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Self-modulation of fast radio bursts.

Authors :
Sobacchi, Emanuele
Lyubarsky, Yuri
Beloborodov, Andrei M
Sironi, Lorenzo
Source :
Monthly Notices of the Royal Astronomical Society; Jan2021, Vol. 500 Issue 1, p272-281, 10p
Publication Year :
2021

Abstract

Fast radio bursts (FRBs) are extreme astrophysical phenomena entering the realm of non-linear optics, a field developed in laser physics. A classical non-linear effect is self-modulation. We examine the propagation of FRBs through the circumburst environment using the idealized setup of a monochromatic linearly polarized GHz wave propagating through a uniform plasma slab of density N at distance R from the source. We find that self-modulation occurs if the slab is located within a critical radius R <subscript>crit</subscript> ∼ 10<superscript>17</superscript>(N /10<superscript>2</superscript> cm<superscript>−3</superscript>)(L /10<superscript>42</superscript> erg s<superscript>−1</superscript>) cm, where L is the isotropic equivalent of the FRB luminosity. Self-modulation breaks the burst into pancakes transverse to the radial direction. When R ≲ R <subscript>crit</subscript>, the transverse size of the pancakes is smaller than the Fresnel scale. The pancakes are strongly diffracted as the burst exits the slab, and interference between the pancakes produces a frequency modulation of the observed intensity with a sub-GHz bandwidth. When R ∼ R <subscript>crit</subscript>, the transverse size of the pancakes becomes comparable with the Fresnel scale, and the effect of diffraction is weaker. The observed intensity is modulated on a time-scale of 10 µm, which corresponds to the radial width of the pancakes. Our results suggest that self-modulation may cause the temporal and frequency structure observed in FRBs. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00358711
Volume :
500
Issue :
1
Database :
Complementary Index
Journal :
Monthly Notices of the Royal Astronomical Society
Publication Type :
Academic Journal
Accession number :
147399695
Full Text :
https://doi.org/10.1093/mnras/staa3248