Search results for "mass ratio"

showing 10 items of 40 documents

Influence of self-gravity on the runaway instability of black-hole-torus systems.

2010

Results from the first fully general relativistic numerical simulations in axisymmetry of a system formed by a black hole surrounded by a self-gravitating torus in equilibrium are presented, aiming to assess the influence of the torus self-gravity on the onset of the runaway instability. We consider several models with varying torus-to-black hole mass ratio and angular momentum distribution orbiting in equilibrium around a non-rotating black hole. The tori are perturbed to induce the mass transfer towards the black hole. Our numerical simulations show that all models exhibit a persistent phase of axisymmetric oscillations around their equilibria for several dynamical timescales without the …

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Angular momentumAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesTorusMechanicsGeneral Relativity and Quantum Cosmology (gr-qc)Mass ratioInstabilityGeneral Relativity and Quantum CosmologyBlack holeNumerical relativityGeneral Relativity and Quantum CosmologyClassical mechanicsRotating black holeSpin-flipAstrophysics - High Energy Astrophysical PhenomenaPhysical review letters
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Deceleration of antiprotons from MeV to keV energies

1993

Trapping of antiprotons for high precision measurements at the Low Energy Antiproton Ring (LEAR/CERN) requires the deceleration of the antiproton beam from typically 5.8 MeV energy down to 10 keV for final capture in standard Penning traps. Two methods, the degradation of the beam in thin foils and the deceleration of the beam in an inverse cyclotron are investigated so far. The foil technique was successfully demonstrated with trapping efficiencies up to a few 10−4 and is now routinely used in the high precision measurement of the antiprotonproton mass ratio. The degradation foil method is compared with the deceleration technique using an inverse cyclotron tested also at LEAR.

PhysicsNuclear and High Energy PhysicsLarge Hadron ColliderCyclotronTrappingMass ratioCondensed Matter PhysicsAtomic and Molecular Physics and Opticslaw.inventionNuclear physicsAntiproton beamPhysics::Plasma PhysicslawAntiprotonPhysics::Accelerator PhysicsPhysics::Atomic PhysicsPhysical and Theoretical ChemistryAtomic physicsNuclear ExperimentBeam (structure)FOIL methodHyperfine Interactions
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A direct determination of the proton-electron mass ratio

1978

The cyclotron resonance of protons and electrons in a magnetic field of 5.7 Tesla produced by a superconducting solenoid has been measured. Protons and electrons were alternately confined in an electrostatic quadrupole trap. The quotient of the cyclotron frequencies provides a first direct determination of the proton-electron mass ratio. The result ofM p /M e =1836.1502(53) agrees with other more precise but indirect determinations of this quantity.

PhysicsNuclear and High Energy PhysicsNuclear TheoryCyclotronCyclotron resonanceElectronProton-to-electron mass ratioFourier transform ion cyclotron resonanceElectron cyclotron resonancelaw.inventionNuclear physicslawQuadrupolePhysics::Accelerator PhysicsAtomic physicsIon cyclotron resonanceZeitschrift f�r Physik A: Atoms and Nuclei
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A direct determination of the proton electron mass ratio

1980

The cyclotron frequencies of free protons and electrons in a magnetic field of 5.81 Tesla with superimposed electrostatic quadrupole field have been measured. The increase of energy connected with a transition at cyclotron frequency is detected by the measurement of the time of flight through an inhomogeneous magnetic field. From the ratio of the measured cyclotron frequencies of both particles the proton electron mass ratio is deduced. The resultm p /m e =1,836.1527(11) agrees within the limits of error (0.6 ppm) with the value of the indirect determination.

PhysicsNuclear and High Energy PhysicsTime of flightlawCyclotronCyclotron resonanceElectronAtomic physicsProton-to-electron mass ratioElectron cyclotron resonanceFourier transform ion cyclotron resonanceIon cyclotron resonancelaw.inventionZeitschrift f�r Physik A: Atoms and Nuclei
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Observation of mass-asymmetric fission of mercury nuclei in heavy ion fusion

2015

Background: Mass-asymmetric fission has been observed in low energy fission of $^{180}\mathrm{Hg}$. Calculations predicted the persistence of asymmetric fission in this region even at excitation energies of 30--40 MeV.Purpose: To investigate fission mass distributions by populating different isotopes of Hg using heavy ion fusion reactions.Methods: Fission fragment mass-angle distributions have been measured for two reactions, $^{40}\mathrm{Ca}+^{142}\mathrm{Nd}$ and $^{13}\mathrm{C}+^{182}\mathrm{W}$, populating $^{182}\mathrm{Hg}$ and $^{195}\mathrm{Hg}$, respectively, using the Heavy Ion Accelerator Facility and CUBE spectrometer at the Australian National University. Measurements were ma…

PhysicsNuclear and High Energy Physicseducation.field_of_studyIsotopeSpectrometerFissionNuclear TheoryPopulationMass ratioSaddle pointNeutronAtomic physicsNuclear ExperimenteducationExcitationPhysical Review C
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$a_0-f_0$ mixing in the Khuri-Treiman equations for $\eta\to 3\pi$

