0000000000240444

AUTHOR

Sylwia Lewicka

0000-0002-5071-2255

showing 3 related works from this author

Annihilation Characteristics of Confined 2D Positronium

2012

The 2D Positronium (2D Ps) atom confined in the 2D cave has been considered and its properties were compared with the 3D Positronium located in the infinity square well potential. Basing on the solution of Schrödinger equation for the 2D hydrogen atom the wave function of the 2D Ps was given. It allows us to calculate, for instance the angular correlation of the annihilation radiation (ACAR) of such a system. It was shown that the ACAR is much broad than ACAR for the 3D Ps and that for the Ps in the bubble model.

PhysicsAnnihilationMechanical EngineeringBubbleHydrogen atomCondensed Matter PhysicsSchrödinger equationPositroniumCondensed Matter::Materials Sciencesymbols.namesakeMechanics of MaterialsAtomAnnihilation radiationsymbolsFinite potential wellGeneral Materials SciencePhysics::Atomic PhysicsAtomic physicsMaterials Science Forum
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Two-photon positron–electron annihilation in a strong magnetic field

2013

Abstract We consider the two-photon positron and electron annihilation in flight, it means the annihilating particles exhibit the middly relativistic momenta in a super strong magnetic field. Such particles are present in the corona of pulsars and magnetars. The paper presents how the total emission rate for the two-photon process is affected not only by magnetic field but also by the relativistic momentum of the annihilating particles. We found that the momenta influence significantly the total emission rate and the directions of the emitted photons. Additionally, the total emission for the two-photon process is comparable to that for the one-photon process at the momentum of annihilating …

MomentumPhysicsNuclear physicsAnnihilationPhotonPositronAstrophysics::High Energy Astrophysical PhenomenaAstronomy and AstrophysicsElectronMagnetarSpectral lineMagnetic fieldAstroparticle Physics
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Positron Annihilation Characteristics in Superstrong Magnetic Fields

2010

The recent interest in positrons distribution in the space revealed the anomalous presence of high energetic positrons. There are different possible origins of such positrons, including the decay of heavy particles in the dark matter, also pulsars or neutron stars. In our study we calculated the annihilation properties of the electron – positron bound system in superstrong magnetic fields expected for neutron stars. For this aim we use solutions of the (relativistic) Bethe-Salpeter equation derived by L.B. Leinson and A. Perez [1]. The results indicate strong dependency of the annihilation properties (rate and intensity) on the value of the magnetic field.

PhysicsAnnihilationAstrophysics::High Energy Astrophysical PhenomenaMechanical EngineeringDark matterElectronCondensed Matter PhysicsPositroniumMagnetic fieldNuclear physicsNeutron starPositronPulsarMechanics of MaterialsGeneral Materials ScienceAtomic physicsMaterials Science Forum
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