# n63 — pre-registration: the stellar kill battery (before the runs)

Three attempts to kill the model with existing stellar data. Each
confrontation gets: the model's measured shape (toy), the data, and the
kill condition. Written before the Q-factor run.

## Blade 1 — binary pulsars vs the wake friction
Data: PSR J0737-3039, orbital decay = GR quadrupole to 1.3e-4 (Kramer
et al. 2021). Model: universal wake friction, measured Lorentzian
(n61): P_drag ~ Omega^2/gamma^2 below the knee. Toy measurement
registered here: the drainage Q-factor Q(Omega/gamma) =
|E_bind| * Omega / P_drag from the n61 machinery.
KILL CONDITION: if the units mapping puts the drainage decay within
1.3e-4 of the GR quadrupole decay for J0737's Omega, the model dies.
SURVIVAL CHANNEL, declared: n62's fast audit (gamma pushed up by
neutron interferometry) suppresses the friction as (Omega/gamma)^2 —
the same bound that killed Lambda-naive protects the binaries. The
chain must be CONSISTENT: one gamma satisfying COW-floor AND
pulsar-friction ceiling. Report the toy Q curve and the inequality
structure.

## Blade 2 — neutron-star masses vs the exhaustion bump
Data: heaviest known pulsar 2.35 Msun (J0952-0607); NICER radii;
GW170817 tidal deformability — all GR-consistent at the few-percent
level. Model (measured, n57): G_eff(F) rises +19% near budget
activation, then falls 7.6x. A +19% G in a NS core changes maximum
masses at the tens-of-percent level; a falling G caps the maximum mass
at the exhaustion scale.
KILL CONDITION: if the exhaustion scale sits at or below NS core
depletion, observed 2.35 Msun objects and GW170817 kill the model.
STANDING PREDICTION (either way): the model REQUIRES a hard maximum
compact-object mass at its exhaustion scale — any future object above
the cap (once units fix it) is a kill; conversely the observed NS
maximum-mass cliff (~2.2-2.5 Msun) is a candidate SIGNATURE of budget
exhaustion, flagged as the model's most falsifiable astrophysical
reading. Report: the G_eff(F) shape vs the qualitative M-R requirement.

## Blade 3 — solar p-modes and pulsating stars vs universal damping
Data: solar p-mode linewidths (micro-Hz precision), Cepheid amplitude
stability over decades. Model: every T00 redistribution bleeds energy
at the measured Lorentzian. At Omega_pmode ~ mHz << gamma (fast audit),
suppression (Omega/gamma)^2 applies.
KILL CONDITION: any units mapping in which the residual damping exceeds
the unexplained fraction of p-mode linewidths. Same consistency chain
as Blade 1: one gamma must clear all three.

## The synthesis to report
A single inequality chain on the one physical rate:
  gamma >= COW floor (n62)  AND  gamma >= pulsar-friction floor
  AND gamma >= p-mode floor — all pushing the SAME direction (fast
  audit), hence mutually consistent; the model survives the stellar
  battery IF AND ONLY IF the audit is fast, which n62 already forced.
  The unified statement: every stellar blade sharpens the same edge —
  the knee is fast, and prediction 1's laboratory search is the
  decisive test. Blade 2 is the exception: it cuts on density, not
  rate, and stays live regardless of gamma.

## RESULTS (same day; Q-factor run in the session record)
- Blade 1 MEASURED: the drainage Q-factor is Q = c * gamma/Omega with
  c ~ 0.02 in toy units (Q = 0.68, 0.24 at Omega/gamma = 0.03, 0.1 —
  the 1/Omega growth confirmed below the knee). Structure: the faster
  the audit, the more protected the binaries — the SAME direction n62
  forced. With order-unity toy coupling, J0737-3039's 1.3e-4 decay
  agreement would demand gamma ~ 1e12/s (knee at THz); recorded with
  its loud caveat: the physical drag coefficient carries gravitational-
  sector suppression absent from the toy (kappa_read = 1 is arbitrary),
  so only the STRUCTURE transfers — pulsars are a gamma floor, not yet
  a number. Blade 1 verdict: cannot kill today; sharpens the knee-is-
  fast chain.
- Blade 3: same chain, same protection, same caveat. Cannot kill today.
- Blade 2 verdict: LIVE, and converted into the model's sharpest
  stellar prediction — A HARD MAXIMUM COMPACT-OBJECT MASS at the budget
  exhaustion scale, with the measured approach signature (+19% G_eff
  bump, then the 7.6x fall). The observed neutron-star maximum-mass
  cliff (~2.2-2.5 Msun) is the model's candidate reading of budget
  exhaustion; any future compact object above the (units-fixed) cap
  kills the model outright; and the bump predicts the cliff is
  approached from ABOVE GR expectations — a shape statement testable
  against the NS mass function as it fills in.