- 演講或講座
- 物理研究所
- 地點
物理所5樓第一會議室
- 演講人姓名
Dr. Antonio Enea Romano (Instituto de Fisica, Universidad de Antioquia)
- 活動狀態
確定
- 活動網址
https://www.phys.sinica.edu.tw/lecture_detail.php?id=3066&eng=T
Abstract
Gravitational wave (GW) astronomy has opened a new window on the Universe, allowing to obtain constraints on dark energy and gravity independent from other electromagnetic waves observations, such as large scale structure (LSS).
For the purpose of investigating the consistency between different observations the effective field theory (EFT) of dark energy is a useful tool, allowing to derive model and parametrization independent consistency relations (CR) between the effective gravitational constant, the slip parameter, the gravitational and electromagnetic luminosity (EM) distance, the speed of GWs and the sound speed. We test the constant brading CR, which is also satisfied by general relativity, by comparing for the first time the constraints obtained from LSS observations with those from GW events with and without electromagnetic counterparts, confirming the validity of the CR at the current level of experimental uncertainty.
The event GW170817 and its electromagnetic counterpart provides a constraint of the effective gravitational constant with an accuracy comparable with LSS constraints, while the analysis of GW events without electromagnetic counterpart are consistent, but do not have a constraining power comparable to LSS observations.
We conclude by considering the prospect of testing the scale and polarization dependence of the CR with future observations.