Tensorial Quantum Gravity and the Cosmological Constant Problem

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dc.creatorReal, Christophe
dc.date2007-11-09
dc.date2007-11-10
dc.date.accessioned2026-07-07T08:44:23Z
dc.date.available2026-07-07T08:44:23Z
dc.descriptionIn the present article, which is the first part of a work in three parts, we build an equation of quantum gravity. This equation is tensorial, is equivalent to general relativity in vacuum, but differs completely from general relativity inside matter. This new equation possesses a dimensionless gravitational coupling constant, and passes all experimental tests that also passes general relativity. This quantum gravity and general relativity diverge essentially in the domain of cosmology : we prove that quantum gravity gives the solution to the whole set of problems left over by the standard cosmological model based on general relativity. Essentially, we prove that the initial singularity, the big bang, is smoothed out by quantum gravity, that the flatness problem finds a precise solution : quantum gravity predicts that Omega should be just a little greater than 1, which fits perfectly with the observed 1.02. The cosmological constant problem finds also its solution since we prove that the Lambda term does not come from any dark energy, but comes from nonperturbative quantum corrections to classical relativity, and has the exact tiny but strictly positive value needed. Furthermore, the quantum equation of gravity possesses, with no further efforts, features of unification. Indeed, our equation governs at the same time the large scale of the universe, as did general relativity, but also the structure of particles.
dc.description108 pages
dc.identifierhttps://arxiv.org/abs/0711.1441
dc.identifierhttp://arxiv.org/abs/0711.1441
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142640
dc.subjectGeneral Physics
dc.titleTensorial Quantum Gravity and the Cosmological Constant Problem
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