Standard Model of Cosmology Made Simple

This book is a Weekend Pocketbook on Everything You Should Know About Lambda Cold Dark Matter (Lambda-CDM), the standard model cosmologists use to explain the history, structure, and expansion of the universe. Written in everyday language, we explore how one framework connects the Big Bang, dark matter, dark energy, galaxies, cosmic background radiation, and the unresolved mysteries still troubling modern cosmology.
How can a single model describe almost everything we observe in the universe? We begin with the expanding universe, from Edwin Hubble's discovery that distant galaxies are racing away from us to Vera Rubin's evidence for invisible dark matter and the 1998 supernova observations that revealed cosmic expansion is accelerating. Together, these clues led scientists to the lambda cold dark matter (Lambda-CDM) model: a universe made mostly of dark energy and dark matter, with ordinary matter forming only a tiny fraction of the cosmic budget.
We explore why Lambda-CDM has become the dominant map of cosmology. It explains the cosmic microwave background (CMB), the faint afterglow of the Big Bang; the large-scale web of galaxies; and the early formation of light elements through Big Bang nucleosynthesis. But we also ask why this powerful model may not be the final word. There are shortcomings with it, such as the Hubble tension, the lithium problem, missing satellite galaxies, the core-cusp problem, and others.
The James Webb Space Telescope (JWST), Euclid, the Nancy Grace Roman Space Telescope, dark matter detectors, and future surveys may either strengthen Lambda-CDM or force it to evolve.