Small orbits

被引:37
作者
Borsten, L. [1 ,2 ]
Duff, M. J. [3 ]
Ferrara, S. [4 ,5 ,6 ]
Marrani, A. [4 ]
Rubens, W. [3 ]
机构
[1] Univ Turin, Sez Torino, Ist Nazl Fis Nucl, I-10125 Turin, Italy
[2] Univ Turin, Dipartimento Fis Teor, I-10125 Turin, Italy
[3] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2AZ, England
[4] CERN, Theory Unit, Dept Phys, CH-1211 Geneva 23, Switzerland
[5] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy
[6] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
来源
PHYSICAL REVIEW D | 2012年 / 85卷 / 08期
关键词
MAXWELL-EINSTEIN SUPERGRAVITY; EXTREMAL BLACK-HOLES; EXCEPTIONAL GROUPS; VECTOR MULTIPLETS; N=2 SUPERGRAVITY; II SUPERSTRINGS; CENTRAL CHARGES; BPS STATES; U-DUALITY; ATTRACTORS;
D O I
10.1103/PhysRevD.85.086002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study both the large and small U-duality charge orbits of extremal black holes appearing in D = 5 and D = 4 Maxwell-Einstein supergravity theories with symmetric scalar manifolds. We exploit a formalism based on cubic Jordan algebras and their associated Freudenthal triple systems, in order to derive the minimal charge representatives, their stabilizers and the associated "moduli spaces." After recalling N = 8 maximal supergravity, we consider N = 2 and N = 4 theories coupled to an arbitrary number of vector multiplets, as well as N = 2 magic, STU, ST2 and T-3 models. While the STU model may be considered as part of the general N = 2 sequence, albeit with an additional triality symmetry, the ST2 and T-3 models demand a separate treatment, since their representative Jordan algebras are Euclidean or only admit nonzero elements of rank 3, respectively. Finally, we also consider minimally coupled N = 2, matter-coupled N = 3, and pure N = 5 theories.
引用
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页数:27
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