Quantum Gravity can explain dark matter

Quantum Gravity can explain dark matter In the quantum vacuum, there are many carriers temporary acceleration of the average size of a randomly oriented. When the vacuum is an accelerated frame, the carriers will be displayed in the frame will be reduced, carriers and chassis improves, leading to a net polarization of the vacuum. While under the acceleration g is small, the effect is linear, and if the vacuum is filled with the coefficient vector of polarization is unity. The standard term for the exponential suppression of high-energy fluctuations must also be applied. Therefore, the polarization of vacuum, g exp (g / a). The terms of the exponent multiplied by the dipole moment have the dimensions of energy. The rest of the galaxy frame, for example, in relation to the accelerated local inertial frames that are in the middle. In this context, the residual vacuum is becoming more polarized and the galaxy? S gravitational field g. We have g = g + -GM/r2 exp (g / a), where g is considered negative. For g larger than one, the exponential is negligible and Newton's law results. But for less than one g, the exponential can be expanded to 1 + g / a, we obtain g2 = aGM/r2 This is precisely the formula found by Milgrom empirically to describe the motion of stars and galaxies in the region of weak - zone , unless the law of gravity is altered, not the law of motion. (Scientific American, August 2002). He believes that about one Angstrom per second squared, which is near? Surface gravity? of an electron, the field of one kilogram of mass to one meter, or area of a galaxy in outer parts. The place is not far from the value of the cosmological constant, in units where c = 1 In this model, you can be saturated as the field of quantum vacuum. Using the proper law of quantum gravity, there is no need to postulate the existence of dark matter of the severity observed.