Investigating the Dainotti Relation in Gamma-Ray Bursts through Multipolar Electromagnetic Radiation
Emre S. Yorgancioglu, Daban Mohammed Saeed, Rahim Moradi, and Yu Wang

TL;DR
This paper proposes that multipolar magnetic fields in magnetars can explain the Dainotti relation in gamma-ray burst afterglows, accounting for observed diversity and linking luminosity and plateau duration.
Contribution
It introduces a multipolar magnetic field model for magnetars as a physical basis for the Dainotti relation, extending beyond traditional dipole models.
Findings
Multipolar fields can reproduce the slope and normalization of the Dainotti relation.
The model explains the diversity of afterglow decay indices in GRBs.
Higher order multipoles account for the range of plateau energies.
Abstract
The Dainotti relation empirically connects the isotropic plateau luminosity () in gamma-ray bursts (GRBs) X-ray afterglows to the rest-frame time at which the plateau ends (), enabling both the standardization of GRBs and their use as cosmological probes. However, the precise physical mechanisms underlying this correlation remain an active area of research. Although magnetars, highly magnetized neutron stars, have been proposed as central engines powering GRB afterglows, traditional dipole spin-down radiation models fail to account for the full diversity of observed behaviors. This limitation necessitates a more comprehensive framework. We propose that multipolar magnetic field emissions from magnetars offer a plausible explanation for the Dainotti relation. Unlike simple dipole fields, higher-order multipolar configurations enable more complex energy dissipation processes.…
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Taxonomy
TopicsGamma-ray bursts and supernovae
