@inproceedings{e860db7aa6d946948e1c6f52d291b453,
title = "Diversity of the GRB-supernova connection: X-ray flashes and dark hypernovae",
abstract = "We review the following types of the GRB-Supernova (SN) connection, which has revealed interesting diversity. (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 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.",
keywords = "Gamma rays: bursts, Nuclear reactions, nucleosynthasis, abundances, Stars: abudances, Stars: population II, Supernovae: general, Supernovae: individual (SN 2006aj)",
author = "K. Nomoto and N. Tominaga and M. Tanaka and K. Maeda",
year = "2007",
doi = "10.1063/1.2774847",
language = "English",
isbn = "0735404348",
series = "AIP Conference Proceedings",
pages = "108--119",
booktitle = "THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS",
note = "THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS ; Conference date: 11-06-2006 Through 24-06-2006",
}