A quantum Friedmann flat spacetime: Uncertainty Relations, Thermodynamics and some cosmological consequences
arXiv:1712.09125 · doi:10.1142/9789813226609_0490
Abstract
We present Friedmann flat spacetime uncertainty relations (STUR) together with some cosmological implications. An interesting link between the Principle of "gravitational stability against localization of events" (PGSL) and the holographic Bekenstein entropy bound (HEB) is also investigated. The same theorems leading to our STUR are used to calculate, thanks to the holographic principle, the entropy of the universe at its apparent horizon. The generalized entropy formula can be used to discuss interesting links with a quantum spacetime.
Contributed paper to the Fourteenth Marcel Grossmann Meeting on General Relativity, University of Rome "La Sapienza", Italy, 12 - 18 July 2015; edited by Massimo Bianchi, Robert T Jantzen, Remo Ruffini. (World Scientific, Singapore, 2017) p.3739 - p.3743. Contributions in parts present on arXiv:1102.0894; arXiv:1308.2767; arXiv:1405.6816; arXiv:1506.08573