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ASTROPHYSICAL JOURNAL LETTERS, ISSN 2041-8205, 07/2015, Volume 807, Issue 2
We have performed ab initio neutrino radiation hydrodynamics simulations in three and two spatial dimensions (3D and 2D) of core-collapse supernovae from the... 
MASSIVE STARS | neutrinos | stars: evolution | SASI ACTIVITY | MECHANISMS | 3 DIMENSIONS | supernovae: general | NEUTRINO-HYDRODYNAMICS SIMULATIONS | SHOCK | EXPLOSIONS | TRANSPORT | ASTRONOMY & ASTROPHYSICS | stars: massive | NUCLEOSYNTHESIS | DRIVEN SUPERNOVA
Journal Article
Astrophysical Journal, ISSN 0004-637X, 11/2016, Volume 831, Issue 1, p. 98
We report on a set of long-term general-relativistic three-dimensional (3D) multi-group (energy-dependent) neutrino radiation-hydrodynamics simulations of... 
neutrinos | instabilities | supernovae: general | MASSIVE STARS | ACCRETION SHOCK INSTABILITY | SASI ACTIVITY | CIRCLE-DOT STARS | 3 DIMENSIONS | DRIVEN CONVECTION | EXPLOSIONS | CODE | PROGENITOR | EVOLUTION | ASTRONOMY & ASTROPHYSICS | Physics - High Energy Astrophysical Phenomena
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 03/2015, Volume 801, Issue 2, pp. L24 - 6
We present the first successful simulation of a neutrino-driven supernova explosion in three dimensions (3D), using the PROMETHEUS-VERTEX code with an... 
hydrodynamics | neutrinos | instabilities | supernovae: general | MECHANISM | SASI ACTIVITY | 3 DIMENSIONS | EXPLOSION MODELS | CIRCLE-DOT STAR | RADIATION HYDRODYNAMICS | TRANSPORT | CODE | COLLAPSE SUPERNOVAE | ASTRONOMY & ASTROPHYSICS | HYDRODYNAMICS SIMULATIONS | Cooling | Neutrinos | Progenitors (astrophysics) | Explosions | Two dimensional | Gain | Downdraft | Three dimensional
Journal Article
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN 1550-7998, 08/2014, Volume 90, Issue 4
The neutrino emission characteristics of the first full-scale three-dimensional supernova simulations with sophisticated three-flavor neutrino transport for... 
MASSIVE STARS | SHOCK | EQUATION-OF-STATE | EVOLUTION | DRIVEN EXPLOSIONS | MECHANISM | SASI ACTIVITY | CONVECTION | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | HYDRODYNAMICS CODE | PHYSICS, PARTICLES & FIELDS
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 06/2017, Volume 468, Issue 2, pp. 2032 - 2051
We present gravitational wave (GW) signal predictions from four 3D multigroup neutrino hydrodynamics simulations of core-collapse supernovae of progenitors... 
NONLINEAR PHASE | MASSIVE STARS | ACCRETION SHOCK INSTABILITY | SASI ACTIVITY | hydrodynamics | STELLAR COLLAPSE | instabilities | supernovae: general | RADIATION-HYDRODYNAMICS | EQUATION-OF-STATE | ASTRONOMY & ASTROPHYSICS | 3-DIMENSIONAL SIMULATIONS | NEWTONIAN HYDRODYNAMICS | gravitational waves | DRIVEN SUPERNOVA
Journal Article
Physical Review Letters, ISSN 0031-9007, 09/2013, Volume 111, Issue 12, p. 121104
The first full-scale three-dimensional core-collapse supernova (SN) simulations with sophisticated neutrino transport show pronounced effects of the standing... 
ACCRETION-SHOCK INSTABILITY | CIRCLE-DOT STAR | MASSIVE STARS | TRANSPORT | MECHANISM | PHYSICS, MULTIDISCIPLINARY | SASI ACTIVITY | CORE-COLLAPSE SUPERNOVAE | GRAVITATIONAL-WAVE SIGNALS | SIMULATIONS | EXPLOSION MODELS
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 09/2016, Volume 829, Issue 1, pp. L14 - L14
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 443, Issue 1, pp. 664 - 670
We use 3D hydrodynamical numerical simulations and show that jittering bipolar jets that power core-collapse supernova (CCSN) explosions channel further... 
Supernovae | General | NEUTRINO-HYDRODYNAMICS SIMULATIONS | SHOCK | TRANSPORT | STAR | SASI ACTIVITY | ASTRONOMY & ASTROPHYSICS | ACCRETION | FEEDBACK MECHANISM | supernovae: general | CASSIOPEIA | KEY | DRIVEN SUPERNOVA
Journal Article
Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 2014, Volume 445, Issue 1, pp. L99 - L103
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2018, Volume 856, Issue 1, p. 22
An important result in core-collapse supernova (CCSN) theory is that spherically symmetric, one-dimensional simulations routinely fail to explode, yet... 
methods: analytical | hydrodynamics | methods: numerical | turbulence | supernovae: general | shock waves | MECHANISM | STANDING ACCRETION SHOCKS | SASI ACTIVITY | CONVECTION | NEUTRINO-DRIVEN SUPERNOVA | STELLAR COLLAPSE | PROGENITOR | ASTRONOMY & ASTROPHYSICS | SIMULATIONS | II SUPERNOVA
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2016, Volume 461, Issue 4, pp. 3864 - 3876
Nuclear shell burning in the final stages of the lives of massive stars is accompanied by strong turbulent convection. The resulting fluctuations aid supernova... 
General | Hydrodynamics-shock waves-turbulence-supernovae | PERTURBATIONS | SASI ACTIVITY | hydrodynamics | turbulence | 3 DIMENSIONS | supernovae: general | WAVE | EXPLOSIONS | PROGENITOR | STAR | NEUTRINO-DRIVEN CONVECTION | ASTRONOMY & ASTROPHYSICS | HYDRODYNAMICS SIMULATIONS | SPHERICAL ACCRETION SHOCK | shock waves
Journal Article