Dark matter is simply zero point energy with positive pressure w < - 1/3 using Einstein's theory with an additional "Shipov" torsion field so that Einstein's "constant" Λzpf is a local variable scalar field in

Guv + Λzpfguv = 0 exotic vacuum eq.

I am saying on-mass-shell "dark matter particles" is a wrong idea - it's qualitatively, wrong. That is, dark matter is an off-mass-shell exotic vacuum effect.

That is all we need in Newtonian limit of Einstein's GR, to keep it simple is

Laplacian of V(Newton) = 4pi(G/c^2)(Energy Density)(1 + 3w)

With w < -1/3

Dark matter is (Energy Density) < 0 (fermion dominated in 3+1 ST)

Dark energy is (Energy Density) > 0 (boson dominated)

where for ZPF

w = -1 on the nose

The sign of the ZPF energy density at a given place-time/scale is controlled by the vacuum ODLRO field.