Search results for "Lorentz"

showing 10 items of 187 documents

Angular Energy Distribution of Collapsar-Jets

2008

Collapsars are fast-spinning, massive stars, whose core collapse liberates an energy, that can be channeled in the form of ultrarelativistic jets. These jets transport the energy from the collapsed core to large distances, where it is dissipated in the form of long-duration gamma-ray bursts. In this paper we study the dynamics of ultrarelativistic jets produced in collapsars. Also we extrapolate our results to infer the angular energy distribution of the produced outflows in the afterglow phase. Our main focus is to look for global energetical properties which can be imprinted by the different structure of different progenitor stars. Thus, we employ a number of pre-supernova, stellar models…

PhysicsJet (fluid)Shock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRotational energyAfterglowCore (optical fiber)StarsLorentz factorsymbols.namesakeSpace and Planetary SciencesymbolsFree expansionAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Galaxy Astrophysics
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Afterglow model for the radio emission from the jetted tidal disruption candidate Swift J1644+57

2012

The recent transient event Swift J1644+57 has been interpreted as emission from a collimated relativistic jet, powered by the sudden onset of accretion onto a supermassive black hole following the tidal disruption of a star. Here we model the radio-microwave emission as synchrotron radiation produced by the shock interaction between the jet and the gaseous circumnuclear medium (CNM). At early times after the onset of the jet (t < 5-10 days) a reverse shock propagates through and decelerates the ejecta, while at later times the outflow approaches the Blandford-McKee self-similar evolution (possibly modified by additional late energy injection). The achromatic break in the radio light curve o…

PhysicsJet (fluid)Supermassive black holeAccretion (meteorology)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaSynchrotron radiationFluxAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curve01 natural sciencesAfterglowLorentz factorsymbols.namesake13. Climate actionSpace and Planetary Science0103 physical sciencessymbols010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
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Test of Time Dilation Using StoredLi+Ions as Clocks at Relativistic Speed

2014

We present the concluding result from an Ives-Stilwell-type time dilation experiment using 7Li+ ions confined at a velocity of β=v/c=0.338 in the storage ring ESR at Darmstadt. A Λ-type three-level system within the hyperfine structure of the 7Li+3S1 →3P2 line is driven by two laser beams aligned parallel and antiparallel relative to the ion beam. The lasers' Doppler shifted frequencies required for resonance are measured with an accuracy of <4×10(-9) using optical-optical double resonance spectroscopy. This allows us to verify the special relativity relation between the time dilation factor γ and the velocity β, γ√1-β2=1 to within ±2.3×10(-9) at this velocity. The result, which is singled …

PhysicsKennedy–Thorndike experimentQuantum mechanicsTime dilation of moving particlesIves–Stilwell experimentGeneral Physics and AstronomyResonanceTime dilationLorentz covarianceAtomic physicsRelativistic Doppler effectRelativistic speedPhysical Review Letters
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Hydrodynamical and Emission Simulations of Relativistic Jets: Stability and Generation of Superluminal and Stationary Components

2001

We present 2D hydrodynamical and emission simulations of the jet stabilityafter the introduction of strong perturbations on a relativistic jet. These simulations show that the interaction of a single strong perturbation with the underlying jet results in the formation of multiple conical shocks with very specific observational properties.

PhysicsLorentz factorsymbols.namesakeSuperluminal motionClassical mechanicsAstrophysical jetAstrophysics::High Energy Astrophysical PhenomenasymbolsPerturbation (astronomy)High Energy Physics::ExperimentConical surfaceCosmologyComputational physics
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Ab Initio Computation of the Longitudinal Response Function in Ca40

2021

We present a consistent ab initio computation of the longitudinal response function ${R}_{L}$ in $^{40}\mathrm{Ca}$ using the coupled-cluster and Lorentz integral transform methods starting from chiral nucleon-nucleon and three-nucleon interactions. We validate our approach by comparing our results for ${R}_{L}$ in $^{4}\mathrm{He}$ and the Coulomb sum rule in $^{40}\mathrm{Ca}$ against experimental data and other calculations. For ${R}_{L}$ in $^{40}\mathrm{Ca}$ we obtain a very good agreement with experiment in the quasielastic peak up to intermediate momentum transfers, and we find that final state interactions are essential for an accurate description of the data. This work presents a m…

PhysicsLorentz transformationNuclear TheoryGeneral Physics and AstronomyFunction (mathematics)State (functional analysis)Integral transformMomentumsymbols.namesakeQuantum mechanicsCoulombsymbolsSum rule in quantum mechanicsNeutrinoPhysical Review Letters
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Partial wave analysis inK-matrix formalism

1995

A description is given of the K-matrix formalism. The formalism, which is normally applied to two-body scattering processes, is generalized to production of two-body channels with finalstate interactions. A multi-channel treatment of production of resonances has been worked out in the P-vector approach of Aitchison. An alternative approach, derived from the P-vector, gives the production amplitude as a product of the T-matrix for a two-body system and a vector Q specifying its production. This formulation, called Q-vector approach here, has also been worked out. Examples of practical importance are given.

