We present a theoretical framework on non-local classical field theory using fractional integrodifferential operators. Due to the lack of easily manageable symmetries in traditional fractional calculus and the difficulties that arise in the formalism of multi-fractional calculus over $\mathbb{ R}^{ \text{ D}}$ space, we introduce a set of new fractional operators over the $\mathbb{ S}^3 \times \mathbb{ R}^1$ space. The redefined fractional integral operator results in the non-trivial measure canonically, and they can account for the spacetime symmetries for the underlying space $\mathbb{ S}^3 \times \mathbb{ R}^1$ with the Lorentzian signature $(+, -, -, -, -)$. We conclude that the field equation for the non-local classical field can be obtained as the consequence of the optimisation of the action by employing the non-local variations in the field after defining the non-local Lagrangian density, namely, $\mathcal{ L}(\phi_{ a}\left(x\right), \mathbb{ \eth}^\alpha \phi_{ a}\left(x\right))$, as the function of the symmetric fractional derivative of the field, e.g. in the context of the kinetic term, and the field itself.
Categories: physics.class-ph hep-th math-ph math.FA math.GR math.MP math.OA