Structure formation in the universe

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Structure formation in the universe / T. Padmanabhan

資料種別:: 図書
出版情報:: Cambridge ; New York : Cambridge University Press, 1993
形態:: xvi, 483 p. ; 25 cm
著者名:: Padmanabhan, T. (Thanu), 1957- <DA00290272>
ISBN:: 9780521414487 [0521414482] (: hbk)
9780521424868 [0521424860] (: pbk)
書誌ID:: BA19830120

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注記:

Includes bibliographical references and index

主題:

Astrophysics; Cosmology

言語:

英語

目次情報:

Preface

The smooth universe / Part 1：

Introducing the universe / 1：

Introduction / 1.1：

Existence of large scale structures / 1.2：

Stars / 1.3：

Galaxies / 1.4：

Models for galaxies / 1.5：

Distribution of matter / 1.6：

Expansion of the universe / 1.7：

Quasars / 1.8：

Radiation in the universe / 1.9：

Determination of extragalactic distances / 1.10：

Age of various structures / 1.11：

Exercises

The Friedmann model / 2：

Kinematic properties of the Friedmann universe / 2.1：

Dynamics of the Friedmann model / 2.4：

Radiative processes in the expanding universe / 2.5：

The Hubble radius / 2.6：

Thermal history of the universe / 3：

Distribution functions in the early universe / 3.1：

Relic background of relativistic particles / 3.3：

Relic background of wimps / 3.4：

Synthesis of light nuclei / 3.5：

Decoupling of matter and radiation / 3.6：

The clumpy universe / Part 2：

Linear theory of perturbations / 4：

Suppression and growth of inhomogeneities / 4.1：

The linear perturbation theory / 4.3：

Gravitational instability in the relativistic case / 4.4：

Solutions to the Newtonian perturbation equation / 4.5：

Dissipation in dark matter and baryons / 4.6：

The processed final spectrum / 4.7：

Statistical properties / 5：

Probability functionals / 5.1：

Gaussian probability functional / 5.3：

Spatial averages and filter functions / 5.4：

Normalization of the fluctuation spectrum / 5.5：

The time evolution of the correlation function / 5.6：

Correlation of high density regions / 5.7：

Mass functions / 5.8：

Microwave background radiation / 6：

Processes leading to distortions in the MBR / 6.1：

Propagation of light in a perturbed universe / 6.3：

Anisotropy due to variations in the potential / 6.4：

Anisotropies due to peculiar velocities / 6.5：

Intrinsic anisotropies / 6.6：

Damping of the anisotropies / 6.7：

Spectral distortions due to the ionized gas / 6.8：

Velocity fields / 7：

Large scale velocity fields / 7.1：

Theoretical constraints on peculiar velocities / 7.3：

Towards a more complete picture / Part 3：

The nonlinear evolution / 8：

Spherical model for the nonlinear collapse / 8.1：

Scaling laws / 8.3：

The masses of galaxies / 8.4：

Zeldovich approximation / 8.5：

The adhesion model / 8.6：

The angular momentum of galaxies / 8.7：

Formation of disc galaxies / 8.8：

Formation of elliptical galaxies / 8.9：

Nonlinear evolution using N-body simulations / 8.10：

High redshift objects / 9：

Primeval galaxies / 9.1：

Quasars and galaxy formation / 9.3：

Absorption spectra of quasars / 9.4：

High redshift radio galaxies / 9.5：

The origin of perturbations / 10：

The concept of inflation / 10.1：

The epicycles of inflation / 10.3：

Origin of density perturbations / 10.4：

Cosmic strings / 10.5：

Dark matter / 11：

Observational evidence for dark matter / 11.1：

Nature of dark matter / 11.3：

Massive neutrinos / 11.4：

Axions / 11.5：

Cosmological constant as dark matter / 11.6：

Epilogue / 12：

Structure formation - an appraisal / 12.1：

Aspects of general relativity / Appendix A：

Aspects of field theory / Appendix B：

COBE results and implications / Appendix C：

Notes and references

Some useful numbers

Index

Preface

The smooth universe / Part 1：

Introducing the universe / 1：

Introduction / 1.1：

Existence of large scale structures / 1.2：

Stars / 1.3：

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