GRB 130427A AND SN 2013cq: A MULTI-WAVELENGTH ANALYSIS OF AN INDUCED GRAVITATIONAL COLLAPSE EVENT

被引：30

作者：

Ruffini, R. ^{[1
,2
,3
,4
,5
]}

Wang, Y. ^{[1
,2
,3
]}

Enderli, M. ^{[1
,2
,4
]}

Muccino, M. ^{[1
,2
,3
]}

Kovacevic, M. ^{[1
,2
,4
]}

Bianco, C. L. ^{[1
,2
,3
]}

Penacchioni, A. V. ^{[5
]}

Pisani, G. B. ^{[1
,2
,4
]}

Rueda, J. A. ^{[1
,2
,3
,5
]}

机构：

[1] Univ Roma La Sapienza, Dip Fis, I-00185 Rome, Italy

[2] Univ Roma La Sapienza, ICRA, I-00185 Rome, Italy

[3] ICRANet, I-65122 Pescara, Italy

[4] Univ Nice Sophia Antipolis, F-06189 Nice 2, France

[5] Ctr Brasileiro Pesquisas Fis, ICRANet Rio, BR-22290180 Rio De Janeiro, RJ, Brazil

来源：

ASTROPHYSICAL JOURNAL | 2015年 / 798卷 / 01期

关键词：

black hole physics; gamma-ray burst: general; nuclear reactions; nucleosynthesis; abundances; stars: neutron; supernovae: general; GAMMA-RAY BURST; PAIR-ELECTROMAGNETIC PULSE; BLACK-HOLE; NEUTRON-STAR; HOST GALAXY; GENUINE SHORT; LIGHT CURVES; AFTERGLOW; EMISSION; SWIFT;

D O I：

10.1088/0004-637X/798/1/10

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We performed a data analysis of the observations by the Swift, NuStar, and Fermi satellites in order to probe the induced gravitational collapse (IGC) paradigm for gamma-ray bursts (GRBs) associated with supernovae (SNe) in the terra incognita of GRB 130427A. We compare our data analysis with those in the literature. We have verified that GRB 130427A conforms to the IGC paradigm by examining the power law behavior of the luminosity in the early 10(4) s of the XRT observations. This has led to the identification of the four different episodes of the binary driven hypernovae (BdHNe) and to the prediction, on 2013 May 2, of the occurrence of SN 2013cq, which was also observed in the optical band on 2013 May 13. The exceptional quality of the data has allowed the identification of novel features in Episode 3 including: (1) the confirmation and the extension of the existence of the recently discovered nested structure in the late X-ray luminosity in GRB 130427A, as well as the identification of a spiky structure at 10(2) s in the cosmological rest-frame of the source; (2) a power law emission of the GeV luminosity light curve and its onset at the end of Episode 2; and (3) different Lorentz Gamma factors for the emitting regions of the X-ray and GeV emissions in this Episode 3. These results make it possible to test the details of the physical and astrophysical regimes at work in the BdHNe: (1) a newly born neutron star and the supernova ejecta, originating in Episode 1; (2) a newly formed black hole originating in Episode 2; and (3) the possible interaction among these components, observable in the standard features of Episode 3.

引用

页数：11

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