27,99 €
inkl. MwSt.
Versandfertig in 6-10 Tagen
14 °P sammeln
Andere Kunden interessierten sich auch für
![Schwarzschild Coordinates]( "Schwarzschild Coordinates")
Schwarzschild Coordinates27,99 €![El problema de tres cuerpos bajo el potencial de Schwarzschild]( "El problema de tres cuerpos bajo el potencial de Schwarzschild")
El problema de tres cuerpos bajo el potencial de Schwarzschild38,99 €![Word Metric]( "Word Metric")
Word Metric23,99 €![Kerr Newman Metric]( "Kerr Newman Metric")
Kerr Newman Metric31,99 €![Wasserstein Metric]( "Wasserstein Metric")
Wasserstein Metric23,99 €![Discrete Mathematics with Applications, Metric Edition]( "Discrete Mathematics with Applications, Metric Edition")
Discrete Mathematics with Applications, Metric Edition66,99 €![Theory of Sets, Groups, Rings, Fields,Integral Domains, Vector Spaces, Metric Spaces and Topoloical Spaces]( "Theory of Sets, Groups, Rings, Fields,Integral Domains, Vector Spaces, Metric Spaces and Topoloical Spaces")
Theory of Sets, Groups, Rings, Fields,Integral Domains, Vector Spaces, Metric Spaces and Topoloical Spaces40,99 €
High Quality Content by WIKIPEDIA articles! In Einstein's theory of general relativity, the Schwarzschild solution (or the Schwarzschild vacuum) describes the gravitational field outside a spherical, non-rotating mass such as a (non-rotating) star, planet, or black hole. It is also a good approximation to the gravitational field of a slowly rotating body like the Earth or Sun. The cosmological constant is assumed to equal zero. In the theory of Lorentzian manifolds, spherically symmetric spacetimes admit a family of nested round spheres. In such a spacetime, a particularly important kind of coordinate chart is the Schwarzschild chart, a kind of polar spherical coordinate chart on a static and spherically symmetric spacetime, which is adapted to these nested round spheres. The defining characteristic of Schwarzschild chart is that the radial coordinate possesses a natural geometric interpretation in terms of the surface area and Gaussian curvature of each sphere. However, radial distances and angles are not accurately represented.