000 01685 a2200229 4500
003 OSt
005 20250308020004.0
008 220704b xxu||||| |||| 00| 0 eng d
020 _a9780128159484
040 _cIIT Kanpur
041 _aeng
082 _a523.1
_bD662m2
100 _aDodelson, Scott
245 _aModern cosmology [2nd ed.]
_cScott Dodelson and Fabian Schmidt
250 _a2nd ed.
260 _bAcademic press
_c2021
_aLondon
300 _axvi, 494p
520 _aModern Cosmology, Second Edition, provides a detailed introduction to the field of cosmology. Beginning with the smooth, homogeneous universe described by a Friedmann-LemaƮtre-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. The Second Edition now also covers nonlinear structure formation including perturbation theory and simulations. The book concludes with a substantially updated chapter on data analysis. Modern Cosmology, Second Edition, shows how modern observations are rapidly revolutionizing our picture of the universe, and supplies readers with all the tools needed to work in cosmology.
650 _aCosmology
700 _aSchmidt, Fabian
942 _cBK
_01
999 _c565693
_d565693