jms4 said:
Summary: Can we increase an object's gravitational force by adding energy? as energy is related to mass, which is related to gravity?
like a shot bullet or arrow has negligibly more gravitational force than a still bullet or arrow?,
this is what I'm asking,
m=e/c^2
F=Gm/r^2,
thus, F=Ge/(c^2*r^2)
where e represents the (mass of the object + energy added to the object)
thus more the energy, more the gravitational force, even though it would be negligible?
I believe one of the best answers to the intent of this question is the Olson and Guarino paper, Olson, D.W.; Guarino, R. C. (1985). "Measuring the active gravitational mass of a moving object".
Gravitation in general relativity has aspects that are not well modeled solely by the idea of force. Because you are asking this question in a GR forum, I am assuming you are interested in what General relativity predicts. Because you quote only Newtonian formula, and because you are asking about it in terms of "force", I am assuming that you are not familiar with the relevant formula of General relativity. This is not surprising, it's a complex theory.
An approach that does work, as described in the paper, is to consider a space-time that is basically flat, consisting only of a swarm of test particles that are initially relativity at rest. What happens during the flyby according to GR is hard to describe in familiar Newtonian terms, because the presence of the moving mass distorts the fabric of space-time. However, both before and after the relativistic flyby, space-time is flat and has the familiar spatial geometry. The space-time geometry may also be familiar, it's the flat space-time geometry of special relativity.
We can observe the relative velocities between particles in the cloud of test particles before and after the flyby. When we do so, we find the velocities s of the test particles are perturbed. In particular, there is a change in the relative velocities between the test particles. We can analyze this pertubation in GR and in Newtonian physics, though neither result is likely to be intuitively familiar, not even the Newtonian one.
The result, as described in the abstract of Olson & Guarnio's paper, is:
Olson et al said:
If a heavy object with rest mass M moves past you with a velocity comparable to the speed of light, you will be attracted gravitationally towards its path as though it had an increased mass. If the relativistic increase in active gravitational mass is measured by the transverse (and longitudinal) velocities which such a moving mass induces in test particles initially at rest near its path, then we find, with this definition, that Mrel=γ(1+β2)M. Therefore, in the ultrarelativistic limit, the active gravitational mass of a moving body, measured in this way, is not γM but is approximately 2γM.
It may be difficult to get a hold of the full text of the Olson & Guranio paper, but the abstract is easy enough to find. The interesting result is that the moving mass has even more impact on the velocities in the cloud of test particles than the relativistic factor of gamma - for an ultra-relativistic flyby, nearly twice as much impact.
The factor of two that we see in the Olson & Guarnio thought experiment is similar to the factor of two we see in the extra deflection of light by massive objects, one of the first experimental tests of General Relativity.
The basic idea of the Olson & Guarino experiment would also approximate such things as the pertubations of orbits of planets in the solar system by the flyby of a relativistic star. This works mainly because gravity in the solar system is weak enough that one can get good approximations of the orbital motions from Newtonian theory.