Search results for "Spectral"

showing 10 items of 3116 documents

Multiplicity results for Sturm-Liouville boundary value problems

2009

Multiplicity results for Sturm-Liouville boundary value problems are obtained. Proofs are based on variational methods.

Partial differential equationSturm-Liouville problem variational methodsApplied MathematicsNumerical analysisMultiplicity resultsMathematical analysisSturm–Liouville theoryMixed boundary conditionMathematics::Spectral TheoryMathematical proofCritical point (mathematics)Computational MathematicsSettore MAT/05 - Analisi MatematicaBoundary value problemMathematics
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Operators on Partial Inner Product Spaces: Towards a Spectral Analysis

2014

Given a LHS (Lattice of Hilbert spaces) $V_J$ and a symmetric operator $A$ in $V_J$, in the sense of partial inner product spaces, we define a generalized resolvent for $A$ and study the corresponding spectral properties. In particular, we examine, with help of the KLMN theorem, the question of generalized eigenvalues associated to points of the continuous (Hilbertian) spectrum. We give some examples, including so-called frame multipliers.

Partial inner product spacesPure mathematicsGeneral MathematicsFOS: Physical sciencesresolventLattice (discrete subgroup)01 natural sciencessymbols.namesakeInner product spaceSettore MAT/05 - Analisi MatematicaPIP-spaceframe multipliers}lattices of Hilbert spacesSpectral analysis0101 mathematicsEigenvalues and eigenvectorsMathematical PhysicsMathematicsResolventframe multipliers010102 general mathematicsSpectrum (functional analysis)Spectral propertiesHilbert spaceMathematical Physics (math-ph)010101 applied mathematicssymbolsspectral properties of symmetric operatorsSpectral theory46Cxx 47A10 47B37
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Purification of Lindblad dynamics, geometry of mixed states and geometric phases

2015

We propose a nonlinear Schr\"odinger equation in a Hilbert space enlarged with an ancilla such that the partial trace of its solution obeys to the Lindblad equation of an open quantum system. The dynamics involved by this nonlinear Schr\"odinger equation constitutes then a purification of the Lindbladian dynamics. This nonlinear equation is compared with other Schr\"odinger like equations appearing in the theory of open systems. We study the (non adiabatic) geometric phases involved by this purification and show that our theory unifies several definitions of geometric phases for open systems which have been previously proposed. We study the geometry involved by this purification and show th…

Partial traceQuantum information[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]FOS: Physical sciencesGeneral Physics and AstronomyGeometry01 natural sciencessymbols.namesakeOpen quantum system0103 physical sciencesGauge theory0101 mathematicsQuantum information010306 general physicsAdiabatic processNonlinear Schrödinger equationMathematical PhysicsMathematicsQuantum PhysicsLindblad equation010102 general mathematicsFibre bundlesHilbert spaceCategoryMathematical Physics (math-ph)Quantum PhysicsMathematics::Spectral TheoryGeometric phasesDynamics of open quantum systemsMixed statessymbolsGeometry and TopologyQuantum Physics (quant-ph)
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Linking gamma-ray spectra of supernova remnants to the cosmic ray injection properties in the aftermath of supernovae

2017

The acceleration times of the highest-energy particles which emit gamma-rays in young and middle-age SNRs are comparable with SNR age. If the number of particles starting acceleration was varying during early times after the supernova explosion then this variation should be reflected in the shape of the gamma-ray spectrum. We use the solution of the non-stationary equation for particle acceleration in order to analyze this effect. As a test case, we apply our method to describe gamma-rays from IC443. As a proxy of the IC443 parent supernova we consider SN1987A. First, we infer the time dependence of injection efficiency from evolution of the radio spectral index in SN1987A. Then, we use the…

Particle numberAstrophysics::High Energy Astrophysical PhenomenaSupernovae: generalFOS: Physical sciencesGamma ray spectraCosmic rayAstrophysics01 natural sciences0103 physical sciences010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy AstrophysicsGamma rays: ISMPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Spectral index010308 nuclear & particles physicsGamma raySpectral densityAstronomy and AstrophysicsAstronomy and AstrophysicCosmic rayParticle accelerationSupernovaSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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Do we have any hope of detecting scattering between dark energy and baryons through cosmology?

