The prompt phase mechanism of gamma-ray bursts

Abstract

Self-organized criticality during the prompt phase of gamma-ray bursts shows that they may arise from magnetic reconnection events.

References

[1] P. Kumar and B. Zhang, The physics of gamma-ray bursts & relativistic jets, Phys. Rep. 561, 1 (2015)

[2] F. Y. Wang and Z. G. Dai, Self-organized criticality in X-ray flares of gamma-ray-burst afterglows, Nat. Phys. 9, 465 (2013)

[3] Z. G. Dai, X. Y. Wang, X. F. Wu, and B. Zhang, X-ray flares from postmerger millisecond pulsars, Science 311, 1127 (2006)

[4] P. Bak, C. Tang, and K. Wiesenfeld, Self-organized criticality: An explanation of the 1/fnoise, Phys. Rev. Lett. 59(4), 381 (1987)

[5] E. T. Lu and R. J. Hamilton, Avalanches and the distribution of solar flares, Astrophys. J. Lett. 380, L89 (1991)

[6] M. J. Aschwanden, A statistical fractal-diffusive avalanche model of a slowly-driven self-organized criticality system, Astron. Astrophys. 539, A2 (2012)

[7] F. Lyu, Y. P. Li, S. J. Hou, J. J. Wei, J. J. Geng, and X. F. Wu, Self-organized criticality in multi-pulse gamma-ray bursts, Front. Phys. 16(1), 14501 (2021)

[8] W. Kluzniak and M. Ruderman, The central engine of gamma-ray bursters, Astrophys. J. Lett. 505(2), L113 (1998)

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