  Although double-peaked narrow emission-line galaxies have been studied
extensively in the past years, only a few are reported with the green pea
galaxies (GPs). Here we present our discovery of five GPs with double-peaked
narrow [OIII] emission lines, referred to as DPGPs, selected from the LAMOST
and SDSS spectroscopic surveys. We find that these five DPGPs have blueshifted
narrow components more prominent than the redshifted components, with velocity
offsets of [OIII]$\lambda$5007 lines ranging from 306 to 518 $\rm km\, s^{-1}$
and full widths at half maximums (FWHMs) of individual components ranging from
263 to 441 $\rm km\, s^{-1}$. By analyzing the spectra and the spectral energy
distributions (SEDs), we find that they have larger metallicities and stellar
masses compared with other GPs. The H$\alpha$ line width, emission-line
diagnostic, mid-infrared color, radio emission, and SED fitting provide
evidence of the AGN activities in these DPGPs. They have the same spectral
properties of Type 2 quasars. Furthermore, we discuss the possible nature of
the double-peaked narrow emission-line profiles of these DPGPs and find that
they are more likely to be dual AGN. These DPGP galaxies are ideal laboratories
for exploring the growth mode of AGN in the extremely luminous emission-line
galaxies, the co-evolution between AGN and host galaxies, and the evolution of
high-redshift galaxies in the early Universe.
