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Description

Here, we analyze the graphs and figures presented in Laha et al. (2022) and compare their slopes to our figures. Laha et al. (2022) includes two graphs, one that shows a comparison between radio fluence vs. x-ray fluence and radio energy vs. x-ray energy. In these graphs, the slopes are anywhere from 3.3e-14 to 2e-5, which are much less than unity. Our figures are consistent with these values, also providing slopes anywhere between the same range. Strong limits on this ratio between radio and x-ray energetics can either support the magnetar progenitor model, or completely dismiss it. Since we found slopes much less than unity, our calculations strongly support the magnetar progenitor model for the 22 FRBs in this work.

Publisher Location

Las Vegas (Nev.)

Publication Date

12-9-2022

Publisher

University of Nevada, Las Vegas

Language

English

Controlled Subject

Solar radio bursts; X-ray spectroscopy

Disciplines

Instrumentation | Stars, Interstellar Medium and the Galaxy

File Format

pdf

File Size

1000 KB

Comments

Faculty Mentor: Bing Zhang

Rights

IN COPYRIGHT. For more information about this rights statement, please visit http://rightsstatements.org/vocab/InC/1.0/

The Analysis of Radio and X-Ray Energetics of Fast Radio Bursts


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