Properties of the instantaneous ergo surface of a Kerr black hole

Classical and Quantum Gravity

Volumn 18, Issue 7, 2001, Pages 1319-1331

  Pelavas, Nicos ^a   Neary, Nicholas ^a   Lake, Kayll ^a  

^a QUEEN S UNIVERSITY   (Canada)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0035531175     PISSN: 02649381     EISSN: None     Source Type: Journal    
DOI: 10.1088/0264-9381/18/7/314     Document Type: Article

References (15)

1. See http://grtensor.phy.queensu.ca/ergo/
2. See, for example, Frolov V P and Novikov I D 1998 Black Hole Physics: Basic Concepts and New Developments (Dordrecht: Kluwer)
3. See, for example, d'Inverno R 1992 Introducing Einstein's Relativity (Oxford: Oxford University Press)
4. See, for example, Hawking S W and Ellis G F 1975 The Large Scale Structure of Space-Time (Cambridge: Cambridge University Press)
5. See, for example, Misner C W, Wheeler J A and Thorne K S 1973 Gravitation (San Fransisco: Freeman)
6. See, for example, Wald R M 1984 General Relativity (Chicago, Il: University of Chicago Press)
7. Pickett C A and Zund J D 2000 Am. J. Phys. 68 746-8
8. Byrd P F and Friedman M D 1954 Handbook of Elliptic Integrals (Berlin: Springer)
9. Kokkotas K D 1988 Gen. Rel. Grav. 20 829-39
10. Smarr L 1973 Phys. Rev. D 7 289-95
11. Sharp N A 1980 Can. J. Phys. 59 688-92
12. Lightman A P, Press W H, Price R H and Teukolsky S A 1975 Problem Book in Relativity and Gravitation (Princeton, NJ: Princeton University Press) problem 17.19
13. Efimov N V 1968 AMS Translations Series 2 66 154-90
14. Do Carmo M P 1976 Differential Geometry of Curves and Surfaces (Eaglewood Cliffs, NJ: Prentice-Hall)
15. GRTensorII is a package which runs within Maple. It is entirely distinct from packages distributed with Maple and must be obtained independently. The GRTensorII software and documentation is available freely from http://grtensor.phy.queensu.ca