Non-BPS attractors in 5d and 6d extended supergravity

被引:40
作者
Andrianopoli, L. [2 ,3 ,4 ,5 ]
Ferrara, S. [1 ,3 ,6 ]
Marrani, A. [1 ,2 ]
Trigiante, M. [4 ,5 ]
机构
[1] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy
[2] Museo Storico Fis & Ctr Ric Enrico Fermi, I-00184 Rome, Italy
[3] CERN, Dept Phys, Theory Unit, CH-1211 Geneva 23, Switzerland
[4] Politecn Torino, Dipartimento Fis, I-10129 Turin, Italy
[5] INFN Sez Torino, Turin, Italy
[6] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA USA
关键词
D O I
10.1016/j.nuclphysb.2007.11.025
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We connect the attractor equations of a certain class of N = 2, d = 5 supergravities with their (1, 0), d = 6 counterparts, by relating the moduli space of non-BPS d = 5 black hole/black string attractors; to the moduli space of extremal dyonic black string d = 6 non-BPS attractors. For d = 5 real special symmetric spaces and for N = 4, 6, 8 theories, we explicitly compute the flat directions of the black object potential corresponding to vanishing eigenvalues of its Hessian matrix. In the case N = 4, we study the relation to the (2, 0), d = 6 theory. We finally describe the embedding of the N = 2, d = 5 magic models in N = 8, d = 5 supergravity as well as the interconnection among the corresponding charge orbits. (c) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:428 / 452
页数:25
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