Search results for "GRAVITY"

showing 10 items of 537 documents

Dynamical generation of wormholes with charged fluids in quadratic Palatini gravity

2014

The dynamical generation of wormholes within an extension of General Relativity (GR) containing (Planck's scale-suppressed) Ricci-squared terms is considered. The theory is formulated assuming the metric and connection to be independent (Palatini formalism) and is probed using a charged null fluid as a matter source. This has the following effect: starting from Minkowski space, when the flux is active the metric becomes a charged Vaidya-type one, and once the flux is switched off the metric settles down into a static configuration such that far from the Planck scale the geometry is virtually indistinguishable from that of the standard Reissner-Nordstr\"om solution of GR. However, the innerm…

High Energy Physics - TheoryNuclear and High Energy PhysicsGeneral relativityPhysical constantDynamical generation of wormholesFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Curvature01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationTheoretical physicsGeneral Relativity and Quantum CosmologySingularityFísica Aplicada0103 physical sciencesMinkowski spaceWormhole010306 general physicsQuantumPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsHigh Energy Physics - Theory (hep-th)Astrophysics - High Energy Astrophysical PhenomenaQuadratic Palatini gravityCharged fluids
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Transplanckian inflation as gravity echoes

2015

In this work, we show that, in the presence of non-minimal coupling to gravity, it is possible to generate sizeable tensor modes in single-field models without transplanckian field values. These transplanckian field values apparently needed in Einstein gravity to accommodate the experimental results may only be due to our insistence of imposing a minimal coupling of the inflaton field to gravity in a model with non-minimal couplings. We present three simple single-field models that prove that it is possible accommodate a large tensor-to-scalar ratio without requiring transplanckian field values within the slow-roll regime.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)FOS: Physical sciences01 natural sciencesGravitationTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesTensor010306 general physicsMinimal couplingPhysicsInflation (cosmology)010308 nuclear & particles physicsFísicaInflatonlcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Einstein field equationslcsh:PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Born-Infeld f(R) gravity

2014

Motivated by the properties of matter quantum fields in curved space-times, we work out a gravity theory that combines the Born-Infeld gravity Lagrangian with an $f(R)$ piece. To avoid ghost-like instabilities, the theory is formulated within the Palatini approach. This construction provides more freedom to address a number of important questions such as the dynamics of the early universe and the cosmic accelerated expansion, among others. In particular, we consider the effect that adding an $f(R)=a R^2$ term has on the early-time cosmology. We find that bouncing solutions are robust against these modifications of the Lagrangian whereas the solutions with {\it loitering} behavior of the ori…

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Борна-Инфельда теория гравитации модифицированнаяmedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyCosmologyкосмологияGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)De Sitter universeBorn–Infeld modelmedia_commonPhysicsквантовая гравитацияFunction (mathematics)UniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Quantum gravityf(R) gravityF(R)-гравитацияквантовые поляAstrophysics - Cosmology and Nongalactic Astrophysics
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Modular fluxes, elliptic genera, and weak gravity conjectures in four dimensions

2019

We analyse the Weak Gravity Conjecture for chiral four-dimensional F-theory compactifications with N=1 supersymmetry. Extending our previous work on nearly tensionless heterotic strings in six dimensions, we show that under certain assumptions a tower of asymptotically massless states arises in the limit of vanishing coupling of a U(1) gauge symmetry coupled to gravity. This tower contains super-extremal states whose charge-to-mass ratios are larger than those of certain extremal dilatonic Reissner-Nordstrom black holes, precisely as required by the Weak Gravity Conjecture. Unlike in six dimensions, the tower of super-extremal states does not always populate a charge sub-lattice. The main t…

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)FOS: Physical sciencesF-TheoryTopological Strings01 natural sciencesTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheorySuperstrings and Heterotic Strings0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsGauge symmetryPhysicsHeterotic string theory010308 nuclear & particles physicshep-thCharge (physics)SupersymmetryF-theoryHigh Energy Physics - Theory (hep-th)lcsh:QC770-798String DualityMirror symmetryParticle Physics - TheoryString dualityJournal of High Energy Physics
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Stability analysis of black holes in massive gravity: a unified treatment

2014

We consider the analytic solutions of massive (bi)gravity which can be written in a simple form using advanced Eddington-Finkelstein coordinates. We analyse the stability of these solutions against radial perturbations. First we recover the previously obtained result on the instability of the bidiagonal bi-Schwarzschild solutions. In the non-bidiagonal case (which contains, in particular, the Schwarzschild solution with Minkowski fiducial metric) we show that generically there are physical spherically symmetric perturbations, but no unstable modes.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Kerr metricFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesInstabilityGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesMinkowski spaceSchwarzschild metric010306 general physicsComputingMilieux_MISCELLANEOUSPhysics[PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Massive gravityClassical mechanicsHigh Energy Physics - Theory (hep-th)Reissner–Nordström metric[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Deriving the Schwarzschild solution[PHYS.HTHE] Physics [physics]/High Energy Physics - Theory [hep-th]
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An alternative scenario for critical scalar field collapse in $AdS_3$

2016

In the context of gravitational collapse and black hole formation, we reconsider the problem to describe analytically the critical collapse of a massless and minimally coupled scalar field in $2+1$ gravity.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Particle physicsBlack HolesCritical phenomenaAstrophysics::High Energy Astrophysical PhenomenaCollapse (topology)FOS: Physical sciencesContext (language use)Critical collapseGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum Cosmology0103 physical sciencesGravitational collapse010306 general physicsComputingMilieux_MISCELLANEOUSPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsMassless particle2+1 gravityHigh Energy Physics - Theory (hep-th)Anti-de Sitter spaceScalar field
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Hawking radiation correlations in Bose-Einstein condensates using quantum field theory in curved space

2013

The density-density correlation function is computed for the Bogoliubov pseudoparticles created in a Bose-Einstein condensate undergoing a black hole flow. On the basis of the gravitational analogy, the method used relies only on quantum field theory in curved spacetime techniques. A comparison with the results obtained by ab initio full condensed matter calculations is given, confirming the validity of the approximation used, provided the profile of the flow varies smoothly on scales compared to the condensate healing length.

