Induced gravitational collapse at extreme cosmological distances: the case of GRB 090423

CONTEXT: The induced gravitational collapse (IGC) scenario has been introduced in order to explain the most energetic gamma ray bursts (GRBs), Eiso=10^{52}-10^{54}erg, associated with type Ib/c supernovae (SNe). It has led to the concept of binary-driven hypernovae (BdHNe) originating in a tight bin...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2014-07
Hauptverfasser:	Ruffini, R, Izzo, L, Muccino, M, Pisani, G B, Rueda, J A, Wang, Y, Barbarino, C, Bianco, C L, Enderli, M, Kovacevic, M
Format:	Artikel
Sprache:	eng
Schlagworte:	Big bang cosmology Binary stars Companion stars Emission Gamma ray bursts Gamma rays Gravitation Gravitational collapse Luminosity Neutron stars Physics - Cosmology and Nongalactic Astrophysics Physics - High Energy Astrophysical Phenomena Population III stars Scaling laws Stellar evolution Stellar populations Supernovae
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!