cint

demos / chirp

Gravitational Wave Chirp in 1024 Bits

A cint program evaluates the 3.5 post-Newtonian (3.5PN) gravitational wave inspiral of two compact bodies in 1024-bit checked integers (I1024). The simulation integrates the TaylorT4 ODE down to the innermost stable circular orbit (ISCO) at v = 1/sqrt(6), followed by spliced quasinormal mode (QNM) ringdown. A relativistic consensus tether pulls the twins into phase lock.

shell
$ cint run chirp.ci
chirp receipt: tick=1000 d0=14576398344542445859 d1=16148053973575091900 d2=6304118998254214534
fuel: 1118030
stdout sha256: 71081748c228b849dbee951e09cfbda79a844dae48d116cecbcc73b5f6d3add5
chirp.ci - 3.5PN compact binary inspiral (I1024)
Leader A: Baseline
Twin B: +10-18 M
Twin C: +2×10-18 M
-- -- ISCO boundary (r = 6 M)
🔇 Audio Muted
metric quadrupole strain h+(t) · sunken slate oscilloscope
tick 0 · t = 0.00 M · 3.5PN Inspiral