The Kerr-Schild double copy in Lifshitz spacetime

被引:0
作者
Gökhan Alkaç
Mehmet Kemal Gümüş
Mustafa Tek
机构
[1] Hacettepe University,Physics Engineering Department, Faculty of Engineering
[2] Middle East Technical University,Department of Physics, Faculty of Arts and Sciences
[3] Istanbul Medeniyet University,Department of Physics Engineering, Faculty of Engineering and Natural Sciences
来源
Journal of High Energy Physics | / 2021卷
关键词
Classical Theories of Gravity; Black Holes;
D O I
暂无
中图分类号
学科分类号
摘要
The Kerr-Schild double copy is a map between exact solutions of general relativity and Maxwell’s theory, where the nonlinear nature of general relativity is circumvented by considering solutions in the Kerr-Schild form. In this paper, we give a general formulation, where no simplifying assumption about the background metric is made, and show that the gauge theory source is affected by a curvature term that characterizes the deviation of the background spacetime from a constant curvature spacetime. We demonstrate this effect explicitly by studying gravitational solutions with non-zero cosmological constant. We show that, when the background is flat, the constant charge density filling all space in the gauge theory that has been observed in previous works is a consequence of this curvature term. As an example of a solution with a curved background, we study the Lifshitz black hole with two different matter couplings. The curvature of the background, i.e., the Lifshitz spacetime, again yields a constant charge density; however, unlike the previous examples, it is canceled by the contribution from the matter fields. For one of the matter couplings, there remains no additional non-localized source term, providing an example for a non-vacuum gravity solution corresponding to a vacuum gauge theory solution in arbitrary dimensions.
引用
收藏
相关论文
共 202 条
[1]  
Bern Z(2010) = 2 Phys. Rev. Lett. 105 061602-undefined
[2]  
Carrasco JJM(2010) = 6 Phys. Rev. D 82 065003-undefined
[3]  
Johansson H(2017) = (2 JHEP 04 069-undefined
[4]  
Bern Z(2017) 0) Phys. Rev. D 95 125010-undefined
[5]  
Dennen T(2017) = (4 Phys. Rev. D 96 065009-undefined
[6]  
Huang Y-T(2018) 0) Phys. Rev. D 97 085019-undefined
[7]  
Kiermaier M(2018)undefined Phys. Rev. D 97 105018-undefined
[8]  
Luna A(2018)undefined JHEP 11 162-undefined
[9]  
Goldberger WD(2018)undefined JHEP 11 065-undefined
[10]  
Ridgway AK(2019)undefined Phys. Rev. D 99 024021-undefined