“Lensing Is Low”: Galaxy-Galaxy Lensing Deficit

The ΛCDM Tension

BOSS galaxy clustering plus the standard galaxy-halo connection under Planck ΛCDM predicts a galaxy-galaxy lensing signal 20 to 40 percent larger than measured, worst (about 30 percent) below 5 Mpc/h (Leauthaud et al. 2017). Baryons, neutrinos, and reasonable GR modifications each move the prediction only a few percent, and a five-survey blind comparison confirms the deficit is real, not instrumental.

The ΛCDM Assumption That Creates It

The halo model assumes clustering and lensing are two readings of the same CDM halos: positions fix masses, masses fix lensing. There is no freedom for the two to disagree by 30 percent, so the model must either inflate halo-occupation flexibility until prediction evaporates or carry an unexplained deficit that points the same way as the S₈ tension.

SCT Resolution: M6 (Coherence Mismatch Between Clustering and Lensing)

SCT replaces the dark matter halo with coherent gravitational amplification of baryons: the effective mass profile is A(r) times baryonic, where the coherence amplification grows from near 1 in inner regions toward the virialized fixed point A* = 5.970 at the virial radius (P50, P52). The radial shape matters: an NFW halo calibrated to match the clustering-implied total mass distributes that mass differently with radius than the coherence profile does, exceeding it precisely at the intermediate radii (0.1 to 5 Mpc/h) where galaxy-galaxy lensing measures. A ΛCDM halo fit to the positions therefore overpredicts the lensing at those radii: lensing is low because the NFW expectation is high, not because mass is missing.

The redshift-and-amplitude bookkeeping closes the same way as the S₈ family: the Planck-normalized clustering amplitude carries coherence contributions a matter-only model attributes to mass, so every late-time lensing observable, cosmic shear, CMB-lensing cross-correlations, and galaxy-galaxy lensing, comes in low against it by the related factor, with sigma8_inferred = A^(1/2) sigma8_true setting the scale. One secondary modulation: assembly-bias-like selection effects are real and absorb part of the small-scale gap, which is why HOD flexibility helps below 1 Mpc/h without resolving the full range.

This is the same coherence physics behind the S₈ deficit, the growth-index excess, and the cluster lensing calibrations. There is no need to invoke 30 percent baryonic feedback or to dismantle the halo model's predictivity.

Falsifier

The discriminating shape: SCT requires the lensing deficit to track the coherence profile, largest at intermediate radii, shrinking toward small radii where A approaches 1 and toward large radii where both models converge on the two-halo term, and diminishing with redshift as A(z) falls. DESI and Euclid measuring a deficit that is flat in scale or constant in redshift would break the coherence reading; full agreement of lensing with NFW-shaped profiles at all radii in a large stacked sample would do the same.

Premise Grounding

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