Multiscale cluster lensing reveals subhalo inner density slopes steeper than collisionless CDM allows and radial distributions that mismatch CDM, while mass functions and truncation radii align.
The right panel of Figure A1 shows the average distribution and the respective 1σconfidence interval
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New Cold Dark Matter Crisis Revealed by Multiscale Cluster Lensing
Multiscale cluster lensing reveals subhalo inner density slopes steeper than collisionless CDM allows and radial distributions that mismatch CDM, while mass functions and truncation radii align.