114 citations · 348 across the 9 of their papers we have counts for
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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…
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…
Pushing 1D CCSNe to explosions: model and SN 1987A
A. Perego, M. Hempel, C. Fröhlich +5
We report on a method, PUSH, for triggering core-collapse supernova explosions of massive stars in spherical symmetry. We explore basic explosion properties and calibrate PUSH such…
Mixing in classical novae: a 2-D sensitivity study
Jordi Casanova, Jordi Jose, Enrique Garcia-Berro +2
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. The mat…
On mixing at the core-envelope interface during classical nova outbursts
Jordi Casanova, Jordi Jose, Enrique Garcia-Berro +2
Classical novae are powered by thermonuclear runaways that occur on the white dwarf component of close binary systems. During these violent stellar events, whose energy release is…