PhysicsMany-body problemScattering amplitudeClassical mechanicsPhase spacePartial wave analysisGeneral Physics and AstronomyLorentz covarianceSpace (mathematics)Two-body problemS-matrixMathematical physicsAnnalen der Physik
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Momentum partition between constituents of exotic atoms during laser-induced tunneling ionization

2015

The tunneling ionization of exotic atoms such as muonic hydrogen, muonium, and positronium in a strong laser field of circular polarization is investigated, taking into account the impact of the motion of the center of mass on the the tunneling ionization dynamics. The momentum partition between the ionization products is deduced. The effect of the center-of-mass motion for the momentum distribution of the ionization components is determined. The effect scales with the ratio of the electron (muon) to the atomic core masses and is nonnegligible for exotic atoms, while being insignificant for common atoms. It is shown that the electron (muon) momentum shift during the under-the-barrier motion…

PhysicsMuonSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciPhysics - Atomic PhysicAtomic Physics (physics.atom-ph)FOS: Physical sciencesElectronLaserResearch group K. Z. Hatsagortsyan – Division C. H. KeitelAtomic and Molecular Physics and Opticslaw.inventionPhysics - Atomic Physicssymbols.namesakelawIonizationPhysics::Atomic and Molecular ClusterssymbolsPhysics::Atomic PhysicsAtomic physicsPhysics - Atomic Physics; Physics - Atomic PhysicsLorentz forceCircular polarizationQuantum tunnellingExotic atom
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Benchmark calculations of electromagnetic sum rules with a symmetry-adapted basis and hyperspherical harmonics

2020

We demonstrate the ability to calculate electromagnetic sum rules with the \textit{ab initio} symmetry-adapted no-core shell model. By implementing the Lanczos algorithm, we compute non-energy weighted, energy weighted, and inverse energy weighted sum rules for electric monopole, dipole, and quadrupole transitions in $^4$He using realistic interactions. We benchmark the results with the hyperspherical harmonics method and show agreement within $2\sigma$, where the uncertainties are estimated from the use of the many-body technique. We investigate the dependence of the results on three different interactions, including chiral potentials, and we report on the $^4$He electric dipole polarizabi…

PhysicsNuclear Theory010308 nuclear & particles physicsLorentz transformationLanczos algorithmInverseFOS: Physical sciences01 natural sciencesNuclear Theory (nucl-th)Dipolesymbols.namesakePolarizabilityHarmonicsQuantum mechanics0103 physical sciencesQuadrupolesymbols010306 general physicsEnergy (signal processing)
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Cosmological perturbations in extended electromagnetism. General gauge invariant approach

2013

A certain vector-tensor (VT) theory is revisited. It was proposed and analyzed as a theory of electromagnetism without the standard gauge invariance. Our attention is first focused on a detailed variational formulation of the theory, which leads to both a modified Lorentz force and the true energy momentum tensor of the vector field. The theory is then applied to cosmology. A complete gauge invariant treatment of the scalar perturbations is presented. For appropriate gauge invariant variables describing the scalar modes of the vector field (A-modes), it is proved that the evolution equations of these modes do not involve the scalar modes appearing in General Relativity (GR-modes), which are…

PhysicsNuclear and High Energy PhysicsIntroduction to gauge theoryCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityKaluza–Klein theoryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)General Relativity and Quantum Cosmologysymbols.namesakeLorenz gauge conditionClassical mechanicssymbolsGauge theoryLorentz forceMathematical descriptions of the electromagnetic fieldAstrophysics - Cosmology and Nongalactic AstrophysicsMathematical physics
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Lorentz Multiplet Structure of Baryon Spectra and Relativistic Description

1997

The pole positions of the various baryon resonances are known to reveal well-pronounced clustering, so-called Hoehler clusters. For nonstrange baryons the Hoehler clusters are shown to be identical to Lorentz multiplets of the type (j,j)*[(1/2,0)+(0,1/2)] with j being a half-integer. For the Lambda hyperons below 1800 MeV these clusters are shown to be of the type [(1,0)+ (0,1)]*[(1/2,0)+(0,1/2)] while above 1800 MeV they are parity duplicated (J,0)+(0,J) (Weinberg-Ahluwalia) states. Therefore, for Lambda hyperons the restoration of chiral symmetry takes place above 1800 MeV. Finally, it is demonstrated that the description of spin-3/2 particles in terms of a 2nd rank antisymmetric Lorentz …

PhysicsNuclear and High Energy PhysicsNuclear TheoryAntisymmetric relationLorentz transformationNuclear TheoryHyperonFOS: Physical sciencesGeneral Physics and AstronomyAstronomy and AstrophysicsParity (physics)Spectral lineNuclear Theory (nucl-th)BaryonHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Dirac spinorsymbolsMultipletMathematical physicsModern Physics Letters A
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