  We study the possibility of texture zeros in Majorana light neutrino mass
matrix in the light of dark large mixing angle (DLMA) solution to solar
neutrino problem where solar mixing angle ($\sin^2{\theta_{12}}\simeq 0.7 $)
lies in the second octant instead of first octant in standard large mixing
angle (LMA) scenario ($\sin^2{\theta_{12}}\simeq 0.3 $). In three neutrino
scenario, we find that LMA and DLMA solutions lead to different set of allowed
and disallowed textures with one and two zeros. While being consistent with
existing bounds from neutrino oscillation data, neutrinoless double beta decay
and cosmology these allowed textures also lead to interesting correlations
among light neutrino parameters which can distinguish LMA from DLMA solution.
We also check the implications for texture zeros in $3+1$ neutrino scenario
using both LMA and DLMA solutions. While LMA and DLMA solutions do not play
decisive role in ruling out texture zeros in this case, they do give rise to
distinct predictions and correlations between light neutrino parameters.
