Search results for "Variant"

showing 10 items of 1267 documents

Amplitude Analysis of theB±→φK*(892)±Decay

2007

We perform an amplitude analysis of B-+/-->phi(1020)K-*(892)(+/-) decay with a sample of about 384x10(6) B (B) over bar pairs recorded with the BABAR detector. Overall, twelve parameters are measured, including the fractions of longitudinal f(L) and parity-odd transverse f(perpendicular to) amplitudes, branching fraction, strong phases, and six parameters sensitive to CP violation. We use the dependence on the K pi invariant mass of the interference between the J(P)=1(-) and 0(+) K pi components to resolve the discrete ambiguity in the determination of the strong and weak phases. Our measurements of f(L)=0.49 +/- 0.05 +/- 0.03, f(perpendicular to)=0.21 +/- 0.05 +/- 0.02, and the strong phas…

Physics010308 nuclear & particles physicsBranching fractionElectron–positron annihilationAnalytical chemistryGeneral Physics and Astronomy01 natural sciencesHelicityNuclear physicsParticle decayAmplitudePair production0103 physical sciencesCP violationHigh Energy Physics::ExperimentInvariant mass010306 general physicsPhysical Review Letters
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Observation ofe+e−→γX(3872)at BESIII

2014

Using data collected with the BESIII detector operating at the Beijing Electron Positron Collider at center-of-mass energies of root s = 4.23, 4.26, and 4.36 GeV, we observe e(+)e(-) -> pi(0)pi(0)h(c) for the first time. The Born cross sections are measured and found to be about half of those of e(+)e(-) -> pi(+)pi(-)h(c) within less than 2 sigma. In the pi(0)h(c) mass spectrum, a structure at 4.02 GeV/c(2) is found. It is most likely to be the neutral isospin partner of the Z(c)(4020)(+/-) observed in the process of e(+)e(-) -> pi(+)pi(-)h(c) being found. A fit to the pi(0)h(c) invariant mass spectrum, with the width of the Z(c)(4020)(0) fixed to that of its charged isospin partner and pos…

Physics010308 nuclear & particles physicsBranching fractionElectron–positron annihilationAnalytical chemistryGeneral Physics and AstronomySigmaElectronMass spectrometry01 natural sciencesNuclear physicsPositronIsospin0103 physical sciencesPiMass spectrumRadiative transitionHigh Energy Physics::ExperimentInvariant massCenter of massAtomic physicsNuclear Experiment010306 general physicsStorage ringPhysical Review Letters
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Anomalous enhancement of the isospin-violating Λ(1405) production by a triangle singularity in Λc→π+π0π0Σ0

2018

The decay of ${\mathrm{\ensuremath{\Lambda}}}_{c}^{+}$ into ${\ensuremath{\pi}}^{+}{\ensuremath{\pi}}^{0}\mathrm{\ensuremath{\Lambda}}(1405)$ with the $\mathrm{\ensuremath{\Lambda}}(1405)$ decay into ${\ensuremath{\pi}}^{0}{\mathrm{\ensuremath{\Sigma}}}^{0}$ through a triangle diagram is studied. This process is initiated by ${\mathrm{\ensuremath{\Lambda}}}_{c}^{+}\ensuremath{\rightarrow}{\ensuremath{\pi}}^{+}{\overline{K}}^{*}N$, and then the ${\overline{K}}^{*}$ decays into $\overline{K}\ensuremath{\pi}$ and $\overline{K}N$ produce the $\mathrm{\ensuremath{\Lambda}}(1405)$ through a triangle loop containing ${\overline{K}}^{*}N\overline{K}$ which develops a singularity around 1890 MeV. Th…

Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadronLambda01 natural sciencesLoop (topology)SingularityIsospin0103 physical sciencesMass spectrumProduction (computer science)Invariant mass010306 general physicsMathematical physicsPhysical Review D
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Big bounce and future time singularity resolution in Bianchi i cosmologies: The projective invariant Nieh-Yan case

2021

We extend the notion of the Nieh-Yan invariant to generic metric-affine geometries, where both torsion and nonmetricity are taken into account. Notably, we show that the properties of projective invariance and topologicity can be independently accommodated by a suitable choice of the parameters featuring this new Nieh-Yan term. We then consider a special class of modified theories of gravity able to promote the Immirzi parameter to a dynamical scalar field coupled to the Nieh-Yan form, and we discuss in more detail the dynamics of the effective scalar tensor theory stemming from such a revised theoretical framework. We focus, in particular, on cosmological Bianchi I models and we derive cla…

Physics010308 nuclear & particles physicsInitial singularityImmirzi parameter01 natural sciencesScalar–tensor theoryTheoretical physicsGeneral Relativity and Quantum CosmologySingularity0103 physical sciencesGravitational singularityInvariant (mathematics)010306 general physicsScalar fieldBig Bounce
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Positioning systems in Minkowski space-time: from emission to inertial coordinates

