This book presents a clear and accessible introduction to the theory of cosmological perturbations. This subject is central to modern cosmology, as scalar cosmological perturbations in the early universe are believed to be the seeds from which today's cosmological structures, such as galaxies and clusters of galaxies, originated.
The text begins with an introduction to the fundamentals of Einstein's theory of general relativity and the key elements of the standard cosmological model. The basic ideas of cosmological perturbations and gravitational instability are first developed within a Newtonian framework, providing an intuitive foundation for the fully relativistic treatment presented in later chapters. The final part of the book explores specific models and generalizations of the standard model, including non-adiabatic pressure perturbations, non-standard dark matter and dark energy models, as well as dissipative phenomena.
Providing a concise yet wide-ranging treatment of the subject, this book serves as an ideal entry point for graduate students and researchers who wish to build the foundations necessary to explore cosmological perturbation theory in greater depth.
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Hardcover. Etat : new. Hardcover. This book presents a clear and accessible introduction to the theory of cosmological perturbations. This subject is central to modern cosmology, as scalar cosmological perturbations in the early universe are believed to be the seeds from which today's cosmological structures, such as galaxies and clusters of galaxies, originated. The text begins with an introduction to the fundamentals of Einstein's theory of general relativity and the key elements of the standard cosmological model. The basic ideas of cosmological perturbations and gravitational instability are first developed within a Newtonian framework, providing an intuitive foundation for the fully relativistic treatment presented in later chapters. The final part of the book explores specific models and generalizations of the standard model, including non-adiabatic pressure perturbations, non-standard dark matter and dark energy models, as well as dissipative phenomena. Providing a concise yet wide-ranging treatment of the subject, this book serves as an ideal entry point for graduate students and researchers who wish to build the foundations necessary to explore cosmological perturbation theory in greater depth. This item is printed on demand. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. N° de réf. du vendeur 9781800619791
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Hardcover. Etat : new. Hardcover. This book presents a clear and accessible introduction to the theory of cosmological perturbations. This subject is central to modern cosmology, as scalar cosmological perturbations in the early universe are believed to be the seeds from which today's cosmological structures, such as galaxies and clusters of galaxies, originated. The text begins with an introduction to the fundamentals of Einstein's theory of general relativity and the key elements of the standard cosmological model. The basic ideas of cosmological perturbations and gravitational instability are first developed within a Newtonian framework, providing an intuitive foundation for the fully relativistic treatment presented in later chapters. The final part of the book explores specific models and generalizations of the standard model, including non-adiabatic pressure perturbations, non-standard dark matter and dark energy models, as well as dissipative phenomena. Providing a concise yet wide-ranging treatment of the subject, this book serves as an ideal entry point for graduate students and researchers who wish to build the foundations necessary to explore cosmological perturbation theory in greater depth. This item is printed on demand. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability. N° de réf. du vendeur 9781800619791
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Hardcover. Etat : new. Hardcover. This book presents a clear and accessible introduction to the theory of cosmological perturbations. This subject is central to modern cosmology, since scalar cosmological perturbations in the early universe are believed to be the seeds from which today's cosmological structures, such as galaxies and clusters of galaxies, originated.The text begins with an introduction to the fundamentals of Einstein's theory of general relativity and the key elements of the standard cosmological model. The basic ideas of cosmological perturbations and gravitational instability are first developed within a Newtonian framework, providing an intuitive foundation for the fully relativistic treatment presented in later chapters. The final part of the book explores specific models and generalizations of the standard model, including non-adiabatic pressure perturbations, non-standard dark-matter and dark-energy models, as well as dissipative phenomena.Providing a concise yet wide-ranging treatment of the subject, this book serves as an ideal entry point for graduate students and researchers who wish to build the foundations necessary to explore cosmological perturbation theory in greater depth. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability. N° de réf. du vendeur 9781800619791
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Hardcover. Etat : Brand New. 428 pages. 6.00x0.64x9.00 inches. In Stock. N° de réf. du vendeur x-1800619790
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Vendeur : AHA-BUCH GmbH, Einbeck, Allemagne
Buch. Etat : Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - This book presents a clear and accessible introduction to the theory of cosmological perturbations. This subject is central to modern cosmology, as scalar cosmological perturbations in the early universe are believed to be the seeds from which today's cosmological structures, such as galaxies and clusters of galaxies, originated.The text begins with an introduction to the fundamentals of Einstein's theory of general relativity and the key elements of the standard cosmological model. The basic ideas of cosmological perturbations and gravitational instability are first developed within a Newtonian framework, providing an intuitive foundation for the fully relativistic treatment presented in later chapters. The final part of the book explores specific models and generalizations of the standard model, including non-adiabatic pressure perturbations, non-standard dark matter and dark energy models, as well as dissipative phenomena.Providing a concise yet wide-ranging treatment of the subject, this book serves as an ideal entry point for graduate students and researchers who wish to build the foundations necessary to explore cosmological perturbation theory in greater depth. N° de réf. du vendeur 9781800619791
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Buch. Etat : Neu. THEORY OF COSMOLOGICAL PERTURBATIONS, THE | Zimdahl Winfried | Buch | Englisch | 2026 | WSPC (Europe) | EAN 9781800619791 | Verantwortliche Person für die EU: Libri GmbH, Europaallee 1, 36244 Bad Hersfeld, gpsr[at]libri[dot]de | Anbieter: preigu Print on Demand. N° de réf. du vendeur 136937129
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