Nuclei in the Cosmos XI Heidelberg, July 22, 2010 Friedrich Röpke DFG Emmy Noether Junior Research Group Max-Planck-Institut für Astrophysik, Garching,

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Presentation transcript:

Nuclei in the Cosmos XI Heidelberg, July 22, 2010 Friedrich Röpke DFG Emmy Noether Junior Research Group Max-Planck-Institut für Astrophysik, Garching, Germany W. Hillebrandt, S. Woosley, S. Sim, I. Seitenzahl, D. Kasen, A. Ruiter, P. Mazzali, M. Kromer, R. Pakmor, M. Fink, F. Ciaraldi-Schoolmann, P. Edelmann Multi-dimensional models of Type Ia supernova explosions

NIC XI 2010Friedrich Röpke, MPA Modeling sequence progenitor system explosion nuclear postprocessing radiation transfer/ synthetic observables

NIC XI 2010Friedrich Röpke, MPA Modeling sequence progenitor system explosion nuclear postprocessing radiation transfer/ synthetic observables see Ivo Seitenzahl's poster #67

NIC XI 2010Friedrich Röpke, MPA Modeling sequence population synthesis/ SN Ia rates progenitor system explosion nuclear postprocessing radiation transfer/ synthetic observables SN Ia observations

NIC XI 2010Friedrich Röpke, MPA Violent WD-WD mergers (Pakmor+, 2010) ► inspiral and merger: 3D SPH code (GADGET3) ► 2 WDs: M 1 = M 2 = 0.9M ⊙

NIC XI 2010Friedrich Röpke, MPA Violent WD-WD mergers ► explosion: 3D MPA SN Ia code (LEAFS) ► detonation after T>2.8 GK ρ = g/cm 3 Ejecta mass: 1.8 M ⊙ 0.1 M ⊙ of 56 Ni 0.1 M ⊙ iron group elements 1.1 M ⊙ intermediate mass elements 0.5 M ⊙ oxygen 0.1 M ⊙ carbon

NIC XI 2010Friedrich Röpke, MPA Violent WD-WD mergers good agreement with observed sub-luminous SNe Ia (“1991bg-like” objects) also supported by population synthesis ► radiation transfer: 3D monte carlo (ARTIS) light curves spectrum

NIC XI 2010Friedrich Röpke, MPA SN Ia sub-classes and rates ► volume-limited (Li+, 2010) Normal70% 91bg18% 91T9% 02cx3%

NIC XI 2010Friedrich Röpke, MPA SN Ia sub-classes and rates ► volume-limited (Li+, 2010) Normal70% 91bg18% 91T9% 02cx3% violent (q~1) WD-WD mergers?

NIC XI 2010Friedrich Röpke, MPA accretion from (normal) binary companion star M Ch model C+O WD M ~ M Ch

NIC XI 2010Friedrich Röpke, MPA Turbulent deflagrations t = sec

NIC XI 2010Friedrich Röpke, MPA Turbulent deflagrations t = sec

NIC XI 2010Friedrich Röpke, MPA Turbulent deflagrations t = sec

NIC XI 2010Friedrich Röpke, MPA Turbulent deflagrations t = sec

NIC XI 2010Friedrich Röpke, MPA Turbulent deflagrations t = sec

NIC XI 2010Friedrich Röpke, MPA Turbulent deflagrations t = sec

NIC XI 2010Friedrich Röpke, MPA Turbulent deflagrations t = sec asymtotic kinetic energy of explosion: ~ 0.58 B ► faint, low energy event ► consistent with peculiar sub-class? M( 56 Ni) ~ 0.32 M ⊙ M(IGE) ~ 0.55 M ⊙ M(IME) ~ 0.16 M ⊙ M(C) ~ 0.31 M ⊙ M(O) ~ 0.39 M ⊙ composition strongly mixed

NIC XI 2010Friedrich Röpke, MPA Turbulent deflagrations SN 2005hk (observation) model spectrum (deflagration simulation) ► radiation transfer: ► preliminary, low resolution ► (Kromer & Sim)

NIC XI 2010Friedrich Röpke, MPA pure (turbulent) deflagrations? SN Ia sub-classes and rates ► volume-limited (Li+, 2010) Normal70% 91bg18% 91T9% 02cx3% violent (q~1) WD-WD mergers?

NIC XI 2010Friedrich Röpke, MPA Delayed detonation model ► detonation of M Ch WD after pre-expansion in initial deflagration phase (Khokhlov 1991) ► requires deflagration-to-detonation transition (DDT) of flame ► probably possible at low densitites (late phase of explosion) if turbulence still strong enough (FR, 2007; Woosley 2007; Woosley+, 2009) FR & Niemeyer, 2007 Mazzali et al., 2007

NIC XI 2010Friedrich Röpke, MPA Synthetic observables ► radiation transfer for 44 2D explosion models (Kasen+, 2009) compared with SN 2003du

NIC XI 2010Friedrich Röpke, MPA delayed detonations? not supported by population synthesis pure (turbulent) deflagrations? SN Ia sub-classes and rates ► volume-limited (Li+, 2010) Normal70% 91bg18% 91T9% 02cx3% violent (q~1) WD-WD mergers?

NIC XI 2010Friedrich Röpke, MPA Sub-M Ch explosions Model 2 ► explosion simulation (Fink+, 2007, 2010) ► minimum He-shell masses (Bildsten+, 2007) ► He shell C+ O core

NIC XI 2010Friedrich Röpke, MPA Sub-M Ch explosions Model 2 ► explosion simulation: (Fink+, 2007, 2010) ► minimum He-shell masses (Bildsten+, 2007) ► C+O core detonation triggers robustly ►

NIC XI 2010Friedrich Röpke, MPA Sub-M Ch explosions ► radiation transfer (Kromer+, 2010) ► iron group elements produced in He shell detonation (Ti, Cr, etc) may be problematic flux re-distribution due to Cr, Ti absorption

NIC XI 2010Friedrich Röpke, MPA Sub-M Ch explosions ► changing C abundance in He shell may help (Kromer+, 2010) ► bare sub-M ch detonations produce promising results (Sim+, 2010) 33% carbon-enriched He shell

NIC XI 2010Friedrich Röpke, MPA delayed detonations? or sub-M Ch detonations? (consistent with population synthesis) pure (turbulent) deflagrations? SN Ia sub-classes and rates ► volume-limited (Li+, 2010) Normal70% 91bg18% 91T9% 02cx3% violent (q~1) WD-WD mergers?