Effects of helium enrichment in globular clusters - I. Theoretical plane with PGPUC stellar evolution code

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Table 2

Physical inputs included in compared SECs.

	Princeton-	Princeton-	Victoria-	BaSTI	GARSTEC	STAREVOL	PADOVA
Physics	Goddard	Goddard-PUC	Regina
	(PG)	(PGPUC)

Opacity Tables
High Temp	OPAL92	OPAL96	OPAL92	OPAL96	OPAL96	OPAL96	OPAL96
Low Temp	B94	F05	AF94	AF94	F05	AF94	AF94
Conductive	HL69+C70	C07	HL69	P99	I83	HL69	I83

Neutrino
Energy Loss	H94	H94	I96	H94	H94	I96	H94

Reaction Rates
¹²C(α, γ)¹⁶O	WW93	K02	BP92	K02	K02	NACRE	WW93
Other	CF88	NACRE	BP92	NACRE	NACRE	NACRE	CF88

Equation of
State	S73	FreeEOS	VB00	FreeEOS	FreeEOS	P95	M90+G96

Boundary
Condition	KS66	Cat07 (our Eq. (1))	KS66	KS66	KS66	KS66	KS66

Mass Loss	R75	SC05	R75	R75	R75	R75	R75

α_MLT (GN93)	1.845	1.886	1.890	1.913	1.739	1.853	1.68(GN98)

Notes. Chemical compositions: GN93 (Z/X = 0.0244, Grevesse & Noels 1993), GS98 (Z/X = 0.0231, Grevesse & Sauval 1998).

References. AF94 (Alexander & Ferguson 1994), BP92 (Bahcall & Pinsonneault 1992), B94 (Bell 1994, unpublished), C70 (Canuto 1970), C07 (Cassisi et al. 2007), Cat07 (Catelan 2007), CF88 (Caughlan & Fowler 1988), FreeEOS (Irwin 2007), F05 (Ferguson et al. 2005), G96 (Girardi et al. 1996), HL69 (Hubbard & Lampe 1969), H94 (Haft et al. 1994), I83 (Itoh et al. 1984), I96 (Itoh et al. 1996), K02 (Kunz et al. 2002), KS66 (Krishna Swamy 1966), M90 (Mihalas et al. 1990), NACRE (Angulo et al. 1999), OPAL92 (Rogers & Iglesias 1992), OPAL96 (Iglesias & Rogers 1996), P95 (Pols et al. 1995), P99 (Potekhin 1999), R75 (Reimers 1975), S73 (Sweigart 1973), SC05 (Schröder & Cuntz 2005), VB00 (VandenBerg et al. 2000), WW93 (Weaver & Woosley 1993).

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