activity
20112020
most citedExploding Core-Collapse Supernovae with Jittering Jets

86 citations · 424 across the 13 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2014★ 39 cited

The response of a helium white dwarf to an exploding type Ia supernova

Oded Papish, Noam Soker, Enrique García-Berro +1

We conduct numerical simulations of the interacting ejecta from an exploding CO white dwarf (WD) with a He WD donor in the double-detonation scenario for Type Ia supernovae (SNe Ia…

astro-ph.SR2014★ 48 cited

A Planar Jitternig-Jets Pattern in Core-Collapse Supernova Explosions

Oded Papish, Noam Soker

We use 3D hydrodynamical numerical simulations and show that jittering bipolar jets that power core-collapse supernova (CCSN) explosions channel further accretion onto the newly bo…

astro-ph.SR2014★ 47 cited

A call for a paradigm shift from neutrino-driven to jet-driven core-collapse supernova mechanisms

Oded Papish, Jason Nordhaus, Noam Soker

Three-dimensional (3D) simulations in recent years have shown severe difficulties producing 10^51 erg explosions of massive stars with neutrino based mechanisms while on the other…

astro-ph.SR2013★ 5 cited

Ejecting the envelope of red supergiant stars with jets launched by an inspiraling neutron star

Oded Papish, Noam Soker, Inbal Bukay

We study the properties of jets launched by a neutron star spiralling inside the envelope and core of a red supergiant. We propose that Thorne-Zytkow objects (TZO) are unlikely to…

astro-ph.SR2013★ 38 cited

Exploding Core-Collapse Supernovae by Jets-Driven Feedback Mechanism

Oded Papish, Noam Soker

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 fo…

astro-ph.SR2012★ 24 cited

The jet feedback mechanism (JFM): from supernovae to clusters of galaxies

Noam Soker, Muhammad Akashi, Avishai Gilkis +4

We study the similarities of jet-medium interactions in several quite different astrophysical systems using 2D and 3D hydrodynamical numerical simulations, and find many similariti…