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Convection- and SASI-driven flows in parametrized models of core-collapse supernova explosions

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A NEW MULTI-ENERGY NEUTRINO RADIATION-HYDRODYNAMICS CODE IN FULL GENERAL RELATIVITY AND ITS APPLICATION TO THE GRAVITATIONAL COLLAPSE OF MASSIVE STARS

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The Astrophysical Journal Supplement Series 222 (2) 20 (2016)
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Parametric initial conditions for core-collapse supernova simulations

Yudai Suwa and Ewald Müller
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A TWO-PARAMETER CRITERION FOR CLASSIFYING THE EXPLODABILITY OF MASSIVE STARS BY THE NEUTRINO-DRIVEN MECHANISM

T. Ertl, H.-Th. Janka, S. E. Woosley, T. Sukhbold and M. Ugliano
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THREE-DIMENSIONAL CORE-COLLAPSE SUPERNOVA SIMULATED USING A 15 M☉ PROGENITOR

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

Oded Papish, Jason Nordhaus and Noam Soker
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PROBING THE ROTATION OF CORE-COLLAPSE SUPERNOVA WITH A CONCURRENT ANALYSIS OF GRAVITATIONAL WAVES AND NEUTRINOS

Takaaki Yokozawa, Mitsuhiro Asano, Tsubasa Kayano, et al.
The Astrophysical Journal 811 (2) 86 (2015)
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PUSHING CORE-COLLAPSE SUPERNOVAE TO EXPLOSIONS IN SPHERICAL SYMMETRY. I. THE MODEL AND THE CASE OF SN 1987A

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The Astrophysical Journal 806 (2) 275 (2015)
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