The Wahlquist exterior: Second-order analysis

Classical and Quantum Gravity

Volumn 23, Issue 18, 2006, Pages 5603-5623

  Sarnobat, P ^a   Hoenselaers, C A ^a  

^a LOUGHBOROUGH UNIVERSITY   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33748095954     PISSN: 02649381     EISSN: 13616382     Source Type: Journal    
DOI: 10.1088/0264-9381/23/18/007     Document Type: Article

References (7)

1. Neugebauer G and Meinel R 1995 General relativistic gravitational field of a rigidly rotating disk of dust: solution in terms of ultraelliptic functions Phys. Rev. Lett. 75 3046
2. Hartle J B and Thorne K S 1968 Slowly rotating relativistic stars. II. Models for neutron stars and supermassive stars Astrophys. J. 153 802-34
3. Sato H and Tomimatsu A 1973 Gravitational field of slowly rotating deformed masses Prog. Theor. Phys. 49 790
4. Bradley M, Fodor G, Marklund M and Perjes Z 2000 The Wahlquist metric cannot describe an isolated rotating body Class. Quantum Grav. 17 351-9 (Preprint gr-qc/9910001)
5. Hoenselaers C A 1994 On the Wahlquist solution Proc. 4th Monash General Relativity Workshop (Department of Mathematics, Monash University, Victoria, Australia, 12-14 July 1993) pp 53-8 (Note the misprint in the equation for the interior Ernst potential)
6. Islam J N 1985 Rotating Fields in General Relativity (Cambridge: Cambridge University Press) pp 44-5
7. Hoenselaers C A and Sarnobat P 2006 Slowly rotating limits of the Wahlquist solution Gen. Relativ. Gravit. at press