Insights from the Gaussian Processes Method for the FRB-associated X-ray Burst of SGR 1935+2154
Ruijing Tang, Dahai Yan, Haiyun Zhang, Qingchang Zhao, Lian Tao,, Chengkui Li, Mingyu Ge, Xiaobo Li, Qianqing Yin, Ce Cai

TL;DR
This paper uses Gaussian processes to analyze X-ray burst light curves from SGR 1935+2154, revealing characteristic timescales and suggesting immediate burst production during energy response, especially for FRB-associated events.
Contribution
It introduces a Gaussian processes approach to model X-ray burst variability, identifying specific timescales and dynamics linked to FRB-associated bursts, which is novel in this context.
Findings
High broken frequency of 35 Hz in FRB 200428 burst
Retarding timescale of 0.03 s for FRB-associated burst
Immediate production of X-ray burst during system response
Abstract
Gaussian processes method is employed to analyze the light curves of bursts detected by Insight-HXMT, NICER, and GECAM from SGR 1935+2154 between 2020 to 2022. It is found that a stochastically driven damped simple harmonic oscillator (SHO) is necessary to capture the characteristics of the X-ray bursts. Variability timescale of the X-ray bursts, corresponding to the broken frequencies in the SHO power spectral densities (PSDs), are extracted. In particular, a high broken frequency of 35 Hz where the index of the SHO PSD changes from -4 to -2 is constrained by the HXMT-HE burst associated with FRB 200428. It is suggested that the corresponding timescale of 0.03 s could be the retarding timescale of the system driven by some energy release, and the production of the HE photon should be quasi-simultaneous with the response. The other special event is a NICER burst with a retarding…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astronomical Observations and Instrumentation · Astronomy and Astrophysical Research
