0000000000136578

AUTHOR

Antonio Ferreiro

0000-0001-7448-9046

showing 8 related works from this author

Pair creation in electric fields, anomalies, and renormalization of the electric current

2018

We investigate the Schwinger pair production phenomena in spatially homogeneous strong electric fields. We first consider scalar QED in four-dimensions and discuss the potential ambiguity in the adiabatic order assignment for the electromagnetic potential required to fix the renormalization subtractions. We argue that this ambiguity can be solved by invoking the conformal anomaly when both electric and gravitational backgrounds are present. We also extend the adiabatic regularization method for spinor QED in two-dimensions and find consistency with the chiral anomaly. We focus on the issue of the renormalization of the electric current $\langle j^\mu \rangle$ generated by the created pairs.…

High Energy Physics - TheoryChiral anomalyPhysicsSpinor010308 nuclear & particles physicsHigh Energy Physics::LatticeConformal anomalyHigh Energy Physics::PhenomenologyFOS: Physical sciencesComputer Science::Digital Libraries01 natural sciencesRenormalizationTheoretical physicsPair productionHigh Energy Physics - Theory (hep-th)Regularization (physics)Electric field0103 physical sciences010306 general physicsAdiabatic processPhysical Review D
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Adiabatic expansions for Dirac fields, renormalization, and anomalies

2018

11 pags.

High Energy Physics - TheoryRenormalizationConformal anomalyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyRenormalizationGeneral Relativity and Quantum CosmologyDirac fieldFriedmann-Lemaître-Robertson-Walker spacetime0103 physical sciencesMinkowski spaceRenormalization; anomalies010306 general physicsAdiabatic processYukawa couplingMathematical physicsPhysicsMaterialesSpacetime010308 nuclear & particles physicsYukawa potentialAdiabatic expansionCosmologyHigh Energy Physics - Theory (hep-th)Regularization (physics)anomaliesScalar fieldPhysical Review D
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Adiabatic regularization with a Yukawa interaction

2017

We extend the adiabatic regularization method for an expanding universe to include the Yukawa interaction between quantized Dirac fermions and a homogeneous background scalar field. We give explicit expressions for the renormalized expectation values of the stress-energy tensor $\langle T_{\mu\nu} \rangle$ and the bilinear $\langle \bar\psi\psi\rangle$ in a spatially flat FLRW spacetime. These are basic ingredients in the semiclassical field equations of fermionic matter in curved spacetime interacting with a background scalar field. The ultraviolet subtracting terms of the adiabatic regularization can be naturally interpreted as coming from appropriate counterterms of the background fields…

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsConformal anomalyHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologySemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Yukawa interaction01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsRegularization (physics)Friedmann–Lemaître–Robertson–Walker metric0103 physical sciencessymbols010306 general physicsAdiabatic processScalar fieldEffective actionMathematical physics
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Role of gravity in the pair creation induced by electric fields

2018

We analyze the pair production induced by homogenous, time-dependent electric fields in an expanding space-time background. We point out that, in obtaining the semiclassical Maxwell equations, two distinct notions of adiabatic renormalization are possible. In Minkowski space the two recipes turn out to be equivalent. However, in the presence of gravity only the recipe requiring an adiabatic hierarchy between the gravitational and the gauge field is consistent with the conservation of the energy-momentum tensor.

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyRenormalizationGravitationsymbols.namesakeClassical mechanicsMaxwell's equationsHigh Energy Physics - Theory (hep-th)0103 physical sciencesMinkowski spacesymbolsTensorGauge theory010306 general physicsAdiabatic process
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R-summed form of adiabatic expansions in curved spacetime

2020

The Feynman propagator in curved spacetime admits an asymptotic (Schwinger-DeWitt) series expansion in derivatives of the metric. Remarkably, all terms in the series containing the Ricci scalar R can be summed exactly. We show that this (non-perturbative) property of the Schwinger-DeWitt series has a natural and equivalent counterpart in the adiabatic (Parker-Fulling) series expansion of the scalar modes in an homogeneous cosmological spacetime. The equivalence between both R-summed adiabatic expansions can be further extended when a background scalar field is also present.

PhysicsSpacetime010308 nuclear & particles physicsScalar (mathematics)FOS: Physical sciencesPropagatorGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyHomogeneous0103 physical sciences010306 general physicsAdiabatic processSeries expansionScalar fieldMathematical physicsScalar curvature
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Running gravitational couplings, decoupling, and curved spacetime renormalization

2020

We propose to slightly generalize the DeWitt-Schwinger adiabatic renormalization subtractions in curved space to include an arbitrary renormalization mass scale $\mu$. The new predicted running for the gravitational couplings are fully consistent with decoupling of heavy massive fields. This is a somewhat improvement with respect to the more standard treatment of minimal (DeWitt-Schwinger) subtractions via dimensional regularization. We also show how the vacuum metamorphosis model emerges from the running couplings.

PhysicsHigh Energy Physics - TheorySpacetime010308 nuclear & particles physicsHigh Energy Physics::LatticeFOS: Physical sciencesDecoupling (cosmology)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyRenormalizationGravitationDimensional regularizationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencesMass scale010306 general physicsAdiabatic processCurved spaceMathematical physics
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Running couplings from adiabatic regularization

2019

We extend the adiabatic regularization method by introducing an arbitrary mass scale $\mu$ in the construction of the subtraction terms. This allows us to obtain, in a very robust way, the running of the coupling constants by demanding $\mu$-invariance of the effective semiclassical (Maxwell-Einstein) equations. In particular, we get the running of the electric charge of perturbative quantum electrodynamics. Furthermore, the method brings about a renormalization of the cosmological constant and the Newtonian gravitational constant. The running obtained for these dimensionful coupling constants has new relevant (non-logarithmic) contributions, not predicted by dimensional regularization.

PhysicsCoupling constantHigh Energy Physics - TheoryNuclear and High Energy PhysicsSemiclassical physicsFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)lcsh:QC1-999General Relativity and Quantum CosmologyRenormalizationGravitational constantDimensional regularizationHigh Energy Physics - Theory (hep-th)Regularization (physics)Adiabatic processlcsh:PhysicsMathematical physics
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Renormalization, running couplings, and decoupling for the Yukawa model in a curved spacetime

2021

The decoupling of heavy fields as required by the Appelquist-Carazzone theorem plays a fundamental role in the construction of any effective field theory. However, it is not a trivial task to implement a renormalization prescription that produces the expected decoupling of massive fields, and it is even more difficult in curved spacetime. Focused on this idea, we consider the renormalization of the one-loop effective action for the Yukawa interaction with a background scalar field in curved space. We compute the beta functions within a generalized DeWitt-Schwinger subtraction procedure and discuss the decoupling in the running of the coupling constants. For the case of a quantized scalar fi…

High Energy Physics - TheoryPhysicsField (physics)Yukawa potentialFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Decoupling (cosmology)Yukawa interactionGeneral Relativity and Quantum CosmologyRenormalizationTheoretical physicsHigh Energy Physics - Theory (hep-th)Beta function (physics)Scalar fieldCurved spacePhysical Review D
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