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Synopsis
The origin and evolution of the primordial perturbation is the key to understanding structure formation in the earliest stages of the Universe. It carries clues to the types of physical phenomena active in that extreme high-density environment. Through its evolution, generating first the observed cosmic microwave background anisotropies and later the distribution of galaxies and dark matter in the Universe, it probes the properties and dynamics of the present Universe. This graduate-level textbook gives a thorough account of theoretical cosmology and perturbations in the early Universe, describing their observational consequences and showing how to relate such observations to primordial physical processes, particularly cosmological inflation. With ambitious observational programmes complementing ever-increasing sophistication in theoretical modelling, cosmological studies will remain at the cutting edge of astrophysical studies for the foreseeable future.
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About the Authors
David H. Lyth is Professor of Particle Astrophysics in the Physics Department at Lancaster University.
Andrew R. Liddle is Professor of Astrophysics in the Department of Physics and Astronomy at the University of Sussex.
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The Primordial Density Perturbation: Cosmology, Inflation and the Origin of Structure
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Cambridge University Press, 2009
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The Primordial Density Perturbation
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The Primordial Density Perturbation: Cosmology, Inflation and the Origin of Structure
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ISBN 10: 052182849X
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The Primordial Density Perturbation
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The Primordial Density Perturbation: Cosmology, Inflation and the Origin of Structure
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ISBN 13: 9780521828499
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The Primordial Density Perturbation: Cosmology, Inflation and the Origin of Structure
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The Primordial Density Perturbation (Hardcover)
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Hardcover. Condition: new. Hardcover. The origin and evolution of the primordial perturbation is the key to understanding structure formation in the earliest stages of the Universe. It carries clues to the types of physical phenomena active in that extreme high-density environment. Through its evolution, generating first the observed cosmic microwave background anisotropies and later the distribution of galaxies and dark matter in the Universe, it probes the properties and dynamics of the present Universe. This graduate-level textbook gives a thorough account of theoretical cosmology and perturbations in the early Universe, describing their observational consequences and showing how to relate such observations to primordial physical processes, particularly cosmological inflation. With ambitious observational programmes complementing ever-increasing sophistication in theoretical modelling, cosmological studies will remain at the cutting edge of astrophysical studies for the foreseeable future. The origin and evolution of the primordial perturbation is key to understanding structure formation in the earliest stages of the Universe. Giving a thorough account of theoretical cosmology and perturbations in the early Universe, this graduate-level textbook describes their observational consequences and how such observations relate to primordial physical processes. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability. Seller Inventory # 9780521828499
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The Primordial Density Perturbation: Cosmology, Inflation and the Origin of Structure
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Cambridge University Press, 2009
ISBN 10: 052182849X
ISBN 13: 9780521828499
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The Primordial Density Perturbation: Cosmology, Inflation and the Origin of Structure
Published by
Cambridge University Press, 2009
ISBN 10: 052182849X
ISBN 13: 9780521828499
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