Search results for "Stability"

showing 10 items of 3085 documents

On AdS7 stability

2019

AdS$_7$ supersymmetric solutions in type IIA have been classified, and they are infinitely many. Moreover, every such solution has a non-supersymmetric sister. In this paper, we study the perturbative and non-perturbative stability of these non-supersymmetric solutions, focusing on cases without orientifolds. Perturbatively, we first look at the KK spectrum of spin-2 excitations. This does not exhibit instabilities, but it does show that there is no separation of scales for either the BPS and the non-BPS case, thus proving for supersymmetric AdS$_7$ a well-known recent conjecture. We then use 7d gauged supergravity and a brane polarization computation to access part of the spectrum of KK sc…

High Energy Physics - TheoryNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi Matematicistability: nonperturbativeComputationSuperstring VacuaType (model theory)AdS-CFT Correspondence01 natural sciencesInstabilityStability (probability)orientifoldmembrane modelTheoretical physicsHigh Energy Physics::Theory0103 physical sciencesexcited stateanti-de Sitterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsPhysicsSupersymmetry BreakingpolarizationConjecture010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thbubbleSpectrum (functional analysis)Gauged supergravityHigh Energy Physics::PhenomenologyFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIBPSlcsh:QC770-798supergravityBranesupersymmetryAdS-CFT Correspondence Superstring Vacua Supersymmetry BreakingParticle Physics - TheoryJournal of High Energy Physics
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Instability of black holes in massive gravity

2013

We show that linear perturbations around the simplest black hole solution of massive bi-gravity theories, the bi-Schwarzschild solution, exhibit an unstable mode featuring the Gregory-Laflamme instability of higher dimensional black strings. The result is obtained for the massive gravity theory which is free from the Boulware-Deser ghost, as well as for its extension with two dynamical metrics. These results may indicate that static black holes in massive gravity do not exist. For the graviton mass of the order of the Hubble scale, however, the instability timescale is of order of the Hubble time.

High Energy Physics - TheoryPhysics and Astronomy (miscellaneous)Field (physics)Scale (ratio)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFieldGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesInstabilityGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum Cosmology0103 physical sciencesBlack stringStrings010306 general physicsPhysics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]GravitonP-BranesBlack holeMassive gravityHigh Energy Physics - Theory (hep-th)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
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Quantum Backreaction on Three-Dimensional Black Holes and Naked Singularities

2016

We analytically investigate backreaction by a quantum scalar field on two rotating Ba\~nados-Teitelboim-Zanelli (BTZ) geometries: that of a black hole and that of a naked singularity. In the former case, we explore the quantum effects on various regions of relevance for a rotating black hole space-time. We find that the quantum effects lead to a growth of both the event horizon and the radius of the ergosphere, and to a reduction of the angular velocity, compared to the unperturbed values. Furthermore, they give rise to the formation of a curvature singularity at the Cauchy horizon and show no evidence of the appearance of a superradiant instability. In the case of a naked singularity, we f…

High Energy Physics - Theoryblack hole: rotationeffect: quantumvelocitysemiclassicalEvent horizonperturbationspace-time: black holeGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)angular momentum01 natural sciencesErgospherePenrose processGeneral Relativity and Quantum Cosmologyhorizon[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]black hole: BTZGeneral Relativity and Quantum CosmologyQuantum mechanics0103 physical sciencescurvature: singularity010306 general physicsRing singularityPhysics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]formationNaked singularitycoupling: conformalstabilityfield theory: scalarBlack holeClassical mechanicsHigh Energy Physics - Theory (hep-th)Apparent horizonback reaction: quantum[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]massGravitational singularitysuperradianceblack hole: geometry
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On gravitational waves in Born-Infeld inspired non-singular cosmologies

2017

We study the evolution of gravitational waves for non-singular cosmological solutions within the framework of Born-Infeld inspired gravity theories, with special emphasis on the Eddington-inspired Born-Infeld theory. We review the existence of two types of non-singular cosmologies, namely bouncing and asymptotically Minkowski solutions, from a perspective that makes their features more apparent. We study in detail the propagation of gravitational waves near these non-singular solutions and carefully discuss the origin and severity of the instabilities and strong coupling problems that appear. We also investigate the role of the adiabatic sound speed of the matter sector in the regularisatio…

High Energy Physics - Theorycosmological modelCosmology and Nongalactic Astrophysics (astro-ph.CO)[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmology[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th][ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GravitationTheoretical physicsGeneral Relativity and Quantum CosmologyBorn–Infeld modelgravitational radiation: propagation0103 physical sciencesMinkowski spacestrong couplingphysics of the early universeMinkowski010306 general physicsAdiabatic processmodified gravityPhysics010308 nuclear & particles physicsGravitational waveNon singular[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Astronomy and Astrophysicsalternatives to inflationstabilityvelocity: acousticBorn-Infeld modelregularizationHigh Energy Physics - Theory (hep-th)gravitationRegularization (physics)adiabaticStrong coupling[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]primordial gravitational waves (theory)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Spectroscopy of short-lived radioactive molecules: A sensitive laboratory for new physics

2019

The study of molecular systems provides exceptional opportunities for the exploration of the fundamental laws of nature and for the search for physics beyond the Standard Model of particle physics. Measurements of molecules composed of naturally occurring nuclei have provided the most stringent upper bounds to the electron electric dipole moment to date, and offer a route to investigate the violation of fundamental symmetries with unprecedented sensitivity. Radioactive molecules - where one or more of their atoms possesses a radioactive nucleus - can contain heavy and deformed nuclei, offering superior sensitivity for EDM measurements as well as for other symmetry-violating effects. Radium …