2020

We consider the possibility that dark energy and baryons might scatter off each other. The type of interaction we consider leads to a pure momentum exchange, and does not affect the background evolution of the expansion history. We parametrize this interaction in an effective way at the level of Boltzmann equations. We compute the effect of dark energy-baryon scattering on cosmological observables, focusing on the Cosmic Microwave Background (CMB) temperature anisotropy power spectrum and the matter power spectrum. Surprisingly, we find that even huge dark energy-baryon cross-sections $\sigma_{xb} \sim {\cal O}({\rm b})$, which are generically excluded by non-cosmological probes such as col…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundCosmic background radiationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)cosmic background radiationAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesCosmologyGeneral Relativity and Quantum Cosmologycosmic background radiation cosmological parameters cosmology observations dark energy large-scale structure of UniverseHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencescosmological parametersdark energy010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsEquation of state (cosmology)Matter power spectrumSpectral densityAstronomy and AstrophysicsCosmic varianceHigh Energy Physics - Phenomenologyobservations13. Climate actionSpace and Planetary ScienceDark energylarge-scale structure of UniversecosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Study of e+e−→γωJ/ψ and Observation of X(3872)→ωJ/ψ

2019

We study the e^{+}e^{-}→γωJ/ψ process using 11.6  fb^{-1} e^{+}e^{-} annihilation data taken at center-of-mass energies from sqrt[s]=4.008  GeV to 4.600 GeV with the BESIII detector at the BEPCII storage ring. The X(3872) resonance is observed for the first time in the ωJ/ψ system with a significance of more than 5σ. The relative decay ratio of X(3872)→ωJ/ψ and π^{+}π^{-}J/ψ is measured to be R=1.6_{-0.3}^{+0.4}±0.2, where the first uncertainty is statistical and the second systematic (the same hereafter). The sqrt[s]-dependent cross section of e^{+}e^{-}→γX(3872) is also measured and investigated, and it can be described by a single Breit-Wigner resonance, referred to as the Y(4200), with …

Particle physicsElectron–positron annihilationGeneral Physics and Astronomy01 natural sciencesSpectral linelaw.inventionLuminosityNuclear physicsCross section (physics)law0103 physical sciencesInvariant massCollider010306 general physicsPhysicsAnnihilationMass distribution010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyOrder (ring theory)ResonanceBaryonPhase spaceHigh Energy Physics::ExperimentCenter of massAtomic physicsEnergy (signal processing)Storage ringBar (unit)X(3872)Physical Review Letters
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Observational signatures of Higgs inflation

2016

We investigate the dependency of Higgs inflation on the non-renormalisable matching between the low energy Standard Model limit and the inflationary regime at high energies. We show that for the top mass range $m_t \gtrsim 171.8$ GeV the scenario robustly predicts the spectral index $n_s \simeq 0.97$ and the tensor-to-scalar ratio $r\simeq 0.003$. The matching is however non-trivial, even the best-fit values $m_h=125.09$ GeV and $m_t=173.21$ GeV require a jump $\delta \lambda \sim 0.01$ in the Higgs coupling below the inflationary scale. For $m_t\lesssim 171.8$ GeV, the matching may generate a feature in the inflationary potential. In this case the predicted values of $n_s$ and $r$ vary but…

Particle physicsMatching (statistics)Cosmology and Nongalactic Astrophysics (astro-ph.CO)STANDARD MODELFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesphysics of the early universeinflationELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMBosonInflation (cosmology)PhysicsSpectral index010308 nuclear & particles physicsINDUCED GRAVITY INFLATIONHigh Energy Physics::PhenomenologySpectral densityBOSONAstronomy and Astrophysics115 Astronomy Space scienceHigh Energy Physics - Phenomenologyparticle physics - cosmology connectionJumpHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Axion cold dark matter: Status after Planck and BICEP2

