Data Science Intern
St. Andrews, Scotland, United Kingdom
Analysing large hydrodynamical simulations in vHDM cosmology and working with cutting-edge observational data, by developing parallelised Fortran and Python algorithms, in search of a plausible solution to the observed Hubble tension and whether recent, consistent, bulk flow and Hubble dipole observations are realistic.My analyses found that the Hubble tension could plausibly be solved in this cosmological model and that a reversal of the bulk flow direction occurs often at a radius in line with observations, adding greater tension to the current, leading cosmological models.