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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
File Size
1000 KB
Recommended Citation
Huerta, Emily, "The Analysis of Radio and X-Ray Energetics of Fast Radio Bursts" (2022). Undergraduate Research Symposium Posters. 145.
https://digitalscholarship.unlv.edu/durep_posters/145
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IN COPYRIGHT. For more information about this rights statement, please visit http://rightsstatements.org/vocab/InC/1.0/
Comments
Faculty Mentor: Bing Zhang