2014

We investigate the axion dark matter scenario (ADM), in which axions account for all of the dark matter in the Universe, in light of the most recent cosmological data. In particular, we use the Planck temperature data, complemented by WMAP E-polarization measurements, as well as the recent BICEP2 observations of B-modes. Baryon Acoustic Oscillation data, including those from the Baryon Oscillation Spectroscopic Survey, are also considered in the numerical analyses. We find that, in the minimal ADM scenario, the full dataset implies that the axion mass m_a = 82.2 pm 1.1 {\mu}eV (corresponding to the Peccei-Quinn symmetry being broken at a scale f_a = (7.54 pm 0.10)*10^10 GeV), or m_a = 76.6 …

Particle physicsNuclear and High Energy PhysicsCold dark matterCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)INFLATIONPlanckAxionPhysicsSpectral indexHigh Energy Physics::PhenomenologyFísicaPlanck temperatureINVISIBLE AXIONBARYON ACOUSTIC-OSCILLATIONS; DIGITAL SKY SURVEY; INVISIBLE AXION; COSMOLOGY; INFLATION; DISTANCEBaryonHigh Energy Physics - PhenomenologyCOSMOLOGYDISTANCEsymbolsDark energyAstronomiaDIGITAL SKY SURVEYBARYON ACOUSTIC-OSCILLATIONSAstrophysics - Cosmology and Nongalactic Astrophysics
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Two-particle angular correlations in e(+)e(-) interactions compared with QCD predictions

1998

Two-particle angular correlations in jet cones have been measured in e(+)e(-) annihilation into hadrons at LEP energies (root s = 91 and 183 GeV) and are compared with QCD predictions using the LPHD hypothesis. Two different functions have been tested. While the differentially normalized correlation function shows substantial deviations from the predictions, a globally normalized correlation function agrees well. The size of alpha(s)(eff) land other QCD parameters) and its running with the relevant angular scale, the validity of LPHD, and problems due to non-perturbative effects are discussed critically. (C) 1998 Elsevier Science B.V. All rights reserved.

Particle physicsNuclear and High Energy PhysicsHadronMonte Carlo methodJet (particle physics)01 natural sciencesPartícules (Física nuclear)Spectral lineNuclear physicsMONTE-CARLO0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SPECTRA010306 general physicsDELPHIPhysicsQuantum chromodynamicsMONTE-CARLO; JETS; SPECTRAAnnihilation010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFunction (mathematics)LARGE ELECTRON POSITRON COLLIDERPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHILarge Electron–Positron ColliderJETSPARTICLE PHYSICSFísica nuclearHigh Energy Physics::ExperimentParticle Physics - Experiment
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Unraveling the pattern of the XYZ mesons

2014

We present a plausible mechanism for the origin of the $XYZ$ mesons in the heavy meson spectra within a standard quark-model picture. We discuss the conditions required for the existence of four--quark bound states or resonances contributing to the heavy meson spectra, being either compact or molecular. We concentrate on charmonium and bottomonium spectra, where several new states, difficult to understand as simple quark-antiquark pairs, have been reported by different experimental collaborations. The pivotal role played by entangled meson-meson thresholds is emphasized.

Particle physicsNuclear and High Energy PhysicsMesonNuclear TheoryHigh Energy Physics::LatticeNuclear TheoryFOS: Physical sciencesQuantum entanglementSpectral lineNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)Bound stateB mesonNuclear ExperimentPhysicsQuark modelEta mesonHigh Energy Physics::PhenomenologyFísicalcsh:QC1-999J/psi mesonHigh Energy Physics - PhenomenologyHigh Energy Physics::Experimentlcsh:Physics
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