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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2018, Volume 475, Issue 3, pp. 3305 - 3323
Journal Article
PHYSICA SCRIPTA, ISSN 0031-8949, 09/2019, Volume 94, Issue 9, p. 94002
In the context of core-collapse supernova explosions, the interaction of standing accretion shocks with upstream vorticity perturbations is investigated by... 
INSTABILITY | PHYSICS, MULTIDISCIPLINARY | CONVECTION | STABILITY | EXPLOSION | SUPERNOVA | turbulence | shock wave | CORE-COLLAPSE | EVOLUTION | supernovae | SIMULATIONS | SPHERICAL ACCRETION SHOCK
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
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2020, Volume 494, Issue 4, pp. 5360 - 5373
ABSTRACT The explosion of massive stars in core-collapse supernovae may be aided by the convective instabilities that develop in their innermost nuclear... 
Journal Article
PHYSICAL REVIEW D, ISSN 2470-0010, 08/2014, Volume 90, Issue 4
The late collapse, core bounce, and the early postbounce phase of rotating core collapse leads to a characteristic gravitational wave (GW) signal. The precise... 
NEUTRINO-HYDRODYNAMICS SIMULATIONS | BLACK-HOLE FORMATION | EQUATION-OF-STATE | ROTATING MASSIVE STARS | INSTABILITY | PRESUPERNOVA EVOLUTION | ASTRONOMY & ASTROPHYSICS | ASYMMETRIC SUPERNOVAE | AXISYMMETRICAL SIMULATIONS | RELATIVISTIC SIMULATIONS | DRIVEN SUPERNOVA | PHYSICS, PARTICLES & FIELDS
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2009, Volume 392, Issue 1, pp. 52 - 76
An increase in the central density of a neutron star may trigger a phase transition from hadronic matter to deconfined quark matter in the core, causing it to... 
hydrodynamics | stars: oscillations | methods: numerical | relativity | stars: rotation | stars: neutron | Hydrodynamics | Stars: neutron | Relativity | Methods: numerical | Stars: oscillations | Stars: rotation | Fluid dynamics | Nuclear physics | Gravity waves | Detectors | Fluid mechanics | Astrophysics | Numerical analysis | Simulation | Stars & galaxies
Journal Article
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2015, Volume 450, Issue 1, pp. 414 - 427
Journal Article