SIMBAD references

2026MNRAS.545f2043C - Mon. Not. R. Astron. Soc., 545, part no 6, 2043 (2026/January-2)

The energy structure function of fast radio bursts supports a stochastic origin model.

CHEN Y.-N., ZHANG Y.-K. and DAI Z.-G.

Abstract (from CDS):

The origin of fast radio bursts (FRBs) has remained a mystery up to now. There are two kinds of process invoking neutron stars as an origin of FRBs, namely inner-driven starquakes and outer-driven collisions with interstellar objects (ISOs). The former origin should exhibit an earthquake-like statistical behaviour, while the latter should show a stochastic process. In this paper, we introduce a new statistical method by making use of the energy structure function of active repeating FRBs and earthquakes. We find that the energy structure function of FRBs exhibits a very different statistical behaviour compared to that of earthquakes. On small time-interval scales, the energy of an earthquake shows a tendency to decay with time interval, and the energy difference of a pair of events increases with time interval. Such a behaviour is not found in FRBs, whose energy function is very similar to that of a stochastic process. Our result shows that repeating FRBs may have an origin process differing from that of earthquakes, i.e. FRBs arise from a series of unrelated events such as collisions of a neutron star with ISOs.

Abstract Copyright: © The Author(s) 2025. Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): methods: statistical - stars: magnetars - fast radio bursts

Simbad objects: 6

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