The Structure and Evolution of the UniverseUniversity of Chicago Press, 1983 - 718 pages |
Contents
RELATIVISTIC THEORY OF | 20 |
THE PROPAGATION OF PHOTONS AND NEUTRINOS | 33 |
THE COSMOLOGICAL CONSTANT | 99 |
INTRODUCTION TO PART II | 117 |
THERMODYNAMIC EQUILIBRIUM AT THE BEGINNING | 134 |
Chargeasymmetric Universe | 151 |
THE RADIATIONDOMINATED PLASMA AND | 189 |
INTRODUCTION TO PART III | 237 |
RESEARCH ON PERTURBATIONS USING THE RELIC | 419 |
GRAVITATIONAL WAVES IN COSMOLOGY | 449 |
INTRODUCTION TO PART IV | 477 |
Form | 490 |
THE PHYSICS OF PROCESSES DURING | 511 |
A GENERAL ANALYSIS OF HOMOGENEOUS | 530 |
THE COSMOLOGICAL SINGULARITY | 569 |
PHYSICAL PROCESSES NEAR A SINGULARITY | 581 |
INSTABILITY IN THE HOT MODEL | 265 |
GRAVITATIONAL INSTABILITY IN THE GENERAL | 285 |
STATISTICAL THEORY | 310 |
THE NONLINEAR THEORY OF PERTURBATIONS | 325 |
THEORIES OF GALAXY FORMATION | 350 |
metry of the Elementary Particles | 613 |
| 675 | |
AUTHOR INDEX | 699 |
| 705 | |
Common terms and phrases
adiabatic adiabatic perturbations amplitude angular momentum annihilation antibaryons antimatter approximation assumed baryons bremsstrahlung calculation clusters of galaxies cm³ comoving consider const constant coordinates corresponding cosmological model curve decreases density perturbations depends determined dimensionless distribution electrons energy density entropy entropy perturbations equation equilibrium ergs evolution expansion expression factor finite flux formula frequency Friedmann function given gravitational radiation gravitational waves gravitons grows homogeneous hot Universe Hubble hydrogen inhomogeneity initial interaction ionized isotropic limit magnitude mass matter density motion neutrinos nucleons number density observations obtain Ozernoy parameter particles perturbations photons Planck Planck spectrum plasma present pressure processes quantity quarks quasars radiation radius ratio recombination redshift region result rotation scale scattering shock wave singularity solution sources space spectrum sphere stage stars Sunyaev temperature tensor thermodynamic equilibrium tion unperturbed vector velocity volume vortex theory wave vector wavelength Zel'dovich zero Ωο
Popular passages
Page 695 - Wilson, RW, Penzias, AA, Jefferts, KB, and Solomon, PM 1973, Ap. J. (Letters), 179, L107.