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Fidelity of Type Ia Supernovae Nucleosynthesis with Tracer Particles

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The Center for Astrophysical Thermonuclear Flashes ... Eulerian hydro code. Godunov method. PPM. AMR. Highly scalable. Multiplatform. Efficient, parallel IO ... – PowerPoint PPT presentation

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Title: Fidelity of Type Ia Supernovae Nucleosynthesis with Tracer Particles


1
Fidelity of Type Ia Supernovae Nucleosynthesis
with Tracer Particles
  • George (Cal) Jordan
  • Tomek Plewa

2
Reactive Flows in Real World
  • Industry
  • Combustion in Engine
  • Rockets
  • Safety
  • Pool fires

C-Safe ASC center, University of Utah
NASA
3
Reactive Flows in Astrophysics
  • Explosive nucleosynthesis
  • Nova nucleosynthesis
  • Rapid catalyzed proton burning.
  • Type II/Ib/Ic supernovae
  • r-process nucleosynthesis
  • Freezeout from equilibrium
  • Type Ia Supernovae
  • Deflagration
  • Detonation
  • X-Ray Bursts
  • Burning in thin dense layers on surface of a
    compact object, very strong gravity

Nova Vel 1999
Supernova 1987a
Supernova DEM l71
Depiction of accretion leading to an x-ray burst
4
Feasible Reactive Flow Computations
  • Possible to fully model reactive flows with full
    chemistry?
  • Frequently too expensive!
  • Want a cheap way to approximate the continuum
    solution
  • Introduce tracer particles
  • Can use tracer particles to provide a lagrangian
    view of the system
  • Particle records the thermodynamic history of a
    mass element
  • Post-process use this information as input to
    reaction network

5
Particles in Physics Modeling
  • Used to represent gravitating elements
  • Numerical cosmology (PM, SPH, treecodes)
    (Dubinski et al.)
  • Used to track interfaces
  • Level-sets with particles for material interfaces
    (ink jet) (Enright et al.)
  • Used to directly model microscopic processes
  • Direct Simulation Monte Carlo for shockwave
    profiles (Anderson et al.)
  • Multiphase flows
  • fuel solid oxidizer in rocket engines (Rider et
    al.)

6
Requirements for Tracing with Particles
  • Tracer particles follow evolution of individual
    fluid elements
  • Particles evolve simultaneously with the flow
    field
  • Need to make sure that flow/particle coupling is
    strong
  • Is stochastic sampling of the hydro field with
    the particles reliable? (i.e. , can we represent
    the flow field properties with particles
    correctly)?
  • What about properties of the flow field that
    arent resolved in the simulation?
  • Metric for determining accuracy of particle
    sample
  • Post-processing example Compare final yields,
    particle trajectories

7
Turbulent Flows
Non-Reactive turbulent flow
  • Starts as R-T unstable and transits to
    turbulence.
  • Wide range of length scales cant capture all in
    the model simultaneously
  • Must use subgrid scale model to account for
    unresolved scales

Cabot et al. 2005
8
Turbulent Flows
Reactive turbulent flow
0.1 km resolution
0.1cm resolution
Zingale et al. 2005
9
Turbulent Flames with Tracer Particles
Bell et al. (2005)
  • Application of stochastic particles to
    turbulent chemical flames
  • Traces individual atoms through the simulation
  • Particles advect through the system according to
    hydro
  • Diffusion of the particles are treated as a
    random walk
  • Since tracing individual atoms, particles can
    react, this is treated as a Markov process

Concentration of NO, particles compared to
continuum.
10
Particle Tracing Applications
  • Type Ia supernova models
  • Travaglio et al. (2004)
  • Brown et al. (2005)
  • Type II supernova modeling
  • Travaglio et al. (2004)
  • Nagataki et al. (1997)
  • Flash Center
  • validation studies (shock-cylinder)
  • turbulence (BG/L 1,8003 model)
  • turbulent reactive flows (this work)

Tracer particles in Type Ia simulation Travaglio
et al. (2004)
Jordan (2005) Shock-cylinder particles
11
FLASH Modeling Framework
  • The FLASH code
  • Eulerian hydro code
  • Godunov method
  • PPM
  • AMR
  • Highly scalable
  • Multiplatform
  • Efficient, parallel IO
  • Tracer particles

12
FLASH Example K95 Flame Model
  • Simulates Chandrasekhar mass white dwarf
  • Starts with flame at bottom of domain.
  • Evolving RT-unstable deflagration front, followed
    by turbulent mixing
  • Question Can we characterize the complex flows
    of the flame?
  • Answer Yes, use tracer particles

Zhang et al. (2006) Simulation of turbulent
flame. Based on calculation and setup in Khokhlov
(1995)
13
Tracer Particles in FLASH
(v, T, r, Xi, )i-1,j
(v, T, r, Xi, )i-1,j1
(v, T, r, Xi, )i-1,j-1
Solve with Predictor-Corrector Method
(v, T, r, Xi, )i,j1
(v, T, r, Xi, )i,j-1
(v, T, r, Xi, )i,j
(v, T, r, Xi, )i1,j
(v, T, r, Xi, )i1,j-1
(v, T, r, Xi, )i1,j1
Tracer Particle
14
K95particles Turbulent 2-D Flame Model
15
K95particles Turbulent 3-D Flame Model
  • 125,000 total tracer particles
  • The particles were uniformly seeded 100 km above
    the initial position of the flame spread over a
    height of 120 km
  • Examine particles and continuum properties in
    horizontal slabs (specifically temperature and
    density)

16
Temperature Distribution for Complete Set of
Particles
  • Temperature bins are in units of 1X108 K
  • Colors
  • Contours of percentage of particles in a
    temperature bin
  • Black line horizontal average temperature from
    hydro (continuum)

17
Temperature distribution from random samples of
10 and 1 of the particles
18
Density Distribution for Complete Set of Particles
  • Density bins are in units of 2x106 g/cm3
  • Colors
  • Contours of percentage of particles in a
    density bin
  • Black line horizontal average of density from
    hydro (continuum)

19
Summary
  • Post-processing is a necessary element of complex
    hydrodynamic models with nuclear reactions
  • The concept of tracer particles successfully
    implemented in the FLASH code and used in actual
    applications
  • Studies underway towards understanding of
    convergence properties of particle-enabled
    simulations towards continuum limit
  • Proven to work in other applications, there is a
    promise we can put strict error limits on our
    thermonuclear hydro results
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