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  FRBs lensed by point masses I. Lens mass estimation for doubly imaged FRBs

Chen, X., Shu, Y., Zheng, W., & Li, G. (2021). FRBs lensed by point masses I. Lens mass estimation for doubly imaged FRBs. The Astrophysical Journal, 912(2): 134. doi:10.3847/1538-4357/abf119.

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FRBs lensed by point masses I. Lens mass estimation for doubly imaged FRBs.pdf (beliebiger Volltext), 3MB
 
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 Urheber:
Chen, Xuechun, Autor
Shu, Yiping1, Autor           
Zheng, Wenwen, Autor
Li, Guoliang, Autor
Affiliations:
1MPI for Astrophysics, Max Planck Society, ou_159875              

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 Zusammenfassung: 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 M and redshift zl in the form of M(1 + zl) can be directly computed from two observables—the delayed time Δt and the flux ratio of the leading peak to the trailing peak R. For a point-mass + external shear lens model, upper and lower limits in M(1 + zl) can also be obtained from Δt and R for a given external shear strength. In particular, tighter lens mass constraints can be achieved when the observed R is larger. Lastly, we show the process of constraining lens mass using the observed values of Δt and R 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.

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 Datum: 2021-05-13
 Publikationsstatus: Online veröffentlicht
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 Identifikatoren: DOI: 10.3847/1538-4357/abf119
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Titel: The Astrophysical Journal
Genre der Quelle: Zeitschrift
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Ort, Verlag, Ausgabe: Bristol; Vienna : IOP Publishing; IAEA
Seiten: - Band / Heft: 912 (2) Artikelnummer: 134 Start- / Endseite: - Identifikator: ISSN: 0004-637X
CoNE: https://pure.mpg.de/cone/journals/resource/954922828215_3