Search results for "General relativity and quantum cosmology"

showing 10 items of 941 documents

Gravitational footprints of massive neutrinos and lepton number breaking

2020

We investigate the production of primordial Gravitational Waves (GWs) arising from First Order Phase Transitions (FOPTs) associated to neutrino mass generation in the context of type-I and inverse seesaw schemes. We examine both "high-scale" as well as "low-scale" variants, with either explicit or spontaneously broken lepton number symmetry $U(1)_L$ in the neutrino sector. In the latter case, a pseudo-Goldstone majoron-like boson may provide a candidate for cosmological dark matter. We find that schemes with softly-broken $U(1)_L$ and with single Higgs-doublet scalar sector lead to either no FOPTs or too weak FOPTs, precluding the detectability of GWs in present or near future measurements.…

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Spontaneous symmetry breakingDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Computer Science::Digital Libraries01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciences010306 general physicsPhysics010308 nuclear & particles physicsMass generationHigh Energy Physics::PhenomenologyLepton numberlcsh:QC1-999High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Theory (hep-th)Higgs bosonNeutrinolcsh:PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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QUANTUM EFFECTS IN ACOUSTIC BLACK HOLES: THE BACKREACTION.

2004

We investigate the backreaction equations for an acoustic black hole formed in a Laval nozzle under the assumption that the motion of the fluid is one-dimensional. The solution in the near-horizon region shows that as phonons are (thermally) radiated the sonic horizon shrinks and the temperature decreases. This contrasts with the behaviour of Schwarzschild black holes, and is similar to what happens in the evaporation of (near-extremal) Reissner-Nordstrom black holes (i.e. infinite evaporation time). Finally, by appropriate boundary conditions the solution is extended in both the asymptotic regions of the nozzle.

High Energy Physics - TheoryNuclear and High Energy PhysicsSonic black holeEvent horizonWhite holeAstrophysics::High Energy Astrophysical PhenomenaHAWKINGFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Charged black holeGeneral Relativity and Quantum CosmologyACOUSTICPhysics::Fluid DynamicsMicro black holeGeneral Relativity and Quantum CosmologyQuantum mechanicsPhysicsBLACK HOLEBACK REACTIONFLUIDCondensed Matter - Other Condensed MatterBlack holeHigh Energy Physics - Theory (hep-th)RADIATIONSchwarzschild radiusOther Condensed Matter (cond-mat.other)Hawking radiation
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Relations for Einstein–Yang–Mills amplitudes from the CHY representation

2017

We show that a recently discovered relation, which expresses tree-level single trace Einstein-Yang-Mills amplitudes with one graviton and $(n-1)$ gauge bosons as a linear combination of pure Yang-Mills tree amplitudes with $n$ gauge bosons, can be derived from the CHY representation. In addition we show that there is a generalisation, which expresses tree-level single trace Einstein-Yang-Mills amplitudes with $r$ gravitons and $(n-r)$ gauge bosons as a linear combination of pure Yang-Mills tree amplitudes with $n$ gauge bosons. We present a general formula for this case.

High Energy Physics - TheoryNuclear and High Energy PhysicsTrace (linear algebra)High Energy Physics::LatticeFOS: Physical sciencesYang–Mills existence and mass gap01 natural sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryQuantum mechanics0103 physical sciencesEinstein010306 general physicsLinear combinationMathematical physicsPhysicsCondensed Matter::Quantum GasesIntroduction to gauge theoryGauge boson010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGravitonlcsh:QC1-999High Energy Physics - Theory (hep-th)Supersymmetric gauge theorysymbolslcsh:PhysicsPhysics Letters B
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Wilson Loop Form Factors: A New Duality

2017

We find a new duality for form factors of lightlike Wilson loops in planar $\mathcal N=4$ super-Yang-Mills theory. The duality maps a form factor involving an $n$-sided lightlike polygonal super-Wilson loop together with $m$ external on-shell states, to the same type of object but with the edges of the Wilson loop and the external states swapping roles. This relation can essentially be seen graphically in Lorentz harmonic chiral (LHC) superspace where it is equivalent to planar graph duality. However there are some crucial subtleties with the cancellation of spurious poles due to the gauge fixing. They are resolved by finding the correct formulation of the Wilson loop and by careful analyti…

High Energy Physics - TheoryNuclear and High Energy PhysicsWilson loopgauge fixingHigh Energy Physics::LatticeFOS: Physical sciencesDuality (optimization)Type (model theory)Superspace01 natural sciencesSuperspacesspace: EuclideanGeneral Relativity and Quantum CosmologyWilson loopQuantum mechanics0103 physical sciencesMinkowski spacelcsh:Nuclear and particle physics. Atomic energy. RadioactivityMinkowskiScattering Amplitudes010306 general physicssuperspaceMathematical physicsGauge fixingPhysicsform factor010308 nuclear & particles physicsEuclidean space[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thAnalytic continuationWilsonLoop (topology)chiralCERN LHC CollHigh Energy Physics - Theory (hep-th)’t Hooft and Polyakov loopslcsh:QC770-798dualitysupersymmetryParticle Physics - TheoryDuality in Gauge Field TheoriesLorentz
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Brane cosmology with an anisotropic bulk

