The First Acoustics Peak CMBR and Cosmic Total Density

Boomerang measured the first peak in CMBR to be at location of $l_D=196\pm 6$,whichexcitesourstronginterestinginit\mathrm{.}Awidelycitedformulais$l_D\simeq 200\Omega_T^{-0.50}$ to estimate the cosmic total density. Weinberg shows it is not correct and should be $l_D\propto {\mathrm{\Omega }}_T^{-1.58}$ near the interest point $({\mathrm{\Omega }}_m,{\mathrm{\Omega }}_{\mathrm{\Lambda }})=(0.3,0.7)$. We show further that it should be $l_D\propto {\mathrm{\Omega }}_T^{-1.43}{\mathrm{\Omega }}_m^{-0.147}$ or ${\mathrm{\Omega }}_T^{-1.92}{\mathrm{\Omega }}_{\mathrm{\Lambda }}^{0.343}$ near the same point in the more veracious sense if we consider the effect from the sound horizon. We draw a contour graph for the peak location, show that the recent data favor to a closed universe with about ${\mathrm{\Omega }}_T\simeq 1.03$. If we insist on obtaining a flat universe, a point $(0.36,0.64)$, i.e., more matter and less vacuum energy, is still possible, which has a more right-side first peak $l_D=208$ in CMBR and a smaller acceleration parameter $-q_0=0.10$ for the $z=0.4$ redshift SNIa.