Spinless Salpeter equation non-locality

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The discussion centers on the Spinless Salpeter equation, which generalizes the Schrödinger equation to a relativistic framework using the Hamiltonian form H = T + V, where T = √(p² + m²) and V(𝑥) = 0. The participants explore the non-locality of this equation, suggesting that the non-local nature can be observed through the propagator or by analyzing the Lagrangian, which includes terms that are not solely functions of the fields or their derivatives. The infinite series expansion of the kinetic energy operator indicates that higher-order derivatives influence the properties of distant points, confirming the non-local characteristics of the theory.

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ChrisVer
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A straightforward attempt to generalize the Schrödinger equation to a relativistic equation, is obtained by taking the Eigenvector/value equation:
H |a_k> = E_k |a_k>

with a hamiltonian of the form H= T+V,

In the relativistic case we have T=\sqrt{p^2+m^2} , and taking also (for my purposes) the case that V(\vec{x})=0 we get the Spinless Salpeter equation:

\sqrt{p^2 +m^2} |a_k> = E_k |a_k>

(http://arxiv.org/abs/hep-ph/9807342 , below eq.1)

I was wondering, how can someone see immediately that this form of the Hamiltonian is non-local? I think that someone sees this by looking at the propagator? Or does someone get this by writting the Lagrangian and seeing it's non-local (contains terms that are not functions of the fields or their derivatives)?
 
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The point is that you can taylor expand the kinetic energy operator w.r.t. p and it will be an infinite series. But the momentum operator in that series is a derivative operator and that means that operator(T) is in fact differentiating to infinite order. But the higher the derivative, the more points you need and those points get farther from the point your considering which, for an infinite order differentiation, means the points very very far from a point affect the properties of that point and so the theory is non-local.
 

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