Diversity of the supernova-gamma-ray burst connection

K. Nomoto, N. Tominaga, M. Tanaka, K. Maeda, T. Suzuki, J. S. Deng, P. A. Mazzali

研究成果: Article査読

20 被引用数 (Scopus)

抄録

The connection between the long Gamma Ray Bursts (GRBs) and Type Ic Supernovae (SNe) has revealed interesting diversity. We review the following types of the GRB-SN connection. 1) GRB-SNe: The three SNe all explode with energies much larger than those of typical SNe, thus being called Hypernovae (HNe). They are massive enough for forming black holes. 2) Non-GRB HNe/SNe: Some HNe are not associated with GRBs. 3) XRF-SN: SN 2006aj associated with X-Ray Flash 060218 is dimmer than GRB-SNe and has very weak oxygen lines. Its progenitor mass is estimated to be small enough to form a neutron star rather than a black hole. 4) Non-SN GRB: Two nearby long GRBs were not associated SNe. Such "dark HNe" have been predicted in this talk (i.e. just before the discoveries) in order to explain the origin of C-rich (hyper) metal-poor stars. This would be an important confirmation of the hypernova-first-star connection. We will show our attempt to explain the diversity in a unified manner with the jet-induced explosion model.

本文言語English
ページ(範囲)1207-1222
ページ数16
ジャーナルNuovo Cimento della Societa Italiana di Fisica B
121
10-11
DOI
出版ステータスPublished - 2006 10 1
外部発表はい

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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