Scale-invariance in the repeating fast radio burst 121102

doi:10.1093/mnras/stz3149

ITP OpenIR > SCI期刊论文

	Lin, Hai-Nan ; Sang, Yu 1
	Scale-invariance in the repeating fast radio burst 121102
Source Publication	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Language	英语
Keyword	HOST GALAXY REDSHIFT
Abstract	The statistical properties of the repeating fast radio burst FRB 121102 are investigated. We find that the cumulative distributions of fluence, flux density, total energy, and waiting time can be well fitted by the bent power law. In addition, the probability density functions of fluctuations of fluence, flux density, and total energy well follow the Tsallis q-Gaussian distribution. The q-values keep steady around q similar to 2 for different scale intervals, indicating a scale-invariant structure of the bursts. The statistical properties of FRB 121102 are very similar to that of the soft gamma repeater SGR J1550-5418. The underlying physical implications need to be further investigated.
	2020
ISSN	0035-8711
Volume	491 Issue:2 Pages:2156-2161
Cooperation Status	国内
Subject Area	Astronomy & Astrophysics
MOST Discipline Catalogue	Astronomy & Astrophysics
DOI	10.1093/mnras/stz3149
Indexed By	SCIE
Citation statistics	Cited Times:2[WOS] [WOS Record] [Related Records in WOS]
Document Type	期刊论文
Identifier	http://ir.itp.ac.cn/handle/311006/27083
Collection	SCI期刊论文
Affiliation	1.Chongqing Univ, Dept Phys, Chongqing 401331, Peoples R China 2.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
Recommended Citation GB/T 7714	Lin, Hai-Nan,Sang, Yu. Scale-invariance in the repeating fast radio burst 121102[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,491(2):2156-2161.
APA	Lin, Hai-Nan,&Sang, Yu.(2020).Scale-invariance in the repeating fast radio burst 121102.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,491(2),2156-2161.
MLA	Lin, Hai-Nan,et al."Scale-invariance in the repeating fast radio burst 121102".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 491.2(2020):2156-2161.

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