Where is the proof for your statement: "The outward particle always has the positive energy."
I suggest you look up with work of Hawking. If you want something a little more digestable, try the last few chapters
here. It's the lecture notes of a course an ex-student of Hawking gives and which Hawking used to give himself.
It basically comes down to how the space-time alters the 4-momentum vector of the particles. If you don't understand the Hawking process, look up the Penrose process. An infalling particle has positive energy but when it enters the ergosphere the space-time changes signature so that the energy goes from E to -E, because $$g_{ab} \sim \textrm{diag}(1,-1,1,1)$$. This is a classical process which allows energy to be at least partially extracted from a rotating black hole.
Thus, a MBH, once created, would always grow larger.
Even if the particles weren't always having postive energy, the net flux of energy be outwards, once the black hole is hotter than the surrounding space, or else what does it mean to give it temperature? If an object is hotter than it's surrounding region it will cool down, losing energy, as per thermodynamics.
So if a black hole is hotter than the surrounding space, it must be pumping energy out to cool itself down.
It would be accelerated away from the singularity, due to its 'negative mass' ['negative energy']
Show your calculations. Don't just do something like "-m put into $$F = \frac{GMm}{r^{2}}$$, I want the full blown relativistic workings. At least comparable, on the level of technical detail as the lecture notes I just linked to.
Besides, I didn't say negative mass, I said negative energy. Obviously you need a quick schooling on relativistic principles again...
Define a 4-momentum vector $$P^{\mu} = (E,\mathbf{p})$$ where E is the energy of the particle with said 4-momentum and
p is it's 3-momentum. We take out metric signature to be (-1,1,1,1). By definition, $$-m^{2} \equiv g_{\mu\nu}p^{\mu}p^{\nu}$$. In flat space-time or normal coordinates, this becomes $$-m^{2} \equiv \eta_{\mu\nu}p^{\mu}p^{\nu} = -p^{0}p^{0}+|\mathbf{p}|^{2}$$. Rearranging and you have the standard formula $$E^{2} = m^{2}+|\mathbf{p}|^{2}$$.
But in a black hole you have something different. For a start, within the ergosphere you have a signature which is (1,-1,1,1), so your formula becomes $$-m^{2} = E^{2}-p_{1}^{2}+p_{2}^{2}+p_{3}^{2}$$. The relationship between energy and matter is different. Slightly arm wavey, the 4-momentum expression used in the equations for computing energy (which I can provide, but if you have a copy of Wald it's explained in there) is now effectively $$(-E,-p_{1},p_{2},p_{3})$$. The sign on the mass term hasn't changed, it's still $$-m^{2}$$ but the sign on the energy has changed.
As explained in those lecture notes and pretty much any graduate textbook on black holes (like Wald), if you have a spacially varying $$g_{00}$$ term (equivalent to come kind of potential) in the black hole like system, then provided there's a few basic things true, like the potential gets weaker as you further away and the strong energy condition, then the effect on the energy of virtual particles is that they are always boosted into a frame which makes them have positive energy when they are emitted.
Even black holes which don't have ergospheres have the same effect, just you cannot tell. The metric signature changes on the event horizon for non-rotating black holes and changes the sign of the energy of the infalling particles.
Can you prove it is true?
I can demonstrate that your grasp of relativity is worse than someone who has sat a couple of courses on it in university and doesn't even do research into it. Considering the time and effort you put into this, I am
staggered you are not able to provide multiple sources for your claims and demonstrate your claims using detailed calculations. Instead, I constantly find you unable to back up your claims with sources and you demonstrate an ignorance of basic mathematical methods or physical concepts which are essential to a decent understanding of graduate level relativity, which Hawking radiation is.
Tell me, do you understand the lecture notes I linked to? Namely Chapters 8 and 9? I don't mean "I know what some of the words mean", I mean do you follow each line of the calculations, understanding why each was done?