2015

A reliable determination of the isospin breaking double quark mass ratio from precise experimental data on $\eta\to 3\pi$ decays should be based on the chiral expansion of the amplitude supplemented with a Khuri-Treiman type dispersive treatment of the final-state interactions. We discuss an extension of this formalism which allows to estimate the effects of the $a_0(980)$ and $f_0(980)$ resonances and their mixing on the $\eta\to 3\pi$ amplitudes. Matrix generalisations of the equations describing elastic $\pi\pi$ rescattering with $I=0,\,2$ are introduced which accomodate both $\pi\pi/K\bar{K}$ and $\eta\pi/K\bar{K}$ coupled-channel rescattering. Isospin violation induced by the physical …

PhysicsQuarkParticle physicsHigh Energy Physics::PhenomenologyDalitz plotResonanceMass ratioFormalism (philosophy of mathematics)High Energy Physics - PhenomenologyAmplitude[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]IsospinPiHigh Energy Physics::ExperimentNuclear Experiment
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Meson decay studies from MAMI A2

2019

Decays of the light mesons π0, η, ω, and η’ provide a unique laboratory to test fundamental aspects of hadron physics. Precision studies of such diverse topics as the light quark mass ratio, π−π scattering lengths, and searches for physics beyond the Standard Model are possible. Additionally, Dalitz decays of light mesons provide a way of measuring the electromagnetic meson transition formfactors in the time-like region. The A2 tagged photon facility at the Mainz Microtron provides a high yield of light mesons produced by photo-induced reactions on protons, which makes the experiment ideal for high precision measurements of meson decays. Presented here are the contributions made by the A2 c…

PhysicsQuarkParticle physicsPhotonMeson010308 nuclear & particles physicsScatteringPhysicsQC1-999Physics beyond the Standard ModelHigh Energy Physics::PhenomenologyNuclear TheoryMass ratio01 natural sciencesHadron physics0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsMicrotronEPJ Web of Conferences
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Non-smooth modelling of billiard- and superbilliard-ball collisions

2008

Abstract A description of billiard-ball collisions using a ‘discontinuous’ model is presented considering a two-step situation corresponding to the ball–ball interaction followed by ball-supporting surface interaction. It is applied to the inelastic impact of a cue ball having arbitrary pivotment and ‘English’ spins against an object ball initially at rest. This formulation provides a simplified approximation to the ‘continuous’ models of impact and considers two different regimes of impact: gross slip, and slip–stick, described in terms of coefficients of friction and restitution. As a result, the angles of scattering of the balls just after the impact (post-collision angles) and when the …

PhysicsSpinsScatteringMechanical EngineeringBilliard ballMechanicsSlip (materials science)Mass ratioCondensed Matter PhysicsNon smoothMechanics of MaterialsBall (bearing)General Materials ScienceDynamical billiardsCivil and Structural EngineeringInternational Journal of Mechanical Sciences
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Breaking Symmetry Effects on Heavy Tetraquarks

2017

In this contribution we present symmetry arguments that can be applied to study the stability of four-quark systems with two different masses. The role played by different symmetry breaking effects and the non-Abelian algebra of color forces is discussed in detail. In the particular case of hidden-flavor all-heavy four-quark states, QQ (Q) over bar(Q) over bar, the system becomes unstable for standard color-additive models. Differences and similarities between Qq (Q) over bar(q) over bar and QQ (q) over bar(q) over bar configurations are presented. In the latter case, its stability when the mass ratio M/m increases was established almost forty years ago. In the former case, we find a kind o…

PhysicsThesaurus (information retrieval)010308 nuclear & particles physicsHigh Energy Physics::Phenomenologystabilitytetraquarkalgebra01 natural sciencescolorFew-body systemsTheoretical physicssymmetry breaking: effectalgebra: nonabelian[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]0103 physical sciencesTetraquarksHigh Energy Physics::Experimentmass ratiocolor: forceSymmetry (geometry)010306 general physicsInternational Journal of Modern Physics: Conference Series
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SATELLITES AROUND MASSIVE GALAXIES SINCE z ∼ 2: CONFRONTING THE MILLENNIUM SIMULATION WITH OBSERVATIONS

2012

Minor merging has been postulated as the most likely evolutionary path to produce the increase in size and mass observed in the massive galaxies since z$\sim$2. In this Letter, we test directly this hypothesis comparing the population of satellites around massive galaxies in cosmological simulations versus the observations. We use state-of-the-art, publically available, Millennium I and II simulations and the associated semi-analytical galaxy catalogues to explore the time evolution of the fraction of massive galaxies that have satellites, the number of satellites per galaxy, the projected distance at which the satellite locate from the host galaxy, and the mass ratio between the host galax…

Physicseducation.field_of_studyCosmology and Nongalactic Astrophysics (astro-ph.CO)Epoch (astronomy)media_common.quotation_subjectDark matterPopulationFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsMass ratioUniverseCosmologyGalaxySpace and Planetary ScienceSatelliteeducationAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysicsmedia_commonThe Astrophysical Journal
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