  Big Bang Nucleosynthesis (BBN) is an important stage of a homogeneous and
isotropic expanding universe. The results of calculation of the synthesis of
light elements during this epoch can then be compared with the abundances of
the light elements. The theoretical calculation of the BBN model depends on the
initial conditions of the early universe and reaction cross sections measured
by the nuclear physics experiment. Recently, an update of the NACRE (Nuclear
Astrophysics Compilation of REactions) database is presented. This improved
compilation comprises thermonuclear reaction rates for 34 two-body reactions on
light nuclides (fifteen are particle transfer reactions and nineteen are
radiative capture reactions). In this work, we calculate the BBN abundances by
using these updated thermonuclear reaction rates in the framework of the code
\texttt{AlterBBN}. Our results suggest that the new numerical result of the
primordial Lithium abundance is 7.1 percent larger than the previous
calculation.
