Search results for "Nuclear and High Energy Physic"

showing 10 items of 8253 documents

Testing standard and nonstandard neutrino physics with cosmological data

2012

Cosmological constraints on the sum of neutrino masses and on the effective number of neutrino species in standard and nonstandard scenarios are computed using the most recent available cosmological data. Our cosmological data sets include the measurement of the baryonic acoustic oscillation (BAO) feature in the data release 9 CMASS sample of the baryon oscillation spectroscopic survey. We study in detail the different degeneracies among the parameters, as well as the impact of the different data sets used in the analyses. When considering bounds on the sum of the three active neutrino masses, the information in the BAO signal from galaxy clustering measurements is approximately equally pow…

AstrofísicaNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic background radiationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesCosmologyPower spectrumsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino oscillationTelescope010303 astronomy & astrophysicsDigital sky surveyPhysicsHubble constantCosmologia010308 nuclear & particles physicsMatter power spectrumBig-bang nucleosynthesisCMB cold spotHigh Energy Physics - Phenomenology13. Climate actionParameterssymbolsBaryon acoustic-oscillationsBaryon acoustic oscillationsNeutrinoData releaseAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's lawPhysical Review D
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Neutrino mass hierarchy extraction using atmospheric neutrinos in ice

2008

We show that the measurements of 10 GeV atmospheric neutrinos by an upcoming array of densely packed phototubes buried deep inside the IceCube detector at the South Pole can be used to determine the neutrino mass hierarchy for values of sin^2(2theta13) close to the present bound, if the hierarchy is normal. These results are obtained for an exposure of 100 Mton years and systematic uncertainties up to 10%.

AstrofísicaNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesStatistical analysis010306 general physicsNeutrino oscillationPhysicsHierarchy (mathematics)010308 nuclear & particles physicsAstrophysics (astro-ph)DetectorAstrophysics::Instrumentation and Methods for AstrophysicsHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoMass hierarchy
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Atmospheric neutrinos in ice and measurement of neutrino oscillation parameters

2010

The main goal of the IceCube Deep Core array is to search for neutrinos of astrophysical origins. Atmospheric neutrinos are commonly considered as a background for these searches. We show that the very high statistics atmospheric neutrino data can be used to obtain precise measurements of the main oscillation parameters.

AstrofísicaNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemCosmic neutrino backgroundHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomy
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Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

2014

The surface detector array of the Pierre Auger Observatory provides information about the longitudinal development of the muonic component of extensive air showers. Using the timing information from the flash analog-to-digital converter traces of surface detectors far from the shower core, it is possible to reconstruct a muon production depth distribution. We characterize the goodness of this reconstruction for zenith angles around 60° and different energies of the primary particle. From these distributions, we define Xμmax as the depth along the shower axis where the production of muons reaches maximum. We explore the potentiality of Xμmax as a useful observable to infer the mass compositi…

AstrofísicaPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomyCiencias Físicasmuonshadronic interaction modelsAstrophysics01 natural sciencesHigh Energy Physics - ExperimentAuger//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Air showersProduction depthSURFACE DETECTOR ARRAY[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHigh-Energy Cosmic Rays[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsDetectorAstrophysics::Instrumentation and Methods for Astrophysics[ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Pierre Auger ObservatoryObservableInstrumentation and Detectors (physics.ins-det)COSMIC-RAYSlongitudinal developmentCore (optical fiber)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayNuclear physicscosmic rays[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesextensive air showers[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasPierre Auger ObservatoryMuon010308 nuclear & particles physics[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Física//purl.org/becyt/ford/1.3 [https]ASTROFÍSICA[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomíaMODELExperimental High Energy PhysicsHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][ PHYS.ASTR.IM ] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]muonic componentSYSTEM
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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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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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Accretion disks around binary black holes of unequal mass: General relativistic MHD simulations of postdecoupling and merger

2014

We report results from simulations in general relativity of magnetized disks accreting onto merging black hole binaries, starting from relaxed disk initial data. The simulations feature an effective, rapid radiative cooling scheme as a limiting case of future treatments with radiative transfer. Here we evolve the systems after binary-disk decoupling through inspiral and merger, and analyze the dependence on the binary mass ratio with $q\ensuremath{\equiv}{m}_{\text{bh}}/{M}_{\mathrm{BH}}=1,1/2$, and $1/4$. We find that the luminosity associated with local cooling is larger than the luminosity associated with matter kinetic outflows, while the electromagnetic (Poynting) luminosity associated…

AstrofísicaPhysicsNuclear and High Energy PhysicsActive galactic nucleusX-ray bursterAstrophysics::High Energy Astrophysical PhenomenaAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsMass ratioBlack holeBinary black holeIntermediate-mass black holeAstronomiaStellar black holeSpin-flipAstrophysics::Galaxy AstrophysicsPhysical Review D
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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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(Standard model) universe dominated by the right matter

2009

14 pages, 3 figures. References on late time enthropy release included, several points clarified. PACS numbers: 14.60.Pq, 98.80.Cq. ArXiv pre-print available at http://arxiv.org/abs/0806.4389

AstrofísicaPhysicsNuclear and High Energy PhysicsParticle physicsGrand-Unified-TheoryDark-MatterHigh Energy Physics::PhenomenologyElectroweak interactionDark matterBaryogenesisFísicaAstrophysics::Cosmology and Extragalactic AstrophysicsTime Entropy ProductionBaryogenesisBaryon asymmetryDecaying ParticlesConstraintsHigh Energy Physics::ExperimentGravitinoNeutrinoNeutrino MassNeutrino oscillationPhenomenology (particle physics)Inflationary UniversePhysical Review D
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