@@ -430,19 +430,19 @@ constexpr double Q_HYDROGEN_BURNING = 6.4E18 * MSOL_TO_G / (
430430constexpr double L0_RITTER_HIGH_Z = 1995262.3 ; // Luminosity constant which depends on metallicity in Ritter 1999, eq 10
431431constexpr double L0_RITTER_LOW_Z = 31622.8 ;
432432constexpr double WD_HE_SHELL_MCRIT_DETONATION = 0.05 ; // Minimum shell mass of He for detonation. Should be composed of helium (so, exclude burnt material), but not implemented yet. Ruiter+ 2014.
433- constexpr double WD_LOG_MT_LIMIT_PIERSANTI_RG_SS_0 = -6.84 ;
434- constexpr double WD_LOG_MT_LIMIT_PIERSANTI_RG_SS_1 = 1.349 ;
435- constexpr double WD_LOG_MT_LIMIT_PIERSANTI_SS_MF_0 = -8.115 ;
436- constexpr double WD_LOG_MT_LIMIT_PIERSANTI_SS_MF_1 = 2.29 ;
437- constexpr double WD_LOG_MT_LIMIT_PIERSANTI_SF_Dt_0 = -8.313 ;
438- constexpr double WD_LOG_MT_LIMIT_PIERSANTI_SF_Dt_1 = 1.018 ;
439- constexpr double WD_LOG_MT_LIMIT_NOMOTO_REDGIANT_0 = -8.3302 ;
440- constexpr double WD_LOG_MT_LIMIT_NOMOTO_REDGIANT_1 = 2.8825 ;
441- constexpr double WD_LOG_MT_LIMIT_NOMOTO_REDGIANT_2 = -0.9802 ;
442- constexpr double WD_LOG_MT_LIMIT_NOMOTO_STABLE_0 = -9.2176 ;
443- constexpr double WD_LOG_MT_LIMIT_NOMOTO_STABLE_1 = 3.5732 ;
444- constexpr double WD_LOG_MT_LIMIT_NOMOTO_STABLE_2 = -1.2138 ;
445- constexpr double WD_MP = 5.7E-4 ;
433+ constexpr double WD_LOG_MT_LIMIT_PIERSANTI_RG_SS_0 = -6.84 ; // Constant from Piersanti et al. 2014 see Table A1
434+ constexpr double WD_LOG_MT_LIMIT_PIERSANTI_RG_SS_1 = 1.349 ; // Constant from Piersanti et al. 2014 see Table A1
435+ constexpr double WD_LOG_MT_LIMIT_PIERSANTI_SS_MF_0 = -8.115 ; // Constant from Piersanti et al. 2014 see Table A1
436+ constexpr double WD_LOG_MT_LIMIT_PIERSANTI_SS_MF_1 = 2.29 ; // Constant from Piersanti et al. 2014 see Table A1
437+ constexpr double WD_LOG_MT_LIMIT_PIERSANTI_SF_Dt_0 = -8.313 ; // Constant from Piersanti et al. 2014 see Table A1
438+ constexpr double WD_LOG_MT_LIMIT_PIERSANTI_SF_Dt_1 = 1.018 ; // Constant from Piersanti et al. 2014 see Table A1
439+ constexpr double WD_LOG_MT_LIMIT_NOMOTO_REDGIANT_0 = -8.3302 ; // Quadratic fit to results from Nomoto et al. 2007 Table 5
440+ constexpr double WD_LOG_MT_LIMIT_NOMOTO_REDGIANT_1 = 2.8825 ; // Quadratic fit to results from Nomoto et al. 2007 Table 5
441+ constexpr double WD_LOG_MT_LIMIT_NOMOTO_REDGIANT_2 = -0.9802 ; // Quadratic fit to results from Nomoto et al. 2007 Table 5
442+ constexpr double WD_LOG_MT_LIMIT_NOMOTO_STABLE_0 = -9.2176 ; // Quadratic fit to results from Nomoto et al. 2007 Table 5
443+ constexpr double WD_LOG_MT_LIMIT_NOMOTO_STABLE_1 = 3.5732 ; // Quadratic fit to results from Nomoto et al. 2007 Table 5
444+ constexpr double WD_LOG_MT_LIMIT_NOMOTO_STABLE_2 = -1.2138 ; // Quadratic fit to results from Nomoto et al. 2007 Table 5
445+ constexpr double WD_MP = 5.7E-4 ; // White dwarf mass parameter determining where mass-radius relation changes for low-mass white dwarfs
446446constexpr double WD_BELCZYNSKI_SN_CONSTANT = 1.34 ; // Constant from Eq 62, Belczynski+ 2008
447447constexpr double WD_BELCZYNSKI_SN_LINEAR = 4.0E8 ; // Linear term factor from Eq 62, Belczynski+ 2008
448448constexpr double WD_BELCZYNSKI_IMMEDIATE_FLASH = 1.64E-6 ; // Accretion limit from eq 61, Belczynski+ 2008.
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