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The Hubble tension arises when comparing two different methods of determining$H_{0}$: one based on local measurements within our cosmic vicinity and anotherderived from observations of the early universe, specifically the cosmicmicrowave background (CMB). In this article, we investigated the Hubble tensionby coupling neutrinos to Rastall gravity. We estimate the $H_{0}$ in both Ealyand the Local universe. The data were use in this paper are CMB(plikTTTEEE+lowl+lowE), and Lensing. BAO, CC, and Pantheon + Analysis. In theEarly universe for (CMB + Lensing) the $H_{0}$ value is $69.2 \pm 1.52$ and forthe Local universe (CC + BAO + Pantheon + Analysis) is $70.14 \pm 0.98$. Thereis a 0.54$\sigma$ deviation in comparing the $H_{0}$ value in the Early and theLocal universe. As a result, it can be concluded that the Hubble tension may beresolved.

Generalized Rastall Gravity coupled with neutrinos could solve the Hubble Tension