All extremal instantons in Einstein-Maxwell-dilaton-axion theory

被引:6
|
作者
Azreg-Ainou, Mustapha [1 ]
Clement, Gerard [2 ]
Gal'tsov, Dmitri V. [3 ]
机构
[1] Baskent Univ, Dept Math, TR-06490 Ankara, Turkey
[2] Lab Phys Theor LAPTH CNRS, F-74941 Annecy Le Vieux, France
[3] Moscow MV Lomonosov State Univ, Dept Theoret Phys, Moscow 119899, Russia
来源
PHYSICAL REVIEW D | 2011年 / 84卷 / 10期
关键词
GRAVITATIONAL INSTANTONS; WORMHOLE SOLUTIONS; INTEGRATION; SYMMETRIES; UNIVERSES; TOPOLOGY; SOLITONS; DUALITY; ENTROPY; METRICS;
D O I
10.1103/PhysRevD.84.104042
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We construct explicitly all extremal instanton solutions to N = 4, D = 4 supergravity truncated to one vector field (Einstein-Maxwell-dilaton-axion theory). These correspond to null geodesics of the target space of the sigma-model G/H Sp(4, R)/GL(2, R) obtained by compactification of four-dimensional Euclidean Einstein-Maxwell-dilaton-axion on a circle. They satisfy a no-force condition in terms of the asymptotic charges and part of them (corresponding to nilpotent orbits of the Sp(4, R) U-duality) are presumably supersymmetric. The space of finite action solutions is found to be unexpectedly large and includes, besides the Euclidean versions of known Lorentzian solutions, a number of new asymptotically locally flat instantons endowed with electric, magnetic, dilaton and axion charges. We also describe new classes of charged asymptotically locally Euclidean instantons as well as some exceptional solutions. Our classification scheme is based on the algebraic classification of matrix generators according to their rank, according to the nature of the charge vectors, and according to the number of independent harmonic functions with unequal charges. Besides the nilpotent orbits of G, we find solutions which satisfy the asymptotic no-force condition, but are not supersymmetric. The renormalized on-shell action for instantons is calculated using the method of matched background subtraction.
引用
收藏
页数:30
相关论文
共 50 条
  • [21] Effect of the dilaton field and plasma medium on deflection angle by black holes in Einstein-Maxwell-dilaton-axion theory
    Javed, W.
    Babar, R.
    Ovgun, A.
    [J]. PHYSICAL REVIEW D, 2019, 100 (10)
  • [22] Power law of shear viscosity in Einstein-Maxwell-Dilaton-Axion model
    Ling, Yi
    Xian, Zhuoyu
    Zhou, Zhenhua
    [J]. CHINESE PHYSICS C, 2017, 41 (02)
  • [23] Bound on Lyapunov exponent in Einstein-Maxwell-Dilaton-Axion black holes
    虞成业
    陈德友
    高钏泓
    [J]. Chinese Physics C, 2022, 46 (12) : 316 - 324
  • [24] Holographic dual of linear dilaton black hole in Einstein-Maxwell-dilaton-axion gravity
    Li, Ran
    Ren, Ji-Rong
    [J]. JOURNAL OF HIGH ENERGY PHYSICS, 2010, (09):
  • [25] Quantum tunnelling radiation of Einstein-Maxwell-Dilaton-Axion black hole
    Yang, SZ
    Jiang, QQ
    Li, HL
    [J]. CHINESE PHYSICS, 2005, 14 (12): : 2411 - 2414
  • [26] Bound on Lyapunov exponent in Einstein-Maxwell-Dilaton-Axion black holes*
    Yu, Chengye
    Chen, Deyou
    Gao, Chuanhong
    [J]. CHINESE PHYSICS C, 2022, 46 (12)
  • [27] Holographic dual of linear dilaton black hole in Einstein-Maxwell-dilaton-axion gravity
    Ran Li
    Ji-Rong Ren
    [J]. Journal of High Energy Physics, 2010
  • [28] Power law of shear viscosity in Einstein-Maxwell-Dilaton-Axion model
    凌意
    冼卓宇
    周振华
    [J]. Chinese Physics C, 2017, 41 (02) : 66 - 75
  • [29] U(1,1)-Invariant Generation of Charges for Einstein-Maxwell-Dilaton-Axion Theory
    Oleg Kechkin
    Maria Yurova
    [J]. General Relativity and Gravitation, 1997, 29 : 1283 - 1293
  • [30] Analytic solutions of the geodesic equation for Einstein-Maxwell-dilaton-axion black holes
    Flathmann, Kai
    Grunau, Saskia
    [J]. PHYSICAL REVIEW D, 2015, 92 (10):