The Mathematical Theory of Black Holes

E7948

The Mathematical Theory of Black Holes is a landmark monograph that presents a rigorous, comprehensive treatment of the physics and mathematics underlying black hole solutions in general relativity.


Statements (47)
Predicate Object
instanceOf book
monograph
non-fiction book
academicDiscipline differential geometry
relativistic astrophysics
theoretical physics
author Subrahmanyan Chandrasekhar
covers Kerr metric
Kerr–Newman metric
Penrose diagrams for black hole spacetimes
Reissner–Nordström metric
Schwarzschild metric
horizon structure and surface gravity
perturbations of black hole metrics
radiation from perturbed black holes
describedAs comprehensive monograph on the mathematics of black holes
rigorous treatment of black hole solutions in general relativity
field astrophysics
general relativity
mathematical physics
focusesOn causal structure of spacetime near black holes
classical (non-quantum) black hole theory
exact mathematical formulation of black hole spacetimes
global structure of black hole solutions
genre scientific literature
influenced graduate-level education in general relativity
research in mathematical relativity
intendedAudience advanced students of general relativity
researchers in gravitational physics
language English
mainSubject Einstein field equations
Kerr black hole
Reissner–Nordström black hole
Schwarzschild black hole
black holes
event horizons
exact solutions in general relativity
geodesics in black hole spacetimes
gravitational collapse
horizons and singularities
perturbation theory in general relativity
quasi-normal modes
stability of black hole solutions
notableFor mathematical rigor
systematic treatment of classical black hole solutions
timePeriodDescribed classical general relativity era
workType technical reference text

Referenced by (1)
Subject (surface form when different) Predicate
Subrahmanyan Chandrasekhar
notableWork

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