| 000 | 01357cam a2200253 a 4500 | ||
|---|---|---|---|
| 003 | GSU | ||
| 005 | 20240819112146.0 | ||
| 008 | 021227s2003 caua b 001 0 eng d | ||
| 020 | _a9780122191411 (hardback) | ||
| 040 |
_cGSU _beng _erda |
||
| 050 | 0 | 0 |
_aQB981 _bDOD |
| 100 | 1 |
_aDodelson, Scott. _eauthor |
|
| 245 | 1 | 0 |
_aModern cosmology / _cScott Dodelson. |
| 260 |
_aSan Diego, California : _bAcademic Press, _c2003. |
||
| 264 | 4 | _c©2003 | |
| 300 |
_axiii, 440 pages. : _billustrations ; _c26 cm. |
||
| 336 |
_atext _2rdacontent |
||
| 337 |
_aunmediated _2rdamedia |
||
| 338 |
_avolume _2rdacarrier |
||
| 504 | _aIncludes bibliographical references (p. 426-434) and index. | ||
| 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 | ||
| 650 | 0 | _aCosmology. | |
| 942 |
_2lcc _cBK _hQB981 _kQB _mDOD _n0 |
||
| 999 |
_c2281 _d2281 |
||