Search results for "FOS"

showing 10 items of 15075 documents

Free Fields for Chiral 2D Dilaton Gravity

1998

We give an explicit canonical transformation which transforms a generic chiral 2D dilaton gravity model into a free field theory.

AstrofísicaPhysicsGravitacióNuclear and High Energy PhysicsGravity (chemistry)Canonical quantizationHigh Energy Physics::LatticeFOS: Physical sciencesCanonical transformationGeneral Relativity and Quantum Cosmology (gr-qc)Free fieldGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyGravity model of tradeQuantum gravityDilatonMathematical physics
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Gravitational wave content and stability of uniformly, rotating, triaxial neutron stars in general relativity

2017

Targets for ground-based gravitational wave interferometers include continuous, quasiperiodic sources of gravitational radiation, such as isolated, spinning neutron stars. In this work we perform evolution simulations of uniformly rotating, triaxially deformed stars, the compressible analogues in general relativity of incompressible, Newtonian Jacobi ellipsoids. We investigate their stability and gravitational wave emission. We employ five models, both normal and supramassive, and track their evolution with different grid setups and resolutions, as well as with two different evolution codes. We find that all models are dynamically stable and produce a strain that is approximately one-tenth …

AstrofísicaPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveGeneral relativityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Compact star01 natural sciencesGeneral Relativity and Quantum CosmologyArticleGravitational energyNumerical relativityClassical mechanicsTests of general relativity0103 physical sciencesAstronomiaTwo-body problem in general relativityAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGravitational redshift
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The stratified two-sided jet of Cygnus A. Acceleration and collimation

2015

High-resolution Very-Long-Baseline Interferometry observations of relativistic jets are essential to constrain fundamental parameters of jet formation models. At a distance of 249 Mpc, Cygnus A is a unique target for such studies, being the only Fanaroff-Riley Class II radio galaxy for which a detailed sub-parsec scale imaging of the base of both jet and counter-jet can be obtained. Observing at millimeter wavelengths unveils those regions which appear self-absorbed at longer wavelengths and enables an extremely sharp view towards the nucleus to be obtained. We performed 7 mm Global VLBI observations, achieving ultra-high resolution imaging on scales down to 90 $\mu$as. This resolution corr…

AstrofísicaPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Jet (fluid)010504 meteorology & atmospheric sciencesRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAcceleration (differential geometry)Astrophysics01 natural sciencesBase (group theory)WavelengthAstrophysical jetSpace and Planetary Science0103 physical sciencesAstronomiaCygnus AAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSchwarzschild radius0105 earth and related environmental sciences
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Revising the observable consequences of slow-roll inflation

2009

We study the generation of primordial perturbations in a (single-field) slow-roll inflationary Universe. In momentum space, these (Gaussian) perturbations are characterized by a zero mean and a nonzero variance Delta(2) (k, t). However, in position space the variance diverges in the ultraviolet. The requirement of a finite variance in position space forces one to regularize Delta(2) (k, t). This can (and should) be achieved by proper renormalization in an expanding Universe in a unique way. This affects the predicted scalar and tensorial power spectra (evaluated when the modes acquire classical properties) for wavelengths that today are at observable scales. As a consequence, the imprint of…

AstrofísicaPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Slow roll010308 nuclear & particles physicsFOS: Physical sciencesUnivers inflacionariPrivate communicationGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyManagementHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum mechanics0103 physical sciences010306 general physicsUltraviolet radiationAstrophysics - Cosmology and Nongalactic Astrophysics
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Dynamic transition to spontaneous scalarization in boson stars

2010

We show that the phenomenon of spontaneous scalarization predicted in neutron stars within the framework of scalar-tensor tensor theories of gravity, also takes place in boson stars without including a self-interaction term for the boson field (other than the mass term), contrary to what was claimed before. The analysis is performed in the physical (Jordan) frame and is based on a 3+1 decomposition of spacetime assuming spherical symmetry.

AstrofísicaPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Scalar bosonGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum CosmologyTheoretical physicsNumerical relativityNeutron starStarsQuantum mechanicsAstronomiaQuantum gravityQuantum field theoryBosonPhysical Review D
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Constraint preserving boundary conditions for the Z4c formulation of general relativity

2010

We discuss high order absorbing constraint preserving boundary conditions for the Z4c formulation of general relativity coupled to the moving puncture family of gauges. We are primarily concerned with the constraint preservation and absorption properties of these conditions. In the frozen coefficient approximation, with an appropriate first order pseudo-differential reduction, we show that the constraint subsystem is boundary stable on a four dimensional compact manifold. We analyze the remainder of the initial boundary value problem for a spherical reduction of the Z4c formulation with a particular choice of the puncture gauge. Numerical evidence for the efficacy of the conditions is prese…

AstrofísicaPhysicsNuclear and High Energy PhysicsGeneral relativityMathematical analysisBoundary (topology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologySymmetry (physics)Constraint (information theory)Numerical relativityTheory of relativityClassical mechanicsAstronomiaCircular symmetryBoundary value problem
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An intermediate γ beta-beam neutrino experiment with long baseline

2008

In order to address some fundamental questions in neutrino physics a wide, future programme of neutrino oscillation experiments is currently under discussion. Among those, long baseline experiments will play a crucial role in providing information on the value of theta13, the type of neutrino mass ordering and on the value of the CP-violating phase delta, which enters in 3-neutrino oscillations. Here, we consider a beta-beam setup with an intermediate Lorentz factor gamma=450 and a baseline of 1050 km. This could be achieved in Europe with a beta-beam sourced at CERN to a detector located at the Boulby mine in the United Kingdom. We analyse the physics potential of this setup in detail and …

AstrofísicaPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsPhase (waves)FOS: Physical sciencesOrder (ring theory)hep-phType (model theory)7. Clean energy01 natural sciencesHigh Energy Physics - PhenomenologyLorentz factorsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencessymbolsSensitivity (control systems)Neutrino010306 general physicsNeutrino oscillationJournal of High Energy Physics
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Super-NOvA: a long-baseline neutrino experiment with two off-axis detectors

2005

Establishing the neutrino mass hierarchy is one of the fundamental questions that will have to be addressed in the next future. Its determination could be obtained with long-baseline experiments but typically suffers from degeneracies with other neutrino parameters. We consider here the NOvA experiment configuration and propose to place a second off-axis detector, with a shorter baseline, such that, by exploiting matter effects, the type of neutrino mass hierarchy could be determined with only the neutrino run. We show that the determination of this parameter is free of degeneracies, provided the ratio L/E, where L the baseline and E is the neutrino energy, is the same for both detectors.

AstrofísicaPhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemType (model theory)Particle identificationNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorMeasurements of neutrino speedInvariant massHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationParticle Physics - Phenomenology
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Disentangling neutrino-nucleon cross section and high energy neutrino flux with akm3neutrino telescope

2007

The energy--zenith angular event distribution in a neutrino telescope provides a unique tool to determine at the same time the neutrino-nucleon cross section at extreme kinematical regions, and the high energy neutrino flux. By using a simple parametrization for fluxes and cross sections, we present a sensitivity analysis for the case of a km^3 neutrino telescope. In particular, we consider the specific case of an under-water Mediterranean telescope placed at the NEMO site, although most of our results also apply to an under-ice detector such as IceCube. We determine the sensitivity to departures from standard values of the cross sections above 1 PeV which can be probed independently from a…

AstrofísicaPhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesCosmic raySolar neutrino problemAstrophysicslaw.inventionTelescopeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorlawMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationPhysical Review D
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Neutrino masses and their ordering: global data, priors and models

2018

We present a Bayesian analysis of the combination of current neutrino oscillation, neutrinoless double beta decay and CMB observations. Our major goal is to carefully investigate the possibility to single out one neutrino mass ordering, Normal Ordering or Inverted Ordering, with current data. Two possible parametrizations (three neutrino masses versus the lightest neutrino mass plus the two oscillation mass splittings) and priors (linear versus logarithmic) are examined. We find that the preference for NO is only driven by neutrino oscillation data. Moreover, the values of the Bayes factor indicate that the evidence for NO is strong only when the scan is performed over the three neutrino ma…

AstrofísicaPhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyCosmic background radiationFOS: Physical sciencesAstronomy and AstrophysicsObservableParameter space01 natural sciencesPartícules (Física nuclear)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesPrior probabilityHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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