Search results for "Auxiliary field"

showing 2 items of 2 documents

Cosmological Horizon Modes and Linear Response in de Sitter Spacetime

2009

Linearized fluctuations of quantized matter fields and the spacetime geometry around de Sitter space are considered in the case that the matter fields are conformally invariant. Taking the unperturbed state of the matter to be the de Sitter invariant Bunch-Davies state, the linear variation of the stress tensor about its self-consistent mean value serves as a source for fluctuations in the geometry through the semiclassical Einstein equations. This linear response framework is used to investigate both the importance of quantum backreaction and the validity of the semiclassical approximation in cosmology. The full variation of the stress tensor delta bi contains two kinds of terms: (1) those…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsQuantum field theory in curved spacetimeCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCauchy stress tensorDe Sitter spaceSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyAuxiliary fieldGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum cosmologyQuantum mechanics0103 physical sciencesEinstein field equations010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsMathematical physics
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Inflation with mixed helicities and its observational imprint on CMB

2018

In the framework of effective field theories with prominent helicity-0 and helicity-1 fields coupled to each other via a dimension-3 operator, we study the dynamics of inflation driven by the helicity-0 mode, with a given potential energy, as well as the evolution of cosmological perturbations, influenced by the presence of a mixing term between both helicities. In this scenario, the temporal component of the helicity-1 mode is an auxiliary field and can be integrated out in terms of the time derivative of the helicity-0 mode, so that the background dynamics effectively reduces to that in single-field inflation modulated by a parameter $\beta$ associated to the coupling between helicity-0 a…

PhysicsHigh Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCosmic microwave backgroundCosmic background radiationFOS: Physical sciencesObservableGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsInflaton01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsAuxiliary fieldsymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencesTime derivativeEffective field theorysymbolsPlanck010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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