High Energy Physics - TheoryNuclear and High Energy PhysicsHAWKING RADIATION[PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]Black-hole evaporationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesCONDENSATI DI BOSE EINSTEINGeneral Relativity and Quantum Cosmologylaw.inventionGravitationGeneral Relativity and Quantum CosmologyCorrelation functionlawQuantum mechanics0103 physical sciencesQuantum field theory010306 general physicsCurved spaceCondensed Matter::Quantum GasesPhysicsQuantum field theory in curved spacetime[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Condensed Matter::Other010308 nuclear & particles physicsBlack holeHigh Energy Physics - Theory (hep-th)Quantum Gases (cond-mat.quant-gas)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Condensed Matter - Quantum GasesBose–Einstein condensateAnalog gravityHawking radiationPhysical Review D
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Holographic duals of 6d RG flows

2018

A notable class of superconformal theories (SCFTs) in six dimensions is parameterized by an integer $N$, an ADE group $G$, and two nilpotent elements $\mu_\mathrm{L,R}$ in $G$. Nilpotent elements have a natural partial ordering, which has been conjectured to coincide with the hierarchy of renormalization-group flows among the SCFTs. In this paper we test this conjecture for $G=\mathrm{SU}(k)$, where AdS$_7$ duals exist in IIA. We work with a seven-dimensional gauged supergravity, consisting of the gravity multiplet and two $\mathrm{SU}(k)$ non-Abelian vector multiplets. We show that this theory has many supersymmetric AdS$_7$ vacua, determined by two nilpotent elements, which are naturally …

High Energy Physics - TheoryNuclear and High Energy PhysicsPure mathematicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciSuperstring VacuaFOS: Physical sciencesAdS-CFT Correspondence01 natural sciencesHigh Energy Physics::Theory0103 physical sciencesSupergravity ModelField theory (psychology)lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsMultipletPhysics010308 nuclear & particles physicsGroup (mathematics)hep-thGauged supergravityAdS-CFT Correspondence Supergravity Models Superstring VacuaFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIAdS/CFT correspondenceNilpotentHigh Energy Physics - Theory (hep-th)Domain (ring theory)lcsh:QC770-798Partially ordered setSupergravity ModelsParticle Physics - TheoryJournal of High Energy Physics
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The geometry of N=3 AdS4 in massive IIA

2018

The geometry of the ${\cal N} = 3$, SO(4)--invariant, AdS$_4$ solution of massive type IIA supergravity that uplifts from the ${\cal N} = 3 $ vacuum of $D=4$ ${\cal N} = 8$ dyonic ISO(7) supergravity is investigated. Firstly, a $D=4$, SO(4)--invariant restricted duality hierarchy is constructed and used to uplift the entire, dynamical SO(4)--invariant sector to massive type IIA. The resulting consistent uplift formulae are used to obtain a new local expression for the ${\cal N} = 3 $ AdS$_4$ solution in massive IIA and analyse its geometry. Locally, the internal $S^6$ geometry corresponds to a warped fibration of $S^2$ and a hemisphere of $S^4$. This can be regarded as a warped generalisati…

High Energy Physics - TheoryNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciSuperstring VacuaFOS: Physical sciencesDuality (optimization)AdS-CFT Correspondence Flux compactifications Supergravity Models Superstring VacuaGeometryType (model theory)AdS-CFT Correspondence01 natural sciencesTwistor theoryAdS-CFT correspondencesupergravity modelsFlux compactifications0103 physical sciences010306 general physicsPhysicsSpinor010308 nuclear & particles physicsPhysicsSupergravityFibrationFísicaAdS/CFT correspondenceHigh Energy Physics - Theory (hep-th)Killing spinorsuperstring vacuaflux compactificationsSupergravity Models
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Non-supersymmetric AdS6 and the swampland

2021

We discuss infinite families of non-supersymmetric AdS$_6$ solutions in Type IIB string theory. They are siblings of supersymmetric solutions which are associated with $(p,q)$ 5-brane webs and holographically dual to 5d SCFTs engineered by those brane webs. The non-supersymmetric backgrounds carry identical 5-brane charges and are connected to the supersymmetric ones by RG flows. We study the stability of the non-supersymmetric solutions, identifying perturbative and non-perturbative decay channels for all the backgrounds explicitly available. We also identify likely decay mechanisms for solutions that have not been constructed explicitly but may be expected to exist based on brane web cons…

High Energy Physics - TheoryNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciSuperstring VacuaFOS: Physical sciencesQC770-798domain wallAdS-CFT Correspondencestring model: Type IIB01 natural sciencesGauge-gravity correspondenceHigh Energy Physics::TheoryNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciences010306 general physicsAdS-CFT Correspondence Gauge-gravity correspondence Superstring Vacua Supersymmetry BreakingSupersymmetry Breaking[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsbubbleComputer Science::Information RetrievalAdS-CFT Correspondence; Gauge-gravity correspondence; Superstring Vacua; Supersymmetry Breakingduality: holographystabilitydecay: nonperturbativeHigh Energy Physics - Theory (hep-th)renormalization group: flowD-brane: 5spin: 2Journal of High Energy Physics
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