  The full data set of the Daya Bay reactor neutrino experiment is used to
probe the effect of the charged current non-standard interactions (CC-NSI) on
neutrino oscillation experiments. Two different approaches are applied and
constraints on the corresponding CC-NSI parameters are obtained with the
neutrino flux taken from the Huber-Mueller model with a $5\%$ uncertainty. For
the quantum mechanics-based approach (QM-NSI), the constraints on the CC-NSI
parameters $\epsilon_{e\alpha}$ and $\epsilon_{e\alpha}^{s}$ are extracted with
and without the assumption that the effects of the new physics are the same in
the production and detection processes, respectively. The approach based on the
weak effective field theory (WEFT-NSI) deals with four types of CC-NSI
represented by the parameters $[\varepsilon_{X}]_{e\alpha}$. For both
approaches, the results for the CC-NSI parameters are shown for cases with
various fixed values of the CC-NSI and the Dirac CP-violating phases, and when
they are allowed to vary freely. We find that constraints on the QM-NSI
parameters $\epsilon_{e\alpha}$ and $\epsilon_{e\alpha}^{s}$ from the Daya Bay
experiment alone can reach the order $\mathcal{O}(0.01)$ for the former and
$\mathcal{O}(0.1)$ for the latter, while for WEFT-NSI parameters
$[\varepsilon_{X}]_{e\alpha}$, we obtain $\mathcal{O}(0.1)$ for both cases.
