Search results for "Hill sphere"

showing 2 items of 2 documents

Minidisk dynamics in accreting, spinning black hole binaries: Simulations in full general relativity

2021

We perform magnetohydrodynamic simulations of accreting, equal-mass binary black holes in full general relativity focusing on the impact of black hole spin on the dynamical formation and evolution of minidisks. We find that during the late inspiral the sizes of minidisks are primarily determined by the interplay between the tidal field and the effective innermost stable orbit around each black hole. Our calculations support that a minidisk forms when the Hill sphere around each black hole is significantly larger than the black hole's effective innermost stable orbit. As the binary inspirals, the radius of the Hill sphere decreases, and minidisk sconsequently shrink in size. As a result, ele…

Astrofísica010504 meteorology & atmospheric sciencesGeneral relativityastro-ph.GAgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLuminosityGravitationGeneral Relativity and Quantum CosmologyBinary black hole0103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)Astronomy and AstrophysicsMass ratioAstrophysics - Astrophysics of Galaxies3. Good healthBlack holeSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Hill sphereAstronomiaAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Chaotic dynamics around cometary nuclei

2017

We apply a generalized Kepler map theory to describe the qualitative chaotic dynamics around cometary nuclei, based on accessible observational data for five comets whose nuclei are well-documented to resemble dumb-bells. The sizes of chaotic zones around the nuclei and the Lyapunov times of the motion inside these zones are estimated. In the case of Comet 1P/Halley, the circumnuclear chaotic zone seems to engulf an essential part of the Hill sphere, at least for orbits of moderate to high eccentricity.

Lyapunov function010504 meteorology & atmospheric sciences[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]CometChaoticFOS: Physical sciencesAstrophysics01 natural sciencessymbols.namesake0103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsEarth and Planetary Astrophysics (astro-ph.EP)AstronomyAstronomy and AstrophysicsNonlinear Sciences - Chaotic DynamicsCelestial mechanicsNonlinear Sciences::Chaotic DynamicsSpace and Planetary Science[NLIN.NLIN-CD]Nonlinear Sciences [physics]/Chaotic Dynamics [nlin.CD]symbolsHill sphereAstrophysics::Earth and Planetary AstrophysicsChaotic Dynamics (nlin.CD)Eccentricity (mathematics)Astrophysics - Earth and Planetary Astrophysics
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