Книга Partial Differential Equations in General Relativity Alan Rendall

Partial Differential Equations in General Relativity

Автор: Alan Rendall
Език: Английски език
Корици: С меки корици
Издател: Oxford University Press
Наличност: Външен склад
Изпращаме след 10-18 дни
75.85 148.34 лв
A graduate level text on a subject which brings together several areas of mathematics and physics: p...

Информация за книгата

Автор
Език
Английски език
Корици
Книга - С меки корици
Издадена
2008
страници
296
EAN
9780199215416
ISBN
0199215413
Enbook ID
04034262
Издател
Теглоt
450
Размери
157 x 232 x 18

Пълно описание

A graduate level text on a subject which brings together several areas of mathematics and physics: partial differential equations, differential geometry and general relativity. It explains the basics of the theory of partial differential equations in a form accessible to physicists and the basics of general relativity in a form accessible to mathematicians. In recent years the theory of partial differential equations has come to play an ever more important role in research on general relativity. This is partly due to the growth of the field of numerical relativity, stimulated in turn by work on gravitational wave detection, but also due to an increased interest in general relativity among pure mathematicians working in the areas of partial differential equations and Riemannian geometry, who have realized the exceptional richness of the interactions between geometry and analysis which arise. This book provides the background for those wishing to learn about these topics.It treats key themes in general relativity including matter models and symmetry classes and gives an introduction to relevant aspects of the most important classes of partial differential equations, including ordinary differential equations, and material on functional analysis. These elements are brought together to discuss a variety of important examples in the field of mathematical relativity, including asymptotically flat spacetimes, which are used to describe isolated systems, and spatially compact spacetimes, which are of importance in cosmology.

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