even wrong".3) My head hurts.
I despise AIniggers so much. They have ruined my favorite board.
>>16917997It's literally just jeet newfriends with too much free time on their hands
