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On the Variability of the Gravitational Constant by the Evolution of Stars and Galaxy Clusters


De Mees, Thierry


Research Papers





Date Published:

February 16, 2017




gravitomagnetism, gravitational constant, sun, white dwarf, red giant, galaxy clusters: relaxed, unrelaxed


Gravitomagnetism, initiated by O. Heaviside [1] and further developed by O. Jefimenko [2] consists of the Newtonian gravity and gyrotation, which is totally analogous to magnetism. This model successfully explained an important number of physical and cosmic phenomena [3]. Striking is the possibility of gravitational repel by particles with like-oriented spins. I also showed [5] why the gravitational constant is varying locally and I prove that, the particles in rotating bodies will preferentially form distributions that globally attract. This explains why masses have never been found to be repulsive. I deduced a new definition for “mass” as a vector, and conclude that the gravitational constant’s value is the sum of the orientations of the elementary vector-masses while taking their spacing into account. I found why the gravity force is so weak and why cohesion forces are so large. In this paper, I attempt to define the variations of the Gravitational Constant in the evolution of stars, and show that, for the same global mass of a star during its evolution, white dwarfs possess a much stronger gravitational constant than the red giant stars. Based upon these findings, I study the possibility that relaxed galaxy clusters possess, due to the same process, a much lower gravitational constant than unrelaxed galaxy clusters. This might be the reason why gravity lensing is a hundred times larger than the visible mass.


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