Table B.1
SNIa and SNcc yield models, taken from literature and used in this work.
Category | Name | Reference | Remarks |
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SNIa | |||
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Classical | W7 | 1 | Deflagration, ρ9 = 2.12 |
Classical | W70 | 1 | Deflagration, ρ9 = 2.12, zero initial metallicity |
Classical | WDD1 | 1 | Delayed-detonation, ρ9 = 2.12, ρT,7 = 1.7 |
Classical | WDD2 | 1 | Delayed-detonation, ρ9 = 2.12, ρT,7 = 2.2 |
Classical | WDD3 | 1 | Delayed-detonation, ρ9 = 2.12, ρT,7 = 3.0 |
Classical | CDD1 | 1 | Delayed-detonation, ρ9 = 1.37, ρT,7 = 1.7 |
Classical | CDD2 | 1 | Delayed-detonation, ρ9 = 1.37, ρT,7 = 2.2 |
Bravo | DDTa | 2, 3 | Delayed-detonation, fits the Tycho SNR, ρT,7 = 3.9 |
Bravo | DDTc | 2, 3 | Delayed-detonation, fits the Tycho SNR, ρT,7 = 2.2 |
Bravo | DDTe | 2, 3 | Delayed-detonation, fits the Tycho SNR, ρT,7 = 1.3 |
Ca-rich gap | CO.45HE.2 | 4 | Ca-rich SNe, MCO = 0.45, MHe = 0.2 |
Ca-rich gap | CO.5HE.2 | 4 | Ca-rich SNe, MCO = 0.5, MHe = 0.2 |
Ca-rich gap | CO.5HE.15 | 4 | Ca-rich SNe, MCO = 0.5, MHe = 0.15 |
Ca-rich gap | CO.5HE.2N.02 | 4 | Ca-rich SNe, MCO = 0.5, MHe = 0.2, 2% N in He layer |
Ca-rich gap | CO.5HE.2C.03 | 4 | Ca-rich SNe, MCO = 0.5, MHe = 0.2, 30% mixing core-He layer |
Ca-rich gap | CO.5HE.3 | 4 | Ca-rich SNe, MCO = 0.5, MHe = 0.3 |
Ca-rich gap | CO.55HE.2 | 4 | Ca-rich SNe, MCO = 0.55, MHe = 0.2 |
Ca-rich gap | CO.6HE.2 | 4 | Ca-rich SNe, MCO = 0.6, MHe = 0.2 |
2D | C-DEF | 5 | 2D deflagration, ρ9 = 2.9 |
2D | C-DDT | 5 | 2D delayed-detonation, ρ9 = 2.9, ρT,7 = 1.0 |
2D | O-DDT | 5 | 2D delayed-detonation, ρ9 = 2.9, ρT,7 = 1.0, off-centre ignition |
3D | N1def | 6 | 3D deflagration, ρ9 = 2.9, 1 ignition spot |
3D | N3def | 6 | 3D deflagration, ρ9 = 2.9, 3 ignition spots |
3D | N5def | 6 | 3D deflagration, ρ9 = 2.9, 5 ignition spots |
3D | N10def | 6 | 3D deflagration, ρ9 = 2.9, 10 ignition spots |
3D | N20def | 6 | 3D deflagration, ρ9 = 2.9, 20 ignition spots |
3D | N40def | 6 | 3D deflagration, ρ9 = 2.9, 40 ignition spots |
3D | N100Ldef | 6 | 3D deflagration, ρ9 = 1.0, 100 ignition spots |
3D | N100def | 6 | 3D deflagration, ρ9 = 2.9, 100 ignition spots |
3D | N100Hdef | 6 | 3D deflagration, ρ9 = 5.5, 100 ignition spots |
3D | N150def | 6 | 3D deflagration, ρ9 = 2.9, 150 ignition spots |
3D | N200def | 6 | 3D deflagration, ρ9 = 2.9, 200 ignition spots |
3D | N300Cdef | 6 | 3D deflagration, ρ9 = 2.9, 300 centred ignition spots |
3D | N1600def | 6 | 3D deflagration, ρ9 = 2.9, 1600 ignition spots |
3D | N1600Cdef | 6 | 3D deflagration, ρ9 = 2.9, 1600 centred ignition spots |
3D | N1 | 7 | 3D delayed-detonation, ρ9 = 2.9, 1 ignition spot |
3D | N3 | 7 | 3D delayed-detonation, ρ9 = 2.9, 3 ignition spots |
3D | N5 | 7 | 3D delayed-detonation, ρ9 = 2.9, 5 ignition spots |
3D | N10 | 7 | 3D delayed-detonation, ρ9 = 2.9, 10 ignition spots |
3D | N20 | 7 | 3D delayed-detonation, ρ9 = 2.9, 20 ignition spots |
3D | N40 | 7 | 3D delayed-detonation, ρ9 = 2.9, 40 ignition spots |
3D | N100L | 7 | 3D delayed-detonation, ρ9 = 1.0, 100 ignition spots |
3D | N100 | 7 | 3D delayed-detonation, ρ9 = 2.9, 100 ignition spots |
3D | N100H | 7 | 3D delayed-detonation, ρ9 = 5.5, 100 ignition spots |
3D | N150 | 7 | 3D delayed-detonation, ρ9 = 2.9, 150 ignition spots |
3D | N200 | 7 | 3D delayed-detonation, ρ9 = 2.9, 200 ignition spots |
3D | N300C | 7 | 3D delayed-detonation, ρ9 = 2.9, 300 centred ignition spots |
3D | N1600 | 7 | 3D delayed-detonation, ρ9 = 2.9, 1600 ignition spots |
3D | N1600C | 7 | 3D delayed-detonation, ρ9 = 2.9, 1600 centred ignition spots |
Sub-MCh | 0.9_0.9 | 8 | WD-WD violent merger, MWD ≃ 0.9, ρ9 = 1.4 × 10-2 |
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SNcc | |||
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Nomoto | Z0 | 9,10,11 | Zinit = 0 |
Nomoto | Z0_cut | 9,10,11 | Zinit = 0, restricted to ≤40 M⊙ |
Nomoto | Z0.001 | 9,10,11 | Zinit = 0.001 |
Nomoto | Z0.004 | 9,10,11 | Zinit = 0.004 |
Nomoto | Z0.008 | 11 | Zinit = 0.008 |
Nomoto | Z0.02 | 9,10,11 | Zinit = 0.02 |
Nomoto | Z0+PISNe | 9,10,11,12 | Zinit = 0, incl. contribution from PISNe (up to 300 M⊙) |
HW | Z0+PISNe | 13,14 | Zinit = 0, incl. contribution from PISNe (up to 260 M⊙) |
Notes. The inner core densities ρ9 are given in units of 109 g/cm3. The transitional deflagration-to-detonation densities ρT,7 are given in units of 107 g/cm3. The masses of the CO core and of the He layer (respectively MCO and MHe, “Ca-rich gap” models), and the mass of each of the two merging WD (MWD, “DD channel” model) are given in units of M⊙.
Reference. (1) Iwamoto et al. (1999); (2) Badenes et al. (2003); (3) Badenes et al. (2006); (4) Waldman et al. (2011); (5) Maeda et al. (2010); (6) Fink et al. (2014); (7) Seitenzahl et al. (2013b); (8) Pakmor et al. (2010); (9) Nomoto et al. (2006); (10) Kobayashi et al. (2006); (11) Nomoto et al. (2013); (12) Umeda & Nomoto (2002); (13) Heger & Woosley (2002); (14) Heger & Woosley (2010).
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