TY - JOUR
T1 - Magnetic black holes with higher-order curvature and gauge corrections in even dimensions
AU - Maeda, Hideki
AU - Hassaïne, Mokhtar
AU - Martíneza, Cristián
PY - 2010
Y1 - 2010
N2 - We obtain magnetic black-hole solutions in arbitrary n(≥ 4) even dimensions for an action given by the Einstein-Gauss-Bonnet-Maxwell-λ pieces with the F4 gaugecorrection terms. This action arises in the low energy limit of heterotic string theory with constant dilaton and vanishing higher form fields. The spacetime is assumed to be a warped product M 2 × Κn-2, where Κn-2 is a (n-2)-dimensional Einstein space satisfying a condition on its Weyl tensor, originally considered by Dotti and Gleiser. Under a few reasonable assumptions, we establish the generalized Jebsen-Birkhoff theorem for the magnetic solution in the case where the orbit of the warp factor on Κn-2 is non-null. We prove that such magnetic solutions do not exist in odd dimensions. In contrast, in even dimensions, we obtain an explicit solution in the case where Κn-2 is a product manifold of (n-2)/2 two-dimensional maximally symmetric spaces with the same constant warp factors. In this latter case, we show that the global structure of the spacetime sharply depends on the existence of the gauge-correction terms as well as the number of spacetime dimensions.
AB - We obtain magnetic black-hole solutions in arbitrary n(≥ 4) even dimensions for an action given by the Einstein-Gauss-Bonnet-Maxwell-λ pieces with the F4 gaugecorrection terms. This action arises in the low energy limit of heterotic string theory with constant dilaton and vanishing higher form fields. The spacetime is assumed to be a warped product M 2 × Κn-2, where Κn-2 is a (n-2)-dimensional Einstein space satisfying a condition on its Weyl tensor, originally considered by Dotti and Gleiser. Under a few reasonable assumptions, we establish the generalized Jebsen-Birkhoff theorem for the magnetic solution in the case where the orbit of the warp factor on Κn-2 is non-null. We prove that such magnetic solutions do not exist in odd dimensions. In contrast, in even dimensions, we obtain an explicit solution in the case where Κn-2 is a product manifold of (n-2)/2 two-dimensional maximally symmetric spaces with the same constant warp factors. In this latter case, we show that the global structure of the spacetime sharply depends on the existence of the gauge-correction terms as well as the number of spacetime dimensions.
KW - Black Holes
KW - Black Holes in String Theory
KW - Classical Theories of Gravity
UR - http://www.scopus.com/inward/record.url?scp=79960762598&partnerID=8YFLogxK
U2 - 10.1007/JHEP08(2010)123
DO - 10.1007/JHEP08(2010)123
M3 - Article
AN - SCOPUS:79960762598
SN - 1126-6708
VL - 2010
JO - Journal of High Energy Physics
JF - Journal of High Energy Physics
IS - 8
M1 - 123
ER -