2019MNRAS.489.5688M


Query : 2019MNRAS.489.5688M

2019MNRAS.489.5688M - Mon. Not. R. Astron. Soc., 489, 5688-5694 (2019/November-2)

Self-trapping as the possible beaming mechanism for FRBs.

MACHABELI G., ROGAVA A. and TEVDORASHVILI B.

Abstract (from CDS):

Enigmatic fast radio bursts (FRBs), still eluding a rational explanation, are astronomical millisecond-scale radio flashes. They are thought to be of an extragalactic origin, with luminosities orders of magnitude larger than any known short time-scale radio transients. Numerous models have been proposed in order to explain these powerful bursts but none of them is commonly accepted; it is not clear which of these scenarios might account for real FRBs. The crucial question remains: what makes FRBs so exceptionally powerful and rare? If the bursts are related to something happening with a star-scale object and its immediate neighbourhood, why do all detected FRB events take place in very distant galaxies and never in our own Galaxy? In this paper we argue that a non-linear phenomenon - self-trapping - providing efficient but very rarely occurring beaming of radio emission towards an observer, coupled with any other, also rare but powerful, phenomenon providing a strong enough initial 'primary' radio burst, may be responsible for the ultra-rare appearance of FRBs.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): radio continuum: transients

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 FRB 170827 rB 00 49 18.66 -65 33 02.3           ~ 46 0
2 NAME FRB 180814.J0422+73 rB 04 22 44.0 +73 39 52           ~ 83 0
3 FRB 20181119D rB 05 31 58.6980 +33 08 52.588           ~ 719 0
4 M 1 SNR 05 34 30.9 +22 00 53           ~ 6193 1
5 FRB 180924 rB 21 44 25.255 -40 54 00.10           ~ 113 0

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