O Sarbach and E Winstanley 2001 Class. Quantum Grav. 18 2125 doi:10.1088/0264-9381/18/11/310
O Sarbach1 and E Winstanley2
Show affiliationsUsing a recently developed perturbation formalism based on curvature quantities, we investigate the linear stability of black holes and solitons with Yang-Mills hair and a negative cosmological constant. We show that those solutions which have no linear instabilities under odd- and even-parity spherically symmetric perturbations remain stable under odd-parity, linear, non-spherically symmetric perturbations.
Issue 11 (7 June 2001)
Received 14 February 2001
O Sarbach and E Winstanley 2001 Class. Quantum Grav. 18 2125
Jean-Pierre Amiet and Stefan Weigert 1999 J. Phys. A: Math. Gen. 32 2777
Jacek Rożynek and Grzegorz Wilk 2009 J. Phys. G: Nucl. Part. Phys. 36 125108
M J Martínez-Pérez et al 2009 Supercond. Sci. Technol. 22 125020
S Graffi and F Unguendoli 1994 J. Phys. A: Math. Gen. 27 4281
Zhang Jia-Guo et al 2009 Chinese Phys. Lett. 26 112901
Y. Sheffer et al 2009 ApJ 701 L63
E V Zolotojabko and V N Kashcheev 1977 J. Phys. C: Solid State Phys. 10 4599
E. Amato and J. Arons 2006 ApJ 653 325
Jafferson K L da Silva et al 2007 J. Phys. A: Math. Theor. 40 F953