Search results for "Observable"

showing 10 items of 634 documents

Progress in three-particle scattering from LQCD

2017

We present the status of our formalism for extracting three-particle scattering observables from lattice QCD (LQCD). The method relies on relating the discrete finite-volume spectrum of a quantum field theory with its scattering amplitudes. As the finite-volume spectrum can be directly determined in LQCD, this provides a method for determining scattering observables, and associated resonance properties, from the underlying theory. In a pair of papers published over the last two years, two of us have extended this approach to apply to relativistic three-particle scattering states. In this talk we summarize recent progress in checking and further extending this result. We describe an extensio…

Physics010308 nuclear & particles physicsScatteringFormalism (philosophy)PhysicsQC1-999High Energy Physics - Lattice (hep-lat)FOS: Physical sciencesObservableLattice QCD01 natural sciencesResonance (particle physics)Scattering amplitudeTheoretical physicsHigh Energy Physics - Lattice0103 physical sciencesBound stateQuantum field theory010306 general physicsEPJ Web of Conferences
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An iterative method in a probabilistic approach to the spectral inverse problem - Differential emission measure from line spectra and broadband data

2010

Inverse problems are of great importance in astrophysics for deriving information about the physical characteristics of hot optically thin plasma sources from their EUV and X-ray spectra. We describe and test an iterative method developed within the framework of a probabilistic approach to the spectral inverse problem for determining the thermal structures of the emitting plasma. We also demonstrate applications of this method to both high resolution line spectra and broadband imaging data. Our so-called Bayesian iterative method (BIM) is an iterative procedure based on Bayes' theorem and is used to reconstruct differential emission measure (DEM) distributions. To demonstrate the abilities …

Physics010504 meteorology & atmospheric sciencesIterative methodProbabilistic logicFOS: Physical sciencesAstronomy and AstrophysicsObservableAstrophysicsInverse problem01 natural sciencesMeasure (mathematics)Spectral lineComputational physicsSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceRobustness (computer science)Sun: corona / Sun: UV radiation / Sun: X-rays gamma rays / atomic data / methods: data analysis / techniques: spectroscopic0103 physical sciencesBroadbandPhysics::Space PhysicsAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciences
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Strongly correlated states of trapped ultracold fermions in deformed Landau levels

2015

We analyze the strongly correlated regime of a two-component trapped ultracold fermionic gas in a synthetic non-Abelian U(2) gauge potential, that consists of both a magnetic field and a homogeneous spin-orbit coupling. This gauge potential deforms the Landau levels (LLs) with respect to the Abelian case and exchanges their ordering as a function of the spin-orbit coupling. In view of experimental realizations, we show that a harmonic potential combined with a Zeeman term, gives rise to an angular momentum term, which can be used to test the stability of the correlated states obtained through interactions. We derive the Haldane pseudopotentials (HPs) describing the interspecies contact inte…

PhysicsAngular momentumZeeman effectStrongly Correlated Electrons (cond-mat.str-el)Quantum GasesFOS: Physical sciencesObservableQuantum entanglementLandau quantizationQuantum Hall effectCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsCondensed Matter - Strongly Correlated Electronssymbols.namesakeQuantum Gases; Strongly Correlated ElectronsTotal angular momentum quantum numberQuantum Gases (cond-mat.quant-gas)Quantum mechanicsQuantum electrodynamicsQuantum GasesymbolsStrongly Correlated ElectronsCondensed Matter - Quantum GasesStrongly correlated states of trapped ultracold fermions in deformed Landau levelsRelative angular momentum
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Cluster Formation during Expansion of Hot and Compressed Nuclear Matter Produced in Central Collisions of Au on Au at 250AMeV

1995

Complete distributions of the light and intermediate mass fragments ({ital Z}=1--6) produced within the polar angular range 1{sup {circ}}{le}{Theta}{sub lab}{le}30{sup {circ}} in highly central collisions of 250{ital A} MeV Au+Au are presented. The results of this measurement and a model analysis are used to study the expansion and clustering of the hot and compressed transient state formed in central collisions of such a heavy system. The influence of the initial conditions on the final observables is discussed.

PhysicsAngular rangeCluster (physics)General Physics and AstronomyPolarObservableAtomic physicsNuclear ExperimentNuclear matterPhysical Review Letters
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Electron-positron density-functional theory.

1986

A two-component density-functional theory is presented for electron-positron systems. The phase diagram of a two-component Fermi-Coulomb system is discussed, and explicit expressions are derived for exchange-correlation functionals for use in the local-density approximation. The scheme is then applied in a fully self-consistent calculation of electron and positron densities in atomic vacancies in metals, treated in the jellium model. Comparison with conventional calculations, which do not meet true electron-positron self-consistency, reveals considerable changes in the density distributions. However, we demonstrate that there are cancellation effects which render the corresponding changes i…

PhysicsAnnihilationPositronQuantum mechanicsJelliumObservableDensity functional theoryElectronPhase diagramPhysical review. B, Condensed matter
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Novel type of CPT violation for correlated Einstein-Podolsky-Rosen states of neutral mesons.

