Christian Mcdowell

In the quantum vacuum there are many temporary acceleration vectors of mean size a randomly oriented. If the vacuum is viewed from an frame, the vectors going with the frame appear reduced, and the vectors going against the frame appear increased, resulting in a net polarization of the vacuum. If the frame's acceleration g is small, the effect is linear, and if the vacuum is filled with vectors the coefficient of the polarization will undoubtedly be unity. The typical exponential term for controlling high-energy fluctuations must also be applied. Ergo the vacuum polarization is g exp (g/a). If you are interested in law, you will probably need to discover about case for galaxy 4 10.1. The conditions of the exponent when multiplied by the dipole moment have the dimensions of energy.

The rest frame of the universe, as an example, is multiplied with respect to local inertial frames that fall under the center. In this rest frame the machine seems polarized and promotes the galaxy's gravitational field g. So we have

g= -GM/r2 + g exp (g/a)

where g is thought as bad. For g much greater, the exponential is minimal and Newton's law effects. However for g significantly less than a, the exponential can be expanded to 1 + g/a and we get

g2 = aGM/r2

This is precisely the system found empirically by Milgrom to describe the motion of stars and galaxies in the weak-field region, except the law of gravity is altered, not the law of motion (Scientific American, August 2002). He sees that an is approximately one Angstrom per second squared, which will be close to the "surface gravity" of an, the field of a mass at one meter, or the field of a galaxy in its outer parts. Visit tab 4 10.1 case to research the inner workings of it. Also, the square of a isn't far from the worthiness of the cosmological constant, in units where c=1. In the saturated field energy of the quantum vacuum this model, a could be viewed.

The findings can be acceptably explained by assuming a probable amount of common matter M and utilising the correct quantum law of gravity. There is number dependence on dark matter.

The resulting clear polarization would improve the acceleration, and indeed could potentially cause the acceleration, after the proces