Search results for "Initial singularity"

showing 3 items of 3 documents

Big bounce and future time singularity resolution in Bianchi i cosmologies: The projective invariant Nieh-Yan case

2021

We extend the notion of the Nieh-Yan invariant to generic metric-affine geometries, where both torsion and nonmetricity are taken into account. Notably, we show that the properties of projective invariance and topologicity can be independently accommodated by a suitable choice of the parameters featuring this new Nieh-Yan term. We then consider a special class of modified theories of gravity able to promote the Immirzi parameter to a dynamical scalar field coupled to the Nieh-Yan form, and we discuss in more detail the dynamics of the effective scalar tensor theory stemming from such a revised theoretical framework. We focus, in particular, on cosmological Bianchi I models and we derive cla…

Physics010308 nuclear & particles physicsInitial singularityImmirzi parameter01 natural sciencesScalar–tensor theoryTheoretical physicsGeneral Relativity and Quantum CosmologySingularity0103 physical sciencesGravitational singularityInvariant (mathematics)010306 general physicsScalar fieldBig Bounce
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Cosmological solutions in theD=5 Einstein-Maxwell theory coupled to matter

1991

We study the Einstein-Maxwell theory in five dimensions coupled to matter in two distinct ways. In the first we reduce the Lagrangian to an effective four-dimension one and then we couple it to matter; in the second, we introduce matter directly in the original five-dimensional theory. In both cases we use a non trivial configuration for the Maxwell potential. We find non singular solutions which present a repulsive gravitational phase. When this phase is absent, the initial singularity is unavoidable.

PhysicsGravitationsymbols.namesakeSingularityPhysics and Astronomy (miscellaneous)Initial singularitySingular solutionGeneral relativitySpace timesymbolsEinsteinCosmologyMathematical physicsGeneral Relativity and Gravitation
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Entropy signature of the running cosmological constant

2007

Renormalization group (RG) improved cosmologies based upon a RG trajectory of Quantum Einstein Gravity (QEG) with realistic parameter values are investigated using a system of cosmological evolution equations which allows for an unrestricted energy exchange between the vacuum and the matter sector. It is demonstrated that the scale dependence of the gravitational parameters, the cosmological constant in particular, leads to an entropy production in the matter system. The picture emerges that the Universe started out from a state of vanishing entropy, and that the radiation entropy observed today is essentially due to the coarse graining (RG flow) in the quantum gravity sector which is relat…

PhysicsHigh Energy Physics - TheoryInitial singularityEntropy productionAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyMetric expansion of spaceGravitationGeneral Relativity and Quantum CosmologyVacuum energyHigh Energy Physics - Theory (hep-th)Quantum gravityEntropy (arrow of time)Mathematical physics
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