The sharpest empirical handle on the vacuum: w = −1 is an identity for a true vacuum energy (Lorentz invariance forces T_μν = −ρ g_μν), not a fit parameter — so observation can test it. From this registry's corrected CPL fit (w₀ = −0.849, wₐ = −0.548), w crosses −1 at z = 0.380 and is phantom above it, at Δχ² = 6.97 on 2 dof = 2.16σ. That is NOT a detection: 24% of the way to 5σ, which needs σ(w₀) ≤ 0.030.
The one place in the vacuum-energy question where data rather than philosophy does the work. CORRECTED 2026-07-26: first admitted with the pre-Lyα-fix values (w₀ = −0.836, 2.396σ, z_cross = 0.3685); restated against the corrected fit. Also recorded: the often-quoted '~1% drift since z=1' badly understates it — z = 1 sits where the rising and falling branches cancel; across the real data window the drift is far larger.
Falsify-box — how to kill this claim
Verification record — every quoted number, re-run 2026-07-26
| quantity | measured | verdict |
|---|---|---|
| w = −1 crossing redshift | z = 0.380 (from corrected w₀ = −0.849, wₐ = −0.548) | MATCH |
| significance | 2.16σ (Δχ² = 6.97, 2 dof) — 24% of the way to 5σ | MATCH |
| σ(w₀) required for 5σ | 0.0302 — roughly 5× the current effective data volume | MATCH |
| correction applied | pre-Lyα-fix values (2.396σ, z = 0.3685) superseded on 2026-07-26 | MATCH |
Provenance
script status: PRESENT
datasets: information-seam-scripts (downloadable from /data — run it yourself)
re-run: 2026-07-26
Edges
Status, honestly
verified by adversarial re-run (workflow, 2026-07-26); CORRECTED same day after the DESI Lyman-α covariance fix superseded its input values — restated, not quietly edited. Status here is computed from evidence — the author cannot set it, and neither can we. Independent reproduction would move it; nothing else will.
The founder's own run of this script, captured verbatim. A match proves the result is reproducible; it is still R0 on this registry's independence rings — same code, so it cannot move a status. Only an outside run does that.
OSED FORM vs NUMERICAL rho_DE: max relative disagreement
best fit: 3.094e-14 (GL in ln a), 1.861e-15 (composite GL in a),
2.613e-13 (RK4 on the ODE). Arithmetic validation only -- carries
ZERO evidence weight about nature.
[H2] PERCENT CHANGE IN rho_DE, z = 1 -> today:
best fit (w0=-0.836, wa=-0.609): -1.178 % [rho ratio 0.988218]
LCDM / true vacuum: +0.000 % EXACTLY, by construction
Peak excursion: +7.589 % at z = 0.369 (the w=-1 crossing).
DO NOT quote the z=1 number alone -- it is small only because it
sits where the rising and falling branches cancel. Largest
|drift| in the z <= 2.5 data window: 30.75 % at z = 2.50; at the
window edge z = 2.5 it is -30.75 %.
NO ERROR BAR: no covariance was supplied. PART F shows this
number's SIGN is not established over a plausible parameter grid.
[H3] w = -1 CROSSING REDSHIFT (best fit): z_cross = 0.3685 (a = 0.730706).
Registry reports z ~ 0.37; verified from the fitted parameters.
LCDM: no crossing -- w is pinned at -1 identically.
Phantom (w < -1) for ALL z > 0.369.
[H4] rho_DE(a)/rho_DE(1) as a -> 0 (best fit): -> 0, from above.
Exponent on a is +1.3350 > 0; exp() factor -> 6.2152 (finite).
STRICTLY POSITIVE for all a > 0; NO sign change anywhere in
0 < a <= 1 -- but CPL cannot produce one for ANY parameters, so
that is a fact about the parameterization, not a measurement.
Not an energy floor: dark energy switched on.
[H5] EVIDENCE: Delta chi^2 = 8.2 (2 extra parameters) = 2.40 sigma.
3 sigma needs Delta chi^2 = 11.83 (have 69%, short by 3.63)
5 sigma needs Delta chi^2 = 28.74 (have 29%, short by 20.54)
NOT A DETECTION. Data are CONSISTENT with a constant vacuum and
MILDLY PREFER evolution. Honest label: PROVISIONAL.
[H6] REQUIRED sigma(w0) FOR A 5-SIGMA STATEMENT at the current central
value: |w0+1|/5 = 0.164000/5 = 0.032800.
(3 sigma would need 0.054667.) Rough current-scale estimate 0.068446
-> factor 2.09 tighter, ~4.4 x the effective data volume.
