2D water-alcohol mixtures stay fully miscible with micro-segregation that grows with alcohol chain length, driven by water self-aggregation but limited by rim contacts, due to reorganization of fluctuations under charge ordering.
Numerical Fourier and Bessel transforms in logarithmic variables , year =
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New UNIONS galaxy-galaxy lensing data around CMASS galaxies indicates no significant lensing is low problem, with joint HOD fits to GGL and GC favoring a slightly lower matter power spectrum amplitude than Planck.
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Aqueous-alcohol mixtures in dimension two: miscibility and micro-segregation
2D water-alcohol mixtures stay fully miscible with micro-segregation that grows with alcohol chain length, driven by water self-aggregation but limited by rim contacts, due to reorganization of fluctuations under charge ordering.
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Revisiting the 'Lensing is Low' Problem with UNIONS
New UNIONS galaxy-galaxy lensing data around CMASS galaxies indicates no significant lensing is low problem, with joint HOD fits to GGL and GC favoring a slightly lower matter power spectrum amplitude than Planck.