Sudden discharge of young charged magnetars as a new model for FRBs
Marcio G.B. de Avellar, Pedro P.B. Beaklini, S\'ilvia P. Nunes, Pedro, H.R.S. Moraes, Manuel Malheiro

TL;DR
This paper introduces a novel model where sudden discharges of charged young magnetars produce FRBs through curvature radiation, aligning well with observed durations, power, and frequency ranges.
Contribution
It presents a new theoretical framework modeling charged magnetar discharges as the origin of FRBs, incorporating relativistic particle acceleration and magnetic reconnection processes.
Findings
Discharge timescales of several milliseconds match FRB durations.
Total emitted power of 10^{42-43} erg/s aligns with observed FRB energies.
Model parameters are consistent with known magnetar properties.
Abstract
We propose a new model for Fast Radio Bursts (FRBs) based on a sudden discharge of a charged young magnetar, caused by the short falling timescale of oppositely charged particles onto the magnetar. In this scenario, curvature radiation is emitted by particles accelerated at relativistic by the strong electric fields produced by the disconnection and the subsequent reconnection of the magnetic field lines, a process triggered by the sudden discharge. We modeled the magnetars as charged neutron stars in the static approximation using the exterior metric by the Reissner-Nordstr\"om. We also adopted an electrical charge distribution proportional to the mass-energy density, although our results are not strongly sensitive to the specific star charge distribution, only to the total charge. Our calculations show that the discharge and emission timescales are several milliseconds, compatible…
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