Search results for "vacuum"

showing 10 items of 352 documents

ON QUANTUM GRAVITY, ASYMPTOTIC SAFETY AND PARAMAGNETIC DOMINANCE

2012

We discuss the conceptual ideas underlying the Asymptotic Safety approach to the nonperturbative renormalization of gravity. By now numerous functional renormalization group studies predict the existence of a suitable nontrivial ultraviolet fixed point. We use an analogy to elementary magnetic systems to uncover the physical mechanism behind the emergence of this fixed point. It is seen to result from the dominance of certain paramagnetic-type interactions over diamagnetic ones. Furthermore, the spacetimes of Quantum Einstein Gravity behave like a polarizable medium with a "paramagnetic" response to external perturbations. Similarities with the vacuum state of Yang-Mills theory are pointed …

High Energy Physics - TheoryPhysicsGravity (chemistry)Vacuum stateAsymptotic safety in quantum gravityFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Fixed pointRenormalization groupGeneral Relativity and Quantum CosmologyRenormalizationHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Space and Planetary ScienceQuantum gravityFunctional renormalization groupQuantumMathematical PhysicsInternational Journal of Modern Physics D
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Cosmology with self-adjusting vacuum energy density from a renormalization group fixed point

2001

Cosmologies with a time dependent Newton constant and cosmological constant are investigated. The scale dependence of $G$ and $\Lambda$ is governed by a set of renormalization group equations which is coupled to Einstein's equation in a consistent way. The existence of an infrared attractive renormalization group fixed point is postulated, and the cosmological implications of this assumption are explored. It turns out that in the late Universe the vacuum energy density is automatically adjusted so as to equal precisely the matter energy density, and that the deceleration parameter approaches $q = -1/4$. This scenario might explain the data from recent observations of high redshift type Ia S…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsDeceleration parametermedia_common.quotation_subjectCosmic microwave backgroundAstrophysics (astro-ph)FOS: Physical sciencesAstrophysicsCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsRenormalization groupAstrophysicsGeneral Relativity and Quantum CosmologyCosmologyUniverseHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Vacuum energyHigh Energy Physics - Theory (hep-th)Mathematical physicsmedia_commonQuintessencePhysics Letters B
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N-quantum approach to quantum field theory at finite T and mu: the NJL model

1999

We extend the N-quantum approach to quantum field theory to finite temperature ($T$) and chemical potential ($\mu$) and apply it to the NJL model. In this approach the Heisenberg fields are expressed using the Haag expansion while temperature and chemical potential are introduced simultaneously through a generalized Bogoliubov transformation. Known mean field results are recovered using only the first term in the Haag expansion. In addition, we find that at finite T and in the broken symmetry phase of the model the mean field approximation can not diagonalize the Hamiltonian. Inclusion of scalar and axial vector diquark channels in the SU(2)$_{rm f}$ $otimes$ SU(3)$_{\rm c}$ version of the …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryScalar (mathematics)Order (ring theory)FísicaHigh Energy Physics - Phenomenologysymbols.namesakeBogoliubov transformationVacuum energyMean field theorysymbolsQuantum field theoryHamiltonian (quantum mechanics)PseudovectorMathematical physics
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Gauge and Yukawa unification with broken R-parity

1998

We study gauge and Yukawa coupling unification in the simplest extension of the Minimal Supersymmetric Standard Model (MSSM) which incorporates R-Parity violation through a bilinear superpotential term. Contrary to what happens in the MSSM, we show that bottom-tau unification at the scale M_GUT where the gauge couplings unify can be achieved for any value of tan(beta) by choosing appropriately the sneutrino vacuum expectation value. In addition, we show that bottom-tau-top unification occurs in a slightly wider tan(beta) range than in the MSSM.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsUnificationHigh Energy Physics::PhenomenologySuperpotentialYukawa potentialFOS: Physical sciencesFísicaGauge (firearms)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)R-parityHigh Energy Physics::ExperimentBeta (velocity)Vacuum expectation valueMinimal Supersymmetric Standard ModelPhysics Letters B
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Acceleration radiation and the Planck scale

2008

A uniformly accelerating observer perceives the Minkowski vacuum state as a thermal bath of radiation. We point out that this field-theory effect can be derived, for any dimension higher than two, without actually invoking very high energy physics. This supports the view that this phenomenon is robust against Planck-scale physics and, therefore, should be compatible with any underlying microscopic theory.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsQuantum field theory in curved spacetime010308 nuclear & particles physicsVacuum stateFOS: Physical sciencesAcceleration (differential geometry)RadiationObserver (physics)01 natural sciencesPartícules (Física nuclear)Classical mechanicsHigh Energy Physics - Theory (hep-th)0103 physical sciencesMinkowski spaceThermalMicroscopic theory010306 general physicsPhysical Review D
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Spatial correlations of field observables in two half-spaces separated by a movable perfect mirror

2023

We consider a system of two cavities separated by a reflecting boundary of finite mass that is free to move, and bounded to its equilibrium position by a harmonic potential. This yields an effective mirror-field interaction, as well as an effective interaction between the field modes mediated by the movable boundary. Two massless scalar fields are defined in each cavity. We consider the second-order interacting ground state of the system, that contains virtual excitations of both mirror's degrees of freedom and of the scalar fields. We investigate the correlation functions between field observables in the two cavities, and find that the squared scalar fields in the two cavities, in the inte…

High Energy Physics - TheoryQuantum PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciHigh Energy Physics - Theory (hep-th)FOS: Physical sciencesVacuum Field Fluctuations Dynamical Casimir Effect Quantum Field TheoryQuantum Physics (quant-ph)Settore FIS/03 - Fisica Della Materia
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Space and Time Averaged Quantum Stress Tensor Fluctuations

