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Updated: Apr 27, 2026

Measurement of Particle Size Distribution in Turbid Solutions by Dynamic Light Scattering Microscopy
Published on: January 9, 2017
Value of H(0) in the inhomogeneous universe
Ido Ben-Dayan1, Ruth Durrer2, Giovanni Marozzi2
1Deutsches Elektronen-Synchrotron DESY, Theory Group, D-22603 Hamburg, Germany.
Abstract:
Local measurements of the Hubble expansion rate are affected by structures like galaxy clusters or voids. Here we present a fully relativistic treatment of this effect, studying how clustering modifies the mean distance- (modulus-)redshift relation and its dispersion in a standard cold dark matter universe with a cosmological constant. The best estimates of the local expansion rate stem from supernova observations at small redshifts (0.01
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