Magnetars in Binaries as the Engine of Actively Repeating Fast Radio Bursts
Bing Zhang (HKU, UNLV), Rui-Chong Hu (UNLV)

TL;DR
This paper proposes a unified model where most active repeating fast radio bursts originate from magnetars in binary systems with aligned axes, explaining diverse observational features and the rarity of active repeaters.
Contribution
It introduces a novel binary magnetar framework that accounts for various FRB behaviors and predicts a small fraction of magnetars in binaries with specific alignments.
Findings
A few percent of magnetars are in binary systems.
Binary systems with aligned axes can produce diverse FRB phenomena.
The companion may trigger or sustain FRB activity.
Abstract
The association between FRB 20200428D and the Galactic magnetar SGR J1935+2154 makes magnetars the leading engine of cosmological fast radio bursts (FRBs). However, there is a list of puzzles for this magnetar-for-all-FRBs scenario: known Galactic magnetars are all isolated and none of them are active repeaters; some cosmological repeaters have extremely high repetition rates but without any measurable spin-related periodicity; some show long-term periodic active windows; and some show diverse rotation measure (RM) evolution patterns, such as quasi-periodic fluctuations, sign reversals, and abrupt RM flares. Here we propose a unified theoretical framework for FRBs within the framework of magnetar engine: Most active repeating FRBs originate from magnetars in binary systems with nearly aligned rotation and magnetic axes, some of which with a triple-aligned geometry, i.e. with an…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsPulsars and Gravitational Waves Research
