Formation-population gate showing ordinary hierarchical relaxation cannot assemble the required near-critical compact boson-star seed.
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Updated
Aug 6, 2026 - Python
Formation-population gate showing ordinary hierarchical relaxation cannot assemble the required near-critical compact boson-star seed.
Action-derived Palatini/complex-scalar Engrenage controls and TEST 028 archive; charge repair passes but Einstein constraints fail refinement.
Primordial-production gate showing a minimal scale-invariant spectator cannot generate the required coherent boson-star seed population.
Palatini boson-star equilibrium benchmark isolating the dense-model factor-of-two coupling discrepancy in the published equations.
Cross-candidate bosonic production-collapse overlap gate identifying a rare many-soliton L-ball route while leaving the single-star seed problem open.
Constant curvature-coupling successor audit finding no cosmologically admitted route that preserves the earlier compact-star collapse action.
The GrokGarcia Conjecture proposes a unified scalar field model uniting dark matter, dark energy, and cosmic acceleration through innovative cosmological research.
Inflaton-portal feasibility audit finding severe ultralight-mass radiative-naturalness failure in the declared unprotected action.
General-relativistic self-interacting complex-scalar equilibrium and collapse archive with controlled turning points and horizon formation.
Read-only identifiability audit of sealed Palatini FEED1 histories, withholding flux-to-geometry response where transport and endpoint data do not close.
This code solves the Einstein-Klein-Gordon field equations for constructing spinning (mini) boson stars.
Working manuscript on action reconciliation, an independent spherical BSSN/PIRK implementation, and controlled Palatini horizon formation.
Invariant proper-time and conserved-flux admission audit for quadratic Palatini boson-star continuation, with inflation and ordinary-gas claims withheld.
Negative mass in general relativity: proof that the negative-mass Schwarzschild instability is a point-mass effect, with exact thresholds for finite stars, and stability of a negative-mass boson star. Two papers plus the code that verifies them.
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