114 citations · 348 across the 9 of their papers we have counts for
9 papers
Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses
Anthony Mezzacappa, Pedro Marronetti, Ryan E. Landfield +8
We present gravitational wave emission predictions based on three core collapse supernova simulations corresponding to three different progenitor masses. The masses span a large ra…
On the character of turbulence in self-consistent models of core-collapse supernovae
Jordi Casanova, Eirik Endeve, Eric J. Lentz +4
Neutrino-driven convection plays a crucial role in the development of core-collapse supernova (CCSN) explosions. However, the complex mechanism that triggers the shock revival and…
123-321 Models of Classical Novae
Jordi Jose, Steven N. Shore, Jordi Casanova
High-resolution spectroscopy has revealed large concentrations of CNO and sometimes other intermediate-mass elements in the shells ejected during nova outbursts, suggesting that th…
Two-dimensional simulations of mixing in classical novae: the effect of the white dwarf composition and mass
Jordi Casanova, Jordi Jose, Steven N. Shore
Context. Classical novae are explosive phenomena that take place in stellar binary systems. They are powered by mass transfer from a low-mass main sequence star onto a white dwarf…
Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations
Kevin Ebinger, Sanjana Sinha, Carla Fröhlich +6
We report on a method, PUSH, for triggering core-collapse supernova (CCSN) explosions of massive stars in spherical symmetry. This method provides a framework to study many importa…
Three-dimensional simulations of turbulent convective mixing in ONe and CO classical nova explosions
Jordi Casanova, Jordi Jose, Enrique Garcia-Berro +1
Classical novae are thermonuclear explosions that take place in the envelopes of accreting white dwarfs in binary systems. The material piles up under degenerate conditions, drivin…