Strong gravitational lensing by Bardeen black holes in 4D EGB gravity: constraints from supermassive black holes
arXiv:2203.00957
Abstract
Observation indicates that many nearby galaxies host supermassive central black holes. Modelling Bardeen models in four-dimensional Einstein-Gauss-Bonnet (4D EGB) gravity, with additional parameters and charge , as central black holes in various galaxies, we investigate gravitational lensing properties in strong deflection limits. Interestingly, the spherical photon orbit radius , the critical impact parameter , the lensing coefficient , the deflection angle , angular position are decreasing with and whereas the other lensing coefficient and angular separation have opposite behaviour. Taking the supermassive black holes Sgr A* and M87* as the lens, we also compare observable signatures of 4D EGB Bardeen black holes with those of the Schwarzschild black holes. The angular position for Sgr A* (23.1853, \; 25.56427) as, whereas for M87* it is ( 17.941,\; 19.7819) as. Further, the angular separation , which is an increasing function of and for Sgr A* and M87* differs significantly, respectively, in (0.031997,0.14895) as and (0.0247, 0.1152) as. The deviations of the lensing observables and for 4D EGB Bardeen black hole () from the Schwarzschild black hole, respectively, can reach up to as and as for Sgr A* , as and as for M87*. On the other hand, the relative magnification (4.65751,\; 6.82173). Considering twenty-two massive central black holes as lens, we also estimate the time delay between the first and second relativistic image to find that, e.g., the time delay for Sgr A* and M87*, respectively, can reach ~min and ~min.
14 pages, 13 figures, 4 tables, references updated