Abstract
In the previous paper (JMP 2014) we showed that there exists a NeoMinkowskian Gravitational Expanding Solution of GR (General Relativity) with CC (Cosmological Constant). We prove now that NeoMinkowskian Vacuum (non-baryonic Fluid), with gravitational (first) density (dark energy) and gravitational waves (at light speed), corresponds to the Gravitation Field of a Cosmological Black Hole (CBH). The latter predicts furthermore a basic emission of Radiation (CBR) from Hubble spherical singular Horizon to the inside of CBH (unlike Hawking’s emission) at an initial singular time. Our solution is then compatible with a well-tempered Big Bang and Expanding Universe (Escher’s Figure, see Penrose, 3) but incompatible with inflation. The latter is based on Hypothesis of a so-called Planck’s particle (Lemaitre’s primitive atom) characterized by a so-called Planck length. We prove that we can short-circuit this unstable particle with a stable cosmological Poincare’s electron with gravific pressure. It is well known that electron is a stranger in usual Minkowskian vacuum (dixit Einstein). The stranger electron can be perfectly integrated in NeoMinkowskian Radiation fluid and then also (with its mass, charge and wavelength) in (second density of) CBR. Everything happens as if the leptonic mass of the electron were induced by our cosmological field. The unexpected cosmological model proposed here is the only one that predicts numerical values of (second) density and temperature of CBR very close to the observed (COBE) values.
Highlights
NeoMinkowskian Gravitational Vacuum as Solution of GR with CCLet’s summarize first how we come to an unexpected Gravitational NeoMinkowskianExpanding Vacuum which “looks like” de Sitter’s Expanding Vacuum [1] [2].(1) Gravitational Density of NeoMinkowskian Vacuum Let us consider Einstein’s equation of General Relativity (GR) with Cosmological Constant (CC)Λ and Perfect Fluid Tμν ≡
In the previous paper (JMP 2014) we showed that there exists a NeoMinkowskian Gravitational Expanding Solution of GR (General Relativity) with CC (Cosmological Constant)
The observer is in the right place to measure the CBR emission. This the reason why we suggest going beyond the notion the notion of “ Hole” and replace it with that of the “W(hole) World” or “The Black Whole Universe” given that it is filled with Cosmological black radiation of the kind CBR
Summary
Expanding Vacuum which “looks like” de Sitter’s Expanding Vacuum [1] [2]. (1) Gravitational Density of NeoMinkowskian Vacuum Let us consider Einstein’s equation of General Relativity (GR) with Cosmological Constant (CC). (1) Gravitational Density of NeoMinkowskian Vacuum Let us consider Einstein’s equation of General Relativity (GR) with Cosmological Constant (CC). The density of VACUUM, simulated by a Non-Baryonic ( Gμν = 0 ) NeoMinkowskian Fluid, depends on the Gravitational Constant (see 14): ρ+p= 0. In basic equation (0), NeoMinkowskian Vacuum is based on cancellation ( ρ + p =0 ) of Einstein’s Tensor ( Gμν = 0 ) whilst deSitterian Vacuum is based on cancellation ( p= ρ= 0 ) of Tensor of Perfect Fluid ( Tμν = 0 ): Gμν + Λgμν =0. Newton law of gravitation to a space point (we are in the framework of GR) that is to say a non-baryonic (non-material) pseudo-mass. We propose the numbering “anti”-6 for three reasons: 1) deSitterian Hubble constant is not connected with density ( ρ = 0 ) and so to a determined gravitational dynamic (5 bis).
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