The core helium flash revisited: I. One and two-dimensional hydrodynamic simulations

Details The core helium flash revisited: I. One and two-dimensional hydrodynamic simulations The core helium flash revisited: I. One and two-dimensional hydrodynamic simulations

2008-05-09

arxiv.org/abs/0805.1355v1

Astronomy and Astrophysics

Astrophysics

13 pages, 23 figures

Scientific paper

10.1051/0004-6361:200810169

We investigate the hydrodynamics of the core helium flash near its peak. Past research concerned with the dynamics of this event is inconclusive. However, the most recent multidimensional hydrodynamic studies suggest a quiescent behavior and seem to rule out an explosive scenario. Previous work indicated, that depending on initial conditions, employed turbulence models, grid resolution, and dimensionality of the simulation, the core helium flash leads either to the disruption of a low-mass star or to a quiescent quasi-hydrostatic evolution. We try to clarify this issue by simulating the evolution with advanced numerical methods and detailed microphysics. Assuming spherical or axial symmetry, we simulate the evolution of the helium core of a $1.25 M_{\odot}$ star with a metallicity Z=0.02 during the core helium flash at its peak with a grid-based hydrodynamics code. We find that the core helium flash neither rips the star apart, nor that it significantly alters its structure, as convection plays a crucial role in keeping the star in hydrostatic equilibrium. In addition, our simulations show the presence of overshooting, which implies new predictions concerning mixing of chemical species in red giants.

Affiliated with

Also associated with

No associations

Rating

The core helium flash revisited: I. One and two-dimensional hydrodynamic simulations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The core helium flash revisited: I. One and two-dimensional hydrodynamic simulations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The core helium flash revisited: I. One and two-dimensional hydrodynamic simulations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-332524