arXiv · 2209.08598
The game of life on a magnetar crust: from $\gamma$-ray flares to FRBs
Abstract
This paper presents a model to unify the diverse range of magnetar activity, through the building and release of elastic stress from the crust. A cellular automaton drives both local and global yielding of the crust, leading to braiding of coronal loops and energy release. The model behaves like a real magnetar in many ways: giant flares and small bursts both occur, as well as periods of quiescence whose typical duration is either $\lesssim 1$ yr or $\sim 10-30$ yr. The burst energy distribution broadly follows an earthquake-like power law over the energy range $10^{40}-10^{45}\,{\rm erg}$. The local nature of coronal loops allows for the possibility of high-energy and fast radio bursts from the same magnetar. Within this paradigm, magnetar observations can be used to constrain the poorly-understood mechanical properties of the neutron-star crust.
Explore related subjects
Keep this discovery
S. K. Lander. 2022-09-18. The game of life on a magnetar crust: from $\gamma$-ray flares to FRBs. https://doi.org/10.3847/2041-8213%2Facca1f
Cite the original work for its findings. Save a collection to share your selection of sources.