CDN-234 decomposes the cluster missing sector into GCFT response plus residual matter. At the CDN-230 separation threshold q=8. 71 and fiducial collisionless baryon share fcoll=0. 12, anchor-only GCFT supplies Xi/bar=0. 365 against the CDN-232 cluster target Xi/bar=5. 836, leaving residual matter R/bar=5. 471. Zero residual matter requires environmental amplification Aₑnv=16. 000 relative to the CDN-229 held-out galaxy response. Below that boundary, the GCFT dark sector remains two-component: coherent response plus residual matter.
Nicky Joseph Hubertus Catharina Hacquier (Sun,) studied this question.
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