Semi-classical models including Newton-Schrödinger, its Bohmian analogue, and the Döner-Grossardt interpolator produce no gravitationally induced entanglement, unlike the standard Newtonian potential.
Correlations and signaling in the Schr¨ odinger–Newton model
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Absence of gravitationally induced entanglement in certain semi-classical theories of gravity
Semi-classical models including Newton-Schrödinger, its Bohmian analogue, and the Döner-Grossardt interpolator produce no gravitationally induced entanglement, unlike the standard Newtonian potential.