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\u003cp\u003e\u003ci\u003eModern Cosmology, Third Edition\u003c/i\u003e provides a detailed introduction to the field of cosmology. Beginning with the smooth, homogeneous universe described by a Friedmann-Lemaître-Robertson-Walker metric, this trusted resource includes careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. The reader is then introduced to perturbations about an FLRW universe: their evolution with the Einstein-Boltzmann equations, their primordial generation by inflation, and their observational consequences: the acoustic peaks in the CMB; the E/B decomposition in polarization; gravitational lensing of the CMB and large-scale structure; and the BAO standard ruler and redshift-space distortions in galaxy clustering.\u003cbr\u003e\u003cbr\u003eThis revised third edition includes updates such as new sections on gravitational waves, line intensity mapping, and emergent analysis techniques; expanded sections of CMB secondaries; and revised figures and pedagogy. These revisions serve to enhance a comprehensive foundational text, as well as provide users with improvements that are aligned with recent advances in the field, as well as modern focuses in the classroom. \u003c/p\u003e\u003cul\u003e\u003cli\u003eOffers a unique and practical approach for learning how to perform cosmological calculations\u003c/li\u003e\u003cli\u003eIncludes new material on theory, simulations, and analysis of nonlinear structures\u003c/li\u003e\u003cli\u003eContains substantial updates on new developments in cosmology since the second edition, including new content on gravitational waves, as well as a new section on emergent analysis techniques and improved pedagogy around figures and imagery\u003c/li\u003e\u003c/ul\u003e |
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