On the Energy-Momentum Tensor of Bopp-Type Non-Local Field
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Expanding the characteristic function ε(x)in the Lagrangian in derivatives of δ(x)and applying the variation principle of general relativity, we obtained the symmetrical energy-momentum tensors for the Bopp-type non-local fields. They are free from the defects accompanying the expressions proposed by Bopp and Heisenberg and can be ragarded as the most natural extension of the local fields.
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- On the Energy-Momentum Tensor of Bopp-Type Non-Local Field