CONDITIONAL on the central value not moving toward -1. If
w0 = -1 is the truth, no precision ever gets to 5 sigma.
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INTERPRETATION (honesty rules apply)
==============================================================================
THIS IS THE ONE PLACE IN THE WHOLE VACUUM-ENERGY QUESTION WHERE DATA,
NOT PHILOSOPHY, DOES THE WORK.
Tests 13 and 14 in this wave could not be settled by computation
because the obstacle there is conceptual: nobody knows whether
zero-point energy should gravitate, and no amount of arithmetic
decides it. The w = -1 question is different in kind. A vacuum
energy has w = -1 exactly and forever -- not approximately, not on
average, not as a best fit. Lorentz invariance of the vacuum state
makes it an identity. So w is a knob that observation can turn, and
it is turning.
WHAT THE DATA CURRENTLY SAY, in one sentence: consistent with
constant, mildly prefers drift, not a detection.
Quantitatively, from the registry's own fitted values:
* The measured w(z) crosses -1 near z = 0.37 and is PHANTOM above
it -- behaviour a vacuum energy is structurally incapable of.
* The implied density drift is modest but NOT uniformly tiny, and
the tempting one-line gloss is wrong. rho_DE rises to ~8% above
today's value at the crossing, is back within ~1% of today at
z = 1 (a coincidental cancellation, not a smallness result), and
is ~31% BELOW today's value by z ~ 2.5 at the edge of the data.
So: a few-percent wiggle for z < 1, a tens-of-percent decline
across the full window. Not a dramatic switch-on; not a wiggle
either.
* Delta chi^2 = 8.2 for two extra parameters is 2.40 sigma. Three
sigma needs 11.83; five needs 28.74. We have 69% of the way to
the weaker of those two bars. That is a preference.
* Without the fit covariance -- which the registry did not supply --
even the SIGN of the z=1 drift is not established across a
plausible parameter range. This is the largest single caveat on
the page and it is a caveat about bookkeeping, not about nature.
THE CONNECTION, STATED AND NOT OVERCLAIMED. IF w != -1 is confirmed
by Euclid, DESI DR3 or LSST, then dark energy is not a fixed energy
floor and the constant-Lambda interpretation FAILS -- regardless of
how the cosmological constant problem is resolved. That is a real
and unusual logical structure: a measurement that would falsify the
vacuum reading without needing to understand it first. Reaching 5
sigma at today's central value needs sigma(w0) ~ 0.033 -- roughly
twice today's precision, on a back-of-envelope inversion that PART F
labels as sloppy. Whether that happens depends on the central value
staying put, which is exactly the part nobody can forecast.
WHAT THIS DOES NOT DO -- SAID EXPLICITLY.
* NOTHING HERE SOLVES THE COSMOLOGICAL CONSTANT PROBLEM. Not
partially, not in principle. The magnitude discrepancy between
predicted vacuum energy density and the observed value is ~10^60
with a TeV cutoff and ~10^120 with a Planck cutoff -- and quoting
either number without its cutoff assumption is meaningless,
because the 'prediction' is not the output of any complete
theory. A tens-of-percent drift in rho_DE is orthogonal to a
60-to-120-ORDER-OF-MAGNITUDE mismatch. Confirming w != -1 changes
WHICH problem we have, not answer this one.
* NO NEW FIT IS CLAIMED. Four numbers (w0, wa, Delta chi^2, and
the crossing redshift) came in from claim USR-2026-0001. No
likelihood was evaluated, no data were read, no chain was run.
Everything printed above is an exact consequence of those four
inputs plus textbook cosmology. REPRODUCED, NOT DISCOVERED.
* CPL IS NOT A THEORY. It is a two-parameter Taylor expansion in
(1-a). Its w=-1 crossing, its positivity, and its a -> 0
behaviour are all partly artifacts of that functional form. The
strongest honest version of this test's conclusion is a
CONDITIONAL, and the condition is 'if CPL is the right shape'.
* THE PROJECT'S OWN AUDIT SAYS 3-4 SIGMA, and published DESI DR2
analyses span ~2.8 to ~4.2 sigma depending on the supernova
compilation. That spread is dataset choice, not statistics. A
result whose significance depends on which SN sample you pick is
by definition not yet a measurement of nature.
BOTTOM LINE: the vacuum's constancy is TESTABLE, is BEING TESTED, and
currently PASSES -- weakly, with a mild and unstable pull away from
-1 that has not earned the word 'detection'. Provisional.
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