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The “fully charged” spin-2 field solution is presented. This is an analog of the Coulomb solution in electrodynamics and represents the “non-waving” part of the spin-2 field theory. Basic facts and definitions of the spin–2 field and conformal Yano-Killing tensors are introduced. Application of those two objects provides a precise definition of quasi-local gravitational charge. Next, the 3+1 decomposition leads to the construction of the momentary gravitational charges on initial surface which is applicable for Schwarzschild-like spacetimes.

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