Shadow revisiting and weak gravitational lensing with Chern-Simons modification

Understand

Dynamical Chern-Simons (dCS) gravity has been attracting plenty of attentions due to the fact that it is a parity-violating modified theory of gravity that corresponds to a well-posed effective field theory in weak coupling approximation.

• In particular, a rotating black hole in dCS gravity is in contrast to the general relativistic counterparts.
• In this paper, we revisit the shadow of analytical rotating black hole spacetime in dCS modified gravity, based on which we study the shadow observables, discuss the constraint on the model parameters from the Event Horizon Telescope (EHT) observations, and analyze the real part of quasi-normal modes (QNMs) in the eikonal limit.
• In addition, we explore the deflection angle in weak gravitational field limit with the use of Gauss-Bonnet theorem.