2004

In the context of brane cosmology, a scenario where our universe is a 3+1-dimensional surface (the ``brane'') embedded in a five-dimensional spacetime (the ``bulk''), we study geometries for which the brane is anisotropic - more specifically Bianchi I - though still homogeneous. We first obtain explicit vacuum bulk solutions with anisotropic three-dimensional spatial slices. The bulk is assumed to be empty but endowed with a negative cosmological constant. We then embed Z_2-symmetric branes in the anisotropic spacetimes and discuss the constraints on the brane energy-momentum tensor due to the five-dimensional anisotropic geometry. We show that if the bulk is static, an anisotropic brane ca…

High Energy Physics - TheoryNuclear and High Energy Physicsmedia_common.quotation_subjectFOS: Physical sciencesContext (language use)Perfect fluidGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesBrane cosmologyTensor010306 general physicsmedia_commonPhysicsSpacetimeExtra Large Dimensions010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Astrophysics (astro-ph)Cosmology of Theories beyond the SMUniverseHigh Energy Physics - Theory (hep-th)Brane
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Revising the Predictions of Inflation for the Cosmic Microwave Background Anisotropies

2009

4 pages, 1 figure.-- PACS nrs.: 98.70.Vc; 11.10.Gh; 98.80.Cq.-- ArXiv pre-print available at: http://arxiv.org/abs/0901.0439

High Energy Physics - TheoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Cosmic microwave backgroundFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)[PACS] Cosmic background radiations01 natural sciencesGeneral Relativity and Quantum CosmologySpectral lineRenormalizationHigh Energy Physics - Phenomenology (hep-ph)[PACS] Particle-theory and field-theory models of the early UniverseQuantum mechanics0103 physical sciencesQuantum field theory010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsSpectral densityCMB cold spot3. Good healthHigh Energy Physics - Phenomenology[PACS] Renormalization in quantum field theoryHigh Energy Physics - Theory (hep-th)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Particle production in the interiors of acoustic black holes

2019

Phonon creation inside the horizons of acoustic black holes is investigated using two simple toy models. It is shown that, unlike what occurs in the exterior regions, the spectrum is not thermal. This non-thermality is due to the anomalous scattering that occurs in the interior regions.

High Energy Physics - TheoryPhononAstrophysics::High Energy Astrophysical Phenomenatoy modelFOS: Physical sciencesParticle production Black holesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologythermalGeneral Relativity and Quantum Cosmology0103 physical sciencesThermal010306 general physicsPhysicsSIMPLE (dark matter experiment)Condensed matter physicsAnomalous scattering010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]scatteringhorizon: acoustic[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]field theory in curved spaceblack hole: acousticFormal aspects of field theoryHigh Energy Physics - Theory (hep-th)Quantum Gases (cond-mat.quant-gas)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]ParticleCondensed Matter - Quantum Gasesphonon: production
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U(N) tools for loop quantum gravity: the return of the spinor

2011

We explore the classical setting for the U(N) framework for SU(2) intertwiners for loop quantum gravity (LQG) and describe the corresponding phase space in terms of spinors with appropriate constraints. We show how its quantization leads back to the standard Hilbert space of intertwiner states defined as holomorphic functionals. We then explain how to glue these intertwiners states in order to construct spin network states as wave-functions on the spinor phase space. In particular, we translate the usual loop gravity holonomy observables to our classical framework. Finally, we propose how to derive our phase space structure from an action principle which induces non-trivial dynamics for the…

High Energy Physics - TheoryPhysics and Astronomy (miscellaneous)FOS: Physical sciencesLoop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesake0103 physical sciences010306 general physicsWave functionMathematical PhysicsMathematical physicsPhysicsSpinor010308 nuclear & particles physicsHilbert spaceObservableMathematical Physics (math-ph)High Energy Physics - Theory (hep-th)Phase spacePhysical Sciencessymbols[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Quantum gravitySpin network
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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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The metric on field space, functional renormalization, and metric-torsion quantum gravity

2015

Searching for new non-perturbatively renormalizable quantum gravity theories, functional renormalization group (RG) flows are studied on a theory space of action functionals depending on the metric and the torsion tensor, the latter parameterized by three irreducible component fields. A detailed comparison with Quantum Einstein-Cartan Gravity (QECG), Quantum Einstein Gravity (QEG), and "tetrad-only" gravity, all based on different theory spaces, is performed. It is demonstrated that, over a generic theory space, the construction of a functional RG equation (FRGE) for the effective average action requires the specification of a metric on the infinite-dimensional field manifold as an addition…

High Energy Physics - TheoryPhysics010308 nuclear & particles physicsAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization group01 natural sciencesGeneral Relativity and Quantum CosmologyRenormalizationGeneral Relativity and Quantum CosmologyTorsion tensorHigh Energy Physics - Theory (hep-th)0103 physical sciencesQuantum gravityFunctional renormalization group010306 general physicsQuantumIrreducible componentMathematical physics
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