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Self-anisotropizing universe and gravitational waves in Horndeski theory
- Title Self-anisotropizing universe and gravitational waves in Horndeski theory
- Speaker
- Date
- Venue
CAS Key Laboratory of Theoretical Physics | |
Institute of Theoretical Physics | |
Chinese Academy of Sciences | |
Seminar | |
Title 题目 |
Self-anisotropizing universe and gravitational waves in Horndeski theory |
Speaker 报告人 |
Hiroaki Tahara |
Affiliation 所在单位 |
Research Center for the Early Universe, University of Tokyo |
Date 日期 |
2018年11月15日(周四)上午10:00 |
Venue 地点 |
Conference Room 6420, ITP new building |
Abstract 摘要 |
As opposed to Wald’s cosmic no-hair theorem in general relativity, we find that the Horndeski theory admits anisotropic inflationary attractors if the Lagrangian depends cubically on the second derivatives of the scalar field. We name such a solution a self-anisotropizing inflationary universe, because anisotropic inflation can occur without introducing any anisotropic matter fields such as a vector field. Next, we investigate perturbations in homogeneous anisotropic background, and find that speed of gravitational waves depend on direction of its propagation. This investigation reveals, however, that the speed of gravitational waves in some directions diverges in the self-anisotropizing inflationary background and it suggests unfitness for representing our present universe. On the other hand, it is also revealed that as long as our universe is anisotropic, speed of gravitational waves can have angular dependence. Such a nature is not seen in general relativity, and it shows us abundance of phenomenology in Horndeski theory. |
Contact Person 所内联系人 |
Rong-Gen Cai |