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We examine the characteristics of nucleosynthesis in 'hypernovae', i.e., supernovae with very large explosion energies ($ \gsim 10^{52} $ ergs). We carry out detailed nucleosynthesis calculations for these energetic explosions and compare…

We investigate mass ejection from accretion disks formed during the collapse of rapidly-rotating Wolf-Rayet stars. The neutrino-cooled, black hole (BH) accretion disk system that forms at the center of the star -- and the ensuing outflows…

高能天体物理现象 · 物理学 2024-03-15 Coleman Dean , Rodrigo Fernández

Magnetorotational supernovae are a rare type of core-collapse supernovae where the magnetic field and rotation play a central role in the dynamics of the explosion. We present the post-processed nucleosynthesis of state-of-the-art…

We report nucleosynthetic results for both $^{44}$Ti and nickel isotopes for eighteen three-dimensional (3D) core-collapse supernova (CCSN) simulations extended to $\sim$20 seconds after bounce. We find that many of our long-term models are…

高能天体物理现象 · 物理学 2024-08-06 Tianshu Wang , Adam Burrows

We investigate the fraction of metal nuclei in the relativistic jets of gamma-ray bursts associated with core-collapse supernovae. We simulate the fallback in jet-induced explosions with two-dimensional relativistic hydrodynamics…

高能天体物理现象 · 物理学 2015-06-17 Sanshiro Shibata , Nozomu Tominaga

Collapsars may be a source for the long Gamma Ray Bursts (GRBs) in the BATSE catalog. Collapsars may radiate gamma rays anisotropically by beamed jet emission close to the observer's line of sight. These jets must penetrate the…

天体物理学 · 物理学 2007-05-23 E. A. Gomez , P. E. Hardee

A type Ia supernova is thought to be a thermonuclear explosion of either a single carbon-oxygen white dwarf or of a pair of merging white dwarfs. The explosion fuses a large amount of radioactive 56Ni. After the explosion, the decay chain…

高能天体物理现象 · 物理学 2017-06-14 E. Churazov , R. Sunyaev , J. Isern , J. Knödlseder , P. Jean , F. Lebrun , N. Chugai , S. Grebenev , E. Bravo , S. Sazonov , M. Renaud

Precursor emission has been observed in a non-negligible fraction of gamma-ray bursts.The time gap between the precursor and the main burst extends in some case up to hundreds of seconds, such as in GRB041219A, GRB050820A and GRB060124.…

天体物理学 · 物理学 2008-11-26 Xiang-Yu Wang , Peter Meszaros

Long-duration gamma-ray bursts (LGRBs) associated with supernovae (SNe) are possibly born out of the death of a massive star. After the star collapses, a stellar-mass black hole (BH) is formed, surrounded by a hyperaccretion disk with…

高能天体物理现象 · 物理学 2019-02-27 Cui-Ying Song , Tong Liu

In this review I discuss the various gamma-ray emission lines that are expected and have been observed from radioactive explosive nucleosynthesis products. The most important gamma-ray lines result from the decay chains of Ni-56, Ni-57, and…

天体物理学 · 物理学 2009-11-10 Jacco Vink

We have studied whether the jet in a collapse-driven supernova can be a key process for the rapid-process (r-process) nucleosynthesis. We have examined the features of a steady, subsonic, and rigidly rotating jet in which the centrifugal…

天体物理学 · 物理学 2009-10-31 S. Nagataki

Jets in long-duration $\gamma$-ray bursts (GRBs) have to drill through the collapsing star in order to break out of it and produce the $\gamma$-ray signal while the central engine is still active. If the breakout time is shorter for more…

高能天体物理现象 · 物理学 2017-10-11 Maria Petropoulou , Rodolfo Barniol Duran , Dimitrios Giannios

The role of relativistic jets in unbinding the stellar envelope during a supernova (SN) associated with a gamma-ray burst (GRB) is unclear. To study that, we explore observational signatures of stellar explosions that are driven by jets. We…

高能天体物理现象 · 物理学 2022-08-17 Moshe Eisenberg , Ore Gottlieb , Ehud Nakar

We consider gamma-ray burst (GRB) jets that are choked by extended material as sources of high-energy cosmic neutrinos. We take into account the jet propagation physics both inside the progenitor star and the surrounding dense medium.…

高能天体物理现象 · 物理学 2018-10-12 Nicholas Senno , Kohta Murase , Peter Meszaros

We study the flow structure in the jittering-jets explosion model of core-collapse supernovae (CCSNe) using 2.5D hydrodynamical simulations and find that some basic requirements for explosion are met by the flow. In the jittering-jets model…

太阳与恒星天体物理 · 物理学 2015-06-16 Oded Papish , Noam Soker

A variety of arguments suggest that the most common form of gamma-ray bursts (GRBs), those longer than a few seconds, involve the formation of black holes in supernova-like events. Two kinds of ``collapsar'' models are discussed, those in…

天体物理学 · 物理学 2009-10-31 S. E. Woosley

The jet axes and the orbital planes of microquasar systems are usually assumed to be approximately perpendicular, eventhough this is not currently an observational requirement. On the contrary, in one of the few systems where the relative…

天体物理学 · 物理学 2009-11-07 Yousaf M. Butt , Thomas J. Maccarone , Nikos Prantzos

Core-collapse supernovae are found in galaxies with ongoing star-formation. In a starburst galaxy hosting an active galactic nucleus with a relativistic jet, supernovae can take place inside the jet. The collision of the supernova ejecta…

高能天体物理现象 · 物理学 2019-02-20 F. L. Vieyro , V. Bosch-Ramon , N. Torres-Albà

Jet-induced supernovae (SNe) have been suggested to occur in gamma-ray bursts (GRBs) and highly-energetic SNe (hypernovae). I investigate hydrodynamical and nucleosynthetic properties of the jet-induced explosion of a population III…

天体物理学 · 物理学 2008-12-18 Nozomu Tominaga

We reanalyze $r$-process nucleosynthesis in the neutron-rich ejecta from a prompt supernova explosion of a low-mass (11 M$_\odot$) progenitor. A pompt explosion is not yet ruled out as a possibility for low-mass supernova progenitors.…

天体物理学 · 物理学 2009-11-06 K. Sumiyoshi , M. Terasawa , G. J. Mathews , T. Kajino , S. Yamada , H. Suzuki