Table 1: WMAP+SBBN primordial abundances predicted when $\eta = (6.14 \pm 0.25) \times 10^{-10}$ (or $\Omega _{\rm b} h^2 = 0.0224 \pm$ 0.0009; Spergel et al. 2003) is adopted.
Coc et al. (2004) Cyburt (2004) Serpico et al. (2004)

D/H (2.60 $^{+0.19}_{-0.17}) \times 10^{-5}$ (2.55 $^{+0.21}_{-0.20}) \times 10^{-5}$ (2.58 $^{+0.19}_{-0.16}) \times 10^{-5}$

Y $_{\rm P}$ $0.2479\pm0.0004$ $0.2485\pm0.0005$ $0.2479\pm0.0004$

³He/H (1.04 $\pm 0.04)\times 10^{-5}$ (1.01 $\pm 0.07) \times 10^{-5}$ $1.03\pm0.03$

⁷Li/H (4.15 $^{+0.49}_{-0.45}) \times 10^{-10}$ (4.26 $^{+0.91}_{-0.86}\times) 10^{-10}$ (4.6 $^{+0.4}_{-0.4}) \times 10^{-10}$

**Table 1:** *WMAP*+SBBN primordial abundances predicted when $\eta = (6.14 \pm 0.25) \times 10^{-10}$ (or $\Omega _{\rm b} h^2 = 0.0224 \pm$ 0.0009; Spergel et al. 2003) is adopted.
	Coc et al. (2004)	Cyburt (2004)	Serpico et al. (2004)
D/H	(2.60 $^{+0.19}_{-0.17}) \times 10^{-5}$	(2.55 $^{+0.21}_{-0.20}) \times 10^{-5}$	(2.58 $^{+0.19}_{-0.16}) \times 10^{-5}$
Y $_{\rm P}$	$0.2479\pm0.0004$	$0.2485\pm0.0005$	$0.2479\pm0.0004$
³He/H	(1.04 $\pm 0.04)\times 10^{-5}$	(1.01 $\pm 0.07) \times 10^{-5}$	$1.03\pm0.03$
⁷Li/H	(4.15 $^{+0.49}_{-0.45}) \times 10^{-10}$	(4.26 $^{+0.91}_{-0.86}\times) 10^{-10}$	(4.6 $^{+0.4}_{-0.4}) \times 10^{-10}$

Source LaTeX | All tables | In the text

	1 The lithium paradigm
	2 The "Lithium plateau debate''?
	3 Sample selection: a critical analysis of the literature
	4 Stellar parameters: I. Gravity, metallicity, and microturbulence
	5 Stellar parameters. II. The temperature scale and its weaknesses
	6 Our final choice: temperature and data-sample(s)
	7 The lithium abundance
	8 Preliminary results on the mean lithium abundance and the dispersion
	9 Evolutionary status of the stars
	10 The lithium abundance along the plateau for the dwarf stars
	11 The lithium abundance in evolved stars
	12 Duplicity and variability
	13 Stars with extreme Li abundances
	14 Implications for stellar structure and evolution
	15 Summary and conclusions
	References
	Online Material