2017MNRAS.469L..39K


Query : 2017MNRAS.469L..39K

2017MNRAS.469L..39K - Mon. Not. R. Astron. Soc., 469, L39-L42 (2017/July-3)

Fast radio bursts as pulsar lightning.

KATZ J.I.

Abstract (from CDS):

There are striking phenomenological similarities between fast radio bursts (FRBs) and lightning in the Earth's and planetary atmospheres. Both have very low duty factors, <=10–8-10–5 for FRBs and (very roughly) ∼10–4 for the main return strokes in an active thundercloud. Lightning occurs in an electrified insulating atmosphere when a conducting path is created by and permits current flow. FRBs may occur in neutron star magnetospheres whose plasma is believed to be divided by vacuum gaps. Vacuum is a perfect insulator unless electric fields are sufficient for electron-positron pair production by curvature radiation, a high-energy analogue of electrostatic breakdown in an insulating gas. FRB may be 'electrars' powered by the release of stored electrostatic energy, counterparts to soft gamma repeaters powered by the release of stored magnetostatic energy (magnetars). This frees pulsar FRB models from the constraint that their power not exceeds the instantaneous spin-down power. Energetic constraints imply that the sources of more energetic FRBs have shorter spin-down lifetimes, perhaps even less than the 3 yr over which FRB 121102 has been observed to repeat.

Abstract Copyright: © 2017 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): pulsars: general - radio continuum: general - radio continuum: general

Simbad objects: 2

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Number of rows : 2
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 20181119D rB 05 31 58.6980 +33 08 52.588           ~ 933 0
2 NAME FRB 121102 host galaxy G 05 31 58.698 +33 08 52.60           ~ 35 0

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