Executed research experiments

Calibration, empirical chronology, interacting matter, reciprocal dynamics, release and reserved predictions. Each result retains its stated physical scope.

Findings and frozen runs · Full program

Ordinary calibration and unidentified field response

Reserved capture discrepancies are below one percent. Two-nucleon energy curves agree at the ordinary calibration point and spread as the assumed field response increases.
Three capture energies calibrate one E1 counterterm; seven other source-curve energies are reserved. The shaded drawing-width scale is not measured experimental covariance. Explicit OBE fits agree on ordinary deuteron binding but diverge under independent contact-response scenarios and predict an unwanted bound singlet. These fits do not resolve the printed source convention. Provenance · Data · PNG

Empirically calibrated alpha–alpha continuum

Changing the unmeasured contact response changes which alpha variation binds Be-8. Reserved interpolation error drops from about 2422 eV to 17 eV.
A separate Coulomb-resummed cluster EFT matches the empirical 91.84 keV, 5.57 eV Be-8 pole. Complex outgoing poles replace the real-axis approximation above 10 keV; widths below that scale are negligible at the stated precision. Short-range derivatives are scenarios, not measured inputs. Greedy interpolation uses 64 disjoint direct EFT checks; its accuracy is neither lattice accuracy nor an EFT-theory error estimate. Provenance · Data · PNG

Measured chronology in a joint history likelihood

The short excursion has a wider conditional interval. Alternative direct half-life calibrations move the apparent excursion and change whether zero lies in its interval.
Real Re/Os and corrected W observations are combined with an affected compressed Pb/Pb anchor. The left two panels use the historical Lindner direct half-life. The right panel substitutes the later Galeazzi and Arnaboldi measurements, treating their quoted statistical/systematic errors as independent Gaussian terms. These alternatives are not combined into a consensus. Unknown x/y correlation, additional common W error and W-to-Re closure delay are zero in this display; the full results scan alternatives. A calibration-dependent displacement is not a detection of changing constants. Provenance · Data · PNG

Dense candidate versus a gas confined by the box

The cosine model confines dense matter and a nonzero field within about two kilometers; the QCD field returns near zero and matter fills the numerical box.
Both actions use the same ordinary saturation anchors, fixed baryon number and weak shell gravity. The cosine candidate passes radial energy-curvature and outer-box tests; the QCD gas radius follows the box. Muons are included after the electron-only audit identified their threshold. A local minimum of this phenomenological cold functional is not a matched astrophysical object. Provenance · Data · PNG

Formation and removal within the same cold benchmark

Specified seeds form central contrast, but the density-normalized seed stays below three billionths of a radian while its supporting cloud expands. Removing matter from the confined candidate produces recurring contrast rather than monotonic decay.
Large specified seeds form contrast in smooth spherical matter at n≈0.12 fm⁻³, f_a=10¹⁶ GeV. A coherent seed normalized to the stated reference density instead remains tiny through 80 microseconds as the ordinary cloud expands. That linear response uses reciprocal zero-seed matter trajectories in a larger box with two grid/packet resolutions. The reference density is a design assumption. Matter removal is a separate intervention; its subsequent periodic contrast oscillates. These controls supply neither a stellar lifetime nor an astrophysical occurrence rate. Provenance · Data · PNG

Release, transport and genuinely reserved element ratios

Carbon delivery changes sharply when the release budget reaches deeper shells. Most transported abundance differences shrink after ordinary alternatives are fitted.
Contiguous exterior shells are released from actual helium-exhaustion profiles under an explicit binding budget and 1.4 M☉ retained-mass floor. This is not terminal ejecta or a compact-remnant identity. Released species and winds enter conservative delayed recycling. Ordinary energy and burst fraction are fit to C/O and N/O, with the family selected on those channels alone; Ne/O and Mg/O remain reserved. All displayed rate histories are imposed conditional cases. Provenance · Data · PNG

Transported patterns drive thermal and gravitational response

Matched-metallicity temperature and perturbation histories depend on the transported C/O pattern and end at their stated opacity boundary.
At Z=10⁻⁴ and one initial Jeans wavelength, the displayed trajectories stop at optical depth unity. Other runs stop at the linear-perturbation limit. Different final amplitudes can refer to different stop densities and must not be compared as fragment counts. Atomic C/O cooling, molecular/dust omissions and specified free-fall backgrounds delimit this calculation; no IMF is predicted. Provenance · Data · PNG