High Energy Physics - TheoryexceptionalNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]collinearFOS: Physical sciencesnucleus: structure function[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)ionizationPhysics::Atomic PhysicsNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear Experimentenhancementnew physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]stabilitysensitivitylaserradiumelectron: electric momentHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)radioactivity[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]many-body problemnucleus: deformation
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Pseudospectrum and Black Hole Quasinormal Mode Instability

2020

We study the stability of quasinormal modes (QNM) in asymptotically flat black hole spacetimes by means of a pseudospectrum analysis. The construction of the Schwarzschild QNM pseudospectrum reveals the following: (i) the stability of the slowest-decaying QNM under perturbations respecting the asymptotic structure, reassessing the instability of the fundamental QNM discussed by Nollert [H. P. Nollert, About the Significance of Quasinormal Modes of Black Holes, Phys. Rev. D 53, 4397 (1996)] as an "infrared" effect; (ii) the instability of all overtones under small-scale ("ultraviolet") perturbations of sufficiently high frequency, which migrate towards universal QNM branches along pseudospec…

High Energy Physics - TheoryperturbationcompactificationQC1-999[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]FOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesInstabilityStability (probability)General Relativity and Quantum Cosmologyoperator: spectrumGeneral Relativity and Quantum CosmologyTheoretical physics0103 physical sciencesQuasinormal modestructurenumerical calculations010306 general physicsMathematical PhysicsPseudospectrumPhysicsCompactification (physics)[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsPhysicsOperator (physics)black hole: stabilityMathematical Physics (math-ph)Schwarzschildquasinormal mode: spectrumBlack holeHigh Energy Physics - Theory (hep-th)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]spectralSchwarzschild radiusPhysical Review X
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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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Optimization of ZnO:Al/Ag/ZnO:Al structures for ultra-thin high-performance transparent conductive electrodes

2012

Al-doped ZnO (AZO)/Ag/AZO multilayer coatings (50-70 nm thick) were grown at room temperature on glass substrates with different silver layer thickness, from 3 to 19 nm, by using radio frequency magnetron sputtering. Thermal stability of the compositional, optical and electrical properties of the AZO/Ag/AZO structures were investigated up to 400 °C and as a function of Ag film thickness. An AZO film as thin as 20 nm is an excellent barrier to Ag diffusion. The inclusion of 9.5 nm thin silver layer within the transparent conductive oxide (TCO) material leads to a maximum enhancement of the electro-optical characteristics. The excellent measured properties of low resistance, high transmittanc…

High transmittanceDiffusionrf-Magnetron sputteringElectro-optical characteristicGlass substrateTransparent conductive oxide RF magnetron sputtering Optical properties Electrical resistivity Al-doped zinc oxide Silver MultilayersSettore ING-INF/01 - ElettronicaSUBSTRATE-TEMPERATUREAg diffusionAl-doped ZnOLow resistanceMultilayerZNOMaterials ChemistryVisible spectral rangeMULTILAYER FILMSAl-doped zinc oxideOptical propertiesMetals and AlloysAZO filmElectrical resistivityOPTICAL-PROPERTIESOXIDE-FILMSSurfaces and InterfacesZinc oxide AluminumRadio frequency magnetron sputteringSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsOptical and electrical propertieElectrodeOptoelectronicsFilm preparationLayer (electronics)Magnetron sputteringUltra-thinRF magnetron sputteringMaterials scienceSilverThermodynamic stabilityOpticsTransparent conductive oxideElectrical resistivity and conductivityThermal stabilityElectrical conductorTransparent conducting filmRoom temperatureThin film solar cellbusiness.industryTransparent conductiveOptical propertieSilver layerHigh transmittanceMultilayersMulti-layer-coatingZnO Electric conductivityMeasured propertiebusinessSubstrate
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Modeling the hydrological and mechanical effect of roots on shallow landslides

2016

This study proposes a new methodology for estimating the additional shear strength (or cohesion) exerted by vegetation roots on slope stability analysis within a coupled hydrological-stability model. The mechanical root cohesion is estimated within a Fiber Bundle Model framework that allows for the evaluation of the root strength as a function of stress-strain relationships of populations of fibers. The use of such model requires the knowledge of the root architecture. A branching topology model based on Leonardo's rule is developed, providing an estimation of the amount of roots and the distribution of diameters with depth. The proposed methodology has been implemented into an existing dis…

Hillslope instabilityVegetation root cohesionRoot topological modelSettore ICAR/02 - Costruzioni Idrauliche E Marittime E IdrologiaShallow landslidesHillslope instability; Hydrological modeling; Root topological model; Shallow landslides; Vegetation root cohesion; Water Science and TechnologyShallow landslideHydrological modelingWater Science and Technology
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Improved modelling of fatigue loads in wind farms under non-neutral ABL stability conditions

2018

HistoryABL010504 meteorology & atmospheric sciencesbusiness.industry020209 energy02 engineering and technologyStructural engineering01 natural sciencesComputer Science ApplicationsEducationStability conditions0202 electrical engineering electronic engineering information engineeringEnvironmental sciencebusiness0105 earth and related environmental sciencesJournal of Physics: Conference Series
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