Cosmology and the Large-Scale Structure of the Universe
Cosmology studies the universe as a physical system: its origin, expansion, composition, geometry, thermal history, structure formation, and large-scale distribution of matter. This article examines the cosmological principle, FLRW spacetime, scale factor, redshift, Hubble expansion, Friedmann equations, ΛCDM, radiation, baryons, cold dark matter, dark energy, inflation, primordial perturbations, the cosmic microwave background, acoustic peaks, baryon acoustic oscillations, galaxy surveys, weak lensing, cosmic web morphology, linear perturbation growth, transfer functions, matter power spectra, halo formation, N-body simulations, hydrodynamic simulations, observational tensions, DESI-era dark-energy questions, and the future of survey cosmology. Selected R and Python workflows model FLRW expansion, distance-redshift relations, linear growth, and toy matter power spectra, while the linked GitHub repository expands the article with reproducible cosmology workflows.