2021

We extend previous work on the numerical diagonalization of quantum stress tensor operators in the Minkowski vacuum state, which considered operators averaged in a finite time interval, to operators averaged in a finite spacetime region. Since real experiments occur over finite volumes and durations, physically meaningful fluctuations may be obtained from stress tensor operators averaged by compactly supported sampling functions in space and time. The direct diagonalization, via a Bogoliubov transformation, gives the eigenvalues and the probabilities of measuring those eigenvalues in the vacuum state, from which the underlying probability distribution can be constructed. For the normal-orde…

High Energy Physics - TheoryVacuum stateDegrees of freedom (physics and chemistry)Thermal fluctuationsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)kosmologia114 Physical sciences01 natural sciencesGeneral Relativity and Quantum Cosmology0103 physical sciencesMinkowski space010306 general physicskvanttifysiikkaEigenvalues and eigenvectorsQuantum fluctuationPhysicsQuantum Physics010308 nuclear & particles physicsCauchy stress tensorMathematical analysisgravitaatioHigh Energy Physics - Theory (hep-th)gravitaatioaallotQuantum Physics (quant-ph)Scalar field
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Method to compute the stress-energy tensor for a quantized scalar field when a black hole forms from the collapse of a null shell

2020

A method is given to compute the stress-energy tensor for a massless minimally coupled scalar field in a spacetime where a black hole forms from the collapse of a spherically symmetric null shell in four dimensions. Part of the method involves matching the modes for the in vacuum state to a complete set of modes in Schwarzschild spacetime. The other part involves subtracting from the unrenormalized expression for the stress-energy tensor when the field is in the in vacuum state, the corresponding expression when the field is in the Unruh state and adding to this the renormalized stress-energy tensor for the field in the Unruh state. The method is shown to work in the two-dimensional case wh…

High Energy Physics - Theorydimension: 4space-time: SchwarzschildField (physics)Vacuum stateFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)coupling: scalarcoupling: minimal01 natural sciencesGeneral Relativity and Quantum Cosmologyrenormalizationvacuum stateGeneral Relativity and Quantum Cosmologyblack hole: formation0103 physical sciencesStress–energy tensorsymmetry: rotationTensordimension: 2010306 general physicsMathematical physicsPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsshell modelfield theory: scalarfield theory in curved spacegravitation: collapseBlack holeFormal aspects of field theoryUnruh effectHigh Energy Physics - Theory (hep-th)tensor: energy-momentum[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]quantizationSchwarzschild radiusScalar fieldPhysical Review D
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Oh, wait, O8 de Sitter may be unstable!

2021

We analyze the stability of four-dimensional de Sitter vacua constructed by compactifying massive Type IIA supergravity in the presence of two O8 sources [1]. When embedded in String Theory the first source has a clear interpretation as an O8$_-$ plane, but the second one could correspond to either an O8$_+$ plane or to an O8$_-$ plane with 16 D8-branes on top. We find that this latter solution has a tachyonic instability, corresponding to the D8-branes moving away from the O8$_-$ plane. We comment on the possible ways of distinguishing between these sources.

High Energy Physics - Theoryvacuum state: de SitterNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi Matematicidimension: 4compactificationSuperstring VacuaFOS: Physical sciencesD-braneString theory01 natural sciencessupergravity: Type IIADe Sitter universeFlux compactifications0103 physical sciencesC++ string handlingBrane cosmologylcsh:Nuclear and particle physics. Atomic energy. RadioactivityD-brane010306 general physicsMathematical physicsPhysicsCompactification (physics)010308 nuclear & particles physicsPlane (geometry)[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Supergravitytachyon: stabilitySuperstring Vacua D-branes Flux compactificationsHigh Energy Physics - Theory (hep-th)D-branesstringlcsh:QC770-798
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Multi-boson block factorization of fermions

2017

The numerical computations of many quantities of theoretical and phenomenological interest are plagued by statistical errors which increase exponentially with the distance of the sources in the relevant correlators. Notable examples are baryon masses and matrix elements, the hadronic vacuum polarization and the light-by-light scattering contributions to the muon g-2, and the form factors of semileptonic B decays. Reliable and precise determinations of these quantities are very difficult if not impractical with state-of-the-art standard Monte Carlo integration schemes. I will review a recent proposal for factorizing the fermion determinant in lattice QCD that leads to a local action in the g…

High Energy Physics::Latticeaction: local01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Vacuum polarizationcorrelation functionQuantum Chromodynamics Lattice gauge theory Computational PhysicsMonte CarloBosonPhysicsform factorPhysicsHigh Energy Physics - Lattice (hep-lat)lattice field theoryPropagatorpropagator [quark]hep-phParticle Physics - Latticestatistical [error]Lattice QCDFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIHigh Energy Physics - Phenomenologyerror: statisticalquark: factorizationquark: propagatorMonte Carlo integrationQuarkParticle physicsQC1-999fermion: determinantdeterminant [fermion]FOS: Physical scienceshep-latbaryon: massHigh Energy Physics - LatticeFactorization0103 physical sciencesmagnetic moment [muon]hadronic [vacuum polarization]010306 general physicsnumerical calculationsParticle Physics - Phenomenologymuon: magnetic moment010308 nuclear & particles physicsvacuum polarization: hadronicHigh Energy Physics::Phenomenologyphoton photon: scatteringB: decaylocal [action]Fermiondecay [B]mass [baryon]scattering [photon photon]gauge field theoryHigh Energy Physics::Experimentfactorization [quark]
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