000 | 02689cam a2200313 a 4500 | ||
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001 | 13042958 | ||
003 | ZW-GwMSU | ||
005 | 20221108103111.0 | ||
008 | 021227s2003 caua b 001 0 eng d | ||
020 | _a0122191412 | ||
020 | _a9780122191411 | ||
035 | _a(DLC)13042958 | ||
040 |
_bEnglish _cMSULIB _erda |
||
042 | _alccopycat | ||
050 | 0 | 0 | _aQB981 SCO |
100 | 1 |
_aDodelson, Scott. _eauthor. |
|
245 | 1 | 0 |
_aModern cosmology / _ccreated by Scott Dodelson. |
264 | 1 |
_bElsevier, _c2003. |
|
264 | 4 | _c©2003. | |
300 |
_axiii, 440 pages; _bIllustrations _c24 cm. |
||
336 |
_2rdacontent _atext |
||
337 |
_2rdamedia _aunmediated _bn |
||
338 |
_2rdacarrier _avolume _bnc |
||
504 | _aIncludes bibliographical references and index. | ||
505 | _a1. The Standard Model and Beyond 2. The Smooth, Expanding Universe 3. Beyond Equilibrium 4. The Boltzmann Equations 5. Einstein Equations 6. Initial Conditions 7. Inhomogeneities 8. Anisotropies 9. Probes of Inhomogeneities 10. Weak Lensing and Polarization 11. Analysis A. Solutions to Selected Problems B. Symbols C. Numbers D. Special Functions Bibliography | ||
520 | _aModern Cosmology begins with an introduction to the smooth, homogeneous universe described by a Friedman-Robertson-Walker metric, including careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. From this starting point, the reader is introduced to perturbations about an FRW universe: their evolution with the Einstein-Boltzmann equations, their generation by primordial inflation, and their observational consequences. These consequences include the anisotropy spectrum of the cosmic microwave background (CMB) featuring acoustic peaks and polarization, the matter power spectrum with baryonic wiggles, and their detection via photometric galaxy surveys, redshift distortions, cluster abundances, and weak lensing. The book concludes with a long chapter on data analysis. Modern Cosmology is the first book to explain in detail the structure of the acoustic peaks in the CMB, the E/B decomposition in polarization which may allow for detection of primordial gravity waves, and the modern analysis techniques used on increasingly large cosmological data sets. Readers will gain the tools needed to work in cosmology and learn how modern observations are rapidly revolutionizing our picture of the universe. Provides foundations, calculations, and interpretations which illuminate current thinking in cosmology; covers the major advances in cosmology over the past decade; includes over 100 unique, pedagogical figures" | ||
650 | 0 | _aCosmology. | |
942 |
_2lcc _cB |
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999 |
_c160158 _d160158 |