  In this paper, we considered the interaction neutrino with three scalar
fields(phantom, quintessence, and quintom model) and put constraints on the
total mass of neutrinos, and comparison the interaction constant $ \beta $ in
these models. The data were used in this paper are supernova type Ia(pantheon
catalog), CMB and BAO data. For each model, we first investigate the results
obtained from Pantheon data, then survey the CMB and BAO data, and finally, the
total data from these catalogs. It seems that using a combination of data
produces more favorable results. For combination data, we find that the total
mass of neutrino $\sum m_{\nu}< 0.121 eV$ $(95\% $ Confidence Level (C.L.) for
quintom model and $\sum m_{\nu}< 0.19 eV$ $(95\% $ Confidence Level (C.L.) for
phantom model and $\sum m_{\nu}< 0.124 eV$ $(95\% $ Confidence Level (C.L.) for
quintessence model. These results are in good agreement with the results of
Planck 2018 where the limit of the total neutrino mass is $\sum m_{\nu}<0.12
eV$ ($95\%$ C.L., TT, TE, EE+lowE+lensing+BAO)
