Geodesics in black hole space-times
✍ Scribed by N. A. Sharp
- Publisher
- Springer US
- Year
- 1979
- Tongue
- English
- Weight
- 560 KB
- Volume
- 10
- Category
- Article
- ISSN
- 0001-7701
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## Abstract For both extremal and non‐extremal spherically symmetric black holes in theories with massless scalars and vectors coupled to gravity, we derive a general form of first‐order gradient flow equations, equivalent to the equations of motion. For theories that have a symmetric moduli space
Let (H,h) be a Riemannian manifold and assume f: H-~ (0, oo) is a smooth function. The Lorentzian warped product (a, b) : x H, -oo ~< a < b ~< oo, with metric ds 2 = (\_\_f 2 dt 2) • h is called a standard static space-time. A study is made of geodesic completeness in standard static space-times. Su