2009

The coordinate transformation between emission coordinates and inertial coordinates in Minkowski space-time is obtained for arbitrary configurations of the emitters. It appears that a positioning system always generates two different coordinate domains, namely, the front and the back emission coordinate domains. For both domains, the corresponding covariant expression of the transformation is explicitly given in terms of the emitter world-lines. This task requires the notion of orientation of an emitter configuration. The orientation is shown to be computable from the emission coordinates for the users of a `central' region of the front emission coordinate domain. Other space-time regions a…

Physics04.20.Cv95.10.JkInertial frame of reference45.20.DdPhysics and Astronomy (miscellaneous)Positioning systemAstrophysics::High Energy Astrophysical PhenomenaCoordinate systemMathematical analysisFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Domain (mathematical analysis)General Relativity and Quantum Cosmology04.20.-qTransformation (function)Orientation (geometry)Minkowski spaceCovariant transformation
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Removal of Resonances

2001

From the perturbative procedure in the last chapter we have learned that in the proximity of resonances of the unperturbed system, resonant denominators appear in the expression for the adiabatic invariants. We now wish to begin to locally remove such resonances by trying, with the help of a canonical transformation, to go to a coordinate system which rotates with the resonant frequency.

PhysicsAdiabatic invariantCoordinate systemCanonical transformationPrimary resonanceExpression (computer science)Adiabatic processMathematical physics
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Analysis of the γγ→DD¯ reaction and the DD¯ bound state

2021

In this work, we investigate the reaction of $\ensuremath{\gamma}\ensuremath{\gamma}\ensuremath{\rightarrow}D\overline{D}$, taking into account the $S$-wave $D\overline{D}$ final state interaction. By fitting to the $D\overline{D}$ invariant mass distributions measured by the Belle and BABAR Collaborations, we obtain a good reproduction of the data by means of a $D\overline{D}$ amplitude that produces a bound $D\overline{D}$ state with isospin $I=0$ close to threshold. The error bands of the fits indicate, however, that more precise data on this reaction are needed to be more assertive about the position and width of such a state.

PhysicsAmplitudePosition (vector)IsospinHigh Energy Physics::PhenomenologyBound stateInvariant massState (functional analysis)Mathematical physicsPhysical Review D
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Can conformal Transformations change the fate of 2D black holes?

1998

By using a classical Liouville-type model of two dimensional dilaton gravity we show that the one-loop theory implies that the fate of a black hole depends on the conformal frame. There is one frame for which the evaporation process never stops and another one leading to a complete disappearance of the black hole. This can be seen as a consequence of the fact that thermodynamic variables are not conformally invariant. In the second case the evaporation always produces the same static and regular end-point geometry, irrespective of the initial state.

PhysicsAstrofísicaHigh Energy Physics - TheoryNuclear and High Energy PhysicsGravitacióFOS: Physical sciencesConformal mapGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Dilaton
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Improved cosmological bound on the thermal axion mass

2007

Relic thermal axions could play the role of an extra hot dark matter component in cosmological structure formation theories. By combining the most recent observational data we improve previous cosmological bounds on the axion mass m_a in the so-called hadronic axion window. We obtain a limit on the axion mass m_a < 0.42eV at the 95% c.l. (m_a < 0.72eV at the 99% c.l.). A novel aspect of the analysis presented here is the inclusion of massive neutrinos and how they may affect the bound on the axion mass. If neutrino masses belong to an inverted hierarchy scheme, for example, the above constraint is improved to m_a < 0.38eV at the 95% c.l. (m_a < 0.67eV at the 99% c.l.). Future da…

PhysicsAstrofísicaNuclear and High Energy PhysicsParticle physicsStructure formationAxion Dark Matter ExperimentPhysics::Instrumentation and DetectorsHot dark matterAstrophysics (astro-ph)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGeneral Relativity and Quantum CosmologyCosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Invariant massHigh Energy Physics::ExperimentNeutrinoAxion
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Chiral perturbation theory study of the axial N -> Delta(1232) transition

2008

We have performed a theoretical study of the axial Nucleon to Delta(1232) ($N\to\Delta$) transition form factors up to one-loop order in covariant baryon chiral perturbation theory within a formalism in which the unphysical spin-1/2 components of the $\Delta$ fields are decoupled.

PhysicsBaryonHigh Energy Physics - PhenomenologyNuclear and High Energy PhysicsParticle physicsChiral perturbation theoryGeneral Physics and AstronomyOrder (ring theory)FísicaAstronomy and AstrophysicsCovariant transformationNucleonMathematical physics
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