Peter Breitenlohner and D H Tchrakian 2009 Class. Quantum Grav. 26 145008 doi:10.1088/0264-9381/26/14/145008
Peter Breitenlohner1 and D H Tchrakian2,3
Show affiliationsWe have constructed, numerically, both regular and black hole static solutions to the simplest possible gravitating Yang–Mills–Higgs (YMH) systems in 4p spacetime dimensions. The YMH systems consist of 2p th power curvature fields without a Higgs potential. The gravitational systems consist of the 'Ricci scalar' of the pth power of the Riemann curvature. In 4 spacetime dimensions this is the usual Einstein–YMH (EYMH) system studied in [1, 2], whose qualitative results we emulate exactly.
04.50.-h Higher-dimensional gravity and other theories of gravity
53C21 Methods of Riemannian geometry, including PDE methods; curvature restrictions (See also 58J60)
81T13 Yang-Mills and other gauge theories (See also 53C07, 58E15)
Issue 14 (21 July 2009)
Received 9 April 2009, in final form 29 May 2009
Published 25 June 2009
Peter Breitenlohner and D H Tchrakian 2009 Class. Quantum Grav. 26 145008
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The KLOE collaboration et al JHEP12(2007)105
Konstanze Jaehne et al 2008 New J. Phys. 10 095019
L Fernández-Jambrina and R Lazkoz 2007 J. Phys.: Conf. Ser. 66 012015
K P Nayak and K Hakuta 2008 New J. Phys. 10 053003
E Marinari and V V Kerrebroeck 2008 J. Phys.: Conf. Ser. 95 012014
R Goebel et al 2009 Metrologia 46 01012