2024MNRAS.527.1364S


Query : 2024MNRAS.527.1364S

2024MNRAS.527.1364S - Mon. Not. R. Astron. Soc., 527, 1364-1367 (2024/January-1)

Constraint on the relativistic motion of fast radio bursts based on the maximal electric field.

SHEN J.-Y. and ZOU Y.-C.

Abstract (from CDS):

Fast radio bursts (FRBs) are millisecond radio signals from cosmological distances. As they propagate, FRBs can interact with ambient photons and initiate a quantum cascade that can limit the electric field strength. This paper examines whether some observed bright and brief FRBs may challenge this limit if the source is not relativistic. The size of a static FRB source is estimated as R ∼ ct, where t is the time-scale of the FRB and c denotes the speed of light. But for a relativistic source moving at the Lorentz factor Γ, the size is R ∼ 2Γ2ct. Using an FRB catalogue, we plot the luminosity-duration distribution. Most FRBs fall below the limit for a static source, but two events have higher luminosity and shorter duration. This suggests these bursts may originate from relativistic sources, although more data are needed to confirm this.

Abstract Copyright: © The Author(s) 2023. Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): plasmas - fast radio bursts

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 FRB 191108 rB 01 33 47.0 +31 51 30           ~ 19 0
2 FRB 20221128A rB 07 30.0 -42 30           ~ 6 0
3 FRB 150807 rB 22 41 33.75 -53 05 39.9           ~ 66 0

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