2004

We discuss modifications to the concept of an "antiparticle," induced by a breakdown of the CPT symmetry at a fundamental level, realized within an extended class of quantum gravity models. The resulting loss of particle-antiparticle identity in the neutral-meson system induces a breaking of the Einstein-Podolsky-Rosen correlation imposed by Bose statistics. This is parametrized by a complex parameter associated with the contamination by the "wrong symmetry" state. The physical consequences are studied, and novel observables of CPT violation in phi factories are proposed.

PhysicsAntiparticleMesonCPT symmetryFísicaGeneral Physics and AstronomyObservableQuantum entanglementSymmetry (physics)symbols.namesakeTheoretical physicsQuantum mechanicssymbolsQuantum gravityHigh Energy Physics::ExperimentEPR paradoxPhysical review letters
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The neutrino charge radius is a physical observable

2004

We present a method which allows, at least in principle, the direct extraction of the gauge-invariant and process-independent neutrino charge radius (NCR) from experiments. Under special kinematic conditions, the judicious combination of neutrino and anti-neutrino forward differential cross-sections allows the exclusion of all target-dependent contributions, such as gauge-independent box-graphs, not related to the NCR. We show that the remaining contributions contain universal, renormalization group invariant combinations, such as the electroweak effective charge and the running mixing angle, which must be also separated out. By considering the appropriate number of independent experiments …

PhysicsAstrofísicaNuclear and High Energy PhysicsParticle physicsElectroweak interactionFOS: Physical sciencesWeinberg angleObservableRenormalization groupRenormalizationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Charge radiusNeutrinoLepton
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Dark, Cold, and Noisy: Constraining Secluded Hidden Sectors with Gravitational Waves

2018

We explore gravitational wave signals arising from first-order phase transitions occurring in a secluded hidden sector, allowing for the possibility that the hidden sector may have a different temperature than the Standard Model sector. We present the sensitivity to such scenarios for both current and future gravitational wave detectors in a model-independent fashion. Since secluded hidden sectors are of particular interest for dark matter models at the MeV scale or below, we pay special attention to the reach of pulsar timing arrays. Cosmological constraints on light degrees of freedom restrict the number of sub-MeV particles in a hidden sector, as well as the hidden sector temperature. Ne…

PhysicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsGravitational waveDark matterHigh Energy Physics::PhenomenologyDegrees of freedom (statistics)FOS: Physical sciencesAstronomy and AstrophysicsObservablehep-ph01 natural sciencesStandard ModelHidden sectorHigh Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Pulsar0103 physical sciencesastro-ph.COAstrophysics - Cosmology and Nongalactic AstrophysicsGauge symmetryParticle Physics - Phenomenology
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Diagnostics of stellar flares from X-ray observations: from the decay to the rise phase

2007

The diagnostics of stellar flaring coronal loops have been so far largely based on the analysis of the decay phase. We derive new diagnostics from the analysis of the rise and peak phase of stellar flares. We release the assumption of full equilibrium of the flaring loop at the flare peak, according to the frequently observed delay between the temperature and the density maximum. From scaling laws and hydrodynamic simulations we derive diagnostic formulas as a function of observable quantities and times. We obtain a diagnostic toolset related to the rise phase, including the loop length, density and aspect ratio. We discuss the limitations of this approach and find that the assumption of lo…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Phase (waves)X-raystars: flare X-rays: stars stars: coronaeFOS: Physical sciencesAstronomy and AstrophysicsObservableFunction (mathematics)Coronal loopAstrophysicsAstrophysicsAspect ratio (image)law.inventionLoop (topology)Space and Planetary SciencelawAstrophysics::Solar and Stellar AstrophysicsFlare
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Shock-cloud interaction in the Vela SNR II. Hydrodynamic model

2006

In the framework of the study of the X-ray and optical emission in supernova remnants we focus on an isolated X-ray knot in the northern rim of the Vela SNR (Vela FilD), whose X-ray emission has been studied and discussed in Paper I. We aim at understanding the physical origin of the X-ray and optical emission in FilD, at understanding the role of the different physical processes at work, and at obtaining a key for the interpretation of future X-ray observations of SNRs. To this end we have pursued an accurate ``forward'' modeling of the interaction of the Vela SNR shock with an ISM cloud. We perform hydrodynamic simulations and we directly compare the observables synthesized from the simul…

PhysicsAstrophysics::High Energy Astrophysical PhenomenacloudsISMAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsObservableAstrophysicsThermal conductionVelaAstrophysicsSpectral lineindividual objectVela SNRISMShock wavesSupernovakinematics and dynamicsISMsupernova remnantKnot (unit)Space and Planetary ScienceThermalIntercloudHydrodynamicsISMAstrophysics::Galaxy Astrophysics
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