LEADER 03060cam a22003258a 4500 001 991003547869707536 008 080410s2008 nyu 000 0 eng d 020 $a9780198526827 035 $ab13713528-39ule_inst 040 $aDip.to Fisica$beng 082 00$a523.1$222 084 $aLC QB981 084 $a52.9.512 100 1 $aWeinberg, Steven$09971 245 10$aCosmology /$cSteven Weinberg 260 $aNew York :$bOxford University Press,$c2008 300 $axvii, 593 p. :$bill. ;$c26 cm 505 0 $a1. The Expansion of the Universe -- 2. The Cosmic Microwave Radiation Background -- 3. The Early Universe -- 4. Inflation -- 5. General Theory of Small Fluctuations -- 6. Evolution of Cosmological Fluctuations -- 7. Anisotropies in the Microwave Sky -- 8. The Growth of Structure -- 9. Gravitational Lenses -- 10. Inflation as the Origin of Cosmological Fluctuations -- A. Some Useful Numbers -- B. Review of General Relativity -- C. Energy Transfer between Radiation and Electrons -- D. The Ergodic Theorem -- E. Gaussian Distributions -- F. Newtonian Cosmology -- G. Photon Polarization -- H. The Relativistic Boltzmann Equation. 520 1 $a"This book is unique in the detailed, self-contained, and comprehensive treatment that it gives to the ideas and formulas that are used and tested in modern cosmological research. It divides into two parts, each of which provides enough material for a one-semester graduate course. The first part deals chiefly with the isotropic and homogeneous average universe; the second part concentrates on the departures from the average universe. Throughout the book the author presents detailed analytic calculations of cosmological phenomena, rather than just report results obtained elsewhere by numerical computation. The book is up to date, and gives detailed accounts of topics such as recombination, microwave background polarization, leptogenesis, gravitational lensing, structure formation, and multifield inflation, that are often treated superficially if at all in treatises on cosmology. Copious references to current research literature are supplied. 520 8 $aAppendices include a brief introduction to general relativity, and a detailed derivation of the Boltzmann equation for photons and neutrinos used in calculations of cosmological evolution. Also provided is an assortment of problems."--BOOK JACKET. 650 0$aCosmology 907 $a.b13713528$b10-09-08$c10-04-08 912 $a991003547869707536 945 $aLE006 52.9.51 WEI$g1$i2006000162135$lle006$op$pE57.07$q-$rl$s- $t0$u4$v0$w4$x0$y.i14719691$z10-04-08 945 $aLE006 52.9.51 WEI$g1$i2006000162142$lle006$op$pE57.07$q-$rl$s- $t0$u9$v1$w9$x0$y.i14719708$z10-04-08 945 $aLE006 52.9.51 WEI$g1$i2006000162128$lle006$op$pE57.07$q-$rl$s- $t0$u5$v2$w5$x0$y.i14719721$z10-04-08 945 $aLE006 52.9.51 WEI$g1$i2006000162449$lle006$op$pE56.27$q-$rl$s- $t0$u8$v0$w8$x0$y.i14825193$z10-09-08 996 $aCosmology$9808651 997 $aUNISALENTO 998 $ale006$b10-04-08$cm$da $e-$feng$gnyu$h0$i0