We describe the detonation mechanism composing the "pulsationally assisted" gravitationally confined detonation (GCD) model of Type Ia supernovae. This model is analogous to the previous GCD model reported in Jordan et al.; however, the chosen initial conditions produce a substantively different detonation mechanism, resulting from a larger energy release during the deflagration phase. The resulting final kinetic energy and Ni-56 yields conform better to observational values than is the case for the "classical" GCD models. In the present class of models, the ignition of a deflagration phase leads to a rising, burning plume of ash. The ash breaks out of the surface of the white dwarf, flows laterally around the star, and converges on the collision region at the antipodal point from where it broke out. The amount of energy released during the deflagration phase is enough to cause the star to rapidly expand, so that when the ash reaches the antipodal point, the surface density is too low to initiate a detonation. Instead, as the ash flows into the collision region (while mixing with surface fuel), the star reaches its maximally expanded state and then contracts. The stellar contraction acts to increase the density of the star, including the density in the collision region. This both raises the temperature and density of the fuel-ash mixture in the collision region and ultimately leads to thermodynamic conditions that are necessary for the Zel'dovich gradient mechanism to produce a detonation. We demonstrate feasibility of this scenario with three three-dimensional (3D), full star simulations of this model using the FLASH code. We characterized the simulations by the energy released during the deflagration phase, which ranged from 38% to 78% of the white dwarf's binding energy. We show that the necessary conditions for detonation are achieved in all three of the models.
- THE DETONATION MECHANISM OF THE PULSATIONALLY ASSISTED GRAVITATIONALLY CONFINED DETONATION MODEL OF Type Ia SUPERNOVAE
- G. C. Jordan - University of ChicagoC. Graziani - University of ChicagoR. T. Fisher - University of Massachusetts DartmouthD. M. Townsley - University of AlabamaC. Meakin - University of ArizonaK. Weide - University of ChicagoL. B. Reid - NTEC Environm Technol, Subiaco, WA 6008, AustraliaJ. Norris - University of ChicagoR. Hudson - University of ChicagoD. Q. Lamb - University of Chicago
- The Astrophysical journal, Vol.759(1), pp.1-15
- Iop Publishing Ltd
- 15
- English
- AST-0909132 / National Science Foundation; National Science Foundation (NSF) INCITE program at ALCF at ANL DE-AC02-06CH11357 / Office of Science of the US Department of Energy; United States Department of Energy (DOE) B523820 / US Department of Energy (DOE); United States Department of Energy (DOE) 1107445 / Direct For Mathematical & Physical Scien; National Science Foundation (NSF); NSF - Directorate for Mathematical & Physical Sciences (MPS)
- Department of Physics
- Journal article
- 9914417702501301