Topology of Emergent Time
Author(s):
Cuesta Gutierrez FJ
We delve into the topology and morphology of the emergent time that arises from a electrons kinetic cloud virtually confined in a toroidal shape due to high-opacity environments. Different results using the most usual opacity models are shown. We analyze the dynamics that best represent such complexity, especially for stellar environments, focusing on the inner, mid and outer zones of the radiative layer. Detailed results of the expected induced Gravity, including their values and the time needed to be conserved over cosmological Time are shown. Then we extrapolate the results of the Gravity induced by the emergent time for different types of stars in function of their percentage per size and by mass, infering that the 95% of the Gravity created in the stars ranges from -43% till 19% of the emergent gravity arised in Sun-like stars. Finally we show how the variabilty of the gravitational constant could be demonstrated by experiments carried out on the Earth itself and how a new discipline “PaleoGravity” based on them could help us to study the origin of any chemical element present on Earth, the solar system and even asteroids.
