Search results for "Energy condition"

showing 2 items of 2 documents

Phantom Dirac-Born-Infeld dark energy

2017

Motivated by the apparent discrepancy between Cosmic Microwave Background measurements of the Hubble constant and measurements from Type-Ia supernovae, we construct a model for Dark Energy with equation of state $w = p / ��< -1$, violating the Null Energy Condition. Naive canonical models of so-called "Phantom" Dark Energy require a negative scalar kinetic term, resulting in a Hamiltonian unbounded from below and associated vacuum instability. We construct a scalar field model for Dark Energy with $w < -1$, which nonetheless has a Hamiltonian bounded from below in the comoving reference frame, {\it i.e.} in the rest frame of the fluid. We demonstrate that the solution is a cosmologica…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsKinetic termRest frame01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesake0103 physical sciencesAttractorsymbolsEnergy conditionDark energyHamiltonian (quantum mechanics)010303 astronomy & astrophysicsScalar fieldAstrophysics - Cosmology and Nongalactic AstrophysicsMathematical physicsHubble's lawPhysical Review D
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Regular black hole metrics and the weak energy condition

2014

In this work we construct a family of spherically symmetric, static, charged regular black hole metrics in the context of Einstein-nonlinear electrodynamics theory. The construction of the charged regular black hole metrics is based on three requirements: (a) the weak energy condition should be satisfied, (b) the energy-momentum tensor should have the symmetry $T^{0}_{0}=T^{1}_{1}$, and (c) these metrics have to asymptotically behave as the Reissner-Nordstr\"{o}m black hole metric. In addition, these charged regular black hole metrics depend on two parameters which for specific values yield regular black hole metrics that already exist in the literature. Furthermore, by relaxing the third r…

PhysicsNuclear and High Energy PhysicsWhite holeAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyBlack hole electronBlack holeTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsde Sitter–Schwarzschild metricNonsingular black hole modelsExtremal black holeBlack braneEnergy conditionPhysics Letters B
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