General virial theorem for modified-gravity MOND

الأصل · EN

An important and useful relation is known to hold in two specific MOND theories. It pertains to low-acceleration, isolated systems of pointlike masses, mₚ, at positions rₚ, subject to gravitational forces Fₚ. It reads sumₚ rₚ.Fₚ=-(2/3)(Ga0)¹/²[(∑ₚ mₚ)³/²-∑ₚ mₚ³/²]; a0 is the MOND acceleration constant. Here I show that this relation holds in the nonrelativistic limit of any modified-gravity MOND theory. It follows from only the basic tenets of MOND (as applied to such theories): departure from standard dynamics at accelerations below a0, and space-time scale invariance in the nonrelativistic, low-acceleration limit. This implies space-dilatation invariance of the static, gravitational-field equations, which, in turn, leads to the above point-mass virial relation. Thus, the various MOND predictions and tests based on this relation hold in any modified-gravity MOND theory. Since we do not know that any of the existing MOND theories point in the right direction, it is important to identify such predictions that hold in a much larger class of theories. Among these predictions are the MOND two-body force for arbitrary masses, and a general mass-velocity-dispersion relation of the form sigma²=(2/3)(MGa0)¹/²[1-∑ₚ (mₚ/M)³/²], where M is the total mass.