Dark Matter Admixed Type Ia Supernovae
arXiv:1509.01871 · doi:10.1088/0004-637X/812/2/110
Abstract
We perform two-dimensional hydrodynamic simulations for the thermonuclear explosion of Chandrasekhar-mass white dwarfs with dark matter (DM) cores in Newtonian gravity. We include a 19-isotope nuclear reaction network and make use of the pure turbulent deflagration model as the explosion mechanism in our simulations. Our numerical results show that the general properties of the explosion depend quite sensitively on the mass of the DM core M: a larger M generally leads to a weaker explosion and a lower mass of synthesized iron-peaked elements. In particular, the total mass of Ni produced can drop from about 0.3 to 0.03 as M increases from 0.01 to 0.03 . We have also constructed the bolometric light curves obtained from our simulations and found that our results match well with the observational data of sub-luminous Type-Ia supernovae.
11 pages, 14 figures, accepted by The Astrophysical Journal. Metadata updated
References in corpus (19)
- Modules for Experiments in Stellar Astrophysics (MESA)
- Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector
- Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core?
- WIMP Annihilation and Cooling of Neutron Stars
- Compact Stars as Dark Matter Probes
- Double-detonation sub-Chandrasekhar supernovae: synthetic observables for minimum helium shell mass models
- Constraining Asymmetric Dark Matter through observations of compact stars
- Dark matter and the first stars: a new phase of stellar evolution
- Deflagrations in hybrid CONe white dwarfs: a route to explain the faint Type Iax supernova 2008ha
- Constraints on Bosonic Dark Matter From Observations of Old Neutron Stars
- The ejected mass distribution of type Ia supernovae: A significant rate of non-Chandrasekhar-mass progenitors
- The effect of helium accretion efficiency on rates of Type Ia supernovae: double-detonations in accreting binaries
- Possible Detection of the Stellar Donor or Remnant for the Type Iax Supernova 2008ha
- Dark matter burners
- Detonating Failed Deflagration Model of Thermonuclear Supernovae I. Explosion Dynamics
- The Zero Age Main Sequence of WIMP burners
- Equilibrium Structure and Radial Oscillations of Dark Matter Admixed Neutron Stars
- A new hydrodynamics code for Type Ia Supernovae
- Constraining decaying dark matter with neutron stars
Cited by in corpus (20)
- Explosive Nucleosynthesis in Near-Chandrasekhar Mass White Dwarf Models for Type Ia Supernovae: Dependence on Model Parameters
- New Type Ia supernova Yields and the Manganese and Nickel Problems in the Milky Way and Dwarf Spheroidal Galaxies
- Explosive Nucleosynthesis in Sub-Chandrasekhar Mass White Dwarf Models for Type Ia Supernovae: Dependence on Model Parameters
- Single Degenerate Models for Type Ia Supernovae Progenitor's Evolution and Nucleosythesis Yields
- Tidal Deformability of Dark Matter Admixed Neutron Stars
- Evolution of ONeMg Core in Super-AGB Stars towards Electron-Capture Supernovae: Effects of Updated Electron-Capture Rate
- Electron Capture Supernovae of Super-AGB Stars: Sensitivity on Input Physics
- Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- I: Formation of Low-mass Neutron Stars
- Delayed Detonation Thermonuclear Supernovae With An Extended Dark Matter Component
- Exploring non-radial oscillation modes in dark matter admixed neutron stars
- Exploration of Aspherical Ejecta Properties in Type Ia Supernova: Progenitor Dependence and Applications to Progenitor Classification
- Hydrodynamics and Nucleosynthesis of Jet-Driven Supernovae I: Parameter Study of the Dependence on Jet Energetics
- Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- II: Rotation and Gravitational-wave Signals
- Dark Matter-admixed Rotating White Dwarfs as Peculiar Compact Objects
- Type Ia Supernova Magnitude Step from the local Dark Matter Environment
- Triggering Electron Capture Supernovae: Dark Matter Effects in Degenerate White-Dwarf-like Cores of Super-Asymptotic Giant Branch Stars
- Type Ia Supernovae and their Explosive Nucleosynthesis: Constraints on Progenitors
- Primordial Black Hole Triggered Type Ia Supernovae II: Comparison with Supernova Remnants and Galactic Chemical Evolution
- Effects of light-mass fermionic dark matter on the equilibrium and stability of white dwarfs
- Revisiting the Perseus Cluster III: Role of Aspherical Explosions on its Chemical Composition and Extension to Metal-Poor Stars and Galaxies