English

FRBs Lensed by Point Masses I. Lens Mass Estimation for Doubly Imaged FRBs

Astrophysics of Galaxies 2021-05-26 v1 High Energy Astrophysical Phenomena

Abstract

Fast radio bursts (FRBs) are bright radio transient events with durations on the order of milliseconds. The majority of FRB sources discovered so far have a single peak, with the exception of a few showing multiple-peaked profiles, the origin of which is unknown. In this work, we show that the strong lensing effect of a point mass or a point mass ++ external shear on a single-peak FRB can produce double peaks (i.e. lensed images). In particular, the leading peak will always be more magnified and hence brighter than the trailing peak for a point-mass lens model, while the point-mass ++ external shear lens model can produce a less magnified leading peak. We find that, for a point-mass lens model, the combination of lens mass MM and redshift zlz_l in the form of M(1+zl)M(1+z_l) can be directly computed from two observables -- the delayed time Δt\Delta t and the flux ratio of the leading peak to the trailing peak RR. For a point-mass ++ external shear lens model, upper and lower limits in M(1+zl)M(1+z_l) can also be obtained from Δt\Delta t and RR for a given external shear strength. In particular, tighter lens mass constraints can be achieved when the observed RR is larger. Lastly, we show the process of constraining lens mass using the observed values of Δt\Delta t and RR of two double-peaked FRB sources, i.e. FRB 121002 and FRB 130729, as references, although the double-peaked profiles are not necessarily caused by strong lensing.

Keywords

Cite

@article{arxiv.2105.05868,
  title  = {FRBs Lensed by Point Masses I. Lens Mass Estimation for Doubly Imaged FRBs},
  author = {Xuechun Chen and Yiping Shu and Wenwen Zheng and Guoliang Li},
  journal= {arXiv preprint arXiv:2105.05868},
  year   = {2021}
}

Comments

11 pages, 5 figures, ApJ in press